ES — r # ‘i й РС lie РАМЕ + 14 LUE NOT GRR Du Е u в ea к. | | и | A ALES Sr. a. N ds $1 Bi у > ' д: и Br р ve € ci О à à 1 в | 5 ® U Ум M Lt a LATE PE LA à 30 AUG. isvi ЗАПИСКИ _ ИМНЕРАТОРСКОЙ АКАДЕМТИ НАУКЪ ФИЗИКО - математическому OTABAEHIIO. KEIM ЕСТ. (СЪ 22 ТАВЛИЦАМИ), ==ф=———— _ РАСАРЕМТЕ IMPÉRIALE DES SCIENCES _ DE ST.-PETERSBOURG. CLASSE DRS SCIENCES EM ET ATHERATIOUNG, VII SERIE. | TOME XIII. ых (AVEC 22 PLANCHES), | | к) Vu 4" Fee —feo С-ПЕТЕРБУРГЪ. 1903. ST. -PETERSBOURG. Продаетса у комисс1онеровъ ИмпеРАТОРСКОЙ Ака- | Commissionnaires de l’Académie ТмрРЕВТАЬЕ des Scien- k ‘деми Haykr: ces: > я. И. Tansyuona, М. Irrepca и Komm. и К, Л. Риккера |}. Glasounof, M. Eggers & Cie, et С, Ricker à St.-Pöters- -. 88 C.- 6yprb, | bou té LA 1. т С.-Петербург, МосквЪ, Bap- | №. Karbasnikof à St.-Pétersbourg, Moscou, Varsovie et 355 ‚ шавЪ и ВильнЪ, Vilna _ №. Я, Оглоблина въ C.- -Петербург® u Kierb, N. Oglobline à st. -Pétersbourg et Kief, _ М. В, Клюкина въ МосквЪ, M. Klukine & Moscou, + LIL Pacnonosa въ Oxeccé, Е, Raspopof à Odessa, И, Киммеля въ Puré, №, Kymmel à Riga en (Г, Гэсеель) въ Лейпциг, Voss’ Sortiment “<. llaessel) à Leipsic, и Коми, BB ТовдонЪ, Luzac & Cie, à Londres. | k 3 Цьна: 16 руб. = Prix: 40 МУК. | Er } % PURE: ER D er 30 ro ЗАПИСКИ ИМПЕРАТОРСКОЙ АКАДЕМШ НАУКЪ DISHRO-MATEMATHARCROMS OTAB.IEHIIO. ÉCRIT I. (СЪ 22 ТАБЛИЦАМИ). р — MÉMOIRES L'ACADÉMIE IMPÉRIALE DES SCIENCES ST.-PÉTERSBOURG. CLASSE DES SCIENCES PHYSIQUES ET MATHÉMATIQUES. Vor SÉRIE. DOTE ZE LIL. (AVEC 22 PLANCHES). —— <= С.-ПЕТЕРБУРГЪ. 1903. ST.-PETERSBOURG. Продается у комисс1онеровъ ИмпеЕРАТОРСКОЙ Ака- | Commissionnaires de l’Académie ImpErıaLe des Scien- деми Наукъ: ces: И, И, Глазунова, M. Эггерса и Коми, и К, Л, Риккера | J. Glasounof, M. Eggers & Cie, et С, Ricker à St.-Péters- въ С.-ПетербургЪ, bank: H, I. Карбасникова въ C.-Ilerep6ypré, МосквЪ, Bap- | N. Karbasnikof à St.-Petersbourg, Moscou, Varsovie et il шавЪ и ВильнЪ, Vilna, H. Я. Оглоблина въ C.-Ilerepöypr& и Kiesb, N. Oglobline à St.-Pétersbourg её Kief, M. В. Клюкина въ МосквЪ, M. Klukine à Moscou, Е, II, Распопова въ ОдессЪ, Е, Raspopof à Odessa, Н, Киммеля въ Pur, №, Кушше! à Riga, Фосеъ (Г, Гэесель) въ Лейпциг, Voss’ Sortiment (©, Haessel) à Leipsic, Люзакъ и Коми, въ Josxoné. Luzac & Cie, à Londres. Цьна: 16 руб. = Prix: 40 МК. Напечатано по распоряженю AuneparoPpckoï Академ Hayk®. С.-Петербургъ, Мартъ 1908 г. НепремЪнный секретарь, Академикъ Н. Дубровин. ТИПОГРАЯЯ ИМПЕРАТОРСКОЙ АКАДЕМШИ НАУКЪ. Bac. Остр., 9 зип., № 12. СОДЕРЖАНТЕ XIII ТОМА. — TABLE DES MATIÈRES DU TOME XII. № 1. ®. Ренцъ. ОпредБлене noxoxeniä спутни- ковъ Юпитера изъ Фотограчй, снятыхъ въ Пулков$ г. Костинскимъ и въ Гель- сингФорс$ г. Доннеромъ. 2-я часть. 1902. ХХУШ-н 271 страницъ. №2. A. Ляпуновъ. Объ одномъ рядЪ въ теорш линейнаго дифххеренщальнаго уравненя второго порядка съ пер1одическими коэФ- Фищентами. 1902. 70 страницъ. № 3. Н. Андрусовъ. О кардидахъ солоноватыхъ водъ. Выпускъ Г. (Съ 7 таблицами и 5 œu- гурами въ текстЪ). 1903. 82 страницы. № 4. Отчеть по Николаевской Главной Физи- ческой Обсерватор!и за 1901 г., предста- вленный Императорской Академш Наукъ М. Рыкачевымъ, директоромъ Николаевской Главной Физической Обсерватории. 1903. II-+-153 страницъ. № 5. В. Паттенъ. О строеши- рода Tremataspis и классихикаци трематаспидовъ. (Съ 2 та- блицами). 1903. 33 страницы. № 6. В. Фаусекъ. Паразитизмъ личинокъ Апо- donta. (Съ 8 таблицами). 1903. ТУ +141 страницъ. N 7. В. Заленскй. Анатомическя изслБдованя надъ аппендикуляртями. I. Oikopleura Vanhoeffeni Lohmann. (CE 5 таблицами). 1903. 42 страницы. № 1. № 2. F. Renz. Positionen der Jupiterstrabanten nach photographischen Aufnahmen berech- net. II. Teil. Oppositionen 1896 — 98. 1902. XXVIII-+- 271 Seiten. А. Liapounoff. Sur une série dans la théorie des équations différentielles linéaires du second ordre à coefficients périodiques. 1902. 70 pages. № 3. М. Andrussoff. Studien über die Brackwasser- № 4. № 7. cardiden. Lieferung L (Mit 7 Tafeln und 5 Figuren im Text). 1903. 82 Seiten. Compte rendu de l'Observatoire Physique Central Nicolas pour 1901, présenté à l’Académie Impériale des Sciences par M. Rykatchev, directeur de l'Observatoire Physique Central Nicolas. 1903. II + 153 pages. . W. Patten. On the structure and classifica- tion of the Tremataspidae. (With two pla- tes). 1903. 33 pages. . V. Раиззек. Parasitismus der Anodonta-Lar- ven. (Mit 8 Tafeln). 1903. IV-+-141 Seiten. W. Salensky. Etudes anatomiques sur les appendiculaires. I. Oikopleura Vanhoeffeni Lohmann. (Avec 5 planches). 1903. 42 pa- ges. ГЕ ЧМО ПОЛЯНА AR LUE = 1 à I Fe] ar RR er пой а го a SORT 20 — 105 Г roots IST. TE Защ à во TE HIER D one al ant of ins ut orage À 2 и. вы < nb eines ler) Anoitenps Bub. ÿ sy boE Е Aa Keira AU or SORT“ | зов я Bis ieh) re Hulk) 8 раны pal | À CA «вдову ET ви arms x евр «ата» 9ОТ 55 иБиот. Be я д Мала LORL ano авар або” ur бУиЗО 24h" Jfahiaqil ооо nano D bn ‚vadaleiy М à CL US PM DT Нара и | ste sh net rat. Le и I sr. Br | EN чи Е MAT" olans Ke et Tea. anal Tr Ar je Fa er QT «АУ ë Be mai я | 30 Aus 1907 ЗАНИСКИ HMHEPATOPCROÏ АБАДЕМИИ HAYKR. MEMOIRES DE L’ACADEMIE IMPERIALE DES SCIENCES DE ST.-PETERSBOURG. УЕ SÉRIE, mo. ФИЗИКО-МАТЕМАТИЧЕСКОМУ OTIBIEHI. | CLASSE PHYSICO-MATHEMATIQUE. Tome XII № 1. } Volume XIII. N 1. POSITIONEN JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN BERECHNET YON a _ №. нева Là р a — U. TEIL. OPPOSITIONEN 1896—1898. | (Vorgelegt am 4. Ociober 1900). в. _ПЕТЕРБУРГЪ. 1909. ST. _ PÉTERSBOURG. à _ Продлетвя у комиссюнеровъ ИМПЕРАТОРСКОЙ Commissionnaires de l’Académie Inräriaun des E _Академи Наукъ: Sciences: _ в. и. Tansynona, № М, Irrepea и Коми. и К, Л, en É er М. Eggers & Cle, et С. Ricker à St. „Pöters- 7 2 рбур в; п. ов жа въ С.-Петерб., Москв, Bapınank и | №, Karbasnikof à St,-Pötersbourg, Moscou, Varsovie et | Vilna HA Oraodamıa въ C, „Петербург 1 и Kienb, 180 Iobline "a St-Pétersbourg et Kief, . M. `В. Клюкана въ МосквЪ, М. Klukine à EE В, п. gg въ ‚m Onecch, f Е, Вазророй à Odessa, gg въР - X. Kymmel à Riga, = _ Фоесъ (Г Fe) въ Лейпциг, Voss’ Sortiment (6. mul) à Leipsic, у фе» и Коми, въ Лондон%. - Luzac & Cle, à Londres - Inua: 4 Руб. 40 коп. — Prix: 11 Mark. ei < . Pr ——-- ЗАШИСКИ HMIIEPATOPCKOH АКАДЕМИИ HAYKB. MÉMOIRES DE L’ACADEMIE IMPERIALE DES SCIENCES DE ST.-PÉTERSBOURG. УЕ SERIE. ПО ФИЗИКО-МАТЕМАТИЧЕСКОМУ ОТДЗЪЛЕНТЮ. CLASSE PHYSICO-MATHÉMA TIQUE. Tome ХЕ. № 1. Volume XIII. № 1. POSITION EN » JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN BERECHNET VON Е`. Renz. П. TEIL. OPPOSITIONEN 1896—1898. (Vorgelegt am 4. October 1900). 1 С.-ПЕТЕРВУРГЪ. 1902. ST.-PÉTERSBOURG. Продается у комисс1онеровь ИмпЕРАТОРСКОЙ Commissionnaires de l’Académie Imp£rıaue des адеми Наукъ: Sciences: ‚LH. rue М. Эггерса и Коми, и K. Л. Риккера | J, Glasounof, М, Eggers & Cie, et С, Ricker à St.-Péters- въ С.-Петерб : Ур bourg, < Й. I. Карбаеникова въ С.-Петерб., МосквЪ, Варшавф и | №, Karbasnikof à St.-Pötersbourg, Moscou, Varsovie et ВильнЪ, Vilna, Н, Я. Оглоблина въ С.-Петербург и Kiert, N m. à St-Pétersbourg et Kief, М. В. Клюкяна въ МосквЪ, М, Klukine à Moscou, Е. II, Распопова въ Oxeccé, Е, Raspopoff à Odessa, Н. Киммеля въ Purb, = N. Kymmel à Riga, Фосеъ (Г. Гэссель) въ Jeñouurb, Voss’ Sortiment (6, Haessel) à Leipsic, Люзакъ и Коми, въ Jonnont. Luzae & Cie, à Londres. Inna: 4 руб. 40 коп. — Prix: 11 Mark. * Pos N я FETE ET: No PET En И } N I IN Tensitiier NE un Se u A “ri, tie | MERE ERW TR bee г MOT ARE GE PM OSB MESA RENE My A M вх Date AVE à lives ES no de Е, И: 41 HF Ic у | e {< à * Pa j RE ee QU > CRETE PATTES Fr EA u à у А } р UNE, x PE Ser el Hera Tee we) in ne go de eu à ah FAT Bank Bye Er À VORWORT. à Der vorliegende zweite Band der Jupiterspositionen berechnet nach photographischen Aufnahmen umfasst die Oppositionen 1896—1898. Während mir bei Bearbeitung des ersten Teils nur Helsingforser Clichés zu Gebote standen, ist in den Jahren 1896 und 1897 sowol - von Herrn Professor Donner, als auch von Herrn Kostinsky in Pulkowa und endlich im | IK Jahre 1898 nur am letzteren Orte eine so grosse Anzahl von Aufnahmen des J upitersystems _gemacht worden, dass das in diesen Oppositionen gesammelte Material das früher publicierte 4 an Umfang bedeutend übertrifft. a Die Helsingforser Aufnahmen sind genau nach dem im ersten Bande beschriebenen Schema angeordnet, während Herr Kostinsky jede Platte nur an einem Abend exponierte und zunächst mit längeren oder kürzeren Zwischenzeiten auf jedes Cliché, westlich und | _ östlich vom Centrum, je еше aus vier bis acht Einzelaufnahmen bestehende Reihe brachte, р | ar ab jedoch su Een Vorschlag stets sechs и machte, die symmetrisch _ Meridian vertheilt sind. Diese Gruppierung bietet den Vorzug einer gewissen Vereinfachung der Rechnung. Dank der Benutzung von Diaphragmen zeigen die Jupitersbilder auf den и а _ Pulkowaer Platten schärfer begrenzte Ränder, als auf den Helsingforser Negativen, dagegen - ” ist der vierte und schwächste Trabant auf ersteren bisweilen unterexponiert. в Herr Professor Donner und Herr Kostinsky haben ihren Aufnahmen folgende Daten | beigefügt: Son, Физ.-Мат. Отд. 1 Il К. Renz, Opposition 1896. I. Helsingforser Clichés. к ® 5 a яя s| 2 Е Thermometer ы Е а ae En BE „= © =.2|\der Exposition.| © & = mn Е Baum В ЕЕ FAT ma ая o& Bemerkungen. 5) я 3 a. Tubus. äusseres. |SN =| Sternzeit. 52 | Зо I ra Ks ré AS 128 | A | 1895 Nov. 27 | 7629 | — 68 R. | — 77 R. |— | 5* 17“ 50° | 10° | NW |Praesepe. | a 2027 8 Luft 1 (ruhig und durch- | b 21 54 8 sichtig). с 2215 8 а 22. 43 8 | е 23.08 8 | В | 1895 Nov. 28 | 766.0 | — 5.4 — 6.3 — | 5 58 34 20 | SW |Praesepe. | a 6 KO 49 8 Luft 1. b Ka; 8 с 15240 8 d 2! ТО 8 e 2, 32 8 C* | 1895 Dec. 27 | 769.1 | —10.0 — 10.9 — | 3 -0,31 10 SO |Praesepe. | a 3. 2067 15 L.3(etw. unruh. u.nicht ganz b 3 44 15 scharfe Bild.)St. Wind v. NO. € 4 41 15 Während der zweiten Expo- d 5,25 IS sition schwankt der Tubus e 02.7 15 etwas. D | 1896 Jan. 11 | 760.0 | — 5.0 | — 6.3 u 70897 57 10 NO | Ргаезере. а 738429 8 Luft 1—3.Leichter Eisnebel. b 39 37 8 € 40 24 8 d ATEN 8 e A2 UT 8 | 29 | A | 1896 Jan. 15 744.7 | — 6.2 — 7.4 — 1137 4007 25 NW | Praesepe. | a 7 SOME 20 Luft 1. b 51.122, 21220 | с 559 20 d 52 36 20 е ee 20 В | 1896 Jan. 17 | 753.2 | — 2.1 — 27 — | 6 34 34 25 SW | Praesepe. a 6 36 12 20 Durch Wolken. Luft 1, b 36 50 20 € 37.30) 20 d 38 16 20 e 2138 2006 20 С | 1896 Jan. 20 | 765.9 | — 49 — 5.7 — | 8 43 16 25 SO | Praesepe. à a ОН 20 Luft 1. b 46 25 20 ‘ с Я UE 20 а 47 47 20 е 48 25 20 PosITIoNEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNMEN. Ш Datum. der Platte. en “x 4 1 Soit $ а Le 1896 Jan. 23 | 1896 Jan 26 1896 Jan. 30 C | 1896 Febr. 1 r & 1896 Febr. 17 ‚| 1896 Febr. 18 | 1896 Febr. 10 Barometer mm 753-2 743-5 767-4 745.6 745.0 762.9 768.0 Thermometer a. Tubus. üusseres. — 23 В. — т В. — 8.3 — 93 + 15 + 0.6 me — 6.9 . — 0.2 , — 0.9 — 14 — 22 ми — 11.2 — 3.1 | — 4.3 =: = PR | = О 9 < Mitte 8. ‚8-3 | der Exposition.| = 8 -2 a | Helsingforser | $ Е © : = 25 Sternzeit À en = — | 6 37" 24° | 25 a 6 39 10 20 b | 39 54 | 20 с 40 35 20 а | т 12 20 е at 55 20 = 6 50 44 30 оз ю | 30 b 54 56 30 с 54 53 30 а 55 39 30 e 56 25 30 a 9 14 43 20 b 15 20 с 1$ 58 20 а 16 40 20 е 17° 16 20 — 9.19.0 20 1—| 8 59 20 20 а Ad: 97 20 b 1 56 20 с 2 34 20 а 311 22 20 € 3 49 20 — | 8 32 59 25 a 535 (© 20 b 35 44 20 С 36 22 20 d 36 59 20 € FE т) 20 — | 8 19 20 25 "a 8 22 44 20 b 23 22 20 e 27.» 32 20 d 27 38 20 e 28 13 20 — | 6 43 27 25 а 6 45 39 20 b 46 16 20 с 46 51! 20 а 47 33 20 е 48 6 20 — | 9 56 20 25 а 9.50.39 20 b SX ET 20 с О 4193 20 а 92.132 20 e 53 15 20 Lage gegen das Centrum. Zi © NW SW 50 NO NO Bemerkungen. Praesepe. Luft 1. | Praesepe. Luft 3. Luft 1—2 (durchsichtig, et- was unruhig). Praesepe. Praesepe. Гай 1. Praesepe. Luft 1. Pracsepe. Wolken ziehen vorüber. Praesepe. Luft 3—1. Ргасзере. Luft 1. Ргаезере. Luft 1. Durch dünne Wol- ken. 1* IV Reihe. 32 | A 33 | A Е. Renz, Datum. 1896 Febr. 18 1896 März 9 1896 März 14 1896 März 16 1896 März 31 1896 April 1 1896 April 7 Barometer. 761.4 755-3 759.8 759.5 754.9 760.7 Thermometer a. Tubus. — 5.0 äusseres. — 4.5 В. Fran — 5.8 135 — 4.6 = 35 + 0.8 Bezeichn. дег Aufnahme хаос © sacs | | < us or | < «оса | хаоса [sas cs [sansca der Exposition. Helsingforser Mitte Sternzeit. 10 11 II Expositions- Lage gegen das Centrum. NO NW SW SO NO NW SW Bemerkungen. Luft 3. Neblig. Praesepe. Luft 3. Neblig. Schnee zu erwarten. Praesepe. Luft 3. Praesepe. Luft beinahe 1. Praesepe. Praesepe. Luft 3. Luft 2 (durchsichtig, aber etwas unruhig). Praesepe. PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. у ПИ. Pulkowaer Clichés. .. = = 2 à . ” Nr - 2 © ? |& ав| 3 | £ = S Thermometer TS à Mitte а. Е 5, | = = = Я -= | der Expositi HIS) | Е = Datum. Е 1e < т = = a | |: Bemerkungen. = я : a о . 2 >| > | 5 = Е: inneres. äusseres. |2 Sternzeit. u ET 3 cn a = 3/3 | ] la о | А | 91| 1895 Oct. 11 | 587.3 | + 70 R. | + 88 © |—| 4 т | 20° о | Bild.3—4. [Undurchs. | a 15 | 01) Luft. Leicht. Wolken. b | А 2 10 DieAufn.folg.d.Reihe с 4 34.2 10 о | nach von S nach N. | d | 20 f=47.8. | e 5 | B f 10 | W | 9 E m 20 . h 4 49.2 20 3 | Bilder 4. 0 30 . k 40 А | 18 | 1895 Nov. 25 | 590.4| — 03 — 05 а | 15 Die Aufnahmen sind b 6h 67” 5 in AR angeordnet. | с 20 а | ь 20 f=46.9. e 8,10 | 20 DieAufn.verl.v.N n.8. T 18 10 20 Wind, 9 20 35 то h 22 15 10 р 242 5 136 | A | 27 | 1895 Dec. 27 | 598.4 | —12.0 — 16.4 a RON 20 | O |2 b* 2138 15 с ASIA 10 N nach $5. 2 d 5-36 10 - e 6 46 10 if 8 9 5 f=46.5 B 9 7237.36 20 | W | 4 | Bilder 3—4. h 2512.23 15 р 26 39? |s?(10?) S nach N. k 28 31 10 Гы Зо 10 т* 31 14 5 р. — 7 40.0 34 4 | Ргаезере. 137 | A | 28 | 1896 Jan. 1| — — ‘|! о — |1 6 89 9 т о | Ргаезере. ve. | а 6 48 10 | 25 3 | Mondsch. Undurchs. b 50. 12 20 : Bilder 2. [Luft. с 52.4 15 f—=46.4. . а SE «17 10 N nach $. e 55 47 | 10 À à 57 44 15 A | 82 | 1896 Jan. 20 A! — 6.2 — 9. | в 20.7 п 2 er | % a 6 28 17 20° 2 | Bilder 3—4, unruhig. b 29 59 15 S=46.6 с 39 29 15 d 41 32 10 e 42.33 10 F 43 44 | 15 1) Zwischen den Lagen O und W blieb die Cassette immer unberührt am Instrument. 9 т а У Г. Renz, : Mitte der Exposition. Pulkowaer Sternzeit. Thermometer "N Datum. Bemerkungen. dauer. inneres. "äusseres. г] der Platte Reihe. Pulk. lauf. № Barometer. Bezeichn. der Aufnahme. Expositions- Lage gegen das Centrum. Diaphragma. aa* 2 h | s om й 39*| A | 33 | 1896 Jan. 26 de —414.0 С. | — | 7° 177 28 3 3 | Bilder 4. | a | 7 28-53 10° | 3 b 30 35 15 с 38. 53 10 а 32.1353 10 e 34 6 5 | 40 36 | 1396 Jan. 27 | — — —15.0 — | 5 54 3 2 2 | Pracsepe. Leichte A a | 16 anus 15 | O | 2| Wolken. b 3 48 10 с 4 48 10 N nach 8. d ss 15 ex 6 53 20 f=46.3? Bilder 2. B Я 6 Jo 13 Ро: М2 9 11 48 10 h 12, 146 то S nach М. î а 15 h* 17 зв 41, 38 | 1896 Febr. 1 | 597.3 | — 6.5 В. | — 9.5 —| 7 58 55 7% 3 | Ргаезере А al 8 4 32 15° | O | 3 | Mondsehein. b 6 о 10 ec 6 52 15 N nach S. d 8 o 10 е 8 45 10 à f—=46.5. B iR Sr 2 77 5 | W | 3 | Bilder 4. 9 3417 8 h 13 58 5 S nach N. à 14 40 то | k* 15 40 10 42 39 | 1896 Febr. 3 | 587.4| — 2,5: — 4.0 — | 8 18 4 4” 4 | Ргаезере. А #18: 125 29 10° | | 4 |Starker Wind. b 26 29 то N nach 5. с 270029 10 d 28 26 IS f=47.0 er DET IS Bilder 2—8. B НЕ 10 | \М|4 I 34 37 5 h 35 19 10 В nach N. р 36 6 15 k 37 16 15 43 | A | 42 | 1896 Febr. 4 | 5944| — 7,5 —11.0 CÉSAR TL 15 3 | Auf die Platte fiel E | b 34 34 | 10 N nach S., [Licht. с 3534 To 1 —46.5. а 36 34 10 Bilder 3. eig ЗА 5 — |7 44 9 3” 3 | Ргаезере. 44 | А | 45 | 1896 Febr. 6 | 590.2 | — 1,3 — 10 вто 54 10° | О | 2 | Undurchsicht. Luft. b 11 34 10 € 12 49 10 N nach S. ka 13 752 er e* 14 57 бт | NO 29-93 2, Praesepe. B тя м f=47.1. POoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN A UFNAHMEN. vu ur =. . — fi u 3 5 Thermometer ЗЕ Mitte Е de ВЕ Е ps © EE A Datum. 5 Rn 3 Е ные 2 Е = Г: £ Bemerkungen. 5 Е. inneres. äusseres. [SZ| Sternzeit. = р а FA = ЗА ‘le о о 1896 Febr. 6 | 590.2 | — 1.3 В. = 60.Cobg-| 737“ 5 8 | W.| 2 | Bilder 2. . h 38 55 8 N nach 5. т 40 4 то k 41 14 10 1896 Febr. 7 | 589.6 | —11.2 — 12.5 a 9 29 54 то | O | 3 | Recht durchsichtige b 31 14 10 Luft. с 32 34 10 N nach S. d 3731 15 - € 34 17 р —| [9 540. 9 3 f=46.4. f | 9 46 44 10 | М Bilder 1—2. 9 48 11 15 h 49 4 10 N nach 8. 8 49 54 10 |. k so 55 8 1896 Febr. 19 | 603.1 | — 5.8. — 8.8 ga 18 55 21 70% b 56 39 10 с. -57 29 10 N nach S. 5 d 58 14 10 er 59 12 Sn — | 9 4 54 3 Praesepe. /=46.7. - 9 19 42 S В. Bilder 2. 9 20 44 10 N nach 8. h 21 39 10 iv 22 49 10 k 24 6 15 54 | 1896 Febr. 22 | — — — 12.0 ae} #7. 39 SI 10 | O | 2 | Mondschein. b Art #3 8 С 41 52 8 N nach 8. d 42 34 5 e* 43 34 5, — | 7 50 6 3 Praesepe. /—46.4 Palo" SL ai 10 | W Bilder 3—4. 9 I 10 h | 8 % я 8 N nach $. р 1 52 8 k* 2:64 8 1896 Febr. 23 | 610.6 | —10.8 —14.0 О та 15 | O | 3 |3,Trab. sichtb.; um | b 6 45 10 7°20"erschien der 4te c* 7:45 10 Bilder 4. [am Westr. d 8 52 15 N nach S. e 10 25 10 —| 7 18 30 5. Ргаевере. Но 33; © 1$ | М f—=46.4. 9 34 35 10 Leichte Wolk. ziehen h 35 25 10 ü.d.Himmel. B.3.N—8. $ 36 25 10 k* 37 26 8 1896 Febr. 24 | 610.4 | — 8.1 —11.0 8117 12 27 15 | W |3 Um 7*21” Eintrittdes > b 13 50 10 erstenTrab.in d.Jupi- с 15 12 15 N-S.[tersch.am Ostr. d wa 10 Bilder 2—3. VII F. Вами, — Pulk. lauf. № ^ u Datum. N der Platte. Reihe Barometer. 1 50 | A | 59 51 | А | 63 52°| А | 66 | 1896 März 8 | 593 52b| A | 70 | 1896 März 9 / 1896 Febr. 24 610.4 1896 Febr. 25 | 610.3 1896 Febr. 26 | 606.6 596.6 Thermometer inneres. äusseres. Bezeichn.der Ашвавше 1 5° a IS Ses re аа > * — 6.0 — 80 2 >. 25 |ysacoc = x uhr) De 2: >. ras * o| — 3.9 |sayes ==. u * — 4-7 -— au ER | < = < + * Mitte der Exposition. Pulkowaer Sternzeit. 10 10 h Expositions- dauer. Lage gegen das Centrum. Diaphragma. Bemerkungen. Praesepe. f=46.4. Ders. Trab. tritt aus am Westr. um 9°35”, Auf einig. Aufn.ist er hartamRanded.Plan. Sn.N. [deutl. sichtb. Bilder 3. Eine Aufnahme ist verschoben. Mond sehr nahe. N nach 8. Praesepe. f==46.1. Bilder 2. N nach 5. Mond sehr nahe. N nach В. f=46.7. Praesepe. f=46.7. N nach 5. Bilder 4. N nach В. Praesepe. f—=47.0. Bilder 3. N nach 5. Bilder 3. N nach 5. Praesepe. Bild. 3—4. f=47.0. Bilder 2—8. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. IX | | | | | | | | ] x 2 5 2 Eis £| . i . $ Thermometer 3 = Mitte я. 8 а s| 2 Е 2 88 | der Ex osition.| 38 [25 ® | A = = Datum. Е cE een "| FE 8 5 Bemerkungen. | 3 я | à 3 inneres. äusseres. БЕ Sternzeit. ae [False CR [ee] = A514 г. lle о Li N 70 | 1896 März 9 | 596.6 | — 4.7 В. — В | 10/34" 27 15 | W}21]N nach 5. i 35 30 10 36 40 10 72 | 1896 März 11 | 593.4 | — 4.6 =# Cle 9 25 10 20 | O | 3 | Bilder 8. b* 27 : 22 15 с 28 45 10 а 30." :5 10 e AU LS 10 — 9 87 55) 13730 Praesepe. Bilder 2—3. f | :9 46 20 20° | W f—=46.9. h 47 42 15 N nach В. h 49 2 15 р SOUS 10 k* SitLa2S 10 А | 75 | 1896 März 16 | 596.4 | — 5.0 — aug 31 550 20 | О | 3 | Bilder 4—5. Гм ; b 32 52 15 Windig. e 33 54 16 N nach В. d* BE, 15 e 36 10 20 —| 9 42 30 в Praesepe. ; fl бат 10 20° | W f=46.7 9 4807 15 Bilder 3—4. № 49 5 20 N nach 5. р 49 55 10 k* so 55 10 76 | 1896 März 24 | 592.4 0.0 — а | 9 49 54 15 | O | 3 | Mond sehr nahe. Cir- 2 b ST: +12 20 Bilder2. [ruswolken. 6 52 29 IS 4 53 34 и — |210 5 2 2 Praesepe. e|ıo 11 17 20° | W f=47.2. “à 12 14 15 Bilder 2. 9 132. © 15 |! h 14 12 10 56 | A | 77 | 1896 März 29 | — - — 8.0 a* ? 20 О | 3 | Bilder 4—5. Di b | 10 ı 9 15 4 ce 3 15 d 4 4 15 N nach S. 6* 5 19 25 f 6 24 ЗЫ. — | 10 11 32 3 30 Ргаезере. 9|ю 18 10 25 | W —46.7 h 19 9 IS Bilder 4. ie 20 9 15 N nach 5. k 24.27 20 I 22; 22 10 F ” | A | 79 | 1896 März 30 596.9 — 7.0 = а 10.719: 33 20 |. О | 2 | Bilder 8. . 20 55 15 с 22 30 15 N nach 5. d 23 28 10 | е 24 18 10 — | 10 28 3 2” Praesepe. Bilder2—3. | X F. Renz, = R ae n- a El = $ Thermometer ЗЕ Mitte а; FEI 2 52 | der Exposition.| ‘= м | S a Datum. Е Et р 53 |®2|&|. Bemerkungen. ze S 3&| Pulkowaer оз [20 =. = kn inneres. äusseres. |S Е Sternzeit. 7 |& ls en 22 а als 1896 März 30 Pe 9 36 30 15 h 37 30 15 S nach N. р 38 18 то | k 58 | A | 81 | 1896 März 31 | 594.1 | — 5.0 — 7.0 ба mor 2010 Undurchsicht. Luft. b 10 46 15 Bilder 2—3. С 1136 15 N nach В. e* 13410 10 — | 10 18 54 a. Praesepe. Bild. 2-3. B у то 27108 20° | М f=46.65 ' 9 25 36 15 N nach S. Bilden Bu ie ac 59 | A | 83 | 1896 April 8 | 595.4 О аа ТЫС L.a-l-10- 40.43 25 0 b 42 20 20 С 43-30 - 20 N nach 5. d 44 52 15 e* 452 55.11 Dal & — | 10 55 30 3 Praesepe. Bild, 8—4. B 771.10/,022738 25 | W f—47.4. № 9 3 50 20 Bilder 4 7 h 4 52 15 N nach В. $ 5,82 IS k 6 52 IS 60 | A | 86 | 1896 April 10 | 593.9 | + 0.5 + 0.8 а| им 44 59 20 |0 Bilder 4. b 46 19 20 6 48 21 15 | d SD" 15 N nach 8. e* 51:34 10, | — | 11 57 9 3 Praesepe. Bilder 4. B a AS 25 | W Bilder 3. f—47.4. 9 6* 29 20. | h m 59 20 S nach N. р OÙ т 15 k* то 16 15 - 61 | А | 87 | 1896 April 14 | 597.2 | + 3.1 — 4.5 в тез 25 0: Bilder 3. : b 8 10 20 Uudurchsicht, Luft. € 8 so 20 dx 9 37 15 е 10 12 B CE J=47.5. — | 11 16 0 3 39 Praesepe. Bilder 4. B Sr Jan 2038 15, AU | Bilder 3—4. - g* 22.05 20 Durch Wolken. h 23 3 25 $ 23 48 25 k 24 45 30 62 | А | 90 | 1896 April 19 | — = + до Mondsch. Undurchs. Bilder 4. [Luft. N nach 5. à A3 (>) м [®) ь о © © LE] = D = = un PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN À UFNAHMEN. XI | * 5 a à ag = 8 Thermometer =8 } Mitte 5. |586 à | der Exposition.| = bal $ Datum. Е | pe ЕЕ рн FE о 3 | Bemerkungen. Е inneres. äusseres. |S2| Sternzeit. “> [als a à A ASIA 1896 April 19 | — — de 40204 па: hast ar $ 10° | O |; e* 32 25 10 — | 11 38 80 3 Ргаезере. BEN IN 4335 ı0° | W Bilder 4. f=47.4. 9 44 5 10 Die Corr.desChron.ist h 44 37 15 unbekannt; jedenfalls i 45 12 15 überst. sie nicht 1-5”, k 45 50 20 S nach N. . Opposition 1897, I. Helsingforser Clichés. ; | 5 œ яя 5 Thermometer =5 Schluss я. | в 2 ‚8.3 | der Exposition. 3 5 DE Bemerk = | 2E| Helsingforser | За | 23 um. сх Е а. Tubus. äusseres. | 3| Sternzeit, eo Е = 2 FA [ea] Has К : > . | 1897 März 22 759.1 — 5:5 в. | — 77 R | a | 12* 49" 48° 10° | NW |Luft 1. ti | b so 22 10 - с 50 48 10 d SL! 1} 10 re SE 138 10 | | | |[— | 12 55 27 | 10 D. М. +26°2343 | 1897 März 26 752.27 63-3 — 4.7 alıo 39 21 10 | SW |Luft 2. 1 b 39 56 10 € 40 25 10 ра 40 50 10 I Le 4ı «17 10 | | — | 10 44 56 10 D, M. -1-26°2348. 1897 März 28 745.3 | — 1.45 — 2.8 AN 20 3% 10 so | | b 217 38 10 % 22 24.5 10 ' hd 235 33 10 ‚be 23 58 10 à HE NI TE Le D, M. +26°2343. [897 März 30 | 733.5 | — 0.7 Le" [Ван 5 À ıo | NO ‚Го 5 39 10 | с 6.18 10 d 71: 16 15 e 70:54 10 Windstoss bei der letzten | | — | 11 15 37 40 D. M. -+26°2343. [Exposit. 1897 April 15 | 763.5 te 2.5 +12 а | 13 36 30 12 | NW [Luft 3—4. : b 37 10 12 д” XII № — der Platt Reihe = _ > 65 | A Datum. 1897 April 15 1897 April 18 1897 April 23 1897 April 24 1897 April 25 1897 April 26 1897 April 28 1897 Mai 8 1897 Mai 15 Barometer. mm 763.5 747.8 762.6 763.5 766.3 769.2 761.5 763.0 766.5 Thermometer a. Tubus. + 25 R. + 4.65 + 5.8 + 8.4 pr 95 + 6.5 + 8.4 +-14.6 F. Renz, äusseres. о + 1.2 В. + 2.0 252933 + 45 + 4.1 + 5.0 + 7.0 13.2 Bezeichn. der Aufnahme. |sasoa | + &o 8 [sas [os uses [ones [onsosa [sas © а SS [sas der Exposition. Helsingforser Sternzeit. Schluss Expositions- dauer. Lage gegen das Centrum. 2 = SW so NO NW SW 50 NO NW Bemerkungen. D. M. -+26°2343. Luft 3. D. M. -+26°2343. [D. M. +-26°2548. Luft 3—2. D. M. -+26°2343. Luft 2. Тай 3—2. D. М. +-26°2343. . Гай 2—3. D. M. +26°2343. Luft 3. D. М. -+-26°2348. Die Luken waren kurz vor- her geüffnet worden. D. М. -+26°2343. Luft 1—3. POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Datum. der Platte. Pulk. lauf. № 150 1897 Mai 15 В | 1897 Mai 17 с | 1897 Mai 18 1897. Mai 20 Datum. Barometer mm 766.5 762.4 759.8 760.3 Barometer. 1897 Febr. 5 585.6 151 | 1897 Febr. 15 | 594.4 | —12.0 — = Thermometer a. Tubus. äusseres. +146 EN 32 В. 10.5 + 9.2 —=14.6 +13.2 3 +-10.6 + 9.2 IL Pulkow Thermometer inneres. äusseres. 140 R. —190 —16.5 = 0 < [7 a 33| Schluss |&.|%5 [5 = | 4ег Exposition.| 25 | GE © : a 5 © 52| Helsingforser 2а | 20 KE Sternzeit. я an a“ A |" а | 14* 41” 26° 12 | NW e 41 56 12 — | 14 45 27 12 о А ит 15 SW b 320,17 15 € 32 55 15 d 33 31 15 e 34 II 15 — | 15 36 4 IS DAT 2 LS 15 so b 25.152 15 € 26 25 15 а 27 4 15 e 27 38 15 — | 15 29 9 15 — 30 46 15 а | 1$ 18 142 15 NO b TON 15 15 € 19 45 15 d 20 12 15 е 20 44 15 — | 15 22 47 15 aer Clichés. Erz a а и = Mitte Е 5 ‚i3| der Exposition.| 5 | £ 2&8| Pulkowar | 35 | 4 SZ| Sternzeit. MERS [62] A A ee 3713 5 а 8 34 4 20 b 36. 32 16 с 37 46 16 а 39 16 16 e 40 32 16 f AT 44 20 a | 10 38 10 16 3 b 39 34 16 с 40 57 10,, — | 10 56 2 2 BAL TANT 10° e 1} 10 16 f 27.12 20 XIII Bemerkungen. D. М. -+26°2343. Luft 1. D. М. -+26°2343. Exp. v.D.M.-+-26°2343 war d. Turmw. im Wege. Diese тн der erst. [ist daher zu verwerfen. D. M. 2602343. Bemerkungen. Ргаезере. Bilder 4—5. Bilder 4. Die Aufn. sind symmetrisch gegen d. Plattencentr. an- f—46.4. (geordnet. Bilder 2—3. Praesepe. Mond sehr nahe. Bilder 2—3. f=46.4. XIV F. Renz, PE: | : в | 3 < 5 Thermometer ЗЕ Mitte а 5 | ’ > a ss + | || 81 = 2 5373| der Exposition. | € a N El = atum. а ‘a Е у | AE = Datum Е Е Е Palkomsan à Е Bemerkungen < = S inneres. äusserés. |SZ| Sternzeit. > ‚3 : = à = em [ea] А | ], ы a « [2 9 о h ОО т i N 69 | 154 | 1897 März 7 | 599.3 | — 5.5 В. |» — 6.0 С. | — | 11 14 35 2, | 3 |Praesepe. В ad | Trans 20 Bilder. 3. Undurchs; Luft. ||! b 24 17 15 | с 2519 и f=46.7. | а 26 23 16 \ e EP CE 20 | 18 28 57 25 | 70 | 156 | 1897 März 9 | 602.4 | — 80 —10.9 — 54 36 2" |, 3 | РЕаезере. Bilder 2, а | 11 53 46 20° | Bilder 1—2. b 55} В 15 e 56 8 15 I=46.7, d 57 46 » | 20 1 e 58 44 16 р $ 59 51 10 71 | 161 | 1897 Мага 10 | — — — 11.0 a | 8 40 36 20 |3 |Bilder 2. | b 42; ТА 16 } с 42 16 1 —=46.5. | d 44 34 24 | е 45 48 16 | ай 46 46 10 N | —| 8 52 46 2" || |Praesepe. Bilder 2—3. : || | | 72 | 162 | 1897 März 11 | 599.8 | — 7.0 — 9.0 — | 9 30 15 2 3 |Praesepe. Bilder 3: | " д] 957 25 20° Bilder 2—3. IE b 38 23 16 } | € 39 21 12 f=46.6. 1 а 43.222 14 e 42 23 16 р 43 24 18 73 | 163 | 1897 März 11 | 599.5 | — 9.0 — 12.0 —- | 1018 95 2” | 3 | Ргаевере. Bilder 3—4. a | 14 36 29 30° Bilder 3. b 37 57 26 k с 305112 24 f=46.6. ' 3 d AL, US 22 Die Zeit der letzten Aufn. ist | e 42 14 20 nicht verzeichn ; das hier |f “A (43 15?) |. 18 я agree Moment kann um ||. ; einige Sec. fehlerh. sein. ||! 74 | 167 | 1897 März 23 | 593.4 | — 6:7 — — | 9 10 50 2” | 3 |Praesepe. Bilder 2-3, | a 23:8 24° |: |Bilder 2. | 29 30 20 h : 30 42 16. —46.75. у 32080 20 | e 3% т 18 | f 34 17 14 75 | 168 | 1897 März 23 | — — — 90 — 1 90, 2760 2" | 3 |Praesepe. Bilder 1—2. | р т ee 16 28° Bilder 3. | | 54 42 В И |: 5 55 50 20 ]=46.75. } 57 о 20 р } е бт 18 | : F. 59 28 24 34 32 т 3 | Ргаезере. Bilder 3. 76 | 171 | 1897 März 27 | — pros A а Bilder 2—3. Nebel. | > oo ws . © — > D > 4 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. XV * 5 Thermometer S Е Mitte E 5 5 2. Dat А id Bi ЕЕ der Exposition. | € 5 = Biherk pe un. © 2.3| Pulkowaer 82 |= ar nn a = Е inneres. äusseres. |S2| Sternzeit. | Ta 9 = FA = A ‘le h m 5 5 1897 März 27 | — — —- b 9: 4) "17 20 3 6 4т 42 20 f—47.0. d 42 54 16 e 43 SI 22 f 44 53 18 8 | 1897 März 27 x — | 10 39 47 |ı"30'| 3 | Praesepe. Bilder 2. f=47.0. _| 1897 März 31 | — — 0,0 C. | a | 13 38 48 20° ‚ern 3. Windig. ah b 39 57 18 —47.8. с 40 56 16 Praesepeu. 4% sind an versch. d 42 6 16 Tagen aufg. worden, In 4. e 43 5 14 Zwischenz. war die Casset. L N #3 2 12 ann. Fe blieb die DB . у atte unber . 1897 April 2 | 582.9 | + то В. _ — | 10 12 58 2” | 3 |Praesepe. Bilder 2. alıo 35 7 18° br; 1—2. b 36 6 16 — 5 e ИЕ, 14 а | EU 14 e 39 2 12 F 40 3 10 1897 April 6 | 599.4 | + 2.0 — — | 10 18 10 2") 4 Pure а | 10 24 40 20 er 8. \ x b 25 41 18 ce 26 28 16 f=41.4. d 27 28 16 e 28 19 18 f 29 17 14 11897 April 7 | 602.4 | +- 1.0 — = 1997773 = 4 | Bilder 3. 395,59 т с 40 49 18 FAT. d 41 48 16 е 42 28 16 7 43 23 14, з — | 10 52 20 2 Praesepe. Bilder 3—4. 2 | 1897 April 9] — — + 4.0 — | 10 = 43 2, 3 | Praesepe. Bilder 4. eee 7% @ | 10 27 42 e re М b 28 45 16 Fe 4. Windig. с 29 41 16 —47.5. а 30 46 14 6 31 40 14 | Л 32 37 12 1897 April 10 | — — _ — | 10 4 49 2” 3 | Ргаевере. Bilder 3. бы adlro 9 28 2 Bilder = b 2,27 I —47.5 с 53 26 14 L а 54 23 12 . 5 e 55 13 12 К. F 56 4 10 | 1897 April 13 | — — = | 14 0.08 2" | 3 |Praesepe. | Е аи 17: 18 20 Bilder 3. Mond nahe. b 18 27 18 XVI F. Renz, Mitte der Exposition. Pulkowaer Sternzeit. Thermometer Bemerkungen. Aufnahme. inneres. äusseres. Diaphragma. Bezeichn. der Expositions- Fr] © = Fan | + 3 =) к: = = al = . © > 3 =] её a 188 | 1897 April 13 190 | 1897 April 15 | Ргаезере. Bilder 8. f=47.5. 191 | 1897 April 23 \ Praesepe. Bilder 3—4. Bilder 3. 41.4. Opposition 1898. Pulkowaer Clichés. o Mitte der Exposition.| : Pulkowaer Sternzeit. Thermometer Bemerkungen. inneres. äusseres. der Platte. Barometer. Bezeichn. der Aufnahme Expositions- Diaphragma. Pulk. lauf. 1 267 | 1598 März 16 Bilder 2—3, f=46.3. [Sos cs Coma Berenicis. Bilder 3. 270 | 1898 März 25 Bilder 2—3. f=46.7 [Sssasse ComaBerenicis. Bilder 2—3. 271 | 1898 März 26 | 603.7 | — 8.5 Bilder 2. S 8 ` PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. XVII | x 2 Е = mi n = MIS: 5 Thermometer = à Mitte я. E = Е © ЕЕ der Exposition. | 85 | # 2 À и Datum. Е Е Е PA == Е Bemerkungen. | 5 Е Е inneres. äusseres. 3 £| Sternzeit. cs Е lle ° о 1898 März 26 | 603.7 | — 35 В. | —120 C. | e | 11? 47” 22° 18° | 3 d 48 42 18 f—46.4. e 49 58 18 и а. 20 — | 11 56 51 40 Coma Berenicis. Bilder 2. 1898 März 27 | — = — 9.0 о 12:30 1,53 a 3 |Bilder 8. CT ME I с 34 6 18 f=46.5. d 35 10 18 e 36 12 18 f 37 23 20 ВЕ > — | 12 41 3 40 Coma Berenicis. Bilder 3. 1898 April 11 | 587.6 | — 1.1 — 1.6 a.| 11,19 9 20 3 |Bilder 2—3. b 20 26 18 Der Schatten eines Trabant. с она 18 ist am NW-Rande der Ju- а 22 50 18 f—47.2. [pitersch. sichtb. е 24 8 18 "2 25 19 20 — | 11 34 — 30 Coma Berenicis. Bilder 2, 1898 April 14 | 605.0 | — 3.2 — 5.0 а | 12 1 49 20 3 Bilder 2. b 2.58 18 Um 11” 59”tritt ein Trab, am с 4-20? 18? SW-Rande aus; auf der а 5.23 18 Scheibe ist sein Schatten р H so 18 f—=46.9. [sichtbar. 9 20 — | 12 15 19 40 Coma Berenicis. Bilder 2. | 1897 April 23 | 603.6 | + 1.0 — - 13 M + = 3 | ВИаег 2. с 49 9 20 а 50 19 20 —=47.3. е SI 49 20 Л 19 20 À: #8 — | 13 57 44 30 Coma Berenicis. Bilder 2. 1898 April 24 | 602.5 | -+ 2.0 + 3.0 а 12 $ 19 4 3 |Bilder 3—4. | 29 с 7.23 18 f=47.4. d $8 25 18 Die Bilder verschlechtern : 59 31 o sich schnell. 22:1 10 39 I — [13 7 30 40 Coma Berenicis. Bilder 4—5, 1898 April 25 | 598.6 — +5 а | ı2 ат 52 20 | 3 | ВИаег 3. b 43 10 20 Der Chron, war nicht mit der с 44 1413 20 Normalubr vergl. worden; а 45 20 20 / seine Corr. ist —0 angen. e 46 30 20 —47.5. f 47 50 20 — | 12 52 — 40 Coma Berenicis. 1898 April 28 | 597.8 | + 2.3 + 15 2 12, 16 54 = 3 |Bilder 8. У: из I с 18 6 16 XVII Е. Renz, 7] № der Platte. Mitte der Exposition. Pulkowaer Sternzeit. Thermometer Bemerkungen. я © = © = © >= LA FA inneres. äusseres. Bezeichn. der Aufnahme Expositions- Diaphragma. Pulk. lauf. № 1 95 | 283 | 1898 April 28 eu +23 R | +156. | à | 12% 19 6 | 16" | 3 (year; e рота 18 J 21 20 20 — | 12 27 14 40 Coma Berenicis. Bilder 3—4. 96 | 284 | 1898 April 29 | 599.5 | -+ 0.5 + 0.5 @ | м 32 16 20 3 | ВИаег 3—4. b 33 36 20 в 34 56 20 а 36 6 20 He e 37 16 20 if 38 36 20 — | 13 42 46 40 Coma Вегешс1з. Bilder 4. 97 | 285 | 1898 Mai 1 | 598.6 | -- 4.0 + 5,5 GRAS SNL PTT 21 3 | Bilder 2. b 12 26 20 с 13 40 20 а 15 16 20 1=47.5. e 16 40 20 f 17 50 20 — || 79.62% 80 40 Coma Berenicis. Bilder 2. 98 | 287 | 1898 Mai 2 | 598.4 | - 4.0 + 45 A 5. TO 20 3 | Mondschein. b 6 16 20 Bilder 3. € я. 12 20 а 8 222| 20 f=47.5. e 9 22 20 Der Chron. war nicht vergl. 23 10 16 20 worden; Corr. —0 angen. NE 1015 30 Coma Berenicis. Bilder 3. 99 | 288 | 1898 Mai 16 | — — + 9.0 @ |116 в 42 24 3 |Bilder 3—4. b 4 42 24 Leichte Wolken. e 5 42 24 f=41.1. а 6 42 24 e 7 36 24 f 8 48 24 — | 15 16 30 т Coma Berenicis. Bilder 3. 100| 289 | 1898 Mai 19 | 600.8 | + 7.8 10.0 ам 197.30 20' | 3 | ВИаег 3—4. b 12 17 22] Wind. Der Himmelsgrund ist с NT 24 sehr hell. d 14 22 24 71—11. е 15 31 22 ед 16 30 20 14 22 20 40 Coma Berenicis. Bilder 3. POsITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. XIX In obiger Zusammenstellung sind die besten Bilder mit 1, die schlechtesten mit 5 bezeichnet. f ist die Focaleinstellung. Die von Herrn Kostinsky benutzten Diaphragmen haben nachstehende freie Öffnungen: EU”, 27270 2357, — 210”, 511937". Um die Arbeit nicht übermässig anwachsen zu lassen, wurden auf den Pulkowaer Clichés des Jahres 1896 nur vier Bilder aus jeder Reihe gemessen; die ausgeschlossenen sind durch Sternchen bezeichnet. Ferner konnten nicht verwandt werden: Platte 28 Reihe C, weil die Anhaltsterne unterexponiert und alle Jupitersauf- » 34 wegen Beschädigung der Platte, [nahmen in AR verlängert sind, » 35 wegen Mangels an geeigneten Anhaltsternen, » 39 weil sie beim Einsetzen in den Rahmen zerbrach, » 68 weil sie durch den Mond geschwärzt ist. Der Bearbeitung unterlagen somit 70 Platten mit 121 Reihen oder 592 Einzelauf- nahmen. Alle Messungen sind in der früheren Weise an dem der Kaiserlichen Akademie der Wissenschaften gehörigen Repsold’schen Apparat ausgeführt worden mit Anbringung der im Jahre 1897 durch eine eingehende Untersuchung ermittelten Instrumentalcorreetionen. Die damals gefundenen Fehlerwerte wurden bis zum Schluss der Messungen als constant angenommen; eine im Sommer dieses Jahres zur Controlle vorgenommene Bestimmung der - Abweichung der Schlittenführung von der Geraden, bei der ich am leichtesten eine Verände- rung vermutete, gab innerhalb der Grenzen der wahrscheinlichen Fehler dieselben nume- rischen Beträge, wie die frühere. Der Bequemlichkeit der Rechnung wegen suchte ich das Objectiv des Mikroskops vor Inangriffnahme der Arbeit derart einzustellen, dass zwei Schraubengänge möglichst nahe einem Scalenteil entsprächen. Das gelang fast vollständig, wie aus folgender Zusammenstellung ersichtlich: 1 Scalenteil=Schraubenrev. Temp. Platte. 1 Scalenteil—Schraubenrev. Temp. Platte 1897 Oct. 2 270011 — 36 1897 Nov. 15 270004 <+14.4R. 44 5 2.0010 <+13.2R. 37 19 2.0001 —+-15.4 45 12 2.0007 -+14.6 38 Dec. 9 2.0008 -+12.0 46 16 2.0011 — 40 24 2.0004 --14.0 47 20 2.0011 -+16.0 41 28 2.0006 <+14.0 48 Nov. 4 2.0012 -+15.6 43 1898 Еег.14 2.0003 <+13.0 49 9 2.0006 — 42 19 2.0003 —+-14.6 50 ш* XX Е. Rexz, 1 Scalenteil—Schraubenrev. Temp. Platte. 1 Scalenteil—Schraubenrev. Temp. Platte. 1898 Febr.26 179999 <+14.5R. 51 1898 Пес. — 1:9993 <+14.6R. 32 März 3 2.0010 — 52“ 1899 Jan. 26 1.9999 +15.1 33 — 2.0008 -+15.3 54 Febr. 6 1.9989 -+14,3 67—70 — 2.0006 15.6 59? 16:1 UI, 10 И 79 26 2.0006 -+-16.9 53 — 1.9992 +17.5 73—75 April 1 2.0003 —+-12.9 55 März 18 1.9996 <+15.0 76—78 4 2.0008 <+14.6 56 April 1 1.9995 <+14.6 79—81 8 2.0008 —+15.0 57 22 1.9994 -+-15.5 82,63,83 27 2.0008 +13.6 58 Juli 24 1.9995 <+19.4 64 Mai 10 2.0005 -+-15.0 59 — 2.0001 -—-14.5 65 14 2.0009 <+14.3 60 — 2.0003 -+16.2 84, 85 Juni — 2.0006 -+14.2° 61, 62 — 1.9995 -+14.5 66 25 2.0003 <+17.5 28 — 21.9995 -+14.4 86—88 Juli 2 2.0002 <+17.8 294 Oct. 7 1.9997 —<+14.0 89—91 Sept. 7 2.0009 <+15.5 29B,C,D 28 1.9997 —+-14.1 92—96 26 2.0006 -+12.8 30 Nov. 15 2.0003 —+14.1 97—100 Oct. — 2.0000 <+14.3 31 Im Laufe der Zeit ist eine unbedeutende Abnahme des Verhältnisses te а bemerkbar; eine Abhängigkeit von der Temperatur lässt sich wegen ihrer geringen Schwan- kungen ail nachweisen. Die Berechnung der Messungen wurde nach den im n ersten Bande Seite 19—21 gege- benen Formeln?) ausgeführt, auf die ich auch wegen der Bedeutung der im weiteren Text vorkommenden Buchstaben und Bezeichnungen verweise. Zur Bestimmung der Plattenconstanten (des Scalenwerts f,, f, und des Winkels ö,, 4, den der Meridian des Centrums resp. die Tangente an den Parallel mit der Schlittenführung des Apparats bilden) ist auf den Helsingforser Negativen von 1896 und den Pulkowaer von 1896 und 1897 kurz vor oder gleich nach den Jupitersaufnahmen die Praesepe photographiert worden, während der Sternhaufen in der Coma Berenicis zu dem gleichen Zwecke von Prof. Donner während der Opposition 1897 und von Herrn Kostinsky im Jahre 1898 benutzt wurde. Die Positionen der Anhaltsterne in der Praesepe entnahm ich den Göttinger Astronomischen Mitteilungen, Teil IV, mit Berücksichtigung der von Prof. Schur aus der Vergleichung seiner Messungen mit den Bonner abgeleiteten Eigenbewegungen. Während 1) Durch ein Versehen bei der Abschrift des Manuskripts ist in der Refractionscorrection dx das К in die Klammer gesetzt, die Formeln auf Seite 21 müssen demnach lauten: Es cotg?n cotgn cos(N-+-28,) u cotg?n dx = K sin?(N-+8,) ww 1] 2—К cos 5 вш? (№5,) " y und Г «= at À Ge ce 1) POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. XXI ich mit diesen Rechnungen beschäftigt war, veröffentlichte Herr Е. Schlesinger die Resultate seiner Bearbeitung der Rutherfurd’schen Aufnahmen der Praesepe'). Wenngleich die photo- graphischen Positionen die Heliometermessungen in Göttingen unzweifelhaft an Genauigkeit übertreffen, schien es mir doch nicht zweckmässig, erstere meinen Reductionen zu Grunde zu legen, da ihre Epoche über zwanzig Jahr zurückliegt. Nachstehend sind die Positionen der zur Verwendung kommenden Sterne nach Schur und Schlesinger (Е. В. nach Schur) nebeneinandergestellt: Bezeichn. des Sterns. « 1896.0. 5 1896.0 № п. Schur. — Göttinger Heliometer. Ruth. Göttinger Heliometer. Ruth. 2 N 8" 31” 38:307 38:309 +20° 5 42/23 41.79 4 R 31 49.118 49.100 +19 37 47.23 46.50 15 Z 33 44.169 44.177 +20 8 41.34 40.82 17 и, 33 52.752 52.736 +19 54 26.49 25.79 *) 20 У 33 59.820 59.818 +19 54 29.73 29.09 23 X 34 12.612 12.618 +20 20 18.43 17.643) 26 |. 34 22.667 22.653 —=19 42 59.57 58.88 27 5 34 23.934 23.928 —20 2 15.39 14.52 29 W 34 27.467 27.503 +20 32 59.22 58.49 31 у 34 29.137 29.136 —=19 54 45.48 44.68 34 М 34 45.012 45.008 +20 5 15.61 14.67 37 T 34 58.414 58.418 +19 56 56.56 55.88 40 Q 35 21.247 21.241 +19 37 49.60 49.03 Die fast auf demselben Parallele sich befindenden Sternpaare M, N und ©, В dienten zur Ableitung des Scalenwerts in AR und des Winkels $ in Declination, während V und W, da sie nahezu in der Richtung des Meridians liegen, sich zur Ermittelung des Scalenwerts in Declination und des Winkels 2, eignen. Auf allen Helsingforser Clichés von 1896 und den Pul- kowaer von 1897 bezeichnet der Stern 5 den Mittelpunkt der Platte; während der Opposition 1896 dagegen hatte Herr Kostinsky den Stern des Centrums häufig gewechselt, so dass nach einander М, 5, T, Г’, Z, U, X, У diesen Platz einnehmen. Die beiden Sternbögen M N und Q В geben einen um 0.00021 von einander abweichenden Scalenwert. Bei Benutzung der Schlesinger’schen photographischen Positionen wird dieser Unterschied auf 0.00011 herabgesetzt, die Mittel aus beiden Systemen stimmen dagegen bis auf wenige Einheiten der fünften Stelle überein. Eine starke Differenz (0.00023) ergiebt sich für den Winkel &,, jenachdem man ihn aus den Göttinger oder den photographischen Sternörtern ableitet, doch 1) The Praesepe Group; Measurement and reduction 2) Ruth.-+ 10”. of the Rutherfurd photographs by Frank Schle- 3) Ruth. — 10’ zu corrigieren. singer, New-York 1898. XXII К. Вами, ist dieser Unterschied von geringerer Bedeutung, da 4, mit einem Factor multipliciert wird, der im Maximum 0.5 des Coefficienten von f, beträgt. f, (Gött.) — f, (Ruth.) finde ich — +0.00001; à, (Gött.) — à, (Ruth) = -+0.00006. Zur Berechnung der mit dem Sternhaufen Comae Berenicis versehenen Platten wurden zunächst die Heliometermessungen von Chase am Yale Observatory !) verwandt, welche für 1897.0 folgende Positionen der Anhaltsterne geben: | № Yale. Bezeichn. des Sterns. о 1897.0. à 1897.0. 3 0 12” 13” 50°463 +26° 34° 49759 5 Е 15 1.51 +26 34 22.44 d J 17 "1927 +26 25 3.30 18 I 18 53.329 +26 25 20,35 19 K 19 8.742 +26 40 10.70 20 L 19 16.676 +26 9 12.84 24 H 22029021 +26 28 56.17 Den Mittelpunkt der Platte markiert bei Prof. Donner der Stern I, bei Herrn Kostinsky J. Den Scalenwert in AR und den Winkel #, geben auf den Helsingforser Clichés die Sternbögen IF und JH, auf den Pulkowaer der Bogen О J; f, und i, wurden gefunden aus dem Sternpaar К L. Zwischen dem aus den beiden Sternbögen ermittelten Scalenwert in № zeigte sich eine so beträchtliche Abweichung (0.0006), dass ich mich genötigt sah, die Rectascensionsunterschiede der Sterne О, I, Е, J, H am hiesigen Passageninstrumente von neuem zu bestimmen. Als Mittel aus sechs Abenden erhielt ich: Au 1897.0 Pulk. Ах 1897.0 Yale. 0— I= —75 43/39 42"99 F—-I—= —56 27.06 25.77 J—I— —23 92494 24.03 Н—Т = +53 59.70 59.83 Die in Pulkowa beobachteten Ax ergeben nur einen Unterschied f, (FD—-f, (HJ)= —0.00002. Demnach muss der Stern F eine jährliche relative Eigenbewegung von etwa —0"15 besitzen oder aber die am Yale-Heliometer bestimmte Position um beiläufig 1” fehler- haft sein?). 1) Transactions of the Astronomical Observatory of | bestätigt, während die andern hier benutzten Sterne nur Yale University, Vol. I. Part V. 1896. eine dem ganzen System zukommende Fortrückung auf- 2) Durch die während des Druckes dieser Abhand- | weisen. Berücksichtigt man diese E. B. bei Berechnung lung erschienene Broschüre von Walter Kretz: The | der Rectascensionsdifferenz F—I, so erhält man für die positions and proper motions ofthe principal stars in the | Helsingforser Aufnahmen des Jahres 1897 einen um cluster of Coma Berenicis, New-York 1900, wird das Vor- | 0.00006 kleineren Scalenwert LE handensein einer Е. В. von obigem Betrage bei Stern F POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. xxıu Der Scalenwert berechnet sich für die Helsingforser Platten, wie folgt: 1896. 1897. Platte. Scalenwert (Æ). Temp. Platte. Scalenwert (AR). Temp. 28А 0.99808 x HR 634 0.99796 En UE. B 0.99804 к Ва В 0.99794 Be D 0.99787 —= 30 C 0.99773 Bag er À 294 ° 0.99817 ив D 0.99777 03 B 0.99796 VE 644 0.99778 + 2,5 С 0.99796 7 B 0.99776 ER D 0.99800 — 2.3 Ö 0.99777 + 4.65 304 Оо ^^ — 83 D 0.99779 + 5.8 B 0.99789 1 654 0.99773 + 84 C 090797 — 58 B 0.99770 + 5.5 D 0.99796 8 C 0.99767 + 6.5 314 0.99784 = 14 D 0.99766 я В Baar: 10 664 0.99777 +14.6 С 0.99784 | B 0.99767 +10.5 Bes. — 2%, C 0.99774 +14.6 32А 0.99796 _ 95 D 0.99765 +-10.6 PR er, —,50 Mittel: 0.99776 С ° 0.99805 BG i nen‘. 0.99802 gr N. 33А 0.99795 94 вы к 0.99800 ° -+ 1.5 Mittel: 0.99797 Eine Abhängigkeit des f von der Temperatur ist nicht nachweisbar. Eigentümlich ist _ deutlicher in die Augen fällt, wenn man die entsprechenden Beträge für die früheren Oppo- _sitionen danebenstellt. Es war: р, 1891 = 0.99808 f, 1894/5 = 0.99801 1892/3 = 0.98807 1896 =0.99797 1893/4 = 0.99802 1897 —0.99776 XXIV Е. Renz, Wie H. Prof. Donner mir mitteilt, ist gleichzeitig eine fortschreitende Änderung der Focallänge an seinem Instrumente constatiert worden, woraus sich schliessen lässt, dass die Krümmung der Linse mit der Zeit abnimmt. Der Scalenwert der Pulkowaer Platten ist unzweifelhaft eine Function der Temperatur (resp. der Focaleinstellung). Es wurde gefunden: Platte. A Focus. Temp. beobachtet. 7 berechnet. 36 0.99298 0.99295 —0.00003 46.5 —12°0 В. 37 0.99294 0.99298 == 4 46.4 ee 38 0.99287 0.99292 a 5 46.6 u 6 40 0.99296 0.99301 а 5 463), 41 0.99290 0.99295 = 5 46.5 = 64 49 0.99278 0.99280 a 2 47.0 -— 9.8 43 0.99293 0.99295 =, 2 46.5 = 075 44 0.99276 0.99277 = 1 47.1 — 13 45 0.99297 0.99298 = 1 46442211 46 0.99296 0.99289 7 46.7 — 5.8 47 0.99288 0.99298 =: 10 46.4 > 48 0.99305 0.99298 + 7 464. 10:8 49 0.99301 0.99298 + 3 46.4 В 50 0.99286 0.99289 "= 3 46.7 2 640 51 [0.99294] 0.99289 Е 5 467. та 52% 0.99280 0.99280 0 47.0 Her 52? 0.99281 0.99280 u 1 47.0 EU 4 53 0.99291 0.99288 + 8 46.9 4! 46 54 0.99289 0.99289 0 46.7 = 8.0 55 0.99273 0.99274 = 1 47.2 0.0 56 0.99298 0.99289 ei 9 46.7 u. 57 0.99297 0.99292 Lai 5 46.6 ua 58 0.99292 0.98290 + 2 466501020510 59 0.99257 0.99268 des 11 47.4 0.0 60 0.99274 0.99268 + 6 47.4 4.0.5 61 0.99259 0.99265 a 6 47.5 + 3.1 62 0.99264 0.99270 — 6 47.4 = 1896 Mittel: 0.99286 46.78 Розичомек DER J UPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN, Platte. Be 67 69 70 71 72 72. 74 75’ 76 m 78 79 80 81 ER.» 88 DEN, 54 Me 65 897 Mittel: er + ze + Ce 22] в - $ beobachtet. 0.99291 0.99287 0.99296 0.99299 0.99289 0.99288 0.99296 0.99296 0.99288 0.99281 0.99264 0.99277 0.99270 0.99266 0.99265 0.99265 0.99265 0.99270 0.99281 0.99290 0.99282 0.99289 0.99276 0.99258 0.99270 0.99256 0.99251 0.99249 9.99254 0.99258 0.99251 0.99251 `` 0.99240 Л berechnet. 0.99299 0.99299 0.99290 0.99296 0.99293 0.99293 0.99288 0.99288 0.99281 0.99281 0.99272 0.99269 0.99275 0.99266 0.99266. 9.99269 0.99266 0.99269. 0.99288 0.99276 0.99285 0.99281 0.99261 0.99269 0.99258 0.00254 0.99252 0.99254 0.99258 ' 0.99252 0.99252 0.99246 0.99246 _ А —0.00008 — 12 + 6 +- 3 —- 4 — 5 + 8 + 8 + 7 0 — 8 + 8 — 5 0 -- 1 —- 4 — 1 — a +-0.00002 + 6 + 4 — 5 — 3 + 1 — 2 — 3 — 3 0 0 — 1 == $? ЕЕ: 6 +- 2 Focus, 46,4 46.4 46.7 46.5 46.6 46.6 46.75 46.75 47.0 47.0 47.3 47.4 47.2 47.5 47.5? 47.4 47.5 47.4 47.00 1463 46,7 46.4 46.5 47.2 46.9 47.3 47.4 47.5 47.4 47.3 47.5 - 47.5 47.7 47.7 47,15 Temp. —14?0 В. — 160 — 8.0 — 7.0 — 9.0 +5657 XXI Е. Renz, Die merkliche Abweichung des Scalenwerts von der Einheit beim Pulkowaer photo- graphischen Fernrohr hat den Übelstand im Gefolge, dass in den Correctionsgrüssen der Reductionsformeln x und y teilweise durch f,x und f,y ersetzt werden müssen. Sucht man f, durch die Formel 0.99286-+0.00003ж(46.78—Р) für 1896 und 1897 und durch 0.99267-+0.00003%x(47.00—F) für 1898 darzustellen, so bleiben die unter A gegebenen Differenzen zwischen Beobachtung und Rechnung übrig. Die Abnahme des f, in der letzten Opposition liegt wol kaum am Instrumente, wie in Helsingfors, vielmehr vermute ich, dass sie auf systematischen Fehlern in der Distanz der Anhaltsterne beruht. Überhaupt würde die photographische Ortsbestimmung bei der vorliegenden Arbeit noch bedeutend mehr zu leisten imstande sein, wenn nicht die ungenügende Genauigkeit der Positionen der An- haltsterne ihr eine Grenze setzte. Als Unterschied f,—f, ergiebt sich: Helsingfors 1896: —0.00003 1897: —0.00021 Pulkowa 1896: 0.00002 1897: —-+0.00005 1898: —0.00004 Eigenthümlich ist die grosse Abweichung für Helsingfors 1897, die sich nicht durch Fehler in den Positionen der Anhaltsterne erklären lässt, da im Jahre 1898 in Pulkowa dieselben Sterne benutzt worden sind !). Dem Einfluss der Phase auf photographierte Planetenscheiben wurde eine besondere Untersuchung gewidmet. Nach einer von Herrn Kostinsky gelegentlich mit verschiedenen Expositionszeiten gemachten Aufnahme der Venus glaubte ich schliessen zu müssen, dass die theoretisch berechnete Phase in der Photographie keine Giltigkeit habe, dass vielmehr an der Lichtgrenze eine andere Irradiation wirke, als am voll beleuchteten Rande. Bezeichnen wir den Aequatorial- und Polardurchmesser des Jupiter, ihren Zuwachs infolge der Irradiation und den Abstand des Jupiter von der Erde zur Zeit der Opposition und Quadratur mit 4 und b, resp. a und $’, 2 und 2’, р und р, und die Phase mit р, so muss, wenn z und z in allen Radien denselben Betrag hat, die Relation bestehen: a—b= (db +p) oder p— 2a) — (a —0). Aus vielfachen Messungen?) leidlich gut begrenzter Jupitersbilder, die in der Nähe 1) Durch Einführung der nach Seite ххи Anm. 2 Abplattung = dem Stern F zukommenden Е. В. wird dieser Wert auf -+0.00015 herabgesetzt. 2) Unter Annahme eines Polardurchmessers —182/20 für die Entfernung 1 folgt aus diesen Messungen eine ee die aber jedenfalls zu stark ist, da der Aequatorialdurchmesser des Jupiter auf den Platten häufig durch Unregelmässigkeiten im Gange des Uhr- werks vergrössert erscheint, POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. XXVII der Opposition und zur Zeit der maximalen Phase aufgenommen waren, wurde der Wert von p empirisch gefunden: Phase À Platte, gem. nach Math. A | 56 0/19 0"32 +-0"13 57 0.42 0.32 —0.10 58 0.43. 0.33 —0.10 i 59 0.18 0.35 +0,17 60 0.46 0.35 — 0.11 61 0.45 0.35 — 0.08 62 0.39 0.35 —0.04 Mittel: 0.36 #0!03 0.34 №. | Dis Übereinstimmung mit der Ephemeride von Marth ist bei der Schwierigkeit der N essungen fast als vollständig zu betrachten, folglich kann die theoretisch berechnete Phase ol hne Bedenken auf photographische Aufnahmen der Planetenscheiben angewandt werden. Für die x und y wurde die Phasencorrection mit Vernachlässigung der Abplattung ermittelt nach Ben Formeln: Corr. in &,-,, = —?% sin ?Q » » У; = —2/ cos ni er der Astrographen erhalten habe, sondern nur die Versicherung, dass dieselben, soweit À tunlich, beseitigt waren. Da der Unterschied des иона zwischen dem Jupiter | iel hen zu müssen, wurden nur ‘dires dazu re die in der Nähe der Elongation _ stand PT; d ххуш Е. Renz, POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Wahrscheinliche Fehler der Messungen. in № in Decl. RER RE CR Re Aa Ge Opposition. | Trabant—Jupiter | Trabant— Trabant | Trabant— Jupiter | Trabant — Trabant 5 des Jupiter. Einzel- Einzel- | 31.7 | ре: |, mel | differenz. | Mittel. Mittel. Mittel. Mittel. differenz. differenz. differenz. Helsingforser Platten. +o/119 | #0.053 ME 0.118 = 0.092 | 0.041 | ==0.174 | = 0.078 | = 0,072 11. Pulkowaer Platten. =0:081 | 0.040 | ==о.100 | =0/050 | # 0.076 =.0.067 | 0.027 | = 0.097 | 0.040 | = 0.082 0.084 | 0.034 | =# 0.116 | =0.047 | = 0.088 Die Zusammenstellung der Messungen ist im Allgemeinen ebenso angeordnet, wie im ersten Bande, nur sind die Colonnen x 0°, æ180° und 490°, y270° fortgelassen, da sich keine systematischen Unterschiede zwischen den Messungen der Aufnahmen а, 6, с und d,e,f gezeigt haben, und ist unter der Überschrift Trabant — Jupiterscentrum noch die mit Ph. bezeichnete Correction wegen Phase hinzugekommen. In die am Schluss gegebenen definitiven Positionen der Trabanten sind die wegen Phase corrigierten Oerter aus den früheren Oppositionen mit aufgenommen. Wie bei der Bearbeitung des ersten Bandes, so hat sich auch jetzt wieder meine Schwester in dankenswerter Weise an den Controllrechnungen beteiligt. 2 à Е. Renz. Pulkowa, September 1900. HI ZUSAMMENSTELLUNG DER MESSUNGEN. à: OPPOSTTION 1896. dE . HELSINGF ORSER CLICHES, 2 F. Renz, 25 A. 1895. November 27. № | Scalenablesung. Helsingforser Sternzeit. Object. Bilder. P -Kr. 0° |t+-k| P.-Kr.180° |t-+# der Aufnahmen, | Mittel. 1 .- _mm_ mm_|_mm Fe 1000 и 10000] 10000 En Ir Ctr, | 66.5109 61.8762 я 66.5100 |= 9| 61.8753 |+ 9 oO 0.0000 4 М | 71.4553 [+14] 56.9208 |+10| о] -+ 4.9501 3—4 М 27.5600 |-+23| 100.8240 |-+ 4|-+18] — 38.9466 о 5 Q 80.0165 |-+19| 48.3692 |+-19|— 3|+13.5060 >» 17 50 4—5 у В 29.9852 |+-29| 98.3912 |+ 8]-+21| —36.5172 4—5 ellipt. | y 66.2000 |-+18| 62.1725 |+15| ©] — 0.3034 3 ‚. т 67.3490 |+20| 61.0342 |+26]| о] -н 0.8398 4—5 ищегехр. %а | 55.5105 |+ 2| 72.8900 |+16 — 11.0078 Ag 55.9165 |+ 2| 72.4850 |+14 — 10.6022 — 10.6035 И Я) 4—5*) Ag 56.3120 |+ 2| 72.0770 |+-14 — 10.2004 1%6, | 55.4900 + 2| 72.9130 |-+-15 — 11.0295 be 55.8970 | 2! 72.5020 |+15 — 10.6205 — 10,6250 24 54 4—5 b, 56.2915 | 2] 72.1055 |+13 —10.2249 20 55.5155 |+ 1| 72.8825 |+14 — 11.0015 се 55.9155 |+ 1| 72.4895 |+-12 — 10.6049 — 10.6038 Eile 5 2270008 3—4 En 56.3140 |= ı| 72.0880 |+12 — 10.2049 dw | 55-4965 |+ 72.9055 |+14 — 11.0225 de 55.9045 + 1| 72.5010 |+14 — 10.6162 — 10.6190 22 +03 3—4 | do 56.2990 |+ 1| 72.1000 |+12 — 10.2184 %ew 55.4820 0| 72.9185 |-+13 — 11.0362 n CA 55.8905 O| 72.5170 |+13 — 10.6312 — 10.6329 22 1.8 Е 3—4 Gr 56.2935 ©] 72.1200 |+11 — 10.2312 Trabant — Jupiterscentrum. | j ty | Mittel. ага) Тиби) Ph. | Да cos 5 | тт mm Та | 56.9070 |+12| 71.4670 |+15 — 9.5975| 1.0060 3 b | 56.8865 |-+12| 71.4840 |-+14 — 9.6162] 1.0088 9—3 с | 56.9080 |+11| 71.4685 |+13 — 9.5977| 1.0061 | -+1.0068 | <+1:0053 | -+0:0004 | -+0:0025 | +1:0082 | 2—3 d | 56.8910 +10] 71.4820 |-+13 — 9.6130] +1.0060 2 е 56.8770 |+10| 71.4940 |+12 — 9.6260) -+1.0069 93 Па | 57.8480 |+ 8| 70.5315 |+15 — 8.65941 —+1.9441 3 b 57.8260 + 8| 70.5475 |+14 — 8.6784| +1.9466 2—3 в | 57.8470 |+ 7| 70.5290 |+13 — 8.6586] -+1.9452 | -+1.9451| -+1.9421 | +-0.0008 | -+0.0025 | -+1,9454 | 2—3 а | 57.8310 |+ 6| 70.5440 |+13 — 8.6742] 1.9448 ' 9—3 e | 57.8170 [+ 6| 70.5580 |-+12 — 8.6882] +1.9447 3 Ша | 60.6970 I+-13) 67.6740 |+20 — 5.8062| -+4.7973 2—8 6 | 60.6790 |-+12| 67.6950 |+19 — 5.8257| 4.7993 2—3 с | 60.6985 |+11| 67.6750 |+19 — 5.8060] -+4.7978 | +4.7967 | -+4.7894 | -+0.0020 | -+0.0025 | +4,7939 | 2—3 4 | 60.6780 |+11| 67.6930 |-+-18 — 5.8252| +4.7938 2 е | 60.6660 11| 67.7060 |-+18 — 5.8377| -+4.7952 2 ТУ а | 47.1590 |-+12| 81.2180 |+19 —19.3470| —8.7435 3—4 b | 47.1400 |+-ı1) 81.2380 |+18 — 19.3665] —8.7415 3 e | 47.1570 +11] 81.2185 |-+17 — 19.3482] —8.7444 | —8.7446 | —8.7313 | —0.0036 | -+0.0025 | — 8.7324 | 3 d | 47.1375 |-ı1]l 81.2390 |+16 — 19.3682] —8.7492 9 e | 47.1300 |-10| 81.2500 |-+15 —19.3774| —8.7445 3 Scheinbare Rdiff: M— Centrum = + 5:2688 F4 = 999847 — 1° „= —0.00029 N— » — — 41.4028 Q— » = -+14.3257 Га = 0.99808 —iy =— 0.00015 X 1, =- 05 В > = —38.7017 Refr. = — 18 | У и = — 0.3175 Те, =— 103 \— » — + 0.8843 Го —0.99848 x = 0.00136 h m ay =8 46.9 | *) Alle Jupitersbilder sind von einer grossen Aureole umgeben, so dass die Ränder schwer erkennbar sind. уе 4 *: 1h ine. \ 7 _ Scalenablesung. „Кг. 90°] (--A|P.-Rr. 270° En 63.7437 62.2878 59.2802 58.7613 86.7335 86.7243 81.5663 51.5113 54.6120 54.9845 55.3600 56.0700 56.4500 56.8170 57.5905 57.9635 58.3395 58.9035 59.2740 ^ 59.6320 60.4330 60.7950 61.1750 55-2585 56.7165 58.2290 59.5340 61.0680 55.5860 52.3150 53-7735 55.2920 56.5910 58.1260 t+k 1895. November 27. einbare Decldif: М— Centrum + 30030 ==-+ 3.4488 = —24.4283 = —24.4657 = —19.2618 =-+30.7278 dy = +-18° 27:8 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. — — - Пес]. 2 -% 2 2 u | — 195 sin 1’ | mm | mm | 0.0000 — 0.0013 — 0.0806 — 0.0094 — 0.0690 0.0000 0.0000 + 8.7660 + 7.3052 + 5.7875 + 4.4807 + 2.9487 ve | Mittel. mm mm —0.2817 —0.2812 —0.2766 | —0.2780 —0.2737 —0.2769 —0.6102 —0.6057 —0.6081 | —0.6074 — 0.6067 —0.6062 —1.4912 —1.4890 —1.4913 | —1.4899 — 1.4905 —1.4875 -+2.6622 2.6668 | -+2.6661 | -+2.6671 —+-2.6713 —-2.6693 J?a = 0.99866 fs =0.99799 l'a — 0.99572 Trabant — Jupiterscentrum. 1 et | 8 (Уе'- Уз) | Ts (&—%2) Нева —0/2776 —0:0003 —0.6066 | —0.0005 — 1.4880 —0.0013 2.6637 | -+0.0024 $73 = —0.00024 iz == -+0.00003 Js = —0.00028 у x? . , —5 96 sin 1 mm + 1.4552 —+ 4.4603 + 4.9028 — 22.9970 —23.0535 — 17.8250 +-32.2319 +-0/0010 | —0/0002 —+0.0018 | —0.0002 -+0.0039 | —0.0002 —0.0127 | -+0.0002 x 34 =-н 0!1 Bemerkungen zur Aufnahme. an —0:2771 —0.6055 —1,4856 -+2.6532 ы bd + ы — -ч SIR саосо DA SD 6 LS AR Scalenablesung. Е; Renz, 1895. November 28. № Р.-Кг. 0° | + mm 66.6168 66.6160 71.5688 27.6683 80.1360 30.0937 66.3150 67.4545 56.4710 56.8885 57.2890 56.4760 56.8700 57.2530 56.4830 56.8710 57.2625 56.4810 56.8865 57.2850 56.4590 56.8520 57-2460 55.1115 55.0945 55.1095 55.1085 55-0865 59.4235 59-3990 59.4135 59.4120 59.3870 60.7885 60.7610 60.7775 60.7780 60.7530 48.5500 48.5315 48.5415 48.5430 48.5255 Scheinbare №4: M— Centrum = + 5.2688 mm 10000 + 8 4-12 +22 +20 +30 +19 —=20 SN + 9 a ЕЕ + о © Une 4-10) 10 —-10 —= го +10 —+10 P.-Kr.180° mm 61.7609 62.7600 56,8095 101.7063 48.2482 98.2802 62.6595 60.9255 71.9265 71.5165 71.1070 71.9200 71.5320 71.1480 71.9135 71.5320 71.1355 71.9215 71.5120 FAST 71.9450 71.5525 71.1420 73.2645 73.2885 73-2755 73-2770 73.2930 68.9500 68.9755 68.9640 68.9630 68.9885 67.5850 67.6130 67.6020 67.6000 67.6230 79.8300 79.8510 79.8405 79-8445 79.8575 t+-h mm mm 10000! 10000! mm 9 о 0.0000 9 o|+ 4.9518 + 3]-+17| —38.9443 +28|— 3|-+13.5152 +- 9|-+-20] —36.5182 —=1$] 0] — 0.3000 26] о] -н 0.8362 +12 — 10.1558 +12 — 9.7421 : +13 — 9.3372 +12 — 10.1501 +12 — 9.7591 +13 — 9.3756 +12 — 10.1434 +12 — 9.7586 +13 — 9.3636 13| | —10.1484 +13 — 9.7408 +14 — 9.3414 +14] ' — 10.1712 +14 — 9.7784 HIS — 9.3762 or Bo +2 0 3 mm 9-7450 9.7616 9.7552 9.7435 9.7753 der Aufnahmen. 5° 58”. 34° 2 49 32 м Helsingforser Sternzeit. Mittel. Trabant — Jupiterscentrum. Tt—Ly | Mittel. | би) и] Ph, | Aa cos d mm mm 4-13 —11.5052] —1.7602 +14 —11.5257| —1.7641 +-14 —11.5117| —1.7565 | —1.7614| —17586 | —0!0006 | +0.0025 —14 —11.5129] — 1.7694 HIS —11.5320| —1.7567 +14 — 7.1914] +2.5536 +14 — 7.2164] +2.5452 —15 — 7.2034] +2.5518 | 2.5474 | —+2.5433 | -+0.00I0 | -+0.0025 HIS — 7.2036] +2.5309 —16 — 7.2289] 2.5464 —19 — 5.8266] 3.9184 —19 — 5.8544] +3.9072 —-20 — 5.8406] 3.9146 | 3.9112 | 3.9050 | —-0.0014 | 0.0025 +-20 — 5.8394] -3.9041 +21 — 5.8634] +3.9119 + 8|-+ 2] — 18.0674] — 8.3224 + 8]-= 2| — 18.0872) —8.3256 + 9|-= 2] —18.0770| —8.3218 | — 8.3246 | —8.3113 | —0.0029 | -+0.0025 + 9]+ 2| — 18.0783] — 8.3348 i + 9]+ 2| —18.0935| —8.3182 F° à = 0.99838 —i°, = —0.00015 N— » — — 41.4028 Q— » =+143257 Л» = 9.99804 —iy =— 0.00006 R—- » — —38.7017 Refr: =— 12 V— м. 1=— 03175 I) RO W— » — + 0.8843 1’. = 0.998410 7. = — 9.00113 В, и, =8 46.8 | Bilder,) я | #| Starke Aureole um den 2—3 2 —1:7567 | 2—3 3 2—3 2 1-7 +-2,5468 | 2—3 h 3 2—3 2—3 | 2—3 Plattezi + 39089 | 2—3 D | } 3 2 3 2—3 — 8,3117 | 2—3 3—4 2—3 X $, = 0.2 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. о | 1295. November 25. 1 | 9. Пес]. E Scalenablesung. TE 2 2 Bemerkungen — 5 у т име. — —tg8 sin 1’ y — > tgù sin 1’ x | 909] + P.-Kr. 270° |++X zur Aufnahme, т тт т т 63.7437 Р £. 63.7428 0.0000 0.0000 68.7298 — 0.0013 +. 3.0065 60.2130 -— 0.0806 + 3.4470 88.1940 — 0.0094 —24.4585 88.1765 — 0.0690 —24.5070 83.0232 0.0000 —19.2856 32.9695 0.0000 +-30.7718 65.0200 65.3830 — 1.6348 65.7565 66.5350 _ 66.9040 — 3.1498 67.2485 67.9845. 68.3495 — 4.5957 68.7060 69.4260 69.8100 — 6.0580 70.1860 70.8940 71.2590 — 7.STI10 71.6310 Trabant — Jupiterscentrum. Е т Уг— Уз | Mittel. Ira eva) 7 (r—2)|-(rrt-223) т Ph. | 43 mm mm 64.8210 0,5550 66.3340 0.5583 = | 4 67.7815 —50.5556 | 0.5544 | 0.5337 | +0/0004 | —0'0018 | —0'0002 | +0'5591 69.2510 40.5489 70.6985 - +-0.5 540 66.2140 —0.8427 67.7310 —0.8406 - ‘69.1850 " —0.8467 | —0.8438 | —0.8427 | —0.0006 | -+0.0021 | —o.0002 | —0,8414 70.6440 —0.8483 7e 72.0900 —0.8406 о! 66.6400 —1.2680 - 68.1460 — 1.2603 69.6020 —1.2690 | —1.2653 | —1.2637 | —0.0008 #0.0029 | —0.0002 | —1,2618 71.0635 — 1.2683 72.5095 — 1.2608 62.7955 —+-2.5796 64.3100 +-2.5802 65.7600 : 2.5771 | 2.5771 | 2.5738 | -+0.0017 | —0.0113 | —0.0002 |. +-2,5640 67.2320 +-2.5704 | 68.6750 2.5783 е Deeldif: M-—-Centrum 198 = 0.99865 125 = —0.00018 N— » hy 2 » fs = 0.99807 13 = 0.00001 X ig—= 00 à V— » J'a = 0.99873 Уз = —0.00020 - W— » à dy = -+18° 28/1 < À 1* К. Renz, 28 D. 1896. Januar 11. № Scalenablesung. Helsinglorser Sternzeit Object. Bar © ur Foren Bilder. | P.-Kr. 0° |+ Р.-Кт.180°] +5 n der Aufnahmen. Mittel. | mm р | mm 10000 mm mm тт à | Cir, | 66.6078 61.7865 | S 66.6070 |+ 8| 61.7855 3 unterexp. | M 71.5585 |+11| 56.8265 — РМ 27.6458 |+-22] 100.7390 и Schimmer = 110 80.1318 |-+-21| 48.2612 Ч м Schwacher Schit! Der 30.0805 |-31| 98.3070 3—4 У 66.3128 |-+2!| 62.0775 2—3 W | Nicht silchtblar. зав | 75.4992 |+ 7| 52.9140 Ag 75.9160 | 7| 52.4740 + 9.3088 TE BBC 29 2—3 do | 76.3445 |+ 7| 52-0545 %6ь | 75-4755 |+ 7| 52.9320 LH, SE be | 75.9060 |+ 7) 52.4970 + 9.2942 00 7497 2 vielleicht » b, | 76.3400 |+ 7| 52.0625 verlängert В % с 75.5000 |+ 8| 52.9155 ве 75.9180 | 8| 52.4755 + 9,3115 40 24 7 Et 2 eo 76.3550 |+ 8| 52.0485 | %@ | 75.4600 |+- 8| 52.9470 de | 75.8754 |+ 8| 52.5125 + 9.2696 AN QI 2 d 76.3045 | 8| 52.0985 Феи | 75-4770 |+ 9| 52.9335 . ес 75.8910 |+ 9| 52.5030 R + 9.2864 42 207 2 во | 76.3235 |+ 9] 52.0725 + 9.7147 Trabant — Jupiterscentrum. &—&%y | Mittel. | и] Ch, | Да cos $ тт mm Та | 74.0065 |-+12| 54.3790 + 7.4036| —1.9052 ‚3 b | 73.9885 |-+13| 54.4010 + 7.3836] — 1.9106 2—3 с | 74.0050 |+13| 54.3785 + 7.4031| —1.9084 | —1.9109 | —1:9074 —+0'0005 | 00002 | —1:9067 | 2—3 а | 73.9570 |+13| 54-4285 + 7.354 | —1-9155 ‚ [2-3 e 73.9750 |-+14| 54.4110 + 7.3718| — 1.9146 2—3 Па | 72.4800 |-+11| 55.9105 + 5.8747| —3-4341 3 b | 72.4685 |-+12| 55.9210 + 5.8636] —3.4306 - | 2—8 с | 72.4800 |-+12| 55.9065 + 5.8768] —3.4347 | —3.4338| —3-4275 | 0.0009 | 50.0002 —3,4264| 3 d | 72.4385 |+12| 55.9510 + 5.8337| —3.4359 | 2—3 е 72.4575 |-+13| 55.9320 + 5.8528] —3.4336 у 3 III Geht du/rch |die Jupiters IV a | 79.2455 |+ 6| 49.1445 +12.6394| +3.3306 3 b | 79.2280 |+ 6| 49.1625 +-12.6218| + 3.3276 3—4 с | 79.2450 |+ 7| 49.1410 + 12.6410] -+3.3295 | +3.3275| 3.3214 | —0.0009 | -+0.0002 | +8,3207 | 2—8 4 | 79.2030 |+ 7| 49.1895 —+12.5958] 3.3262 3 e 79.2160 | 7| 49.1740 -+12.6100] -+3.3236 2—3 | Scheinbare ЖаШ: M-—Centrum = + 5.2695 Fa = 0.99816 —i° = 0.00001 т Е № = —41.4055 Q— » —=+143257 Га —=099787 — = +0.00003 x uw=—ol R—- » = — 38.7047 Re, = — 2 У— » : =— 03185 Try = + 90 W— nn =-+ 0.8857 « =0.99816 J, = +0.00091 m au = 8" 33.3 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. ` 1296. Januar 11. Decl. a ice nn пон ns | 2 Bemerkungen y = — 298 sin 1’ — — tgd sin 1’ ГР. Кг. 270+ 3 | 2 | | д ni | zur Aufnahme, 63.7437 A mm mm mm 66.6677 0.0000 — 2.9206 63.6555 -— 0.0013 + 0.0880 63.1382 — 0.0806 + 0.5190 91.1147 — 0.0094 — 27.3752 91.1160 — 0.0690 — 27.4388 0.0200 — 22.2116 65.1595 13| 64.7535 — 1.0076 64.3620 63.7110 = | 63.2980 — + 0.4448 _ 62.9030 + |: 62.2330 + 13| 61.8205 + —+ 1.9245 3|, 61.4265 + 607690 + 60.3650 = + 3.3793 59.9750 = 59.3280 + 58.9260 , + + 4.8220 ‚58,5340 + " к. а Ê vus | Mittel |foue-m| Забавы) еек ть | м И тт тт | Be ' т: RE р rte _— 58.3730 0.4702| -+0.5374 0.9876] -+0.5428 2.4670] 0.5425 | 0.5420 +#-0:5412 | +-0/0009 +-0/0016 0'0000 —+ 05437 3.9182| -+0.5389 5.3706] -+0.5486 rer À 677455 — 0.0016] -+1.0060 915 + 1.4518] -+1.0070 60.8100 . + 2.9344| -+1.0099 | -+1.0087 | -+1.0072 | -+0.0016 0.0026 0.0000 +-1,0114 6] 59.3550 —+ 4.3872| -+1.0079 15| 57.9100 + 5.8349] <+1.0129 $ 2.0552| —1.0476 — 0.6002] — 1.0450 + 0.8779] —1.0466 | —1.0452 | —1.0436 — 0.0015 — 0.0038 0.0000 — 1,0489 + 2.3320] —1.0473 + 3.7826] —1.0394 sur ереси: _М—Сештиа — = -+ 3/0030 198 = 0.99847 & 3 = —0.00046 N— ь = 3.4500 “ TER, 8: D = —24.4302 18 —0.99797 î5 =— 0.00040 X 3 ——1!4 Zn » = —24.4660 я У— » =- 49.2632 f's = 0.99847 Js = —0.00046 W— о =-+30.7293 64 = -+19°27}5 8 F. Renz, р 29 А. 1896. Januar 15. № Scalenablesung. À Helsingforser Sternzeit В $ х a 0 P.-Kr. 0° | t-+k| P.-Kr. 180° | t+-k ; der Aufnahmen, Mittel. 10000! 10000] 10000 " E mm mm mm _ mm mm Ctr, | 64.7456 63.6395 S 66.2942 |11| 62.0895 ©] + 1.5494 2—5 M 71.2385 |+13| 57.1382 o| + 6.4972 2—3 N 27.3407 |-+24| 101.9385 |+ 4|+16| —37.3994 LIEFEN ; 8 ellipt. Q 79.8150 |+19| 48.5705 —+15.0689 Я я 3 Е 29.7770 |+29| 98.5983 —34.9610 2 У 65.9925 |+18| 62.3827 О] + 1.2520 3 W | 67.1195 |+20| 61.2420 + 2.3754 ча, | 56.1080 |+ 2] 72.2820 — 8.6406 а; | 56.5920 |-+12| 71.8160 — 8.1656 — 8.1622 TL - RONDES а, | 57.0805 |+12| 71.3350 7.6804 %6 | 56.1420 |+ 1| 72.2690 — 8.6171 Г b, 56.6190 |+11| 71.7780 8.1326 — 8.1324 51.822 4—5 b, 57.1105 |+II| 71.2999 7.6474 с 56.1080 |+ 1| 72.2980 8.6186 ce | 56.5830 [+11] 71.8150 8.1691 — 8.1674 к 050 7h 51" 59° 4—5 о 57.0720 |+-11| 71.3350 7.6846 % dy | 56.1540 0| 72.2495 8.6014 de | 56.6410 |+10| 71.7715 8.1184 — 8.1212 52 36 4—5 do | 57.1135 |4-10| 71.2950 7: Ze | 56.1050 | 72.2920 8.6471 ес 56.6010 |+10| 71.8030 — 8.1541 — 8.1558 53.312 4—5 € 57-0860 |+10| 71.3120 — 7.6662 Trabant — Jupiterscentrum. &t— xy | Mittel. Рае) Лиз) Ph, | Ac cos 8 EE ET TE] mm mm Ia 55.7365 |+ 2| 72.6395 — 9.0052] —0.8430 b | 55.7675 |+ 1| 72.6100 — 8.9750] —0.8426 > с | 55.7355 |+ 1| 72.6425 — 9.0072| —0.8398 | —0.8375 | --0!8362 | —0:0002 | +0.0001 —0:8363 | а | 55.7875 | ©] 72.5890 — 8.9545] —0.8333 е 55.7585 o| 72.6200 — 8.9844] —0.8286 Па | 53.8485 |+ 6| 74.5265 —10.8924| —2.7302 b | 53.8755 |+ 6| 74.5010 —10,8661| —2.7337 Е С 53.8460 |+ 5| 74.5300 — 10.8954] —2.7280 | —2.7282| —2.7239 | —0.0007 | 0.0001 —2.1245 а 53.8970 |+ 4] 74.4805 — 10.8452] —2.7240 е 53.8640 |+ 4| 74.5190 — 10.8808] — 2.7250 Ша | 58.8490 |+13| 69.5280 — 5.8928] -+2.2694 b | 58.8815 |-+12| 69.4985 — 5,8618] -+2.2706 с | 58.8455 |+12| 69.5290 — 5.8950] -+2.2724| +2:2731| -+2.2696 | -+0.0005 | +0.0001 +-2,2702 |. а | 58.8950 |+11| 69.4820 — $.8468| 2.2744 1 е 58.8625 |+11| 69.5105 — 5.8773] -+2.2785 IV а 47.6440 |-+23| 80.7295 — 17.0954] —8.9332 b | 47.6705 |+22| 80.7005 — 17.0676) —8.93 52 с | 47.6360 |+22| 80.7370 — 17.1030] —8.9356 | —8.9342 | —8.9205 | —0.0022 | 0.0001 —8.9226 d | 47.6865 |+21| 80.6890 —17.0538| —8.9326 е | 47.6485 |-+21| 80.7235 —17.0901| —8.9343 Scheinbare ÆRdif: M—Centrum = + 5'2697 Fa = 0.99846 —i°, = 0.00000 N— » = —41.4058 | Q— » = +-14.3260 fa = 099817 —i, = +0.00002 x iy= —0:1 R— » = —38.7051 Refr: =-= 2 V— DS" 0,3183 Tzy =— 86 W— » = + 0.8858 fu =0.99846 Ja ——0,00086 - ay = 84312 1396. Januar 15. Decl. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. | lenablesung. 4nt% ot 4 A LT VOTRE sr. Bemerkungen ыы P.-Kr. 270° + р у 3 = = = 196 sin 1 y — 5-90 811 zur Aufnahme. La | ag mm mm 6265 10000] 10000] mm RR Se 62.5515 +10 0] + 2.9150 — 0.0001 + 2.9149 59.5435 [#17] О] -+ 5.9212 — 0.0022 + 5.9190 Гай 1. 59.0250 |--26|]— 3| + 6.4408 — 0.0742 + 6.3666 1| 87.0030 |-+ 1|+ 4] —21.5348 — 0.0117 —21.5465 | 86.9938 |-+-12|-+-10] —21.5320 — 0.0632 —21.5952 81.8360 |-+ 2|+ 2] —16.3730 0.0000 —16.3730 317713 |#20|—10 —33.6942 0.0000 —+33.6942 _ 55.6580 |+ 1 + 9.8118 56.1125 |+ 1 + 9.3738 + 9.3694 56.5490 |+ 1 + 8.9225 57.1955 |411 -+ 8.2798 | 97.6490 |+ 7 + 7.8352 + 7.8343 58.0850 |+ 7 + 7.3880 58.6400 |-+12 + 6.8407 _ 99.0769 |-+12 + 6.4076 + 6.4014 59.5180 +12 + 5.9560 | 60.2755 ‚ [+ 5.1948 | 60.7150 |+-12 + 4.7638 + 4.7590 _ 61.1540 |+12 + 4.3183 _ 61.5590 |411 —= 3.9081 ’ 62.0080 |+11 +- 3.4700 - + 3.4657 3| 62.4550 |1 + 3.0199 Trabant — Jupiterscentrum. NUS | Mittel. \f'atur—v2) |7 (ar) (итал Ph, | 48 : тт тт } 55.8430 |+2 + 9.6226] -+0.2532 373735 +12 + 8.0915] -+0.2572 : 58.8080 |-+-13 + 6.6562| -+0.2548 | -+0.2546 | +0:2542 | 0.0001 | —0:0008 0'0000 | -+0!2535 60.4505 |+17 + 5.0108] -+0.2518 _ 61.7410 |+12 + 3.7216] -+0.2559 55.2650 |+ 3 10.1990] -+0.8296 56.7970 |+13| + 8.6666] -+0.8323 58.2320 |+ 9 + 7.2309] -+0.8295 | 0.8308 | -+0.8296 | -+0.0004 —0.0027 0.0000 | -+0,8273 59-8735 |-+18 + 5.5883] -+0.8293 61.1620 |+14 + 4.2992| -+0.8335 56.7020 + 8.7610] —0.6084 8| 58.2340 + 7.2297] —0.6046 sl 59.6705 -+ 5.7918| —0.6096 | —0.6078 | —0.6069 | —0.0094 | -+0.0016 0.0000 | —0.6057 61.3130 + 4.1488| —0.6102 62.6040 + 2.8594] —0.6063 53.6355 —+11.8266| -1-2.4572 55.1670 +-10.2964| -+2.4621 56.6030 + 8.8608| -+2.4594 | 2.4602 | -+2.4565 | -+0.0012 | —0.0117 0.0000 | -+2.4460 58.2440 + 7.2182] -+2.4592 59.5320 + 5.9286] -+2.4629 in bare Decldif: M-—Centrum — + 3'0030 f°5 =0.99851 1° = —0.00014 I N— » = + 3.4500 | m » = — 24.4302 fs = 0.99801 is =—9,.00019 X 13 = —0:3 — » = —24.4660 У— » = —19.2632 f's = 0.99550 Js; = —0.00014 W— » =-+30.7293 dy = +19°35:7 > — 10 Е; Renz, 29 1$. 1896. Januar 17. № Scalenablesung. Helsingforser Sternzeit Object. Е 5 æ ыы P.-Kr. 0° | ++ Р.-Кг.180° #-% à der Aufnahmen. Mittel. mm mm mm La 10000! шт 10000] 10000! mm AN Ctr. | 64.7456 63.6403 Г 64.7440 |+-16| 63.6395 |+ 8] © 0.0000 M Durch elin Jlupitersbild |verd{eckt. N 25.7943 |-+-25| 102.5963 | 5|-18]| —38.9508 Q 78.2580 |+20| 50.1285 |-+14— 3|-+13.5121 6° 34” 34 В 28.2192 |-+33| 100.1677 |-+11|-=18| —36.5240 7 64.4411 |+17| 63.9405 |-FI4 о] — 0.3022 W | 65.5852 |-+22| 62.8018 |-+24| ' o| + 0.8390 2% ay | 53.7880 |-+ 3| 74.6090 |+-10 — 10.9635 Ge 54.2430 | 3| 74.1595 |-+12 — 10.5114 — 10.5 100 6 161042 а) | 54.7010 |— 1] 73.7045 |+12 — 10.0550 %Dby | 53.8015 |+ 3| 74.5970 — 10.9508 D, 54.2660 |+ 3| 74.1400 — 10.4902 — 10.4948 36 so bo 54.7170 |— 1| 73.6970 — 10.0434 3 с 53-7745 ı+ 3| 74-6130 — 10.9723 , ce 54.2515 |#+ 3] 74.1565 — 10.5056 — 10.5108 373296 6" 37” 34° бо 54.6965 |— 1| 73.6990 — 10.0546 % dy | 53-8090 + 4] 74.5905 — 10.9438 de 54.2700 |+ 4| 74.1420 — 10.4891 — 10.4874 38 16 do 54.7230 ©] 73.6750 — 10.0293 Ze | 53.7940 |+ 4| 74.6030 — 10.9576 ес 54.2560 |+ 4| 74.1530 — 10.5016 —10.4994 38 56 ео 54.7195 o| 73.6910 — 10.0391 Trabant — Jupiterscentrum. ааа | Mittel. 'ater22) Taur—va)| Ph. | Au cos à mm mm Та | 54.7250 |— ıl 73.6630 —10.0223| +0.4877 b 54.7350 |— 1| 73.6500 —10.0108| -+0.4840 e | 54.7340 |— ı| 73.6520 0.4984 | -+0.4913 | —+0!4905 | -+0/0002 0/0000 | -+-0:4907 d | 54.7479 0] 73.6400 —=0.4876 e | 54.7490 | © 73.6430 —=0.4990 Па | 56.1355 |— 1| 72.2480 —=1.9005 b | 56.1425 |— 1| 72.2380 —= 1.8938 e | 56.1310 |— 1| 72.2510 —+-1.8975 | +1.8930| +-1.8897 | -+0.0008 0.0000 | -+1,8905 d 56.1400 0] 72.2420 1.8832 e 56.1350 0] 72.2470 1.8901 Ila | 58.8950 |10| 69.4855 4.6619 b 58.9010 |+10] 69.4780 4.6534 с | 58.8960 |-10| 69.4810 +-4.6654 | +-4.6566| +4.6486 | -+0.0018 0.0000 | -=4.6504 а | 58.9000 |+11| 69.4785 —+-4.6453 e | 58.8995 |+11| 69.4785 +-4.6570 ТУа | 45.0460 |-+19| 83.3415 —9.1894 b | 45.0570 |-+19] 83.3290 —9.1928 с | 45.0520 |-+18| 83.3335 —59.1816| —9.1894| —9.1736 | —0.0034 0.0000 | —9,1770 d | 45.0620 |-+18| 83.3255 —9.1960 } е 45.0565 |-+18| 83.3265 —9.1873 Scheinbare Ædiff: M— Centrum —+ 5/2697 . f°,—0.99828 —i°, = —0.00020 N— » — —41.4058 | Q— » =-+-14.3260 Fa == 0.99796 —îy = —0.00014 № = + 05 R— » = — 38.7052 Refr. =— 6 V— „We 0,3183 Тех =— ro W— » —+ 0.8858 Fu = 0.99828 Jy =-— 0.00130 ay = 8" 30.2 *) Trabant I stört bei der Einstellung auf den Ostrand. **) 2 stört. POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. 11 1896. Januar 17. Decl. y Ant+ac+%s “EUER Е. А Bemerkungen PSE JA Tape 5 #0 an] zur Aufnahme, 65.4657 mm mm mm 8 64.0257 \ 0.0000 +- 1.4402 Jlupitersbild : 60.4918 — 0.0806 + 4.8949 | — 0.0094 — 23.0218 | —-10|+-11 — 0,0690 —23.0676 83.3152 |— $2 0.0000 — 17.8469 33.2485 |+20|— 8 0.0000 +-32:2204 63.6510 |+11 4.0880 |H-11 —+ 1.3890 4.5225 |+11 65.2070 |-+19 65.6410 |+13 66.0605 |-+13 66.6520 |+11 67.0800 |+11 67.4930 |+ 68.1560 |+16 — 68.5410 |+16 — 68.9550 |+16 — +19 +19 --— в... == Trabant — Jupiterscentrum. 4 Г Ira (ye—Y2) 173 (ареал —0.1230 | —o.1218 | —o!1216 0:0000 | -+0!0005 0.0000 | —0'1211 70.1770 64.6790 |+-18 + 66.2220 |+12 — 0.7584 67.6590* |+20 — 2.1955| — 0.5979 | —0.5973*| —0.5964 | —0.0002 -+0.0019 0.0000 | — 0,5947 69.1145 |-+15 — 3.6512] —9.5930 70.6480 |+-14 — 5.1847] —0.5945 —1.3752 —1.3713 —1.3722 | —1.3722 | —1.3702 | —0.0005 —0.0039 0.0000 | —1,3668 — 1.3712 — 1.3713 -+2.5960 —+2.6017 : -+2.6020 | -+2.6011 | -+2.5973 | 0.0009 | —0.0144 0.0000 | -+-2,5838 -+2.6036 2.6020 — ieinbare Decldif: M—Centrum= + 3:0032 fs = 0.99852 8 = —0.00011 j 2 N— » = + 3.4502 = . ’ у Q— » = —24.4305 fs =0.99798 1; = 0.00002 X o=-+ ol R—- » = — 24.4663 V— » ——19.263$ f's —=0.99852 Js = —0.00010 W— » = -+30.7298 ©? y = +19° 39.8 | 12 Г. Renz, 29 С. 1896. Januar 20. | Æ 87. Scalenablesung. Helsingforser Sternzeit Object, раша: АНН Bilder. = 0.99824 Jy =+0.00120 P.-Kr. 0° le P.-Kr.180°|+-+# der Aufnahmen. Mittel, 10000 10000] 10000 Ctr, | 647726 |" | 686182 |” и ры S 64.7710 |+16| 63.6123 |+ 0.0000 2 M Durch elin Jlupitersbild Beh eckt, N 25.8193 |-+25| 102.5698 |+ 5|+-18| — 38.9522 к MUR 2—3 Q 78.2935 |--21| 50.0892 |-+-15|— 5|-1-13.5222 8 43 16 3 Е 28.2487 |+34| 100.1297 |-+12 Bis — 36.5165 2 Li 64.4740 |18| 63.9095 |+15 — 0.2973 1—2 W | 65.6050 |-+22| 62.7785 |--24 О 0.8334 2—3 %а„ | 75.6065 |-+10| 52.7885 |+10 ро а; | 76.0810 |#+-10| 52.3210 |-+14 —=11.3001 11.3040 81 24510017 4—5 Go | 76.5595 |190] 51.8345 |+14 —+11.7826 % Da | 75.6280 |+ 8| 52.7555 |+ 9 +-10.8565 D, 76.1120 |+ 8| 52.2930 |+13 -+-11.3296 —+-11.3274 46 25 4—5 b, 76.5730 |-+ 8| 51.8210 |-+13 —=11.7960 % с 75.5920 |+ 8| 52.7970 |+ —=10.8178 j ce 76.0680 |-+ 8| 52.3210 +-11.2886 +-11.2943 472.6 8%; 417" 1.4 4—5 Co 76.5550 |+ 8| 51.8420 +11.7766 % dy | 75.6075 |+ 7| 52.7845 +-10.8318 de 76.0865 |+ 7| 52.3060 +11.3103 -+-11.3084 47 47 4 do | 76.5600 | 7| 51.8340 +11.7830 Yen | 75.5960 | 7| 52.8035 -+10.8165 ес 76.0575 |+ 7| 52.3270 +-11.2853 +-11.2906 48 25 4—5 ео 76.5560 |+ 7| 51.8560 —-11,7700 Trabant — Jupiterscentrum. mie | Mittel. Рыба) Лишь Ph. | Au cos $ mm тт Та 73.9410 |-+14| 54.4340 + 9.1742] —2.1298 2 b | 73.9580 |+13| 54.4180 + 9.1907| — 2.1367 2 с | 73.9350 |+13| 54.4415 + 9.1674] —2.1269 | —2.1308| —2!1270 | -н0'0007 0'0000 |. —2.1263 | 1—2 d | 73.9430 |-+12| 54.4310 + 9.1767| —2.1317 | 2—3 е 73.9300 |+12| 54.4480 |- 4 + 9.1617| —2.1289 2 Па | 79.4550 +9] 48.9180 |+-16 —+-14.6884| +-3.3844 1—2 b | 79.4720 |+ 8| 48.9020 |+16 +14.7048| -3.3774 2 С 79.4460 |-+7| 48.9270 |-+15 —+14.6793| 3.3850 | +3.3806 | —-3.3747 | —0.0012 0.0000| —+3,3735 | 1—2 а | 79.4545 |+ 7| 48.9215 |-+15 —14.6863| 3.3779 1—2 € | 79.4355 |+ 6| 48.9370 |+14 +-14.6690| -+-3.3784 1 Ша | 70.6200 |+13| 57.7580 |+ 8 + 5.8516] —5-4524 1 b | 70.6380 |+13| 57.7370 |+ 7 + 5.8711| —5.4563 1 € | 70.6130 |+12| 57.7615 |+ 7 + 5.8463| —5.4480| —5.4531| —5.4435 | —+0.0019 0.0005 | —5.4416 | 1—2 d | 70.6205 |+12| 57.7525 |+ 6 + 5.8546] —5.4538 1 e 70.6030 |+-12| 57.7730 |+ 6 + 5.8356] —5.45 50 1—2 IVa 75.2455 |-+13| 53.1345 |+10 +10.4760! —0.8280 2 D | 75.2645 |+11| 53.1170 |+ 9 -=10.4942| —0.83 32 | 2 с | 75.2420 |+11| 53.1370 |+ 9 -4-10.4729| —0.8214 | —0.8271 | —0.8257 | —-0.0004 0.0000 | —0,8253 | 2—3 d | 75.2485 |--ı0l 53.1290 |+ 8 —+-10.4802| —0.8282 у 2 е 75.2350 |+10| 53.1440 |+ 8 —+10.4659] —0.8247 2 Scheinbare Rdif: N— Centrum = —41.4060 Fu = 0.99824 +12 4 = -+0.00001 Q— » = -+14.3261 Е— » == —38.70$4 и = 0.99796 —iy =-0.00001 == ` 90 У— » = — 0.3183 Вет. =+ I W—- » = + 0.8859 Tom 118 —24.4562 —24.4402 —19.2900 +-30.7784 — 7.8150 — 7.3750 — 6.9408 72.4105 71.8490 — 6.3709 71.4090 — 5.9284 70.9650 — 5.4964 70.3630 — 4.8921 69.9170 — 4.4421 69.4590 — 4.0021 68.8925 — 3.4200 68.4505 — 2.9742 67.9950 — 2.5300 67.4675 — 1.9944 67.0240 — 1.5490 66.5820 — 1.1102 72.2395 — 6.7762 70.7990 —.5.3352 69.3050 — 3.8442 67.8470 — 2.3867 66.4140 — 0.9536 73.8195 — 8.3584 72.3810 — 6.9194 70.8900 — 5.4279 69.4300 — 3.9694 67.9985 — 2.5377 71.2900 — 5.8285 69.85 10 — 3.3906 68.3580 — 2.8986 66.9010 — 1.4400 65.4650 — 0.0059 72.4960 — 7.0335 71.0550 — 5.5930 69.5680 — 4.1068 68.1100 — 2.6475 66.6760 — 1.2138 sinbare Decldiff: N—-Centrum — + 3.4503 Е — ) = —24.4307 » — —24.4663 У— » = —19.2635 W— » = +-30.7300 dy = +19° 46:1 Decl. Zat2ct%s 3 = а 5.9319 4.4454 2.9747 1.5512 mm mm +-0.6007 , +-0.5967 +-0.6012 | -+0.5968 —+-0.5880 +-0.5976 -—0.9815 —0.9875 —0.9825 — 0.9947 —0.9865 -+1.5484 +1.5413 -+-1.5468 —1.5347 —1.5453 —0.3434 0.3389 -+0.3386 +-0.3272 —0.3374 — 0.9865 —-1:5433 0.3371 198 = 0.99850 fs = 0.99801 1’; = 0.99850 1896. Januar 20. 2 = > tgù sin 1’ mm 0.0000 — 0.0806 — 0.0094 — 0.0693 0.0000 0.0000 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. x? ей у—- #96 3ш1 тт 0,0000 + 3.4535 — 24.4656 — 24.5095 — 19.2900 +-30.7784 Trabant — Jupiterscentrum. m R T У: — Ух | Mittel. % ау) Ja (ага +] 0/5959 | <+-0:0002 —0.9850 | —0.0003 =+1.5410 | -+0.0005 -+0.3366 | -+0.0001 $? = —0.00010 ig ——0.00011 Уз = —0.00009 -1-0/0023 _ 0.0046 -0.0049 #-0.0010 X ig = —0:4 Bemerkungen zur Aufnahme. Luft 1. 0.0000 0.0000 0,0000 39 +-0:5984 —0,9899 +-1,5464 -+0.3377 14 Е. Rexz, 29 D. 1296. Januar 233. Scalenablesung. Helsingforser Sternzeit ео Object.| — — — —— Bilder, Mu P.-Kr. 0° | tt P.-Kr.180° |t-+%k der Aufnahmen. | Mittel. 1 тт mm_| тт m 10000] тт 10000] 10000 m Cir. | 64.7571 63.6282 S 64.7555 |+16| 63.6273 |+ 9| 0 0.0000 2 M 69.7055 |-=16| 58.6730 [+10 © 2 MW N 25.8045 |-+25| 102.5840 |+ 5|+17 ь LISTE 3 | Q 78.2722 |+21| 50.1130 |+16|— 4 6 37...24 3 | R 28.2280 |+-34} 102.1517 |+13[+21 2—3 etwas ellig У 64-4505 |+19| 63.9298 |+17| © 1—2 ” я 65.6000 |-+22| 62.7858 |+23| O 2—5 ZA | 69.0220 |-+14| 59.3720 |+10 Ce 69.4920 |-+14| 58.8990 |+10 + 4.7379 6 Bolero 4 а, | 69.9835 |17| 58.4140 |+-10 out 2b | 69.0335 |-+14| 59.3670 |+10 | be 69.5120 |+17| 58.8820 |+10 + 4.7475 391054 4 bo | 69.9870 |+17| 58.4135 |+10 % Cp 69.0620 |-+15| 59.3320 |+11 DER e 69.5200 |+18| 58.8750 —+ 4.7648 40135 6 40 33 4 Co | 69.9940 +18] 58.3955 % dy | 69.0330 |-+15| 59.3710 | de 69.5090 |-18| 58.9020 + 4.7380 RE 4—5 dy | 69.9700 |-+18| 58.4260 % y 69.0435 |+-16| 59.3480 & | 69.5175 H-19] 58.8850 + 4.7550 41.55 4 ео 69.9890 |-+19] 58.4025 - - | 1 Trabant — Jupiterscentrum. dès | Mittel. и] Ph. | Au cos à EE РИ ИЕ Е Е DR GR AIRES CE ne es mm mm Та | 70.5585 [+13] 57.8190 |+ 5 + 5.8057] +1.0678| 4 2 b | 70.5630 |-+13| 57.8130 |+ 5 + 5.8110] 1.0635 + 1—2 с | 70.5820 |+13| 57.7950 |- 6 + 5.8294| +-1.0646 | 1.0627 | —+1:0609 | —0:0001 0.0000 | -+1:0608 | 1—2 4 | 70.5450 |+14| 57.8295 |+ 6 + 5.7937| +1.0557 | 2% e | 70.5690 |-+15| 57.8075 |+ 7 + 5.8167| -+1.0617 19 Па | 71.3250 |+13| 57.0535 |+ 9 + 6.5715] -+1.8336 2 b | 71.3350 |+13| 57.0430 |+ 9 + 6.5818] +-1.8343 1—2 e | 71.3600 |#-13| 57.0195 |+-10 + 6.6060] -нт.84т2 | 1.8389 | —+-1.8358 | — 0.0001 0.0000! -+1,8357 | 1—2 d | 71.3270 |+14| 57.0490 |+10 + 6.5748] +1.8368 1 ' е | 71.3560 |+-I5| 57.0200 |-+11 + 6.6038] 1.8488 | 1—2 } Ша | 74.4620 |-+12| 53.9170 |+ 3 + 9.7085] +4.9706 2 b | 74.4700 |-+13| 53.9090 |+ 3 + 9.7166] 4.9691 2 е | 74.4930 |+13| 53.8855 |+ 3 + 9.7398] -+4.9750 | +4.9735| 44-9651 | —0.0003 0.0000 | 4,9648 | 1—2 а | 74.4640 |+13| 53-9145 |+ 4 + 9.7108] +4.9728 -2 е | 74.4865 |+14| 53.8890 |+ 4 + 9.7348| +4.9798 у 2 IV а | 77.6950 | 8| 50.6810 |+10 -+12.9424| 8.2045 2 b | 77.7070 |+ 8| 50.6730 |-+190 -+12.9524| -8.2049 | | 1—2 с | 77.7240 | 9] 50.6525 |-1о -+12.9712| -+8.2064 | -+8,2069 | -+8.1930 | —0.0005 0.0000 | -+8,1925 | 1—2 а | 77.6990 |+ 9] 50.6800 |+10 12.9449] -+-8.2069 j 1—2. е 77.7175 |10| 50.6550 |411 +-12.9667| 8.2117 1—2 Scheinbare Rdif: M-—Centrum = + 5'2697 Fra = 0.99832 —1°y = —0.0003 1 | N— » = —41.4062 | 9— » = +14.3261 fx =9.99800 —i, =— 0.00025 x i„=-+0:8 | Е » ——38.7056 Refr. =— 5 У— » = — 0.3184 Tr + so W— » = + 0.8860 fu =0:99851 Ju = --0.00020 т 92, = 8/ 26.9 és mA 1 CLR 1 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1896. Januar 23. Decl. } 8 le. 3 Scalenablesung. 154 Der Bnt20+2%5 Ar; ! au à ’ — 5 60811 y— = 19651 1 т , 90° ne. т 65.1657 66.9568 у 63.9465 + 1.5188 63.4180 -+ 2.0462 91.4138 — 25.9444 91.3945 —25.9309 86.2457 — 20.7817 36.1755 —+29.2885 59.7920 59.3610 + 6.1174 58.9310 + 6.5460 58.2780 + 7.1928 57.8410 + 7.6379 57.4080 —= 8.0646 56.8030 56.3800 55.9450 Trabant — Jupiterscentrum. : T vs | Mittel. |raW-m| 3 ео] (опал) 62.5605 -Е 2. —0.3157 61.1100 +4. —0.3235 59.6700 — 5. —0.3208 58.1520 = We —0.3217 56.6785 + 8. — 0.3154 62.7210 + 2. — 0.4795 61.2790 +4. —0.4918 59.8350 — 5. —0.4858 | —0.4879 | —0.4871 58.3215 + 7. —0.4922 у 56.8505 + 8. —0.4900 63.6120 + 1.808] —1.3670 4| 62.1610 + 3.3004] —1.3753 2| 60.7160 —+ 4.7432] —1.3696 | —1.3720 59.2045 + 6.2568] — 1.3750 | 57.7340 + 7.7267] —1.3729 64.4200 —= 1.0444] —2.1734 62.9695 + 2.4930] — 2.1827 4| 61.5220 + 3.9401| —2.1727 —2.1748 60.0150 + 5.4476) —2.1842 58.5400 —= 6.9222| —2.1774 inbare Decldif: M—Centrum = -+- 3.0022 198 = 0.99847 12 = —0.00010 + N— » = + 3.4503 . 3 \ — D 0=—24.4307 15 = 097% is = -+0.00003 X 14 = +01 — |, » =— 24.4663 У— » ——19.2635, f's = 0.99846 Уз = —0.00008 W— » = -+30.7300 Bemerkungen zur Aufnahme. Qt 16 30 A. = 1396. Е. Renz, J re 26. № : Scalenablesung. Helsingforser Sternzeit Object. — "© æ Ra Pres P.-Kr. 0° jé P.-Kr. 180°| é-+-7 - der Aufnahmen. Mittel. mm mm mm 10000 10000] 10000 ; Ctr, | 66.8163 61.5757 a Ha 5 66.8155 |+ 8| 61.5748 |=- 9] о 0.0000 M 71.7643 |-=12| 56.6160 |+-10| о] -н 4.9540 N 27.8610 |+23| 100.5285 |+ 4|-+17| —38.9514 NEE Q 80.3362 |+19| 48.0522 |-+27|— 2|-+13,5211 6 50 41 R 30.2825 |-+-29| 98.0920 |-+ 8|-+18| — 36.5222 У 66.5095 |+16| 61.8645 |+15] ol — 0.2978 W | 67.6490 |+30| 60.7370 |-+26| ol +- 0.8359 % dy | 52.3020 |+10| 76.0885 |+ тон 1] —14.5134 le 52.8675 |+-10| 75.5315 |+-10-- 1] —13.9522 —13.9472 6 Бе -то ay | 53-4410 |+10| 74.9525 |+13[4- 1] —13.3761 by | 52.3530 |+10| 76.0375 |+ 9]- 1] —14.4624 be 52.8910 |+10| 75.5145 |+ 9|4+ 1] —13.9319 — 13.9281 SAUT, b, 53.4270 |+10| 74.9665 |+12}+ 1| — 13.3930 % Cp | 52.3730 |+10| 76.0080 |+ 8|-= 1] — 14.4376 à 4955 Ge | 52.9185 |+10| 75.4990 |+11|+ 1] —13.9105 —13.9075 54 53 6 54 52 Co | 53-4465 |+10| 74.9550 |+11]H- 1] —13.3745 % dyp | 52.3410 |+ 9| 76.0530 |+ 8H 1] —14.4762 de | 52.8865 |+ 9] 75.5255 |+ 8 1] —13.9396 —13.9439 55 39 do | 53-4065 |+ 9] 74.9980 |+11|+ 1] —13.4160 Фе | 52.3535 |+ 8| 76.0470 |+ 7] + 1] —14.4667 ес 52.8865 |+ 8| 75.5190 |+ 7|-+ 1] —13.9364 —13.9278 56 25 ео | 53-4395 |+ 8| 74.9590 [+184 1] —13.3804 Trabant — Jupiterscentrum. 