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The
Zlj as-Sanjarl of Gregory Chioniades:
Text, Translation and Greek to Arabic
Glossary
by Joseph Gerard Leichter
B.A., Queens College, CUNY, 1984
M.A., Queens College, CUNY, 1987
M. A., University of Illinois at Urbana-Champaign, 1992
Thesis
Submitted in partial fulfillment of the requirements
for the Degree of Doctor of Philosophy
in the Department of Classics at Brown University
PROVIDENCE, RHODE ISLAND
May, 2004
Copyright (c) 2004 by Joseph Gerard Leichter
CONTENTS
I Introduction 1
II Translation 18
Summary 19
1 The Known Epochs 21
1.1 The Nychthemeron^ the Month and the Year 21
Nature of the Nychthemeron 21
Nature of the Month 21
Nature of the Year 22
1.2 Epoch, Month and Year -Nature and Knowledge 23
Nature of the Epoch 23
Arab Epoch 24
Epoch of Mu^tadit 24
Roman Epoch 25
Persian Epoch 25
Epoch of Malikshah 29
Epoch of Nebuchadnezzar 29
Epoch of Philip 29
1.3 Beginnings and Conversions of Epochs 29
1.3.1 The Weekday on Which Years and Months Begin 30
vi
1.3.2 Days and Months of Each Epoch 31
1.3.3 Conversion of Epochs 33
1.3.4 Elevation of Years and Months 33
1.4 Weekdays and Epoch Conversion by Tables 34
1.4.1 Weekday on Which Years and Months Begin 35
Roman 35
Persian 36
Sultanic 36
1.4.2 Extraction of Epochs from The Arabic Epoch 37
1.5 Easter and Other Feasts 38
1.5.1 Lunar Mansions 39
1.5.2 The Great Christian Fast 39
1.5.3 Other Christian Holidays 40
1.5.4 Muslim Feast and Fast Days 41
1.5.5 Persian Feast and Great Days 45
1.5.6 Names of Persian Days and Months 48
1.5.7 Christian Feasts, Great Days and Month Names 49
2 Trigonometry 52
2.1 On Interpolation 52
2.1.1 Interpolation Continued 54
2.2 Arcs of Sines and the Sagitta 54
2.2.1 Interconversion of Arc and Sine 55
2.2.2 Interconversion of Arcs and Sines with a Table 56
2.3 The Tangent 56
3 Declinations, Latitudes, Rising Times 57
3.1 First and Second Declination 58
3.2 Latitude of Cities 58
vii
3.2.1 Latitude by Stars 59
3.3 Mid-Day Altitude of Sun and Stars 59
3.4 Rising Times 60
4 Ascensional Difference 62
4.1 Rising Azimuth 62
4.2 the Ascensional Difference and its Sagitta 63
4.2.1 On the Arrow of the Day 64
4.3 Length of the Nychthemeron 64
4.3.1 On the Equinoctial Hour 65
4.3.2 Seasonal Hour 65
4.4 Rising Times 65
5 Motion of the Fixed Stars 67
5.1 True Longitude of the Stars 68
5.2 Latitude 68
5.2.1 On Learning the Distance of the Stars from the Circle of the
Equalization of Daylight 69
5.2.2 On the Knowledge of the Ascent of the Equation of Daylight . 69
5.3 Simultaneously Culminating Degree 69
5.4 Simultaneously Rising Degree 70
5.4.1 Simultaneously Setting Degree 71
5.5 Time of Rising 71
6 Hours of the Day 72
6.1 Solar Arc from Altitude 73
6.1.1 Altitude Given the Solar Arc 73
6.1.2 At Night 74
6.1.3 Seasonal Hours Since Risiner 74
vni
6.2 Hour from Rising Time 75
6.2.1 Rising Time and the 10th House 75
6.3 Arc from Rising Time 76
6.4 Apprehension of the 12 Houses 76
6.5 Direction of Altitude 78
6.5.1 Direction of Rising Continued 78
6.5.2 Direction of Rising Continued 79
6.6 Terrestrial Meridian 79
6.7 the Qibla 80
7 Mean Motion of the Planets 82
7.1 Mean Motions for 90 Degrees 83
7.1.1 Correction of the Apogee 85
7.2 Correction of Mean Planetary Motion 85
7.2.1 Nativity Casting 86
7.3 Sultanic Years 86
7.3.1 Sultanic Year 87
7.3.2 Ordinary or Intercalary Year 87
7.4 Radix of the Solar Longitude 88
8 True Position of the Planets 90
8.1 True Longitude of the Sun and Planets 92
8.1.1 True Solar Longitude 92
8.1.2 Lunar Longitude 93
8.1.3 Longitude of the Node 95
8.1.4 Planetary Longitudes 95
8.2 Direct and Retrograde Motion 97
8.2.1 Direct and Retrograde Motion 97
8.2.2 98
ix
8.3 Planetary Latitudes 98
8.3.1 Lunar Latitude 98
8.3.2 Latitude of the Outer Planets 99
8.3.3 Latitude of Venus 100
8.3.4 Latitude of Mercury 101
8.4 Solar and Lunar Velocity and Diameter 104
8.4.1 Solar Diameter from Velocity 104
8.4.2 Lunar Diameter from Velocity 104
8.4.3 The Diameters and Velocities from Tables 105
9 Parallax 106
9.1 Various Methods of Calculation 106
9.1.1 Angle between Ecliptic and Circle of Altitude at the Ascendant 106
9.1.2 At General Position 107
9.1.3 On the Three Cases of Angles 107
9.1.4 Parallax from the Tables 108
9.1.5 Components of Parallax in Longitude and Latitude 109
9.2 Parallax from Theon's Tables 109
9.2.1 Tables Continued 110
9.2.2 Useful Things for Parallax Ill
9.2.3 Correction for the Degrees of the Zodiacal Signs Ill
9.2.4 Interpolation for Geographical Latitude 112
9.2.5 Correction for Lunar Anomaly 112
9.3 Longitudinal and Latitudinal Lunar Parallax 113
9.3.1 Direction of Longitudinal Parallax 113
10 Luni-solar Conjunctions and Oppositions 115
10.1 Conjucntions and Diameters 115
10.1.1 (Determination of the Hour) 115
X
10.1.2 Variant 117
10.1.3 Determination of Longitude 117
10.2 Lunar Eclipses 118
10.2.1 Whether an Eclipse Will Occur or Not by Computation .... 118
10.2.1.1 Conditions for Latitude 118
10.2.1.2 Condition for Eclipses 119
10.2.1.3 Partial Eclipses 119
10.2.1.4 Duration of the Phases of Eclipses 120
10.2.1.5 Duration of Totality 120
10.2.2 On the Eclipse of the Moon by Means of Tables 121
10.2.2.1 (Magnitude) 121
10.2.2.2 Time of a Lunar Eclipse 122
10.2.2.3 Time of a Lunar Eclipse Continued 122
10.3 Third Calculation 122
10.3.1 Solar Eclipse Tables 123
10.3.1.1 Interpolation of Parallax for Geographical Latitude . 123
10.3.1.2 Interpolation of Parallax for Longitudes within a Zo-
diacal Sign 123
10.3.1.3 Correction for Lunar Anomaly 124
10.3.2 Methods of Computation, Correction for Parallax 124
10.3.2.1 On the Correction of the Hour of the Mid-Eclipse . . 126
10.3.2.2 Whether an Eclipse Will Occur or Not 128
10.3.2.3 On How Much of the Sun will be Eclipsed and the
Knowing of the Time by Means of a Table 129
11 Visibility of Moon and Planets 131
11.1 On the Necessary Computations 132
11.1.1 132
XI
11.1.2 Parallax 133
11.1.3 Equation of Time 134
11.1.4 Correction for Latitude 134
11.1.5 Ripeness of the Crescent 135
11.1.6 Delay of Moonset after Sunset 135
11.1.7 Arc of Sun Below Horizon at Moonset 135
11.1.8 Altitude of the First Crescent 136
11.2 Angles 137
11.2.1 The Arc from 10 until 12 Degrees 137
11.3 First Visibility of the Moon 138
11.3.1 First Visibility of the Moon 139
11.3.2 Second Visibility 139
11.4 First Visibility in Digits 140
11.4.1 Sighting with Astrolabe 140
11.5 First and Last Visibility of the Planets 141
11.5.1 Appearance and Disappearance 142
11.5.2 Date of Planetary Rising and Setting 142
11.6 First Visibility of the Moon 143
11.6.1 Arc of Time 143
11.6.2 (Variant) 144
12 Year Beginnings and Nativity Casting 145
12.1 Beginnings of Complete Years 146
12.1.1 Entrance of the Years 146
12.1.2 Entrance of Place of 'Tortune" 147
12.1.3 Rising Time for the Middle of the Earth 148
12.2 Configuration of Celestial Bodies 149
12.2.1 Distance of the Stars from a Center 149
xn
Xlll
12.2.2 Circle of Motion 150
12.2.3 Aspects 150
12.2.4 Aspects from Rising Times 152
12.3 Motion of the Haylaj 154
12.3.1 Degree of the Haylaj 155
12.3.2 Degree of the Haylaj Continued 156
12.4 Motion of the Degree of the Fortune 158
12.4.1 Motion of the Fortune in a Year 158
12.4.2 159
12.4.3 Motion of the Fortune of the Entrance 160
12.4.4 Motion of the "Fortune" Continued 160
A First Scholium 162
III Glossary 163
IV Greek Text 366
PART I
Introduction
Introduction
The Characters
Gregory Chioniades
The main sources for the biography of Gregory Chioniades — bishop, physician, and
translator of Persian and Arabic texts — are the prologue of Chrysococces's Persian
Syntaxis^ 15 or so letters written by Chioniades himself, a short text entitled the
Profession of Faith^ and the Greek texts of az-Zij as-Sanjar^ az-Zij al-^AWi and
the Zij-i IlKhdm . ^
In his prologue to his Persian Syntaxis^ written circa 1347^, Chrysococces begins
by reminding his bother, John, that he had wanted to learn this Persian Syntaxis for
a long time. He then states that he acquired a teacher named Manuel in the city of
Trebizond. Manuel explained to Chrysococces 'how this Syntaxis came from Persia
and who translated it into Greek'. There was, he explained, a certain Chioniades
who, after growing up in Constantinople, fell in love with the sciences. Since he
heard that unless he travelled to Persia he would never satify his desire, he set out
^See Westerink [13] for a complete discussion of the sources, as well as for the text of the
Profession of Faith.
^ az-Zij al-^Ald^i has been edited and translator by Pingree [7]. Zij-i IlKhdm is lost, but was
th basis for Chrysococces' Persian Syntaxis.
^Pingree [6] p. 141, Westerink [13] p. 234
to go there. After this Chioniades passed through Trebizond,
... in a short while he was taught by the Persians, having both con-
sorted with the King, and met with consideration from him. Then he
desired to study astronomical matters, but found that they were not
taught. For it was the rule with the Persians, that all subjects were
available to those who wished to study, except astronomy, which was
for Persians only. He searched for the cause, which was that a certain
ancient opinion prevailed among them, concerning the mathematical sci-
ences, namely, that their king will be overthrown by the Romans, after
consulting the practice of astronomy, whose foundation would first be
taken from the Persians. He was at a loss as to how he might come to
share this wonderful thing. In spite of being wearied, and having much
served the Persian king, he had scarcely achieved his objective; when, by
Royal command, the teachers were gathered. Soon Chioniades shone in
Persia, and was thought worthy of the King's honor. Having gathered
many treasures, and organized many subordinates, he again reached Tre-
bizond, with his many books on the subject of astronomy. He translated
these by his own lights, making a noteworthy effort. There are in fact
other books of the Persian Syntaxis which he translated, those having
certain examples with the years systematically at the beginning. How-
ever, he handed on the Syntaxis alone, the best and most accurate of
all, as our teacher said, who appeared to be telling the truth. He trans-
lated seperately the commentary, which was taken from the Persians by
word of mouth alone. In this way, the Syntaxis, called the Handy, was
produced.^.
From this we learn among other things that Chioniades' work forms the basis for
the Persian Syntaxis of Chrysococces and that Chioniades went through Trebizond
on his way to study astronomy in an unnamed Persian city. It is clear from the
letters of Chioniades, however, that the city to which he travelled was the Mongol
capital, Tabriz.
The letters^ of Chioniades which are important for a reconstruction of his life are
^The translation of this paragraph is from Mercier [4] pp. 35-36
^ These are collected in I. V. Papdopoulos, FpriYopLou Xioviahou toO daTpovo^ou 'ETiLaxoXaL,
'EnioTTWiovixfi ' ETi£Tir]pl^ xf]^ $LXoaocpLxf]^ ExoXf]^ toO navsTiLaTrj^Lou ©eaaaXovLxf]^, I (1927), pp.
151-205.
summarized in Westerink as follows:^
• Letter 4. This was written in Constantinople to Constantine Lucites. It states
that thanks to the warm reccommendations of Chioniades, many students from
Constantinople were able to go to Trebizond to follow the courses of Lucites.
• Letter 5. This was written in Constantinople to the emperor Alexis II (1297
— 1339) of Trebizond. In this letter Chioniades states that the emperor of
Constantinople (Andronicus II Palaeologus 1282 — 1328) and the Synod had
made him archbishop of Tabriz, and so he was asking for permission to cross
the territory of Trebizond on the way to his diocese. He promises to pay back
the emperor in services.
• Letter 6. This was also sent to to the emperor Alexis II (1297 — 1339) of
Trebizond. Chioniades received the requested permission.
• Letter 7. This was written to Lucites of Constantinople. In this letter Chioni-
ades denies having calumnied or insulted his correspondant.
• Letter 8. This was sent to Lucites from Trebizond. Lucites has gone into
campaign with the emperor. The date of the expedition is September 1301.
• Letter 9. This was written in Tabriz to the partriarch. A patriarchal letter has
been read to the Christian people. The precarious position of Chioniades in
the midst of the barbarians is described. He apologizes for not being able to
do a canonic visit to the patriarch, citing his old age and the dangers of travel.
• Letter 10. The axpaxriyLXciTaTOc; to whom Lucites will give the letter is un-
doubtedly the emperor himself. Alexis is on campaign, and he should come
back quickly for the feast of the Martyrs (Eugene and his companions, 21
January).
• Letter 11. This is written to an archbishop. Chioniades excuses himself for not
being able to travel because of his health and becasue of Lent.
• Letter 12. This is written to Lucites. Chioniades must make a demand that he
finds embarassing. Westerink suggests that it might be a request for money.
• Letter 15. This was written to a certain John — 6 yXuxuc; 'Icodwrjc;. This is
perhaps the emperor John Glykus (before his patriarchate of 1315 -1319).
Another important biographical document is the Profession of Faith^ 'O^oXoyLa
ToO LaxpoaocpLaToO XLOVLdSou, dated to about 1305. After spending so many years
among the Persians, the Chaldaeans and the Arabs, Chioniades had apparently been
^Westerink [13] pp. 235 - 236.
5
accused of heterodoxy and of astrological superstition, and wrote the Profession in
defense of himself/ It is also possible that it was written as a result of Chioniades'
nomination for the episcopate of Tabriz, since it was in 1304 that the Mongolian
Ilkhans, whose capital was Tabriz, opted definitively for Islam. ^ The Profession^
Westerink notes, ^ could have been a way for Chioniades to distance himself from
that conversion.
The following is a summary of the Profession'}^
Submitting with filial piety to the direction of the patriarch, Chioni-
ades wants to repeat publicly the profession of faith that he has already
committed during a private interview with his patriarch. Some suspect,
he says, that because of his long stay among the Arabs he has been pol-
luted by their beliefs. If such a thought ever came to him, he should
share the punishment of Judas, his body should be devoured by the ani-
mals and the birds of prey and the worm that never dies. He declares as
anathema 1) those who believe that Moses and the prophets relied upon
astrology for their predictions and miracles, 2) the fatalists and 3) those
who regard Chaldaean theology as superior to that of Moses. If he has
ever expressed any Jewish, or Ismaelite doctrine other than to expose its
fallacies, his name should be erased from the book of life. He declares a
curse against those who do not accept the seven Ecumenical councils.
Based on the evidence presented above, as well as on some other documents,
Westerink provides the following tentative sketch of the life of Chioniades:
• 1240 or 1250 - Chioniades is born. (Letter 9, in which he speaks of himself as
an old man, can probably be dated between 1310 and 1314. This would place
his birth 65 to 75 years earlier according to Westerink. )
•
1294 - He begins the study of astronomy and of the Arabic and Persian lan-
guages, perhaps in Trebizond^^.
^Westerink [13] p. 236. The Profession of Faith is reproduced in Greek ibid,, pp. 243 — 245
^Westerink [13] p. 240.
i^Westerink [13] p. 242.
^^ See the discussion of some of Chioniades' early notes on the subjects on ff. 113-115 of Smith
Western Add. in Pingree [7] pp. 18 ff.
• 1295 - 1297 - He studies in Tabriz with Shams al-Bukhan and does preliminary
work on the zijesP
• 1297 or 1299/1300 - He returns to Trebizond (He is already a priest at this
time).
• 1301 -1302 - He is in Constantinople^^
• 1305 - He is ordained a bishop (letter 5) and writes the Profession of Faith.
• 1310 - 1314 - He is again in Tabriz (letter 9).
• After 1315 - He stepped down and lived as a monk. (Letter 11, in which
Chioniades is referred to as a monk, might belong to this period)
al-KhazinI
Abu Mansur '^Abd al-Rahman al-Khazinl was the Greek slave of Shaykh al-^Amld
al-Qadl Abu al-Hasan '^AlT ibn Muhammad, al-Khazin, who resided in Merv, the
modern Mary in Turkmenistan^^. al-Khazinl's floruit is given as ca. 1115. After he
was given an education in mathematics, the philosophical disciplines and geometry,
he was employed by the Seljuk court as a mathematician, most likely at Merv. It was
here that Sanjar ibn Malikshah ruled and that al-KhazinI composed az-Zij as-Sanjari
in his honor.
al-Khazinl's two other known works are the Risdla fi^ l-dldt (Treatise on In-
struments) and Kitdb mizdn al-hikma}^ The Risdla is found in codices 682 f.l and
681, pp 1-32 of the library of the Sipahsalar Mosque in Teheran and has not yet
been published. ^^ It is a short work concerning several astronomical instruments.
^^Here Westerink assumes Chioniades is the author of the Greek az-Zij as-Sanjari, az-Zij al-^ AWi
and the Zij-i IlKhanT , an assumption which will be discussed shortly. See Pingree [7] p. 21 for the
dating of these texts.
13 Pingree [7] p. 22 notes that the tables of the various zijes were put in their final form by
Chioniades in Constantinople.
^^The following description of al-KhazinI is adapted from Hall [3].
^^ See Hall [3] p. 338 ff. for a complete bibliography of these two works.
i^See SayiH [10].
including the astrolabe. The Kitdb has been published as the Kitdb mizdn al-hikma
(Hyderabad, Deccan, A. H. 1359 [A.D. 1940-1941 ]) and as the Mizdn al-hikma^ Fu'ad
Jaml^an, ed. (Cairo, [1947]). This text deals with weights and the construction of
balances.
Shams al-Bukharl
Shams is described in full in Pingree [7], pp. 16 - 17. He was born 11 June 1245
in Bukhara. His references to NasTr al-Dln at-TusT indicate that he may have had
contact with the famous observatory at Maragha^''. Shams was also the author
of several astronomical treatises, Greek translations of some of which have come
down to us in the same manuscripts as Chioniades' work. These include On the
Genethlialogical Computation^ which concerns the horoscope of a certain Fakhr al-
Dln born in Tabriz on 25 August 1268^^ and a treatise on the astrolabe dedicated to
Andronicus Palaeologus (Andronicus II, Byzantine Emperor 1282 - 1328).^^ Shams
al-Bukharl was in Tabriz in the 1290's, as is clear from example computations in
az-Zij al-^AWi ?^ It is also clear that he was Chioniades' teacher, since Chioniades
himself mentions the ''oral teaching" of Shams in the Revised Canons of az-Zij al-
^AWi — dcTio cpcovfjc; xoO Sa^cJ; MTiouxocpfj,^^ as well as in the second appendix of
az-Zij as-Sanjan — OLub cpcovfjc; xoO Sd^cJ; .
I'^Pingree [6] p. 143.
^^Pingree [7] p. 16.
i9pingree [7] p. 17 notes that this is found in v ff. 237 - 245v, Vaticanus graecus 210, ff. 3-7v,
and Marcianus graecus 309, ff. 154-160v. A large fragment is also found in Parisinus Coislin 338,
ff. 259-261V, he states.
^opingree [7] p. 17.
2ipingree[7] p. 306-307.
History of az-Zij as-Sanjari
The text of az-Zij as-Sanjan ( the Astronomical Handbook of Sanjar ) has had a
complex history^^. The Zij was originally composed in Arabic in Iran by Abu Mansur
'^Abd al-Rahman al-Khazinl and dedicated to the Sultan, Sanjar ibn Malikshah, who
ruled from 1118 to 1157. This version exists, at least partially, in two incomplete
manuscripts: Oriental 6669 of the British Library, dated by the scribe to 26 July
1223 A.D. and Arabo 761 of the Vatican Library. Each of these manuscripts of the
Zij has 13 chapters, or maqdldt^ ten of which are devoted to the central astronomical
material of the Zy (though the London manuscript omits all of maqdla 10). There
are also about 145 astronomical tables that belong to this version of the Zij but
neither of the two manuscripts contains all of them.
In 1131 AD an Arabic epitome of this first version of the Zij was made by Khazinl
himself, and was named the Wajiz. This summary exist in two essentially complete
manuscripts: number 859 in the Hamadiye Collection in the Suleymaniye Library
in Istanbul, and number 682 in the Library of the Sipahsalar Mosque in Teheran.
The date of copying of the former is given in the manuscript as between 8 December
1268 and 5 January 1269. The date of the copying of the latter is given as between
31 May and 29 June 1234. The Wajiz covers the same material as the 10 central
maqdldt of the first version of the Zij but in 12 maqdldt. As for the astronomical
tables, the Wajiz contains only 45, of which 30 are related to material in the Zij.
Gregory Chioniades translated this Wajiz into Greek in Tabriz in the 1290's,
with the help of his teacher. Shams al-Bukharl^^. There are three manuscripts of
this version: Vaticanus Graecus 211, copied before 1308; Laurentianus 28, 17 Flo-
rence, copied in 1323; and Vaticanus Graecus 1058^^, copied in the middle 1400's.
^^The following textual history of the Zij is adapted from Pingree [9].
^^Pingree[6]
^^ Vaticanus Graecus 1058 is clearly a direct copy of Vaticanus Graecus 211.
With the exception of a few passages, some clearly attributed to Shams al-Bukharl,
Chioniades' translation is a fairly faithful rendering of the Arabic of the Wajiz. There
are forty-one astronomical tables in Chioniades' version, but they are preserved only
in the two Vatican manuscripts. Thirty three of these tables are similar to tables in
the Wajiz.
Nature of the Text
Authorship
Pingree [6, 7, 8] suggested that Chioniades was the author of the Greek of az-Zij
al-^AWi and az-Zij as-Sanjan. In short, he has argued, ^^ we have the testimony of
Chrysococces, who states that he is basing some of his work on a set of astronomical
tables which were translated into Greek by Chioniades. ^^ Some of these tables to
which Chrysococces refers are found in the Greek version of az-Zij as-Sanjan. This
Greek version was made in Tabriz, which we know from his letters '^^ that Chioniades
visited. Pingree then concluded that it was likely that Chioniades was the author of
these texts.
Mercier, however, has argued somewhat unconvincingly, that since some of the
material in Chrysococces's work is taken from the Zij-i IlKhdni of NasTr al-Dln
at-TusT, Chioniades cannot be the author of those two Greek zijes. Pingree^^ has
pointed out that while some of Chrysococces's material is taken from NasTr al-Dln
at-TusT's Zij^ most of the material is in fact taken from az-Zij al-^AWi and az-Zij as-
Sanjan. In addition, Mercier's suggestion seems to ignore completely Chrysococces's
own words as to the authorship of the source of his work.
^^The following argument summarizes Pingree [8] p. 436
^^See page 3 of this introduction and following.
^^See page 4 of this introduction and following.
^^ Pingree [8].
10
What is perhaps another indication that Chioniades was the author of az-Zij as-
Sanjan is the way Muslims and the Islamic faith are described in that work. Time
after time^^ they are referred to as the impious (ol daepsLc;.). Their daily prayers
are referred to as 'an accursed cry'. The author calls down God's wrath on the
city of Mecca. It could be the case that this was the way Muslims were usually
refered to in Constantinople at that time. It could also be the case that the author
was trying to distance himself from Islam. We must recall that in 1305 - about
the time these zijes were put in their final form ^^- Chioniades was called upon to
write the Profession of Faith^ a work in which he refers to unbelievers as xcov octi'
alcovoc; aae^cdv^^. These disparaging remarks made in az-Zij as- Sanj an Siie perfectly
consistent with an author who had been trying to defend himself against a possible
charge of heterodoxy - the very position in which Chioniades found himself in in the
early 1300's.
It also seems fairly clear that az-Zij al-^AWi and az-Zij as-Sanjan are works
of the same author. They have come down to us as a group in the manusrcripts.
The authors of both mention Shams al-Bukharl as a teacher. ^^ Neugebauer has
noted^^ that ''this [mention of Shams al-Bukharl in both zijes] shows that it is not
accidental that the text and table of the az-Zij al-^AWi are combined in the same
manuscript with text and tables of the az-Zij as-Sanjan^ Both zijes not only use
the same technical terminology,^^ but also the same incorrect technical terminology.
For example, in chapter forty-one of az-Zij al-^AWi , the author writes Tiepl xfjc;
^^See 1.5 of the text of az-Zij as-Sanjari for a few examples
^opingree [7] p. 22.
^^Mercier [4] p. 244 1.39
^^See page 7 of this introduction.
^^ Neugebauer [5] p. 31 .
^^See Neugebauer [5].
11
expoXfjc; xfjc; xuxiQ^^^ ''on the extraction of the fortune" , when he clearly means not
fortune (tuxtq)? but ascendant.^^ This type of repeated egregious error would suggest
that rather than being the work of a ''school" of Greek scholars working in Tabriz,
these texts are the work of a single individual.
The Method of Translation
Unlike az-Zij al-^AWi ^ which seems to have been composed by Chioniades in Greek
via a Persian intermediary (i.e., Shams would orally translate Arabic into Persian,
which would then be translated into Greek by Chioniades^''), az-Zij as-Sanjanseems
to have been composed directly from Arabic with the help of a small Arabic-Greek
dictionary. That this was the method of translation seems clear from the fact that
there are far fewer transliterations of Arabic technical terms in the text than in
Chioniades' version of az-Zij al-^AWi^^ ^ and there are seemingly no Persian terms. ^^
The size or rather complexity of the dictionary Chioniades used is perhaps best
indicated by the fact that apxiQ is used to translate such varied terms as Jjl, iiaU,
Jfli"Xo,?^IIio, j^lj and Ijj. This lack of transliterations of Arabic technical terms
- transliterations which abound in az-Zij al-^AWi — would also seem to indicate
that az-Zij as- Sanj an wSiS composed later than az-Zij al-^AWi ^ during which time
^^Pingree [7] p. 184.
^^See page 11 of this introduction for a discussion of the (mis)use of tuxtt] for the term 'ascendant'
in az-Zij as-Sanjari.
^^See Pingree [7] p. 17.
^^See Pingree [7] pp. 395 - 401. See also the glossary of the az-Zij as-Sanjan.
^^The one notable exception is perhaps Chioniades' use of totioc; Tf]c; tuxttjc; -place of fortune- for
the Arabic term »i\]AA,rising time. Jli? in Persian means luck, which may explain Chioniades' use
of terminology involving the word tuxtt). This, however, is a mere guess.
12
Chioniades had improved his Arabic!^^
Technical Commentary
Neugebauer [5] provides an extensive discussion of the technical terms and techniques
used in Chioniades' az-Zij as-Sanjan. A full technical commentary, however, will be
provided with the edition of the Arabic Wajiz.
Notes on the Present Text
The Edition of Chioniades' az-Zij as-Sanjari
The sigla for the edition of Chioniades' text of az-Zij as-Sanjan are as follows:
• V - Vaticanus Graecus 211, ff. 38-106, copied before 1308.
• V - Vaticanus Graecus 1058, ff. 273v-316, copied in the middle 1400's and a
direct copy of V.
• L - Laurentianus 28, 17, Florence, ff. 81-167, copied in 1323.
A complete list of the other contents of these manuscripts is given in Pingree [7] pp
23 - 28. What follows is a partial list of the contents of the manuscripts:
• Ff. Ir - 74r. The Persian Composition of Astronomy.
• Ff. 74r - 79v. On the Genethlialogical Computation.
• Ff. 169r-178r. ^Ilm al-hay'a text.
• Ff. 179r- 201r. Revised Canons.
• Ff. 201r- 223v Short astronomical texts based on Shams al-Bukharl, az-Zij
as-Sanjari.
^^This is consistent with the dating for the two texts proposed by Pingree [7] p. 21 ff. on internal
evidence.
13
— V—
• Revised Canons.
• Ff. 37r. Arabic-Greek glossary preceeding chpater 23 of The Persian Compo-
sition.
• Ff. 38r-106r. az-Zij as-Sanjan.
• Ff. 106v-115r. ^Ilm al-hay'a text.
• Ff. 122r-159v. Tables of az-Zij as-Sanjan.
• Ff. 161v-234r. Tables of the Persian Composition [az-Zij al-^AWi).
• Ff. 92r-118v. George Chrysococces's Introduction to the Persian Composition.
• Ff. 237r-245v. Shams al-Bukharl's On the Use of the Astrolabe.
• Ff. 261-272v. Revised Canons.
• Ff. 273v-316r. az-Zij as-Sanjari.
• Ff. 316r-321r. ^Ilm al-hay'a text.
• Ff. 332r-369v. Tables of az-Zij as-Sanjari.
• Ff. 370r-440v. Tables of az-Zij al-^AWi .
The English Translation of Chioniades' az-Zij as-Sanjari
The works referred to in the translation are as follows:
• Al - 859 in the Hamadiye Collection in the Suleymaniye Library in Istanbul
• A2- 682 in the Library of the Sipahsalar Mosque in Teheran.
• A - di reading in the Wajiz where both Al and A2 agree.
• Biruni - Chronology of Ancient Nations. See Alblrunl [1]
14
• Ginzel - Handbuch der mathematischen und technischen Chronologie. See
Ginzel [2]
• Neugebauer - ''Studies in Byzantine Astronomical Terminology" . See Neuge-
bauer [5].
Greek - Arabic Glossary to Chioniades' az-Zvj as-Sanjari
The glossary was made by comparison of the Greek of the edition of az-Zij as-Sanjan
to the Arabic of the two manuscripts of the Wajiz.
Software
This text was typeset with various flavors of Donald Knuth's TgX, including emTgX
teTgX and MiKTgX. ArabTgX and IbyGreek were employed for the critical edition,
as well as a version of EDMAC modifled to produce an apparatus criticus consistent
with that of the flrst volume of this series. Perl and Java were used extensively, as
was the macro package LaTgX. The text editor used was Emacs.
15
Chrysococces's Prologue to the Persian Syntaxis
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XapaavLTTrjv
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\ll\lvflOXOVTOC, dxOUe. IIpCOTOV TOLVUV d^LOV £TiL^vir]a6f]vaL tcov sxslvou tlvo^, otico^ £X
nepalSo^ sxo^LaGr] auTr] f] auvxa^L^ xal Tiapd tlvo^ elc, Trjv tXXaha {iettivex^^ yXcoxxav.
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he TOV ^L^d^ovxa. (vo^o^ ydp ev nepal^L, Tidvxa ^ev id ^aGrj^axa tol^ PouXo^svol^
s^SLvaL ^av6dv£LV, daxpovo^lav he ^ovol^ tol^ IlepaaL^, 6 he Trjv alxLav e^exdaa^ xal
^a66v ho^av elval xLva TiaXatdv £TiLxpaTir]air]aav Tiap' auxoL^, 6^ [cpSaprjaeaGaL] Trjv
exsLvcov paaiXsLav utio 'Pco^alcov if] Tsx^fl ^"H^ daxpovo^lac; xp^^^vcov, Tiap' sxslvcov
TipoTspov TauTTTjc; XapovTSc; dcpop^dc;, 5Lir]Tiop£LTO ti6c; dv toO toloutou ^exdaxoL xaXoO).
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Xe^d^evoc; xal tioXXouc; UTnrjXoouc; XTTTjad^evoc; sic; Trjv TpaTieCoOvxa TidXtv dcplxexo,
TioXXd ptpXla ToO Tf]c; daxpovo^lac; ^aGrj^axoc; ^£0' eauToO* olxela ht yvw^r] TaOxa
e^eXXrjVLaac; ^vrj^rjc; d^Lov epyov STioLrjaev. elal [itv oOv xal exepa ptpXla Tf]c; auvxd^ecoc;
t6v Ilepawv, dTiep auxo^ e^eXXrjVLaev UTioSsLy^axd xLva ^sGo^Lxa ev dpxf] ex^^^^^ stiox^v
TauTrjv he ^ovrjv Trjv auvxa^Lv, f]v xal 6^ xpelxTova Tiaawv xal dxpLpeaxepav TiapeScoxev,
6c; 6 f]^6v ^L^daxaXoc; eXeye xal dXrjGeucov ecpalvsTO, x^p'^^ ep^rjveLac; e^eXXrjVLaev, outco
TauTrjv Se^d^eov^ ex Ilepawv Std C6air]^ ^ovr]^ E:p^ir]V£uo^£vir]v cpcovf]^* outco^ sxo^LaGr]
auTiT] f] auvxa^Lc;, f] xal Tipox^ipoc; XeysTaL.^-*-
4iUsener [12] pp. 356-357
BIBLIOGRAPHY
[1] Alblrunl. The Chronolgy of Ancient Nations; An English Version of the Arabic
Text of the Athdr-ul-Bdkiya of Alhiruni, or Vestiges of the Past. Published for
the Oriental Translation Fund of Great Britain and Ireland by W. H. Allen and
CO., London, 1879. Translated by Dr. C. Edward Sachau.
[2] Friedrich Karl Ginzel. Handhuch der mathematischen und technischen Chronolo-
gic, das Zeitrechnungs der Volker^ volume I. J. C. Hinrichs, Leipzig, 1906-1914.
[3] R. E. Hall. Dictionary of Scientific Biography^ volume 7, pages 335-331. Scrib-
ner. New York, 1973. ed. Charles Gillispie. The entry al-Khazim.
[4] R. Mercier. The Greek 'Persian Syntaxis' and the Zlj-i Ilkham. Archives inter-
nationales d^histoire des Sciences^ 34:35-60, 1984.
[5] Otto Neugebauer. Studies in Byzantine Astronomical Terminology. Transac-
tions of the American Philosophical Society^ 50, 1960.
[6] David Pingree. Gregory Chioniades and Palaeologan Astronomy. Dumbarton
Oaks Papers, 18:133-160, 1964.
[7] David Pingree. The Astronomical Works of Gregory Chioniades, volume I.
Corpus des astronomes byzantins IL J.C. Gieben, Amsterdam, 1985.
[8] David Pingree. In Defence of Gregory Chioniades. Archives internationales
d^histoire des Sciences, 35:436-438, 1985.
16
17
[9] David Pingree. A Preliminary Assessment of the Problems of Editing the Zlj
al-Sanjarl. In Yusuf Ibish, editor, Editing Islamic Manuscripts on Science^ pages
105-113, London, 1999. al-Furqan Islamic Heritage Foundation.
[10] A. Sayili. Al -Khazinl's treatise on astronomical instruments. Ankara Univer-
sitesi Bil ve Tarih-Cografya Fakultesi Dergisi^ 14:18-19, 1956.
[11] Tihon. L'astronomie byzantine (du V^ au XV^ siecle ). Byzantion, 51:603-624,
1981.
[12] H. Usener. Ad historiam astronomiae symbola. In Kleine Schriften^ volume III.
E.G. Teubner, Leipzig, 1914.
[13] L. Westerink. La profession de foi de Gregoire Chioniades. Revue des etudes
byzantines, 38:233-245, 1980.
PART II
Translation
18
19
The Beginning of the Book of Sanjan
Book One:
On the known epochs.
Book Two:
On the principles of the calculations which are very useful for the operation of
the astronomical composition, namely interpolation^^, the Sine of the arc, the sagitta
and the tangent^^.
Book Three:
On the first and second declinations to the North and to the South, the latitude
of cities, the culmination of stars^^, and rising times in right ascension. ^^
Book Four:
On the equation of daylight with the arc of day and night and the equinoctial
hours along with sections of the seasonal hours and the places of the zodiacal signs
for all the klimata along with the width of rising.
Book Five:
On the motion of the fixed stars from their true longitudes, their latitude, that
is, their distance from the celestial equator^^, the culmination of fixed stars^'', the
degree of a zodiacal sign which is together with the star on the meridian, the degree
which rises with the star, the degree setting with the star, and the apprehension of
that hour of their rising and setting in the day and the night.
Book Six:
^^lit. excess
^^lit. shadow
^^lit. the ascent of stars to the circle of the middle of the day
^^lit. place of fortune with a straight line
^^lit. circle which moves in a nychthemeron
^^lit. the ascent of the fixed (stars) to the middle of the day
20
On the apprehension of the number of hours of the day that have passed, the
number of degrees in a seasonal hour, (the distance) to the hours of the ascendant,
the equalization of the 12 houses, and the apprehension of the point of each ascension
and the point of each praying.
Book Seven:
On the extraction of the mean motions of the 7 planets and their proper motions,
the apogees and equations of each, the apprehension of the weekday on which the
Sultanic year begins from the months and the years of the epochs, the end of this
(year), and the equation together with the base longitude (of the planets), because
from the astronomical position of this base longitude the true longitude is calculated
for one year of the Sun by means of the true longitude.
Book Eight:
On the extraction of the true longitude of the 7 planets and the ascending node,
the direct and retrograde motion of the planets and their latitude, and the change
in position of each and their diameter.
Book Nine:
On the increase and diminution of the visibility of the sighting of the Moon, and
the rectification of its location in longitude and latitude.
Book Ten:
On the apprehension of conjunctions and oppositions of the sun and the Moon
together with their longitude and change in position, and of eclipses of the sun and
the Moon. This tenth book is divided into three chapters.
Book Eleven:
On the Moon appearing new, and the 5 planets.
Book Twelve:
On the ascendant of the years and of the four seasons, the entrance of the ascen-
dant of that year, nativity-casting, and the stars' casting of the rays.
BOOK 1
On the Known Epochs
This is divided into 5 chapters:
Chapter 1: On the nature of the nychthemeron^ the month and the year.
Chapter 2: On the nature of the epoch, and how many epochs are manifest with
respect to our year.
Chapter 3: On comprehending by epoch the weekday on which the year and
month begin, and (on) the extraction of one epoch from another by calculation.
Chapter 4: On the weekday on which the years and months begin, and (on) the
extraction of one epoch from another by tables.
Chapter 5: On the festivals, the great days and the manifest (days) observed in
(each) nation both through calculations and through tables.
1.1 On the Nature of the Nychthemeron and the
Month and the Year
The day and the night, namely, the nychthemeron^ is the return of the (celestial)
sphere in its motion from one point back to the same (point), which is completed in
24 hours. Each nation sets its own beginning to this. The Arabs reckon the beginning
of the nychthemeron from the setting of the sun. Since they reckon their months
21
22
from the appearance of the new Moon, these (months) are reckoned through its (the
Moon's) motion. The Moon appears new after the setting of the sun. The Muslims
reckon the beginning of the day from the rising of the sun [until its setting], since
this is the manner in which they conduct their fasts. The astronomers reckon the
beginning of the nychthemeron from mid-day^ because the data for the planets are
set down (in tables) for mid-day. For if they were set down for the beginning (of
the day), since the length of day increases and decreases, the data would not be
consistent.
The day is reckoned from the rising of the sun until (its) setting, and the night
(is) that (time which is) after the setting of the Sun until its rising again.
On the Nature of the Year
A year is the motion of the Sun through the zodiacal circle from a zodiacal sign
and degree (and its) return to the same zodiacal sign and degree, the completion of
the 4 seasons, and the revolution of approximately 365 and 1/4 days. This is the
year of the Sun.
This is the (calculation of the number of days in a) (year) of the Moon: the mean
(daily) motion of the Sun is subtracted from the mean (daily) motion of the Moon.
If anything (i.e., whatever) remains, 360 degrees are divided by that. If anything
comes out, it is the (number of) days of one month of the Moon.
This calculation was made in the composition, and there were discovered (to
be) 29; 31, 50^ days and first (sexagesimals) and second sexagesimals. This was
multiplied by 12, and the days of one year of the Moon appeared to be 354; 22, 2
days and first (sexagesimals) and second sexagesimals. From this it was clear that
the Moon passes through the 12 zodiacal signs in this (number of) days.
^lit. the middle of the day
^ The semicolon here and elsewhere indicates the position of sexagesimal point. Thus the number
in question is equivalent to 29 + |^ + ^ .
23
Others combine these two (types of) years. They reckon the year through the
motion of the Sun, and the month through the motion of the Moon. They also
reckon their great days and their Easter through lunar calculations. Every three
years, many times also (every) two, there is a shortfall and an excess between the
two (types of years), (the year) of the Sun and (the year) of the Moon. At any rate,
one month is added so that they are again equal. There are 354 days in the case of
that year in which no excess occurs, (and) there are 384 days in the case of the year
in which there is an excess of a month.