202 | Mittel. [Рыба иги Ph. | Aa cos à mm mm Та | 54.3515 |+ 6| 74.0300 |+15[-+- 1) —12.4599| -+1.4873 b 54.3595 | 6| 74.0190 |-+14|-= 1] —12.4504| +1.4777 i , с | 54.3860 |+ 5| 73.9945 |+13|4- 1] —12.4248| +-1.4827 | -+1.4864 | —+-1'4838 | +-0:0006 00000 | —+-1:4844 а | 54.3570 |-+- 5| 74.0210 |-+13|-= 1] —12.4526| +-1.4913 e 54.3755 |+ 4| 74.0040 |+-12|-+ 1] —12.4348| #1.4930 Па | 51.5195 |-+15| 76.8590 |-+12|-= 1] —15.2898| — 1.3426 b | 51.5295 +14| 76.8460 |--I1l-+- 11 —15.2783) —1.3502 ce 51.5615 |-+14| 76.8170 |-+лоНн 1] —15.2478| —1.3403 | —1.3409 | —1.3386 | —0.0006 0.0000 | —1,3392 Я | 51.5285 |+13| 76.8485 |+-10|+- 1] —15.2800| —1.3361 |. е 51.5470 |-+12| 76.8330 |-+- ol |—15.2630] —1.3352 Ша | 49.6435 |+ 9] 78.7370 |+10|+ 2] —17.1669] —3.2197 6 | 49.6500 |+ 8| 78.7280 | 9]|-= 2|—17.1592] —3.23 11 с | 49.6765 |+ 8 78.7005 |-= 8|-+- 2| —17.1321| —3.2246| —3.2266| —3.2209 | —0.C013 0.0000 | —3,2222 а | 49.6385 |+ 7| 78.7400 |+ 7l-+- 2| —17.1708| —3.2269 е | 49.6510 |+ 6| 78.7280 |-+- 7|-= 2| —17.1586| —3.2308 IV a | 60.9785 |+13| 67.3975 |-+19 о]-— 5.8296] 8.1176 b | 60.9865 |+12| 67.3890 |+ 9] 0]|— 5.8214] 8.1067 с | 61.0125 |+12| 67.3645 |+ 9 o]— 5.7962] 8.1113 | 8.1109 | —-8.0967 | -4-0.0032 0.0000 | 8,9999 а | 60.9735 |-+-11| 67.4040 |- 8] o|— 5.8354| 8.1085 е 60.9920 |+11| 67.3870 |+ 8] о] — 5.8176] + 8.1102 | Scheinbare Ædiff: J1—Centrum = -+ 5'2697 F° x = 0.99826 —®, = —0.00004 N— » — —41.4063* Q— » — -+14.3261 Fa = 9.99795 — = 0.00001 X = R— » — — 38.7058 Refr. =— У— » = — 0.3184 Try =— 146 W— » — + 0.8861 Га = 099825 I, = — 9.00149 т ay = 8} 25.2 Bilder. | 4 unterexp. | 4 4—5 | 90°) Р.-Кг.270° ++ m > 65.6200 62.7218 59.7085 59.1865 87.1770 87.1582 82.0060 31.9448 54.0350 54.5715 55.1285 55.5900 56.1295 56.6170 57.0905 57.5860 58.0710 58.5440 59.0760 59.5620 _ 99.9860 61 0270 54.9720 56.5155 57.9800 59.1620 60.9140 54.1400 55.6865 57-1475 58.6300 69.0890 53.7195 55.2635 56.7300 58.2070 59.6540 56.8330 58.3800 59-8450 61.3270 62.7850 — . ЕЕ ЕЕНЕЕ ЕЕ ЕЕ 5 einbare Decldif: M-Centrum = +- 3/0033 - N- — » = + 3.4504 Q— » = —24.4310 Е— » = —24.4666 Ув = — 19.2637 W—- » = 30.7305 dy = +-19° 581 mm +11.0558 95159 + 8.0456 + 6.5688 + 5.1198 mm mm —0.4099 —0.4163 —0.4108 | —0.4144 —0,4146 — 0.4204 +-0.4230 +-0.4158 | —+0.4214 | -+0.4166 —+-0.4164 —0.4066 —0.8440 —0.8409 —0.8514 | -+0.8428 —-0.8388 -+0.8400 — 2.2722 — 2.2807 —2.2774 | —2.2797 — 2.2804 — 2.2877 195 = 0.99862 Ss = 0.99819 f'a = 0.99861 1396. Januar 26. Decl. AS Ех 8 © > POSITIOXEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNABMEN. тт Trabant — Jupiterscentrum. —0'4138 | —o'ooo1 -0.4160 | -+0.0001 —+-0.8416 | -+0.0002 —2.2765 | —0.0005 De: = —0.00008 14 = +40,00003 Js = —0,00006 . | т! Yı—yz | Mittel. Ir lue—va)|Ioleı—a2)|-w2-a22] -+0'0021 —0.0020 —0.0053 +-0.008$ № в = 0 Bemerkungen zur Aufnahme, Luft 3. 0.0000 0.0000 0,0000 —0:4118 +0,4141 + 0,3365 —2,2685 18 F. Renz, 30 B. 1896. Januar 30. № Scalenablesung. Helsingforser Sternzeit |. ‚Object. 2 5 x FF EHE Bilder, | P.-Kr. 0° | ++ P.-Kr.180°| 1-+-k der Aufnahmen. Mittel. Le | _тт_ _mm_|_mm_ m 10000| mm 10000110000] mm Le Ctr. | 66.5628 61.5274 | 5 66.8620 |-+ 8| 61.5265 + 9] 0 0.0000 2—3 M 71.8175 |+12| 56.5730 |- 9] ©] + 4.9547 3 N 27.9035 |-22| 100.4905 |+ 2|-+17| —38.9585 К. 3 Q 80.3845 |-+20| 48.0025 |+28]— 3]+13.5226 9" №9». © 3 R 30.3332 +30) 98.0447 | 9|-+19| — 36.5205 3 KE 66.5623 |-+17| 61.8203 |-+15] 0] — 0.2966 2—3 № | 67.6920 |+30| 60.6925 |-+-25| ©] + 0.8323 3 шиегехр. — %а | 55.6530 |— 1| 72.7350 |+13 — 11.2094 FR LIT TEA le 56.1520 |— 1| 72.2480 |+II —10.7163 — 10.7 142 9 / №4003 3—4 Ag 56.6495 — 1| 71.7470 | '— 10.2170 45 | 55.6630 |— 1| 72.7340 +14 — 11.2040 b. 56.1780 — 1| 72.2240 |+12 — 10.6914 — 10.6954 19221 4 b, 56.6760 |— 1| 71.7210 |+12 — 10.1908 Ze 55.6520 — 1| 72.7365 |+14 — 11.2107 с. 56.1620 |— 1| 72.2435 |412 —10,7091 — 10.7090 19 58 9 16" 0 3—4 Co 56.6630 |— 1| 71.7405 |-+12 —10.2071 % dy | 55.6570 | — 72.7435 |+14 —11.2117 de | 56.1690 |— 72.2300 |+-12 — 10.6988 — 10.7049 16 40 3—4 do | 56.6655 |— 1| 71.7370 |+12 — 10.2041 Hem | 55.6315 O| 72.7545 |-+15 —11,2300 ес 56.1465 | ©] 72.2510 |+13 — 10.7206 — 10.7212 2741.16 4 ео 56.6590 O| 71.7485 |+13 —10.2131 Trabant — Jupiterscentrum. ое | Mittel. | аи ии Ph. | Да cos à FREE, IRON RS Е RO ENS ee ER | mm mm Та | 57.0955 + 9] 71.2795 |+12 — 9.7598] 0.9544 2 b | 57.1110 |+ 9| 71.2640 |+12 — 9.7444| +0.9510 2—8 е | 57.0975 + 9| 71.2770 |+12 — 9.7576] +0.9514 | -+0.9523 | -=0:9506 | -+0:0003 о'о00о | +-0:9509 | 2 d | 57.0990 |-+10| 71.2755 |+12 — 9.7560] 0.9489 2 е 57.0900 |-+10| 71.2855 |+12 — 9.7656] -+0.9556 | 2 Па | 57.9520 |+ 5| 70.4225 |+16 — 8.9035] +1.8107 2 b | 57.9700 |+ 5| 70.4060 |+17 — 8.8863| +1.8091 : 2—3 e | 57.9625 |+- 5| 70.4110 |+17 — 8.8926] +1.8164 | +-1,8173 | +-1.8140 | -+0.0005 0.0000 | +-1.8145 | 2—3 d | 57.9705 + 6| 70.4045 |+17 — 8,8852] +1.8197 2—3 e 57.9620 | 6| 70.4070 |+18 — 8.8908| +1.8304 2—3 Ша | 61.0075 |-+10| 67.3665 |+ 9 — 5.8472| 4.8670 2 6 | 61.0315 |+10| 67.3460 |+ 9 — 5.8249] 4.8705 2 с | 61.0175 |#+11| 67.3560 |+10 — 5.8369] +4.8721 | -+4.8729 | -+4.8640 | -+0.0014 0.0000 | 4,8654 | 2 4 | 61.0220 |+11| 67.3525 |+10 — 5.8329] 4.8720 р 2 е 61.0180 |+12| 67.3590 |-11 — 5.8382] 4.8830 2 IV a | 50.8605 |-+11| 77.5205 |+ 8|+ ı| —15.9974| — 5.2832 3 b 50.8765 |-+10| 77.5030 |-= 8|-= 1] —15.9808| —5.2854 3 е | 50.8665 10) 77.5130 |-+ of+ |—15.9908| —5.2818 | —5.2821 | —5.2725 | —0.0014 | 0.0000 | —5.2739 | 2—3 | а | 50.8655 |109 77.5105 |+ 9] | —15.9900! —5s.2851 2—5 | e 50.8625 |11| 77.5195 |+ 9+ 1] —15.9960| —5.2748 3 | Scheinbare Adiff: M-Centrum = -+ 5'2697 19а = 0.99818 —®, = -+0.00006 N— » = —41.4066 0— » = +-14.3262 fa =0.99789 —ig =-0.00004 X y = —0:1 R— » = —38.7061 Ве. =+ 2 У— » = — 0.3185 Та =— 114 W— » =+ 0.8863 у = 0,99818 Jy — 0.00108 0, = Br 23.0 64.1607 61.1542 88.6200 88.6055 83.4537 33.3835 63.8590 64.3240 65.3790 65.8690 66.7880 67.2680 67.7365 68.2260 68.7120 69.1760 + 8| 69.7300 70.2170 70.6940 64.6000 66,1300 67.5330 68.9720 70.4860 64.7870 5 120 7.7195 69.1630 70.6780 65.6310 . 67.1605 68.5660 70.0065 71.5330 63.0080 64.5360 65.9365 67.3790 68.9000 м т R— ne. w- mm 65.6200 60.6255 . 64.7925: 66.3170. bare Decldiff: M—Ce | 7 ntrum » » » » » 1396. Januar 30. mm 1.0142 0.5154 1,9191 3.3576 4.8712 0,8279 0,6970 2.1051 3.5496 5.0643 0.0160 1.5451 2.9519 4.3918 5.9130 2.6091 1.0788 0.3226 1.7644 — 3.2814 ЕТЕТТ И ыы. ГА + 3.0033 + 3.4505 — 24.4312 — 24.4667 — 19.2638 -+30.7308 Зи = -+20° 6'2 Decl. Znt%ect?%; 3 —0.2862 — 0,2374 —0.2797 | —0.2829 — 0.2781 — 0.2830 —0.4725 — 0.4690 —0.4657 | —0.4707 — 0.4701 —0.4761 — 1.3164 — 1.3171 —1.3125 | —1.3166 — 1.3123 — 1.3248 +1.3087 +-1.3068 —+1.3168 | -+1.3108 +1.3151 —1.3068 128 = 0.99844 fs = 0.99795 Ду = 099844 | | и 2 РозимохЕх DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 2 x #95 sin I’ у— — 196 sin Г тт тт 0.0000 + 1.4584 — 0.0013 + 2.4633 — 0.0806 + 4.9112 — 0.0094 23.0090 — 0,0690 — 23.0573 0.0000 — 17.8347 0.0000 +-32.2382 —0.2825 | —0:0001 —0.4700 | —0.0002 —1.3145 —0,0006 -+1.3087 | -+0.0006 д = —0.00013 3 = —0.00017 J3 = — 0.0012 era zur Aufnahme. Bemerkungen | | Luft 1—2 (durch- | sichtig, aber et- was nnrubig). | Trabant — J upiterscentrum. в fs ru») Ja(cr—23) | ее) +-0!/0010 —0.0919 0.0043 — 0.0075 x ia = —06 0.0000 0.0000 0.0000 — 0:2816 —0.4683 20 к. Renz, 30 C. 1296. Februar 1. № Scalenablesung. Е L Helsingforser Sternzeit Object. tie 8 x Paie te TENUE TRES DER RN N Bilde P.-Kr. 0° |t+k| Р.-Кт.180° t+-k der Aufnahmen. Mittel. | mm _mm | тт р 10000 10000! 10000 N Ctr. | 66.8731 61.5160 FR a 5 66.8723 |+ 8| 61.5150 |+10| O 0.0000 Da M 71.8243 |-+12| 56.5588 |+ 9] 0|-+ 4.9544 2 N 27.9163 |+22| 100.4735 |+ 2|—18| +38.9544 А \ 3 Q | 80.3940 |+21| 47.9913 |+20]+ 3) +13.5221 8° 59” 20 3 В 30.3435 |+31| 98.0300 |+10]—21| —36.5186 9-3 У 66.5725 |+18| 61.8078 |-+16] 0] — 0.2961 9—3 | 67.7090 |+30| 60.6800 |-+25] ©] + 0.8362 3 unterexp. %а„, | 81.6630 |+ 4| 46.7335 |+12[+- 2] 14.7856 вет ас | 82.1580 |-+ 4| 46.2375 |-+18|+ 2 15.2808 +15.2802 он 3 ap | 82.6530 |+ 5| 45.7455 |+18|# 2] 15.7744 2 by | 81.6615 |+- 3| 46.7385 |1\|-= 2| +14.7824 > 82.1545 |+ 3| 46.2375 |+17|+ 2] 15.2790 +15.2791 156 3 bo | 82.6540 [+ 4] 45.7435 |+17| 2] +15.7758 % Cw | 81.6635 |+ 2] 46.7355 |--и|-= 1]-+14.7849 „ AR Ce | 82.1580 |+ 2| 46.2500 |+17|+ 1] +15.2746 +15.2790 21034 De DE 3—4 en 82.6500 | 3| 45.7365 |+17|+ 1) +15.7774 % dy | 81.6450 |+ 2] 46.7435 |+10]+ 1] 14.7717 ас | 82.1615 |+ 2] 46.2420 |-+16|+ 1]+15.2804 15.2734 3,12 3 dy | 82.6430 |+ 3| 45.7485 |+16|+ 1| 15.7680 Zen | 81.6510 |+ 1| 46.7420 |+ 9] 1] +14.7754 ес | 82.1500 |+ 1| 46.2515 |+-15|+ 1] +15.2699 —15.2687 3 49 2—3 CA 82.6380 |+ 2| 45.7580 |+15l+ 1 -н15.7607| Trabant — Jupiterscentrum. Tt—%y | Mittel. f'det-22) (leva) Ph. | Ао. cos à md loss EP LR DT И Та | 81.4760 |+17| 46.8990 14.6100] —0.6702 3 b | 81.4640 |+16| 46.9100 -+14.5985| —0.6806 9-3 с | 81.4660 |+15| 46.9120 +14.5986] —0.6804 | —0.6783 | —0!677I | -+0:0003 | —0'000т | —0.6769 | 3 а | 81.4595 |+-ı5| 46.9160 14.5934] —0.6800 3—4 е 81.4555 |-+14| 46.9215 +-14.5886| —0.6801 2 Па | 79.3090 |+ 8| 49.0680 —+12.4414] —2.8388 925 b | 79.2935 |+ 7| 49.0820 +-12.4266| — 2.8525 2—3 с | 79.2985 |+ 7| 49.0790 +-12.4307| —2.8483 | —2.8472 | —2.8422 | 0.0012 | —0.0001 | —2.8411 | 2—3 а | 79.2915 |+ 6| 49.0860 +-12.4236| —2.8498 3 e 79.2900 |+ 6| 49.0880 -+12.4220| —2.8467 93 Ша | 83.8515 |— 3| 44.5240 16.9838] +1.7036 2 b | 83.8475 |— 4| 44.5330 —=16.9772| +1.6981 ПЗ с | 83.8460 |— 5| 44.5295 +-16.9782| +1.6992 | -+1.7007 | 1.6977 | —0.0009 | —0.0001 | -+1,6967 | 2 а | 83.8440 |— 6| 44.5360 —+16.9740] 1.7006 2—3 е | 83.8395 |— 6| 44.5380 —+-16.9708| 1.7021 2 IV a | 72.6945 +15] 55.6870 + 5.8258] —9.4544 2—3 b | 72.6895 |-+14| 55.6920 + 5.8208] —9.4583 3 с | 72.6925 |-+14| 55.6860 + —9.4536| —9.4544 | —9.4380 | -н0.0040 | —0.000т | —9,4341| 3 d | 72.6820 |+13| 55.6950 + —9.4578 2—3 e 72.6870 | 55.6900 + — 9.4481 2—3 Scheinbare 2841: D1—Centrum = + 5.2697 Fa = 0:99825 —1° y = —0:00001 N— » — —41.4067 Q— » = +-14.3262 fu = 099797 —iy = 0.00000 x = 00 В— » — — 38.7062 Пей’. =-н 2 У » = — 0.3185 Try =+ 163 W—- » — + 0.8863 Го = 099826 о. = —0,00165 hm ay = 8 21.9 er SE POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN, 21 1396. F'ebruar 1. Decl. Zn+20+%; x? tod sin 1/ R x? 1gö sin 1/ Bemerkungen PR ETES НЕЕ —— anale о Sin я == Р.-Кт. 270° |t-+k 5 - > чм has mm mm 675196 10000] 10000 тт тт тт тт 65.6185 о 0.0000 0.0000 0.0500 62.6063 0] + 3.0125 — 0.0013 + 3.0112 Luft 1. 62.0832 + 3.5362 — 0.0806 + 3.4556 90.0750 —24.4555 — 0.0094 — 24.4649 90.0570 — 24.4381 — 0.0690 — 24.5071 84.9080 — 19.2893 0.0000 —19.2893 34.8378 —-30.7804 0.0000 —30.7804 74.3930 — 8.7734 73.9365 — 8.3112 — 8.3073 73.4610 7-8374 72.9080 7.2900 72.4540 6.8186 — 6.8227 71.9840 6.3596 71.4815 — 5.8562 71.0195 — 5.3889 — 5.3900 70.5510 — 4.9249 69.9895 4.3728 69.5335 — 3.9070 — 3.9079 69.0730 3.4439 68.5300 — 2.9158 68.0840 — 2.4483 — 2.4473 67.6020 1.9778 Trabant — Jupiterscentrum. Ye VX | Mittel. \F'atur—v2) |7 (ra) eie-222) 7] 73-7620 1] — 8.1482| -+0.1591 72.2770 |+17|+ 1] — 6.6651| -+0.1571 # 70.8445 1| — 5.2308] -+0.1592 | -+0.1605 | -+0'1603 | -+0:0001 +-0/0011 00000 | -+0'1615 69.3610 |+19] 0|— 3.7468| <+0.1611 67.8960 9] — 2.2818] -+0.1655 73-1670 ©] — 7.5536] 0.7537 71.6845 |+16] ©] — 6.0698| -+0.7529 4 70.2535 |-+21 0] — 4.6400| -н0.7500 | -+0.7548 | -+0.7536 | -+0.0003 —+-0.0042 0.0000 | -+0,7581 68.7645 |+18| 0|— 3.1498| -+0.7581 67.3045 |+13| 0] — 1.6880] -+0.7593 74.4450 |-+18|+ 1|— 8.8334| — 0.5261 72.9630 |-+19|-= 1] — 7.3486] —0.5259 3 71.5305 |-+-17|- |— 5.9163| —0.5263 | —0.5240 | —0.5232 | —0.0002 — 0.0929 0.0000 | —0.5263 70.0430 |-+22|- 1] — 4.4298] — 0.5219 ; 68.5790 |+19|+ 1] — 2.9672| —0.5199 | 71.4720 |+15 — 5.8568] -+2.4505 8| 69.9990 |+19 — 4.3788] -+2.4439 68.5570 |+16 — 2.9392| -+2.4508 | -+2.4514 | -+2.4477 | 0.0009 —-0.0107 0.0000 | -+2,4593 67.0710 |-11 — 1.4528] -+2.4551 65.6080 |+13 + 0.0092| -+2.4565 abare Decldif: M—Centrum — + 3.0033 f°5 = 0.99850 | N— » —=+ 3.4505 . j . © » ——24.4312 fs —0.99801 5 —=—0,00013 X i5 = —0:4 — » = —24.4667 У » =—49.2638 f'5 = 0.99849 Js = —0.00009 W—- » =-+-30.7308 \ dy = -+20°10'0 3+ 22 Е. Renz, 30 D. 1896. Februar 10. 4! № De: —- — — | Scalenablesung. Helsingforser Sternzeit й | Object. а ae u et “ Bilder. | | P.-Kr. 0° | $+ { P.-Kr.180° | $5 3 der Aufnahmen. Mittel. eo | | mm mm_| mm | mm 10000] шт 10000] 10000 тт тт Cir. | 66,8368 61.5468 Ss 66.8355 | 8| 61.5453 |+10| о 0.0000 2—3 M 71.7815 |11| 56.5960 |+ 9] o]+ 4.9478 2 N 27.8820 |+21| 100.5073 |+ 3|+ 7| —38.9560 PR Ce 2—3 Q 80.3505 |-+22| 48.0330 |+30|— 4|+-13.5130 8 32 59 3 В 30.2940 |-+32| 98.0822 |+11|H+-19] —36.5362 8: У 66.5295 |-+19| 61.8535 |-+17| 0|— 0.3069 2 т 67.6825 |+30| 60.7020 |+24| ©] -н 0.8456 5 %а | 77-4390 |+ 8| 50.9450 |HI0 -+10,6019 @ | 77.9340 |-- 8| 50.4710 |#+ 5 +-11.0866 +-11.0865 87 NASA 3—4 C2 78.4235 |+ 8| 49.9920 |+ 5 +-11.5709 4b | 77.4245 + 9] 50.9620 |-10 -+-10.5862 b, 77.9400 |+ 9| 50.4625 |+ 5 11.0940 11.0885 35 44 3—4 bo 78.4275 |+ 9| 49-9675 |+ 5 11.5852 % Co | 77-4570 + 9| 50.9385 |+10 -+10.6142 р LH бо 77.9360 |+ 9| 50.4690 |+ 5 +11.0887 +-11.0930 36. 122 8 36 21 2—3 Co 78.4175 |+ 9| 49.9760 |+ 5 —11.5760 2% dy | 77-4485 |+ 9] 50.9600 |+10 —+10.5992 de | 77.9445 | 9| 50.4680 |+ 5 —11.0934 —=11.0919 36 59 2—3 do | 78.4215 |+ 9| 49.9655 |+ 5 11.5832 Фев | 77.4295 |10| 50.9655 |+11 +-10.5870 € 77.9375 |+-10| 50.4795 |+ 6 +-11.0840 —11.0841 31 #27 3 во 78.4285 |+10| 49.9770 |+ 6 11.5810 Trabant — Jupiterscentrum. ee | Mittel. |o(er—22) Joie] Ph. | Да cos $ тт тт Та | 76.4825 |+ 7| 51.8955 |+11 + 9.6483| —1.4382 1—2 b | 76.4790 | 8| 51.8955 |1 + 9.6466] —1.4419 1—2 с | 76.4815 |+ 8| 51.8960 |+11 + 9.6476] —1.4454| —1.4453| —1:4428 | —0:0003 | —0:0003 —1'4428 | 2—3 а | 76.4730 | 8| 51.9050 |+12 + 9.6388| —1.4531 —2 е 76.4700 |+ 9| 51.9070 |-+12 + 9.6364] — 1.4479 1—2 Па | 80.9505 |+14| 47.4250 |+ 9|— 1|-14.1179] +3.0314 1—2 b | 80.9540 |-+14| 47-4210 |+ 8|— 1|+-14.1217| +3-0332 1—2 с | 80.9570 +15] 47.4185 |= 8]— 1| +14.1245] +3.0315 | +3.0321 +-3.0268 | —0.0906 | —0.0003 | -+3,0259 | 2—3 а | 80.9530 |+ı5| 47.4205 |-+ 8]— 1|-+14.1215| -+3.0296 2 e 80.9520 |-+16| 47.4250 |+ 9|— 1]+14.1188] -+3.0347 2 Ша | 72.6620 |+14| 55.7130 + 5.8302| —5.2563 1—2 b | 72.6635 |-+14| 55.7135 |— + 5.8308] —5.2577 1—2 e | 72.6660 |-+15| 55.7085 + 5.3346] —5.2584 | —5.2589 | —5.2497 | —+0.0011 | —0.0003 —5,2489 | 1—2 а | 72.6600 |-+15| 55.7150 + 5.8282| —5.2637 : 1—2 е 72.6570 |-+16] 55.7170 + 5.8258] —5.2583 1—2 IV a | 87.5500 |— 6| 40.8315 |-+25|— 2| 20.7125] 9.6260 1—2 b | 87.5510 |— 6| 40.8260 |-+24|— 2] 20.7158] 9.6273 Ä 2 е | 87.5530 |— 6| 40.8290 |+24|-— 2|-+20.7153| +9.6223 | +9.6242| -+9.6073 | —0.0019 | —0.0003 9,6051 | 2 а | 87.5510 |— $| 40.8355 |+-24|— 2]+20.7111] 9.6192 2 e | 87.5480 |— 5| 40.8345 |+24|— 2]+20.7101| +9.6260 2 Scheinbare ЖАШ: M—Centrum = -+ 5:2699 F? «= 0.99824 —1°4 = —0.00041 N— » — —41.4074 | Q— » = -+14.3264 fa = 0.99796 —м ——0.00041 X = 14 R— » — —38.7069 Мег. === I У » = — 0,3187 Те = 120 W—- » — + 0.8861 f'x = 0.99824 Jy = +0.00080 ay = 8" 173 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 23 1396. Februar 10. he Decl. “Scalenablesung. Bemerkungen 2 2 AT el nt ds ar: or er я is sin 1 y—z198 sin 1 zur Aufnahme. i x. 900f P.-Kr. 270° mm | mm 10000] 10000 mm mm mm 65.6200 67.1360 0] — 1.5171 0.0000 — 1.59171 64.1292 — 0.0013 + 1.4863 63.5835 — 0.0806 + 1.9548 91.6048 — 0.0094 — 25.9920 Luft 1. 91.5615 — 0.0690 — 26.0142 86.4292 0.0000 | —20.8117 36.3535 0.0000 +-29.2652 64.5570 + 64.1040 + + 1.5278 63.6415 + 63.0895 +- 62.6350 En + 2.9896 62.1825 Eu 61.6450 + 61.2010 1 + 4.4250 60.7540 + 60.1920 + _ 59.7570 в + 5.8845 59.2950 =; | 58.7510 + _ 58.3120 —- + 7.3212 57.8550 + Е к Trabant — Jupiterscentrum. 3 у T и-—у» | Mittel. |/’з иглу |Ist@—anler-| ph | 48 mm mm 63.7325 + 0.3564 62.2670 + +-0.3582 60.8265 + +0.3654 | -+0.3617 | -+0!3611 | —0!0005 —=0'0017 0:0000 | —+0:3623 59.3685 + -0.3619 57-9275 + —0.3666 64.8825 + —0.7978 63.4199 =. — 0.7944 61.9810 == —0.7909 | —0.7945 | —0.7932 | -+0.0012 | —0.0041 0.0600 | — 0,7961 60.5260 == — 5.7971 59 0840 + —0.7925 62.7195 ie +-1.3645 61.2485 + +-1.3720 | 59.8140 + +1.3772 | -+1.3709 | -+1.3687 | —0.0020 | -+0.0049 0.0000 | -—+1,3716 58.3580 + +-1.3705 56.7225 + +1.3702 66.5525 — —2.4638 65.0925 + — 2.4662 63.6525 | + — 2.4602 | —2.4633 | —2.4592 | -#0.0037 —0.0165 0.0000 | —2,4720 62.1980 — —2.4643 60.7595 + —2.4622 M—Centrum— + 3/0033 1°з = 0.99837 i°3 — +-0.00036 N— » =+ 3.4507 + | 3 Q— » ——244316 fs = 9.99789 $4 = 0.00056 X в =-+ 1.2 Е— » = — 24.4670 У » =-—192641 Г’ = 0.99837 Тз = -+0.00038 W— ь —=-+30.7314 $ = +20° 26.0 24 Е. Renz, 31 A. 1896. Februar 11. 7 Hi À Scalenablesung. Helsingforser Sternzeit Bilder, | Object. x : P.-Kr. 0° |5 Р.-Кт.180°| +5 der Aufnahmen. Mittel. В 30000 une.) Ctr, | 622892 |"" | 661495 | I | т. Ss 62.2382 | +10] 66.1485 |-+19 0 0.0000 2—3 M 67.1890 |+ 9| 61.1938 |+I1 + 4.9526 2—3 N 23.2755 |+26| 105.1138 — 38.9614 PER LESER 3—4 verwaschet Q 75.7573 |-+18| 52.6345 13.5164 8$ 19 20 3 В 25.6955 |+35| 102.6792 —36.5338 $ Я и 61.9348 |-+17| 66.4468 — 0.3008 A 2. Я W | 63.0785 |-+21| 65.3085 0) + 0.8395 3 unterexp. « 2% dy | 46.9050 |-+12| 81.4850 2| —15.3350 @ | 47.3845 |-+12| 81.0145 2| —14.3599 —14.8609 8 и 3 &o | 47-8580 |+23| 80.5450 2] —14.3878 я % by | 46.9740 |+11| 81.4210 |-+16|-+ 2] —15.2684 D, 47-4430 |+11| 80.9640 |-+16|-= 2] — 14.8054 — 14.8022 277022 3 b, 47.9105 |+22| 80.4875 |-+16|- 2] —14.3328 с 46.9590 |-+11| 81.4260 |+15|-+ 2) —15.2784 с. 47.4270 |+11| 80.9795 |-=15|-= 2| —14.8211 — 14.8166 az sh 25” 48° |3 Co 47.8990 |-22| 80.5110 |-+15|- 2] —14.3503 2 dy | 46.9360 |109] 81.4470 |+15|+ 1| —15.3005 de | 47.4210 [+10] 80.9860 |-+-15|-+- т| —14.8275 —14.8318 27. 138 2—8 do | 47.8850 |--21| 80.5310 |-+15|-= 1| —14.3674 Zen | 46.9710 |+ 9] 81.4270 |-+14|-= 1] —15.2730 | ес 47.4250 |+ 9] 80.9785 |+14|+ т|—14.8218 —14.8153 28! ‹ 113 2 CA 47-8940 |+20| 80.5075 |+14|+ 1] —14.3512 Trabant — Jupiterscentrum. 4 — 0 | Mittel. ща) иг зд Ph, | Au cos à mm тт Та 49.3245 |+16| 79.0515 | 9|-+ 1| —12.9079] 1.9530 2—3 b | 49.3745 |+16| 79.0060 |-н 8|-= 1] —12.8601| -+-1.9421 - 2—3 e | 49.3745 |+15| 79.0050 |+ 7|-+ 1] —12.8592| -+1.9570 | -+1.9543 | 1.9506 | -0:0009 | —0:0003 | +19512| 2 а | 49.3605 |-+15| 79.0180 | 7|-= 1] —12.8731) -+1.9587 2—8 е | 49.3790 |+14| 78.9990 | 6|+ 1] —12.8544] 1.9609 ; 2—3 Па 48.2795 |+22| 80.0950 |+-I1|-+ 1| —13.9520] -+0.9089 2 b | 48.3240 |-+22| 80.0540 |19|-= 1) —13.9092| +-0.8930 2—8 с | 48.2980 |+21| 80.0780 |-+ 9|-+ 1] —13.9342| 0.8824 | -+0.8887 | -н0.887о | -#0.0005 | —0.0003 | 0.8872 | 2—8 4 | 48.2840 |+21| 80.0935 |-+ ol 1| —13.9489] 0.8829 < 2 € 48.2940 |+20| 80.0835 |+ 8|+ 1] —13.9289] -+-0.8764 ; 2—3 Ша | 42.8610 |-+-25| 85.5115 |+ 1] 3] —19.3686| —4.5077 2 b | 42.9100 |-+24| 85.4650 | 1|- 3| —19.3214] —4.5192 2 с | 42.9085 |-+24| 85.4650 ol+ 3| —19.3216| —4.5050| —4.5073 | —4.4988 | —0.0022 | —0.0003 | —4,5013 | 2 d | 42.8960 |-+23| 85.4790 |— т|- 2] —19.3350] —4.5032 : . 2 e 42.9135 |-+23| 85.4600 |— 1|- 2] —19.3167| —4.5014 , 2 IV a 56.3715 |+ 1| 72.0115 |-+13| 0] — 5.8654] +8.9955 = bs 2—3 b | 56.4170 |+ 1] 71.9685 |-12| o|— 5.8212| 8.9810 D 2—3 e | 56.4055 o| 71.9785 |-+12] o|— 5.8320| +-8.0846 | -+8.9863 | -+8.9694 | —+0.0042 | —0.0003 | 8.9665 | 2—3 d | 56.3940 ©] 71.9945 |+11| oo] — 5.8456] -+8.9862 2—3 е 56.4085 ol 71.9795 |+и| 0] — 5.8309] 8.9844 у 3 Scheinbare ÆRdiff: M— Centrum = + 52699 Fa =0.99812, —i° „ = —0.00017 | N=. » = —41.4074 3 0— » — -+14.3264 Га = 9.99784 —iy =- 0.00017 X = + 06 R— » = —38.7069 Refis = о V— USE 0,3187 HA Try =— 162 W— » = + 0.8861 Га —=0.99812 Ju. ‘ = — 0.00179 ау = 8 16.8 65.1700 62.5508 59.5413 59.0162 87.1110 86.9915 81.8440 31.7673 53-7545 54.2880 54.7400 55.4640 55.9100 56.3409 56.8900 57-3270 57-7580 58.3320 58.7720 59.2030 59.8020 4| 60.2330 {| 60.6680 54.7900 56.3985 Е 60.7370 4.5805 и 1840 57.6090 59.0565 60.5215 61.1250 62.5860 У t+k 10000} 10000, + 9 --15 +27|— + 1|+ +-10|-+- +10|+ + 6|-н + 6]-+- + 6|-+- + 6+- +16|+- +16|-- +-12|+- +-12|+ +-17|+- +17|+ Æ2II +21 +17|+ CRC O|+- 4 +12] +10 +19] —10 1896. F'ebruar 11. = ol + 2.9211 С] + 5.9268 3] + 6.4563 —21.5382 —21.5225 —16.3736 +33.7042 -+11.6220 +11.1910 -+-10.7385 -+10.0160 + 9,5780 + 9.1407 + 8.5875 + 8.1575 + 7.7212 + 7.1389 —= 6.7046 + 6.2720 + 5.6716 + 5.2466 + 4.8115 I -+10.6766 -+ 9.0693 + 7.6386 —= 6.1919 + 4.7301 —10.8865 -+ 9.2820 + 7.8574 + 6.4088 + 4.9466 +-12.4192 —10.8138 + 9.3868 + 7.9366 + 6.4744 + 8.8232 + 7.2158 + 5.7938 + 4.3440 + 2.8834 е Decldifr: re —+ 3/0033 V— = pe Ce SON = —24.4316 = —24.4670 = — 19.2641 =-r30.7314 dy = -+20° 27'7 3ar. Физ.-Мат. Отд. Пес]. 9+9 +9: —11.1838 + 9.5782 + 8.1554 + 6.7052 + 5.2432 тт тт —0,5072 —0.5089 —0,5168 —0.5233 —0.5121 —0.2973 —0.2962 —0.2980 —0.2964 —0.2966 +1.2354 +-1.2356 +-1.2314 +-1.2314 —+1.2312 —2.3606 —2.3624 — 2.3616 —2.3612 —2.3598 —0.5117 —0.2969 41.2330 — 2,3611 128 = 0.99836 fs —0.99787 fs =0,99835 2 — 58 sin 1’ mm ЕЕ —0:5109 | —0'0001 —0.2964 0.0000 -+-1.2309 | -+0.0002 — 2.3572 | —0.0004 $2; = —0.00006 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTORRAPHISCHEN AUFNAHMEN. RS « , y— ztgösinl mm + 2.9211 + 5.9255 + 6.3757 — 21.5476 —21.5915 — 16.3736 +-33.7042 Trabant — Jupiterscentrum. Е т vva | Mittel. |Яз (иги Ja (er—22)|-(œrt-222)] -+0.0029 0.0014 —0.0084 —+0,0101 Хх ig = —0:2 Bemerkungen zur Aufnahme. Wolken ziehen vor- über. 0'0000 | —0'5081 0.0000 | —0,2950 0.0000 | -+1.2227' 0.0000 | —2,3475 4 31 В. Object. mm Ctr. | 62.4334 5 62.4325 M 67.3805 N 23.4702 Q 75-9530 Е 25.8958 18 62.1298 т 63.2760 ZA 50.5855 Ag 51.0650 Go | 51.5425 2b | 50.5820 be 51.0675 bo | 51.5365 Ч Си, 50.5935 Ce 51.0680 Co 51.5470 %а | 50.5900 de | 51.0710 do | 51.5540 %ер 50.6130 ee 51.0810 CA 51.5560 Та | 49.1965 b | 49.1895 € | 49.2030 d | 49.1995 e 49.2160 Па | 54.3770 b | 54.3730 € | 54.3770 d | 54.3725 е | 54.3890 Ша | 56.5120 ‚6 56.5025 € 56.5100 d | 56.5070 е 56.5225 IV а | 51.9275 Ь | 51.9270 € 51.9280 d | 51.9230 e 51.9360 Scalenablesung. | Scheinbare Adiff: | P.-Kr. 0° | = Р.-Кг.180° 65.9592 65.9582 61.0005 104-9212 52.4410 102.4822 66.2500 65.1144 77-8040 77-3460 76.8560 77.8120 77-3355 76.8600 77.8025 77-3375 76.8545 77.8050 77-3320 76.8425 77.7880 77.3260 76.8520 79.1750 79.1820 79.1720 79.1750 79.1610 73.9995 74.0015 73-9945 74.0015 73.9885 71.8660 71.8710 71.8625 71.8670 71.8520 76.4545 76.4605 76.4525 76.4645 76.4480 F. Renz, 1896. Februar 14. № Helsingforser Sternzeit t+k der Aufnahmen, | Mittel. _mm_| mm 100001 10000 an +10] о 0.0000 4 +10] 0J-+ 4.9528 3—4 + 7|+18]| —38.9599 FRE = ui —=20]— 2] -+13.5186 6 43 27 3—4 verwasch —+13|--19] —36.5272 4 verwaschen — 0] — 0.2971 3—4 m ol + 0.8432 3—4 unterex . | — 11.8462 И “113776 —11:3725 6 45 39 2 — 10.8938 — 11.8520 — 11.3710 —11.3739 46 16 2 — 10.8988 — 11.8416 — 11.3718 — 11.3681 46 51 6” 46” 53° — 10.8908 | —11.8450 —11.3676 —11.3647 4717038 2—3 —10.8814 —11.8245 — 11.3596 — 11.3564 48 6 2 — 10.8851 Trabant — Jupiterscentrum. REN | Mittel. Later) Jutr-va)| Ph. | Аа cos à mm mm — 13.2260] —1.8535 2—3 —13.2330] —1.8591 3—4 —13.2213| —1.8532| —1.8557| —1'8523 | —0!0007 | —0'0005 | —1:8535 | 3 —13.2246] —1.8599 ; а —13.2093| —1.8529 2—3 — 8.04881 3.3237 3 — 8,0518) -+3.3221 3 — 8.0464] -+3.3217| -+3.3198| #+3.3137 | 0.0013 | —0.0005 | +3,3145 | 2—8 — 8. +3.3127 2 — —+3.3190 2 _ +-5.4583 2—3 — 5.4524 2 N — 55.4546 | +5.4554| -+-5.4454 | -+0.0020 | —0.0005 | 5,4469 | 2—3 eiförm — +5.4475 2—3 ER +5.4544 ] 2 + —10.5004| —+-0.8721 3 + 8 —10.5037| +-0.8702 3 —10.4992| +-0.8689 | -+0.8663 | -+0.8647 | -+0.0005 | —0.0005 | 0,8647 | 3 + 8 —10.5077| -0.8570 8 + 9 — 10.4930] <+-0.8634 5 M—Centrum = + 52699 f°4 = 099818 —1° y = —0.00017 N— › ——41.4077 : | Q— » = +14.3264 fu =9.99787 — =— 0.00012 x = +04 R— » = —38.7072 Refr. = — 4 V— » = — 0.3187 Try =— 124 W— » = + 0.8861 Ги =0.99817 Je = — 0.00140 ay = 8% 154 re POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 27 1296. K'ebruar 14. Decl. 2 2 B k Ре 65.1700 тт тт тт 64.0368 0.0000 — 1.4369 Luft 3—1. 61.0235 — 0.0013 + 4.4455 60.5058 — 0.0806 —+ 4.8849 88.4928 — 0.0094 —23.0278 88.4790 — 0.0690 —23.0808 83.3228 0.0000 — 17.8554 33.2510 0.0000 +-32.2233 63.6415 64.0735 + 1.3993 64.5215 65.0260 65.4690 + 0.0105 65.9105 66.5170 66.9595 — 1.4797 "67.4010 68.0170 68.4535 — 2.9771 68.8915 69.4890 69.9210 — 4.4443 _ 70.3540 . Trabant — Jupiterscentrum. 3 T - ° | уу» | Mitten. [far] rate) er) Pa ai тт тт | 63.5770 -+ 1.8888] -+0.4895 | Br —- 0.5046| -0.4941 | : b | 66.4560 — 0.9891| —+0.4906 | -+0.4919 | 04911 | +-0!0005 — 0.0025 0'0000 | -+0:4892 19] 67.9480 — 2.4828| -+0.4943 69.4190 — 3.9532] -+0.4911 64.9740 + 0.4899] -— 0.9094 66.3575 — 0.8948| —0.9053 67.8480 — 2.3854| —0.9057 | —0.9064 | —0.9049 | —0.0008 | -+0.0035 0.0000 | — 0,9022 69.3460 — 3.8822| —0.9051 70.8130 — 5.3508] — 0.9065 65.5070 — 0.0432| —1.4425 66.8905 — 1.4276] —1.4381 | 68.3770 — 2.9174] —1.4377 | —1.4403 | —1.4378 | —0.0014 | -+0.0051 0.0000 — 1.4341 | 69.8830 — 4.4200] —1.4429 71.3470 — 5.8848] — 1.4405 644175 + ASE —0.3461 .8010 — 0.3316] —0.3421 k ^- ; se — + ton SAIS —0.3426 | —0.3420 | —0.0002 +-0.0010 0.0000 — 0,3412 68.7885 — 3.3192| —0.3421 — 4.7843| — 0.3400 bar Decldiff: Rue sen =-+ 3/0033 193 = 0.99834 8 = —0.00028 — 2 + 3.4507 в Q— 2 =-24.4318 Sa =0.99781 ig = —0.00016 x в=—0.5 R—- » — — 24.4671 у У— » =-—19.2642 Ла = 0.99831 Jg = — 0.00025 W— » — -+30.7316 dy =-+20° 32/3 28 Е. Renz, 31 C. 1896. Februar 17. № Scalenablesung. Helsingforser Sternzeit 4w+#c+#o P.-Kr. 0° kl P.-Kr. 180° 1-+-% 3 der Aufnahmen. Mittel. mm mm. mm mm 10000 mm 10000] 10000 mm mm Ctr, | 62.4264 65.9612 5 62.4255 |+ 9| 65.9595 |-+17| © 0.0000 De M 67.3755 | 9| 61.0100 [+10] o|+ 4.9501 2 М 23.4630 |-+25| 104.9272 |+ 7|-+18| —38.9620 а, 8 Q 75.9555 |-+20]| 52.4318 |+21|— 3|+13.5289 9 56 20 3 R 25.8960 |-+37| 102.4822 |-+-14|-+-20| —36.5226 3 У 62.1308 |-+19| 66.2535 |417] 0|— 0.2938 5 м W | 63.2520 |+21| 65.1302 |+30| o|-+- 0.8278 3 ищегехр. | Фа | 76.3470 |+12| 52.0550 |--14]— Т|-+13.9132 ag | 76.8060 |+-12| 51.5975 |-+-14|— 1|-+14.3714 14.3719 D 50039 2 ao | 77-2670 |+ı12| 51.1395 |-13|— 1]+14.8310 2b | 76.3240 |-+10| 52.0680 |-+14|— 1|-+1т3.8951 - bu | 76.8045 |+10| 51.6045 |+-14]— 1|-+14.3671 -+-14.3615 AU | 2—3 6, | 77-2575 |#+10| 51.1470 |+13]— 1|-+14.8224 YC 76.3550 [+10] 52.0525 |+-13|— 1|-+13.9184 | ce 77.8100 |+10| 51.5990 |-+13|— 1] -+14.3726 -+-14.3753 51 53 9° 5155" 3 бо 77.2650 |+10| 51.1295 |+121— 1) -+-14.8350 % dyp | 76.3380 |H-10| 52.0615 |-+12|— 1|+13.9954 с | 76.8035 |+10) 51.6040 |+12|— 1|-+14.3670 —-14.3647 ЖЕ 2—3 do | 77-2555 |+-10| 51.1465 |-+11|— 1|-+14.8218 Zew | 76.3435 |+ 9] 52.0545 |-+12|— 1|-+13.9116 CA 76.8030 |+ 9 51.6065 |-+12|— 1|+-14.3654 +14.3666 Bruns 2—3 eo | 77-2585 |+ 9] 51.1475 |-+11]— 1) +-14.8227 Trabant — Jupiterscentrum. 2 — y | Mittel. Рыба) Tätve—v) Ph. | Au cos à CR RETTEN EEREEREEREEEEEERERETEEREEIEEEEE VERHEERSTEHREESEETETEEREEREER TIRREEEEREREEREHTTTTETTERTETN mm mm Та | 75.6065 |I4-10| 52.7730 |-10]— 1]-+-13.1840| — 1.1879 2 etwas e ig D | 75.5975 |+ 9| 52.7840 |+- 9|— 1]-1-13.1740| — 1.1875 7 j с | 75.6090 I+ 8| 52.7710 |+ 9l— 1|-+13.1862] —т.189т | —1.1910| —1'1888 | -+0/0005 | —0!0006 | —1:.1889 | 2 d | 75.5935 I4- 7| 52.7860 |-н 8|— 1] -+13.1719] —1.1937 2 4] e | 75.5910 |+ 7| 52.7860 | 8|— 1] -+-13.1698| —1.1968 2 etwas elli Па | 79.6080 |+11| 48.7645 |+17|— 1] -1-17.1888] -+-2.8169 2 b | 79.6030 |+10| 48.7740 |--16|— 1|+17.1815| -+2.8200 1—2 с | 79.6240 [10] 48.7545 |-15]— 1|-+17.2018| -+2.8265 | -+2.8233 | -2.8181 | —0.0013 | —0.0006 | 2.8162 | 2 а | 79.6120 |+- 9| 48.7685 |-+15|— 1|-+17.1888| -=2.8241 1—2 е 79.6170 |+ 9| 48.7620 |--14]— 1] -+17.1956] 2.8290 2 Ша | 71.7395 |-+13| 56.6365 |+-12 + 9.3184] —5.0535 2 b | 71.7310 |+12| 56.6425 |--11 + 9.3116] —5.0499 | 1—2 e | 71.7455 |-+12| 56,6290 |+11 + 9.3256] —5.0497 | —5.0513| —5.0419 | -+0.0023 | —0.0006 | —5.0402| 2 4 | 71.7320 |+-11| 56.6435 |+-10 + 9.3117| —5.0530 1—2 е 71.7355 |-+11| 56.6380 |+10 + 9.3162| —5.0504 2 IV a | 68.2690 |-+19| 60.1135 |-+17 + 5.8452] —8.5267 2 b | 68.2630 |+-19| 60.1200 |+16 + 5.8390] —8.5225 2 с | 68.2790 |-18| 60.1055 |+-16 + 5.8542] —8.5211 | —8.5249 | —8.5091 | -0.0037 | —0.0006| —8.5060 | 2 а | 68.2640 |-18| 60.1225 |+15 + 5.8383] —8.5264 2 € | 68.2650 |-+18| 60.1220 |-+-15 + 5.8390] —8.5276 2 Scheinbare Adiff: M--Centrum = + 52700 Fra = 999814 —® = -+0.00020 N— » = —41.4079 Q— ь —=+14.3265 fax == 099784 — == +0,00016 x %=—05 Е » = —38.7074 Refr. = + 4 У— » = — 0.3188 Try =+ 157 W— » = + 0.8860 Го = 099814 Ju = +0.00177 ` а» = 8 14.0 Decl. в: Scalenablesung. ИО +2 Рае P.-Kr. 90° „= P.-Kr.270°| + 65.4698 EG a 65.4682 62.4608 Oo] + 3.0081 61.9438 |-+26|— 2] + 3.5274 89.9308 |— 4|-+ 5] —24.4576 89.9230 | 8]-14| —24.4502 84.7620 |— 2|-+ 2| —19.2924 34.6830 |-+20]— 8] 30.7874 73.7880 |-17|- 1| — 8.3122 73.3670 |-18|-= 1] — 7.8857 — 7.8854 72.9320 ° |-+18|- ı| — 7.4582 72.3180 |+16 — 6.8417 71.8840 |+16 — 6.4030) — 6.4108 71.4620 |+16 — 5.9877 70.8630 |-+17 — 5.3884 70.4410 |+21 — 4.9592 — 4.9597 70.0060 |-+21 — 4.5316 69.4890 |-+18 4.0128 69.0540 |+18 3,5796 — 3.5785 68.6335 |-+18 3.1493 67.9810 |+23 — 2.5050 67.5490 |+-23 — 2.0695 — 2.0772 67.1390 |+13 — 1.6570 рр | Mittel. mm mm 73.0690 — 7.5992| +-0.2862 71.5970 — 6.1252| -+0.2856 70.1425 — 4.6756] —+-0.2841 | -+0.2848 68.7650 — 3.2972] -+0.2813 67.2580 — 1.7904| -+0.2868 74.0680 — 8.6094| —0.7150 73.5960 — 7.1271| — 0.7163 71.1430 — 5.6780] —0.7183 | —0.7193 69.7660 — 4.3007| —0.7222 68.2705 — 2.8017| —0.7245 72.0750 — 6.6092| -+1.2762 70.6000 — 5.1365] -+1.2743 69.1490 — 3.6848| -+1.2749 | 1.2745 67.7705 — 2.3076] 1.2709 66.2660 — 0.8010] -+1.2762 71.2820 |+13 — 5.8136] -2.0718 69.8060 |-+17 — 4.3394] -+2.0714 68.3590 |+19 — 2.8908] -+2.0689 | 2.0699 66.0810 |+9 — 1.5116] -+2.0669 65.4740 |-+17 — 0.0068] -+2.0704 heinbare Decldif: M—Centrum = + 3.0033 195 = 0.99833 N— » = + 3.4508 Q— » = —24.4320 fs = 0.99782 Е— » = —24.4672 У » =—19.2643 f'a = 0.99833 W— » = +-30.7318 dy = +20° 37:0 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1396. Februar 17. mm mm 0.0000 0.0000 — 0,0013 + 3.0068 — 0,0806 + 3.4468 — 0.0094 — 24.4670 — 0.0690 —24.5192 0.0000 —19.2924 0.0000 +-30.7874 Trabant — Jupiterscentrum. у т F'avr—-y2) | Ts(tr—23) | Не-а) з] -+0'2843 | -+0!0003 —+0'0018 — 0.7181 | —0.0007 —0,0049 +-1.2724 | 0.0013 -+0.0065 +-2.0664 | -+0.0021 0.0094 325 = —0.00026 3 =-— 0.00035 X ig = —12 Js = —0.00025 Bemerkungen zur Aufnahme, Luft 1. 00000 0.0000 0.0000 4* Ai —+0:2864 — 0.7237 1,2502 +-2,0779 30 Е. ВЕми, 31 D. 1896. Februar 18. AR Scalenablesung. Helsingforser Sternzeit À Object. SEE PRE $ x ARRETE mA Bilder, P.-Kr. 0° ++ P.-Kr. 1809 1-5 8 der Aufnahmen, Mittel. | тт тт mm 10000 10000] 10000 Cr. | 624141 65.9741 ci Эр Ss 62.4132 |+ 9| 65.9730 |+1I1 [6) 0.0000 2 4 M 67.3662 | 8| 61.0185 |10] 0] + 4.9538 2—3 ellipt. 7 N 23.4538 |-+25| 104.9345 — 38.9578 Е 3—4 ум Q 75.9420 |-+2I| 52.4470 —+13.5268 8 Bord 3 В 25.8810 |-+37| 102.4940 — 36.5228 2—3 ellipt. 14 62.1201 |-+20| 66.2640 — 0.2918 2 я т 63.2460 |+21| 65.1402 0] + 0.8324 3 %G | 77.3220 |+ 9| 51.0715 1] 14.9051 pes ir À ; Ag 77.7565 |+ 50.6435 —=15,3363 15.3426 8 Вей то 1 au | 78.2060 |+ 8| 50.1935 -+15.7863 2b | 77.3150 [+ 9| 51.0825 |+10]— 1] +14.8961 LA 77.7580 |+ 8| 50.6485 |+10l— 1|-+15.3346 15.3332 а À 1 b, 78.1895 |+ 8| 50.2120 |+ 5|— 1|-+15.7688 Фе | 77.3140 |+10| 51.0840 |+rol— 1|+14.8949 за Ce 77.7520 |+ 9| 50.6505 |--rol— 1] -+15.3306 15.3315 391025 8 39747 1 бо 78.1900 |+ 9| 50.2120 [+ 5|— 1|-+15.7691 % dy | 77.3205 |-+-10| 51.0790: |+ то|-— 1| -+14.9006 de | 77.7585 | 9 50.6375 |+10]— 1|-+15.3404 15.3354 40 8 1 do | 78.1860 |+ 9] 50.2160 |+ 5|— 1[-+15.7651 Zew | 77.3135 [+11] 51.0825 |+11|— 1} -+14.8954 CA 77.7500 |[+10| 50.6525 |+11|— 1] +15.3286 -+15.3315 40 59 1 eo | 78.1915 |-+-10] 50.2110 |+ 6[— 1] +-15.7704 Trabant — Jupiterscentrum. т | Mittel. Иа) аби Ph. | До cos d mm mm \ Та | 79.2350 |+ 6| 49.1510 |+14l— 1] 16.8215] -+-1.4789 2 etwas ellipf b | 79.2205 |+ 6| 49.1640 |+-13|— 1] +16.8078| -#1.4746 2..3 »! € | 79.2190 |+ 7| 49.1690 |+13|— 1] +16.8046! +1.4731 | 1.4713 | -=1'4686 | —0.0008 | —0'0007 | +-1:4671 | 2 d | 79.2145 |+ 7| 49.1700 |+13l— 2] 16.8018] 1.4664 2—3 е 79.2085 |+ 7| 49.1775 |-+14|— 2] 16.7950] 1.4635 2 Па | 79.3325 |+ 6| 49.0540 |-+14|-— 1] -+16,9188| +-1.5762 2 etwas ellip b | 79.3290 |+ 6| 49.0580 |+13l— 1]-+16.9150| -+1.5818 2 a с | 79.3340 + 7| 49.0540 |+13]— 1] -+16.9196] +1.5881 | +-1.5846 | +-1.5817 | —0.0007 | —0.0007 | -+1,5803 | 2 а | 79.3370 |+ 7| 49.0495 |+13|— 2] +16.9232] +-1.5878 2—3 е 79.3350 |-+- 7| 49.0530 |-+-14|— 2] -+16.9204| +1.5889 2 Ша | 72.9200 |-+13| 55.4580 |— 1 —+-10.5117| —4.8309 1—2 b 72.9110 |+14| 55.4680 |— т -+-10.5022] —4.83 10 2 etwas elli с | 72.9170 [+14] 55.4650 |— 1 —10.5068| —4.8247 | —4.8278| —4.8189 | -+0.0024 | —0.0007 | —4,8172 | 2 4 | 72.9165 |-+14| 55.4625 [6) —+-10,5077| —4.8277 3 2 etwas ellip e 72.9175 |[+15| 55.4650 о 10.5070] —4.8245 DT № IVa | 68.2520 |+19| 60.1300 |-+14 + 5.8412] —9.5014 2 b | 68.2440 |-+19| 60.1375 |+14 — 5.8335] —9.4997 2 с | 68.2425 |+20| 60.1390 |-+15 + 5.8320| —9.4995 | —9.5009 | —9.4834 | -+0.0044 | —-0.0007 | —9,4797 | 2 а | 68.2430 |-+20| 60,1380 |-+15 + 5.8328] —9.5026 2—3 e | 68.2410 |+21| 60.1415 |+16 + 5.83009] —9.5015 2—3 Scheinbare ВАШ: M—Centrum = + 52700 Fa = 0.99816 —i° y = -+0.000т5 N— » = —41.4080 Q—- » =-14.3265 fx = 099788 —iy = -0.00015 X y = —0!5 Е— » — —38.7075 Refr. = + т V— » = — 0.3188 Try =+ 168 W—- » — + 0.8860 Г’ = 099816 I, = —0.00184 h т ay = 8 13.6 *) Trabant I und II berühren sich. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 31 1896. F'ebruar 1s. Decl. %п+Фе+%, т ue 2 Bemerkungen у Ph Зет - — 7 1961 1 У— = 196511 zur Aufnahme. 65.4700 ne к ar ps 66.9505 — 1.4814 0.0000 — 1.4814 Luft 1. 63.9408 + 1.5268 — 0.0013 + 1,5255 Durch dünne Wol- 63.4218 + 2.0492 — 0.0806 + 1,9686 ken. 91.4108 — 25.9365 — 0.0094 — 25.9459 91.3975 — 25.9266 — 0,0690 —25.9956 86.2428 — 20.7726 0.0000 — 20.7726 36.1610 -+29.3090 0.0000 —+29.3090 65.3000 + 0.1777 64.8955 + + 0,5861 64.4730 = 63.8409 = 63.4370 Е + 2.0414 63.0305 + 62.3875 + 61.9920 + + 3.4920 61.5830 + 60.9195 + 60.5220 + + 4.9529 60.1280 + 59.4820 + 59.0860 + + 6.3953 58.6795 = Е 4 Trabant — Jupiterscentrum. a т Yt—Y2 | Mittel. Nawı-va)| Табе | ева) Ph. | 45 тт тт ©] — —0.4347 O| + —0.4382 р : Г ol + —0.4312 | —0.4324 | —0.4317 | —0!0003 — 0.0026 0.0000 | —0!4346 п + — 0,4283 : 1| + — 0.4299 о] +- — 0.3911 ©] + —0.3927 ©] + —0.3888 | —0.3908 | —0.3901 | —0.0003 — 0.0028 0.0000 | —0,3932 |- —0.3905 1l-+ —0.3907 + +1.2743 —- +-1.2692 + +-1.2734 | 1.2718 | —+-1.2696 | -+0.0009 | -+0.0069 0.0000 | -+1,2774 + +1.2703 + -+1.2718 + +2.3519 Es —+2.3470 + -+2.3499 | +2.3494 | -2.3454 | +0.0017 +-0.0110 0.0000 | -+2,3581 + +-2.3476 + —+2.3505 einbare Decldiff: M--Centrum = + 3:0033 f°3 = 0.99829 #° 3 = —0.00020 О === » О — 44ю fy =09 = MU = Е— » —24.4672 V— :» —19.2643 f’z = 0,99829 Js = —0.00018 W— » -+30.7318 32 Г. Rexz, 32 A. 1896. März 9. AR вы Scalenablesung. иен Helsingforser Sternzeit P.-Kr. 0° = P.-Kr.180° B der Aufnahmen. Mittel. mm mm | mm | un 1000| mm 10000] 1000| mm сиг, | 64.2977 64.0850 5 64.2968 |+- 9] 64.0842 |- 8 0 0.0000 3 M 69.2532 |+14| 59.1275 |+11 О] + 4.9566 3 N 25.3400 |-+27| 103.0465 |+ 6|-+-17| — 38.9568 ВА 2 A Q 77.8102 |+19| 50.5742 |-+18|— 2|-+13.5115 8 44 13 3—4 В 27.7578 |+32| 100.6148 |-+-11]+-18| —36.5320 3 У 63.9920 |+16| 64.3878 |+14| 9] — 0.3042 923 W | 65.1430 |-+28| 63.2362 |+25] o|+ 0.8472 3 ра 56.8340 |+12| 71.5460 |+-14 — 7.4624 a 57.3050 |-+12| 71.0875 |+-14 — 6.9977 — 6.9974 8" "N 3 ay | 57.7680 |+ 8| 70.6190 |+14 — 6.5322 %6 | 56.8400 |+-11| 71.5420 |+13 — 7.45974 be | 57.3105 || 71.0835 |+13 — 6.9930 — 6.9892 39 59 3 b, 57.7870 |+ 7| 70.6080 |+13 — 6.5172 #6 56.8450 |--11| 71.5360 |+13 — 7.4520 с, 57.3200 |+I1| 71.0735 |+13 — 6.9832 — 6.9806 40 36 8^ 40” 36° 3 cé 57.7940 |+ 7| 70.5940 |+13 — 6.5066 %а 56.8440 |+10| 71.5420 |+12 7.455 de 57.3160 |+-10| 71.0805 |-+12 — 6.9887 — 6.9864 CE 3 dy | 57.7810 |+ 6| 70.5980 |+12 — 6.5152 Ze | 56.8590 |+10| 71.5250 |+12 7.4394 ес 57.3345 |+10| 71.0630 |-+12 — 6.9707 — 6,9721 AL St 3—4 ео 57.7980 |+ 6| 70.5970 |+12 — 6.5062 Trabant — Jupiterscentrum. о | Mittel. Лии) (ии у») Ph. | Ac cos à mm mm Та | 58.4330 |-= 8| 69.9495 |+17 — 5.8650] 1.1324 3 b 58.4335 |+ 7| 69.9470 |+17 — 5.8636] 1.1256 у 3 с | 58.4430 |+ 7| 69.9400 |+16 — 5.8553] -#1.1253 | -+1.1254| 11234 | -+0':0004 | —0'0017 | +1:1221| 3 а | 58-4290 |+ 6| 69.9485 |-+16 — 5.8666] 1.1198 3 e 58.4490 | 6| 69.9320 |+-16 — 5.8484] +1.1237 3 Па | 58.2005 |-+ 8] 70.1815 |+17 — 6.0973| -+0.900т 3 b 58.2050 | 7| 70.1705 |+17 — 6.0896] +-0.8996 3—4 e | 58.2195 |+7| 70.1595 [+16 — 6.0768] -+0.9038 | -+0.9025 | -+0.9009 | -+0.0002 | — 0.0017 | 0,8994 | 3—4 а | 58.2090 |+ 6| 70.1600 |+16 — 6.0854| +0.9010 5—4 е 58.2305 |+ 6| 70.1450 |-+16 — 6.0641| -+0.9080 3 Ша | 53.8650 | 6| 74.5090 |+12 —10.4286| — 3.4312 3 b | 53.8650 |+ 5| 74.5060 |-+-II — 10.4272] — 3.4380 2—3 с | 53.8790 |+ 5| 74.4920 |+11 —10,4132] —3.4326 | —3.4356 | —3.4296 | —0.0009 | —0.0017| —3,4322| 3 d 53.8670 |-+- 4| 74.5060 |+-10 — 10.4262] —3.4398 N = е 53.8845 |+ 4| 74.4880 |+10 — 10.4084] —3.4363 3 IVa | 53.3680 |+10| 75.0110 |+13 —10.9280| — 3.9306 3 b 53.5765 |-+ 9] 75.0055 |+12 — 10.9210] — 3.9318 AA с 53.3880 + 9| 74.9945 |+I1 —10.9097| —3.9291 | —3.9291 | —3.9222 | —0.0012 | —0.0017 | —3,9251 | 3—4 d 53.3825 |+ 8| 75.0030 |-+I1I —10,9168| — 3.9304 Ben e 53.4030 |-+ 8| 74.9815 |+10 — 10.8957] — 3.9236 9—3 Scheinbare Adi: M-—Centrum = + 5'2700 Ха =0.99824 —® = — 0.00040 N— » = —41.4093 Q— » = +-14,3270 fa —0.99796 —1y = —0,00040 № = +14 R— » — —38.7087 Refr. = + I V— » = — 0.3187 Try =— 78 W— » = + 0.8860 Л’. = 0.99824 I =— 0.00117 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896, März 9. he. | Decl. я Scalenablesung. nt % 1-2 2 : 2 Bemerkungen — 8 y их — + 10631 1’ у— 196 sin № Е -K -90°| 2 P.-Kr. 270° ++ 8 x A u eu à pu # ы SR 62.9352 + 2.9170 0.0000 + 2.9170 Luft 3. Neblig. 59.9245 + 5.9246 — 0.0013 + 5.9233 59.3868 —= 6.4654 — 0.0806 + 6.3848 87.4038 —21.5508 — 0.0094 — 21.5602 87.3618 — 21.5126 — 0.0690 —21.5816 82.2270 —26.3776 0.0000 — 26.3776 32.1520 +3 3.6992 0.0000 —33.6992 56.3890 + 9.4740] , 56.8170 —+ 9.0442 + 9.0363 57.2630 + 8.5906 57.9020 + 7.9570 58.3405 + 7.5184 + 7.5172 58.7740 + 7.0762 59.3355 + 6.5266 59.7590 + 6.0951 + 6.0867 60.2140 + 5.6384 60.8090 + 5.0506 61.2400 + 4.6178 + 4.6148 61.6770 + 4.1761 62.2195 + 3.6417 3| 62.6435 + 3.2154 + 3.2100 9| 63.0805 + 2.7728 Trabant — Jupiterscentrum. Yı—ya | Mittel. u) |5 (1—2) Hart) Ph. ° 48 тт "mm + 8.7348| —0.3015 + 7.2132] —0.3040 + 5.7833] —0.3034 | —0.3023 | —0.3018 | -+0!0004 +-0:0008 | -+oloooı | —0/3005 + 4.3162| —0.2986 "| -= 2.9059] —0.3041 + 8.8600| —0.1763 + 7.3346| —0.1826 + 5.9040] —0.1827 | —0.1811 | —0.1808 | -+-0.0003 +-0.0006 | +0.0001 | —0,1798 + 4.4355) —0.1793 + 3.0254] —0.1846 —+$9.8412| -+0.8049 + 8.3199] -+0.8027 —= 6.8886] -+0.8019 | -+0.8036 | -+0.8023 | — 0.0011 —0.0034 | -+0.0001 | -+0,7979 —+ 5.42209] -+0.8072 + 40112] -+0.8012 —+10.0928| -+1.0565 + 8.5687| 1.0515 + 7.1388] 1.0521 | +1.053r | 1.0514 | —0.0012 —0.0039 | +0.0001 |. -+1,0464 + 5.6672| -+1.0524 + 4.2630] -+1.0530 57.1155 58.6390 60.0670 61.5320 62.9450 56.9910 58.5170 59-9445 61.4135 62.8250 _ 56.0055 se 955 61.8350 55.7610 57.2830 58.7125 60.1855 61.5845 e Decldif: M—Centrum — + 3/0037 15 = 0.99842 39} = +-0.00030 N— » = + 3.4510 8- » ——24.4325 fs =0.99794 - is = -+0.00029 x ig=-r1'0 _» = —24.4680 V— » = —19.2648 fs = 0,99841 Js = -+0.00032 W— » —+30.7327 dy = 20° 58:6 a Зап. Физ-Мат. Отд. 33 34 Е. Renz, 32 B. 1896. März 14. IR за Scalenablesung. 5 Zt Helsingforser Sternzeit P.-Kr. 0° ++ P.-Kr.180° t-+k | Е der Aufnahmen. Mittel. mm mm BELLE 1000| m 10000110000 Ctr. | 64.3196 61.0630 ei ra S 64.3188 |- 8| 64.0622 0.0000 2—3 M 69.2700 |+-14| 59.1068 + 4.9540 ) 2 N 25.3700 |+-26| 103.0155 — 38.9482 a EDR 3 Q 77.8345 |-+20| 50.5540 —-13.S114 10 25 33 3 Е 27.7852 |-+33| 100.5855 — 36.5248 2—3 У 64.0158 64.3642 — 0.3024 2—3 W | 65.1618 63.2150 + 0.8453 3 %а | 49.0175 79.3460 —15.2921 a. 49.5285 78.8715 — 14.7998 — 14.8019 10 19 58 4—5. a, 50.0165 78.3875 — 14.3138 4b | 49.0345 79.3470 —15.2841 b. 49.5300 78.8680 — 14.7972 — 14.8010 20 41 3—4 b, $0.0100 78.3970 —14.3218 Зе | 49.0495 _ 79.3390 —15.2726 | ce 49.5230 78.8655 — 14.7996 — 14.7959 21 20 10* 21” 21° 4 бо | 50.0155 78.3900 — 14.3156 З 2 dy | 49.0705 79.3215 — 15.2534 ь de | 49.5485 78.8490 — 14.7786 — 14.7786 211059 4 do | 50.0230 78.3740 — 14.3039 Фе» | 49.0265 79.3550 —15.2922 | ec | 49.5200 78.8920 — 14.8143 — 14.8125 22 45 4 eo | 49-9940 78.3990 — 14.3309 | Trabant — Jupiterscentrum. + Rn — Ty | Mittel. 'ater-22) Jayr—v2)| Ph. | Aa. cos à À mm mm 1 Та 51.5500 76.8270 — 12.7666) +2.0353 2 b | 51.5380 76.83 50 — 12.7766] -+2.0244 | 2 е | 51.5550 76.8240 —12.7626| -+2.0333 | -+2.0300 | -+2!0269 | -но!оото | —0'0020| +2:0259] 2—3 а | 51.5570 76.8210 — 12.7601] -+2.0185 2—3 е 51.5430 76.8350 — 12.7742] 2.0383 Па | 50.0655 s| 78.3085 — 14.2498] 0.5521 2—8. b 50.0565 |+ 5| 78.3195 —14.2599| +0.5411 2—3 с | 50.0715 |+ 5| 78.3105 —14.2479] +0.5480 | -+0.5436 | -+0.5428 | 0.0004 | —0.0020 | 0.5412 | 2—3 а | 50.0695 | 6| 78.3110 — 14.2491} -+0.5295 2—3 e 50.0550 |+ 6| 78.3285 — 14.2652] -0.5473 2—3 Ша | 54.1380 |+ 3| 74.2320 — 10.1758] -+4.6261 4 2 b 54.1420 |+ 3| 74.2395 —10.1776| -+4.6234 | 2 € | 54.1410 | 3| 74.2335 —10.1750] +-4.6209 | +-4.6209 | -+4.6138 | -+0.0023 | —0.0020 | 4,6141 | 2—3 а | 51.1470 |+ 4| 74.2330 — 10.1668] +4.6118 Е 2—3 е 54.1250 |+ 4| 74.2480 —10.1903| -+4.6222 2—3 IV а | 58.4675 |+ 5] 69.9135 — 5.8519] 8.9500 2 b | 58.4660 |+ 5| 69.9180 — 5.8549] -+8.9461 | 2—3 с | 58.4740 |+ 6| 69.9035 — 5.8436] -+8.9523 | -+8.9489 | -+8.9351 | -+0.0042 | —0.0020 | -+8,9373 | 2 а | 58.4775 |+ 7| 69.9040 — 5.8421| -+8.9365 3 e 58.4670 |+ 8| 69.9150 — 5,8528] -+8.9597 2—3 Scheinbare Rdiff: M—Centram—+ 5'2700 f° y = 0.99844 —®, = —0.00032 N— » = —41.4095 | 4 Q— в = 14.3271 fu == 9.99813 —iy =- 0.00037 хи =+ 13 R— » — —28.7088 Ве. =-н 6 У— » = — 0,3186 Try =— 165 W— ‘» = + 0.8860 f'x = 0.99846 7. =- 0.00196 ay = 8" 63 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1896. März 14. Decl. 4 _Scalenablesung. : 2 2 Bemerkungen 4 у ие — + tù sin 1’ y ——=tg8 sin К ce 90°] 1-51 Р.-Кх. 270° [++ 2 : zur Aufnahme. | mm mm + PT | || ”” ca u. Tr + 8] 64.3802 |+ 8| ol-+ 1.4706 0.0000 — 1.4706 Luft 3. #9| 61.3715 |+12 o|-- 4.4779 — 0.0013 + 4.4766 Neblig. Schnee zu +35] 60.8232 |-+26|— 2|-+ 5.0278 — 0.0806 + 4.9472 erwarten, 88.8475 |— 2|-+-11| —22.9832 — 0.0094 — 22.9926 +40) 88.7970 |-+ 9|+-26| — 22.9468 — 0,0690 — 23.0158 +18) 83.6740 |— 3|-+ 2] — 17.8216 0.0000 — 17.8216 33.5977 21121] +42.2503 0.0000 -+42.2503 63.2755 |415 + 2.5751 - 63.7425 |-+14 — 2.1146 + 2.1141 о |-+13| 64.1995 |+14 + 1.6525 о |-+14| 64.7820 |-+22 + 1.0739 14| 65.2360 |-+22 + 0.6219 + 0.6222 № 65.6810 |-+22 + 0.1709 14| 66.1530 |-+16 — 0.3048 14| 66.6090 |+-14 — 0.7492 — 0.7544 —=14| 67.0645 |-+14 — 1.2092 67.6745 |+24 1.8199 19| 68.1280 |+24 — 2.2724 — 2.2741 19| 68.5810 |-+24 2.7300 rs 69.0720 |+19 3.2196 +15] 69.5405 |-+22 — 3.6788 — 3.6805 -15| 69.9940 |-+22 — 4.1430 м Trabant — Jupiterscentrum. ve | Mittel. feu) went] PL | 48 | тт тт +13] 64.2475 |+13| |+ 1.5996] —0.5145 4 14 65.7355 |+15 —+- 0.1120| —0.5102 i 4 +15| 67,1140 |+-13 — 1.2668] —0.5124 | —0.5113 | —0'5106 | -+0'0008 | -но!оозт | -но!0о0г | —0!'5066 +19] 68.62 +-18 — 2.7812] —0.5071 | | ! ID 70.0400 |+21 — 4.1928| —0.5123 63.9345 |+14 + 1.9125| —0.2016 5.4210 |-+22 + 0.4259| —0.1963 14 66.7965 |+-14 — 0.9524] —0.1980 | —0.1975 | —0.1973 | -+0.0002 | -+0.0009 | -+0.0001 | —0.1961 ‚68.3165 |-+24 — 2.4701] —0.1960 15 69.7220 |+22 — 3.8760] —0.1955 3| 64.9190 |-+19 + 0.9265| —1.1876 3| 66.4050 |+13 — 0.5607| —1.1829 67.7850. |+-21 — 1.9410] —1.1866 | —1.1840 | —1.1822 | +0.0019 -+0.0064 | -но.ооот | —1,1738 -14| 69.3000 |-+-16 — 3.4590] —1.1809 9] 70.7063 |-+15 — 4.8626] — 1.1821 | 11| 65.8830 |+-11 — 0.0327| —2.1468 67.3665 |+ 9 — 1.5158] —2.1380 68.7544 |+14 — 2.9022| —2.1478 | —2.1425 | —2.1393 | +0.0037 |: +0.0103 | -+0.0001 | —2,1252 70.2635 |+-17 — 4.4130] —2.1389 71.6710 |-+12 — 5.8215| —2.1410 inbare Decldiff: 1/— Centrum = + 3/0037 f°3 =0.99852 $28 =-+0.00038 [ N— » =+ 3.4510 | к ` _0— » = — 24.4325 fs = 0.99799 iz = 0.00026 X 14=- 009 R— » = —24.4681 V— » =-19.2648 J'a =0.99853 Уз = -+0.00041 W—- » = -+30.7328 dy = -+21° ılı 36 Е. Renz; 32 С. 1896. März 16. № Scalenablesung. à Helsingforser Sternzeit À Object. | — "+5 œ Зоо Bilder. P.-Kr. 0° t-il P.-Kr.180° | ++ 3 der Aufnahmen. Mittel. A mm mm 10000110000 mm mm mm Ctr. | 64.2870 64.0994 S 64.2862 |+ 8| 64.0985 | 9] © 0.0000 2—3 M 69.2352 [#14] 59:1390 |+-10| 0|+ 4.9545 2 N 25.3338 |+-26| 103.0520 |+ 5|+-18) — 38.9500 I APTE 3 Q 77.8030 |+21| 50.5822 |+20|— 3|-+13.5164 955 11 3 Е 27.7505 |-+34| 100.6230 |+-13]H-20| —36.5270 2—3 у 63.9835 |-+18| 64.3905 |+15] 0) — 0.2962 2 W | 65.1275 |-+28| 63.2520 |-+23] ©|- 0.8442 3 Ayo | 72.5938 |+-15| 55.8040 |+ 2 + 8.3018 ас | 73-0820 |+15| 55.3145 |+ 2 + 8.7906 + 3.7952 9 50 46 3—4 ао | 73-5795 |+15| 54-8070 |+ 2 tr 9.2931 bw | 72.5890 |+14| 55.7995 |+ I + 8.3016 be | 73.0860 |+14| 55.3170 |+ 1 + 8.7914 + 8.7915 5 62 3. bo | 73.5695 |-+14| 54.8200 |+ 1 + 9.2816 %Cw | 72.6010 |-+-14| 55.8020 |+ 1 + 8.3064 4170 ее | 73-0870 |+14] 55.3140 |+ ı + 8.7934 + 8.7942 52.129 9% 52” 10 3 Co 73.5680 |+14| 54.8160 |+ I + 9.2828 3% dy | 72.5960 |+-13| 55.7990 о + 8.3054 de | 73-0920 |+13] 55.3180 о + 8.7938 + 8.7929 52 52 3—4 do | 73-5710 [+13] 54.8255 о + 9.2796 "Ze | 72.5920 |-+13| 55.8070 о +- 8.2994 ес 73.0955 |+13| 55.3100 о + 8.7996 -+ 8.7986 ат 2—8 во 73.5850 |-+13| 54.8050 о + 9.2968 Trabant — Jupiterscentrum. 2—2 | Mittel. Е] РВ. | Ac cos 5 ee —А———Ч—/——” . тт тт Та | 74.4440 |-+15|] 53.9290 |+ —+10.1642| -+1.3690 2 b | 74.4360 |-+14| 53.9355 |+ 10.1569] +-1.3654 2 с | 74.4415 |-+13| 53.9350 |+ -+10.1598] -+1.3656 | -+1.3625| 13603 | —0:0003 | —0'0021 | +1:3579| 2—3 а | 74.4285 |+13| 53.9455 |+ -+10.1482| +-1.3553 2 e 74.4360 |-+ı12| 53.9380 |+ +-10.1556| -+1.3570 ' 2—5 u bedeckt Ша | 70.1270 |+18| 58.2410 |+ 8 + 5.8497| —2.9455 2 6 | 70.1220 |-+17| 58.2505 |+ 7 + 5.8424] —2.9491 2 с | 70.1190 |17| 58.2500 |+ 6 + 5.8412| —2.9530 | —2.9527| —2.9478 | -+0.0005 | —0.0021| —2.9494 | 2 а | 70.1130 |+-16| 58.2570 |+ 6 + 5.8347| —2.9582 1—2 e | 70.1190 |-+-16\ 58.2510 |- 6 + 5.8407] —2.9579 2 IV a | 80.3210 |+ı1] 48.0610 |-+23|— 2] 16.0354] 7.2402 ds b | 80.3150 [+10] 48.0670 |+-22|— 2] -+16.0294| +-7.2379 | 2—8 с | 80.3210 |+ 9| 48.0615 |-+22|— 1] +16.0352| -+7.2410 | +7.2372| 7.2253 | —0.0014 | —0.0021 —7,2288 | 2 а | 80.3110 |+ 9] 48.0720 |-+21|— 1|-+16.0250| +-7.2321 2 е | 80.3185 |-+- 8| 48.0630 |-+20|— 1| +16.0332] 7.2346 2—3 Scheinbare ÆRdiff: МЬ— Centrum = + 5:2701 Fa = 0:99835 —1°,, = —0.00018 N— » = — 41.4096 Q— » =-14.3271 fu = 9.99805 —iy = —0.00022 х i,= + 0.8 В— » = — 38.7089 Refr. =-+ 4 У » —— 0.3186 Try == 98 W—- » = + 0.8859 Ло = 0.99836 Л. —+0,00080 ay = gt 6.0 = | Sealenablesung. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1596. März 16. 8 у 3 5 -Kr.270° [1+1 тт | тт 1000010000 65.8486 2% +10! 65.8470 |+16| о 0.0000 +16| 62.8388 |+11| о|- 3.0048 -=27| 62.2935 |+25|-— П|-+ 3.5528 - 90.3128 |— 3|-+ 5| —24.4618 38] 90.2662 |-+ 8|+14| —24.4229 21| 85.1330 |— 2|-+ 2| —19.2894 35.0662 |+21|— 8] 30.7789 2| 72.7920 |+16 — 6.9389 + 2| 72.3250 |+14 — 6.4706 + 2| 71.8725 |+14 — 6.0196 12| 71.3450 |+15 — 5.4954 8| 70.8920 |+15 — 5.0360 8 70.4320 |-15 — 4.5836 13| 69.8610 |+19 — 4.0102 H13| 69.4170 |+16 — 3.5614 +13 68.9640 |+16 — 3.1111 -17| 68.3940 |+21 — 2.5429 Fl 17 67.9445 |+21 — 2.0896 +13 67.4945 |+-21 — 1.6421 ) 66.9650 |+-11 — 1.1142 66.5090 |+11 — 0.6536 66.0350 |+13 — 0.1842 72.6760 — 6.8290 71.2370 — 5.3934 69.7610 — 3.9166 68.2920 — 2.4484 66.8520 — 1.0092 71.6525 |+13 — 5.8111 70.2125 |-+18 — 4.3738 68.7370 |+15 — 2.8957 67.2680 |-+10 — 1.4282 +10 65.8295 |+12 — 0.0112 ) |-+10] 74.1165 |-+18]-= 1|— 8.2692 + 6] 72.6755 |+19]+ 1] — 6.8285 +16| 71.2020 |+18|-+ 1] — 5.3530 о |-+17| 69.7345 |-+22| 0|— 3.8872 о ie 68.2940 |+24| 0]— 2.4484 î А, are Decldif: M—Centrum = -= 3/0036 N— » —+ 3.4507 Q— » =-—24.4328 Е— » = —24.4683 У— » = —19,2649 W— : » —+30.7328 dy = -+21° 1:8 Decl. Znt2%2cot%5 3 mm mm mm —0.3526 —0.3551 —0.3557 —0.3569 —0.3585 —0.3558 —+0.6653 0.6645 -+0.6652 +-0.6633 0,6619 — 1.7928 — 1.7902 — 1.7921 —1.7957 —1.7977 +-0.6640 —1.7937 {75 = 0.99859 fs = 0.99808 f'a = 0.99859 2 р n ’ — 7:95 sin 1 veus | Mittel. aweum 7 аа) вез р x? < _- у— > 195 sin 17 тт тт 0.0000 0.0000 Luft 8. — 0.0013 + 3.0035 — 0.0806 -+ 3.4722 — 0.0094 —24.4712 — 0.0690 —24.4919 0.0000 —19.2894 0.0000 +-30,77389 Trabant — Jupiterscentrum. —0!3553 | +0'0006 | —o'o01$ | +-0/0001 —=0.6631 | —-0.0012 +-0.0024 | +0.0001 —1.7911 | -+0.0030 | —0.0101 | +0.0001 $28 = +0.00038 ig = 0.00030 X 13 =- 10 75 = -+0.00041 37 Bemerkungen zur Aufnahme. —0:3561 + 0.6644 —1,7981 38 Е. Renz, 32 D. 1896. März 31. Scalenablesung. Helsingforser Sternzeit P.-Kr. 0° == P.-Kr, 180°|+-+-# 8 der Aufnahmen. Mittel. mm mm 10000] 10000 Ctr. | 61.2830 64.1054 en К 64.2822 64.1045 M 69.2318 59.1445 + 4.9550 М 25.3278 103.0608 — 38.9526 Q 77.7960 50.5880 +-13.5148 R 27.7435 100.6290 — 36.5285 УТ | 63.9770 64.3995 — 0.2999 W | 65.1242 63.2545 + 0.8462 % un | 74.1925 54.1885 3 + 9.9136 ae | 74.6685 53.7330 |+ 3 —+-10.3793 +-10.3760 & | 75-1180 53.2705 |+ 7 +10.8351 4b. | 74.2185 54.1705 |+ 3 + 9.9356 74.6760 53.7145 |+ 3 —+-10,3924 +-10.3921 75.1305 53.2565 |+ 7 —10.8484 . 74.1965 54.1845 |+ 3 + 9.9176 74.6490 53.7485 |+ 3 —+10.3618 —+10.3665 10° 21” 38° 75.1015 53.2840 |+ 7 —+10.8202 74.2105 54.1950 |+ 3 + 9.9194 74.6585 53.7205 |+ 3 +-10.3806 +-10.3778 75.1160 53.2720 |+ 7 —10.8334 74.1940 54.1935 | 4 + 9.9120 74.6725 53.7410 Ir 4 10.3774 +-10.3724 23 VD 75-1070 53.2740 |-+ 8 -+-10.8279 Trabant — Jupiterscentrum. 2 — 0, | Mittel, Fate (ии) Ph. | Au. cos à RER EN ER JE ET UE CE SR AL u el I > mm | тт Та | 73-1285 55.2530 + 8.8496] —1.5264 b | 73.1415 55.2390 + 8.8632| —1.5289 с | 73.1260 55.2585 + 8.8457| —1:5208 —1!5208 | -+0'0003 | —0:0027 | —1:5232 d | 73.1385 55.2470 + 8,8577] —1.5201 Е | 73.7310 55.2510 + 8.8520] — 1.5204 Па | 77.6860 50.6870 —=13.4105] 3.0345 b | 77.7010 50.6745 +-13.4242| +-3.0321 се | 77.6815 50.6930 -+13.4053| 3.0388 -+3.0310 | —0.0007 -+3.0276 d | 77.6910 50.6820 +-13.4156| +-3.0378 e | 77.6825 50.6865 13.4090] 3.0366 Ша | 70.1145 58.2590 5.8396] —4.5364 Ъ | 70.1295 58.2440 5.8546] —4.5375 e | 70.1050 58.2670 5.8308] —4.5357 +-0.0009 —4,5311 Я | 70.1150 58.2560 5.8414] —4.5364 e | 70.1095 58.2645 5.8344] —4.5380 IV a | 83.2200 45.1670 -+18,9366| -+8.5606 b | 83.2310 45.1520 —18.9497| +8.5576 e | 83.2130 45.1720 -+18.9308| +8.5643 —+8.5432 d | 83.2205 45.1620 -+18.9395] -+8.5617 е | 83.2175 45.1650 +18.9365| +-8.5641 Scheinbare Adiff: M-—Centrum =-н 5.2702 Fu = 0.99833 —i%, —=—0.00030 N— » = —41.4104 à Q— » =--14.3274 fx = 0.99802 —iy = —0.00036 an w 41 le) Trabant — Jupiterscentrum. хе» | Mittel. | >) Лигу») Ph. | Aa cos 8 ER RELEASES Ji ne 7 EEE ee —0!0004 | —0!0028 0.0006 | —0.0028 —0.0008 | —0.0028 —0.0014 | —0.0028 | —®. = +0.00013 — = +0.00010 ae = + 4 PAU т 97 Mittel. 9% 46” 39° —1:8207 +-2,8395 —4,0679 —1.2553 х = Bilder. 2—3 ellipt. 3—4 3—4 19 N N © D —3 eiförmig. 9 IN © © ND © © W © © —3 geschwe —3 eiförmig 19 D 19 LR Ro So at SE © a POsITIONEN DER J UPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 43 1896. Арки 7. Пес]. Znt2ct%; x? 2 Bemerkun ET — 3 tgù sin 1’ Y—+ tgd sin 1’ upper io zur Aufnahme, 63.9813 = 8| 63.9805 0.0000 0.0000 Luft 2. + 9| 60.9745 — 0.0013 + 3.0069 351 60.4495 |+301— ı]-+ 3.5323 — 0.0806 + 3.4517 2 88.4438 |— П-+ $] —24.4568 — 0.0094 —24.4662 ail 88.4300 |-+-10l-+ 14] —24.4470 — 0.0690 —24.5160 | -19| 83.2748 |-+ 2|+ 2] —19.2936 0.0000 -— 19.2936 2| 33.1975 |+19|— 8|+30.7839 0.0000 +-30.7839 1| 64.3345 |+-11 — 0.3425 +11| 64.7295 |-+19 — 0.7422 — 0.7464 -12| 65.1390 |+19 — 0.1544 2| 65.8025 |+13 — 1.8173 2| 66.2150 |-13 — 2.2270 — 2.2272 12] 66.6220 |+13 — 2.6373 -13| 67.2695 |+11 — 3.2829 H13| 67.6745 |-+21 — 3.6866 — 3.6897 68.0840 |-r21 — 4.0996 68.7040 |+16 — 4.7157 3| 69.1150 |+-16 — 5.1246 — 5,1245 3) 69.5260 |+16 — 5.5332 | 70.1800 |-+-19 — 6.1900 2 8 70.5870 |+15 — 6.5944 — 6.5996 5| 71.0020 |-+15 — 7.0144 Trabant — Jupiterscentrum. ФУ | Mittel. | Хауз) Тоби аз) (и? Ph. | 48 тт тт 64.2760 — 0.2962| -+0.4502 65.7590 — 1.7776| -+0.4496 | ; À x 67.2220 — 3.2399] <+0.4498 | +0.450$ | —<+-0!4498 | 0,0003 —0:0020 | —+-0:0002 —+0:4483 68.6550 — 4.6720] -+0.4525 70.1325 6.1493| --0.4505 65.4410 — 1.4598] --0.7134 | : 66.9225 — 2.9406| —0.7134 6| 68.3830 — 4.4012] —0.7115 | —0.7131 | —0.7120 | —0.0004 | -+-0.0023 | -+0.0002 — 0.7099 69.8200 — 5.8378] —0.7133 71.2955 — 7.3136] —0.7140 63.7545 + 0.2256] -+0.9720 65.2305 — 1.2544] -+0.9728 66.6940 — 2.7182] -+0.9715 | -+0.9734 | -+0.9719 | -+0.0006 —0.0048 | -+0.0002 0,9679 68.1240 — 4.1472] -+0.9773 . 69.6040 — 5.6260] -н0,9736 63.0445 + 0.9370] -+1.6834 64.5240 — 0.5437| —+1.6835 à 65.9880 — 2.0066] 1.6831 | -+1.6837 | -+1.6809 | -+0.0011 —0.0100 | -+0.0002 +-1,6722 67.4210 — 3.4402| -+1.6843 68.8970 — 49154] —+-1.6842 inbare Decldif: M—Centrum —-+ 3.0035 f°3 = 0.99843 13 = —0.00017 О . EE » = + 3.4507 4 à E 0» =-243 Js —099792 3 = —0.00025 x ig = —0!9 R— » = —24.4690 nr V— » =-—19.2653 18 = 0.99342 Ja = —0.00015 W— » = +30.7335 dy = 20° 58'9 | й 4 FAR PEN x “ Ut К Ужа У АЕ \ r . mcm LE OS ne doré nn + P 4 ы z 2 ы } т 7 je | у ’ y à, F ar r 2 Г en BA ‹ - | | кт | | - ù LA | Si ir PU у : р : hy > Br h R . , 2% } } | PRET ER CET - à | 2; re seal de - Pasta | LE à р Hp à re (ge Re fi 24 Dé x è $ . ыыы — ih tre at Обе | ‘ 3 Zi Е 5 A ME f : Cats SORTE 24-71 fé { BURN Г |! 3 ” { ; а Зои | у da j As и $ - 1 YA er 007 : 17 | | | ИА ЕЩЕ \ НА 8 et ее za, x ’ nt es nat о че --- “ >! + — nn. —— a + |1 x A. OPPOSITION 1896. 84:2 Ze] AER CLICHÉS. et nn 7 ee — ARME NH PULKOW =; 53$ je \ a iM == NS ee Er — ne } EU Ve RAT’ a EN реа: Но 14 СЯ И Шо... BL. BEST 4 у 2 L'v., | } | | 1 | — С | АА У! > 1 | В д À L „ iR | L rs CD “+ | р Le À u” à Ci u, м DA At x, £ к ‚ : f , т | ь 46 36 A. ао Object. 61.0805 64.0797 19.9499 72.7047 22.4112 66.3983 66.8400 67.3118 66.4728 66.8940 67.3438 66.3963 66.8316 67.2898 66.4428 66.8626 67.2964 68.8181 68.8786 68.8196 68.8471 mm 100uU +14 +13 Em 15) +13 Geht durch 69.8361 69.8850 69.8161 69.8456 64.4068 64.4538 64.3868 64.4148 Scalenablesung. P.-Kr. 0° |t+-k|P.-Kr.180° mm 64.3104 64.3096 108.4413 55.6879 105.9765 62.0105 61.5537 61.1160 61.9330 61.4948 61.0650 62.0075 61.5642 61.1224 61.9570 61.5202 61.1044 59.5767 59.5152 59.5748 59.5462 die Jupitelrsch 58.5522 58.5062 58.5782 58.5468 63.9870 63.9426 64.0110 63.9815 Scheinbare Adift: + BR —- — 3—4 -- = an 3—4 = —- LE 3—4 + — + 3 -i- Trabant — Jupiterscentrum. MERE | Mittel. | Рег аз) Te Que из) Ph. | Au cos 8 ne EP Е тт mm se ni Fr. de sch + 4.7966] +1.97 , Sr , ' verwaschen. | + 4.7373] 10851 -+-1,9800 | +-1:9667 0:0009 | 0.0009 | 1.9667 | 45 verwasche + 4.7653| 1.9804 5 | = +-2.9972 ы 2—3 и. — —+2.9868 sul о | 4 verwaschen. I as 2.9864 | +-2.9663 0.0014 | -+0.0009 | +2,9658 | 4 yerwaschen. is +-2.9797 d 3 + —2.4351 : 3 + —2.4472| AN _o1: unterexp. de Sp 2.4450 2.4285 | —+-0.0099 | 0.0009 2,4267 5 oo. 2.4533 N—Centrum = —46!6732 Fra = 0.99327 — = -+0.00121 = - 9.0567 7 = —43.9725 fx = 0.99295 — = А 00123 X im —4:2 AB Ве". = > 92, = 8 40.2 во — f'x =0.99328 “= avoit 10000 —+18|-+28 _mm_ 70000 8 + 14 +11 M ed +10 +10 HR: +10] +10, и +14 +14 +14 +15 +10 +10 = 15) и + ть eibe. Е. ВЕКЕ, 1895. December 37. № 103. Pulkowaer Sternzeit Z2w+r#c+%o Bilder. der Aufnahmen, Mittel. mm 3 —4 etwas ellip р POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 47 1#95. December 27. Decl. | Scalenablesung. Ant 3 +2 23 Beinerkungen = т Я у ——— y — = 5 sin 1/ zur Aufnah P.-Kr, 90° tt P.-Kr.270°| 1-44 2 Re 15) à usé gs 10000] 10000 mm RR Lin Éd 64.7332 o 0.0000 0.0000 0.0000 Bilder 3—4. 64.2386 0] + 0.4970 — 0.1022 + 0.3948 92.3328 |— 3|+- 6] —27.5950 — 0.0038 — 27.5988 92.3519 |-++11|+-21| —27.6161 — 0,0890 — 27.7051 56.6302 + 5.1190 Die erste Jupiters- 60.0645 + 4.6864 + 4.6869 aufnahme scheint 60.4878 + 4.2552 in Decl. verzerrt, ielleicht durch Er- 62.7701 + 1.9732 Ina 63.1769 + 1.5669 + 1.5648 schütterung des 63.5862 + 1.1544 Fernrohrs. 65.9510 1.2019 66.3588 — 1.6164 66.7641 — 2.0268 67.5348 — 2.7962 67.9376 — 3.1944 „683434 Trabant — Jupiterscentrum. vv» | Mine, |) |Jor—e2-(e2-2398| mm mm 60.6347 en ZN | 63.7581 + 0.9800] —0.5848 | _ 5 ae. Le” IL даль — 05865 66.9430 — 2.2054| —0.5904 0.5868 0.5830 0.0027 0.0007 0.0001 0.5865 68.5208 — 3.7842] —0.5874 60.9955 + 3.7001 en | en = ый er Bat —0.9444 | —0.9382 | —0.0041 | —o.0013 | —0.000: | —0.9427 68.8770 — 4.1413] —0.9445 59.4398 + 5.2964] -+0.6095 a = Gers в = +0.6143 | 0.6103 | -+0.0033 |. +0.0004 | —o.0001 | -+0,6139 "67.3198 "| — 2.5800] -+0.6168 7 / inbare Decldiff: N—Centrum = + 0!4467 fa = 0.99348 19; = —0.00132 | Q— » = —27.4328 и R—- » = —27.4690 Ss = 0.99299 1) =— 0.00126 X 15 = —43 l'a = 0.99352 Js = 0.00137 dy =-+18°9 59:4 48 Е. Renz, 36 B. 1895. December 27. | A 104 ——— Scalenablesung. ° Pulkowaer Sternzeit Object. = s < art Poney ВИдег. | P.-Kr. 0° | ++ P.-Kr.180° à der Aufnahmen. ' Mittel. Anhaltstierne| wie 36 A. mm 10000 » mm mm mm mm %9щ | 60.1404 |-+14| 68.2628 — 3.9465 A LE Ice | 60.5792 | +10] 67.7991 — 3.4954 — 3.4951 7 23 36 3 do 61.0450 |+10| 67.3618 — %hy | 60.1569 |+14| 68.2394 | he | 60.5992 |+10| 67.7921 = — 3.4845 25 0023 2 ho 61.0350 |+10| 67.3648 PET + Zip | 60.2079 |+14| 68.1954 — ie 60.6227 |+10| 67.7706 — — 3.4580 26 _39(36) 2—3 2 61.0555 |-10| 67.3568 — %Ъ | 60.1499 |-+14| 68.2578 — ke | 60.5728 |+10| 67.8271 = — 3.5129 28.031 2—5 ko | 60.9970 |+10| 67.4008 к Trabant — Jupiterscentrum. 1—1 | Mittel. |7’ ТРИ, | Ac cos à mm mm То | 62.6097 |+ 9| 65.7861 — —+2.0217 3—4 h | 62.6127 | 9| 65.7826 — +2.0144 ‚ ‚ , , 3—4 Е UE. 9 en R res 2.0184 | +2!0049 | —o!ooos | +0.0009 | +2:0053| 3 k | 62.5907 | 9| 65.8081 — —+-2.0191 3—4 IL Geht dulrch |die Jupiter . ne 63.5282 |+ 9| 64.8660 — —+-2.9407 3 » | 63.5238 |+ 9| 64.8680 — +-2.9269 3 er dec) ИС = ee -+2.9288 | +2.9091 | —0.0008 | -+0.0009 | +2.9092 | 54 | k | 63.4912 | 9| 64.9030 — -=2.9216 2—3 B a ee + $] 70.2878 — —2.4805 4 verwaschen, | 58.1020 |+ $| 70.2938 — —2.4971 | 3 $ 58.1280 |+ 5| 70.2673 Е —2.4972 2.4939 | —2.4771 | 0.0005 | 4-0.0009 — 2,4757 пре k | 58.0720 |-+ $| 70.3284 — —2.5009 Scheinbare Ædiff. wie 36 A. 199 = 2.993097 —® = +-0.00121 fa =0.99298 —iyg = 0.00123 Хи = —42 Refr. = — > Try = — J'x = 0.99328 da =. 00083 » h m ay = 8 40.2 ен P.-Kr.270° [+ 62.7332 Yı 92 mm —0.5989 —0.6031 —0.596т — 0.6013 68.8101 —0.9313 67.0914 —0.9381 65.5832 —0.9249 64.0500 —0.9273 67.2518 +-0.6264 65.5362 +-0.6221 64.0305 —+-0.6293 62.4958 -+0.6293 dy = +189 59/4 Znt%ct?%s Js = 15 =09929 is ——0.00126 f’s = 0.99351 у 4 1895. December 27. Decl. о > | PAC 7 5 #76 sin.1 mm mm 68.3018 67.8830 — 3,1408 67.4688 66.5717 66.1654 — 1,4222 65.7616 65.0690 64.6662 + 0.0779 64.2628 63.5268 63.1280 + 1.6138 y — tgù sin 1’ POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 49 Bemerkungen zur Aufnahme. Bilder 3—4. Trabant — Jupiterscentrum. Mittel. Wawe-m)| абы г | ее] Ph | —0.5998 | —0.5959 | —0.0027 —0.9304 | —0.9244 | —0.0059 +0.6268 | -+0.6227 | -+0.0033 0.99348 $25 = —0.00132 Js =— 0.00134 -+0:0005 | —olooor —0.0206 | —0.0001 —0.0012 | —0.0001 X 15 =—43 2) — 0.5982 —0.9278 —+0.6247 50 F. Rexz, 37. 1896. Januar 1. | AR 105, Scalenablesung. Pulkowaer Sternzeit Object. s х RS ля MC ВДОХ ЛИ COR EUR DR ИЖ Bilder. | P.-Kr. 0° = P.-Kr.180°| + В der Aufnahmen. Mittel. mm mm mm an 1000| mm 100001100000 mm mm Ctr, | 64.1421 64.2495 1 M 69.1180, |-+14| 59.2698 4—5 verwaschen» 5 64.1413 64.2487 A Bene 4—5 » м М 24.9906 103.3993 6 3 22 4—5 » Q | 77-7455 50.6465 4—5 a R 27-4476 100.9399 4—5 » ха 66.4748 61.9380 Er a 66.9140 61.4802 + + 2,7730 6 Aa” то’ a5 ао | 67.3793 61.0340 5 2b, | 66.5192 |+- 9] 61.8936 ar b. | 66.9605 | 9| 61.4353 + + 2.8174 бо... а 4—5 db, | 67.4218 |+ 9] 60.9900 — 2 Cry | 66.4942 |+ 8| 61.9220 = Ce | 66.9190 |+ 8| 61.4762 = + 2.7773 52 4 4—5 en 67.3693 | 8| 61.0420 SE 6” 53 ge % dyp | 66.5472 | 8| 61.8710 ni - de | 66.9560 |+ 8| 61.4418 + + 2.8160 54 17 4—5 do | 67.3978 |+ 8| 61.0135 : ar Zen | 66.4942 |+ 8| 61.9200 A ес | 66.9110 |+ 8| 61.4918 + 2.7632 + 2.7683 55 47 4—5 ео 67.3498 |+ 8| 61.0550 + 3.2010 %) | 66.4918 |+ 8| 61.9220 + 2.3384 Je 66.9296 | 8| 61.4782 + 2.7792 + 2.7767 57 44 4—5 Yo 67.3628 | 8| 61.0450 + 3.2124 | Trabant — Jupiterscentrum. 21—20 | Mittel. fete) Лиз) Ph. | Да cos d mm mm | I Geht durch |die Jupiter|schelibe. Иа | 64.9370 |+17| 63.4532 |+ 9 + 0.7960] — 1.9770 ‘| 3—4 D | 64.9865 |+17| 63.4048 |+ 9 + nn — 1.9724 3—4 с | 64.9600 |+16| 63.4308 |+ —+ 0.8186] —1.9587 р ‚ ‚ 27 | 3—4 nee lie pan à + о8621| —1.9839| —1.9602 | —1'9470 | +-0/0006 | +0/0007 —19457| 3, e 64.9580 |--16| 63.4338 |+10 + 161] —1.9522 4 f | 64.9720 |+16| 63.4208 |-+10 + 0.8296] — 1,9471 3 Па | 70.1839 |+17| 58.2034 |+ $] | 6.0446] +3.2716 3—4 b | 70.2344 |+16| 58.1574 |+ 5 + Eee en 4 с 70.2054 |-+16| 58.1864 |+- 6 —= 6.0637} 3.2564 4 а 70.2404 +16 ито ЕАО + 6.1048] -+3.2888 -+3.2842| -+3.2621 | —0.0009 | 0.0007 | -+-3,2619 3 е | 70.2004 |+16| 58.1939 |+ 6 — 6.0574] +3.2801 3 f | 70.2144 |+16| 58.1794 |+ 7 + 6.0716] -+3.2949 3 IV a | 58.8181 |-+12| 69.5757 |+17 — 5,3254] —8.0984 4 b | 58.8646 |-+11| 69.5282 |+-16 — 5,2784] —8.0958 3—4 С 58.8311 |+11| 69.5622 |-+16 — 5.3121] —8.0894 | _ dr 3—4 4 | 588746 lool 69.212 [+16 — 5.2699] —8.0859 8.0911 8.0365 | -+0.0022 | -+0.0007 | —8,0336 | 53 e | 58.8920 |+10| 69.5712 |+16 — 5.3212] —8.0895 3—4 Л | 58.8331 |+-10| 69.5612 |+17 — 5,3107] —8.0874 3 Scheinbare Adif: Zf—Centrum = + 5!2695 f° à = 0.993 26 — = +-0.00062 N— » = —41.4048 . Q—. » = +14,3257 fa = 0.99294 —iy =-0,00068 X = —25 Е— » = —38.7040 Вей’. = — 5 Try = + 28 Г’ = 099325 Ч = +0.00091 65,2015 62.1700 65.1999 61.6790 89.7714 89.7904 59.9400 60.3668 60.7801 61.7616 62.1759 62.5992 63.2508 63.6546 64.0035 66.4323 66.8301 67.2429 68.1324 68.5372 68.9360 | 69.5072 69.9326 $] 70.3398 | $ 3| 59.7186 61.5342 6| 63.0110 9! 66.1904 67.8970 69.2828 61.2848 63.1030 64.5777 67.7616 69.4668 70.8550 59.7661 61.2389 64.4203 66.1310 67.5128 57.9510 - POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 51 1396. Januar 1. ес]. Un+2 +2 2 2 Bemerk y PÈRE © aan 3 — 198 sin 1’ y—-tgdsin! | zur Aufnahme. mm mm mm mm ©] + 3.0300 — 0.0013 + 3.0287 Mondschein. Un- ï 0.0000 0.0000 durchsichtige Luft. . — 0.0804 + 3.4416 Bilder 2. —24.5666 — 0.0094 —24.5760 —24.5874 — 0.0689 —24.6563 + 5-2744 + 4.8486 + 4.8509 —+ 4.4298 + ce + 3.0335 + + + + 1.5580 + 1.6240 3.3244 — 4.7160 Trabant — Jupiterscentrum. угу» | Mittel. [углу | 7 (ere) era] PL | 4 тт —=0.6344 —+-0.6365 +-0.6351 0.6376 +-0.6304 +-0.6343 —0.9331 —0.9347 —0.9329 ея + 5 A —0.9330 | 99346 | —0.9285 0.0027 0.0015 0.0001 0,9328 —0.9388 —0.9350 +-2,4037 р -+2.4034 + 3.9658| -+-2.4078 + 0.7838] -+-2.4078 — 0.9284] -+2.3960 — 2.3091| -+2.4069 +0.6347 | 26306 | -+0/0016 | -+0'0004 | —oloooı | -+0/6325 PERS РГ —+2.4042 | -+2.3885 | 0.0069 —0.0010 | —0.000т | -+2,3943 M—Centrum — + 3/0030 N— » = + 3.4498 Q— » = —24.4298 R— » = —24.4658 8% = +19° 8/1 128 = 0.99347 fs =0.99294 f's = 099347 $23 = —0.00086 is = —0.00073 Js = —0.00085 11 LD Object. Dos aa SORA HR RP SR Se QE SR P.-Kr. 0° mm 64.2516 64.2508 20.1194 72.8796 22.5768 66.9615 67.4163 67.8970 66.9990 67.4458 67.9110 66.9860 67.4218 . 67.8806 66.9900 67.4188 67.8640 66.9595 67.3913 67.8451 66.9735 67.4143 67.8696 65.2878 65.3118 65.2868 65.2724 65.2508 65.2708 70.8376 70.8746 70.8520 70.8426 70.8206 70.8431 61.8770 61.9036 61.8920 61.8820 61.8586 61.8780 66.1749 66.2054 66,2089 66.2049 66.1819 66.2084 Scalenablesung. ны P.-Kr.180° | t-+k “mm 10006! 10006 + 8 ES ven: +11|-— 2 —+-18|-+-29 —-10 +10 +-10 +10 +-10 —то +10 +10 +10 +10 +10 +10) и 1 +11 +11 =-1] и РО +10 +10 61.1361 64.1353 108.2677 55-5084 105.8086 61.4612 60.9950 60.5288 61.4098 60.9535 60.5092 61.4353 60.9905 60.5352 61.4378 60.9845 60.5478 61.4568 61.0095 60.5657 61.4478 60.9860 60.5458 63.1050 63.0790 63.1065 63.1194 63.1444 63.1270 57.5492 57.5212 57.5382 57.5502 57.5782 57.5512 66.5102 66.4842 66.5008 66.5162 66.5368 66.5172 62.2184 62.1924 62.1839 62.1889 62.2114 62.1849 Scheinbare Adif: — ох \D 00 00 00 0010 J Onunun un À OO O \O \0 IETRETISSETITTIEETTIT ЕЕ ЕЕ ЕЕ ЕЕ НЕЕ Е ЕЕ ЕЕ, ВЕ! ВЕН Centrum = —46!6757 Ka 099320 = + 9.0563 h = —43.9750 То = 0.992387 —i, = -+0.00125 xı,=—43 he 9% Try ay —=8 28.6 Ta —=10:99818 dy =: 00158 Е. Renz, 1896. Januar 20. Pulkowaer Sternzeit der Aufnahmen. Mittel. mm 1081575 —= 3.1896 + 3.1636 Ты + 3.1594 + 3.1362 42 1132 44 + 3.1552 43 Trabant — Jupiterscentrum. aan) Ли) Ph, | Ar cos à Lt— Ty | Mittel. тт тт 4 1.0340] —2.1233 ds en 4 etwas ep Е ER — 2.1344) — 2/1198 | -+0:0009 o!cooo | — 2.1189 a 0.9958] — 2.1404 4 T.0144| — 2.1408 3—4 6.5868] -+-3.4295 4—5 6.6194] +-3.4298 : À 6528 Her -+3-4309 | 3.4075 | —0.0015 | 0.0000| +3,4060| 3—4 6.5638] 3.4276 3—4 6.5884] +3.4332 > 3—4 2.37421 —5.5315 3—4 4 2.3480] —5.5376 à A elli if eo. т —5.5324| —5.4947 | —+0.0024 0.0000 | —5.4923 | 3—4 a 2.3968] — 5.5330 3—4 2.3774| —5.5326 3—4 | 1.9206] —1.2367 4 Е | 1.9488| —1.2408 + ellij | ie ee. —1.2176| —1.2093 | -+0.0007 0.0000 | —1,2086 en 1.9275] — 1.2087 3—4 1.9540] — 1.2012 3—4 —1°% = +0.0C118 Refr: =— y =+ POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 53 1896. Januar 20. Decl. %1+% +7; Bemerkungen ey Later ti yes 3 EE ide 2 x ci ’ У—= #96 sin 1 zur Aufnahme, 90°] ++ P.-Kr. 270° | ++ 61.6674 64.6658 0.0000 0.0000 ВИ4ег 3—4, unruhig. 64.1704 — 0.1022 + 0.3932 92.2655 — 0.0038 — 27.6013 92.2875 — 0.0890 — 27.7090 59.5527 59.9875 60.4458 61.2164 61.6447 62.0760 62.7422 63.1684 63.5957 64.43 18 64.833 1 65.2469 66.0950 _ 66.5112 66.9380 fiat .2519 68.6912 + 4.6890 74.0333 + 1.5084 — 0.1601 ГЕН +++ +++ Е — 1.8383 — 3.5802 Trabant — Jupiterscentrum. и-у» | Mittel. fav [За ег) |Чер-еы"| вы. | 48 тт тт _ 59.3898 = +-0.5908 . Bene -- ме: | 62.5562 + —0.6034 ‚ р , : |. | 64.2314 bh +-0:5979 +0.6001 ‚| -+0'5961 | -+0:0028 | -+0!0004 0.0000 | -+0:5993 65.9036 — —=0.6039 67.6457 — +0.6036 60.9620 + —0.9828 | и —- вает” р _ 64.1410 + —0.9804 | _ 2e не 1% | av" | 65.815: ke 0.9853 || 0.9814 0.9749 0.0045 0.0018 0.0C00 0,9812 11| 67.4868 — —0.9791 69.2319 —. — 0.9838 58.4118 + —+-1.5646 60.0594 + en 1.5932 Er +1.5672 В 63.2644 = +-1,5667 +1.5678 | 1.5574 | +0.0073 | -+0.0092 0.0000 | -+1.5649 64.9410 _ +1.5667 | 66.6802 — +-1.5684 59.5272 —- -+0.4522 QUE + A2 2.710 = +0,44 2 6 43838 + +-0.4469 0.4513 | -+0.4483 | -+0.0016 -+0.0003 0.0000 | -+0.4502 66.0574 +0.4505 67.8016 +-0.4477 re Decldiff: N—Centrum = +- а Sa =0.99343 4 =—0.00135 — » =—27.433 à | — № 7 fs = 0.99287 д = —0.00120 X в=— 4/1 f'a =0.99340 Js = —0.00132 6% = +19° 45:9 | | | Pulkowaer Sternzeit 54 К. Renz, 40 A. 1896. Januar 27. № НВ Scalenablesung. р 4 ино LOSS оса Lo Se SS ay = 8" 24.7 P.-Kr. 0° |&-+X| P.-Kr.180°|#+% der Aufnahmen. Mittel. mm mm | 10000] 10000 63.0401 65.3484 с a 59.8560 68.5308 |+16| © 3 \ 15.7262 112.6613 |+ $|-+32 5 à 2—3 ellipt. 63.0392 65.3468 |-+16@ 0 5 54 3 3 68.4794 59.9114 |+20]— I 2—3 18.1810 110.2052 |+ 9|+-31 2—3 64.1294 |+10| 64.2834 |+ 9 —+ 1.0772 Ba 64.5592 |-+18| 63.8421 |+ 9 + 1.5132 + 1.5126 6 arts 3—4. Der We 65.0010 |-+18| 63.4153 |+ 9 + 1.9474 ' bei allen A schärfer be 64.1799 |+ 9| 64.2159 |+ 8 + 1.1362 [als de 64.5907 |-+17| 63.8081 |- 8 + 1.5459 + 1.5480 3 48 2—3 } 65.0150 |-+17| 63.4003 |+ 8 + 1.9620 Gh 4” 19 64.1664 | 9| 64.2389 |+ 8 + 1.1180 64-5772 |+17| 63.8226 |+ 8 + 1.5319 + 1.5343 4 48 2—3 65.0055 |+17| 63.4088 |-н 8 + 1.9530 64.1490 |+ 8| 64.2539 |+ 8 + 1.1017 64.5752 |-+16| 63.8211 |+ 8 + 1.5316 + 1.5344 2—3 65.0220 |+-16| 63.3913 |+ 8 + 1.9699 | Trabant — Jupiterscentrum. Lt—Ly | Mittel. Рае) Лигу Ph, | Ax cos à mm тт 62.7766 |+11| 65.6182 |+11 — 0.2666] —1,7792 . à ù 62.8066 |-+10| 65.5892 |-+-10 — 0.2372] —1.7852| __ ne , р __ 477 — 62.7861 |-+10| 65.6132 |+10 — 0.2594] —1.7937 1.7880 1.7760 | -+0!0007 o!oooo | —1:7758| 3 62.7856 |+ 9| 65.6127 |+10 — 0.2594] — 1.7938 3 67.8590 |+19 a +14 Bir и = : 67.8990 |+-19| 60.4982 |+14 —+ 4.8548| 3.3068 MA — 67.8786 |+18| 60.5172 [+14] |-+ 48350] +3.3007 -+3.3038 | 3.2816 0.0014 0.0009 | 3,2802 | 53 67.8810 |+-18| 60.5142 |+15 + 4.8377| --3.3033 2—3 59.0485 |+12 DT +14 — 3,9956 — 5.5082 us 59.0810 |-11| 69.3124 |+14 — 3.9617] —5.5097 | _ oi am 20.0605 In-tıl 693308 ia — 3.9811] —$.5154 5.5114 5.4744 | -+0.0023 0.0009 | —3.4721 | 3 59.0645 |+11| 69.3284 |+13 — 3.9779] —5.5123 3 70.2814 |-+17| 58.1114 + 5 + 7.2398] 5.7272 . | À ; 70.3158 |+17| 58.0810 |#+ 5 + 7.2722] +-5.7242 at —3. 20.2028 кб des roto/ let Pre Febr +-5.7207 | -+5.6823 0.0025 0.0000 | -+5,6798 2—3 70.2928 |-+16| 58.1034 |+ 6 + 7.2494] 5.7150 3 Scheinbare Adiff: M— Centrum— — 3:3498 13 =0.99331 —1° y = +0.00136 N » = — 50.0260 i Q— » = + 5.7065 fa = 0.99296 —% = -+0.00145 X Ww=— 50 R— » = — 47.3255 Ве. = — 7 Try = + 16 Га = 0.99329 Je —+0.00154 Bilder, | | POoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. - 55 1896. Januar 27. Decl. Nr, Bemerkungen У — 5 tgù sin 1 zur Aufnahme. 61.0160 mm mm mm mm 55.6558 + 8.3601 — 0.0006 + 8.3595 Leichte Wolken. 55.1630 + 8.8554 — 0.1174 + 8.7380 Bilder 2. 64.0152 À 0.0000 \ 0.0000 . 83.2534 —19.2354 — 0.0015 —19.2369 83.2717 — 19.2564 — 0.1030 — 19.3594 58.9805 + 5.0422 59.3893 + 4.6386 + 4.6395 59.7921 Ar 60.5862 + 3.4352 8] 60.9870 + 3.0400 — 3.0403 | 61.3828 + 2.6456 62.2714 + 1.7510 62.6726 + 1.3562 + 1.3559 63.0710 + 0,9606 63.9560 + 0.0688 _ 64.3708 — 0.3448 — 0.3421 64.7791 — 0.7504 Trabant — Jupiterscentrum. = T : Ye —У% | Mittel. |" ë (и— уз) Ja (ее з) | - (ии? Ph. | 45 тт тт + —+-0,4855 . . 6 1; ’ r U [3 x и = pau +-0.4839 | +0!4808 | +0/0030 | -+oloooı 0!0000 | -+0'4839 9| 63.8786 + —=0.4814 Ban = —0.9071 1.8920 = TONNES AE me pe = Ge | 63.5757 = 09131 0.9117 | —0.9058 0.0055 0.0011 0.0000 0.9124 | 65.2718 — — 0.9135 57.8630 Eu +1,5155 | Laura 35 Saas +1.5158 | -+1.5060 | 0.0091 | —0.0007 0.0000 | -+1,5144 2 62.8411 + —+1,5174 Bean -= — 1.6201 © 2.6007 = —1.6233 | _ 21 2 : _4 6993 8 64.2828 Er —1.6207 1.6209 1.6103 —0,0095 —0.0027 0.0000 1.6225 65.9800 — —1.6195 | - с | bare Decldif: M—Ceutrum—+ 8'3180 fg =0.99355 5 = —0.00168 N— » = + 8.7652 ; р ie » = —19.1165 fs = 0.99297 13 = —0.00149 X ig=— 5ı — D» == —19.1518 4 Г; =0,.99352 J5 = —0.00165 62 = -+20° 0.0 56 Е. Вами, 40 1. 1896. J anuar 27. № Scalenablesung. PRE UE Pulkowaer Sternzeit 10 с о Р.-Кг. 0° tt P.-Kr.180° |#-+X 5 der Aufnahmen. Mittel. Anbhaltstlerne| wie 40 A, mm mm mm 10000 10000] 10000 mm mm mm fa | 61.0020 |+10| 67.4078 |+ 9 — 2.0487 an D ФВ fe | 61.4348 [10] 66.9615 |+ 9 — 1.6092 — 1,6061 CN 8" 3 un 61.8930 |+ 9| 66.5222 |+ 9 — 1.1604 %9щ | 61.0510 |+-10) 67.2518 |+ 8 — 2.0012 д Je | 61.4898 |+10] 66.9145 |+ 8 — 1.5581 — 1.5637 11 48 2—3 go | 61.9200 |+ 9 66.4922 |+ 8 — 1.1319 вт %hy | 61.0130 |+11| 67.3943 |+ 8 — 2.0364 he | 61.4328 |+11| 66.9635 |+ 8 — 1,6110 — 1,6076 12 .43 2—3 ho | 61.8760 -+-10| 66.5352 |+ 8 — 1.1754 SER %1 | 61.0430 |+11| 67.3568 |+ 8 — 2.0026 ie 61.4862 |+11| 66.9250 |+ 8 — 1,5651 — 1.5675 13; 45 2—3 dp 61.9180 |+10| 66.4962 |+- 8 — 1.1348 Trabant — Jupiterscentrum. aa» | Mittel. его (ии) Ph. | а cos $ mm mm If | 59.6292 |-+14| 68.7671 |-+14 — 3.4148 nn 3 g À 59.6752 |+14| 68.7246 |+13 — 3.3705| —1.8068 | _ „| mm р ‚ er 3 h | 39.6252 |+15| 68.7706 |+13 — 3.4184] — 1.8108 1.8113 1!7992 | --0:0006 0/0009 1.7986 | ; i 59.6566 |-+-15| 68.7376 |-+13 — 3.3862] —1.8187 2—3 ПТ | 64.7456 |-+16| 63.6477 |+ 9 1.7034| 3.3095 2—3 = 9 | 64.7981 |+16| 63.5972 |-+ 8 + 1.7559] 3.3187 3 2—3 h | 64.7521 |+16| 63.6437 |+ 8 + 1.7088] +3.3164 3.3146 | -+3.2924 0.0011 0.0000 | -+3,2913 = | i 64.7901 |-+17| 63.6067 |- 8 1.7463] +3.3138 2—3 I f 55.9266 |— ı| 72.4708 |-+11 — 7.1186 BE 3 à 9 55.9720 ol 72.4238 |+11 — 7.07231 —5.5086 | _ 18 Kir 2— № | 55.9250 0| 72.4672 |1 — 7.1175] —5.5099 5.5119 5.4749. | -+0.0018 0.0000 5.4731 2—3 i 55.9575 | ı| 72.4328 |+12 — 7.0840] —5.5165 3 IVf | 67.1450 |-+ 8| 61.2508 |1 + 4.1011|+$5.7072 : 2 4 9 67.1899 |+ 8| 61.2069 |+t1 + 4.1455| -+5.7092 LA. „n| 2— Dieses ut da lee din | 3408) +-5.6670 0.0020 | 0.0000 | -+5,6650| 5 8 67.1749 |+ 9] 61.2169 |+10 + 4.1331| 5.7006 | 2—3 Scheinbare Adiff. wie 40 A. 719% =0.99331 —®, =-0.00136 Ло = 099296 —iy = -+0.00145 X y —=— 50 Refr. = — 7 Try =— 17 Г’: = 0.99329 Л, —=+0.00121 Iy= 8 24.7 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTORRAPHISCHEN AUFNAHMEN. 1896. Januar 27. Decl. Zat%o+2% 2 2 8 y 5 — 408 sin 1’ y — = tgù sin 1" [НН Р.-Ке. 270° ++ y 3 егпе| wie 40 А mm mm 10000] 10000 66.3258 — 2.2902 Br 65.9090 — 1.8792 — 1.8754 65.4838 — 1.4568 64.5457 — 0.5186 64.1440 — 0,1146 — 0.1149 63.7376 —+ 0.2884 62.6642 + 1.3667 62.2738 —+ 1.7554 + 1.7619 61.8590 + 2.1636 60.9056 + 3.1244 60.4892 + 3.5368 + 3.5355 | 60.0760 + 3.9453 Trabant — Jupiterscentrum. > р т У: — 99 | Mittel. fa (иг у») |7 (ве) (и-ал)з тт тт 65.3998 —- #04933 3.0502 Е —-0.4867 р у ri 61.7691 = +-0.490$ —=0.4900 | -+0:4868 | <+-0:0031 0.0005 59.9930 + +-0.4893 ral — —0.9136 5.0510 = —0.9194 | _ тв e 63.1749 ar 0.9174 0.9178 0.9118 0.0055 0.0000 61.4063 5. — 0.9209 64.3778 — -+1.5182 2.0192 <= +1.5151 т 12 60.7382 = 1.618 а +1.5076 -+0.0091 0.0026 58.9645 En +-1.5179 | 2.393 = en 5.7552 == —1.6201 | _ у LR Г. - 8| 63.8746 + 0.1442| —16177 1,6186 1.6081 0.0094 0.0008 Я | 62.1020 + 1.9158 —1.6197 e Decldifr. wie 40 A. 198 =0.99355 $2; = —0.00168 18 = 0.99352 Уз = — 0.00165 6% = +20° 0!0 San. Физ,-Мат. Отд. fs = 0,99297 13 — —1,00149 < 13 = —$'I 57 Bemerkungen zur Aufnalıme, 0/0000 0.0000 0.0000 0.0000 -+0:4894 —0,9173 1,5141 —1.6183 58 F. Renz, 41 A. 1896. Februar 1. Æ Scalenablesung. Pulkowaer Sternzeit Object. 8 = and nm. P.-Kr. 0° | P.-Kr.180° + der Aufnahmen, Mittel. mm 10000 10006] 10000 Ctr. | 62.8325 65.5532 |. . S 62.8316 |+ 9] 65.5522 |+10 0.0000 3 М | 67.8101 |+19| 60.5722 |+10 + 4.9798 N 3 N | 23.6768 |+26| 104.7060 |+ Le —39.1516 7 68" 55 2—3 Q 76.4476 |+20| 51.9410 |-+21|-— 4] +13.6132 2—3 В 26.1406 |-+37| 102.2396 |+14|+21] —36.6859 3 4b, | 68.7072 |+13| 59.7096 |+14 + 5.8591 6, | 69.1184 |-+13| 59.2828 |+10 + 6.2783 + 6.2839 о 6, | 69.5537 |-+13| 58.8461 |-+10 + 6.7143 3 сш | 68.7252 |+13| 59.6866 |+-14 + 5.8796 Co 69.1584 |-+13| 59.2429 |+10 + 6.3182 — 6.3171 От D 69.5932 |-+13| 58.8071 |+10 + 6.7536 $ 7 оф 3—4 2% dy | 68.6882 |+13| 59.7166 |+15 + 5.8460 de | 69.1144 |-+13| 59.2868 |+711 + 6.2742 + 6.2760 (DM (©) dy | 69.5498 |-+13| 58.8550 |-11 + 6.7078 2 %е | 68.6962 |+14| 59.7102 |+15 + 5.8533 ес 69.1330 |-+14| 59.2798 |--11 + 6.2871 + 6.2853 8 45 CA 69.5552 |+14| 58.8451 |+11 + 6.7156 2—3 Trabant — Jupiterscentrum. 4 —ay | Mittel. |f’ Ic u) Ph. | Au. cos à mm тт I Geht durch |die Jupiterlsche|i ПЬ | 66.4612 |+11| 61.9316 + 3.6252] —2.6587 = с 66.4908 |+10| 61.9050 + 3.6533| —2.6638 , , Br, _ оф г а | 66.4478 10] 61.9480 + 3.6112] —2.6648 —2.6647| —2:6466 | +0:0011 0.0001 2.6456 | 9_3 е | 66.4518 |+10| 61.9450 + 3.6138] —2.6715 3 ШО | 71.0770 |+12| 57.3148 + 8.2416] +1.9577 ut. € | 71.1100 |-+12| 57.2828 + 8.2740] +-1.9569 a |, 2— 4 | 71.0640 |-+12| 57.3258 + 8.2296] +-1.95 36 Ba er 0.0001 | 1.9888 3 e 71.0650 |-+13| 57.3258 —= 8.2300] +-1.9447 2—3 IV b 59.6692 |-+15| 68.7246 — 3.1672| —9.4511 “sh с 59.6976 |+ 15| 68.6956 — 3.1386| —9.4557 | __ Je dl a — а | 59.6632 |+14 я — 3.1756] —9.4516| 94551 9.3906 | —0.0038 0.0001 9.3869 | 3 e 59.6602 |-+-14| 68.7342 — 3.1766] —9.4619 2—3 Scheinbare ВАШ: M— Centrum =-+ 5,2698 Fa = 9.993138 —i?, = +-0.00088 N— »› = —41.4067 Q— » =-+14.3263 16 = 0.99290 —y GE х = — 3.1 В— э — —38.7063 Ве". — Try = + Г’ = 0.99318 Та = ви 109, Bilder. ® H mm mm 1000011000) mm 61.9056 64.9040 |+16| о 0.0000 61.8762 |+10] o|+- 3.0282 61.3854 |-+27|— 2| + 3.5190 89.4786 |— 2|-+ $|—24.5716 89.5031 |+ 9]-+14| —24.5970 62.9930 |+11 + 1.9210 63.4013 |+-11 + 1.5179 63.8001 |+10 + 1.1186 64.7581 |+18 —+ 0.1634 65.1649 |+-18 — 0.2457 65.5662 |-+-12 — 0.6469 66.4758 |+10 — 1.5606 66.8766 |-+-1о — 1.9610 67.2768 |+10 — 2.3604 68.2089 |-+20 — 3.2918 68.6117 |+-15 — 3.6956 69.0150 |+15 — 4.0976 62.6806 |+10 + 2.2290 64.4453 |+ 9 + 0.4640 66.1649 |+11 — 1.2546 67.8906 |+19 — 2.9809 63.9770 |+10 + 0.9306 65.7392 |+12 — 0.8304 67.4578 |+-10 — 2.5491 69.1789 |+3 — 4.2718 60.9356 |+11 —+ 3.9782 62.6916 |+10 + 2.2171 64.4178 |+ 9 —= 0.4956 66.1430 |+-11 — 1.2319 N— »› =+ 3.4505 Q— +» = —24.4312 R— » = —24.4665 dy =-+20° 9:9 Decl. %п+%е+2; 8 тт + 1.5192 — 0.2431 — 1.9607 — 3.6950 9—9» | Mittel. mm mm —0.7098 +0.7071 -0.7061 -0.7 141 —0.5886 —0.5873 —0.5884 —0.5768 +-2.4590 +-2.4602 +-2.4563 +-2.4641 128 = 0.99330 fs = 099282 fa = 0.993239 +0.7093 —0.5853 2.4599 POSITIONEN DER J UPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 15396. Februar 1. x? < _. x? . — 5 9681 Г у—- toÿ sin l’ mm mm 0.0000 0.0000 — 0.0013 + 3.0269 — 0.0805 + 3.4385 — 0.0094 —24.5810 — 0.0693 —24.6663 Trabant — Jupiterscentrum. | 'з(уг— уз) | Jg (21—24) | Не-а. +-0/0014 +0:7046 | -+0:0024 —0.5814 | —0.0018 —0.0015 -+2.4434 | -+0.0086 —0.0016 $75 = —0.00093 ig = —0.00090 X ig—=— 3 Js = —0.00091 59 Bemerkungen zur Aufnahme, Mondschein. Bil- der 4. „0.0000 +0'7084 0,0000 —0,5847 0.0000 +-2,4536 60 Е. Renz, A1 153. 1396. F'ebruar 1. № Scalenablesung. Pulkowaer Sternzeit Obi ET ua le x Pac a SR RE ee“ Bilder. P.-Kr. 0° a P.-Kr. 1800|:+-% 3 '| der Aufnahmen. Mittel. Anbaltstlerne| wie 41 A, mm mm mm 10000 10000! 10000 3 mm mm mm mm 2] w | 59.3484 |11| 69.0600 |+14 — 3.4956 sts fe | 59.7482 |+15| 68.6572 +14 — 3.0941 — 3.0863 Ве: 13 2—3 Fo | 60.1699 I+-ı5| 68.2284 |+19 — 2.6691 %9щ | 59.3224 |-+ 10| 69.0810 |+14 — 3.5192 de | 59.7541 |-+14| 68.6552 |+14 — 3.0902 — 3.0908 тт 2—3 90 | 60.1764 |-+14| 68.2224 |+19 — 2.6629 8* gm 30° %Й | 59.3728 |+-10| 69.0315 |+-14 — 3.4692 he | 59.7731 |-++14| 68.6297 |+14 — 3.0680 — 3.0621 13 58 2 ho | 60.1909 |-+14| 68.2094 |+19 — 2.6492 Zip | 59.3603 |-+11| 69.0500 |+13 — 3.4846 Le 59.7891 |+15| 68.6107 |+13 — 3.0504 — 3.0507 Ио 2—3 %0 60.2194 |+15| 68.1739 |+18 — 2.6170 Trabant — Jupiterscentrum. a | Mittel. Аж] Ph. | As cos Ô | тт mm Geht dufrch |die Jupiter|schelibe. ИЛ | 57.0754 |+ 9| 71.3238 |+13 — 5.7640 N er unterex] 9 | 57.0650 |+ 9| 71.3288 |-+13 — 5.7718 —2.6810| __ aller р er BR. = № | 57.1040 |+ 9! 71.2964 |+12 — 5.7360] —2.6739 2.9773 29584 00004 ООО 2.6586 unterexponie р 57.1100 |+10| 71.2838 |+12 — 5.7266 —2.6759 III f a —=10| 66.7062 |+10 — 1.1482 u à 9 | 61.6796 | 9 66.7166 |+- 9 — 1.1582| +1.9326' ER + h | 617116 |+ 9 66.6836 |+ 9 — 1.1256] +1.9356 -+1.9345 | -+1.9213 0.6003 0.0001 | 1.9209 | 23 à | 61.7172 |+ 9] 66.6776 |+ 8 — 1.1198] -+1.9309 3 IV f АН + 5| 78.1030 |+ 9 mr Er area 9 50.2928 |+ 5| 78.1070 |+- 8 —12.5469] —9.4561| __ 2 8 22 — р h 50.3278 |+ 6| 78.0730 |+ 8 — 12.5124] —9.4503 3408 aaa 79.0084 nn 9.3882 2 unterexpo. р 50.3364 |+ 6 78.0670 |- 8 —12.5050] —9.4543 Scheinbare Ædiff. wie 41 A. fe PR 0.993 18 Die, 1000088 То = 0.99290 —i, =-0.00089 Xi = 3" ; Ref. = ö ВИТ Try = — 33 a = 0.99318 J, = 0.00056 h т ay =8 219 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 61 1296. Februar 1. Decl. Bemerkungen zur Aufnahme. x «+ 47 ЕВА — = #06 sin 1 у—- tgèsin1 P.-Kr. 270° t-+-k wie 41 A, er mm mm 68.9770 — 4.0615 68.5932 — 3.6762 — 3.6739 68.1999 — 3.2840 67.1734 2.2579 "66.7791 — 1.8596 — 1.8600 66.3803 1.4624 65.3973 — 0.4842 65.0265 — 0.1054 — 0,1021 64.6312 + 0.2833 63.6397 + 1.2784 63.2374 + 1.6814 + 1.6837 62.8281 + 2.0914 Trabant — Jupiterscentrum. и — Ух | Mittel. р "а (ии) Jy(a—ay)|-w2-2)% Ph. 45 mm mm | — 0.7119 de а +0.7108 | -+0:7060 | 0,0024 | --0!0013 0.0000 | +0:7071 + —+-0.7106 | 69-1714 — — 0.5872 Ben: = Mere —0.5878 | —0.5839 | —0.0018 | +-0.0004 0.0000 | —0,5853 63.8121 == —0.5869 14| 66.1180 — +-2,4669 “are 23 Bee -+2.4650 | -+2.4485 | -+0.0086 | —0.0079 0.0000 | -+2,4492 60.7636 => -+2.4632 ЕТ Su. nb e Decldiff. wie 41 A, 15e = 0.99330 ws = —0.00093 fs = 0.99282 is =—0.00090 № ig=—3!1 J'a = 0.99329 Is =-— 0.00091 dy =-+20° 9'9 ' 42 A. " F. Renz, 1896. Februar 3. A Scalenablesung. Pulkowaer Sternzeit P.-Kr 0° |+ Р.-Кг.180° 1+5 3 der Aufnahmen. | Mittel. mm mm mm N 10000 10000] 10000 Ctr, | 64.1128 64.9738 7% ou U 64.1120 | 8| 64.2730 |+ 8 Ге) 0.0000 3 M 76.4498 |+-11| 51.9337 |-+15|— 1| -+12.3383 2—3 N 32.3094 |-+24| 96.0730 | 4|+10] —31.7993 М PRE ee 2 Q 85.1176 |-+ 6| 43.2688 |--27|— 4] +21.0034 8 №4 2 R 34.8074 |-+28| 93.5776 |+ 3|-+-10] —29.3024 2—3 У 71.2164 |-+17| 57.1688 |-+13 Ol + 7.1045 2 т 72.2538 |+28| 56.1281 |+15|— 5] -= 8.1435 3 ZA | 70.с075 |+16| 58.4018 |-н 5 + 5.8839 à @с 70.4413 |-+16| 57.9605 |+ 5 + 6.3214 -+ 6.3236 8 25.229 2—3 a, 70.8910 |-+12| 57.5218 |+ 5 —= 6.7654 %6, | 69.9685 |-+16| 58.4383 |+ 5 + 5.8462 : x} GENE Ь; | 70.4028 |-+16| 58.0010 |+ 5 + 6.2820 + 6.2825 26 29 8 26 58 2—3 b, 70.8476 |+12| 57.5707 |+ 5 + 6.7193 %Cy | 69.9970 |-+16| 58.4143 [+ 5 + 5.8724 Ce 70.4243 |+16| 57.9855 |+ 5 + 6.3004 + 6.3049 27-209 2—3 A 70.8686 |-+12| 57.5468 |+ 5 + 6.7418 2% dy | 70.0230 |-+16| 58.3903 |+ 6 + 5.8974 de 70.4578 |+-16| 57.9430 |+ 6 + 6.3384 + 6.3385 28 26 3 do | 70.9060 |+-12| 57.5082 |+ 6 + 6.7797 Trabant — Jupiterscentrum. Lt—2% | Mittel. Later) Java! Ph. | Ac cos à mm mm 28 68.6322 |-+14| 59.7611 |+14 + — 1.8076 sen 68.5802 |-+13| 59.8101 |-+-14 + 4.4655] —1.8170| __ rh р Ber, A8 — nl 68 Ao6a Laura | бомб: Let + 44808| —1.8151 1.8146 1.8020 | -+0!