The Hebrews and the Indians employ this (luni-solar) year. The Hebrews reckon
the beginning of the year when the Sun is in conjunction with the Moon in Libra from
the 24th of Abh until the 27th of Elul, the Indians when the Sun is in conjunction
with the Moon in Aries.
1.2 On the Nature of the Epoch, the Month and
the Year, How They Are Known, and How
They Come About
The ancient astronomers came to know the calculation of the months from seeing
that the Moon waxes and wanes and the (calculation of the) years from the fact that
those 4 seasons - which comprehend a year - always circle back upon themselves in
their changes in quality-from hot to cold and back again- in one and the same time
period, that is, in a year. So they wished to see in (precisely) what time period this
occurred. Since the greatest festival days and all (human) endeavors are seasonal,
the year was set down by them and reckoned.
It is also necessary to say what an epoch is. An epoch is that (time) from which
the years are counted. (This starting point is chosen) because at that time a great
heavenly or earthly occurrence took place, such as the appearance of a prophet, or
24
someone's good fortune, or the destruction of the world, or an earthquake and flood,
or the total eclipse of the Sun and (or) Moon, or other things similar to these which
happen during the passage of many years.
Whichever the nation, its epoch as well as its year is peculiar (to it). These
(national) years were bound up with these (national) epochs for the comprehension
of past time, as will be said.
And so these things were set down separately (in tables).
On Comprehending the Epochs Which are Manifest in our
Own (Calendar) Time
They are 7 (epochs).
One of them (is) that of the Arabs. The beginning of this epoch was reckoned
from the beginning of that year in which Mohammed fled from Mecca to Medina.
Years of the Moon were bound up with this epoch. Its months are counted from the
appearance of the new Moon. All Muslims employ this calculation. The beginning of
this epoch was a Friday. The (number of) days (in the) months of this epoch are not
equal. For the sake of easiness, we reckon (the number of days in) this (Arab) month
with a mean calculation, namely, of 30 and of 29 (days each) until the completion
of the year. Why? Because when the fraction of a day is more than half a day, one
(full) day is reckoned. Why is this done ? Because the motion of the planets was set
down in this book according to this epoch. For if the (number of) days of the month
were not manifest, how could the calculation of (the longitudes of) the planets be
made? And how would these (other) epochs be extracted from this (Arab) one? In
this composition, the names of the months in this epoch were set down in tables so
that the days of their months are both combined and separated there.
The second of these epochs, that of Mu'^tadit.
The years of this epoch are Roman, and the months are (given) with Persian
25
names and computation. The beginning of this epoch is the 11th (day) of Haziran.
5 epagomenal days are placed at the end of the month Abh. Why? Because the
ancients who worshipped fire established it so.
Third, the epoch of the Romans.
The years of this (epoch) are solar. Its months are (given) in the Syrian dialect.
The beginning of this epoch is a Monday. Each of these years is 365 | days. There-
fore, when that | becomes more than half of a day, it is reckoned one day. That
additional day is added to the end of Shubat. That year is 366 days. So from the
years of the Sun reckoned as a foundation in every 110 years one month^ is addi-
tional. The names and the days of the months were set down in two places near
those months both combined and separately. When the need arises, the months and
the days are sought there (in tables).
Fourth, the year of the Persians.
This was set down at the time of Yazdijird (the son of) Shahryar. The beginning
of this epoch is a Tuesday. This year was established in 2 ways: the first is in
accordance with their religion, which is a basUa year. They always reckon 365 days
for each year (of this type), and 30 days for each (of its) months. 5 epagomenal days
are placed at the end of Aban. The names of the months and of the days of this
epoch were set down in a table.
The other (Persian) year, which is called kahisa^ was established in accordance
with the labors of the 4 seasons and (in accordance with) the beginning of their
(associated) labors. This year is established with several (characteristics). One is
that each month has thirty days and each day has its own name, and that the 5
epagomenal days are placed at the end of the year. The second is that the day of
the entrance of the Sun into Aries, namely, the ''new (day) of the days", is always
at the beginning of the month of Farwardin in this (type of) year. The third is that
^the mss. read one day
26
whenever the year is intercalary, one day is ^not^ added at its end. Every 120
years, however, when these (additional) days have been brought together, there is
one additional month. Why? because the excess of the year of the Sun with respect
to the year of the Moon at this time is about 30 days.
And so the months of this calendar were divided into two (varieties) for the sake
of (agricultural) labor. This is one type (of year): the months of this are coextensive
with the 4 seasons, and the beginning of this year is Farwardln, and Isfandarmadh
is at its end. The 5 epagomenal days are placed at the end of Isfandarmadh. The
great days of the festival and the famous (days) are (arranged) the same way in the
months of a kahisa year.
The second (variety)^ is that (in which) the months are not fixed in one spot
with respect to the 4 seasons. Every 120 years, one month is put in the place of the
first month. The arrangement of this is such that a month of this sort (i.e., of 30
days) is added again at the beginning of Spring after Winter. Every 1494 years the
first month - Farwardln - is again found in its proper location. The beginning of
the first day of Farwardln is the entrance of the Sun into Aries.
(This arrangement) came about in the following way: the man who established
this epoch maintained that from the beginning (of the time) of those first men (who
lived) when the fiood took place, there were two months of Farwardln — the first fixed
in its own place, and the second moving from place to place instead. The Sun was
(then) in the beginning of Aries on the first day of the latter month. 4336 years have
passed from that time until the beginning of the Persian epoch. The Sun entered
Aries in the month of Adhar during the year of (the founding of) the Persian kingdom,
and so Adhar was (then) opposite the fixed Farwardln. 5 epagomenal days were
established at the end of the month Aban opposite to the fixed Isfandarmadh. At
the beginning of the epoch of Yazdijird the month Dai was opposite the beginning of
ipingree: Intercalation destroys the system.
27
the fixed Farwardln. This month (opposite the fixed Farwardln) is called paramone.
It is necessary to know this month (i.e., paramone) by means of calculation. The
full years of the epoch of Yazdijird are reckoned, and 123;0,2 (years and first sexa-
gesimals and second sexagesimals) are added to these. The result is doubled. And
again the result is divided by 249. The result is the months of a kahisa (year). That
(number of months) is subtracted from the month Adhar. Wherever the calculation
leaves oflF, the 5 epagomenal days are added to the end of that month. Then one
examines the month before this one. If the latter is equal to the former, this is called
a month of the paramone.
This (above) mentioned calculation was (in use) towards the end of Persian in-
fiuence. When the Arabs conquered them, the following arrangement was adopted
and the 5 epagomenal days were comprehended at the end of Aban until the Persian
year 375 from the epoch of Yazdijird. The cycle (of months) was completed at that
time and the Sun was then entering Aries at the beginning of Farwardln opposite
the fixed month. Some Persians established the 5 epagomenal days at the end of Is-
fandarmadh. Others comprehended them at the end of Aban. Why? Because those
who worship fire believe that if it were done diflFerently and the days were established
otherwise, their religion would be disturbed, which is not the case.
When the Sun was in the vernal equinox in the 500th (year) of the Persian cal-
endar, it was in the entrance of Aries at 90 degrees longitude at the beginning of
the moveable month of Ardibihisht. Those 5 epagomenal days were (then) estab-
lished at the end of the moveable Farwardln because the first of the moveable month
Ardibihisht coincided with the first of the fixed month Farwardln. Every year which
is set down in this table has a 13th intercalary month, and the month of Farwardln
occurs a second time in that year - one (time) at the start of the year, and the other
at its end. The manifest and great days of the feasts are not established in that later
Farwardln. That year is 365 days. When the beginning of the moveable Ardibihisht
28
and the beginning of the fixed Farwardin coincided, it was the 12th of the month of
Rabi*^ II - a Sunday- in the Arab year 525. On that day the Sun was at the entrance
to Aries. From the epoch of the flood until that time 4836 years passed, and until
the epoch of Yazdijird there were 500 years, and until the epoch of Alexander (there
were) 1446 years.
And so, since mistakes have arisen concerning (the computation) of these months
due to the fact that the influence (of this kingdom) has been overthrown, this com-
putation has (often) been comprehended in a meaningless fashion. So we have set up
a table into which the months of that base value have been placed. Those compre-
hended months have been placed there. Two epochs have been set up in this table -
one the Roman epoch, and the other the Persian epoch. The years are incomplete.
(Table 6.7)
Persian Table of Nachizak
Months of the Paramone
Roman Epoch
1
:^
a;
-+^
5-1-1
o
?-l
.o
g
Months of the
Base-point of
the Ancients
a;
a; -o
1 1 K^
o
a;
B ^
8 ^
1 1 K^
^ >^ -1^ _d
§ le fa ft
i ^ 1 1 'i
6
7
7
1
1
2
2
3
3
4
4
5
5
6
Khurdadh
Tir
Murdadh
Shahriwar
Mihr
Aban
Adhar
Dai
Bahman
Isfandarmadh
Farwardin
Ardibihisht
Khurdadh
Tir
Farwardin
Ardibihisht
Khurdadh
Tir
Murdadh
Shahriwar
Mihr
Aban
Adhar
Dai
Bahman
Isfandarmadh
Farwardin
Ardibihisht
376
500
624
749
873
998
1122
1247
1371
1497
1620
1745
1869
1994
14
13
12
11
10
9
8
7
6
5
4
3
2
1
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
Adhar
1318
1442
1562
1791
1815
1940
2064
2189
2313
2438
2562
2287
2811
2936
4
5
6
7
8
9
10
11
12
13
14
15
16
17
Table 1.1:
29
The 5th of these famous epochs is the epoch of Malikshah. The Sultan or-
dered that the true longitudes for this epoch be established at the beginning of that
epochal year, when the Sun entered the beginning of Aries. (He also ordered that)
the beginning of each month (be) when the Sun changes from one zodiacal sign to
another. The mean motions of the planets are extracted from other calendars. And
so true longitude is established for this epoch for the sake of easiness. The beginning
of this epoch was the first day of the month Sha'^ban, in the year 468 of the Arabs.
Every 220 years there are 53 intercalary days- 45 of these are intercalary because
every 4 years there is one intercalary day. 8 of these are intercalary because every
^2^5 years there is one intercalary day, so that the total is 53.
The 6th of these famous epochs is the first epoch - that of Nebuchadnezzar.
Its years are Egyptian as well as its months. The beginning of this epoch was a
Thursday. There is a difference of 499,802 days between this epoch and that of the
Arabs. 503,425 days have passed by from this epoch until the epoch of Yazdijird.
The 7th of these famous epochs is the epoch of Philip, the brother of Alexander
II. There is a difference of 348,665 days between this epoch and that of the Persians.
One year has 365 days and is Egyptian.
1.3 On Comprehending the Weekday on Which
the Year and Month of the Epochs Begin,
and (on) the Extraction of one Epoch from
another by Calculation.
This is divided into 4 sections.
30
1.3.1 On the Weekday on Which Years and Months Begin
by Calculation
If you wish to know the weekday (of the) beginning of the year and (of the) beginnings
of the months, always multiply the full years of whatever epoch you wish, that is,
''beat" them: (Table 1.2 )
Arab Epoch
Roman Epoch
Persian Epoch
Sultanic Epoch
Ordinary
Intercalary
By 131. If anything
is found, 14 is al-
ways added to it.
Then the result is
divided by 30. The
fractional parts are
cast away. The re-
sult is multiplied by
this.
By 5. It anything
is found, 2 is added
to it. The two
are then divided by
4. The fractional
parts are cast away.
If nothing is com-
prehended, the year
is intercalary. If
anything is found,
it is multiplied by
this.
Nothing is added.
(It is done) with
the number of each
month of the in-
tercalary year by
two's.
By 203. If anything
is found, 102 is
added to it. And in
turn if anything is
found, it is divided
by 120. The result
is left in the middle
(of the workspace),
and what is found is
kept in mind.
Table 1.2:
Then the result is then added to the following and examined:
Ordinary
Intercalary
Ordinary
Intercalary
6
1
2
3
3
1
The remainder upon division by 7 of that which is apprehended (after the addi-
tion) is then taken. The result is the weekday of the beginning of the year.
If you wish to know on which weekday the months of that year begin, add the
(number of) days of the previous months of that year. [Table 1.3)
If anything is found in excess (of 7), it is divided by 7, that is, it is reduced
modulo 7 so that the weekday on which that month begins may become clear.
31
Arab Epoch
Roman Epoch
Persian Epoch
Sultanic Epoch
Ordinary
Intercalary
For every one
month, two (days)
and for the next
month, one (day).
(Do this) until the
end of the year.
For every month
completed of 30
days, two (days)
are added. For
every month ex-
ceeding 30 days,
three (days) are
added. In the case
of an intercalary
year, one (day) is
added for Shubat.
In the case of an
ordinary year,
nothing is added
for Shubat.
Two
(days)
are
added
for
each
month,
but
none
are
added
for
Aban.
For each month by
two's until the end
of the month Aban.
For each month
completed in 29
days one (day) is
added. For each
month completed
in 30 days, two
(days) are added.
For each month
completed in 31
days three (days)
are added. For
each month com-
pleted in 32 days
four (days) are
added.
Table 1.3:
1.3.2 On Making the Days of the Years and the Days of the
Months for Each Epoch
When it becomes necessary to employ this method, one must first come to know the
weekday on which that year and month begin. That day should be evident from the
calculation of the weekdays. This is necessary for the epoch of the Arabs because
the calculation (of the number of days) in their months is reckoned in two ways:
one is (by) the appearance of the new Moon after conjunction, and the other is that
the number of days (in a month) is 29 or 30. This is called the mean number. The
number of the weekday is reckoned by the mean number. The day sought is correctly
determined by this calculation.
When you wish to make the days and years for an arbitrary epoch, multiply the
full years, that is, ''beat" them. {Table I.4)
The days of the current incomplete month are added to the days of the full month.
It is necessary (to) mention how the days of the full month are comprehended.
{Table 1.5)
The result is the days of the year and the months of that epoch. That is the
day for which the calculation was made. The check of this method is by this test.
Whatever days are found below (in the table) are added to the (number of) days of
32
Arab Epoch
Roman Epoch
Persian Epoch
Sultanic Epoch
Ordinary
Intercalary
By 10,321. If any-
thing is found, 14 is
added to it. If any-
thing results, 30 is
added to it. If any-
thing is found, the
fractional parts are
cast away, and the
result is examined.
By 461. Iwo is
always added to
this. The result is
divided by 4. If
anything is found
(of a) high (sex-
agesimal degree),
it is reckoned and
the fractional part
is cast away. If
nothing is compre-
hended, the year is
intercalary.
By
364
By 365. Multiply
the excess by that.
If anything is found
for this reason, that
every month has 30
days because the
year is intercalary,
the result is exam-
ined.
By 80,353. 102
is added to the re-
sult. This result
is divided by 220.
The fractional part
is cast away and the
result is examined.
Table 1.4:
Arab Epoch
Roman Epoch
Persian Epoch
Sultanic Epoch
Ordinary
Intercalary
One month is reck-
oned with 30 days
and the other with
29 until the end (of
the year).
I'he days ot
this year are
reckoned for
the month
just as they
are set down
in the table.
The month
of Shubat is
reckoned with
28 days, 29
days in an
intercalary
year.
They are
reckoned
with 30
days
for each
month
and 35
days for
Aban.
Whatever has
passed from the
first of the fixed
Farwardln is added
to this (with the
number of each of
the months past
being 30 days).
And the days of
the current month
that have passed
are (also) added to
this.
The days of the
month are added as
is set down in the
table.
Table 1.5:
each epoch. {Table 1.6)
Arab Epoch
Roman Epoch
Persian Epoch
Il-Kham Epoch
Ordinary
Intercalary
5
1
2
2
Table 1.6:
The result is divided by 7, that is, it is reduced modulo 7. If the result is equal to the
day of the week for which this computation was made, the computation is correct.
If it is not equal, the computation is not correct.
33
1.3.3 On Knowing the Calendar Dates of Unknown Epochs
from the Calendar Dates of Known Epochs
It is possible to know this if the difference in the number of days between the two
epochs is known. ^ Therefore know that the difference in the number of days between
the epoch of the Romans and the epoch of the Arabs is 340,701. The difference in
the number of days between the epoch of the Romans and that of the Persian basUa
is 344, 324. The difference in the number of days between the Roman epoch and
the Sultanic is 506,401. Likewise, the difference in the number of days between the
Arab and the Sultanic is 165, 700. The difference in the number of days between the
epoch of the Persians and the Sultanic is 162,077.
And so if the known epoch is prior, this (number of) days is subtracted from the
day (number) of the known epoch, and so the day number of the unknown epoch is
discovered. If the days of the known epoch are later, the difference in (the number
of) days between the two epochs is added to them and so the day number of the
unknown epoch is discovered.
1.3.4 The (sexagesimal) Elevation of the Years and the Months
When it becomes necessary to employ this (method), those days are multiplied (as
follows): {Table 1.7)
The result of the divisions of those days is the (number of) full years of each epoch.
If anything remains, it is divided by the following amount:
Arab
Roman
Persian
Il-KhanI
by 30
by 4
by nothing
by 120
The result of these divisions is the days. Dispose of them in the following order:
Table 1.8)
^lit. It is possible to know this if the difference in (the number of) their days is known.
34
Arab Epoch
Roman Epoch
Persian Epoch
Il-Khani Epoch
Ordinary
Intercalary
By 30. The result
is added to 14. The
result is divided by
10,631
By 4. The result is
added to 2. This
result is divided by
1461.
(By)
nothing.
It is
(instead)
divided
by 365.
By nothing. It
is doubled and
divided by 90, 885.
The result is (in
the) arrangement
of the months of
the intercalary
year. Each month
is reckoned as 30
days. The result
is subtracted from
that number. This
result is divided by
.S65.
(By) 80,353. 102
of the excess is
added. If anything
is found, (it is
divided) by 220-
<and subtract >
the result. . .
Table 1.7:
Arab Epoch
Roman Epoch
Persian Epoch
Il-Kham Epoch
Ordinary
Intercalary
For one month
there are 30 days,
and for the next
there are alter-
nately 29. This
sequence starts
with the month
of Muharram.
Count the (days)
as indicated until
the end of the year.
In each month
whatever is clear
of its days. The
beginning (of
this sequence) is
from Tishrin I. If
nothing is compre-
hended from the
division by 4, the
month of Shubat is
reckoned with 29
days.
30 (days) for
each month. The
beginning (of this
sequence) is from
Farwardln, and
for the 8^^ month
there are 35 days.
30
days
for
each
month.
For each month the num-
ber of days that is writ-
ten (for it) in the table.
(Continue) with this se-
quence until the end of
the year. If what is com-
prehended - i.e., the frac-
tional part of the year
in our computation — is
greater than 165, the year
is intercalary, and the last
month has 31 days. If it
is less, it has 29 days.
Table 1.8:
If any days remain, if they are less than one month, those days — together with
the day for which the calculation was made — are called an incomplete month.
1.4 On Comprehending the Weekday on which
the Years and the Months of the Year Begin,
and on Extracting One Epoch from Another
by Means of Tables
This method (chapter) is divided into 2.
35
1.4.1 On Comprehending the Weekday on which the Years
and the Months of the Year Begin by Means of a Table
When there is need for this, the (number of) the incomplete years is placed in the
workspace. The cycles are subtracted from this (number), that is, (the years of) the
Arabic epoch are reduced modulo 210. If anything is comprehended, it is sought
in the two tables of the years, joint and separate. The result is reckoned opposite
those two years in days of the week. And so that (result) is the weekday upon
which the year begins. This calculation is correct whenever the comprehended years
are found in the two tables. Whenever they are not found in the two tables, 30 is
subtracted from those apprehended years. If anything is apprehended, entrance is
made opposite it into the tables of the joint years. Entrance is also made into the
table of single years opposite those 30 subtracted years. (The result) follows in the
way that was mentioned. Likewise in the case of months, entrance is made opposite
the months in their tables, and the days of the week are reckoned. The result is
added to the weekday of the year's beginning. And so the weekday upon which that
month begins is found.
The Epoch of the Romans
Their cycles are subtracted (from that number), that is, it (that number) is
reduced modulo 28. If anything is apprehended, it is sought in the table of single
years. If it is found in black (ink), the year is ordinary, if it is found in red ink, the
year is intercalary. Then the day of the week is reckoned opposite whatever is found.
This weekday (is the day upon which) that year begins. If someone wishes to know
the days upon which each month begins, if the year is ordinary, entrance is made
into the table opposite the months of the ordinary (year). If the year is intercalary,
entrance is made into the table opposite the intercalary year. The weekdays are
reckoned opposite that (result). It (i.e., this result) is added to the weekday upon
which the year begins, and so the day upon which the month begins is found.