/0007 0.0001 1.8014 | ; а | 68.6352 |-+13| 59.7566 |-r15 + 4.5197] —1.8188 2—3 Па | 73.7152 |-++13| 54.6766 |— 1 + 9.6c05| -+3.2769 an b | 73.6702 |-+12| 54.7226 |— 1 + 9.5550] -+3.2725 Bi ie = в даб || 1840056 en gr BE -+3.2764 | -+3.2536 0.0014 0.0001 | -+3.2521 | $ d | 73.7306 |-+12| 54.6616 Ге) + 9.6156] 3.2771 2—3 =: 64.9845 |-+17| 63.4128 |+ 9 + 0.8668] — 5.4568 5 a ” 64.9326 |-+17| 63.4588 | 9 + 0.8178] —5-4647 | __ ns m‘ Ge: = e | 649615 Lr16l 63.4303 +9 + 0.8464] — 5.4585 5.4610 5.4231 | -Н0.0023 0.0001 5,4209 3 а | 64.9890 |-+16| 63.4013 |+ 9 + 0.8747| —5-4638 |" 3 IV : nie +10] 66.5802 |-+ 8 — 2.3000] —8.6236 ав 1.7696 |-+-10| 66.6277 |- 8 — 2.3484| —8.6309 | __ т у RN — e | 61.8011 |+ gl 66.5947 [+8 — 2.3162] —8.6211 8.6250 8.5652 | +-0.0036 0.0001 8.5617 | 3 а | 61.8501 |+ 9| 66.5632 |+ 8 — 2.2860] —8.6245 . 2—3 Scheinbare ВАШ: M-—-Centrum = -+13!0662 1 =0.99306 —1° 4, = +0.00086 N— » = —33.610$ : Q— » = -+22.1227 fa =0.99275 —, —=-+0,00086 x Üy= —30 Fe tee ИИ Es » = à x % = W— » = 8.6657 о =0.99306 Ja —+0.00154 0.2, = % 20.9 Bilder, M 61.6938 64.6922 54.7874 53.3375 81.3782 81.4558 76.8119 25.8726 61.1629 61.5732 61.9840 62.8950 63.3044 63.7032 64.5637 64.9690 65.3728 _ 66.3098 66.7222 67.1324 „61.0554 rg! 4.479 66.2379 62.4518 1| 64.1769 65.8441 67.5967 mm mm 10000! 10000 mm +16 о 8 о 2 une | +21|4- 4 —+-29l+ 6 + т -=27|—16 +12 НЕТ +11]. ER LI == +10 0.0000 +18 +18 +18 РЕ +++ +++ #12 +10 +10 = +10:8177 bare Decldiff: M—Centrum À) D —+r11.2652 — » = — 16.6170 — D .=—16.6523 УМХ » =-—11.4497 W— » = +38.5452 6% ==-н209 13'7 Decl. An+ac+%s + 3.1327 + 1.4047 0.2618 2.0177 -+0,4726 +0.4753 —0.4794 —-0.,4781 —0.8858 ‚—0.8829 —0.8834 —0,8817 —+1.4601 +-1,4608 —+1.4643 -+1.4611 +-2.3113 -+2.3099 -+2.3106 +2.3093 -+0.4764 —0.8834 +1.4616 +-2.3103 198 = 0.99323 f'a = 0.99322 1596. Februar 3. 0.0000 0,0080 0.0534 0.0227 0.0443 0.0026 0.0036 x? = 7 195 sin 1’ POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. x? Sn _. y— + tgù sin Г тт 0.0000 —-10.8994 11.3006 —16.7095 —16.8076 —11.5216 -+38.8150 Trabant — Jupiterscentrum. : . 23 vs | Mittel. |FatıY2 | Лаба) | бий-еалут] +0:4732 | -+0,0021 —0'оото —0.8774 | —0.0038 —0.0028 —+1.4517 | -+0.0063 -+0.0021 -+2.2947 | -+0.0100 —+0.0018 328 =—0.00118 13 —=—0.00117 X ig = —4.0 Is = - 0.00118 63 Bemerkungen zur Aufnahme, Bilder 2—3. Starker Wind. 0'0000 | -+0'4763 0.0соо | — 0,8840 0.0000 | -+1,4601 0.0000 | -+2,3065 64 Е. Rexz, 42 1. 1296. Februar 3. RR Scalenablesung. Pulkowaer Sternzeit Object. — à 5 2 Zur P.-Kr. 0° ++ P.-Kr.180° 1-й 8 der Aufnahmen. Mittel. Anhaltstierne| wie 42 A, ь тт mm mm 10000 10000! 10000 mm mm mm mm 4f | 62.1464 |+10| 66.2548 |+12 — 1.9738 RL Fe 62.5702 |+10| 65.8216 |+12 — 1.5453 — 1,5455 8685 139 3 ER 63.0070 |+10| 65.4018 |+18 — 1.1173 Zn | 62.1669 |-+ 9] 66.2329 |+11 — 1.9526 he | 62.6042 |+ 9| 65.7946 |+11 — 1,5148 — 1.5168 RS. О 3—4 ho | 63.0425 |+ 9] 65.3688 |+17 — 1.0830 gi 25" ger Zip | 62.1739 |+ 9| 66.2369 |+10 — 1.9510 Ag 62.6082 |+ 9| 65.7946 |+10 — 1.5128 — 1.5071 26 тб 3—4 d 63.0710 |+ 9 65.3464 |+16 — 1.0576 kp | 62.1729 |-+10| 66.2158 |+-Io — 1.9410 № | 62.6192 |+10| 65.7771 |--10 — 1.4984 — 1.4945 87.26 3—4 ko | 63.0840 |+10| 65.3324 |-+16 — 1.0440 Trabant — Jupiterscentrum. 1—2 | Mittel. ааа иги РВ. | Au cos ö тт mm a San BE +10 ER +19 — 3.3804 Bei 2—3 0.7596 |-+-10| 67.6342 |+19 — 3.3572] —1.8404 | __ rs , Ne AT 2—3 à | 60.7666 |-+-10| 67.6267 |-+18 — 3.3500] — 1.8429 1.8392 1.8264 | -+0'0003 0.0001 1:8262 3 k | 60.7821 |11| 67.6082 |+18 — 3.3329] —1.8384 3 au a +11| 62.5408 |+11 + 1.7371| -+3.2826 2 h 5.8866 |+-10| 62.5118 |+10 + 1.7679] +3.2847 Ei N = р 65.8950 |+10| 62.4972 |+10 + 1.7794] 3.2865 + 3.2870 | +3.2642 0.0006 0.0001 | +-3,2635 2—3 k | 65.9150 |+-10| 62.4768 |+ 9 —= 1.7996] -+3.2941 2—3 uf 57.1060 |+ 9| 71.2854 |-+13 — 7:0094 —5.4639 +2 ki 57.1344 | 9| 71.2594 |+12 — 6.9822| —5.4654| __ u RN Зи 3 ё | 571444 |+ OÙ 71.2459 |+-12 — 6.9704] — 5.4633 5.4634 5.4255 | —-0.0010 0.0001 5,4246 | 5__3 k | 57.1584 |+-10| 71.2299 |+12 — 6.9554] —5.4609 ve 53-9580 + 3 АВ +13 —10.1604! —8.6149 Е 12 | 53.9825 |+ 3| 74.4138 |-+12 — 10.1356] —8.6188| __ mx 1$ RS -1 3 © | 53.9940 |+ 3] 74-3988 |-+-12 — 10.1224] —8.6153 8.6138 8.5540 | --0.0016 0.0001 8,5525 | оз k 54.0150 |+ 4| . 74.3763 |+12 —10.1006] —8.6061 2—3 Scheinbare Ædiff. wie 42 A. fa = 0.99306 —® = -+0.00086 fa —=0,99278 —, —=+000086 Xi =— 30 Kefr. = [6) a —— 16 Г’ = 9.99306 То = —+0.00070 Les oo. lenablesung. т 69.8171 69.4198 69.0085 66.4602 66.0590 o| 65.6562 64.7002 64.2858 63.8600 63.0210 62.6067 62.1939 68.9240 70.2948 66.9430 ‚63.1589 6 63.4918 A УЕ +44 dy = +20° 13.7 POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 65 1396. Februar 3. Decl. Ant ot Bun; STE; Bemerkungen у EL; RE à #96 sin 1 > 190 sin 1 zur Aufnahme. mm mm 5.1144 4.7125 — 4.7112 4.3067 1.7534 1.3508 — 1.3513 0.9498 0.0069 0.4229 + 0.4240 0.8422 1.6830 2.1000 + 2.0982 2.5116 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. | 'з(иг-уз)| аби-гь |- Нейт] P > 52 тт тт 4.2250] -+0.4862 0.8686] —-0.4827 0.9100] -+0.4860 2.5808] -+0.4826 5.5978] —0.8866 2.2463| —0.8950 0.4646| —0.8886 1.2036] —0.8946 3.2380] -+-1.4732 0.1118] 1.4631 1.8941| -+1.4701 3.5630] +-1.4648 2.3924] 2.3188 0.9554| -+2.3067 2.7377| 2.3137 4.4088| -+-2.3106 —+-0.4844 +0/4811 +-0.002I —0!0005 0:0000 | -+0'4826 —0.8912 | —0.8852 | —0.0037 0.0000 | —0,8890 —+1.4678 | 1.4578 | -+0,0063 — 0.0025 0.0000 | 1,4616 +2.3124 | -+2.2967 | <+0.0100 | —0.0054 0.0000 | +2,3013 | о о ST — 195 = 0.99323 19; =-0.00118 Ss —=099275 ig =- 0.007 f's = 0,99322 Js = 0.00118 X ig=—40 em НИ 66 Е. Вами, 43. 1896. Februar 4. AR Scalenablesung. Pulkowaer Sternzeit Object. Ya Forms ВИС P.-Kr. 0° tk Р.-Кг. 180°| + a der Aufnahmen. Mittel. mm mm mm BEN 1000 mm 10000] 10000] mm pe Ctr. | 62.2399 66.1490 M Durch ет Jlupitersbild |verdjeckt. S 62.2390 |-+ 9| 66.1480 |+10] 0 0.0000 4 - N 23.0836 |-+25| 105.3010 | 7|-+17| —39.1516 7h 44" 9 4 Q 75.8686 |+-20| 52.5231 |-+16]— 3|-+13.6273 8 Е 25.5668 |-+37| 102.8230 |-+14|-=21| —36.6703 4 %а | 66.5012 + 9] 61.8870 |+ 9 -+ 4.2616 $ à ag | 66.9775 |+ 9| 61.4228 |+10 + 4.7318 + 4.7312 7” Bel 4 ао | 67.4508 | 9] 60.9595 |+-10 + 5.2002 2 byp | 66.5487 |+ 8| 61.8730 |+ 9 + 4.2924 b, 66.9930 | 8| 61.4093 |-+-10 + 4.7463 + 4.7428 34 34 4 b, | 67-4363 |+ 8| 60.9655 |+10 +- 5.1898 | 2 C 66.5222 |+ 8| 61.8850 |+ 9 + 4.2731 | р a 66.9660 |-+- 8| 61.4408 |+10 + 4.7170 + 4.7179 nie 35 34 7" 35” 34° 3 Co | 67-4238 |+ 8| 61.0053 |+10 + 5.1636 %а | 66.4788 | 8| 61:9340: |-+-10 + 4.2268 de | 66.9290 |+ 8| 61.4752 |+11 + 4.6813 —+ 4.6762 36 34 4’ do | 67.3703 [+ 8 61.0380 +1] + 5.1206 %е, | 66.5302 |+ 8| 61.8870 |+-10 —+ 4.2760 р ес | 66.9460 |+ 8| 61.4578 |1 + 4.6985 — 4.6995 И, 3 ео 67.3753 |+ 8| 61.0360 |+#11 + 5.1240 | | 4 ee. DC аа опппаиинижиаиинн “ L N Trabant — Jupiterscentrum. Е — Lo | Mittel. и] Tavr-—1)| Ph. | Aa cos à у , h mm mm Та | 69.0690 |+14| 59.3258 |+ 5 + 6.8266] +-2.0954 | 13 b | 69.0794 |+13| 59.3188 |+ 5 + 6.8352] -+2.0924 у 3—4 с | 69.0574 |-+13| 59.3408 |- $] + 6,8132] 2.0953 | -+2.0951 | -+2!0809 | —0‘o011 | —0'0002 +-2:0796 | 3—4 d | 69.0150 |+13| 59.3858 |- 6 + 6.7695] -+2.0933 | 4 4 e | 69.0440 |+13| 59.3568 + 6] + 6.7985] -+2.0990 | 2—3 Па | 67.5042 |+ 9] 60.8930 [+10 + 5.2601| -+0.5289 | b | 67.5082 |+- 8| 60.8916 |+10 + 5.2628] -+-0.5200 4—5 . с | 67.4828 |+ 8| 60.9146 |--то + 5.2386] 0.5207 | -+0.5174| +0.5139 | —0.0004 | —0.0002 | -+0,5133 | 4 { d | 67.4293 |-+ 8| 60.9655 |-HII + 5.1863] +0.5101 . 4 e 67.4518 |+ 8| 60.9470 |+11 + 5.2068] -+0.5073 i 4 ПТа | 62.7156 |+10| 65.6762 |+10 + 0.4742] —4.2570 14 4 b | 62,7242 |-10| 65.6722 |+-10 + 0.4806] —4.2622 с © 457 108 с | 62.7032 |+ 9| 65.6926 |-+-10l' + 0.4598| —4.2581 | —4.2575 | —4.2287 | +0.0023 | —0.0002| —4,2266| 4 d | 62.6642 |+ 9| 65.7326 |+11 + 0.4202| —4.2560 4 e | 62.6896 |+ 9| 65.7082 |+11 + 0.4452] —4.2543 3—4 1Уа | 60.5388 |--ı1] 67.8560 |+-18 — 1.7044| —6.4356 Ù || 3—4 . b | 60.5518 |+11| 67.8446 |-+18 — 1.6922] —6.4350 | ищегехро с | 60.5282 |-11| 67.8676 |+-18 — 1.7155] —6.4334 | —6.4334| —6.3898 | -+0.0035 | —0.0002 | —6.3865 | 3—4 | а | 60.4862 |+10| 67.9086 |-+18 — 1.7570] —6.4332 р 3—4 e 60.5148 |+10| 67.8840 |+19 — 1,7305] —6.4300 3 Scheinbare Adif: N—Centrum = —41:4067 Ju 0:99322 — = -+0.00149 — » = +-14,3263 Е » — —28.7063 fa = 099293 —ig =. DM X 4 = —50 Refr. = — Try =+ 2 Го = 0.993822 Ad =. 00196 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 67 1=96, Februar 4. Decl. Scalepablesung. “пн с+%; P.-Kr. 270° | ++ 3 Bemerkungen x? = _e 5 1 — 5 196 sin 1’ en FT #08 sin 1’ zur Aufnahme. тт_| тт 10000] 10000 verdleckt. +16 o 0.0000 0.0000 0.0000 Bilder 3. _ 64.6404 61.1426 |+27|— 2|-+ 3.4953 — 0.0805 + 3.4148 89.2070 |— 3|-+ 51 —24.5694 — 0.0097 — 24.5791 89.2587 |-+ g|+13] — 24.6180 — 0.0690 — 24.6870 61.0840 + 3.5708 61.5008 + 3.1496 + 3.1467 61.9386 + 2.7198 62.8560 + 1.7952 63.2838 + 1.3696 + 1.3706 63.7082 — 0.9469 64.6267 + 0.0273 65.0400 — 0.3890 .— 0.3889 65.4553 — 0.8050 66.3134 — 1.6586 66.7362 — 2.0842 — 2.0817 67.1509 — 2.5022 68.0740 — 3.4203 68.4738 — 3.8208 — 3,8182 68.8680 — 4.2134 Trabant — Jupiterscentrum, ve | Mittel. lfati-va а tee—az)-art-ar)t| Ph. ab 4 mm mm | 62.0540 —0.5565 63.8291 —0.5556 9] 65.5882 —0.5542 | —0.5539 | —0:5502 | —0'0030 | —0.0013 0'0000 | —0:5545 _ 67.2758 —0.5494 o| 69.0180 —0.5536 _ 61.7002 _—0.2013 63.4718 —0.1976 - 65.2279 —0.1969 | —0.1952 | —0.1939 | —0.0007 — 0.0003 0.0000 | —0,1949 66.9180 —0.1913 68.6532 — 0.1890 60.3108 +-1.1818 62.0910 -+1.1830 J 63.8496 +-1.1820 | +1.1837 | +1.1758 | -+0.0061 +-0.0012 0.0000 | +1,1831 01 65.5368 +-1.1873 67.2778 +-1.1845 59.7372 -+1.7605 a +-1.7588 7| 63.2764 1.7577 | -+1.7613 | 1.7495 | -+0.0092 +-0.001 1 0.0000 | -+1.7598 64.9610 +-1.7643 / 66.7012 +-1.7654 128 = 0.99332 #3 — —0.00144 Fes » abare Decldif: N-—-Centrum | : SUR fs = 0.99283 is =— 0.00139 X ig = —4:8 f's = 0,99331 4 = hl. Mid бу = 20° 15'4 — + —4 оса RSS LIT Lens | bd -ч ТУ P.-Kr. 0° mm 65,5304 65.5294 21.3892 74.1336 23.8220 60.2396 61.4032 69.8650 70.2978 70.7386 69.8546 70.2848 70.7256 69.8161 70.2449 70.6746 69.8550 79.2794 70.7226 71.0290 71.0020 70.9650 79.9940 72.2049 72.1879 72.1539 72.2004 74.5362 74.5162 74.4802 74.5152 Verfinst 44 A. += P.-Kr.180° mm 10000 10 +23 +-26 +39 —+-26 +20 +16 +16 +12 +-16 +16 +12 +16 +-16 -+-I2 +-16 +16 +12 ert. Scalenablesung. 62.8562 62.8552 106.9944 54.2538 104.5592 68.1383 66.9847 58.5350 58.1065 57.6680 58.5580 58.1160 57.6800 58.5880 58.1560 57.7360 58.5560 58.1160 57.6905 57.3655 57.3900 57.4310 57.4025 56.1895 56.2065 56.2435 56.1990 53.8545 53-8745 53-9150 53.8840 Scheinbare Adiff: Е. Renz, 1396. Februar 6. + der Aufnahmen. Mittel. mm mm 10000] 10000] mm тт +10] о 0.0000 2 + $|-+25| —44.1363 2 +15|— 2]+ 8.6032 7h 93" 397 2—3 À +-19|+-30| —41.7017 2 etwas еШр +-26|-+ 1|— 5.2864 1—2 | +21|+ 1|— 4.1278 ‚1—2 + SP + 4.3284 HS + 4.7591 + 4.7620 7. am 34 2—3 5 + 5.1986 +5 + 4.3118 +5 == BTS + 4.7485 11 34 2—5 „1500 т к м и: TR + 6 + 4.2774 + 6 + 4.7078 + 4.7059 12 49 2 «= + 5.1325 + 6 —= 4.3129 + 6 + 4.7451 + 4.7457 13 52 2—3 + 6 + 5.1792 Trabant — Jupiterscentrum. Tt—Ly | Mittel. Раба) Лав: уз Ph: | Ax cos à тт тт + 9 + 5.1948 -+0.73 28 Ar + 9 + 5.4690] -1-0.7205 , dut ох р 2— ит. + 5.4300] +0.7241 +0.7226| +0!7176 0/0001 0:0002 | +-0:7173| 5 —=10 + 5.4588 +0.7131 3 — 1 + 6.6712| +-1.9092 : 2—3 . Er a +1.9115 | -+1.8982 | —0.0003 | —0.0002 | +1,8977 ar: Ге) + 6.6642] 1.9185 3 + 3 + 9.0041| -H4.2421 2—3 + 4 + 8.9840] -+4.2355 AR AP 2—3 me: + 8.9458| +-4.2399 +-4.2376 | -+4.2081 0.0007 0.0002 | 4,2072 | 9__3 EA + 8.9788] —+4.233 1 3 N— Centrum = — 46/6767 F? x = 0:99306 — = +0.00011 — № —=-+ 9.0565 В— » = —43.9762 Fa = 0.99276 — —+0.00014 X и=- 0:5 У— » = — 5.5883 Вей. = — 3 W— » — — 4.3838 Try =-+ SI Г’, = 0.99305 Ju = -—0.00062 ay =8 19.4 Pulkowaer Sternzeit POosITIONEN DER J UPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 69 = 1896. Februar 6. | Dec]. Bemerkungen #nt%o+%s Le tgù sin 1’ y они sin 1’ о] ++] P.-Kr. 270° | ++ a! 3 Zur Anfiahrme. 65.5818 тт тт тт 65.5807 0.0000 0.0000 Bilder 2. Undurch- 65.0356 — 0.1022 + 0.4431 sichtige Luft. 93.1992 — 0.0038 — 27.6168 93.1618 — 0.0889 — 27.6700 87.9974 — 0.0014 —22.4162 37.6573 — 27.9229 63.1030 63.5092 63.9200 64-7776 5.1974 65.6007 66.5478 66.95 10 67.3518 68.2354 68.6472 69.0460 Trabant — Jupiterscentrum. | Mittel. ra We—va|Ts (орга ое р. | 48 у: 63.6502 |+I1 + 1.9364] —0.1452 Fée re Si pe Cart —0.1439 | —0:1429 | —0:0002 | —0‘0004 0.0000 | —0:1435 68.7781 |-+16 — 3.1918] —0.1418 64.0240 |+11 + 1.5630] —0.5186 DURE Es Е ие Е —0.5205 | —0.5169 | —0.0005 | —0.0012 0.0000 | —0,5186 69.1594 |-+16 — 3.5722] —0.5222 . 64.5967 |-+20 -+ 0.9862] —1.0954 | ob be. a2 pn а — 1.0926 | —1,0851 | —o.oo11 | — 0.0031 0.0000 | —1,0893 69.7232 |-+-20 4.1394] —1.0894 N— Centrum = -+ 0.4473 195 =0.99317 23 = —0.00026 — » = —27.4348 > : Е— » ——27.4702 fs = 0.99268 $5 = —0.00019 X 13 —=— 0.7 V— » = —22.2673 W— » =-+27.7277 f's =0.99317 Js = —0.00026 = Ôy = +-20° 19:0 70 F. Renz, 44 B. AR Scalenablesung. 2 w+#cH+?%o 3 P.-Kr. 0° tr] P.-Kr. 180° |+-+-% Anhaltstierne) wie 44 A, 1896. Februar 6. Pulkowaer Sternzeit der Aufnahmen. Mittel. Emm? _mm_|_mm_ 10000 10000] 10000 4 62.7896 + 9 65.6145 +-10 75712 9 +709 . ee), à. 62.3668 |-+ 9| 66,0190 [+10 — 3.1632 — 3.1613 № "С." 2 do 61.9700 |-+ 9| 66.4380 |+10 — 2.7496 2 hy | 62.8021 | 9] 65.6040. |+10 — 3.5996 he | 62.3663 |+ 9] 66.0355 |+-10 — 3.1718 — 3.1698 38 55 2 ho | 61.9400 |-- 9] 66.4650 |+10 — 2.7381 7h 39” 90° Zi | 62.7956 |+ 9] 65.6040 |+11 — 3.6047 % 62.3563 | 9| 66.0360 |-+11 — 3.1770 — 3.1744 40 4 2—3 Я 61.9370 |+- 9| 66.4720 |-+11 — 2.7414 Yky | 62.7756 |+ 9| 65.6340 |+11 — 3.6262 ke | 62.3428 |+ 9| 66.0635 |+ — 3.1976 — 3.1967 AT 14 3 ko | 61.9170 | 9| 66.4950 |+11 — 2.7664 Trabant — Jupiterscentrum. | mate | Mittel. |’), (из) Ph. | Aa cos $ mm тт Ig | 62.9895 | 9] 65.4050 — 2.5452 Lee pres h | 62.9760 |+ 9] 65.4150 — 2.5570| 50.612 ' , ay р — | in |'énpééo Le orgue 33672] 06072 +-0.6096 | —-0/6054 0/0000 0:0002 | +-0:6052 | à x k | 62.9400 |+ 9| 65.4540 — 2.5945] -+0.6022 ’ 3—4 > По | 64.3518 | 8| 64.0460 — 1.1843] +-1.9770 unterexp tn h | 64.3398 |+ 8| : 64.0510 — 1.1928] +1.9770 N 2— 1 рав 4 cube — 111920] +1.9824 +-1.9809 | 1.9671 | 0.0001 0.0002 | 1,9670 3 k | 64.3234 |+ 8| 64.0681 — 1.2095] 1.9872 2—3 219 66.5567 |+ 8 Fu ir Lo Mes ‚8 66.5418 |+ 8 1.8500 + 1.0087! -+4.1785 EB в | бо 8a + 1.0049] +-4.1793 | *4-1790 || 4.1499 -+0.0002 0.0002 4149 23 k | 66.5152 |+ 9| 61,8830 + 0.9790] -+4.1757 2—3 IV Verfinstlert. Scheinbare Adiff. wie 44 A. fu = 0.99306 —i°, =-+0.00011 1». = 099276 —y = -+0.00014 X y =— 05 Refr. =— I f'a = 0.993804 из 8} 19.3 Те, =— 34 Л. =—10.00021 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 71 1896. Februar 6. Decl. Bemerkungen EE 06 ait 1’ BR AA EET о 908 Y— 7% zur Aufnahme. 4 Из егие| wie 44 A. сы. mm + -+ 1.9925 + %4.9330 + 65.3438 + + 0.2495 65.7511 — 66.7282 — 67.1380 — — 1.5430 67.5468 — 68.3513 — 68.7656 — — 3.1664 69.1634 — 3.5673 Trabant — Jupiterscentrum. | T Fe | Mittel. Ira (и—у»)| To (ое er] Ph. | AB PE “= mm | 63.7152 —0.1209 Zur | Ben. -—-0.1147 | —0/1140 | —0'0001 | -+o/ooor o’oooo | —0'1140 68.8610 —0.1085 8 64.1354 ee 67.6622 ив = —0.5391 | —0.5354 | —0.0004 | -+0.0004 | о.00бо | —0.5354 69.2888 —0.5374 64.6802 —1.0851 er №: —1.0811 | —1.0740 | —0.0009 | -+0.0004 0.0000 | —1,0745 69.8246 — 1.0752 праге Decldiff. wie 44 A. f°8 = 0.99317 13 = —0.00026 fs —0,99268 is = —0.00019 x ig = —0:7 fs = 0.99315 Js; = — 9.00023 9% = +20° 19:0 72 Г. Renwz, 45 A. 1596. Februar 7. № Scalenablesung. | Pulkowaer Sternzeit . $ RE RE cites P.-Kr. 0° 2; Р.-Кг.180°| ++ der Aufnahmen. Mittel, an En _mm_|_mm_ 65.2716 65.1174 |0000 10000 65.2700 63.1165 + 9 O0 0.0000 70.2494 58.1328 |+ 5 о] + 4.9818 26.1208 102.2645 |-+ 4|-+-17| —39.1462 78.8617 8| 49.5264 |+15|[— 4] -+13.5903 28.5597 99.8217 |+12|-+21 ® 64.9689 63.4123 |+16| о 66.1081 62.2711 |-+14| © 68.0400 60.3695 |-+14 68.4700 59.9415 |+14 у + 3.1901 68.9045 59.5015 |-+-14 68.0455 60.3625 |-+14 68.4685 59.9365 |-+14 x + 3.1888 31 68.8955 59.5155 |+-14 68.0110 60.3925 |-+14 68.4255 59.9715 |-+14 . + 3.1520 32 68.8525 59.5510 |+-14 68.0460 60.3630 |+15 68.4695 59.9265 |H#15 - == 3.1936 33 68.8985 59.5010 |-+15 тт Trabant — Jupiterscentrum. Lt —Ly | Mittel. latex О) Ph. | Aa cos 5 mm тт - LI Lo оса RNA > ner à —0.7977 : 7.6690 0.7205 x —0:7912 | __ р т | 67.6430 60.7480 : — 0.7812 0.7861 -1-0.0001 —0:7809 67.6920 60.7000 5 —0.7744 71.3495 57.0425 à —+2.8865 71.3450 57.0485 р -+2.8825 71.3065 57.0860 у —+-2.8812 71.3475 57.0450 I 2.8806 an 54.5700 : 53595 то 54.5730 ; 45.3572 Ai 73.7830 54.6060 2 45.3600 +5.3586 0.0004 us 54.5650 .5915] 5.3579 72.5360 55.8590 ü +-4.0721 72.5385 55.8560 } +-4.0760 72.5040 55.8890 h —+4.0790 72.5485 55-8430 a -+4.0827 -+2.8827 — 0.0002 4.0774 — 0.0002 ‘ Scheinbare Adifi: M— Centrum = + 5:2698 fa = 0.99326 —#° „ = —0.00005 N— » = — 41.4068 Q— » = -+14.3263 fat 099297 —iy —=—0.00008 X и=- 03 Е » = —38.7063 Refr,. = + 3 V— » — — 0.3185 Try —=+ 34 W— » = +- 0.8860 Го = 0.99326 ‘Ju =—0.00029 ay = 8" 188 POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 73 1296. Februar 7. 1e. Decl. 4 Scalenablesung. Bemerkungen zur Aufnahme. x? CT x — — tgô sin 1’ Yy—— t-+-k 3 4 Kr.90° вые P.-Kr. 270° 64.6517 mm mm mm 64.6500 61.6264 61.0913 89.2370 89.2081 84.0385 33.7182 61.1710 61.5710 61.9695 62.7410 63.1370 63.5270 64.3290 64.7220 65.1125 0.0000 0.0000 Bilder 1—2. Recht 66.1350 |+-11 66.5380 |+ 9 66.9420 |-+ 9 61.3320 62.8960 64.4875 66.2970 62.3810 63.9420 65.5250 0.0013 — 3.0185 durchsichtige Luft. 0.0805 + 3.4767 ‘ 0.0094 — 24.5944 0.0689 —24.6292 0.0000 — 19.3903 -+30.9302 0.0000 -+30.9302 + 1.5239 — 0.0590 — 1.8784 Trabant — Jupiterscentrum. У: — У» | Mittel. |’ (из Ja (его) без Ph. | AG mm тт -Н0.2331 +0.2323 0.2267 +0.2326 —0.8165 —0.8133 —0.8144 —0.8094 + 3.3218 S ae +-0.2312 | +0:2297 | —0/0001 —+0'0003 0:0000 | -+0!2999 1.6458 2.2722 0.7106 0.8734 2.6878 —0.8134 | —0.8081 +0.0003 —0.0015 0.0000 | —0,8093 67.3399 A + 1.6446] — 1.4441 4.5715 + 0.0761] —1.4478 | _ HR su ры 61540 15058] —1.4448 1.4451 1.4358 | -0.0006 0.0034 0.0000 1.4386 67.9700 — 3.3220] —1.4436 5.3095 —+ 2.1448] —0.9439 4.0745 + 0.5782] —0.9457 | _ ЕЕ. = = . 65.6550 — 1.0036]. —0.9446 0.9444 0.9383 | 0.0004 0.0023 0.0000 0.9402 67.4740 2.8219] — 0.9435 + ЕЕ УЕ ЕЕ ЕТ + [ill р ’ Be - übare Decldiff: M—Centrum = + 3.0045 195 = 0.99353 $25 = +-0.00010 | N— » =+ 3.4510 à ь Q— » = —24.4312 fs = 0.99304 is = -+0.00004 X ig—+ о! R— » = — 24.4665 У— » = — 19.2638 fs = 0.99353 7 = 0.00011 W— » —+307310 Ôy = +20? 21.0 3au. Физ.-Мат, Отд. 10 D hr une 74 45 B. Scalenablesung. Object. P.-Kr. 0° ++ P.-Kr. 180° Anbaltstierne mm 62.0595 62.4615 62.8935 62.0235 62.4465 62.8750 62.0555 62.4680 62.8960 62.0200 62.4430 62.8755 61.7580 61.7390 61.7670 61.7475 65.3155 65.2855 65.3065 65.2820 67.8120 67.7840 67.8105 67.7820 66.5790 66.5545 66.5835 66.5610 66.6365 66.6555 66.6265 66.6465 63.0750 63.1030 63.0820 63.1080 60.5795 60.6030 60.5800 60.6065 61.8170 61.8370 61.8105 61.8340 НЕ mm_| mm 10000} 10000 +10 +10 +10 +10 Scheinbare ЖА, wie 45 A. Е. Renz, 1896. Februar 7. — 312238 — 2.8154 — 2.3858 3.2564 2.8324 2.4072 3.2280 2.8137 2.3852 3.2572 2.8312 2.4060 ЕЕ ЕЕЕН НН тт 2.8083 2.8320 2.8090 2.8315 Pulkowaer Sternzeit 49 54 der Aufnahmen. Bilder. Mittel. 000 we eu) Trabant — Jupiterscentrum. аа | Mittel. Аж] Ph. | Au cos à 0 СИИ mm —0.7079 0.7033 —0.6978 —0.6951 —+2.8519 -+2.8465 -+2.8444 -=2.8417 5.3479 —5-3458 55.3475 5.3425 +-4.1122 —+4.1136 +-4.1183 +-4.1178 тт —0.7010 | —0:6963 —+2.8461 | <+-2.8270 +5.3459| 55-3099 -+4.1154 | —+4.0877 J° x = 0.993 26 Га = 0.99297 fa = 0.99327 -+0.0003 +-0.000$ +-0.0003 —1°,, = —0.00005 —4 = —0.00008 Ве. = + 4 Try Je гы 30 —0,00054 —0:6966 2-3: | 140 о. —5.3102 -+4.0878 х = + 03 SI Qt PoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1596. Februar 7. Рес]. “пн с; 3 Bemerkungen zur Aufnahme, rs RE , ед — 7 106811 у — = 19681 1 $ тт т тт 61.9395 + 2.7146 62.3365 + 2.3211 + 2.3214 62.7280 + 1.9284 63.5535 -+ 1.1090 -= 0.7083 + 0.7082 + 0.3073 — 0.6410 — 1.0298 — 1.0304 — 1.4205 — 2.4101 — 2.8071 — 2.8047 — 3.1968 Trabant — Jupiterscentrum. уу» | Mittel. (fati-un 7 ера) Чей-аь | Ph. A5 mm mm + 2.5391| -+0.2177 ie es чо -+0.2098 | +0:2084 | —0':0001 | —0!0003 0.0000 | -+0:2080 — 2.5964| -+0.2083 + 1.5163] — 0.8051 ue м ee —0.8068 | —0.8016 | -+0.0004 | -+0.0004 0.0000 |: — 0,8008 — 3.6090] —0.8043 LUE + 0.8744] —1.4470 - 9] 65.3850 — 0.7372] —1.4454 | _ = D. 10| 67.1310 — 2.4807| —1.4503 1.4467 1.4374 | +0.0007 0.0000 0.0000 1.4367 68.8995 — 4.2488] —1.4441 | РЯ + 2a рые. 4.9010 — 0.2487| —0.9569 à. 66.6440 — 1:9922| —0.9618 —0.9581 | —0.9519 | -+0.0005 —0.0003 0.0000 0,9511 68.4130 — 3.7620] —0.9573 bare Decldiff. wie 45 A. 123 = 0.99353. 28 = -но.ооото fs = 0.99304 is = 0.00004. X ig=+ о fx = 0.99354 Лу = -+0,00013 6 = -+20° 21'0 san оса us a8 оса P.-Kr. 0° mm ann 62.9528 62.9519 66.7005 22.5694 75.3152 25.0108 61.4244 62.5600 68.83 11 69.2429 69.6682 68.8211 69.2369 69.6422 68.8346 69.2419 69.6582 68.8426 69.2578 69.6612 67.2429 67.2269 67.2414 67.2459 65.9390 65.9190 65.9330 65.9386 67.9935 67.9845 67.9990 68.0090 59.9595 59.9430 59.9570 59.9655 Scheinbare Ædif: M— Centrum = + 3:9698 Scalenablesung. th P.-Kr.180° 65,4299 65.4283 61.6820 105.8 160 53-0753 103.3736 66.9602 65.8258 59.5772 59.1550 58.7372 59.5842 59.1659 58.7626 59.5732 59.1564 58.7482 59.5672 59.1510 58.7406 61.1470 ' 61.1674 61.1529 ` 61.1490 62.4532 62.4738 62.4612 62.4562 60.3953 60.4063 : 60.3903 60.3808 68.4298 68.4498 68.4358 68.4283 $ О en И W— » ЕЕ УЕ УЕ ++ Е. Renz, 1896. F'ebrüar 19. 4.2864 4.2682 4.2827 4.2868 2.9816 2.9612 2.9745 2.9798 5.0379 5.0431 5.0528 Hart ЕЕ Hr tt 5.0279 2.9968 3.0150 3.0010 2.9930 + 6.2842 + 6.2700 + 6.2815 + 6.2892 Trabant — Jupiterscentrum. he ‘ие аби) Ph. | До. cos Ô m2» | Mittel. mm mm — 1.9978 — 2.0018 — 1.9988 — 2.0024 — 2.0002 — 3.3026 3.3088 —3.3070 — 3.3094 — 1,2463 — 1,2421 — 1.2384 — 1.2364 — 9.2810 — 9.2850 —9.2825 —9.2822 —3.3069 — 1.2408 —9.2827 Ju = 0:99324 = —42.7097 -+13.0262 ини “ оо 8 fa = 0.939296 fu = 099324 +-1:9866 — 3.2845 — 1.2324 —9.2199 Pulkowaer Sternzeit der Aufnahmen. 8 rl 58 14 —i°, =-+0.00019 —iy = -+9.00018 X in=— 06 Refr. = + I Try = + 69 То, = —+-0,00088 +0'0004 +-0.0008 +-0.0093 —=0.0021 2 —0:0008 | —4'9870 | 5 _; 2 2 —0.0008 | —8.2845 | 27 © 1—2 3-4 — 0.0008 | —1.2329 а 2 1-2 —0.0008 | — 9,2186 2 2 Mittel. | co 0) ЕЯ vr 8” 56” 56° LA no | A PosırIonEn DER J UPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 77 1896. Februar 19. Decl. к L. Scalenablesung. пн +2; ZE MO ÉD) MN Bemerkungen Е т ы у в” — + tg5 sin 1’ y— 7 tgè sin 1’ zur Aufnahme. Kr.90°/#+- P.-Kr.270°]t-+k 4 mm 21159 | 61368 ge Ye ‘ 64.2675 0.0000 0.0000 Bilder 2. 53.6988 — 0.0007 —+10.5693 53.1699 — 0.0856 11.0162 81.3064 — 0.0078 — 17.0414 81.2860 — 6.0737 — 17.0922 76.1098 — 0.0001 — 11.8422 . 25.7818 0.0003 —+38.4877 60.7751 + 61.1764 + 61.5702 + 62.3723 == 62.7601 + 63.1414 + 64.0430 + 64.4293 = 64.8182 — 65.8011 er 66.1939 66.5752 Trabant — Jupiterscentrum. d 7 T Yı—yz | Mittel. Ir alye—y2) | 8(8:—x3) 22-2394] mm mm 60.6612 |+11 + 3.6126 we 62.2479 |+10 + 2.0272| -+0.504 0 , D ‚ ле 63.9190 as + 0.3552| -+0.5061 —+0.5057 | 0.5023 | -+0'0004 +-0:0012 0:0000 | 0.5039 65.6762 — 1.4019] -н0.5075 se + 3.9634 Ze 1.897 + 2.3779] —0.8553 ‚oe ‚8525 63.5702 D 664: —08554 -+0.8559 | -+0.8502 | -+0.0006 0.0017 0.0209 | -+0,8525 65.3244 — 1.0519] — 0.8575 ns = 3.4956 Be 2.365 -+ 1.9078| -+0.3852 64.0405 + 0.2338| -+0.3847 +0.3861 | -+0.3835 | —+-0.0002 0.0008 0,0000 |. +0.3845 65.7961 — 1.5224] -+0.3870 | "pe + 5-45 Là Br 0.4058 + 3. —+-2.3462 ; ‚332% RR + 2.1933| +2.3442 —+2.3445 | -=2.3289 | 0.0016 -+0.0017 0.0000 | +2,3322 + 0.4350] -2.3444 _ 63.8411 bare Decldif: M—Centrum = -+10'5022 195 = 0.99337 195 = —0.00019 } N— » = -+10.9497 я К 7 Q— » = —16.9332 fs = 0.99289 is =— 0.00022 x is = —0:8 В— SUN = — 16.9683 V— » =-117655 f’s = 0.99336 I = — 0.0018 W— » =4-38.2307 dy = -+20° 39.7 10* 78 Е. Rexz, 46 в. | 1896. Februar 19. AC Scalenablesung. Ve Pulkowaer Sternzeit 1 er о Object. tk der Aufnahmen. Mittel. P.-Kr. 0° | ti P.-Kr.180° Anhaltstlerne| wie 46 А, mm 72.1330 71.7022 71.2858 72.1124 71.6922 71.2854 72.0884 71.6776 71.2638 mm %9 | 56.2828 [6) de 56.6252 |-+-10 do 57.1140 |+-10 hm | 56.2954 |— 1 ke 56.7072 |+ 9 ho | 57.1180.|-+ 9 29%, | 56.3168 |— I de 56.7306 |+ 9 to 57.1430 |+ 9 %Ё | 56.2878 |— 1| 72.1260 ke | 56.7112 |+ 9] 71.6962 | ko 57.1344 |- 9] 71.2664 Trabant — Jupiterscentrum. 20a | Mittel. Au] Ph. | 42 cos à тт тт I а о 73-7372 и. 54.0022 с] 73.732 — 2.040 u Dr un ис —9' $ | 54.6892 |— 1| 73.7066 —2.0359 2.0383 2'0244 0/0093 0.0008 2.0255 k | 54.6616 |— 1|, 73.7326 — 2.0433 wg 53.3648 + 8| 75.0280 et № | 53.3728 |+ 8| 75.0225 —3.3298 |__ a 5 N Вы = | 2 à | 53.3988 [+ 7| 74.9960 3.3253 3.3288 3.3053 0.0004 0.0208 | —3.3075 2—3 k | 53.3698 + 7| 75.0220 — 3.3335 3 II я 55.5312 о De ee | , Ps h | 55.5392 0] 72.8540 —1.1629| _ Br u в EN etwas ell $ 85.5702 ıl 72.8191 — 1.1517 1.1566 1.1488 0.0092 0.0098 11498! о. - | Г 55.5502 ı| 72.8401 —1,1529 3—4 | IV 9 47.4268 a —9.2642 | 2 | k | 47.4333 + 0.9600 —9.2684 1—2 | ё | 47.4662 |+ à 30.06 Dar —9.2641 | —9.2015 | —9.0012 | —0.0008 | —9,2037 | № | 47.4378 |+ 8| 80.9535 —9.2652 Scheinbare Adiff. wie 46 A. fa = 0.99324 =? = +0,09019 fa = 0.99296 — = 0.00018 X y =— 06 ; Ren, == 2 ‚Jay, =— 69 Га = 0.99325 3. =— 0.00049 ay —8 13.2 Decl. 2% n+% c+% 5 8 10000] 10000 тт тт + 3.3722 + 2.9748 + 2.9787 + 2.5892 62.6842 + 1.5950 63.0640 + 1.2140 —+ 1.2137 63.4478 + 0.8322 64.4148 — 0.1332 64.7901 — 0.5104 — 0.5137 65.1749 — 0.8976 $ 66.1149 — 1.8348 66.5142 — 2.2323 — 2.2310 66.9080 — 2.6259 0.5162 +0.5189 +-0.519$ -+0.5220 +-0.8667 —0.8687 —0.8689 —=0.8700 -+0.3638 +0.3625 +-0.3659 +-0.3634 +#-2.3505 +2.3539 +-2.3540 +2.3552 +0.5192 0.9686 +-0.3639 +2.3534 f°3 = 0.99337 fs = 0.99289 f's = 0.99337 dy =-+20° 39:7 1896. Februar 19. ea — 7 tgù sin 1’ Розитомех DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 2 у—= 108 sin 1’ Trabant — Jupiterscentrum. i hy Yı 92 | Mittel. |. аи уз | Ja(ar—22)| (eat -+0:5158 | 0.0003 — 0.0016 0.8628 | -+0.0005 — 0.0029 —+0.3615 | 0.0952 —0.0999 —+2.3378 | +0.0013 —0.0111 1°5 = —0.00019 is = —0.00022 № = —0:8 Js = —0.00015 — Bemerkungen zur Aufnahme. 0.0005 0.0000 000% +0:5145 +-0,8604 +0,3608 2,3280 47 A. Scalenablesung. F. Rexz, 1=96. Februar 22. Pulkowaer Sternzeit Object] — Bild P.-Er. 0° |t+%| P.-Kr.180° |t-+% der Aufnahmen, Mittel. | mm mm mm 10000 10000] 10000 Ctr. | 61.4834 66.8973 ai К Z 64.4824 |+10| 66.8964 + 9 © 0.0000 2 , M 75.8559 | 8| 52.5243 |+ 8] o|+14.3728 2—3 м N 31.7204 |-+19| 96.6611 |+ 1|+ 7| — 29.7618 à UNS 2—3 ellipt. i0 Q 84.4810 |+ 9| 43.9049 |+31|—11|-+22.9928 7 50 6 3—4 Е 34.1728.|-+36| 94.2093 |-+ 9|-+13| —27.3086 2—3 У 70.5868 |-+25| 57.7929 |+16|— 4] -+ 9.1040 3 т 71.7068 |-+19| 56.6750 |+21|— 2] +10.2226 3 жар | 65.7785 |+11| 62.6216 |+ 9 + 4.2855 2 ac 66.1895 |+11| 62.2110 |+ 9 + 4.6963 — 4.6991 7,0897, EST 2 @0 66.6051 |+ 9| 61.7880 |+ 9 + 5.1155 %6, | 65.7560 |109] 62.6436 |+ 9 + 4.2632 т b 66.1824 |-+10| 62.2230 |+ 9 -+ 4.6867 + 4.6824 seh op 7” 41” 2 2 с 3 db, 66.5951 [+ 8| 61.8140 |+ 9 + 5.0974 % Co 65.7815 |+10| 62.6196 |-+10 + 4.2879 Ce 66.1890 |+10| 62.2115 |-+10 + 4.6957 + 4.6988 A 052 1—2 Ро 66.6051 |+ 8| 61.7930 |-+10 + 5.1129 2d | 65.8050 |-н10| 62.5951 |+10 + 4.3119 de 66.2025 |-+10] 62.2025 |+10 —= 4.7070 + 4.7081 ere fl 1 do 66.5971 | 8| 61.8000 |+10 + 5.1054 Trabant — Jupiterscentrum. EBEN | Mittel. О] Ph. | Aa cos à mm mm Та | 67.8815 [+19] 60.5038 |+14 + 6.3960] -+1.6969 2 b | 67.8600 |+-18| 60.5284 |+14 +- 6.3730] +1.6906 2 oe р ar 1850 | 3—4 verwa с | 67.8780 |+18| 60.5084 |+-15 в 6.3919 1.6931 +1,6921 | -+1!6805 0:0000 0:0010 | -+1.6795 9—3 | d | 67.8840 |-+18| 60.5064 +15 + 6.3959] +1.6878 3 Па | 65.4019 |-+17| 62.9860 |+ 9 + 3.9153] —0.7838 2—3: 71 | 65.3819 |+16| 63.0100 |- 9 —+ 3.8932| —0.7892| __ HN 4 >> 3—4 verwa в 1.62.5080 4:6] 6299000 +0 + 39117 0.7871 0.7890 0.7836 0.0000 0.0010) —0.7846 | 5 а | 65.4004 |-+16| 62.9910 |+10 + 3.9120] —0.7961 2—3 Ша | 70.0475 |-+17| 58.3364 |-+ 5 + 8.5631| -+3.8640 2 b | 70.0270 |-+16| 58.3609 |+ 6 + 8.5405] -+3.8581 5 3 “ 70.0445 Lrél 58.3414 Le 6 + 815590 +3.8602 3.8591 | 3.8326 | -+0.0001 | —0.0010 | -+3,8817 | оз а | 70.0485 |-+16| 58.3389 |+ 6 + 8.5622| -+3.8541 2 IV a | 64.1734 |+ 9| 64.2170 + 8 -+ 2.6852] —2.0139 2—3 b | 64.1595 |+ 9] 64.2315 |+ 8 + 2.6710] —2.0114 =» | 3—4 unte с | 64.1840 + 8| 64.2075 + 9 ВР ИЕ 7) —2.0084| —1.9946 | —0.0001 | —0.0010| —1,9957 | оз _ а | 64.1905 |-+ 8| 64.1980 |+ 9 + 2.7032| —2.0049 2—8 unter Scheinbare Adiff: M—Centrum = -+15'2108 Fa = 0.99316 —1°, = —0.00062 N— » = —31.4672 Q— » = +-24.2673 Te. = 0199288 —i, =— 0.00069 X и=Ь-2и Е— » — —28.7667 Ве". = — I V— » = + 9.6225 x Try = + 52 W— » =-10.8272 Ги =0.99316 Ja = —0.00009 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896, Februar 22. 81 ihe. Decl. | Scalenablesung. à, аа 2 Е hic ЕВ ? у вт = = — 5 19631 1 у— = 196 sin 1’ zur Aufnahme P.-Kr.90° tt P.-Kr. 270° ++ 3 : 3 mm mm 65.0854 10000 10000 тт тт тт тт 65.0838 |+16 o 0.0000 0.0000 — 3.4606 Bilder 3—4, Mond- 68.5352 |+17| 0] — 3.4498 — 0.0471 — 2.9831 schein. 68.0226 |-+34|+- ı| — 2.9360 — 0.0274 — 31.0802 96.1430 |+ 6|+15 — 0.0387 — 31.0995 96.1480 |-+13|-+14 — 0.0043 — 25.8711 90.9555 |— 5I+15 — 0.0057 —+ 24.4611 40.6194 |+27|— 4 61.5702 |+10 + 61.9570 + + 3.1376 62.3449 = 63.2040 + 63.5962 + + 1.5020 63.9805 |+ 9 + 1.1133 64.9745 |+17 + 0.1207 65.3639 |+17 — 0.2620 — 0.2645 65.7466 |+11 — 0.6522 , 66.7261 |+9 * 1.6344 67.1050 |+ 9 — 2.0078 — 2.0063 67.4708 |+ 9 — 2.3767 Trabant — Jupiterscentrum. 9—9 | Mittel. |f's(yr—Y2) |7 (ту) |227 Е Ad mm mm 62.3949 +10) 2 6937 —0.4439 4.0305 + 1.0603| —0.4417 | _ Fer ‚ т. _p 65.7995 2 0.710] —0.4461 0.4444 0:4414 | —+0/0008 O!0011 | -+0!0001 0:4416 67.5416 — 2.4521| —0.4458 61.7975 + 3.2868| -+0.1492 63.4289 —= 1.6615] -+0.1595 15 65.1980 — 0.1090] +0.1555 | +91545]°#0.1535 |’ 0,0004 | +0. Bel +-0.0001 | —0,1586 66.9445 — 1.8526] -+0.1537 62.9840 |-+11 + 2.1036] —1.0340 64.6176 |-+18 + 0.4717| —1.0303 | _ 22 LE Pe Had Lei 3014|, —1.0368 1.0341 1.0272 | -+0.0019 0.0028 | —-0.0001 1.0280 68.1300 |+-20 — 3.0414] —1.0351 61.3339 10 + 3.7574] -+0.6198 82.9690. |+. 9 = 2.1239] +0.6219 | 66200 | +0.6158 | —0.0010 | -+0.0008 | --o.0001 | -+0.6157 64.7351 |-+16 + 0.3550] -+0.6195 66.4798 |+10 — 1.3873| —0.6190 | heinbare Decldif: M—Centrum = — 3/4292 1°5 = 0.99332 $25 — -+0.00047 | N— » = — 2.9820 $ | Q— » — — 30.8643 fs = 0.99283 is = 0.00051 X 15 =-+1.8 R—- » = —30.9002 У— » = —25.6970 f'5 = 0.99330 Js = 0.00045 W—- » = -+24.2990 dy = 20° 43'6 | | | | 11 Зап. Физ.-Мат. Отд. 82 47 B. Scalenablesuug. Object. 5 P.-Kr. 0° = P.-Kr. 1800| ++ Anhaltst\erne| wie 47 А, mm mm mm 10000] 10000 mm mm %}р | 50.3849 72.0185 |-11 75 56.7840 71.6061 |+-II To 57.2050 71.1900 |-+12 #9 | 56.3974 72.0055 |+11 de 56.8160 71.5846 |+11 do 57.2290 71.1685 |+12 Zh | 56.3524 72.0520 |+11 he 56.7610 71.6356 |+11 Re 57.1940 71.2075 |+12 Zi | 56.3844 72.0155 |+12 de 56.7950 71.6051 |+12 0 57.2120 71.1900 |+13 If | 58.4299 !+ 6| 69.9590 9 | 58.4394 |+ 6| 69.9495 h | 58-3964 |+ 5| 69.9970 @ | 58.4154 |+ 5| 69.9735 ИХ | 55.9350 0| 72.4508 9 | 55-9450 O| 72.4418 № | 55.9030 |— 1| 72.4898 î 55.9210 |— 1| 72.4664 ШХ | 60.6111 |-н1т| 67.7740 9 | 60.6211 |+10| 67.7606 h | 60.5811 |-+-10| 67.8056 $ 60.6006 |+10| 67.7856 IV f | 54.8280 o| 73.5602 9 | 54.8490 | ©] 73.5456 № | 54.8100 |— 1| 73.5832 i | 54.8335 |— 1| 73.5566 Scheinbare Adiff. wie 47 A. Dee KEN al 1896. Februar 2%. F. Renz, Ж 121 В Pulkowaer Sternzeit у = 2 u+2cH+%o Bilder. | ? der Aufnahmen. Mittel. mm — 4.7001 т ИЕ 2 — 4.6793 Ge т 2 | 8^ 0” 19° — 4.7246 Во ю 52 2 — 4.6965 тс 1—2 Trabant — Jupiterscentrum. ee | Mittel, >] Лии) Ph. | Aa cos à mm mm —+1.6420 2 |] А -+1.6318| +1/6206 | -н+0!000б | —o!ooıo | —1'6201 ar тегтазо —+1.6238 2—3 LE —0.8514 9 _ № — 0.86 2—3 И 2 —0.8616 | —0.8557 | —0.0002 | —0.0010 | —0,8569 a Veran | —0.8699 3 ui 3.8253 2—3 №. а 3.8177 | 3.7915 | 0.0012 | —0.0010| -+3,7917 “ay | | —+-3.8105 3 | 9 2 N —1.9592 | —1.9458 | —0.0007 | —0.0010| —1,9475| 54 unterexp. 4 —1.9587 3 | _ Та = 9.993 16 —®, = —0.00062 fx = 0.99288 —1% =— 0.00060 X и = +21 Ве’. = Ге) Try = — 52 Fu = 0.99316 Л. = — 0.00112 P.-Kr. 90° tr} P.-Kr. 270° 63.4964 68.1090 | 67.7191 | 66.8240 66.4279 66.0350 ‚65.1270 64.7351 64.3389 63.3534 02.9740 62.5791 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. | Anhaltstierne| wie 47 A. 65.0510 65.4354 65.8180 60.7161 62.3979 64.0925 65.8565 60.1080 61.7900 63.4824 65.2500 61.3104 62.9915 64.6861 66.4538 59.6711 61.3539 63.0510 64.8180 t+k 1896. Februar 22. Decl. mm 10000) cheinbare Decldiff. wie 47 A. mm 5.1901 4.8037 4.4146 3.5146 3.1210 2.7260 1.8198 1.4296 1.0302 0.0450 0.3368 0.7253 Е +++ ЕЕ + +4 4.3741 2.6920 0.9976 0.7665 4.9813 3.2992 1.6040 0.1607 3.7766 2.0975 0.4023 1.3642 5.4176 3.7371 2.0400 0.2723 +++ ЕЕ I +44 ЕН бу = +20° 43.6 Znt%ctH%s 3 mm —+ 4.8028 + 3.1205 — 1.4265 — 0.3399 2 — > $06 sin 1" Trabant — Jupiterscentrum. y— + 105 sin 1’ Bemerkungen zur Aufnahme. Y—yz | Mittel. Узи N ee aa mm —0.4287 —0.4285 — 0.4289 —0.4275 -+0,.1785 0.1787 —0.1775 —=0.1783 — 1.0262 — 1.0230 — 1.0242 —1.0252 +-0.6148 0.6166 -+0.6135 —0.6113 тт —0.4284 —+0.1782 — 1.0246 —0.6140 175 = 0.9933 2 fs =0.99283 f’s = 0.99330 — 0.4255 0.1770 — 1.0177 —-0.6099 —+-0/0008 —0,0004 -+0.0019 —0.0010 1° 5 = +0.00047 is = —+0.00051 Js = +0,00050 —0':0007 | -+oloooı —0.000$ | -+0,0001 +-0.0012 | —-0.0001 —0.0012 | -+0.0001 X в = +18 83 —0.4239 —+0,1762 —1,0145 —+0,6078 84 Е. Rexz, : 48 А. 1296. Februar 33. AR 1% Scalenablesung. Pulkowaer Sternzeit Object. i iz turen Bilder. | P.-Kr. 0° tet P.-Kr.180° | i-+-k | 2 der Aufnahmen. Mittel. | mm mm 10000! тт __ 10000 BE m A Ctr. | 61.5491 66.8325 D 61.5482 + 9| 66.8317 о 0.0000 3%) M 58.3645 |+ 8| 70.0155 Be 0] — 3.1844 3 N 14.2381 |+28| 114.1428 | 5|+-32 PA NE 3 Q 66.9817 |+17| 61.4032 4 18 30 3—4 В 16.6803 |+-34| 111.7000 3—4 У | 53.0875 |+13| 75.2939 3—4 W 54.5321 |-+18| 74.1518 3 | | za, | 65.8610 |+11| 62.5394 + ас | 66.2750 |+11| 62.1320 + —+ 4.7163 Я 90:12 4 @ | 66.6961 |+ 9| 61.7136 + db | 65.8296 |+-11| 62.5863 + d, | 66.2405 |+11| 62.1650 + —= 4.6789 6 45 1,4 b, 66.6601 |= 9| 61.7560 + от 48 2 dy | 65.8396 |-+ то| 62.5663 + de | 66.2684 |+-10| 62.1325 + + 4.7135 Sn Hs? 4—5 do | 66.7141 |-+ 8| 61.6921 + Ze | 65.8410 |+10| 62.5683 —- ес 66.2564 |+10| 62.1495 —= — 4.6965 LORS 4 о 66.6771 |+ 8| 61.7276 + Trabant — Jupiterscentrum. Lt — 2 y | Mittel. faulen) Лигу Ph, | До cos d mm mm Та | 65.1070 |+17| 63.2894 |+ 9 + 3.5509] —1.1654 3—4 b | 65.0740 |-+17| 63.3194 + 9 == ЗО 5505 | М р Sr N 3 Я | 65.1180 |-+16 63.2759 +10 + 3.5630] —1.1505 1.1558 НЫ | ВЫ SE 1.1480 4 à e 65.1065 |+-16| 63.2894 |+10 + 3.5506] —1.1459 4 unterexponier Па | 63.0900 |+10| 65.3039 |+16 + 1.5344| — 3.1819 3—4 р b 63.0545 |+10| 65.3379 |+16 —= 1.4997| — 3.1792 | __ ‚er m; en 3 а | 63.0930 + ol 65.2979 +17 + 15388] —3.1747 3.1783 3.1571 | 40.0011 0.0010 31570 | , е | 63.0745 |+ 9| 65.3189 |-+17 + 1.5191| —3.1774 4 Ш Geht dulrch |die Jupiter|schelibe. IV a | 67.6981 |+19| 60.6901 |++-10 —= 6.1462] 1.4299 Be) b | 67.6726 |+-18| 60.7171 |+10 + 6.1198] -+1.4409 Er: 2“ 4—5 а | 67.7121 |-+18| 60.6746 |-+11 + 6.1608] -+-1.4473 ЕДЫ a re 00010 | +1.4831 4 e 67.7076 |-18| 60.6826 |+11 + 6.1546] 1.4581 4 ве Scheinbare ÆRdiff: M—Centrum = — 3.3502 8, = 0.9933 5 — = +-0.00075 N— » — — 50.0278 Q— » = + 5.7067 Fax = 9.99305 —% u > R— » = 47.3277 Ве. = — У » = — 8.9385 Try =-+ W—- » = — 7.7338 Ne — 0.993341 Jr =. 00133 ay —=8" 11.6 *) Auf dieser Platte sind alle Bilder grau, wahrscheinlich zu kurze Zeit entwickelt. **) Alle Bilder des Trabanten IV fallen auf einen Netzstrich. | [P.-Kr. 90° +51 Р.-Кг. 270° 10000 44.9092 | 50.0910 ] 100.4154 | 6. 6056 | 67.2150 | 67. 8290 65.8016 65.4139 1% 05.0290 | 62.2809 $ 1.8660 61.4602 60.63 11 60.2260 9.8170 Scheinbare Decldiff: POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. Scalenablesung. 64.2521 64.2513 55.8875 55.3564 83.4910 83.4705 78.2956 27.9777 60.8035 61.1940 61.5812 62.6031 62.9930 63.3779 66.1400 66.5366 66.9510 67.7820 68.1800 68.583 1 60.8700 62.6766 66.2244 67.8660 60.3390 62.1420 65.6921 67.3299 die Jupiteris 61.4149 63.2200 67.7680 68.4079 t+k 1896. Februar 23. mm 0.0000 —=16|— 7|-+ 8.8935 EI SLI +10 Tr. +10 +10) +11 AB FLT ÈS) +19 +19 +14 N— » Q— » В— » У— » W— »› _тт_ 10000 10000 + 8 о - 9 o|+ 8.3652 — 6]|-+ 2| —19.2383 —19]|-+15| —19.2200 —12|-+ 1] —14.0441 +-24|—14|+-36.2748 led со [e] Où Pitt 2.8414 1.0366 2.5139 4.1506 DEE: M— Centrum = -+- 8'3183 + 8.7655 — 19.1173 — 19.1527 —13.9495 —+36.0465 dy = -+20° 44:8 ес]. Я%ин%с+%; >} о тт + 3.0701 + 1.2703 — 2.2785 — 3.9205 mm -+0.3171 -+0.3103 -+0.3 100 -+0.3117 —0.8469 —-0.8445 —=0.8413 —0.8477 —0.2287 —0.2337 —0.2354 —0.2301 195 =0.99358 fs = 0.99308 fs = 0.99356 +-0.3123 —0.8451 —0.2320 2 RATE ROM OO NON © 2 > = _. — tqù sin 1’ тт 0.0000 + 8.3647 + 8.7761 — 19.2398 — 19.3231 — 14.0478 —+-36.2719 Trabant — Jupiterscentrum. —0'3 103 —0'0010 —0':0005 -+0.8397 | -+0.0026 —=0.0011 —0.2305 | —0.0012 — 0.0009 1°$ = —0.00088 $5 — —(.00080 x 18 = Js = —0.00086 | Mittel. I" (1—2) 175 (aaa) |- (x? =) Ph. x? . У—5 1968 sin 1’ CO ел Bemerkungen zur Aufnahme, Bilder 4. Leichte Wolk. ziehen über den Himmel. Im Ganzen sind3 Tra- bant. „zu sehen, um 7*20” erschien der vierte am Ostr. des Jupiter. —+o'o001 | -+(,3119 —-0.0001 —+0'8435 0.0001 —0.2325 86 4= B. Scalenablesung. Object. P.-Kr. 0° +5 Р.-Кт. 180° Anhaltstierne| wie 48 A. mm 10000 mm mm %Л | 56.5212 |+I1) 71.8870 Je | 56.9250 |+11| 71.4748 № | 57-3434 11] 71.0670 %9 | 56.5062 |+-10| 71.8970 Te 56,9140 |-+10| 71.4928 go | 57-3244 |-+10| 71.0830 2% hop | 56.5356 |-+10| 71.8665 he 56.9450 |H-I10| 71.4538 Ro | 57.3654 |+10| 71.0450 Zip 56.5691 |+ 9 71.8450 % | 56.9750 |+ 9| 71.4294 io | 57.3894 |+ 9] 71.0105 If | 56.4674 |+ 1| 71.9270 9 | 56.4554 | ©] 71.9385 h | 56.4984 o| 71.8915 8 Nicht eilnstel|lbar. ПЛ | 54.0150 | 4| 74.3799 9 | 54.0015 |+ 4| 74.3939 № | 54.0445 |+ 3] 74.3599 ® | 54.0665 |+ 3| 74.3299 IL | 56.1025 |+ 1| 72.2954 9 | 56.0795 | ©] 72.3149 № | 56.1090 ol 72.2814 i SoAra LS, |— 1 72.2674 IV f | 58.7221 |+11| 69.6691 9 | 58.7071 |+11| 69.6836 h 58.7416 |+11| 69.6506 р 58.773 т |-+10| 69.6246 t+k mm 10000 +12 Se Er ro 1) —=11 HI? +12 II 12 -+I2 HI] = 7) 2 +12 Zeil! Sm! 13; +12 T2 —I2 —=12 —-II +11 HU +17 +16 +16 +16 ` Scheinbare Adiff. wie 48’ A. F. Renz, 1896. Februar 33. ee ala CA m 5.0886 5.1004 5.0554 7.5412 7.5549 7.5164 7.4904 5.4553 5.4766 5.4450 5.4238 2.8321 2.8468 2.8130 2.7844 44 8 № Y wE#cH?%o 4—2 | Mittel. 3 mm 4.6316 4.6464 4.6116 4.5837 der Aufnahmen. 36 Pulkowaer Sternzeit Mittel. 12° 35 9 34” 54° 25 25 Trabant — Jupiterscentrum. mm mm —0.4570 р —0.4540 | —0.4516 | —0:4486 0:0000 | —0:0010 —0.4438 —2.9096 en —2.9074 | — 2.8881 | -+-0.0002 | —0.0010 — 2.9067 —0.8237 m, —0.8318 | —0.8263 0.0000 | —0.0010 — 0.8401 1.7995 —=1.7992 | +1.7873 | —0.0001 | —0.0010 =+1.7993 Ja = 0.99335 —и = +0.00075 Ja = 0.99305 —iy = 9.00078 Вей. =+ 3 Try =— SI Г’ = 0.99335 Л, = 0.00030 11.6 Para) Te 0702) Ph. | Au cos à — 04496 | 3—-4unterexp. M Schimmer 4 2—3 —2,8889 | 3 À | 4—5 unterexp. | 4 3—4 verwasche 3—4 » — 0.8273 | , Е 4 у = 3 | + 1.7862 | 3% unterezääg ala à x и =— — 2:7 1% Bilder. | 3 unterexp. I | jeihe. z Scalenablesung. = &-|- у | P.-Kr. 90° th) P.-Kr. 270° |t+% Anhaltstlerne| wie 48 A. mm mm | 10000] 10000 | mm тт тт 69.5443 58.8710 |+12 + 5.3952 59.2589 |+12 —= 5.0056 59.6481 |+16 + 4.6198 60.6326 |-+12 -+ 3.6340 61.0085 |-+12 + 3.2510 61.3869 |+12 + 2.8756 62.3479 |411 + 1.9174 62.7246 |-+11 — 1.5336 63.1090 |-+11 + 1.1491 64.1420 |+10 + 0.1258 64.5212 |418 — 0.2606 63 64.9070 |-+18 — 0.6502 | 59.2859 59.1130 |+12 + 5.1450 | 67.5312 |-+21| 60.8640 |-rı2 + 3.3924 | 65.8046 -+13| 62.5946 |+ —+ 1.6634 || Nicht ei nstelllbar. | 69 +20| 58.4578 |+ 9 + 5.80c0 ! -=22| 60.2085 |+-18 + 4.0472 —=14| 61.9375 |-+13 + 2.3198 —=20| 63.7301 |-+12 + 0.5264 +16] 59.0970 |-+12 + 5.1564 +21| 60.8525 |-+12 + 3.4036 +13) 62.5741 |+-11 + 1.6808 ‚|--11| 64.3634 |+10 — 0.1096 HIS] 59.5701 |-+15 —= 4.6860 —=10| 61.3249 |+11 + 2.9288 -=18| 63.0500 |+-10 + 1.2046 +10| 64.8485 |-+17 — 0.5887 scheinbare Decldif. wie 48 A. ] #=-20° 44:9 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTORRAPHISCHEN ÄUFNAHMEN. 87 1896. Februar 23. Decl. пн сн; PE 2 En Bemerkungen 3 — 5 96 sin 1 у — = to sin 1 у с, тт Bilder 3. + 5.0069 3.2535 Trabant — Jupiterscentrum. - T Yt—Y3 | Mittel. fa (г—у) | 7з (еее) | вае-айз)з) тт тт +-0.1381 -+0.1389 —0.1300 -+0.1357 | +0:1348 | -+0!0003 — 0.0002 | -но'осот | -+0:1350 —=0.793 1 +0.7937 +-0.7864 —=0.788 1 —+0.7903 | 0.7852 | 0.0021 —0.0019 | 0.0001 —+-0,7855 +-0.1495 +0.150I +-0.1474 —+0.1521 —0.1498 | -+0.1488 | 0.0006 —0.0004 | —-0.0001 —+-0,1491 —0.3209 —0.3247 —0.3288 —0.3270 —0.3254 | —0.3233 | —0.0013 -+0.0008 | -+0.0001 | —0,3237 32; = —0.00088 is =— 0.00080 Js = — 0.00072 f°s = 0.99358 fs = 0.99308 f'a = 0.99357 X в=—217 88 Г. Renz, 49 A. 1896. Februar 34. № Scalenablesung. Pulkowaer Sternzeit О — 0h. ne öl he © Barres Pat et A ар И Bilder. P.-Kr. 0° |t-+%| P.-Kr.180°| #&-+-% - der Aufnahmen. Mittel. Ha 10000 mr 10000 10000 jeu gun | Cir. | 66.7737 61,6154 } Z 66.7729 |+ 8| 61.6144 |+10 (o) 0.0000 2—5 M 81.1443 |+15| 47.2398 |+ 9]— 1|-+14.3733 1—2 М 37.0163 |-+23| 91.3738 |— 6|+ 6] —29.7558 р 1—2 Q 89.7445 |+ 8| 38.6441 |-+36|-—10] +22.9686 7 BO; 2—3 R 39-4435 |+40| 88.9409 |+ 5|+-15| — 27.3246 1—2 14 75.8579 |-=21| 52.5306 |+18|— 2] + 9.0844 2 W | 77.0183 |+17| 51.3731 |+-22]— 2|-+10.2430 2 24,0 | 61.7101 |+ 9| 66.6866 |+ 8 — 5.0674 Ge 62.1210 |+ 9| 66.2839 |+10 — 4.6606 — 4.6604 я. ет 2—3 ao | 62.5228 |+ 9| 65.8710 |[+10 — 4.2533 %Dy | 61.7976 |+10| 66.6041 |-+ 8 4.9823 D, 62.1844 |+10| 66.2155 [+10 — 4.5947 — 4.5920 15 150) 2 b, 62.5813 |-+10| 65.8210 |-+-10 4.1990 ТВ 14” 40° %Cy | 61.6671 |+10| 66.7256 |- 8 — 5.1083 вс 62.0825 |+10| 66.3150 |+10 — 4.6954 — 4.6976 т 002 2—3 Co 62.4874 |-+10| 65.9075 |+10 4.2892 % dy | 61.7151 |+10| 66.6840 |-- 9 — 5.0636 de | 62.1080 |-+10| 66.2830 |-+II — 4.6667 — 4.6630 Bl 2 d 62.5188 |+10| 65.8780 |-11 — 4.2588 Trabant — Jupiterscentrum. Lt—Ly | Mittel. |?„(@:—xz,) Лич) Ph, | Av cos à I Als Erhlöhun)g am Ostralnde | bei |Aufnahme| с und d | zu erken nen. Ir 63.9090 |+ 8| 64.4809 |+- 9 — 2.8652 +1.7952 de 2—3 63.9875 |+ 8| 64.4049 |+ 8 — 2.7878| +1.8042 = , , р 1—2 Е 63.8875 не. ue В 53 ne RÉ +-1.80$1| —-1/7930 | -+0:0008 | —o!o010 | -+1!7928 2—3 а | 63.9240 |+ 9] 64-4674 |+ 8 — 2.8508] -+1.8122 2 ur Diner + 95| 70.6501 |+12 — 9.0355] —4.3751 2—3 57-8060 |+ 6| 70.5851 |-+12 — 8.9690] —4.3770| __ 21 1—2 е | 57.6986 |+6| 70.6906 |+12 — 9.0754] —4.3778 4.3780 4.3487 | —0.0021 | —0.0010) —4,3518 | > Я | 57.7291 |+ 7| 70.6601 |+13 — 9.0450] —4.3820 2 ТУ 2 3 + 8| 61.4998 |+11 + 0.1186] -+4.7790 2 6.9715 |+ 8| 61.4239 |-+I0 —= 0.1946] -+4.7866 2 с 66.8660 |+ 9| 61.5248 |+10 + 0.0914] +-4.7890 4.7866 | 4.7545 | +0.0021 | —0.0010| +4,7556 2—3 а | 66.9045 |+ 9] 61.4888 |+10 + 0.1286] -+4.7916 2 Scheinbare Adiff: M— Centrum— +15:2108 f° 4 =0.99330 —1° 4 = —0.00142 №М— » = — 31.4672 Q— » = +-24.2673 fu = 9.99301 —iy ——0.00140 № 1, = + 48 Е » — —28.7667 Refr. = — 2 V— » — 4.0.6225 Try =— SI W— » =-10.8272 Го = 0.99330 Ja —=—0.001% т ay = 8" II.I ihe. ,.-Е . 90° 62.9374 62.9365 60.0278 31 ‘4 31.899 : 2 6 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896. Februar 24. Scalenablesung. y t-+] P.-Kr.270° +R mm mm |_mm_ 10000! 654474 | 10000] 10000 mm + 9| 65.4457 |+17| о 0.0000 +17| 68.9095 |-+19| 0] — 3.4612 —+25| 68.3614 |-+32|+ 1] — 2.9120 +#-33| 96.5158 |+-I1o|-+-I15| —31.0634 96.4838 |-н11|-14| —3 1.0348 91.3200 |— 3|- 6] —25.8701 40.9959 |-+29|— 4] +24.4522 64.7101 |-+16 + 0.7434 65.0950 |-+16 + 0.3629 65.4718 |+16 — 0.0187 62.9140 |+ 9 + 2.5443 63.2779 |+ 9 + 2.1814 63.6436 |+ 8 + 1,8101 61.1450 |+10 + 4.3094 61.5312 |+ 9 + 3.9294 61.9090 |+ 9 + 3.5481 59.4302 |+14 + 6.0252 59.8080 |+14 + 5.6503 60.1825 |+-14 + 5.2705 Decl. Antares 3 тт + 0.3625 + 2.1786 + 3.9290 + 5.6487 Us Erh öhun)c am Ostralnde | bei | Aufnahme| а und 6 zu | erkennen. 65.5152 |+10 — 0.0636 — 0.4261 = 63.6996 |+ 8 1.7193] —0.42522 78 61.9480 |+ 9 + 3.5045| —0.4245 0.4263 60.2320 |-+14 + 5.2194] — 0.4293 64.0010 |+ 9 + 1.4488] -+1.0863 62.1890 |+-10 + 3.2631] -+1.0845 oh 60.4339 |-+Is + 5.0173] -+1.0883 HT, 58.7151 |-+11 + 6.7364| --1.0877 u +11 — 0.7118) —1.0743 4.3599 |+ 9 + 1.0935| —1.0851 | _ 62.6031 |+-10 + 2.8502| —1.0788 1.0804 60.8899 |+-11 + 4.5654] — 1.0833 heinbare Decldiff: M—Centrum = — 3/4292 f°5 = 0.99352 — » = — 2.9820 Q— » = —30.8648 15 —0,99303 R— » = — 30.9002 У » =—25.б97о fs = 0.99351 W— » = +-24.2990 92 = +-20° 46:0 Зап. Физ.-Мат. Отд. 2 RAR ee ’ — > 190691 1 тт 0.0000 | 0.0000 — 0.0108 104720 — 0.0471 — 2.9591 — 0.0274 — 31.0908 ut Le — 0.0057 | —+-24.4465 Trabant — Jupiterscentrum. 3 5 T Yt—Y2 | Mittel. ra (из) 7 (ео) aa), Ph. y — > 108 sin 1" Bemerkungen zur Aufnahme. Um 7^ 21” Eintritt des ersten Tra- banten in die Ju- piterscheibe am Ostrande. Bilder 2—5 AG —0:4235 | -+0!0023 —+0'0007 | +o!ooor | —0:4204 —1.0776 | —0.0055 —0.0033 | -+0.0001 | -—1,0689 —1.0733 | -+0.0060 0.0012 | +0.0007 | —1.0660 125 = +0.00124 is = 0.00130 X в =- 45 Ту = +0.00125 * 12 90 Е. Rexz, 49 1. 1896. Februar 24. № 12 Scalenablesung. Pulkowaer Sternzeit (Object. RSR nn 29 æ . аси ue DR: ыы | Bilder. P.-Kr. 0° |+ ЁР.-Кт. 180°| + 3 der Aufnahmen. Mittel. Anbaltstierne| wie 49 A, mm _mm_|_ mm _ 10000 10000) 10000 mm mm mm mm hi | 71.2085 |-+13| 57.2005 |+10 + 4.4250 5 he | 71.5916 |+12| 56.8006 |H-10 + 4.8164 + 4.8195 9’ BUN 1—2 Ro 71.9930 |+-12| 56.4019 о + 5.2170 Zip 71.1560 |-+13| 57.2440 |+10 + 4.3770 ie 71.5591 |-+12| 56.8460 |+10 + 4.7775 + 4.7765 2 © 2—3 CA 71.9550 |-+-12| 56.4479 о + 5.1750 gi 95" 30° Ak | 71.1725 |+-13| 57.2315 |+ 9 + 4.3916 ke 71.5701 |-+12| 56.8270 |+ 9 + 4.7926 + 4.7963 25.1957 2 ko 71.9820 |+12| 56.4159 |— 1 + 5.2046 21» | 71.2115 |-+14| 57.1900 |+ 9 — 4.4318 % 71.6061 |+13| 57.7925 |+ 9 + 4.8278 —+ 4.8307 26 57 2 % 72.0090 |+13| 56.3869 |— 1 + 5.2326 Trabant — Jupiterscentrum. Lt—Ly | Mittel. |f„(&:—22) Лии Eh? Ac cos 6 I Als Erhlöhun/g am Westrlande| bei |Aufnahmel, n und 0| zu erken/nen. тт тт ПРА | 73.8215 |+12| 54-5741 —+ 7.0452] 2.2257 1—2 © | 73-7780 |+13| 54.6206 + 7.0002| +2.2237 | 4,2276 | +2'2127 | +0'0004 | —olooro | +2'2121 | 2 k | 73.8010 |-+13| 54.5921 —= 7.0260] 2.2297 2—5 | 73.8385 |+14| 54.5576 + 7.0620] +-2.2313 2 IT | 66.9935 |+ 9| 61.4004 + 0.2173| —4.6022 2 x î | 66.9420 |+ 9| 61.4489 + 0.1674] —4.6091| __ В г. ZX LE 2—3 м. MECS бы 4.6071 4.5761 0.0009 0.0010 | —4,5780| 5 1 | 66.9950 |+11| 61.3954 -+ 0.2207] —4.6100 2 IVh а ++ 9| 51.7440 + 9.8750] -+5.0555 5 г р 76.6061 |#+-10| 51.7915 —= 9.8280] +5.0515 : er 5] 2 en ee о ea -+0.00I0 0.0010 | +-5.0215 | 5 1 | 76.6641 +11| 51.7300 + 9.8879] +5.0572 1—2 Scheinbare Adiff. wie 49 A. f?r = 0.99330 —1°,, = —0.00142 fa = 0.99301 —1% =— 0.00140 x Ay 4.8 Refr. = + 3 я Try = + 53 Га = 0.99330 J, = — 9.00084 т ay = 8* 11.2 LA POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. в Io Scalenablesung. + P.-Kr.270° |t+k IP.-Kr.90° pe il sc rn wie 49 A, Anhaltstierne EuL ie 10000 о. eco — > тт тт 59.5551 |-+16| 68.8405 |+16 59.9305 |-+16| 68.4808 |-+21 1 60.2974 |+16| 68.1030 |+21 | 61.3209 +12| 67.0765 |+ 1 61.6966 |+-11| 66.7081 |+11 62.0660 |+11| 66.3349 |+13 63.1290 |+11| 65.2689 |+19 63.5102 |+10| 64.8975 |+19 63.8910 |+I0| 64.5046 |+19 64.9066 |-+18| 63.4988 |+12 65.2840 |+18| 63.1210 |+12 65.6551 |-+12| 62.7446 |+12 | Als Erhjöhun|g am Westrjande 59.3829 69.0105 |+16 | 61.1500 67.2450 |+ı1 62.9650 66.4289 |+19 64.7331 63.6606 |-+11 ‚| 61.0710 67.3219 |+11 65.5581 |+13 63.7391 |#11 61.9695 |+12 69.6161 |+21 67.8560 |+23 66.0370 |-+15 64.2704 |+13 Scheinbare Decldiff. wie 49 A. 1596. Februar 24. mm 10000] 10000 mm 3.3877 3.0204 2.6480 1.6228 1.2508 0.8796 0.1846 0.5609 0.9478 1.9592 2.3368 2.7102 ЕЕ +44 dy = -+20° 46.1 Decl. "пн ен; uv | Mittel. [/“з(илую I таз) |Чей-гту а тт 3.0187 — 1.2511 + 0.5644 + 2.3354 bei [Aufnahmelm,n und o zu| erkennen. mm mm 35590] —0.5403 — 1.7924| —0.5413 | _ + 0.0227| — 0.5417 0.5418 + 1.7916| —0.5438 — 1.8706| -+1.1481 — 0.1062] —+-1.1449 + 1.7117| —+1.1473 #1.1465 + 3.4811| —+1.1457 — 4.1648| —1.1461 — 2.4036| —1.1525 Be: — 0.5846| — 1.1490 ET + 1.1826| —1.1528 795 = 0.99352 fs = 099303 fs = 0.99351 91 x? x? — 5 196 sin’ у— 5 tgÿ sin 1’ Trabant — Jupiterscentrum. a ЧЕРВИ, —0:5383 | -+0!0030 —0.0014 | -+0!ooo1 +-1.1391 —0.0063 —0.0013 | -+0.0001 —1.1426 | -+0.0069 —0.0041 | -0.0001 12; = -+0.00124 is = 0.00130 X i8—=+ 45 Js —+0,00137 Bemerkungen zur Aufnahme. Trabant I tritt aus am Westr. 9" 35". Bilder 3. um AG —0:5366 —1.1342 —1.1455 92 Е. Rexz, 50 A. 1296. F'ebruar 25. Æ 121 Scalenablesung. Pulkowaer Sternzeit Object. $ 7 Pas eh "ect Bilder. | Р.-Кт. 0° |{+k| P.-Kr.180° |t+k 5 der Aufnahmen. Mittel. mm mm mm Cr. | 66.2984 [1000| 63.6929 Tune "т Fe S 66.2974 |+10| 62.0920 |+ 9] о 0.0000 2—8 M Durch eiln Julpitersbild |verdleckt. N 27.1456 |+23| 101.2404 |+ 3|4-17| —39.1474 Ne 2... ö Q 79.8360 |+21| 48.5540 |+23|— 4] 13.5378 49 35 2 eiförmig. Е 29.5320 |+-31| 98.8564 |+11|+22| —36.7618 У 65.9560 |-+20| 62.4298 |-+16| 09] — 0.3394 2—8. W | 67.2001 |+20| 61.1823 |+25| ©] -н 0.9059 2 bp | 10.6457 |-=12| 57.7531 ENS —+ 4.3436 b. 71.0345 |+12| 57.3609 |+ 9 + 4.7342 + 4.7375 8 40 10 2 bo | 71.4394 |-+12| 56.9645 |+ 9 + 5.1348 2% Cw | 70.5861 |+12| 57.8090 |+ 5 — 4.2862 | er 70.9875 |+ı12| 57.4139 |+ 9 + 4.6842 —= 4.6827 A1 [6) 2—3 Co 71.3784 |-+12| 57.0189 |+ 9 — 5.0776 si 44” 95° 2% dy | 70.6176 |+12| 57.7866 |+ 6 + 4.3130 de | 71.0075 |-+12| 57.3929 |+10 + 4.7046 + 4.7059 41 50 2 dy | 71.4044 |+12| 56.9990 |+-10 —= 5.1090 Lex | 70.6321 |+13| 57.7656 |+ 6 —+ 4.3308 ee 71.0360 |+13| 57.3699 [10 + 4.7504 —+ 4.7299 42 50 2—3 Ba 71.4324 |+13| 56.9700 |-+-10 + 5.1286 | Trabant — Jupiterscentrum. хр — xy | Mittel. |f’„(&—-22)\ о (yı ya) Ph. Au. cos à mm mm Ib 71.9650 |+11| 56.4274 |— I + 5.6666] --0.9291 2 с | 71.9160 |+11| 56.4778 o + 5.6169] +0.9342 , , ET ' 2 а | 71.9440 |+11| 56.4518 . + 96430] + 0.9380| * 29352 —+0:9288 | -+0:0004 0.0011 | +-0:9281 | 5 _o | е 71.9685 |-+12| 56.4259 Ге) + 5.6692] +-0.9393 2—3 à Ib 73.1405 |+-13| 55.2514 |— I + 6.8425| 2.1050 1—2 |} с | 73.0845 |-+13| 55.3089 (6) + 6.7857| +-2.1030 г: x | 2 d | 73-1060 |+13| 55.2854 (6) + 6.8082| +-2.1023 72.1010 Об 7: 9.0015 0.0011 | -+2.0865 2—3 р е 73.1220 |+14| 55.2709 |+ 1 —= 6.8234] 2.0935 2—8 № II b 65-2345 +11 u +9 — с — 5.1008 а р Ir с 5.8805 |-+10| 62.50 + 9 — и —5.0995 | __ ке a ei я icht neben % Я | 65.9060 |+10| 62.4828 |+10 — 0.3912| — 5.097 1 3.0991 5.0641 SO we 5.0674 2 а e | 65.9255 |+10| 62.4584 |+10 — 0.3692| —5.0991 2—3 | ТУЬ | 78.5921 |+ 6| 49.8020 |+ 6 +-12.2923| +7.5548 2 7 с | 78.5392 |+ 6| 49.8550 | 6 -+12.2394| 7.5567 + 1—2 (4 d | 78.5626 | 6| 49.8330 |+ 6 +-12.2620| -+7.5561 En Such +7,5052 2 [И е 78.5846 |+ 7| 49.8125 |+ 7 +12.2833| +7.5534 2—3 | Scheinbare Adiff: М— Селгиш = — 41.4085 I 090m —i°, = —0.00214 Q@—- » = +-14.3267 { r } Е В— № = 38.7078 fu = 0.99286 —iy =- 0.00215 X = + 74 У— » = — 0.3188 Ве. = = I W— » — + 0.8860 Try = + SI FL = 0,99314 Jy = —0.00163 ay —8" 10.8 зу; 4 | | | | | | | | | | | | | | Scalenablesung. P.-Kr. 90° POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. $ | tt P.-Kr.270° | #+% mm 10000 63.4139 63.4130 |+ 9| 64.9819 Durch ein Ju pitersbild 67.0541 38.7966 38.9224 44.0230 94.3549 65.2249 64.8615 64.4902 63.5088 63.1454 62.7810 61.7111 61.3489 60.9725 59.9225 59.5506 59.1854 64.63 56 62.9255 61.1235 59.3329 64.2579 62.5512 60.7491 58.9610 66.1834 64.4698 62.6691 60.8785 63.0595 61.3454 59.5452 57.7551 +24 +31 9257 19 =: +17 +17 +17 +10 +10 +10 +10 It am À IS +15 lon (1 +18 +11 +12 +12 ТЕТ —-12 +13 +13 +10 + 8 ir 9 +10 +15 -+-16 +20 +11 64.9836 61.3399 89.5985 89.4698 84.3732 34.0433 63.1840 63.5472 63.9140 64.8940 65.2644 65.6281 66.6941 67.0600 67.4289 68.4822 68.8550 69.2280 63.7640 65.4708 67.2749 69.0665 64.1350 65.8476 67.6471 69.4344 62.2124 63.9255 65.7281 67.5156 65.3419 67.0535 68.8550 70.6431 А 12 110 +10 +10 EETS 10000 10000 Sa ER a A + ol 39 — 6|+ 2 211 — +11 +10 +10 +18 +15 +18 an D +11 +19 +II +16 +11 +13 —+21 +16 +10 AL, +11 +19 +21 +13 +18 +17 1896. Februar 25. Decl. Scheinbare Decldif: N—Centrum =-+ 3/4510 = » R— 5 У » Т— » 2 2 y — + tgÿ sin 1’ у— + 96 sin 1’ zur Aufnahme. mm mm mm mm 0.0000 0.0000 0,0000 Bilder 2. Mond selır nahe. —= 3.6418 — 0.0805 + 3.5613 6] —24.6138 — 0.0094 —24.6232 —24.4866 — 0.0689 , —24.5555 — 19.3888 0.0000 — 19.3888 —30.9386 0.0000 —=30.9386 + 1.8056 — 1.4424 + 1.4404 + 1.0733 + 0.0918 — 0.2750 — 0.2740 — 0.6388 — 1.7066 — 2.0706 — 2.0735 2.4433 3.4950 — 3.8674 — 3.8663 4.2366 Trabant — Jupiterscentrum. e HE ^ vs | Ма. |Узби-у | Лаби--2з) |229) a mm mm —+ 1.2210] —0.2194 NE we mr —0.2167 | —0!2153 | -+0:0020 | —0.0006 | -+0:0001 | —0:2138 — 4.0822| —0.2159 + 0.8443] —0.5961 Æ 2 me —0.5906 | —0.5867 | -+0.0046 | —0.0014 | -но.осот | —0,5900 — 4.4520] —0.5857 + 2.7704] -+1.3300 Ein CFA Hs —1.3304 | +1.3216 | —0.0111 —=0.0012 | -+0.0001 | <+-1,3118 — 2.5342| -+1.3321 — 0.3566| —1.7954 = A в — 1.7954 | —1.7835 | -+0.0165 —0.0071 | 0.0001 | —1,7740 — 5.6594] — 1.7931 195 = 0.99338 19$ = 0.00214 = —24.4322 . — m0 fs = 0.99290 is = 0.00213 X 5 =+73 = —19.2643 - = -+30.7322 f's = 0.99337 Уз = -+0.00216 % пн 0%; Bemerkungen 9 9 94 50 1. Scalenablesung. Object. P.-Kr. 0° I P.-Kr.180° Anhaltstierne| wie 50 A. mm 10000 mm mm 27, | 61.1964 |+11| 67.2070 Te 61.5926 |+10| 66.8110 I 61.9930 |+10| 66.4089 %9% | 61.2354 |+I1| 67.1695 de 61.6371 |+10| 66.7750 do 62.0290 |+10| 66.3744 Ah | 61.2389 |+10| 67.1595 Re 61.6311 |+ 9) 66.7745 ho | 62.0335 |+ 9] 66.3709 Zip | 61.1030 |--10| 67.3044 вс 61.5062 |-+ 9| 66.9020 Zn 61.9125 |+ 9| 66.4934 If | 62.6391 |-+10| 65.7551 g 62.6741 |+10|) 65.7211 й | 62.6851 |+ 9] 65.7096 à 62.5581 |+ 9] 65.8350 ПЛ | 63.6166 |+ 9| 64.7746 9 | 63.6431 | 9] 64.7496 k 63.6491 | 8| 64.7406 è 63.5152 | 8| 64.8760 ШУ | 56.5168 | 1| 71.8745 9 | 56.5498 | ©] 71.8456 № | 56.5568 0| 71.8346 | р 56.4269 — 1| 71.9640 ТУЛ | 69.1839 |-=14| 59.2095 9 | 69.2169 |+-13| 59.1790 й | 69.2249 +13) 59.1700 О 69.0960 |-+13| 59.2984 НА mm mm 10000] 10000 10) +10 10 —=11 +-16 —+-16 +16 +17 +12 zn II II +10 +10 НЕТ —=11 Scheinbare Ædif. wie 50 A. Е. Rexz, 1296. Februar 25. № a 2 + 2 +40 Pulkowaer Sternzeit > der Aufnahmen. Mittel. ee mm = 31079 — 47118 — 4.7101 9° hen’ 2 — 4.3107 5.0696 — 4.6716 — 4.6722 0,30 2 4.2754 9° 6” 50 — 5.0630 — 4.6744 — 4.6696 то 1—2 — 4.2715 — 5.2034 — 4.8006 — 4.7991 В 2—3 — 4.3933 Trabant — Jupiterscentrum. D. | Mittel. Later То ии) Ph. | Au cos à mm mm — 3.6608| <+-1.0493 1—2 13 + ве —1.0519 | —1'0447 | -+0'0007 | —o'oo11 | -+4'0443 5 — 3.7413| 1.0578 2—3 — 2.6821] -+2.0280 2 FE Fe pete +-2.0200 | -+2.0061 | 0.0015 | —o.oor1 | -+2.0065 HT — 2.7836| +2.0155 2 — 9.7822] —5.0721 2 = er = 2 Tr Re Erle — 5.0741 | —5.0393 | —0.0035 | —0.0011 | — 9.0439 13 — 9.8719] — 5.0728 2 + 2.8846| +-7.5047 2 “+ 1: Re +7.5932| +7.5412 | +0.0048 | —о.оотт | -+7.5449 En + 2.7962| +7.5953 2 Fra = 0.99314 —i9, = — 0.00214 fx = 0.99286 —м =- 0.00215 XL =+ 74 Rec 2 Try = — SI Fa = 099315 \ ——0.00264 h m a,=8 10.8 127 Bilder. eihe. Scalenablesung. . Аша] (5 егпе р. | = | | 68.5648 ] 68.2020 1 67.8225 ] 66.7790 66.4079 | 66.0415 | 65.0380 | 64.6821 | 64.3034 63.3359 | 62.9635 | 62.5806 IE b | +19 +1] ар +10 +18 +10 + 8 Es D +19 +21 IS IE +11 +17 +10 +11 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. wie 50 A, mm 59.8421 60.2104 60.5786 61.6271 62.0005 62.3604 63.3629 63.7316 64.1010 65.0710 65.4569 65.8226 60.4559 62.2384 63.9776 65.6916 60.7821 62.5611 64.3019 66.0110 58.8775 60.6581 62.3979 64.1110 62.0270 63.8046 65.5456 67.2549 P.-Kr.90° |t-+R| P.-Kr.270°|6+R mm mm 10000] 10000 +14 +14 +10 Scheinbare Decldiff. wie 50 A. dy = -+20° 47'2 +++ ТЕ III +++ +++ +44 РИН ++ 1=96. Februar 25. Decl. Buy a0 on о ^^ хо > 4.5286 2.7452 1.0070 0.7076 4.2068 2.4236 0.6819 1.0278 6.1066 4.3253 2.5858 0.8708 2.9593 1.1804 0.5606 2.2713 Znt%2c+%s о mm + 4.7782 + 2.9916 + 1.2566 — 0.4605 тт — 0.2496 — 0.2464 — 0.2496 —0.2471 —0.5714 —0.5680 —0.5747 — 0.5673 —+1.3284 —1.3337 1.3292 1.3313 — 1.8189 — 1.8112 —1.8172 —1.8108 —0.5704 +1.3306 —1.8145 198 = 0.99338 fs = 0.99290 f's = 0.99338 ei И — 2 tg0 sin 1 x? as , у— = 19051 1 Trabant — Jupiterscentrum. —0!2466 —0.5666 —+1.3218 — 1.8025 +0:0023 » +-0.0044 — 0.0111 —0.0167 195 = -+-0.00214 is = -+0.00213 Js = —0.00218 . у нь va | Mittel. Fol) Jat—2)|-ee-22)) Ph. Bemerkungen zur Aufnahme. -+0:0004 | +-0.0001 +-0.0008 | -+o!ooo1 —0.0041 | +-0.0001 —+-0.0007 | -+0.000т x 18 = +73 —0:2438 —0,5613 +1.3067 —1.7850 96 Е. Renz, 51 A. 1896. Februar 26. № 1% Scalenablesung. Pulkowaer Sternzeit Object. г ® Zur ce, Bilder. P.-Kr. 0° t--k| P.-Kr.180° tk 3 der Aufnahmen. | Mittel. mm n 10000 n Ctr, | 64.6386 63.7508 +, de S 64.6370 |+-16| 63.7500 0.0000 3 M Durch elin Jlupitersbild N 25.4968 |-+25| 102.8929 — 39.1392 Е 3—4 Q 78.2449 |+21| 50.1435 13.6068 8" Hr mod. 3 В 27.9462 |-+34| 100.4432 — 36.6891 3—4 124 64.3545 |+17| 64.0341 — 0.2836 3 W 65.4608 |-+28| 62.9284 + 0.8225 3 %а, | 68.9900 |+14| 59.4169 + 4.3428 ag | 69.3908 |+14| 59.0045 —+ 4.7494 + 4.7514 8 35 46 4—5 ag 69.8020 |-+17| 58.5901 + 5.1624 %6, | 69.0080 |-+13| 59.3954 + 4.3626 A 324803 be | 69.3948 |-+13| 59.0080 + 4.7496 + 4.7518 36 54 В ВЫ 3—4 b, 69.7826 |+16| 58.6091 + 5.1432 % Cp 69.0085 |-+13| 59.3934 + 4.3638 Ce | 69.3964 |+13| 59.0045 + 4.7522 + 4.7554 37 44 3—4 C6 69.7906 |+-16| 58.6031 + 5.1502 %а, | 68.9670 |-+-13| 59.4379 + 4.3208 de 69.3598 |-13| 59.0480 + 4.7121 —= 4.7149 38 44 4 do | 69-7571 |+-16| 58.6461 + 5.1118 Trabant — Jupiterscentrum. 2 — Ty | Mittel. и] РВ. | Au cos à mm mm Та | 67.8370 |+19| 60.5542 + 3.1980] —1.5534 3—4 b | 67.8335 |-18| 60.5606 + 3.1930] —1.5588 r , Bu en 3 с | 678370 |+18| 60.5556 + 3.1973| —1.5581 — 1,5588 | —1:5482 | -н0'0004 0.0011 1:5489 | 3 Я | 67.7900 |18| 60.6032 + 3.1498] — 1.5651 3 | Па | 66.4204 |+11| 61.9775 —= 1.7776] — 2.9738 3—4 | 6 | 66.4198 |+-10| 61.9750 + 1.7786] —2.9732 _9 9% 3 e | 66.4254 [+19] 61.9710 + 1.7834| —2.9720 — 2.9741 | —2.9540 | -+0.0008 | —0.0011 2.9548 | 5_3 а | 66.3784 |+-10| 62.0155 + 1.7376] —2.9773 3—4 Ша | 67.3848 | 9| 61.0090 + 2.7440] —2.0074 3—4 b 67.3878 |-= 8| 61.0050 —= 2.7474] —2.0044 Е 2—5 с | 67.3984 |+ 8| 60.9945 + 2.7580] —1.9974 —2.0027 | —1.9891 | -+0.0006 | —0.0011 1.9896 | 24 d | 67.3538 |+ 8| 61.0390 + 2.7134| — 2.0015 3 N IV a | 78.4898 |+ 8| 49.9080 —+-13.8472] -+9.0958 3—4 unterex р b | 78.4898 |+ 8| 49.9050 13.8486] -+9.0968 2 N с | 78.4978 \+- | 49.8995 +-13.8554| -+9.1000 +-9.0964 | -+9.0347 | —0.0025 | —0.0011| +9,0311| 5 1! а | 78.4494 |+ 8| 49.9460 —13.8079| -+9.0930 4 unterer Scheinbare Ва. wie 50 A. Fra = 9.993 22 —i° , = +-0.00062 À Ja = 0,99294 —i, = 0.00061 x = —21 Refr. =+ I Try = + 91 f'ax =0.99322 Ja —+000115 В т ty = 8 10.5 Das Sternpaar NS giebt einen stark abweichenden Wert für f°,, daher ist der aus dem Bogen QR abgeleitete Scalenwert bi corrigiert um die halbe mittlere Differenz f°,, (NS) — f°, (QR). A P.-Kr.90° | 63.6695 | 63.6690 | Durch e | 67.1880 | 39-0945 | 39-0770 | 44.2743 | 94.6123 | 67.1995 . 66.8230 | 66.4399 65.4059 65.0405 64.6701 63.6611 63.3049 62.9310 | 61.9026 ‚61.5286 | 61.1640 | 67.1940 | 65-4159 63.6751 61.9090 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. tt P.-Kr. 270° _тт_ 0000| тт 64.7272 + 8| 64.7256 in Jlupitersbild +25| 61.2033 +30) 89.2999 +39| 89.3147 +19| 84.1166 — 2| 33.7852 + 9| 61.203 + 9| 61.5872 +-11| 61.9640 +17| 62.9980 +17| 63.3728 +17| 63.7266 + 9| 64.7401 +10| 65.1160 +10) 65.4654 +10) 66.5092 +-10| 66.8800 —=11| 67.2444 + 8| 61.2055 -+16| 62.9840 * + 8| 64.7246 + 9| 66.4928 +18| 60.8420 +10| 62.6196 + 8| 64.3619 + 9| 66.1275 + 8| 61.0120 +10| 62.7896 + 8| 64.5316 + 9| 66.3019 +22| 63.7700 15| 65.5492 16| 67.2944 +16| 69.0570 _ Scheinbare Decldif. wie 50 A. k $ 1596, Februar 26. Decl. 2 _ > $05 sin 1’ dy = +20° 48:3 Зап. Фяз.-Мат. Отд. RS or уУ—- #9581 1 Mond sehr nahe. t+k mm mm 10000] 10000 тт тт тт тт 16| о 0.0000 0.0000 0.0000 verdleckt. +26|— т|-н 3.5209 — 0.0805 + 3.4404 — 2|+ 6| —24.5718 — 0.0094 — 24.5812 + Ai ROME — Se —24.6559 — 7|-+ 2] —19. .0000 —19.3912 +-21|—20| +30.9391 0.0000 + 30.9391 +12 + 3.5266 +11 + 3.1465 +1 + 2.7666 +1! + 1.7330 +11 + 1.3628 +10 — 1.0008 +18 — 0.0112 +-18 — 0.3772 +18 0.7389 +10) 1.7746 +10 2.1470 +10 — 2.5114 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. Ir uva) | в (его) впал) Ph. | тт тт +II + 3.5228| -+0.3762 Bar = ar Er | -+0.3790 | -+0/3765 | -=0'0012 | +-0'0006 | +0:0001 НТ — 1.7633] -н0.3810 11 + 3.8874] -+0.7408 АЕ + N о 0.7427 | -+0.7378 | -++0.0023 | -+0.0011 | -+0.0001 +11 — 1.3997| -+0.7446 +II + 3.7145] +0.5679 ur + Я BL, -+0.5695 | -+0.5657 | 0.0016 | -+0.0008 | -+0.0001 +11 — 1.5744] -+0.5699 +13 + 0.9577] —2.1889 +В = ER: Zn —2.1872 | —2.1728 | —0.0073 | —0.0093 | -+-0.0001 +18 — 4.3292| — 2.1849 1°5 = 0.99339 125 — —0.00082 fs = 0.99291 is =— 9.00033 Xi, = —29 f's = 0.99338 Js; = —0.00080 Bemerkungen zur Aufnahme. Aù +0:3784 —+0,7413 —+0,5682 —2,1893 51 B. Object. Scalenablesung. P.-Kr. 0° Anhaltstierne| wie 51 А, mm 59.5992 60.0020 60.3939 59.5772 59.9660 60.3509 59.5896 59.9795 60.3839 59.5526 59.9415 60.3279 58.3789 58.3459 58.3639 58.3149 56.9890 56.9550 56.9760 56.9290 58.0395 58.0075 58.0340 57-9915 69.0955 69.0645 69.0800 69.0405 t-+k| P.-Kr.180° mm 10000 +15 0 15 +14 +14 +14 +14 +14 +14 +14 +14 +14 — лм DO 0000 un DO УЕЕЕ ЕУЕЕ ЕЕ ЕЕ +13 mm 68.8025 68.4019 67.9960 68.8240 68.4344 68.0410 68.8110 68.4129 68.0080 68.8570 68.4628 68.0650 70.0135 70.0450 70.0290 70.0790 71.4039 71.4389 71.4189 71.4688 70.3534 70.3854 70.3589 70.4039 59.2994 59.3294 59.3129 59-3544 НЕ тт | mm 10000] 10000 Scheinbare Жане. wie 51 А. Siehe Anmerkung zu 51 А. ЕЕ | + F. RENZ, 1896. Februar 26. 6.2617 6.2940 6.2770 6.3266 7.6514 7.6860 7.6655 7.7140 6.6014 6.6334 6.6067 6.6507 4.4543 4.4238 4.4398 4.3992 ER ее Pulkowaer Sternzeit : der Aufnahmen. Mittel. mm — 4.6448 9 52” 46° 3—4 — 4.6782 53 34 2—3 gr — 4.6572 54 34 3—4 — 4.7045 55 34 3—4 Trabant — Jupiterscentrum. re | Mittel. >) Tome ya) Ph. | Aa. côs 5 mm тт — 1.6169 ä 2—3 m —1.6186| —1'6076 | +o:ooor | —o:oo1ı | —1'6086 И — 1.6221 2—5 — 3.0066 2—3 EE —3.0080| —2.9876 | +0.0001 | —o.0011 | —2,9886 “à —3.0095 2 — 1.9566 3 er —1.9519| —1.9386 | +0.000т | —0.0011 | —1,9396 3 — 1.9462 3 49.0991 2 - 2—3 a -+9.1004 +9.0387 | —0.0003 | —0.0011 | +9.0873 | 57 —9.1037 ‹ 2 1% =0.99322*). _ —® = -+0.00062 До = 0.99294 —4 = 0.00061 X Ty = — 21 Вей. = + 4 Try mi SI f'x = 0.99322 J, = —0.00014 т ay = 8” 10.5 12) Bilder. | eihe. P.-Kr.90° Scalenablesung. t-il P.-Kr. 270° Anhaltstierne mm 67.2475 66.8815 66.4962 65.4734 65.1100 64.7396 63.6831 63.3204 62.9345 61.9020 61.5392 61.1715 67.2680 65.5006 63.7051 61.9325 67.6211 65.8580 64.0640 62.2904 67.4324 65.6656 63.8655 | 62.0900 64.6751 | 62.9065 | 61.1085 | 59.3319 Scheinbare Decldiff. wie 51 A. +10 +12 +10 HE IX +21 +13 +11 +12 +10 +12 +10 +1] +17 +10 ue) Ем POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. wie 51 А, mm 61.1480 61.5332 61.9140 62.9255 63.3014 63.6571 64.7176 65.0880 65.4628 66.4982 66.8745 67.2340 61.1320 62.8960 64.6911 66.4634 60.7735 62.5392 64.3339 66.1070 60.9650 62.7301 64.5292 66.3029 63.7246 65.4914 67.2884 69.0680 t-+k mm mm 10000] 10000 FI +10 +10 #10 +10 Rs +17 +17 +17 ARE 29 ug +11 +10 +17 +11 +12 ll +10 +12 +11 +10 +17 +11 9 +17 m) +14 тт 3.5784 3.2028 2.8198 1.8030 1.4334 1.0704 0.0110 0.3554 0.7358 1.7694 2.1389 2.5024 ГЕ +++ + 3.5966 1.8311 0.0354 I +++ 1.7368 3.9530 2.1882 0.3938 1.3796 3.7624 1.9966 0.1965 1.5778 1.0044 0.7641 2.5612 4.3395 РНЕ Ba: 99 1396. Februar 26. Dec]. % % 2 2 В k ВЕНЕ Son (los usa | Ви mm + 3.2003 + 1.4356 — 0.3601 — 2.1369 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. u) Лаба |-e-22)) Ph. 45 тт тт —+-0.3963 a +0.3968 | +0!3942 | -но’оотт —0.0010 | -но’ооот | -+0:3944 —-0.4001 —+-0,7527 Rae +0.7541 | 0.7491 | 0.0021 —0.0020 | 0.000: | -+0,1493 —=0.7573 —0.5621 $ one —+0.5597 | <+0.5560 | -+0.0014 —0.0012 | -+0.0001 | -+0,5563 +-0.5 591 —2.1959 Eu — 2.1998 | —2.1853 | —0.0065 0.0011 | -+0.000т | — 2.1906 — 2.2026 ? f°5 = 0.99339 1°5 = —0.00082 fs —0.99291 is =— 0.00083 X is ——2g f's = 0.99341 Js = —0.00072 t+k 100 52a A. Scalenablesung. Object. P.-Kr. 0° tt P.-Kr.180° mm mm mm Ctr. | 63.7259 64.6592 S 63.7251 |-+ 8| 64.6576 М | Durch elin Jlupitersbild N 24.5596 |4-26| 103.8244 Q 77.3628 |+21| 51.0206 R 27.0522 |+34| 101.3272 1% 63.4607 |+-18| 64.9160 W | 64.5073 |+28| 63.8697 %Q, | 68.0780 |-+19| 60.3179 a. 68.4668 |-+19| 59.9295 а, | 68.8595 |+14] 59.5302 ZDy | 08.0965 |+19| 60.3048 b. | 68.4708 |+-19| 59.9280 bo | 68.8555 |+14| 59.5392 %а4., | 68.0690 |+18| 60.3294 de | 68.4508 |-+-18| 59.9610 do | 68.8310 |+-13| 59.5626 %е, | 68.0640 |+18| 60.3329 ес 68.4464 |-+18| 59.9540 ео | 68.8206 |+13| 59.5746 Та | 66.6571 |+ 9] 61.7346 b | 66.6651 | 8| 61.7286 а 66.6441 |+ 8| 61.7451 e | 66.6381 |+ 8| 61.7476 Па | 65.1700 |+17| 63.2170 b | 65.1780 |+17| 63.2155 d | 65.1495 |-+16| 63.2429 е | 65.1440 |+-16| 63.2459 Ша | 69.4224 |+14| 58.9625 b | 69.4219 |-+13| 58.9665 а | 69.3929 |+13| 58.9940 е 69.3784 |-+13| 59.0080 IV Bei der | Mes|sung Scheinbare ВАШ: N-—-Centrum über|sehe Fr De W— 10000] 10000 ] verdjeckt. + 6|+17 +20|— 4 +-13|+22 mm mm +16 о —22 O +24| о 14 +14 +14 IA +14 +14 +16 +15 +15 HIS —=15 —=15 SO ri 9 „21,9 —-IO) + 9 519 39 +10 +-10 +10 +11 IN n. » » » » Е. Renz, 1896. März =. Ж 136 Pulkowaer Sternzeit AT ЗЫ Bilder. р der Aufnahmen. Mittel. mm mm 0.0000 3 — 39.1630 5 2—3 +-13.6374 31” 37 3 —36.6676 2 — 0.2612 1—2 + 0.7856 3—4 — 4.3470 + 4.7356 + 4.7380 13 14 2 Sous + 4.3628 + 4.7383 —+ 4.7420 BA, 32 1—2 . 8 т Er 881 15”. 18 — 4.3366 + 4.7117 == 4.7164 CRE 2 + 5.1008 + 4.3324 + 4.7130 + 4.7117 И 9 2 + 5.0896 Trabant — Jupiterscentrum. 1—2 | Mittel. Иез) Зиг уз) Ph, | Az cos à mm `тт + 2.9279] —1.8 тот - Е + 2.9348] —1.8072 ' , A A: == | ть ER т. ‚ —1.8044 | — 1.7919 | -+0/0010 0.0017 1.7926 | 5 unterexponie: + 2.9118] — 1.7999 | Schimmer. — ie —3.2944 : N =. en ZN —3.2950| —3.2722 | +0.0019 | —0.0017 | —3.2720| > _4 unterexp. + 1.4160] —3.2957 3 пибегехроше + 5.6968] -+-0.9588 2 | Е 73 ee +-0.9504 | -+0.9438 | —0.0007 | —0.0017| 0.9414 | 34 | + 5.6520| 0.9403 3 | — — 41/4093 f° «= 9.993083 —1°, = +0.00180 = +-13.3270 т = — 38.7087 fx = 9.99280 —1, =—0.00180 X 1, —=— 62 — 0.3187 Refr. = о — + 0.8860 Try =+ SI Г’. = 0.99308 Jy =-+0.00231 ой M ау=8 7.4 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896. März =. sihe. Decl. Scalenablesung. = - 5 y etes — = $05 sin 1’ у— 8 sin 1’ P.-Kr. 90°|t+R|P.-Kr. 270° | ++ тт тт тт Вов | еее | Tr Е 7 sé 64.0720 |+ 8| 64.3158 |+ 8 о 0.0000 0.0000 0.0000 Durch еш Jlupitersbild |verdleckt. 67.5541 |-+35| 60.8319 |<10]— 1|+ 3.4842 — 0.0805 + 3.4037 39.5086 |+-30| 88.8769 |— 2]-+ 6| —24.5600 — 0.0094 —24.5694 39.4280 |+40| 88.9470 |- 9]-+15| —24.6346 — 0.0689 —24.7035 44.6741 |-+19| 83.7078 |— 7|-+ 2| —19.3934 0.0000 —19.3934 95-0171 |— 2| 33.3712 |+-19|— 8| +30.9430 0.0000 —30.9430 67.5976 |+18| 60.8040 |+11 + 3.5190 67.2365 + 8 61.1790 |+и + 3.1505 + 3.1511 66.8620 |+ 8| 61.5378 |+11 + 2.7838 65.9720 |-+10| 62.4289 |+10 —+ 1.8934 65.6171 |+10| 62.7900 |+10 + 1.5354 + 1.5370 65.2590 |-+16| 63.1390 |+10 —+ 1.1822 62.5831 + 9| 65.8240 |+и 1.4986 62.2349 |+ 9| 66.1810 |+11 — 1.8512 — 1.8543 61.8660 + 9| 66.5358 |-+11 — 2.2131 - 60.8580 |+10| 67.5416 |+19 — 3.2204 60.5076 |+10| 67.9045 |+19 — 3.5770 — 3.5760 60.1460 |-+14| 68.2504 |-+19 — 3.9306 | | | 67.6801 |-+18| 60.7161 |+11 66.0660 |+10| 62.3289 |+10 M 62.6711 + 9| 65.7256 |+17 60.9540 |+10| 67.4414 |+ 9 68.0570 |-+18| 60.3359 |+1s 66.4419 10| 61.9550 |+10 63.0515 |+ 9] 65.3474 |+17 61.3319 |+10| 67.0650 |+ 9 66.9250 + 9| 61.4678 |+12 65.3094 |+17| 63.0850 |+ 61.9200 |+10| 66.4738 |+12 60.2010 |+15| 68.1895 |-+20 | Bei der | Messung überselhen. Scheinbare Decldif: N-—Centrum — » R— » 7— » W— » Trabant — Jupiterscentrum. к и т Yt—Y2 | Mittel. [из ии | 7з (ро) mm mm 3.6042] -+0.4531 1.9904| 0.4534 1.4058| -+0.4485 3.1218] -+0.4542 3.9826] -+0.8315 2.3654| -+0.8284 1.0264| -+0.8279 2.7446| —+0.8314 —+0.4523 | —-0:4492 | -+0:0034 —0'!0007 | = -+0.8298 | -+0.8242 | -+0.0062 —0.00т1 art —= 2.8504| —0.3007 LA a wo —0.3002 | —0.2982 |. —0.0018 | —0.0006 — 3.8726] —0.2966 = + 3.4510 198 = 0.99327 $78 = —0.00188 = — 24.4325 = —24.4680 fs = 0.99279 is =— 0.00188 X 5 —=— 6.5 = —19.2648 5 N = 30.7327 Га =0.99325 Js = —0.00187 dy = -+20° 57.9 De + 0/0001 —+-0,4534 —-0.0001 —+0'8316 —+-0.0001 —0.3005 101 Bemerkungen zur Aufnahme. Bilder 4. Die Luft wird dunstig. Ph. | Ad 13* 102 522 B. Object. Lan! — — >. за 8.8 >. за u III IV Scalenablesung. P-Kr..0- Anhaltstierne mm 58.6151 59.0380 59.4499 58.5751 58.9960 59.3954 58.5882 58.9940 59.4004 58.5911 59.0065 59.4004 57-4604 57.4209 57-4294 57.4359 55.7690 55.7231 55.7246 55.7336 59.7101 59.6611 59.6641 59.6651 Bei der th) P.-Kr. 180° | wie 522 A, mm tk mm _|_mm 10000] 10000 +16 +13 +13 +16 +13 +13 +16 +13 +13 +16 +13 +13 +12 —I2 +12 T2 +14 +13 +13 +13 +13 +13 IS +13 10000 mm —11| 69.7760 +11] 69.3749 +11] 68.9450 —11| 69.8195 —=11| 69.4139 —=11| 68.9990 —10| 69.8080 —+-10| 69.4129 --10| 69.0020 —70]| 69.8105 +-10| 69.4079 +10] 68.9975 -Н11| 70.9250 —10| 70.9690 —=10| 70.9590 229127 0.9559 + || 72.6201 ol 72.6631 0| 72.6621 — 1| 72.6561 +15) 68.6751 +15| 68.7196 —=14| 68.7211 +-14| 68.7191 Meslsung über|sehe In. Scheinbare Adiff. wie 52% A. F. Renz, 1=96. März =. Ж 3 Pulkowaer Sternzeit der Aufnahmen. Mittel. 1140 Se 4.7019] — 4.6990 où es 2—3 4.2810 5.1558 4.7424 — 4.7445 40 9 1—2 4.3352 9 40” 24 5.1436 4.7430 — 4.7403 Я 12 4.3343 5.1434 4.7342 — 4.7365 42 2 2—3 4.3320 Trabant — Jupiterscentrum. Lt — Ty | Mittel. Later) Te (из) Ph. | Aa. cos à mm mm 6.2657| —1.5667 à 2 6.30 —1,5630 r r r == — ОВ = —1.5608 | —1:5500 | +0.0005 | —0.0017 | —1:5512| 5 unterexponiert. 6.2920| —1.5555 3 unterexponiert. 7.9596] — 3.2606 2—3 8.0040| —3.2 + Ex 2 8.5028 Е — 3.2604 | —3.2378 | +0.0011 0.0017 3.2384 | > unterexponiert, 7.9953| —3.2588 3 4.0158] +0.6832 2 а ne +-0.6800 | -+0.6753 | —0.0003 | —0.0017 | 0,6733 ER 4.0603] 0.6762 3—4 Fa = 0.99308 —®, = 0.00180 fx =0.99280 —iy = -0.00180 X = — 6.2 Вет. =-н 4 Try — — SI Г’, = 0.993140 Ju = 0.00138 ay= % 7.4 131. Bilder. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCBEN AUFNAHMEN. 1596. März =. 5 y t-+k mm mm 10000] 10000 mm +10 + 5.1194 +14 —+ 4.7292 +14 —= 4.3339 —=то + 3.4533 +10 + 3.0722 + 9 — 2.6852 + 9 + 1.6722 +9 + 1.2900 +9 ++ 0.9099 + 8 — 0.0234 +16 — 0.4114 +16 — 0.7832 1 + 5.1322 т! + 3.4728 +10 —= 1.6880 + 9 — 0.0037 +13 + 5.5616 +17 —+ 3.9049 +12 + 2.1190 +11 + 0.4299 +14 + 4.4917 +10 —+ 2.8404 + 9 + 1.0558 +16 — 0.6380 eihe. Scalenablesung. |Р.-Кг. 90° tk) P.-Kr. 270° | Anhaltstlerne| wie 52° А, | mm 10000 ‚| 69.1985 |-+15| 59.2040 °| 68.8110 |-+т15| 59.5966 1 68.4119 |+20| 59.9885 67.5308 |10| 60.8680 ‚ | 67.1585 |-+10| 61.2580 66.7635 +10| 61.6371 ‚ | 65.7510 |-+12| 62.6506 | 65.3769 |-+18| 63.0415 64.9870 |+18| 63.4119 ‚ | 64.0540 |+10| 64.3449 63.6691 |+10| 64.7350 | 63.2969 |+10| 65.1065 Л | 69.2055 |-+15| 59.1855 | 67.5482 |+-21| 60.8475 ‚ | 65.7630 |-+13| 62.6311 | 64.0745 [+11] 64.3259 `| 69.6331 |+-16| 58.7540 ı | 67.9755 |-+21| 60.4099 ‚ | 66.1905 |-+13| 62.1965 64.5042 |-+19| 63.8890 `| 68.5621 |-+14| 59.8225 '| 66.9120 | 9] 61.4748 ‚| 65.1270 |-+17| 63.2599 |] 63-4349 |+10| 64.9540 H — Ве! der | Messung überselhen. _ Scheinbare Decldiff. wie 522 A. би = -+20° 57'9 Decl. 9 и+% +9, + 4.7275 + 3.0702 -+ 1.2907 — 0.4060 x? NE x? . — Ztg8 sin Г у — + 96 sin 1" Trabant — Jupiterscentrum. . му veux | Mittel. [а иг-уз)| 7 иг) тт тт —+0.4047 —+-0,4026 —0.3973 —+0.4023 +0.8341 +0.8347 0.8283 0.8359 —0.2358 —0.2298 —0.2349 —0.2320 +-0.4017 +-0.8332 —0.2331 125 = 0.99327 fs = 0.99279 f's = 099328 0/3990 | —<+0!0028 —0/0010 +0.8276 | —+0.0058 —0.0023 —0.2315 | —0.0012 —0.0003 2; = —0.00188 iz =— 0.00188 Js = — 0.00179 x ig = —6:5 103 Bemerkungen zur Aufnahme, Bilder 3. Ph. —+-0/0001 —+0.0001 —+0.0001 +-0:4009 0,8312 — 0,2323 104 Е. Renz, 52b А. 1896. März 9. AR Scalenablesung. Pulkowaer Sternzeit Object. A MSA out) Bilder. P.-Kr. 0° tt P.-Kr.180°| #-+# der Aufnahmen. Mittel. vn 10000 10 10000 10000 vun тт Cir. | 64,3334 64.0468 M 64.3326 |+ 8| 64.0460 |+ 8 (6) H 2 N: 20.1966 |-+23| 108.1853 |+ 5]|-25| —44.1342 En Rte 2 etwas ellipt. 1 Q 72.9526 |+27| 55.4345 |+11|— 2|-+ 8.6214 10° 25 5 2 R 22.6392 |-+38| 105.7332 |-+17|-=32] —41.6860 2 У 59.0541 69.3203 |#+25|-+ 1] — 5.2765 1—2 W 60.1918 68.1908 |-+32|+- 1] — 4. 2 %а | 68.6421 59.7600 |+14 + Ge 69.0710 59.3359 |+-10 + + 4.7234 TON 2145 2—3 y | 69.4924 58.9100 |+-IO + 2b, | 68.6186 59.7820 |+-14 + be | 69.0340 59.3689 |+10 +- + 4.6887 7] 2—3 bo | 69.4444 58.9550 |-+10 „+ 10% 15” 13° 2% dun | 68.6486 59.7580 |+15 + de | 69.0445 59.3584 |+I1 + + 4.7016 16 20 2—3 do | 69.4469 58.9540 |+11 + Hey | 68.6411 59.7600 |+15 + ес 69.0530 59.3574 |-11 + + 4.7028 ТИ ИО 2—3 ео 69.4509 58.9515 |-+11 + Trabant — Jupiterscentrum. Lt—Ly | Mittel. Ре) Tavt—y)| Ph. | Да cos à mm mm Je 69.8740 |+17| 58.5202 |+10 + 5.5340] +-0.8106 à 69.8300 |-+17| 58.5616 |+10 + 5.4912] -+-0.8025 , BR, у р 4 | 60.8355 [+16| свеса |+ 4976] 0/7560 —0.7989 | -н0:7934 0:0002 0.0017 | +0:7915| 3 е 69.8290 |-+16| 58.5641 |-+11 + 5.4894] +0.7866 3 > 70.2335 |-+17| 58.1550 .|#+ 5 + 5.8966] <+1.1732 B 70.2030 |+16| 58.1905 |+ 5 + 5.8635] +1.1748 Le 4 а | 70.2260 |+-16| 28.1670 |+ 6 + ©8867] +1.1851 +-1.1806 | -+1.1725 0.0003 0.0017 | +1.1705 | 3 е 70.2290 |+16| 58.1590 |- 6 + 5.8922| 1.1894 3 Ша | 65.4339 |+17| 62.9520 |+ 9 + 1.0980 mes 5 b 65.3954 |+17| 62.9920 | 9 — 1.0588] — 3.6299 | __ ae + ns р а | 65.4094 |+16| 62.0835 |+10 + 1.0700| —3.6316 3.6313 3.6064 | -+0.0009 0.0017 3.60721 3 e 65.4029 |+16| 62.9880 |+10 + 1.0644| — 3.0384 3 IV a | 65.2584 |+17| 63.1290 |+ 9 + 0.9218] — 3.8016 4 b | 65.2270 |+17| 63.1620 |+ 9 + 0.8896] — 3.7991 | __ Ai и. EN 3 а | 65.2480 |+16| 63.1420 |+10 —= 0.9100] — 3.7916 3.7960 LUS | en 2.0047 3.7706 3—4 e 65.2500 |+16| 63.1420 |+10 + 0.9110] — 3.7918 ищегехрошег! Scheinbare ВАШ: N—Centrum— —46!6793 Fa = 0.99312 —1° 4 = +0.00060 — » = 9.0570 с R— » = —43.9787 fa = 0.99281 —iy = -+0.00055 X i,=— 19 У » — — 5.5887 Вет. + 6 W— » = — 4.3842 Try —=+ 52 » Го = 0.99313 I = 0.00113 h т GOOM el reihe. L à pe POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. Scalenablesung. P.-Kr.90° tr P.-Kr. 270° 63.3748 |10000 63.8740 64.4095 36.2665 36.2792 41.4542 91.7947 67.4149 67.0185 66.6211 65.6661 65.2769 64.8880 62.2330 61.8540 61.4832 60.5861 60.2055 59.8290 21900 5.0530 61.6371 59.9860 66.7680 65.0285 61.6081 59-9510 67.8555 66.1190 62.6986 | 61.0460 | 68.0270 66.2869 -62.8710 | 61.2190 Scheinbare Decldiff: +10 +10 +10 +10 615104 64.5088 63.9812 92.1243 92.0996 86.9239 36.5953 60.9920 61.3849 61.7840 62.7371 63.1340 63.5198 66.1735 66.5501 66.9280 67.8235 68.1995 68.5718 61.6001 63.3429 66.7600 68.4089 61.6356 63.3689 66.7880 68.4419 60.5342 62.2770 65.6936 67.3469 60.3639 62.1090 65.5232 67.1825 1396. März 9. y t+k mm mm 10000] 10000 um 16| о 0.0000 4-25 о + 0.5319 — 3|-+ 6] —27.6092 + 11|4-20| —27.5891 — 3|-+ 3] —22.4153 +-22]— 7] +27.9154 +12 + 3.5291 +12 + 3.1344 +11 + 2.7362 +11 + 1.7823 +11]. + 1.3896 и -+ 1.0022 +12 1.6526 +10 — 2.0302 10 2.4046 +20 3.3014 +20 — 3.6794 -+20 — 4.0538 +1 + 2.9126 +11 + 1.1732 +10 — 2.2436 +20 — 3.8939 +11 + 2.8839 +11 + 1.1479 +10 — 2.2722 20| — 3.9279 +II —+ 3.9788 +10 + 2.2388 +11 — 1.1798 + 9 — 2.8326 +15 + 4.1495 +10 + 2.4068 т — 1.0084 + 9 — 2.6639 Q— » Е— ь У— » W— » Зап. Физ.-Мат. Отд. N—Centrum = + 0.4473 = — 27.4717 = —22.2685 = +-27.7290 dy = -+20° 58.6 Decl. 9% +9, 3 mm + 3.1332 + 1,3914 2.0291 3.6782 тт тт — 0.2206 —0.2182 —0.2145 — 0,2157 —0.2493 —0.2435 —0.2431 —0.2497 —=0.8456 —0.8474 —0.8493 —+-0.8456 —0.2172 —0.2464 +-0.8470 +-1.0163 +-1.0154 +-1.0207 +1.0143 +-1.0167 f°s =0.99338 fs —0.99285 Г’; = 099337 es Heine r — > 96311 тт 0.0000 0.1022 0.0038 0.0890 0.0014 0.0009 ars] Trabant — Jupiterscentrum. 2 gi vs | Mittel. fa ги) Je гы) — 0.2158 | —0!0004 —0.2448 | —0.0006 -0.8414 | -0.0018 +-1.0100 | -+0.0019 13 = —0.00052 3 = —0.00064 Js = —0.00050 Ka, r у — — 9031 1 0.0000 + 0.4297 — 27.6130 — 27.6781 —22.4167 27.9145 105 Bemerkungen zur Aufnahme. Bilder 2— Bilder 3. —0:000$ | 0.0001 —0.0007 | -+0.0001 0,0011 | -+0.0001 —-0,0012 | 0.0001 X ig—— 212 14 о 2, —0:2166 —0,2460 —=0,8444 +-1,0132 106 52 B. Scalenablesung. Object. - P.-Kr. 0° ++ P.-Kr. 180° Anbaltstlerne| wie 52? A. mm 10000 mm тт %7 | 59.2055 |+-11| 69.2000 ИС 59.6126 |+15| 68.7850 do 60.0290 |--15| 68.3704 %hyp | 59.2210 |+ 11| 69.1850 he 59.6246 |15| 68.7750 ko 60.0300 |+15| 68.3744 Zip | 59.2260 |10| 69.1780 ie 59.6011 |+14| 68.7890 Lo 60.0105 |-+14| 68.3879 %kyp | 59.2210 |10| 69.1850 ke 59.6136 |+14| 68.7910 ko 60.0100 |+-I4| 68.3919 If | 60.3314 |+ı5| 68.0550 h | 60.3289 |-+15| 68.0610 à 60.3134 |+-14| 68.0730 k | 60.3064 |+14| 68.0840 Ne 60.8540 |+11| 67.5282 h | 60.8715 |-+11| 67.5172 i 60.8670 |+-10| 67.5212 Е | 60.8705 |+10| 67.5172 II f | 55.9445 |+ 1| 72.4429 h | 55.9470 | ©] 72.4399 и 55.9375 ©] 72.4539 k | 55.9320 |— 1| 72.4579 ТУТ | 55.8565 |+ ı| 70.5361 h | 55.8690 O| 70.5231 р 55.8635 |— 1| 70.5311 k 55.8655 |— 1| 70.5311 НА mm. mm 10000] 10000 +14 +14 +19 +13 +13 +18 +13 +13 +18 +14 +14 +19 +19 +18 +18 +19 +18 +18 +19 +19 Ета +11 +11 +12 +13 +12 +12 +13 Scheinbare Adiff, wie 52b А. mm — 5.1407 — 4.7294 — 4.3142 — 5.1254 — 4.7184 — 4.3156 — 5.1194 — 4.7372 — 4.3322 — ASS — 4.7320 — 4.3345 4.0053 4.0095 4.0233 4.0324 3.4808 3.4665 3.4708 3.4671 8.3930 8.3903 8.4020 8.4069 8.4837 8.4710 8.4778 8.4768 KIEL IA ay = 8? Е. RENz, 1896. März 9. 2 w+r#c+#o mm — 4.7281 10” — 4.7198 — 4.7296 — 14-7307 Pulkowaer Sternzeit der Aufnahmen. 36 40 Mittel. 10° 347 40: Trabant — Jupiterscentrum. 1—2 | Mittel. mm тт —-0.7228 —0.7103 +0.7063 —+-0.6983 1.2473 +1.2533 —+1.2588 +1.2636 о 0 er —3.6710 | —3.6458 —3.6762 —3.7556 Щ— 37582 | —37503| —3.7246 —3-7461 +-0.7094 | —+0.7045 —=1.2558 | —+1.2472 Ли =0.99312 fa =0,99281 Га = 099315 F'a(tt—22) 0'0000 0.0000 —+0.C00I —+0.0001I —0.0017 — 0.0017 —0.0017 — 0.0017 — = +0.00060 —% = 0.00055 Ве. = + 7 Ty = — 52 I, = -+0.00010 Лит РВ. | Au. cos Ô +0:7028 1.2455 —3.6474 —3,7262 < = — 9, 133. Bilder. PoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. P.-Kr.90° 1-Е 1596. März 9. Пес]. UntBcH®%s 3 x? >. 1’ ть $00 sin x? . y— to sin 1’ 107 Bemerkungen zur Aufnahme. ны P.-Kr.270° Anhaltstierne mm 68.9690 68.5841 68.1945 65.4839 65.1000 64.7080 63.7605 63.3959 63.0245 62.0130 61.6401 61.2739 f | 68.3774 h | 64.8950 à | 63.1945 61.4474 68.3129 64.8240 63.1210 61.3719 69.4389 65.9530 64.2500 62.5046 69.5876 66.1025 64.4004 62.6551 wie 52? A, mm 59.4292 59.8195 60.2140 62.9175 63.3114 63.6936 64.6426 65.0085 65.3809 66.3849 66.7660 67.1350 60.0110 63.4976 65.1990 66.9460 60.0870 63.5671 65.2709 67.0200 58.9510 62.4349 64.1400 65.8870 58.8045 62.2919 63.9950 65.7436 — $Scheinbare Decldifi. wie тт_| тт 10000] 10000 dy = 20° 58:6 УЕ ЕН ld! +++ ТИ ТГ ТЕ 5,0876 4.7000 4.3082 1.6014 1.2124 0.8254 0.1236 0.4888 0.8608 1.8682 2.2451 2.6126 4.5012 1.0170 0.6848 2.4314 4.4310 0.9467 0.7574 2.5061 5.5619 2.0769 0.3728 1.3734 5.7096 2.2232 0.5205 1.2265 mm —= 4.6986 + 1.2131 — 0.4911 — 2.2420 mm —0.1974 —0.1961 —0.1937 —0.1894 —0.2676 —0.2664 —0.2663 —0,2641 —0.8633 —0.8638 0.8639 —=0.8686 —+1.0110 -+-1.0101 +1.0116 -+1.0155 mm —0.1942 — 0.2661 +-0.8649 —+1.0120 778 = 0.99338 fs —0.99285 f'a = 0.99339 Bilder 3—4. Trabant — Jupiterscentrum. : u У — 9% | Mittel, [зи (ор о) |-e- 22235 Ph. —0:1929 | —0:0003 —0.2643 | —0.0006, +-0.8592 | <+0.0017 —1.0053 | —-0.0017 28 = —0.00052 3 = —0.00064 Уз = —0.00048 —+-0:0003 | -+0!0001 -+0.0005 —0.0001 —0.0027 | 0.0001 — 0.0028 | -+0.000I Хх 8 =— 2!2 AG —0:1928 —0.2643 +-0.8583 +-1.9043 108 Е. Renz, 53 A. 1896. März 11. AR Pulkowaer Sternzeit Scalenablesung. Object Km A ne M P.-Kr. 0° ны P.