36
The Persian Epoch
In the case of the Persian hasita year, the cycles are reduced modulo 8. If anything
is apprehended, it is sought in the table. Wherever it is found is the day upon which
the year of that epoch begins. The day upon which the month begins is apprehended
in the same way as was mentioned in the other (sections) on the Arabic and Roman
(years). The Persian kahisa year was discussed earlier at the end of the second
chapter {page 25). Comprehension of this method was discussed there.
Sultanic Epoch
Its cycles are reduced modulo 220. If anything is apprehended, one is subtracted
from it. Then entrance is made into the tables opposite that which has been appre-
hended (and) the weekdays are reckoned opposite the (columns of) single years, 10
years and 100 years. If anything is found, one day (and) 102 parts (of a day) are
added to it. If that fractional part is greater than 220, it is reduced modulo 220.
And for each 220 (cast away), 1 is added to (the number of) those days. Then the
quantity of that result is examined. If it is greater than 167, it is clear that the
coming year is intercalary, if it is less than that (amount), it is ordinary. If that
fractional part is less than 55, the beginning of the year is one of those weekdays.
If it is greater than 55, the beginning of the year is on another weekday. If it is
less than 55, the beginning of the year is the day previous. If the fractional part is
greater than 55, the beginning of the year is on the coming day. If (the number) of
days is greater than 7, it is reduced modulo 7.
Whenever there is need for the comprehension of the beginning of each month,
the weekday on which the year began is examined. This is sought along the top of
the table. Entrance is made into the table opposite that month. If anything is found
opposite the two entries, it is the day upon which the month begins.
37
1.4.2 On Extracting The Roman, Persian and Sultanic Epochs
from the Arab Epoch by Table
Before (undertaking) this labor, all the Arab years are comprehended and set down
in the workspace, and the full months are in turn placed beneath them, as well as
the current days of the (current) incomplete month (as reckoned) with the mean
number (of days) since the beginning of the month. ^ For the incomplete (number)
of days of the (current) month are reckoned with that mean calculation, not by
the sighting (of the lunar crescent). (This number) is placed beneath the month.
Then the total (number of) days is reckoned opposite the full months and is placed
under the previously reckoned (number) of days. Then those months are cast off
from the (number of) days taken together, and the (number of) complete Arab
years is retained above together with (the number of) current days of the (current)
incomplete year. Then entrance is made into the table of the thirty year periods of
the Arab epoch, and their full years are sought. If any number is found there equal
to those (full years), so be it. If one is not found, the greatest number less than that
placed in the workspace is sought, and entrance is made into the table opposite that
number. And so the full years of the Persian, Roman or Sultanic epoch are found.
The days are reckoned opposite and before the years. The years are placed in
the workspace at the top and the days at the bottom. Then the Arab years for
which entrance was made into the table are subtracted from (the number of) those
years placed earlier in the workspace. If anything is comprehended, entrance is made
opposite that in the table of single Arab years, and so (the number of) years and
days is reckoned, and (those numbers) are added to those (numbers) of years and
days reckoned from the table of thirty year periods. Then that (number of) days of
the Arab epoch is added to the (number of) days of each of the three epochs, that
is, the number of days of whatever epoch is necessary is added to (the number of
^See page 31.
38
days of) the Arab epoch. Then an examination is made. If (the number of) days of
those epochs is greater than 365, 365 is subtracted from (the number of) days and
1 is added to (the number of) years. If anything is found, it is (the number of) full
years. Whatever the year is, one is always added to it. And so the incomplete years
of that epoch are found.
The (number of ) days of that epoch comprehended is examined. Entrance is
made opposite that number into the required table of days and months. If this
number is not found there, the greatest number less than it is sought. The month
found opposite this number is examined. This (month) is not reckoned, but the
one after it (is reckoned), and it is placed underneath the (number of ) years in the
workspace. Then the (number of) days discovered in the table is subtracted from
the (number of) days reckoned. If anything is comprehended, it is placed beneath
those months. If nothing is comprehended, one is always added beneath the months.
Whatever is found is the years, months and days of that epoch. The Persian basUa
year is known.
It is necessary also to know the Persian kahisa year. The (number of) full Persian
years is set down in the workspace and 121 is added to this number. The result is
divided by 124. If anything results, it is the (number of the) month of the kahisa
year in this order, that is, counted form the month of Adhar. Wherever the counting
ends up, those 5 epagomenal days are placed at the end of that month.
1.5 On Comprehending the Easter of Each Na-
tion and Their Manifest and Greatest Days
Some of the manifest days are (tied to) the days of the month, and are always fixed
to their own location (in the month), other manifest days are (tied to the calculation
39
of the) weekdays of the moveable month'', others are manifest because they are (tied
to) the years of the Sun and of the Moon, and other manifest days are (tied to) the
weekdays of these two types of years. This chapter is divided into seven sections.
1.5.1 On Comprehending the Times and the Extraction of
the 28 Lunar Mansions
All the lunar mansions are equal (in longitude) on the circle of the ecliptic. The
beginning of the motion (in the counting) of those mansions is from the first of
Aries. The forms of the mansions are composed of the fixed stars. These forms vary
in both shape and location. As for the times when these mansions rise, that is, when
they appear with the Sun at a distance, the first mansion rose in the Roman year
1452 on the 28th day of Nisan. After 13 days the second mansion rose, and the other
mansions (after it) rise after 13 days in a similar fashion. The 15th mansion, whose
name is Gafir^ rises after 14 days. The rest of the mansions after it rise, in turn,
after 13 days.
What has been said (about this) holds true for an ordinary year. In the case of
an intercalary year, the 15th mansion, whose name is Zoumpra^ rises after 14 days.
So whenever one mansion rises in the East, the 15th mansion (counting from it) sets
in the West.
These mansions have been set down in a table for the hour when each rises. They
are comprehended from this table.
1.5.2 On Comprehending the Great Fast of the Christians
The beginning of this fast is always a Monday. This Monday should be the closest
to the conjunction of the Sun and Moon which occurs from the second of Shubat
^A: They vary with the calculation of the weekdays.
40
until the 8th of Adhar. It should not go beyond this. If the year is intercalary,
the conjunction should take place from the 3rd of Shubat until the 8th of Adhar.
If the conjunction takes place on the Monday before the second of Shubat, that
conjunction is not reckoned, but is cast away, and the next conjunction after it is
sought. Then the Monday closest to this conjunction is reckoned, and that is the
Monday of the Great Fast. This calculation is made from the epochal value. If
this must be comprehended from the astronomical composition, a table has been set
down there from which to comprehend the fast.
1.5.3 On Comprehending the Occurrence of the Great Days
with Respect to the Great Fast
Know that twenty- two days before the Monday of the Fast, there is the fast of
Nineveh, which is always a Thursday, and its fast-break is a Friday. Twenty four
days after the Great Fast is the so-called feast of Faruq, which is always a Wednesday.
42 days after the Great Fast is the Day of the Palms. Its fast break is 49 days after
the Great Fast. That day is always a Sunday. The Thursday before the Thursday
of the Fast is Great Thursday. The Friday after it is the crucifixion of Christ.
The Friday after the fast-break is the little day of Palms. 40 days after the fast is
the Resurrection of Christ. 11 days after the Resurrection is the festival of the Holy
Spirit. The Sunday of the fast after the festival is called the Sunday of the Dialogue or
of Thomas. The Tuesday after the Pentecost is called the fast of as-salhayn ^jjlpJljJI.
The Friday after that is called Golden Friday. The fast of as-salhayn (JJlpJljJI lasts 48
days, and the 49th day after the fast is called the fast-break of as-salhayn (JJlpJljJI.
It is always a Sunday. Thirteen days after thatis the so-called fast-break of dikrdn
mdrmdrd ^jCaJd jlj/"^. 50 days after the fast-break of as-salhayn (JJl^JljJI is the
fast of Elias. That day is always a Tuesday. This fast lasts 48 days and the 49th day
is the day of the fast-break.
41
1.5.4 On the Feast Days of the Mushms and Their Fast
Days
Muharram
The V^ - it is considered great by them because it is the first of their year.
The 9*^ - the day in which the son of '^Ali began the battle against Yazid.
The 10*^ - the day in which Yazid killed the son of '^Ali.
The 16*^- the fixing of the qibla in the direction of Jerusalem.
The 17 *^- when the city of Jerusalem was attacked by elephants.^
Safar
The V^- when the head of the son of '^Ali was brought to Damascus.
The 16*^- the sickness of the impious Mohammed.
The 20*^- when the head of the son of '^Ali was brought back to the place where
he had been killed.
The 24*^- the departure from the caves -after their fiight-of the impious Mo-
hammed and Abu Bakr.
Rabl^ I
The V^ — the death of the impious Mohammed.
The 3^^ — the entrance of the impious one into a dark grave in the house of his
wife.
The 8*^- the arrival of the impious one in Medina.
The 10*^- the day upon which he married his wife Khadija.
The 12*^ — the birth of the impious one.
The 14*^— the death of Yazid.
Rabl^ II
The 3^^ — the burning of Mecca by al-Hajjaj.^
^qdum ashah al-fil J^l ^[^^\ >^j3 "The arrival of the companions of the elephant."
^"The Kaaba was burned at the time when Al Hajjaj besieged ^Abd Allah b. Zubair" Biruni p
42
The 14*^- (the establishment of the injunction of)^^ prayer for those traveUing
or remaining at home.
Jumada I
The 8*^— the birth of ^All bin Abu Talib. ^^
The 15*^ — the battle with camels.
Jumada II
The 3^^- the death of the impious one's daughter, Fatima.^^
The 9*^— the death of Abu Bakr.^^
The 15th — the casting down of their prayer by ibn al-Zubayr.
Rajab
The V^- the impious one's victory over Barmuk
The 4*^ — the day on which '^Ali and Mu'^awiya joined in battle at Siffin.
The 26*^ — the impious one's revelation to the impious that he was a prophet.
The 27*^ — the night the impious one traveled to Jerusalem, ^^ and from there, as
they foolishly allege, he ascended to the sky. The truth, however, is that he went to
the house of his father, the devil.
Sha^ban
The 3"^— the birth of Hussayn the son of "AlP^
The 5*^- the birth of Hassan son of '^Ali^^
329.
10
taqdim farad al-salawati o^^Lkll j^y c -^
^^ Mohammed's son-in-law and cousin. This day is given as the 15^^ day of Rabi^ II in Biruni.
^^This day is given as the 8^^ day of Jumada I in Biruni.
^^This day is given as the 2^^ day of Jumada II in Biruni.
^^A2 reads mhsd hardm >l^ -Lu^. Al reads msgd hardm >l^
^^husayn bin ^ali ^ ^ U^r^
^^Not in Al.
43
The 13*^, 14*^ and 15*^ — the white days.
The night of the 15*^ is (the night of) their accursed prayer named bar^dt l^s-j}^.
On that same night the direction of their accursed prayer was set to Mecca. ^^
Ramadan
The V^ — the descent, as they foolishly allege, of the book of Abraham from the
sky.
The 6*^ — the descent of the book of Moses from the sky.^^
The 10*^ — the death of Khadija, the wife of the impious one.
The 12*^ — the descent of the book from the sky to David. ^^
The 17*^ — the battle of Badr in ten days, with the impious one driving back
thousands.
The 18*^ — the descent of the Gospel as they foolishly allege. ^^
The 19*^ — the conquest of Mecca.
The 21'*— the death of "^All bin Abu Talib, and the death of "^All al-Rida, his
son.
The 24*^ — the descent, as they foolishly allege, of the Koran to the Prophet. It
is better to say it was the ascent of the Koran to him from his father the devil .
The 26*^ — the casting out^^ of al-Birqu^i.
The 27*^ — the night of the worshipping of trees. ^^
^^"The night of innocence."
^^sarafat al-qihlat min hayt al-mqda Id 1-ka^hat <1«X)I J I All I oaJ ^ UJlII oij^ "The direc-
tion of the qihla was changed from Jerusalem to the Kaaba."
^^tazul al-twuryti ^li mwsd ^y> ^ h.j3y^^ JjJr' "The descent of the Torah to Moses."
'^^tazul zahur ^ali ddwadi ^jlS ^ jyj Jjjj* "The descent of the Psalms to David."
'^^tazul al-ingali ^ald ^ysi ^j^ ^ J^*"^' Jjjr' "The descent of the Gospel to Jesus."
^^Biruni has "revolt" rather than "casting out".
^^la'latu l-qdrjXa}\ 2j "The night of Fate."
44
Shawwal
The V^ — the break of their accursed fast.^^
The 2^^ — the first of 6 days of their accursed prayer.
The 4*^ — the conversation of the impious one with the Christians.
The 7*^ — the battle of Uhud and the death of the impious one's uncle. ^^
The 22^^ — the swallowing up of Jonah by the whale^^
Dhu al-qa^da
The 14*^ — the expulsion of Jonah from the belly of the whale.
The 15*^ — the descent from the sky, as they foolishly allege, of the Kaaba, and
the forgiving of Adam.^''
The 29*^ — the sprouting up of the Citrullus Colocynthis^^ plant over Jonah.
Dhu al-hijja
The V^ — the marriage of Fatima to '^Ali. The first ten days of this month
are called ''well-known". While their accursed prayer occurs on all these days, the
shouting of their prayer on the 8*^ of these 10 days is the loudest. ^^
The 9*^ — the day when they strip naked and pray in a Dionysiac frenzy.^^
'^^^ydu 1-fitri j^\ XcS- "The holiday of the fast-break" - the lesser Bairam
'^^ gazawatu ^hdin wamqtl hamizati 'SyP' J^^3 :^' '^3J^ "Someone's military incursion and the
death of hamizati V^ ."
^^This day is given as the 28^^of Shawwal in Biruni.
^^ al-rhmt 'li ^adam slwdt al-lahi 'lyh <uU 5DI 0)3^^ >il ^J^ 'L^J\ "The compassion shown to
Adam, may the blessing of Allah be upon him." The descent of the Kaaba is given as the 5^^of
Dhu al-qa^da in Biruni. The forgiving of Adam is given as the lO^^of Muharram in Biruni.
^^This is the yaqtin plant in Biruni.
^^A has an S^^day, ya^mu 1-trwyti ajjJOI >y^ "The day of quenching."
^^j^SS\ 7^\ yjn 'isy- ^rft hwa ^l-hagg al-akbr "(The visit to) Arafat. It is (during) the great
pilgrimage."
45
The 10*^ — the fast-break, which is called the slaughter. ^^
The 11*^ — the day of seizing. ^^
The 12*^ — the day of everyone's escape from their prayer. ^^
The 13*^- the sitting for three days.^^
The 17*^- the slaying of '^Uthman by the companions of the impious one.^^
The 25*^ — the slaying of ^Umar bin Abi Talib ^^
The 27*^ — the great heat at Medina. Many died because of it.^''
1.5.5 The Feast and Great Days of the Persians, Who Count
The Days as Coming before the Nights
Farwardin
The V^— New Year's Day.
The 6*^— Royal New Year's Day.
The 17*^— The Day of Serosh.^^
The 19*^ — Farwardingan.^^
31
32,
34 ••
^^p«JI >^^ (^^*-^' •^ ^ydu l-dhd ya^mu 7-na/in "The feast of the victims. The day of slaughter."
^^ya^mu 1-farr ^1 >yj^ "The day of escape."
^ya^m al-nafari jili\ >y^ "The day of flight."
^3:»^^l >\j\ A^* Ia jXuai\ >y^ "The day of the heart. These are the three days of tashriq^
^^ j lisi jj jUis^ JjS "The slaying of ^Uthman bin ^Afan." A has an IS^^day: l> ^^jJ- gadir
guman.
^^A has a 24^^day at ik^ ^li y\ ^ Ji ^xJl "^AlT bin Abu Talib gives away his seal. "
^^cLaoJu o^it AiJj "The occurrence of heat at Medina."
^^ According to Biruni, Serosh flrst ordered the Zamzama. He is also said by Biruni to be perhaps
the angel Gabriel.
^^"On the 19^^, or Farwardin-roz, there is a feast called Farwardagan on account of the identity
of the name of the day and of the month in which it lies. A similar feast-day they have got in every
46
Ardlbihisht^o
The 3^^ — Ardibihishtagan, its feast.
The 6*^ — The first of hrgini 1-sugd jj«JLJI Cf^J^
The 26*^ — The first of Gahanbar. Five days.
Khurdadh
The 6*^ — the feast of Khurdadhagan. The V^of nysg al-sugd AiJLJl /h-^.
The 26*^— the first of Gahanbar.
Tir
The 6*^— Chashn-i-nilufar.4i
The 13*^ — the lesser feast of Tiragan.
The 18*^ — the greater feast of Tiragan.
Murdadh
The 6*^ — istdhna 1-sugd jJiJJ\ ^\lJ\
The 7*^ — the feast of Murdadhagan.
Shahriwar
The 4*^ — the feast of Shahrlwaragan and Adhar-chashn^^.
The 6*^ — maziyhand al-sugd AiJJl JC^ -Ja.
The 16*^ — the first autumn. This day is (the first) of the 5*^ Gahanbar, which
lasts 5 days.
Mihr43
month." Biruni p. 209. Note that in the case of the Persian names, I use the trasliterations found
in Ginzel.
^^ Biruni states that the month name Ardibihisht means "truth is the best" or "the utmost of
good" .
^^The day of the water lilies
^^ feast of the fires
^^ Biruni states that the month name Mihr means "love of the spirit".
47
The V^ — the second autumn.
The 6*^ — fagagdn as-sugd JJtiJi jlSCii
The 16*^ — the feast of Mihrajan.
The 2V^— the Great Mihrajan.
Aban
The 6*^ — abandg as-sugd AijJl /T^'-
The 10*^ — the feast of Abanagan.
The 25*^ — the first of Farwardajan.
The 3V^ — the first of the 5 epagomenal days. (The first day of the) 6*^ Ga-
hanbar. In (the case of) the fixed months, these 5 days are (placed) at the end of
Isfandarmadh.
Adhar
The V^ — the riding of the thin-bearded man. It is called Bahar-chashn or Ther-
sites.
The 9*^— Adhar-chashn.
Dai
The V^ — Khuram-raz.
The 8*^— their feast.
The 11*^ — the first of Gahanbar and the night of the 15*^ is the feast of kdktl
The 23^^— the feast.
Bahman
The V^ — zimadanig as-sugd JJtiJi ^ ^.j
The 2^^ — the feast of Bahmanagan.
Isfandarmadh
^The feast of kaktl Ji5iris given as the 10^^ of Dai in Biruni.
48
1-145
The 1** — awwalu husumu 's-sugd A*iJI ^y^ Jjl*
The S*'* — the feast of Isfandarmadhagan.
The 11*'^ — the first (day of) the second Gahanbar. Five days.
The 16*'^ — Misk-i-taza,'^^ namely, the time of Spring.
The 26*'^ — the flowing of (the river) Zadarudahan jblijjSj into Isfahan jl^i
1.5.6 The Names of the Persian Days of the Month
The first of the month, Hormuz.
The T"^— Bahman.
The 3'"'^— Ardlbihisht.
The 4*'' — Shahriwar.
The h^^-Isfanddrmadh.
The 6^''—Khurdddh.
The 7*'^— Murdddh.
The S*'*— Dai-ba-Adhar.
The g*'*- Adhar.
The 10*'^— Abdn.
The 11*'^— ir/twr.
The 12^^— Mdh.
The 13*'^— Tzr.
The 14*'^— Gosh.
The 15*'^ — Dai-ba-mihr.
The 16*'^— M«7tr.
The 17*'^— ^ros/z.
The 18*'^— i?a5/in.
^^Biruni states that the month name Isfandarmadh means "intelligence" or "ripeness of mind"
*®This is "fresh musk" according to Biruni.
49
The 19*'^ — Farwardm.
The 20*'^— Bahram.
The 2P*— Ram.
The 22"*^— Badh.
The 2?,'"^— Dai-ba-dm.
The 24*'^— Z)«n.
The 25*'^— ^rd
The 26*'^— Ashtdd.
The 27*''— Asmdn.
The 28*'^— Zamidd.
The 29*'^— Marisfand.
The 30*'^ — ^neran.
The Names of the 5 Epagomenal Days
The P*— ^/inaud.^^
The 2"'^— Ushnaud.
The S*"*^ — Isfandhmadh.
The 4*^^— M/a5/iat
The S*'* — Washat wush.
1.5.7 On the Christian Feasts, Great Days and Month Names
Tishrin I
The Q*'* — Murdddmd maFtadid.
Tishrin II
The S*'* — Shahriwarmd ma'^tadid.
^'^These 5 transliterated from A.
50
The 22^^— the feast of Hunaqat}^
Kanun I
The V^ — the feast of hathdrat^^ .
The 8*^ — Mihrmd ma^tadid.
This month has 35 days, and in an intercalary year 36.
Shabat
The 2^^— Shama^i^^,
The 7*^ — the first heat from the earth.
The 11*^ — Adharmd ma^tadid. He was Caliph and his year was established for
this.
The 14*^ — the second heat from the earth.
The 15*^ — the beginning of the growth of plants.
The 2V^ — the third heat from the earth.
Adhar
The 8*^ — the appearance of swallows and storks.
The 13*^ — Daimd ma^tadid.
Nisan
The 12*^ — Bahman ma^tadid.
The 24*^ — dikrdnu margurgas
The 25*^— the birth of John.
lyar
The 12*^ — Isfanddrmd ma^tadid.
^^the consecration
^^the annunciation
^^wax candles
^^This is the commemoration of "Marcus, author of the second Gospel" according to Biruni.
51
The 13*^— the flooding of the Nile.
The 18*^ — the passing by of summer and the movement of the winds, 40 days
Haziran
The 11*^ — the V^ of Farwardmmd ma^tadid.
The 2V^ — the birth of hy bin dkryd li^i> jj ^
The 24*^ — the blowing of the West wind.
The 27*^— the end of the 40 days.
Tammuz
The 3^^ — dikrdnu marmd tumd loy lo^ <J^ifk'
The 11*^ — Ardibihishtmd ma^tadid.
The 19*^ — the flrst day of the heat of the lapis lazuli(l).
Abh
The V^ — the fast for the Virgin.
The 6*^ — transflguration day.
The 10*^ — Khurdddhmd ma^tadid.
The 15*^ — the fast-break for the Virgin.
The 24*^ — the death of hy bin dkryd li^i> jj ^
Ilul
The 2^^ — (the day) on which the star^^ rises in Iraq.
The 9*^ — Tirmd ma^tadid.
The 13*^- the feast of the raising of the cross.
52
Canopus
BOOK 2
On the Comprehension of
Interpolation, Sine, Arc, The
Sagitta^ and Tangent^— Things
Which are Very Useful for the
Astronomical Composition
This book is divided into 3 chapters.
2.1 On Interpolation
It is necessary to know the nature of a table. That number which has been placed at
the edge of a table is a gate, as it were, into calculations involving that table. That
number which is the difference of (two adjacent) entries in the table and that number
at the edge of the table are always precise with respect to (calculations involving)
4it. shadow
52
53
tabular difference. That tabular difference, however, which involves values (inter-
mediate) between two (adjacent) table entries, is not always precise (with regard to
such calculations). If this tabular difference (of adjacent entries) in the table has
been written down for this table, and the zodiacal signs go (in order) from the top of
the table down, then the tabular difference is reckoned opposite that number (with
which you enter the table). If the zodiacal signs go (in order) from the bottom of the
table up, the tabular difference is reckoned opposite the next number (after the one
with which you enter the table). If the tabular difference has not been written down
in this table, the number with which entrance was made into the table is examined.
The number after it is examined, and the smaller (of the two) is subtracted from the
larger. If the second number is greater, that column^ is said to be increasing. If the
first is greater, that column is said to be decreasing. This is a column of entries in
the body of the table, since a column at the edge (of the table) is always increasing.
When it is necessary to engage in this labor, if the number we have reckoned does
not have a fractional part, there is no need for (further) labor. The (desired) result is
reckoned opposite that number. If, however, our number does have a fractional part,
entrance is made (into the table) from the edge of the table opposite the degrees of
our reckoned number, and the (desired) number is found and reckoned in the body of
the table and examined. Then its tabular difference is made clear, and that tabular
difference is multiplied by the fractional part of our reckoned number. The result is
divided by the tabular difference (of the two corresponding entries) at the edge of
the table. If anything comes out, if the column in the body of the tables — after
reckoning and examination — is increasing, this result is added to it (i.e., the number
in the body of the table opposite the integer part of our number). If (the column)
is decreasing, it is subtracted, so that the interpolated number may be complete.
lit. number
54
2.1.1
If the number we have reckoned is a (type of) number in the body of the table,
and if it is necessary that the (corresponding) number at the edge of the table be
made clear from this (number of ours), the number we have reckoned is sought in
the body of the table. If a number is found there equal to ours, the number at the
edge of the table is reckoned opposite ours, and there is no need for anything else
for this calculation. If, however, a number equal to ours is not found there (i.e., in
the body of the table), the greatest number less than the number we have reckoned
is sought in the body of the table. Then the number at the edge of the table is
reckoned opposite this (found) number and examined. Then that number found in
the table — opposite which entrance was made into the table — is subtracted from
the number we reckoned. The result is multiplied by the tabular difference of the
number at the edge of the table and the result is divided by the tabular difference
(of the corresponding numbers) in the body of the table. The resulting sexagesimal
firsts and seconds are added to the number reckoned at the edge of the table so that
the number reckoned at the edge of the table may be complete.
2.2 On the Comprehension of the Arcs of Sines
and the Sagitta
The ancients divided the circle on the sphere into 360 equal parts. They called those
parts degrees. They divided the diameter of the circle into 120 units. Each of their
degrees was divided into 60 parts, and they called each of them a sexagesimal first.
Each of those (sexagesimal firsts) was in turn divided into 60 parts, each of which
they called a sexagesimal second. This process of division was continued in the same
way on the successive parts (of the circle) until (they reached) sexagesimal tenths.
It is necessary to know that the Sine is a base-point for the comprehension of its
55
arcs. Astronomers employ the Sine for all their computations. The maximum value
of the Sine is half the diameter, the length of which (half) is 60 units.
It is necessary to find the Sine of an arc given the arc. If the arc is less than 90,
the Sine is reckoned opposite that arc. If the arc is greater than 90 and less than
180, the diflFerence between that arc and 180 is reckoned, that is, the smaller value is
subtracted from the larger value. The Sine is reckoned opposite that result. If that
arc is greater than 180 degrees, its value is subtracted from 360 degrees. The Sine
is reckoned opposite this result.
If it is necessary that the sagitta be reckoned opposite the arc, if the arc is less
than 180 degrees, the sagitta is extracted opposite that (arc). If the arc is greater
than 180 degrees, its value is subtracted from 360. The sagitta is reckoned opposite
the result. The maximum value of the sagitta is the (length) of the diameter of the
circle, and this is 120 units. This (i.e., 120) is the sagitta of an arc of 180 degrees.
2.2.1 On Knowing the Sine from the Arc and the Arc from
the Sine
When we wish to engage in this labor, entrance is made into the table opposite the
arc at the top of the beginning of the Sine values. The Sine is extracted from the
body of the table opposite this value. If there are fractional parts to the arc in
question, that Sine becomes complete with interpolation. This was discussed at the
beginning of the first chapter (page 52). The result is the Sine of that arc. If it is
necessary that the Sine be of the complement of that arc, the arc is subtracted from
90. The result is the complement of the arc and the Sine is reckoned from this. The
result (of that calculation) is the Sine of the complement of that arc.
Whenever we have reckoned a Sine, that Sine is sought in the body of the table
of Sines, and its arc is reckoned opposite it (going down) from the top of the table.
56
as was discussed in the beginning of the second chapter^ ( page 55 ).
2.2.2 On Comprehending the Sagitta from the Arc and the
Arc from the Sagitta Using the Sine Table
Whenever we have reckoned an arc, and we wish to know its sagitta^ the arc is
examined. If it is less than 90, the Sine of the complement of that arc is subtracted
from 60. If the arc is 90 degrees, the sagitta is 60 units. If the arc is greater than 90,
it is subtracted from 90. The Sine of this result is reckoned and added to 60. The
result is the sagitta of that arc.
Whenever we have a sagitta and we wish to extract its arc from the table of Sines,
the sagitta is examined. If it is less than 60, it is subtracted from 60. The result is
a Sine. Its arc is reckoned and the result is subtracted from 90. That result is the
arc of the sagitta. If the sagitta is 60 units, it is right and its arc is 90 degrees. If
the sagitta is greater than 60, it is subtracted from 60. The result is a Sine. Its arc
is reckoned. The result is added to 90 and the arc of the sagitta is found.
2.3 On the Tangent^
(A tangent table) in fingers and feet has been set down along side the Sine table.
Entrance is made opposite the altitude and the tangent is reckoned.
^lit. "the section of the first chapter" -but this is incorrect
^lit. shadow
BOOK 3
On the First and Second
Declination to the North and to
the South, (on) the Latitude of
Cities, the Culmination of Stars
and Rising Times in Right
Ascension
This Chapter is divided into 4 sections.
^lit. the place of "fortune" with the straight hne
57
58
3.1 On the First and Second Declination
The obliquity of the ecliptic^ is the angle between the ecliptic^ and the celestial
equator^, that is, the circle which makes a complete rotation in a nychthemeron.
(This angle) is 23 degrees and 35 sexagesimal firsts. The second (type of) declination
(which can take on values) greater than the first (type) is divided into two (kinds).
The one (kind) is called ''first" , and it is needed for the comprehension of the ascent
of the Sun to the meridian and for the equation of day. The second (kind of)
declination is useful for the distance of stars, that is, the distance of stars from the
celestial equator. Therefore a table has been set up for these two declinations, so
that entrance is made opposite the degrees of the zodiac and the measure of the
declination is reckoned. If it is necessary to know whether this declination is to
the North, to the South, ascending or descending, the (number of) zodiacal signs
is examined. If it is less than 6, it is to the North. If it is greater than 6, it is to
the South. If the zodiacal signs are between 9, and 3, it is ascending. If they are
between 3, 6 and 9, it is descending.
3.2 On the Comprehension of the Latitude of
Each City
The mid-day altitude of the Sun^ is comprehended and the first declination is reck-
oned opposite the degrees of the Sun. That declination, if it is to the South, is added
to the mid-day altitude of the Sun. If it is to the North, it is subtracted. The result
^lit. great declination
^lit. circle of the zodiac
^lit. complete zone of day
^lit. the altitude of the Sun on the circle of the middle of the day
59
is then subtracted from 90, and that result is the latitude of the city.
If, instead of the Sun's declination, the distance of a star from the celestial
equator^ is used, a method is employed similar to the one just described.
3.2.1 On the Comprehension of the Latitude of a City by
Means of a Star Which is Always Visible and Never
Sets
The altitude of that star is sought and reckoned at two times, when it is at its
greatest distance from the earth, and when it is closest to the earth. Then these two
altitudes are added and the result is divided by 2. The result is the latitude of the
city.
Whenever the Sun enters the first of Cancer, the complement of the altitude is
reckoned with an astrolabe at mid-day. 24 is subtracted from this. The result is the
latitude of the city where the altitude was reckoned. If it is reckoned in Capricorn, 24
is added to the altitude and in this case, as in the earlier one, the latitude of the city
in question is revealed. It is necessary to know that the result of the subtraction or
addition of 24 is subtracted from 90 and so becomes the complement of the latitude.
3.3 On Comprehending the Mid-Day Altitude of
the Sun and the Rest of the Stars
After the latitude of the city is reckoned, it is subtracted from 90 and so the co-
latitude (of that city) is found. Then the first declination is reckoned from the degrees
of the Sun — or the distance of the star from the celestial equator is reckoned. If
the declination — or the distance of the star — is to the North, that declination or
^lit. the complete circle of day
60
distance is added to the co-latitude of the city. If it is to the South, it is subtracted
from that co-latitude. If the result is less than 90, it is the altitude of the Sun or
star on the Southern part of the meridian circle. If the result is greater than 90, it
is subtracted from 180. The result is the altitude of the Sun or star on the Northern
part ( of the meridian circle).
3.4 On Comprehending the Place of the ^Tortune''
of the Zodiacal Signs with the Straight Line
This is the calculation: whenever this is necessary, the Sine of that degree is mul-
tiplied by the Sine of the complement of the declination. The result is divided by
the Sine of the complement of that degree. This result is the Sine of the place of
the ''fortune" with the straight line. The arc of the Sine is reckoned and that (arc)
is the place of the ''fortune" of that degree. A table has been set up for the place
of the "fortune". The order of the table is from the first of Capricorn. Whenever it
is necessary, the place of the "fortune" is reckoned from the degrees of the zodiacal
signs. The zodiacal sign is sought at the top of the table and the degrees along the
side. The place of the "fortune" is reckoned in the body of the table opposite the
two (numbers).
If we have reckoned a place of the "fortune" and we wish to know its corresponding
degree and zodiacal sign, that place of the "fortune" is sought in the body of the
table. Its zodiacal sign and degrees are reckoned opposite the place where it has
been found (counting) from the beginning of the table. Interpolation is used and
employed as in the way described earlier.
If we wish the place of the "fortune" to be (counted from) Aries instead of from
Capricorn, 90 degrees are subtracted from the degrees of the place of the "fortune"
in the table, or 270 degrees are added to them, since one number results from both
61
calculations. The result is the that (the rising time) counted from Aries.
BOOK 4
On the Correction of the Dayhght
with the Arrow, the Arc of the
Day and the Night, the Degrees of
the Seasonal Hours, the Places of
the Zodiacal Signs for all the
klimata with the Latitude of
Rising
4.1 On Whether the Latitude of Rising is Southerly
or Northerly
If the declination of the Sun or the distance of the stars from the complete circle of
day to the north is greater than the completed of the latitude of the city, that star
62
63
is always visible and does not set below the earth. If its declination or its distance
is to the south, that star is always below the earth. In both these cases there is no
latitude of rising. If its declination or its distance is each opposite to the complement
of the latitude of the city, the latitude of rising is 90 degrees. If the declination or
the distance is less than such a latitude of the city, that star rises and again sets,
and so its latitude of rising exists.
When there is need for this calculation, the Sine of the declination, or the dis-
tance, is divided by the sine of the co-latitude of the city. The result is raised by one
step and the Sine of the latitude of rising is found. Its arc is reckoned, and so the
latitude of rising is found.
On Knowing Whether the Latitude of Rising is
Northerly or Southerly
If the declination is northerly, so is this latitude of rising. If this declination is
southerly, so is this latitude of rising southerly. If the Sun has no declination, or the
star a distance, then they are on the complete circle of day and thus they do not
have a latitude of rising.
4.2 Correction of the Daylight and the Arrow of
the Day
If the Sun has no declination or the star a distance, they do not have a correction
of daylight, and so one half the arc of daylight is 90 degrees. If the Sun and the
star have a declination and a distance, the Sine of each is multiplied by the Sine
of the latitude of the city. The result is divided by the Sine of the complement of
each. This result is called the radix. Then this radix is divided by the Sine of the
64
complement of the latitude of the city. The result is lowered by one (sexagesimal)
step, and the Sine of the correction of daylight is found. Its arc is then reckoned.
This is the correction of daylight.
We have set up a table for this, namely, for the complete equation of daylight.
The Sine of the correction of daylight is reckoned opposite the latitude of whatever
city we wish. Proportional parts ^ are reckoned opposite the degrees of the Sun.
These parts are mulitipled by the Sine of the correction of daylight. The result is
then lowered by one step, so that the Sine of the correction of daylight is found.
Then the arc of this Sine is reckoned and the correction of daylight in degrees of the
Sun is found for that day. If the correction of daylight is doubled, the (complete)
difference of the daylight ^ is found.
4.2.1 On the Arrow of the Day
If the declination or the distance is northerly, the Sine of the correction of daylight is
added to 60. If the declination or the distance is southerly, the Sine of the correction
of daylight is subtracted from 60. Thus the arrow of the correction of daylight is
found either in addition or in subtraction.
4.3 On the Arc and The Hour of the Nychthemeron
and the Degrees of a Seasonal Hour
The ancients held that one nychthemeron is 360 time degrees and again that this
nychthemeron is 24 hours. This chapter is set down to explain this.
If the declination or the distance is northerly, the correction of daylight is added
to 90. If these are southerly, they are subtracted from 90. The result is half the arc of
^ "coefficients of interpolation" Neugebauer.
^Neugebauer p. 14 under izEpiooEia
65
daylight. This is doubled and so the complete arc of daylight is found. Alternatively,
if the declination or the distance is northerly, the (complete) difference of the day is
added to 180 degrees. If the declination and distance are southerly, the declination
or the distance is subtracted from 180 degrees, and the daylight of the arc is found.
If the arc of daylight is subtracted from 360, the arc of night is found.
4.3.1 On the Equinoctial Hour
The arc of daylight is divided by 15 and the equinoctial hour of every day becomes
clear. This complete hour of every day is subtracted from 24, and the hour of every
night is found. If the arc of daylight is divided by 12, the parts of a seasonal hour
of the day are found. If these are subtracted from 30, the parts of a seasonal hour
of the night are found.
4.3.2 (Seasonal Hour)
If an equinoctial hour is multiplied by 5 and the result is divided by 4, the parts of
the seasonal hour are found. If the parts of the seasonal hour are multiplied by 4
and the result is divided by 5, an equinoctial hour is found.
4.4 On Obtaining the place of the ^Tortune'' (As-
cendant) of the Zodiacal Signs for the Lati-
tudes of All the Klimata.
The correction of daylight is subtracted from the place of ''fortune" of the zodiacal
signs with the straight line which is from the beginning of Aries in the case of the
northerly zodiacal signs. In the case of the southerly zodiacal signs, the correction
of daylight is added to the place of ''fortune" of the zodiacal signs. The result is the
66
place of "fortune" at the latitude of the city.
BOOK 5
On the Motion of the Fixed Stars from Their True
Longitudes and Their Distances from the Circle
which Moves in a Nychthemeron, That is, Their
Distance to the Circle of Mid-day, the Ascent of
Such Stars, that Degree of that Zodiacal Sign Which
is Together with the Star on the Circle of Mid-day,
the Degree Which Rises with the Star, the Degree
Which Sets with the Star, and that Hour of their
Rising and Setting in the Day or the Night.
This book is divided into 5 chapters.
67
68
5.1 On the Knowledge of the True Longitude of
the Stars
It is necessary to know that (the positions of) 25 stars from those that are visible
were set down in this book (corrected for) for the beginning of the Arab year 509.
Whenever it is necessary to apprehend their true longitude, 509 is subtracted from
the (current number of) Arabic years. The result is divided by 68. The result is
in degrees. These are multiplied by 53 seconds. The result is added to their true
longitude set down in the table, and the true longitude of those stars is found for
that year.
5.2 On the Distance, that is, the Distance of the
Stars from the Circle Which Moves in a Ny-
chthemeron and their Extreme Ascent
An examination is made. If the star has no latitude, the first declination is reckoned.
This is the distance of the star from the circle of equalization. If the star does have a
latitude, the second declination is reckoned and examined. It is determined whether
(the declination) is northerly or southerly and whether the latitude is northerly or
southerly.
Then an examination is made. If the two-the declination and the latitude- are
both northerly or southerly, they are added. If the one is northerly and the other
southerly, and if the two are equal, the star is on the circle and has no distance. If
they are not equal, the smaller is subtracted from the larger. The result is examined.
If the larger is northerly, this distance is northerly. If the larger is southerly, that
(distance) under consideration is southerly. Then an examination is made. If the
star is in degree zero of Cancer or in degree zero of Capricorn, the result of this
69
computation is its distance from the circle of daylight. If the star is in neither of
these-namely, Cancer or Capricorn- but elsewhere, that which we reckoned is the
degree of distance from the circle of equalization of daylight.
5.2.1 On Learning the Distance of the Stars from the Circle
of the Equahzation of Dayhght
The Sine of the degree of the distance is reckoned and multiplied by the Sine of
the completed greatest declination. The result is divided by the completed second
declination of the true longitude of that star. The Sine of the distance from the
circle of the equalization of daylight is found.
If the true longitude of the star has no declination, the result of the multiplication
by the Sine of the completed declination is lowered by one step. The result is the
Sine of the distance from (the circle) of the equalization of daylight. Its arc is taken.
5.2.2 On the Knowledge of the Ascent of the Equation of
Dayhght
This has already been discussed (4.2).
5.3 On Knowing the Degrees of those Zodiacal
Signs which are Together with the Star on the
Circle of Mid-day
If a star has no latitude, that star is at the circle of mid-day together with the degree
of its true longitude. If the star has a latitude and if that star is within (the arc)
Cancer, Libra and Capricorn, that latitude is southerly and that star sets before its
proper degree reaches mid-heaven. If the star is within (the arc) Capricorn, Aries
70
and Cancer, its latitude is northerly and the star rises before its proper degree is at
the mid-day circle.
The Sine of the completed latitude is reckoned and is multiplied by the Sine
of the distance of the star from the beginning of Cancer or from the beginning of
Capricorn, whichever of these zodiacal signs is closer to the star. The result is divided
by the completed Sine of the distance of the star from the circle of the equalization
of daylight. The result is the Sine of the correction. Its arc is taken. Then an
examination is made. If the true longitude of the star is after Cancer or Capricorn,
that correction is added to the place of ''fortune" , to degree zero of Cancer or degree
zero of Capricorn, with the straight line. Entrance is made into the tables of the
place of ''fortune" with the straight line, and opposite that number the zodiacal
signs are reckoned above (the table) and the degrees along the side. The second
calculation, that between the two tables, is carried out as mentioned (earlier) (2.1).
The result is the degree so that it reaches mid-heaven together with the star.