-Kr.180° |t+7 - der Aufnahmen. Mittel. т 10000 LUE 10000 10000 zum Gp Ctr. | 64.5191 63.8593 У 64.5175 |+16| 63.8585 |+ 8| о 0.0000 1—2 M 68.2591 |-+22| 60.1161 |+17| ©] + 3.7418 1—2 N 24.1250 |-+29| 104.2561 |-+10]-+19] —40.3936 5 1—2 Q 76.8857 |+17| 51.4984 |+17|— 1| +12.3636 ‘9 187° 55° 1—2 Е 26.5817 |-+30| 101.7974 |+10|+-20| —37.9348 1—2 У 62.9934 |-+14| 65.3836 |-21 0] — 1.5254 1—2 W | 64.1115 |+25| 64.2710 |+24| ©] — 0.4096 1—2 2% ay | 68.8080 |+14| 59.6070 |-+14 + 4.2706 ас | 69.2155 |+14] 59.1920 |+10 + 4.6820 + 4.6849 9 25 10 2 а, | 69.6340 |-+17| 58.7710 |-то + 5.1020 YCyw | 68.8260 |+13| 59.5720 |+14 + 4.2970 er 69.2260 |+13| 59.1835 |+10 — 4.6915 + 4.6923 28 45 ii Co 69.6235 |+-16| 58.7875 [+10 — 5.0884 gE 287 49° % dy | 68.8580 |-=13| 59.5400 |+15 + 4.3290 de | 69.2580 |+13| 59.1490 |+11 + 4.7247 + 4.7283 SON 1 dy | 69.6650 |+16| 58.7435 |-+11 + 5.1311 %€ | 68.7710 |+14| 59.6290 |-+-15 —+ 4.2410 ес 69.1825 |+14| 59.2320 |-HII + 4.6455 + 4.6452 JUNE 1—2 ео 69.5855 |+17| 58.8280 |+11 + 5.0492 Trabant — Jupiterscentrum. Tt—Ly | Mittel. | Гео) Ju 72) Ph. | Au. cos à mm mm Та | 68.6460 |+14| 59.7400 |+14 + 4.1181| —0.5668 1—2 с | 68.6370 |+13| 59.7525 |-14 - 4.1123] —0.5800| __ ей , r N |2. a | 68.6640 |[æ13| 59.7210 |-rıs + A.1415| —0.5868 0.5816 0:5777 | -+o.ooor | —0.0019 | —0:5795 | 5 e 68.5755 |+13| 59.8110 |-+15 + 4.0522] —0.5930 3 Па 67.0550 |+ 9] 61.3295 |--10 — 2.5328| —2.1521 2 с | 67.0510 |-+ 8| 61.3340 |+10 + 2.5285] —2.1638| __ LE 1—2 а | 67.0860 |+ 8| 61.3030 [+11 + 2,5614| —2.1669 2.1636| —2.1489 | -+0.000$ | —0.0019| —2.1508 | 5_3 e 66.9965 |-+ 8| 61.3895 |+11 — 2.4734] —2.1718 2 Ша | 66.0985 |+11| 62.2865 |+ 9 + 1.5762] —3.1087 2 с | 66.1140 |+-10| 62.2695 |+ 9 + 1.5924] —3.0999 + 1—2 а | 66.1570 |+10| 62.2305 |+10 + 1.6334] —3.0949 —3.0999,|ı 773-9789|,4-0.0009 | 76-0019 3.0799 | 5 e | 66.0730 |+10| 62.3150 |+10 + 1.5491| —3.0961 1—2 IV a | 71.9690 |-+12| 56.4190 |— I + 7.4458| 2.7609 2 с 71.9855 |--11| 56.4060 |— I + 7.4604| -+2.7681 1—2 a | 72.0250 I-rı1l 36.3650 а = 7.5006] -+-2.7723 2.7678 | 2.7491 | —0.0006 | —0.0019 | 2,1466 | ; е 71.9410 |+12| 56.4520 о + 7.4152] 2.7700 2 Scheinbare Adiff: M—Centrum = + 3'9700 Ло = 9.99320 —i°, = -+0.00056 №М— » = —42.7093 k р Q— » —+13.0272 fa = 0.99291 —iy = -0.00053 X 1x =— 18 Е— » — — 40.0087 Ве. = --0.00003 V— » — — 1.6187 Те» =+ 52 W— = — 0.4140 fu = 0.99320 J, = —0.00108 h 134 Bilder. eihe. | À u wu 1 mm 63.6793 63.6785 74.2491 74.7689 46.6520 46.6450 51.8359 102.1706 67.2005 66.8120 66.4260 63.7735 63.4045 63.0335 62.0060 61.6310 61.2570 60.3190 59.9400 59.5650 Я + #5 66.9230 63.5200 61.7450 69.0580 67.3040 63.8995 62.1255 60.4360 67.6220 _ 64.2135 62.4395 60.7460 66.2635 62.8580 | 61.0780 _ 59-3870 | | || | | | ] | | N un AN ON Te N P.-Kr.90° mm 10000 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. mm 64,7011 64.6995 54.1283 53.6179 81.7352 81.7339 76.5429 26.2118 61.2080 61.6000 61.9860 64.6300 65.0050 65.3730 66.4120 66.7750 67.1490 68.0920 68.4700 68.8460 61.4700 64.8730 66.6480 68.3350 61.0860 64.4620 66.2660 67.9555 60.7655 64.1745 65.9510 67.6420 62.1285 65.5390 67.3150 69.0950 tt P.-Kr.270°|:+% mm mm 10000] 10000 +-24|—16 +12 ыы ТТ +18 +18 +18 +10) +10 +10 +20 +20 RES: Scheinbare Decldif: Z{—Centrum N— »› Q— » K— » У— » W— » 1896. März 11. mm 0.0000 3.2373 0.1660 1.9406 3.6278 3.6198 0.2146 1.5594 3.2491 3.9395 0.5304 1.2450 2.9376 2.5784 0.8297 2.6076 4.2983 Be ANIME Faute. PAL A = -+10'5025 —10.9498 — 16.9337 —16.9692 — 11.7660 +38.2317 dy = 20° 59:7 Decl. #12 0% “x? 2 Tu — 198 sin 1’ y— > tù sin I’ mm mm тт 0.0000 0.0000 — 0.0007 == 10.5710 — 0.0856 —=11.0006 — 0.0078 — 17.0380 — 0.0737 — 17.1060 — 0.0001 — 11.8425 0.0000 —=38.4877 + 3.1182 — 0.2889 — 2.0627 3.1533 Trabant — Jupiterscentrum. vx | Mittel. \Nawva)|st@r—ez) ваза] Ph | mm mm —+0.1191 —=0.1229 0,1221 —+0.1255 -+0.1224 | +0!1216 | -+0!0003 —-0:0003 —0.5016 —50.5035 0.5033 —0.5042 —0.5032 | -+0.4999 | -#0,0012 0.0008 40.8213 —0.8193 —0.8177 —+0.8157 —0.5398 —0.5408 —0.5449 0.5450 —0.8185 | +0.8131 | +0.0017 0,0011 —0.5426 —0.5390 | —0.0015 —0.0019 F°5 = 0.99341 fs =0.99292 is f's = 0.99340 $75 = —0.00056 = —0.00062 Js = — 0.00054 pa 5 = —2!1 109 Bemerkungen zur Aufnahme. Bilder 2—3. Bilder 3, Ai -+0!ooor | -+0:1223 —+0.0001 | -+0,5020 +-0.0001 |. +0,8160 —=0.0001 | —0,5423 14* 110 Е. RENz, 53 1$. 1896. März 11. AR 135 Scalenablesung. Pulkowaer Sternzeit Objeenj ma Е И 2 ВЫ Иа re TA ee БЕ Nes Bilder. P.-Kr. 0° | 2. P.-Kr. 1800| 1-+% 3 der Aufnahmen. Mittel. Anhaltstierne| wie 53 А, mm mm mm 10000 10000] 10000 mm mm mm mm 2fw | 59.3910 |-+11| 69.0100 |-+14 — 5.1396 5 DORE Je 59.8070 |+15| 68.5975 |+-14 — 4.7251 — 4.7248 9 46 20 2—3 To 60.2250 |+15| 68.1840 |+19 — 4.3096 %9% | 59.4395 |+11]) 68.9645 |+13 — 5.0925 de 59.8520 |-+15| 68.5505 |-+13 — 4.6790 — 4.6817 д 142 1—2 Io 60.2580 |+15| 68.1450 |+18 — 4.2736 9 48” 17° ZR | 59.3910 |+10| 69.0090 |+13 — 5.1390 he 59.7930 |+14| 68.6140 |-+13 — 4.7404 — 4.7358 49 2 1—2 ho 60.2050 |+14| 68.2010 |+18 — 4.3281 PE 59.3985 |H-10| 69.0030 |+14 5.1324 ig 59.8055 |-+14| 68.6100 |+14 — 4.7322 — 4.7324 395 2 ОИ 60.1980 |-+14| 68.2030 |+19 — Trabant — Jupiterscentrum. Л’, (ya) Ph. | Aa cos à u | Mittel. mm mm 5.3878| — 0.6630 г —0.6738 р р р À oo ES —0.6734| —0'6688 0.0000 | —0:0019 | —0:6707 5.4150] —0.6826 6.9355] —2.2107 6.9012| —2.2195 6.9542] —2.2184 6.9565] —2.2241 7.7772] — 3.0524 а OR — 3.0477 | — 3.0271 0.0000 | —0.0019 | — 3.0290 7.7760| —3.0436 1.9169] -+2.8079 | ©) 59.1700 |-+11| 69.2210 |+13 59.1150 |+10| 69.2745 |+13 59.ттто |+10| 69.2810 |-+13 Q D D ND If | 59.1355 [+11] 69.2510 |+14 9 h à If | 57.5890 I+ 6| 70.7995 [+13 9 | 57.6230 | 6| 70.7650 |+12 h 57.5700 + 5| 70.8180 |-+12 1 57.5680 |+ $| 70.8205 |+12 EE —2.2182 | —2,2032 0.0000 | —0.0019| —2,2051 PART | II | 56.7450 |-+11| 71.6395 |-+12 9 | 56.7930 |--11| 71.5970 |-+11 h | 56.7410 |109] 71.6420 |+11 0 56.7460 | 9| 71.6380 |+11 IV f | 62.6075 +10] 65.7815 |+10 ПГТ | © D O9 © Pen © D ND D O2 © 9 | 62.1505 |+10| 65.73 +10 — 1.8744] +-2.8073 a о ВЕ о. м и 2.8125 | -+2.7936 0.0000 | —0.0019 | +2,7917| 5 _ 3 © | 62.6125 |+ 9| 65.7805 [+11 — 1.9140] 2.8184 Scheinbare Жан wie 53 A. fra = 995320 —i°, = +0.00056 Ло = 0.99291 —iy = 0.00053 X = -—- 18 Refr. = + 4 Try = — 52 Г’, = 0.99322 Ju = 0.00005 еше. ct. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. P.-Kr.90° | НН P.-Kr. 2700| tk 1 Anbaltst erne mm |. 68.7940 |-+14 _| 68.4050 |-+19 «| 68.0100 |+19 ‚| 67.0725 1 66.6910 |+ 9 66.3020 |-HI1 ‚| 65.4530 |+17 _| 65.0670 |+17 64.6845 |+17 63.6610 |+ 9 63.2820 |+10 62.9100 |+10 68.5370 |+15 66.8285 |+10 | 65.2060 |+18 р 63.4260 |-+11 68.9130 |-+15 67.2020 |+10 65.5820 |-+18 63.8000 |+10 69.2010 |+16 67.4865 |+21 65.8670 |+13 64.0870 |+11 | 67.8355 |+19 “| 66.1250 |-+11 | 64.5010 |+17 | 62.7195 +10 wie 53 A, mm 59.6190 60.0050 60.4010 61.3390 61.7220 62.1010 62.9570 63.3375 3.7185 64.7500 65.1260 65.4950 59.85 30 61.5650 63.1810 64.9630 59.4760 61.1890 62.8075 64.5900 59.1830 60.8990 62.5210 64.3030 60.5580 62.2685 63.8910 65.6745 — Scheinbare Decldiff. wie mm 1896. März 11. Decl. mm 10000] 10000 EIS ах тт 5.0984 4.7111 4.3156 3.3776 2.9954 2.6114 1.7592 1.3760 0.9943 0.0340 0.4114 0.7770 УЕ +44 ЕЕ пн с+%; о тт + 4.7084 —+ 2.9948 —+ 1.3765 — 0.4075 x? SEP 7 — 5 6g0 sin 1 x? os ’ y— 5 1903ш1 Bemerkungen zur Aufnahme, 4.8529 3.1426 1.5238 0.2579 5.2296 3.5174 1.8986 0.1156 | +++ 5.5201 3.8051 2.1840 0.4030 4.1501 2.4392 0.8164 0.9666 УЕ #444 ++ +4 dy = +20° 59'7 У: — Ух | Mittel. 2 | Табе) иеаль Ph. | mm +-0.1445 +-0.1478 0.1473 0.1496 0.5212 -+0.5226 0.5221 0.5231 —0.8117 —0.8103 —=0.8075 —0.8105 —0,5583 —0.5556 —0.5601 —0.5591 mm —0.1473 -+0.5222 -+-0.8100 —0.5583 19 = 0.99341 fs = 0.99292 fs = 0.99342 Trabant — Jupite +0/1463 | —0!0003 —+0.5188 | 0.0011 —0.8047 0.0016 —0.5546 | —0.0015 1°$ = —0.00056 is =— 0.00062 Js = —0.00052 rscentrum, —0/0004 | -+0.0001 —0.0015 | +-0/0001 —0.0022 | +0.0001 —+-0.0010 | -+0.0001 Хх 15 = —2'1 AÔ +-0:1463 —+0,5185 +0,8042 112 54 A. Scalenablesung. Object. $ P.-Kr. 0° |t+-k%| P.-Kr.180° |t+-% mm mm mm m 10000] mm 10000] 10000 Ctr, | 62.9144 65,4768 5 62.9135 [+ 9| 65.4751 |+17| oO M Durch elin Jlupitersbild |verd)eckt. N 23.7469 |+26| 104.6379 |+ 7|+17 Q 76.5527 |+21| 51.8337 |[+21|— 3 В 26.2460 |+-36| 102.1308 |-14|+-20 14 62.6504 |+18| 65.7275 |-+17 о т 63.6846 |+20| 64.6945 |+ 31 Ге) Zap | 67.1885 |+ 9| 61.2150 |+-I0 de 67.5985 |+19| 60.8120 |+10 ao 67.9905 |+-19| 60.3990 |+-14 %byp | 67.2055 | 8| 61.1860 |+10 be 67.5985 |-+18| 60.7990 |+10 b, 68.0035 |+-18| 60.4000 |+14 Z Co 67.2430 | 8| 61.1630 |+11 Ce 67.6440 |-+18| 60.7675 |+I1 о 68.0320 |-+18| 60.3580 |+15 % ед 67.2240 | 8| 61.1760 |+11 ес 67.6245 |-+18| 50.7775 |1 ео 68.0225 |-+18| 60.3730 |+-15 Та | 69.0950 |-+14| 59.2940 |+10 b | 69.1080 |-+13| 59.2820 |--10 с | 69.1335 |-+13| 59.2595 |+ е 69.1190 |+13| 59.2690 |-+12 Il Verfinstlert. Ша | 64.7165 |-+17| 63.6730 |+ 8 b | 64.7290 |-+16| 63.6610 |+ 8 ce 64.7545 |-+16| 63.6340 |- 9 е | 64.7400 |-+16! 63.6455 |+ 9 IV а | 74.9170 |--11| 53.4700 |+ 7 6 | 74.9260 |+10| 53.4555 | 8 с 74.9580 |+10| 53.4300 |+ 9 е | 74.9465 |+11| 53.4390 |+ 9 г Scheinbare Adiff: N—Centrum Е. Renz, 1896. März 16. Pulkowaer Sternzeit x Zwtr2cet%o р der Aufnahmen. | Mittel. mm mm 0.0000 3 —39.1616 - К 3 +13.6404 9° 427 30 3 — 36.6581 3 — 0.2573 2—3 + 0.7757 2—3 + 4.2679 , + 4.6749 + 4.6733 9 Ед PE: — 5.0772 —+ 4.2908 2 + 4.6814 + 4.6851 SAS) 9" 33” 49° 3—-4 + 5.0832 — 4.3210 + 4.7198 + 4.7197 33 54 It + 5.1184 + 4.3050 + 4.7050 + 4.7054 36 10 2—3 + 5.1061 Trabant — Jupiterscentrum. en | Mittel. | Foul) Лии) Ph. | Au cos mm mm — 6,1819| +1.5086 2—3 rs г м. -+1.5044 | -+1.4942 | —olooıo | —0'0021 | +-1'4911 3 + 6.2062| -+-1.5008 3 —= 1.8034| — 2.8699 3 13 di. En —2.8735 | —2.8540 | -+0.0017 | —0.0021 | — 2,8544 ak —+ 1.8288| —2.8766 2—3 —=12.0049] -+7.3316 3 —= 12.0166] 7.311 3 же. nr —+7.3298 | +-7.2799 | —0.0047 | —0.0021 | +7.2781| 5 12.0350] -+7.3296 3 = —41'4098 Fu = 0.99318 —1° 4, = -+0.00207 = -+14.3275 = — 38.7090 les — 0,99289 1% = -+0.00204 x = —7о = — 0.3182 Вей’. =+ 3 = + 0.8862 Ts Ar 52 Лк =0.99319 Ja = —0.90259 р № 95 = 8 6.0 Bilder. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 113 | 1596. März 16. Reihe. Decl. à Hi Scalenablesung. } т Unes Е. шт, = Be Bemerkungen — |Р.-Кг.90° tt P.-Er. 270° |t+k - Lions LÉ KE ae. | | ü mın mm mm (4 | 63.5739 615150 10000] 10000 тт тт тт mm | 63.5730 |+ 9 64.8140 |-+16] 0] 0.0000 0.0000 0.0009 À Durch elin Jlupitersbild |verdleckt. Li 61.3340 |+10|— 1|+ 3.4808 0.0805 + 3.4003 ) | 89.3733 + 5| —24.5567 — 0.0094 — 24.5661 Bilder 4—5 ea | 89.4476 |-+ 9|-+12| —24.6346 0.0689 —24.7035 le | 84.2035 |— 7|-+ 2] —19.3892 0.0000 —19.3892 33.8740 |+-20|— 8] +30.9412 0.0000 —+30.9412 61.3190 + 3.5027 7 61.7045 + 3.1220 — 3.1230 s 62.0755 + 2.7444 + п | 65.3445 |+16| 63.0590 + 1.7639 е | 64.9795 |+16| 63.4360 + 1.3929 == 1.3939 ‚ | 64.6065 |+16| 63.7990 + 1.0250 , 63.5400 |+ 9| 64.8580 — 0.0386 се | 63.1740 |-+ 9| 65.2290 — 0.4070 — 0.4075 м 62.8035 |-+ 9] 65.5985 — 0.7768 h | 60.1320 |-+14| 68.2650 — 3.4459 с | 59.7550 |-14| 68.6480 — 3.8256 — 3.8230 E 59.3810 |-10| 69.0170 — 4.1974 | - Trabant — Jupiterscentrum. | Yt—Y2 | Mittel. и "slye—Y2) | 75 (@1—22) Неа Ph. 5 тт тт а | НЫ +11 gan ER + 2.7411| —0.3819 ` 4.5900 |-+17| 63.8030 |+10 + 1.01 — 0.3792 , dr ' р ' c | 62.7895 |+10| 65.6030 |+12 — SFR me —0.3795 | —0:3770 | —0:0029 —0:0010 | +0o!oooı | —0:3808 е | 59.3740 |11| 69.0180 |+15 — 4.2014] —0.3784 | | Verfinstlert. |. 67.3390 Er +10 + 3.7658| -+0.6428 -6130 2.7760 | 2.0 .646 ” | о ор Fe 28 + Tor +-0.6446 | -+0.6404 | +0.0055 | -+0.0010 | --0.0001 | 0,6470 | 60.3965 67.9910 |+18 — 3.1766| -+0.6464 рот 63:494p +13 + 1.3250] —1.7980 3.1780 .21 о — 0.3978] —1.791 61.3750 6.01 13 2 Zar Be. —1.7936 | —1.7818 | —0.0142 —0.0069 | +-0.0001 | —1,8025 57.9610 70.4295 |-+20 — 5.6140] — 1.7910 4 Scheinbare Decldif: et = Be 198 = 0.99344 195 =—0.00195 ‘ Е » =- 24.4683 fs =0.99294 is =— 0.00202 x is = —6!9 У » = —19.2652 W—- » = +30,7328 f's = 0.99343 Js = —0.00193 | Зап. Физ.-Мат, Отд. ^ dy = 21° 1/8 114 F. Renz, | 54 В. 1896. März 16. } AR 13H: Scalenablesung. À Pulkowaer Sternzeit | Object. ыы 3! Es en | à x DER ET EEE re Е Bilder. P.-Kr. 0° +51] P.-Kr.180° ЕЁ ? der Aufnahmen. Mittel. | Anhaltstierne| wie 54 A, mm mm mm 10000 10000] 10000 mm mm mm mm % fo | 57.7685 |+ 6| 70.6210 |+-12 — 5.1454 RE Je 58.1715 |+ 6| 70.2220 |+-16 — 4.7446 — 4.7413 OA О 4 To 58.5870 + 6| 69.8160 |+16 — 4.3338 %9щ | 57.8170 |+ 6| 70.5810 |+12 — 5.1011 de 58.2115 |+ 6| 70.1920 |+16 — 4.7096 — 4.7102 о 3 90 | 58-5960 |+ 6| 69.7975 |+16 — 4:3200 9" 48” gg %й | 57.7890 | + 6| 70.6005 |+12 — 5.1248 he | 58.2005 |+ 6| 70.2020 |-+16 — 4.7196 Е тот 1 49 5 9 ho 58.6080 |+ 6| 69.7955 |+16 — 4.3130 %iw | 57.8160 [+ 5| 70.5810 |+13 — 5.1017 ie | 58.2060 |+ 5| 70.1940 |+-17 TA — 4.7137 49 55 2—3 о 58.5910 | 5| 69.8040 |+17 — 4.3259 Trabant — Jupiterscentrum. ee | Mittel, Хата) Лиз) Ph. | Aa с035 mm mm If | 59.6340 |+ı5| 68.7540 |+13 — 3.2787| +1.4626 - | 9 | 59.6580 +15] 68.7310 |+13 — 3.2552] 1.4550 v a+ ALT , | Bl le alu ns: +-1.4587 | <+1/4488 0:0006 0!0021 | +-1/1461 3 | р 59.6570 +14| 68.7300 |+14 — 3.2553] 1.4584 3 Il II Verfinstlert. | | ШУ | 55.2695 |+ ı| 73.1150 [+14 — 7.6422| —2,9009 21" | 9 | 55.2925 | ©] 73.0910 |+13 — 7.6187| —2.9085 | _ У Le ce | о о о. о. 2.9041 2.8844 | 0.0010 0.0021 2.8855 3 | î 55.2950 |— 1| 73.0970 |+13 — 7.6205] —2.9068 3 | IV f | 65.4905 |+11| 62.8990 |+ 9 9 | 65.5120 |10| 62.8780 |+ 9 h | 65.5120 -+10| 62.8765 |+10 i | 65.5120 |+10| 62.8790 |+-10 Scheinbare Adiff. wie 54 A. 2.5770] +7.3183 3 unterexponier|}} m р: ne +7.3140| -+7.2643 | —0.0028 | —0.0021 | +7,2594 3 À + 2.5977| +7.3114 3 » | | De 0:99:08 —®, = +0.00207 fu =0.99289 —ù, —-+000204 X à, = —7'0 Refr. = + 4 Do == — 52 Fa =099820 I, = -+0.00156 teihe. с î Scalenablesung. P.-Kr.90° 2. P.-Kr.270° Anhaltst|erne mm 68.0570 68.2770 67.8950 66.3700 66.5080 66.1400 65.1325 64.7680 64.3950 63.4550 63.0975 62.7400 67.8990 66.1300 64.3930 62.7250 +20 +12 +10 FA D Verfinstlert. 68.9220 67.1570 65.4150 63.7520 66.4830 64.7035 ` 62.9620 | 61.3020 Scheinbare Decldiff. wie +16 +11 +19 +11 +10 +16 19 +10 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. wie 54 À, mm 59.7449 60.1300 60.5070 61.5300 61.9040 62.2610 63.2650 63.6465 64.0105 64.9435 65.3130 65.6615 60.4940 62.2630 64.0045 65.6710 59.4670 61.2340 62.9755 64.6405 61.9215 63.6920 65.4340 67.0955 1396. März 16. 115 Decl. "2,252 2 =. 2 А Bemerkungen у И = = 196 sin 1’ 4 > 290 sin 1 zur Aufnahme) t-+k mm mm 1000012000) Ex Bilder 3—4. +15 + 5.0774 +15 + 4.6946 + 4.6957 | 15 — 4.3151 —=1о —+ 3.2908 +10 —+ 2.9228 + 2.9237 +10 + 2.5604 +10 = 1.5550 + 9 + 1.1820 + 1.1835 + 9 + 0.8136 +17 — 0.1237 +17 — 0.4872 — 0.4836 +11 — 0.8399 Trabant — Jupiterscentrum. vx | Mittel. faune) В. | 4 тт тт 1 + 4.3238| — 0.3719 ; / — 0,3693 р ’ ! r у р я = Be or —0.3695 | —0:3671 | —0.0028 | —0'0006 | +olooor | —0:3692 и — 0.8522| —0.3686 +13 + 5.3485] +0.6528 ме ыы ИЯ a +0.073 +-0.6529 | -+0.0056 | —0.0020 | -+0.0001: | +0.6566 +19 —+ 0.1762] -+0.6598 +10 —+ 2.9016] —1.7941 + 1.1270] —1.796 en ES SAT we: —1.7955 | —1.7838 | —0.0140 | -+0.0008 | +o.ooor | — 1,7969 + 9 — 2.2758] —1.7922 ©? y=-r21° 1.8 Л°5 = 0.99344 fs = 0.99294 f's = 0.99344 о 2; = —0.00195 is =— 0.00202 Ту = —0.00192 x ig = —69 116 Е. REnwz, 55 A. 1896. März 24. № 138) Scalenablesung. . Pulkowaer Sternzeit | Object. a $ & Fa Bilder. " P.-Kr. 0° |+ Р.-Кг.180° |t-+%k der Aufnahmen. Mittel. mm mm 10000 mm mm mm Ctr. | 63.6970 64.6914 X | 63.6962 |+ | 64.6897 3 M 71.3508 |+22| 57.0360 — 1|[+ 7.6548 2—3 N 27.2073 |-30| 101.1826 — 36.4878 I STARS 3—4 Q 79.9674 |+25| 48.4190 —+-16.2700 10° 15.72 4 у R 29.6474 |+35| 98.7265 — 34.0394 3—4 ellipt. У 66.0731 |+27| 62.3091 + 3 W | 67.2035 |+11| 61.1833 + 2—3 Фа, | 66.8265 |+ 9| 61.5655 —= а; | 67.1990 |+ 9| 61.2050 + + 3.4962 9 49 54 1 а, | 67.5685 |-+19| 60.8305 — % by | 66.7855 |+ 8| 61.6145 — b. | 67.1665 |+ 8| 61.2380 + + 3.4593 Gin 12 1—2 bo | 67.5395 |+-18| 60.8670 = ’ gr 51” 47° %Cyw | 66.7870 |+ 8| 61.6110 + Ce 67.1625 | 8| 61.2430 + —= 3.4609 S2 20 | 2 Co 67.5435 |4-18| 60.8570 + y % dy | 66.8000 |+ 8| 61.5990 + : lé | 67.1700: | 8| 61.2330 |+11 + —+ 3.4653 3024 1—2 do | 67.5335 |+18| 60.8630 |+11 + Trabant — Jupiterscentrum. Lt —&y | Mittel. F'uer—22) Лигу Ph, | Av cos à mm mm Та 65.9080 |+11| 62.4845 |+ 9 + 2.2090| —1.2872 2 à b 65.8750 |+-10| 62.5180 |+ 9 2 7001-2036) er ' Eu _ 47 2— с | 65.8830 [4-10 | 62.5100 [+9 + 2.1838] —1.2771 1.2810 1.2721 | +-0.0001 0.0024 12744 3 d | 65.8885 |+10| 62.5045 |+10 + 2.1892| —1.2761 3 Па | 70.2805 |+17| 58.1055 |+ 5 + 6.5853| 3.0891 2 4 6 | 70.2420 |+16| 58.1480 |+ 5 — 6.5448] -+3.0855 EG JE 2— eh | 7012465 [16| | 81440 |6 DE ool 3,088 —+3.0872| -+3.0658 0.0002 0.0024 | 3.063? | 5 d | 70.2475 |+16| 54.1405 |- 6 + 6.5512) +3.0859 N 2 ИГа | 62.3525 |-10| 66.0365 |+10 — 1.3448| —4.8410 2—3 b 62,3125 |+10| 66.0765 |+10 — 1.3848| —4.8441| _ Ir E se 2—3 я 62,3135 [+ 9| 66.0730 |-rıo — 1.3826| —4.8435 4.8448 4.8110 | —-0.0002 0.0024 4,8132 3 а | 62.3100 |+ 9| 66.0750 |+11 — 1.3854| —4.8507 2—3 Ina 59.4525 |+11| 68.9360 |+13 — 4.2446| —7.7408 : 2—3 59.4195 [+11] 68.9715 |+13 — 4.2789] —7.7382 | — or — pese | 2—8 С 59.4255 |+10| 68.9670 |+13 — 4.2737| —7.7346 7.7374 7.0836 | 0,004 I 7.6856 3 unterexponiel d | 59.4280 |+10| 68.9630 |+14 — 4.2705| —7.7358 2—3 Scheinbare Ædiff: M— Centrum = + 8/0993 F° 4 = 0.99303 —i°, = —0.00010 N— » — —38.5810 Q— » —= 17.1563 fa = 0.99273 —iy =-— 0.00014 хи =- 05 E— » = —35.8802 МЕЛ: =— 4 — » —= — 2.5107 Те» =+ 3 W— » = + 3.7150 f'a = 0.99304 Л. = 0.00071 „hm AY = 8 5.6 veihe. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. $ Scalenablesung. et $ P.-Kr. 90°|t-HR|P.-Kr. 270° ++ mm mm _mm m 10000! mm 10000] 10000 60,5665 67,5285 60.8655 |+10| 67.5270 |-+18| о ” | 45.7124 |-+15| 82.6792 |+ 5$] 1 I 46.2461 |+30| 82.1478 |-+17|- 7 | 18.0998 |+31| 110.2971 |+ 8-12 18.1055 |+37| 101.2713 |+19|+21 23.2886 |+24| 105.1010 |+ 8]+14 M 73.6369 |+12| 54.7589 o о | 66.5655 |+ 8| 61.8430 |--10 I 66.2225 |+10| 62.1925 |+10 ‚ | 65.8720 |+10| 62.5385 |+10 64.7993 |+16| 63.6090 | 9 64.4490 |+ 8 63.9630 |+ 9 64.0910 |+ 8| 64.3155 |+ 9 63.1030 |+ 9| 65.3020 |-+-17 62.7545 |+ 9 65.6550 |+-11 62.3970 |+ 9 66.0115 |+11 61.3490 |+10| 67.0550 |+ 9 61.0050 |+10| 67.4100 |+ 9 60.6580 |+-10| 67.7510 |+19 66.5450 |+ 8| 61.8530 |+10 64.7710 |+16| 63.6250 |+ 9 63.0750 |-+9| 65.2325 |+17 61.3250 |+10 67.0705 |+ 9 65.4320 |-+17| 62.9630 |+11 63.6595 |+ 9] 64.7345 |+18 61.9670 |-=т0! 66.4270 |-+12 60.2165 |+15| 68.1750 |-+20 7.3875 |+ 9| 61.0050 |+10 65.6120 |+11| 62.7780 |+ 9 63.9190 |+ 9 64.4740 |+16 | 62.1675 |+10 66.2220 |+10 68.1035 a 60.2910 |+-1$]. 66.3330 |+12) 62.0640 |+10 61.6365 |+18 63.7610 |+ 9 62.8865 |+11| 65.5160 |+11 Scheinbare Decldif: M— Centrum N— » = R— » У— » W— » 8% 1596. März 24. Decl. À nr 2 2 2 Bemerkungen q п с 5 x Se Zu : ’ я 3 ие г У— +8 sin 1 zur Aufnahme, mm mm mm mm 0.0000 0.0000 0.0000 — 15.1516 — 0.0031 — 15.1547 — 14.6184 — 0.0704 — 14.6888 — 42.7652 — 0.0136 — 42.7788 Bilder 2. Mond sehr — 42.7488 — 0,0596 — 42.8084 nahe. Cirri. — 37.5728 — 0.0003 — 37.5731 —+-12.7708 — 0.0007 —+-12.7701 = 5.692 | + 5.3462 + 5.3455 + 4.9979 + 3.9265 + 3.5741 + 3.5731 + 3.2188 + 2.2312 + 1.8808 + 1.8803 + 1.5288 + 0.4782 + 0.1291 + 0.1305 — 02158 Trabant — Jupiterscentrum. à п Ye Y2 Mittel. fa (уг 92) | То (ая) |-вг-2) Ph. 48 2 mm mm + 5.6770] <+0.3315 0.331 r r r 1 Ь x Bes Be —+0.3281 | +0:3259 | —0.0003 +0:0004 | -+0'0002 | —+0,3262 + 0.4584] 2.3279 + 4.5660| —0.7795 + 2,7932] —0.77 ! Fa “HA DO —0.7794 | —0.7740 | -+0.0007 | —0.0017 | -+0.0002 | —0:7748 — 0.6484| —0.7789 + 6.5214] -+1.1759 Be ie Be —1.1744 | +1.1664 | —0.0011 -+0.0006 | -+0.0002 | —1,1661 + 1.3039] 1.1734 + 7.2376] 1.8921 = 453 el +1.8907 | 1.8777 | —0.0019 —0.0003 | -+0.0002 | -+1,8757 + 2.0194| —+-1.8889 = = 1,9490 195 = 0.993 15 12$ = +-0.00024 = — 14.60! == —42.4855 fs = 0.99264 is = 0.00014 x щ=- 0.5 — — 42.5208 = — 37.3178 fs = 0.99314 I; = 0.00025 = -+12.6808 = -+21° 3.0 re se -ч -+ res 4 bd Len | nl = SSH = о Scheinbare В. wie 55 A. DB. Scalenablesung. P.-Kr. 0° |t-+k| P.-Kr. 180° Anhaltstierne| wie 55 А, mm 10000 mm mm 57.4240 | 5| 70.9795 57.7980 |+ 5| 70.6050 58.1720 |+ 5| 70.2325 57.4320 | 5| 70.9740 57.8050 | 5| 70.6030 58.1775 |+ 5| 70.2260 57.4220 |+ 5| 70.9850 57.7870 | 5| 70.6195 58.1570 | 5| 70.2470 57.3965 + 6| 71.0075 57.7600 |-+ 6| 70.6500 58.1225 |+ 6| 70.2830 56.5855 [+ 9| 71.8080 56.5860 + 9| 71.8055 56.5800 |+ 9| 71.8130 56.5545 +10] 71.8340 60.8680 |+10| 67.5180 60.8670 |+10| 67.5200 60.8550 |+10| 67.5320 60.8260 |+11| 67.5635 52.9315 |+ 8| 75.4565 52.9320 |+ 7| 75.4570 52.9210 |+ 7| 75.4680 52.8910 |+ 7| 75.5025 50.0760 |+ 6| 78.3165 50.0800 |+ 6| 78.3150 50.0685 |-+ 6| 78.3260 50.0420 |+ 6| 78.3500 t+-k mm 10000 mm 6.2809 5.9066 5.5336 6.2742 5.9022 — 5.5276 6.2847 5.9194 5.5484 6.3086 5.9482 5.5836 7.1142 7.1126 7.1194 7.1426 2.8282 2.8298 2.8418 2.8720 — 10.7765 — 10.8088 — 13.6232 —13.6204 —13.6317 —13.6570| — 7.7102 Е. Renz, 1396. März 24. h m VX = 8 5.6 Pulkowaer Sternzeit è der Aufnahmen. Mittel. mm h m 5 — 599% то щиту 59015 Ta EA 10° 12” 43° ee [rl 13 9 — 5.9468 IA то Trabant — Jupiterscentrum. van | Mittel. Рабина Л» из) Ph. | Au cos à mon mm — 1.2072 — 1,2113 р р р — 1.2019 — 1.2040 | —1.1956 | —0.0002 | —0.0024 —1.1958 3.0788 Be —3.0752 | -+3.0539 | -+0.0007 | —0.0024 —+3.0748 zu — 4.8641 ER —4.8609 | —4.8271 | —0.0010 | — 0.0024 — 4.8620 — 7.7162 mire —7.7149 | —7.6613 | —0.0016 | —0.0024 ЛЗ. = 0.99303 —®. — — 000010 fx = 0.99273 —iy, = —0.00014 X y = 05 Ве. = 6 Try = 66 Г,» = 0.99305 Ju =- 0.00086 160} WW > 3 ищегехроше ll ©> ©> © DDDD ны D . Bilder. CE лев: are 2—5 unterexp. » | | » в | Е POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 119 e 1896. März 24. teihe. Decl. } Scalenablesung > T- 5. 2 2 semerkungen 00 _ 5 y Ferre — —tg8 sin 1’ Y— = $05 sin 1’ P.-Kr. 90° НН Р.-Кг. 270° + à 3 2 zur Aufnahme. Anhaltstierne| wie 55 A. mm mm mm 10000 10000] 10000 mm mm mm mm | 64.9740 |-+18| 63.4300 |+ 9 + 4.1036 | 64.6235 |+18| 63.7860 |+ 9 + 3.7504 + 3.7486 64.2640 |-+10| 64.1430 |-+ 9 + 3.3917 63.2315 |+11| 65.1690 |+-17 + 2.3621 | 62.8800 |+11| 65.5315 |+11 + 2.0054 + 2.0094 | 62.5320 |-+11| 65.8730 |+11 + 1.6606 | 61.4805 |-+12| 66.9220 |+ 9 + 0.6106 | 61.1350 |-+12| 67.2675 |+ 9 + 0.2650 + 0.2635 | 60.7885 |+12| 67.6200 |+19 — 0.0850 | 59.7970 |+16| 68.6080 |+14 — 1.0742 | | 59.4650 |-+12| 68.9520 |-+14 — 1.4124 — 1.4121 MR | EP EE 59.1235 |-+12| 69.2850 |-+14 — 1.7497 а та = -d'apitérseentenmh) Чо пою À À | — Jupiterscentrum. es Mittel. (Ps (гу) | 78 (2) |-@#-27)3| Ph | A mm ee м ИТТ | 64.9320 |-+19| 63.4610 |-+11 +- 4.0670| -+0. os | . Di: a = es 057 ot +0.3151 | +0!3129 | —0/0003 | —0'0008 | +o'ocoz | -+0:3120 | 59.7725 |-+17| 68.6305 |-+15 — 1.0978| —<+0.3143 о + 9| 64.5570 |+16 + 2.9683| —0.7803 | — | | ОНИ EE es пе Le D seb Eee —0.7814 | —0.7760 | -+0.0008 | -+0.0016 | +0.0co2 | —0,7734 | 58.6740 |-+11| 69.7220 |+16 — 2.1931] —0.7810 | | 65.7975 |-H14| 62.5915 |+14 + 4.9342| -+1.1856 | ИЯ В Fu Re ue En ен 1.1852 | +1.1771 | —0.0013 | —0.0045 | 0.0002 | -+1.1715 | 60.6365 |-+14| 67.7540 |-+23 66.5130 |-+13| 61.8850 |+1s 64.7765 |-+21| 63.6200 |+14 63.0255 |-+14| 65.3720 |-+22 61.3525 |-+15| 67.0460 |+14 5.6450] -+1.3964 3.6098] -+1.9504 a 2 г 21 | 2175| 18946 | tr 8968 | -+1.8838 0.C022 0.0084 | -+0.0002 +1,8754 0.4844| —1.8965 0.2280] 1.1841 | | ] | +++ Scheinbare Decldiff. wie 55 A. f°5 = 0.99315 5 = 0.00024 fs =0.99264 is = 0.00014 X ig = +05 f's =0,99316 Is = +0.00028 64, = -н21° 3.0 120 FRE nz: 56 A. 1596. März 29. AR Scalenablesung. Pulkowaer Sternzeit ‚Object. ’ $ 2 Zur | P.-Kr. 0° |t-+%| P.-Kr. 180° | t+-%k % der Aufnahmen. Mittel. | т m, IT mm = ОО TL тт тт | Ctr, | 64.2711 64,1177 4 64.2703 |+ 8| 64.1168 |+ 9 Ге) 0.0000 М 74.9525 |+13| 53.4000 |+10|— 1| 10.6996 М 30.8249 |+22| 97.5327 |+ 4|+11| —33.4286 MORE: Q 83.5684 |+ 1| 44.8737 |-+24|— 4| +19.2691 10 11 32 В 33.2581 |-+27| 95.1713 |- 4|4-10| — 31.0312 У 69.6710 |+21| 53.7439 |+15 0] + 5.3872 ШТ 70.8204 |-+28| 57.4565 |-+25|— 4| + 6.6050 %65 | 68.3465 |+19| 60.0600 |+14 + 4.0668 | D, 68.7300 |+14| 59.6650 |+-14 — 4.4558 + 4.4595 10 к, 0 b, 69.1310 |-+14| 59.2660 |+10 + 4.8560 %Cyw | 68.2790 |+18| 60.1315 |+-15 + 3.9972 Ce | 68.6750 |-+13| 59.7340 |+15 +- 4.3937 + 4.3941 3 9 ео 69.0700 |+13| 59.3340 |511 + 4.7914 10 3” 59° % dy | 68.3150 |+18| 60.1070 |+15 —+ 4.0274 F de | 68.7925 |+13| 59.7090 |+15 + 4.4200 + 4.4231 AO do | 69.1023 |-+13| 59.3050 |+11 + 4.8219 Zfw | 68.3010 |+19| 65.1295 |+16 + 4.0592 fe | 68.6925 |+14| 59.7370 |+16 + 4.4010 + 4.4041 6 24 fo | 69.0885 |+14| 59.3310 |-+12 +- 4.8022 Trabant — Jupiterscentrum. x —%z, | Mittel. рва) угу) Ph. | До cos à mm mm Ib | 66.8745 |+ 9| 61.5120 [+ 9 + 2.6046] —1.8549 с | 66.8105 |+ 8| 61.5815 |+ 9 + 2.5378] —1.8563 | __ ENT, Kun 28 Br d | 66.8430 |+ 8| 61.5550 |-н1то + 2.5672] —1.8559 ESA ых ея в 1.8185 У | 66.8230 |+ 9| 61.5860 |-+11 + 2.5417] —1.8624 IT b | 65.9700 |+11| 62.4195 |+ 9 + 1.6986] —2.7609 С 65.9065 |-+-10| 62.4870 |+ 9 = 910531 2.7070) к EEE (| LES + u ; И Fe oe Е oe) 2 vhs 2.7632 2.7447 0.0011 0.0026 2,7484 Х | 65.9200 |+11| 62.4920 |+ +- 1.6373| —2.7668 ШО | 71.3960 |-+12| 56.9910 |+ 9 + 7.1260 но С 71.3360 |-+12| 57.0610 |+10 + 7.0609] 2.6668 2 u Bl 713600 |121 Vertes re | М +-2.6614| —2.6436 | 0.0011 0.0026 | -+2,6421 f | 71.3380 |+13| 57.0725 |+12 + 7.0561| +2.6520 IV | 74.8970 |+10| 53.5020 |+ 3 +-10.,6212| +6.1617 e | 74.8415 |+10| 53.5625 |+ 4 +10.5631| 6.1690 + ее м я en —+6.1684 | -+6.1271 | 0.0023 0.0026 | -+6,1268 f | 74.8620 |-+12| 53.5555 |+ 6 +-10.5768| -+6.1727 | Scheinbare Вай: M— Centrum = +11!3000 18 = 0:99328 —i° „ = —0.00220 N— » — —35.3803 Q— » = -+20.3570 Ги = 0.99298 —% =— 0.00224 X и=- R— » = — 32.6795 Ве. =+ 5 У » === 5.7113 , Л» == 49 W—- » = + 6.9157 fx = 0.99330 I = — 9.00170 25 —gh de | ee à wo r [ae] 1 O2 3 3—4 3 3 2—3 3—4 3—4 3 2—3 3 3—4 3 2—5 2—3 140 | Bilder. | | | 3 unterexponiert 3 ишегехроше № | | SI 1 | | с ek: [ | POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 121 1396. März 29. teihe. Е ес]. = r à Scalenablesung. Dot 2 2 Bemerkungen et 5 y Их — 199 sin 1’ y — = t9ù sin l’ s MAÉ _ [P.-Kr.90° th P.-Kr.270° |t+x - RE ae 50 10000 zum 10000 10000 Rn 62.9138 65.4666 u sans im 62.9129 |+ 9 65.4650 |-+16| о 0.0000 0.0000 0.0000 73.7082 |-+16| 54.6409 |-+ 3|— 1| +10.8106 — 0,0060 —10.8046 74.3850 |-+24| 54.0980 |-+19|— 3| 11.4198 — 0.0592 —+-11.3606 46.0710 |-+23| 82.2561 | 7|-+ 3| —16.8150 — 0.0191 — 16.8341 46.2525 |+26| 82.2156 |-+16|- 5| — 16.7042 — 0.0495 — 16.7537 1 51.3091 |#H11) 77.0531 |+11| Cl —11.5956 — 0.0015 — 11.5971 | тот.64т9 |+ 5| 26.7289 |-+-24|—16| -+38.7304 — 0.0023 -+38.7281 65.3810 |+17| 63.0155 [+10 + 2.4595 Bilder 4—5. 650190 |-+17| 63.3835 |+-ı0 + 2.0945 —+ 2.0913 64.6420 |-+17| 63.7555 |+9 + 1.7200 “| 63.6610 |+ 9] 64.7390 |+17 + 0.7370 63.2940 |+10| 65.1010 |+17 + 0.3720 —+ 0.3674 62.9115 |+10| 65.4770 |+17 + 0.0067 61.8440 |+10| 66.5490 |+ 9 — 1.0760 61.4790 |+11| 66.9280 |+ 9 — 1.4480 — 1.4477 | 61.1020 |+11| 67.2935 |+ 9 — 1.8192 58.3825 |+ 6| 70.0100 |+17 4.5378 58.0160 |+ 6| 70.3840 [+17 Le 4.9082 — 4.9067 57-6470 |+ 6| 70.7475 |+13 == Trabant — Jupiterscentrum. Yt — У» | Mittel. ra we-va)| Ta ео) e-229 7) Ph. | AG mm mm 04625 —+16| 62.9250 |+10 + 2.5454] +0.4541 .7405 |+ 8| 64.6470 7 + 0.8227] +0. р ' ‚ ле в 1 6 ER x И a +0.4546 | 0/4516 | —o!oo43 | -+0!0007 | -+0/o002 | -+0/4482 58.4640 |+10| 69.9220 |+17 4.4530| 0.4537 » 65.6850 |-+10| 62.7065 |+10 2.7656| -+-0.6743 + 63.9620 |+ 8| 64.42 1.0446 0.6772 re russ =, EEE BR je ur oe : о | 0.6765 | +0.6720 | —0.0066 | -+0.0009 | 0.0002 | -+0,6665 58.6895 |+10| 69.7000 |+17 — 4.2292] -+2.6775 es +9 ee +11 + 1.3770] —0.7143 2.5640 |+10 .8080 |-+13 — 0.3458] —0.7132 “ vn: | 0 FR ÉD a = ne Bi: —0.7126 | —0.7079 | -+0.0063 —0.0017 | +0.0002 | —0,7031 57.2880 |+10| 71.0800 |+15 — 5.6198] —0.7131 63.6035 |-+12| 64.7620 |+20 + 0.6968] —1.3945 | 61.8800 |+13| 66.4810 |-+14 — 1.0252| — 1.3926 à 8 DES || бо.оббо |-+18| 68.2080 |-+-22 nn 2.8403] —1.3926 — 1.3943 | —1.3852 | 0.0147 —0.0052 | -+0.0002 | —1,3755 | 56.6020 |+13| 71.7630 |+15 — 6.3042] —1.3975 3 Scheinbare Decldif: M-—Centrum = -+10’7647 f°5 = 0.99346 125 = +0.00236 N— » =-+11.2118 0—- » = —16.6718 Ss = 0.99295 is = 0.00226 X = + 78 В— » = — 16.7073 У— » = —11.5042 fs = 0.99346 Л; = -+0.00233 W—- » =-+38.4915 8, = +21° 2:4 Зап. Физ.-Мат, Отд. 16 mm 10000 122 56 B. Scalenablesung. Object. P.-Kr. 0° |i+k| P.-Kr. 180° t-+%k Anbaltstierne| wie 56 A. mm mm 10000 10000 mm mm #9 | 58.8530 |+11| 69.5490 |+13 de 59.2530 |+11| 69.1460 |+13 do 59.6640 |+15| 68.7300 |+13 ZN | 58.8890 |+10| 69.5200 |+13 he 59.2790 |+10| 69.1250 |+13 ho | 59.6820 |+14| 68.7190 |+13 %Ёр | 58.9515 |+-10| 69.4630 |+14 ke 59.3395 |+10| 69.0760 |+14 ko 59.7330 I+-14| 68.6740 |+14 2 15 58.8855 |+11| 69.5395 |+14 le 59.2620 |+-11| 69.1570 |+14 lo 59.6425 |+15| 68.7730 |+14 Ig 57.3785 |+10| 71.0030 |+I2 № | 57.3980 |+-10| 70.9910 |+12 Ih 57.4545 |+ 9| 70.9430 |+13 1 57.3790 |+ 9| 71.0290 |+13 II g | 56.4650 |--10| 71.9165 |+11 h 56.4825 ор 71.9060 |+11 Г 56.5440 |+ 9| 71.8560 |-+12 1 56.4640 |+ 9| 71.9455 |+12 III ag | 61.8780 |+10| 66.5105 |- 8 h | 61.8930 |+ 9| 66.4980 |- 8 k | 61.9500 |+ 9| 66.4520 |+ 9 1 61.8680 |+10| 66.5370 |-+-10 [IV g 65.4465 |+17| 62.9435 |+ 9 № | 65.4640 |-16| 62.9305 |-+-10 k | 65.5330 |+16| 62.9725 |+-10 1 65.4525 |+17| 62.9635 |+11 Scheinbare ЖА. wie 56 A. mm 5.4248 5.0233 4.6096 5.3924 4.9998 4.5952 5.3326 4.9452 4.5472 — 5.4038 5.0244 4.6422 6.8890 6.8733 6.8212 6.9019 7.8025 7.7885 7.7328 7.8176 Are 2.3928 2.3792 2.3277 2.4112 1.1752 1.1904 1.2538 1.1681 +++ a 8! Е. Rexz, 1596. März 29. № ; 142 2 40480 Pulkowaer Sternzeit } ie der Aufnahmen. Mittel. mm — 5.0192 о” 187. ло’ 4 — 4.9958 вто de; 107 20” 17° р — 4.9417 200027 3 Mi h — 5.0235 22122 2—3 к Trabant — Jupiterscentrum. й &— то | Mittel. A) Лу») Ph. | Aa cos à mm mm 1 —1.8698 3 | — 1.877755, 8 ве Schr, Le a 3 unterexponierl — 1.8705 1.8763 1.8637 0.0012 0.0026 1:8675 34 | —1.8784 3 unterexponierif —2.7833 3 | Es —2.7903 | —2.7717 | —0.0018 | —0.0026 | —2,7761 x — 2.7941 3 2.6264 || 3 | .6166 2—3 he —+2.6173 | 2.5998 | +0.0019 | —0.0026 | +2,5991 | à —-2.6123 : 3 —+6.1944 3 à Be: 6.1919 | —6.1504 | -+0.0038 | —0.0026 | +6,1516 an u +6.1916 3 unterexponier " Е Bros, D p | Fra — 0.99328 199 = 009220 À fu =0.99298 —î, =—00022 Xu 77 1 Refr. = + 6 | Try = — 56 | Га = 0.99331 Ju = — 0.00274 | т 5-7 | | — Scheinbare Decldiff. wie ne P.-Kr. 90° mm 67.1440 66.7645 66.3830 65.5080 65.1390 64.7620 61.9815 61.6185 | 61.2470 60.2330 59-8745 59.5260 67.2240 65.5895 62.0785 60.3395 67.4505 65.8190 62.3040 60.5640 66.0440 64-4155 60.8990 | 59.1595 | 65.3440 | 63.7130 60.1940 | 584525 ++ P.-Kr.270° POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. mm 61.2750 61.6480 62.0420 62.9170 63.2850 63.6525 66.4395 66.8005 67.1690 68.1825 68.5470 68.9020 61.1860 62.8230 66.3395 68.0795 60.9620 62.5970 66.1105 67.8490 62.3515 63.9800 67.4940 69.2360 63.0410 64.6770 68.1950 69.9310 t-+k mm_| mm 10000] 10000 И +10 ЕЕ +19 Sm +10 Sat à +19 + 9 + 8 +18 —-13 +10 ЕР —19 17 56 А. 1896. März 29. Decl. mm + + -= 3.8308 LE + + + 2.2026 — — — 1.3171 — — 3.0566 a № , — 5 #90511 1 x? . y— = tgù sin 1’ Bilder 4. Bemerkungen zur Aufnahme. 123 0.4646 +0.4572 0.4631 0.4629 BE. 0.6898 +-0,.6850 0.6903 0.6902 Par —0.7080 —0.7084 —0.7043 —0.7054 [Mr — 1.4026 — 1.4086 — 1.4073 — 1.4068 Alan 9—9 | Mittel. —-0.4620 —0.6888 —0.7065 — 1.4063 725 = 0.99346 fs = 0.99295 Да = 0.99348 Trabant — Jupiterscentrum. +0:4590 | —0:0045 —0.6843 | —0.0067 —0.7018 +-0.0063 — 1.3971 | -+0.0149 1° 5 = -+0.00236 is = 0.00226 Js = +0,00241 Уве) 78 (аз) ее) т Ph. | —0/0012 | +0/0002 —0.0020 | +0,0002 -+0.00II | -+0.0002 —0.0013 | +0.0002 — + 0/4535 —+-0.6 + ot [92] —0.6942 —1.3807 124 Е. Renz, | 57 A. 1296. März 30. 142 | al Scalenablesung. Pulkowaer Sternzeit | ОБА. Шо. и eh Bilder. | P.-Kr. 0° 1-1 P.-Kr.190° t+k der | der Alnahmen: Lite Mittel. | 50 10000 er 110006] 10000 10000 mm Ctr. | 62,9323 65.4446 U 62.9314 | 9| 65.4429 |+17 0.0000 12 M 66.6790 |11| 61.6940 |-H12 4 + 3.7486 2 EN 22.5495 |-+28| 105.8289 |+-10|--20| —40.3806 h 5 1—2 Q 75.2936 |+18| 53.0918 |-+13|— 1| +12.3572 10° 1287 25. 2 R 24.9867 |+-33| 103.3895 |-+I1 2 — 37.9424 1—2 7 61.3991 |+15| 66.9759 |-+13 — 1.5322 1—2 W | 62.5412 |+25| 65.8375 |+-26 — 0.3920 2 Фа | 70.3925 |+17| 57.9870 |+ 1 + 7.4595 Ge 70.8030 |-+13| 57.5980 |- 5 + 7.8590 + 7.8657 10 955 2—3 a, | 71.2275 |+13| 57.1830 |+ 9 + 8.2786 % св | 70.3565 |-+16| 58.0430 |+ 5 + 7-4134 Ce 70.7675 |+12| 57.6395 |+ 5 — 7.8205 + 7.8214 2270,80 3 cn 71.1760 |-+12| 57.2280 |+ 9 —+ 8.2303 104 22" 97° 2 dyp | 70.3880 |+16| 58.отбо |- 6 + 7.4426 de | 70.7790 | +12] 57.6245 |+ 6 + 7.8337 + 7.8354 23 28 2 do 71.1755 |+12| 57.2280 |+10 —= 8.2300 %Cy | 70.3475 |+17| 58.0560 |-н 6 — 7.4024 ес 70.7430 |+13| 57.6640 |+ 6 + 7.7960 —= 7.7976 ит 2 en 71.1400 |-+13| 57.2640 |+10 + 8.1943 Trabant — Jupiterscentrum. Lt—Xy | Mittel. |’ шага) I ya) Ph. | Au. cos à mm mm Та | 72.7180 |+14| 55.6680 |— 1 + 9.7819| +1.9162 x ce 72.6830 |+13| 55.7080 о + 9.7443] -+1.9229 р Во lu ' 8 HE cl les à Ся и 1.9186 | 1.9189 | +-1/9060.| —0/0004 | —0:0026 +-119030 5—3 e 72.6520 |-+14| 55.7345 [+ 1 + 9.7156] -+1.9180 2 Па | 69.9930 |+17| 58.3915 |+ 5 + 7.0575| —0.8082 2 С 69.9655 |-+16| 58.4200 |+ 5 + 7.0294] —0.7920| __ ns Fe — 07947 | 2 а | 69.9830 |+16|] 58.4050 + 6 + 7.0456] —0.7898 0.7946 0.7893 | —-0.0002 0.0026 | — 0,7917 | 5 е | 69.9455 |+17| 58.4401 |+ 6 — 7.0094] —0.7882 2—3 Ша | 69.2705 |+14| 99.1150 |+Io + 6.3341| —1.5311 s х с | 69.2275 |+13| 59.1640 |+10 + 6.2880] —1.5334| __ + gs —1,52 а. d | 69.2370 |-+13| 59.1500 |+11 —= 6.2998] —1.5356 р LS ый ЕР о: 2—3 е 69.1935 |+14| 59.1940 [+11 + 6.2560] —1.5416 3 ТУа | 78.7490 |+ 6| 49.6365 |+ 5 -+15.8124| 7.9467 ei С 78.7190 |+ 6| 49.6700 |+ —=15.7806| -+7.9592 ры 1% = | 2-3 а | 78.7305 |[+- 6| | добубо. |466 16.7933] 7.9579 | 779551 —+7.9018 0.0017 0.0026 | +7.8975 | 5_3 е | 78.7925 |+ 7| 49.6960 |[+ 7 +15.7543| +7.9567 2—3 Scheinbare Adiff: M— Centrum = + 3/9702 19, = 9.99328 —i?, = +0.00007 N— » = — 42.7105 : . 9— » =-13.0272 fa = 0.99297 —м = +, LU X = 01 R— » = —40.0095 em, === У— » = — 1.6185 и» = W— = — 0.4142 Г’, = 0.99330 Je = 0000% hm CHAN Side) POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. ‚еще. — Scalenablesung. ct. - P.-Kr.90° tt) P.-Kr. 270 |t+% Г _тт_ _mm_| mm_ mm 10000 mm 10000] 10000 ‚| 63.2885 65.0884 63.2875 |-+10]| 65.0368 |-16| о 73.8579 |-+12| 54.5200 0] о 74.4063 |-+28| 53.9819 |+20|— 6 76.2505 |-+18| 82.1355 |+ 5+2 46.2803 |-+31| 82.0953 |-+17|-+ 8 51.4430 |-+12| 76.9325 | 9 о 101.7809 |-+ $| 26.6060 |-+22|—16 66.7990 |+ 9| 61.5975 |+11 66.4110 |-+11| 61.9950 |-11 66.0135 |-+11| 62.3905 |+ 63.3060 |-+10| 65.0945 |-18 62.9200 |-+10| 65.4880 |-+18 62.5270 |-+10| 65.8725 |-+12 61.6795 |10| 66.7220 |+10 61.3040 |+-I1| 67.1010 |+10 60.9210 |+-ı1) 67.4775 |+10 60.0410 |-+15| 68.3630 |+-20 59.6630 |-+15| 68.7435 |-+15 59.2945 |-+11| 69.1020 |-+15 65.9270 |+13| 62.4640 |+12 62.4430 |-+12| 65.9430 |-+13 60.8380 |13| 67.5570 |+21 59.1920 |+13| 69.1970 |+16 66.6505 | 9| 61.7375 |-+11 63.1605 |-+10| 65.2230 |-+18 61.5580 |-+10| 66.8355 |-10 59.9145 |-+15| 68.4770 |+20 66.7120 |+ 9| 61.6740 |+11 63.2240 |-+10| 65.1595 |-+18 | 61.6230 |10| 66.7680 |+10 59.9810 |+15| 68.4085 |+2с | 64.5595 |-+22| 63.8285 |+13 | 61.0750 |-+16| 67.3160 |+13 1 59.4690 |+16| 68,9220 |-+18 | 57.8310 [+11] 70.5609 |+17 Scheinbare Decldif: M-—-Centrum N— » Q— » R— » У— >» W—- » 8% 1596. März 30. mm 0.0000 +10.569$ —-11.1120 [| — Oo = о 00 Allee LAY = -+10/5027 = +10.9498 = — 16.9338 — — 16.9693 = — 11.7662 = +38.2325 =-r21° 2,2 Dec]. AntYcH% = VER RN Bemerkungen = = > = > tgÿ sin 1’ YES > 195 sin 1’ zur Aufnahme. mm mm mm 0.0000 0.0000 — 0.0007 —=10.5688 — 0.0861 —+-11.0259 — 0.0078 — 17.0495 Bilder 2—3. — 0.0742 — 17.0802 — 0.0001 — 11.8448 0.0000 38.4850 Bilder 3. + 3.1067 — 0.3840 == 9955 — 3.6354 Trabant — Jupiterscentrum. Л: [2 m = Yt—Y2 | Mittel. Ir S(Yr—Y2) [Зови еее РВ. | As mm mm —0.4752 — 0,4661 6 ’ 6 0 ’ r ’ - 0.4607 — 0.4673 —0'4642 | -+0:0003 —0.0019 | —-0/0002 —. 04656 — 0.4673 —+-0.2497 ose —+0.2541 | -Н0.2524 | —0.co01 —0.0006 | —0.0502 | +0.2531 0,25 38 —+-0.3121 Be —0.3190 | -+0.3169 | — 0.0002 +-0.0012 | -+0.0002 | +0,3181 0.3214 — 1.8408 —1.8364 | _ 8 8 1.8305 — 1.8273 1.8335 | —1.8214 | -+0.0012 —0.0105 | -+0.0902 | —1,8305 —1.8294 195 = 0.99342 $25 = -+0.00013 fs = 0.99289 is = 0.00000 X =0.0 f's = 099342 Лу = -+0.00015 16* Qt 126 57 5. Scalenablesung. Object. sı '@ P.-Kr. 0° |6-H1|P.-Kr.180°| +1 Anhaltstierne| wie 57 A, mm mm mm 10000 10000] 10000 mm mm mm %9 | 57.8525 |+ 5| 70.5430 |417 — 5.0897 Je | 58.2445 |+ 5| 70.1475 |+-17 — 4.6960 Jo | 58.6570 |+10] 69.7420 |+17 — 4.2867 ZN | 57.8300 |+ 5| 70.5775 |+16 — 5.1182 he 58.2260 |+ 5| 70.1760 |-+16 — 4.7194 ho | 58.6200 |-+10| 69.7785 |+-16 — 4.3234 % y 57.8520 |- 5| 70.5480 [+16 — 5.0924 Ve 58.2460 | 5| 70.1580 |+16 — 4.7004 0 58.6420 |-+10| 69.7645 |+16 — 4.3054 %Ёш | 57.8670 |-- 6| 70.5270 |+16 — 5.0744 ke 58.26C0 |+ 6| 70.1380 |+16 — 4.6834 о 58.6605 |+11| 69.7430 |+16 — 4.2854 То | 60.1520 |-+14| 68.2350 |+19 — 2.7856 h | 60.1235 |+14| 68.2610 |+19 — 2,8128 р 60.1455 |+15| 68.2450 |+-18 — 2.7938 К | 60.1600 |-+15| 68.2250 |+18 — 2.7765 II g 57.5060 |+ 5| 70.8810 |+13 — 5.4318 h 57.4825 |+ S| 70.9045 |4-12 — 5.4552 р 57.5070 |+ 6| 70.8805 |-+-12 -— 5.4309 Г 57.5270 |+ 6| 70.8590 |+-12 — 5.4102 Шо | 56.6700 |-= 9] 71.7135 |+12 — 6.2658 h | 56.6430 |+ 9] 71.7460 |--11 — 6.2954 0) 56.6605 |+10| 71.7225 |+I1 — 6.2749 Е | 56.6730 [+10] 71.7130 |-+11 — 6.2639 IV д | 66.2095 |-+19| 62.1740 |+-Io + 3.2739 h 66.1850 |-+10| 62.2025 [+10 + 3.2474 й 66.2080 |+-10| 62.1835 |+ 9 + 3.2684 k | 66.2240 |+11| 62.1630 |+ 9 —= 3.2868 Scheinbare Adiff. wie 57 A. ay = 8" Е. RENz, 1896. März 30. № Ясно Pulkowaer Sternzeit 3 der Aufnahmen. Mittel. mm x — 4.6908 10° 36” 30° 2 — 4.7203 О 2—3 10° 37” 56° — 4.6994 38 18 2 — 4.6811 39 28 2 Trabant — Jupiterscentrum. 2—2 | Mittel. Е угу») Ph. | Да cos à mm тт —+-1.9052 2—3 re #-1.9057 | +1!8929 | <-0!0002 | —0!0026 | -+1'8905 21 —-1.9046 2—3 —0.7410 2—3 Fa —0.7341 | —0.7292 | —0.0001 | —0.0026 | —0,7319 Se, —0.7291 2 — 867150 3 op —1.5771| —1.566$ | —0.0001 | —0.0026 | —1,5692 “ar —1.5828 2—3 —=7.9647 2—3 НИ 7.9670 | -+7.9137 | -+0.0008 | —0.0026 | 7,9119 a x —-7.9679 2—3 19а = 0.99328 —i°y = 0.00007 До = 0.99297 — —= -0.00002 X = — 0.1 Refr. = + 8 Try = — 52 Fu = 0.99331 Ju = —0.00042 m 5.8 Bilder. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896. März 30. Weihe. Decl. Scalenablesung. 2 : B k t. s y nets | бы р убить | zur Aufnahme P.-Kr.90° tk P.-Kr.270°|t+k Anhaltstjerne| wie 57 А, mm mm mm 10000 10000] 10000 mm mm mm mm 61.4885 |+11| 66.9200 |-+ 9 — 1.8157 61.8750 |11| 66.5365 |+ 9 — 1.4307 — 1.4313 62.2550 |+11| 66.1500 |+11 — 1.0476 63.2195 |[11| 65.1890 |-+17 — 0.0851 63.6050 |+10| 64.8040 |-+17 —= 0.3001 + 0.2959 63.9730 |+-10| 64.4270 |+17 — 0.6726 65.0800 |-+18| 63.3260 |+10 + 1.7774 65.4420 |-+18| 62.9580 |+10 + 2.1424 + 2.1450 65.8170 |-+12| 62.5865 |-+-10 + 2.5153 66.8800 |+10| 61.5310 |-11 + 3.5744 67.2510 |+10| 61.1580 |+11 — 3.9464 —+ 3.9456 67.6155 |+20| 60.7845 |+1ı — 4.3159 Trabant — Jupiterscentrum. ye—yy Mittel. | sun) Лобо) его Ph. A mm mm 61.3935 +11| 66.9980 |- 8 — 1.9022] —0.4709 - 10] 65.26 6 — о. —о. , , ‚ BAR Er re » 9 #3 Pet Fée —0 4690 | —0:4659 | +0/0003 —0:0008 | 0.0002 —0:4646 66.7730 |+ 9| 61.6200 |+ 9 + 3.4764] —0.4692 61.1040 |+11| 66.2870 |-+11 — 1.1916] -+0.2397 en 341 ER u * Be и: —+-0.2404 | +0.2388 | — 0.0001 —0.000$ | +0'0002 -+ 0,2384 67.4775 |+10| 60.9130 |-+11 + 4.1822| -+0.2366 62.1920 |-+12| 66.1960 |+12 — 1.1020] -+0.3293 pre a re Ep 22 a ei: +-0.3306 | -+0.3284 | —0.0003 —0.0010 | +0.0002 +0,3273 67.5680 |-+21| 60.8205 |-+12 + 4.2742| -+0.3286 Bo —=14| 68.3825 |+-19 — 3.2866| — 1.8553 1.7410 |+ 66.6480 |+ — 1.5536] —1.8 ‹ 63.5075 57 8 64.7975 +17 ыя 0.2955 LE —1.8510 | —1.8389 | -+0.0014 | —<+0.0006 | +0.0002 —1.8367 |. 65.3880 |16| 63.0050 |+-Io + 2.0918| —1.8538 } — Scheïinbare Decldiff. wie 57 А. 195 = 0.99342 39; = -+0.00013 fs = 0.99289 is = 0.00000 X 15 = 0:0 fs = 0.99344 Js = +0.00018 dy —=+21° 2.2 128 Е. Rexz, 53 А. 1896. März 31. AR 144 Scalenablesung. Pulkowaer Sternzeit Object. Aut Bilder, P.-Kr. 0° tk) P.-Kr.180° t-+k der Aufnahmen. | Mittel. mm mm mm In | an 10000] 10000 В m Ctr, | 59.1811 69.2019 T 59.1801 |-10| 69.2006 |+13| Oo 0.0000 2 a M 56.0078 + 2| 72.3743 |+14 ©| — 3.1734 2 ù N 11.8724 |+24| 116.5120 |+ 6|-+-30] —47.3055 ñ Le 2 " Q 64.5984 |+25| 63.7859 |+14]— 1|+ 5.4171 10° 18” 54° 2 - R 14.2898 |-+33| 114.0870 | 8|+32] — 44.8838 1—2 || 14 50.7085 |-+16| 77.6720 |+13|+ 1] — 8.4711 2 || W 51.8862 |+26| 76.4938 |+23|+ 4] — 7.2928 1—2 2 % ay | 63.2130 [+10] 65.1855 |+16 + 4.023 1 ag 63.5950 [+ 9| 64.8010 |+16 —= 4.4070 + 4.4068 10 Chen 2 2—3 | Ay 63.9810 | 9| 64.4220 |-+-16 + 4.7896 5 %Dyp | 63.1840 [10] 65.2145 |+16 + 3.9948 AD | be 63.5675 |+ 9| 64.8395 |+16 + 4.3740 + 4.3717 10 46 10 11 4 2--3 | b, 63.9405 |+ 9| 64.4690 |- 8 + 4.7462 Ср 63.2270 |+ 9] 65.1705 |-+16 + 4.0383 d Ce 63.6080 |+ 8| 64.7910 |+-16 + 4.4185 —+ 4.4199 167 #36 2—3 | Co | 63.9950 |+ 8] 64.4100 |+ 8 + 4.8029 я % dy | 63.1800 |+ 9] 65.2150 |-+16 -+ 3.9926 À de 63.5615 |-+ 8| 64.8390 |+16 + 4.3712 —+ 4.3706 12 07 2—3 $ d 63.5385 | 8| 64.4635 |+ 8 —+ 4.7479 Trabant — Jupiterscentrum. | Fe | Mittel. | Лив) July —va) Ph. | Aa co у ВЕ RP QU НЫ Ч es ES ne LU ) mm mm N Та | 61.9690 |+-10| 66.4210 |+11 — 2.7844| — 1.6224 2—3 | b | 61.9370 |+10| 66.4555 |-+11 = 2.7911] —1.6206 || __ er ‚ RAT ие 2 в 61.9850 |+ 9) 66.4080 |+11 + 2.7988] — 1.6211 1.6207 16697 ее 9:960> a 1.6122 2—3 d | 61.9385 + 9| 66.4550 |-11 + 2.7520| —1.6186 2 à Па | 66.6345 | 9| 61.7525 |+ 9 + 7.4514| +-3.0446 2 | b | 66.6000 | 8| 61.7890 |+ 9 + 7.4158] +3.0441 в a2 ii. 2 al ae re Dell оо 3.0430 | -1-3.0224 0.0004 0.0027 | -+3.0193 y а | 66.5975 |+ 8| 61.7925 |+-10 —= 7.4128| +3.0422 2—3 : III & | 59.0645 |-11| 69.3220 |-+14 — 0.1185| —4.5253 Ai { b 59.0285 |-+11ı]| 69.3600 |--13 — 0.1554] —4-5271| __ EX LE Be 2— 4 с | soo7ro -rııl 693170 |+13 tant 242526 4.5294 4.4987 | -+-0.0005 0.0027 4.5008 | 5 # d | 59.0210 |--10| 69.3650 |-+13 — 0.1618] —4.5324 2—3 IV а | 72.1935 |+12| 56.1950 |— I —=13.0103| -+8.603 5 „a й Ь | 72.1585 |-+11| 56.2330 (6) —+-12.9738| -+8.6021 мы 4 — | аа 13.0224] 8.6025 —+8.6025 | 8.5444 0.0011 0.0027 | +8,5406 | о d | 72.1580 |11| 56.2350 (о) +-12.9724| -+8.6018 2—3 | Scheinbare Ædiff: M—Centrum = — 3.3502 Ло = 0.99323 —1 = 0.00004 3 N— » = —50.0308 р Q— » = + 5.7068 fa = 0.99292 —iy =— 0.00001 MR = R—- » = —47.3298 Вей’. = + 5 У » = — 8.9388 ль» = 49 W— » = — 7.7347 f'x =0.99324 Jz = 0.00053 т ay = 8” 5.9 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. eihe. Scalenablesung. ‚ [P.-Kr.90° t+k tt) P.-Kr. 270° 44.8569 |+36| 83.5266 |+10 50.0025 |-+10| 78.3840 100.3345 :|+ 7| 28.0524 67.5630 |+ 8| 60.8560 |+10 о | 67.1980 |+ 8| 61.2150 [+10 ‚ | 66.8300 |-+ 8| 61.5730 |+9 „| 65.8710 |+10| 62.5310 |+9 , | 65.5160 |+-10| 62.8850 65.1625 64.2420 63.8820 63.5270 62.6210 62.2609 61.9020 63.2370 64.1655 64.5255 64.8760 65.7780 66.1460 66.5020 67.5960 65.9240 64.2875 62.6660 66.4290 | 64.7550 63.1160 61.4975 60.7960 62.4690 64.1085 65.7280 61.9610 63.6380 65.2750 66.8925 60.1160 61.7880 63.4270 65.0420 63.2400 64.9130 66.5520 68.1685 Lu) 68.2725 › | 66.6010 64 9650 63.3400 | 65.1520 | 63-4760 | 61.8395 60.2190 у тт ; 10000 m 10000 г, | 61.0440 61.3424 | 64.0430 |+10| 64.3415 |+ 9 Г | 72.4116 |+14| 55.9772 |+ 2 | 72.9825 |+34| 55.4041 |+17|-— 4 44.7972 |+18| 83.5932 |— 7|+ 10000 а 1596. März 31. ТИ +44 ++ 3.5496 1.8768 0.2388 1.3818 2.3832 0.7080 0.9307 2.5483 4.2277 2.5557 0.9186 0.7021 1.1055 0.5697 2.2070 3.8258 Scheinbare Decldif: FD js per — + 813183 | = 22 | 7— W= Зап, Физ,-Мат, Отд. ^ 0% = —19.1538 — 13.9505 = -+36.0482 ES 27 г ° +1.0903 Decl. 91+ +9; 3 + 3.1403 1.4654 0.1704 9—9 | Mittel. тт тт -+0.4093 +-0.4114 —+-0.4092 +-0.4095 —0.7571 —0.7574 — 0.7603 —0.7570 +-1.0874 +-0.4098 —0.7580 +-1.0890 +-1.0890 —+-1.0892 —2.0348 —2.0351 —2.0366 — 2.0345 125 = 0.99341 fs =0.99289 f's = 099341 —2.0352 | x? . x? <: 5 #95 sin 1’ y — = tgù sin 17 mm mm 0.0000 0.0000 — 0.0005 + 8.3665 — 0.1182 + 8.8204 — 0.0015 —19.2489 — 0.1038 — 19.2868 — 0.0037 —14.0453 — 0.0029 +36.2850 Trabant — Jupiterscentrum. 5—5) | Js (1—2) Heat) Bemerkungen zur Aufnahme. Bilder 2—3. Un- durchsichtige Luft. 04071 | —0!0001 +-0/0007 | -+0'0002 | -+0:4079 —0.7530 | —-0.0001 —0.0019 | +0.0002 | —0.7516 +1.0818 | —0.0002 +0.0011 | +0.0002 | -+1,0329 —2.0218 | -+0.0003 —0.0083 | -+0.0002 | —2,0296 $95 = -1-0.00002 is = —0.00009 X 5 = —0:3 Тб = -+0.00004 17 130 F. Renz, 55 DB. 1896. März 31. № 145) Scalenablesung. р Pulkowaer Sternzeit open I. | 5 © Yu Bilder. P.-Kr. 0° th) P.-Kr. 180° |4+% der Aufnahmen. Mittel. Anhaltstierne| wie 58 A, mm mm 10000 10000 mm mm mm fi | 53-7880 |+ 4] 74.6195 |+10 ЕЯ Je $4.1670 | 4| 74.2375 |+12 — 5.0211 TO EAN 3 Jo 54.5570 о] 73.8415 |+12 %9 | 53.7890 |+ 4] 74.6170 |+10 de 54.1610 |+ 4| 74.2365 |+12 — 5.0272 257236 2—3 90 | 545395 | ©] 73.8590 [+12 10° 26" 0 Zh | 53.8225 |+ 3| 74.5855 |+10 ; he | 54.1945 |+ 3| 74.2170 — 4.9958 26 31 2—3 ho | 54.5750 |— 1| 73.8240 Yin | 53.7770 |+ 3| 74.6255 % 54.1505 |+ 3| 74.2530 — 5.0423 27 29 2 to 54.5195 |— 1| 73.8810 Trabant — Jupiterscentrum. 2 — xy | Mittel. Лига) Лии») Ph. | Aa cos à mm mm If | 52.5735 |+ 8| 75.8160 — ee 2 9 | 52.5720 |+ 8| 75.8195 — —1.5861 | — вы Ber Br 4 2 В | 52.6090 |+ 7| 75.7840 a 1.5813 1.5838 115731 0.0002 0.0027 15760! 9_5. î 52.5650 + 7| 75.7270 — —1.5783 2 If 57.2040 |-+10| 71.1830 — +-3.0419 2 9 57.2005 |+ 9| 71.1905 — —+3.0424 Bi 2 2 а Le à anse 3.0448 -+3.0438 | -+3.0231 | -+0.0004 0.0027 | 3.0208 | 9_3 р 67.1900 |+ 9| 71.2025 — +-3.0463 2—3 If Bo + р 78.7695 = —4.5447 Sp 9 | 49.6110 |+ 75.7750 = —4.5444| _ at cs EN 5 h | 496430 |-+ 6| 78.7445 LS mue 4.5450 4.5142 0.0005 0,0027 4,5174 9 à | 49.5960 |+ 5| 78.7935 = —4.5461 2 IV | 62.7610 |+10| 65.6290 + —+8.5975 3 9 | 62.7570 |+ 9| 65.6375 + —8.5973 » 2—3 1 р | 62.7900 [+ ©] 65.6060 En 48.5981 8.5986 | -+8.5406 | -+-0.00I0 0.0027 | -+8.5389 | 2. | $ | 62.7480 [+ 9| 65.6500 + 3.5593| 8.6016 3 unterexponiel ll Scheinbare Adiff. wie 58 A. Fa = 0.99323 —®. = -+0.00004 fe = 0.99292 —iy =— 0.00001 X и =00 Refr. = + 7 Ta = — 56 Fa = 099325 ЛХ. = —0,00050 ay = 8" 5.9 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. 181 | 1896. März 31. Reihe. Decl. Scalenablesung. Г | тн ен 22 198 Re р x2 105 ner Bemerkungen memes ss Pine: ice tes 5 _— — 8 ` ns P.-Kr. 90°) += P.-Kr. 270° |t-+k 3 2 2 BE ALIEN Anhaltst\erne| wie 58 A, mm mm mm 10000 10000] 10000 mm mm mm mm 67.5810 |+12| 60.8305 |-+13 + 3.5244 67.2180 |+12| 61.1870 |-+13 + 3.1656 — 3.1606 66.8450 |+12| 61.5600 |-+12 + 2.7917 65.9220 |-+14| 62.4865 |+12 —+ 1.8670 65.5550 |-+14| 62.8365 |-+12 + 1.5086 + 1.5101 65.2070 |+20| 63.1965 |+12 + 1.1548 64.1810 |-+12| 64.2320 |+11 + 0.1238 63.8215 |+12| 64.5800 |+19 — 0.2304 ‚ — 0.2343 63.4560 |+12| 64.9460 |-+19 — 0.5962 62.4900 |+13| 65.9130 |+13 — 1.5623 62.1395 |-+13| 66.2605 |-+13 — 1.9113 — 1.9123 61.7895 |-+13| 66.6150 |-+11 — 2.2634 Trabant — Jupiterscentrum. д т = Уфу» | Mittel. | aura) | Лобо | бета Ph. | 45 67.6115 |+22| 60.7820 |+15 + 3.5643| -+0.4037 | ER SM ae BE Е. SE ER +0.4025 | -+0!3999 | —o!oooI —o'oo11 | -+0!ooo2 | +0:3989 62.5380 |-+13| 65.8570 |+15 » 66.4440 |+13| 61.9460 |+10 64.7950 |H-19| 63.5960 |+ 9 63.0455 |+12| 65.3435 |+17 61.3705 |+13| 67.0220 |+ 9 1.5104| -+0.4019 2.3984] —0.7622 ен Е —0.7632 | —0.7582 | -+0.0002 +0.0012 | +0.0002 | — 0,7566 2.6764] — 0.7641 BER 68.3020 |-+23| 60.0850 |-20 + 4.2578] -+1.0972 66.6575 |-+13| 61.7340 |#15 + 2.6108] -+1.1007 в HE 63.4810 15 + 0.8625| -+1.0968 +-1.0980 | -+1.0908 | —0.0003 —0.0037 | -+0.0002 | -+1.0870 63.2295 |+14| 65.1570 |-+22 — 0.8150] -+1.0973 | 65.1640 |+17| 63.2300 |+ 9 + 1.1166] — 2.0440 63.5170 |+ 64.8780 |+16 — 0.5316] —2.0417 Æ 65640 RE ee Lea — 2.2807| —2.0464 —2.0448 | —2.0314 | 0.0006 0.0007 | -+0.0002 2.0299 | 60.0875 |-+15| 68.3045 |+18 — 3.9594] — 2.0471 | $ Scheinbare Decldiff. wie 58 A. 175 = 0.99341 $2 = -+0.00002 | fs —=0.99289 is ——0.00009 x ig=—0/3 dy = 21° 1:9 | | f'à =0.99348 Л =-+0.00007 | | 1 у 132 Е. Renz, 59 A. 1896. April &. AR 146 Scalenablesung. Pulkowaer Sternzeit Object. WEI an ви. фа Bilder. P.-Kr. 0° | t-+%| P.-Kr.180° |t-+-%k 2 der Aufnahmen. Mittel. mm mm mm Kern 10000! mm 10000] 10000 mm tr. | 64.0723 64.5119 S 64.0715 |+ 8| 64.3111 [+ 8 о 3 M Durch elin Jlupitersbild | verdleckt. N |. N 24.9029 |+26| 103.9799 |-+- 6|-+17| — 39.1660 3 ellipt. in AR. 77.6654 |+21| 50.7184 |+20|— 3|-+13.5930 10° 55” 30° 1-2.“ В 27.3456 |-+35| 101.0330 |-+13|-2т| —36.7207 2—8 ellipt. У 63.7709 |+18| 64.6060 |+23] © — о. 2—8 W | 61.9180 |+-28| 63.4685 |+24| o|+ 2 %а | 68.3760 |+-19| 60.0300 |-+-14 + ас | 68.7675 +14] 59.6335 |-+14 = — 4.6871 10 MO 743 2—3 а, | 69.1620 |+-14| 59.2390 |+10 + 4b | 68.3645 |-+-18| 60.0330 |-+-14 + 0, | 68.7525 |+13| 99.6590 |+14 + —= 4.6664 42 20 1—2 bo | 69.1280 |+13| 59.2740 |-+-10 + 10° 42" 51° | 2 Cy | 68.3830 |+18| 60.0190 |+15 + | CA 68.7690 |-13| 59.6430 |+15 + + 4.6822 43 30 2 Co | 69.1460 |-+13| 59.2620 |+11 + 2% dun | 68.3860 |-+-18| 60.0110 |-H15 +- de | 68.7620 |13| 59.6420 |+rs -- + 4.6814 44 52 1—2 do | 69.1395 |+13| 59.2650 |+11 + Trabant — Jupiterscentrum. Lt —Ly | Mittel. |’, (ра) Таиз Jahr | До cos à mm mm Га | 70.2455 |+17| 58.1460 |+ 5 + 6.1702] -+1.483 1 Sp b | 70.2215 |-+-16| 58.1690 |+ 5 + 6.1466] -+1.4802 ' N) ОА ' € | 70.2350 |+16| 58.1545 |+ 6 + 6.1606] -+1.4784 +-1.4767 | +-1/4662 -0/0001 0'0028 | +1:4633 2 | а | 70.2205 |+-16| 58.1680 |+ 6 + 6.1466] +1.4652 1 | II Geht dufrch [die Jupiter|scheJibe. Па | 64.3105 |+ 9] 64.0780 |- 8 -+ 0.2361| —4.4510 Nr b 64.2915 |-+- 8| 64.0960 |- 8 + 0.2176] —4.4488| __ Les Je fs | el a 81 | блюдо bh aan 4.4483 4.4167 | -1-0.0004 0.0028 4.4191 19 | а | 64.3055 |-- 8| 64.0815 |+ 9 + 0.2318] —4.4496 2 | DE 60.4300 |-+15| 67.9560 |+19 — 3.6434| —8.3305 er | 60.4110 |+15| 67.9765 |--18 — 3.6631| — 8.3295 | _ 9. = >= = — ce | 60.4255 |+14 67.9620 ral. — 3.6486| —8.3308 8.3319 8.2728 | -+0.0007 0.0028 8.2749 | 9 _3 | а | 60.4180 |+14| 67.9680 |-+-18 — 3.6554] —8.3368 2 Г | Scheinbare ЖАШ: M—Centrum = + 5:2703 F° « = 0.99290 —i°y = —0.00014 N— » — —41.4107 } , 0— » =-14.3275 Ja = 0.99257 —iy = —0.00022 X ty = + 0.8 R— » — —38.7095 Бег. =-+ 8 У » = — 0.3183 Toy =+ 52 W— » = + 0.8857 TS — 0.99291 Je = +-0.00038 Зее. P.-Kr. 90° POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. tt P.-Kr. 270° mm 10000 63.3570 63.3561 |+ 9 Durch еш Jlupitersbild 66.9265 38.7570 38.7900 43.9550 94.3071 66.8680 66.4960 | 66.1250 65.1470 64.7805 64.4220 1 63.5345 | | 63.1790 62.8140 61.8590 | 61.5020 61.1435 66.1105 | 64.3650 62.7910 61.1190 | 67.6150 65.8980 | 64.2905 | 62.6175 | 68.4730 | 66.7530 55.1490 | 63.4755 Scheinbare Decldiff: M—Ce +25 +30|. 6539 +19 =>) BD +11 +11 +17 = DV} ЕВ +10 +10 ID +10 +10 +H и 939 +10 +11 | Geht dulrch mm 5 t+k mm 1896. April =. Decl. < 10000] 10000 in Znt%c+%s 2 4/5 sin 1’ р 8 sin] 3 Tg go Sin У—= 9 sin тт тт тт 0.0000 0.0000 — 0.0811 + 3.4885 — 0.0094 — 24.6054 — 0,0694 —24.6280 0.0000 —19.3959 0.0000 —=30.9476 + 3.1297 + 1.4173 — 0.1894 — 1.8644 Bemerkungen L zur Aufnahme. Bilder 3 3 mm 65,0337 65.0321 |-+16| о 0.0000 verdleckt. 61.4636 |-+27|— 1|+ 3.5696 89.6299 |— 3|-+ $| — 24.5960 89.5899 |-+ 8|-+14| — 24.5586 84.4265 |— 7] + 2| —19.3959 34.0846 |+20|— 9| +-30.9476 61.5510 |+10 + 3.4968 61.9130 |190 + 3.1299 62.2770 |+10 + 2.7624 63.2625 |+10 + 1.7810 63.6330 |+ 9 + 1.4125 63.9825 +9 + 1.0585 64.8720 |+16 — 0.1693 65.2310 |+16 — 0.1880 65.5895 |+11 — 0.5494 66.5500 |+ 9 — 1.5071 66.9140 |+ 9 — 1.8676 67.2575 |+ 9 — 22186 62.2780 |+11 + 2.7546 63.9935 |+10 —= 1.0390 65.5990 |+12 — 0.5658 67.2690 |+10 — 2.2366 die Jupiter|schelibe. 60.7740 |+10 — 4.2592 62.1895 |+ 9 + 2.5426 64.0975 |+ 8 —= 0.9348 65.7700 |+10 — 0.7380 59.9190 |+-I4 + 5.1156 61.6390 |+ 9 + 3.3954 63.2420 |+ 9 + 1.7922 64.9155 |+16 + 0.1180 ntrum— + 3.0035 №. » = + 3.4507 Q— » = —24.4330 Ru nz — — 24.4690 т + = — 14.2653 W—- » = +30.7335 dy = -+20° 58:3 Trabant — Jupiterscentrum. = и--у» | Mitte. [Из иги)? (иго) (ее-ааз)з]| Pi. тт тт ment 09:31 3 Fu, u ’ 0 er r — 0.3764 0.3755 0.3729 | -+0'с005 0'0009 | 00902 —9.3722 —+-1.1295 ul +1.1264 | +1.1187 | —0.0014 | -+0.0012 | -+0.0002 +-1,1264 +1.9859 Ho +-1.9820 | -+1.9684 | —0.0028 -+0.0005 | -#+0.0002 —1.9824 fa =0.99315 39 = -+0.00032 fs = 0.99259 is = 0.00016 X 14 =-+ 06 fs = 0.99315 Js = -+0.00034 1 —0:3731 —1.1187 —+1,9663 134 59 3. Scalenablesung. Object. P.-Kr. 0° th) P.-Kr. 180° Anhaltst/erne| wie 59 A, mm 10000 mm mm %9 | 58.9480 |+11| 69.4530 de 59.3500 |+11| 69.0495 90 | 59.7555 |+15| 68.6405 % hop | 58.9600 +10] 69.4490 Re 59.3580 |-+10| 69.0595 ho | 59.7540 |-+14| 68.6505 Zip 58.9660 |+10| 69.4410 ie 59.3580 |-+-10| 69.0480 бо 59.7480 |+-14| 68.6530 %k | 58.9470 |+10| 69.4581 ke 59.3400 |+10| 69.0685 ko 59.7310 |+14| 68.6771 Та | 60.7635 |+11| 67.6250 h | 60.7700 |+10| 67.6225 р 60.7660 |+10| 67.6250 К | 60.7390 |+10| 67.6535 II Geht du/rch |die Jupiter II g | 54.9280 0| 73.4655 h | 54.9325 0| 73.4580 В 54.9370 |— 1| 73.4560 k | 54.9175 |— И 73.4755 UI g | 51.0165 |+11| 77.3770 h 51.0225 |-+11| 77.3715 р 51.0230 |+11| 77.3710 k 51.0000 |+10| 77.3940 нЕ mm 10000 +13 +13 +135 Sl) +13 +13 Г Zi) +13 +13 +14 +13 +18 +18 —I9 +19 scheli +13 +13 +-13 mm 10000 Scheinbare Adiff. wie 59 A. La | Г Ки тт 5.1328 4.7300 4.3226 5.1248 4.7311 4.3284 5.1178 4.7254 4.3326 5.1359 4.7446 4.3532 3.3113 3.3068 3.3102 3.3379 9.1496 9.1436 9.1404 9.1600 — 13.0604 —13.0546 — 13.0541 —13.0772 Xy—= 8% Е. Веки, 1896. April &. № 147 | 2 6% 0 Pulkowaer Sternzeit м 4 = der Aufnahmen. Mittel. | — 4.7285 11? 650 3—4 — 4.7281 д 152 3 | 11: о — 4.7253 SZ 2 — 4.7446 6 52 2 Trabant — Jupiterscentrum. о | Mittel. [fu (ær—22) I 0702) Ph. | Aa соз 5 mm mm —+-1.4172 3 -+1.4213 ' р JF? r109x | 3—4 r.atsı | НТ-4ТТ | 51-4051 | 40.0002 0.0028 | 1.4025 | 5 1,4067 3 —4.4211 3 | se —4.4168 | —4.3856 | —0.0007 | —0.0028 | —4,3891 - ь | | —4-4154 2—5 LU 2 RS ОО CH A. в _R 975 | | 8.3288 8.3300 8.2712 0.0013 0.0028 8.2753 | 3 | | —8.3326 2—3 | Fu = 0.99290 —®, = —0.00014 | Ja = 0.99257 —i4 = -— 0.00022 X = + 018 Вет. =+ 10 Та =— 53 Го =0.99294 7. =- 0.00065 т 7.0 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. пе. Scalenablesung. P.-Kr. 90° t-+-k tt P.-Kr. 270° Geht dulrch |die Jupiter|schelibe, 67.4920 Anhaltstierne| wie 59 А, _тт_ _mm_| тт_ 10000 10000] 10000 тт тт 66.7550 |+ 9| 61.6540 |+10 66.3720 |+11| 62.0310 [+10 65.9910 |+11| 62.4190 |+10 65.0100 |-+17| 63.3930 |+-10 64.6300 |+17| 63.7810 64.2635 |+ 9| 64.1490 63.2980 |+10| 65.1075 |+17 62.9300 |-+10| 65.4720 |+17 62.5600 |+10| 65.8490 |+11 61.5665 |+11| 66.8370 61.1975 |+ı1| 67.2120 60.8315 |+11| 67.5870 Kar 66.0080 |+11| 62.3880 |+ 1$ 64.2660 |-+- 9| 64.1290 62.5620 |-+10| 65.8340 ах 60.8320 |-+11| 67.5600 |+18 -=21| 60.8990 |+13 65.7575 |-+13| 62.6375 |+12 64.0460 |-+11| 64.3470 |-+11 62.3160 |12| 66.0770 |-+13 41 68.3600 |-+23| 60.0360 |+19 66.6225 |+13| 61.7765 |+14 64.9150 |+21| 63.4815 |+14 63.1850 |-+14| 65.2080 |-r21 - Scheinbare Decldiff. wie 59 А. dy = +20° 58,3 II II +++ ++ Mitt I +++ Mira mm 3.3888 3.0089 2.6244 1.6472 1.2632 0.8956 0.0668 0.4330 0.0862 1.7968 2.1688 2.5398 2.6484 0.9069 0.7976 2.5260 4.1352 2.3984 0.6878 1.0422 5.0006 3.2613 1.5554 0.1735 1596. April =. Decl. “пн с; 3) ie FO in, — 5 96 sin № У — = 1901 1 тт + 3.0074 + 1.2687 — 0.4353 — 2.1685 Trabant — Jupiterscentrun. À T vo—ys | Mittel. |fstu-v2)| Льгота) тт тт —0.3590 —0.3618 —0.3623 —0.3575 —-0/0006 -+0/0006 —0.3602 | —0!3577 —+1.1278 —+-1.1297 —+1,1231 +1.1263 —+1.9932 —+-1.9926 —+-1.9907 —+1.9950 +1.1267 | +1.1190 | —0.0017 —0.0035 +-1.9929 | -+1.9793 | —0.0032 — 0.0083 $2; = +-0.00032 is = —+0.00016 Js = +0,00038 128 =0.99315 fs =0.99259 f's =0.99318 Bemerkungen zur Aufnahme. Bilder 4. Ph. —+-0/0002 —=0.0002 —=0.0002 X is = 0.6 45 —0:3563 1,1140 +1,9680 Scalenablesung. 136 60 A. Object. Р.-Кг. 0° mm тт Ctr, | 66.8068 |000 M 66.8060 |+ 8 N 22.6692 |-+24 Q | 75-4368 |+24 R 25.1241 |+-39 17 61.5419 |+20 W | 62.6590 |+20 #4 | 71.1245 |+13 ас | 71.5080 |+12 Ay 71.8935 |+-12 % by | 71.1575 |+12 D, 71.5425 |+II b, 71.9210 |-+11 % dy | 71.1110 |+12 de 71.4765 |+12 do | 71.8580 |+-11 %е [71.1315 |-+13 ес 71.4930 |+13 eo 71.8650 |+12 I Geht durch Па | 72.6490 |+-14 b | 72.6835 |+13 d | 72.6385 |+13 e | 72.6575 |+14 Ша | 74.0810 |+13 b 74.1135 |+12 d | 74.0655 |+12 e 74-0805 |+13 IV a | 64.7085 +17 b 64.7325 |+17 а | 64.6805 |+16 e 64.6980 |+16 t-+k| P.-Kr.180° 61.5736 61.5727 105.7152 52.9480 103.2573 66.8357 65.7237 57.2760 56.8935 56.5135 57.2510 56.8600 56.4845 57.2935 56.9300 56.5540 57.2740 56.9075 56.5455 die Jupiter 55.7410 55.7065 55-7535 55.7370 54.3060 54.2755 54.3215 54.3095 63.6855 63.6590 63.7115 63.6995 Scheinbare Adiff: t+k || (D ооо nmaww © © == ITERTIT: _mm_ 10000 _mm 10000 9 + 6 15 +-19|— +17 —+-16|+- +-24| + EN) 8) an © EM 9 = о —=10 +10 +10 +10) +10 +10 schelibe. N— Centrum = —46:6810 = Е. Renz, 1896. April 10. AR 148 Dutch Pulkowaer Sternzeit u |: 2 der Aufnahmen. Mittel. mm Yo 0.0000 2 mar h т 5 2 + 8.6275 ДИ ©) 2 —41.6786 2 — 5.2632 2 — 4.1490 1222 —+ 4.3078 —= 4.6908 + 4.6907 IT Ио 1—2 + 5.0736 — 4.3368 —+- 4.7198 + 4.7195 46 19 1 + 5.1018 11% 48” 13° —+ 4.2922 — 4.6568 + 4.6615 so I 1—2 + 5.0354 + 4-3124 + 4.6763 + 4.6773 SI 34 1 — 5.0432 Trabant — Jupiterscentrum. Lt —Ly Mittel. |f’„(e:—xz) u) РВ. тт тт + 5.8382] -+1.1475 2 5 Ic er +1.1582 | +1/1503 | —0'0004 | —0!0028 | +1:1471 ; + 5.8444] 1.1671 2—3 + 7.2714] 42.5807 2 ae Ds en +-2.5876 | -+2.5699 | —0.0009 | —0.0028 | +-2,5662 4h + 7.2693| +-2.5920 2—3 — 2.1047| —6.7954 2 = os а. —6.7954| —6.7490 | 0.0026 | —0.0028 | —6.7492 = — 2.1170 —6.7943 3 unterexponie 1 Fa =0.99314 —1°,, = +-0.00097 = 9.0572 — —43.9798 fa = 0.99274 о = +0.00082 X i„=— 28 = — 5.5887 Refr. =+ и — — 4.3847 Try =-+ Га = 0.99317 “То, = 70.0131 т ay = 8? 7.4 Scalenablesung. P.-Kr.90° ыы P.-Kr.270° HW 10000 nn 63.6808 64.7006 63.6800 |+ 8| 64.6989 64.2160 |-+24| 64.1753 36.0731 |-+26| 92.3171 36.0863 |-+38| 92.2943 41.2613 |-+25| 87.1208 91.6069 |— 5| 36.7815 67.2420 |+10| 61.1665 66.8870 |+10| 61.5230 66.5260 |+10| 61.8830 65.5340 |-+18| 62.8765 65.1670 |+18| 63.2380 64.8065 |+18| 63.5970 62.0400 |+11| 66.3660 61.6915 |+11| 66.7200 61.3400 |+12| 67.0660 60.3300 |+16| 68.0720 59.9815 |-+16| 68.4210 59.6400 |+16| 68.7660 68.5660 66.8560 ‚63.3790 61.6670 Scheinbare Decldiff: POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Geht durch |die Jupiter|schelib 61.7570 63.4710 66.9520 68.6610 62.0960 63.8120 67.2920 69.0115 59.8260 61.5360 65.0145 66.7310 $ +21 +16 +-12 +12 +11 +16 2-13 2 a >) EL +14 u) +16 + 8 N—Centrum Q— » Ren V— ‘» W— >» Зап. Физ.-Мат, Отд. _mm_ 10000| 10000 +17 я +-27 de 0.5301 +10 Mae —27.6090 — 2|+-36| —27.5891 — 4|-+ 3| —22.4181 +-22|— 6] -+27.9206 E13 23.5475 12 + 3.1918 +12 + 2.8313 +12 + 1.8390 +12 + 1.4747 +12 + Г.1150 +13 — 1.6532 +1] 2.0044 +11 — 12. +21 —3. 1896. Арки 10. тт 0.0000 2.9491 1.2328 2.2480 3.9560 2.6076 0.8930 2.5896 4.2973 4.8798 3.1698 0.3082 2.0220 = + 0.4472 = —27.4365 = — 27.4725 = — 22.2688 = +-27.7300 Decl. An+%c +4 в... ON Fo — > 196 sin 1’ тт тт 0.0090 — 0.1029 — 0.0038 — 0.0896 — 0.0014 — 0.0009 + 3.1902 + 1.4762 — 2.0035 ея , y—-tgèsinl mm 0.0000 + 0.4272 —27.6128 —27.6787 —22.4195 27.9197 137 Bemerkungen zur Aufnahme. Bilder 4. Bilder 4. Trabant — Jupiterscentrum. Yt — 9% | Mittel. —0.2411 —0.2434 —0.2445 — 0.2478 —0.5826 —0.5832 —0.5861 —0.5891 —+1.6896 +-1.6936 —1.6953 1.6862 — 0.2442 —0'2426 — 0.0056 —0.0007 —0.5852 | —0.5813 | —0.0013 —0,0017 -=1.6912 | -+1.6798 | -+0.0036 0.0010 195 = —0.00056 = —0.00085 = —0.00053 17% =0.99325 fs = 0.99257 f's = 0.99327 13 DE) Ла (физ) Je (rr-22)|- 222) +-0/0002 —0.0002 —0.0002 Х8=- 29 —0:2437 — 0.5841 +-1,6846 138 60 18. Scalenablesung. Object. - P.-Kr. 0° tk) P.-Kr. 180°|1+-7 Anbaltst/erne| wie 60 A. mm mm. mm 10000 10000] 10000 mm mm Zfw | 61.7050 |+ 9| 66.7010 |- 9 me 62.0810 |+ 9| 66.3135 |HI1 un 62.4775 |+ 9 65.9340 +1 %9% | 61.7345 |+ 9| 66.6710 |+ 8 de | 62.1140 |+ 9| 66.2895 |+-10 do 62.5030 |+ 9| 65.9090 [+10 %hyn | 61.7350 |+10| 66.6690 |+ 8 he | 62.1080 |+10| 66.2990 [+10 ho | 62.4950 |+10| 65.9160 |+10 Zip | 61.7195 |[--10| 66.6820 |- 8 Le 62.0955 |+10| 66.3150 |+10 2 62.4705 |+10| 65.9395 |+10 I Geht durch [die Jupiter|schelibe. ПЛ | 63.2945 |+ 9| 65.0915 |+17 9 | 63.3195 [+ 9| 65.0650 |+16 h | 63.3290 |+ 9| 65.0540 |-+16 i 63.3100 |+10| 65.0780 |+16 II f | 64.7065 |+16| 63.6800 |- 9 9 | 64.7325 |+16| 63.6565 |+ 8 № | 64.7395 |+-16| 63.6475 |- 8 i 64.7195 |+17| 63.6705 |-+ 8 IVf | 55.3080 |— ı| 73.0805 |+-13 9 55.3300 |— 1| 73.0600 |+13 h | 55.3375 0| 73.0510 |+13 р 55.3185 0) 73.0755 |<+14 Scheinbare Adiff. wie 60 A. mm 5.1146 4.7330 4.3450 5.0848 4.7044 4.3196 5.0835 4.7121 4.3271 5.0978 4.7264 4.3511 1896. April 10. F. Renz, № Pulkowaer Sternzeit ZwtrZcH%o der Aufnahmen. Mittel. mm — 4.7309 12" Ао 2—3 — 4.7029 29 2 12° т” 6 — 4.7076 59 1—2 — 4.7251 I 1 Trabant — Jupiterscentrum. Em: = | Mittel. | 'ater—22)| Turn) Ph. | Да cos 8 mm mm —+1.2154 2 og | 1.2202 | +1!2119 | —olooor | —0!0028 | -+1:2090 1; -+1.2242 2 —+-2.6279 2 .6 2 РЯ +-2.6309 | 2.6130 | —0.0003 | —0.0028 | +2.6099 | 5 +-2.6335 2 —6.7729 2 5 we —6.7724 | —6.7264 | -+0.0009 | —0.0028 | —6,7283 al —6.7707 2—3 Fra —0.99314 —1°,, = +-0.00097 fa —0:99274 —iy, —=—+0.00082 № iy=— 2.8 Refr. = + 21 Try =— $2 Га = 0.99320 I, = 0.00051 ay = 7.4 Bilder. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 139 1596. April 10. пе. Decl. _ Scalenablesung. : я Znt%ct2; Les В Pe FR ie P.-Kr. 90° #54 P.-Kr.270° К 3 = 3 Anhaltst/erne| wie 60 А, mm ы тт_| тт 10000 10000] 10000 тт тт тт тт А 61.7725 |+10| 66.0360 |+ 8 — 1.9419 Bilder 3. 62.1290 |+10| 66.2760 +10 — 1.5636 — 1.5677 62.4960 |+10| 65.9110 |+10 — 1.1976 63.3140 |+10| 65.0890 |+16 — 0.3779 63.6760 |+ 9| 64.7320 |-+16 — 0.0184 — 0.0190 64.0310 |+ 9| 64.3720 |+ 8 + 0.3394 65.0840 |+17| 63.3260 |+9 — 1.3893 65.4370 |-+17| 62.9585 |+ 9 + 1.7496 + 1.7483 65.7990 |-+11| 62.6070 |+ 9 + 2.1060 66.8320 |+ 9| 61.5710 |+ 9 — 3.1404 67.2020 |+ 9| 61.2070 |+10 + 3.5074 + 3.5004 67.5450 |+ 9| 60.8580 |+10 — 3.8534 Trabant — Jupiterscentrum. Ye—y2 | Mittel. fav Ts (ежа) а-я) Ph. | Ad mm mm Geht du/rch (die Jupiter|schelibe. { 61.8645 |+10| 66.5220 |+ 8 — 1.8188] —0.2511 {| 63.4040 |-+10| 64.9820 |-+16 — 0.2794] —0.2604 | __ ОЕ +1, , , ET 65.1700 |-+17| 63.2140 |+ 9 + 1.4883| — 0.2600 0.2501 0.2484 0'0005 +-0:000$ | -+0/0002 0:2452 66.9170 | 9| 61.4740 |+10 + 3.2314] —0.2690 5245 + 9| 66.8630 |+ 8 — 2.1593 —0.5916 3.0650 |+ 9| 65.3210 |H-16 — 0.6184| —0.5994 es 5 = —0 95 64.8310 |416] 63.5535 [+ 8 + 1.1490] —0.5993 0.5987 0.5947 0.0012 —=0.0010 | -+0.0002 0.9547 66.5810 |+ 8| 61.8090 |+ 9 + 2.8958] — 0.6046 pr +11] 64.5680 |+19 + 0.1360| -+1.7037 65.3620 |-+19| 63.0255 |-+12 + 1.6785| <+1.6975 ps so vil 61.2585 [+13 524458 --1.6074 +1.6972 | -+1.6859 | 1.0032 0.0061 | -+0.0002 1.6832 68.8780 |+16| 59.5160 |-+17 + 5.1908| -+1.6904 Scheinbare Decldiff. wie 60 A. 195 = 0.99325 1° $ = —0.00056 fs = 0.99257 is = —0.00085 № 18=— 29 Jf's = 0.99334 Js = — 0.00047 y = -+20° 57:0 140 + bd — >| = < = DOS nor сос ao m 8 Object. 61 A. P.-Kr. 0° mm 62.1483 62.1474 72.8289 28.6804 81.4551 31.1333 67.5570 68.6752 66.4275 66.8110 67.2030 66.4230 67.8130 67.1980 66.4350 66.8200 67.2115 66.4505 - 66.8220 67.1970 64.9735 64.9710 64.9835 64.9850 69.4430 69.4400 69.4540 69.4590 63.1245 63.1155 63.1310 63.1310 70.9210 70.9205 70.9355 70.9405 ti P.-Kr.180° mm 10000 Я ооо 00 00 OO 00 O0 O0 © ЕЕ ЕЕ НЕЕ НН Scalenablesung. mm 66.2386 66.2376 55.5505 99.6994 46.9317 97.2410 60.8217 59.7074 61.9775 61.5855 61.2050 61.9805 61.5950 61.2105 61.9690 61.5885 61.1945 61.9525 61.5820 61.2080 63.4165 63.4220 63.4050 63.4060 58.9440 58.9480 58.9340 58.9280 65.2615 65.2690 65.2530 65.2560 57.4700 57-4715 57.4550 57.4530 Q— BR У W— t+kl „mm: nme! 10000! 10000 mm +-10 +14 +15 о я 9 +10 og во +10 +10 +10 +11 +10 +10 11 mr © ето +10 +10 +10 +10 HI Scheinbare Ædif: M—Centrum = +11:3000 т о nm 0.0000 ЕЕ ЕЕК ЕН У 2.8240 2.8200 2.8347 2.8350 7.2948 7.2913 7.3052 7.3 108 0.9764 0.9681 0.9838 0.9822 8.7710 8.7698 8.7855 8.7890 К. RENZ, 1896. April 14. Л? = 0.99294 — —35.3898 =-#20.3575 fa = 0.99259 = —32.6797 —=-+ 5.7115 — + 6.7152 f'a = 099296 h m ay = 8 8.4 —i°, = —0.00018 : —iy = —0.00028 Refr. = + 11 Try —=+ 52 Jy = =+0.00035 ео AR . 150, , 2 at Pulkowaer Sternzeit En = der Aufnahmen. Mittel. | mm D) nf 2—3 2 11° 167 0° 2—3 2 etwas ellipt, a 2—3 + 4.6574 II Tim, N} 2—3 — 4.6531 г 89) 2—3 R 11} 8,36 | —= 4.6641 Te) 2 —+ 4.6663 то 2 2 Trabant — Jupiterscentrum. авы | Mittel. | У’) Ja (и-уз) Ph. | Ac 058 | м. - 1 Я —I, 331 ME ac 0 Li __1'R9 A ci | —1.8204 1.8318 1:8189 | -+0.0002 0:0028 | —1:8215 | оз À —1.8313 2—3 ne = +2. — en -+2.6403 | 2.6217 | —0.0002 | —0.0028 | +2,6187 | ; ie 2.6445 2—3 — 3.6810 is — 3.6850 + Lars 2— | —3.6803 —3.6826| —3.6566 | -+-0.0003 0.0028 | —3.6591 | 3 — 3.6841 2—3 | —=4.11 36 2—3 1 +-4.1167 er sale à 2—3 pee 4.1186 | -+4.0896 0.0003 0.0028 | +-4,0865 2—3 и +-4.1227 2—3 À x de > у IT и Scheinbare Decldift: M—Centrum POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1896. April 14. Хаби) | Лаба) era] Ph. —+-11.2118 — 16.7078 num +38.4948 би =-+20° 53:9 ihe. Decl. Scalenablesung. ; R Zr A P.-Kr.90°|t--| P.-Kr.270° Le 3 mm mm mm | 10000 = 10000] 10000 = 63.7388 64.6540 a Г 63.7379 |-+ 9| 64.6524 |+16| о 0.0000 — 74.5689 |+13| 53.8122 |- 6] — 1|+10.8362 75-0948 |-+24| 53.2940 |-+23|— 4] +11.3576 46.9597 |-+16| 81.4286 |+20|-+- 3] —16.7768 46.9627 |-+20| 81.4153 |+30|+ 7| —16.7685 | 52.1475 |+11| 76.2346 |+ 8|+- 1| —11.5857 | 102.4940 | 6| 25.3940 |+25|—17| +38.7550 | 67.2770 |- 8| 61.1305 |411 + 3.5307 66.9045 |+ 8| 61.5000 |-11 — 3.1597 + 3.1595 66.5320 |+ 8| 61.8710 |+10 + 2.7880 65.5505 |-16| 62.8590 |+10 + 1.8036 65.1800 |+16| 63.2250 |+10 + 1.4354 + 1.4391 64.8220 |+16| 63.5810 |+ 9 + 1.0784 63.8000 |+ 8| 64.6095 |+17 + 0.0524 63.4325 |+ 9| 64.9715 |+17 — 0.3123 — 0.3124 | 63.0680 |-= 9|- 65.3370 |-17 — 0.6773 | 60.3915 |+14| 68.0110 |+19 3.3524 60.0330 +14] 68.3720 |-+-19 — 3.7122 — 3.7084 59.6825 |-+14| 68.7190 |-+14 — 4.0606 Ма | Mittel. mm mm бо + 3| 61.0365 |+10 + 3.6172 О 5.6350 |+10| 62.7590 |+ 9 — 1.8956] -+0.4565 | 63.8850 |+ 8| 64.5070 |+16 Ре 04586 | A 60.4940 |+14| 67.9000 |-+18 — 3.2456| -+0.4628 66.2420 +11] 62.1470 |-+11 + 2.5051| —0.6544 64.5200 |+17| 63.8690 |+10 + 0.7834] —0.6557 —0.6538 | 62.7720 |+10| 65.6205 |-+12 — 0.9668] —0.6544 5 || 59.3790 |--т1| 69.0120 |+15 — 4.3591] —0.6507 67.7800 |+19| 60.6105 |+10 + 4.0428] —<+0.8833 | 66.0590 |+11| 62.3280 |+ 9 + 2.3232] 0.8841 | зо 8853 64.3080 |+ 9] 64.0790 |- 8 + 0.5722| -+0.8846 г бо.9т80 |-+11| 67.4720 |+ 8 — 2.8192| -+0.3892 | 65.9990 |+11| 62.3940 [+11 + 2.2601| —0.8594 64.2765 |+ 9| 64.1152 |+10 + 0.5382| —0.9009 | _ 00 62.5245 |-+10| 65.8675 |-+12 — 1.2140} — 0.9016 2 59.1330 +II| 69.2610 |+15 — 4.6066| — 0.8982 -+10.7648 f°5 = 0.99322 —16.6718 fs = 0.99263 — 11.5042 f's = 0.99323 ео. , — 5 96511 тт 0.0000 0.0060 0.0592 0.0191 0.0495 0.0015 0.0023 22225 x? <. y— 7 tgösin 1’ mm 0.0000 -+-10.8302 —+-11.2984 —16.7959 — 16.8180 — 11.5872 +38.7527 Trabant — Jupiterscentrum. +-0!4558 | —0!0007 —0.6494 | +0.0010 +-0.8793 | — 0.0014 —0.8939 | 0.0015 $25 = +-0.00034 is = 0.00014 Js = -+0.00037 —0'0008 —0.0018 —=0.0012 — 0.0031 X щ=-505 Bemerkungen zur Aufnahme. Bilder 4. Undurch- sichtige Luft. Bilder 3. +-0/0002 —+0.0002 -+0.0002 —0.0002 18* 141 +0:4561 —0.6500 — 0,8793 —0.5953 142 G1 5. Scalenablesung. DR © P.-Kr. 0° | = Р.-Кг.180° ++ Anhaltstlerne| wie 61 А, mm mm mm 10000 10000] 10000 mm mm Zf: | 57.860 |+ 9| 71.3250 |+-13 fe | 57.4400 |+ 9| 70.9625 |+-13 Jo | 57-8080 |+ 5| 70.5950 |+13 %hy | 57.0630 [+10] 71.3390 |+12 he | 57-4355 [10] 70.9645 |412 ho | 57.8160 |+ 6| 70.5865 |+12 Z%p | 57.0410 |+-10| 71.3550 |+12 Te 97.4130 |#+10| 70.9930 |+12 о 57.7960 |+ 6| 70.6190 |+12 4kp | 57.0515 |+ı1] 71.3520 |+13 ke | 57.4325 || 70.9790 [+13 ko 57.8070 | 7| 70.6025 |+13 If | 55.6100 |— ı| 72.7890 |+14 h | 55.6030 0] 72.7920 |+13 à 55.5875 0] 72.8075 |+13 k | 55.5935 |+ ı| 72.7975 [+14 ПЛ | 60.0945 |+14| 68.2940 |+19 № | 60,0945 |+-ı14| 68.2935 |-+18 à 60.0795 |-+15| 68.3135 |+-18 k | 60.0880 |-+15| 68.3025 |+19 ШТ | 53.7300 |+ 3| 74.6610 |1 й | 53.7255 |+ 4] 74.6645 |+-10 À 53-7060 |+ 4| 74.6835 [+10 Е | 53.7105 |+ s| 74.6770 [+11 IV f | 61.5770 | 9] 66.8170 |+ 9 h | 61.5745 | 9] 66.8190 |+ 8 $ 61.5575 [+10] 66.8370 |+ 8 k 61.5720 |+10| 66.8240 |+ 9 Scheinbare Adiff. wie 61 A. mm — 5.0746 SER OS PRIE PQ 4.7163 4.3488 5.0930 4.7194 4.3404 5.1120 4.7450 3666 1052 7282 3 4. 5. 4. 4.3529 6.5451 6.5500 6.5655 6.5575 2.0548 2.0546 2.0720 2.0623 8.4208 8.4246 8.4439 8.4384 0.5748 0.5770 0.5945 0.5808 F. Rexz, 1896. April 14. № 3 mm — 4.7132 — 4.7079, — 4.7412 — 4.7288 Pulkowaer Sternzeit der Aufnahmen. 21, 38 23 3 2) И 24 45 Mittel. 114 23” 15° Trabant — Jupiterscentrum. Lt—Ly | Mittel. mm mm —1.8319 —1.8324 —1.8243 —1.8287 —+-2.6584 +-2.6630 +-2.6692 +-2.6665 —3.7076 — 3.7070 — 3.7027 — 3.7096 4.1384 4.1406 -+4.1467 4.1480 — 1.8293 —+2,6643 — 3.7067 +4.1434 — 1/8164 —+2.6456 — 3.6807 +-4.1143 Fa = 0.99294 fa = 0.99259 Г’, = 0.99298 —+0!0003 | —0!0028 | —1!8189 “ri 3 | 2—3 | -+0.0004 | —0.0028 | -+2,6432 à | 3 2—3 4 —0.0006 | —0.0028 | —3,6841 3 | 2—3 2 ищегехрошег +-0.0006 | —0.0028 | -+4,1121 5 R Ч 3 » п —1°,, = —0.00018 f —iy — —0,00028 x i,=+ "10 EN: = + 13 7,” = 0.006 Уи) Tu бииз РВ. | Ac cos 5 151 Bilder. | 2—3 Ostrand у | waschen. 2—3 | 2—3 3 unterexponie 1 sihe. Scalenablesung. D mm 61.8355 62.1710 62.5210 65.4320 65.7850 66.1410 67.1770 67.5245 67.8795 68.9570 69.3155 69.6710 62.6300 66.2415 67.9785 69.7660 61.5110 65.1205 66.8580 68.6460 63.0640 66.6760 68.4145 | 70.2030 || 61.2610 {| 64.8720 || 66.6110 {| 68.3960 | — Scheinbare Decldiff. wie 61 A. Anbaltstlerne POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. wie 61 A, mm 66.5790 66.2350 65.8855 62.9820 62.6180 62.2670 61.2315 60.8840 60.5280 59.4510 59.0890 58.7385 65.7685 62.1555 60.4180 58.0295 66.8860 63.2755 61.5360 59.7500 65.3310 61.7185 59.9785 58.1880 67.1380 63.5320 61.9705 59.9980 P.-Kr.90° |t+R] P.-Kr. 270°| +R | 1596. April 14. Пес]. Y mm mm 10000] 10000 mm и — 1.9142 +11 — 1.5744 +11 — 1.2246 +10 + 1.6830 +10 -+ 2.0412 +10 + 2.3947 SEIT + 3.4303 +11 + 3.7783 +11 — 4.1338 п + 5.2108 п + 5.5710 11 + 5.9242 +13 — 1.1117 +12 + 2.5006 +7 + 4.2380 +13 -+ 6.0262 + 9 — 2.2298 —+-10 + 1.3804 +10 + 3.1186 +15 + 4.9056 +20 — 0.6762 +13 — 2.9363 —18 —+ 4.6758 +9 —= 6.4656 +8 — 2.4808 + 8 + 1.1280 + 9 + 2.8678 +14 —= 4.6568 ©? #=-20° 53:9 ZntBctH%s mm — 1.5711 + 2.0396 —+ 3.7808 + 5.5687 Yt— Ya | Mittel. mm +0.4594 —+0.4610 +-0.4572 —=0.4575 —0.6587 —0.6592 —0.6622 — 0.6631 —0.8949 —0.8967 —0.8950 0.8969 —0.9097 —0.9116 —0.9130 —0.9119 тт —0.4588 — 0.6608 —0.8959 — 0.9116 198 = 0.99322 fs =0.99263 f's = 0.99325 ns PE — 7295 sin 1 seh ’ у— = 19631 1 Trabant — Jupiterscentrum. T's (91—92) | 75 (24—22) Не-а) Ph. ! | +-0:4557 —0.6563 —0,8899 —0.9054 —0/0007 —+O.00!1I —0.0015 +-0,0017 175 = -+0.00034 ig =-0.00014 Ту = -+0.00040 — 00012 —+-0.00I0 — 0.0027 0.0012 X ig = +0! 143 Bemerkungen zur Aufnahme. Bilder 3—4. Durch Wolken. —+0.0002 —0'0002 —0.0002 0.0002 5 45 —=0:4540 —0.6540 0,8859 —0,9023 144 Е. Вами, 62 A. 1896. April 19. № 152 Scalenablesung. Pulkowaer Sternzeit Object. IE be ER PES a a Bilder. P.-Kr. 0° th) P.-Kr.180° |1-+-%k der Aufnahmen. | Mittel. mm im mm 10000] 10000 en en Cir. | 62.9103 65,4697 У 62.9094 65.4680 о 0.0000 2 M 66.6505 61.7269 O| + 3.7414 2 N 22.5049 105.8712 H-20| —40.4005 ; ол 2 Q 75.2866 53.0956 — 1|-+12.3753 11° 38 30 1—2 R | 24.9704 103.4093 —19] — 37.9368 2 14 61.3835 66.9919 0] — 1.5244 1—2 т 62.4911 65.8924 ©] — 0.4210 2 ZA | 65.6460 62.7585 + 2.7236 Ag 66.0355 62.3665 + 3.1143 + 3.1166 1172802730 2 Go 66.4390 61.9750 + 3.9118 Zby | 65.6165 62.7800 + 2.6980 SR 2 be 66.0060 62.3920 + 3.0868 + 3.0833 Di LE 11 31 20 *) | 1—2 b, 66.3890 62.0185 + 3.4650 % Co 65.6235 62.7765 + 2.7032 Ce 66.0110 62.3920 + 3.0892 —= 3.0902 раз 2 m 66.4030 |+10| 62.0060 + 3.4782 % dy | 65.6555 |H-10| 62.7430 + 2.7360 de 66.0305 |+-10| 62.3730 + 3.1084 —= 3.1079 32 4 WS 1 dy | 66.4005 |-+-10| 62.0010 —= 3.4794 N Trabant — Jupiterscentrum. Ber | Mittel. ие) Лау Ph. | Az cos à mm mm Та | 65.2160 |-+17 т + 9 —- ве 2 b | 65.1870 |-+17| 63.2010 |- 9 == —0.8102| _ A , EE Em 2—5 verzerrt, с | 65.1860 I+16| 63.2010 |+ 9 SE 0.8176 0.8152 0'8095 | -+-0!0002 0.0028 0:8121 9—3 а | 65.2025 |-+16| 63.1880 |+-10 == — 0.8206 2—3 Па | 64.5250 |-+17| 63.8620 |+ 8 + —1.5050 2 b | 64.4995 |+17| 63.8860 | 8 + —1.4964 | = en + _4 1051 | 2—3 с | 64.5000 |+16| 63.8875 |+ 8 + —1.5038 1.5031 1.4927 | -+0.0004 0.0028 1.4951 2—3 d | 64.5140 |+16| 63.8730 |+-9 — — 1.5073 2 Ша | 69.9020 |-+17| 58.4850 |- 5 + —+-3.8722 2—3 6 | 69.8670 |+16| 58.5140 [+ 5 + —3.8735 Le 1 2 с | 69.8740 [+16] 385100 №5 5 17.8720 -+3.8705 |. 3.8436 0.0011 0.0028 | -+3,8897 | 5__g d | 69.8850 |-+16| 58.5010 |+- 6 + +-3.8643 IV а | 71.4830 |-+12| 56.9035 |+ 9 + +-5.4530 2—8 ellipt. b 71.4470 |+11| 56.9420 |+ 9 + —+-5.4490 le nm 2—3 с | 71.4565 +1 56.9355 [+10]. < =5.4500 —5.4500 | -+5.4121 0.0016 0.0028 | 5.4077 | 5_3 d | 71.4700 |11| 56.9180 |-+-Io + 5.4479 2 N Scheinbare Ва: M—Centrum = + 3'9700 f° x = 0.99302 —1°,, = +0.00078 N— » = —42.7108 р h } Q— » = +-13.0277 Fa = 0.99264 —iy = +0.00065 x = —2!2 R— » = — 40.0097 Refr. = + 14 и я = — 1.6183 Шао, = 34 We = — 0.4148 Г» =0.99304 Ja = —0.90113 h m 0.) = 8 9.9 *) Die Correction des Chronometers ist unbekannt; —0° angenommen. Der Fehler übersteigt jedenfalls nicht #5°. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 145 1896, April 19. ihe. Decl. Я Scalenablesung. иен x? to Hi $ x? 198 a Bemerkungen : mi (OC erg: г Aufnahme. Р.-Кг.90® | 1-5 P.-Kr. 270° | +5 - г : я тт _mm_ JE 10000 10000 110000 mm mm mm mm 63.1516 65.2274 63.1506 65.2258 |-+26 0,0000 0.0000 0.0009 73.7270 54.6507 о ern: — 0.0007 —+10.5759 74.2466 54.1343 |+201— 6|-+11.0938 — 0.0862 -+11.0076 46. ex 82.2630 |+ 5|+ 2] —17.0348 — 0.0078 —17.0426 Bilder 4. Mond- 46.113 82.2618 |-+18 ER — 17.0347 — 0.0742 — 17.1089 schein. Undurch- SI. 2 77-0695 |+ 9| 9] —11.8426 — 0.0001 — 11.8427 sichtige Luft. 101.6496 26.7394 |+22[—17|+38.4904 0.0000 +3 8.4904 ‚68.2450 60.1680 |-:5 + 5.0766 67.8690 60.5310 |+11 + 4.7072 + 4.7059 67.4950 69.9040 |+11 + 4.3338 61.9745 |+10 + 3.2714 62.3360 |+10 + 2.9024 + 2.9021 62.7075 |+Io + 2.5326 3.7080 |+ 9 + 1.5355 64.0635 |+ 9 + 1.1766 — 1.1723 64.4350 |+ 9 —+ 0.3048 65.4675 +11 — 0.2260 65.8140 |+11 — 0.5750 — 0.5762 66.1690 |+11 — 0.9277 Trabant — Jupiterscentrum. Yt—Yz Mittel. |f'a(ye—Y2) | 8 (21—25) Har-222) 2) mm тт | 60.3380 |-+15 + 4.8926| —<+0.1867 a ae: = er cos +0.1874 | +0/1861 | —o!o004 | --o/ooo2 | +o0!o002 | -+0!1869 65.6180 |+11 — 0.3847| -0.1915 60.1800 |-+14 + 5.0511| -+0.3452 Be Ex à Le El re +-0.3449 | -+0.3425 | -+0.0007 | -+0.0004 | -+0.0002 | -+0,3438 65.4620 |+16 — 0.2290| -+0.3472 61.5270 |+I1 + 3.7043| —1.0016 a Bot: ЕЕ о Send —1.0035 | —0.9968 | —0.0019 | —0.0022 | -+0.0002 | —1.0007 66.8090 |+10 — 1.5796] —1.0034 61.9250 |-+12 + 3.3074 вы Ba ET + в PR —1.3998 | —1.3905 | —0.0027 | —0.0035 | +o.0002 | —1.3965 67.2065 ни — 1.9716] —1.3954 ; | cheinbare Decldif: M— Centrum = +10:5028 f°5 = 0.99337 $5 = —0.00050 N— » = + 10.9497 Q— » —= —16.9338 fs = 0.99270 5 =— 0.00076 X 13 = —2.6 R— » = —16.9698 У— » = 11.7662 f's = 0.99335 Js = —0.00049 W—- » = +38.2328 Зап. Физ.-Мат. Отд. 19 146 К. Rexz, 62 B. 1896. April 19. № 1 Scalenablesung. Г Pulkowaer Sternzeit | ne z Part EI ва А а PO RENE Bilder. — P.-Kr. 0° | 2. Р.-Кг.180° ++ 5 der Aufnahmen. Mittel. : Anhaltstierne! wie 62 A, mm mm mm 10000 10000] 10000 mm mm mm mm #9 | 57.7460 |+ 5| 70.6585 |+13 = 641779 ‚а Ie 58.1170 |+ 5| 70.2820 |+17 — 4.8034 — 4.8000 De ze 5 2 do 58.5020 |+ 5| 69.8995 |+17 — 4.4196 ho | 97.8240 |+ 5| 70.5775 |+12 — 5.0974 LA 58.2070 |+ 5| 70.1930 |-+16 — 4.7138 — 4.7110 44 37 2—3 Ро 58.6005 |+ 5| 69.8025 |+16 — 4.3218 ui 44" 56°) LAS 57.7890 |+ 6| 70.6190 [+12 — 5.1356 te 58.1650 |+ 6| 70.2415 |-16 — 4.7590 — 4.7951 AS NE 2 10 58.5520 |+ 6| 69.8520 [+16 — 4.3708 Aka | 57.7715 | 6| 70.6285 |+-16 5.1493 ke | 58.1605 |+ 6| 70.2345 |+-16 AIS — 4.7567 45 50 2 ko 58.5600 | 6) 69.8445 |+16 — 4.3630 Trabant — Jupiterscentrum. фт» | Mittel. Ir u) Тиз) Ph. | Aa cos à mm mm Та 57.2475 |- 9] 71.1390 |-+13 — 5.6662 = > 2—3 h | 57.3375 |+ 9| 71.0510 |+r2 — 5.5772] —0.8662 | __ rn р в, _p 2—3 р 7.2925 |+10| 71.0930 |-r12 — 5.6206] —0.865; 0.8669 0.8609 | —0:000т 0:0028 | —0:8686 | 5 k | 57.2860 |-+10| 71.0980 |+12 — 5.6264| —0.8697 2 По | 56.5750 + 9] 71.8150 |+12 — 6.3404] —1.5404 2—3 h 56.6615 |+ 9| 71.7255 |-11 — 10.2524] Т.И IE ke pi Ne 3 ; s6.6210 |+10| 717650 |+rı — 6.2924| —1.5373 1.5411 1.5304 | -+0.0001 0.0028 1,5331 1 о Е | 56.6115 |+10| 71.7750 |+11 — 6.3021] —1.5454 2—5 UT g | 61.9610 |+ 9| 66.4210 |+11 — 0.9504] 3.8496 2—5 h | 62.0575 | 9| 66.3275 |+1ı — 0.8554] 3.8556 2 er + À 9= | 2—3 $ 62.0115 +9 66,3740 = — 0.9016] -+3.8535 —=3.8524| -+3.8256 0.0003 0.0028 | +3,8225| о 1 62.0095 |-10| 66.3800 |+10 — 0.9056] 3.8511 2—3 IV д | 63.5380 | 8| 64.8550 |+r16 + 0.6208| 5.4208 5—3 ищегехр, | h | 63.6295 + 8| 64.7605 |+17 + 0.7138] +5.4248 di 3 | $ 63.5880 |+ 8| 64.8045 re +- 0.6710 5.4261 5.4239 | #355-386 3} 15.0.0005 0.0028 | -+50831 2—3 | Е | 63.5835 |+ 9| 64.8080 |+16 + 0.6671] -+5.4238 1—2 | Scheinbare №. wie 62 A. F x =0.99302 —i° = +0.00078 fa = 0.99264 —iy = -+0.00065 : , у — = 196 зщ 1 Trabant — Jupiterscentrum. Bemerkungen zur Aufnahme. : | т] S Yı 9% | Mittel. | "(гул 7-2 вп) Ph. 42 mm mm +-0:2107 or +-0.2068 | -+0:2054 | -+0.0004 —0!000$ | +0!0002 | +0:2055 0.2045 —=0.3642 м. +0.3644 | -+0.3620 | +0.0007 | —o.0010 | -+0.0002 | 0,3619 +0.3637 TE En —0.9989 | —0.9923 | —0.0017 +0.0012 | +0.0002 | —0,9926 — 1.0012 — 1.3993 Re —1.3959 | —1.3867 | —0.0024 | <+o.0012 | +0.0002 | —1.3877 — 1.3990 3 f°5 = 0.99337 #5 = —0.00050 fs = 0.99270 is = —0.00076 X is = —.2'6 f's = 0.99338 Js = —0.00045 ANDRE SRE HOOTURU VORE MATT ааа ибо Я Un OL Hé Е Eee. rad rA0t9éE ee $ LT ых | | É + LE задала чай : Weis et | ‘East: =. я wert un ug dm en nu mern nt eng ет her < 7 2 а 4 — Zn 2e | MAT du AT A À , | NZ à EEE RE 7e N | er, | ь 5 L | м a cdi, wer iv De, ae N $ > Ar e « Ur м FAR $ 19* > Г nr QC! =. > мой + © В. OPPOSITION 1897. HELSINGFORSER CLICHES. Г RATÉ 150 Е. Renz, 63 A. 1897. März 22. R 154 Scalenabl | Helsingf S t calenablesung. elsingforser Sternzei Object. ä s | © Евы неа ВИ: РЕН АННА Mes Bilder. P.-Kr. 0° | ++ Р.-Кг.180° | ++ | :: der Aufnahmen. Mittel. mm mm mm у 100000 mm 10000! 10000 Ctr. | 65.3417 63.0334 г z T 65.3400 |+17| 63.0325 |+ 9] oo] 0.0000 D а J 44.3412 |-+20| 64.0344 |— 7|+ 2] —20.9992 2—3. eiförmig. F 14.7530 |[+30| 113.6212 |+ 6|+38| —50.5832 12% 55" 29° 4 ellipt. Н |113.7608 | 4| 14.6158 |-+27|—33|-+48.4139 5 Sd 4—5 ellipt. JE 70.6112 |+18| 57.7622 |+10|— 1|+ 5.2706 3 K 68.7330 |-+19| 59.6470 |+21| ol + 3.3888 2 ZA | 57.8530 + 8| 70.5400 |-18 — 7.4982 Ag 58.3460 + 8| 70.0540 |-18 — 7.0086 — 7.0091 12 49 43 3 Ay 58.8320 |+13| 69.5645 |+18 — 6.5206 Ybw| 57-8575 |+ 7] 70.5430 |+17 — 7.4974 D, 58.3340 [+ 7| 70.0580 |-+-17 — 7.0166 — 7.0150 39 7 3—4 b, 58.8190 |-+12| 69.5720 |+-17 — 6.5309 % Cap | 57.8745 + 7| 70.5245 |+17 — 7.4796 ПЖ Ce 58.3490 |+ 7| 70.0510 |+17 — 7.0056 — 7.0034 so 43 12° 50° 40 3—4 60 58.8275 +12] 69.5685 |-17 — 6.5249 %@ | 57-8775 |+ 6| 70.5205 |+-16 — 7.4762 de | 58.3690 + 6| 70.0315 |-+16 — 6.9859 — 6.9873 SNS ‚|3 do | 58.8530 |+11| 69.5440 |+16 — 6.4999 3 em | 57.8390 + 6| 70.5560 |-+16 — 7.5132 à ec | 58.3310 + 6| 70.0715 |+16 — 7.0249 — 7.0271 SI 30 34 Hi eo | 58.8075 |+11| 69.5850 |-+16 — 6.5432 Ч к | Trabant — Jupiterscentrum. Я Lt — Ty | Mittel. | Pa (tt—22) T{vt—Va)| Ph. | До cos à N mm mm > Га | 59.0700 |-+13| 69.3110 |-+15 — 6.2748| +0.7343 3—4 р b | 59.0740 |-+12| 69.3095 |+14 — 6.2720] -+0.7430 Е 4 | € | 59.0905 [+12] 69.2960 |-+14 — 6.2570] -=0.7464 | -+0.7432 | 0/7420 | —0:0004 | —0:0007 | +0:7409 | 4 | а | 59.1005 |-+-11| 69.2765 |+-13 — 6.2422| 0.7451 4 е 59.0650 |+11| 69.3160 |-+13 — 6.2798| 0.7473 4 р Па | 59.4960 |+17| 68.8740 |+1s — 5.8430] +1.1661 3 | b | 59.4940 |+-16| 68.8765 |+14 — 5.8453| +1.1697 2—3 | с 59.5050 |+15| 68.8715 |-+14 — 5.8374| -+1.1660 | 1.1658 | -+1.1639 | —0.0c05 | —0.0007 | 1.1627 | 3—4 fi а | 59.5195 1$| 68.8570 |+13 — 5.8228] -+1.1645 3 р В е 59.4765 |-+15| 68.8975 |+13 — 5.8646| 1.1625 3—4 nicht kreismt III a | 61.8560 |+11| 66.5220 |+ g — 3.4870| 3.5221 2—3 Ai b | 61.8460 |+10| 66.5260 |+ 9 — 3.4941| +3.5209 2—3 : с | 61.8605 |-+то| 66.5140 |+ 8 — 3.4808| 3.5226 | 3.5203 | -+3.5144 | — 0.0016 | —0.0007 | 3,5121 | 3 à 4 | 61.8710 +10] 66.5045 |+ 8 — 3.4708| +3.5165 2—5 _№ е | 61.8355 |+ 9] 66.5430 |+ 8 — 3.5078| 3.5193 2—3 nicht kreitä l |. ТУ Verfinstlert. т Scheinbare Adiff: J— Centrum = —23'4035 f° y = 0.99824 —i°, = -+0.00130 Е » =—56.4487 H— » = 53.9938 fax = 0.99796 —м =—+0.00130 X Ty =— 45 K— » — + 3.8043 Вей’. = + 18 В Ре, =2353 Try =— 43 | udn Г’, = 0.99833 Л.» = 0.00105 4 ау = 10 17.9 | ‘ | SE POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 151 1397. März 22. leihe. Decl. E: | Scalenablesung. Ant то би D ele Bemerkungen à - 5 у —— — —tg6 sin 1’ y — > tgù sin 1’ [Р-Кг. 90°] 2+5] Р.