5.4 On that Degree which Rises with the Star
If the star has no latitude, that star rises with the degree of (its) true longitude. If the
star has a latitude, its place of "fortune" with the straight line is apprehended, and
its beginning is from the beginning of Capricorn. The result is reckoned. Then an
examination is made. If the distance of the star from the circle of the equalization
of daylight is northerly, the equation of daylight is subtracted from the place of
"fortune" . If the star's distance is southerly, it is added to the place of "fortune" .
Ninety is always subtracted from this result. The result is the place of "fortune" of
the degree with which the star rises. Entrance is made into the table of the place
of "fortune" opposite this result. Wherever this number is found in the body of the
table, there are reckoned opposite this the zodiacal signs above (the table), and the
degrees along (its) side and the parts between the two tables we reckoned in the
71
manner that was described (earlier).
5.4.1 On the Degree Setting with the Star
When there is need for the calculation, the arc of the star in the day is added to the
degree of the place of ''fortune" which rises after it. This result is sought in the table
of the place of ''fortune" for the latitude of that city in zodiacal signs and degrees
in the manner that was described (earlier). 6 zodiacal signs are added to the result,
and the degrees setting with the star are found.
5.5 On When the Star Rises and Sets, Whether
by Night or by Day
That degree rising with the star is sought. If it is between the Sun and its diametri-
cally opposite (point), the star rises in the day. If that degree is found between the
(point) diametrically opposite to the Sun and the Sun itself, (the star rises) at night.
If the star rises in the day, the place of "fortune" of the degrees of the Sun at the
latitude of that city are subtracted from the place of "fortune" of the degrees rising
with the Sun. The result is the revolution from the beginning of that day (until the
time) when the star rises. If the star rises at night, the place of "fortune" of the
degrees of the (point) diametrically opposite to the Sun at the latitude of the city is
subtracted from the place of "fortune" of the star. The result is the revolution from
the beginning of the night until the time when the star rises.
As for this calculation which has been mentioned, if we wish to know when the
star sets, that degree setting is reckoned so that it rises. The method is similar.
BOOK 6
On the Knowledge of How Many
Hours of the Day that Have
Passed, How Many Degrees from a
Seasonal Hour, the Hours of the
"Fortune" , the Correction of the
12 Houses, and the Knowledge of
the Point of Each Altitude and the
Point of Prayer
This book is divided into 7 chapters.
72
73
6.1 On the Knowledge of the Arc of the Sun,
When it Rises at What Time We Wish to
Know This, Namely the Equinoctial and the
Seasonal hour
Whenever there is need to know and to apply this knowledge, first the altitude of the
Sun is reckoned by means of the astrolabe at the time we wish, and this is called the
altitude of the moment (under consideration). Then the maximum altitude of the
Sun for that day is calculated in the same way, and the arrow of the day is sought
and found. Whenever we wish to make this calculation we do as follows: the Sine of
that altitude is divided by the arrow of the day^. The result is divided by the Sine
of the maximum altitude. The result is a Sine. This is always subtracted from the
arrow of day. The result is an arrow. Its arc is taken. The result is called the excess
of the arc^. Then the time of the altitude is examined. If it is before mid-day, this
excess is subtracted from half the arc of daylight. If it is after mid-day, the excess
is added to that and the arc from that hour when the Sun rises until the moment
under consideration is found. The hours (of the arc of the Sun) are extracted from
this.
6.1.1 On Knowing the Altitude of a Star at a Time Which
One Wishes From the Arc
When there is need for this calculation, the excess of the arrow is obtained and is
subtracted from the arrow of day. The result is a Sine. This Sine is multiplied by
the Sine of the maximum altitude at the circle of mid-day. The result is multiplied
^Neugebauer p. 15 under aayiTa
^Neugebauer p. 14 under nepiaaeia
74
by the arrow of day. The result is the Sine of the altitude for that time.
6.1.2 Knowing if Anything has Passed of the Night
The altitude of the fixed star is reckoned. The same method is employed as in the
case of the Sun, and the calculation is the same without any changes. For here, the
Sine of the altitude (of the star) is multiplied by the arrow of day, and the resulting
calculation is the same as in the earlier case. And the arc from that hour when the
star rises until the hour under consideration is found.
6.1.3 For the Knowledge of How Many Hours Have Passed
of the Day in Seasonal Hours
This (number) is apprehended from the altitude for any moment and the altitude
of the circle of mid-day. For the Sine of the altitude for any moment is divided by
the maximum altitude. The result is lowered by one step. The result is a Sine. Its
arc is reckoned and divided by 15. The result is a seasonal hour.
If that altitude is reckoned before mid-day, that discovered seasonal hour is (the
time) from the beginning of the day until then. If this altitude is after mid-day, that
hour is subtracted from 12. The result is the seasonal hour from the beginning of the
day until then. If we wish to know the altitude from the seasonal hours, those hours
are divided by 15. The Sine of the result is divided by the Sine of the maximum
altitude. The result is lowered by one step. The result is the Sine of the altitude for
any moment.
75
6.2 For Knowing the Hour from the Arc and from
Other Things
If there is need to make this calculation, if the arc is in the day, it is added to the
place of ''fortune" of the true longitude of the Sun for the latitude of the city. If the
arc is at night, that arc is added to the place of ''fortune" of the point diametrically
opposite to the true longitude of the Sun for the latitude of the city. Entrance is made
into the middle of the table of the latitude of cities opposite the result (which is the
place of "fortune"), and the zodiacal signs, degrees and minutes are reckoned from
it using the same method of calculation that has been mentioned many times. The
result is the zodiacal signs, degrees and minutes of the "fortune" for that moment
when the altitude was reckoned.
If the hour of the day or night which is passing is known, and that hour is
equinoctial, it is divided by 15. If it is seasonal, it is divided by the parts of a
seasonal hour. The result is the arc from which is extracted the Lot of Fortune.
6.2.1 For Knowing the "Fortune" from the Degrees of the
10th House
The place of "fortune" with the straight line is reckoned from those degrees (of the
10th house), and the beginning of them is from the beginning of Capricorn. Entrance
is made into the middle of the table of the place of "fortune" for the latitude of the
cities, and the zodiacal signs and the degrees are reckoned in accordance with the
method mentioned earlier. The result is the "fortune" .
76
6.3 On Knowing the Arc of the Hours from the
^Tortune''
The true longitude of the Sun and the degrees of the ''fortune" are sought, reckoned,
and examined. If the true longitude of the Sun is between the 7th and the 10th
house, the place of ''fortune" of the true longitude of the Sun^ from the latitude of
the city is subtracted from the place of the "fortune" for the latitude of the city.
The result is the arc from the beginning of the current day.
If the true longitude of the Sun is between the 4th and the 7th house, the place of
"fortune" of the point diametrically opposite to the Sun is subtracted from the place
of "fortune" for the latitude of the city. The result is the arc from the beginning of
the night until the hour of that moment. The equinoctial and the seasonal hour is
extracted from this arc.
6.4 On Knowing the 12 Houses, that is, Correct-
ing them
Whenever it is necessary to use this method, the degrees of the hours and the de-
grees of the "fortune" are found out and doubled. The result is the first correction.
This is always subtracted from 60, and becomes the second correction. These two
(quantities) are examined. Then the place of "fortune" for the latitude of that city
is reckoned. This is called the tenth. This is the calculation set down for the tenth
house.
Then the first correction is added to it. The result is the place of the "fortune" of
the eleventh house. Again, the first correction is added to the place of the "fortune"
of the eleventh house. The result is the place of "fortune" of the twelfth house. Then
^Neugebauer p. 17 under totio^
77
the first equation is added to the twelfth house and so the place of the ''fortune" (of
the first house) is found.
Then the second correction is added to this place of ''fortune" and becomes the
place of "fortune" of the second house. Again, the second correction is added to the
place of "fortune" of the second house, and the place of "fortune" of the third house
is found. Then the second equation is added to the place of "fortune" of the third
house, and the fourth house for the place of "fortune" is found. Then the place of
"fortune" of the 10*^ house is brought to the table of the place of "fortune" with
the straight line from the beginning of Capricorn. Opposite the number that was
found within the table the zodiacal signs are reckoned above and the degrees along
the side with the number found between the two tables. The result is the center of
the 10*^ house. The place of "fortune" of the 11*^ house is examined in the table of
the place of "fortune" with the straight line in the same way. The same holds true
for the remaining houses up to the 4*^, just as we said in the case of the 10*^ house
also. Their centers are found.
The degrees of the 5*^ house are opposite (those) of the 11*^, and the degrees of
the 6*^ house are opposite (those) of the 12*^. The (degrees) of the 7*^ house are
the same as the degrees of the V^ house, and those of the 8*^ house as those of the
2^^. The degrees of the 9*^house are opposite those of the 3^^ house. In this way the
corrections of the 12 houses are completed and the centers of all are found.
Check of this Calculation
If the numbers of the 10*^ and of the 4*^ house are equal in degrees and minutes,
the calculation is correct. Again, if the place of "fortune" extracted earlier and set
down in the case of the 10*^ house is equal to the place of "fortune" which was
extracted then from the tables of the place of "fortune" with the straight line, the
calculation is correct.
78
There is a (time) when the center of the 10*^ house is in its own house, but
sometimes it tends towards the 11*^, and sometimes towards the 9*^ house. When it
tends towards the 11*^, it is said to nod towards it. When it tends towards the 9*^,
it is said to fall. When it tends neither towards the one nor the other, it is said to
stand.
6.5 On Knowing the Point of Ascent
When there is need for this method, the Sine of the ascent is multiplied by the Sine of
the latitude of that city. The result is divided by the completed Sine of the latitude
of the city. The result is the point of the degree of the ascent. Then an examination
is made. If the declination of the Sun or the distance of the star is southerly, the
Sine of the latitude of the rising is added to the point of the degree of the ascent.
If its declination and the distance is northerly, the smaller of these two numbers is
subtracted from the larger. The result is the equation of the point.
6.5.1 For Knowing the Point
The equation of the point is divided by the completed Sine of the ascent. The result
is lowered by one step. The thing found is the Sine of the point. Whether this point
is southerly or northerly is apprehended from this: If the Sun has no declination and
the star no distance, the point of the ascent is southerly. If the Sun has a declination
and the star has a distance and they are southerly, the point of the ascent is also
southerly. If the declination and the distance are northerly, the degree of the point is
examined. If it is greater than the Sine of the latitude of rising, that point of ascent
is southerly. If it is less, it is northerly.
79
6.5.2 For Knowing that Ascent which has no Point
This ascent occurs in the case of those cities towards the north, where the declination
of the Sun or the distance of the star is less than the distance of that city. When
there is need for this calculation, it is computed as follows :
The Sine of the first declination or the Sine of the distance of the star is reckoned
and divided by the Sine of the distance of the city. The result is lowered by one step.
This result is the Sine of that ascent which has no point.
6.6 For the Extraction of the Line of Mid-Day for
the Earth
An accurate correction of the surface of the earth is made when water is poured on
it so that the surface is covered without the water proceeding in any other direction.
Then a circle as large as one wishes in diameter is drawn on this corrected surface
of the earth. A plumb line, of whose two ends the one towards the center is full and
thick, while the one above comes to a point, is positioned at the center of the circle.
The length of this plumb line should be less than the diameter of this circle.
When the Sun rises in the morning, the shadow of the plumb line is examined (to
discover) whether it reaches to the circumference of the circle. When the shadow
reaches the circle, a mark is placed there. Then, when the Sun is declining from
mid-day, the plumb line is examined (to discover) whether its shadow reaches the
circumference of the circle, and a mark is placed there also.
From these two points placed on the circle a line is drawn straight from one point
to the other. Then this line is cut in two at a point, and a line is drawn from the
middle of that line to the center of the circle. This is the line of mid-day. The line
from the former mark on the circle to the other mark is the line of rising and setting.
Then the circle is cut into 4 from the diameter of the circle. It is written in each
80
part: in one East, in another West, in another North, and in the fourth South. Each
quarter of the circle is divided into 90 degrees
6.7 For Knowing that the Abominable Prayer of
the Unholy Persians is reckoned from How
Much has Passed from the Line of Mid-day
If the longitude of the city in which the unholy live is opposite the longitude of Mecca
— may God lay waste to and destroy that place because of the evil-heartedness of
the unholy! — the point of their abominable prayer is with the straight line, that is,
it is straight along the diameter of the circle (mentioned above). If (the longitude)
is greater or less (than the longitude of Mecca), the calculation is made as follows:
The longitude of Mecca and the longitude of the city which we wish are examined,
and the smaller is subtracted from the larger. The Sine of the result is reckoned, and
that Sine is multiplied by the completed Sine of the latitude of Mecca. The result is
lowered by one step. This is the Sine of the complete longitude.
This is examined. Then the Sine of the latitude of Mecca is divided by it. The
result is the Sine of the complete longitude. Its arc is reckoned and added to the
completed latitude of the desired city. Then this result is called the base. Then
that Sine is reckoned, and this is multiplied by the completed Sine of the complete
longitude. The result is lowered by one step. The result is the Sine of the completed
distance between the desired city and Mecca, hateful to God. Its arc is reckoned and
subtracted from 90. The result is the distance between that city and Mecca.
Then the Sine of the complete distance is increased by one step, that is, up. This
is divided by the Sine of the distance between the two — the city (in question) and
Mecca. The result is the Sine of the place with the straight line of the polluted
prayer. An examination is made again. If that base is less than 90, the point of that
81
prayer hateful to God is southerly with respect to the line extending from East to
West. If it is greater than 90, the point of the prayer of the unholy is northerly. If
the number is exactly 90, the place of the abominable prayer of the unholy is to the
point on the straight line extending from East to West. And the point of that most
polluted prayer of the unholy for that city is extracted by means of this calculation
and is set down in this table.
City
Showing of the
Direction
1
5-1-1
O
.2
?-i
o
• S
'-^
o
o
City
Showing of the
Direction
1
Oh
5-1-1
O
.2
?-i
o
bO
• S
'-^
o
o
City
Showing of the
Direction
1
O
.2
?-i
o
bO
• S
'-^
o
o
a;
'bb
1
a;
'bb
1
a;
'bb
1
Babylon^
76
40
Tabaristan
55
Balkh
9
20
Mawsil
82
20
Jilan
57
Khutlan
27
30
Ramadan
64
30
Jurjan
48
40
Tukharistan
26
Rayy
51
55
Kirman
43
30
Ghur
29
Damghan
50
30
Sijistan
18
20
Khwarizm
50
Isfahan
48
Rhaoua^
19
20
Bukhara
40
40
Persia
45
Bouj^
21
30
Samarqand
39
Aoulaz^
49
30
Nishabur
42
50
Siran
48
1
Adharbayjan
70
Marw
38
20
Taras
43
1
Armenia
80
Harah
29
Khutan
36
30
1. For Baghdad. 2. For Ahwaz. 3. For Ghaznah. 4. For Bust.
This calculation of the table was set down in this way from the straight line
beginning from the West, not from the line of mid-day.
BOOK 7
On the Extraction of the Mean
Motions of the Seven Planets
'^Abd ar-Rahman al-Khazinl says the following: let us make a procedure for the
mean motions of the planets in three ways. The first is this: with reference to the
longitude of 90 (degrees) from the edge of the Western sea for the mean motion of this
composition^. The second is this: for the longitude of each city with the correction
for the two longitudes — (that) of the composition and (that) of that city. This is
called the mean motion for the city. The calculations of the true longitudes are made
from this mean motion. The third is that the mean motions are corrected with the
equation of daylight for nativities and entrance (of the years).
This book is about the extraction of the mean motions of the planets and the
apogees and corrections of each, the beginning of Sultanic years in days of the week
with the years for their beginning and end, and (concerning) the knowledge of the
basis of the true longitude for one year of the Sun. This book is divided onto four
chapters.
^Neugebauer p. 12 under [ifpioc,
82
83
7.1 On the Extraction of the Mean Motions of the
Planets for a Latitude of 90 (Degrees)
When there is need for this method, the year of the Arabs is first corrected with the
mean number for the weekday which we wish in the way described earlier (see 1.3.2).
Then the incomplete years of the Arabs are placed in one part of the tablet. The
month which we wish is placed under this, and the number of days of that month
are placed under the month. Then a number equal to the (number of) previously
apprehended years is sought in the table for thirty year periods of the Arabs. En-
trance is made into the table wherever the years equal to these are found. If the
years equal to these in number are not found in the tables, the closer number less
than it is sought.
Entrance is made into the table opposite that (number) and a reckoning is made.
The zodiacal signs, degrees, minutes and seconds, if there are any, (are reckoned)
in the table of the desired planet opposite that, and are placed on the tablet in
the following order: first zodiacal signs, then degrees, then minutes, and after these
seconds.
Then whatever is found of later days and of these from the side is placed sepa-
rately in one part of the tablet.
Then the years in the table from which entrance was made into this are subtracted
from (those) reckoned earlier and placed on the tablet. The result is sought in the
table of single years of the Arabs. Entrance is made into the table of that planet
opposite (the place) where that number is found, and the zodiacal signs, degrees and
minutes are reckoned and placed on the tablet under the previously reckoned mean
motion for the thirty year periods, zodiacal signs under zodiacal signs, and so on.
The weekdays found afterwards are reckoned in the same way and are added to the
days found earlier from the thirty year periods.
84
Then entrance is made into the table of months opposite the month we have
reckoned, and this value of the mean motion of that planet is reckoned in the way
described and placed under the number for the single years — zodiacal signs under
zodiacal signs and so on, just as in the other cases. Then the days after it are
reckoned and added to the days reckoned from the years and the months. Then the
reckoned days of the month are sought in the table of the days. Entrance into the
table of the days of that planet occurs opposite (the place) where they are found. The
result is placed under the number for the months — zodiacal signs under zodiacal
signs and so on, just as in the other cases.
Then the days after it are reckoned and added to the days reckoned from the
years and months. If the number is greater than seven, there occurs subtraction by
sevens. Whatever is left, if they are equal to the previously reckoned days of the
month, the calculation is correct. If they are not equal, the calculation occurs again
starting with the years. If the calculation is correct, all the numbers of the mean
motions are added together. If the number in the seconds place is greater than 60,
60 are subtracted from it, and one is added to the minutes. Again, if the number of
minutes is greater than 60, 60 are subtracted from these minutes, and one is added to
the degrees. If the number of degrees is greater than 30, 30 are subtracted from the
accumulated degrees, and one is added to the zodiacal signs. If in turn the number
of zodiacal signs is greater than the number 12, 12 are left aside, and one (rotation)
is reckoned as remaining.
The result is the mean motion of that planet in zodiacal signs, degrees, and
minutes with respect to the mean motion of the composition for mid-day of that day
for a longitude of 90 (degrees). If there is with us a fraction of an hour, entrance is
made into the table of the hours (which is) under the months opposite that hour.
And the mean motion of that planet is reckoned and added to the mean motion
reckoned earlier.
85
7.1.1 On the Correction of the Apogee
After the mean motion is reckoned, entrance is made opposite that year (into the
table) in years, months and days, and the mean motion of the apogee is reckoned in
zodiacal signs, degrees, minutes, and seconds. Then the apogee under the months of
that planet found for the beginning of the year of the Arabs is added to that motion
of the apogee. The result is the apogee with the correction.
7.2 On the Correction of the Mean Motions of the
Planets
This is done in two ways. The first is this, that from the difference of the two
longitudes, the number of the mean motion of the composition is carried over to the
longitude of the other city. The second is this: the mean motion corrected with the
longitude of the city is complete with the equation of daylight. The first number is
reckoned from two things. It is the difference between the two, the (longitude of the)
city which we wish and the longitude of 90 (degrees). The result is divided by 15
or multiplied by four minutes. The result is an hour or a fraction of an hour. Then
entrance is made into the table of hours under the months opposite those hours, and
the mean motion of that planet is reckoned and examined. Then it is multiplied by
the longitude of that city. If this is less than 90 (degrees), the mean motion reckoned
from the hours is added to the mean motion from the composition. If it is greater
than 90 (degrees), it is subtracted from that, and the mean motion for that city is
found. The difference (in longitude) is for the correction of the mean motion for that
city with the equation of daylight.
Entrance is made into the tables of the equation of daylight opposite the mean
motion of the Sun, and the fraction of an hour is reckoned. Then entrance is made
into the tables of hours under the months opposite this fraction (of an hour), and
86
the mean motion of that planet is reckoned. The result is always subtracted from
the mean motion for that city, and the complete correction of the mean motion for
that city is found.
7.2.1
If this method of true longitudes occurs through nativities, the longitude of the city is
examined. If it is less than 90 (degrees), that hour resulting from the two longitudes
is added to that year in which the birth took place. If the longitude of the city is
greater than 90 (degrees), that hour is subtracted from that year. Then the fraction
(of an hour) of the equation of daylight is subtracted from the year, and the year is
corrected with a complete correction. Then entrance is made into the table of the
mean motions of the planet opposite that year, and the numbers of these from the
composition are reckoned. These mean motions are correct for that moment.