-Кт.270? |5 т zur Aufnabme. LL. pee un | 64.3980 63.9980 ss jr "# 62.4915 |+10 0] + 1.4984 0.0000 + 1.4984 62.7660 |+ı8| o|+ 1.2230 — 0.0317 — 1.1913 53.3185 |-+24]— 10] -+10.6716 — 0.1855 +10.4861 | 58.6680 |-+28|— 4|-+ 5.3250 — 0.1695 + 5.1555 49.7375 78.6398 |+ 9] 1] —14.6512 — 0.0020 — 14.6532 | 80.7602 47.6195 |-+20]— 1|-+16.3700 — 0.0008 -+-16.3692 72.6840 55.7220 o + 8.2818 | 72.2280 56.1940 о —= 7.8176 + 7.8166 | 71.7490 56.6485 |+10 + 7.3504 F 71.1400 57.2640 |+10 —= 6.7382 70.6840 57.7280 |+ 6 + 6.7784 + 6.2791 | 70.2190 58.1790 | 6 — 5.8206 | 69.6705 58.7365 |+ + 5.2672 | 69.2210 59.1960 |+11 + 4.8127 + 4.8109 À 68.7545 59.6490 |+15 + 4.3528 68.2100 60.1865 |-+15 + 3.8120 67.7555 60.6580 |+11 + 3.3492 — 3.3504 | 67.2895 61.1095 |+11 + 2.8900 | 66.7180 61.6900 |+ 9 + 2.3140 66.2660 62.1470 |+10 — 1.8596 —= 1.8547 65.7895 62.6090 |+10 — 1.3904 Ё Trabant — Jupiterscentrum. T Fawva)\Is@-en)-er-,| Ph | № Ve Va | Mittel. mm mm 56.5425 |+10 - 7.4474| —0.3692 58.0820 |+ 6 + 5.910т| — 0.3690 59.5500 |-+15 + 4.4395| —0.3714 | —0.3704 | —0.3699 | —0!0007 | -н0:0003 | -но'осот | —0:3702 61.0180 |-+-11 — 2.9760] — 0.3744 62.5055 |+10 + 1.4866] — 0.3681 56.6180 |+-10 + 7.3714] — 0.4452 58.1540 |+ 6 + 5.8356] —0.4435 59.6240 |+15 + 4.3632| —0.4477 | —0.4462 | —0.4456 | —0.0011 +-0.0004 | —-0.0001 — 0,4462 61.0870 |+11 —+ 2.9040| —0.4464 62.5875 |+10 + 1.4064| —0.4483 57.6140 + 5 + 6.3769] —1.4397 59.1450 |+10 + 4.8434| —1.4357 60.6170 |+10 + 3.3692| — 1.4417 | —1.4394 | —1.4373 | —0.0032 —=0.00тт | -+0,0001 —1.4393 62.0830 |+ 9 —= 1.9076| —1.4428 63.5735 |+ 8 + 0.4174] —1.4373 Scheinbare Decldif. J—Centrum = — 0.2845 1°5 = 0.99816 325 = —0.00116 Е » — + 9.0345 H— » = + 3.5977 fs = 0.99775 iz =— 0.00119 X ig = —4!1 K— » =-+14.8397 1— » = — 16.1255 fs = 0.99855 Js = —0.00095 dy = +12° 0.8 | | Scalenablesung. 65.3436 65.3420 44.3355 14.7498 113.7555 70.6070 68.7245 59.7995 60.2795 60.7610 59.8025 с 60.2725 60.7390 59.8235 Ce 60.2930 бо 60.7720 59.8055 с | 60.2835 60.7490 59.8380 ee 60.3180 ео 60.7890 | SUSE AUS RR IR 62.2510 62.2335 62.2580 62.2335 62.2745 59-5340 59.5190 59-5470 59.5250 59.5590 57.9580 57.9450 57.9760 57.9570 57.9930 51.5350 51.5185 51.5425 51.5285 51.5615 = = + Len | -ч = SUN t-+k| P.-Kr.180° 63.0447 63.0438 84.0428 113.6348 14.6310 57.7740 59.6525 68.5965 68.1225 67.6280 68.5975 68.1280 67.6515 68.5710 68.1020 67.6165 68.5930 68.1175 67.6400 68.5655 68.0845 67.6040 66.1300 66.1520 66.1165 66.1470 66.1040 68.8440 68.8615 68.8335 68.8570 68.8245 70.4190 79.4335 70.4000 79.4175 79.3850 76.8545 76.8670 76.8420 76.8570 76.8290 Scheinbare Adiff: F. Renz, 1897. März 26. mm —+-1.9786 —+1.9683 -+1.9711 —1.9622 ==1.9704 —0.7368 —0.7436 —0.7428 —0.7469 —0.7476 —2.3130 J—Centrum == —23'4036 = — 56.4491 —=-53.9942 = 107 5.0676 5.0771 5.0499 5.0685 5.0346 Helsingforser Sternzeit der Aufnahmen. 10° 44“ 51° | я 40 42 SI 20 45 12 Mittel. 10° 40” 17° Trabant — Jupiterscentrum. mm —+1.9701 — 0.7435 — 2.3131 — 8.7460 Л? = 0.99824 fax = 0.99794 Fa = 0.99822 —1'9666 — 0.7422 —2.3090 —8.7304 —1° —0/0008 0.0004 0.0009 —=0,0036 —0'0008 —0,0008 — 0.0008 —0.0008 а = 0.00126 Ве. =+ Т. Ty Je 2 = +0,00098 = -+0.00128 2 3 ага | Mittel, Раба), у) Ph. | Au cos à —+1:9650 — 0.7426 — 2.3089 —8.7276 Bilder. | 3—4 2—3 4—5 ellipt. 4—5 } 3—4 2 2—3 D 4 3—4 deformiei® 3 dreieckig. 3—4 3 3—4 3 deformiert. ihe. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 153 1397. März 26. Decl. р т || Scalenablesung. into ee DR En che Bemerkungen ki a у МЕНЕ — — + tgù sin Г У — tgèsinl1 zur Aufnahme ‚Ра #1 P.-Kr. 2709 t+k 3 2 Art ыы À м | mm | тт iz 10000] 10000 m т т тп _ 63.3980 63.9980 5; Bi Р 64.3972 3.9971 [+ 9 о 0.0000 0.0000 0.0000 | 64.1155 64.2620 |+17| 0|— 0.2734 — 0.0317 — 0.3051 т | 73.5705 54.8165 |+16|— 7|+- 9.1770 — 0.1856 + 8.9914 Luft 2. | 68.2208 |+35| 60.1635 |-+32|— 3|-+ 3.8285 — 9.1695 + 3.6590 48.2470 |+20| 80.1410 |-+-10|-+ 1] —16.1464 — 0.0020 —16.1484 79.2612 |+ 7| 49.1136 |-+14|— 1|+14.8734 — 0.0028 —14.8726 | 63.0080 |-+10| 65.3890 |-+10 — 1.3905 | 62.5570 |+10| 65.8625 |+10 — 1.8528 — 1.8526 62.0855 |-+10| 66.3145 |+10 — 2.3145 61.5310 |-+11| 66.8680 |+ 8 — 2.8684 | 61.0790 +11) 67.3325 |+ 8 — 3.3266 — 3.3254 60.6160 |+11| 67.7775 |+18 — 3.7811 | 60.0795 |+т15| 68.3210 |+18 — 4.3209 1 59.6200 |+15| 68.7890 |+13 — 4.7844 — 4.7819 59.1580 |+15| 69.2400 |+13 — 5.2404 | 58.5870 69.8170 |+16 — 5.8155 | 58.1415 70.2840 |+16 — 6.2718 57.6765 70.7230 |+12 — 6.7236 | 57.1460 71.2530 |+12 — 7.2536 56.6895 71.7110 |+11 — 7.7108 56.2230 72.1760 |-r11 — 8.1766 I 61.6950 | в | 58.7580 | 57-2755 55.8350 | 62.9290 | | 61.4490 | | 59.9860 58.5090 57.0700 63.4210 61.9450 60.4780 8.9930 | 57.5520 | 66.2425 | 64.7630 | 63.3020 | 61.8180 | 60.3710 al Trabant — Jupiterscentrum. sas | Bene: [Из из) 7 (ешо) ara) Ph. mm mm 66.6940 |-+ 8 68.1650 |+-18 69.6320 |-+16 71.1160 |+712 72.5585 |+13 65.4515 |+17 66.9310 |+ 9 68.3950 |+19 69.8770 |+17 71.3140 |+13 64.9570 |+17 68.4370 |411 67.8965 |+-19 69.3850 |+14 70.8235 |-+13 62.1540 |+14 63.6260 |+13 65.0870 |-+21 66.5740 |+13 68.0135 |+-23 2.6994] —0.8468 4.1724| —0.8470 5.6372] —0.8553 | —0.8496 | —0'8482 | —o!ooao | -+0!ooos | -+olooo2 | —0/8495 7.1204] —0.8501 8.5624] — 0.8487 1.4616| -+0.3910 2.9408| -+0.3846 4.4046] —0.3773 | -+0.3861 | 0.3855 | 0.0007 —0.0002 | -+0.0002 | -+0,3862 5.8842| -+0.3861 7.3221| <+0.3916 0.9683| -+0.8843 2.4460| -+0.8794 3-9094| -+0.8725 | <+0.8776 | -+0.8762 | —+-0.002; —0.0009 5.3961| -+0.8742 6.8360] -+0.8777 1.8443| -+3.6969 0.3689] -+3.6943 ; 1.0928| -+3.6891 | —-3.6930 | -+3.6869 | -+0.0087 —0.0051 | +0.0002 | -+3,6907 2.5780] 3.6923 4.0214| -+3.6923 —=0.0002 | -+0,8788 EB 1 PRET Scheinbare Decldiff: J—Centrum = + 0/2845 195 =0.99814 12; = —0.00112 u Е— » = + 9.0346 H— » =+ 3.5977 fs = 099771 is — —0.00103 X 13 —=— 35 L— » = +14.8397 К— » = — 16.1256 Г’; = 0.99834 I; = —0.00100 dy = +12° 8/3 Зап. Физ.-Мат. Отд. 20 154 Е. Renz, 63 CC. 1297. März 22. Scalenablesung. Helsingforser Sternzeit Bilder. DEEE) 5 ИЯ À a 0 P.-Kr. 0° 1-й Р.-Кг.180° |i+k L der Aufnahmen. Mittel. mm mm mm Fa 10000] um 10000116000] zum Lu Ctr. | 65.1968 63.1930 I 65.1952 |-+16| 63.1920 3 J 44.1860 |+10| 84.1902 — 21.0024 2 Е 14.5805 |-+28| 113.8102 — 50.6118 11 27 0’ 4 Н |118.618$ |+ 3| 14.7728 -+48.4164 = 4 Г 70.4898 |-+25| 57.8960 + 5. 8 K 68.5495 |-+18| 59.8218 = 1 % ap | 69.5530 |-+17| 58.8440 + ас | 69.9945 |+17| 58.4000 Е -= 4.7993 II 20 30 2 ао | 70.4465 |+17| 57-9450 Fb: 2 by | 69.5430 |-17| 58.8560 + LP 70.0050 |-+17| 58.4035 — —+ 4.7985 DI 738 1—2 bo | 70.4500 |+17| 57.9385 = 7% Cywy | 69.5410 |-+16| 58.8570 —- y Е Ce | 69.9945 |16| 58.4075 + + 4.7910 22.220 1 2-м 2 Co | 70.4395 |-+16| 57.9560 a 2% dy | 69.5635 |+16] 58.8390 + de | 70.0135 |+-16) 58.3915 + + 4.8103 23 8 2 do | 70.4595 |+16| 57.9355 + % exp | 69.5425 4-16) 58.8550 + €g | 69.9985 |+16| 58.4125 = + 4.7939 ! 281753 2 ео 70.4470 |-16| 57.9480 En Trabant — Jupiterscentrum. Lt—Xy | Mittel. ее) I (ye—y2)) РВ. Au. cos à mm mm | à Та | 71.0810 |+13| 57.3045 + +1.0871 3 1 b 71.0770 |-+13| 57.3040 |-+11 + —+-1.0862 3 | e | 71.0705 |+12| 57.3185 |+10 + 1.0832 | -+1.0826 | -+1.0805 | —0o:0013 | —0:0009 | -+1'0783 | 3 | d | 71.0875 |+12| 57.2945 |+10 nn +-1.0844 2—3 | e 71.0615 |-+12| 57.3255 |<+10 —- — 1.0723 3 | Па 71.8690 |-+13| 56.5145 |+12 = +-1.8761 2—3 | b | 71.8670 |-+12| 56.5155 [+11 + +1.8753 3 2—3 e | 71.8535 |-+12| 56.5200 |-+-10 + +-1.8740| +1.8778| -++1.8741 | —0.0029 | —0.0009 | +1,8703| 2—3 : В Я | 71.8835 |+11| 56.4935 |+-10 + +-1.8829 2—3 1 е | 71.8685 |11| 56.5160 [+10 —- -+1.8805 3 | Ша | 74.7555 |-+12| 53.6195 |- 6 + +-4.7671 2 b | 74.7535 |-+11| 53.6190 |+ 6 + —+4.7671 2° - № с | 74.7465 |-+11| 53.6285 + 5 + -+4.7664 | +-4.7682| -+4.7588 | —0.0068 | —0.0009 | +4,7511 | 2 | а | 74.7720 I+10| 53.6035 |+ 4 + 4.7723 1-2 4 e | 74.7505 [+10] 53.6235 |+ 4 — —4.7680 2—8 ellipt. | IVa | 62.9575 |+ 9| 65.4320 |+-17 — — 7.0389 3 | b | 62.9575 |+ 9] 65.4305 |+-17 = — 17.0373 2—3 № с 62.9455 | 9| 65.4395 |417 — — 7.0406 | —7.0375 | —7.0236 | 0.0095 | —0.0009 | —7,0150 | 3 4 d | 62.9675 |10| 65.4125 |+16 — — 7.03 50 3 | е | 62.9530 |+10| 65.4325 |+16 — —7.0359 3 { Scheinbare Ædiff: J— Centrum = —23:4037 Fa = 0.99802 —1, = +-0.0029$ у И = —56.4493 5 . , Н— » =-+53.9944 fa = 0.99773 —iy = 0.00296 X = — 10.2 К— » — + 3.8044 Refr. = + 6 DI» = - 5.8354 Tenir 30 f’u = 0.99803 Л. = —0,00332 А m ay — 10 13.8 PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 15 1597. März 2=. Le ih е. Рес]. | Scalenablesung. „2 aim" d „2 95 sin 1” Bemerkungen Jpxr.00° ++ Р.-Кг.270° |+ À р НН | - mm тт | тт | во 10000 65980 10000]10000] zum Lam ‚Be Di 61.3728 67.0168 |+ 9] 0] — 3.0220 0.0000 — 3.0220 61.0525 67.3248 |-+17|-+ 1] — 3.3360 — 0.0317 — 3.3677 70.4735 57.9180 |+22]— S|-+ 6.0778 — 0.1856 —+ 5.8922 | 65.2858 63.1008 |+27| о|-+ 0.8928 — 0.1695 + 0.7233 | 45.2302 63.1575 |+11]+ 2] — 19.1630 — 0:0020 — 19.1650 52.1328 |+12| o|+11.8560 — 0.0008 —+11.8552 71.3715 [+14 — 7.3690 70.9470 |+14 — 6.9417 — 6.9414 70.5120 |-+14 — 6.5134 69.8970 |-+18 — 5.8994 69.4805 |+-15 — 5.4760 — 5.4739 | 69.0485 |-+15 — 5.0464 | 59.9410 68.4530 |-+20 — 4.4562 | 60.3700 68.0335 |+20 — 4.0320 — 4.0294 60.8010 67.6005 |+20 — 3.6000 | 61.3750 67.0180 |+10 — 3.0215 „61.8210 66.5970 |+10 — 2.5880 — 2.5896 | 62.2390 66.1575 |-+12 — 2.1594 62.8750 65.5220 |+18 — 1.5239 63.3080 65.1010 [+18 — 1.0969 — 1.0983 | 63.7235 64.6710 |+18 — 0.6742 Trabant — Jupiterscentrum. veux | Mittel. етих о ее) |ее-альт| Pi. | 48 D mm mm | 57.0290 71.3570 |+15 7.3642] —0.4228 : 58.4910 69.8920 |+19 — 5.9012] —0.4273 , 68.4440 |-+21 — 4.4513| — 0.4219 — 0.4223 — 0.4216 —0.0029 —0:0004 | -+0/0002 — 0/4247 67.0060 |+11 —1 3.0135 0.4239 65.5080 |+13 — 1.5139| —0.4156 71.8070 |+14 — 7.8112| —0.8698 70.3423 |-+19 — 6.3528| —0o.8789 d 68.8920 |+16 — 4.9010] —0.8716 | —0.8741 | —0.8726 | —0.0051 —0.0007 | -+0.0002 — 0.3782 67.4550 |+11 — 3.4660| — 0.8764 65.9645 |+13 — 1.9721| — 0.8738 55.3870 72.9900 |+17 — 9.0022| — 2.0608 56.8490 71.5285 |-+ı5 — 7.5398| —2.0659 58.3010 70.0755 |-+20 — 6.0878| —2.0584 | —2.0620 | —2.0585 | —0.0129 —0.0022 | -+-0.0002 — 2.0734 59.7335 68.6405 |-+17 — 4.6534| —2.0638 | 61.2270 67.1455 |-+12 — 3.1592] — 2.0609 || 60.3085 68.0800 |+18 — 4.0861| -+2.8553 Ni 61.7720 66.6190 |+ 8 — 2.6234| +-2.8505 | | 63.2150 65.1700 |-+16 — 1.1778] -+2.8516 | -+2.8521 | -+2.8472 | 0.0190 —0.0005 | 0.0002 +-2,8669 {| 64.6555 63.7350 |+ 8 + 1.2607| -+2.8503 ыы 62.2395 |+ 9 + 1.7544| -+2.8527 à | Scheinbare Decldif. J-—Centrum —— 0,2844 f° 3 = 0.99806 12; = —0.00282 | F— » = + 9.0346 > | H— » = 3.5976 fs —0.99765 ig ——0.00278 x u=— 96 | К— » = -+14.8397 | L— » © ——16.1257 J's = 0,99830 Js = —0.00270 dy = -+12° 11.9 Qt 156 К. Renz, 63 D. 1897. März 30. AR 157 Scalenablesung. Helsingforser Sternzeit И ee Dee, €. ® Zu FREI = Bilder. P.-Kr. 0° |{+k| P.-Kr. 180° i-+-%k E der Aufnahmen. Mittel. mm mm mm_ an 10000] mm 10000] 10000] am т Ctr, | 65.4268 62.9510 JA 65.4252 |+16 62.9500 |+-IO 0.0000 2—3 | J 44.4180 |+20| 63.9558 |— 6|+ ааа 3 Е 14.8242 |+28| 113.5532 |+ 3|+38| —50.5974 11^ 15” 17° 4 ellipt. Н |113.8458 |+ 2| 14.5320 |+26|—33| 48.4145 4—5 ellipt. L 70.6850 |-21| 57.6875 |+12|— 1 + 5.2612 2—3 К 68.8080 |-+17| 59.5655 |+18 + 3.3833 1—2 % Gp | 72.4290 |+14| 55.9760 |— 1 — 6.9894 ас | 72.8905 |+14| 55.5110 |— I + 7.4526 + 7.4583 II 5 2 2—3*) Go | 73-3680 |-+14| 55.0280 |— I + 7.9328 4b | 72.4395 |-+14| 55.9620 |— I + 7.0016 be 72.9240 |-+14| 55.4850 |— I + 7.4824 + 7.4786 5.34 2—5 bo | 73-3815 [+14] 55.0035 |— 1 + 7.9518 . Ze 72.4375 |#-14| 55.9710 |— 1 — 6.9961 т та 72.9020 4-14| 55.5050 |— I + 7.4614 + 7.4640 CNE 11% 6" 21° 2—3 бо 73-3675 |-+14| 56.0245 |— I + 7.9341 % dy | 72.4245 |+15| 55.9730 | © + 6.9886 de 72.9130 |+15| 55.4950 о + 7.4718 + 7.4730 7026 2 do | 73-3910 15 54.9995 о + 7.9586 Zen | 72.4005 |+16| 56.0050 о + 6.9606 ес 72.8859 |-+16 55.5160 о + 7.4478 + 7.4489 и 2—3 во | 73.3665 +16 55.0155 о + 7.9384 Trabant — Jupiterscentrum. х— 2, | Mittel. |\f’„(@r—2z) Тоби из) Ph. | До cos 6 тт тт I Geht du/rch |die Jupiter| schelib Па | 70.1960 |+-17| 58.1760 |-+ 5 + 4.7727| — 2.6856 3 | b | 70.2255 +17| 58.1500 |+ 5 + 4.8004] — 2.6782 3—4 | с | 70.2050 +18] 58.1665 |+ 6 + 4.7820] —2.6820| —2.6824| —2'6773 | 0,0020 | —o'oo10| —2:6763 | 3 | 4 | 70.2175 |+18| 58.1590 |+ 6 + 4.7920] —2.68 то 3—4 | е | 70.1870 |+19| 58.1850 |+ 7 + 4.7637| —2.6852 3—4 | Ша | 73.4225 |+14| 54.9550 I + 7.9966] +0.5383 2—5 **) | b 73.4245 |+14| 54.9270 |— I —= 8.0216| +0.5430 2—3 | с | 73.4315 |+14| 54.9460 I + 8.0056| +0.5416| 0.5405 | -—н0.5395 | —0.0002 | —0.0010| 0,5383 | 3 | d | 73.4360 |-+15| 54.9370 о + 8.0124] -+0.5394 2—5 | е 73.4120 |+I6| 54.9595 [6) + 7.9892] +-0.5403 2—3 | [У а | 71.2480 |+13| 57.1370 |+ 9 + 5.8178] —1.6405 3—4 | b | 71.2655 |-+13| 57.1220 |+ 9 — 5.8340] —1.6446 3—4 с | 71.2540 |-+14| 57.1280 |+-10 + 5.8253] —1.6387| —1.6386| —1.6354 | -+0.0009 | —0.0010| —1.6355 | 3 | 4 | 71.2650 +14] 57.1180 |+10 + 5.8358] — 1.6372 4 | е 71.2475 |-+15| 57.1380 |+II + 5.8170| —1.6319 4 | | Scheinbare ЖАШ. J—Centrum = —23:4037 195 = 0.99806 —i° „= 0.00116 FOURS — —56.4495 ? : И = -+53.9945 fa = 0.99777 — = 0.00117 x i„=— 40 ‚ К » — + 3.8044 Refr. — + г I— » = + 5,8355 Та = + Ло = 0.99806 Зо =". 00168 h т НОО Ито: 2 *) Trabant IH stört bei Einstellung auf den Ost-Rand. **) Einstellung schwierig, da der Trabant mit dem %-rande zusammenfliesst. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1597. März 30. + пе. Пес]. Scalenablesung. x мине, | P.-Kr.90° #1 P.-Kr. 270° | 5+5 _mm_ _mm_ | 10000 10000] 10000 и _ 61.3980 63.9980 Rz ; ` 60.0965 |+-14| 68.5810 — 4.3875 M 59.7250 |+21| 63.6525 — 4.6637 69.1865 |+31| 59.1994 + 4.7934 63.8298 |-+25| 64.5530 — 0.5620 43.8545 |+-20| 64.5270 —20.5350 M 74.8792 |+11| 53.5058 —=10.4850 ` 64.9050 |-+19| 63.4955 + 0.5051 65.3535 |-+19| 63.0580 + 0.9481 + 0.9543 65.8050 |+19| 62.5865 + 1.4096 66.3925 |+11| 62.0090 + 1.9917 | 66.8400 |+11| 61.5710 + 2.4344 + 2.4374 67.2820 |+11| 61.1095 + 2.8862 67.8340 |+21| 60.5645 + 3.4352 68.2880 |+21| 60.1280 —= 3.8804 + 3,8816 68.7260 |--16| 59.6680 + 4.3292 69.3080 |+-16| 59.0885 + 4.9099 69.7655 |+19| 58.6410 + 5.3626 + 5.3652 | 70.2190 |+19| 58.1740 + 5.8230 | 70.7400 |+-15 57.6595 + 6.3406 71.1950 |-+15| 57.2150 + 6.7902 + 6.7888 71.6350 |+15| 56.7640 — 7.2356 | yr—ÿ2 | Mittel. mm mm Geht du/rch |die Jupiter j 66.5485 |+ 9| 61.8370 + 2.1556] -++1.2013 68.0245 |-+19| 60.3605 + 3.6322] 1.1948 69.4705 |+-14| 58.9105 + 5.0801] +-1.198$ | -н1т.2011 70.9600 |+13| 57.4270 + 6.5666] -+1.2014 2.3910 +12] 55.9955 + 7.9983] -+1.2095 65.2250 [+19] 63.1490 + 0.8384| —0.1259 66.7040 |+11| 61.6740 + 2.3150] —0.1224 68.1475 |+21| 60.2295 —+ 3.7592] —0.1224 | —0.1204 69.6405 |+19| 58.7400 + 5.2506| —0.1146 71.0650 |+15| 57.3210 + 6.6722| —0.1166 | 65.8980 |+11| 62.4980 + 1.5000] -+0.5457 67.3680 |+ 9| 61.0215 + 2.9730] -+0.5356 ‚68.8120 |+14| 59.5810 + 4.4154] +0.5338 | -+0.5403 70.3000 |-+17| 58.0900 + 5.9054] -+0.5402 ‚71.7320 |+12| 56.6625 + 7.3348] -+0.5460 | | Scheinbare Decldif: J—Centrum = — 0'284 195 = 0.99813 mu = 9.0347 | H— ‘5 = + 3.5976 fs —0,99771 | К— » = +14.8397 | L— » = —16.1257 f's = 0.99835 | =-+12° 15.2 тт 0.0000 0.0317 0.1856 0.1695 0.0020 0.0008 Вы Trabant — Jupiterscentrum. fly —y3) | Ja (2—2) wa | jp +1/1991 —0.1202 +-0.5394 2 x A, 7 tgd sin 1 —+-0/0026 — 0.0005 +-0.0016 4° 5 = —0.00109 iz = —0.00103 Js = —0.00097 x? née y — = tgù sin 1” mm — 4.3875 — 4.6954 —+ 4.6078 — 0.7315 —20,5370 —10.4842 —-0/0011 —0.0002 -0,0007 X 15 = —35 +-0/0002 —+0.0902 —+0.0002 Bemerkungen Durch Wolken. exposition. — zur Aufnahme. Windstoss bei der letzten Jupiters- м——Ш—ы "À + | Ph. | A5 +-1:2030 —0.1207 0,5419 1 re EINE be 158 Е. Renz, re 64 A. 1896. April 15. № Scalenablesung. Helsingforser Sternzeit “© а рол ПВ Ce ee 8 x Pan Mae, Bilder, _ P.-Kr. 0° [55 Р.-Кт.180° ik 3 der Aufnahmen. Mittel. mm mm mm 10000 10000] 10000 Ctr. | 60.3665 68.0103 ze м ый 60.3650 |-+15| 68.0085 |+-18| о 0.0000 2—3 J 39-3622 |+25| 89.0132 |— 7|-+ 2] —21.0018 2 Е 9.7758 |-+22| 118.5990 |+ 8|-+39] — 50.585 1 13 41” 36° 3 ellipt. H | 108.7960 |+ 19.5875 |--24|—34|+48.4218 4 K 63.7838 |-+14| 64.5942 |+23|— 1|+ 3.4162 2—3 L 65.6082 |+-16) 62.7670 |+-14| ©] -н 5.2426 2 % Gp | 51.3230 |+13| 77.0605 |+11 — 9.0468 de 51.8420 |+14| 76.5580 |+-II — 8.5360 — 8.5362 13: 5 610221 3 Go 52.3435 |+14| 76.0395 |+ 9 — 8.0258 bp | 51.3555 |-+12| 77.0390 |+10 — 9,0198 я Une b. | 91.8500 |+13| 76.5515 |+10 — 8.5287 — 8.5227 HEC 13 37 58 3 b, 52.3550 |+13| 76.0385 |- 8 — 8,0196 % Cp | 51.3240 |+-12| 77.0630 |-+то — 9.0475 Ce 51.8420 |-+13| 76.5655 |+10 — 8.5397 — 8.5415 371188 3 бо 52.3375 |-+13| 76.0565 |+ 8 — 8.0374 2 dy | 51.2960 |-н11| 77.0835 |+ 9 — 9.0718 de | 51.8115 |+12| 76.5880 |+ 9 — 8.5662 — 8.5653 38 16 3—4 dy | 52.3210 |+12| 76.0810 |+ 7 — 8.0578 Ze | 51.3160 |-+11| 77.0705 |+ 9 — 9.0552 ес 51.8300 |-+12| 76.5745 |+ 9 — 8.5502 — 8.5493 38 48 3 Es 52.3290 |-+12| 76.0580 |+ 7 — 8.0424 | Trabant — Jupiterscentrum. 4—2 | Mittel. А] Eh? | Aa. cos ö mm тт Та | 50.6530 |+13| 77.7345 |1 — 9.71881 — 1.1826 3—4 b 50.6715 |+12| 77.7195 |+ 9 — 9.7020] —1.1793 3—4 с | 50.6500 |+12| 77.7355 |+ 9 — 9.7207| —1.1792 | —1.1814| —ı!1793 | —0:0004 | —o!0016 | —1:1813 | 3 d | 50.6270 |+11| 77.7605 |+ 8 — 9.7447| — 1.1794 3—4 е | 50.6380 |+11| 77.7535 | 8 — 9.7357| —1.1864 3—4 Па | 54.5555 |+ 2| 73.8205 |+13 — 5.8112] 2.7250 3—4 b 54.5830 |+ 1| 73.8055 |+13 — 5.79006] 2.7327 3—4 с | 54.5550 0] 73.8290 |+-12 — 5.8157| +2.7258 | 2.7298 | +-2.7249 | -+0.0010 | —0.0016 | 2,1243 | 3—4 d | 54.5405 ©] 73.8465 |+12 — 5.8317] +2.7336 3—4 e 54.5555 0| 73.8325 |+12 — 5.8172| 2.7321 3—4 Ша | 47.1280 |-+12| 81.2455 |+-17]+ 1] — 13.2370] —4.7008 3 b | 47.1440 |+12| 81.2315 |+16|#+- |—13.2220] —4.6993 3 e | 47.1195 |+12| 81.2565 |-+1$|+ 1]—13.2466| —4.7051 | —4.7014| —4.6931 | —0.0016 | —0.0016 | —4.6963 | 3 4 | 47.1035 |+12| 81.2720 |+15|+ 1| —13.2624| —4.6971 | 3—4 е 47.1105 |+12| 81.2620 |+15|+ 1] —13.2539| —4.7046 3—4 IV а | 48.5020 |-+16| 79.8840 |+11|+ 1) —11.8688| —3.3326 4 unterexponi b | 48.5240 |-+16| 79.8640 |+10|+ 1| —11.8477| —3.3250 4 > 0 e | 48.4970 |+16| 79.8895 |+ gl 1|—11.8730) —3.3324 | —3.3274 | —3.3215 | —0.0010 | —0,0016 | —3,8241 | 4 » а | 48.4875 |-16| 79.9060 |+ 9|-+ 1|—11.8869] —3.3216 4 e 48.4950 |-+16| 79.8895 |<+ 8|-= 1] —11.8748| —3.3255 4—5 Scheinbare ВАШ: J—Centrum = — 23.4042 fa = 0.99808 —°,, = — 0.00050 F— » — —56.4510 у H— » =-+53.9960 Л» = 0.99778 —iy =-— 0.00051 X и = + 1.8 K— » = + 3.8047 Refr. = + 30 L— » = 5.8358 Ту ==. 405 а Ло = 0.99824 Ju =— 0.00076 а = 10° 11.7 пе. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. P.-Kr.90° 62.2988 65.2458 _ 65.0035 74.5092 68.9895 80.1078 49.0842 72.7720 72.2970 71.7850 71.20C0 70.7340 70.2360 69.8140 69.3375 68.8380 68.3480 67.8740 | 67.3935 | 66.8940 66.4200 65.9230 72.8115 71.2510 | 69.8500 | 68.3870 66.9370 71.0640 69.5065 68.1010 67.6390 65.1910 _ 74.2960 _ 72.7330 71.3295 69.8650 68.4190 | 73-5640 71.9960 70.5990 69.1265 67.6810 Scheinbare Decldiff: tt P.-Kr.270° Е re п t+k mm mm mm 10000] 1000| zum 66.0918 63.1415 |+ 9] 0|-+ 2.9490 63.3760 |+21 О] + 2.7105 53.8695 |+24|—10|+12.2158 59.3980 |+-26|— 6| + 6.6918 48.2685 |+19|— 2|-+17.8154 79.2970 |+ 7|+ 1] —13.209$ 55.6270 |+ 4 —10.4697 56.1090 |+ 4 + 9.9911 56.0050 |+ 4 — 9.4871 57.1940 |+14 + 8.8996 57:6780 |-+10 + 8.4248 58.1515 |-10 + 7.9393 58.5860 |-+15 + 7.5108 59.0700 |-+15 + 7.0304 59.5490 |-+15 + 6.5412 60.0480 |+15 + 6.0469 60.5350 |415 + 5.5665 61.0040 |-+15 + 5.0916 61.5000 |+-14 + 4.5934 61.9870 |-+14 + 4.1130 62.4860 |+-14 + 3.6150 55.5850 |+ 5 10.5104 57.1360 |+15 — 8.9541 58.5420 |+16 + 7.5508 60.0025 |-+20 — 6.0889 61.4515 |-+16 —+ 4.6391 57.3190 |-+12 + 8.7692 58.8825 |-+13 —= 7.2088 60.2860 |-+17 + 5.8042 61.7470 |+12 — 4.3424 63.1940 |-+12 + 2.8954 54.0860 |+10|— 1|-+12.с018 55.6550 |- 6|— 1|-+10.4360 57.0490 |-16|— 1| + 9.0362 58.5110 |+17|— 1|-н 7.5736 59.9560 |+21|— 1|-+ 6.1280 54.8335 |-+ 6|— 1| -+11.2622 56.3975 |+ 7|— 1|-+ 9.6962 57.8005 |-+12|— 1|-+ 8.2959 59.2670 |+17|— 1| + 6.8264 60.7100 |-+17|— 1|-+ 5.3817 » 1897. April 15. Decl. J—Centrum = — 0,2843 —=-+ 9.0350 — = 359975 = -+14.8398 = — 16.1262 ’ dy = 12° 32'4 пн сн; —+ 9.9826 + 8.4212 + 7.0275 + 5.5683 + 4.1071 тт -+0.5278 —=0.5329 +-0.5233 -+0.5206 +-0.5 320 — 1.2134 — 1.2124 — 1.2233 — 1.2259 — 1.2117 +-2.0192 —+-2.0148 —=2.0087 —+-2.005 3 —-2.0209 +-1.2796 +1.2750 -+1.2684 —+1.2581 —1.2746 тт +0.5273 —1.2173 —+2.0138 -+1,2711 198 = 0.99810 15 = 0.99768 15 = 0.99867 x? mm 0.0000 0.0317 0.1856 0.1695 0.0008 0.0020 RIRE TT $05 sin 1’ ER N y— 5 tgösinl mm —= 2.9490 + 2.6788 —+12.0302 + 6.5223 17.8146 — 1372016 Trabant — Jupiterscentrum, : T У:— | Mittel. ir С. (из) Js (го) -ве-аль Ph. +-0!5266 —1.2157 —2.0III —+1.2694 —0/0011 -+0.0026 —0.0044 —0,003 1 $25 = +-0.00061 159 Bemerkungen zur Aufnahme. Luft 3—4. —0:0008 | 0.0004 —0.0012 | -+0/0004 —0.0034 | +-0.0004 —0.0022 | -+0.0004 X = +! 9 —+0:5251 —1.2115 2.0037 +-1,2645 160 Е. Renz, 64 1$. 1897. April 18. 159 Scalenablesung. Helsingforser Sternzeit а Object. 8 я Bilder. P.-Kr. 0° += P.-Kr.180° |t+% . der Aufnahmen. | Mittel. | mm ln 10000 me 30000| 10000 im kan Ctr. | 60.4272 67.9568 I 60.4258 |-+14| 67.9550 |+-18 2 J 39.4142 |-+-24| 68.9615 |+13|+ $ 2 | Е 9.8235 |--21| 118.5520 |+ 7|+38 12° 96" 24° 3—4 stark ellipt} Н |108.8488 |+ 5| 19.5335 3—4 ellipt. K 63.8175 |-+13| 64.5600 2—3 L 65.6848 |+17| 62.7012 2 % y | 50.4890 |+10| 77.8970 de 50.9470 |+10| 77.4575 — 9.4873 125 Ро 2—3 *) Go 51.4015 |+-10| 76.9960 4b 50.4780 |4-10| 77-9150 -= be 50.9380 |10| 77.4685 — 9.5019 20 46 122 a2 3 bd, 51.3810 |+I0| 77.0140 % Co 50.4930 |--10| 77.8990 = 6 50.9430 |-+10| 77.4620 — 0.4937 210626 3 © 51.3840 |-+10| 77.0100 == %а | 50.4765 |+10| 77.9090 de 50.9350 |+10| 77.4650 — 9.4986 21 54 2—3 do 51.3895 [+10] 77.0075 %е, | 50.4920 |+11| 77.8940 ee | 59.9365 |+11| 77.4580 — 9.4915 22 26 3 ео 51.3930 |--11| 77.0070 |-+-I1 Trabant — Jupiterscentrum. Mae | Mittel. | щаз) угу Ph. | Au cos 8 mm тт Та | 52.8090 |+ 7| 75.5830 |+ 8 — 1.8651 3 b | 52.7895 [+ 7| 75.5990 |+ 8 — +-1.8619 93 с | 52.8005 |+ 7| 75.5870 |+ 8 — 7.6286] +1.8652 | -+1.8628 | —1.8592 | —o!ooo2 | —0:0018 | +1:8572| 3 d | 52.7915 [+ 8| 75.5955 |+ 9 — 7.6372] +1.8614 3—4 e 52.7975 | 8| 75.5890 |+-10 — 7.6310] -+1.8605 3 II Bedeckt. Ша | 54.6000 |— ı| 73.7730 |+13 — 5.8224| +3.6649 3 b 54.5865 1| 73.7900 |+13 — 5.8376| 3.6643 x 3 € | 54.6025 ol 73.7760 |+14 — 5.8226] +3.6711| -+3.6655 | -+3.6585 | —0.0003 | —0.0018 | -+3,6564 | 3 d | 54.5890 | ©] 73.7870 |+14 — 5.8349] —3.6637 3 e 54.5945 |+ 1| 73.7790 |-+15 — 5.8282] 3.6633 3 IV а 56.2395 |— || 72.1420 |+12 — 4.1871| —+5.3002 3 b 56.2230 |— 1| 72.1640 |+12 — 4.2064| +5.2955 3 с | 56.2395 ©] 72.1510 |+-13 — 4.1916| +5.3021| +5.2978| -#+5.2877 | —0.0005 | —0.0018 | 5,2854 | 3 а 56.2280 O| 72.1595 |+13 — 4.2016] +-5.2970 5 ' e 56.2325 + 2| 72.1555 |-+14 — 4.1973| +-5.2942 3 | Scheinbare Ædiff: J—Centrum = —23'4043 Fa = 0.99804 —1° y, = 0.00069 F— » = —56.4512 Be > = 53.9963 fx = 099776 —iy = +0.00069 Хх = —24 К— №» — + 3.8047 Refr: = + 2 L— » =-+ 5.8359 Tr „m Г’, =0.99819 Ja ый 00021 ty — 10 11.4 *) Jupitersbilder von einer leichten Aureole umgeben. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 161 1897, April 18. he. Decl. | Scalenablesung. 5 к пен; = 495 sin I’ И х2 tgd sin 1/ Bemerkungen | P.-Kr. 90° tt P.-Kr. 270° | ++ \ = ê U _mm mm mm 10000 10000] 10000 on À | 62.2988 66.0918 = Ei; $ 63.7448 | 9) 64.6408 |+16| ol + 1.4482 0.0000 —= 1.4482 Luft 3. 1 63.4865 |+19| 64.8920 |+28| o|+ 1.1933 — 0.0317 + 1.1616 72.9610 |+30| 55.4292 |+20|— 9] +-10.6620 — 0.1856 +-10.4764 67.5410 |-+41| 60.8420 |-+26|]— 4] + 5.2464 — 0.1695 — 5.0769 78.6182 |+ 6| 49.7632 |+ 5|— 1| 16.3240 — 0.0008 16.3232 47-5898 |-+19| 80.8010 |-+15|— 1| —14.7088 — 0,0020 — 14.7108 64.3495 |+13| 64.0540 |+14 + 2.0442 63.9240 |+13| 64.4905 |+-14 + 1.6132 —+- 1.6090 | 63.4670 |-+13| 64.9200 |-+22 — 1.1696 | 62.9130 |+14| 65.4820 |+16 + 0.6119 62.4840 |-+14| 65.9270 |+16 + 0.1749 — 0.1772 62.0470 |+14| 66.3500 |+16 — 0.2551 61.4405 |-+15| 66.9515 |+14 0.8590 60.9850 |-+15| 67.4015 |+-14 — 1.3117 — 1.3002 60.5670 |-+15| 67.8190 |-+24 — 1.7300 59.9915 |+19| 68.4025 |+19 — 2.3090 59.5650 +19) 68.8380 |+-19 — 2.7400 — 2.7421 | 59.1190 |-15| 69.2660 |-+19 — 3.1772 | 58.5185 |+10| 69.8990 |-+22 3.7944 | 58.0770 |+10| 70.3170 |-+22 — 4.2241 — 4.2239 57.6490 |+10| 70.7475 |+18 — 4.6532 | Trabant — Jupiterscentrum. У | Mittel. |fa(y—v2) |7 (&r—22) Нейт Ph | 48 тт тт 63.1150 |+13| 65.2760 |-r21 + 0.8156] —0.7934 | 61.6860 |+-13| 66.7025 |+13 — 0.6118| —0.7890 | 60.2050 |-+18| 68.1785 |+-23 — 2.0905| —0.7903 | —0.7926 | —0o'7911 | —olooos —-0'0010 | 0'0004 | —0:7902 58.7630 |+14| 69.6260 |+21 — 3-5354] —0.7933 57.2760 |+13| 71.1100 |+17 — 5.0207| —0.7968 | Bedeckt. | 62.2760 +12| 66.1075 |+13 — 0.0193| —1.6283 60.8495 |+13| 67.5355 +21 — 1.4469] —1.6241 {| 59.3680 |+13| 69.0145 |+-16 — 2.9269] —1.6267 | —1.6279 | —1.6248 | —0.0009 +0.0018 | -+0.0004 | —-1,6235 | 57-9220 +8 70.4545 |+-19 — 4.3703| —1.6282 56.4390 + 2| 71.9430 |+14 — 5.8561] —1.6322 61.5870 |+12| 66.8060 |+10 — 0.7129| —2.3219 60.1600 |+17| 68.2300 |+20 — 2.1386] —2.3158 58.6745 |+13| 69.7130 |+18 — 3.6230] —2.3228 | —2.3218 | —2.3174 | —0.0013 —0.0023 | 0.0004 | —2,3160 57.2330 |-+12| 71.1540 |+14 — 5.0641| —2.3220 | 55-7485 |+ 2| 72.6410 |+15 — 6.5504| —2.3265 Scheinbare Decldif: J— Centrum = — 0/2843 1°5 = 0.99779 1° 5 — —0.00042 F— » = + 9.0351 H— » =-+ 3.5975 fs = 0.99738 is =— 0.00043 X 15 = —1!S Е— :» = -+14.8399 L— » = —16,1263 f's = 0.99811 Js = —0.00024 dy = +129 33.7 Зап. Физ.-Мат. Отд. 21 162 Е. Renz, 64 С. 1897. April 33. № 16 Scalenablesung. р Helsingforser Sternzeit 1 Object. PIERRE N I ih le Lie ; т RARES ana) ни У EUR, ee | Bilder P.-Kr. 0° 22 P.-Kr.1800|t+% - der Aufnahmen. Mittel. mm mm mm un 10000! mm 10000|10000| nm Br Ctr. | 60.4204 67.9677 I 60.4190 |+-14| 67.9658 |+19| о 0.0000 2—3 J 39.4110 |--24| 88.9668 |— 6|-+- 2] —21.0026 2 Е 9.8230 |--21| 118.5618 | 6|-+37| — 50.5913 12% 18” 59° 3—4 ellipt. Н |108.8472 |+ s| 19.5358 |-+23|—33| +48.4252 3—4 » LAS 63.8142 |+13| 64.5625 |+21 ol + 3.3991 1—2 L 65.6685 |+18| 62.7070 |+15|— 1] + 5.2544 3 { ZG | 64.8450 |#17| 62.6535 |-+12 + 4.4196 ас | 65.3010 |+17| 63.1020 |-+12 — 4.8734 — 4.8719 2 | 5 ГО 2 Go | 65.7445 |-11| 63.5460 |-+12 + 5.3228 2b | 64.8120 |-17| 62.6775 |+11 — 4.3912 be | 65.2705 |4-17| 63.1325 |+-11 —+ 4.8430 + 4.8428 15 40 3 6%, | 65.7215 |+11| 63.5805 |+11 — 5.2942 %с, | 64.8900 |+16| 62.6140 |-+-10 + 4.4620 RR Ce | 65.3280 |+-16| 63.0580 |-+10 + 4.9090 + 4.9121 ОУ 12 16 7 2—3 27 65.7790 |+10| 63.4955 |+10 — 5.3654 % dun | 64.8545 |-+16| 62.6520 |+10 + 4.4252 de | 65.3050 +16] 63.1035 |-+-10 — 4.8747 + 4.8771 16 37 2—3 do | 65.7525 |10| 63.5370 |-нто + 5-3314 Zen | 64.8060 |+-16| 62.6820 |-+то —= 4.3860 ес 65.2610 |-+16| 63.1355 |+10 + 4.8367 — 4.8372 17 I 2—3 ео 65.7110 |+10| 63.5805 |+10 + 5.2889 Trabant — Jupiterscentrum. ne | Mittel. [Ищете Лии») Ph. | Aa cos à mm mm Та | 66.6355 |+-10| 61.7480 |-=12 + 6.2173] 1.3454 2—3 6 | 66.6085 |+ 9| 61.7780 |-+-L1 + 6.1888] -+1.3460 2—3 e | 66.6670 | 9| 61.7160 |+11 + 6.2490] +1.3369 | -+1.3428 | -+1'3402 | —0'0004 | —0:0019 | -+1'3379 | 3 а | 66.6410 |+ 8| 61.7440 |+10 + 6.2220] +-1.3449 2 e | 66.5990 |+ 8| 61.7900 |-+-10 + 6.1780] 1.3408, 2—3 Па | 66.2780 |-+12| 62.1110 |+12 —+ 5.8572] +0.9753 3 b | 66.2510 |-+11| 62.1320 |-+11 + 5.8332] -+0.9804 3—4 с | 66.3195 |+11| 62.0650 |-+11 + 5.9009] -+0.9888 | -+0.9856 | -+0.9837 | —0.0004 | —0.0019 | +0,9814 | 3 а | 66.2895 |--10| 62.0960 |+10 + 5.8704] 0.9933 2—3 e 66.2465 |+10| 62.1395 |+10 + 5.8272] -+0.9900 3 : Ша | 61.3610 |-+11| 67.0130 |+10 + 0.9477| —3.9242 2 b | 61.3325 |1c| 67.0390 |+ 9 — 0.9204| —3.9224 2 С 61.4045 |10| 66.9710 |+ 9 — 0.9904] —3.9217 | —3.9211 | —3.9136 | —+0.0013 | —0.0019| —3,9142 | 2—3 а | 61.3735 |[-10| 67.0015 |+ 8 + 0.9598] —3.9173 2 À e | 61.3330 |10| 67.0455 |+ 8 —= 0.9175] —3.9197 2 IV a | 69.5850 |+19| 58.7990 |+13 —+ 9.1670] <+-4.2951 3 b | 69.5590 |+17| 58.8275 |-+13 + 9.1396] -+4.2968 3 с | 69.6230 |+-17| 58.7635 |+12 + 9.2036] -+4.2915 | -+4.2950| +4.2868 | —0.0014 | —0.0019 | 4,2835 | 3—4 | а | 69.5935 |+16| 58.7895 |+11 + 9.1759] -+4.2988 3 | е 69.5490 |-+16| 58.7365 |-11 + 9.1302| -+4.2930 3 Scheinbare ЖАШ: J—Centrum = —23:4045 Ja 0.99805 —1° y = -+0.00042 F— » — — 56.4516 H— 5 = +53.9967 fx = 0.99777 —iy = -+0.00040 X 1, = —1l'4 K— » — + 3.8047 Вей’. = + 12 L— » — + 5.8360 Try = + 32 fo Л’. = 0.99810 Jy = +0.00084 а) = 10 11.1 > POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897. April 253. Decl. ıne. Scalenablesung. = $ y P.-Kr, 90° tt] P.-Kr. 270° [#+% mm mm mm 10000 10000] 10000] m | 62.2988 66.0918 : 62.2978 |-+10| 66.0908 |+10] о 0.0000 62.0362 |+19| 66.3430 |+22] о0|— 02570 71.5165 |-+34| 56.8722 |+29|— 7|-+ 9.2182 ` 66.0850 |-+27| 62.3000 |-+25|— з|-+ 3.7888 77.1685 |+ 9| 51.2115 ° |-+10] 0|-14.8750 46.1332 |-+14| 82.2488 |-+ 2|— 1] —16.1606 à 56.5270 |+ 9| 71.8740 |-+12 5.7772 56.9530 |+ 9] 71.4540 |+13 — 5.3542 57.3885 |+ 9| 71.0120 |+13 4.9154 58.0185 |+ 5| 70.3820 |-+17 — 4.2858 58.4645 |+ 5| 69.9445 |+17 — 3.8441 | 58.8900 + 9) 69.5100 |+17 — 3.4139 59.5090 |-+14| 68.8900 |-+14 — 2.7940 59.9430 |-+14| 68.4580 |+19 — 42.3012 | 60.3690 |-+14| 68.0265 |-+19 — 1.9325 60.9520 |+10| 67.4425 |+ 9 — 1.3487 61.3900 |+10| 67.0150 |+ 9 — 0.9160 61.8205 |+ 9] 66.5820 |+ 9 — 0.4842 | 62.3730 |+10| 66.0210 |-+11 — 0.0724 | 62.8060 |+ 9| 65.5935 |+11 + 0.5026 63.2350 |+ 9| 65.1625 +17 + 0.9314 A 56.4120 |— 1| 71.9765 |+12 — 5-8864 57.9095 |+ 5| 70.4725 |+17 — 4.3856 59.4010 |+10| 68,9880 |+14 — 2.8972 60.8430 |+10| 67.5380 |-+19 — 1,4514 62.2710 |+ 9] 66.1160 |+11 — 0.0261 | 56.4810 |— ı| 71.9180 |+13 — 5.8227 | 57.9820 |-+ $] 70.4080 |+18 — 4.3172 | 59.4730 |-+10] 68.9180 |-+15 — 2.8262 M 60.9170 |+10| 67.4720 |-+20 — 1.3815 _ 62.3365 |+ 9] 66.0515 |+12 + 0.0388 | 58.5500 |+11| 69.8340 |+16 — 3.7458 ` 60.0480 |-+15| 68.3315 |+18 — 2.2454 61.5340 |+10| 66.8460 |+- 8 — 0.7594 62.9795 |+10| 65.3940 |+16 + 0.6890 64.4030 |+ 9| 63.9800 |+ 8 + 2.1080 55.2490 0| 73.1420 |-+15 — 7.0508 56.7480 |+10| 71.6425 |+13 — 5.5509 58.2360 |+ 6| 70.1550 |+18 — 4.0636 59.6850 |+15| 68.7035 |-+15 — 2.6128 61.1055 |+11| 67.2815 |+10 — 1.1914 Scheinbare Decldiff: J—Centrum = — 0,2843 Е » = + 9.0352 H— » —=-+- 3:5974 K— » = +-14.8400 L— » — —16,1264 | | | | 6 = +12° 34'6 не; — 5.3489 — 3.8479 — 2.3626 — 0.9163 + 0.5021 тт —0.5375 —0.5377 —0.5346 — 0,5351 —0.5282 —0.4738 —0.4693 —0.4636 —0.4652 —0.4633 +-1.6031 —+1.6025 -+1.6032 +1.6053 +1.6059 — 1.7019 — 1.7030 —1.7010 — 1.6965 — 1.6893 mm —0.5346 —0.4670 -+1,6040 — 1,6983 198 = 0.99772 fs =0.99731 f's = 0.99802 x 2 “= ” — — tg8 sin 1’ 2 mm 0.0000 0.0317 0.1856 0.1695 0.0008 0.0020 RIRE 2 y— 195 sin 1’ тт 0.0000 — 0.2887 + 9.0326 —= 3.6193 —+14.8742 — 16.1626 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. bf'atiun)| Iateı—an terra] Ph. —0:5335 | — 00002 — 0.4661 —0.0002 —+1.6008 | -+0.0007 — 1.6950 | —0,0007 $} = —0.00034 13 =— 0.00034 J3 = —0.00017 Bemerkungen zur Aufnahme. —0:0005 | +-0/0004 —0.0003 | -+0.0004 +-0.0008 | -+0.0004 —0.0019 | -+0.0004 X 15 = —1:2 165 —0:5338 — 0.4662 —+1.6027 — 1.6972 164 64 D. Scalenablesung. (Object. P.-Kr. 0° |t-+k| P.-Kr.180° mm 10000 Ctr, | 60.4194 67.9684 7 60.4180 |-+14| 67.9665 J 39.4080 |-+24| 88.9665 Е 9.8190 |-+20| 118.5668 Н |108.8402 |+ 4| 19.5448 K 63.8150 |--12| 64.5598 L 65.6750 |--19| 62.5042 Фа, | 67.3235 |+ 8| 60.1805 ас | 67.7695 |-+18| 60.6160 Go | 68.2135 |-18| 61.0625 % by | 67.3100 |+ 9| 60.1695 De 67.7800 |+19| 60.6330 b, 68.2290 |--19| 61.0795 %с | 67.3465 | 9| 60.1700 Ce 67.7825 |-+19| 60.6100 Co | 68.2260 |+19| 61.0430 % dy | 67.3240 |+ 9| 60.1845 de | 67.7800 |+19| 60.6350 do | 68.2115 |+-19| 61.0695 %е | 67.3235 |+-10| 60.1540 ес 67.7835 |+20| 60.6130 ео | 68.2370 |+20| 61.0640 Та | 66.2710 |+11| 62.1160 6 | 66.2460 |+11| 62.1440 с | 66.2800 |-11| 62.1130 d | 66.2565 |+12| 62.1315 е | 66.2670 |+13| 62.1265 Па | 64.9770 |-+17| 63.4070 b | 64.9515 |+17| 63.4325 с | 64.9895 |+17| 63.4005 d | 64.9640 |+18| 63.4185 e | 64.9720 |+-19| 63.4125 Ша | 67.1850 |+ 9| 61.1900 b | 67.1620 |+ 9| 61.2080 с | 67.1975 |+ 9| 61.1775 d | 67.1755 |+10| 61.1965 e 67.1870 |-+-10| 61.1845 IV a | 69.1585 |+13| 59.2290 b 69.1300 |-+14| 59.2555 с 69.1640 |+14| 59.2240 а | 69.1405 |+14| 59.2445 e | 69.1495 +15] 59.2370 Scheinbare Adiff: AY —= 10* Е. Rexz, 1897. April 24. m 11.0 AR 1€ Helsingforser Sternzeit 5 & Fu cer Bilder. t+-k 5 der Aufnahmen. Mittel. mm mm 10000] 10000] mm тт —19 о 0.0000 2—3 — 6|+- 2| —21.0030 2 + 4138| —50.5948 12% 35” 9° 4 ellipt. +23|—33| +48.4180 3—4 ellipt. +21] o|+ 3.4016 1—2 +15|— 1] + 5.2600 2—3 +14 —= 6.9049 +10 + 7.3516 + 7.3492 12 Baar? 3 +10 + 7.7912 +14 — 6.8897 +10 —+- 7.3484 + 7.3475 31 40 2—3 —=то + 7.8045 +14 + 6.9262 200.20 +10 + 7.3612 + 7.3634 3206 24 12% 32” 12 1-29 —10 + 7.8028 HIS + 6.9012 и + 7.3474 + 7.3456 32 43 2 11 + 7.7882 +15 + 6.9042 и + 7.3602 + 7.3602 5) 9 3 +11 + 7.8162 Trabant — Jupiterscentrum. 2 —ıy | Mittel. рии | Jalur—y) Ph. | Да cos à mm mm + 9 + 5.8521| —1.4971 2 + 9 + 5.8256] —1.5219 2—3 + 9 + 5.8581| —1.5053 | —1.5096| —1:5068 | -+0:0007 | —0'0020| —1!5081 | 3 +-10 + 5.8371| —1.508$ 2—3 +-10 + 5.8449| —1.5153 2—3 +ÿ0 + 4.5599] —2.7893 2—3 + 9 + 45344] —2.8131 3 то + 4.5694| —2.7940 | —2.8009 | —2.7948 | -+0.0014 | —0.0020 | —2,7954| 2-8 то + 4.5476| —2.7980 2 +11 + 4.5546] —2.8056 2—3 +-10 + 6.7720] —0.5772 2 +10 + 6.7514| —0.5961 2—3 +10 + 6.7844| —0.5790 | —0.5837 | —0.5826 | -+-0.0002 | —0.0020 | —(,5844| 2—3 +11 — 6.7640] —0.5816 2 11 + 6.7757| —0.5845 2—3 +10 + 8.7394| +1.3902 2—3 +10 + 8.7120] 1.3645 3 +10 -+ 8.7447| +1.3813 | +1.3768| <+1.3742 | —0.0005 | —0.0020 | -+1.3747 | 3 +10 + 8.7227| +1.3771 2—3 +11 + 8.73109] +1.3708 2—3 J— Centrum = —23'4045 19а = 0.99807 —i° „ = +-0.00052 Е— » — —56.4517 . Е H— » —-53.9968 fax = 0.99779 —iy = -+0.00052 X = — 18 — » = + 3.8047 Вет. = + 15 L— » — + 5.8360 Try —=+ 48 Га = 0.99814 J« = 0.00115 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. sih e. Scalenablesung. $ Р.-Кг. 90°] 1+5 Р.-Кт. 270° |#-# mm mm mm En 1000 um 10000/10000 62,2988 66.0918 60.8760 |+11| 67.5118 |-+18| о 60.6192 |-+20 67.7585 |309] о 70.0918 |+39| 58.2838 |-+25|— 8 64.6600 |+33| 63.7248 |+24|— 1 75.7460 |+ 7| 52.6350 |+ 7| © 1 44.7158 |-+ 18| 83.6662 |— 6|+ 2 64.2220 + 8| 64.1785 |+13 | 64.6430 |+16| 63.7570 |-+13 65.0615 |-+16| 63.3300 |+14 65.7280 |-+10| 62.6690 |+-14 … 66.1700 |-+10| 62.2330 |-+14 | 66.5940 |+-10| 61.7995 |-+14 | 67.1110 |+ 8| 61.2920 |+15 à 67.5335 |+18| 60.8630 |+15 67.9510 |-+18| 60.4400 |+15 68.5830 |-+13| 59.8195 |+19 69.0110 |-+13| 59.3855 |-+15 69.4370 |-+13| 58.9500 |-+15 | 70.0120 |+16| 58.3900 |+10 _ 70.4570 |-+16| 57.9495 |+10 _ 70.8935 |+12| 57.4995 |+10 | 65.2825 |+16| 63.1025 |+10 66.7990 |+ 8| 61.5910 |-+10 68.1750 |-+18] 60.2090 |-+15 69.6470 |+16| 58.7395 +1 71.0980 |-+12| 57.2910 |+10 | 65.8500 |+10| 62.5320 |+10 67.3670 |+ 8| 61.0190 |+11 | 68.7435 |+13| 59.6410 |-+15 | 70.2160 |+16| 58.1685 |+ 6 | 71.6580 |+11| 56.7240 |+10 | 64.7820 |+16| 63.5920 |+ 9 | 66.2940 |-+10| 62.0810 |+10 | 67.6700 |+18| 60.7015 |-+11 | 69.1440 |+13| 59.2305 |+11 | 70.5885 |-+12| 57.7890 |- 6 | 64.1710 |-+ 9| 64.2150 |+-10 65.6885 |+11| 62.7000 |+11 | 67.0635 |+ 9] 61.3180 |-+ı2 | 68.5400 +14| 59.8460 |+16 | 69.9890 |+17| 58.4000 |+ 7 . Scheinbare Decldiff: J—Centrum - — » H— » К— » L— » 6, = 1897. April 24. Decl. YntBc+H%s Bemerkungen y Lin” аи Sur ‘his PET В zur Aufnahme. mm тт тт mm — 1,4218 0.0000 — 1.4218 — 1.6736 — 0.0317 — 1.7053 —= 7.8004 — 0.1856 —+ 7.6148 Luft 2. — 2.3644 — 0,1695 + 2.1949 | +13.4520 — 0.0008 +13.4512 1757178 — 0.0020 — 17.5793 + 1.9180 + 2.3396 + 2.3400 Luft 8—2. + 2.7624 —+ 3.4258 +- 3.8648 + 3.8614 — 4.2936 + 4.8056 + 5.2319 + 5.2299 + 5.6522 — 6.2780 —= 6.7092 + 6.7090 + 7.1399 + 7.7128 + 8.1506 —+ 8.1523 + 8.5936 Trabant — Jupiterscentrum. Е т S Yı--Y% | Mittel. 2 (гу) |7 (ег) | (ео) Ph. 45 тт тт + 2.9868] -+0.6468 + 4.5004] -+0.6390 + 5.8796] -+0.6497 | +0.6450 | 06439 | -но'ооот —0'0007 | -+0:0004 | -+0:6451 + 7.350$| -+=5.6415 + 8.8001| <+0.6478 + 3.5555| -+1.2155 + 5.0704] -+1.2090 + 6.4476] 1.2177 | +1.213I | -++1.21Io | -+0.0001 0.001711 | +0.0004 | -+1.2126 + 7.9208| +1.2118 + 9.3636] -+1.2113 + 2.4918] -+0.1518 + 4.0030| -+0.1416 + 5.3811| —+0.1512 | -+0.1467 | -+0.1464 0.0000 —0.0003 | —+-0.0004 | —+0.1471 + 6.8534| <+0.1444 + 8.2966| -н0.1443 + 1.8744| —0.4656 + 3.3908| —0.4706 + 4.7691| —0.4608 | —0.4647 | —0.4639 | —0.0001 —0.0007 | -+0.0004 | —0,4643 + 6.2434| —0.1656 + 7.6915| —0.4608 = — 0.2843 f°5 = 0.99794 1° 5 = —0.00025 = + 9.0352 = + 3.5974 fs = 0.99753 is = —0.00026 X i=— 0/9 =-+14.8400 = — 16.1264 fs = 0.99829 у = —0.00005 +129 346 166 Е. Renz 65 A. 1897. April 25. № Scalenablesung. Helsingforser Sternzeit Object. “a Bilder P.-Kr. 0° | t+%| P.-Kr.180°| $ ® der Aufnahmen. Mittel. mm _тт_ DE 10000] mm 10006] 1000 Ctr. | 61.9798 66.4018 H 61.9788 |+10| 66.4208 0.0000 2—3 J 40.9742 |+25| 87.4060 nee 2 à Г 11.3670 |-+24| 117.0122 —-50.6070 12° 34” 9 3—4 ellipt. Н |110.4002 |+- 5| 17.9802 -+48.4167 4 ellipt. K 65.3622 +22] 63.0150 — 3.3848 1—2 L 67.2410 |-+14| 61.1305 О] + 5.2662 2 2% ay | 53.8675 | 6| 74.5250 — 8.1182 | а 54.3290 |+ 6| 74.0755 — 7.6626 — 7.6643 12) Зое 3 ау | 54.7700 |+ 2| 73.6150 —= 7.2121 %6 | 53-8765 + 5| 74.5175 8.1099 D, 54.3340 |+ 5| 74.0770 — 7.6609 — 7.6591 ме 3 bo 54.7810 |+ ı| 73.6150 7.2066 9 Cyw | 53.8650 [+ 5| 74.5310 — 8.1224 en, ce 54.3240 |= 5| 74.0690 — 7.6619 — 7.6636 31 34 12 31 32 3 во 54.7775 |+ | 73.6110 — 7.2064 % dy | 53.8910 |+ 4| 74.5140 8.1099 с | 54.3360 | 4| 74.0660 — 7.6544 — 7.6519 31 58 3 do | 54.7860 o| 73.6075 7-2004 %е | 53.8940 |+ 4| 74.5000 |-+12 8.0924 ес 54.3375 | 4| 74.0540 |+12 — 7.6476 — 7.6468 3/2 024 2—3 ео 54.7855 | 73.6070 |-+12 — 7.2094 Trabant — Jupiterscentrum. ага | Mittel. \Patei—22) Tl) Ph: | Az cos à mm mm Ia | 56.1250 |+ 2| 72.2510 |+13 — 5.85261 1.8117 | b 56.1335 | ı| 72.2475 |+-12 — 5.8466] -+1.8125 ] с | 56.1280 ©] 72.2515 |+12 — 5.8514] +1.8122 | 1.8128 | -+1!8093 | —0!0007 | —0:0020 | -+1'8066 3 d 56.1409 | 72.2415 |+11 — 5.8403! +1.8116 e 56.1500 0] 72.2330 |+11 — 5.8310] +1.8158 II Bedeckt. Ша 57.4445 |-+11| 70.9310 |+13 — 4.5324] +3.1319 b 57.4535 |+10| 70.9220 |+13 — 4.5234] 3.1357 € | 57.4505 |+-10| 70.9220 |+12 — 4.5258| 3.1378 | 3.1361 | 3.1302 | — 0.0013 | —0.0020 | +3,1269 2—3 а | 57.4615 |+10| 70.9155 |-+12 — 4.5161| -+3.1358 е 57.4695 |+ 9| 70.9060 |+12 — 4.5074| +3.1394 IV & | 52.6370 |I+10| 75.7505 |+10 — 9.3458) — 1.6815 ) b 52.6440 |-+10| 75.7405 |+ 8 — 9.3372| — 1.6781 с | 52.6475 | 9| 75.7460 |+ 8 — 9.3382) —1.6746| —1.6786| —1.6754 | +-0.0007 | —0.0020 | —1,6767 3 d | 52.6550 |+ 8] 75.7375 |+ 7 — 9.3302| —1.6783 е 52.6540 |+ 8| 75.7305 |+ 7 — 09.3272] —1.6804 Scheinbare Ædiff: J— Centrum = —23'4046 Fu = 0.99801 —1°y = +-0.00126 Е— » — —56.4518 НН — 53.9969 SEN 099775 —м = 0.00126 X y = — 43 К— » — + 3.8047 Refr. — + 15 L— » —=+ 5.8360 Тс = — so f'x = 0.99808 ЛХ. = -—0.00091 “he. IP. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTO@RAPHISCHEN AUFNAHMEN. 167 1897. April 33. Scalenablesung. 5 y P.-Kr. 90° tt P.-Kr. 270° |t+% mm | mm mm 10000 10000] 10000 62.7315 65.6585 GE 65.6745 |+11| 63.2998 |+ 9| o]+ 2.9510 65.3982 |24| 62.9775 |-20] 0|-+ 2.6740 74.8490 |+32| 53.5278 |+21]— 8|+12.1238 69.5065 |-+35| 58.8755 |+27|— 7|+ 6.7787 80.5500 |+14| 47.8270 |+20|— 2] +17.8245 49.5235 |+ 5| 78.8512 |+ 7|+ 1] —13.2004 72.7320 |+17| 55.6620 |+ 2 + 9.9992 72.2960 |+15| 56.1070 |+ 2 + 9.5586 71.8395 |-+15| 56.5520 |+ 2 + 9.1079 71.2585 |+16| 57.1385 |+12 + 8.5237 70.8240 |+16| 57.5865 |+ 8 —+ 8.0826 70.3860 |+16| 58.0090 |+ 8 —+ 7.6524 69.8140 |-+20} 58.5845 |+13 —= 7.0786 69.3780 |-+17| 59.0195 |+13 + 6.6430 68.9270 |-+17| 59.4650 |+13 + 6.1947 68.3250 |+22| 60.0660 |-+14 + 5.5934 67.8865 |-+22| 60.5130 |+10 + 5.1508 | 67.4485 |-+22| 60.9485 |+10 + 4.7141 66.8180 |-+12| 61.5770 |+ 9 + 4.0836 66.3870 |+14| 62.0110 |+ 9 — 3.6518 65.9480 |+-14| 62.4500 |+ 9 + 3.2128 71.4950 |+15| 56.8780 |+ 9 -1- 8.7723 70.0290 |+19| 53.3470 |+ 5 + 7.3052 68.5885 |-+16| 59.7975 |+14 + 5.8591 67.0930 |+11| 61.2800 |+10 + 4.3700 65.5985 |+13| 62.7845 |+ 9 + 2.8707 Bedeckt. 70.8730 |-+14| 57.5030 |+ 9 + 8.1588 69.4080 |-+15| 58.9635 |-+10 + 6.6860 67.9560 |+20| 60.4155 |+14 + 5.2340 66.4670 |+12| 61.9080 |+ 9 + 3.7432 64.9665 |-+18| 63.4050 |+ 9 + 2.2137 73.0895 |+17| 55.3605 |+ 4 —10.3586 71.6250 |-+15| 56.7625 |+14 + 8.8948 70.1735 |+20| 58.2175 |+10 + 7.4420 68.6885 |-+17 59.6970 |+19 + 5.9592 67.1940 |-+12| 61.1960 |+15 + 4.4624 Scheinbare Decldiff.: J—Centrum = — 0,2843 F— » = + 9.0353 H— » = + 3.5974 K— » = +-14.8401 L— » — —16.1264 dy = +12° 34.5 Decl. Zat%ct%s mm + 9.5552 + 8.0862 + 6.6388 + 5.1528 + 3.6494 У: — 95 | тт тт — 0.7829 —0.7810 —0.7797 —0.7810 —0,7828 —0.7787 —1.3964 —1.4002 — 1,1048 — 1.4033 — 1.4096 — 1.4057 0.8034 —+-0.8086 +0.8032 | -+0.8069 —+-0.8064 —0.8 130 175 = 0.99800 fs = 0.99759 Г’ = 0.99834 =; à sin 1’ 219 mm 0.0000 0.0317 0.1856 0.1695 0.0008 0.0020 Pal are) | Trabant — Jupiterscentrum. - 5 т Mittel. (fa (ur—u2)| Ja виа) | - бт) 2 Bemerkungen y — = t9ÿ sin 1’ 2 zur Aufnahme. mm + 2.9510 + 2.6423 11.9382 + 6.6092 Luft 3—2. —17.8237 — 13.2024 —0:7797 | —0.0018 | -+0!0008 | -++0/ooo4 | —0!7803 —1.4010 | —0.0031 0.0012 | -+0.0004 | — 1,4025 —+1.8056 | -+0.0017 —0.0009 | -+0.0004 -+ 0.5068 5 =— 0.00122 is =— 0.00123 X в=-—4:2 Js = — 0.00102 168 Е. Renz, 65 B. 1897. April 26. № 163] Scalenablesung. Helsingforser Sternzeit 1 (HG RP N. + ИИ: 2 Kor о м Bilder, | P.-Kr. 0° ++ Pr. 180° |+-+# > der Aufnahmen. Mittel. À mm mm mm ] 10000 10000] 10000 Ctr, | 61.9100 66.4705 + I 61.9091 + 9| 66.4695 |+10| о 0.0000 2—3 J 40.9060 |--24| 67.4750 |— 4|-+ 2] —21.0026 2 Е 11.2995 |+23| 117.0878 |+ 6|-+-39| — 50.6092 12" 95% 49° 4 ellipt, Н |110.3355 |+ 4| 18.0500 |-+24|-—33| +48.4187 о 8—4 ellipt. 116 65.2922 |+21| 63.0880 |+16| o|+ 3.3826 2 L 67.1720 |+15| 61.2015 |+16| o|+ 5.2654 2—3 % Gp | 52.7515 |+ 7| 75.6440 |+ 7 — 9.1660 ас | 53.2210 + 7| 75.1680 |+10 — 8.6934 — 8.6933 12 12244726 2—3 Go | 53-6945 [+ 3) 74.6955 |+10 8.2206 #6, | 52.7815 + 7| 75.7105 |+ 8 9.1343 be 53.2495 + 7| 75.1630 |+11 — 8.6767 — 8.6794 22 54 2—3 Dr 53.6910 + 3| 74.7050 |+11 8.2272 %Cw | 52.7705 + 7| 75.6180 |+ 8 — 9.1436 БГ 23800 Ce 53.2395 + 7| 75.1470 |+11 — 8.6737 — 8,6811 DE 317 12 23 17 2 ce 53.6915 + 3| 74.7030 |+r1 8.2259 % dy | 52.7765 + 7| 75.6170 |+ 8 — 9.1400 de 53.2375 |+ 7| 75.1585 |#1ı — 8.6804 — 8.6839 23 42 2—3 do | 53.6860 |+ 3| 74.7085 |+11 — 8.2314 Ze | 52.7805 + 8| 75.6125 |+ 9 — 09.1358 ee 53.2390 + 8| 75.1575 |+12 — 8.6792 — 8.6797 DRS 2—3 ео 53.6915 |+ 4| 74.6995 |+12 — 8.2242 Trabant — Jupiterscentrum. 2 — Lg | Mittel. аа) (ye—Y2) Ph. До cos à mm mm Та | 51.4545 |+10| 76.9340 |+ 9 — 10.4594] —1.7661 3—4 b 51.4710 |+10] 76.9140 |+ 9 — 10.4412] — 1.7618 2—5 с | 51.4705 |10| 76.9190 |-+-10 — 10.4440] — 1.7629 | —1.7618 | —ı!7584 | -+0!0006 | —o:oo21 | —1:7599 | 2—3 d | 51.4695 |-+-10) 76.9140 |-+10 — 10.4420] — 1.7581 3 e 51.4735 +11) 76.9135 |+1ı — 10.4398] — 1.7601 3 Па | 56.0625 |— ı| 72.3200 |+12 — 5.8492] +2.8441 5—4 Ь | 56.0755 |— ı| 72.3035 |+12 — 5.8344] 2.8450 8 се | 56.0740 0] 72.3035 |+12 — 5.8351| 2.8460 |-+2.8470 | +2.8415 | —0.0011 | —0.c021 | 2,8883 | 2—3 d | 56.0805 O| 72.3010 |+13 — 5.8306] +2.8533 3 е 56.0765 | 1| 72.3020 |+14 — 5.8332| 2.8465 Ша | 57.8230 |+ 5| 70.5565 |+13 — 4.0869] 4.6064 3 b | 57.8360 + 5| 70.5410 |+13 — 4.0726] +4.6068 2—3 с | 57.8350 [+ 6| 70.5435 |+-14 — 4.0744] -+4.6067 |-+4.6076 | -+4.5986 | —0.0017 | —0.0021 | -+4,5948 | 2—3 d 57.8370 | 6| 70.5445 |+14 — 4.0739] +4.6100 2—3 е 57.8370 |+ 7| 70.5400 |+15 — 4.07 16] 4.6081 2—3 IV a | 48.7390 |+14| 79.6480 |+ 8 — 13.1740| —4.4807 3—4 b | 48.7625 |-+13| 79.6250 |+ 8 —13.1508| —4.4714 m: с | 48.7605 ‚+13| 79.6270 |+ 9 — 13.1528] —4.4717 | —4.4733 | —4.4646 | -+0.0017 | —0.0021 | —4,4650 | 3 а | 48.7635 +13| 79.6310 |- 9 — 13.1533] —4.4694 2—3 e 48.7590 |+13| 79.6260 |+ 9 — 13.1530] —4.4733 3 Scheinbare Ædiff: J—Centrum = —23'4046 Fra = 0.99798 — = 0.00130 — № 2=— 56.4509 Е H— » — +-53.9970 fa =0.99770 —iy —=+0,00130 D К— » — + 3.8047 Refr. =+ 13 L— » = + 5.8369 Try =— 56 Г’. = 0.99804 Jy = 0.00087 А т &y= 10 11.0 PosITIoNEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1597. April 26. Decl. mm + 1.2228 — 0.2413 Da D 9% a Ne} u 169 y——-tgdsin ls mm + 1.4324 —+ 1.1227 —+-10.4154 + 5.0977 + 6.3066 — 14.7236 Trabant — Jupiterscentrum. Bemerkungen zur Aufnahme, Luft 2—3. ne. Scalenablesung. P.-Kr.90° + P.-Kr.270° |+ _mm_| тт_ 10000] 10000 m 627315 65.6585 в 64.1620 64.2242 |+ 8| o|+ 1.4324 63.8815 64.4995 |+19] oJ-+ 1.1544 73.3298 55.0544 |+17|— 11] -+10.6010 | 67-9962 60.3885 |-+31|— 4|+ 5.2672 | 79.0346 49.3460 |--14] o|+16.3074 48.0015 80.3726 |+ 9] 0] —14.7216 64.4010 63.9940 |+-12 + 1.6670 _ 63.9620 64.4400 |+12 + 1.2245 63.5200 64.8930 |-+12 + 0.7770 62.9330 65.4640 |-+14 + 0.1980 62.5035 65.9085 |+-14 — 0.2390 | 62.0570 66.3500 |+14 — 0.6830 _ 61.4620 66.9310 |+12 61.0240 67.3790 |+12 60.5805 67.8245 |-+12 59.9770 68.4140 |+17 59.5540 68.8525 |+17 59.1260 69.2830 |+17 58.5160 69.8815 |+20 58.0850 70.3130 [+20 | 57.6560 70.7450 |-+20 64.6770 63.7110 |+13 + 1.9469 | 63.2060 65.1800 |+21 + 0.4762 61.7385 66.6600 |-+13 — 0.9972 60.2695 68.1225 |-+23 — 2.4632 58.7990 69.5950 |-+21 — 3.9348 62.7245 65.6670 |+12 — 0.0578 _ 61.2540 67-1370 |+-10 — 1.4778 59.7750 68.6040 |-+I5 — 2.9509 58.3140 70.0705 |-+18 — 4.4152 56.8455 71.5415 |+13 — 5-8846 | 61.9940 66.3870 |+11 — 0.7330 | 60.5270 67.8540 |-+19 — 2.2004 | 59.0520 69.3255 |+14 — 3.6734 | 57.5855 70.7925 |+13 — 5.1403 | 56.1110 72.2640 |+12 — 6.6136 65.9110 62.4810 |+16 -+ 3.1784 64.4370 63.9545 |-+15 + 1.7046 62.9700 65.4240 |-+23 + 0,2360 61.5050 67.8860 |-15 — 1.2270 | 60.0315 68.3560 |+25 — 2.6990 | Scheinbare Decldif: J—Centrum = — 0,2843 A № —=-= 9.0353 H— va =-+ 3.5974 K— » = 14.8401 L— » = —16,1264 Sau. Физ.-Мат. Отд. = 6% = +12° 34.4 veux | Mine. зе) 7аы-)|-ве-атьт| вы | 8 тт тт —0.7241 —0.7175 +0.7172 | -#0.7194 +-0.7221 +0.7160 —1.2306 —1.2365 —1.2365 —1.2335 — 1.2299 — 1.2338 —1.9558 —1.9591 —1.9590 | —1.9583 —1.9550 - — 1.9628 —+1.9556 +1.9459 +1.9504 | -#1.9524 +1.9583 —1.9518 1% = 0.99787 fs = 099746 Г’; = 099818 0/7181 | +0!0026 — 1.2313 | —0.0043 —1.9547 | —0.0070 —1.9489 | -+0.0067 is = —0.00132 is =-— 0.00132 у = — 0.00151 — 0.0011 | —+-0/0004 —+0.0013 | -+0.0004 0.0019 | -+0.0004 —0.0032 | -+0.0004 X в=— 45 12 > —+0:7200 —1,2339 —1,9594 +-1,9528 Object. -ч = — rer je = = LOGS оса PS HI a ga m NR P.-Kr. 0° 61.9200 61.9191 40.9052 11.2998 110.3380 65.2942 67.1820 68.3170 68.8005 69.3050 68.3280 68.8180 69.2915 68.3085 68.8135 69.3235 68.3280 68.8220 69.3030 68.3030 68.8115 69.2940 67.8895 67.9000 67.8965 67.9090 67.9080 66.2610 66.2735 66.2710 66.2810 66.2770 67.7630 67.7710 67.7720 67.7710 67.7700 60.9290 60.9420 60.9395 60.9465 60.9480 Scalenablesung. tt} P.-Kr.180° mm 10000 == 9 +24 +23 A +21 +16 +20 +15 IS +-19 +14 +14 +19 +14 4-14 IS +13 +13 +18 +13 +13 +20 +19 +19 +18 —+18 #II SET +10 +10 +10 +-20 +19 +19 +18 +18 HI +1] +12 +13 +14 mm 66,4709 66.4698 87.4822 117.0792 18.0482 63.0902 61.1995 60.0810 59.5850 59.0855 60.0660 59.5930 59.1050 60.0840 59.5880 59.0820 60.0690 59.5880 59.0960 60.0720 59.5845 59-0970 60.5120 60.4905 60.4960 60.4820 60.4800 62.1250 62.1155 62.1165 62.1050 62.1105 `60.6205 60.6090 60.6080 60.6040 60.6105 67.4575 67.4485 67.4525 67.4430 67-4390 Scheinbare Ædif: t-+k u K— L— _mm_ 110000] 10000 +37 J— Centrum № 16 Helsingforser Sternzeit | Luther Bilder. | F der Aufnahmen. Mittel. mm mm 0.0000 3 Er 3 — 50.6096 hernie 4 ellipt. | #452 160 12 35 50 3—4 + 3.3778 2—3 + 5.2666 3 + 6.3936 + 6.8831 + 6.8872 ı2 312036 2—3 + 7.3848 —+ 6.4066 + 6.8878 —= 6.8877 3212404 3 + 7.3688 + 6.3878 п + 6.8881 + 6.8907 2 VAI 12 32 43 3—4 + 7.3963 — 6.4048 + 6.8924 + 6.8921 33 16 3 == 7.3790 | —+ 6.3911 | + 6.8888 — 6.8846 33 48 3—4 5 + 7.3740 Trabant — Jupiterscentrum. 2 —ıy | Mittel. щен) Ли ии) РВ. | Ac cos à mm mm з | + 5.9644] — 0.9228 3 + 5.9804] —0.9073 3 + 5.9759] —0.9148 | —0.9086 | —0!9068 | -+0!0007 | —0'0021 | —0:9082 | 4 + 5.9891| —0.9030 3 + 5.9896] —0.8950 3—4 + 4.3434] —2.5438 3 — 4.3545] —2.5332 3 + 4.3528| —2.5379 | —2.5339| —2.5289 | -+0.0022 | —0.0021 | — 2,5288 | 3—4 El + 4.3634| —2.5287 | 3 | —+ 4.3587| —2.5259 3 + 5.8470] —1.0402 3 | + 5.8568| —1.0309 3 U + 5.8578] —1.0329| —1.0332| —1.0311 | +0.0011 | —0.0021 | —1.0321 | 3—4 + 5.8593| — 1.0328 3 В + 5.8556] —1.0290 3—4 Е — 0.9887] —7.8759 3 — 0.9777| —7.8654 3—4 | — 0.9809| —7.8716| —7.8664| —7.8508 | +0.0069 | —0.0021 | —7,8460 | 3—4 — 0.9726| —7.8647 3 | — 0.9668] — 7.8544 2—3 | Е —=—23'4047 fa = 0.99795 —Ÿ% = +0.00150 = — 56.4520 = 53.9971 fa = 0.99767 —iy = 0.00150 X = — 5.2 = + 3.8047 Refr. = + = + 5.8361 Try —=+ am fu = 0.99802 “То, — + 0.00216 ay = 10° 11.1 F. Renz, 1897. April 28. P.-Kr. 90° + P.-Kr.270° |t-+k POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1597. April 28. Decl. mm nm | nm | Em 10000! mm 10000]10000] zum || 627315 65.6585 62.7305 |-+10| 65.6575 |1] о 0.0000 62.4532 |-+17| 65.9278 |-+22| 0] — 0.2740 71.9055 |-+33| 56.4815 |-+17|— 8] -= 9.1755 66.5720 |-+25| 61.8148 |+26|— 2| + 3.8418 77.6118 |-= 8| 50.7725 |+-11]— 1|-+14.8829 46.5800 |+ 8| 81.8078 |+ 2|— 1| —16.1500 55.9310 | 72.4700 |+12 — 6.8066 56.4045 0] 71.9950 |+12 — 6.3324 56.8870 |+10| 71.5130 |+12 — 5.8496 57-4270 |+ 6| 70.9760 |+13 — 5.3114 | 57.8980 |+ 6| 70.5080 |+13 — 4.8418 | 58.3490 |+- 6| 70.0400 |+17 — 4.3830 58.8230 |11| 69.5690 |+14 — 3.9096 | 59.3340 |+11| 69.0880 |+14 — 3.4136 59.8160 |+11| 68.5800 |+14 — 2.9186 60.3290 |+17| 68.0660 |+19 — 2.4051 | 60.8160 |+11| 67.5920 |+19 — 1.9249 61.2950 |+11| 67.1030 |+ 9 — 1.4404 61.7980 |+-10| 66.6020 |+r1 — 0.9386 | 62.2805 |+10| 66.1230 |-+11 — 0.4578 62.7530 |+10| 65.6430 |+ 11 + 0.0184 56.7340 |+ 9| 71.6550 |+12 — 5.9972 58.2270 |+ $| 70.1690 |+17 — 4.5081 59.6480 |-+14| 68.7430 |+14 — 3.0840 61.1425 |-+10| 67.2575 |+ 9 — 1.5940 | 62.6040 |+ 9| 65.7925 |+11 — 0.1308 ° 97.4525 |+ 9] 70.9410 |+13 — 5.2810 || 58.9375 |[+10| 69.4545 |+14 — 3.7952 | 60.3630 |+14| 68.0260 |+-19 — 2.3682 | 61.8520 |+ 9| 66.5370 |+ 9 — 0.8790 {| 63.3110 |+ 9| 65.0780 |+17 + 0.5796 36.9040 +9| 71.4770 |-rı2 — 5.8232 41 58.3920 |+ 5| 69.9835 |+17 — 4.3328 59.8245 |-+14| 68.5555 |+14 — 2.9020 Al 61,3120 |-+10| 67.0695 |+ 9 — 1.4152 Al 62.7745 |+ 9] 65.6075 |+ + 0.0469 59.6820 |-+15| 68.7125 |+13 — 3.0516 61.1730 |+11| 67.2170 |+ 8 — 1.5584 | 62.5930 |+10| 65.7970 |+10 — 0.1385 | 164:0865 |+ 9| 64.3045 |+ 8 + 1.3546 | 65.5430 |+11| 62.8430 |+ 9 + 2.8136 Scheinbare Decldif. J-—Centrum —— 0,2843 Е » —-+ 9.0354 H— » =+ 3.5974 К— » = +-14.8402 TR» = —16.1265 dy = +12° 33:9 “пн е+%; тт — 6.3295 — 4.8454 — 3.4139 — 1.9235 — 0.4593 91—95 | Mittel. mm 0.3323 +0.3373 +0.3299 +0.3295 +0.3285 —+-1.0485 +-1.0502 +-1.0457 +-1.044$ —1.0389 0.5063 +-0.5126 +-0.5119 +-0.5083 0.5062 +3.2779 -+3.2870 3.2754 —+3.2781 -+3.2729 mm +0.3315 —1.0456 +0.5091 —+3.2783 79 = 0.99775 fs =0.99734 f's = 0.99810 ARE , — 5 #90311 ИИ о 5 a \O A x? <. y — = 196 sin Г тт 0.0000 — 0.3057 + 8.9899 + 3.6723 —= 14.8821 — 16.1520 Trabant — Jupiterscentrum. T fa (гу)! 7 (а) Ph. +0:3309 | —<-0/0010 —+-1.0436 | -+0.0027 —0.5081 0.0011 3.2721 | -+0.0082 $2 = —0.00125 3 = —0.00126 Js = —0.00105 Bemerkungen zur Aufnahme. Luft 3. +-0/0004 | -+0'0004 —+0.0009 | -+0.0004 +-0.0004 | +-0.0004 +-0.0015 | -+0.0004 X ig = — 43 | —0:3327 +-1,0476 +3,2822 172 65 D. Scalenablesung. Object. P.-Kr. 0° |t-+k mm mm 10000 mm Ctr. | 61.9300 66.4561 JA 61.9291 [+ 9| 66.4550 J 40.9170 |+24| 87.4582 JU 11.3078 |-+22| 117.0718 H |110.3495 |+ 4| 18.0390 K 65.3052 +21] 63.0685 L 67.1975 |+17| 61.1835 %аь | 69.7020 |-+16| 58.6935 Ge 70.1220 |+16| 58.2735 &o | 70.5330 |+-16| 57.8680 % by | 69.6605 |-+17| 58.7280 be 70.0945 |-+17| 58.3100 bo 70.5145 |-+17| 57.8810 % Cp | 69.6765 |-+17| 58.7100 Ce 70.0950 |-+17| 58.2900 бо 70.5145 |-+17| 57.8680 %@ | 69.6590 |-+17| 58.7295 de 70.0955 |+17| 58.3085 do | 70.5185 |-+17| 57.8810 Ye | 69.6860 |-+18| 58.7060 ес 70.1070 |-+18| 58.2900 ео 70.5225 |-+18| 57.8680 Та | 69.2160 +14| 59.1655 6 | 69.1855 |-+14| 59.2010 с | 69.1960 |+14| 59.1880 d | 69.1910 |+14| 59.2055 e | 69.1870 |+15| 59.2030 IIa | 67.7955 |+-19| 60.5905 b | 67.7655 |+19| 60.6255 С 67.7795 |+19| 60.6115 а | 67.7655 |-+19 60.6230 е | 67.7665 |+20| 60.6220 Ша | 68.4970 |+19| 59.8870 b 68.4620 |-+19| 59.9230 в 68.4770 |-19| 59.9020 d | 68.4715 |+20| 59.9110 e 68.4760 |+-21| 59.9090 [У а | 77.3479 |+ 9| 51.0480 Ь | 77.3165 |+ 9| 51.0745 с | 77.3250 |+ 9| 51.0640 d | 77.3220 |+10| 51.0750 е | 77.3175 |+10| 51.0745 P.-Kr. 180° t-+X Scheinbare Adif: EEE ee Tee ee mm DOM лммх un D лох = Ce] mm 10000! 10000 on +11 Ге) 0.0000 — 3[+ 3| — 21.0059 + 4-38] — 50.6142 +-24|—33|+48.4140 Е. Rexz, 1897. Мал S. № 16! ee Г Е I t ch Г + #0 elsingforser Sternzei Bilder. р der Aufnahmen. Mittel. у | тт | Е 1—2 pr 2 3 A m 5 2—3 Ой 14° 17 24 3 1—2 р 2 } Ei + 8.1838 14 Wie 2—3 + 8.1553 13 42 2 | + 8.1666 14 16 1 14" 4 |3 | L + 8.1559 14 42 2 | | —+ 8.1722 В то 2 | Trabant — Jupiterscentrum. 2—2 | Mittel. Fit ива) Tale —ya)| Ph. | Ac cos 9 | mm mm +10 + 7.2885| —0.8953 —то + 7.2555| —0.8998 4-10 -+ 7.2672] —0.8994 | —0.9023 | —0!9007 | -+0!0010 | —0:0023 и + 7.2560] —0.8999 тт + 7.2552] —0.9170 то — 5.8660] —2.3178 —10 + 5.8335| —2.3218 +11 + 5.8474| —2.3192| —2,3233 | —2.3192 | +-0.0025 | —0.0023 +11 + 5.8347| —2.3212 +12 + 5.8357| —2.3365 +14 + 6.5683| —1.6155 +14 + 6.5328| — 1.6225 +14 + 6.5508| —1.6158| —1.6183| —1.6155 | -+0.0015 | —0.0023 —15 + 6.5436] —1.6123 Е +15 + 6.5468| —1.6254 +11 -+-15.4124| -+7.2286 -I0 —=19.3839] +7.2286 +10 +-15.3934| +7.2268| +7.2253 | -+7.2126 | —0.0073 | —0.0023 +10 +15.3864| -+7-2305 +10 —15.3844| +7.2122 J—Centrum = —23:4050 fra = 0.99797 —i° = -+0.00147 — » — — 56.4528 Н— » ==-53.9980 fa = 0.99766 —и = —+0.00144 К— » = - 3.8047 Refr. = + 47 1— » —=+ 5.8363 Try =+ 53 Га = 0.99824 I, = 0.00244 h т y = 10 11.9 —(0:9020 | 2—3 — 2,3189 2 2 2 2, 2 2 2 —1,6163 | 2 2 2 = 3 —+7,2030 | 3 3 2 —4 geschwe 1 о 3 | POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. 1897. Mai Я. | CLL е. Decl. | Scalenablesung. . Zt ct 2, ne 2, er Bemerkungen р ——_ — 105 — In zur Auf | P.-Kr.90° tn P.-Kr. 270° + 3 а (9 у а 9 zur Aufnahme, | | I тт_| mm 627315 т = A 7 5e | | 61.2568 67.1280 |+ 8| 0|— 1.4720 0.0000 — 1.4720 60.9778 67.3958 |+19] 0 — 1.7456 — 0.0317 — 1.7773 70.4350 57.9508 |-+23|— 7| + 7.7056 — 0.1856 — 7.5200 Die Luken waren || 65.0975 63.2858 |-+26|— 2] + 2.3695 — 0.1695 + 2.2000 kurz vorher ge- II 76.1315 52.2452 |+12 0] +13.4064 — 0.0008 +13.4056 ölfnet worden. | 45.1060 83.2752 |+ 3|+ 2] — 17.6202 — 0.0020 — 17.6222 64.2600 64.1495 |+10 + 1.5187 || 64.6490 63.7480 |+-10 + 1.9144 + 1.9139 _ 65.0430 63.3475 |411 + 2.3116 65.7100 62.6850 |+11 + 2.9760 66.1230 62.2790 |+11 + 3.3855 + 3.3809 | 66.5125 61.8770 |-+11 + 3.7812 {| 67.1830 61.2240 |+12 + 4.4428 | 67.5890 60.8050 |-12 +. 4.8558 + 4.8524 | 67.9915 60.4020 |-+12 + 5.2586 68.6755 59.7165 |+16 + 5.9429 _ 69.0870 59.3145 |-+12 —+ 6.3498 — 6.3453 69.4760 58.9170 |+12 + 6.7431 70.0680 58.3380 |+ 7 + 7.3290 | 70.4630 57.9485 |+ 7 + 7.7212 + 7.7252 70.8560 57.5330 |+ 7 + 8.1253 | | Trabant — Jupiterscentrum. | ve | Mittel. [fau ||) т. | 4 | | тт тт | 65.0430 63.3470 |+11 + 2.3118| -+0.3979 I 66.5140 61.8770 |+11 + 3.7820] +0.4011 (| 67.9840 60.4090 |+16 + 5.2512| -+0.3988 | -+0.3996 | -+0/3991 | -+0!0007 +-0:0004 | -+o!ooos | -+0!4007 | 69.4745 58.9140 |-+12 —= 6.7438| -+-0.3985 ; | _70.8580 57.5320 |+ 7 —= 8.1268| -+0.4016 il 65.6715 62.7185 |+10 + 2.9400] -+1.0261 | 67.1400 61.2485 |+11 + 4.4091| 1.0282 | 68.6130 59.7750 |-+15 + 5.8824] 1.0300 | -+1.0281 | 1.0268 | 0.0017 | -но.0ото | -+0.0005 | -+1.0300 | 70.1035 58.2835 |+ 6 + 7.3740] -+1.0287 | 71.4845 56.9060 |+10 + 8.7528| -+1:0276 Al 65.2415 63.1420 |+10 + 2.5136] -+0.5997 || 66.7100 61.6695 |-+10 + 3.9837| -+0.6028 | 68.1780. 60.2010 |-+15 + 5.4522] -+0.5998 | -+0.5988 | 0.5981 | -+0.00т2 —0.0007 | -+0.0505 | -+0,6005 || 69.6750 58.7130 |-+11 + 6.9448] 0.5995 | 71.0470 57.3395 |+10 + 8.3174| -+0.5922 Al 61,6695 66.7240 |+13 — 1.0637| —2.9776 Bl 63.1420 65.2490 |-+21 + 0.4094| —2.9715 | 64.6150 63.7800 |-+13 + 1,8814] —2.9710 | —2.9739 | —2.9702 |, —0.0054 —0.0055 | -+0.0005 | —2,9806 Al 66.1050 62.2880 |+14 + 3.3720| —2.9733 | 67.4810 60.9090 |+15 + 4.7494| — 2.9758 | Scheinbare Decldif: J—Centrum = — 0.2843 195 = 0.99796 1#°5 = —0.00124 — » = 9.0357 + ( Hp u H— 120 =-+ 3.5973 fs = 0.99752 is. = — 0.00135 x 15 = —4/6 K— о» = 14.8405 1—5 ——16.1267 Гз =0.99979 Ja = --0.00075 dy = -+12° 27.4 174 Е. Вами, 66 А. 1897. Mai 15. | AR 166 Scalenablesung. Helsingforser Sternzeit | Object. 8 & Зи Фо | Bilder. M P.-Kr. 0° |t--H]P.-Kr.180° th 3 der Aufnahmen. Nittel. | mm mm mm Эй 10000 um 10000] 10000! zum nn (г, | 61.5852 66,7956 T8 61.5842 |+10| 66.7948 |+ 8 0.0000 2 | J 40.5758 |+25| 87.7970 |— 6|-++- 3| — 21.0036 2 1 2h F 10.9738 |-+24| 117.4012 |+ 7|-+-39| —50.6038 14° 45” 2° 3 stark еШрё _ Н |110.0106 |+ 5| 18.3732 |+25|—33|-+48.4196 3 u K 64.9540 |-+22| 63.4160 |+16|— 1|-н 3.3744 1—2 L 66.8625 |-+14| 61.5120 |+15 + 5.2804 2 {1 % Gp | 55.8145 |+ 2] 72.5885 |-12 — 5.7823 ag 56.2110 |+ 2| 72.1940 |+12 — 5.3868 — 5.3905 тд 59120 3 CA 56.5910 |+ 2| 71.8050 |+12 — 5.0023 %6 | 55.7880 |+ 1| 72.6110 |+12 — 5.8068 F ER D, 56.1815 |+ 1| 72.2265 |+12 — 5.4178 — 5.4166 40 -17 14° 40” 48° |2 b, 56.5675 |+ 1| 71.8270 |+12 — 25.0251 YCy | 55.8020 0) 72.5895 |+I1 — 5.7891 en 56.2045 ©] 72.1945 |+11 — 5.3904 — 5.3911 40 51 2—3 Со 56.5960 O| 71.7930 |+II — 4.9938 % dy | 55.7685 C| 72.6260 |+11 5.8241 de | 56.1685 0| 72.2320 |+11 —= 6.4271 — 5.4313 41 20 2 do 56.5515 0] 71.8460 |-11 5.0426 Ye | 55.8160 oO] 72.5805 |+II — 5.7776 CA 56.2125 O| 72.1930 |+11 — 5.3856 — 5.3844 41 50 2 ео 56.6005 0] 71.7900 |--11 — 4.9901 Trabant — Jupiterscentrum. Sy | Mittel. ЛАГ] Ph. | Au cos à mm mm Та | 55.7595 |+ 2| 72.6260 |+14 — 5.8286| —0.4381 2—3 b | 55.7335 |+ 1] 72.6540 |+14 — 5.8557] —0.4391 | Е 4 h 2—3 с | 55.7545 0] 72.6320 |-+13 — 5.8342| —0.4431 | —0.4426| —0'4419 | -+0:0005 | —0:0023 | —1:4437 | 3 d | 55.7135 | ©] 72.6745 |+13 — 5.8760] —0.4447 | 2—3 е 55.7550 O| 72.6290 |+13 — 5.8324| —0.4480 3 Па | 54.2515 |+ 6| 74.1345 |+14 — 7.3367| —1.9462 2 b | 54.2230 |+ 5| 74.1665 |+13 — 7.3670] —1.9504 2—3 deformie) e | 54.2415 [+ $| 74.1435 |413 — 7.3462] —1.9551| —1.9521| — 1.9491 | +-0.0020 | —0.0023 | —1,9494 | 3 а | 54.2020 |+ 4| 74.1830 |+12 — 7.3857| —1.9544 2—3 е 54.2460 | 4| 74.1335 |+12 — 7.3390] —1.9546 2—3 Ша | 54.0525 |+ 6| 74.3295 |+14 — 7.5337| —2.1432 | b | 54.0275 |+ 5| 74.3530 |+13 — 7.5580] —2.1414 e | 54.0535 |+ 5| 74.3255 |+13 — 7.5312] —2.1401 | —2.1397 | —2.1364 | -н0.0019 | —0.0023 | —2,1368 2—3 d | 54.0175 |+ 4| 74.3680 |+-12 — 7.5704] —2.1391 | е 54.0690 |+ 4| 74.3165 |+12 — 7.5190] —2.1346 ТУа | 48.5545 |+17| 79.8285 [+11 —13.0314| —7.6409 3 6 | 48.5360 |-+16| 79.8490 |+10 —13.0509| —7.6343 2—3 с | 48.5585 |+16| 79.8280 |+ 9 —13.0291| — 7.6380 | —7.6369| —7.6252 | -+0.0074 | —0.0023 | —7,6201 | 3 d | 48.5220 |+-ı5| 79.8640 |+ 9 —13.0654| — 7.6341 2—3 e | 48.5655 |-+14| 79.8200 |+ 9 —13.0217| —7.6373 2—3 Scheinbare ARdiff: J—Centrum = —23:4051 ба = 0.99810 —1°,, = +-0.0020$ ee = — 56.4533 , H— » — +-53.9984 fx =0.99777 —% = +0.00201 x in = — 6:9 K— » = + 3.8047 Refr. = + 66 L— » = == 5.8363 Try =— 34 sim f'x = 0.99847 J, = 10.002353 ay = 10 13.2 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 175 1397. Mai 15. e. Dec]. Scalenablesung. Ant Bemerkungen x? NER, 2 . | — я #00 sin 1’ Je 5. 298 sin 1’ zur Aufnahme, | P.-Kr.90° tt P.-Kr. 270°|t-+# mm mm _тт_ _тт_ 10000! mm _ [10000] 10000 66.2250 62.7815 |+ 9] ol+ 3.4420 + 3.4420 63.0630 |+21| O|-+ 3.1544 + 3.1227 53-6362 |+21|—10 —+12.3984 Luft 1—8. 58.9240 |+17|— 6 . — 7.1298 Е 47.8992 |-+20]— 2 . 18.3194 | 49-4555 78.9250 |+ 7+1 : — 12.7048 71.6410 56.7590 |+11 71.2725 57.1350 |+-11 ! —+ 9.0949 | 70.8710 57.5165 |+-11 70.1540 58.2395 |+ 7 à 69.7780 58.6210 |-+12 : — 7.6065 | 69.3880 59.0020 68.6860 59.7170 68.3095 60.0880 Ä — 6.1378 67.9180 60.4720 67.2285 61.1780 66.8540 61.5480 ! — 4.6813 66.4690 61.9265 65.7640 62.6350 65.3960 63.0200 : + 3.2181 65.0030 63.3900 Trabant — Jupiterscentrum. ; о т Ye—Yy | Mittel. 12 (Yyı—Yz) | Jg (&t—xz) ara) mm mm 71.4635 56.9240 69.9815 58.4045 68.5135 59.8770 67.0625 61.3240 65.5915 62.7990 72.1360 56.2510 70.6450 57-7435 69.1740 59.2060 = 67.7210 60.6640 _ 66.2470 62.1350 56.2985 0.2074 —+-0.2141 +0.2119 | +0.2125 | -+0/2123 | -+-0!o005 —=0'0005 | -+0:2131 —+-0.2193 +-0.2097 +-0.8806 —+-0.8761 0.8779 0.8760 | -+0.0022 —+-0.8791 —+-0.8695 —0.8324 57.7890 —0.8271 59.2510 —0.8304 60.7170 - 0.8264 62.1750 4 —0.8257 53-9410 . 3.1918 55-4175 - +3.1993 56.8955 Е —+3.1929 | 3.1947 | 3.1921 -+3.1970 58.3400 ь +3.2011 59.8170 . —3.1883 ЕЕ ЕЕ ЕЕ Scheinbare Decldiff: J—Centrum = — 0/2843 195 = 0.99804 $25 = —0.00181 F— » = + 9.0358 H— » = + 3.5970 fs = 0.99758 is =-— 0.00196 К— » = 14.8403 L— » =--16.1267 f's = 0.99916 Js = —0.00116 dy = 12° 19:1 176 F. Renz, 66 В. 1897. Mai 17. т № 16' Scalenablesung. u Е Helsingforser Sternzeit Г] Object. | $ x 22 В ыы Bilder, } Р.-Кг. 0° +51 P.-Kr.180° те der Aufnahmen, | Mittel. | mm mm mm р 10000 10000] 10000 Ctr. | 61.6059 66.7778 в st в | I 61.6050 |+ 9| 66.7770 |+ 8| ©] 0.0000 23 . IT 40.5920 |-+24| 87.7818 |— 6|-+ 2] —21.0072 3 eiförmig. | Е 10.9910 |-+23| 117.3872 |+ 6|-+39] —50.6074 15" 35” 56° 4 ellipt. | Н |110.0305 |+ 4| 18.3515 |+24|—34| +48.4210 4 ellipt. | K 64.9722 |+21| 62.4020 |+-15|— 1|-н 3.3712 2 2 L | 66.8805 |+15| 61.4935 [+16] @]-+ 5.2794 2—3 й D; Фа, | 56.9435 [+ 9] 71.4560 |+13 — 4.6705 = ag 57.3340 |+ 9| 71.0650 |+-13 — 4.2798 — 4.2764 15 31 34 2 № @ | 57-7305 |+ 5] 70.6595 |+13 — 3.8790 | 2b» 56.9505 | 9] 71.4510 |+13 — 4.6645 : 5.85 | be 57.3365 | 9] 71.0590 |+13 — 4.2755 — 4.2767 32, Хо 15 32 48 2 FA b, 57.7210 |+ 5| 70.6720 |+13 — 3.8900 г % Cp 56.9560 |-+10| 71.4435 |+14 4.6580 Ce 57.3445 |-+10| 71.0550 |+14 — 4.2695 — 4.2688 32 48 2 | GA 57.7335 | 6| 70.6625 |+14 3.8790 %а | 56.9500 |-+10| 71.4470 |-+14 — 4.6628 de 57.3480 |H-10| 71.0525 |-+14 — 4.2665 — 4.2689 3338.28 2 d 57.7330 | 6| 70.6590 |-+14 3.8774 Ze | 57.0000 |-+11| 71.3930 |+-15 4.6108 ес 57.4000 |-+11| 71.0025 |-+15 — 4.2155 — 4.2188 ЗВ 53 2 ео 57.7825 + 7| 70.6140 |-+15 — 3.8302 Trabant — Jupiterscentrum. 2—2 | Mittel. [ео Тиби РВ. | Aa. cos à тт тт Та | 55.7670 |— 1| 72.6210 |+14 — 5.8418] —1.5654 3 ta b | 55.7645 |— 1| 72.6250 |+14 — 5.8450] —1.5683 2—3 N с | 55.7680 ol 72.6205 |+14 — 5.8410] —1.5722 | —1.5694| —1:5676 | +0.0021 | —0.0023 | —1:5678 | 3 ie а | 55.7695 ol 72.6180 |-+15 — 5.8390] —1.570I 3 ellipt. in Deel, | е 55.8190 ol 72.5690 |+-16 — 5.7898] — 1.5710 aa Па | 59.8750 |-+14| 68.5105 |+19 — 1.7320] +2.5444 3 geschweift, b 59.8620 |+14| 68.5210 |+19 — 1.7433] +2.5334 _ LA с 59.8760 |-+15| 68.5065 |+-20 — 1.7296] +2.5392 | -+2.5387 | 2.5358 | —0.0036 | —0.0023 | -+2,5299 | 2—8 ‚ № а | 59.8730 |+15| 68.5150 |+21 — 1.7354| 2.5335 3 1% e 59.9315 |-+17| 68.4550 |-21 — 1.6760| +2.5428 3 | Ша | 61.4505 |-+10| 66.9290 |+ 9 — 0.1532] 4.1232 2—3. geschweil b 61.4410 |+11| 66.9420 |[+10 — 0.1640] -+-4.1127 9% 4 с | 61.4515 |-+11| 66.9305. |+11 — 0.1536] +4.1152| +4.1170| 4.1124 | —0.0058 | —0.0023 | +4,1043 | 2—3 | d | 61.4530 |-+12| 66.9315 |+-11 — 0.1532] 4.1157 2—3 | е 61.5060 |-+13| 66.8790 |-+12 — 0.1005| 4.1183 3 IV а | 51.2030 |+10| 77.1880 |+ 9 —10.4065| —6.1301 . | | b | 51.2005 |+10| 77.1895 |+10 —10.4086| —6.1319 } à le с. | 51.2060 |+10| 77.1850-|-+10 —10.4036| —6.1348 | —6.1338| —6.1269 | +-0.0080 | —0.0023 | —6.1212| ; 3 | d | 51.2010 |-+19| 77.1850 |+10 — 10.4060] —6.1371 KE = + | ne | ох е 51.2550 [+11] 77.1345 |1 —10.3538| —6.1350 | Scheinbare Adiff: in = al: ru = 0.99804 .— y =#+000211 | и | — » = —50.4535 | . : ‘. mu H— Ж8НК53.9985 Ja = 099767 ie -—+0,00204 x и=—7.0 | K— » — + 3.8047 Ве". === 144. %. | | L— »| {+ 5.8363 о Tru = 427 —\ | 7 Гы =099887 Л» = -+0,00321 | ty — 10 13.6 ‘9 PR | | «1 | OR: Ч — POoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 17 | 1897. Mai 17. sıihe. Decl. ра tgö sin 1” y 205 sin 1’ ыы: P.-Kr. 90° t-il P.-Kr. 2700 |t-+k 2 ‘ a | 10000 10000] 10000 ‚| 621620 66.2250 er г” р "т 64.1080 |+ 9| 64.2760 |+ 8| о] -н 1.9476 0.0000 + 1.9476 | 63.8202 |-+16| 64.5515 |+28] о] -+ 1.6652 — 0.0317 + 1.6335 | 73.2598 |+35| 55.1230 |-+17|—10] 11.0998 — 0.1856 10.9142 ° 67.9602 |+35| 60.4205 |+31|— 7|+ 5.8008 — 0.1695 + 5.6313 Luft 1. 78.9830 |+ 6| 49.3942 |+14|— 1|+16.8254 — 0.0008 —+16.8246 47.9600 |+19| 80.4135 |- 9] + 1| —14.1946 — 0.0020 — 14.1966 62.3710 |+12| 66.0220 |+11 + 0.2060 62.0035 |+12| 66.3910 |+11 — 0.1622 — 0.1634 61.6300 |+12| 66.7615 |+ 9 60.9430 [+13] 67.4530 |-+19 60.5785 |+13] 67.8260 |-+-19 60.1970 |+17| 68.2000 |-+19 | 59.4480 |13| 68.9460 |-+14 59.0765 |-+13| 69.3300 |+14 | 58.6840 |+13| 69.7010 |-+17 58.0210 |+ 8| 70.3770 |-+17 57.6500 |+ 8| 70.7520 |+13 57.2690 |+12| 71.1210 |+13 56.5620 |+ 2| 718290 |+12 56.1870 | 2| 72.2080 |-+12 55.8110 |+ 2| 72.5850 |+12 Trabant — Jupiterscentrum. vue | Mitte. (fat) Joan ват Pr | № mm mm 62.6710 |-+12| 65.7130 |+13 + 0.5104] -+0.6738 61.2330 |+13| 67.1535 |+11 — 0.9286] -+0.6669 59.7335 |+17| 68.6570 |+16 — 2.4302] -+0.6665 | -+0.6701 | -+0/6705 | -+0!0003 —0.0006 | -+o!ooos | +0:6708 58.3170 |+ 8| 70.0700 |+19 — 3.8456| -+0.6749 56.8510 |-+12| 71.5355 |+14 — 5.3108] -+0.6685 60.8825 |+11| 67.5015 |+ 9 — 1.2779] —1.1145 59.4400 |+11 68.9435 |<+14 — 2.7204] —1.1249 57.9465 |+ 6| 70.4390 |-+17 — 4.2153] — 1.1186 | —1.1195 | — 1.1201 | —0.0005 —0.0005 | -+0.0005 | —1.1196 56.5230 |+10| 71.8630 |+12 — 5.6386] — 1.1181 в; | 73-3265 |+14 — 7.1007| — 1.1214 60.2180 |-+-15| 68.1570 |-+18 — 1.9382| —1.7748 58.7770 |+1!| 69.6045 |+-16 — 3.3825| —1.7870 57.2770 |+10| 71.1010 |+12 — 4.8806| —1.7839 | —1.7829 | —1.7839 | —0,0008 +0.0006 | -+0.0005 | —1,7836 _55.8590 0] 72.5290 |+-13 — 6.3042] —1.7837 | 54.3950 |+ 4] 73-9865 |+12 — 7.7646] —1.7853 | 64.5060 |+21| 63.8780 |+13 + 2.3459] -2.5093 | 63.0700 |-+14| 65.3185 |-+21 + 0.9059] -+2.5024 | 61.5710 |+14| 66.8250 |+13 — 0.5954] -+2.5013 | -+2.5034 | 2.5047 | -+0.0012 —0,0028 | -+0.0005 | -+2,5036 | 60.1460 |+19| 68.2375 |-+23 — 2.0144] -+2.5061 58.6815 |+15| 69.7065 |-+21 — 3.4813] -+2.4980 | Scheinbare Decldiff: J—Centrum = — 0:2842 f°5 = 0.99815 1° 5 = —0.00164 F— » = + 9.0358 Н— » — + 3.5969 fs =0.99762 is = —0.00156 X i5 —6:4 К— » = -+14.8403 L— » — — 16.1267 f's = 1.00952 Js = —0.00020 dy = +12° 16.2 12 = Зап. Фпз.-Мат. Отд. 178 66 С. Scalenablesung. Object. P.-Kr. 0° + P.-Kr.180° SIT D RS 8 mm 61,5904 61.5895 40.5810 10.9802 110.0210 64.9625 66.8700 66.7480 67.1345 67.5295 66.7235 67.1185 67.5025 66.7340 67.1350 67.5305 66.7100 67.1075 67.4920 66.7250 67.1270 67.5160 68.8515 68.8265 68.8410 68.8120 68.8325 Als Höc 70.7980 70.7730 70.7830 70.7570 70.7800 63.0620 63.0400 63.0550 63.0265 63.0520 mm 10000 9 +24 +23 А +21 +16 ЕЕ rer ЕЕ Fr ТЕ со 00 O0 Do 00 00 Oo 00 O0 \O \O © mm 66.7937 66.7928 87.7920 117.3935 18.3640 63.4090 61.5085 61.6570 61.2595 60.8690 61.6735 61.2740 60.8900 61.6640 61.2645 60.8620 61.6915 61.2920 60.8975 61.6705 61.2760 60.8755 59.5325 59.5635 59.5465 59.5815 59.5555 57.5870 57.6120 57.5975 57.6290 57.6035 65.3200 65.3465 65.3340 65.3605 65.3345 Scheinbare ЖА: НЕ тт + 9 0.0000 — s|-+ 2] —21.0022 + 4|-+37| —50.6004 +-24|—33| 48.4258 +14 + 3.3788 +16|— 1] + 5.2823 12 +13 +13 11 ЕЕ ЕЕ ЕЕ ЕЕ + +17 F. ВЕми, 1897. Mai 18. № Фин Helsingforser Sternzeit 3 der Aufnahmen. Mittel. 2 15° 30” 35° 3—4 ellipt. 3 1—2 555-2292 FH 5-5194 + 5.5364 ] 26 + 5.5063 26 + 5.5259 ^ 27, 30 Trabant — Jupiterscentrum. 2—2 | Mittel. Malern) Лоу) Ph. | Аа cos à mm mm +1.7218 +1.7136 —+1.7124 | +1.7145 | -+1!7125 | —0!0026 | —0:0023 | 17076 +-1.7105 +1.7141 +-3.668; +-3.6630 +-3.6583 | 3.6627 | +3.6585 | —0.0054 | —0.0023 | -+3.6508 +3.6597 | -+3.6643 — 4.0670 —4.0714 45 —4.0747 | —4.0702 | —4.0655 | -+0.0057 | —0.0023 | —4,0621 — 4.0721 —4.0659 J—Centrum = —23'4052 f°4x—= 0.99810 —i9,, = +0.00196 F— » = —56,4536 H— » = +53.9986 fa = 0.99774 —iy —=-1+0,00190 X Ty = —6:5 К— » — + 3.8047 Кей. =+ 130 L— » = 5.8363 Те, =+ 35 JS’ = 0.99885 Ju = 0.00355 3 unterex рош | | POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897. Mai 15. ihe. Scalenablesung. : Е у P.-Kr.90° = P.-Kr. 270° |+-+# _mm_ mm | mm_ 10000| mm 10000] 10000 62.1620 66.2250 я 62.1610 |-10| 66.2240 |109] о 0.0000 61.8750 |+17| 66.5015 |-+22| 0] — 0.2820 71.3132 |+34| 59.0718 |-+28|— 7] + 9.1518 66.0182 |27| 62.3710 |-+26|— 3] + 3.8548 | 77.0372 |-+ 9] 51.3388 |-+-ı1l— 1] +14.8805 46.0138 |-+14| 82.3585 |+ 2|+- 1| —16.1402 56.6060 |-+ 9| 71.7890 |-+12 — 5.5602 56.9880 |+ 9| 71.4080 |+13 — 5.1787 57.3690 |+ 9| 71.0310 |-+13 — 4.7997 58.1010 |+ 5| 70.2930 |+17 — 4.0651 58.4860 |#+ 5) 69.9170 |+17 — 3.6846 58.8650 |+10| 69.5385 |+17 — 3.3056 59.5770 |+-14| 68.8170 |+14 — 2.5885 59.9720 |-+14| 68.4370 |-+19 — 2.2012 60.3580 |+-14| 68.0430 |-rı9 — 1.8112 60.9940 |+10|) 67.4010 |+ 9 — 1.1720 61.3790 |+-10|) 67.0225 |+ 9 — 0.7902 61.7625 |+ 9| 66.6330 |+ 9 — 0.4038 62.4600 |+ 9| 65.9380 |-rıı + 0.2924 62.8430 |+ 9| 65.5520 |+r1 + 0.6769 63.2260 |+ 9| 65.1740 |+17 + 1.0571 56.2420 O| 72.1460 |+13 — 5.9212 57.7400 | 6| 70.6510 |+14 — 4.4244 59.2330 |-+11| 69.1590 |+15 — 2:9317 - 60.6385 |+11| 67.7505 |-+20 — 1.5250 62.0980 |+10| 66.2900 |+12 — 0.0646 № Als Höciker ат Ostrandle er[kenn|bar, D _ 95.4530 0) 72.9305 |+16 — 6.7080 | 56.9550 +10) 71.4365 |+15 — 5.2095 58.4350 |+ 6| 69.9395 |+19 — 3.7214 59.8415 |+15| 68.5350 |+-21 — 2.3156 61.3140 |+11| 67.0700 |+11 — 0.8465 58.5820 |+11| 69.8040 |-+16 — 3.5798 60.0740 |+15| 68.3120 |+18 — 2.0876 61.5740 |+10] 66.8205 |+ 8 — 0.5916 62.9764 |+10| 65.4140 |+16 + 0.8124 64.4395 |+ 9| 63.9510 |+ 8 + 2.2758 Scheinbare Decldif: J—Centrum = — 0/2842 F— » = + 9.0358 Н— » = 3.5969 K= ‘5 = —+-14.8402 L— » = — 16.1267 бу = 12° 14'6 Decl. Ynt+act+4s 2 2 = $95 sin 1’ y — + $05 sin 1’ mm mm mm 0.0000 0.0000 — 0.0317 — 0.3137 — 0.1856 + 8.9662 — 0.1695 + 3.6853 — 0.0008 —+14.8797 — 0.0020 — 16.1422 5.1795 3.6851 2.2003 0.7887 0.6755 | Trabant — Jupiterscentrum, Yı—yz | Mittel. rate 9) |7 (реа) ато) тт —0.7417 —0.7393 —0.7314 —0.7363 —0.740I mm —0.7378 | —0:7380 | —0.0006 | —0:0007 | -+0!0005 —1.5285 — 1.5244 — 1.5211 — 1.5269 — 1.5220 +1.5997 —1.5975 —+1.6087 +1.6011 +1.6003 —1.5246 | —1.5250 | —0.0014 —0.0017 | -+0.0005 —+1.6015 | +1.6019 | —0.0015 -+0.0009 | 0.0005 15 = 0.99813 fs =0.99761 f’s = 1.00027 $ = —0.00166 ts =— 0.00188 Js = —0.00037 №7 Bemerkungen zur Aufnahme. |, 48 —0:7388 —+1,6048 9 180 66 D. Scalenablesung. Object. P.-Kr. 0° ++ P.-Kr.180° mm mm 1000| mm Ctr, | 61.6049 66.7824 41 61.6040 |+ 9| 66.7815 J 40.5942 +24| 87.7835 Е 10.9858 |-+22| 117.3890 H |110.0325 |+ 4| 18.5518 K 64.9755 |+21| 63.4008 L 66.8835 61.4960 4 y | 69.9090 58.4850 a. | 70.3175 58.0750 @о | 70.7200 57.6695 %Dy | 69.9190 58-4880 be 70.3115 58.0850 b, 70.7005 |-+13| 57.6865 %Cy | 69.8995 |+17| 58.5005 Ce 70.3100 |-+17| 58.0795 Co 70.7180 |-+13| 57.6675 % dy | 69.9110 |+17| 58.4950 de | 70.3090 |+17| 58.0920 do | 70.7020 |-+13| 57.6855 Ze | 69.9095 |+-18| 58.4920 ес 70.3090 |+18| 58.0920 ео | 70.7090 |+14| 57.6800 Та | 71.5290 |-+12| 56.8580 b | 71.5105 |-+12| 56.8750 се | 71.5165 [+13] 56.8675 d | 71.5000 |+13| 56.8865 е | 71.5050 |-+14| 56.8790 II Verfinstlert. Ша | 67.4580 |+ 9| 60.9295 b | 67.4430 |+ 9] 60.9395 с 67.4540 |+ 9| 60.9390 а | 67.4420 |+10| 60.9480 е | 67.4410 |11| 60.9490 ТУ Verfinstlert. Scheinbare Adiff: $ D t+-k der Aufnahmen. Mittel. тт mm 10000] 10000 mm 2—3 2 Bi ad nd 3—4 ellipt. 15° 22 40 san 2 2—3 En S +5 + 8.7088 №5 197 34 1—2 ==) то 5 “+ 8.7012 19 8 1—2 2 es) +5 + 8.7026 19 38 15% 19” 36° 2 5 es) +5 —+ 8.6992 20. 2 se + 6 +6 + 8.6998 20 36 2 + 6 Trabant — Jupiterscentrum. Lt—Ly | Mittel. даа) | Тоби Ph. | До cos à mm mm +-1.2156 3 —+1.2054 3 -+1.2108| 1.2061 | -+1!2045 | —0.0019 | —0/0023 | -+1!2003 | 3—4 +1.1965 3 | —+-1.2022 3 unterexponiert] + —2.8558 2—3 + —2.8608 3 + —2.8564 | —2.8603 | — 2.8565 | —0.0048 | —0.0023 | —2,8636] 3 + —2.8635 | 2—3 + — 2.8650 3 J— Centrum= —23'4052 1’. = 0.99801 —i°, = +0.00211 — nn ——58.4537 г с й Н— » =-53.9987 Га = 0.99765 —iy = 0.00205 x = — 10 К— » =-+ 3.8047 Rei — un L— » —=-+ 5.8363 Try =+ 55 fu = 0.99867 Л. = — 0.00376 Г. Renz, 1897. Mai 20. т ay = 10” 14.4 % w+r#ct?%o Helsingforser Sternzeit Bilder. 9 аа nn a = POSITIONEN DER JUPITRRSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897. Mai 20. 8.4338 Trabant — Jupiterscentrum. те. Scalenablesung. $ у |Р.-Кт. 90° ня P.-Kr. 270° [++ 2 тт mm mm Le 10000 10000] 10000 _ 62.1620 66.2250 >> 61.2072 |+11| 67.1772 |+ 8| 0) — 0.9534 60.9190 |+-18| 67.4558 |+20| o| — 1.2370 70.3530 |-+38| 58.0318 |-+23|— 7|-+ 8.1922 65.0618 |-+33| 63.3240 |+26|— 2| + 2.9006 76.0838 |+ 7| 52.2945 |+12| 0] +13.9259 | 45.0604 |+18| 83.3212 |+ 3|-+ 2| — 17.0980 63.9730 | 9| 64.4295 |+-10 + 1.8032 64.3520 |-+ 9| 64.0475 |+10 + 2.1837 64.7370 |+ 9| 63.6545 |-+Io + 2.5727 65.4800 |+11| 62.9185 |+-11 == Я» 65.8605 |-+-т1| 62.5410 |+11 + 3.6912 66.2350 |+ 11| 62.1580 |+11 + 4.0700 66.9145 |+ 9] 61.4845 |+12 + 4.7464 67.3000 |-+ 9] 61.1025 |+12 + 5.1301 67.6830 |+19| 60.7085 |+12 + 5.5191 68.3280 |+19| 60.0710 |-+16 + 6.1602 68.7175 |-+14| 59.6915 [+16 + 6.5444 69.0975 |-+14| 59.3000 |+-12 + 6.9304 69.8340 |+17| 58.5705 |+ 7 + 7.6538 70.2180 |+17| 58.1830 |+ 7 + 8.0495 70.5975 |+17| 57.7940 |+ 7 mr т 63.8595 |-+10] 64.5350 |-+19 + 1.6933 65.3600 |+18| 63.0270 |-+12 + 3.1983 66.8000 |+10| 61.5930 |-+12 + 4.6349 68.2140 |-+20| 60.1740 |+17 — 6.0516 69.7235 +18) 58.6695 |+13 + 7.5588 _ Verfinstlert. 2 65.6230 +10l 62.7625 |+10 + 3.4618 9.1230 + 8| 61.2650 |1 —= 4.9604 68.5675 |+13| 59.8205 |-+15 —= 6.4049 69.9845 |+16| 58.4020 |+ 6 + 7.8232 71.4860 |-+12| 56.8940 |+10 + 9.3276 Verfinstlert. Scheinbare Decldiff: J—Centrum = — 0/2842 — » = + 9.0358 H— » = + 3.5968 K— » = -+14.8402 L— » — —16.1267 dy = 12° 11'4 Decl. Ynt+%c+%s 3 + 2.1865 + 3.6911 + 6.5450 + 8.0457 с о \T vs | Ме. |7а ив ее) |-й-аз| Ph | тт тт — 0.4932 —0.4928 —0.4970 | —0.4927 —0.4934 —0.4869 —+1.2753 —+1.2693 —+1.2730 | -+1.2755 <+1.2782 +-1.2819 195 = 0.99801 fs = 0.99750 f's = 0.99993 —0:4927 | —0:0007 | —0:0007 | -0!0005 +-1.2755 | -+0.0016 +-0.0013 | -+0.0005 $ = —0.00172 î5 = —0.00192 X в=—6.6 Js; = — 0.00056 23* 181 о о Bemerkungen — 5 tgù sin 1 У— = tg0 sin 1 zur Aufnahme. mm mm 0.0000 — 0.9534 — 0.0317 — 1.2687 = 0.1856 —+ 8.0066 =. 0.1695 + 2.7311 — 0.0008 13.9251 — 0.0020 — 17.1000 Ai —0:4936 —+1,2789 [81 ieh NIRISIHIASOOTORT man. ART D aaa women 08 is Te 1000 ee, са тавоу соот | _ В OPPOSITION 4897. IL PULKOWAER CLICHÉS. = ве | < | DIT CICONTT nn | (ci # x Le ——_ ВНЕ ia у 1 > * sin ers; | Los | смех у oo | | rod8.0— ls | | + 1 09.0— | 1 | N hu] . | = À = | } HR | бобоя- | à ‘ Ce | | | у 4 и] | | ir | ‘ ET rn er | $ | | LE : у | [PET | р | : Br 9 : || bc “rt | l,3%0 | с _- 11559. | | {868 | 0 ER: N L f р } } be = nn м rat u MH — =” pe," u "he р LE off 2 110000 - nid» FU À se - = ro => ? m N 9 = Ba B | м [4 Be Re 184 F. Renz, 67. 1897. Februar 5. № 1 Scalenablesung. Pulkowaer Sternzeit | Object. = 8 x Ba Мок Bo PER RSR PORC R Er Bilder. | P.-Kr. 0° tt) P.-Kr.180° t-+-k ? der Aufnahmen. Mittel. = mm mm .. notes mm mm | Ctr. | 62.2934 66.0955 5 62.2925 66.0944 |+I1 I 4—5 | M | 67.2690 61.1052 |+10] 0OJj-+- 4.9829 4—5 | М 23.1355 105.2412 |+ 7 ; я 2 4—5 | Q | 75.8782 52.5060 |+-17 $: 520.120 4 Е 25.5715 102.8032 |-+15 4 v 61.9882 66.3895 |+17 4 | W |63.1375. 65.2438 |+30 4 % ay | 61.8340 66.5685 |+10 | ac | 62.2675 66.1240 |+10 — 0.0284 SE 7 4 | @ | 62.7000 65.6855 |+-10 | ZDy | 61.8499 66.5440 |+18 | b. | 62.2860 66.1110 |-+-IO — 0.0182 36 30 » 3—4 | 6, | 62.6970 65.6895 |+10 %с | 61.8385 66.5630 |+10 | Ce | 62.2595 66.1260 |+10 — 0.0315 37 44 . 3—4 | Co | 62.6975 65.7020 |+10 gr 38” 17° | % dy | 61.8340 66.5705 |+11 | de | 62.2545 66.1405 |+11 — 0.0430 39 14 3 | do | 62.6740 65.7150 |+11 %е | 61.8280 66.5715 |+11 i | ес | 62.2470 66.1410 |-HII — 0.0417 40 30 3 eo | 62.6845 65.7030 |-+11 | fo | 61.8005 66.6085 |+12 | с | 62.2440 66.1515 |+12 — 0.0508 41 42 3—4 | .6 65.68 fe EE т Trabant — Jupiterscentrum. Lt —Ly | Mittel. aan) Лиги Ph, | Aa. cos à mm mm { Та | 61.4405 |+11| 66.9480 — —0.8242 4 | b | 61.4350 |+11| 66.9530 — —0.8396 4—5 unterexp | с | 61.4140 |+-10| 66.9700 — 001681 Fay р р ©" 4 а | 61.4000 [+-10| 66.0880 = D. 0.8472 08415 | -н0:00от | 0.0004 | —0:8410 | 4 unterexp. e | 61.3885 |+10| 66.9955 — —0.8607 4 f | 61.3780 |+11| 67.0085 — —0.8634 5 ишегехроше | Па | 59.1020 |-+12| 69.2850 — 3.1622 4 | b | 59.1010 |+11| 69.2850 — — 3.1718 4 unterexponie | 2 Be: Be = —3.1700| —3.1486 | +-0.0004 | -+0.0004 | — 3.1478 er | е | 59.0780 |+10| 69.3100 : —3.1735 3—4 | f | 59.0685 |+-ı0| 69.3200 — 3.2249] — 3.1741 5 unterexponie® Ша | 64.1590 | 9| 64.2225 + 1.8694] +-1.8978 4 | b | 64.1655 |+- 9| 64.2150 —= 1.8764| -+1.8946 4 | 64.16 64. 8 -1.9058 : 3—4 à Fi RE À ie En N 4-1.9038 | +-1.8909 | —0.0002 | -+0.0004 | 1,8911 | 4 | e | 64.1560 | 9| 64.2300 —= 1.8640] -+1.9057 4 f | 64.1510 |+ 9| 64.2340 + 1.8594| +1.9102 5 IV & | 53.4360 |+10| 74.9510 — 8.8566] —8.8282 4 b | 53.4415 |+ 9| 74.9435 — 8.8500] —8.8318 3—4 ищегехрой | с .4370 |+ .9530 — 8.8570] —8.82 4 » | d sun 53 à te Er 8821 828% — 8.8295 | +8.7698 | 0.0010 | -+0.0004 | —8,7684 | , $ | е | 53.4185 |+ 7| 74.9695 — 8.8746] —8.8329 4 | f | 53.4120 |+ 7| 74.9755 — 8.8809] —8.8 301 5 unterexponl | Scheinbare Adiff: M—Centrum = + 5:2700 Fa —=0:99319 —1°, = —0.00011 | N— » — — 41.4062 9— » —+14:3237 fa = 0.99291 —i, =— 0.00011 X и = + 04 | R— » — —38,7083 Ве. =— 14 | V— » = — 0.3205 Yan = o W—- » = + 0.8887 Хо. = 0.99324 Jy ——0.00025 ay = то" 28.7 bihe. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. mm » 10000] 10000 | Scalenablesung. | F ‚-Кг. 90° te. Кг. 270° 2+ Е mm | 63736 1000 67163 | 63. 3726 |+10| 65.0152 |+-16 р 66.3908 |+10| 61.9920 |-+10 66.9282 |+24| 61.4560 |-+27 | 38.7860 |-+29| 89.6020 |— 4 | 38.8060 |+41| 89.5730 |+ 8 | 43.9782 |+20| 84.4060 |— 7 94.3142 |— 2| 34.0780 |+20 | 68.5110 |+19| 59.8965 |+14 | 68.0945 |+19| 60.3125 |<+14 | 67.6690 |+-19| 60.7260 |+-10 66.8945 |+ 9| 61.5030 |+ 9 | 66.4975 |+11| 61.9140 |+ 9 | 66.0945 |-+11| 62.3075 |+ 9 В 65.3515 |+17| 63.0500 |+9 64.9503 |+17| 63.4620 |+ 9 1 64.5160 |-+17| 63.8680 |+ 9 `62.т97о +10] 66.2080 |+10 | 61.7860 |+10| 66.6200 |+ 8 | 61.3790 |+-10| 67.0170 |+ 8 60.5830 |+-15| 67.8170 |+18 ° 60.1780 |-+15| 68.2210 |+18 59.7625 |+15| 68.6255 |-+18 | 590280 +-11| 69.3720 |-+13 | 58.5940 |-+11| 69.8020 |4-16 | 58.1505 |+ 6| 70.2390 |-+-16 | | 68.5020 |-++14| 59.8930 |-+14 66.9145 + 9| 61.4820 |+10 65.3645 |+17| 63.0305 |+ 9 62.2130 |+10| 66.1835 |+10 60.6050 |+11| 67.7915 |+18 59.0210 |-+-11| 69.3700 |-+13 69.5395 |-+18| 58.8515 |+-11 7.9470 |+20| 60.4490 |+15 6.3960 |+12| 62.0060 |+10 63.2405 |+11| 65.1550 |+17 | ‚61.6270 |+11| 66.7690 [+9 60.0450 |-+16| 68.3480 |+-19 67.1030 |+ 8| 61.2810 |+ıc 65.5050 |+10| 62.8860 |+ 9 1M63-9550 |+ 8| 644390 |+ 8 0.7940 |+10| 67.5940 |+18 | 59.18то |+10| 69.2090 |+-13 Я 57.5990 |+ 5| 70.7875 |+12 à 71.9500 |-+15| 56.4430 |+- 3 70.3505 |+20| 58.0430 |+ 9 1 68.8050 |+17| 59.5920 |+18 65.6455 |-+14| 62.7490 |+13 | 64.0315 |+12| 64.3610 |+12 62.4555 |-+13| 65.9405 |+14 _ Scheinbare Decldiff: М— Centrum RE © В и W— Зап. Pns.-Mar. Отд, 1897. AT: oi AE: ras DIS ISSUE EE EURE E à, LS TE РЕНН = 30.7313 2: 97.3 4.7118 == 31153 +0.4143 -+0.4225 —+0.4274 0.4286 -+-0.4299 —0.4324 —1.4542 1.4555 1.4551 +1.4562 +-1.4526 +1.4554 — 0.9793 — 0.9841 —0.9820 —0.9866 —0.9907 —0.9876 -+3.8639 -+3.8606 3.8664 —+-3.8621 3.8587 —3.8644 1.5616 1.5922 3.2019 4.7854 mm +0.4259 —+1.4548 —0.9850 3.8627 f°5 = 0.99337 fs = 0.99288 Гу = 0.99367 Februar 5. ес]. mm 0.0000 0.0013 0.0811 0,0094 0.0694 0.0000 0,0000 A Trabant — Jupiterscentrum. 2 N mur | Mittel. [fat] 7 (газ виа) 2 RES ’ > tgö sin 1 +-0:4232 | -+0'0002 +-1.4456 | 0.0006 —0.9788 | —0.0003 —3.8383 | -+0.0016 $$ = 0.00050 is = 0.00001 Js; = —0.00017 y — +98 sin 1’ тт 0.0000 + 3.0197 + 3.4763 —24.5936 — 24.6282 —19.3908 —+30.9378 0'0000 0.0000 —0.0091 —0.0020 х is = оо zur Aufnahme, Bilder 4—5. Bilder 4. Ph. 0.0900 0.0200 0.0000 0.0000 Bemerkungen —0:4234 +-1,4462 —0,9792 +-3,8379 Object. (==) + - эконо | = bd -ч -ч bd -ч SOLS TR RO 8 Зозеосеа Togo Se IV Scalenablesung. P.-Kr. 0° 62.4549 62.4540 67.4262 23.2945 76.0610 25.7510 62.1610 63.2760 61.9680 62.4270 62.8835 61.9770 62.4250 62.8685 61.9725 62.4150 62.8585 61.9645 62.4010 62.8505 62.0075 62.4345 62.8840 61.9825 62.4355 62.8845 61.7400 61.7280 61.7185 61.6960 61.7260 61.7145 65.4320 65.4230 65.4220 65.4065 65.4470 65.4415 67.5035 67.4960 67.4950 67.4760 67.5175 67.5050 57-4750 57-4650 57.4590 57-4460 57.4760 57-4650 Scheinbare Adiff: M—Centrum mm 10000 ва) вела © —25 —+-20 SE] +18 +21 Io Io Il ale) —=10 НСО) \O \O _\O \O \O \0 0 0 Fr ЕЕ ЕЕ ея 9 ТО 10 t+-k|P.-Kr.180° mm 65,9293 65.9282 60.9500 105.0882 52.3260 102.6248 66.2120 65.1098 65.4205 65.9735 65.5110 66.4165 65.9735 65.5425 66.4195 65.9885 65.5385 66.4310 65.9970 65.5475 66.3960 65.9665 65.5195 66.4090 65.9670 65.5145 66.6510 66.6620 66.6730 66.6905 66.6635 66.6750 62.9555 62.9675 62.9665 62.9790 62.9405 62.9445 60.8755 60.883 5 60.8905 60.9070 60.8630 60.8730 70.9165 70.9245 70.9310 70.9480 70.9120 70.9230 Е. Renz, 1897. März 7. t+-k mm_| mm 10000! 10000 N eZ » Q— » R— » V— » W— » Egg RARE + 5.2703 — — 41.4077 =-+14.3248 — — 38.7098 = — 0.3202 = -+ 0.8890 h т Xy—= 10 24.3 Lt Ty 0.0398 0.0463 0.0562 0.0222 — 0.0276 Mittel. mm —0.6994 —=3.0т00 +-5.0836 —4.9560 Ja = 0.99322 fu = 0.99287 Ла = 0.99316 Pulkowaer Sternzeit der Aufnahmen. Mittel. 11° 14“ 45° тт 220055 РД 25 7] 117 25” 52° 2604.23 27315 280057 —0.6946 —+2.9894 + 5.0488 —4.9221 —0'0002 — 0.0009 —0.0014 +-0.0014 Trabant — Jupiterscentrum. Лаба (ии) Ph. | До cos à —0!0002 —-0.C002 —0.0002 —0.0002 re: — 1% = +0.00067 о Refr. 31 Ty Je = -+0.00057 + 6 — о = +0.00063 —0:6946 + 2.9883 +-5,0472 —4,9209 x T—— | is al ыы > O9 O2 O9 O9 > ON OÙ © в 3—4 unsymm. (ll Bilder. | | _ М. | | POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 187 1597. März 7. eiıhe. Decl. 3 Scalenablesung. nas + RES Zr Bemerkungen a у ИЕ DRE — 5 #9631 1 y — = #96 sin 1' zur Aufnahme p:-Kr.90° + P.-Kr.270° |t+# 3 3 2 PDA у р тт тт и u mm mm mm mm 63.0798 65.3100 1000110000 | 63.0788 65.3084 |+16 ol 0.0000 0.0000 0.0000 Bilder 3. Undurch- 66.1005 62.2798 |109] o|+- 3.0254 — 0.0013 + 3.0241 sichtige Luft. 66.6242 61.7662 |+26|— 1|+ 3.5439 — 0.0811 + 3.4628 | 38.4955 89.8955 |— 3|-+ 4] —24.5829 — 0.0094 — 24.5925 | 38.4975 89.8790 | 8|-+14| —24.5726 — 0`0694 — 24.6420 | 43.6850 84.6915 |— 2] 2| —19.3868 0.0000 —19.3868 | 94.0222 34.3715 |+-20]—19|-+-30.9374 0.0000 +-30.9374 68.2630 60.1400 |+-14 + 5.1768 67.8495 60.5530 |+10 + 4.7638 + 4.7572 67.4100 60.9790 |+10 + 4.3310 | 66.6570 61.7350 + 9 ze | 66.2540 62.1640 |+ 9 + 3.1602 + 3.1627 | 65.8350 62.5620 |+ 9 + 2.7517 64.9220 63.4735 |+ 8 + 1.8398 64.5150 63.8910 |+ 8 — 1.4326 — 1.4254 ‚64.0870 64.3095 |+ 8 —= 1.0039 61.9660 66.4270 |+ 8 — 1.1155 61.5620 66.8415 |+ 8 — 1.5246 — 1.5275 61.1425 67.2580 |+ 8 — 1.9425 60.2310 68.1680 |+18 — 2.8536 59.8160 68.5870 |+13 — 3.2703 — 3.2742 59.3860 69.0135 |+13 — 3.6986 58.4905 69.9195 +16 — 4.5999 58.0660 70.3465 |-+16 — 5.0256 — 5.0255 | A .76 se 57.6345 er aan Trabant — Jupiterscentrum. . > Ш УЕ— Ух | Mittel. и ‘вгу Ts (ео) ета РВ. | AG mm тт 60.2100 |+14 + 5.1004] -+0.3432 61.7990 |+ 9 + 3.5151| —+0.3524 Bi La ро EN RE +0.3531 | -++0/3508 | -+0/0003 0!0000 0!0000 | +0!3511 68.2245 |+18 — 2.9158| +0.3584 69.9735 |+16 — 4.6649] .-+0.3606 61.9220 |+10 — 3.3898] — 1.3674 an + 9 + 1.8052 13575 —1.3672 Das EA Er ES Se ar —1.3635 | —1.3548 | —0.0014 | —-0.0003 0.0000 | —1.3565 69.9470 |+17 — 4.6375] —1.3633 71.6980 |-+-12 — 6.3883] —1.3628 62.7570 |+10 + 2.5481| —2.2C9I 64.3400 |+ 9 + 0.9653| —2.1974 Be Le = SL: ee — 2.2034 | —2.1892 | —0.0024 | .—0.0007 0.0000 | —2,1923 70.7830 |+13 — 5.4778| —2.2036 72.5300 |+14 — 7.2266] —2.2011 58.2935 |+ 6 + 7.0198] -+2.2626 59.8710 |+15 + 5.4445] 2.2818 а же = IR her -+2.2726 | -+2.2580 | -+0.0024 —0.0007 0.0000 +-2,2597 66.3110 |+11 — 0.9985| -+2.2757 68.0610 |+19 — 2.7502| -+2.2753 Scheinbare Decldif. M--Centrum — + 3/0033 f°5 = 0.9935 1 1° $ = —0.00036 — » =-r 3.4515 . Q— » — — 24.4335 fs = 0.99291 is =— 0.00056 X щ=- 19 K— » — —24.4647 У—‹» — — 19.2648 J's = 0.99357 Лу = —0.00048 W—- » = -+30.7327 188 К. Renz, 70. 1597. März 9. № Scalenablesung. Pulkowaer Sternzeit OH PR ee À & © а re P.-Kr. 0° ыы P.-Kr.180° |#+% > der Aufnahmen. Mittel. mm > To mm Toon Su mm mm (г. | 66.2385 62.1472 S 66.2375 |+10| 62.1462 |+-10| oO 0.0000 9.8 M 71.2125 +13] 57.1618 |= 9 ©] + 4.9799 2 N 27.0792 |-+23| 101.2980 |+ 3|+-18| —39.1522 ñ pre. 1—2 Q 79.8199 |-+21| 48.5642 |+23|— 3] +13.5814 $ 54 36 2 В 29.5108 |+-30| 98.8605 |+11|+21| —36.7174 2 У 65.9255 |+19| 62.4472 |416] 0|— 0.3064 2—3 W 67.0842 |-+20| 61.2930 |+25| o|<+ 0.8497 2 %а | 65.8380 |[11| 62.5565 |+ 9 — 0.4048 ag | 66.2730 |+11| 62.1290 |+ 9 + 0.0264 + 0.0261 тт 153046 3 ap | 66.7015 |+ 9] 61.6970 |+ 9 + 0.4566 2 by | 65.8300 +11) 62.5610 |+ 9 — 0.4110 De 66.2550 |+11| 62.1375 |+ 9 + 0.0132 + 0.0135 55 8 3 b, 66.6830 |+ 9| 61.7150 |+ 9 — 0.4384 YC | 65.8790 |--11| 62.5325 |+ 9 — 0.3723 CE 66.2890 |+11| 62.1025 |+ 9 + 0.0477 + 0.0503 56 18 3 c 66.7170 |+ 9] 61.6750 |+ 9 + 0.4754 117 56” 54 %а., | 65.8210 |+10| 62.5709 |+-I0 — 0.4202 с | 66.2689 |+10| 62.1230 |+10 + 0.0268 + 0.0221 у A6 9—3 dy | 66.7030 |+ 8| 61.6920 |+10 + 0.4598 Ze | 65.8265 |+10| 62.5660 |+-10 — 0.4154 ес 66.2440 |+10| 62.1450 |+10 —= 0.0038 = 0.0082 58 44 2—3 ео 66.6815 |+ 8| 61.7175 |+10 + 0.4362 A fo: | 65.8365 |-11| 62.5595 |-+11 — 0.4072 С 66.2605 |-11| 62.1310 |+I1 + 0.0191 —= 0.0174 59 51 2—8 fo RE Te er Trabant — Jupiterscentrum. ж— хо | Mittel. еее) Te (ги) Ph. | Ac cos à EI EE ER US RU AR ER PP _ mm mm lbs 64.3700 |+10| 64.0165 |+ 9 — 1.8688] —1.8949 2 b 64.3570 |+ 9| 64.0330 |+ 8 — 1.8836] —1.8971 28 с 64.3955 |+ 9| 63.9915 |+ 8 — 1.8436] —1.8939 | __ Аб ах 7 pete 2—3 Fes 61 8] Toro |919 18772 21.8098 1.8997 1.8869 0!0002 0:0002 1:8873 Ш е 64.3445 |+ 8| 64.0430 |+ 9 — 1.8950] —1.9032 2—5 f | 64-3455 |+ 9] 64.0390 |+10 — 1.8924| —1.9098 2—3 Па 63.0605 |+11| 65.3210 |+17 3.1762| —3.2023 2 b | 63.0540 |+10| 65.3309 |+16 — 3.1840] —3.1975 2 С 63.0960 |+10| 65.2910 |+16 — 3.1434] —3.1937 | _ M: LA Ri: & 2—3 а | 63.0630 |+ 9 653190 |+17 — 3.1740] —3.1961 3.1977 3.1762 0.0003 0.0002 3.1767 9—8 e 63.0470 |+ 9| 65.3360 |-+17 — 3.1906] — 3.1988 2—5 f | 63.0580 |+ 9| 65.3265 |+17 — 3.1803| —3.1977 2—3 Ша | 64.5985 |+-18| 63.7875 |+ — 1.6397| —1.6658 2—8 b | 64.5820 |+17| 63.8030 |+ — 1.6557| —1.6692 9—3 с | 64.6225 |+17| 63.7630 |+ — 1.6154] —1.6657 | __ 28, a ar au 2—3 al 64.9825 16| 63.8045 |+ — 1.6563| —1.6784 1.6750 1.6637 0.0092 0.0002 1.6641 2—3 е 64.5635 |+16 63.8200 |+ 9 — 1.6736| —1.6818 2—8 f | 64.5665 |-+17| 63.8195 |+10 — 1.6718| — 1.6892 3 IVa | 57.4500 |+12| 70.9335 |+14 — 8.7875| — 8.8136 о b 57.4380 |+11| 70.9500 |+13 — 8.8018| —8.8153 9 С 57.4790 |--11| 70.9115 |+13 — 8.7620] —8.8123 | _ 2% DR 40 Egg 2 a | 7.4435 +. 70.9415 | +12 — 8.7947| —8.8168 8.8169 8.7576 0.0008 0.0002 8.1586 | 5 е 57.4295 |+ 9 70.9615 |+13 — 8.8118| —8.8200 2 f | 57.4335 |+ 9] 70.9535 |+13 — 8.8058] —8.8232 2 Scheinbare ЖАШ: M—-Centrum = = 52703 70199824 —i°, = —0.00028 N— 1)» = —41.4078 : Q— » =-14.3248 fx = 0.99296 —iy = — 0.00029 X %=- 10 R— » — —38.7099 Ве. =-н 9 У— » = — 0.3202 тои == о W— » —+ 0.8890 f'a = 099327 Л. = — 0.00020 POoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN, 189 1597. März 9. il e. Decl. | Г Scalenablesung. y "пн сн; ы® 52 198 sin 1, + ÿ sin 1’ Bemerkungen ти = —— y — — tgù sin ый . | .-Кт.90° НР. -Kr.270°|t+% 5 - RE Fa N _тт_ тт mm | | 63.3164 10000 65.0740 10000 10000 тт тт тт тт 65.0723 |+17 о 0.C000 0.0000 0.0000 62.0460 ©] + 3.0214 — 0.013 + 3.0201 Bilder 2. 61.5068 — 1]+ 3.5656 — 0,0811 + 3.4845 89.6628 + 4] —24.5884 — 0.0094 —24.5978 89.6212 +13| —24.5631 — 0.0694 —24.6325 84.4620 + 2] —19.3902 0.0009 — 19.3902 34.1352 — 8] +30.9 0.0000 +-30.9358 59.9170 de 60.3305 + + 4.7468 Bilder 1—2. 60.7450 I 61.5110 ge 61.9265 + 3. + 3.1616 62.3220 |+10 — 2.7588 6, 2595 63.1420 |+10 + 1.9378 64.8720 63.5365 |+ 9 + 1.5469 + 1.5430 | 64.4705 63.9400 |+ 9 + 1.1444 | 62.1960 66.1970 |+11 — 1.1218 61.7845 66.6210 + 9 — 1.5394 = 7995 | 61. 3620 67.0330 |+ 9 — 1.9566 60.6035 67.7860 |+19 — Au | 60.2100 68.1880 |+19 — 3.1104 — 3.1126 68.5915 |+19 — 3.5147 69.4510 |-17 — 4.3736 69.8485 |+17 — a — 4.7697 Se LE Trabant — Jupiterscentrum. vx | Mittel. | Уабитиа | Лего) -вы-ай) | Pi. Аз тт тт 59.4810 + 5.5930| 0.8462 61.0725 + 4.0022] -+0 8406 . 62.6860 + 2.3894| -+0.8464 ‚ sh sr ‚ 1220, 65.7690 — 0.6938] 40.8455 —=0.8452 | -+0.8399 0.0004 0.0001 0:00c0 | -+0:8394 67.3380 — 2.2656] +0.8470 68.9970 — 3.9244| <+0.8453 58.9110 + 6.1628| -+1.4160 60.5090 + 4.5728] 1.4112 62.1140 + 2.9589] —1.4159 = = - 66/2000 Ml 1.008 +1.4148 | -+1.4059 0.0006 0.0003 0.0000 | -+1,4050 66.7710 — 1.6951| -+1.4175 68.4270 — 3.3551 +-1.4146 59.4730 + 5.5997] —<-0.8529 61.0625 + 4.0120] -+0.8504 62.6765 + 2.3981| -+0.8551 = И № р 40: 65.7575 ea rer -+0.8550 | -+0.8496 0.0003 0.0001 0.0000 0,8492 .0620 67.3250 — 2.2526| -+0.8600 5 4010 : 68.9855 — 3.9136] -+0.8561 1.8970 56.4940 [6) + 8.5810] -+3.8342 u» 58.0820 |+ 6 + 6.9924 Be .6920 9.6960 |+15 + 5.3768] -+3-833 = a №. 608о 62.7835 ne a 22018 23.8305 —=3.8330 | -+3.8087 0.0017 0.0023 0.00c0 | -+3,8047 ‚64.0405 64.3495 |+-9 + 0.7244| -+3.8370 6. 3805 66. 0140 [+11 — 0.9379] —+3.8318 | Do Decldif: M—Centrum = + 3/0033 f°5 = 0.99347 4° 5 = +0.00008 N— » = + 3.4545 ; 1 Г Q— » == —24.4335 fs = 0.99298 i3 = 0.00006 X 15 = +02 R— » — — 24.4648 У » ——19.2648 f'5s = 0.99367 Лу = -+ 0.00019 W— эм’ =-0.7327 бу = -н11° 30:0 2А* 190 Е. Renz, Ti: 1897. März 10. № Object Scalenablesung. a À + Фо Pulkowaer Sternzeit P.-Kr. 0° Fer” P.-Kr. 180° t+% 3 der Aufnahmen. Mittel. on AL Am le in Ctr. | 62.6870 10599 65,6991 | 1900110000 5 62.6861 + 9| 65.6980 [+11] о 0.000C M 67.6588 |+19| 60.7120 |+10| O|j-+ 4.9799 N 23.5295 |+26| 104.8480 |+ 7|-+18| —39.1504 ; SER DE Q 76.2788 |+19| 52.0998 |#+211— 3|+13.5952 8° 52 46 Е 25.9725 |-+36| 102.3948 |-+14|-+20] —36.7020 у т Go (a Ro mm mm | © D en © 62.3855 |+-18| 65.9815 |+17 0] — 0.2919 —3 63.5190 |+20| 64.8588 |+31 c|+ 0.8356 4 62.2495 | +10) 66.1395 |+10 — 0.4390 а 62.6000 |+10| 65.7055 |+10 — 0.0917 — 0.0055 8 40 36 3—4 63.1110 |+10| 65.2740 |+16 + 0.4242 2b, | 62.2360 |+10| 66.1590 |+10 — 0.45954 be | 62.6580 +10] 65.7260 |+10 — 0.0280 — 0.0326 ИМ 3 bd, | 63.0745 |+10| 65.3150 |+16 + 0.3855 %с | 62.2455 |+10| 66.1485 |+10 — 0-4454 Ce 62.6590 |+10| 65.7195 |+10 — 0.0242 — 0.0219 43 2 h Asa Co | 63.0945 |+10| 65.4980 |+16 + 0.4040 8 48" 48 Zd | 62.2410 |+ 9 66.1545 |-H11 — 0.4508 de 62.6740 |+ 9 65.7160 |+r1 — 0.0150 — DONS 44:34 3 do | 63.1105 |+ 9| 65.2770 |+17 — 0.4224 И Ze. | 62.2360 |+ 9] 66.1560 |+r1 — 0.4540 €; 62.6505 + 9| 65.7380 |-+11 010878 — 0.0334 45 48 2—3 en 63.0850 |+ 9) 65.3130 |+17 + 0.3916 Afw | 62.2015 |+10| 66.1875 |+-12 — 0.4870 Yo 62.6340 |+10| 65.7630 |+-12 — 0.0586 — 0.0655 46 46 2—3 Jo | 63.0400 |+10| 65.3530 |+18 + 0.3492 Trabant — Jupiterscentrum. æ—%y | Mittel. Klare) Ta ev) Ph. | Ac cos à. тт тт Та | 64.5420 |+17| 63.8415 |+ 8 —= 1.8568! +1.8623 2 ‚ D | 64.5165 |-+17| 63.8685 |- 8 —+ 1.8303 Ge 2 с | 64.5275 +-16| 63.8595 |+ 8 —= 1.8404| +1.8623 ' Pi lan "= 2 4 | 64.5380 \rıel 63.8485 |+ 4 1.8512] +1.8657 —+1.8650 | +1:8526 9.0004 0.0022 | +1.8520 | 5 e | 64.5210 |+17| 63.8630 |-+-10 + 1.8354] +-1.8688 2 f | 64.4900 |+17| 63.8980 |+11 + 1.8024] 1.8679 2 II Bedeckt. Ша | 58.1415 |+ 7| 70.2390 |+17 — 4.5432| —4.5377 2 b | 58.1105 |+ 6| 70.2700 |+16 — 4.5742] —4.5416 2 e | 58.1185 |+ 6| 70.2615 |+16 — 4.5660] —4.5441 | _ 28 A AR 2 4 | 581240 + ; are Br En chat 4.5434 4.5131 | —<-0.0009 0.0002 4,5124 | о е 58.1070 |+ 5| 70.2715 |-+17 — 4.57681] —4.5434 2 J | 58.0700 |+ 5| 70.3105 |+17 — 4.6148| —4.5493 Du IVa | 53.6580 |+ 6| 74.7230 |+12 — 9.0268| — 9.0213 2—3 b 522270 9 74.7540 |+1I1 — 9.0578| —9.0252 À e | 53.6420 |+ 5| 74.7440 [+11 — 9.0452] —09:023 3) HA “ ha 4 | 53.6510 |+ 4| 74.7370 |+10 — 09.0372] —9.0227 7 8.96361 --б.00ту > 8.9621 2 е 53-6280 |+ 3| 74.7555 |+10 — 9.0580] —9.0246 2 f | 53.5980 |+ 3| 74.7900 |+11 — 9.0904] —9.0249 2—3 Scheinbare ЖА: M—Centrum = + 5.2703 50.9987 —# = +-0.00028 N— » = —41.4079 Q— » = -+14.3248 fx = 0.99299 —% = +0.00027 X dy = — 09 В » = — 38.7100 Refr. = -= 16 У— » = — 0.}202 Try = о W— » = -+ 0,8890 Ing = 0.99334 4597 = 0.00013 . a Г А т ay = 10 23.0 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 191 Scalenablesung. | P.-Kr.90° tt P.-Kr.270° 65.0148 61.9900 61.4680 89.6002 89.5820 84.4058 34.0778 59.8900 60.3090 60.7200 61.5005 t+k +16 501 64 |79000| 10000 mm 61.9010 |-+ 9 62.3010 |+ 9 63.0330 |+ 9 63.4290 |+ 9 63.8310 |+ 9 66.3410 |+-10 | 66.7580 |+ 8 Ha 1.2220 67.1685 |+ 8 60.3965 67.9985 |+-18 59.9950 68.3920 |+18 59.5955 68.8015 58.8760 69.5115 58.4755 69.9065 5 8.0890 70.3025 61.1250 62.7200 64.2510 67.5750 69.2205 70.7320 58.2645 + 6 59.8610 |+15 61.3910 |+11 64.7145 : |+17 66.3555 |+-11 67.8695 |+19 56.4595 |+ 2 58.0510 |- 8 59.5830 |+17 62.9055 |+12 64.5465 |+19 66.0590 |-+13 1897. März 10. Decl. 2 2 Bemerkung ee ЖИР ee! erkungen 5 tgù sin 1 y— 5 tgösin1 zur Aufnahme, mm mm mın mm 0.0000 0.0000 — 0,0013 — 3.0261 Bilder 2. — 0.0811 + 3.4671 — 0.0094 — 24.5910 — 0.0694 — 24.6389 0.0000 — 19.3933 0.000 -+30,9396 1.3388] -+2.0366 2.8489] -+2.0395 8.5614] -+3.8480 6.9663| —3.8465 raie Re +-3.8466 | -+3.8222 | +0.0011 | —-0.0024 0.0000 | -+3,8209 0.4704| -—+3.8458 1.0416] -+3.8468 -1- + — 4.7134 = — — 3.1196 —+ 3.1198 + 2.7200 + 1.9911 — 1.5896 + 1.5898 + 1.1888 — 1.3198 == 057352 —= 1.7352 — 2.1476 — 2.9757 — 8:3732 == 2:3054 — 3.7774 — — 4.8884 55 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. Ir ‘вуз (и) era) Ph. | A wer + —0.8226 = == —0.8234 La Br —0.8251 | —0:8199 | —0.0002 — 0.0001 0.0000 —0/8202 = —0.8296 — —0.8263 — 6.7525| -+2.0391 + 5.1574 AQU T Е к 2.0377 | +2.0247 | +0.0005 | —0.0006 | 0.0000 | -+2,0246 ЕН = + 3.0033 198 = 0.99334 1°5 = —0.000}32 = + 3.4545 = —24.4335 fs = 0.99285 is = — 0.00034 X 5 = —1'2 = —21.4648 = — 19.2648 fs = 0.99364 Js = —0.00012 = +30.7327 ©’ + | - = = о — x} © 192 Е. ВЕХИ, 72. 1597. März 11. Scalenablesung. Pulkowaer Sternzeit Object. - Bilde Р.-Кг. 0° | t+%| P.-Kr.180° | é+X ре der Aufnahmen. | Mittel. | mm т о mm soie 1 0008 mm mm Ctr. | 60.8095 || 67.5839 | я 60.8085 |-+то| 67.5820 |+19| о 0.0000 3 || M 65.7858 |+11| 62.5952 + 9 O|-+ 4.9826 р ГВ М 21.6510 |+25| 106.7408 |+ 5-18 — 39.1549 , RAR 2 | Q 74.4008 |+25| 53.9868 +13 — 3| + 13.5945 9" 30” 15 D LÉ R 24.0950 |+-38| 104.2835 2166-20 — 36.7040 9 1 й 60.5105 |-+20| 67.8682 |+25 — 0.2919 ео W 61.6382 |+21| 66.7475 |+23 —+ 0.8324 99 фаз | 60.3345 |+15| 68.0720 |+18 — 0.4817 м. Ag 60.7565 |+11| 67.6405 |+18 005621 — 0.0559 9 Sie 3 М. а, | 61.1815 |--м| 67.2180 |-- 8 — 0.3691 N 2b, | 60.3530 |+-15| 68.0450 |+-18 — 0.4590 1 be 60.7745 |11| 67.6170 |+18 — 0.0344 — 0.0353 2821125 . 3 | b, 61.1990 |+-11| 67.1990 |+ 8 + 0.3874 | 2 Co 60.3285 |+15| 68.0790 |+18 — 0.4882 [I ch 60.7275 |+11| 67.6585 |+18 — 0.0786 — 0.0758 39 122 р от 2—3 4: 60 61.1515 |-=11| 67.2475 |+ 8 + 0.3394 9° 39 47 le % dy | 60.3295 |+10| 68.0855 |+19 — 0.4912 | de 60.7390 |+-10| 67.6495 |+19 — 0.0685 — 0.0684 22 3 | do 61.1645 |+10| 67.2300 |+ 9 + 0.3545 И Фе, | 60.3490 |+10| 68.0680 |-+-19 — 0.4728 | er 60.7565 |+10| 67.6420 |+19 — 0.056C — 0.0548 42110628 DB | ео 61.1750 |+10| 67.2205 |- 9 —= 0.3645 Af Verzerrt,| wah/|rscheinlich | dur|c eine Erselhütterung des Ferulrohrs während der |Aufnahme. I Trabaut — Jupitersceutrum. | ar | Mittel. ааа) иен Ph. | Ka cos mm mm Та | 58.7670 |+-Iı| 69.6270 |+17 — 2.0431] — 1.9872 9—3 b 58.7865 |11| 69.6020 |+16 — 2,0208| —1.9855 | 9025 € 58.7475 |+ı1| 69.6440 |+16 — 2.0613| —1.9855 | —1.9868 | —ı!9733 | -+oloco2 | —o'ocoz | —1'9734 | 2—3 d | 58.7510 |+10| 69.6425 |+17 — 2.0589] — 1.9905 ses e 58.7675 |+10| 69.6210 |+17 — 2.0359] — 1.9851 =: Па | 63.7440 |- 9| 64.6455 |+16 + 2.9361| +2.9920 о | b | 63.7635 |+ 8| 64.6260 |+16 —= 2.9556| +2.9909 2—8 | с | 63.7195 |-+ 8| 64.6660 |-+16 + 2.9136] 2.9894 | 2.9886 | -+2.9683 | —0.0004 | —0.0c03 | -+2,9676| 2-3 | d | 63.7235 |+ 8| 64.6660 |+17 + 2.9155| -+2.9839 2—3 | e 63.7380 |+ 9| 64.6480 |+18 + 2,9318] 2.9866 р | Ша 56.1270 |+ 1| 72.2610 |+12 — 4.6804| —4.6245 2—3 | b 56.1500 О] 72.2370 |+I1 4.6568! —4.6215 Be | с 56.1180 o| 72.2770 |+11 — 4.6938] —4.6180| —4.6201 | — 1.5886 | +0.000$ | —0.0003 | —4.5884 | 2 | а 56.1210 |— 1| 72.2710 | И — 4.6884] —4.6200 ® e 56.1370 |— ı| 72.2530 |-+12 — 4.6714] —4.6166 2 IVa 52.7175 |+10| 75.6710 |+ — 8,0894] — 8.0335 о Ь | 52.7430 |+ 9| 75.6495 |+ 5 — 8.0660] —8.0307 | 2 e | 52.7065 |+ 8| 75.6885 |+ 7 — 8.1038| —8.0280| —8.0301| —7.9753 | —o.coo9 | —0.000; | —7,9747 | 2 Я | 52.7115 |+ 7| 75.680 |+ 7 — 8.0996] — 8.03 12 | 2 е 52.7255 + 7| 75.6640 |+ 8 — 8.0821] —8.0273 2—3 Scheinbare Ædiff: M—Centrum ==-н 52703 Fu = 0.99318 —1°, = 0.00034 N— » = — 41.4079 Q— » = +-14.3248 Ja —0,99289 —i, = +0,00032 Е О à Е— » = —38.7100 Пей". = — 4 У » ie 053202 в = о W— » = 0,8890 ’„ =0.99318 Л. = -+0.00028 1 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 193 ; 1897. März 11. яве. Decl. | | Scalenablesung. } тн сн, ый ; Me à gr D Bemerkungen — & у ЕЕ = — 7 90031 1 y — = 96 sin 1' zur Aufnahme BPKr.00° += P.-Kr. 270° [2+ 2 4 631 m mm ann an mm пт тт тт 63.1458 65,2436 —=10| 65.2420 |+16| Oo 0.0000 0.0000 0.0000 Bilder 3. +10] 62.2155 0] + 3.0236 — 0.0013 + 3.0223 +-24| 61.6920 Il + 3 5494 — 0.0811 — 3.4683 +27| 89.8272 5] — 24.5832 — 0.0094 — 24.5926 +41| 89.8082 3] — 24.5683 — 0.0694 — 24.6377 4-20| 81.6300 2] — 19.3897 0.0000 — 19.3897 — 2| 34.3000 8] 50.9392 0.0000 —+ 30.9392 —19| 60.1360 + 5.1116 -=19| 60.5345 + 4.7131 + 4.7111 Bilder 2—8. 60 9415 + 4.3086 61.8910 |+ 9 + 3.3610 62.2920 |+ 9 + 2.9592 + 2.9613 62.6865 +9 = 2.5638 63.5565 |+ 8 + 1.6911 63.9520 |+ 8 —+ 1.2984 —+ 1.2991 64.3415 |+ 8 + 0.9077 66.3940 |+ 8 — 1.1445 66.7995 |+ 8 — 1.5518 — 1.5462 67.1970 |+ 8 —- 1.022 68.0650 |+18 — 2.8178 68.4635 |+18 — 3.2120 — 3.2113 68.8540 |+13 — 3.6042 ‚| wah/rscheinlich |dure/h eilne Erschültterung des Fernrobrs| während der Aufnlahme. Trabant — Jupiterscentrum. Yt—Y2 | Mittel. Ir 072) Пьер год | (еа-ал) т] Ph. 45 тт тт 59.6785 +-0.8531 61.4290 —0.8 511 63.0870 —+0.8567 | -+0.8523 | -+0.8468 | -+0:0007 —0/0001 0:0000 | -+0:8474 65.9405 —0.8504 67.6020 —0.8503 61.8290 — 1.2963 63.5780 — 1.2970 65.2360 — 1.2925 | —1.2953 | — 1.2870 | —0.0010 — 0.0003 0.0000 | —1.2883 68.0840 — 1.2954 69.7490 — 1.2951 58.5730 —1.9607 60.3220 —1.9583 61.9810 +1.9627 | +1.9582 | +1.9456 | -+0.0015 —0.0007 0.0000 | -+1,9464 64.8340 —1.9538 66.4970 +1.9555 57.1760 +3.3557 58.9270 +3.3542 60.5850 + 4.6592] -+3.3601 3.3557 | +3.3341 +0.0027 —0,0020 0.0000 | -+3,3348 63.4330 + 1.8110] +3.3572 65.1020 + 0.1402| -+3.3515 Scheinbare Decldiff: M—Centrum — + 3/003; 195 = 0.99342 1°5 = —0.00022 | ND == 3.4541 . ; | Q— » = —24.4336 fs = 0.99292 is =— 0.00028 X 15 = —1.0 . K— » = —24.4649 У— » — — 19.2649 f's = 0.99358 Js = —0,00033 W—- » = -+30.7328 dy = 11° 39:9 | 12 © Зап. Физ.-Мат. Отд. 194 Е. RENZ, 73. 1897. März 11. № 17 Scalenablesung. у Pulkowaer Sternzeit у | ORNE Pa le | x An Besen Bilder, 8 P.-Kr. 0° г P.-Kr. 1800| ++ % 3 der Aufnahmen. Mittel. | | mm mm mm $ У Ctr. | 676704 10] б6/Аал [1000010000 "т Fi S 61.6605 |+ 9| 66.7132 |+ 9| о 0.0000 D | M 66.6445 |+ 9| 61.7290 |+ 9| ol + 4.9796 о | N 22.5110 |-+25| 105.8698 |+ 6|-+18| —39.1548 ; . 9 | ) 75.2570 |+23| 53.1262 |--17|— 3| +13.5872 10° 8" 24 2 L 24.9452 |+38| 103.4248 |-+15|-+-20] — 36.7148 en) 12 61.3612 |+19| 67.0098 |-+15 ©] — 0.3022 9 | т 62.5110 |+21| 65.8685 |+-25 0] + 0.8429 2 %ар | 60.9160 |+11| 67.4890 |+ 8 — 0.7645 de 61.3500 |+11| 67.0420 |+ 8 — 0.3240 — 0.3211 т 8650 3 Ag 61.7990 |+10| 66.5925 | 8 +. 0.1252 %0р | 60.9435 |+11| 67.4525 |+ 8 — 0.7325 D, 61.3770 |+11| 67.0010 |+ 8 — 0.2900 — 0.2877 5 3 6, | 61.8330 |190] 66.5980 |+ 8 — 0.1594 2 Cp | 60.9415 |+11| 67.4555 |+ 8 — 0.7350 | | RON Ce | 61.3810 |+11| 67.0120 |- 8 — 0.2935 — 0.2938 39 12 14 39 23 3 Co 61.8160 |+10| 66.5720 |- 8 + 0.1440 % dy | 60.9505 |+10| 67.4505 |+ 9 — 0.7281 | de | 61.3815 |-+10] 67.0050 |+ 9 — 0.2898 — 0.2934 дис в | do | 61.8110 [+ 9| 66.5790 |+ 9 + 0.1378 L Len | 60.9565 |+10| 67.4420 |+ 9 — 0.7208 | ес 61.3870 |+10| 67.0155 |+ 9 — 0.2924 — 0.2919 да gl 2—3 1 e, | 61.8110 |+10| 66.5800 |+ 9 + 0.1374 | af Nicht gelmess|en, weil die| Zeit| der| Aufnahme| unsicher ist. | N Trabant — Jupiterscentrum. | xx | Mittel. |’) Julye—-y2) Ph. Да cos d и | 4 mm mm | Та | 60.0590 |+15| 68.3190 |+18 — 1.6083] —1.2872 3 | b 60.1055 |+15|) 68.2820 |+18 — 1.5666] — 1.2789 5 5 | с | 60.0965 |+ı5| 68.2875 |+18 — 1.5738] —1.2800 | —1.2764 | —1!2682 | -н0'0003 | —0'0003 | —1:2682 | 3 | d | 60.1085 |-+14| 68.2700 |+19 — 1.5592] —1.2658 2—3 | е 60.1165 |+14| 68.2640 |+-19 — 1.5522] —1.2603 2 4 Па | 63.7600 |+ 9| 64.6240 |+16 + 2.0895| -+2.4106 Be № b | 63.7940 |+ 9| 64.5905 |+16 + 2.1232] 2,4109 2—3 _ № с | 63.7785 |+ 8| 64.6045 |+16 + 2.1084] 2.4022 | 2.4056 | -+2.3901 | —0.0507 | —0.0003 | +2,3891 | 2 | | d 63.7790 |+ 8| 64.6005 |+17 + 2.1106] -+2.4040 2 и | e 63.7790 |+ 8| 64.6045 |+18 + 2.1086| 2.4005 2 | Ша 57.1910 |+11| 71.1820 |+12 — 4.4737| —4.1526 2 | | b 57.2315 |+10| 71.1445 |+12 — 4.4348] —4.1471 2—3 в | с 57.2210 |+10| 71.1560 |+12 — 4.4458] —4.1520 | —4.1469 | —4.1200 | —но.солт | —0.с003 | —4,1192 | 2 у | d | 57.2305 |+ 9| 71.1490 |+13 — 4.4376] —4.1442 2—3 Mi e 57-2380 |+ 9| 71.1425 |+13 — 4.4306] —4.1387 2 | IV a 53.6700 |+ 6| 74.7140 |-HII — 8.0004| —7.6793 2 _ № b | 53.7100 |+ 5| 74.6790 |1 — 7.9630] —7.6753 3 tt с 53.6960 |+ 4| 74.6875 |+10 — 7.9742| —7.6804 | —7.6748| —7.6252 | +0.0021 | —0.0003 | —7,6234 | 2 u | 4 | 53.7075 |+ 3| 74.6775 |+10 — 7.9635] — 7.6701 2 В | е 53.7080 |+ 3| 74.6730 |+HII — 7.9610] —7.6691 2 В | М ne 2h oi РОННИ tt re ont РЕН СЕНЕ ЕЕ ЕАН Le с Scheinbare Adiff: wie 72. FR 0.993518 —i° = +0.00010 | mn | fa —0.99288 —i, =-0,00006 X i, = —02 a Refr. = + 61 . | . Try = O | Fu = 0.99354 Ju = —0.00067 В т &y = 10 224 ps €. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. | Scalenablesung. |P.-Kr.90° ны P.-Kr. 270° | m um mm 63.0808 || 65.3028 63.0798 -++-10| 65.3012 66.0980 |+10| 62.2745 66.6452 |+24| 61.7368 8.4922 |+27| 89.8920 38.5198 |+41| 89.8520 43.6832 |20| 84.6888 _ 94.0215 — 2| 34.3615 68.2450 |-+19| 60.1490 67.8265 |+19| 60.5840 67.3940 | 9| 60.9950 66.7210 |+ 9| 61.6800 6.2875 |+11| 62.1065 65.8670 |+11| 62.5320 65.1440 |+17| 63.2540 64.7290 |+-17| 63.6620 64.3165 |+ 9| 64.0830 62.0010 |+10| 66.3980 61.5835 |+10| 66.8150 т 1.1740 |-+-11| 67.2205 60.4000 |+15| 67.9970 59.9840 |+15| 68.4060 59.5770 |-+15| 68.8150 5 ge|mess 50.5730 : ‚4650 63.3280 61.7260 en, weil die 60.0500 61.5820 63.1465 66.2895 67.8895 61.5890 63.1100 64.6710 67.8120 69.4060 58.8240 60.3570 61.9170 65.0580 66.6630 57-3640 58.8920 60.4510 63.5925 65.1925 НЕ mm_| mm 10000! 10000 4-16 о der Scheinbare Decldiff. wie 72. | ея УЕ ЕН +44 ИИ 1897. März 11. Decl. Aufnahme ЕЕ ГИУ +++ ЕН 5.2530 3.7222 2.1582 0.9852 2.5858 3.7162 2.1924 0.6326 2.5089 4.1052 6.4756 4.9430 3.3852 0.2458 1.3574 7-9402 6.4117 4.8518 1.7122 0.1104 “ине; —= unsicher ist. Yt—Y2 | Mittel. [Иез | 7 бага) eat)? тт —0.5189 —=0.5183 —0.5151 —+-0.5162 0.5 128 —1.0179 —1.0II5 — 1.0105 — 1.0075 — 1.0066 ++-1.7415 +1.7391 +-1.7421 — 1.7444 1.7412 +-3.2061 3.2078 —+3.2087 —+3.2136 +-3.2090 4.7341 3.2039 1.6431 1.5014 3.0986 тт —0.5163 — 1.0108 +-1.7416 +-3.2090 128 = 0.99341 fs = 0.99290 f’5 = 0,99439 2 — + t9ù sin 1’ x? . у — = 196 81 l’ тт mm 0.0000 0.0000 — 0.0013 + 3.0215 — 0.0811 + 3.4839 — 0.0094 — 24.5962 — 0.0694 — 24.6216 0.0000 — 19.3995 0.0000 — 30.9391 Trabant — Jupiterscentrum. 9/5134 | —0'0010 | —0.0001 —1.005I | +0.0019 | —0.0001 —+1.7316 | —0.0033 —0.0006 +#3.1910 | —0.0059 | —0.0019 1° 5 — -+0.00016 1} = -+0.00006 Js = -+0.00081 X 14 = +02 Bemerkungen zur Aufnahme. Bilder 3—4. Bilder 3. 0'0000 | -+0:5123 00200 | —1.0033 0.0060 | —+1.,7277 0.0000 | -+3,1932 ! >) 196 Е. Renz, 74. 1897. März 33. Ar Scalenablesung. | Pulkowaer Sternzeit u Е ме m НЕВЕ № & ter Et CON ea Een Bilder P.-Kr. 0° |6-+K| Р.-Кт.180 ++ der Aufnahmen. Mittel. | Ни 10000 Re 10000 10000 man um Ctr, | 61.6744 66,7109 Sg 61.6735 |+ | 66.7100 |+ 9 0.0000 1—2 M 66.6468 |+ 9| 61.7268 |+ 9 5 + 4.9782 | 1—2 N 22.5178 |+25| 105.8648 |-н 6|-+18] —39.1525 т e 1 Q 75.2642 |+23| 53.1135 |+17|— 3|-+13.5936 9° 10” 50 1—2 R 24.9552 |+37| 103.4150 |-Hı5 +20 — 36.7086 1—2 У 61.3695 |-+19| 67.0060 |+15 — 0.2968 1—2 И 62.5068 |+21| 65.8698 |+25 пы 0.8366 1 Фар | 61.2210 |+11| 67.1820 |+ 8 — 0.4621 а: | 61.6565 |-+10| 66.7380 |+ à — 0.0224 — 0.0268 9 ве 2—3 Ay 62.0800 |+10| 66.3080 |-+-10 + 0.4042 % by | 61.2550 |+11| 67.1430 [+ 8 — 0.4256 be 61.6870 |+10| 66.7110 |+ 8 —= 0.0064 + 0.0063 29 30 3 b, 62.1190 |+10| 66.2790 |-+-Io + 0.4382 %Cyw | 61.2205 |+11| 67.1750 |+ 8 — 0.4588 Ce 61.6510 |+10| 66.7450 |+ 8 — 0.0286 — 0.0267 30 42 2 * Co 62.0850 |+10| 66.3070 [+10 + 0.4072 gh 31” 46° % dyy | 61.2475 |+10| 67.1530 [+ 9 — 0.4344 de | 61.6740 |+ 9| 66.7160 |- 9 — 0.0028 — 0.0019 32... 10 2—3 do | 62.1140 | 9| 66.2875 [+11 — 0.4314 Zen | 61.2260 |+10| 67.1710 |+ 9 — 0.454? | < 61.6450 |+ 9 66.7505 |+ 9 — 00345 — 0.0306 33 I 2 eo 62.0755 |+ 9| 66.3180 |-11 + 0.3969 %1 | 61.2500 |+11| 67.1440 |+10 — 0.4287 Je 61.6660 |+10| 66.7200 |+10 — 0.0088 — 0.0077 р 1—2 Jo ве a Trabant — Jupiterscentrum. æ—x> | Mittel. Page) иде Ph. | Au cos à mm mm Та | 61.2270 |+11| 67.1570 |+ 8 — 0.4466] —0.4198 | 1—2 b 61.2485 |+11| 67.1350 |+ 8 — 0.4248] —0.4311 2 € 61.2130 |+11| 67.1700 |+ 8 — 0,4601] —0.4334 | __ Wirken р Де _opraeas | 2 d | 61.2325 |+10| 67.1560 |- 9 — 0.4434| —0.4415 0.4357 0.4328 0.0000 0.0007 0.4335 | 5 e | 61.2025 |+10| 67.1815 |+ 9 — 04712] —0.4406 1—2 f | 61.2175 |+11| 67.1650 |-+10 — 0.4554] —0.4477 1 Па 58.8205 |+12| 69.5590 |+17 — 2.8512| —2.8244 1—2 b | 58.8540 |+11| 69.5320 |+16 — 2.8210 SR 1—2 с 58.8165 |+ 11| 69.5675 |+16 —= 285151 2.8308, 0: ER За si 2 а Re, Ze, ie En sa 218360 — 2.8337 2.8313 2.8121 | -+0.0091 0.0007 2.8127 | 5 е 58.8095 |+10| 69.5750 |+17 — 2.8648| —2.8342 1 f | 58.8290 |-н11| 69.5550 [+18 — 2.8451| —2.8374 1—5 III Geht du/rch |die Jupiter|schelib ] |ТУ a 58.9990 |+12| 69.3820 |+14 — 2.6734| —2.6466 1—2 b | 59.0310 |+11| 69.3525 |+13 — 2.6426| —2.6489 Be 6 58.9990 |+11| 69.3910 |+13 2.6778] —2.6511| __ Г 2 Le 9 gaz а | ‘55 №10 602670 lens Е те 2.6532 2.6353 | 0.000171 0.0007 2.6359 | 5 е 58.9890 |+10| 69.3970 |-+14 2.6860] —2.6554 1 7 59.0050 |+11| 69.3790 |+15 — 2.6690] —2.6613 1—2 | Scheinbare Ædiff: М— Centrum= + 5.2703 Я? и ==0.99324 —1°,, = +-0.00916 | N— » — —41.4088 | Q— » — +-14.3249 for=0.99296 —iy —=+0.00014 X = — 05 | R— » == — 38.7104 Ref. = — 4 V— » === 0.3202 15 = O | Wen к 0.8858 Ги =0.99325 Ju = 0.00010 | | h m > — 10/0 u ne. Scalenablesung. B-Kr. 90°] +1 Р.-Кг.270° 63.2068 |! 65.1766 63.2058 65.1750 66.2270 62.1535 66.7575 61.6215 38.6188 89.7650 38.6318 89.7408 ‚43.8095 84.5680 94.1490 34.2332 68.3240 60.0750 67.9150 60.4860 67.4980 60.9020 66.7615 61.6435 66.3460 62.0580 65.9385 62.4685 65.0860 63.3090 64.6740 63.7210 64.2750 64.1345 62.0675 66.3275 61.6510 66.7475 61.2470 67.1600 60.33 10 68.0645 59.9260 68.4620 59.5295 68.8750 58.6120 69.7845 58.2160 70.1790 57.8305 70.5700 68.1300 60.2530 66.5790 61.8140 64.9010 63.4840 1.8840 66.5020 60.1685 68.2220 58.4535 69.9300 69.1810 59.2050 67.6170 60.7710 65.9450 62.4400 62.9240 65.4610 2050 67.1800 4905 68.8935 29.1795 57.6110 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 59.2060 60.7775 62.4440 65.4640 67.1820 68.8950 нЕ 1897. März 33. ll AIRE #IScheinbare Decldif: M—Centrum = + 3/0033 de JS Fe we | » — —24.4654 = —19.2651 =-+30.7330 dy = +129 2.5 Пес]. 9п+3 +9, 3 mm + 4.7009 + 3.1310 — 1.4637 —= 1.5599 — 3.2843 — 4.9947 3 li Yt— Ya | Mittel. Ir а(и— уз) | 7 (ваз) ео) тт тт +-0.2227 —+-0.2364 —+-0.2301 —+0.2358 —+0.2423 —-0.2409 —+1.2722 —+1.2774 —+-1,2738 +1.2761 +-1.2819 —+1.2780 -+0.2364 +1.2766 +-1.2709 +1.2711 +1.2703 —+1.2737 —+1.2789 —+-1.2761 +1.2735 /95 = 0.99327 fs = 0.99278 f's = 0.99343 197 ze 1’ — tg0 sin mm 0.0000 0.0013 0.0811 0.0094 0.0694 0.0000 0.0000 Bal Trabant — Jupiterscentrum. +0:2348 | -0!000т —+-1.2682 +-0.0006 —+-1.265I | -+0.0006 15 = —0.00011 д =— 0.00015 Js; = —0.00021 x? . y— = 196 81 1' тт 0.0000 + 3.0199 —+ 3.4716 — 24.5955 — 24.6360 — 19.3930 30.9409 Bemerkungen zur Aufnahme. Bilder 2—3. Bilder 2. 0:0000 | -+o/oooı | -+0/2350 —0.0002 | -+0.000т | -+1,2687 — 0.0002 | -+0.000т —+1,2656 X 13 =—05 198 Е. Rexz, 75. 1897. März 253. № Scalenablesung. Pulkowaer Sternzeit P.-Kr. 0° | P.-Kr. 180°| i+% 3 der Aufnahmen. Mittel. mm mm. mm mm 63.0474 [10000] 65.8362 | 10000) 10000 mm mm a (г. S 63.0465 |+ 9| 65.3345 |+17| о 0.0000 M 68.0242 |+19| 60.3562 |-+14] ol + 4.9786 М 23.8918 |+26| 104.4885 |+ 7|-=18| —39.1512 5 Ka ; Q 76.6460 |-+21| 51.7348 |+21|— 3|-+13.5997 10 1 50 R У 114 % Gy 26.3380 |+36| 102.0345 |++14|-+-20| — 36.7008 62.7538 |+18| 65.6230 |+17| 0] — 0.2902 63.8735 |+20| 64.5000 |+31| o| + 0.8306 62.6190 |+10| 65.7680 |+-10 — 0.4301 ag | 63.0770 |+10| 65.3120 |-16 + 0.0266 + 0.0215 12 re 4—5 ao | 63.5155 4-10) 64.8675 |+16 + 0.4681 4b. | 62.6415 |+10| 65.7645 |+10 — 0.4171 6; | 63.0720 |+10| 65.3155 |+16 + 0.0224 + 0.0223 54 42 4 6, | 63.5120 |+10| 64.8770 |+16 + 0.4616 Z Cw | 62.6450 |+-10| 65.7505 |+10 — 0.4084 Ce 63.0790 |+10| 65.3170 |+16 + 0.0251 — 0.0273 55 50 + Co | 63.5150 |+10| 64.8730 |+16 + 0.4651 12% 56” 93° % dy | 62.6655 |-+ 9] 65.7345 [+11 — 0.3902 de | 63.1040 |+ 9| 65.2895 |+17 —= 0.0512 + 0.0483 ею 4—5 do | 63.5360 |-+ 9| 64.8560 |+17 + 0.4840 %ey | 62.6630 |+ 9| 65.7360 |-+11 — 0.3922 ес 63.0920 |-+ 9| 65.2950 |+17 —= 0.0426 —= 0.0420 Ge 4 en 63.5260 |+- 9| 64.8630 |+17 + 0.4755 %}р | 62.6740 |+10| 65.7145 |+-12 — 0.3760 je 63.1275 |+-10| 65.2690 |-+18 —= 0.0732 —+ 0.0715 59 28 3—4 : ? 8 5 - Fe 83.5680 [+12 _ 64.8215 _.[4-1 TE Trabant — Jupiterscentrum. av | Mittel. Габи) Лу») Ph. | Да cos ö mm mm Та | 61.7690 |+11| 66.6180 |- 8 — 1.2800] —I.3015 4 b | 61.7530 |+10| 66.6340 |+ 8 — 1.2960] —1.3183 3—4 с 61.7645 |+10| 66.6200 | 8 — 1.2832| — 1.3105 | __ нех р 2h IT 3 а | 61.7765 |+ ol 66.6095 |+ 9 — 1.2721] —1.3204 1.3154 1/3066 | -+0!0003 0.0007 1.3070 ge La e | 61.7735 |+ 9| 66.6145 |+ 9 — 1.2761| —1.3 181 3—4 f | 61.7965 |-+10| 66.5895 |-+-10 — 1.2521] —1.3236 3—4 Па | 59.9855 |+16| 68.4000 |+19 — 3.0630] —3.0845 ù 3—4 b 59-9745 +15| 68.4100 |+18 — 2 me 3 с 59.9865 |-+15| 68.4000 |-18 — 3.0625| —3.0898| __ ge. 24 ox 2—3 а | 80.0005 [+-14| 68.3845 |+19 — 3.0478 —3.0961 3.0914 3.0708 | -+0.0008 0.0007 3.0707 3 € | 59.9980 |14| 68.3845 |+19 — 3.049 | —3.0911 3 f | 60.0290 |+14| 68.3570 |+19 — 3.0198| — 3.0913 3 Ша | 62.6195 |--10| 65.7675 |+10 — 0.4296] —0.4511 4 b | 62.6070 |+10| 65.7780 |+Io — 0.4411] — 0.4634 3—4 с 62.6205 |+10| 65.7680 |+10 — 0.4294| —0.4567 | _ = al ыы 8 4 | 62.6265 |+ 9| 65.7555 |+и — 0.4202] — 0.4685 | — 24521 0.4491 | --0.0002 0.0007 | —0.4496 | ; е | 62.6270 |+ 9| 65.7595 |+11 — 0.4220] —0.4640 3 f | 62.6530 |+ı10| 65.7355 |+12 — 0.3970] —0.4685 3 IV a 59.9735 |-+16| 68.4140 |+19 — 3.0760] —3.0975 3 $ | 59.9600 |+15| 68.4230 |+18 — 3.0872] —3.1095 3—4 с 59.9735 |+15| 68.4120 |+18 — 3.0750] —3.1023 | __ ws #4 ab 3 “| 59.9850 [+14] 68.3095 |+-19 — 3,0631| — 3.1114 3.1061 3.0853 | -+0.0008 0.0007 | —3.0852 | 3 _4 e 59.9850 |-+14| 68.3995 |+19 — 3.0631] —3.1051 3—4 f | 60.0115 |-+14| 68.3780 |+19 — 3.0391| — 3.1106 3 Scheinbare Ædiff. wie 74. Fa =0.99326 —1° y, = 0.00041 fa = 0.99296 —iy = -+0.00037 X и=-— 13 Ве. = + 19 Qi о Го = 0.99333 Л. = 0.00056 ine. Scalenablesung. P.-Kr.90° tt P.-Kr. 2709 ое 10000 70 63.3385 64.9794 63.3375 |+10| 64.9778 66.3632 |-+10| 61.9510 66.8765 |+25| 61.4250 38.7522 |+29| 89.5618 38.7500 |-+41| 89.5478 43.9425 |+20| 84.3662 94.2845 |— 3| 34.0292 68.5260 |+19| 59.7930 ‚68.1100 |+19| 60.2230 67.6770 |+19| 60.6400 66.8920 | 9| 61.4400 66.4810 |+11| 61.8435 66.0695 |+т1| 62.2630 65.1560 |+17| 63.1650 64.7595 |+17| 63.5770 64.3470 |+17| 63.9810 62.1925 |+10) 66.1320 61.7790 |-10| 66.5440 61.3590 |+11| 66.9620 60.5880 |+15| 67.7410 60.1840 |+15| 68.1480 59.7660 |-+15| 68.5540 59.0170 |+11| 69.3140 58.5995 |[+11| 69.7300 58.1775 |-+ 6| 70.1540 58.6265 61.2520 62.9690 65.9410 67.5445 69.1330 58.8500 60.4750 62.1975 65.1690 66.7700 68.3655 59.9060 61.5340 63.2555 66.2255 67.8250 69.4190 | 69.5535 |-+17| 58.7630 | 67.9300 |+19| 60.3860 | 66.2105 |+11| 62.1040 63.2390 |+10| 65.0790 | 61.6370 |+10| 66.6810 | 60.0400 |+15| 68.2710 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1397. März 23. Decl. t+k mm | тт 10000] 10000 m +16] о 0.0000 +10] 0|-+ 3.0266 +10|— 1|+ 3.5468 — 3|-+ 5| —24.5822 + 8]+13| —24.5755 — 7|-+ 2] —19.3898 —=20|— 8|-+30.9462 +14 + 5.1872 +14 + 4.7642 +10 + 4.3394 9 + 3.5464 9 + 3.1393 +9 — 2.7238 + 8 + 1.8164 + 8 + 1.4122 + 8 —+- 1.0039 +10 1.1393 + 8 — 1.5620 + 8 — 1.9809 +18 — 2.7562 +18 — 3.1617 +18 3-5737 +13 — 4.3282 +-16 4.7450 +16 — 5.1683 +14 + 5.3514 +10 + 3.7274 + 9 + 2.0101 +10 — 0.9633 +18 — 2.5662 +-13 — 4.1566 +10 + 6.1286 +14 —+ 4.5017 + 9 + 2.7790 +16 — 0.1931 + 8 — 1.7920 +18 — 3.3874 +14 + 5.0717 9 — 3.4440 +9 + 1.7226 +10 — 1.2498 +18 — 2.8470 E73 — 4.4394 +10 + 6.2160 +14 —= 4.5927 + 9 + 2,8738 4-16 — 0.0998 + 8 — 1.7014 +18 — 3.2952 | Scheinbare Decldiff. wie 74. dy = +12° 2:8 + 1.4108 тт 0.5878 +0.5909 +0.5993 —0.5994 0.5977 —0.5906 +1.3650 —+1.3652 +-1.3682 -+1.3676 +-1.3719 +-1.3598 +-0.3081 +-0.30 or 18 +-0.3109 -+0.3169 +-0.3078 —+1.4524 +-1.4562 —1.4630 1.4609 —+1.4625 +-1.4520 Ye —Yà | Mittel. mm -+0.5940 —+-1.3663 +-0.3105 +1.4579 178 = 0.99329 fs = 0.992738 Г’; = 0,99360 2 — + 1gÿ sin Г АТ о о © © > -+0/5992 | <+-0/0003 —1.3576 | -+0.0006 —0.3085 | —+-0.0001 —+-1.4486 | -+0.0006 $98 = —0.00037 15 = —0.00046 Ту = — 0.00029 x? ЕВ у— > 196311 Trabant — Jupiterscentrum. т Ла (91—95) | Ja (21—25) | еее 0:0000 | <+-0:0001 | -+0'5906 —0.0003 | -+0.000т | -+1,3580 0.0000 | -+0,0001 | -+0.3087 —0.0003 | -+0.000т | -+1,4490 X ig—=— 16 199 Bemerkungen zur Aufnahme. Bilder 1—2. Bilder 3. 200 76. — Object. = = оса QE SR Se DE A8 ee + -ч а ъаесса Е. Renz, 1897. März 37. Scalenablesung. ео Pulkowaer Sternzeit El P.-Kr. 0° tt) P.-Kr.180°| #+% . der Aufnahmen. Mittel. TR 10000 er 10000 70000 mm nm 61.8867 66.5030 61.8858 |+ 9| 66.5020 |+10 0.0000 2 66.8588 |+ 9| 61.5232 |+ 9 ь + 4.9760 2—3 22.7255 |-+25| 105.6625 |-- 8|-18| —39.1576 à К 2, 75.4888 |-+23| 52.8965 |+17|— 3| -+13.6043 9" 34” 32 2 25.1730 |-+38| 103.1985 |-+15 +20 — 36.7014 2 61.5932 |+19| 66.7862 |+-15 — 0.2882 2 62.7058 |-+21| 65.6768 |-+25 + 0.8224 2—3 61.4460 |+-10| 66.9510 |+ 8 — 0.4442 61.8610 |-+10| 66.5305 |+ 8 — 0.0265 — 0.0268 9 Зе 3 62.2810 |+10| 66.1165 |+10 + 0.3904 61.4740 [+10] 66.9350 | 8 — 0.4222 61.8680 |-+-10| 66.5285 | 8 — 0.0220 — 0.0182 Ио IN 2—3 62.2805 |+10| 66.1175 |+10 — 0.3896 61.4500 |+ 9| 66.9450 |+ 8 — 0.4393 61.8600 | 9| 66.5435 |+ 8 — 0.0336 — 0.0324 4т 42 3 62.2640 | 9| 66.1290 |[+10 + 0.3756 gr pr 6’ 61.4690 |+ 9| 66.9335 |+ 9 — 0.4241 61.8770 | 9| 66.5235 |+ 9 — 0.0151 — 0.0170 42 54 2—3 62.2790 |+ 9| 66.1185 |+11 + 0.3883 61.4285 |+ 9] 66.9795 |-+ 9 — 0.4674 61.8410 | 9| 66.5615 |- 9 — 0.0521 — 0.0482 43 49 3—4 62.2650 |-+ 9| 66.1310 |1 —+ 0.3750 61.4720 |+10| 66.9255 |+10 — 0.4186 61.8860 |+10| 66.5135 |+10 — 0.0056 — 0.0060 44 53 3 . 6. F а a ur yet 1. > Trabant — Jupiterscentrum. Lt —Ly | Mittel. ааа, Лигу Ph. | До cos à mm mm 59.9830 |-+15| 68.4015 |-+19 — 1.9013| — 1.8745 2—3 59.9945 |-+15| 68.3910 |-+18 — 1.8902 rie 2 59.9875 |-+15| 68.3975 |-+18 — 1.8970| —1.8646 | __ 22 р Her tn, 2 bas ral Ié6peB et lete — 1.8866] —r.8606 1.3684 1.8556 | +-0!0004 0.0009 1.8561 | о 59.9730 |+14| 68.4135 |+19 — 1.9124] —1.8642 2—3 60.0115 |+15| 68.3705 |+20 — 1.8716] — 1.8656 2 58.8755 |+-12| 69.5080 |-+17 — 3.0084] —2.9816 2—3 58.8865 I+-I1| 69.4990 |+16 — 2.9984| — 2.9802 у 2 58.8755 |+11| 69.5070 |+16 — 3.0078] —2.9754| __ ar m’ cb 2 58.8905 [2-10 6910945 ыы — 2.9942| —2.9772 2.9767 2.9564 | -+-0.0007 0.0009 2.9566 2 58.8665 |+-10| 69.5235 |+17 — 3.0207| —2.9725 8 58.9045 |+-11| 69.4790 |+17 — 2.9794| —2.9734 2 63.5165 |-+ 9| 64.8625 |+16 — 1.6348] 1.6616 2 63.5315 + 9] 64.8545 |-16 + 1.6463] 1.6645 2—3 63.5255 |+ 8| 64.8605 |+16 -+ 1.6402] 1.6726 ет 4 2 бзьсато |518] 1648500 |9 = 1.6532| 41.6702 +1.6716| 1.6602 0.0004 0.0009 | +1,6589| о 63.5145 |+ 9| 64.8665 |+-18 —= 1.6317] +1.6799 3 ellipt 63.5590 | 9] 64.8250 |+19 + 1.6746| 1.6806 2—3 53.2669 |+10| 75.1250 |+12 8.6214] —8.5946 2—3 53.2705 |+ 9| 75.1165 |411 — 8.6150] —8.5968 2 53.2635 |+ 8| 75.1240 |+10 —— 8.0222] —8.5898 | per L4 an 2 3.2755 [+ 7| 75.1140 |+io 8.6112] —8.5942 8.5929 8.5341 | -+0.0020 0.0009 8.5330 9, 53.2505 [+ 7| 75.1435 |+10 8.6385] —8.5903 3 ellipt. 53.2875 |+ 7| 75.0990 |+ 8.5978| —8.5918 2 Scheinbare ВАШ: M—Ceutrum = + 95.2703 Ли = 0:99317 —i°, = -+0.00061 N— » — — 41.4090 Q— » = +14,3250 Je = 0.99288 —iy — -+0.00058 x = — 2'0 R— » = —38.7106 Refr. = — 3 V— » = — 0.3202 Те) = о W— » — + 0.8888 Л’ = 0.99316 I = 0.00055 h %Xy = 10 т 16.2 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 201 1897. März 27. ihe. | Decl. Scalenablesung. пн с+%, 52] _. „2 à Bemerkungen — — tqù sin 1’ y——tgd sin 1" р P.-Kr. 90° #1 P.-Kr. 270° | ++ 3 3 zur Aufnahme. mm mm mm 10000 651966 | 10000/10000 a ne num mn 65.1950 |-+16| о 0.0000 0.0000 0.0000 Bilder 3. 62.1702 |-+10] ©] - 3.0244 — 0.0013 + 3.0231 61.6622 |+26|— 1| + 3.5334 — 0.0811 + 3.4523 89.7745° — 24.5782 — 0,0094 — 24.5876 89.7795 — 24.5878 — 0.0694 —24.6572 81.5932 — 19.3974 0.0000 — 19.3974 34.2545 —+30.9415 0.0000 —30.9415 60.1165 + 5.0897 60.4990 + 4.7016 —+ 4.6982 Bilder 2—3. Nebel. 60.9010 + 4.3032 61.8205 — 3.3803 62.2025 + 2.9970 — 3.0094 62.5596 — 2.6238 63.5100 + 1.6916 63.8950 + 1.3066 + 1.3057 64.2790 + 0.9188 1 66.3920 — 1.1928 д 66.7790 — 1.5770 — 1.5781 61.2330 67.1640 — 1.9646 | 60.2640 68.1295 — 2.9322 59.8760 68.5360 — 3.3292 — 3.3306 | 59.4740 68.9365 — 3.7304 } Е 58.5735 69.8255 — 4.6258 88.178 70.2230 — 5.0220 — 5.0174 N .6070 — 5. _ épis HUE Trabant — Jupiterscentrum. : T Yı--Y2 | Mittel. |’ (гу) | 7 (оо | бий) Ph. | AG mm mm 68.6800 59.7120 + —+-0.7864 61.4115 + —-0.7882 .106 0.78 r D r r ’ ро 0 oe +0.7839 | -+0!7787 | —o'oo14 | —olooor | -+0/o0o2 | +0!7802 67.7445 — —0.7814 69.4285 — —0.7834 59.2200 + -+1.2772 60.9220 + в 62.6140 — 1276 | 65.5010 X +1.2733 —+1.2743 | -+1.2658 | -+0.0023 0.0003 | <+-0.0002 | -+1,2680 67.2555 — +1.2717 68.9370 — —1.2748 61.3110 —= —0.8168 63.0155 + —0.8198 64. —0.8 - Est DE ae —0.8208 | —0,8154 | —0.0013 0.0000 | -+0.0002 | —0,8165 69.3465 — —0.8238 71.0310 — —0.8206 56.9155 + 8.2821| -+3.5839 58.6140 + 6.5810] -+3.5806 60,3065 + 4.8882| -+3.5825 ET = 63.1910 + 2.0053| +3.5834 -+3.5825 | -+3.5587 | -+-0.0065 0.0023 | -+0.0002 | -+3,5631 64.9445 + 0.2506| -+3.5812 66.6270 — 1.4338| +3.5836 | Scheinbare Decldiff: M-— Centrum—-+ 3/0033 195 = 0.99322 15 = —0.00066 N— » = + 3.4542 Q— » ——241.4339 fs = 0.99273 is = —0.00072 xo= —2:5 R— » = — 24.4656 У » = — 19.2652 fs = 0.99336 Js; = —0.00076 W—- ›»› =+30.7331 dy = +12° 10.0 Зап. Физ.-Мат. Отд. 26 202 T7. Scalenablesung. Object. P.-Kr. 0° = Р.-Кг.180° mm ия mm, Ctr, | 63.4321 64,9507 S 63.4312 + 9| 64.9490 M 68.4055 |-+19| 59.9682 М 24.2675 |-+26| 104.1138 Q 77.0215 |+21| 51.3562 R 26.7112 |+34| 101.6608 У 63.1312 |+18| 65.2425 W 64.2622 |+20| 64.1120 % y | 63.0805 +10] 65.3065 ас 63.4805 |+10| 64.9005 а | 63-8830 |+ 9| 64.5030 bp | 63.0855 |+10| 65.3060 b. | 63.4825 |+10| 64.9040 bo | 63.8820 |+ 9| 64.5010 %C | 63.0710 |+I0| 65.3215 Ce | 63-4695 |10| 64.9220 Co | 63.8715 | 9| 64.5115 % dy | 63.0745 |+ 9| 65.3225 de | 63-4745 |+ 9] 64.9215 do | 63.8730 |+ 8| 64.5115 %е, | 63.0350 [+ 9| 65.3560 ee 63.4385 | 9| 64.9500 en 63.8460 |+ 8| 64.5400 fa | 63.0710 |-4-10| 65.3160 De 63.4735 |+10| 64.9170 Jo | 63-8705 |+ 9! 64.5135 Та | 65.0400 |-+17| 63.3445 b | 65.0445 |+17| 63.3410 с 65.0360 |-+16| 63.3530 а | 65.0390 |+16| 63.3515 е 65.собо |-+16| 63.3780 Л | 65.0430 |-+17| 63.3445 Па | 62.8950 |+-10| | 65.4905 b | 62.9035 |+10| 65.4885 [9 62.8905 |+10| 65.4970 d | 62.8980 |+ 9| 65.4915 e | 62.8650 |+ 9| 65.5185 Л | 62.9085 |+10| | 65.4870 Ша | 59.7540 |-+16| 68.6295 b | 59.7540 |+15| 68.6305 с | 59.7435 |-+15| 68.6485 4 | 59.7390 |-+14| 68.6490 е 59.7040 |+14| 68.6850 f | 59.7340 |+-ı4| 68.6520 ТУа | 65.3695 |+17| 63.0175 b | 65.3735 |+-17| 63.0180 с | 65.3550 |+16| 63.0255 а | 65.3625 |-+16| 63.0225 e 65.3360 |-+16| 63.0510 f | 65.3635 |++7| 63.0220 8 т НЕЁ _mm_| mm 10000110000] 77? +17I © 0.0000 +14 ©] + 4.9782 + 6-18] —39.1610 +20|— 3| 13.5917 —=14|-+20] —36.7125 +23 ol — 0.2966 +23 ©] + 0.8342 +16 — 0.3540 +16 —= 0.0490 +16 —= 0.4490 +16 = ©9852 +16 —= 0.0482 +16 + 0.4494 +16 — 0.3662 +16 —= 0.0328 +16 — 0.4390 +17 — 0.3651 +17 + 0.0354 +17 + 0.4396 +17 — 0.4016 +17 — 0.0032 +17 — 0.4118 +18 — 0.3636 +18 + 0.0372 +18 + 0.4374 + 9 + 1.6074 + 9 + 1.6114 9 + 1.6012 +10 —+ 1.6034 +10 + 1.5736 т! -+ 1.6088 +10 — 0.5384 +10 — 0.5332 +10 — 0.5440 и — 0.5376 11 — 0.5676 +12 — 0.5301 +14 — 3.6784 +13 — 3.6788 +13 — 3.6931 +14 — 3.6957 +14 — 3.7312 +14 — 3.6997 29 1935 pet = 1.9374 + 9 —+ 1.9244 +10 + 1.9296 +10 —- 1.9021 +11 —= 1.9304 Е. Renz, 1897. März 31. № Y wo+%cH%o + Fr —+ + œ + Яр 2 mm +1.5594 +1.5626 —+-1.5660 +1.5668 +1.5691 +-1.5718 —0.5864 —0.5820 mo 192 — 0.5742 — 0.5721 —0.5671 —3.7264 —3.7276 —3.7283 — 3.7323 5:73 — 3.7367 1.8877 -+ 1.8886 +-1.8892 +-1.8930 —=1.8976 —-1.8934 Scheinbare ВАШ: M—Centrum —+ 5.2703 = — 41.4090 » —+-14.3250 — 38.7106 — 0.3202 = + 0.8888 Ly—= 10° m 14.9 3 mm 0.0180 0.0488 0.0352 0.0366 0.0045 0.0370 Trabant — Jupiterscentrum. Para и уз) Ph | Au cos | Mittel. mm —=1.5660 —0.5768 37312 +-1.8916 Л?а =0.99313 fu =0.99281 Г’, = 0.99327 Pulkowaer Sternzeit der Aufnahmen. 10° 39“ 47°. (März 27). 13 1.5555 — 0.5729 — 3.7061 —=1.8789 38: 48 39 4202.16 43 un 44 2 — 0.0003 0.0001 -+0.0008 —0.0004 —1°, —+0.00021 —iy Ве. =-н Try Je 31 = O = -+0.00046 —0:0011 —-0.COII —0.0011 — 0.0011 — +0.00015_ Mittel. 13° 417 29° —+1:5541 —(,5739 —3,1064 +-1,8774 3—4 5—4 3—4 4 4 unterexponie) 2—8 3 3—4 3A 4 | 3—4 ищегехро 3 2—3 3 3 3—4 deformier 3 3 unterexpon tell. 2—8. - >| POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. wD © C5 1597. März 31. ihe. Decl. Bemerkungen zur Aufnahme. x? ere x? . — 5 tgù sin l’ у— = tgÿ sin Г P.-Kr.90° t-+k tt P.-Kr.270° 63.6409 | 61/7408 Se я 8 63.6400 |-+ 9| 64.7392 0.0000 0.0000 Bilder 2. Praesepe | 66.6640 |+ 8| 61.7110 — 0.0013 + 3.0253 und Jupiter sind an 67.2008 |-+25| 61.1795 — 0.0811 + 3.4793 verschied. Tagen | 39.0525 |-+29| 89.3245 — 0.0094 —24.5934 aufgenom,. worden. \ 39.0715 |+41| 89.2985 — 0.0694 —24.6300 In der Zwischenzeit M 44.2430 |+20| 84.1278 0.0000 —19.1909 war dieCassette ab ’ 94.5630 |— 2| 33.7965 0.0000 +-30.9413 genom., doch blieb 68.7995 +14| 59.5960 es Die airs …_ 68.4090 |-+-19| 59.9820 + + 4.7615 Bilder 3. Windig. ‚68.0240 |-+19| 60.3660 + ‚67.1345 |+ 9| 61.2590 + 66.7520 |+ 9| 61.6400 + —= 3.1061 66.3700 |+11| 62.0210 + 65.4695 |+17| 62.9270 —= “6s.0910 |+17| 63.3045 -1- + 1.4419 64.7020 |+17| 63.6815 == 62.5020 |+10| 65.8890 = 62.1165 |+10| 66.2645 = — 1.5240 61.7390 |+10| 66.6480 — 60.7910 |+11| 67.5955 == 60.4165 |+15| 67.9740 — — 3.2321 60.0280 |+15| 68.3570 == 59.2270 |+-11| 69.1670 — 58.8420 |-+11| 69.5450 = — 4.8012 | 58.4645 Lis mé ie De Trabant — Jupiterscentrum. { У — У» | Mittel. | "зи To (23) ера) Ph. | дб & mm mm 67.7145 |+18| 60.6700 + —0.6889 pos Hi: 023320 + an 04.3925 + 3.9935 == О + Br D =, ’ _0 61.4250 |+10| 66.0630 ER 0.6950 0.6951 0.6907 | -+0.0004 0.0001 | <-0:0002 0:6902 68.6730 — —0.6972 70.2450 — —0.7010 59.7910 un sos 61.4555 == —+-0,1811 63.1190 + —0.1817 Е 68.0820 En = 01808 +0.1805 | -+0.1794 | —0.0001 0.0000 | 0.0002 —=0.1795 67.7965 — 0.1795 69.3725 — +-0.1718 58.3070 1 u 59.9650 + —1.6695 61.628 1 +-1.6725 bas BE 5040 ce 16716 | +1-6723 | +1.6620 | —0.0009 0.0004 | <-0.0002 | --1,6609 66.2990 — -+1.6747 67.8695 — +-1.6728 629195 —0.9372 2.5750 —0.9394 64.2400 99370 1 23 _ = 67.2070 0.9398 0.9400 0.9342 | -+0.0004 0.0001 | -#-0.0002 0,9337 69.9190 —0.9417 —0.9452 Scheinbare Decldif. M-—Centrum — + 3/0033 f°& = 0.99337 1° 5 = —0.00004 | N— » = + 2.4542 . . , | Q— » —=— 24.4340 fs = 0.99283 3 =-— 0.00018 X 13 = — 06 | Е— » = —24.4658 | У » ——19.2652 1’; = 0.99383 Ту = +0,00024 | W— » —+30.7332 dy = 12° 16:9 204 Е. Renz, 78. 1897. April 2. AR Scalenablesung. Pulkowaer Sternzeit Object. 5 fr a rd) P.-Kr. 0° ++ P.-Kr.180° + : der Aufnahmen. Mittel. 12 10000 10 10000 10000 num nu Ctr. | 64.3140 64.0707 Ss 64.3132 |+ 8| 64.0698 |+ 9 о 0.0000 1—2 M 69.2942 |+14| 59.0870 |+10| ol + 4.9822 2 N 25.1452 |+26| 103.2362 |+ 5|-18| — 39.1643 р ве: - 2 Q 77.9965 |+#21| 50.4755 |+15|— 31 13.5938 10 12 58 1—2 В 27.5878 |-+34| 100.7918 |+13|-+20| —36.7206 2 И 64.0145 |+17| 64.3685 |+15 о] — 0.2986 1—2 Им 65.1532 |-+28| 63.2212 |+24| 0] + 0.8446 1 2 an | 63.9275 |+ 9] 64.4645 |+ 8 — 0.3900 Ge 64.3165 |+ 9| 64.0790 |+ 8 — 0.0028 — 0.0033 ко 55 я 1—2 а, | 64.7015 |+17| 63.6930 |+ 8 —= 0.3830 2b | 63.9165 |+ 9| 64.4730 |- 8 — 0.3994 b, 64.3195 |+ 9| 64.0790 |- 8 — 0.0014 — 0.0060 36 6 2 b, 64.7015 |+17| 63.6935 |+ 8 + 0.3828 % съ | 63.9145 |+ 9) 64.4840 |+ 8 — 0.4064 Ce 64.3030 |+ 9| 64.0965 |+ 8 — 0.0184 — 0.0199 37 5 2 о 64.6835 |+17| 63.7110 |+ 8 — 0.3650 10° 37” 35° Zd | 63.9120 |+ 8| 64.4840 |+ 9 — ON) de 64.3035 |+ 8 64.0905 |+ 9 — 0.0152 — 0.0180 2852.17 1—2 do | 64.6855 |+16| 63.7050 |+ 9 + 0.3690 %е, | 63.9090 | 8| 64.4880 |+ 9 — 0.4112 ee 64.2870 |+ 8| 64.1060 |+ 9 — 0.0312 — 0.0298 DONNEZ 2 CA 64.6705 |+16| 63.7220 |+ 9 + 0.3530 } %fw | 63.9260 |+ 9] 64.4600 |-+-10 — 0.3887 de 64.3290 |+ 9] 64.0660 |+10 + 0.0098 + 0.0009 FORME 2—3 .6 63.6 .38 : fo Da Vi NET TES Be Trabant — Jupiterscentrum. Tt— Ty | Mittel. Ише) Ja (ие) Ph. | До. cos à PE EL ON EU ER Та 66.1760 |+11| 62.2075 |+ 9 + 1.8627| -+1.8660 2 6 | 66.1685 |+11| 62.2120 |+ 9 + 1.8567| -+1.8627 1—2 с 66.1650 |+10| 62.2230 |-- + 1.8494] +1.8693 р , HERR "= 2 а | 66.1655 |+10| 62.2180 |+10 + 1.8521| +-1.8701 18680), 41,8548 22 0.0012 | +1.8536 2 e 66.1555 |+11| 62.2295 |+I1 + 1.8414] +-1.8712 1 f | 66.1840 [+11] 62.2010 |+12 + 1.8698| 1.8689 1—2 II Geht du/rch |die Jupiter|schelibe. Ша | 61.3575 |+12| 67.0240 |+ 9 — 2.9548] — 2.9515 2 b | 61.3540 |+11| 67.0290 |- 8 — 2.9590] — 2.9530 2 с | 61.3495 |+11| 67.0340 |+ 8 — 2.9638| 2.9439 | . à A) Le Ld 1—2 а | 61.3515 |+10| 67.0305 |+ 9 — 2.0611| —2.9431 2.9464 2.9255 0.0001 0.0012 2,9268 | о е 61.3415 |+10| 67.0445 |+ 9 — 2.9731| —2.9433 1—2 f | 61.3710 |+11| 67.0135 |+10 — 2.9428| —2.9437 | 2 ТУа | 71.2080 |+13| 57.1760 | 9 —= 6.8946] -+6.8979 1—2 6 | 71.2035 |+12| 57.1790 |+ 9 -+ 6.8908] -+6.8968 | 2 с 71.1955 |-+12| 57.1880 |+10 —= 6.8822| -+6.9021 & 1 а | 71.1990 |+-13| 57.180 |+11 + 6.8854] +6.9034 +-6.9010| —6.8521 | --0.0002 0.0012 | + 6,8511 1 e 71.1885 |+13| 57.1945 |+12 + 6.8754] +-6.9052 1—2 F 71.2165 |+14| 57.1710 |+-12 + 6.9012| -+-6.9003 1—2 Scheinbare ЖАй: M—Centrum =+ 52703 F° =0.99295 —®, = — 0.00004 N— » = —41.4093 Q— » =+14.3250 fu = 0.99264 —iy =- 0.00008 Xi, 208 R—- » —= —38.7107 Вет. =-+ 2 У » = — 0.3202 И Е о W— » — + 0.8887 fly = 099292 ЛХ. = —0.00006 a7, == 10 143 Bilder, | | : в | | j | | | | | | POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897. April 2. 1ne. | Scalenablesung. Pr. 90° ++ P P.-Kr.270°|t-+k mm _mm_ mm | er 10000 65.1028 10000! 10000! 7” 63.2818 |+ 9| 65.1012 0.0000 66.3038 |+11| 62.0812 ©] + 3.0214 66.8450 61.5390 |+25|— 1|+ 3.5630 38.6870 89.6945 3 38.7140 89.6658 ь 43.8838 84.5008 5 94.2305 34.1538 68.3980 59.9960 68.0330 60.3690 67.6575 60.7330 66.7100 |+ 8| 61.6870 66.3430 |-+-10| 62.0605 65.9750 [+10] 62.4210 64.9930 |+16| 63.4000 64.6375 |-+16| 63.7680 64.2660 |+ 8| 64.1335 62.0895 | | 66.3030 61.7145 |+ 9| 66.6865 61.3385 |+-10| 67.0510 60.4060 |+-14| 67.9992 60.0380 |+14| 68.3585 59.6695 |+14| 68.7270 58.6425 |+10| 69.7545 58.2780 |+ $| 70.1365 $7.9тто |+ 5| 70.4850 67.2155 |+ 8| 61.1715 |-+23 65.5265 |+18| 62.8555 |-+22 63.8215 |+ 8| 64.5680 |-+29 60.8990 |-+10| 67.4890 |-21 59.2250 |-+10| 69.1600 |-26 57.4645 |+ 9| 70.9230 |-+25 Geht dulrch |die Jupiter|schelibe. 59.1870 60.8740 62.5845 65.5050 67.1815 68.9430 63.3500 65.0370 66.7480 69.6660 71.3400 73.1035 69.1970 67.5090 65.8000 62.8800 | 61.2040 | 59.4425 65.0365 63.3490 | 61.6385 | 58.7205 | 57.0495 55.2850 + —+ 4.2280 + G | Scheinbare Decldiff: M-—-Centrum = + 3.0033 » = + 3.4541 - » = —24.4340 » —= — 24.4659 = » = — 19.2652 } | W— » = +30.7333 | dy =-+12° 19.6 | ес]. Znt%2eot%s 3 mm + 4.7437 8.0533 + 1.3428 — 1.5729 — 3.2503 — 5.0112 Ye—Yy | Mittel. mm mm —0.8124 —0.8079 — 0.8070 —0.8126 —0.8079 —0.8088 —0.8094 -+1.1715 1.1747 +-1.1751 +-1.170$ -+1.1717 —+-1.1709 -+1.1724 — 2.9901 —2.9877 —2.9876 — 2.9902 — 2.9851 — 2.9898 —2.9884 198 = 0.99315 fs = 0.99264 Г; =0.99326 205 „р PES 2 cp Bemerkungen — 3 tgù sin 1’ ее > #96 sin 1 zur Aufnahme, mm mm 0.0000 0.0009 Bilder 3. — 0,0013 + 3.0201 — 0,0811 + 3.4819 — 0.0094 — 24.6010 — 0.0694 — 24.6324 0.0000 — 19.3970 0.0000 —=30.9464 Trabant — Jupiterscentrum. à T = ау» Та (реа) | er) РВ. | 45 —0.8039 | -+0!о00т —0:0001 | -+0'0002 | —0:8037 —1.1645 | —0.0001 —0.0003 | -+0.0002 —+1.1643 —2.9683 | -+0.0002 —0.0015 | -+0.0002 — 2,9694 1° 5 = -0.00010 is = 0.00000 X щ=0.0 Js = +0.00003 26* 206 79. Object. ы - bd = = = [= SOU SO Зозоза Зо QE SR 8 NS SA Р.-Кг. 0° |t+-k| P.-Kr.180° 61.5220 61.5211 66.4988 22.3588 75.1232 24.8058 61.2290 62.3465 61.0925 61.4970 61.9090 61.1050 61.5085 61.9090 61.0965 61.5020 61.9030 61.0935 61.4960 61.8995 61.1065 61.5085 61.9175 61.0920 61.4915 61.8950 62.0825 62.0845 62.0715 62.0650 62.0730 62.0530 59.3630 59.3695 59.3580 59.3505 59.3625 59.3420 62.8850 62.8885 62.8785 62.8700 62.8830 62.8620 67.0190 67.0240 67.0150 67.0090 67.0200 67.0025 Scheinbare Вай: M—Centrum = + 5'2704 ЕЕ Scalenablesung. mm 66.8643 66.8635 61.8845 106.0250 53.2620 103.5715 67.1530 66.0335 67.3095 66.8995 66.4870 67.2900 66.8865 66.4895 67.2985 66.8950 66.5000 67.3060 66.8945 66.4960 67.2980 66.8865 66.4790 67.3040 66.8950 66.5020 66.3045 66.2995 66.3135 66.3215 66.3150 66.3340 69.0175 69.0120 69.0245 69.0330 69.0230 69.0430 65.5000 65.4925 65.5050 65.5110 65.5005 65.5200 61.3660 61.3630 61.3735 61.3805 61.3665 61.3860 К. Rexz, 1897. April 6. № Pulkowaer Sternzeit НК der Aufnahmen, | Mittel. mm | mm 10000, 10000 a He -8 о 0.0000 1—2 — 9| о |- 4.9784 1—2 + 6-+18| —39.1600 ‚ De 2 2 +17)— 3| +13.6017 10° 18” 10 2 +16,+-20| — 36.7086 2 +15 0] — 0.2906 1—2 +25| ©] -+ 0.8274 1—2 + 8 — 0.4372 8 — 0.0300 — 0.0284 10 24 40 1—2 + 8 —- 0.3822 + 8 — 0.4212 8 — 0.0178 — 0.0193 РУ 1 + 8 + 0.3810 : + 8 — 0.4297 + 8 — 0.0252 — 0.0274 261128 5 x 1—2 + 8 + 0.3728 10° 26” 59 no — 0.4350 +9 — 0.0280 — 0.0300 27,228 1 + 9 + 0.3729 + 9 — 0.4246 + 9 — 0.0178 — 0.0173 28 19 1—2 + 9 + 0.3904 +-IO — 0.4348 x +10 — 0.0306 — 0.0326 20 1—2 27, TIRE Trabant — Jupiterscentrum. Rare | Mittel, | Хи) Тиби) Ph. | Да cosd mm mm +-10 + 0.5601| -+0.5885 2—3 +10 + 0.5636] -0.5829 1 He a do BR +0.5754| —o!5714 | —o!ooor | —0!0014 | -+0:5699 2 II + 0.5500] -+0.5673 2 +-12 + 0.5306] +0.5632 2 +14 — 2.1562] —2.1278 2 +13 — 2.1502| —2.1309 1—2 +13 — 2.1622| —2.1348| _ se file за 2 ns Bee DTA 2.1222 | -+0.0004 0.0014 2,1232 12 +14 — 2.1593] —2.1420 1—2 +14 — 2.1795] —2.1469 2 —10 | + 1.3636] 1.3920 1—2 +10 + 1.3692| 1.3885 1 6 2 a SE т я 1.3834 | 1.3739 | —0.0002 | —0.0014 | 1.3723 | 1 о +11 + 1.3623| +-1.3796 1—2 +12 + 1.3420] +1.3746 +10 — 5.4976| +5.5260 1—2 +10 + S.S016| +5.5209 jl Il + 5.4918] 5.5192 PR ne 2 Te 6.4853] 5.5153 -Н5.5176| —+-5.4792 0.0010 0.0014 | +5,4768 | ;_o +12 + 5.4948| +5.5121 2 +13 + 5.4792| 5.5118 2 Fa = 0.99308 —1°,, = +0.00046 — » =—41.4094 f Q— » = 14.3251 0277, —iy = +0,00041 x iWw=—15 В— » — —38.7107 Refr. = + I У » = — 0.3201 sn = о W— » = + 0.8886 Га =0.99305 Ja = -+-0,00042 h 9.2) = 10 т 13.3 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897. April 6. Decl. 1ne. | Scalenablesung. I y |P.-Kr.90° += P.-Kr.270° | ++ р тт mm mm 66h 4 |10000 617081 10000] 10000 ne 63.6805 + 9| 64.7065 |+16| о 0.0000 66.7028 | 8| 61.6790 |+10] 0o|-+ 3.0252 67.2335 |+24| 61.1505 |-+27|— 1| + 3.5546 39.0880 |+28| 89.2962 |— 2| + 5| —24.5888 “390970 |-+-41| 89.2782 |+11|-+13| —24.5744 44.2830 |+20| 84.1005 |— 7|+ 2] —19.3938 94.6250 |— ı| 33.7595 |+20|— 8] +30.9442 -68.8200 |-+14| 59.5765 |+14 + 5.1351 68.4245 |+19| 59.9655 |+14 + 4.7431 68.0330 |-+19| 60.3680 |+-14 + 4.3461 67.2340 |-+ 9] 61.1650 |+10 + 3.5478 66.8475 |+ 9| 61.5500 |+ 9 + 3.1621 66.4660 |+ 9| 61.9335 |+ 9 + 2.7796 ‘65.5805 |+11| 62.8160 |+ 9 + 1.8957 65.1960 |+17| 63.2015 |+ 9 + 1.5110 64.8135 |+17| 63.5850 |+9 + 1.1280 | 62.5435 |+10| 65.8550 |+10 — 1.1424 62.1500 |-+-10) 66.2440 |+10 — 1.5336 61.7700 |+10| 66.6295 |+ 8 1.9163 60.8460 |+-11| 67.5490 |+18 — 2.8385 60.4640 |-+15| 67.9350 |+18 — 3.2223 60.0750 |+15| 68.3200 |+-18 — 3.6093 59.1575 |+11| 69.2400 |+13 — 4.5230 58.7725 |+ı1) 69.6250 |+16 — 4.9132 58.3980 |+ 6| 69.9990 |+16 5.2876 | 68.2130 |+19| 60.1740 |+14 + 4.5331 1“66.6410 |+ 9| 61.7450 |+ 9 + 2.9614 64.9920 |+17| 63.3950 |+ 9 + 1.3122 | 61.9485 |+10| 66.4370 |+10 — 1.7310 60.2560 |+15| 68.1290 |+18 — 3.4233 8.5730 |+11| 69.8150 |+16 — 5.1079 | E +15) 58.9920 |+11 + 5.7148 | 67.8180 |+20| 60.5680 |-rıı + 4.1388 | 66.1700 |+-12| 62.2170 |+10 + 2.4900 | 63.1290 |#11| 65.2570 |+17 — 0.5510 | 61.4370 |+12| 66.9495 |+ 9 — 2.2428 | 59.7525 |-++16] 68.6350 |+ 14 — 3.9278 ‚67.7260 |-+19| 60.4560 |+-14 + 4.2486 66.3550 |+11| 62.0320 |+9 + 2.6750 64.7000 |+17| 63.6840 |+ 8 + 1.0218 ‚61.6600 |+10| 66.7240 |+ 8 — 2.0186 92.9660 15| 68.4150 |+18 — 3.7113 58.2840 |-+- 6| 70.1000 |-+16 — 5.3952 66.2150 |+10| 62.1730 |+10 + 2.5344 | 64.6415 |+16| 63.7480 |+ 9 + 0.9604 | 62.9920 |+ 9 65.3945 +17 — 0.6883 | 59.9430 |+14| 68.4395 |+19 — 3.7352 58.2560 |+ 5| 70.1325 |+17 — 5.4255 | 56.5730 |+- 9] 71.8180 |-+12 — 7.1093 Scheinbare Decldiff: M—Centrum = + 3/0034 N— » = + 3.4541 Q— » = —24.4340 Е » =-—24.4659 V— » = —19.2652 W— » = +-30.7334 dy =-+12° 24:7 Чин с; тт + 4.7414 + 3.1632 + 1.5116 — 1.5308 — 3.2234 — 4.9079 тт —0.2083 —0.2018 —0.1994 —0.2002 —0.1999 —0.2000 —+-0.9734 —0.9756 —+0.9784 0.9798 —0.9806 —0.98 от —0.4928 —0.4882 — 0,4898 —0.4878 —0.4879 —0.4873 — 2.2070 — 2.2028 — 2.1999 — 2.2044 — 2.2021 — 2.2014 тт — 0.2016 —+-0.9780 —0.4890 —2.2029 795 = 0.99326 fs =0.99274 Г: =0.99336 2 Es , — 7 190511 тт 0.0000 0.0013 0.0811 0.0094 0.0694 0.0009 0.0000 PAIE) x? . у— = tgÿ sin 1’ mm 0.0000 + 3.0239 + 3.4735 —24.8982 —24.6438 — 19.3938 —30.9442 Trabant — Jupiterscentrum. - T уг ух | Mittel. Ir "sy —y2) | Jo(tr—22) | Не-а) Ph. —0:2003 | —0:0002 —0.9715 | -+0.0006 —0.4858 | — 0.0004 — 2.1882 | —0.0015 19; = —0.00018 is =— 0.00029 Лу =— 0.00027 207 Bemerkungen zur Aufnahme. Bilder 3—4. Bilder 3. 00000 | -+0'0002 —0,0001 | -+0.0002 —0.0001 | -+0.0502 — 0.0010 | -+0.0002 X ig —=—1:0 —0:2003 : +-0,9722 — 0,4861 — 2,1905 208 „F. Renz, so. 1897. April 7. № Scalenablesung. Pulkowaer Sternzeit Object. 8 x Toto wo P.-Kr. 0° == Р.-Кт.180°] + der Aufnahmen. Mittel, D 10000 pre 10000 10000 m on Ctr, | 62.7454 65,6362 5 62.7445 |+ 9| 65.6345 |-+17| о 0.0000 2 M 67.7208 |-+19| 60.6505 [+10] ol+ 4.9810 1—2 N 23.5800 |-+26| 104.7988 | 7|-+18]| —39.1612 : м. 2 Q 76.3420 |+20| 52.0412 |11|— 3|-+13.5954 10° 52 20 2—3 Е 26.0230 |-+37| 102.3480 |-+14|-+20| —36.7154 1-9 LA 62.4435 |-+18| 65.9270 |+17| o| — 0.2963 1—2 W | 63.5795 |-+20| 64.8015 |+31| c|<+ 0.8338 2—3 % y | 62.2825 |--10| 66.1080 |+10 — 0.4674 а; | 62.6950 |+ 10| 65.6950 |+10 — 0.0546 — 0.0575 то 89:12 2—3 Go 63.1005 |+10| 65.2920 |+16 —+ 0.3494 2b, | 62.3000 |+10| 66.0905 |+10 — 0.4498 6; | 62.7135 |-+10| 65.6820 |+10 — 0.0388 — 0.0398 39 59 2—3 b, 63.1210 |[+10| 65.2730 |-+16 + 0.3691 7 Cp | 62.2765 |+10] 66.1125 |+10 — 0.4726 Ce | 62.6830 [10] 65.6990 |+10 — 0.0626 — 0.0609 40 49 EB 2—3 co | 63.1030 |+-109| 65.2880 |+16 + 0.3526 10° 41” 15° Zdy | 62.2710 |+ 9| 66.1200 |+11 — 0.4792 de | 62.6870 |+ 9| 65.7010 |-11 — 0.0617 — 0.0672 41 48 2—3 do | 63.0920 |+ 9] 65.3035 |-+17 —+ 0.3392 Zen) | 62.3060 |+ 9] 66.0915 |-11 — 0.4474 ес 62.7030 |+ 65.6775 |+11 — 0.0420 — 0.0407 42 28 923 en 63.1185 | 9| 65.2740 |+17 + 0.3672 Zfw | 62.3055 +10] 66.0900 |+-12 — 0.4470 Je 62.7050 [+10] 65.6850 |-+12 — а — 0.0434 43 23 2—3 gp 7 rt TR Trabant — Jupiterscentrum. 1—2 | Mittel. Уаз и (уу he | Да cos à mm mm I Bedeckt. Па | 60.9210 |+11| 67.4580 |+ 8 — 1.8230] —1.7655 D) b | 60.9460 |+11 67.4365 + Е — 1.1997 me Е {Я 60.9255 |-+-11 7.4590 |+ — 1.8212] — 1.7603 | __ ra 9) р Ar Br LE а | 60.9220 |+10| 67.4620 |+ 9 — 1.8246] —1.7574 1.7588 1.7465 | -+0.0001 on 1.7478 2—3 e 60.9520 |+10| 67.4320 |+ 9 — 1.7946] — 1.7539 . 2—8 Л 60.9470 |+11| 67.4360 |+-10 — 1.7990] —1.7556 2 Ша | 59.9410 |+16| 68.4395 |-+19 — 2.8040] —2.7465 2 b 59.9565 |+15| 68.4240 |+18 — APE —2.7487 2? с 59.9355 |+15| 68.4460 |-+18 — 2.8100] —2.7491 | __ Каз 4 Fe а | 39.0285 [+14] 68.4560 [+19 — 2.8196] —2.7524 2.7504 2.7311 | -Н0.0002 0.0014 | —2,7323 | 5 е 59.9550 |-+14| 68.4280 |+19 — 2.7914] —2.7507 1—2 Х | 59.9465 |H-15| 68.4340 |-+-20 — 2.7986] —2.7552 1—2 IV а | 65.3350 |-+17| 63.0460 |+ 9 + 2.5903| 2.6478 2 b | 65.3555 |17| 63.0275 |+ 9 + Re BE 2 с 65.3355 |-+16| 63.0480 |+ 9 + 2.5895] 2.6504 Ar Le 9 а 65.3240 +16] 63.0600 Ira + 2.5777| +2.6449 2.6462 | -+2.6276 0.0002 0.0014 | -+2,6260 2 e 65.3490 |-+17| 63.0345 |411 + 2.6030] -+2.6437 1—2 f | 65.3435 |+-17| 63.0400 |+12 + 2.5974] 2.6408 2 Scheinbare Ædiff: M—Centrum == + 5.2704 Ja = 0.99303 —1°, = -+0.00222 N— » = —41.4094 3 Q— » =-14.3251 fa = 099270 —iy = -+0.00015 X y =— 05 R— » = —38.7107 Refr, = + 2 У— » = — 0.3201 Ира — о. W— » — +- 0.8886 Île = 099298 ЛХ. —+0.00017 h т 0, = 10 13.1 Bilder! etwasel ыы... | À PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 209 1897. April 7. Decl. Bemerkungen Fe. RER y—- 190311 zur Aufnahme. 66.6490 ‚66.2540 65.8670 ‚65.0120 ‚64.6160 64.2290 ‚62.0290 61.6350 61.2550 ‚57.8690 à 68.6370 ‚66.9575 | 65.3180 | 62.3405 ‚60.6960 58.9505 | 69.1850 |] | 59.0185 | 57.2765 | Scheinbare Decldiff: } | Bedeckt. aaa Tr =" 65.2128 |+10 62.1845 |+10 о 0.0000 О] + 3.0256 61.6505 |+26|]— П-н 3.5622 89.8062 |— 3|-+ 5] —24.5902 89.7752 |+ 8|+13| —24.5642 84.6038 |— 2|+ 2] —19.3916 34.2618 |+20|— 8]+-30.9512 60.0720 |+-14 60.4610 |+14 60.8600 |+10 61.7430 |+ 9 62.1420 |+ 9 62.5315 |+ 9 63.8860 |+ 8 64.2770 |- 8 64.6660 |+ 8 66.3640 |+10 66.7570 |+ 8 67.1485 |+ 8 68.0150 |+18 68.3960 |-+18 68.7890 |+13 69.7640 |+16 70.1450 |-+-16 70.5280 |+16 59.7470 61.4280 63.0650 66.0460 67.6920 69.4350 59.2015 61.4345 63.1080 64.7465 67.7280 69.3700 71.1090 Q— PE ve We Зап. Фяз.-Мат. Отд. » » » » » ac a a ВИ u — — 0.0526 30 46 2—3 LR nr À — — 0.0326 31 40 2 1 + ge | — — 0.0294 38 6,37 2 | Trabant — Jupiterscentrum. &t—%y | Mittel. fax) Iulyı—-yz)) Ph. Aa cos à mm mm 9 3 - + 1.5255 — + 1,5298 2—8 ellipt. 9 + +-1.5306 ‚ De Es Pa 2—3 1 Le 1.5320 | 715337 | 51.5228 0.0001 о'оотб | +1:5207 9 + —=1.5390 2 + —+1.5418 2—3 —- —0.6393 2 | + +0.6380 2—3 elliptinl + +-0.6326 2—3 u Е. 0.6275 0.6309 | -+0.6264 0.0900 | —0.0015 | -+0,6249 8 Ё = +-0.6258 р \ — +-0.6223 2—3 = —3.4488 2 |. — — 3.4462 te ellipt.… =. 73-4439)... De De set mi — 3.4428 3.4435 3.4192 | 0.0001 O.COIS 3.4206 2 — —3.4406 2 = — 3.4388 2 — —3.6483 2 4 — —3.6502 2—3 ellipt = = и Ki Bt 2—3 в =: —3.6584 3.6544 3.6286 | 40.0001 -0.0015 3.6300 2—3 Я — —3.6581 2 = —3.6580 2—3 Va 9:99297 —i° = +-0.00012 4 = —41.4094 | = -+-14.3252 fa = 099266 —14 = +0.00007 X 1, = —02 | | — —38.7107 Refr. = + I A ==— 0.3200 Try = о = + 0.8885 Fa = 0,99294 Jy = —0.00008 Е у 593 “632459 | 1000 | 63.2450 | 66.2650 66.8018 |- 38.6485 |: | 38.6650 43.8410 94.1942 67.6110 66.8025 _ 66.4115 66.0320 65.0625 64.6760 64.2900 62.0860 61.6970 | 61.3130 60.4160 _ 60.0300 _ 59.6440 . 58.7690 58.3805 _ 58.0050 | 67.3280 65.7410 ‚64.0010 61.0210 59-3430 _ 57.7080 67.7895 | 66.2030 _ 64.4670 . 61.4920 | 59.8200 58.1810 Ы _ 69.3930 _ 67.8050 66.0650 il 63.0925 61.4155 59.7750 ‚69.65 то _68.0670 || 66.3260 63.3520 || 61.6800 | 60.0380 |р.-Кг.90° _ Scalenablesung. += P.-Kr. 270° POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1897, April 9. Decl. Фен, Е з 65.141 4 [10006] 10000 vn mm 65.1398 N 62.1100 ©] + 3.0252 61.5785 . 89.7342 —24.5930 89.7065 —24.5701 84.5345 —19.3978 34.1908 —=30.9475 59.9915 |-+14 Ра 60.3890 |+-14 — 4.7534 + 4.7559 60.7830 |+10 + 4.3622 61.5945 |+9 + 61.9810 |+ —= + 3.1660 62.3610 |+ + 63.3280 |+ + 63.7170 |+ 4 + 1.4277 64.1055 | + 66.3170 |+ — 66.6995 |-- — — 1.5521 67.0790 |- 8 — 67.9905 |+18] |— 68.3630 |-+18 — — 3.2216 68.7515 |-13 — 69.6280° |+16 — 70.0170 |+16 — — 4.8663 70.3910 61.0580 62.6475 64.3860 67.3655 69.0390 70.6835 60.5940 62.1805 63.9185 66.8950 68.5670 70.2060 58.9890 60.5770 62.3150 65.2940 66.9685 68.6115 58.7340 60.3205 62.0600 65.0340 66.7070 68.3480 +Scheinbare Decldif: M—Centrum = » Y—Yy | Mittel. mm mm —0.6733 —0.6715 —0.6725 —0.6723 —0.6788 —0.6741 —0.2100 —0.2070 —0.2057 —0.2015 —0.2041 —0.1989 —+1.3941 —1.3962 +-1.3951 +-1.3988 +-1.3930 —1.3959 +-1.6507 +1.6552 +1.6531 —1.6585 —+1.6560 1.6589 — 0.6738 В бы — 0.2045 РРР 1.3955 BETT +1.6554 Е 195 = 0.99311 Ss = 0.99259 f's = 0.99320 ^ 64, = -+12° 27'9 x? . — а tgù sin Г x? ne N У — = (9681 1 тт. тт 0.0000 0.0000 — 0.0013 + 3.0239 — 0.0811 + 3.4781 — 0.0094 — 24.6024 — 0.0694 — 24.6395 0.0000 — 19.3978 0.0000 —=30.9475 Trabant — Jupiterscentrum, 211 Bemerkungen zur Aufnahme. Bilder 4, Windig. т fat) Is иг) Чет Ph —0.6692 | —0.0002 — 0.0001 | 40/0003 —0.205I | —0.с001 0.0000 | -+0 0c03 +1.3860 | -+0.0005 | —0.0C04 | 0.0003 1.6441 +-0.0005 —0.0C04 | -+0.0003 | 1° 5 = —0.00004 î5 =- 0.00016 X is = —0:6 Is = —0.00014 — 0.6692 | 0.2029 1,3864 | +1,6445 212 Г. Renz, 82. 1897. April 10. Ж Scalenablesung. s Pulkowaer Sternzeit | Object © mar cut) Bilder, P.-Kr. 0° ыы P.-Kr.180°| t-+k © der Aufnahmen. Mittel. 25 10006] „gm 1000610006] mm dat Ctr, | 63.2671 65.1190 5 63.2662 |+ 9| 65.1173 |-+17| о 0.0000 2 M 68.2398 |+19| 60.1350 |-+14|] o|<+ 4.9786 2 A N 24.0960 |-+26| 104.2855 |-+ 6|-+-18| — 39.1660 к Вере > 1—2 etwas el Q 76.8705 |#+22| 51.5135 |+21|— 3|-+13.6042 10° 44 49 1—2 | R 26.5488 |-+35| 101.8242 |-+-14|-+20| — 36.7087 2 У 62.9722 |+-19| 65.4000 |-+23| ©] — 0.2882 2 W | 64.0895 |+20| 64.2900 |-+23| ol + 0.8256 ‘1—2 % &yp | 62.5005 |+10| 65.8950 |+10 — 0.7713 Ag 62.9070 |+10| 65.4840 |-+16 — 0.3628 — 0.3638 10: 5-28 2 @ | 63.3200 |+10| 65.0860 |+16 + 0.0426 | % by | 62.5080 |+10| 65.8865 |+10 — 0.7634 b. 62.9150 |+10| 65.4830 |+-16 — 0.3584 — 0.3579 5241 27 2 bo | 63.3240 |-10| 65.0790 |+16 + 0.0482 %Cyw | 62.5005 |+10| 65.8935 |+10 — 0.7706 Ce 62.8990 |+10| 65.4955 |+-16 — 0.3726 — 0.3704 52 26 2 ch 63.3060 |+10| 65.0935 |+16 -+ 0.0319 10% 53” 50° % р | 62.5150 |+ 9| 65.8795 |+11 — 0.7564 | de | 62.9090 |+ 9] 65.4860 |-+17 — 0.3630 — 0.3619 54 23 2 do | 63.3075 | 9| 65.0915 |-+17 + 0.0336 Zen | 62.5360 |+ 9| 65.8600 |+11 — 0.7362 ес 62.9345 |+ 9| 65.4600 |+17 — 0.3372 — 0.3358 55 13 1—2 ео 63.3395 |+ 9| 65.0585 |+17 + 0.0660 Zfw | 62.5430 |+10| 65.8540 |-+12 — 0.7296 Je 62.9380 |+10| 65.4610 |+18 — 0.3360 — 0.3363 56 4 2 an | à En ae a dr Fe ee Trabant — Jupiterscentrum. 2 — Ty | Mittel. A) J{yt—Y2)| Ph. Au. cos à mm mm Та | 61.0500 |+11| 67.3350 |+17 — 2.2168] —1.8530 2 b | 61.0525 |+11| 67.3305 |- 8 — 2.2134 в. 2—3 с | 61.0435 |+11| 67.3420 |- 8 — 2.2232] —1.8528 | _ Ace , be ar 2—3 4 | érosos |+10| 67.3380 [+ 9 — 2.2172| —1.85$5 1.8566 1.8435 +-0:0004 0.0015 1.8446 | 5 е | 61.0700 |+10| 67.3175 |+ 9 — 2.1978| — 1.8620 2—3 Л | 61.0725 |11| 67.3185 |-+10 — 2.1970] —1.8607 2 Па | 59.8605 |--16| 68.5235 |+-14 — 3.4054| —3.0416 2 b Pa +15 a +13 — 3.4030] —3.0451 5 € 59.8545 |+15 .5315 |+13 — 3.4124] —3.0420| __ ce la to, а | 59.8630 |+14| 68.2240 [#14 — 3.4046] —3.0427 3.0441 3.0226 | —+-0.0097 0.0015 3.0234 о е 59.8845 |+-14| 68.5040 |+14 — 3.3838] —3.0480 2—3 f | 59.8860 |-н15| 68.5010 |+-14 — 3.3815] — 3.0452 2 III Verfinstlert, IVa | 56.6350 |+-11| 71.7525 |+12 — 6.6328] —6.2690 2—3 b 56.6400 |+-10| 71.7485 |+12 — 6.6284] —6.2705 2—3 | С 56.6310 |+-10| 71.7580 |+-11 — 6.6376] —6.2672| _ >, А | In. xt, DE | а | 36.6850 |+ 9| 717560 |+ — 6.6346] —6.2727 6.2728 6.2285 | +0.0014 0.0015 6.2286 | о | е 56.6560 |+ 9| 71.7330 |+-12 — 6.6127| —6.2769 2—3 LE У | 56.6525 |+ 9] 71.7375 |+12 — 6.6167| —6.2804 2—3 | Scheinbare ÆRdiff: M—Centrum= + 5,2704 Fu = 0.99298 —1° y = #+0:000$4 | N— » = —41.4094 3 | À Q— » = +14.3252 fa = 0.99265 —iy = 0.00047 ig = — 15 В— » = —38.7107 Refr. =+ 3 V— » —— 0.3200 1K == о W—- » — + 0.8885 fu = 0.99291 Ло = 0.00050 h Lu) D NOM 12.5 SEE == = = BE nn ıne. р.-Кг. 90° 63.1630 63.1620 66.1848 ‚66.7110 38.5715 38.5758 43.7620 94.1110 68.2790 67.8940 67.5080 66.7030 66.3150 65.9270 65.1150 64.7360 64.3500 61.9695 61.5870 61.2175 60.35c0 59-9740 59.5960 58.6840 58.3080 57.9390 POSITIONEN DER J UPITERSTRABANTEN NACH PHOTO@RAPHISCHEN AUFNAHMEN. Scalenablesung. ны Р.-Кг. 270° тт 65,2241 65.2225 62.1960 61.6722 89.8168 89.7972 84.6168 34.2762 60.1170 60.4985 60.8965 61.6990 62.0845 62.4710 63.2900 63.6615 64.0500 66.4290 66.8020 67.1810 68.05 10 68.4230 68.8015 69.7200 70.0910 70.4630 59.7050 61.2860 62.8690 66.0040 67.6280 69.2940 59.1780 60.7660 62.3440 65.4800 67.1050 63.7660 57-7855 t+k 9 ЕЕ ЕЕ Е EEE +16 mm _| тт 10000] 10000 1897. April 10. 213 Decl. y %п+ с; EURE ET bn > Bemerkungen 3 Bu cc TR a zur Aufnahme, mm mm mm mm 0.0000 0.0000 0,0000 Bilder 3. + 3.0250 — 0.0013 + 3.0237 + 3.5498 — 0.0811 + 3.4677 — 24.5900 — 0.0094 —24.5994 —24.5772 — 0.0694 —24.6466 —19.3956 0.0000 —19.3956 +30.9460 0.0000 30.9460 + 5.1118 + 4.7286 + 4.7257 Bilder 2—3. — 4.3368 — 3.5326 ! + 3.1456 + 3.1457 + 2.7586 + 1.9434 + 1.5682 + 1.5641 + 1.1806 — 1.1991 — 1.5768 — 1.5756 — 1.9510 — 2.8201 — 3.1941 —>В-1953 30018 — 4.4877 — 4.8614 — 4.8604 Trabant — Jupiterscentrum. ; T R veus | Mittel. |Maw-m|Is@-en)-er-eg| Ph | 2 mm mm + 5.5190] +0.7933 + 3.9385] -+0.7928 X 627, een -+0,7938 | -+0'7885 +0/0007 | —0.0002 | -+0:0003 | -+0:7898 — 2.4028| -+0.7925 — 4.0676| -+0.7928 + 6.0456] -+1.3199 + 4.4614| 1.3157 À ge ый +1.3187 | 41.3098 | + 0.0011 | —0.0004 | +0.000; | 1,3108 — 1.8778] —+1.3175 — 3.5402] -+1.3202 + 7.4384| —+2.7127 — 5.8598] —+2.7141 т $ Pre: -2.7153 | +2.6971 —+-0.0023 —0.0014 | <+0.0003 | -+2,6983 — 0.4822| —+2.7131 — 2.1426| -+2.7178 —=+ 3.0034 195 = 0.99319 15 = —0.00026 = + 3.4540 о ь = —24.4341 fs = 0.99265 iz =— 0.00041 X 13 = —1:4 = —24.4660 — —19.2652 у = 0.99327 Js = — 0.00036 =+30.7334 | dy =-+12° 28,8 ar ay —= 10” 12.0 *) Stern- und Jupitersbilder zeigen bei allen Aufnahmen dieses Abends eine graue Färbung. fa = 0.99295 214 F. Renz, 55. 1897. April 13. AR 1 Scalenablesung. Pulkowaer Sternzeit | Object. - 8 Lt LU A D Bilder. M P.-Kr. 0° tt) P.-Kr.180°|t+-7% der Aufnahmen. Mittel. nu | mm m mm = mm r mm Ctr, | 62.9284 |1000| 65.4517 | 10009 10050 S 62.9275 |+ 9| 65.4500 |+17| о 0.0000 3 *) у M 67.9024 |+19| 60.4672 |+-14| ol + 4.9795 2—3 N 23.7622 |+-26| 104.6210 |+ 7|-+18] —39.1650 FRE ее; | 3 Q 76.5280 |+22| 51.8564 |-+21|— 3|-+13.5972 11° 10 28 2—3 Е 26.2050 |+37| 102.1650 |+-14|-+-20|] — 36.7152 2—3 etw. el № 62.6268 |-+-19| 65.7455 |+17| o|— 0.2971 2—3 [radial, W | 63.7622 |+20| 64.6188 |+-31| ©] + 0.8328 2—3 %ар | 62.5055 |-+10| 65.8975 |+10 — 0.4344 ас | 62.9230 |+10| 65.4790 |-16 — 0.0166 — 0.0155 тт 075018 4 ау | 63.3385 |+-10| 65.0520 |+16 + 0.4046 % by | 62.5225 |-+10| 65.8800 |+10 — 0.4171 : b. 62.9370 |-+10| 65.4670 |-+-16 — 0.0036 — 0.0060 18 0027 3—4 b, 63.3370 |+Io| 65.0540 |+16 + 0.4028 %с | 62.5185 |+ 9| 65.8800 |+10 — 0.4192 Сс 62.9205 |+ 9| 65.4815 |+16 — 0.0192 — 0.0172 19 22 3—4 Co | 63.3190 |- 9] 65.0680 |+16 —+ 0.3868 11% 19” 51° Zd | 62.4875 |+ 9] 65.9070 |+11 — 0.4482 de | 62.8960 |+ 9| 65.5015 |+17 — 0.0415 — 0.0438 20 24 3—4 do | 63.2895 |+ 9] 65.0955 |+17 + 0.3582 Фе, | 62.5000 |+- 9| 65.8940 |--ı1 — 0.4354 ес 62.8995 |+ 9] 65.4915 |+17 — 0.0348 — 0.0348 РТВ 3—4 ео 63.2980 | 9| 65.0890 |+17 + 0.3658 Zfyw | 62.4820 |+10| 65.9060 |+12 — 0.4504 о 62.9020 |+10| 65.4965 |-+18 — 0.0360 — 0.0381 BI 05 3—4 a a a и ВПП à je Trabant — Jupiterscentrum. mes | Mittel. |fo(er—22) Jéor—un)| Ph. | ввоз mm mm Та | 63.8495 |+ 9] 64.5350 |+16 + 0.9186] +0.9341 2—3 b 63.8555 | 9| 64.5310 |+-16 -+ 0.9236] +0.9296 3 ER À С 63.8390 |+ 8| 64.5480 |-+-16 —= 0.9068] -+0.9240 р Фет р р 2—3dichtneb а | 63.8065 |+ 8| 64.5790 |+-17 + 0.8750] -+0.9188 07210 LEROAAAS оодот |179,0016 LED АЯ 2—3 [Ster е 63.8135 |+ 9| 64.5755 |+18 —= 0.8802] 0.9150 3 % Х | 63.7975 | 9| 64.5875 |-++19 + 0.8662| +-0.9043 3 | Па | 61.1565 |+r11| 67.2250 |- 8 — 1.7724] —1.7569 3 | b 61.1605 |+11| 67.2220 |+ 8 — 1.7690] — 1.7630 | с | 61.1505 |+10| 67.2350 |+ 8 — 1.7805] — 1.7633 | __ IR ый As 2—3 : d 61.1170 +10] 67.2705 [+ 9 — 1.8150] —1.7712 1.7684 1.7560 | -+0.0002 0.0016 1.7574 9_3 | е | 61.1220 |+10| 67.2620 |+ 9 — 1.8083| —1.7735 | : 2—3 у f | 61.1105 |+-11| 67.2755 |+10 — 1.8208] —-1.7827 3 Ша | 64.7970 |--17| 63.5805 | 8 + 1.8704| -+1.8859 2—3 ll b | 64.8020 |-+17| 63.5775 |+ 8 + 1.8744] +1.8804 san | с 64.7900 |+-16| 63.5885 |- 8 + 1.8628| + 1.8800 2 4 2— |. | а | 64.7610 |+16| 63.6285 |+ 9 + 1.8284] 1.8722 о 2 0.0016 | +1.8602 2—3 2 e 64.7690 |+17| 63.6175 |+10 + 1:8378| -+1.8726 2—3 1! f | 64.7520 |+17| 63.6330 [+11 + 1.8214] 1.8595 2—3 [У а 55.0190 |+ 2| 73.3645 |+14 — 7.9117| —7.8962 2—3 b 55.0310 | 1| 73.3570 |-+14 — 7.9020] —7.8960 RE } с 55.0235 o| 73.3615 |+13 — 7.9080] — 7.8908 д 4 tie 2— а | 54.9975 I- 1l 73.3885 #13 — 7.9346] —7.8908 — 7.8952 7.8395 | 0.0006 0.0016 | —7.8405 | 5_3 у е 55.0035 |— 1| 73.3820 |+14 —: 7.9284| —7.8936 2—3 f | 54.9905 1| 73.3960 |+14 — 7.9418] —7.9037 3 | Scheinbare Adiff: M—Centrum = + 5.2704 Fu = 0.99300 —i° = +0.00022 | — » = —41.4094 Q— » = 14.3252 Ло = 0.99265 — = -0.00013 X = — 0.4 В— » = — 38.7108 Refr. = +- 6 4 Т— » = — 0.3199 Try = о | W— » =-- 0.884 УХ. —-+0.00019 es = PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 215 1897. April 13. il e. Decl. 4 Scalenablesung. : Ant, Le me Bemerkungen .|P.-Kr.90° #1 P.-Kr.270° t+k 3 2 zur Aufnahme, IE m un mm en mm mm gas |] бон6 [oo ions 62.8918 |-+10| 65.4900 |+16 g 0.0000 0.0000 0.0000 Bilder 3.Mond nahe. 65.9130 |+10| 62.4605 |-+-10 + 3.0256 — 0,0013 + 3.0243 66.4555 |+27| 61.9265 |+26|— 3 + 3.5638 — 0,0811 + 3.4827 38.2982 |+28| 90.0885 |— 3|-+ 4] —24.5938 — 0.0094 —24.6032 | 38. 3215 |-+40| 90.0495 |+ 8|-13| —24.5617 — 0.0694 — 24.6311 43.4920 |+22| 84.8845 |— 2]-+ 2] —19.3954 0.0000 —19.3954 93.8410 |— 3| 34.5472 |-+20]— 8] +30.9444 0.0000 -+30.9444 68.0090 |+19| 60.3830 |-+10 + 5.1134 67.6150 |+19| 60.7890 |+10 + 4.7128 67.2190 |+19| 61.1805 |-+10 + 4.3191 66.3840 |[+11| 62.0110 |+ 9 + 3.4860 65.9750 [+11] 62.4130 |+ 9 + 3.0805 | 65.5975 |+11| 62.8120 |+ 9 + 2.6922 64.7280 +17| 63.6665 |+ 8 + 1.8306 64.3330 |+ 9| 64.0555 |+ 8 + 1.4382 63.9555 |+ 9] 64.4450 |+ 8 + 1.0547 61.6750 |+10| 66.7215 |+ 8 — 1.2238 61.2810 |-+11| 67.1140 |+ 8 — 1.6170 60.9080 |-11| 67.4890 |+ 8 — 1.9910 60.0120 |+15| 68.3850 |+13 — 2.8870 59.6215 |+15| 68.7710 |+13 — 3.2752 1 59.2375 |+1| 69.1630 |+13 — 3.6634 58.2920 | 6| 70.1005 |+-16 — 4.6054 57. 9075 + р о +16 — 4927 875165 | к НЯ Trabant — Jupiterscentrum. : т | viva | Mittel. зе) Js еее | A5 | mm mm | 67.2510 [+ 8| 61.1330 [+10 + 4.3583| —0.3568 65.6195 +10] 62.7690 |+ 9 + 2.7247| —0.3615 3.9740 | 8| 64.4095 |+ 8 + 1.0816] — 0.3596 | _ A , р , LE | 60.9265 |+10| 67.4590 [+ 8 El 0,3502 0.3563 0.3539 0:0000 0:0000 | -+0.0003 0:3536 59.2680 |+10| 69.1180 |+-13 — 3.6258| —0.3506 57.5490 |+ 5| 70.8385 |+12 — 5.3457| —0.3529 68.4270 |+19| 59.9580 |+14 + 5.5342] +0.8191 DS + 9| 61.5910 [+ 9 —+ 3.9032] -+0.8170 5.1510 |-+-17| 63.2370 |+ 9 — 2.2568] -+0.8156 ВА 9 62.1040 |+1с| 66.2850 [+10 — o,7911| —+0.8195 —0.8185 | +0.8130 0.0000 0.0001 | -+0.0003 | 0,8133 60.4395 |+15| 67.9470 |+18 — 2.4545| 0.8207 | | 58-7190 +11| 69.6650 |+16 — 4.1738| 0.8190 | 66.3990 + 8 61.4885 |+11 + 4.0045| —0.7106 то 16| 63.1120 |+10 + 2.3787| —0.7075 3.6260 |+ 8| 64.7620 |+17 —= 0.7310] —0.7102 |. _, vu [a 15740 |+1о| 678080 |+19 — 23180| — 0.7074 0.7072 0.7025 0.0000 —0.0001 | -+0.0003 0,7023 58.9165 +10] 69.4720 |+14 — 3.9786| —0.7034 57-1975 |+ 9| 71.1890 |+13 — 5.6966] —0.7038 70.8615 |+15| 57.5305 |+ 8 + 7.9652] -+3.2501 69.2240 |+16| 59.1630 |+r + 6.3300] 3.2438 | 67.5770 |+2!| 60 8090 : + 4.6838] : +-3.2426 ` 4 +13 ji +3. Е | 4.5270 |+19| 63.8590 [ri + 1.6338] +3.2444 3.2442 | -#3.2225 | 0.0001 —0.0020 | 0.000; | -+3,2209 | 62.8605 |+12| 65.5240 |+13 — 0.0324| -+3.2428 И 61.1430 |+13| 67.2440 |411 — 1.7510] -+3.2418 “| Scheinbare Decldif: M—Centrum = + 3/0034 195 = 0.99323 $25 = -+0.00010 „ Иов —=+ 3.4540 Q— » = — 24.4341 fs = 0.99265 ts =— 0.00009 X ig—=— 0:3 R— » — —24.4660 У— » = — 19.2653 Г’; = 0,99329 I; = —0.00001 W—- 5 = -+30.7336 dy = 129 311 Scheinbare Adiff: *) Alle Jupitersbilder sind unterexponiert oder durch einen Bölkntederschlag grau gehn 216 84. AR Scalenablesung. Pulkowaer Sternzeit Object. Fo? со Bilde P.-Kr. 0° tt P.-Kr.180°| $ = der Aufnahmen. Mittel. от 10000 Te 10006] 10006 10000 mm zum Ctr. | 63.7823 64.6040 S 63.7815 |+ 8| 64.6024 |+16 0.0000 2 М | 68.7555 |+14| 59.6198 |+10 — 4.9789 2 N | 24.6115 |-+26| 103.7732 |+ ee — 39.1673 1 Pre: 2 Q 77.3818 |-+21| 50.9980 |+-20|— 3|-+-13.6025 1 8 4 2 R 27.0635 |+34| 101.3082 |+-13 vai —36.7084 2—8 ellipt. У | 63.4872 |-+18| 64.8868 |+23 — 0.2892 2 , W | 64.6008 |-+28| 63.7790 |-+23 —+ 0.8220 2 %ар | 63.3505 |H-10| 65.0425 |-16 — 0.4354 ас | 63.7365 |+ 9| 64.6425 |+-16 — 0.0425 — 0.0385 II 15 24 4—5 *) ау | 64.1515 |+- 9] 64.2485 |+ 8 + 0.3624 %Dy | 63.3590 |+-10| 65.0210 |+-16 — 0.4204 be | 63.7605 |+ 9| 64.6275 |+-16 — 0.0230 — 0.0278 16 25 4—5 bo | 64.1515 |+ 9] 64.2535 | 8 + 0.3599 2 Cn | 63.4030 |-+-I0| 64.9795 |+16 — 0.3777 Ce | 63.7980 | 9| 64.5909 |+16 + 0.0145 + 0.0130 17 26 4—5 Co | 64.1880 |+- 9| 64.2055 |+ 8 + 0.4022 11? 18" 11° 2 à 63.3185 |-+ 9] 65.0720 |+17 — 0.4663 а 63.7135 | 8| 64.6780 |+17 — 0.0718 — 0.0718 18 36 4—5 do | 64.1110 | 8| 64.2875 |+ 9 + 0.3226 Ze | 63.3690 | 9| 65.0370 |+-17 — 0.4236 eg | 63.7415 | 8| 64.6455 |+17 — 0.0416 — 0.0423 о 4—5 во | 64.1235 |+ 8| 64.2685 |+ 9 + 0.3383 Afro | 63.3910 |+10| 64.9990 |+17 — 0.3935 Je | 63.7680 | 9] 64.6205 |+17 0.0158 — 0.0122 Dan CES 4—5 ТТ poses Trabant — Jupiterscentrum. Tt—Ly | Mittel. Fate) Juvi-—va)| Ph: | Ду cos à mm mm | Га | 63.2250 |+10| 65.1555 |+17 — 0.5548] —0.5163 2 b | 63.2305 |+10| 65.1540 |+-16 — 0.5512 Br | 2 ; с | 63.2660 |--10| 65.1185 |+-16 — 0.5157] —0.5287 | _ 20 р в, pr 2— 4 63.1695 Le ol 65.2130 |+17 me pr 0.5333 0'5295 | +-0:0001 0:C017 0:5311 | 5 e | 63.1920 |+ 9| 65-1865 |-+17 — 0.5868| —0.5445 2 f | 63.2205 |+10| 65.1605 |+17 — 0.5595| —0.5473 2 Па | 66.2125 |+11| 62.1720 |+ 9 + 2.4312| 2.4697 ) b | 66.2255 |+11| 62.1570 |+ 9 + о 2.4725 | с | 66.2690 |+10| 62.1150 |+ 9 + 2.4879| 2.4749 зе Sa: d | 66.1790 [+10] 62.2070 [+10 + 2.3968] 2.4686 a less SDR 0.0017 | +2,4533 { : e | 66.2140 |4-11| 62.1700 |+10 + 2.4329| +2.475 2 ] f | 66.2460 |+11| 62.1405 |-+11 + 2.4636] 2.4758 ) III a | 59.0930 |-+12| 69.2900 |+14 — 4.6878| —4.6493 02 b | 59.1065 |+-11| 69.2790 |+13 — ess mu | 2 с | 59.1455 |+11| 69.2400 |+13 — 4.6365| —4.6495 | __ in | ta Là y 2 Доре | égaré tan ro ee бе ВЕ Te 5 е | 59.0845 [10] 69.3000 |+14 — 4.6971| —4.6548 2 f | 59-1145 |-=10| 69.2730 |+14 — 4.6686] —4.6564 2—3 IV a | 60.0715 |+16| 68.3090 |+19 — 3.7080| —3.6695 ) b | 60.0850 |-+15| 68.2985 |+18 — 3.6960 и | с | 60.1295 |+15| 68.2575 |+18 — 3.6533] —3.6663 | __ ve A — 3.642 4:| 60.0425 |+14| 68.3430 |+19 — 3.7396| —3.6678 3.6668 3.6410 | +-0.000$ 0.0017 3.6422 ( 2 e | 60.0745 |-+14| 68.3100 |+19 — 3.7072) —3.6649 f | 60.1050 |+14| 68.2785 |+19 — 3.6762] — 3.6640 M—Centrum = + 5:2704 Хи = 0:99299 —1°,4 = -н0.00039 N— » — —41.4094 3 ‹ Е 9— » = +14.3252 Ja = 0.99265 —y =). 00039 X 1, —— 10 R— » — — 38.7108 Refr. =- У— » = — 0.3199 Try W— » — + 0.8884 Л’ = 0.99295 Ла, = + 0.00036 ay == 10" 11. 7 Е. Renz, 1897. April 15. ee ES le Зак ЧФ A \P.-Kr. 90° К т Fern mm un. mm a 1000| 64.7990 |10000 10000 LE. 5860 |-+ 8| 64.7974 |+16] | 0.0000 66.6078 |-+ 9| 61.7688 |+10] o|+ 3.0256 67.1308 |-+25| 61.2485 |-+17|— 2] + 3.5470 Zr vn = go ` POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1597. April 15. Decl. 10 е. Scalenablesung. t+k +в P.-Kr.270° 38.9938 |+29| 89.3875 |— 38.9948 |+40| 89.3762 |+ 9 _ 44.1850 |+19| 84.1928 |— 94.5395 |— 2| 33.8498 |+-20 68.6890 |+13| 59.7195 |+14 68.3120 +18] 60.0755 |+-14 à 9350 |+18| 60.4490 |-+14 Е +13 + 2 67.9740 |+ 8| 61.4195 |+ 66.5990 [+ 8| 61.7940 | 66.2280 |+10| 62.1635 |+ + == + 65.4080 |-+16| 62.9940 65.0200 |+16| 63.3635 64.6550 |+16| 63.7350 62. 3760 |+ 9| 66.0210 |+10 62.0015 |+ 9| 66.3895 +10 в .6295 |+ 9| 66.7640 |+ 8 60.6650 |-+10| 67.7330 |+18 + +14) 68.0940 |-+18 59.9240 +14| 68.4610 |+18 а +10| 69.3610 |+13 +10) 69:7190 |-+16 à LÀ + 5| 70.0805 |+16 el w ie со Ne} oc 59.8200 |+14 61.5300 |+ 9 63.0990 |+ 9 66.1220 |-+-10 60.5575 |-+11| 67.8295 |+18 58.9400 |+-11| 69.4455 |+13 67.2010 |+ 8| 61.1830 |+11 65.4880 |+16| 62.8940 |+10 & .9190 |+ 8| 64.4640 |+ 9 РЕ тт 60.8950 |+10| 67.4900 |+ 9 Be +10] 69.2040 |+14 II +++ x 57.5600 |+ 5| 70.8260 |+13 70.3000 |+18| 58.0850 |+ 6 68.5950 |-+15| 59.7900 |+15 57.0210 +10] 61.3640 |+11 53.9965 |+10| 64.3860 |+ 9 ‚62.2820 |+11| 66.0990 [+11 ‚60.6650 |+12| 67.7180 |+19 69.7145 |-+17| 58.6730 |+10 58.coso |-+19| 60.3800 |-+14 66.4310 [+11] 61.5530 |+9 63.4080 |-+10| 64.9760 |-+16 61.6980 |+10| 66.6910 |+ 8 60.0790 |-+15| 68.3080 |+18 +++ и, Scheiubare Decldif. M—Centrum =-+ 3.0034 N— » = + 3.4539 Q— »› ——24.4341 Е— » — — 24.4661 У— » = — 19.2653 PNR 36:30:7337 dy = +12 32:4 Зап. Физ.-Мат. Отд. пен“, 3 mm + 4.7216 + 3.0101 + 1.4382 — 1.5885 — 3.2936 — 4927 | veux | Mittel. УИзбиглуь I аа) ве тт 0.2575 0.2605 —+0.2618 +-0.2666 +-0.2634 +0.2749 — 1.1066 — 1,1067 — 1.1046 — 1.1029 —1.1125 — 1.1056 —+-1.9926 —+1.9985 —+1.9964 71199095 -+1.9912 -+2.0009 —+-1.4056 —1.4087 1.4070 —+1.4103 1.4033 1.4131 тт -+0.2641 — 1.1065 -+1.9966 -+1.4080 f°5 = 0.993 12 fs = 0.99255 Ta = 0.99319 т 1/ — 5 tg0 sin тт 0.0000 0.0013 0.c811 0.0094 0.0694 0.0000 0.0000 Ki y — #06 sin 1’ mm 0.0000 + 3.0243 + 3.4659 — 24.5981 — 24.6502 —19.3963 —30.9490 Trabant — Jupiterscentrum. +0!2623 | -+0'0002 —1.0990 | —0.0011 —1.9830 | -+0.0020 —+-1.3984 | -+0.0016 1° 5 = —0.00034 5 =— 0.00052 Уз = —0.00044 217 Bemerkungen zur Aufnahme. Bilder 3. Ph. | AS 0'0000 | +0:0003 —0:2628 —0.0002 | 0.0003 — 1,1000 —0.0007 | -+0.0003 +-1,9846 —0.0004 | -+0.0003 +-1,3999 X ig=— 18 218 | Е. ВЕКА | ? =5. 1897. April 23. AC Scalenablesung. Pulkowaer Sternzeit Object. = & EA dr À Lame ЖЕ ВНЕ DR comen _ Bilder. P.-Kr. 0° tt P.-Kr. 180° |t+-% = der Aufnahmen. Mittel, mm mm mm сиг. | 66191 [10000] 637587 [0000 7 1” S 64.6175 |-+16| 63.7578 |+ 9 0.0000 2 М 69.5930 |-+17| 58.7778 2 N 25.4510 |-+26| 102.9185 1 Re: } 2 Q 78.2290 |-+21| 50.1435 12 16 44 у 1—2 | Е 27.9190 |-+34| 100:4500 2 etwas ellipt) 7 64.3312 |+17| 64.0362 1—2 W | 65.4315 |+-28| 62,9438 2 ZA | 64.2080 |+ 9| 64.1805 |+ 8 ag | 646070 |+17| 63.7825 |+ 8 — 0.0180 12. 26529 2—3 | ау | 65.0050 |+17| 63.3860 |+ 8 | %6., | 64.1855 |+ 9| 64.2145 |+ 8 | | 6; | 64.5885 |-+17| 63.8095 |+ 8 — 0.0438 27033 2—5 | 6%, | 64.9815 |+17| 63.4150 |+ 9 | ZC | 64.1855 | 9| 64.2060 |+ 8 | | Сс 64.5760 |+17| 63.8085 |+ 8 — 0.0435: 28 32 2—3 | Co 64.9845 |-+17| 63.4130 |+ 9 19 29” 6 | %а | 64.2080 |+ 8| 64.1875 |+ 9 | 1 de | 64.5950 |+16| 63.7890 |- 9 100277 29 43 «| 2 ии А, | 65.0000 |+16| 63.3890 |-+ 9 | и Ze | 64.1840 | 8| 64.1995 |+ 9 — о. | ес 64.5810 |-+16| 63.8130 |+ 9 — 0.0458 — 0.0452 BOMAT 2—3 en 64.9740 |-+16| 63.4180 |+10 + 0.3481 : 2% fo | 64.1880 |+ 9| 64.2055 |-+10 — 0.4390 Te 64.5720 |--17| 63.8240 |+10 — 0.0558 — 0.0522 31 48 . 2—5 Ir 64.9685 |4-17| 63.4325 |+11 + 0.3381 | Trabant — Jupiterscentrum. а» | Mittel. (ааа и ии») Ph. | Aa cos à I 65.9855 +11] 62.3960 |+ 9 + 1.3646 +1.3826 juge 29 | 65.9560 |+11| '62.4220 |+ 9 — 1.3369] 1.3807 | —» | 65.9595 |+10| 62.4230 |+ 9 + 1.3381| 1.3816 r Betr во р | ны Е 113486] +1.3723 +-1.3767 | 1.3671 0.0005 0.0020 | +1:3646 —2 65.9500 |+10| 62.4335 [+10 + 1.3280] -+1.3732 65.9390 |+11| 62.4435 |+11 + 1.3176| +-1.3698 П 65.5425 |+-11| 62.8390 |+ 9 — 0.9216] 0.9396 23.5055 +11 > +9 + и: Lee UE ss | 5.5450 |+10| 62.8350 |+ 9 + 0.9248|[+-0.9683 23 Th у — 8 deformiel 65.3505 |+10| 62.8345 |+10 + 0.9278] -+-0.9515 -+0.9525 | —+-0.9459 0.0004 0.0020 | -1-(,9435 65.5405 |+10| 62.8450 |+10 +- 0.9176] -+0.9628 В 65.5340 |-11| 62.8545 |+11 + 0.9096] =0.9618 ed - + 60.6370 |+12| 67.7445 |+19 60.6160 |+11| 67.7640 |+18 60.6195 |-11| 67.7600 |+18 3.9843] —3.9663 4.0946] — 3.9608 410008] 3.9573 — 3.9598 | —3.9324 | 0.0014 | —0.0020 | —3,9330 a gsaa Ta Lo SO Toegswa no I = Fee SI © со [ex LS] ND D ND ND + MLATTN D D DD = юн [Le] | | | 60.6380 |+-10| 67.7490 |-+-19 — 3,9625 —2 | 60.6220 |+10| 67.7600 |+19 3.9996] —3.9544 | 60.6125 |+10| 67.7700 |+19 4.0094] —3.9572 y —2 | IV 68.9350 |+14| 59.4460 |+10 + 4.3145] 4.3325 2 | ne —+13| 59.4725 |-+-10 —+ 4.2892] +4.3330 2 | .9130 |+13| 59.4710 |+11 + 4.2909] +-4.3344 =; | 68.9240 |+13| 39.4605 lei Le 4.3016] 44.3253 -+4.3308 | 4.3007 | —0.0014 | —0.0020 | 4,2973 . | 68.9165 |-+14| 59.4770 |+-12 + 4.2896| 4.3348 у | 68.8950 |+14| 59.4900 |+13 + 4.2724| 4.3246 > | Scheinbare Adiff: ns — + 5.2705 SE == 099314 —®. = 0.00088 — » = — 41.4095 Q— » ==-+14.3256 fx = 0.99270 — = 0.00069 X i, = — 24 R— » — — 38.7108 Refr: = + 14 V— » =— 0.3197 Try. = о) W— » = + 0.8882 J'a = 0.99305 J, = 0.00083 | т | Xy—= 10 III POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 219 1597. April 253. r e. Dec]. > A Scalenablesung. а 2 Bemerkungen 5 y PETER — = tgù sin l’ У— 408 sin 1’ ба .