7.3 On the Entrance of the Well Known Sultanic
Kahisa Years
Know that one year of the Sun is 365; 14,27,20,36,47 (days). Such is the year of the
Romans, and such are the fractions for it^. The excess of the year of the Sun is
0;0,32,39,23,13. These fractions make one complete day in 110 years. The year of
the Persians is less than the year of the Sun by 0;14,27,20,36,47 (days). The year of
the Moon is such: 354;22,1,36,51 (days). The year of the Sun is greater than the year
of the Moon by so much: 10;52,25,43,45,55 (days). The cycle of the week exceeds
the year of the Sun by one day (in addition) to as many fractions as a year of the
Persians is less than a year of the Sun. A table has been set down for this for the
Sultanic year in which the years are set down in 20 (year intervals) of the Sun.
^See Neugebauer, appendix 15
87
7.3.1 For Knowing this, on what Day the Perceptible Years,
Namely the the Well Known Sultanic Years, Begin in
Those Three Calendars and in the Days of a Week
Entrance is made into the table of thirty year periods and single years opposite the
completed Sultanic years. The result is reckoned opposite the two tables for the
years of the three calendars. In the same way the days of the years along with their
first and second (sexagesimal) parts (are found) on the side. Then the days of the
week which are at the end of the tables and their first and second (sexagesimal) parts
are examined, as well as their arrangement. If the number of seconds is greater than
60, 60 are subtracted from them, and one is added to the minutes. If these, in turn,
are greater than 60, 60 are subtracted from them, and one is added to the days. If
these days are greater than the days of a year, the days of a year are cast out, and
one is added to the years. Then it is multiplied by the reckoned minutes of the days
of a week. If this result is less than 15, the year's beginning is from the reckoned
days of the week. If these are more than 15, the year's beginning is on another day.
One day is added to the days found, and one day is added for each calendar of the
three.
7.3.2 On Knowing that the Coming Year is Basita or Kahisa
An examination is made into the reckoned minutes of the days of the week. If they
are less than so many: 0;45,35, the coming year is hasita and the days of that year are
so many: 365. If those minutes are greater than 0;45,35 the coming year is kahisa.
Its days are so many: 366. This calculation is for a longitude of 90 (degrees), not
for the longitude of other cities.
7.4 On the Base of the True Longitude of the Sun
for One Year of the Sun
A table has been made for the motion of the planets for one year of the Sun and
for the months of that year. These months are set up in such a way that at the
beginning of each month the Sun is at the beginning of a zodiacal sign. Then on
whatever day, month and year of the calendar of the Arabs the beginning of the year
of the Sun occurs , entrance is made (into the table) at that year, month and day,
and the mean motions of the planets are reckoned and their apogees extracted. The
proper motions and those mean motions are corrected with the difference of the two
longitudes in the way described (7.1). And the apogee of each planet is subtracted
from its mean motion. The result is called the center^. All these things extracted
have one name-the base of the beginning of the year. All these things are set down
for the beginning of the month Farwardin according to the Sultanic calendar - each
in its own place just as it was arranged - and in the table which was (made) for this
purpose.
Mention must be made of how many tables are necessary. Five tables were set
down for the epochs and the days of the week, two tables for the center and the true
longitude of the Sun, five tables for the Moon and its mean motion and its proper
motion and the center and the true longitude of the descending node.
Each of the 5 planets has three tables: one for the center, one for the proper
motion, and one for the true longitude. Other tables have been set down: one for
the declination of the Sun, one for the latitude of the Moon, and five for the latitudes
of the planets. Two others were set down for the hours of rising.
When all the completed tables have been set down, this base — the mean and
proper motion and the rest — is written down for the beginning of the month Far-
^Neugebauer p. 10 under xevxpov
89
wardln. Then entrance is made into the table of the motion of the seven planets and
of the descending node for the months of the Sultanic year of the Sun. The motion
of the planets is reckoned opposite each month. Whatever is found of the motion of
the planets is always added to that base of the planets — the motion of the Sun to
the base of the Sun's true longitude and so on.
The beginning of each month from Farwardln until the end (of the year) is placed
at the beginning of each leaf. The number for the motions of the planets resulting
opposite each month is always added to the base of that planet. That which is found
is placed at the beginning of the true longitude. Then entrance is (made) into the
tables of days. The number for one day is reckoned from two, the number for five
days is reckoned from six, the number for ten days is reckoned from eleven, and the
number for 15 days is reckoned from 16. Each one is added to the base of each
month, and the number for that day of that month is written down.
When one is comfortable with the calculation of the mean motion from the
months and the days, then each true position of that planet in longitude and lati-
tude is extracted. The (number) of the mean motion is written in the table of true
longitude. When this has occurred, the number for the true longitude is divided for
each day with the help of God.
90
91
BOOK 8
On the True Position of the Planets in Longitude
and Latitude and on Some Other Things of those
Planets whose True Position is Extracted in Lon-
gitude: the Sun and the Moon and their Velocities
More or Less, for the Knowledge of their Diameter
and the True Longitude of the Descending Node
and the True Longitude of the Five Planets, and
for the Knowledge of the Direct and Retrograde
Motion of the Planets; and of those Planets whose
True Position is Extracted in Latitude — the Moon
and the 5 Planets — whose Latitude is Extracted
to the North or to the South
All these things, having been examined, were written in the tables of the corrections
of the planets. Two columns have been set up opposite these at the beginning of the
92
tables. The name measure was given to these two (columns). The calculation of the
complete circle (or sphere) was set down there.
The first column is for the calculation of the zodiacal signs from zero through
the fifth zodiacal sign, and there is the calculation of the degrees from to 180. The
number(s) in the second column (go) in reverse, being made from the bottom to the
top. The beginning of this is from the six zodiacal sign through Aries, through which
the reckoning of the entire sphere is completed. With the calculation of the degrees,
the beginning is from 181 up to 360 degrees for this calculation of the sphere.
There is another calculation if the calculation is in zodiacal signs, from the begin-
ning of nine zodiacal signs with their arrangement through zero (namely Aries) and
the beginning of three (zodiacal signs). This is called the upper half of the sphere,
with the calculations of the degrees from 270 to 360 and up to 90. This is called the
lower half of the sphere, from three zodiacal signs through six zodiacal signs and the
beginning of nine. With the calculations of degrees, (this is) from 90 degrees to 180
and up to 270 degrees.
This book is divided into 4 chapters.
8.1 On the Knowledge of the True Longitude of
the Sun, the Moon, the Five Planets and of
the Descending Node
This chapter is divided into 4 (sections).
8.1.1 On the True Longitude of the Sun
When we wish to calculate the true longitude of the Sun, we do as follows: The mean
motion of the Sun is set down in two places on the tablet, and the apogee of the
Sun is subtracted from one place of the mean motion. The result is the argument
93
of the Sun. Entrance is made into the table of corrections of the Sun opposite that
argument, and this argument is sought in the two tables of the first and second
column. The correction is reckoned opposite this (place) where it is found in the
third column, and the difference (2.1) is reckoned from the fourth column. These two
(values) are placed on the tablet. If the argument has minutes with the calculation
of the two tables, the computation of the correction is rectified, and the correction
becomes complete.
Then an examination is made. If the argument is in the first column, the correc-
tion is subtracted from the mean motion. If it is in the second column, the correction
is added to the mean motion, and the true longitude of the Sun is found. If the cor-
rection is subtracted from the argument or added to it, then the complete apogee
is added to the argument found later more or less by addition or subtraction, and
again that is the true longitude of the Sun.
8.1.2 On the True Longitude of the Moon
The mean motion, the proper motion, and the argument of the Moon are placed on
the tablet, as well as the mean motion of the ascending node - everything in its own
place. Then entrance is made into the tables of corrections of the Moon opposite
the argument, and the argument is sought there in the first and second column.
Entrance is made into the third column where it is found opposite this, and the first
correction of the Moon^ is reckoned with the number between the two tables.
Then an examination is made. If the argument is found in the first column, the
first correction is added to the proper motion. If it is found in the second column,
it is subtracted from that, and the final proper motion is found.
This is examined. Then entrance is made into the table of the fourth column
opposite the argument, and the proportional parts are reckoned and are placed in
^Neugebauer p. 14 under 6p6coaL^ TipcoTir]
94
one section of the tablet^. Then entrance is made into the table of corrections of
the Moon opposite the final proper motion, and the proper motion is sought in the
first and second columns of the argument. Entrance is made into the table of the
fifth column opposite the place where this is found, and the second correction of the
Moon is reckoned with this number found between the two tables, and is placed in
one section of the tablet. This is not the final correction.
Then entrance is made into the table of corrections of the Moon in the first and
second column opposite the final proper motion. Entrance is made into the table of
the sixth column opposite that (place) where this is found. The nearer^ distance is
reckoned — degrees and minutes. It is divided by the proportional parts. The result
is always added to the second correction, and the second correction becomes final.
Then an examination is made. If the final proper motion is found in the first
column, this second final correction is subtracted from the mean motion. If it is
found in the second column, it is added to the mean motion, and the true longitude
of the second sphere of the Moon is found.
If we wish to calculate the true longitude of the first sphere of the Moon, the mean
motion of the descending node is added to the true longitude of the Moon. The result
is the portion of latitude^ of the Moon. If the true longitude of the descending node
is subtracted from the true longitude of the Moon, the result again is the portion of
latitude of the Moon. Then entrance is made into the table of the corrections of the
Moon opposite this, and it is sought in the second column. Entrance is made into the
table of the seventh column of the Moon opposite that (place) where it is found, and
the minutes of the third correction of the Moon are sought and reckoned. Then the
^See Neugebauer pp. 19-20 for the procedure.
^Neugebauer p. 12 under \ifixoc, eyyuTspov
^Neugebauer p. 15 under TiXdioc;. The argument of latitude is "the distance from the ascending
node to the Moon" .
95
portion of latitude of the Moon is examined. If it is less than three zodiacal signs,
more than six zodiacal signs, and less than nine zodiacal signs, the third correction
is subtracted from the true longitude of the second sphere of the Moon. If it is it
greater than three zodiacal signs, less than six, or more than nine zodiacal signs, this
third correction is added to the true longitude of the Moon, and becomes the true
longitude of the first sphere of the Moon. This first sphere of the Moon is ''correct"
together with the sphere of the twelve zodiacal signs.
8.1.3 On the True Longitude of the Descending Node and
the Ascending Node
After the extraction of the mean motion of the descending node in the way described,
it is subtracted from twelve zodiacal signs. The result is the true longitude of the
descending node. Six zodiacal signs are added to this, and it becomes the true
longitude of the ascending node.
8.1.4 On the Knowledge of the True Longitude of the Five
Planets
The mean motion, the proper motion and the apogee of the planet are placed on
the tablet, each in its own (place). The apogee is always subtracted from the mean
motion, and the argument is found.
Then the argument is sought in the first or the second column of the measure^
in the tables of planetary equations. Entrance is made into the table of the third
column opposite the place where it is found. And the first equation is reckoned in
degrees and seconds with the calculation of what is found between the 2 tables.
Then the argument is examined. If it is in the first column, the first equation is
^ See p.92
96
added to the proper motion and subtracted from the argument. If the argument is
in the second column, the first equation is added to the argument and subtracted
from the proper motion. And the two (equations) become final. Then entrance
is made into the table of the fourth column opposite the the final argument, and
the proportional parts are reckoned. If they are written in red, there is an excess,
if in black, a deficiency. These (proportional parts) are placed in one part of the
tablet. Then entrance is made into the first and second column in the tables of
equations opposite the final proper (motion). Entrance is made into the table of the
sixth column opposite the (place) where this is found. And the second equation is
reckoned — in degrees and minutes — and the computation between the 2 tables.
This is not the final equation.
Once again entrance is made (into the table) opposite the final proper motion.
If the proportional parts are in excess, (the entrance) is opposite the table of the
sixth column, and the nearer distance^ is reckoned. But if the proportional parts
are a deficiency, entrance is made into the table of the fifth column, and the further
distance'' is reckoned. The result is always multiplied by the proportional parts.
That result, if the proportional parts are in red, is added to the second equation.
If they are in black, they are subtracted from it, and the second equation becomes
final.
Then an examination is made. If the final proper (motion) is in the first column,
the final second equation is added to the final argument. If it is found in the second
column, it is subtracted from it. Then the apogee is always added to this result,
and the true longitude of the planet is found. This same method is used for the
remaining planets.
^Neugebauer p. 12 under \ifixoc, eyyuTspov
^Neugebauer p. 12 under \ifixoc, £TiL^ir]X£aT£pov
97
8.2 On the Direct and Retrograde Motion of the
Planets
When it is necessary to know this, entrance is made into the tables of equation for
the planet in the first or second column opposite the final argument of that planet.
Entrance is made into the table of the eight column opposite the place where this
is found, and the first station is reckoned and kept aside. Then this (result) is
subtracted from twelve zodiacal signs and becomes the second station. Then the
final proper motion is examined. If it is equal to the first station, the planet is
standing still, that is, is stationary. It is then about to retrograde. If the final
proper motion is greater than the first station and less than the second station, the
planet is retrograde. If this final proper motion is opposite (i.e., equal to) the second
station, the planet is stationary and is about to move directly. If it is greater than
the second station and less than the first, the planet moves directly.
8.2.1 On Knowing When a Planet Moves Directly and When
it Retrogrades
If the planet moves directly and we wish to know when it turns, the final proper
motion is subtracted from the first station. The result is divided by the proper
motion of the planet in a nychthemeron. The result is the time when the planet
begins to retrograde. If we wish to know for how many days the planet moves
directly, the second station is subtracted from the final proper motion. The result
is divided by the proper motion of the planet which it moves in one nychthemeron.
The result is the time, for as many days as the planet moves directly.
98
8.2.2
If the planet is retrograde and it is sought when it will move directly, the final proper
motion is subtracted from the second station. The result is divided by the proper
motion which the planet moves in a nychthemeron. The result is the time when
the planet will move directly after this (station) is completed. If you wish to know
for how many days the planet is retrograde, the first station is subtracted from the
final proper motion. The result is divided by what has been frequently mentioned^.
The result is the time when the planet is retrograde. That proper motion of the
planet moving in a nychthemeron (is as follows:) Saturn 0;57, Jupiter 0;54, Mars
0;28, Venus 0;37, Mercury 3;6.
8.3 On the Northern and Southern Latitude of
the Planets
This is divided into three (sections).
8.3.1 On the Latitude of the Moon
The true longitude of the ascending node is subtracted from the true longitude of the
Moon, and the portion of the latitude is the remainder, or the mean motion of the
ascending node is added to the true longitude of the Moon, and the portion of the
latitude becomes clear. Then entrance is made into the tables of the correction of
the Moon in the first and second column opposite the portion of latitude. Entrance
is made into the table of the ninth column opposite (the place) where the portion
of latitude is found, and the latitude of the Moon is reckoned with the computation
found between the two tables. Then the portion of the latitude is examined. If it
^i.e., the proper motion of the planet in a nychthemeron.
99
is in the first column, the latitude is northern. If it is in the second (column), the
latitude is southern. If it is from zero to three zodiacal signs, there is northerly
ascent. If it is from three to six zodiacal signs, northerly descent. If it is from six
to nine zodiacal signs, southerly descent. If it is from nine zodiacal signs to zero,
southerly ascent.
8.3.2 On the Latitude of the Planets above the Sun - Saturn,
Jupiter and Mars
The final argument is sought in the tables of the equations of the planets in the first
and second column for Saturn and Jupiter. If the argument is found in the first
column, entrance is made opposite the ninth column, and the proportional parts are
reckoned. If the argument is found in the second column, entrance is made opposite
the table of the tenth column, and the proportional parts are reckoned. Then an
examination is made. If the proportional parts are in red, the latitude is northern.
If they are in black, the latitude is southern. This (result) is placed seperately in one
part of the tablet. Then the final proper motion is sought in the the tables of the
equations in the first and second column. Entrance is made opposite that (place)
where it is found, and the latitude is reckoned, southern or northern.
In the case of Mars, entrance is made into the table of the ninth column opposite
the final argument and the proportional parts are reckoned. If they are in red, the
latitude is northern. If they are in black, the latitude is southern. Then entrance
is made opposite the final proper (argument). If the proportional parts are in red
in the table of the tenth column, the northern latitude is reckoned . If they are in
black in the table of the eleventh column, thence the southern latitude is reckoned.
Then the proportional parts are multiplied by the latitude, and the final latitude,
whether southern or northern, is discovered.
If it must become clear whether it is an ascent or descent, an examination is
100
made. If the final proper argument is less than six zodiacal signs and the latitude is
northern, it is a northern ascent. If the latitude is southern, it is a southern descent.
If the final proper argument is greater than six zodiacal signs and the latitude is
northern, it is a northern descent. If the latitude is southern, it is a southern ascent.
8.3.3 On the Latitude of Venus
This (planet) has three latitudes.
First Latitude
Entrance is made into the tables of Venus in the way mentioned earlier. Entrance is
made into the table of the thirteenth column opposite the final argument, and the
fractional parts of the latitude are reckoned. This latitude is always northern. (The
fractional parts), (placed) in one part of the tablet, are examined.
Second Latitude
Entrance is made into the tables of the ninth column opposite the final proper
(motion), and the proportional parts are reckoned and, (placed) in one part of the
tablet, are examined. The sign^ of this is reckoned as follows:
If the argument is in the first column, the sign is one. If the argument is in the
second column, the sign is two. That sign is reckoned. Then entrance is made into
the table of the tenth column opposite the final proper (motion), and the latitude is
reckoned.
Then this is reckoned thus:
If the proper (argument) is in the upper hemisphere, its sign is one. If it is in
the lower hemisphere, its sign is two. This sign is reckoned. Then the latitude is
multiplied by the proportional parts reckoned in this (way), and the final latitude is
^See Neugebauer under arj^SLOv, p. 15 and his appendix 8.
101
found, kept aside, and examined. Then if the two signs are two and two^ or the two
(signs) are one and one, the latitude is northern. If one (sign) is two and the other
(sign is) one, the latitude is southern.
Third Latitude
As for the third (latitude), entrance is made into the table of the eleventh column
opposite the final argument, and the proportional parts are reckoned. If it is in the
upper hemisphere, its sign is one. If it is in the lower hemisphere, (its sign) is two.
These are examined. Then entrance is made into the table of the twelfth column
opposite the final proper (motion), and the latitude is reckoned. Its sign is this: if
the proper (motion) is in the first column, (the sign) is one. If it is in the second
column, (the sign) is two. Then its latitude is multiplied by its proportional parts.
The final latitude is found. Then an examination is made. If the two signs are equal,
the latitude is northern. If the two signs are not equal, the latitude is southern.
Then the three latitudes are placed each in its own place on the tablet. If the
three are northern, then the three are added together, and the latitude of Venus
is then found. If one latitude is southern, and another northern, the northern and
the southern are reckoned separately. Then an examination is made. The smaller
is subtracted from the larger. The result is the latitude of Venus in the direction
where the latitude was greater. If the two are equal, (one) northern (and the other)
southern, Venus has no latitude.
8.3.4 On the Latitude of Mercury
This (planet) has three latitudes.
102
First latitude
Entrance is made into the table of the equations of Mercury opposite the final argu-
ment. Entrance is made into the table of the thirteenth column opposite that (place)
where in either the first or the second column it is found, and the proportional parts
of the latitude are reckoned and kept aside. These are always in a southern direction.
Second latitude
Entrance is made into the table of the ninth column opposite the final argument, and
the proportional parts are reckoned and examined. This is its sign: if the argument
is in the first column, (its sign is) two. If it is in the second column, (its sign is)
one. These are examined. Then entrance is made into the table of the tenth column
opposite the final (proper) motion, and the latitude is reckoned. Its sign is this: if
the proper (motion) is in the upper hemisphere, (its sign is) one. If it is in the lower
hemisphere, (its sign is) two. Then the latitude is multiplied by its proportional
parts, and the final latitude is found.
Then an examination is made. If the two signs are equal, the latitude is northern.
If they are not equal, the latitude is southern.
Third Latitude
Entrance is again made opposite the final argument into the table of the eleventh
column, and the proportional parts are reckoned. Its sign is this: if (it) is in the
upper hemisphere, (its sign is) one. If the argument is in the lower hemisphere, (its
sign is) two. These are reckoned. Then according to two, entrance is made into
the table of the twelfth column opposite the final proper (argument), and the third
latitude of Mercury is reckoned. This latitude is called ''not final".
When it is necessary to know its correction, that latitude is set down in two
places, and the one is examined. The other is multiplied by six minutes. The result
103
is the correction of the latitude. Then an examination is made. If the final argument
of Mercury is in the upper hemisphere, this correction is subtracted from the third
latitude which was examined. If (it) is in the lower hemisphere, (it) is added to this,
and the latitude becomes final for this equation.