-Кт. 90°] #51 Р.-Кг. 270° |t+k = 3 - zur Aufnahme. = mn mm ne ue тт mm тт mm 10000 64.9226 10000] 10000 64.9210 |-+16| о 0.0000 0.0000 0.0000 Bilder 3—4. 61.8940 |-+11 0] + 3.0270 — 0.0013 + 3.0257 61.3760 |-+26|— 2] + 3.5462 — 0.0811 + 3.4651 89.5045 |— 2|-+ 5| —24.5826 — 0.0094 —24.5929 89.4988 |- 9|-+13| —24.5762 — 0.0694 —24.6456 84.3145 |— 7|-+ 2] —19.3928 0.0000 —19.3928 33.9835 |+21|-— 8|-+30.9406 0.0000 —+30.9406 59.8095 |+14 + 5.1164 60.2005 |+14 + 4.7309 + 4.7345 Bilder 3. 60.5720 |+14 + 4.3562 61.4850 |+9 + 3.4456 61.8670 |+ 9 -+ 3.0692 + 3.0643 62.2485 |+ 9 + 2.6782 63.0920 |+ 9 + 1.8409 63.4760 |+ 9]. |- 1.4563 == 1.4577 63.8540 |+ 8 + 1.0768 66.1430 |+10 — 1.2061 66.5200 |+ 8 — 1.5855 — 1.5852 66.9000 |+ 8 — 1.9640 5 67.7855 |+18 — 2.8538 68.1650 |+18 — 3.2318 — 3.2306 68.5360 +18 — 36062 69.3760 |+-13 — 4.1437 63:7445 +16 — 2 — 4.8154 Be ва m Trabant — Jupiterscentrum. : Mm Ye--Y2 | Mittel. Ira W—v2)|Ts (ааа) |Hart-222) Ph. | Ai mm тт 60.7270 |+11 + 4.19331 — 0.5412 62.3949 |+10 + 2.5310] —0.5333 LA Es à ve = Be —0.5366 | —0!5330 | —0'0007 | —o!ooor | -+0!0004 | —0'5334 68.6910 |+-14 — 3.7670| —0.5364 70.2730 |+17 5.3486] —0.5332 60.6240 |+11 + 4.3020] —0.4325 62.2870 |+10 + 2.6370 were 63.9090 |+ 9 + 1.0164| [—0.4413 x к г Kar 66.9470 |+ 9 — 2.0215| —0.4363 0.4358 0.4329 0.0005 0.0000 | -4-0.0004 0.4330 | 68.5995 |+14 — 3.6718] —0.4412 70.1830 |+17 — 5.2569] —0.4415 58.5590 |+10 — 6.3658] -+1.6313 re +16 + 4.6996 we 1.8420 |+ 9 + 3.0840] -+1.6263 = us 1 р 64.8795 |+16 + 0.0449] -+1.6301 +1.6295 | 1.6187 | -+0.0020 0.0005 | 0.0004 | -+1.6206 66.5310 |+ 8 — 1.6050] -+1.6256 68.1130 |+18 — 3.1872] -+1.6282 61.8920 |--11 + 3.0337] —1.7008 63.5580 |+10 + 1.3678 meer 65.1655 |+18 — 0.2410] —1.6987 | _ eu = рты Е 68.2055 [+20 — 3.2800] —1.6948 1.6967 1.6854 0.0022 0.0006 | -+0.0004 1.6878 69.8515 |418 — 4.9246] —1.6940 71.4360 |+-14 — 6.5108] —1.6954 Scheinbare Decldif: M— Centrum— + 3'0035 195 =0.99336 125 = —0.00038 N— » =-+ 3.4533 à = ; р Q— » = —24.4342 fs = 0.99262 is =—0.00072 X ig— —2:5 Е— » = —24.4662 У » ——19.265; fs = 0.99336 Js; = —0.00052 e . wesent завалено ноотов$ arhovmratadrasernl aan ие Ч or + < парта. ge un 443 ar LE A Bee: ФУ 174 099 =. Dates Be 6 2 A BAER SEA He + ER ET) НЕ FE Ad et | eh С => 1 вел: (rer lou? Tr и: = ) DC ù 4 | у 1 а | у 1% D | ln zogen mr Er пы лан ul PORC! - ц | : на mit N D мое. "x x EC . ‘4 US = | FL £ À г. 7 y à x | = u 18000 = Е \ О Е: = PS} и DEZ Lgnnisikeri - été Lermerier sinne oil dois Мула an Be Lois aval тж TT be ax 77m м Ще a вом кезтТ MO зо nager Bier 2! Е Вали ie 09604 2 4 Май чай. в: Bahn“ wis oradisti mor din banıdım Aublid mpımadız anb intel ot A unais voter Object. —+ -ч р Зоо a8 So зос8 III <> Г) Lun! а ATI To as P.-Kr. 0° mm 65.8075 65.8065 44.7078 95.5875 mm 62,5700 62.5691 83.6690 32.7880 mm 10000 ГО 87.0198 41.3555 89.0198 39.3528 61.7820 |+10| 66.6110 62.2200 |-+10| 66.1840 62.6525 |+10| 65.7340 61.7610 |+10| 66.6345 62.1940 |[--10| 66.2100 62.6275 |+10| 65.7605 61.7685 |+10) 66.6170 62.2115 |+10| 66.1860 62.6505 |+10| 65.7435 61.7480 |+ 9| 66.6425 62.1935 | 9| 66.2060 62.6275 |+ 9| 65.7685 61.7720 | 9| 66.6165 62.2225 |+ 9| 66.1900 62.6600 |+ 9| 65.7310 61.7695 |-+10| 66.6200 62.2175 |+10| 66.1845 62.6535 |+-10| 65.7340 60.7420 |+12| 67.6405 60.7235 |+I1| 67.6625 60.7505 |11| 67.6315 60.7220 |+10| 67.6605 60.7610 |+10| 67.6250 60.7615 |11| 67.6240 63.6655 |-+ 9| 64.7190 63.6315 |+ 9| 64.7475 63.6525 |+ 9| 64.7280 63.6070 |+ 8| 64.7710 63.6360 |+ 8| 64.7420 63.6340 |+ 9| 64.7500 63.6930 | 9| 64.6840 63.6650 |+ 9| 64.7165 63.6800 |+ 9| 64.6975 63.6430 | 8| 64.7360 63.6715 |+ 8| 64.7105 63.6650 | 9| 64.7125 57.2410 |+11| 71.1405 57.2190 |+Iı| 71.1625 57.2400 |+10| 71.1415 57.2150 |+ 9| 71.1690 57-2490 | 9| 71.1315 57.2460 |+ 9| 71.1355 Scheinbare Adiff: Trabant II und III berühren sich und es zeigt sich die schon einmal bemerkte Erscheinung, dass der kleinere gleicham durch grösseren verschoben wird, wodurch er ein verzerrtes Aussehen erhält. Beide Trabanten sind durch eine weisse Lücke von einal Scalenablesung. ны P.-Kr.180° Е. Renz, 1298. März 16. der Aufnahmen. Mittel. mm h т О 12 19 30 — 0.3604 12 11 248 — 0.3850 320 +10 — 0.3685 — 0.3673 AO +1C + 0.0722 12% 5" 44 +11 — 0.8286 HI] — 0.3876 — 0.3893 6 so +11 + 0.0482 +11 — 0.8036 +11 — 0.3651 — 0.3618 8 10 +11 + 0.0832 +12 — 0,8066 +12 — и — 0.3643 9 28 Ч | Trabant — Jupiterscentrum. een | Mittel. fete) Te (evo) РЬ. | Au cos à mm mm x +19 — 1.8308| —1.4704 +18 — 1,8511] —1.4661 +18 — 1.8221] —1.4548 | Ba , р Ber Br = sel — 1.4617 1.4589 1:4490 | +-0:0010 | -+0.0001 1:4479 +19 y IGN) +19 — 1.8129] —1.4486 +16 + 1.0916] -+1.4520 —=16 + 1.0604] 1.4454 —16 + 1.0806] 1.4479 sé, > Er os] 41.4256 +1.4371| -+1.4273 00009 | -+0.0001 | +1,1265 Ze —+ 1.0653] 1.4271 +18 + 1.0603] +1.4246 +16 + 1.1229] +1.4833 +16 —= 1.0926 ue +16 —= 1.1096| +-1.4769 e Me + 1.0718] +1.4611 —+-1.4697 | +1.4597 0.0007 | -+0.0001 | 1,4591 +17 + 1.0988| +1.4606 +18 + 1.0946] -1.4589 +13 — 5.3306| —4.9702 +13 — 5.3532 ne +12 — 5.3321] —4.9048| __ er er A — 5,3584] —4.9691 4.9658 4.9319 | —-0.0034 | -+0.0001 4,9284 +13 — 5.3227| —4.9609 +13 — 5.3262] —4.9619 I— Centrum = -+23'4017 Fu = 0.99318 —iy = +0.00177 — » — —33.0465 K— » = +-27.2018 fa = 0.99290 —ig, —0.00177 X y = — L— » =+202335 Refr. =—— 5 А m ay=12 26.6 f'a = 0.99318 Pulkowaer Sternzeit Try O у + 0.00172 getrennt, welche einen Kreisabschnitt des grösseren bildet, während sie vom kleineren ein Segment abschneidet. Bilder] 2—3 3 etwas ellipts M 2—3 2—3 PA DD © | C9 C9 © 61 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 223 139=. März 16. ГГ е. Decl. Scalenablesung. %ин% с м. VE Lu Bemerkungen : one er DE u: у — a — = = #95 sin 1’ 2 > tgè sin 1’ zur Aufnahme. mm mm mm 63.8897 10000 645 Г 68 10000] 10000 nm mm mm mm 63.8888 |+ 9| 64.5160 |+ 8], о 0.0000 0.0000 0.0000 Bilder 3—4. 64.2445 |+17| 64.1668 |-+14| o|+ 0.3526 — 0.0317 + 0.3209 73.2798 |+25| 55.1170 |-+15|— 3]+ 9.3952 — 0.0635 + 9.3317 79.2015 |+17| 49.2072 |-++21|— 3|-+15.3102 — 0,0432 —+-15.2670 48.0372 |#+31| 80.3722 |+17|+ 4| — 15.8528 — 0.0491 — 15.9019 69.0715 |-+14| 59.3558 |+14 + 5.1714 68.6610 |+14| 59.7670 |-+14 —= 4.7606 + 4.7591 Bilder 3. 68.2395 |+19| 60.1762 |+14 + 4.3454 67.5245 |+ 9| 60.3958 |+-10 + 3.6278 67.1210 |#+ 9| 61.3176 |+10 = 3.2152 + 3.2159 66.7050 |+ 9| 61.7224 |+ 9 + 2.8048 65.9370 |+11| 62.4815 |+ 9 + 2.0414 63260 +11| 62.9038 |+ 9 + 1.6248 + 1.6258 65.1060 |-+17| 63.3116 |+ 9 + 1.6112 62.8200 |10| 65.5997 |+10 — 1.0763 62.4185 |-+10| 66.0210 |+10 — 1.4877 — 1.4895 61.9935 |-+10| 66.4294 |+10 — 1.9044 61.2410 |-+11| 67.1768 |+ 8 — 2.6542 60.8335 |+11| 67.5902 |+18 — 3.0652 — 3.0654 60.4200 |-+11| 68.0000 |-+18 — 3.4768 59.6465 |+-15| 68.7720 |+-13 — 4.2491 2280 —1!| 69.1914 |+13 — 4.6682 — 4.6644 Г 69.602 — 5. Ее + ER Mo. 5.0759 Trabant — Jupiterscentrum. : и à Ve | Mittel. Узи у) | dater) ео) Ph. | As mm mm 59.1523 |-+10 + 5.3671| -+0.6080 60.6964 |+10 + 3.8228] -+0.6069 62.2936 5 .5986 ‚ р р р 1= 65.4028 а т: 0.8856 Be +0.5989 | +o!so54 | 0,0024 0!0000 0!0000 | -+0!5978 66.9930 |+ 8 — 2.4728| -+0.5926 68.5892 |+13 — 4.0810) -+0.5834 60.2676 |--IO + 4.2502] —0.5089 61.8071 |+ 9 + 2.7142| —0.5017 3 63.3973 |+ 9 + 1.1240] —0.5018 | _ Br = Lx 66.5070 |+-10 — 1.9855| —0.4960 0.4989 0.4960 0.0024 0.0000 0.0000 0.4984 68.0836 |-+18 — 3.5607| —0.4953 5.1540] —0.4896 4.3443| —0.4148 2.8036| —0.4123 —0.4104 | _ br er 3 Fr 1.8934| —0.4039 0.4097 0.4073 0.0025 0.0000 0.0C00 0.4098 3.4729] —-0.4075 5.0738| —0.4094 6.7176] +1.9585 5-1734| +1.9575 69.6764 |-+16 60.1734 |-+14 61.7154 |+ 9 63.3081 |+ 9 66.4148 |+10 67.9915 |+18 69.5972 |-+16 57.8016 |+ 7 59.3467 |+12 cd +++ 60.9406 |-+12 —+1.9524 , 10 64.0546 [+10 0.4653| +1.9548 —+1.9534 | -+1.9420 | -+0.0083 +-0,0001 0.0000 | -+1,9504 65.6362 |+12 1.1176] -+1.9478 67.2334 |+10 2.7150] -+1.9494 Scheinbare Decldiff: I—Centrum =-+ 0,2848 195 = 0.993 36 195 = —0.00162 F— » = + 9.3177 К > = +-15.1243 fs = 0.99296 is = —0.00162 xi=—5'6 L— » = —15.8407 f's = 0.99416 Уз = —0.00167 294 Е. Веки, 57. 1898. März 25. № & Scalenablesung. Pulkowaer Sternzeit | | Object. Зое Bilde г, | P.-Kr. 0° ++ Р.-Кт.180° ++ 3 der Aufnahmen. Mittel. LI mm ит mm um mm mm 1 | Ctr, | 63.6190 [10000] 647601 [10000 1000 | I 63.6182 |+ 8| 64.7585 |+-16 0.0000 9 ni J 84.7252 |— 2| 43.6550 |+19]— 5 —+21.1044 7. 2 ит O 16.4765 |+-28| 111.8740 |+ 6[+32] —47.1239 13° 28 } 1—2 | K 88.0652 |— 1| 40.2665 |+31|— 5 +-24.4678 1—2 Ru | L 90.0920 |— 1| 38.3342 |-=29]— 6] -+26.4474 о | % an | 63.1880 |+10| 65.1870 |+-17 — 0.4243 { | ас 63.6130 |+ 9| 64.7680 |+17 — 0.0074 — 0.0049 T3 TA MMS 2 № а, | 64.0325 |+ 9] 64.3390 |+17 -+ 0.4169 в | %6 | 63.1860 |+10| 65.1995 |+16 — 0.4365 | | 6; | 63.6120 | 9| 64.7765 |+16 — 0.0120 — 0.0131 16 10 1—2 NL bd, 64.0280 |+ 9| 64.3500 |+16 + 0.4092 || %е | 63.1900 [+10] 65.1990 |+16 — 0.4342 | | | Ce 63.6070 |+ 9| 64.7880 |+16 — 0.0203 — 0.0174 ©) 1—2 on €) 64.0260 |+ 9| 64.3615 |+-16 + 0.4024 43° 17" 43° М %а | 63-1980 |-- 9| 65.1970 |+17 — 0.4294 | de | 63.6180 |+ 8| 64.7820 |+17 — 0.0119 — 0,0112 18.923 2 { do | 64.0320 |+ 8| 64.3570 |+17 — 0.4076 | %е | 63.2165 |+ 9| 65.1910 |+17 — 0.4171 | ес 63.6280 |-- 8| 64.7815 |+17 — 0.0066 — 0.0012 10022 2 | en 64.0515 | 8| 64.3515 |+17 —+ 0.4201 | %7 | 63.1985 |-+-10| 65.2000 |-+18 — 0.4306 Fe 63.6320 |+ 9| 64.7820 |-+-18 — 0.0049 — 0.0053 DOI © Jr 64.0525 |+ 9| 64.3535 |-+18 0.4196 | Trabant — Jupiterscentrum. 4—2 | Mittel. |1’ (1—2) „из Р ь | Да cos à mm mm I Bedeckt. | Па | 62.9745 |+11| 65.3920 |+-17 — 0.6384] —0.63 3 5 1—2 №: b | 62.9765 |+10| 65.3945 |+16 — 0.6388] —0.6257 2 ' | с | 62.9875 |+10| 65.3900 |+16|- — 0.6310] —0.6136| _ ‚ , р pr 2 It a | 62.9895 [+ ol 65.3975 |+17 — 0.6338| —0.6226 0.6203 | —0!6160 | -но:000т 0.0000 0:6159 9 e | 63.0080 |+ 9] 65.3810 |+17 — 0.6164] —0.6152 2 и f | 63.0105 |--109] 65.3835 |-18 — 0.6164| —0.6111 2 | | Па | 58.6750 |+13| 69.6830 |+17 — 4.9336] —4.9287 | | b ee +12 69.6935 Hi — 4.9424 298 | е 39-0735 | HI1| 09.0925 ET — 4.9392] —4.9219 | __ 2 RN | d | 58.6745 |+10| 69.7010 |+16 — 4.9430] —4.9318 4.9289 4.8950 | -+0.0028 0.0000 4,8922 2 | e | 58.6880 |+10| 69.6935 |+17 — 4.9326] —4.9314 и Л | 58.6875 10] 69.6990 |+17 — 4.9356] —4.9303 ) | IV а | 66.1735 |+-ı1) 62.1960 |+ 9 + 2.5594] 2.5643 № 6 | 66.1650 |+11| 62.2155 |+ 9 + 2.5454] -+2.5585 | с 66.1695 |+-11| 62.2140 |+ 9 + 2.5484] -+2.5658 { | Я | 66.1680 |+10| 62.2215 |-+10 + 2.5438] -+2.5550 2.5578 | -+2.5402 | —0.0009 9.0000 | +-2,5393 2 il e 66.1775 |+10| 62.2175 |+10 — 2.5506] -+2.5518 Г f | 66.1755 |-+11| 62.2240 |+I1 + 2.5462] +-2.5515 | Scheinbare Adiff: I—Centrum = +23:4021 090 — = 0.00107 0— » = — 52.3146 K— » =+27.2023 fa = 0.99282 — = 0.00106 X x = — 3.6 L— » = -+29.2340 Вей’. = + 13 Tir — р O uy =12" 224 fly = 0.99312 I, =-0.00119 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 225 1395. März 25. 188 e. “ Decl. à Scalenablesung. € ‘ En+ots en Sr a ER? Bemerkungen P.-Kr. 90° t-il P.-Kr. 270° |t-+ 3 N > Tara aa. in ai Bras Po GG [oo m т” til "я 63.8715 |+ 8| 64.5108 |+ 8] о 0.0000 0.0000 0.0000 Bilder 2—8. 64.2425 |-+18| 64.1388 |+15] ©] -+ 0.3716 — 0.0317 -+ 0.3399 73.7510 |-+29| 54.6270 |+16— 7|-+ 9.8816 — 0.1595 + 9.7221 79.1958 |+-18| 49.1798 |+22|— 4] 15.3270 — 0.0432 15.2838 48.0350 |+-32| 80.3452 |418 4| —15.8344 — 0.0491 — 15.8835 ‚69.0290 |-+13| 59.3640 |+14 + 5.1521 68.6320 |-+13| 59.7700 |-+14 + 4.7506 + 4.7513 68.2320 |-+18| 60.1695 |+14 + 4.3511 67.4400 |+ 8| 60.9540 |-10 + 3.5626 67.0445 |+ 8| 61.3580 |+10 + 3.1628 + 3.1646 66.6485 |+ 8| 61.7510 |+9 + 2.7684 65.8160 |+-10| 62.5830 |+9 + 1.9362 65.4190 |-+16| 62.9820 |+ 9 + 1.5385 + 1,5411 65.0250 |-+16| 63.3680 |+ 9 + 1.1485 62.7320 |+ 9| 65.6650 |+-10 — 1.1469 62.3430 |+ 9| 66.0585 |+10 — 1.5382 — 1.5363 61.9570 |+ 9| 66.4440 |+10 — 1.9239 61.1325 |-+10| 67.2625 |+ 8 — 2.7452 60.7380 |+10| 67.6695 |-+-18 — 3.1365 — 3.1406 60.3400 |+10| 68.0590 [+18 — 3.5402 59.5040 |+10| 68.9010 |+13 — 4.3790 59.1030 [+10] 69.3010 |-+13 — 4.7795 — 4.7782 58.7025 |+10| 69.6940 |+13 — 5.1762 Trabant — Jupiterscentrum. ve | Mitte. Mat) Табе erg] Pa | & mm mm Bedeckt. _ 68.7245 -=14| 59.6605 |+14 + 4.8516] -+0.1003 51.1350 + 9| 61.2520 |-10 + 3.2611| -+0.0965 .50 62.876 1.6366 . `, р р ‚ р Br: Sch a go 14298 ее 0.0937 | +0!0932 | +0/0015 0'0000 0!0000 | +0'0947 .8185 |+11| 67.5660 |-+18 — 3.0544] -+0.0862 59.1855 |+11| 69.2005 |+13 — 4.6880] -+0.0902 0.9995 |-+14| 57.3810 |+10 + 7.1291| -2.3778 24135 +15 ne +11 + 5.5411| -2.3765 67. 2 0.5930 11 8 г Die wer 63.0680 er 9 и Be en —+2.3770 | -+2.3631 | —+-0.0118 0.0000 0.0000 | -+2,3749 63.1040 |+11| 65.2775 |+17 — 0.7674| -+2.3732 ‘61.4705 |-+12| 66.9120 |+ 9 — 2.4010] -+2.3772 ‚67.8400 |+18| 60.5440 |-+11 + 3.9680] —0.7833 D +10) 62.1325 |+10 + 2.3814| —0.7832 64.6350 |+16| 63.7520 |+ 9 +- 0.7610| —0.7801 61.5595 |+- ol 66.8295 |+9 — 23154| —0,7791 —0.7815 | —0.7768 | —0.0061 0.0000 0.0000 | —0,7829 59.9490 |-+14| 68.4380 |+19 — 3.9251] —0.7845 58.3150 |+ $| 70.0670 |+17 — 5.5570] —0.7788 Scheinbare Decldiff: 1—Centrum = + 0.2848 198 = 0.99336 1° 5 = —0.00246 0— » = + 9.7699 Е » —+165.1245 fs =0.99294 is = —0.00252 xiu=—8l L— » = — 15.8406 ы f's = 0.99415 Js = —0.00239 dy = —0° 40.6 Зап. Физ.-Мат. Отд. 29 | | К" = 226 Е. Renz, ==, 1292. März 26. № IE Scalenablesung. Pulkowaer Sternzeit P.-Kr. 0° t+-H|P.-Kr.180° 3) 3 en Mittel, 63,6670 64,7116 Ш | 63.6662 64.7100 |-+16| о 0.0000 84.7735 43.6082 |-+19|— 2] -+21.1037 1—2 16.5298 101.8498 —47.1334 2 ellipt. 88.1122 40.2650 +-24.4438 2 90.1362 38.2458 26.4654 1 63.2445 65.1535 0.4326 63.6740 64.7305 0.0064 — 0.0064 9-3 64.0990 64.3040 0.4198 63.2590 65.1360 0.4165 63.6840 64.7095 0.0092 —= 0.0101 64.1165 64.2860 0.4376 63.2595 65.1360 0.4162 63.6860 64.7090 0.0104 — 0.0055 64.1005 64.3005 0.4224 11^ 47" 58° 63.2610 65.1340 0.4146 63.6810 64.7190 0.0028 — 0.0058 64.1080 64.2940 0.4292 63.2805 65.1125 0.3941 63.7055 64.7065 0.0214 — 0.0229 64.1185 64.2800 0,4415 63.2770 65.1190 0.3991 63.7040 64.7010 0.0234 -+ 0.0207 64.1240 64.2930 0.4378 Г мм CCE = See ee > re En en menge ig ee me - \O DO O соо сс \0 ЕЕ ЕЕ ЕЕ EEE SE = Trabant — Jupiterscentrum. ac» | Mittel. Лао) Лии) Ph. | Аа cos à mm mm Geht durch [die Jupiter|schelibe. pl u! | © Hs a Oo LRO SR 9 RE SA 3.1122 -=3.1099 -=3.1125 3.1149 —3.1136 —-3.1195 —4.1172 —4.1193 — 4.1161 —4.1104 — 4.1119 4.1047 66.7760 61.6090 66.7900 61.5945 66.7880 61.5965 66.7895 61.5925 66.8055 61.5770 66.8095 61.5735 59.5450 68.8370 59.5580 68.8210 59.5565 68.8225 59.5635 68.8175 59.5790 68.8015 59.5835 68.7960 L -+3.1138 | -+3/0926 | —0:0035 0:0000 | +3.0891 ЕЕ | lem! ut Lou | = ee. 2e I = —4.1133 | —4.0852 | +0.C041 0.c000 | —4.0811 [al Do» DIESES | -DDDDD аннююю ND HN HN N IV 63.1210 65.2620 — —0.5421 —3 k 63.1315 65.2560 — —0.5503 ll: 63.1250 65.2640 — — 0.5530 | _ N A BE №: 63.1250 [+9] 65.2595 M _oss12| — 9.5514 0.5476 | <-0.0016 0.0000 | —0,5460 ь 63.1370 |+ 9| 65.2480 — —0.5565 k 63.1355 |-+ 9| 65.2480 — —0.5551 = у Scheinbare Adiff: 1—Centrum == 23.4021 To 09998 —1°,, = +0C.00242 % 0— » = — 52.3146 | К— » =+27.2024 fu = 0.99289 — = 0.00242 хи = —8'3 L— » = -+29.2341 Вей’. = — 8 pe B Ни | h O ay= 12" 21.9 Л’, = 099318 Te +0.00234 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1298, März 26. Decl. LL e. - Scalenablesung. 5 y ?.-Kr. 90° НР. -Kr. 270° |+ ss 10000 61.4450 10006] 10006 10000 Le 63.9360 | 8| 64.4442 о 0.0000 64.3075 |+18| 64.0740 He ol + 0.3710 .8195 |-+29| 54.5565 |-+16|- 4|-= 9.8856 2602 |-+18| 49.1140 |+-22|— 4| +15.3266 .0970 |-+32| 80.2800 |-+18|— 7] —15.8363 69.1210 |-+13| 59.2770 |+-10 + 5.1762 .7190 |-+13| 59.6830 |-14 —+ 4.7720 68.3090 |+18| 60.0910 |+14 + 4.3633 67.5160 |+ 8| 60.8760 |-+-10 + 3.5740 67.1160 |-+- 8| 61.2840 Se —= 3.1700 66.7145 |+ 8] 61.6840 + 2.7793 65.9420 |+-10| 62.4550 + 1.9976 65.5375 |+10| 62.8575 + 1.5942 65.1460 |-+16| 63.2495 + 1.2027 62.8050 |+ 9| 65.5925 |+10 — 1.1397 62.4055 | 9| 66.0005 |+10 — 1.5434 .0070 I+ 9| 66.3920 |+10 — 1.9384 61.2400 |+10| 67.1600 — 2.7058 60.8460 |+10| 67.5500 se — 3.0983 60.4530 |-+10| 67.9440 |+18 — 3.4918 69.6755 |+14| 68.7190 |+13 — 4.2676 59.2755 |-+10| 69.1190 |-+13 — 4.6678 58.8890 -++-10| 69.5105 |-+13 — 5.0568 Geht dulrch | die Jupiter|schelibe. 1 67 7.2115 |-+ 8| 61.1750 |-+11 -+ 3.2722 5.6135 |-+10| 62.7720 |-+-10 + 1.6748 6. 0345 |+ 8| 64.3510 |+9 + 0.0958 60.8960 |+10| 67.4865 |+ 9 — 3.0411 59.3395 |+10 69.0460 |+14 — 4.5994 7770 | $| 70.6070 |-+13 — 6.1613 70.4775 |+18| 57.9070 |+ 6 + 6.5400 68.8770 |-+15| 59.5055 |+11 + 4.9400 67.2970 |-+10] 61.0899 |+11 + 3.3580 64.1625 |+10| 64.2190 |+ 9 + 0.2259 62.6030 |+т1| 65.7800 |+11 — 1.3344 79375 +12] 67.3445 |+ 9 — 2.8992 69.3900 |-+14| 58.9940 |+10 + 5.4523 67.7910 |+19 60.5935 |+-10 + 3.8533 66.2210 |+11| 62.1675 |+ + 2.2810 63.0865 |-+10] 65.2960 |+16 — 0.8510 61.5310 |-+11 66.8595 |+ 8 — 2.4100 59.9695 +15| 68.4170 |+18 — 3.9698 Scheinbare Decldif: 1—Centrum = + 0/2848 O— » = + 9.7699 K— » = -+15.1245 L— » = —15.8406 тн е+н%: тт + 4.7705 + 3.1744 + 1.5982 — 1.5405 — 3.0986 — 4.6641 Yt—Y2Z | Mittel. тт тт —1.4983 — 1.4996 — 1.5024 5006 | —14998 —1.5008 — 1.4972 1.7695 —1.7656 —+1.7598 +-1.7664 —+1.7642 —=1.7649 —+-0.6818 —0.6789 —+0.6828 —+0.6895 —+0.6886 +-0.6943 1.7651 0.6860 125 = 0.99332 fs = 0.99292 [’з = 0.99410 2 — = 106 sin 1’ тт 0.0000 0.0317 0.1595 0.0432 0.0491 Kr) 0.0000 Bilder 2. Trabant — Jupiterscentrum. Fu -Y2) | Js(tr—22) На 225) т | Ph. —1:4909 | —0!0077 +1.7546 | -+0.0102 +-0.6820 | 0.0014 125 — —0.00241 is = —0.00239 Js = —0.00247 0:0000 0:0000 0.0000 0.0000 0.0000 0.0000 X в=—8!2 > Bemerkungen zur Aufnahme. A8 —1:4986 —+1,7648 —+0.,6834 — 228 =9. Scalenablesung. Object. P.-Kr. 0° ыы P.-Kr.180° me 10000 = Ctr, | 64.5228 63.8529 a 64.5220 |+ 8| 63.8520 J 85.6302 |— 3| 42.7488 O 17.3802 |-+28| 110.9922 K 88.9740 |— 2| 39.3960 L | 90.9842 | © 37.3945 %а, | 64.1130 |+ 9| 64.2825 Ag 64.5520 |+17| 63.8340 a | 64.9960 |+17| 63.3910 2% ban | 64.1655 |+17| 64.2360 De 64.5965 |+17| 63.8020 b, 65.0150 |+-17| 63.3790 %Cyw | 64.1585 |+ 9| 64.2435 Ce 64.5840 |-+17| 63.8170 es 65.0030 |+17| 63.3905 2% dy | 64.1700 |+ 8| 64.2245 de | 64.5935 |+16| 63.8035 do | 65.0095 |-+16| 63.3860 Zen | 64.1690 | 8| 64.2250 ес 64.5930 |+16| 63.8050 es | 65.0140 |+16| 63.3805 %1 | 64.1815 |+ 9| 64.2130 Fe 64.6165 |+-17| 63.7930 A 65.0310 |+17| 63.3665 Та | 65.5575 |+11| 62.8255 b | 65.5990 |+11| 62.7900 с 65.5895 |-11| 62.7950 а | 65.6050 |+10| 62.7785 е | 65.6110 |+10| 62.7750 f | 65.6290 |-+11| 62.7515 Па | 64.0935 | 9] 64.2860 b 64.1235 |+ 9| 64.2595 с 64.1090 |+ 9| 64.2745 а | 64.1140 |+ 8| 64.2660 е 64.1075 |+ 8| 64.2710 f | 64.1235 |-+ 9] 64.2540 III Bedeckt. |IVa | 60.6800 |+-12 67.7030 b | 60.7100 |+11| 67.6715 с | 60.6975 |+-I1| 67.6850 d | 60.7070 |+10| 67.6720 e 60.7030 |-+-10| 67.6770 f | 60.7210 |-+10| 67.6635 Scheinbare Вай: Г. Renz, 1298, März 27. Æ 1 ; Pulkowaer Sternzeit к 8 Kae Е, Bilder. | t+k au der Aufnahmen. Mittel. м mm | тт ji 10000] 10000! 2" ve | + 9] о 0.0000 2 +21|— 2] 21.1044 ное. 2 * + 6]-+32| —47.1366 12° Mm” 3 2 etwas ellipt, -+30|— 5] -+24.4520 2 2 +28|— 6| +-26.4579 2 Ro’: ES — 0.4196 } + 8 + 0.0245 + 0.0243 12 Bas 2—3 4 +8 + 0.4680 A = — 0.3698 | + 8 + 0.0628 + 0.0588 SU "9 2—3 | 8 + 0.4835 | 8 — 0.3774 у + 8 + 0.0490 + 0.0478 340006 2 | + 8 + 0.4718 12% 34” 38 | + 9 — 0.3622 | + 9 + 0.0604 — 0.0585 35 10 2 р + 9 + 0.4772 ! +9 — 0.3630 { + 9 + 0.0594 + 0.0595 2602 2 + 9 — 0.4822 À +10 — 0.3508 | +10 — 0.0772 + 0.0747 37 23 { +10 + 0.4976 | Trabant — Jupiterscentrum. | Tt—Ly | Mittel. Рае Jatur—va)| Ph, | Ac cos 6 ) mm mm + 9 + 1.0312] -+1.0069 3 | + 9 —= 1.0696| +1.0108 2—3 1 + 9 + 1.0624| +1.0146 , Der р вор 2 A + 1.0783] +1.0198 —+1.0174 | +1/0103 O'O0II 0'0000 | +-1:0092 9 — то —= 1.0830| -+1.0235 2 Я +11 + 1.1038] <+-1.0291 2—3 etwasel + 9 — 0.4312| —0.4555 2—3 | + 8 — 0.4029] —0.4617 2—3 Pa) + 8 — 0.4176] —0.4754 | _ Ru № 2 | о — 0.4110] — 0.4695 0.4689 0.4656 | —-0,0008 0.0000 | — 0.4648 | 5 | + 9 — 0.4168| —0.4763 À 2 и +10 — 0.4002| —0.4749 2 etwas ellipt | a 1 +19 — 3.8468] —3.8711 3 +18 — 3.8160] —3.8748 3 +-18 — 3.82909] —3.8768 | _ ar an 2—3 3 +18 — 3.8178| —3.8763 3.8770 3.8501 | -+0.0042 0.0000 | —8.8459 | о 19 — 3.8223] —3.8818 2 | +19 — 3.8066| —3.8813 2 etwas ellipt 1— Centrum= +-23/4021 ΰ y = 0.99304 —i° , —+-0.00192 | — » = —52.3146 К— » =-+27.2024 fa = 0.99276 —iy = 0.00192 x = — 6.6 | L— » = -+29.2341 Refr. = + 3 | „m Try — [e) 2 &y — 12 21.4 Го —=0.99304 Ло —+0.00195 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 229 1595. März 27. ihe. Decl. к bl R ’ L Poslena esung 9 CPR TELT 2; ne m 2 оу Bemerkungen р. Kr. 90° = Р.-Кг. 270° |t-+k - ы 1 zur ‚Anfuahme. ‘a Pr mm = тт тт тт. 64,5261 | 63. 64.8245 Г 0.0000 0.0000 Bilder 3. | 63. 64.4670 + 0.3596 — 0.0317 + 0.3279 3 . 54.9145 + 9.9099 = 2955 — 9.7504 78.86 49.5060 +15. — 0.0432 +15.2739 80.6745 —15.8480 — 0.0491 —15.8971 59.6100 + 5.2246 60.0255 + 4.8058 —+ 4.8056 60.4470 —= 4.3864 61.2460 = 61.6650 — + 3.1760 62.0680 + 62.8205 1 63.2270 + + 1.6126 63.6260 + 65.9780 — 66.3760 = — 1.5379 6: 1.6280 66.7735 60.8560 67.5410 — 60.4620 67.9410 — — 3.1041 60.0560 68.3410 —- 9.2910 69.1040 5 E25 69.5160 — — 4.6714 69.9050 = Trabant — Jupiterscentrum. и УЗ A | не. Lam a [ее] №. | № Mittel. Maya) Jo еее) Ph | № 60.5940 +- 4.2370 —0.5686 62.2190 —+ 2.6109] —0.5651 63.7870 + 1.0435] — 0.5691 | _ 2 Er ns 66.9345 Bl 0.5081 0.5687 0.5653 0.0020 0:0000 0.0000 0:5673 68.5055 — 3.6768] — 0.5727 70.0695 — 5.2402| —0.5688 59.6070 + 5.2211] -+0.4155 61.2300 —= 3.5998| +0. ve ch a on к 4280 +0.4252 | +o. 4ER +-0.0009 0.0000 0.0000 | -+0.4236 67.5045 — 2.6760] -+0.4281 69.0675 — 4.2382] -+0.4332 57.8325 —+ 7.0003] -+2.1947 39-4525 + 5.3796 +2. wer 1.0190 + 3.8111] -+2.1985 р ers + 0.6680| -+2.2059 +-2.2027 | -+2.1895 +-0.0072 0.0000 0.0000 | -+2,1967 65.7270 — 0.8984] -—2.2057 67.2930 |+ 8 — 2.4637| —2.2077 | Scheinbare Decldiff: 1—Centrum = + 0'2848 f°5 =0-99329 175 = —0.00188 0— » =-+ 9.7699 \ L К = -+15.1245 fs =0.99288 is =— 0.00190 X в =—65 (4 L— » = — 15.8406 Ру = 0.99404 Is =— 0.00187 230 Е. Renz, 90. 1898. April 11. ER 18 \ Scalenablesung. Pulkowaer Sternzeit ; Object 5 YZ Dan Pac Зав. б.р Bilder, | P.-Kr. 0° tt P.-Kr. 1809 ++ . der Aufnahmen. Mittel. | mm er mm u mm mm | | сиг. | 63.5594 [10000 65,1429 [10000 10000 | J 63.2585 |+ 9] 65.1112 |+17 0.0000 2 | | 7 84.3768 |— 7| 44.0048 |+19|— taste 5 Dent. I 200 u 0 16.1138 |+28| 112.2602 |+ 6]-+32| —47.1432 11 34 1—2 ellipt.« K 87.7195 |— 1| 40.6522 |+30|— мы: 1—2 | L 89.7320 |— 1| 38.6468 |+30|— 6] +26.4672 i 2 2% &yw | 63.2190 [+10] 65.1670 |+16 — 0.0476 ! Ge | 63.6475 |+ 9| 64.7465 [+16 + 0.3769 + 0.3758 IT 10089 2 | Go | 64.0720 | 9] 64.3295 |+ 8 + 0.7980 %byn | 63.2260 |+-10| 65.1645 |+16 — 0.0428 N be 63.6565 |+ 9| 64.7375 |+16 + 0.3859 —+ 0.3840 20 26 1—2 b, 64.0840 |-+ 9| 64.3200 |- 8 — 0.8088 %сь | 63.2310 |+10| 65.1645 |+16 — 0.0403 ce 63.6470 |+ 9| 64.7465 |+16 + 0.3766 + 0.3818 211° 1828 2 | во 64.0790 |+ 9| 64.3145 |- 8 —+ 0.8090 11° 29" 43 | 2 dy | 63.2225 |+ 9] 65.1695 |+17 — 0.0472 : {| de | 63.6495 |+ 8| 64.7445 |+17 —+ 0.3788 + 0.3795 221,350 2 Höcker am do | 64.0800 |+ 8| 64.3195 |+ 9 + 0.8070 pi | Zen | 63.2185 |+ 9] 65.1780 |+17 — 0.0534 ес 63.6410 |+ 8| 64.7640 |+17 — 0.3648 + 0.3656 С.В 2 ео 64.0550 |+ 8| 64.3375 |+ 9 + 0.7854 %] | 63.2125 |+10| 65.1825 |+-18 — 0.0586 м 63.6480 |+ 9] 64.7585 |-+18 + 0.3710 + 0.3700 PS) 2 | Fe | 64.0690 | 9| 64.3270 |+-10 — 0.7977 Trabant — Jupiterscentrum. 2% — Ty | Mittel. [Рая Лат Ph. | Ac cos 6 mm mm I Geht durch |die Jupiter/sche|i Па | 60.5475 |+12| 67.8325 |+19 — 2.7161| —3.0919 2 b | 60.5505 |-11| 67.8290 |-+18 — 2.7128 M. se с | 60.5495 |+11| 67.8320 |-+18 — 2.7148] —3.09 an EN , ber __ar а | 60.5435 |10| 67.8380 |+19 — 2.7210] —3.1005 3.0980 3.0759 | +0.0029 0.0003 | —8.0783 | 15 е 60.5300 |+-10| 67.8505 |+-19 — 2.7340] —3.0996 1—2 Х | 60.5305 |+10| 67.8480 |+19 — 2.7324] —3.1024 2 Ша | 66.0545 |+11| 62.3240 |- 9 + 2.7921| +2.4163 1 b | 66.0615 |+10| 62.3185 |+ 9 + 2.7983 м = с 66.0655 |-+-10| 62.3140 | 9 + 2.8026] 2.420 + + = AIRES ere rel lez Arte + 27998] +-2.4203 -+2.4203 | 2.4031 0.0026 0.0003 | 2.4002 | о e 66.0555 |+11| 62.3285 |+I1 + 2.7902] -+2.4246 1—2 | 7 | 66.0605 |-11| 62.3230 |+12 + 2.7954] +2.4254 1—2 IV а | 65.2730 |+17| 63.1060 |- 9 + 2.0106] +1.6348 2 b | 65.2780 |+17| 63.1050 |+ 9 —+ 2.0136 ве 5 | с | 65.2745 |+16| 63.1075 |+ 9 + 2.0106| +1.628 A г К d | 65.2635 |+16| 63.1150 |+-10 + 2.0013] —+1.6218 a rx 0.0003 | +-1.6126 2 | e | 65.2510 |+16| 63.1320 |+10 + 1.9866] +-1.6210 2 | f | 65.2490 |+17| 63.1325 |+ + 1.9853| 1.6153 1—2 || Scheinbare Adiff: 1—Centrum = -+23'4028 2 ==0:09287 —i9,, = -Н0.00201 г 0— » ——52.3147 : й в К— » = -+27.2032 fa = 0.99258 —iy =-0.00202 X ig 69 4 L— » = +29.2350 Refr. = — IL à 5 т Try = O ay —=12 14.6 Га = 0.99288 Л, = 0.0011 pr POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 1598. April 11. тре. Decl. | Scalenablesung. 2 тж, а Re se “rt Bemerkungen =—=_ = ——= —— sin : P-Kr.90° |#-1| P.-Kr.270° [tn 2 Lie vice zur Aufnahme. р Eu _mm_ a _тт | mm Pr 654018 |'0000| 649766 | 10000) 10000 63.4008 |10| 64.9750 |+16| c| 0.0000 0.0000 0.0000 Bilder 2. | 63.7632 |-+17| 64.6138 |-+23| o|+ 0.3618 — 0.0317 + 0.3301 73-3040 |+30| 65.0755 |+16|— 7| -+ 9.9016 — 0.1595 —+ 9.7421 78.7230 |+17| 49.6500 |+13|— 4| 15.3237 — 0.0432 15.2805 47.5515 |+32 80.8248 |-+24|+ 4] — 15.8484 — 0.0491 — 15.8975 68.5750 |+18| 59.8230 |-+14 + 5.1636 68.1690 |+18| 60.2260 |+14 + 4.7591 + 4.7588 Bilder 2—3! Der ‚67.7610 |-+18| 60.6290 |+-10 + 4.3538 Schatten eines Tra- 66.9900 |+ 8| 61.4130 |+ + 2.6758 banten ist am NW- 66.5845 |+ 8] 61.8170 |+ 3 + р + 3.1727 Raude der Jupiter- 66.1805 +10] 62.2120 |+ 9 + 2.7722 scheibe sichtbar. 65.4070 |+16| 62.9895 |+ 9 + 1.9965 65.0070 |+16| 63.3900 |+ 9 + 1.5962 — 1.5963 64.6080 |-+т6| 63.7910 |+ 8 + 1.1963 62.2645 |+ 9| 66.1310 |+10 1.1459 61.8600 |-+ 9] 66.5405 |+ 8 — 1.5528 — 1.5505 61.4615 |+ 9] 66.9420 |+ 8 1.9528 60.6730 |+10| 67.7270 |+18 — 2.7400 60.2680 |+14] 68.1255 |+18 — 3.1416 — 3.1408 59.8740 |+14| 68.5300 |+18 — 3.5408 59.1480 |+-10| 69.2490 |-+13 — 4.2632 58.7350 [+10] 69.6550 |-+16 — 4.6729 — 4.5708 8.3390 |-+10| 70.0660 |+-16 — 5.0764 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. 12 (иг) 7 (ео) ве) Ph. | Ad mm mm } “Geht dufrch [die Jupiter|schelibe 1 69.6580 |-+17| 58.7230 [+10 + 6.2552] <+1.4964 8.0820 |-+19| 60.3050 |-+14 + Е 1.5035 6.5050 |-+11| 61.8830 |+9 + 3.0985| —1.5022 Вы р ' р , 13530 Lerol 65.0320 [+16 0,0514] 1.499! —+-1.5023 | 1.4930 | -+0:0066 0'0000 0'0000 | -—1'4996 1.7700 |-+10| 66.6155 |+ 8 — 1.6352| —+1.5056 60.2410 |+11| 68.1430 |-+18 — 3.1640] —1.5068 740 + 8| 61.6065 |+10 + 3.3710] —1.3878 65.1955 |+16| 63.1830 [+10 + 1.7940 я ‚63.6170 |-+ 8| 64.7640 |+17 + 0.2134] — 1.3829 | _ LS =. + 60.4650 Irı4l 67.9120 |+19 ^ 2.9364| 1.3859 1.3850 1.3764 0.0052 0.0000 0.0000 1.3816 58.8760 |--10| 69.5060 |-+14 — 4.5278| — 1.3870 97.3440 |+ 9 71.0360 |-+13 — 6.0588] —1.3880 61.1975 +18] 60.5870 [+11 + 4.3930| —0.3658 6 .2200 |+10| 62.1625 |+10 — pet —0.3565 64.6410 |+16| 63.7420 |+ 9 + 1.2368] —0.3595 | _ Cr == 7 24 61.4965 [r10| 66.8890 [+ 9 re 1.0088 0.3583 0.3580 0.3558 0.0034 0.0000 0.0000 0.3592 59.9065 |+14| 68.4745 |+19 — 3.4968| —0.3560 58.3820 |+ 5] 70.0015 |+17 — 5.0230] —0.3522 | Scheinbare Decldiff: I—Centrum — + 0:2847 f°5 =0.99307 125 =—0.00205 0— » =+ 9.7702 K— » = 15.1248 fs = 0.99266 is =-— 0.00201 x в=- 69 L— » = —15.8412 Г; —0.99381 УТ; = —0.00212 9% = +0° 8.9 232 Е. Renz, 91. 1895. April 14. № Scalenablesung. Pulkowaer Sternzeit Object. x een Bilde P.-Kr. 0° tt P.-Kr.1800| t-+% der Aufnahmen. Mittel. I mm oo mm _ mm mm Ctr. | 64.1088 64.2656 J 64.1080 |+ 8| 64.2648 0.0000 о I 85.2208 |— 2| 43.1585 —+-21.1082 ; Pr 2 О | 16.9640 |-+28| 111.4095 —-47.1400 12° 15” 19° 1—2 ellipt. K 88.5630 |— 2| 39.8075 -+24.4540 1—2 УР 90.5810 ol 37.7995 26.4671 2 Z ay | 63.6635 | 9| 64.7305 — 0.4505 ас | 64.0805 |-+ 9| 64.3210 — 0.0418 — 20.0351 12 т 49 9—3 ay | 64.5070 |+ 9] 63.8900 — 0.3869 %Dbw | 63.6690 | 9| ‘64.7200 — 0.4474 bd, | 64.0970 |+ 9] 64.2925 — 0.0193 — 0.0202 2 58 3 bd, | 64.5260 |+ 9| 63.8705 — 0.4062 3 Cw | 63.6650 |+ 9] 64.7190 — 0.4490 Ce | 64.0925 | 9| 64.3065 — 0.0286 — 0.0252 Fe) 9—3 Co | 64.5220 |+ 9] 63.8750 + 0.4020 128 4” 3» Z du | 63.6525 |+ 8| 64.7405 — 0.4660 de | 64.0780 | 8| 64.3125 — 0.0389 — 0.0394 5722 9—3 do | 64.5045 |-+ 8| 63.8880 — 0.3866 %е | 63.6805 | 8| 64.7170 — 0.4403 €e | 64.1000 |-+- 8| 64.3000 — 0.0216 — 0.0172 6 so 3 eo | 64.5285 |+ 8| 63.8645 + 0.4104 %Лш | 63.6850 |= 9| 64.7130 — 0.4360 | Je | 64.1065 |+ 9] 64.2895 — 0.0131 — 0.0116 81789 3—4 fo | 64.5350 |+ 9] 63.8630 + 0.4144 Trabant — Jupiterscentrum. Cr — 24 | Mittel. (ваз) Jatur—v2)| Ph. | Az cos à mm mm DEEE Га | 66.0120 |11| 62.3695 + 1.8998| 1.9349 A b | 66.0340 |+11| 62.3475 + ‚92 1.9420 ot с | 66.0295 |10| 62.3540 —= 1.9162] +-1.9414 р nr 1% , = £ а RTL in ва Ыб: | 10440] 9519402 +-1/9286 | —0'0020 | —0!0004 | 19262 ME e | 66.0430 |10| 62.3420 + 1.9289] 1.9461 5, Х | 66.0445 |+11| 62.3365 + 1.9324| +1.9440 = 9 Па | 62.5875 |+11| 65.7915 — 1.5236] —1.4885 1 2 6 | 62.6055 |+-10| 65.7760 = ро ых 5 с | 62.5935 |+10| 65.7860 — ee DE, Е} APPLE d | 62.5790 |+ 9] 65.8015 СЕ 153301 дозб РЭА loop AAA 26 0 006 | TB: LEA SES ze е | 62.5935 |+ 9| 65.7850 — 1.5174] —1.5002 er f | 62.5925 |+ 9] 65.7860 — 1.5184] —1.5068 - III Geht dulrch [die Jupiterschefibe; | als Vorsplrung am [NW-rande erkennbar. IVa | 56.9010 |+-11| 71.4785 — 7.2105] — 7.1754 } b | 56.9205 |+10| 71.4600 — 2 ZU | e 6.9145 |+10| 71.468 — 7.1958] — 7.1730 | _ СЕ: à а 36.9000 +10 Во — 72120] —7.1726 | 7.1747 | 7.1243 | +-0.0076 | —0.0004 | ATI 2 N е | 56.9200 |+ 9| 71.4615 — 7.10925] —7-1753 ] f | 56.9210 [+ 9] 71.4610 — 7.1918] —7.1802 J Scheinbare Adiff: a ag F? «= 0.99298 —i°, = -+0.00214 — » — —52.314 K— » =+27203 Хи —0.99270 —ty = -+0.00214 X te —= "74 ==) — —29.2352 Refr. = — 2 h т 1155 = O | ay—12 133 Л = 0.99298 JT, = -+0.00212 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 233 1595. April 14. < t+k tk) P.-Kr.270° mm En mm mm Sim 10000| 646236 | 10000] 10000 64.6220 |+16 o 0.00C0 64.2612 |+15 ©] + 0.3650 54.7278 |+16|— 7| + 9.8982 49.2965 |-+22 80.4715 |+18 ‚68.9510 59.4380 68.5420 59.8515 | 68.1390 60.2600 _67.3770 61.0170 66.9670 61.4330 66.5570 61.8380 65.7960 62.6050 ( 63.0140 63.4195 65.7400 66.1450 66.5495 67.3135 67.7130 68.1130 68.8915 69.3025 69.7020 4 +++ +++ ЕЕ Oz 60.7705 62.3465 63.9320 67.0640 68.6330 70.2145 58.9650 60.5380 62.1240 65.2520 66.8180 68.3950 (le ARE TR UE —+ eht dulrch |die Jupiter|schelibe; —14| 56.2435 (o) + 8.3868 +15| 57.8170 |+ 6 + 6.8121 +16) 59.4035 |+11 + 5.2259 +13| 62.5300 |+10 + +11] 64.1025 |+ 9 + .6980 |-+12| 65.6840 |-+11 | Scheinbare Decldiff: I--Centrum = + 0.2847 De Un, == 9.7703 К— » = -+15.1248 L— » = —15.8413 _ San. Физ.-Мат. Отд. Decl. Znt%ch%s mm —+ 4.7830 — 3.2047 —+ 1.6221 — 1.5102 — 3.0783 — 4.6647 Ye—Yy | Mittel. 0.9256 —0.9254 0.8856 —+3.6038 —+-3.6074 +-3.6038 +-3.6068 —+3.6058 —+-3.6077 —3.6059 f°3 = 0.99318 fs = 0.99278 Гу =0.99387 ‚и х2 у. Bemerkungen — з tg9 sin 1 у— 5 196311 zur Aufnahme. mm mm 0.0000 0.0009 Bilder 2. — 0.0317 + 0.3333 — 0.1595 + 9.7387 — 0.0432 —+15.2806 — 0.0491 — 15.8939 Um 11* 59” tritt ein Trabant am SW- Rande aus; auf der Scheibe ist sein Schatten sichtbar. Trabant — Jupiterscentrum. T 2 Хаби уз) | Та и--аз) ве-аз]| Ph | № —0'9197 | —0!0042 0'0000 | -+0:0001 —0:9238 —0.8802 | -+0.0033 0.0000 | —-0.0001 —+-0,8836 +3.5838 | +0.0156 0.0000 | --0.0001 —3,5995 195 = —0.00216 13 =- 0.00216 x ig = —7:4 Ту = —0.00218 30 234 Е. Rexz, 92. 1298. April 33. AR Scalenablesung. Pulkowaer Sternzeit Object. tut Lot Bo P.-Kr. 0° t-+k der Aufnahmen. | Mittel. tt P.-Kr.180° un 10000 re 10000 10000 Ctr. | 64.4906 63.8841 J 64.4898 |+ 8| 63.8832 [+ 9] о 0.0000 2 a 85.6050 |— 3| 42.7785 |-+22|— 2| 21.1086 h 1—2 0 17.3402 |-+28| 111.0358 |+ 6|+32| —47.1468 13° 57044 2—3 1—2 2 тт тт К 88.9478 |— 2| 37.4232 |+28|— 5| +24.4570 L 99.9595 ©| 39.4172 |+30|— 6] +-26.4658 ZA | 64.1035 |+ 9] 64.2940 |+ 8 — 0.3984 Ge 64.5125 |-+17| 63.8825 |+ 8 — 0.0122 — 0.0146 13, 408539 2 Go 64.9300 |+17| 63.4645 |- 8 + 0.4300 2b | 64.0955 |+ 9| 64.3030 |+ 8 — 0.4070 be 64.5095 |-+17| 63.9020 |+ 8 —= 0.0010 + 0.0036 AS 9 2 b, 64.9160 |-+17| 63.4770 |+ 8 + 0.4167 % Co 64.1050 |-+ 9| 64.2875 |- 8 — 0.3944 Ce 64.5180 |+-17) 63.8800 |+ 8 + 0.0162 = 010177 49 9 k 2 es 64.9275 |-+17| 63.4595 |+ 8 + 0.4312 13° 49” 59% % dy | 64.0885 | 8| 64.3070 |- 9 — 0.4126 de | 64.5025 |-16| 63.9010 |+ 9 — 0.0022 — 0.0010 50 19 2 do 64.9105 |-+16| 63.4810 |- 9 + 0.4118 %е, | 64.1115 |+ 8| 64.2840 |+ 9 — 0.3896 en 64.5220 |+16| 63.8725 |-+ 9 + 0.0218 —= 0.0217 SI 49 2 en 64.9355 |-+16| 63.4640 |+ 9 — 0.4328 Afaw | 64-1110 |+ 9] 64.2850 |-+I10 — 0.3903 Я 64.5300 |-+17| 63.8790 |+10 -+ 0.0226 + 0.0242 34.0) 2 Te 64.9405 |-+17| 63.4540 |+10 — 0.4404 Trabant — Jupiterscentrum. 21—92, | Mittel. Wate-aa)| Ja Wu-v2)| Ph. | Au cos à rap ре бя о ue Та | 66.1350 |--11| 62.2450 |+ 9 + 1.6418] +1.6272 2 b | 66.1220 |+11| 62.2600 |+ 9 + 1.6278] +-1.6242 2—3 с | 66.1300 |+-10| 62.2490 |+ 9 + 1.6373] +1.6196 ‚ pis < фе , 2 d | 66.1100 |+11| 62.2725 |+-10 + 1.6156] +1.6166 „71-6180, |) DES GEL Ze AO 2 e | 66.1285 |+ı1) 62.2555 |+-10 + 1.6333| -+1.6116 95 f | 66.1285 |-+11| 62.2560 |-11 + 1.6330| 1.6088 2—3 Па 66.6815 |+ ©| 61.7000 |- 9 + 2.1876] 2.1729 2 b | 66.6755 |+ 9| 61.7060 |+ 9 + 2.1815| +2.1779 | 1—2 с 66.69c0 |+ 8| 61.6909 |+ 9 — 2.1967| +2.1790 u 2 d 66.6800 |+ 8| 61.7065 |+10 + 2.1834| +2.1844 +2.1820| +2.1665 | -+0.0026 0.0008 | +2,1683 2 e | 66.7040 | 9] 61.6780 |-н11 + 2.2096] 2.1879 2—3 Х | 66.7085 |+ 9| 61.6730 |+12 + 2.2144] 52.1902 2 Ша 59.6615 |-+16| 68.7180 |+14 — 4.8314] —4.8460 1—2 b | 59.6520 |-+15| 68.7280 |+13 — 4.8412 № 1—2 с 59.6665 |-+15| 68.7120 |+13 — 4.8259] —4.8436| _ AR Le a enxell 2 а | 59.6475 |+14| 687310 +13 — 4.8459] —4.8440 4.8444 4.8100 | -+0.0050 0.0008 4,8058 2 е | 59.6710 |+-14| 68.7110 |+14 — 4.8232] —4.8449 2 f | 59.6745 |+14| 68.7055 |+14 — 4.8188] — 4.8430 2 IV а | 72.5410 |-+13| 55.8400 |— 1 — 8.0480| 8.0334 1—2 b | 72.5330 |+13| 55.8500 о + 8.0389 Bo 1—2 С 72.5480 |+13| 55.8360 o + 8.0534] +8.0357 és u 2 d | 72.5310 [4141] 55.8530 [+ 1 + 8.0364| +8.0374 +8.0359| -+7.9788 0.0087 0.0008 | -+7,9698 12 е 72.5535 |-+14| 95.8310 |+ 2 + 8.0586] +-8.0369 2 Л | 72.5570 |-+15| 55.8300 |-+ 2 — 8.0609] -+8.0367 2—3 Scheinbare ВАШ: 7—Centrum == +23/4033 Fu = 0.99286 —1 = -+0.00200 0— э» = —52.3149 R | К— » = -+27.2036 Fa = 0.99256 —iy = -+0.00198 x = — 6:8 L— » = -+29.2357 Refr. = + 24 <, р Try — O 2, — 120 0.8 Г’, =0.99290 Jr = 0.00222 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. Scalenablesung. 59.9180 |+14 60.3060 |-14 60.6965 |+10 61.4800 |+ 9 61.8850 |+ 9 62.2555 |+ 9 63.0610 |+ 9 63.4550 |+ 9 63.8370 |+ 8 66.1950 |+10 66.6010 |- 8 66.9805 |+ 8 67.7810 |-+18 68.1740 |+18 68.5615 |-+18 69.3265 |+-13 69.7225 |+-16 70.1155 [+16 61.0095 |+11 62.5680 |+10 64.1430 |+ 9 67.2830 |+ 9 68.8660 |+14 70.4120 |-+17 61.4730 |+11 63.0320 |+10 64.6130 |+17 67.7565 |+19 69.3400 |-+14 70.8885 |+13 58.0400 |+ 6 59.5990 HIS 61.1785 |-+11 64.3180 [+ 9 65.9040 |+11 67.4505 |+ 9 64.2090 |--11 65.7720 |+13 67.3510 |+11 70.4900 |-+19 72.0765 |+14 + 1] 73.6255 |+15 1898. April 23. Decl. >,-Kr. 90° tt P.-Kr. 270° ++ тт ou m mm 33.3311 65.0481 |10000|10000 93.3302 65.0465 |+16| о 0.0000 3.6888 64.6892 |-+23| o|+ 0.3580 .2480 55.1348 |+16|— 7|+ 9.9151 49.7242 |+15|— 4] +15.3206 80.9050 |-+25|-+ 4| —15.8570 ЕЕ +44 ++ FR & > о © [| > a о РЕ ПГ | è & Е + II EI 4 le ö Scheinbare Decldif: I— Centrum — + 0.2846 K— Be » » » = 15.1248 = —15.8415 dy = +0° 381 mm + 4.7493 + 3.1858 — 1.6065 — 1.5346 — 3.1163 — 4.6674 тт — 0.7092 — 0.7030 +-2.2617 -+2.2636 —+-2.2667 —+-2.2648 +-2.2622 —+-2.2680 —3.9079 — 3.9059 — 3.9065 — 3.9070 — 3.9109 — 3.9070 mm —0.7011 — 1.1709 * +2.2645 3.9075 /95 = 0.99292 fs = 0.99249 f's = 0.99373 тт 0.0000 — 0.0317 — 0.1595 — 0.0432 — 0.0491 0.0000 Bilder 2. Trabant — Jupiterscentrum. — 0.6967 — 1.1636 -+2.2504 — 3.8830 — 0.0027 —0.0036 —+-0.0081 —0.0135 12; = —0.00184 is = —0.00193 Js = —0.00169 Ye--Y2% | Mittel. |’ (гу) | 7 r—22)|-8-222) 3] Ph. | 45 0,0000 | -+0'0002 0.0000 —0.0502 0.0000 —+0.0002 —0.0001 —=0.0002 X is — — 6:6 Bemerkungen 12 © Qt zur Aufnahme. —0:6992 —1.1670 +-2,2587 —3,8964 Scalenablesung. Object. ni — >= SOL or Us ra no LIT оса P.-Kr. 0° mm 64.7046 64.7030 85.8258 17.5515 89.1625 91.1828 64.2480 64 6985 65.1435 64.2405 64.6855 65.1250 64.2510 64.6990 65.1400 64.2890 64.73 10 65.1525 64.2910 64.7275 65.1710 64.2550 64.7055 65.1400 63.4275 63.4360 63.4485 63.4765 63.4870 63.4605 66.4970 66.4880 66.5055 66.5205 66.5260 66.4910 61.9750 61.9765 61.9895 62.0190 62.0280 61.9980 73-2425 73.2380 73.2550 73.2740 73.2830 73.2560 t+k P.-Kr.180° mm 63.6673 63.6665 42.5572 110.8178 39.2045 37.1920 64.1400 63.7030 63.2480 64.1435 63.7140 63.2600 64.13C0 63.6990 63.2490 64.1030 63.6690 63.23С0 64.1010 63.6695 63.2195 64.1440 63.7010 63.2440 64.9530 64.9500 64.9390 64.9095 64.8960 64.9210 61.8905 61.8920 61.8785 61.8640 61.8590 61.8900 66.4000 66.3960 66.3820 66.3570 66.3475 66.3770 55-1445 55-1565 55-1370 55-1140 55.1040 55-1335 Scheinbare Adif: 1595. April 24. t+k mm mm 10000] 10000 Fer rer ЕЕ © 0900 0 wo 0 © + TEL оо ох Lt — Ty тт — 1.2631 — 1.2466 — 1.2478 — 1.2456 — 1.2384 — 1.2328 DaB +-1.8037 —+1.8088 +1.8114 +1.7996 —-1.8000 +-1.7983 УЕ —2.7127 —2.6990 —2.6985 —2.6978 — 2.6933 —2.6917 —8.5496 -+8.5522 —8.5574 -+8.5520 —+8.5566 8.5598 I—Centrum == -+23!4033 O— » = —52.3149 К— » == -+27.2037 1— » = -+29.2358 жа 12° 9.5 Е. Renz, 0.0148 0.0165 Pulkowaer Sternzeit der Aufnahmen. | 59 O 23 25 31 39 Trabant — Jupiterscentrum. | Mittel. P'ati—22)a из) Ph. | Au cos à —1.2368 —8.4930 тт Nee 0.992890 Л» = 0.99251 Ло = 0.99280 0/0012 | —0'0097 —0.0017 +-0.002$ —0.0094 ВАР —i°, = 0.00225 —iy = -0.00224 Вет. = + 10 Try = о я = —+0.00234 Mittel. —1:2363 [| | Bilder, ei 4 unterexpon 3—4 | +1,7882 | 3—4 —2.6776 —8.48:9 a EEE a = _. р ie RR, = ER ee м а POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 237 ine. — Scalenablesung. D Кг. 90° + P.-Kr.270° mm 64.1568 64.1560 63.7942 54.2598 48.8252 80.0068 58.8775 3 mm 612166 1598. April 24. Decl. 4 2 Bnt2ch%s t-+-k 3 mm mm mm 10000] 10000 + 8 о 0.0000 +16] о] -+ 0.3655 —=20]|— 7] + 9.9000 59.3150 + 4.8593 59.7350 60.5330 60.9670 -+ 3.2066 61.3880 62.1160 62.5490 + 1.6311 62.9580 65.2855 65.7085 — 1.5330 66.1150 66.8330 67.2520 — 3.0784 67.6670 68.3550 68.7760 — 4.6103 69.2050 Yt—Y2 | Mittel. mm 58.7945 + 5.3680] -+0.5087 60.4500 + 3.7131| -+0.5065 62.0340 + 2.1302] -+0.4991 65.1880 — 1.0274] -+-0.5056 IB 66.7400 — 2.5768| 0.5016 68.2740 — 4.1130] -+0.4973 60.0210 |-+15 + 4.1422] — 0.7171 61.6785 |-+10 —= 2.4848| — 0.7218 63.2500 |+10 ЗЕ 0.91124 —-0.7199 | _ 166 66.4080 |+11 — 2.2472| — 0.7142 я 67.9535 — 3.7909] —0.7125 69.4880 — 5.3241| — 0.7138 58.2400 + 5.92I4| —+-1.0621 59.9000 — Aa —+1.0565 61.4795 —= 2.6810] -+1.0499 64.6360 — 0.4750] —-1.0580 1140561 66.1870 — 2.0249| -+1.0535 67.7145 — 3.5535] -+1.0568 63.3250 —= 0.8410| —4.0183 64.9745 — 0.8092| —4.0158 66.5570 — 2.3928| —4.0239 — 4.0175 69.7105 — 5.5472| —4.0142 , 71.2585 — 7.0953| — 4.0169 72.7890 — 8.6261| —4.0158 Scheinbare Deeldiff: I-Centrum —+ 0.2846 f° 3 = 0.99296 -- » —=-+ 9.7705 3 К— » =-+15.1248 fs = 0.99255 L— » = —15.8415 f’s = 0,99365 82 = + 0° 40:1 x? n — 5 tù sin 1’ аи) о реа) вет Pa | Bemerkungen Enns У — 5 190 8ш 1 zur Aufnahme, mm mm 0.0000 0.0000 Bilder 4—5. — 0.0317 + 0.3338 — 0.1595 + 9.7405 — 0.0432 +15.2864 — 0.0491 —15.8956 Bilder 3—4. Die Bilder ver- schlechtern sich schnell, Trabant — Jupiterscentrum. Ad —+0'4999 | -+0:0026 0:0000 | -+0!0002 —+0:5027 —0.7120 | —0.0038 0.0000 | +-0.0002 — 0,7156 —1.0494 | -+0.0057 0.0000 | 0.0002 +-1,0553 —3.9920 | —0.0179 | —0.0001 | -+0.0002 —4.0098 12 = —0.00216 14 =— 0.00220 X 4=— 76 Js = —0.00210 30* 238 Е. Renz, 94. 1898. April 25. № | Scalenablesung. Pulkowaer Sternzeit у О ER en nn le © = ns low Га ВИЙ Bilder P.-Kr. 0° tt P.-Kr.180° |t+% der Aufnahmen. Mittel. К п 10000 70 10000 10000 un mn EM Ctr. | 62.3949 65.9760 | 1 J 62.3940 | 9| 65.9750 |+10| о 0.0000 2 br J4 83.5098 |+ 2| 44.8640 |+18|— 2]+21.1124 3 в 2 1—2 ns (0) 15.2378 |+-30| 113.1310 |+ 5|-+32| —47.1516 12 52 2 etwas ellip@ 7 K 86.8535 |+ 1| 41.5162 |#+28|— 5] +24.4574 1—2 | В L 88.8740 o| 39.5010 |+30|— 6] 26.4750 1—2 %ар | 61.9510 | +ти! 66.4425 |+11 — 0.4552 | ag | 62.3630 |+11| 66.0255 |+11 — 0.0407 — 0.0390 12 И 92 2 | ao | 62.7825 [11] 65.6060 |+11 + 0.3788 | %Dby | 61.9565 |+10| 66.4380 |+10 — 0.4502 bi, bu | 62.3780 |-10| 66.0170 |+10 — 0.0290 — 0.0320 43 ТО 2 И. 6, | 62.7895 |+10| 65.6040 |+10 + 0.3833 u сш | 61.9350 | +10] 66.4550 |+-10 — 0.4694 K Ce 62.3595 |+10| 66.0330 |+10 — 0,0462 — 0.0451 44 14 2 Я cr 62.7875 |+10| 65.6080 |+10 + 0,3803 12 44” 19° +) u % dy | 61.9560 |+ 9| 66.4430 |-+11 — 0.4530 En de | 62.3715 |+ 9] 66.0225 |+ — 0.0350 — 0.0365 45 20 2 do | 62.7845 |+ 9| 65.6085 |+11 + 0.3784 u Ze | 61.9525 |+ 9| 66.4440 |+H11 — 0.4553 | CA 62.3725 | 9| 66.0220 |+11 — 0.0343 — 0.0343 46 30 2 ИЕ eo | 62.7925 |+ 9| 65.6000 |1 + 0.3867 _ |) %]ш | 61.9375 |+10| 66.4540 |-+12 — 0.4678 № с 62.3765 |+-10| 66.0225 |+12 — 0.0326 — 0.0359 47 50 2 В 75 62.7960 |+10| 65.5915 |+12 + 0.3927 N Trabant — Jupiterscentrum. ARTEN | Mittel. ива Ja tea) Ph. | Aa cosö mm mm Ia 63.0295 |+10| 65.3455 |-+16 -+ 0.6322] +0.6712 2 b | 63.0300 |+10| 65.3490 |+16 + 0.6308] -+0.6628 2 с | 63.0185 |--109| 65.3610 |+16 — 0.6190] <+0.6641 ' ES, a, р а | 63.0200 |+ 9| 65.3600 |-+17 + 0.6202] --0.6567 +0.6579| -+0:6531 0:0005 0:0008 | +-0:6518 9 e 63.0155 |+ 9| 65.3620 |+17 +- 0.6169] +0.6512 2 f | 63.0060 |+-10| 65.3745 |+18 + 0.6059] -+0.6418 2—3 Па 59.5970 |-+16| 68.7845 |-+14 — 2.8031| —2.7641 1—2 h b 59.6025 |+15| 68.7750 |-+13 — 2.7956] — 2.7636 1—2 | 1 с 59.5875 |-+15| 68.7900 |+13 — 2.8106] —2.7655 | __ 2% ’B я h а | 59.5960 |+14| 68.7870 |+13 — 2.8049] —2.7684 2.7674 2.7474 | +0 0033 0.0008 | —2,7499 | 5 Ih e 59.5960 |+14| 68.7850 |+-14 — 2.8040] —2.7697 2 en Л | 59.5920 |+14| 68.7905 |+-14 — 2.8087] —2.7728 3 iR Ша | 63.7005 |+ 9| 64.6745 |4+-16 + 1.3032] +1.3422 1—2 li b | 63.7110 |+ 9| 64.6630 [+16 + 1.3142] +1.3462 1—2 h с 63.7030 |+ 9| 64.6720 |-+16 + 1.3057] -+1.3508 er A : 2 | В a | 63.7155 |+ 8| 64.6630 [+17 + 13164] +1.3529 1.3514 | +1.3417 0.0021 0.0008 | -+1,3388 2 | е | 63.7195 |+ 8| 64.6570 |+17 + 1.3214] +T.3557 2 h f | 63.7220 |+ 9| 64.6530 |+18 + 1.3246| -+-1.3605 2 il IVa | 70.2530 |+17| 58.1265 |+- 5 + 7.8544| -+-7.8934 2 6 | 70.2560 |+16| 58.1235 [+ 5 + 1.8574 —-7.8894 1—2 с 70.2460 |+16| 58.1360 |- 6 + 7.8460] +7.8911 с. в 2 d | 70.2540 |-+17| 58.1290 |+ 7 + 7.8536] -+7.8901 7.8895 | 47.8326 0.0084 0.0008 | +-7.8284 2 | е 70.2540 |+17| 58.1295 |+ 7 + 7.8533] 7.8876 2—3 И f | 70.2500 |-+18| 581330 |+ 8 + 7.8496] -+7.8855 2—3 | Scheinbare Adif: РИН = -+23'4034 f° x = 0.99277 —1°, = +0.00228 N — .» = —52.3149 K— » =-+27.2037 fa = 0.99249 —№ = 0.00228 X = — 78 L— » = +-29.2358 Refr. = + 7 A m Toy = O ОА“ © f'x = 0.99278 Л. = -+0.00235 *) Der Chronometer war nicht mit der Normaluhr verglichen worden; die angenommene Correction könnte bis --5° unsic ne. Scalenablesung. y Р.-Кг.90° ++ P.Kr.270°| ++ HS 10000 7 10000 10000 mu 63.9959 64.3800 63.9950 |+ 9] 64.3792 |+ 8| oJ 0.0000 64.3675 |-+17| 64.0095 |-+14]| о] -н 0.3712 73.8930 |-+30] 54.4832 |+20]— 7| + 9.8968 79.3250 |-+17| 49.0418 |-+21|— 4|-+15.3330 48.1518 |-+31| 80.2252 |+-18|-+ 4] —15.8436 69.1720 |+14| 59.2260 |+10 + 5.1652 68.7760 |-+14| 59.6215 |+14 — 4.7693 68.3845 |+14| 60.0170 |-14 + 4.3758 67.5965 |+ 9] 60.7955 |+-10 + 3.5925 67.1970 |+ 9| 61.2020 |+10 + 3.1895 66.8070 |+ 9| 61.5905 |-+10 + 2.8002 66.0260 |+11| 62.3680 |+ 9 + 2,0212 65.6280 |+11| 62.7690 |+ 9 + 1.6216 65.2220 |-+17| 63.1710 |+ 9 + 1.2180 62.9000 |+10| 65.4960 |+10 — 1.1060 62.5030 |+10| 65.9090 |-+-10 — 1.5108 62.0890 |+10| 66.3020 |+-10 — 1.9144 61.3240 |+11| 67.0665 |+ 8 — 2.6790 60.9270 |+11| 67.4800 |+ 8 — 3.0843 60.5190 |+-11| 67.8770 |-H18 — 3.4873 59.7510 |+ı5| 68.6420 |+13 — 4.2534 59.3450 |+I1] 69.0460 |+13 — 4.6586 58.9400 |+-11| 69.4580 |+13 5.0670 68.5480 |-+14| 59.8370 |+-14 + 4.5476 66.9775 |+ 9] 61.4050 |+10 + 2.9782 65.4060 |+17| 62.9750 |+ 9 + 1.4080 62.2725 |+-10| 66.1075 |+10 — 1.7254 60.7020 |+11| 67.6800 |+18 — 3.2973 59.1280 |+11| 69.2540 |-+13 — 4.8710 5 ‚1615 |-+18| 58.2175 |+ 6 + 6.1646 8.5950 |+15| 59.7830 |+15 + 4.5980 67.0205 |+-10| 61.3570 |+11 + 3.0238 63. 8860 |+10| 64.4950 |+ 9 — 0.1124 62.3140 |-+11| 66.0670 |+ — 1.6844 60. .7405 |+12| 67.6410 |+19 — 3.2586 67.8760 |+18| 60,5010 |-+14 + 3.8798 66.3050 |-+-10] 62.0730 |+ 9 + 2.3081 64.7300 |-+16| 63.6500 |+ 8 + 0.7324 61.5910 |+ 9| 66.7855 |+ 8 — 2.4052 60.0165 |+14| 68.3590 |+18 — 3.9794 58.4395 |+ 5| 69-9350 [+16 — 5.5562 65.2070 |+17| 63.1730 |411 + 1.2094 63.6370 |+ 9| 64.7475 |+18 — 0.3636 62.0665 |+10| 66.3140 |-+12 — 1.9318 58.9300 |+11| 69.4550 |+-15 — 5.0706 57.3575 |+10| 71.0320 |+14 — 6.6454 55-7810 0] 72.6040 |+15 — 8.2202 Scheinbare Decldiff: I—Centrum = + 0/2846 0— » = + 9.7706 К— » = +-15.1248 L— » = —15.8416 POosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1898. April 25. Decl. dy = + 0° 42:1 Чин с; тт + 4.7701 + 3.1941 —+ 1.6203 — 1.5104 — 3.0835 — 4.6597 mm —0.2225 —0.2159 —0.2123 —0,2150 —0,2138 —0.2113 1.3945 —+1.4039 1.4035 +1.3980 +1.3991 +1.40II —0.8903 —0,8860 — 0,8879 —0.8948 —0.8959 —0.8965 —3.5607 mn: 0/1 —3.5521 — 3.5602 — 3.5619 — 3.5605 mm —0.2151 —+1.4000 —0.8919 —3.5588 195 = 0.99294 fs =0.99258 f's = 0.99362 тт 0.0000 0.0317 0.1595 0.0432 0.0491 a x? ву 7 95 sin 1 x? Ssi ’ Y— 3 19 sin 1 mm 0.0000 1103395 219278178 —+15.2898 —15.8927 Trabant — Jupiterscentrum. Yt—Y2 | Mittel. Ira ya) | 7-2 о P —0!2137 | —olooıs —+1.3911 | -+0.0064 —0.8862 | —0.0031 — 3.5362 | —0.0181 195 = —0.00234 ts = —0,00237 Js; = —0,00230 0/0000 0.0000 0.0000 —0,0001I X 5 = —8:1 239 Bemerkungen zur Aufnahme, Bilder 3. —+-0/0002 0.0002 0.0002 0.0002 —0:2150 +-1,3977 —0,8891 Bilder 240 Е. Renz, 95. 1898. April 28. № Scalenablesung. Pulk г St it Object: n ung A je ел о А ulkowaer ernzel P.-Kr. 0° |+ P.-Kr. 1609) + 3 der Aufnahmen. Mittel, 19 10000 HT 10000 10000 u) (I (г. | 64.2436 64.1253 J 64.2428 |+ 8| 64.1245 |+ 8] о 0.0000 1—2 Mi 85.3582 |— 2| 43.0182 |+21|— 2] -+21.1095 à De 0 17.0922 |+29| 111.2874 |+ 6|+32| —47.1524 12° 2:4" K 88.6970 |— 2| 39.6695 |-+32|— 5| +24.4524 2 L 90.7240 o| 37.6522 |-+29|— 6] 26.4747 2 ар | 63.7740 |+-10| 64.6105 |+-17 — 0.4774 ag | 64.1855 |+10| 64.1965 + 9 — 0.0646 — 0.0676 12 154.54 2—3 ао | 64.5905 |+10| 63.7940 |+ 9 + 0.3392 4b | 63.8010 |- 9] 64.5838 |- 8 — 0.4501 be 64.2210 |+ 9| 64.1655 |+ 8 — 0.0314 — 0.0363 ТВ 1—2 D, 64.6230 |+ 9| 63.7595 |+ 8 + 0.3726 % ст | 63.7705 |-+ 9| 64.6130 |+ 8 — 0.4804 Ber 64.1830 |+ 9| 64.2145 |+ 8 — 0.0748 — 0.0755 OC 2 бо 64.5805 |+ 9] 63.8050 |- 8 + 0.3286 12^ 18" 38° Zd | 63.7445 |+ 8| 64.6355 |+ 9 — 0.5047 de | 64.1665 |+ 8| 64.2335 |+ 9 — 0.0927 — 0.0945 Toy 216 2 do | 64.5670 + 8| 63.8205 |+ 9 + 0.3140 Ze | 63.7510 |+ 8| 64.6300 |+ 9 — 0.4987 ео 64.1600 |+ 8| 64.2300 |+ 9 — 0.0942 — 0.0917 PONS 1—2 en 64.5700 |+ 8| 63.8160 |+ 9 + 0.3178 Zfw | 63.7580 |+ 8| 64.6270 |- 9 — 0.4937 Te 64.1635 |+ 8| 64.2185 |+ 9 — 0.0867 — 0.0859 DIE 324 2 T0 64.5780 |+ 8| 63.8145 | 9 + 0.3226 Trabant — Jupiterscentrum. ee | Mittel. |f' (xx) Ta(r—v2) Ph. | Да cos 5 тт тт Та | 65.5580 |+11| 62.8195 |+ 9 + 1,3102| 1.3778 1-9 b | 65.5895 |+11 0 +9 + 1.3400 ве. à 3 с 65.5585 [+11 2.8250 |+ 9 + 1.3077] 1.3832 ‚ Re er 1, 22 da | 626480 [+10] 628360 [+10 BE 0 me +1.3857 | 1.3758 0:0018 0.0009 | +1:3731 2_3 е 65.5490 |[+10| 62.8255 |+-10 + 1.3026] 1.3943 2 f | 65.5540 |-+r1| 62.8250 |+11 — 1.3054| +1.3913 9-3 Па | 63.8590 |+10| 64.5245 [+ 9 — 0.3918] —0.3242 2 b | 63.8800 |-+ 9| 64.5000 |+ 8 — 0.3691 wi 2 2 С 63.8405 |+ 9| 64.5425 |+ 8 — 0.410 | —0.3346 | _ ig MR ue — 4 | 63.8245 |+ 8| 64.5590 [+9 — 0.4264] —0.3319 0.3343 0.3319 | —-0.0008 0.0009 | —0.3320 | 3 e 63.8235 |+ 8| 64.5565 |+ 9 — 0.4257| —0.3340 2 Х | 63.8135 | 8| 64.5630 |+ 9 — 0,4340| —0.3481 1—2 ПТа | 65.3600 |+18| 63.0155 |+10 + 1.1135] +1.1811 2 b | 65.3830 |+17| 62.9905 |+ 9 + 1.1375| +1.1738 ; Ä с | 65.3425 |+17| 63.0335 |+ 9 + 1.0958] 1.1713 | _ Eh 4 2: а | 65.3230 |-+16| 63.0530 [+10 —= 1.0762| 1.1707 OU ТО on 6.0009 1 116 2—3 е 65.3265 |+16| 63.0490 |+10 + 1.0799] 1.1716 2 J | 65.3220 |+17| 63.0520 [+11 —= 1.0762| 1.1621 2 IV a | 64.5505 |H-18| 63.8290 |+ 9 + 0.3920] 0.3696 1—2*) b 64.5690 |+17| 63.8100 |+ 8 + ER a AT с | 64.5295 |-+17| 63.8555 |+ 8 — 0.2783] 0.353 1 ue №: = au бабло тб 63.870010 + 0,2632] 0.3577 0.3570 | -+0.3544 0.0005 0.0009 | + 0,3530 3 e 64.5185 |+16| 63.8700 |- 9 + 0.2654] -+0.3571 2—3 f | 64.5120 |+16| 63.8730 |+ 9 + 0.2607| -+0.3466 2 Scheinbare Ædiff: I-—Centrum = +23:4025 9 — 9199282 —1® = 0.00241 0О— » = —52.3150 K— » =-+27.2038 fu = 0.99254 —iy = 0.00241 X 14 = — 8.3 L— » = -+29.2359 TO 2 в т Try = [e) ay=ı2 8.2 Г’ = 0.99283 Ju = 0.00243 *) Hart am Rande des Jupiter; Einstellung daher schwierig. 2 etwas ellipt, munie = = TS — 3 = рек e PoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 241 1595. April 28. ihe. Decl. Scalenablesung. À n+% 0% 2 ы 2 Bemerkungen — 8 y ще — < tgù sin 1’ — + tgÿ sin 1’ . Ir.90°|2-+-X|P.-Kr. 2709 + 3 1) pra ns | — (ele № ыы de 63.9038 63.9030 |+ 8| о 0.0000 0.0000 0.0000 Bilder 3—4. 63.5362 |-+15 С] + 0.3690 — 0.0317 + 0.3373 54.0200 |+-20|— 7] + 9.8852 — 0.1595 + 9.7257 48.5705 |+23|— 4 — 0.0432 —+15.2859 79.7475 |+19l+ 4 — 0.0491 — 15.8901 58.7420 |+10 59.1305 + 4.7834 Bilder 3. 59.5160 60.3200 60.7160 + 3.1979 61.1050 61.8850 62.2840 + 1.6340 62.6745 65.0175 65.4200 — 1.5005 | 65.8065 61.7910 | 66.6030 61.4045 66.9965 130797 61.0105 67.3840 EC 68.1615 59.8325 68.5660 — 4.6445 59.4460 68.9460 Trabant — Jupiterscentrum. | ” т ^ Yt—Y2 | Mittel. Узи ул) Toter) | ви?) Ph. | as mm mm | 59.8425 + —0.7188 61.4310 - —0.7198 us Бы en —0.7232 | —0/7187 | —0!0033 0!0000 | +0'0002 | —0!7218 67.7100 = —0.7273 69.2730 — — 0.7212 58.7900 + 40.3349 ‚60.3660 + mn 61.9380 + —0.340 | ER = 30.3381 | +0.3427 -+0.3406 | 0.0008 0.0000 | -+0.0002 | 0.3416 66.6410 — —+-0.3467 6 68.1995 — +0.3523 | 59.4290 + —0.3058 61.0150 + —0.3043 | 62.5770 + —013 045 HE a > — 0.3025 65.7100 РУ —0.3026 0.3018 0.2999 0.0028 0.0000 | -+0.0002 0.3025 67.2855 — —0.2970 68.8475 —- —0.2965 58.9100 + +-0.2162 60.4990 ' + +-0.21 38 62.0680 - -+0.205 “ ‚214 did a 0.2127 | 92144 | 50.2131 | + 0.0008 0.0000 | -+0.0002 | -+0,2141 66.7720 — —0.2195 68.3350 — 4.4257| -+0.2188 Scheinbare Decldiff: I--Centrum = +- 0!2845 f°5 = 0.99313 1° 5 = —0.00240 | | O— » _=-+ 9.7707 N 1 К » =-15.1248 fs = 0.99273 3 = —0.00240 X 15 = —8.; | L— » —= —15.8417 Из =0.9979 Js = —0.00238 В... Физ.-Мат, Отд. = 242 Е. Вами, 1 96. 1595. April 29. | р | № 8 Il Scalenablesung. : Pulkowaer Sternzeit | Objectif ana гПа 2 Ко Bilder) P.-Kr. 0° = Р.-Кг.180° ++ . der Aufnahmen. Mittel. в} 2 mm mm _ | тт | Ctr, | 626527 [10000 65.7199 10000] 10000 mm GRID Dh J 62.6518 |-= 9] 65.7188 |+11| о 0.0000 2 LÉ JB 83.7642 |— 7| 44.6155 |-+18|— 2| 21.1065 à À 2 | В O 15.4948 |-+29| 112.7722 |+ 5|+-32| —47.1507 13° 42” 46 2 à: IE 87.1038 |+ 1| 41.2665 |+-30|— 5| -+24.4503 2 LÉ L 89.1255 ol 39.2460 |-+30]— 6| -+26.4712 2 М 2 y | 62.1680 |++10| 66.2250 |+10 — 0.4949 u Ge | 62.6075 |+10| 65.7750 |+-10 — 0.0502 — 0.0513 13, A226 3—4 | A Go | 63.0510 [10] 65.3350 |+-16 + 0.3913 4 %6 | 62.1950 |+10 66.2015 |+-10 — 0.4696 {: be 62.6305 |+10| 65.7595 |+10 — 0.0309 — 0.0324 33 36 3—4 LL 6, | 63.0650 |+-10| 65.3250 |+-16 — 0.4033 | В 2 Cp | 62.1840 [+10] 66.2130 [+10 — 0.4809 №: Ce 62.6260 |+10| 65.7620 |+10 — 0.0344 — 0.0320 343.858 3—4 (] Co | 63.0685 |#+10| 65.3165 |-+16| -|-+ 0.4193 13^ 35" 08° W % dy | 62.1860 | 9| 66.2050 |+11 — 0.4760 k de | 62.6395 [+ 9] 65.7480 |-=11 — 0.0208 — 0.0271 36.06 O-rand ganz do | 63.0700 |+ 9| 65.3055 |+17 — 0.4154 waschen; м в %е | 62.2315 | 9| 66.1630 |-+11 — 0.4322 Ag № ee 62.6590 |+ 9| 65.7410 |+-LI — 0.0075 — 0.0088 26) 3 р en 63.0775 | 9| 65.3170 |+-17 + 0.4134 il A fr | 62.2220 |10| 66.1650 |-+12 — 0.4380 | Je | 62.6475 |+10| 65.7450 |+12 — 0.0152 — 0.0117 38 36 3 EL 16 63.0780 |10| 65.3085 |+-18 + 0.4180 N . Trabant — Jupiterscentrum. | u | Mittel. [щаз Лии») Ph. | N | Та | 60.7365 |-+12| 67.6500 |+19 — 1.9235 — 1.8722 F0 | 3 | b | 60.7585 |[+11| 67.6240 |-+18 — 1.8995 м 3 € 60.7445 |-+11| 67.6415 |-+18 — 1.9152] —1.5832 | __ ny р War nr 3—4 Al" 60.7435 Lerol 67.6448 |+19 — 191741 —1.8903 1.8758 1.8625 | -+0!0023 0.0010 1:8612 3 e 60.7775 |+10| 67.6045 |-+19 — 1.8804] —1.8716 2—3 f | 60.7780 |+10| 67.6090 |+19 — 1.8824] — 1.8707 3 Па | 59.7915 |+16| 68.5910 |+14 — 2.8660] —2.8147 8—4 b 59.8130 |-+15| 68.5620 |+13 — 2.8408] —2.8084 2 € 59.8010 |-+15| 68.5825 |+13 — 2.8570| —2.8250 | __ IE A ar 4 d | 59.8020 |+14| 68.5830 |+-14 — 2.8569] — 2.8298 ат SAUT) 30.0032 0210 2:7927 4 е 59.8410 |+14| 68.5420 |+14 — 2.8169! —2.8081 2 IE 59.8450 |-14| 68.5425 |+14 — 2,8152] —2.803 5 SE) Ша | 59.5525 |+16| 68.8200 |+14 — 3.1000| —3.0487 3 b 39.5740 IS an +13 — ie oo - с 59.5560 |-+15 .8200 |+13 — 3.0983| —3.0663 | _ er u er а |’ 50.5550 |+-14| 68.8270 14 = 31024 =3.0753 3.0588 3.0371 | +-0.0042 0.0010 3.0339 | оз е 59.5895 |+14| 68.7895 |+14 — 3.0664] —3.0576 3 f | 59.5845 |-+14| 68.7935 |+-14 — 3.0709] —3.0592 2—3 IV a | 59.6335 |+16| 68.7495 |+14 — 3.0243] —2.9730 3—4 b 59.6540 |-+15| 68.7245 |+13 — 3.0016] —2.9692 8 С 59.6345 |+-15| 68.7560 |+13 — 3.0270] —2:9950 | ‹_ м _ 095 4 а | 50.6255 |+14| 68.7526 [+14 — 3.0299] —3.0028 2.9846 2.9634 | —0.0045 | —0.0010 2,9599 24 е 59.6650 |+14| 68.7140 |+-14 — 2,9909| — 2.9821 2 f | 59.6610 |+14| 68.7220 |+14 — 2.9969] —2.9852 3 Scheinbare Adiff: JI--Centrum = = 3403 5 Ja 0.99288 —i°,, = +-0.00237 | — » = —62, | K— » =4+27.2038 fu —=0.99258 —iy = +0,00236 x = —8!1 | L— » = -+29.2360 Ref. = + 20 | hm Try = о { а = 12 7.9 la = 0,99290 Ju = +0.00256 POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN, 24 1595, April 29. 1.4237| —+-1.6463 3.0106| -+1.6482 66.2130 |-+11 67.7980 |+19 то .1020 |-+18| 58.2830 |+ 6 8.5750 |-+15| 59.8120 |-+15 66.9645 —=10| 61.4270 |-+11 3.8185 |+10| 64.5670 |+17 Вов 11| 66.1010 |+11 60.6990 |+12| 67.6870 |+19 + 6.5079] -+1.7436 + 49793 Be —= 3.3665] 1.74 + 0.2232| 1.7456 | 197524 | +1.7414 0.0063 0.0000 | +0.0002 | -+1.7479 — 1.3120] —+-1.7580 — 2.8962| 1.7626 he. Decl. Scalenablesung. Antrotr#s ca MU AA ne Bemerkungen $ 4 NON FRE Зы: ’ a Fi / hehe 2 90° te. -Kr. 270° |t-+-k 4 5 ren A an. ee m m mm тт тт тт тт тт 2000 10000! 647856 [10000 10000 63.5891 + 9| 64.7840 |-+16| о 0.0000 0.0000 0.0000 63.9555 I+17| 64.4192 |+14| 0|-+ 0.3661 — 0.0317 + 0.3344 Bilder 4 73-4840 |-+31| 54.8898 |+-16|— 7| + 9.8950 — 0.1595 19.7355 ь 78.9172 |-+17| 49.4525 |+21|— 4| -+15.3294 — 0.0432 —15.2862 47-7410 |+31| 80.6318 |-+24|- 4] —15.8468 — 0.0491 — 15.8959 68.7890 |+14| 59.6035 |+-14 + 5.1906 68.3620 |+19| 60.0290 |-+14 + 4.7646 —+ 4.7643 67.9350 |+-19| 60.4560 |+-14 + 4.3376 Bilder 3—4. 67.2480 |+ 9| 61.1585 |+10 + 3.6425 66.8210 |+ 9| 61.5740 |+ 9 + 3.2213 + 3.2235 66.4055 |+ 9| 61.9875 |+ 9 + 2.8068 65.6380 |+-11| 62.7540 |+ 9 + 2.0399 | 65.2300 |+17| 63.1730 |+ 9 -+ 1.6267 + 1.6179 64.7835 |-+17| 63.6055 |+ 9 + 1.1872 62.4960 |+10| 65.9010 |-+18 — 1.1051 62.0735 I+-10| 66.3150 |+18 — 1.5234 — 1.5224 61. 6635 [+10] 66.7370 |+ 8 — 1.9388 60.9310 +11| 67.4585 |+18 — 2.6663 0.5280 |-+11| 67.8640 |-+18 — 3.0706 — 3.0700 60.1235 -+15| 68.2650 |+18 3.4731 +11| 69.0460 |+13 — 4.2496 58.9405 +11] 69.4535 |413 — 4.6588 — 4.6588 8.5330 |+ 11| 69.8640 |+16 5.0680 } Trabant — Jupiterscentrum. | угу» | Mittel. eva) | Ле та) ебал Ph | 48 тт тт 6 59.1380 |+10 -+ 5.6508| -+0.8865 60.6685 |+-10 + 4.1205 BR 62.2830 +9 + 2.5059] --0.8880 ' ' р ' р Gags leté 18 :6405| "0.8822 +-0.8904 +0.8848 0.0040 0.0000 | +0.0002 | -+0:8890 66.9660 |-н 8 — 2.1780| —0.8920 68.5535 |+13 — 3.7621| —+0.8967 58.7680 |+-10 —+ 6.0234] —+1.2591 о +14 + 4.4930 ЕЕ 1.9160 |+ 9 + 2.8759] —1.25800 ésésas 16 — 026581 +1.2566 +-1.2628 | +1.2549 | -+0.0059 0.0000 | +0.0002 | -+1.2610 66.5940 |+ 8 — 1.8044| -+1.2656 68.1790 |-+18 — 3.3911| 1.2677 58.3930 |+ 6 + 6.3960| -+1.6326 59.9235 +15 + 4.8650 Be 1.5350 |+11 + 3.2540| -+1.6361 = 64.6780 [+17 I ae +-1.639$ | -+1.6292 | -+0.0065 0.0000 | +0.0002 | -+1,6359 Scheinbare Decldif: I—Centrum = + 0/2845 f°3 = 0.99295 $2; = —0.00223 АСК 97107 Е » =-15.1248 fs =0,99253 13 = —0.00231 X в=-79 L— » = —15.8417 f’& = 099371 Js = —0.00211 © 244 bd - [о Le = — — а оао сеа ооо Зо LOS Зо NSS Object. 97. mm 62,2361 63.2352 84.3480 16.0775 87.6855 89.7162 62.8445 63.2225 63.6100 62.843 5 63.2200 63.6055 62.8400 63.2165 63.5960 62.8415 63.2200 63.6000 62.8645 63-2435 63.6270 62.8710 63.2405 63.6280 61.6220 61.6205 61.6200 61.6250 61.6515 61.6605 65.4210 65.4145 65.4085 65.4030 65.4235 65.4260 69.0420 60.0435 60.0400 60.0445 60.0705 60.0790 55.6200 55.6170 55.6100 55.6100 55.6300 55.6380 P.-Kr. 0° Scalenablesung. 4 P.-Kr.180° 65.1470 65.1453 44.0328 112.3038 40.6908 38.6642 65.5505 65.1695 64.7790 65.5510 65.1595 64.7850 65.5625 65.1770 64.7920 65.5555 65.1675 64.7915 65.5295 65.1500 64.7720 65.5275 65.1440 64.7670 66.7650 66.7645 66.7695 66.7640 66.7355 66.7260 62.9610 62.9685 62.9755 62.9815 62.963 5 62:9585 68.3415 68.3405 68.3435 68.3395 68.3140 68.3080 72.7660 72.7710 72.7780 72.7790 72.7600 72.7535 Scheinbare Adiff: нЕ Fr ЕЕ о _\O \O \O 00 O0 \0 K— Hi +32 10000} 10000 mm +17 +19|— + 6 +30|— +-30|— +16 +-16 +-16 +16 +16 +16 +16 +16 +16 +17 +17 +17 +17 +-17 +17 +18 +18 +18 +19 +10 +10 +II +19 +18 +18 +19 +19 +19 IS +14 +14 +13 1— Centrum = -+-23'4036 » » » mm [e) 2 5 6 Ge der Aufnahmen. Mittel. mm mm 0.0000 сво —+-21.1116 à } — 47.1534 13° 24” 20 2 —+24.4508 —2 —+-26.4793 — 0.3978 — 0.0184 — 0.0152 ID то. 5 1 + 0.3706 — 0.3986 — 0.0146 — 0.0159 12 26 1 —+ 0.3654 — 0.4061 — 0.0251 — 0.0214 13 40 1 + 0.3671 13% 14” 30° — 0.4020 — 0.0187 — 0.0205 ISWTÉ 1 — 0.3592 — 0.3774 + 0.0018 + 0.0023 16 40 1 = 0.3825 — 0.3732 —= 0.0033 —= 0.0052 НО 1 + 0.3855 Trabant — Jupiterscentrum. Tt—%Xy | Mittel. шего | ии) РВ, | Av cos à mm mm — 1.6160] —1.6008 1—2 — 1.6164| —1.6005 1—2 — 16192] 1.5978 8 EN , hr ar Le? — 1.6149] —1.5935 1.5940 1.5826 | -+-0.0019 0.0010 1.5817 | ; — 1.5866| — 1.5889 1—2 — 1.5772] — 1.5824 1—2 + 2.1858| --2.2010 1—2 + 2.1788| -+2.1947 1—2 + 2.1723| -+2.1937 си et, р 1—2 + 2.1665] +-2.1870 -+2.1907 | -+2.1750 0.0025 0.0010, +2,1715| 1 _5 + 2.1858] -+2.1835 1—2 + 2.1895|.-+2.1843 1 — 3.1944] —3.1792 2 = 7 —3.1778 = — 3.1964] —3.1750| __ Yu u 28 — 3.1923| —3.1718 3.1729 3.1502 | -+0.0036 0.0010 3.1476 1—2 — 3.1666| —3.1689 1—2 — 3:1593| —3.1645 2 — 7.6182] — 7.6030 1 — 7.6222] — 7.6063 il — 7.6292] —7.6078 | _ У: u 2% 1—2 — 7.6297| —7.6092 7.6079 7.5533 | 0.0103 0.0010) —7.5440 | 10 — 7.6104] —7.6127 2 — 7.6030] —7.6082 2 Fu =0.99280 —1° y = +0.00261 — 52.3149 . à } == +-27.2039 fa = 0.99251 —% = 0.00260 x 1,= — 89 = +-29.2361 Refr. = + 14 т Ид == о CH 9-3 fu —0,99282 Ju = 0.00274 1898. Mai 1. Е. Rexz, № 2 wtr#%ct%o Pulkowaer Sternzeit POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1=9=. Mai 1. Рес]. й =. L в. } Scalenablesung. y >-Kr.90° t-il P.-Kr.270° |t-+%k $ mm FAIR 10000! 647424 |10000/10000| ””" 64.7105 |+16| (| 0.0000 64.3420 |-+15] o|+ 0.3714 54.8318 |+16|— 7| + 9.8809 49.3750 +-15.3360 80.5515 — 15.8382 59.5850 + 5.1348 59.9510 + 4.7686 60.3 160 =. 44034 61.1840 + 3.5368 61.5545 + 3.1664 61.9105 + 2.8096 62.7500 + 1.9694 63.1140 — 1.6058 63.4750 + 1.2420 65.9050 1.1856 66.2720 — 1.5512 66.6340 — 1.9152 67.4630 — 2.7578 67.8275 — GITES 68.1890 — 3.4733 69.0310 — 4.3098 69.4095 — 4.6785 69.7635 5.0426 59.2445 + 5.4730 60.8425 + 3.8740 62.4080 + 2.3032 65.5705 — 0.8534 67.1275 — 2.4098 68.6985 — 3.9788 60.8695 + 3.8450 62.4670 + 2.2484 64.0310 + 0.6843 67.1910 — 2.4751 68.7370 — 4.0234 70.3050 — 5.5912 53.6260 + 6.0862 60.2255 + 4.4878 61.7935 - 2.9217 64.9530 — 0.2400 66.5145 — 1.7980 68.0805 — 3.3668 56.2000 + 8.5170 57-7990 + 6.9190 Be + 5.3558 62.5220 + 2.1964 64.0740 + 0.6448 65.6415 — 0.9234 Scheinbare Decldif: JI-—Centrum = + 0:2845 | — » =+ 9.7707 Е— 4 =-+-15.1248 L- ов = —15.8417 Znt2% c+*% 5 тт + 4.7689 “+ 3.1709 + 1.6057 P u Yı—y2 | Mittel. и "ага 7 (оо) a mm —0.7041 +-0.7031 +-0.7025 —-0.6973 +-0.7045 +0.6982 —0.9239 —0.9225 — 0.9214 — 0.9244 —0.9091 —0.9142 —1.3173 —+1.3169 +-1.3160 +-1.3107 +-1.3163 +1.3102 —+3.7481 +3.7481 43.7501 +3.7471 +3.7591 +3.7536 1.5507 3.1143 4.6770 mm +-0.7016 —0.9192 +-1.3 146 —+3.7510 f°5 = 0.99300 fs = 0.99259 f's = 099371 x? < _. — > 081 1 mm 0.0000 0.03 17 0.1595 0.0432 0.0491 ; у— tg sin 1’ тт 0.0000 — 0.3397 + 9.7214 15.2928 —15.8873 Trabant — Jupiterscentrum. -+0'6972 | —-0/0039 —0.9134 | —0.0053 —1.3064 | -+0.0077 +3.7274 | -+0.0185 15 = —0.00252 is = —0.00258 T3 = —0.00244 Bemerkungen zur Aufnahme. Bilder 2. Ph. 0:0000 | —+-0:0002 0.0000 | +0.0002 0.0000 | -+0.0002 —0.0001 | -+0.0002 X is = — 89 31* +0:7013 —0.9185 —+1,3143 —+3.7460 246 92. Scalenablesung. Object P.-Kr. 0° let] Р.-Кг.180° Ctr, | 61.0518 [7000| 64.3186 J 64.0510 |+ 8| 64.3178 TL 85.1740 |— 2| 43.2042 O 16.9018 |-+29| 111.4662 K 88.5140 |— I| 39.8560 L 90.5390 0) 37.8380 #4, | 63.5485 |+10| 64.8405 а | 63.9830 |+10| 64.4030 @о | 64.4295 |+10| 63.9640 Ab | 63.5655 |+ 9] 64.8235 be 64.0055 | 9| 64.3870 bo | 64.4350 |+ 9] 63.9500 #6, | 63.5660 |+ 9] 64.8230 Ce | 64.0255 |+ 9] 64.3795 ch 64.4620 |+ 9| 63.9245 Zdp | 63.5960 |+ 8| 64.7935 de 64.0370 |+ 8| 64.3545 do | 64.4655 |+ 8| 63.9270 Zen | 63.5825 |+ 8| 64.8095 ee 64.0230 |+ 8| 64.3725 eo | 64.4610 |+ 8| 63.9250 %fw | 63.5980 |+ 9) 64.7930 Fe 64.0275 |+ 9| 64.3630 Jo | 64.4590 |- 9] 63.9320 Та | 64.8635 |+17| 63.5160 b | 64.8710 |-+17| 63.5030 € 64.8850 |-+17| 63.4880 Я | 64.8930 |+16| 63.4880 e 64.8845 |+16| 63.4950 Ti 64.8800 |-+17| 63.4960 Па | 61.4060 |+12| 66.9715 b | 61.4150 |-нт!| 66.9615 с 61.4360 |+11| 66.9420 d | 61.4405 |+10| 66.9380 e 61.4400 |+10| 66.9415 if 61.4340 |+10| 66.9420 Ша | 64.8700 |+17| 63.5050 D | 64.8915 |+17| 63.4810 с 64.9090 |-+-17| 63.4600 d | 64.9255 |+16| 63.4505 e 64.9210 |+16| 63.4525 Л | 64.9265 |+17| 63.4495 IV «a | 55.4950 |+ 2| 72.8850 b 55.5075 |+ 2| 72.8730 € 55.5255 |+ ı| 72.8545 @ | 55.5375 | ©] 72.8385 € | 55.5375 |— 1] 72.8450 Л | 55.5325 |— 1| 72.8475 Scheinbare Adiff: I— Centrum = -+23!4036 Ka IE t+k » Е. Renz, 1898. Mai 2. Pulkowaer Sternzeit 3 der Aufnahmen. Mittel. mm ë 1—2 —+21.1170 р AU 1—2 —47.1444 14 17 15 9 —+24.4603 1—2 —+-26.4818 1 = — 0.0745 14 SO 2—3 —+- — — 0.0591 6 16 2 ТЕ = — 0.0456 T2 3 == 14° У 46° *) == — 0.0295 80722 2—3 ar = — 0.0402 91122 2—3 + — — 0.0341 то 16 2—3 — Trabant — Jupiterscentrum. 2—2 | Mittel. 7’ (ex), (иги) Ph. | Ac cos d тт | mm + —0.8820 2—3 + +-0.8769 2 2 BE +0.8718 | +0:8656 | —0:0008 | —o'oo1r | +0:8637 5 A + +0.8686 3 + 0.8598 2 - —2.5747 2—3 — —2.5786 2—8 er —2.5794 | —2.5611 | -+0.0035 | —0.0011 | — 2,9087 a — 2.0 2—3 — — 2.5865 2 + —0.8958 2—3 + —-0.8981 2—3 0.90 2—3 an Inst, -+0.5022 | —0.8958 | —0.0018 | —0.0011 | +0,8929 2 + +-0.9982 2—3 + 0.9063 р >) — —8.4878 2—3 = 5.4862 ME = —8.4862 | = Е к 38 > — 8.4883 8.4874 8.4270 | -+0.0107 0.0011 8.4174 9, — — 8.4808 2—3 — —8.4907 2 12а = 0.99282 =. = —-0.00239 — 52.3149 A À : 2 = -+27.2039 fx = 0.99251 —iy = 0.00237 X 44, = — 8 = +-29.2361 Бей. == == 30 д т Try = O а =12 7.0 Го = 0.99288 I, =-+0.00267 Bilde a ie u u a gi рать de а *) Der Chronometer war nicht verglichen worden, die = 0 angenommene Correction dürfte um höchstens =+ 5° fehlerhaft sein PoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 247 1395. Mai 2. Decl. Scalenablesung. Znt20o+% ER re рад Bemerkungen $ y —1— + — — 195 sin Г y — — 6 sin 1’ zur Aufnah P.-Kr.90° = Р.-Кг.270$ | i-+%k 3 2 ; HAN тт 1000 Er) mm mm mm 64,1634 64.1626 в 0.0000 0.0000 Bilder3. Mondschein, 63.7955 ©] + 0.3701 — 0.0317 + 0.3384 | 54.2712 — 171--.49:8917 — 0.1595 2004322 48.8265 —+15.3336 — 0,0432 —+15.2904 80.0102 — 15.8452 — 0.0491 — 15.8943 58.9690 + 59.3970 + + 4.7820 59.8015 + 60.5515 im 60.9820 + + 3.1976 61.3945 ss 62.0965 + 2 | 62.5290 + + 1.6454 ° | 62.9590 -= 65.2655 65.6910 — — 1.5147 66.1040 == 66.8270 — 67.2600 — — 3.0834 67.6840 -- 68.4150 — 68.8350 — — 4.6566 69.2420 Trabant — Jupiterscentrum. . 7 ^ у | Mittel. | Лаби- уз) | 7-2) (ига) Ph. | AB mm mm 59.7130 SE 79.3293 61.2910 - —0.3214 ASE 2 res —0.3218 | —0.3198 | —0.0019 0.0000 | -+0'0002 | —(0!3215 67.5730 — —0.3222 69.1350 — —0.3118 58.0640 + —+-1.3212 59.6430 + +1.3254 Prat $ 0.1869 PRE +1.3257 | -+1.3174 | <+0.0056 0.0000 | -+0.0002 | -+1,3232 65.9260 — +-1.3242 67.4890 — +1.3348 60.0540 + 4.1070] — 0.6750 61.6370 + 2.5260] —0.6716 “HE LA 0.9692 mo —0.6754 | —0.6712 | —0.0020 0.0000 | <+0.0002 | — 0,6730 67.9265 — —0.6792 69-4960 — —0.6742 55.3630 + 8.8055] -+4.0235 : 56.9465 + 7.2192| -+4.0216 - бо 22 res er +-4.0233 | 3.9981 | 0.0185 | —0.0002 | +0.0002 | -+4,0166 63.2305 -+ 0.9364| -+4.0198 64.7925 — 0.6264] -+4.0302 Scheinbare Decldiff: I-—Centrum = + 0'2845 195 = 0.99286 - 395 = —0.00238 ms » К— » у -- » nn ©? + Il о о A > a = +15.1248 fs =0.99242 is = —0.00249 X 15 = —8:6 Из = 0.99373 Уз = —0.00218 248 99. Scalenablesung. Object. P.-Kr. 0° = P.-Kr.180° mm ОВО mm Ctr. | 64.1768 64.1940 J 64.1760 | 8| 64.1932 I 85.2920 |— 2| 43.0800 (0) 17.0152 |+29| 111.3518 IK: 88.6325 |— 2| 39.7380 L 90.6590 ©] 37.7105 2% ay | 63.7235 |+10| 64.6680 ас | 64.1355 |+-10| 64.2525 Ay 64.5480 |+10| 63.8400 2% by | 63.7430 |+ 9| 64.6480 b, 64.1545 | 9| 64.2310 b, 64.5700 | 9| 63.8200 7% Cyw | 63.7510 |-+ 9| 64.6380 CG 64.1640 |+ 9| 64.2310 en 64.5785 |+ 9| 63.8100 2% dy | 63.7770 | 8| 64.6135 de 64.1870 |+ 8| 64.2c09 do | 64.5975 |+ 8| 63.7980 Hey | 63.7780 [+ 8| 64.6080 ес 64.1905 |-+ 8| 64.1965 ео 64.6045 |+ 8| 63.7885 %]ь | 63.7555 | 9] 64.6340 fe | 64.1700 |+ 9] 64.2145 о | 64.5890 |+ 9| 63.8030 Та 65.6850 |-+ 11| 62.6905 b | 65.7055 |+11| 62.6725 с | 65.7130 |+11| 62.6680 а | 65.73c0 |+10| 62.6490 e 65.7350 |+10| 62.6450 Л | 65.7085 |+11| 62.6705 Па 62.3015 |-+11| 66.0770 b 62.3220 |+10| 66.0570 с | 62.3290 |10| 66.0500 d | 62.3450 |+ 9| 66.0320 e 62.3465 |+ 9| 66.0275 f | 62.3220 |+ 9) 66.0570 II Bedeckt. IV a 60.2310 |+17| 68.1450 b | 60.2495 |+16| 68.1305 с | 60.2600 |-+15| 68.1200 d | 60.2750 |+14| 68.1030 e 60.2800 |+14| 68.0980 f | 60.2585 |+14| 68.1210 Scheinbare Adif: F. Renz, 1898. Mai 16. AR ++ Pulkowaer Sternzeit 3 | © || ©> ©2 O9 Я © N © N TRES © | oo O2 CA ©? D 19 © | co Le t+k der Aufnahmen. Mittel. mm mm 100001 10000 п var + 8 Ге) 0.6000 —=21|— 2|+21.1132 ‚Уфе, + 6]-32| —47.1554 15 16 30 31| — 5] 24.4537 +29|— 6| 26.4809 +17 — 0.464C + 9 — 0.0498 — 0.0504 IS D а» + 9 —= 0.3626 : +16 — 0.4442 8 — 0.0296 — 0.0301 A‘MEA? + 8 + 0.3836 +16 — 0.4352 + 8 — 0.0248 — 0.0224 ОР + 8 — 0.3929 15° 6” 12° +17 — 0.4101 + 9 —= 0.0020 — 0.0001 97 + 9 + 0.4083 +17 — 0.4068 +9 —= 0.0056 —= 0.0051 я 50 + 9 + 0.4166 +12 0.4308 +10 — 0.013; — 0.0143 8 48 +-IC —= 0.4016 Trabant — Jupiterscentrum. ae | Mittel. Para) Ja un) Ph. | Aa cos 5 mm mm + 0 + 1.5060| -+1.5564 + 9 + 1.5252] +1.5553 A: = er en +1.5508| +1/5399 | —o!oo2ı | —0!0016| +1!5362 +10 + 1.5536| 1.5485 +11 + 1.5276] -+1.5419 и — 1.8792| — 1.8288 +10 — 1.8589] — 1.8288 и. ЕЕ в De —1.8340| —1.8211 | +0.0032 | —0.c016 | —1,8195 +11 — 1.8320] — 1.8371 +1) —: 1.8590] —1.8447 +19 — 3.9485] — 3.8981 +19 — 3.9320] —3.9019 als 2 de Er — 3.9032) —3.8757 | +-0.0068 | —0.0016 | — 3,8705 +18 — 3.9006] — 3.9057 +19 — 3.9229] —3.9086 1— Centrum = -+23'4039 «19 = 0.99275 — = +0.00257 0— » = — 52.3149 K— » = +-27.2046 fa = 0.99240 —iy = -0.00252 "= L— » = +-29.2369 Refr. = + 63 h m Try = О ах==12 4.3 fl = 0.99295 Л. = -+0.00315 L e. Decl. т. Scalenablesung. x Ynt ach”; и ? 2 : Bemerkungen | у стати = = tgd sin 1’ y — = 95 sin 1’ zur Aufnahme. L-Kr.90° tt P.-Kr. 270° |t-+% $ тт тт | тт 642023 [000 647713 [0000/1000 MM ee 2m nm 64.2015 + 8] 64.1705 |+ 8 о 0.0000 0.0000 0.0000 Bilder 3. 64.5660 |+-26| 63.8045 |-+15| 0] + 0.3660 — 0.0317 — 0.3343 Leichte Wolken. 1 70.0995 |+29] 54.2712 |+20]— 7| + 9.8986 — 0.1595 + 9.7391 79.5292 |+20) 48.8365 |-+22|— 4 -+15.3306 — 0.0432 +-15.2874 48.3515 |-+32| 80.0152 |--18|-= 4] —15.8460 — 0.0491 — 15.8991 69.3725 +13] 59.0220 |-+-10 + 5.1596 Bilder 3—4. 68.9780 |-+13| 59.4170 |-+10 + 4.7654 68.5765 |-+13| 59.8110 |-+10 + 4.3676 67.7850 |+ 8| 60.6145 |-+10 + 3.5698 1 67.3845 | 8| 61.0020 |+10 + 3.1758 7 66.9860 |+ 8] 61.4030 |+10 + 2.7761 1 66.2205 [10] 62.1770 |+ 9 + 2.0065 ‚65.8220 |-+10| 62.5670 |+ 9 + 1.6122 1 65.4240 |10| 62.9650 | 9 + 1.2142 Я 63.0660 |+ 9] 65.3235 |416 — 1.1444 62.6660 | 9] 65.7180 |+10 — 1.5414 62.2780 + 9] 66.1130 |+10 — 1.9328 61.4870 +10] 66.9060 |- 8 — 2.7247 61.0895 |+10| 67.2960 |+ 8 — 3.1184 60.6980 |-+10| 67.6920 |+18 3.5127 | №5 9.9205 |-+14| 68.4660 |+13 — 4.2880 59.5270 |+-14] 68.8670 |-+13 — 4.6852 59.1290 |+10| 69.2620 |+13 — 5.0820 Г Trabant — Jupiterscentrum. И У:—У% | Mittel. [изу EZ (@r—23) Нели у тт тт 68.2820 |-н18| 60.0910 |+15 + 4.0804| —0.6838 66.6980 | 8| 61.6845 |+10 + 2.4914] —0.6825 65.1400 |+16| 63.2380 |+10 — 0.9360] —0.6750 | _ RT Be, р r rn, ML dl sors nr ER Ah 06: 0.6784 0.6745 0.0027 0.0000 | +0:0004 0:6768 60.4110 |-+14| 67.9665 |-+-19 — 3.7933] —0.6747 58.8420 |+10]| 69.5360 |+17 — 5.3626] —0.6775 69.9790 |-+17| 58.4000 |+ 5 + 5.7748] +1.0106 68.3875 |-+19| 59.9910 |+14 + 4.1832] -+1.0093 6.8300 |+ 9] 61.5500 |+ 9 + 2.6247| 1.0137 | 410126 | +1.0068 | -+0.0032 0.0000 | -+0.0004 | -+1.0104 .6795 | 9] 64.7010 |+16 — 0.5264] 1.0131 < 1 у : 62.1030 |+10| 66.2750 |190 — 2.1013] -+1.0173 60.5320 |-+11| 67.8475 |+18 — 3.6734] -+1.0117 Bedeckt. Й 71.1175 |-+13| 57.2660 |+-10 + 6.9106] -+2.1464 | Br +17 32.8530 +11 + 5.3230| -+2.1491 | 67.9690 |+19| 60.4125 |+15 + 3.7632| <+2.1522 < , nal 63.5660 Le à 2 Han 129 -+2.1484 | -+2.1360 | +0.0069 0.0000 | -+0.0004 | -+2,1433 "63.2250 |+10| 65.1450 |+-17 — 0.9706| -+2.1480 61.6675 |+10| 66.7150 |+ 9 — 2.5390] -+2.1461 Scheinbare Decldif: I- Centrum = + 0/2843 f° 5 = 0.99296 195 — —0.00222 — » = + 9.7712 ь : £ К » =-+H15.1250 fs = 099247 is = —0.00241 X в=-—83 L— » = —15.8421 1’; = 0.99426 Js = —0.00177 dy—=-+1° 93 Ban. Физ.-Мат. u POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 1598, Mai 16. Отд. 249 82 Object. [en — bd -ч -ч ыы = Зоо SR So LOS AS NR Scalenablesung. mm Innnn 63.5310 63.5302 84.6495 16.3770 87.9905 90.0075 63.1175 63.5330 63.9520 63.1295 63.5580 63.9810 63.1005 63.5235 63.9395 63.1235 63.5355 63.9475 63.1155 63.5365 63.9540 63.1140 63.5270 63.9495 Bedeckt. 64.5980 64.6130 64.5880 64.5820 64.5875 64.5765 66.1830 66.1950 66.1730 66.1795 66.1800 66.1675 55.3655 55.3855 55.3605 55.3650 55-3690 55.3590 5 = NO NO O O9 00\0 CO OO\D \O ЕЕ Fre НЕЕ 64.8411 64.8395 43.7272 111.9908 40.3788 38.3628 65.2690 64.8570 64.4395 65.2535 64.8310 64.4005 65.2835 64.8730 64.4430 65.3685 64.8555 64.4355 65.2770 64.8515 64.4335 65.2800 64.8610 64.4395 63.7800 63.7700 63.7975 63.7950 63.7925 63.8055 62.1885 62.1740 62.2010 62.1945 62.1960 62.2080 73.0155 72.9990 13.0235 73.0200 73-0175 73.0245 Scheinbare Adif: *) Die Platte ist vom Mondlicht geschwärzt. P.-Kr. 0° | til P.-Kr. 180°| + Е. Renz, 1898. Mai 19. № 2 pt + % 0 Pulkowaer Sternzeit 2 der Aufnahmen, Mittel. mm mm 10000] 10000 mm Ken +16| о 0.0000 1—2 *) —=19|— 2] +21.1150 ь WERE fd, 2 + 6|4-32] — 47.1475 14 22 20 2 +31|— 5| +24.4588 2 —+-291— 6] +-26.4753 2—3 +17 — 0.4160 +17 — 0.0073 — 0.0041 14 0) 130 3 | +17 + O.4110 +16 — 0.4072 . +16 — 0.0182 + 0.0187 Пт 8 +16 —= 0,4450 +16 — 0.4368 +16 — 0.0200 — 0.0179 132012 3 4-16 “+ 0.4030 14 13” 43° А +17 — 0.4178 Dante +17 — 0.0054 — 0.0042 14622 : +17 + 0.4106 +17 — 0.4261 9 +17 — 0.0029 — 0.0047 ONE +17 —+ 0.4148 18 — 0.4284 3 +18 — 0.0124 — 0.0104 102830 +18 0.4096 Trabant — Jupiterscentrum. Lt— Lo | Mittel. Лаз] Лии) РИ, | Aa cos d mm mm + 8 —= 1.0645] —+-1.0686 2—3 + 8 + 1.0770| 1.0583 3—4 +8 + 1.0508| +1.0687 ' #04 pv р 2—3 ae Dr ue +-1.0596| -+1'0520 00009 00018 | +1:0493| ; == о + 1.0529] +1.0576 3 +10 —+ 1.0409] +1.0513 3 +9 + 2.6524] +2.6565 3 +9 + 2.6656] +2.6469 4 .6 .6 3 ны = ere ne +2.6520| -+2.6331 | —0.0027 | —0.0018| +2,6286| 5, +10 + 2.6470] -+2.6517 3 +11 —+ 2.6358] -+2.6462 2—3 +16 — 8.1706| —8.1665 3 +14 — 8.1523] —8.1710 3 unterexpon +14 9. О ‘2 a gt 3—4 +13 — 81731] —8.1689 8.1665 8.1082 | +0.0097 0.0018 8.1008 | > | —13 — 8.16991 —8.1652 3 ищегехроп! +14 — 8.1784] —8.1680 5 | I—Centrum = +23'4040 Ve 099279 —19, = +0.00222 = — —52.3143 К— » = +-27.2047 fu = 0.99248 —iy = 0.00219 X dy =-75 L— » = -+29.2370 Refr. = + 33 в т Try = O ay = 12 3.9 flo = 0.99286 Jy == 0.00252 nn nn = => => = = m POoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 251 ВКТ. 90°) tek | P.-Kr. 270° |#+% 64.2171 [10000 64.2162 64.5770 74.1265 79.5372 D 59.9335 59.5370 59.1400 f Bedeckt. Scheinbare Decldiff: mm 64.1588 |+ 8 63.8002 |+15 1595. Mai 19. mm 61.1596 10000] 10000 о 0.0000 ©] + 0.3602 54.2436 |+20]— 7| + 9.9124 48.8312 |+22|— 4 80.0115 |+18]+ 4 59.0400 |+-10 59.4360 59.8580 60.5610 60.9740 61.3720 62.1760 62.5960 62.9910 65.2910 65.7015 66.1040 66.8610 67.2675 67.6790 68.4600 68.8650 69.2545 59.7630 61.3235 62.9400 66.0465 67.6160 69.2000 60.4980 62.0320 63.6510 66.7625 68.3300 69.9180 55.5985 57.1310 58.7510 61.8620 63.4330 65.0200 He ESS » » » III +44 +++ #44 Al Les) Ye ТЕ I—Centrum = + 0.2843 697713 =-+-15.1250 = — 15.8422 dy = +12 10/6 Decl. 2 1 2 ; Bemerkungen — tgdsin 1/ y — > tgù sin 1’ zur Aufnahme. Bilder 3. Bilder 3—4. Wind. 4.7294 Himmelsgrund sehr hell. 3.1987 1,5791 1.5311 — 3.0999 — 4.6902 Trabant — Jupiterscentrum. 2 T Yt—Y2 | Mittel. Ir "s(yı—Y2) | Та (1—2) | ета) Ph. | 45 тт тт —0.3582 —0.3596 — 0.3551 — 0.3525 — 0.3523 —0.3485 —1.0695 — 1.0727 — 1.0715 — 1.0699 — 1.0688 — 1,0662 —0.3544 | —o!3521 | —0!0018 0/0090 | -+0!0004 —0.0045 0.0000 | -+0.0004 —3.8370 3.8329 -+3.8327 —3.8344 3.8305 3.8331 0.0140 —0,0002 | -+0.0004 | -+3,8243 f° 3 = 0.99299 15 =— 0.00193 fs = 0.99254 is =— 0.00205 X в=-—70 f's = 0.99387 TJ = —0.00171 р рае - дывнме Kanne nova soie ИРИНА dat ИНО CHÈRE a it ed FPS LOT К CASTRES | Sr дм } à Li р И ны al ht, ar a 4 |. | BERN Lee da | 555 SE GEBETE LCR 1 AD à AYSS 41.2770 POSITIONEN DER JUPITERSTRABANTEN WÄHREND DER OPPOSITIONEN 1891—1898. 254 F. Renz, Opposition 1891. Trabant — Jupiterscentrum. Mittlere Aberra- № der Trabant. Pulk. Zeit. tionszeit. Platte. Zahl der Aufnahmen. September 22*) | то“ 37” 33° September 22 September 24 October October October October October October November 2 *) Für die durch Cursivschrift bezeichneten Daten wurden die Plattenconstanten vorhergehenden oder nach- folgenden Abenden entnommen. POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. November November November December December December December 19 ‘ December 22 August Mittlere Pulk, Zeit. Trabant — Jupiterscentrum. +2 + I T5 — 2 — 2 — 2 73 ee. — 1 F3 + 4 9 2.99 52.63 18.28 12.98 6.14 59.60 24.09 27.32 27.97 18.90 40.23 12.36 41.53 49.96 14.16 26.80 53.21 23.20 9.99 43-22 31.34 25.21 7.59 57-96 Aufnahmen. Aberra- tionszeit. X der Platte. 256 F. Renz, Trabant — Jupiterscentrum. Mittlere Aberra- Ns der Trabant. Zahl der Aufnahmen. Pulk. Zeit. tionszeit. Platte. August August September September September September September September September September October October October 17 Mittlere Aberra- X der Pulk. Zeit. tionszeit, Platte. Zahl der Aufnahmen. October October October October November November November December © op м B Qt Où Qt December December 1893. Januar Januar Februar 14 Зап. Физ.-Мат. Отд. 33 258 Г. Rexz, 5 : я Mittlere Trabant — Jupiterscentrum. & Е АВЕС № der =" Pulk. Zeit. A За tionszeit. | Platte. < Februar 14 7" 38” 48° III +0’ 5505 0097 | 5 45" 20” 15) IV + 5 45.65 -+2 41.26 März 11 8 10 2 I + 1 34.86 +0 38.56 5 47 43 17В II +2 28.40 НТ 337 III — 1 13.92 — 0 17.66 ТУ —4 58.95 — 2 16.68 Opposition 1893 — 1894. October 20 13 44 50 I +2 491 + 0 21.52 5 34 23 18 А III +2 18.42 —— 0 48.88 IV — 5 32,25 — О 41.69 October 21 тт 58 48 I — 1 51.62 — 0 18.28 6 34 19 18B II +3 49.28 +0 48.70 II +5 44.02 + 1 19.81 IV —2 3.10 +0 6.11 October 27 12 31 49 I +2 25.88 +0 30.80 4 33 59 18 C II — 1 22,83 —0 3.86 Ш + 1 20.79 +0 39.10 IV +9 37.27 + 1 49.64 October 30. 12 49, (53 II — 0 41.39 — 0 43.70 б 33 St 180 II +1 47.33 +0 1.99 IV — 3 48.55 — 0 47.03 | October 31 9 26 25 I -но 40.86 +0 035 5 33 49 19 A II НО 49.92 +0 25.29 II — 2 51.78 — 0 57.30 | IV — 4 13.20 — Г 28,21 November 7 12 бо [51 II +0 55.77 +0 27.35 5 3355 19 В ш —2 44.37 — © 56.74 18% — 0 26.25 +0 28.74 November 8 II 9 40 IT НЗ 35.28 — +0 43.06 5 23 033 19C III —6 1.60 — Г 27.10 Ay: + 3 29.12 НТ 20,72 November 9 й 45. 115 IL — Г 20.16 — 0 32.97 5 33 33 19D ш — 5 30.21 — 1 3.89 IV + 6 36.70 +1 58.53 November 13 12 32/38 I — 1 39:58 — 0 16,85 5 33 29 20 A II — 3 55.90 —0 56.79 II +3 9.97 +0 23.80 IV —+ 8 47.44 + I 41.41 | 3 - Mittlere Е Trabant — Jupiterscentrum. Е Е уе Kin 1893. = =а Pulk. Zeit. Я вх Ad & = tionszeit. Platte. 4 November 15 114 24” 43° u + 3’ 46:37 + 0/ 49.21 5 33” 28° 20 B II — 5 48.46 — 1 29.12 13 +1 58.26 —0 6.56 December 5 8 34 33 I + 2 24.44 +0 36.62 5 35: 56 20 C U — 2 22.93 — 0 25.38 III -+0 57.38 —0 7.32 IV — 9 26.18 — 2 39.44 December 17 4029 +0 u +3 43.47 +0 56.75 5 34 41 20 D ш +4 52.78 НГ 27.47 IV +6 44.53 НГ 20.64 December 18 & 24 12 I — 1 6.54 — © 24.41 4 34 45 21 A II — 1 17.70 —O© 33.97 ш +5 44.43 НГ 22.99 IV +3 7-93 +0 18.54 1894. Januar 24 7 91 46 I — 0 33.48 +0 2.31 5 38 44 21 В III +1 7.59 +0 0.66 IV — 8 14.47 — 2 26.32 Februar 2 8 45 16 I — 1 5.05 — 0 22.63 5 39 55 22 A Ш —5 7.04 — Г 23.25 IV +8 53.49 + 2 28.41 Februar 7 8 34 48 I +1 483 но 11.69 5 | 4 35 22B II — 0 31.91 —0 33.32 III +2 19.21 +0 21.73 3 IV — 1 30.70 —0 14.18 Februar 8 19 53 20 Il +3 10.66 +0 51.79 4,5 40 44 22 C III — 2 23.62 — 0 52.03 . ТУ —4 4.31 — 1 26.90 Februar 9 8 29 44 I — О 28.31 — О 13.45 5 40 51 22D II — 4 50.94 — I 20.36 IV — 6 27.98 — 1 59.38 Februar 22 74 28 I | — 12720 — 0 18.21 5 42 36 23 A u +2 16.30 +0 41.72 III —0 22.75 — О 21.32 IV +4 59.40 +0 56.77 April 10 9 28 5 I +0 32.68 +0 1.30 5 48 о 23 В II +2 8.83 +0 19.33 III + 1 55.06 +0 34.0 IV +7 22.79 + 1 35.88 April 13 9 35 27 Г | +1 21,61 +0 18.13 5 48 16 23 C IT +2 41.91 +0 33.30 IV +5 21.45 + 0 47.96 88* 260 Е. Renz, Mittlere Aberra- № der Pulk. Zeit. tionszeit. Platte. Zahl der Aufnahmen. December SUR : | December } Е December December Januar Januar Februar PosITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 261 Mittlere - Trabant — Jupiterscentrum. Midi Mie Ort der Aufnahme. Pulk. Zeit. tionszeit. | Platte. Au AG я ых 5: == P-| oJ <: = März 19 9 та I +2’ 6.21 —0o 0.22 5 | 42" 25° | 26D II — 2 17.27 +0 4.25 II — 1 52.93 +0 9.10 IV — 8 27.69 — 0 13.31 März 22 8 29 58 I — 0 50.23 +0 2.56 5 42 49 27 À u — 3 9.74 —O 3.43 ИТ +4 7.99 — 0 7.04 IV — 6 55.27 —0 6.26 Opposition 1895 — 1896. November 27 3 TA 24 I +1 3.77 — 0 16.63 5 39 31 28 A H. II +2 3.05 — 0 36.33 ш +5 3:20 | —1 29.14 IV —9 12.52 +2 39.19 November 28 13 52 45 I — 1 51.13 +0 33.13 5 39 24 | 28B H. II +2 41.09 —O© 50.48 ш +4 7.24 — 1 15.71 IV — 8 45.91 + 2 33.84 December 27 12 39 37 I +2 4.79 во 35.19 4 | 36 41 | 36A г. ш +3 8.17 — 0 56.62 IV — 2 33.99 +0 36.83 December 27 13 I 28 I +2 7.24 — 0 35.89 4 36 41 36B 12 II +3 4.58 — 0 55.67 IV — 2 37.10 +0 37.48 1896. Januar 1 12 8 46 IL —2 3.58 +0 37.95 6 36 23 37 PR; ш + 3 27.14 —0 55.97 IV — 8 30.33 +2 23.66 Januar 11 12/39 9 I —2 134 +0 32.62 5 35 15711 80 H. IL — 3 38.06 +1 0.68 IV + 3 31.29 — 1 2.93 Januar 15 12` 34 ! I — 0 53.26 --0 15.21 5 35 so | 29A H; II — 2 53.53 +0 49.64 Ш + 2 24.58 — 0 36.34 ГУ —9 28.42 + 2 26.76 Januar 17 FPT US 7 I +0 31.27 — 0 7.27 5 35 48 29 В H. II +2 0.45 — 0 35.68 III + 4 56.26 — 1 22.01 IV — 9 44.87 +2 35.03 Januar 20 10 38 41 I — 2 15.10 ‚ +0 35.96 6 35 46 | 38 2. II +3 37.13 — 0 58.87 ш — 5 50.33 +1 33.89 IV — 1 17.06 +0 27.01 1896. Januar Januar Januar Januar Januar Januar Februar Februar Februar Februar Februar Februar 23 26 30 Pulk. Zeit. 10 12 II II 12 12 10 Mittlere SI 53 37 45 58 21 27 37 32 37 19 48 58 45 49 34 42 12 30 Trabant. Г. Renz, Trabant — Jupiterscentrum. Ac AG — 2! 15757 + 0’ 35/90 +3 35.12 2005930 — 5 47.00 + 1 32.78 — 0 58.62 -+ О 20.26 +1 7.67 —0 19.18 +1 57.118 — 0 29.30 5 16.69 — 1 22.25 +8 42.53 — 2 10,99 + 1 34.76 —O 24.71 — 1 25.49 +0 24.85 — 3 25.72 0750.19 + 8 36.95 — 2 16.11 — 1 53.36 + O 29.03 +3 29.42 —0 54.74 — $ 49.45 + 1 30.86 +6 2.60 a5 — 1 54.85 +0 29.36 + 3 30.13 —O 55.04 — 5 49.52 + 1 30.85 +6 1.75 — 1 37.10 + I 0.76 — 0 16.90 +1 55.93 — 0 28.10 — 5 10.82 — 1 18.65 — 5 37.08 + I 18.11 — 2 49.12 + 0 42.50 +2 13.92 — О 35.08 —10 0.15 +2 27.22 — 2 49.94 +0 42.43 +2 2.77 — 0 35.12 = 10.70.23 + 2 26.95 — © 43.27 +0 9.69 —3 161 + 0 45.49 + 1 48.42 — 0 31.58 =10 73.17 +2 27.56 — 1 55.19 +0 28,58 +3 27.93 - —0 53.04 — 46.69 + 1 27.61 —9 7.60 + 2 18.39 — 1 56.78 + 0 28.96 + 3 28.66 — 0 53.34 — 5 46.92 +1 27.70 —9 7.01 +2 18.08 + 2 13.00 —0 33.27 +0 32.83 —0 11.69 — 4 30.3$ : -FI 10.99 Zahl der Aufnahmen, ot Aberra- tionszeit. 35” 35 35 35 35 35 35 35 35 35 35 35 46 46 46 47 47 49 52 52 52 55 55 57 № der Platte. 29 C 29 D 30 А 40 A 40B 30B 41 A 41B 30C 42 A 42B 43 En © TT + = о Aufnahme. Le Po8ITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHNEN. 263 Trabant — Jupiterscentrum. Mittlere АЪегга- | № der Pulk. Zeit. tionszeit, | Platte. Zahl der Aufnahmen. Ort der Aufnahme, Februar Februar Februar Februar Februar Februar Februar Februar Februar 19.93 Februar к 30.87 51.62 21.65 19.68 Februar ù 26.50 9.22 1.68 36.94 PNEU EE PE ee 264 Г. Renz, Trabant — Jupiterscentrum. Mittlere Aberra- | X der Pulk. Zeit. tionszeit. | Platte. Zahl der Aufnahmen. Ort der Aufnahme, Februar Februar Februar ь À д | Februar Februar Februar Februar Februar Februar , 1896. | | März | März März März | März März März März zu | März März März 11 11 14 16 16 16 24 24 29 30 | Pulk. Zeit. 11 10 Зап. Физ.-Мат. Отд. 54 34 40 33 49 47 Mittlere 47 42 34 28 41 Trabant. Trabant — Jupiterscentrum. Au A Zahl der Aufnahmen. Aberra- tionszeit. 38" 38 38 38 38 39 39 39 40 40 40 40 20 33 33 53 39 39 47 53 A 32 В 54 A 54 В 32 С 55 А 55 В 56А 57 А 34 Ort der Aufnahme. 266 Е; Renz, Trabant — Jupiterscentrum. Mittlere Aberra- Pulk. Zeit. tionszeit. Ort der Aufnahme. я 5 © rs & ='e аа NS а | E POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN ÄUFNAHMEN. 267 - — 1 m 5 © Mittlere Е Trabant — Jupiterscentrum. Е Е diet UE ds ЗЕ 1896. A 5 | Is a ` Pulk. Zeit. |: A Ad Er: tionszeit. | Platte. 53 < April 19 9% 37" 45° I — 0/ 5213 + of 11.21 4]. 44" 24 1.629 À Р. II — I 35.98 +0 20.63 II + 4 6-45 — I 0.04 IV +5 47.08 — 1 23.79 — © 55.44 +0 12.33 u — 1 38.42 +0 21.71 ` ие +4 5.34 — 0 59.56 IV Ну 45.50 — I 23.26 Opposition 1897. _ 1897. ‘Februar 268 F. Renz, Trabant — Jupiterscentrum. ÄAberra- Mittlere tionszeit, Ort der Aufnahme, Pulk. Zeit. Я 5 € = "à Е NS < POSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 269 Е Mittlere - Trabant — Jupiterscentrum. = = at Га + | са 7 Pulk. Zeit. за tionszeit. | Platte. 53 > < ! | ' April 15. | 12 21” 52° I — г’ 18.61 +0’ 31751 5 | 39" 46° | 64A H. м II + 2 47.44 — 1 12.69 IT — 4 48.70 +2 0.22 ‚ IV — 3 24.34 + 1 15.87 2 April 18 10 54 0 I +1 54.16 —0 4741 6 | or $ 64 В Н. ОШ + 3 44.74 — 1 37.41 а IV +-5 21.85 — 2 18.96 4 Г ? April 23 10 20 35 I + 1 23.89 = 0 32:00 6 | 40 40 | 85 P. A Il +o 58.00% — 0 25.98 4 II — 4 1.81 +1 37.24 IV + 4 24.15 — 1 41.27 10 29 8 I + 1 22.25 — 0 32.03 5 | 40 40 | 64C H. I +1 0.33 —0 27.97 II —4 0.05 +1 36.16 IV +4 23.30 — 1 41.83 10 41 14 I — 1 32.71 о 38.71 5 | 40 47 | 64D H. IT — 2 51.86 + 1 12.76 II — 0 35.93 +0 8.83 IV +1 24.32 — 0 27.86 10 36 38 I + 1 51.05 — 0 46.82 5 | 40 54 | 65A В In +3 12.20 — 1 24.15 IV | —1 43.08 +0 48.41 10 24 28 I — г 48.19 +0 43.20 5 At. 72 65 B H. IL +2 54.47 — 1 14.03 III + 4 42.43 — 1 57.56 IV — 4 34.52 +1 57.17 10. 26 1 I — 0 55.85 +0 19.96 5 4т 16 65 C H. uU — 2 35.47 +1 2.86 TIL — 1 3.45 +0 30.60 IV —8 2.42 + 3 16.93 I1 27 53 I — 1 5543 +0 24.04 5 | 42 32 | 65D | H. И — 2 22.49 +1 1.80 II — 1 39.32 +0 36.03 IV +7 22.51 — 2 58.84 it 26 54 I — 0 27.25 +0 12.79 5 43 26 66 A H. I — 1 59.72 о 52.67 UI — 2 11.23 +0 49.79 IV — 7 48.08 + 3 11.82 12 10 44 I — 1 36.27 НО 40.25 5 43 42 66 В H. d II +2 35.33 —1 7.18 ш +4 11.99 — 1 47.02 IV — 6 15.92 + 2 30.22 22, 3-25 I + 1 44.84 — 0 44.33 5 43 50 66 C H. II + 3 44.12 — 1 31.66 IV — 4 9.43 + 1 36.29 INA. 57 I + 1 13.67 — 0 29.62 5 44 6 66 D H. Ш — 255.79 - +1 16.73 270 F. Вани, | | Opposition 1898. Trabant — Jupiterscentrum. Mittlere Aberra- | N der tionszeit. | Platte. nent nn ha a Ti де Zahl der Aufnahmen. Ort der Aufnahme. Pulk. Zeit. A А 2 38° + 0/ 35/87 29.90 24.59 57.02 5.68 22.49 — 0 46.97 29.92 45.89 41.00 34.04 25.42 11.80 29.98 22.90 21.55 55-43 $3.02 35:97 41.95 10.02 15.52 53-78 30.16 42.94 3.32 0.59 12.90 23.86 53.35 33.25 43.31 20.50 18.15 12.85 53.34 15.66 38.15 + 1 44.87 PoSITIONEN DER JUPITERSTRABANTEN NACH PHOTOGRAPHISCHEN AUFNAHMEN. 271 | : u $ Маме = Trabant — Jupiterscentrum. Е Е Atari IS de Е Е 1898. 5 | sd Pu)k. Zeit. Ё АБ АЗ Œ tionszeit. | Platte. 53 мы I — 173491 + 0' 42:08 6 | 38" 38° | 97 а II +2 10.31 —0 55 т II — 3 8.88 + 1 18.86 IV — 7 32.70 + 3 44.76 24 33 I +0 51.83 — 0 19.29 6 38 43 98 à Il — 2 33.55 + 1 19.39 | 1091 +0 53.58 — 0 40.38 IV; | — 825.128 +4 1.00 27 46 I + 1 32.19 — 0 40.61 6 40 4 99 в: U — 1 49.19 +1 0.62 IV — 3 52.28 +2 8.60 23 38 u +1 2.97 — О 21.21 6 | 40 23 100 B III +2 37.75 — 1 4.03 IV — 8 6.13 +3 49.46 ———— PRESENTED 30 ÀUG. 1907 Fr Pi EN KR ER LE AT Ann. oe ; : à 4 DEA ET 7 | ist | Faces ag и и к hs RTS 4 | | NER Г N ech < ao PA Е * > в. L ” < IX FR FA L 1 STAR 1 > % 30 Aut. QU Г _ ЗАИНСКИ HMITEPATOPCKON ARALEMIR HAYKL. | ео: MÉMOIRES | DE L'ACADÉMIE IMPÉRIALE DES SCIENCES DE ST.-PETERSBOURG. | | УЕ SERIE. | хе "mo ФИЗИКО-МАТЕМАТИЧЕСКОМУ ОТДЪЛЕНТЮ. | CLASSE PHYSICO-MATHÉMA TIQUE. 4 | Toss XIII. № 2. Volume ХИТ. № 2. | SUR UNE SERIE DANS LA THÉORIE Dis ÉQUATIONS DIFFÉRENTIELLES LINBAIRES DU SECOND ORDRE À À CAEN де РАВ A. Liapounoff. | (Lu le 25 septembre 1902.) С.-ПЕТЕРБУРГЪ. 1902. ST.-PETERSBOURG. | Hpoxaeren y комисс!онеровъ ИмпеРАТОРСКОЙ Commissionnaires de l'Académie ImpÉRIALE des %à . Акадеши Наукъ: Sciences: и. Глазунова, M. Эггерса и Коми, и К, Л. Риккера | J. те M. Eggers & Cie. et С, Ricker à St.-Péters- 1 = 88 С.-Петербург, bou | N I ae pie C. -Петерб, Москв$, Варшав% и | У, Karbasulkof à St-Pétersbourg, Moscou, Varsovie et RTE я, Lies въ С. Петербург n КевЪ, - Oglobline” à St-Pétersbourg et Kief, RS О "|" М. В, Клюкана въ МосквЪ, = | М, Klukine à Moscon, _| В, I. Pacnonora въ Oxecck, | т Raspopoff à Odessa, . Il. Kummean въ РигЪ, - IN. Kymmel à Riga, С. ; 11 3 __ Фоееъ (Г. Ге) въ Лейпциг%, | Voss’ Sortiment (6, Haessel) à Leipsic, | “doser | и Комп. въ ЛондонЪ. Luzac & Cie, à Londres. ая Цьна: 1 Руб. 20 коп. — Prix: 3 Mark. 1 | SANHCKA ИМПЕРАТОРСКОЙ ARANEMIR HAYRB. MÉMOIRES DE L’ACADEMIE IMPERIALE DES SCIENCES DE ST.-PÉTERSBOURG. VIEIL: SERIE. ПО ФИЗИКО-МАТЕМАТИЧЕСКОМУ OTIAEJEHIW,. | CLASSE PHYSICO-MATHÉMA TIQUE. Tome XIII. № 2. | Volume XIII. № =. к | SUR UNE SÉRIE | 4 1 DANS LA THÉORIE | DES EQUATIONS DIFFERENTIELLES LINEAIRES DU SECOND ORDRE À COBFFIGIENTS PÉRIODIQUES. PAR А. Liapounoff. (Lu le 25 septembre 1902.) et nn — —— зн USÈ à (à © FA ch 2 Rp 1) I 1 ou A? = 1; car c’est cela ce qu’il faut connaître avant tout, lorsque on veut savoir si les solutions de l’équation proposée sont des fonctions limitées, c’est-à-dire telles que leurs modules restent au-dessous de certaines limites, quel que soit +. | Cette question peut être rattachée à la considération de l’expression de ) (7 + по), n étant un entier quelconque. Cherchons cette expression. La relation (2) montre que ф (x + по) est une solution de’ l'équation aux differences finies Ynız — 24Y,,, м CG 0. Or, si l’on pose pe (4+V4—1) —(4— FAR a 2VA2— 1] le cas de 4? — 1 étant considéré comme cas limite, 7, vérifiera la même équation, et d’ailleurs 7, et 7,_, en seront des solutions indépendantes. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COBFFICIENTS PÉRIODIQUES. 3 1 Donc, eu égard à ce que 1, = 0, 7, =1, Т_ = — 1, on aura й (3) ф(2- по) = Туе-о)—Т (x). | = Si À est un nombre réel, il convient de poser: dans le cas de 4°? < 1, A = C08 &, et dans le cas de 4° > 1, | А= (а). Alors il viendra: dans le premier cas, sin n& T,, Ra TA et dans le second, "AN ar — а? = aa contraire, illimitées, et la même chose aura lieu dans le cas où A est un nombre imaginaire. Ê En ce qui concerne le cas de 4? = 1, on aura toujours des solutions limitées; mais on _ pourra aussi avoir celles illimitées. Dans ce cas il viendra PSE)", ф(&-н по) = (+1) 1 (2) + (HD) [4 (x +0) + L(x)] п. De là on voit que, si la fonction Y(x+vw) (x) m'est pas identiquement nulle, la solution 4 (x) sera illimitée; mais la fonction (4), qui est _ encore une solution, sera limitée, puisque, cette fonction étant désignée par 0 (2), la re- lation (2) donne | | 9(2-но) = + 0 (x). 1* 4 ‚A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE Il pourra d’ailleurs arriver que toutes les solutions vérifieront la relation Il n’y aura alors que des solutions limitées. On voit donc que le cas de A? — 1 exige une discussion complémentaire, tandis que dans tous les autres cas la question se résout immédiatement. Lorsque, pour l'équation proposée, опа 4°— 1, il est en général très difficile de le constater. C’est de quoi provient la principale difficulté de la question. Mais ce cas ne se présentera que très rarement, et le plus souvent on se trouvera dans l’un des autres cas, ce que l’on pourra toujours reconnaître en calculant A avec une approxi- mation suffisante. Si la fonction р est réelle, la constante À le sera aussi, et ces derniers cas se réduiront à deux: 4° < 1 et 4° > 1. Dans ce qui suit, nous proposons une méthode pour les reconnaitre, lorsque la fonction р ne devient jamais négative. Cette méthode réussit toujours, à moins que l’on ne se trouve dans le cas de 4? = 1. 2. Pour le calcul approximatif de la constante caractéristique on peut proposer plu- sieurs méthodes, plus ou moins expéditives suivant les cas, et entre autres, on peut signaler divers développements de cette constante en séries. Or, parmi ces séries, il y a une qui mérite une attention particulière. C’est cette série que nous allons considérer ici. Soient f (x) et ф (x) deux solutions de l’&quation (1), définies par les conditions suivantes: F0) =, Г =0: Ф(0) = 0, BAD) — 1, La relation (2) donnera 2А = f(w) + f(—w). Or il est facile de prouver que l’on a f(—0) =. En effet, la fonction ?(v)f(r+w)—f'(v) Фано) est une solution de l’équation (1), et cette solution se réduit, pour x = 0, à 1, puisque l’on a f (@) g'@)— + (@) [а = 1, DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COBFFICIENTS PÉRIODIQUES. 5 poupe que soit 2. En même temps, sa dérivée s’annule pour 5 = 0. Cette solution ne peut nc différer de f(x), et l’égalité fo = Po) Гео) —f'(w) 9 (x + w) De cette manière nous ini \ 24 = f(w)+?'(w), а? a + иру =0, _ Pour cette nouvelle équation, toute solution, qui est définie par des conditions initiales ir dépendantes de м. pourra être développée suivant les puissances ascendantes de 14 (entières et positives), ce qui conduira à une série convergente, quel que soit = et quel que soit u. D'ailleurs, la première dérivée de cette solution se représentera par la série, dont les termes fofo — fu +, 1— $: (2) № + PT)? RM... où / Lo, 8 9, (x) sont des fonctions que Гоп calculera par les formules récurrentes 1. (=) «| az | pt, (x) dx, 2, (2) = | as | р9,„_, (2) de, | 1 partant des fonctions . RES № (2) = 1, 9%) = x. 6 : А. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE De ces développements, en posant |. = 1, on déduit | Га =1—1@®-ЬБ@®—Ь@-..., $(2) = 2 — 9, (x) +9) —(@)-.... Par suite, si l’on pose Г, (®) +9, (0) = 24,, on aura cette expression pour À: (6) AI Ach о le terme général étant (— 1)"A,. Nous avons déjà considéré cette série dans le Travail intitulé Problème général de la stabilité du mouvement, où nous en avons déduit certaines conclusions à l’égard de À, en supposant que la fonction р ne change jamais de signe. On voit que, si cette fonction est négative, les termes de la suite А,, À;; À;, Ay sis seront alternativement négatifs et positifs, de sorte que la série (6) aura tous ses termes positifs. On aura donc, dans ce cas, toujours À > 1. Si, au contraire, la fonction p est positive, les A, le seront aussi, et les termes de la série (6) seront alternativement positifs et négatifs. D’ailleurs, à partir d’un certain rang, ces termes iront constamment en décroissant en valeurs absolues, comme le montre l’inégalité A А 7—1? qui а été établie dans le Travail cité *). Par cette inégalité on voit que, si 4, < 2, on aura certainement Arad, PAD Lo par suite de quoi il viendra 1>A4>1 A, et l’on aura 4? 1. An *) Comme on le verra dans la suite, on peut obtenir une inégalité analogue qui donne, pour A ‚ une у, | N—1 |’ limite supérieure plus précise. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 7 Quant à la condition 4, < 2, elle se réduit à в с) о [par 1, ou 4° < 1, à volonté. Donc, le résultat que nous venons de signaler contient tout ce qu’on peut dire sur le signe de A?— 1, si l’on ne connaît que le premier terme de la suite Ay 4, А, ..., Der ne sait rien de plus à l’égard de p, si ce п ’est que c’est une fonction positive. Dans ce qui suit, nous allons montrer ce qu’on peut tirer de la considération des termes _ suivants. м _ 8. Les formules (5) conduisent à diverses expressions de A, sous forme des intégrales . multiples, dont nous allons signaler quelques-unes. En entendant par %,, %,, %5, ... diverses notations de la variable indépendante x, pe qe, pour abréger, = Pan Pam, CET Alors, pour les fonctions f,(@), 9, (2), nous aurons ces expressions: Le 2 Lon—1 Ё, (2) = | as | | DD Ds 0 9 0 ыы D Lon—1 $," 2| а», | az. | 2:21... 1,42), 0 0 0 où Dern par rapport à x, doit être effectuée entre les limites 0 et x, ,, en rem- ” 1 Ton—1 А, = = an | de, a. (D, Ds. Din + Ds Di --- Dan) Чт 0 0 0 8 A. LrapouNorr, SUR UNE SÉRIE DANS LA THÉORIE Pour п = 1, cette formule, qui contient alors une intégrale double, se réduit à w 4=$ | par 0 Une semblable réduction est possible aussi dans le cas général, l’intégrale multiple d'ordre 2», qui figure dans la formule (9), se réduisant toujours à une intégrale d’ordre 7. En effet, reportons-nous aux formules (8) et, en remarquant que les intégrales qui y figurent peuvent être considérées comme celles étendues aux valeurs des variables x,, 2,,..., 2, Vérifiant, si & > 0, les inégalités ии... PL 0 et, si x 0, celles-ci аа. AE effectuons l'intégration, pour f, (x), par rapport aux variables &,, 2.,..., &,, , et, pour Фи (&), par rapport aux variables x,, ©,,..., &,,. Alors, en introduisant pour les n variables qui restent la notation ©, &,,...,%,, nous obtiendrons © © In—ı 1, (&) =] Pi ax | Pa dm. | (1—4) (a —%)... (4%, , —%,)p,d2,, 0 0 0 т dy T1 Фи (2) = | nas | 2 a. | (1—2, (1, — %3) ++ 1 —%,) &, в, da. 0 0 0 Par suite, nous aurons © 7 Ln—1 (10) 4, = +] P, ax | Pa 3%, = (o—2,-+8,) (2—2, (2,—2.)...@,_-—2,) 2, da, 0 0 0 Si l’on introduit la fonction [292=Р®=В on pourra obtenir, pour A,, encore d’autres expressions sous forme des intégrales d’ordre n. On les obtiendra, en effectuant les intégrations dans les formules (8) par rapport à n variables quelconques dont les indices diffèrent entre eux au moins de deux unités. DES EQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 9 La plus simple de ces expressions s'obtient en effectuant l'intégration, pour f, (x), par rapport aux variables 2,, &,,...,2,, et, pour 9, (2), par rapport aux variables x,, 4, ..., Sn. De cette manière, en nai A P@)=P, Р(0)=В, _ et en changeant la notation des variables, on trouve X A = [af da... fem (В,—Р)...(Р, ‚—Р)(Р,— Р)аа,, Er у x = En Г. «= | an, | du. | РЕ — В). (RB ,—Po)de. Be 0 0 0 De là, si l’on pose ‘ w | pdı=Q, 0 | И мен и) А, = = + [af da,. | (Q- Р-Р) (P- )(B-P,)...(B,_,-P,) dx, 4 в. qui а une grande analogie avec celle (10). au 2 4, Avant d’aller plus loin, nous nous arr&terons, pour un moment, aux formules précé- dents, pour signaler quelques inégalités qui en découlent immédiatement, et qui donnent | une idée sur la manière dont converge la série (6). Nous nous bornerons à la supposition que р est une fonction réelle ne changeant jamais |" signe. _ Ilest clair que, dans ce cas, 4, sera compris entre des limites de la forme wen Ln ” 1.2.8...(2n — 1) 2n? L étant la plus grande ou la plus petite valeur de р. Mais on peut obtenir des limites plus précises pour 4,. _ Reportons-nous, à cet effet, à la formule (9), et supposons, pour fixer les idées, que l’on a toujours p > 0. | Ban. Физ.-Мат. Отд. 2 10 А. LiapouNorr, SUR UNE SÉRIE DANS LA THÉORIE En remarquant que 1 PM P3- ` ож n (2 Ds DATE А, { 1 ee | nous aurons ® x Lon—1 = ) ax | da... | (PHP... + р) 9%. 0 0 0 Or l'intégrale qui figure ici est égale au produit de celles-ci: wo x w Ca) Don —2 | p'dx et [ an | am... | HAE 0 0 0 0 Il viendra donc w Au | (12) 4, < 1.2.5...(2n —1)2n | 145 0 Pour obtenir une limite inférieure, nous nous servirons de l'inégalité Pa Pare б-р... ee Pen Z 2 Ур, VD... Ур, en vertu de laquelle il viendra 4, > re ‚vr dx)". Remarquons que le second membre représente ici une limite inférieure précise de A,, étant donnée la valeur de l’intégrale ГУ» ах, puisque cette limite est atteinte, lorsque la fonction p se réduit à une constante. D DES ÉQUATIONS DIFFERENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 11 De même, la limite supérieure, définie par l’inégalité (12), est une limite précise, étant donnés » et la valeur de l’intégrale ы п |: ат. 1 _ En partant de la formule (10) ou de celle (11), on peut obtenir, dans la même suppo- “A sition p > 0, une autre limite supérieure pour A,. м En supposant, comme il est permis, > 0*), le champ de l'intégration dans la for- 5 À mule (10) se représentera par les inégalités u > ap 20. Or, en vertu de ces inégalités, les quantités DRE, Das Ша, een nd _ зе er toutes positives. u. о dé 2 „Par suite, leur somme étant égale à w, on aura (o—2,+7,) (2, —2) 9 —2)...(&,_, —2,) < + A, < 47 (р de), 2* 12 А. LTAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE On pourrait présumer que la limite supérieure précise de cette espèce fût donnée par l'expression (13) m (u [ir de). Mais il ne nous a pas réussi à le démontrer d’une manière générale, et nous ne pouvons l’affirmer que pour les deux cas les plus simples, ceux de n = 2 et de n — 3. Tout revient à prouver que l'expression ci-dessus est une limite supérieure pour A, Or, dans le cas de n — 2, on le prouve aisément en partant de la formule ® æ А, = +] ax | (O— PHP) (Р-Р, da. 0 0 En effet, on en déduit w [0) [0) 2 o 4=a| Pair | rar (| Pas) 30| Раз, Jo 0 0 0 ce qui, en posant peut être présenté sous la ne A, = ju 0 2. De là, en remarquant que В ne peut jamais être négatif, on conclut (14) А, < 51670, et le second membre de cette inégalité n’est autre chose que l'expression (13) pour na Le cas den — 3 présente plus de difficulté, et nous le traiterons plus tard. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORTFICIENTS PÉRIODIQUES. 13 5. Passons à l’objet principal de ce Mémoire. Nous nous proposons de démontrer que, dans le cas où р est une fonction positive, la série (6) jouit de cette propriété que le rapport An An—ı d&eroit constamment, lorsque n augmente. A cet effet, nous allons établir une formule, qui donnera une certaine expression pour le produit A, 4, de deux termes quelconques de la suite р А, 4,, Ау, Pour arriver à cette expression, nous pouvons nous servir indifféremment de la formule (10) ou de celle (11). Nous nous arrêterons à cette dernière. Nous allons considérer » -+ m variables Dit us. 4 ИРА ie) LE et, en entendant par J,, Jg, ..., J, des nombres quelconques de la suite 1, 2, 3, ..., п-т, nous poserons, d’une manière générale, BB) ER) 8, Вов, os ce À La formule (11) pourra alors s’écrire ainsi 3 w Ti Tn—) 4=+| аа, | аа... | Пана ade, 0 0 0 _ et l’on aura D © бп Tn--m—ı ы у А =+| dx | dx a In+1,n+2,...,n-+m] da, - 0 0 im ° De là, pour le produit 4 A, 4,, il résulte cette expression HAE, 9... 0] In+1,n+2,....n+m] dx, dx,...dx ‘п-т ' = 14 A. LTAPOUNOrF, SUR UNE SÉRIE DANS LA THÉORIE l’intégrale multiple d'ordre n + m étant étendue à toutes les valeurs des variables ©, æ,, . .., 7, т, Qui satisfont aux inégalités - | DRE > FH (15) \ а И. ПО: Or cette intégrale est égale à la somme des intégrales de la même forme qu’on obtient en supposant que chacune des variables nr? Topos es ит se trouve dans l’un des intervalles (0, %,), (2, Aa er) (х,, 1;), (2 &), et en faisant, à cet égard, toutes les hypothèses compatibles avec les inégalités (15). Considérons une de ces intégrales et permutons y les notations des variables de telle manière que le champ de l’intégration soit exprimé par les inégalités Ш, > see 0 Nous aurons alors, pour cette intégrale, une expression de la forme 1 2 Ят--п—1 | an, | аа... | ER PR о М EDEN 0 0 0 ds do ...) т étant des nombres inégals de la suite ЧЕ’ Эк Е rangés dans l’ordre croissant, et Л, Jg ..., Л, les autres nombres de la même suite, rangés aussi dans l’ordre croissant. En faisant toutes les suppositions possibles à l'égard des nombres ö,, 4, ...,2,,, nous aurons toutes les intégrales en question, et leur somme représentera notre intégrale primitive. De cette manière nous obtiendrons © T1 Lm+-n—1 a ал, = | ва | am. | > Be MR ver 0 0 0 où la somme est étendue à toutes les combinaisons possibles de m +» nombres de la suite 1, 2, 3,.... т--и pris m & m, les nombres de la combinaison représentant les valeurs DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CUEFFICIENTS PÉRIODIQUES. 15 дей, &,,..., ©, les autres nombres de la même suite celles de 7,, 7,, ..., J,, et cela de _ telle manière qu’on ait 1 Gi Е д <»<}<... <). Tr 6, Nous allons maintenant nous occuper de certaines transformations de la somme DR bee NN . qui représente la fonction à intégrer dans la formule précédente; mais, pour quelques sim- plifications de nature purement formelle, au lieu de cette somme elle-même, nous allons con- _ sidérer son rapport à l'expression [5.25% + т]. > fü; ia, 0 ба] Dis Je) 3 fn] 9 _ [1, 2, 3, ..., т] introduisons les notations suivantes : man—ı min m-n—ı? PR-—-B=D, P,—-P,=D,, uns P Alors il viendra ея à im 4 0,8... м-в = D D,D;.. Di =D, D,...D et en posant [&, VA a т] LE Li» Des ..., In] ge: Di, Di, . ‚Din бт? D;, Dj, ... D;, IS а nous aurons =\ и | 5 = Ку, 15 +) т K, ;,, In" Considérons de plus près les expressions désignées par K, zum et Km PR 16 А. Liapounorr, SUR UNE SÉRIE DANS LA THÉORIE Chacune de ces deux expressions à la forme d’une fraction, dans laquelle le numérateur et le dénominateur sont des produits d’un même nombre de facteurs. Par exemple, dans la première, le numérateur est le produit de m facteurs рвов, и $2} i #3? m—ı Or ces facteurs peuvent être exprimés au moyen des D... Par exemple, on а P,—P,=D,+D,,,+...+D, = D, et l’on aura des expressions analogues pour P,—P,, P,—P. to t3 t4 ре PER Im—ı im Quant à ce qui concerne ie facteur Q—P, =, pour le présenter sous la шёше = forme, il faudra étendre la definition des D, aux valeurs de $ qui surpassent m—+-n, en ad- 4 mettant les égalités de la forme a Alors, en posant nous aurons il “a Q— P, + É, — D. im Il viendra donc il: A RE A > 5 Pr ea | GE = АО ШВ. i, in im et pareillement, en posant Ц .r KENNEN IH on aura jet il Fra) KO tar se) в = DD; > Die, ému À dm À En Ja In *) Par la notation Zus k et 1 % étant des entiers, nous entendrons toujours la somme étendue à toutes. valeurs entières de s, de % à inclusivement. 4 DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 17 в. Nous remarquons maintenant que chacune des sommes, qui figurent dans ces expres- sions, peut se réduire à un seul terme, ce qui aura lieu, pour quelques-unes d’entre elles, _ toutes les fois que, parmi les nombres у ) . . .! . | * . ar N Er. ape TROT VE Eng И ES Br / > En. Be — И s’en trouve qui soient éguax à 1. iR Dans ce cas, le numérateur et le dénominateur au moins d’une des fractions à Я К, ‚К, .; auront des facteurs communs, et, si Гоп désigne par g le nombre des + Detmr Jin Jn à termes égaux à 1 dans la suite №. к. a Lo — —%, ...у à — À { № et par № celui des termes égaux à 1 dans la suite @ 7 к ah: u PE CICR Л — у des termes de la première fraction auront д facteurs communs et ceux de la seconde 4. Ces fractions seront donc réductibles, et il est facile de voir qu'après la réduction _ complète le nombre des facteurs au dénominateur sera le même pour les deux fractions, en | nd autres termes, que Гоп aura Be m—g—=n—h. En effet, introduisons la notation 4 Bi, étant considéré comme une certaine caractéristique du nombre i, dans la suite 2,, %,, ..., бу et, en posant m — g = |, désignons par &,, &, ..., &, ceux-là des nombres &,, pour lesquels > 1. Il est évident que, si l’on considère tous les nombres contenus dans les intervalles . . ” . . 1 . . when hei ln, = (&, +80), (а, +8), ..., (a, щ- dm), (da, — 1) + (Day — 1) +...+ (0x, — 1) =", (da, — 2) + (day — 2) +... + (0x, — 2) = h, et de là il vient в — № =. _ Cela posé, effectuons la réduction de nos fractions. Ban. Физ.-Мат, Отд, 3 18 А. LIAPOUNOrr, SUR UNE SÉRIE DANS LA THÉORIE Nous aurons о God 4+8: —1 и a CA Lo (2) ee D, D 00e . et pareillement, en posant sh ET Ÿ Is —j, CYR ... Amin = у, et en entendant par ß,, B,, ..., В, ceux-là des nombres j,, pour lesquels à, >> 1, B,+0B,—1 Bo+0B—1 В+ 08, —1 2 D > D ZD Bi в, в; у 717729 fn о + пет Nous supposerons <<, LU Lee Ep Bi << Ba Be << В. Alors nous aurons nécessairement : ou bien ar —1= 8, +, —1=В,, ..., 9-6 —1 =, ou bien аб —1= 8, rin Ih, ..., м-н 6 — 1 = Ву тя. Pour s’en assurer, il n’y а qu’à remarquer que les nombres de la suite и, +0, —1, 8, —1, .:., 0—1, si а, da, —15т-ни, ou ceux de la suite \ и ба —m—n—1l, œ+Üm—1, ..., 6—1, si ©, + ба, >> т + и, appartiennent au groupe (7,,/», ...; ,), ont des caractéristiques 97, supérieures à 1 et sont rangés dans l’ordre croissant, Pareillement, nous aurons toujours : ou bien + Ian, BB lan, ..., В +08 len тю, DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. ou bien В, 88, lu, Blau, ..., B, +08, —1 =&.. Par suite, si Œ, Rp ae VAE В,, da u. B,, rangés dans l’ordre croissant, il viendra nn: sv ‚> À A x RS: Az 21—1 21 ; бт Л) D, D,, В, D,, où l’on à posé CN NV = А +m+n. п’ = ‚ A SE Tel 4 у. Mr KH... м — А =”, Le x - ou bien celle-ci : , KAHN №. мм =. й 4 En effet, la somme | RAM) + Qi) + 4 Ag №) égale : dans le cas de À, =, à * \ (Da, — 1) + (Day — 1) +. + Ba — var | lans celui de À, =В,, à (58, — ee, + (8, — 1) = m. 7. La formule (16) conduit à celle-ci: K К esse У Du, Dag:* Du, LIEBER т Ju ln ar D), р), NS Dj ? 3* ых. _ Вешатацопз que les nombres À,, À, ..., A,, vérifieront toujours ou bien la relation 19 20 А. LIAPOUNOrF, SUR UNE SÉRIE DANS LA THÉORIE où la somme est étendue à toutes les valeurs de p,, appartenant à la suite À, À +1, ..., № №, » №, » » » As À + 1, ...) À — 1, a se. Ve ae, je Va la een et je Ce le + Ce els О И ПК ев НИЯ Cette somme contient deux termes égaux à 1, dont l’un correspond à la supposition : № =^,, Ba = À; ...) bar == Хр l’autre à celle-ci : = Hg ces By =. Quant aux autres termes, ils seront de la forme Ds, Ds, а Dp, RTS oe Da, Da, Be Da, (18) а, Gy ..., а, étant des nombres de la suite Е A et 6,, b,, ..., В, des nombres de la suite qui different des а. Considérons ces termes de plus près, en supposant, pour fixer les idées, а<а<а<...<а,, DD, < bete ЗО Tout d’abord, nous remarquons que les nombres @,, 4, ..., а,, k étant supposé plus grand que 1, vérifieront nécessairement les inégalités аа—@а>1 а—а>1 ..., 9 —%,>1 a+mrn—a>l. En effet, toutes les fois qu’on а DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 21 ш, ne pourra recevoir que les deux valeurs A, et À,,,, et, par suite les nombres À, et À,,, ei . . _ ne pourront se rencontrer tous les deux dans la suite а,, @,, ..., a,. Pareillement, lorsque a у : ÀA+m+n—ly = 1, … №; ne pourra recevoir que les deux valeurs A,, et A,, et les nombres A,, et A, пе зе rencon- _ treront pas en même temps dans la suite а, &, ..., @. ar Dans le cas où les nombres A,, Ay, ..., À,, satisfont aux inégalités М > ль... А — А >1, А-т-—м>Ь j | у aura des termes pour lesquels # = 21. Tous ces termes s’obtiendront en attribuant à Bay Han. Hay des valeurs satisfaisant aux inégalités KIH< et _celle de la seconde par Х, on a 2>q+2(—9, #>49+20—94). On voit donc que le nombre k ne surpassera pas le plus petit des nombres Z et > ; et _ de ces derniers l’un est égal à m, l’autre à n, car on a 5 =т-ни, et 3, comme nous avons vu au numéro précédent, est toujours égal à n ou à m. er) Dans ce qui suit, nous supposerons m < и, et, conformément à ce que nous venons de у - m er, nous ne donnerons à # que des valeurs qui ne surpassent par m. 8. Reprenons l’expression 5 Es » K;, ty) bus | т K;, Ja hé Im! - Chaque terme est ici une somme de la forme (17), et cette somme, outre les termes de la forme (18), qui sont tous distincts, contient encore deux termes égaux à 1. + 24 A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE En considérant d’abord ces derniers termes, nous obtenons, pour leur somme dans l’ex- pression ci-dessus, 9 (n +1) (n +2)... (n-+ m) 1.2.3...m car le nombre des termes de l’expression S est celui des combinaisons qu’on peut former de n + m éléments m à m. Passant ensuite aux termes de la forme (18), nous remarquons que chacun d’eux sera répété dans l’expression 5 autant de fois qu’il y a de suppositions distinctes sur les nombres 1, в, +. би, dans lesquelles la suite (21) De Le No er contienne tous les nombres а, @,, ..., a. i le nombre de ositions. Soit N, ou a, @ nombr ces supp En introduisant la notation connue 0. ати о" RES ETS Po UE nous aurons k=m ЗБ Пу Ь S — AC re 2 N Gy, nd, Da, Da, weis Da, i où la seconde somme est étendue à toutes les suppositions possibles qu’on peut faire sur les nombres appartenant à la suite 1, 2, 3, ..., m-+n, en les assujettissant successivement à chacune des deux conditions (19) et (20). Reste à calculer le coefficient N, .,,..,.,, qui dépendra, comme nous verrons tout de suite, non pas des valeurs des a,, mais seulement de leur nombre k. En nous arrêtant à un groupe déterminé des nombres а,, @,, ..., &,, considérons toutes les combinaisons possibles (4, à, ..., 2) conjointement avec les combinaisons correspon- dantes (j,, 2, -..,,), et toutes ces combinaisons partageons en diverses classes suivant le mode de la distribution des nombres a,, a,, ..., a, entre les deux groupes (i,, %, ..., 2) et (In Ja +++ 2). Comme chacun des nombres a, peut appartenir à chacun de ces deux grou- pes, le nombre de tous les modes de distribution et, par suite, aussi des classes sera égal à au Cela posé, considérons un mode de distribution quelconque et voyons, combien y a-t-il de combinaisons (4,, %,, ..., 2) de la classe correspondante qui remplissent cette condition que la suite (21) contient chacun des nombres а,, &, ..., @,. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 25 № : Soient 7 у | ceux-là des nombres a, qui appartiennent au groupe (&, &,,..., iu), et Br Е В, Bay PES В; | ceux-là d’entre eux qui appartiennent au groupe (71, Ja ---,J,), à et j étant des entiers po- _sitifs ou nuls liés par la relation à +) —k. _ En supposant que a, est le plus grand des « et В; le plus grand des ß et en nous re- portant à ce qui а été montré au numéro 6, nous pouvons affirmer que les nombres «a ..., 4, ne pourront se rencontrer tout à la fois dans la suite (21) que si les nombres "1 (re 1 9+1 ..., +1 (oua+1—m"m—n) 4 | appartiennent au groupe (7, Ja » + «3 J,) et les nombres 1 Ga и: 1, В,-+1, AR: B;+ 1 (ou В; + 1—m— я) E Deroupe M7). _ Par conséquent, le groupe (&, &,, ..., „) devra contenir les k nombres suivants a, ВТ, Bel B; +1 (ou В; +1 —т®— я), q N sont tous distincts, comme cela résulte de ce que les a, satisfont aux inégalités 3 Vis м Ga >. 4421 ON EE RFA —a > 1. < 4 > : _ En même temps, le groupe (7, Ja ..., j,) devra contenir les k nombres 4. р. Rue: Ba ...) В; че PURES a, +1 (ou &,+ 1—m—n), qui sont encore tous distincts. Cette condition nécessaire est d’ailleurs suffisante. h % “On voit donc que la condition que doivent remplir les combinaisons considérées se ré- duit à celle-ci: les 2% nombres fixes de la suite 1, 2, 3,...,m+n doivent être répartis ВАК, et d’une manière déterminée, entre les deux groupes (à, 4», ..., 2) её (as Jan ++ Je Il s’ensuit que le nombre des combinaisons en question est celui des combinaisons qu’on peut former de ж--п— 2% objets m— 4% à m — k. | San. us.-Mar.Orx, 4 26 А. LIAPOUNOrr, SUR UNE SÉRIE DANS LA THÉORIE De tout ce qui a été dit il résulte Qyy ау ve) ау, п--т— 2} la notation в étant employée avec la convention connue 0, a IR (a = 0,1,2, 3, Les coefficients N étant ainsi déterminés, nous n’avons plus rien d’inconnu dans l’ex- pression de 5, que nous pouvons maintenant présenter sous la forme m A == У Е Be, n+-m—2% k=0 en posant S == 2 et en entendant par S,, pour k > 0, la somme de tous les termes de la forme D, Ть,... Do, DDR DE qui correspondent à une valeur donnée de k. Quant à cette somme, on pourra écrire — (0 Dh, .:. D, D D el) (22) 8, = ı 02 у. a, а а к = Da, Ра, +++ Па, Dp, Dh, -:: Do en supposant que la sommation s’étend à toutes les combinaisons possibles de a + m nombres de la suite 1, 2, 3, ..., п-т pris 24 à 2%, les nombres de chaque combinaison représen- tant les valeurs des a, et des 6, conformément aux inégalités а. в. 9. Revenons maintenant à l’expression de 44,,4, qui а été obtenue au numéro 5. Cette expression peut être présentée sous la forme o я Ят--п— 44а, = | ax | ds, … | S D, DD I EU 0 0 men 0 \ TMC DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 27 | | ad Я Par suite, en posant à м = u Tm+n—1 1 0 0 0 21 та et en supposant m 9° Br I К k—0 C’est cette formule que nous avons voulu établir. Vu les applications que nous en aurons à faire, il est utile de remarquer que la quan- _ tité désignée par J, ne dépend des nombres m et n que par l’intermédiaire de la combinaison тп. C’est ce qu'on voit par les formules (23) et (22), en tenant compte de la significa- _ tion du signe sommatoire dans la dernière. $ Donc, la somme m + п ayant une valeur constante, la quantité J, пе dépendra que du nombre k. _ Remarquons encore que l’on a t ты | у 10. Nous allons à présent supposer que la fonction р ne peut recevoir que des valeurs positives ou nulles, supposition que nous retiendrons dans tout ce qui suit. _— * Ceci admis, l'intégrale | Р= | pda a une fonction croissante de x, et les quantités D,, D,, ..., D,,,,, ne pourront pas de- ir négatives, lorsque les x, vérifient les inégalités rot pipe DR qui définissent le champ d'intégration dans la formule (23). _ Ilen résulte que, dans la supposition adoptée, tous les J,, ainsi que les A,, seront des nombres positifs. р Dp, Dh, ++ Do, Ва Dé 40e DER 4* 28 A. LıaAPounorF, SUR UNE SÉRIE DANS LA THÉORIE et la formule (22) donnera H 5, = 2 pire ? d’où l’on voit qu’on aura yfak (25) J, > О Нач le signe d'égalité se rapportant au cas de 4 = 0. En se servant de cette inégalité, on pourra déduire de la formule (24) diverses inéga- lites entre les quantités A,, dont nous allons signaler les plus importantes. En premier lieu, posons, dans cette formule, m— 1. Il viendra 4,4,={(n+1)%+2J,, ce qui, en vertu de (25), conduit à cette inégalité AA, Sm: De là, en remplaçant n par и — 1, on tire А (26) 4, Se An ce qui donne, pour le rapport A al une limite supérieure plus précise que celle signalée au n° 2. Maintenant, en entendant par $ un entier positif ou nul, remplaçons, dans la formule (24), п par n +2 et m par n — 1. Nous aurons n—i ur k nn—i—k) 4 À, FR Be 2 ER Ju k=0 % où, d’après се que nous avons dit au numéro précédent, les J, ne dépendront point du nombre $. Nous aurons donc, avec les mêmes valeurs des J,, ces deux formules N AS an—2k k=0 n—1 a k mIn—ı—k) 2% A Er 24 - En In k=0 №. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 29 dont la seconde pourra être écrite ainsi : 4,_,4 22 > pu n—k Omar dh N n+-1—k “an—2k k=0 ou bien ] a й et c’est la proposition que nous avons voulu démontrer. d On peut d’ailleurs obtenir un résultat plus précis. и @—1)* ®—® Ay: Nie N _ (n—1)(n+1—+%) а J,. Or il est facile de s’assurer que la somme, qui figure au second membre, représente une quantité positive. _ En effet, cette somme est plus grande que la quantité 3 4 : |? (п—2) — (т) CR Je отл, un: an—4 и , п’оп obtient en rejetant tous les termes pour lesquels 4 > 2, et cette quantité, en vertu de (25), est plus grande que celle-ci | Lei Ed LM _ (m?—3)(n+-2) in ` Pen 2n—4 т =? am A on G(n?— 1) on an" On voit donc que l’on aura ‘a | | fr (27) А > Pr 1 did - _ pour toutes les valeurs de п à partir de n — 2. 30 A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE 11. Nous venons de montrer que le rapport An An—ı décroît constamment, lorsque x augmente. Il en résulte que, si, pour une valeur quelconque de n, on a 4,< À tainement n_1> OD aura cer- Я, > 4,,, > Ааа Par suite, si, en calculant successivement A,, Ay, Ay, ..., on parvient à un terme À, qui ne surpasse pas le précédent A, _,, on pourra conclure que la valeur de À est comprise entre les limites 1—A +4, — А, ... 2 et 1—A4,+4—4,+...+(—1) "4, ,+(—1)"4,, et que les calculs ultérieurs conduiront à des limites de plus en plus resserrées. D'ailleurs, si l’on pose A=1l—A+4,—A4,+...+(—1) (4, —R,), on aura, d’une part, В, < 4, Dad er A ee) nr *9 et d’autre part, В, > 0, в,> Янка 7-42) ...у d’où Гоп pourra tirer des conclusions utiles, sans pousser le calcul en du terme 4), l’on connaît des limites supérieures et inférieures des termes À А А n+-1 n-+2) 7-+37 НЫ Par exemple, si l’on se sert de l’inégalité (27), on pourra conclure в An? An—ı 2 et l’on aura A=1—4,+4,—14+,..+(—1) A, (ро An Ê Ал 9 étant une quantité comprise entre 0 et 1. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 31 x Remarquons que cette formule sera exacte non-seulement dans le cas où 7. : mais encore dans tous les cas où l’on а 4,,, > 4,,,, п ayant une valeur quelconque su- _ périeure à 1. в. Si l’on а 4, < 4,, les conclusions précédentes seront applicables quel que soit п, et l'expression я € 1—4,+4,—4,+...+(—1) 4, 1 se rapprochera constamment de 4, à mesure que n augmente en restant toujours pair, ou _ toujours impair. Si, au contraire, on a A, > À,, la suite А,, А}, À, ira jusqu’à un certain terme en croissant, et l’expression ci-dessus ne commencera à se rap- _ procher de À qu’à partir de la valeur de » qui correspond au terme maximum. N Quant à cette valeur, elle sera toujours plus petite que VA, , comme on le voit par _ l'inégalité (26). _ Il est à remarquer que, si Гоп a À, <6, on aura toujours A, < 4,. C’est ce que montre l'inégalité (14), que nous pouvons présenter sous la forme IA (8) 4, < 54}. Comme dans le cas de 4, < A, па À < 1, il en résulte que la condition A, < 6 as- ni > 4h, 0n aura: dans le cas de n impair 12. Toutes les fois que А A>1—A, +4,—4,+...+(—1) 4,, ke ‚ dans celui de » pair A<1i—A,+4,—4,+...+(—1) 4. _ Раг suite, si, dans le cas de » impair, on trouve (29) NN PT PS AT EPST TP 6 _ а étant un nombre donné quelconque, on pourra conclure l'inégalité À > «a. 32 А. LIAPOUNOrr, SUR UNE SÉRIE DANS LA THÉORIE Pareillement, si, x étant pair, on a (30) 1—a— À, +4, —4,+...+(—1) 4, <0, on pourra conclure À < я. Nous avons supposé A, ,, > 4,,,, condition nécessaire pour que les conclusions ci- dessus soient légitimes. Mais, dans certains cas, cette condition sera déjà impliquée dans cel- les (29) et (30). Tel sera, par exemple, le cas où le nombre « est compris entre — 5 et +1. Dans ce cas, la condition (29) ou (30), suivant que n est impair ou pair, entrainera non-seulement l'inégalité À | > 4,,,, mais encore, sin >> 1, celle 4,_, > 4, et, pour и = 1, celle HEAR En effet, d’après ce que nous avons remarqué au numéro précédent, on ne peut avoir А, > À, que si l’on a A, > 6, et d’autre part, l’inégalité A, > 4,_,, pour п > 1, entraîne celles-ci : N+-A1 MA DAD IE Donc, si l’on avait 4, > 4,_,, pour n > 1, ou 4, > A, pour n=1, le premier membre des conditions (29) et (30) serait, dans le cas de » impair, inférieur à — х— 5 et, dans celui de n pair, supérieur à 1 —«, et aucune de ces conditions ne pourrait être remplie pour les valeurs considérées de «. Par suite, dans le cas que nous venons de signaler, la condition (29), # étant impair, assure toujours l’inégalité À >> « et celle (30), n étant pair, assure toujours l'inégalité À -Ь DER А... ed, SUN ar о —ÀA +4, —A,+...—A >20, » » A>-l. 2n+1 — 13. La proposition que nous venons d’énoncer conduit à une méthode pour décider si A se trouve dans l’intervalle (— 1, + 1), ou non. Pour résoudre cette question, on commencera par calculer A,. Alors, si l’on trouve À, < 2, on sera certain que — 1<4 2, on caleulera À, et l’on distinguera les trois cas suivants qui pourront se présenter : DAS A —2, 94а паза. Dans le premier cas on pourra conclure А < — 1, et la question sera résolue. Dans le deuxième cas on aura seulement À < 1 et l’on devra encore décider si Гоп а A>—1, ou A<—1. А cet effet, on calculera A,. Alors, si l’on trouve ИИ От = `` À, < А,— À; +2, оп conclura que À > — 1. Si, au contraire, on trouve 4,> 4, — À, +2, _ on calculera A,, et la question sera résolue, si l’on а À,< A3 — À, + À, — 2, . auquel cas on aura À < — 1. Dans le cas contraire, on calculera A,, et Гоп continuera _ ainsi de suite, jusqu’à ce qu’on arrive à une inégalité de la forme * 4 AS À TAN FEAT, TA laquelle пе manquera pas à se présenter, si À n’est pas égal à — 1. Alors, si x est pair, on “ aura À < — 1 et, sin est impair, on aura А > — 1. + Dans le troisieme cas on devra distinguer les trois cas suivants: D: WAZ WLAN SER, . où l’on a posé pour abréger à А, — À, = 83. Si, après avoir calculé A,, on se trouve dans le premier de ces cas, il sera certain que _ АР р et la question sera résolue. _ Si l’on se trouve dans le deuxième cas, on pourra seulement conclure À > — 1, et … l'on devra encore décider si l’on a À < 1, ou 4> 1. | On calculera done A,. Alors, si l’on trouve À, < А, —4, + А,, Зап, Физ.-Мат. Отд. 5 34 | A. LTAPOUNOrF, SUR UNE SÉRIE DANS LA THÉORIE on aura À < 1, et la question sera résolue. Dans le cas contraire, on calculera A,: Si l’on trouve alors A; A, — À, + A4, — À,, on aura À > 1. Si, au contraire, on a À, > À,— 4, + 4, — À,, on calculera A,, et l’on continuera les calculs jusqu’à ce qu’on parvienne à une inégalité de la forme AURA Sad; ELF ce qui ne manquera pas à arriver, si A n’est pas égal à 1. Alors, sin est un nombre pair, on aura À < 1 et, si c’est un nombre impair, on aura À > 1. En ce qui concerne enfin le troisième cas, on le subdivisera en trois © qui зе distin- gueront par la valeur de A,. En posant | AS = АА he ces cas seront les suivants : 1) AE В В, à DTA Dans le premier de ces nouveaux cas la ов sera résolue immédiatement, car оп aura А —1. Le deuxième cas se traitera de là Far manière que le deuxième cas défini brécédem- ment par la valeur de A,. Quant au troisième, on le divisera en trois cas nouveaux, qui se distingueront par la valeur de À, et qui présenteront les mêmes circonstances que les is cas relatifs aux уа- А } | 000% от 8 sol 60 On voit donc que chacun des termes de la suite - A 27 Е ИЯ. ЕЕ Ts | Home tés A conduit à une distinction de trois cas, dont le troisième se subdivise en nouveaux trois cas, qui se distinguent par la valeur du terme suivant. | S ab «id Il est évident que l’on ne pourra pas se trouver toujours dans le troisième cas, et que Гоп finira par tomber ou sur un des premiers cas, où la question se résout immédiatement; ou bien sur un des deuxièmes que Гоп traitera comme il a été montré. x р N DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 35 | La méthode ne sera en défaut que si Гоп а А == + 1, cas dans lequel les calculs pour- _ ront se prolonger à l'infini sans conduire à une conclusion décisive. C’est ce qui est du reste dans la nature de la chose, la méthode n'étant au fond qu’une suite а’ approximations suc- cessives. ei 14, Dans certains cas, on pourra simplifier les calculs exigés par la méthode en se ser- ant des limites supérieures des A,. Supposons, par exemple, qu'après avoir calculé À, 4,, Аз; en. 4 N) . om ait réconnu que À vérifie l'inégalité À < 1, mais qu'on ne connaisse pas encore si Гоп а A>—1,ou 4<—1. On aura alors Pr % € u’ ра # LE №. ce ве - let l’on devra examiner si À,,, vérifie l'inégalité Ао A, дис A 1 nn вс. А, 2, АРА? MENT" et que l’on veuille savoir si l’on a 1 104 а. 4 Shi A+ 2. Les inégalités (26) et (27) donnent, pour A,, ces deux limites supérieures : А, А, © © A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE La seconde, en vertu de (28), étant plus précise, posons 1 42 L == 9 FR . Nous aurons ainsi V’inegalite (32) À? —2A,A, + 24,(4, — 2) < 0, qui assurera celle (31). Voyons, en quels cas pourra-t-elle être vérifiée. Tout d’abord, elle exige que les racines de l’équation @ —2Ax<+24,(4, — 2) = 0 soient réelles, ce qui s’exprime par l'inégalité A, < 4. Elle exige ensuite que A, soit compris entre ces racines. Pour exprimer cette dernière condition, il suffira d’écrire (33) A > A ИА puisque, sous la condition A, < 4, on aura toujours A, < 4,. Une condition doit encore être satisfaite, pour que-l’inégalité (33) soit possible: еп vertu de (28), on doit avoir | 1 ER RE Wer 542 > 4, —VA,(4—4,), ce qui se réduit à (34) 4>—124°?+ 724 —144<0 et exige que A, ne surpasse pas le nombre 3,345..., représentant la racine réelle unique de l’équation 2 — 120° + 72х — 144 — 0. On voit que la condition (32) assure non-seulement l'inégalité À > — 1, mais encore celle À € 1. 15. Pour le calcul successif des termes A,, A,, 4,, ... exigé par la méthode, on peut se servir des formules (5), qui permettent de calculer de proche en proche les fonctions f (x), р, (2), Ь (2), ..., 91 (2), $, (2), ga (2), ..., d’où l’on déduit les A, par la formule 4,= 7 [,(@) + 9, (©). у | DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 37 Ч À : Е - ; | On peut aussi зе servir des formules que nous avons signalées au n° 3 et qui permettent В de calculer immédiatement un terme quelconque. Toutefois, dans le cas le plus important, celui où la fonction р est donnée sous forme d’une suite des sinus et des cosinus des mul- tiples de x, ces formules ne sont pas assez commodes pour les calculs, et avant de les appli- quer, il convient de les faire subir certaines transformations. C’est ce que nous allons main- _ tenant faire pour la formule (11) dans les cas de n = 2 et de п — 3, En ce qui concerne le cas de n — 2, nous avons trouvé au n° 4 1 1 А, = 300 —-R, Р= | раз. Nous choisirons cette constante de manière à avoir [0] | P dx = +wQ. 0 Alors il viendra ge IM 02) dx =0, _et nous aurons [0] FR | (P—0%) ae. | о Remarquons que Р —о= est une fonction périodique de x à période w et que, pour la détermination adoptée de P, l'intégrale de cette fonction sera encore une fonction périodique. 38 А. Lıapounorr, SUR UNE SÉRIE DANS LA THÉORIE nous aurons P—0Q[t+0'()], ©’ (0) étant la dérivée d’une fonction périodique © (1) ayant pour période 1. 4 Avec ces notations, nous obtenons : 0 4 iR [+] 9” at | WR. 0 16. En général, si l’on pose pour abréger t+ 0" (#) = Q, en ajoutant l'indice à, lorsque i est remplacé par £,, la formule (11) donnera Ai 4 0007, où ы 1 я In—ı у = +| а, | di, cl фе Q, ra Q,) (9, Ta Q,) à а dt,. Nous venons de trouver 1 (35) a = 4-3 | 0° dt. Occupons-nous maintenant de la transformation de l’expression - tı le | 1 4; = +] dt, | dt, | (1 0. > Q,) (Q, — Q,) (9, — Q,) dty. 0 0 0 7 La fonction à intégrer se réduit ici à ©, 9, я 9, 9, EN Q, OR SE 9, + (©, RE Q,) Q 3 (Q, TE 9.) 97 + (Q, — Q,) 9;. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. Par suite, en remarquant que 1 tı 173 1 th Ja | as, | at = | Q, dt, | 1, Qt, I м te 1 hi | dt, | dt, | 9,0, dt, =] (1 — À) ©, dt, | 9, dt,, 1 t, tz 1 t, [1 | 4, | 09, ©, dt, = Q, dt, | (и —&) 9, ав, Е fa dt a7 Q, di, 2{ (1—t)t0Q° dt, t [a [ a [ чаи [| 9" a (4 — 4) ©, 4, 173 1 tr | [af dt, ‚ вели, = | 9 a, | 1, 0, dt, t er dt, ‘a „di, -[ Q, dt, [ 5 Q, dt, wi 0, QE dt, -[ (ti) Qat [ Q, dt, “a | ‘di Е 70,08 dt, [ane Г. Q2dt,, [a | af a = | 0, 44 и (41) бла, 39 40 A. L14POUNOFF, SUR UNE SÉRIE DANS LA THÉORIE Remplaçons maintenant О par son expression # + ©'(). La fonction © ({) étant périodique à période 1, nous aurons 1 1 | 9 dt = 79 0 en vertu de quoi il viendra 1 1 1 „l Jeu [ет алое т В Qt. 0 0 0 0 Pour aller plus loin, nous devons définir d’une manière précise la fonction © (é), qui n’a été définie que par sa dérivée. C’est се que nous ferons en admettant l'égalité (36) | 904 = 0. D’ailleurs, pour simplifier les calculs, nous supposerons © (0) = 0(1) = 0. C’est une restriction; mais nous verrons qu’elle n’a rien d’essentiel. Cela posé, on trouve facilement 4 1 1 [гов ош fre 0 1 Ja at | AR = | sou + [oa 0 0 1 t, Je a (0, — 0) Q, di, = 5-4 | ров fort [ea 1 1 |? orat—2 | oc, 0 0 С DES.EQUATIONS DIFFERENTIELLES LINÉAIRES DU SECOND ORDRE À COBFFICIENTS PÉRIODIQUES. 41 et d’après cela il vient 1 (87) 4, = 5 — [rar [ в [о 90° dt. м 0 0 Nous avons établi cette formule dans la supposition que © (0) — 0. Mais il est facile de _ s'assurer que la formule est exacte quelle que soit la valeur de © (0). En effet, la constante caractéristique de l’équation dy + mp(+c)y= 0, с étant un nombre constant quelconque, est la même que celle de l’équation а? аа + UD (&) y = 0. . Donc, en considérant le développement de cette constante suivant les puissances du para- mètre м. on parvient à la conclusion que la valeur de A, ne change pas, si l’on remplace, da ns son expression, p(z) par p(x -+ с). Er _ Пе là il résulte que la valeur de a, ne sera pas changée, si l’on remplace la fonction © (0 par O(f+ <), « étant une constante arbitraire. |. Я Cela posé, prenons pour « une des valeurs de # qui annulent la fonction © (1), et dont l'existence est assurée par la condition (36). Nous aurons pour a, une expression qui s’ob- Вы ni a en remplaçant dans celle (37) la fonction 9 = © (0 par © (4 + <), et comme, dans cel Че expression, les intégrales пе porteront que sur des fonctions périodiques, nous pour- rons supprimer & sans changer les valeurs des intégrales. Nous retrouverons donc la for- mule (37). _ 17. En partant de la formule (37), on peut établir que l’expression (13) pour n = 3 rep réserite une limite supérieure pour A,. Tout d’abord nous remarquons que l'intégration par parties donne BR :; a 1 fora=—t | вто" 0 Par suite la formule (37) peut être présentée sous la forme а, = 375 — A fova 3 [eat [owner 0 San. Фив.-Мат. Отд. 42 A. Lıarounorr, SUR UNE SÉRIE DANS LA THEORIE . ou bien 1 1 1 г (38) nn] T(@" + 1) dt, 0 en posant 1 1 т | в°а— 18 [eu 607 0 0 “Or, en vertu de la supposition que la fonction р ne devient jamais négative, on a 9"+12>0, puisque l'égalité P(wt) = Q[t+0'(#)] donne w p(ot) = Q[1 + 9”(6)]; et nous allons maintenant montrer qu’on aura toujours F0: De là il résultera 1 A, < 750 et, par suite, (39) А, < 375 0, où le second membre est la valeur de l’expression (13) pour = 9 Pour établir l'inégalité T > 0, nous allons nous servir de la proposition connue que toute fonction périodique dont la dérivée est continue peut être développée en une série uni- formément convergente suivant les sinus et les cosinus des multiples de l’argument. En vertu de cette proposition, la fonction ©”(#) étant continue (puisque la fonction p est supposée continue), nous aurons, pour @’({), une expression de la forme 9’) = У (a, cos 2rkt + В, sin 2kt), les «, et les В, étant des constantes, et la sommation s'étendant à toutes les valeurs entières et positives de К, à partir de # — 1. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COERFICIENTS PÉRIODIQUES. 43 De là, en tenant compte de la condition (36), on déduit LA 06 = У р (%, sin 2rkt — В, cos 2rkt). Par ces expressions de ©’ et © on trouve *) | | 9’ dt = У (ав), 1 1 - | ©? dt 2 sr + BP), : | _ ве qui fait voir que VE 1 1 _ (41) | 0°? dt — 4m? | 0: dt > 0. у 1 0 0 _ En même temps, on obtient M DPI Va + Br» _ d’où, en remarquant que + NC ых Г _ Or cette inégalité donne 1 1 2T > [ea зв [oa 0 о < *) Remarquons que les formules (40), les «, et les В, étant donnés par des intégrales définies connues, sont “exactes dans des conditions beaucoup plus générales que celles admises ici. Dans une des séances de la Société Ma- À: ématique de Kharkow, nous avons montré que ces formules ne dépendent point de la possibilité du développement | de la fonction ©’ en série de Fourier et qu’elles sont valables toutes les fois que ©’ est ce qu’on appelle une fonc- ti ion intégrable, pourvu que cette fonction satisfasse à la condition Le dt = 0. зи 44 A. Lıapounorr, SUR UNE SÉRIE DANS LA THÉORIE et de 15, en vertu de (41), il vient T > 0. On voit d’ailleurs qu’on ne pourra avoir 7 — 0 que dans le cas où la fonction © est identiquement nulle. 18, L’inegalit& (39) donne, pour A,, une limite supérieure qui peut être utile dans les considérations que nous avons développées au n° 14. Eu introduisant au second membre de cette inégalité la quantité A,, on trouve Ar A 8 — 90 Donc, si l’on a (43) 4, > 54-4, —2, on pourra conclure l’inégalité A < Ин 62 et, par suite, celle-ci А > — 1. Il est d’ailleurs facile de montrer que la condition (43) assure aussi l’inégalité À < 1. En effet, en vertu de (28), cette condition n’est possible que si l’on a +A> A+ A —2, ou bien (44) А — 154, + 904, — 180 < 0, ce qui exige que À, ne surpasse pas le nombre 3,7859 ..., représentant la racine réelle unique de l’équation 43 — 152 + 90%— 180 = 0; et nous avons vu que pour À, < 6 on а toujours À < 1. Du reste il est facile d'obtenir, pour A,, une limite supérieure plus précise. _ En effet, l’inégalité (42), en vertu de (41), donne 1 or>(1—2)[o*a, 0 ce qui, eu égard à (35), peut être présenté sous la forme т> (1— =) (56). Le k DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 45 ыы Par suite, la formule (38) conduit à cette inégalité L 1 1 9\/1 | а, < я— в (1— =) (и—4), laquelle, dans le cas de р — const., se réduira à une égalité. En tenant compte de cette circonstance, on obtient, après avoir multiplié les deux membres par 0? 0°, A< nm —(13)2 (444), A AE 15 — 43 6x2 бое 4 ce qui donne la limite dont il s'agissait. En vertu de cette inégalité, si l’on a (45) (1—4, 4, > ВР AA 2, on aura certainement À = À, — 4,+2. _ Il est facile de voir que la condition (45), comme celle (43), ne peut être remplie que u satisfait à l’inégalité (44). Par suite, sous la condition (45), on aura, comme précé- _ demment, non-seulement À > — 1, mais encore À < 1. y On voit que la condition (44) embrasse un peu plus de cas que celle (34), à laquelle nous avons été conduit au n° 14. Mais on ne peut pas dire la même chose relativement à Ja condition (45) rapprochée de celle (32), puisque, pour des valeurs de À, assez voisines ) de 2, la condition (32) a, évidemment, plus d’étendue. Il serait important d’avoir, pour A,, une limite supérieure précise, correspondant à des / valeurs données de А, et A,. Mais la recherche de cette limite est, évidemment, un pro- _blème très difficile +. et nous ne nous y arrêterons pas. 19. Revenons à notre objet, la recherche des formules pour le calcul de A, et A,. _ Présentons la fonction р sous la forme p = C+®d" (x), 3 *) La difficulté de ce problème, où l’on doit avoir égard à l'inégalité @"” +1 Z 0, provient principalement de Ч la presence dans la formule (37) du terme Г 00/2 ar. _ Pour le cas, où ce terme est égal à zéro, nous aurions pu donner la solution du problème. Mais il serait inutile de la reproduire ici, puisque, dans ce cas, le calcul de A, ne présente pas plus de difficulté que le calcul de A,. 46 А. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE où C désigne une constante et Ф” (2) la dérivée du second ordre d’une fonction périodique Ф (x) = D satisfaisant à la condition | Ф (2) dx = 0. Nous aurons Q= Co, 0”) =-’® et, par suite, 9'0 =. $'@, 00—=7x PM). Donc il viendra Со? 2, = — 923 et les formules (35) et (37), eu égard à ce que A, = a, C"w”, donneront u) ‚_ 620% LA] rg ее 24 “hf dz, о w [07 [07 0306 Cw3 р : = D? dx +- 200 | sas | PH * dx. о 0 0 Telles sont les plus simples formules pour le calcul de A, et A,, dans le cas où l’on connaît le développement de la fonction р en série de Fourier. Par ces formules on voit que. A, se présentera sous forme d’une série simple, tandis que, pour A,, grâce à la présence dans son expression de l’intégrale [07 | ФФ”? dx, 0 on aura, en général, une série double. Mais, si cette intégrale est égale à zéro, on aura, pour À, aussi, une série simple. C’est ce qui aura lieu, par exemple, si Ф (x) est une fonc- tion impaire, ou, plus généralement, si, par un choix convenable du nombre «, on peut rendre la fonction ® (x +- x) impaire. Si l’on présente le développement de la fonction Ф” sous la forme со Ф” (x) = x C, sin en =) —=1 DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 47 les C, et les а, étant des constantes, il viendra со д a 2 24 167? k2 * > 4 Quant à l’expression de A,, sans nous arrêter au cas général, supposons que tous les Le soient égaux entre eux. Alors, en posant à ak | @ == @, == =... ==; _ nous aurons P'(a— x) = — P’(a + %) Г: t L . et, par suite, ke | P(a— x) = — P(u + x). Nous aurons donc to } | ФФ? ах =0, К. > А, Ber TS Соб У CNE 02 720 16r4 6 k2) k2 k—1 у u _ 90. Appliquons les considérations que nous avons développées à des exemples. у En premier lieu, considérons l’équation dy ae + С (1-- Л cos x + в cos 24) y = 0, Ф” (2) = С (À cos %+ u. cos 2x), D'(x) = or sin z + + 5 № sin 22), D (2) = — С (^ cos © + tu cos 2x ), et nous pouvons prendre w == 25. 48 А. LIAPOUNOFY, SUR UNE SÉRIE DANS LA THÉORIE Nous aurons donc 0) | ФФ’ 45 = — ст 03, 0 et les formules du numéro précédent donneront A, = 260; А, = zo — m (2) 08, Я == 2 08 — Sr Le = rn pi) CS + 4m Ce+ sw) 03 + mu Cr Pour pouvoir appliquer les résultats que nous avons obtenus, nous devons supposer que la fonction р = C(1 +2 cos x + u cos 2%) ne peut recevoir que des valeurs positives ou nulles. А cet effet nous devons supposer С > 0 et 1 + X cos & + cos 220, quel que soit x. Cherchons les conditions que doivent remplir À et pour que cela ait lieu. Tout d’abord, en posant successivement 1 == 0, æ = 5 t=r, on trouve ces condi- tions nécessaires 1+1+u20, 1—u>0, 1—À1+p>0. On voit donc que p. doit être compris dans l'intervalle (— 1,+ 1), et que À doit vérifier la condition (46) № <(1—+ в}. Dans le cas de u. x 0 cette condition devient suffisante, puisque, dans ce cas, le minimum de la fonction 1 + À 008% + cos 2% = DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CUBFFICIENTS PÉRIODIQUES. 49 est égal à la plus petite des deux quantités ТЪА-ы, 1—ЛА-ы; Ро et la même chose aura lieu dans le cas de м > 0, si l'on а ^* >> 162, се qui, en vertu de _ (46), exige que Гоп aitp<+. | Si, au contraire, p étant positif, on а А? < 1612, le minimum de la fonction ci-dessus sera égal à 12 1— М -— вк — (47) 22 < 8 (1 — в). Le second membre de cette inégalité est plus petit que le second membre de l’inéga- | С lité (46) toutes les fois que № n’est pas égal à =. Néanmoins l'inégalité (47) ne représente Е une nouvelle condition que dans le cas de u > =, car, pour | <=, elle sera remplie en . vertu de l’inégalité À? < 16u°. 6 _ En résumé, М étant la fonction de м définie par les formules M=(1+4), si U<—, Zu | M=8p(—p), si p>5 _ 1ез conditions requises pourront être exprimées par les inégalités suivantes : _ (48) —1I1 — 1, donne ps een: Е TA Don 5? et, Su > _ il faudra qu’on ait 32 2 2 — — —— HT ab TT ce qui exige M 168 7 20 508 On voit donc que р. doit être compris entre les limites 4 162 15" — = — = 0,275 “u... 812 — à +R 0,748... DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 51 | р 4 et que À doit vérifier les inégalités M>X> aa: Ces conditions étant remplies, les racines de l’équation 13-3® +3 г?) — 2%2=0 seront réelles, et comme le coefficient du premier terme est ici toujours positif, puisque в... + 1 < М ть Зи <, | on sutisra à à la condition (49) en prenant pour п* C une valeur quelconque, comprise entre Ч pentes racines. ns # Quant à ces racines, elles seront toujours comprises entre les nombres 1,548... et _2,823..., représentant les racines de l'équation (и ато, я ot seront séparées par le nombre 2. so 7 _ 99, Examinons maintenant la condition À, < A, — À, + 2, s laquelle on aura certainement À > — 1. En posant, pour abréger, + es mtr rt) + (4 ти) Os Im ru, ь nous aurons 4 4=®b0, A, —rac", et la condition en question prendra la forme nal? — nd? + 2m C—2 <0. 5 h . Nous allons montrer que, sous les conditions (48), La premier membre est une fonction A | croissante de C. 7* 52 é A. LIAPOUNOrF, SUR UNE SÉRIE DANS LA THÉORIE A cet effet, en remarquant que la dérivée de cette fonction est égale à (51) т? (3aC? — 2bC + 2), | il suffit d’e&tablir l’inégalité (52) P—6a<0, en vertu de laquelle l’expression (51) sera toujours positive. Nous avons Hi А и Ur ue “NE: SE FRE N b 6a =, + (5 Burst 24) в (5—5 в, d’où Гоп voit que, pour démontrer l'inégalité (52) en général, il suffit de le faire pour les deux valeurs extrêmes de À: 0 et М. Or, en posant À = 0, on trouve et, comme ps? ne surpasse pas 1, il en résulte 23 2 À B ie sn 0m où le second membre est, évidemment, négatif. Considérons ensuite l'hypothèse À = М. En supposant d’abord | < > nous aurons M = (1 в се qui donnera 1 10 16 97\ 8 4 D — ба = DU Е + (= 1— 28) 2 +( jt B3+rzZm— gm. Or il est facile de s’assurer que les coefficients de и? et de в sont ici positifs. Donc - cette expression ne surpassera pas sa valeur pour u = =, ce qui permet de conclure ve + SER Bi 130 _a 4 4 [72 ба < 42 16.81 81 + 57 П Ben et le second membre est ici négatif. x DES ÉQUATIONS DIFFÉRENTIELLES LINÉATRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 53 $ Soit maintenant м >, cas ой il faudra poser 4 № = 8u(1—). 3 - De, En le faisant et en remarquant que nous aurons une limite supérieure pour 6°— 6a À en remplaçant dans son expression т? par 10 et т* par 97, nous obtenons l'inégalité suivante : 5? — Ga < 60u! -- 88 м3 + 132 + 21u — 8 Le N 28 PAC EME TS Or, p. étant plus petit que 1, l'expression qui figure à la deuxième ligne est, évidem- ment, négative, Nous aurons donc à plus forte raison P— Ga < 60 — 883 + 12 -н 21, — 8, x. _ et le second membre se réduit ici à — 38 —(1— в [ (60 + 28) TE rer] _et, par suite, est négatif. Donc l'inégalité (52) est établie. Ne Ayant ainsi démontré que le premier membre de la condition (50) est une fonction _ croissante de С, nous pouvons conclure que cette condition est équivalente à celle-ci ох, À (53) о 6 — nr 2115 — 21 =0. Il est facile de s’assurer que x est toujours plus petit que 2. En effet, le premier membre de l'équation (53) étant désigné par f(x), on trouve Un Ве (тт — 2) + (32-=6и— 3") Re, _et cette expression, pour les valeurs considérées de x, est toujours positive. On a donc _ f(2)> 0, et de là, f(x) étant une fonction croissante, оп conclut bien x < 2 Ainsi on voit que, sous la condition (50), on aura toujours r° U< 2, et que, par suite, _ А, sera plus petit que 4. De là, eu égard à ce qui a été remarqué au n° 11, il résulte que sous la condition con- .sidérée on aura non-seulement À > — 1, mais encore А<1. 54 А. Lxapounorr, SUR UNE SÉRIE DANS LA THÉORIE 23. La quantité x est une fonction de À et x, et nous allons maintenant chercher les valeurs extrêmes de cette fonction, À et р. étant toujours assujettis aux conditions (48). En ce qui concerne la plus grande valeur de x, il est facile d'établir qu’elle uses à la supposition En effet, soient f(x) et x, ce que diviennent dans cette supposition f(x) et x. Nous aurons fix) = ho + [re (3 4 Вы] 2] + | (3 ох a et, comme on a f,(x,)— 0, il en résultera 1 —= [=— (3 m ’—4— чи)» JA + = ler T° — 1). — 1? | п Or nous venons de voir que x est toujours plus petit que 2. Donc on aura x, < 2, et en vertu de cela le terme en X? dans la formule obtenue sera toujours positif. É D'autre part, on peut établir que (er 1) x, — 7 > 0. A cet effet, la fonction f, (x) étant croissante, il n’y а qu’à établir l'inégalité (RD < Zr et on le fera aisément en remarquant que ДО = (5 mt— +" + Jar (7—4) 21 (x — 1), d’où il vient (ee (= ин) D’après cela l’expression ci-dessus de f(x,) permet de conclure Г (х,) > 0, et cette inégalité fait voir que l’on aura toujours x 2 < 212 —1 zn # $ | le coefficient de À? est ici toujours positif. ре > Done, en posant ат — mb < пм +0). Bi Voyons comment varie la fonction 9 (м) da l'intervalle (— 1,+ 1). о я == та М=(1-— u), et la dérivée 0’(u) de cette fonction sera donnée par 1 Vespression el: »—4— u) 21-2 [=— (3 = — 1) ] р. De là il vient 0'(— 1) = —+ [#— (5 nt — 1)=], (= Ferre). 56 А. Lıarounorr, SUR UNE SÉRIE DANS LA THÉORIE On a donc (—1)<0,, 5%, ce qui fait voir que l'équation 9' (2) =0, qui est du second dégré en pu, a une racine dans l’intervalle (—1, - 5) et que, cette racine étant désignée par м; оп à te) Oh. Bi, el neue и()>0, si bo LE з. Soit maintenant pe >=. Nous aurons M=8p (1 — м) et, par suite, d'u) = 8 [= — (+= —4— À) 2] (1—2u) + бедны | (5—1)з] и. Pour p. + on en deduira la même valeur que précédemment, ce que l’on voit im- médiatement par l’identité (1 и)? — 8 (1 — в) = (l— BR). On aura donc #’(1)> 0, et l’on trouve ‚ 15 2 9 (1) = — 5 м — (3—5) 2], се qui est une quantité négative. Donc l’équation 6’(k)= 0, qui, dans la nouvelle supposition, sera encore du second dégré, admet une racine dans l'intervalle (7 da et, si Гоп désigne cette racine par pu, on aura н x Bu) 20, я ee (u) < 0, и а ий Par suite de cela on arrive à la conclusion que la fonction 0 (м), qui varie toujours continüment avec y, décroît, quand p croît de —1 à fm, Die, wet. 8.07 Щи ПО Тиль м6 NT. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 57 Comme on a I 1) = 0 (1), _ И ев résulte que la plus grande valeur de 0 (4) dans l’intervalle (— 1, 1) correspond à = tu. 1 Donc nous aurons 4 2 В. ах — mb Зум 0 (м), d'où l'on voit que la plus grande valeur cherchée de f(x) correspondra à la supposition 1 Mi rasen) =. Soit F'(x) cette valeur. 4 Considérant 2 comme une inconnue, nous allons montrer que l’équation F(x) = 0 a une racine dans l’intervalle ( ) , et qu’elle n’en a d’ailleurs qu’une seule, at ne 3 Tout d’abord, il est facile de voir que, x croissant de 0 à 3 - 2 la fonction F(x) LT? — 8 _ croît constamment. _ En effet, en vertu de ce que nous avons montré au numéro précédent, on а f'@) > 0, le que 5016 la valeur réelle de x, pourvu que À et u vérifient les conditions (48). Or, , №) étant ce que devient f(x) en posant à №8 = Зы (1 — в), et x étant compris dans l'intervalle (9 ; Z ) ‚ опа MT: Zn — 3 La" 4 d’ où il vient Е (2) = f(x, 1), Ole), df(æ м) аш. EL Р'(® = | ва: Fi и 1% Ra et cette expression se réduit à FL F' (a) = Ton = ? puisque l'équation 0' (и) = 0, à laquelle satisfait y, est équivalente à celle-ci MUR | Be Yan) ( ou г ER Зап. Физ.-Мат. Отд. 8 58 A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE Donc on obtiendra F'(x), en posant dans la dérivée f’(x) № = 8p(l—p), pm et, par conséquent, on aura F'(x) > 0 pour toutes les valeurs de x dans l’intervalle considéré. Cela étant, pour justifier notre assertion, nous n’avons qu’à montrer que les valeurs 3—1 FO) еще ci ) ont des signes opposés, et, comme on а F(0) = f(0) = — 27", il ne reste qu’à établir l’inégalité А cet effet, nous remarquons que па |3 CYR rs 3 3 = Gin UE et à — — En 2m 97 +9 + Grp (1 — в) (4 +), et que l'équation 9’ (x) = 0, qui définit м, si l’on y pose se réduit à Зы бы — 4 = 0. Or, en vertu de cette équation, on trouve 14 4 № (1 — |) (4+ = TE, et, comme la racine que nous avons à considérer surpasse =, il en résulte ш (1— nu) (4 +1) > 1. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 59 Nous obtenons donc и (3—1) er zes а SR rt + 4° + 2, т 3 _ et le second membre est, évidemment, positif. Cela posé, soit x, la racine de l’équation F(x) = 0, _ dont l'existence vient d’être établie. Comme on а f(æ) < F(x) _ pour toutes les valeurs de x dans l’intervalle (9 : = ) , il s’ensuit » * Ш — 474 f (%o) = 0, et de 18 on peut conclure x> x. Donc x, est la plus petite valeur cherchée de x. D CHilona | POS %e; | L à condition (50) sera remplie, et l’on aura A? < 1, quels que soient À et в satisfaisant aux inégalités (48). Il est donc intéressant de connaître une valeur approchée de x,, et nous al- à Es former les équations dont dépend l'évaluation de x, avec la valeur correspondante de 4. Nous avons fu) = (3er + 2#— 2)+ 0a‘, | (54) [(62r? — 309) u — 108p°— 32 (m — 6)]x = 31? (314. — 16). En substituant la valeur de x, tirée de cette équation, dans l'expression de 9 (x), on Su? (312 — 64u + 28) 1 и — 16 Donc, en égalant f(x, x) à zéro, il vient 4 2 Bi Зы? (31 42 — 64 + 28) 5—3 +25 x mei) — a 8* 60 A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE Les équations (54) et (55) sont celles qu’il fallait obtenir. On pourrait en déduire une équation du 6-&me dégré en x, mais elle serait trop compliquée, et il est préférable de traiter directement les équations précédentes. Par ces équations, & et м étant assujettis aux inégalités 0Lr< ;—— > Zu в on trouve и — 0224071, 2 По, et la valeur de x est celle de x,. Donc, si l’on a rm C < 1,3859, on pourra conclure A? < 1, quels que soient A et x choisis conformément aux con- ditions (48). 24. Parmi les conditions, où ne figurent que les trois premiers termes de la suite А, Ay Ay À, ung et qui conduisent à des conclusions décisives à l’égard du signe de A? —-1, il y en a encore une, celle À, = À, NE À;, sous laquelle on aurait À > 1. Mais on s’assure aisément que cette condition est impossible pour l’équation considérée. . En effet, le premier membre de la condition (50) étant une fonction croissante de C, et C'étant un nombre positif, on a maC—rbC+2mC> 0, et cette inégalité n’est autre chose que SAN Donc, si pour l’&quation considérée on avait À > 1, on ne pourrait le constater que par la considération des termes qui suivent A,. 25. Pour un autre exemple, nous prendrons l'équation dy ge + À cos" æ y = 0, où » est un entier positif et À une constante positive quelconque. Comme on a Bi MOD eos (2n —4)z 7 2 2" cos" = cos 2nx + + COS (2n — 2)x + TE 2% (2n — 1)...(n + 2) cos 2% + + 1 2n(2n—1)...(n+ 1) NE CRT en Ann } ‘a qu’on peut présenter sous la forme A En - = ul +23 AT: k=1 _ nous aurons, avec les notations du n° 19, BR и BEN n g'@=20Y( +) (1-5). -(1 и cos 2х. #1 _ De là il vient [еее 0 Г п ое 2 Co 0 —ı m us aurons A | А, => С, =1(5— 2708 2 _ се qui donne DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. Ile, 61 62 А. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE En nous bornant à ces formules et en remarquant u la condition A, <2 ne demande aucune discussion, passons à celle-ci HEAR Cette condition se réduit à (56) (5—4) 4—4 +28 <0 et d’abord exige que les racines de l’équation (57) (5—1) #—та-2т = 0 _soient réelles, се qui s’exprime par l’inégalité (58) Fe Or, en se reportant à l'expression de J,, on voit que c’est une fonction croissante de n. Donc l'inégalité (58), si elle se trouve remplie pour une valeur donnée quelconque de n, le sera encore pour toutes les valeurs plus grandes. Pour x = 1 cette inégalité n’est pas remplie, puisqu'on a Mais pour n — 2 on la trouve déjà satisfaite, car 65 п? 10 60 heu т. et, par suite, elle sera satisfaite pour toutes les valeurs de n à partir de n — 2. Ainsi, sauf le cas de п — 1, les racines de l’équation (57) seront réelles, et, si on les désigne par x, et х,, en supposant x, < %,, la condition (56) se réduira à 2 Sa Up Voyons en quelles limites peuvent varier les valeurs de x, et x,, le nombre n étant plus grand que 1. Pour n — 2 l’équation (57) devient n2 65 9 (F- a)? —T°x + 21 — 0, DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 63 et, en la résolvant, on trouve 24% u = = er Pre as Sek +. 247% НИЕ ЕЕ АР | 2? бп— 130—122 4,8805.... р Ces formules donnent la plus grande valeur de x, et la plus petite valeur de %,, Car, _ J, étant une fonction croissante de n, x, le sera aussi et x, sera une fonction décroissante. On voit d’ailleurs que x, sera toujours plus grand que 2. On aura donc 2 << 3,3886..., m>4,8805.... D’ailleurs, » croissant indéfiniment, x, tendra vers 2 et x, croitra indéfiniment. Cela résulte de ce que u Tr? lim J, = 6°? n=cO mer (en Se m étant un entier quelconque plus petit que n. Donc, en faisant le nombre n assez grand, on pourra rendre la racine x, aussi voisine de 2 qu’on voudra et la racine x, aussi grande qu’on voudra. К Cela posé, si nous considérons À, comme une quantité donnée et indépendante du - nombre n, се qui est permis à cause de la présence du facteur X dans la formule + 2 4 = MEN, _ nous pouvons faire la conclusion suivante. | 1 Quelle que 501% la valeur donnée de A,, pourvu qu’elle soit supérieure à 2, la condition _ (56) sera remplie, dès que n sera assez grand. у Par suite, si À, >2, on aura toujours А — 1 pour des valeurs assez grandes de п. _ Я d’ailleurs la valeur de A, se trouve entre les nombres 3,3886... et 4,8805..., on aura A<—1 pour toutes les valeurs de n à partir de n = 2. 64 А. LiAPOUNOrr, SUR UNE SÉRIE DANS LA THÉORIE 26. Arrêtons-nous au cas de n très grand. En se servant de la formule de Stirling, on peut obtenir pour J, des expressions ap- prochées, où l’approximation pourra être poussée jusqu’à des termes de l’ordre voulu par rapport à =. Telle est, par exemple, l’expression п? Var | Re) + | 1 + qui diffère de J, d’une quantité du second ordre. Nous nous bornerons ici à une expression plus simple, celle т? var 6 о pour laquelle l'erreur est du premier ordre. А l'égard de cette expression on peut établir qu’elle représente une limite inférieure pour J,, de sorte qu’on aura т? Var (59) IE J, < НИ quel que soit n. On peut aussi établir l'inégalité suivante п? Var 2 qui est également exacte pour toutes les valeurs de n. Sans nous arrêter à la démonstration de ces résultats, remarquons seulement que nous les avons obtenus en partant des inégalités о 1 1.2.3...n < Vann ne "im, 1 1 == И — 1.2.3... > V2arn mn" e 12% 360%, Par l'inégalité (59) on voit que la condition (56) sera satisfaite toutes les fois que Гоп а (61) EE д, +28 0. DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À COEFFICIENTS PÉRIODIQUES. 65 Or cette dernière condition se réduit à и. К, Fe NZ эм ES et donne ainsi une limite inférieure des valeurs de п, pour lesquelles on aura 4 < —1, A, т ayant une valeur donnée plus grande que 2. _ Supposons maintenant qu’au lieu de À, l’on donne le nombre n. | Pour que la condition (61) soit possible, ce nombre doit être choisi conformément à E l'inégalité Я a 8V2 se, m nVren +18 ыы. ‹ _ laquelle exige que n ne soit pas inférieur à 5. Cela étant, si nous posons, pour abréger, 2 V2 rVrn — €, la à à condition (61) pourra être remplacée par celle que À, doit être compris entre les limites Der ST et ЛЕТИ Х Ces limites, pour de grandes valeurs de n, représentent des expressions approchées de _ 2 et x, et il est facile de voir qu'avec la même précision relativement à l’ordre de Геггеиг _ les quantités 2, et x, seront aussi données par ces expressions plus simples an re ou [bien par celles-ci | 2+ 2e + 246 et ET PRÊT Е Е ii En Nous nous arr&terons à ces dernières, dont la première représente une limite supé- rieure pour x, et la deuxième une limite inférieure pour 2,, comme on le voit par les абв Vl—4e > 1 — 2=— 2: — 246, а Бы qui donnent 2+9e+ 248 > AE 4; 2 1+1 — 4 Е Vega Зап. Физ.-Мат.Отд. 9 м: RES + 66 А. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE Nous parvenons ainsi à la conclusion que, si l’on a 2 (62) IE HN SER on aura certainement А < — 1. Maintenant, au lieu de A,, introduisons A. Nous avons 13:5. „ата 4, 2.4.6...2n 3 À. Or, en partant des inégalités Es 1 1 1 JS V2rn n° ee "* вв 360% * 12606 р 1 1 k ee 1.2.3...n> V2rnn”e Ian 360%, on parvient à celles-ci “FH TE > Vas Van In П viendra donc | x Vr 1 \ пул ^>4> (1 в) зи À 2Vn d’où l’on voit que les inégalités (62) seront satisfaites, si À vérifie celles-ci rn Vr 2 ву Sr 4 Ух 4 (1) DEAD 24 92e+ 0248; 2Vn et ces dernières, si l’on substitue au lieu de e sa valeur, se réduisent à 4Vn 8V2 N = 8Vn DR Ai on Se EU où An 8V2n 384-8n a NE ца &n—1)miVr к DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 67 On peut d’ailleurs simplifier cette condition en remplaçant N par 3, car il est facile de s’assurer que Гоп а toujours N < 3. Par suite, nous pouvons énoncer la conclusion suivante : Toutes les fois que À vérifie la condition DR 4 В LAEVIn— x Vr n3 8Vn rVr’ Di _ оп aura A — 1. 2 Remarquons que, pour la possibilité de cette condition, il suffit qu’on ait n > 5. Il est utile de rapprocher ce résultat de celui qui découle de la considération de la con- dition A, < 2, et qui peut être énoncé ainsi : Si À ne surpasse pas la quantité av rVr? > on aura À € 1. On voit done que, pour des valeurs de À qui ne surpassent pas le nombre Br ven rVr u (m n'étant pas inférieur à 5), le signe de 4? — 1 ne reste incertain que dans l’intervalle 4Yn à 4Ув , 8V2 ‚3 de кух rVr m3 Vn ? 27. Nous avons vu que sous la condition (32), à savoir, 42—244,+24(4,—2)<0 on aura toujours 4? < 1. _ Appliquons ce résultat à l'équation considérée, en nous bornant au cas de n très grand. En vertu de l’inégalité (60) on trouve RNA ESA 68 А. LIAPOUNOrF, SUR UNE SÉRIE DANS LA THÉORIE Par suite, tant que A, << A,, on aura A3 9A A, (+) dt (4) и Vn тп et la condition considérée sera remplie, si (63) L(E-2)4 if?) Pa ee Or on voit immédiatement que cette dernière condition, comme celle (32), n’est pos- sible que si À, est plus petit que 4, ce qui entraîne l’inégalité A, < A.. Donc, sous la condition (63), celle (32) sera toujours remplie, et nous aurons 4? < 1. Cela posé et en faisant, pour abréger, considérons l’équation 728—227 2%— 4 — 0. Cette équation n’a, évidemment, qu’une seule racine réelle, et, si l’on désigne cette ra- cine par %,, la condition (63) se réduira à À; < To. Développons la racine x, suivant les puissances ascendantes de », се qui donnera д = 2+4n+ 12» + ..., et arrêtons-nous à la valeur approchée 2 + 4n. En substituant cette valeur dans l’équation, on trouve que le premier membre se ré- duit à —8n(3—2%— 127 —8#), et il est aisé de voir que c’est une quantité négative. En effet, l'égalité DIE FLO ie)“ AT TR VER LT 1 4 : montre que l’on à n <>, d’où l’on voit que 21n + 12? + 8% < 3. Par suite, on peut conclure l'inégalité an % > 24 4n, N | | и en vertu de laquelle la condition (63) sera remplie, toutes les fois qu’on aura à Qi т + _ (64) A, <2+4n. me Or nous avons | ce qui fait voir que la condition (64) sera satisfaite, si À vérifie celle-ci EC vs = BIS + PT de set . ‘je sa et cette dernière condition, en remplaçant n par sa valeur, se réduit à AVn 872 16 À _—— —. = m7 Li T3 n3Vrn Done nous pouvons conclure que, si À ne surpasse pas la quantité 4Vn 8V2 16 | 5 x nVr T° TiVrn _ оп aura certainement 4? < 1. Ainsi l’intervalle dont nous avons parlé s’est réduit en Я PL COOP LA PP nVr rn n3Van” nVr 73 Vn |? ‘indéfiniment. Dans cet intervalle, l'équation A+1=0, и DES ÉQUATIONS DIFFÉRENTIELLES LINÉAIRES DU SECOND ORDRE À CORFFICIENTS PÉRIODIQUES. 69 où les limites diffèrent l’une de l’autre par une quantité tendant vers zéro, lorsque n croît étant considéré comme un nombre donné et À comme une inconnue, admet une ra- L u ine et, d’après une proposition générale que nous avons publiée, il y a trois années, 70 A. LIAPOUNOFF, SUR UNE SÉRIE DANS LA THÉORIE ETC. dans les Comptes rendus ($. СХХУШ, 10 avril et 1 mai 1899), elle n’en admet qu’une seule *). Pour cette racine, qui est la plus petite parmi les racines de l'équation А 1 = 0 (n'ayant que des racines réelles), nous obtenons ainsi une valeur approchée, savoir, AVn Re 872 nVr 23 ? | RR Re avec une erreur qui est inférieure à УЕ. N ^ *) En vertu de cette proposition, l’&quation transcendante А? — 1 — 0 (où le premier membre est une fonction entière de À), quel que soit l’entier positif и, admet, outre la racine évidente À — 0, une infinité d’autres, qui sont toutes réelles et positives, et ne peuvent être que simples ou doubles. Ces racines, rangées dans l’ordre croissant, étant désignées par ААА OR OR Tue, à condition que chaque racine double, s’il y en a de telles racines, soit répétée, dans cette suite, deux fois, les termes 17,2%,” à indice $ impair seront des racines de l’équation À + 1 — 0, et ceux à indice pair, des racines de l’équa- tion A—1= 0. D’après cela, si l’on entend par À, et par X, les valeurs de À pour lesquelles on a respectivement À, =%,, А, ==, , le nombre n étant supposé plus grand que 1, l'intervalle (A,,A,) ne pourra contenir qu’une seule racine de équation А? — 1 — 0. En effet, pour À — À, et À — },, la fonction A? — 1 а des signes opposés. Par suite, l’inter- valle (5, À,) contient un nombre impair de racines (toute racine double étant comptée pour deux), et, comme dans cet intervalle on a A, mn dy = À A, a N 1 > ых = \ & À у, ь | kn AL т И р He К в” 11 j AN In и Ve PER ie НИХ are