This latitude is examined. Then an examination is made. If the proper (motion)
is in the first column, its sign is two. If it is in the second column, (its sign) is one.
Then this latitude is multiplied by its proportional parts, and the final latitude is
found.
Then an examination is made. If the two signs are equal, the latitude is northern.
If they are not equal, the latitude is southern. Again the three latitudes are placed
separately on the tablet and examined. If the three (latitudes) are southern, the
three are added together, and the final latitude of Mercury is found in the southern
direction. If one is in the northern direction and one is to the south, the smaller is
subtracted from the larger, and the latitude of Mercury is found in the greater direc-
tion. If the northern and the southern (latitudes) are equal. Mercury is completely
without latitude.
When it is necessary to know the ascent and descent of Venus and of Mercury
in latitude, their latitude is extracted for one time. Then after the passing of a
suflBcient (number of) days from that day, once again their latitude is extracted. If
the (initial) latitude is northern and the extracted latitude is greater, there is an
ascent of the latitude. If it is less, there is a descent. If the latitude is southern and
what is extracted for the second is greater, there is descent. If it is less, there is an
ascent. If the latitude extracted first is northern and that extracted afterwards is
southern, the star is of a northern descent. If that extracted first is southern and
the second is northern, there is a southern ascent.
104
8.4 On the Knowledge of the Velocity of the Sun
and the Moon, the Diameters of them with
Calculation and through Tables
The motion of the planets in true longitude from the mid-day of a day until the next
mid-day of a day is called the velocity. If it is necessary to know the velocity of the
planet for one hour, this velocity of the planet is divided by 24.
8.4.1 [Solar Diameter ]
When it is necessary to know the diameter of the Sun for an eclipse, its velocity is
divided by 58. The result is divided by 105, that is, by 1 degree and 45 minutes. The
result is the diameter of the Sun. Alternatively, the velocity of the Sun for one hour
is divided by 53 minutes. The result is divided by four, and becomes the diameter
of the Sun.
8.4.2 For the Moon
When it is necessary to know the diameter of the Moon for an eclipse, its velocity is
multiplied by five. The result is divided by 121 or 2 degrees and one minute, and it
becomes the diameter of the Moon.
If we wish to come to a knowledege of the diameter of the shadow from its
diameter, the diameter of the Moon is multiplied by thirteen. The result is divided
by five, and the diameter of the shadow is found. This is useful for an eclipse of the
Moon.
105
8.4.3 For Knowing the Velocity of the Sun and the Moon
and their Diameter from the Table in the Case of the
Sun
Entrance is made into the table of the velocity of the Sun and the Moon and the
diameter and the shadow opposite its (the Sun's) argument, and that argument
is sought there in the table of the measures^^. The velocity of the Sun for one
nychthemeron and one hour is reckoned opposite that (place) where it is found, and
its diameter with the correction of the shadow, and each is set down separately.
There is no need for further work. In the case of the Moon, entrance is made into
such a table opposite the proper motion of the Moon. The velocity of the Moon for
one nychthemeron and for one hour is reckoned opposite that (place) where it is
found in the table of measures, and its diameter with the shadow, and all are set
aside. Then the correction of that shadow is subtracted from the diameter of the
shadow. The result is the final diameter of the shadow.
10
See page p. 92
BOOK 9
On Knowing the More and Less of
Vision
It is sought for this with so many calculations through this art with number and
through tables. This (book) is divided into three chapters.
9.1 On these so Many Calculations
This (chapter) is divided into five sections.
9.1.1 On Knowing the Altitude of the Location of the Poles
of the Sphere of the Zodiacal Signs, namely, the Poles
of the Axis around which the Sphere Rotates
The calculation of this is as follows: the Sine of the altitude of the tenth house of the
''fortune" of the house is divided by the Sine of the arc of that which is between the
tenth house and the ''fortune" of the house. The result is lowered by one step, and
the completed Sine of the altitude of the location of the poles of the axis is found.
Its arc of that is taken, and this is subtracted from 90. The result is the altitude of
106
107
the location of the poles.
9.1.2 On the Altitude of Whatever Degree We Wish and the
Altitude of the Moon when it has no Latitude
The calculation is as follows: the Sine of the distance of that which is between the
''fortune" of the house and the degree we wish is multiplied by the Sine of the arc
of that which is between the ''fortune" and the tenth house. The result is the Sine
of the altitude of the degree we wish.
9.1.3 On Knowing the Three Angles from the More and Less
of Vision
It is thus concerning the first angle: if the Moon is in the first degree of the "fortune"
and the "fortune" of the house is 6;0,0, the altitude is zero of Cancer on the circle of
mid-day. The completed angle of the distance^ is for 90, and this is the angle of the
latitude. If the "fortune" of the house is 0;0 — zero degree of Aries, the altitude is
at zero of Capricorn on the circle of mid-day. The completed angle of the distance
is for 90, and this is the angle of the latitude. If the "fortune" of the hosue is not
at zero of Aries or Libra, the altitude of the location of the poles is the completed
angle of the latitude, and this is the angle of the distance.
It is this concerning the second angle: that the Moon is in the degree of the tenth
house at the beginning of Aries or Libra at the declination of the whole distance,
when the completed angle of latitude ... the angle. If the Moon is at the beginning
of Cancer or Capricorn, there is no angle of the distance there. If the Moon is not
in (any of) these four places, the beginning of Aries or Libra is examined, how near
^Neugebauer p. 7 under ycovta has for angle of distance — ycovta toO ^rjxou^ — ''angle between
the circle of altitude and the circle of latitude" .
108
it is to the tenth house. And the distance between either Aries or Libra and the
tenth house is reckoned with the straight degrees of the zodiacal sign(s), and again
the distance^ of the ''fortune" with the straight line is reckoned. Then the Sine of
the two distances is reckoned. Then the Sine of the place of ''fortune" is divided by
the Sine of the distances. The result is lowered by one step. The result is a Sine. Its
arc is taken. The result is the angle of the latitude, and its complement is the angle
of the distance.
Concerning the third angle: If the Moon is not at the "fortune" or at the tenth
house, or between the "fortune" and the tenth house, or between the tenth house and
the seventh house, the Sine of the altitude of the location of the poles is reckoned.
That is divided by the Sine of the completed altitude of the Moon. The result is
lowered by one step. The result is a Sine. Its arc is reckoned. The result is the angle
of the latitude. And this as the completed angle of latitude.
9.1.4 For Knowing the More and Less of Vision for the Cir-
cle of Altitude, which is Necessary for the Eclipse of
the Sun, with the Table
A table is set down for the more and less of vision for the Sun and the Moon.
Entrance is made into that table opposite the completed altitude^ of the Sun and
the Moon, and the more and less of vision is reckoned — in the case of the Sun from
the second column, and in the case of the Moon from the third and fourth column.
Everything is placed on the tablet. Then entrance is made into the table of the
velocity of the Sun and Moon opposite the proper (motion) of the Moon or opposite
the velocity of the Moon. The minutes of the true longitude are reckoned opposite
^This use of \ifixoc, for totio^ is noted by Neugebauer on p. 17 under totio^.
^Neugebauer p. 16 under TSTsXeLCO^evr] dvdpaatc;
109
this. These are multiplied by the number coming from the fourth column. This
result is added to the number coming from the third column. The result is the more
or less of vision of the Moon for the circle of altitude.
Then the more or less of the Sun is subtracted from the more or less of vision
of the Moon, and the reminder is the completed more or less of vision of the Moon,
which is necessary for an eclipse of the Sun.
9.1.5 On the More and Less of Vision of the Moon with
Calculation in Longitude and Latitude
The Sine of each (i.e., the angle of the longitude and of the latitude) is multiplied
separately by the Sine of the more and less of vision of the Moon (on) the circle of
altitude. What is found is lowered by one step and the result is the Sine of the more
and less of vision. Its arc is reckoned, and the ikhtildf manzar^ i.e., the more and
less of vision, is found. If the Sine is of the angle of the longitude, this is for the
longitude. If it is that of the latitude, this is for the latitude.
9.2 On the More and Less of Vision for the Lon-
gitude and the Latitude by Means of a Table,
which is Easier
Know that Theon of Alexandria set down a table for the seven klimata in increments
of half an hour with this calculation when the Moon is at the beginning of each
zodiacal sign. This calculation set out by him was thus: that the more and less of
vision of the Sun is subtracted from the more and less of vision. This calculation is
for an eclipse of the Sun only.
If there is need of another calculation of the Moon, not through an eclipse, each
no
of those things — the more and less of vision of the longitude and the latitude —
is multiplied by eighteen, and the result is divided by seventeen. The location of
the Moon, namely the true longitude, is corrected by that which comes out from
the longitude or the latitude. This more and less of vision of the Moon is reckoned
opposite the hour of the distance from mid-day^. Once entrance is made in the tables
of more and less of vision, that hour^ of distance ought to be taken first. The hour of
that day when the Sun is about to be eclipsed is reckoned and placed on the tablet.
Then the hour of conjunction is also placed on the tablet. The larger of the two is
examined, and the smaller is subtracted from the larger. The result is the hour of
distance. This is examined. If the hour of mid-day is larger, the hour of distance
is before mid-day. If the hour of mid-day is smaller, the hour of distance is after
mid-day.
9.2.1 On the More and Less of Vision of the Moon in Longi-
tude and Latitude with the Calculation of the Latitude
of the City
When there is need for (this) calculation, the table is sought from among the tables
of the more and less of vision so that the latitude of the table is equal to the latitude
of the city. Whatever table is found, the zodiacal sign in which the Moon is is sought
in that table. The hours of distance are sought by depth opposite the table of that
zodiacal sign. If the hour is before mid-day, the hours of distance are sought in the
part of the table above mid-day. If (they are) after mid-day, in the part below. If the
hour is mid-day, entrance is made from this. The more and less of vision in longitude
and latitude is reckoned opposite that (place) where the hour of distance is found.
^Neugebauer p. 12 under wpa toO ^rjxou^
^Neugebauer p. 18 under wpa
Ill
If the hour has minutes, this becomes final with calculation between the two tables.
9.2.2 Very Useful (Things) for the More and Less of Visi-
bihty
If one forgets, it is as follows: these marks o o o are placed between the hour with
which entrance was made into the table and the (hour) following it. Wherever these
marks are found between the two numbers, the diflFerence (of the two numbers) is
not reckoned, but the two numbers are reckoned, added and placed on the tablet in
two places. The (value in) one place is kept aside, and the other is multiplied by the
minutes of the distance of that first hour (up till) mid-day or after mid-day. The
result is examined. If it is equal to the part set aside, it is clear that there is no more
and less of visibility. If it is not equal, the diflFerence between the two is extracted,
namely, the smaller is subtracted from the larger. The result is the more and less of
visibility in longitude.
9.2.3 On the Correction for the Degrees of the Zodiacal
Signs
If the Moon is at the beginning of a zodiacal sign, if anything is found opposite
the zodiacal sign in the table of more and less of visibility, that more and less of
visibility is not final. So when there is need for this (parallax of the zodiacal sign)
to be corrected with the (parallax of the) zodiacal sign after it, the more and less
of visibility is reckoned opposite that (second zodiacal sign). Then the diflFerence
between the two more and lesses of visibility of the middles of the two zodiacal signs
is reckoned. That diflFerence is multiplied by the degrees of the Moon and the result
is divided by 30. The result is the correction. Then, from these two more and lesses
of visibility between the two zodiacal signs, if the more and less of visibility from
the first zodiacal sign is greater than the second more and less, this correction is
112
subtracted from it. If it is less, the correction is added to it.
9.2.4 On the Correction for the Two Latitudes
If the latitude in the table of more and less of visibility is equal to the latitude of
the city we wish, the number is reckoned from this table. If the latitude in the table
is not equal to the latitude of the city, the (greatest) latitude less than that of the
city and nearer to it is sought in the table. Then one seeks another latitude in the
table greater than the first latitude. The difference between the two latitudes —
the larger and the smaller — is reckoned. Then the difference between the latitude
of the city and the smaller latitude in the table is reckoned and multiplied by that
difference. The result is divided by the difference of the two latitudes in the tables.
The result is the correction. Then of the two latitudes reckoned in the table — the
latitudes from which that difference was reckoned — if the value of the first latitude
is greater than the second, the correction is subtracted from the first latitude. If the
(value of the) first is less than the second, the correction is added to it, and so the
more and less of visibility is found. This value is (the time) when the Moon is at the
apogee of its small epicycle.
9.2.5 On the Correction for the More and Less of Visibihty
with the Location of the Moon
Entrance is made into the table of the velocity, diameter, and shadow of the Sun and
the Moon. Entrance is made into the tables of the proper (motion) or the altitude
of the Moon opposite the proper (motion) or altitude of the Moon, and the minutes
found in the table of the more and less for the proper (motion) of the Moon are
reckoned opposite this. The more and less of visibility in longitude and latitude are
multiplied by this result. The result is the complete more and less of visibility. This
is set aside for an eclipse of the Sun.
113
9.3 On the Reliable Method for the Location of
the Moon in Longitude and Latitude
If there is need for this calculation, an examination is made. If the distance of the
Moon from the ''fortune" is less than 90 degrees, the more and less of visibility in
longitude is added to the true longitude of the Moon. If (the lunar distance from
the ascendant) is greater (than 90 degrees), (the longitudinal parallax) is subtracted
from the true longitude. The result is the place of the sighting of the Moon.
9.3.1 Concerning the Solid Calculation of the Place of the
Moon in Longitude
Before making this calculation, it is necessary to know whether the more and less
of visibility is northerly or southerly. This is apprehended from the rising of the
tenth house from the ''fortune" for the (given) moment^ as follows: if the rising of
the tenth house over our heads is southerly, the more and less of visibility for the
latitude is southerly. If (the rising) is northerly, (the parallax) is northerly.
Alternatively, the same thing (is arrived at) through a different method. The
latitude of the city we wish is examined. If (the latitude) is greater than the dec-
lination, the more and less of visibility for the latitude is always southerly. If the
latitude of the city is such that the whole declination when added to the latitude
of the Moon is equal to the latitude of the city, the more and less of visibility in
latitude is sometimes northerly and sometimes southerly. For whatever city this is
true, the more and less of visibility in latitude (for that city) and the latitude of the
Moon are examined. If it is the case that they are both northerly or southerly, the
two are added. If one is northerly and the other southerly, the smaller is subtracted
from the larger. The result is called the latitude of the vision of the Moon, or the
^Neugebauer p. 17 under tuxtt] toO xaLpoO
114
solid latitude''. It is necessary for one wishing to compute the true longitude to make
tables for the more and less of visibility of the Moon for the latitude of the city for
which the true longitude was computed.
This is how we did this: the latitude of our city is 38 (degrees). We computed
this from the two tables from which the latitude of one was 36, and the latitude of
the other was 41.
^Neugebauer p. 28 appendix 9.
BOOK 10
On Conjunctions and Oppositions
of the Sun and Moon
These are computed via three calculations.
10.1 First Calculation: On the Conjunction of the
Sun and the Moon and Their Dianieter(s)
and the Distance of Their Motion
10.1.1 (Determination of the Hour)
The true longitude of the Sun and Moon are examined (to determine) the day they
come together in conjunction or opposition in one (and the same) zodiacal sign, one
degree and one minute. Once this is found, (the calculation) is at the middle of
that day, at conjunction or opposition, and at that degree in which the Sun is in
opposition to or in conjunction with the Moon.
If the true longitude(s) of the Sun and the Moon are not (found in the table)
opposite the middle of that day, two (consecutive) mid-days are sought such that at
115
116
one mid-day the true longitude of the Moon is less than the true longitude of the
Sun, and at the mid-day after that (the true longitude of the Moon) is greater than
the true longitude of the Sun. Then which mid-day is closer is investigated. At that
mid-day the distances of both the Sun and the Moon are reckoned and examined.
Then the velocity of each — the Sun and the Moon — is extracted for the two
mid-days. Then the velocity of the Sun is subtracted from the velocity of the Moon.
The result is called the complete velocity.^
Then the mean distance of the Sun and the Moon is multiplied by 24. The
result is divided by that complete velocity. This result is the hour of the distance^.
This result is kept aside. Then the true longitude (s) of the Sun and the Moon at
that mid-day are examined. If the true longitude of the Moon is less than the true
longitude of the Sun, the hour of the difference is added to the hour of mid-day.
If the result is less than the hours of that whole day^, that (resulting) hour is the
hour of the conjunction or the opposition on that day. If the result is found (to
be) greater than the hour(s) of the whole day, the hour(s) of the day are subtracted
from that. The result is the hour of the conjunction or opposition during the coming
night. If the true longitude of the Moon is greater than the true longitude of the
Sun, the hour of the difference is examined. If it is less than the hour of mid-day, it
is subtracted from that hour of mid-day. The result is the hour of the conjunction
or opposition during that day. If the hour of the difference is greater than the hour
of mid-day, the two are added together and the result is subtracted from 24. The
result is the hour of the conjunction or opposition during the following night.
In order for this computation to be precise, (it is made) for when the true longi-
tude (s) of the Sun and Moon are complete with the equation of the day. If they are
^Neugebauer p. 12 under ^exdpaaLc;
^Neugebauer p. 12 under \ifixoc,
^Neugebauer p. 18 under wpa xf]^ fj^epa^
117
not complete, entrance is (made) into the table of the equation of the days opposite
the true longitude of the Sun, and the equation of the day is reckoned for the minutes
and seconds of the hour. The result is always added to the hour of the conjunction
or opposition, and so the hour becomes complete.
10.1.2 (Variant)
If we wish to make this calculation easier, the true longitude (s) of the Sun and Moon
are calculated for that hour when the conjunction or opposition occurs. If both of
these are equal in degrees and minutes, that hour is correct. If they are not equal,
the difference between these (two longitudes) is reckoned, and is (treated) as was
said in the case of the first calculation (p. 115), so that the hour becomes correct.
10.1.3 On the Determination of That Degree in Which the
Sun and the Moon are in Conjunction or Opposition
That difference (in longitude) which was reckoned between the Sun and Moon is
placed in two (separate) places on the tablet. The one is merely examined and
the other is multiplied by five minutes. The result is the correction of the degree
(of longitude) of the Sun. It is examined separately, and is in turn added to the
distance merely examined. The result is the correction of the degree (of longitude)
of the Moon.
Then the true longitude(s) of the Sun and Moon, which were found for the middle
of that day, are placed on the tablet separately. The correction is placed under each
of these. Then an examination is made. If the true longitude of the Moon is less
than the true longitude of the Sun, the correction of the degree of the Moon is added
to its own true longitude, and in the same manner the correction (of the degree) of
the Sun is added to its true longitude. If the true longitude of the Moon is greater
than the true longitude of the Sun, the correction of each is subtracted from (their)
118
respective true longitude (s).
The result is examined. If they both are equal in degrees and minutes, the
calculation for the Moon is correct. If they are notequal, it is not correct. If the
calculation for the conjunction either in the day or the night is correct, that degree
is always one; that calculation is written down as for the true longitude. If the
opposition is in the day, the degree (of longitude) of the Sun is reckoned. (If it is at)
night, the degree (of longitude) of the Moon (is reckoned). If it is necessary that the
''fortune" for the conjunction or opposition be extracted, the calculation is carried
out in the fashion mentioned earlier.
10.2 Second Calculation. Concerning the Calcu-
lation of an Eclipse of the Moon both by
Computation and by a Table
This is divided into two chapters.
10.2.1 On Knowing Whether the Moon Will Be Eclipsed Or
Not by Computation
This is divided into five subsections.
10.2.1.1 Whether the Moon will be Eclipsed or Not
Here are such things as ought to be controlled. First, that the opposition of the
Sun and Moon should be at night or close enough to night so that there are two
hours or less between daytime and nighttime for the beginning and the totality of
the (eclipse) when the Sun is diametrically opposite the Moon. The second is that
that (the distance) between the lunar nodes and the degrees of the Moon should be
119
less than twelve, or if the latitude of the Moon is less than 63 minutes either to the
north or to the south, the eclipse occurs. If it is greater than these (minutes), it
is not eclipsed. If the Moon is going to be eclipsed, the hour of the conjunction is
called the hour of the middle of the eclipse.
10.2.1.2 On Knowing that the Moon is Going to be Eclipsed or not by
Calculation
When it is necessary to speak by calculation about an eclipse of the Moon, the
diameter (s) of the Sun and of the Moon as well as the shadow — these three are
extracted. Then the diameter of the Sun is added to the diameter of the Moon. The
result is divided by two. This result is called the half of the two diameters. This is
examined. Then the latitude of the Moon is examined for the hour of the opposition.
If this is greater than or equal to the half of the two diameters, the Moon will not
be eclipsed. If it is less, (the Moon) will be eclipsed.
10.2.1.3 On Knowing How Much of the Moon is Going to be Eclipsed,
a Part of it or All; and if a Part of it is Going to be Eclipsed,
How Many Digits, and if All (of it) will be Eclipsed, is it Going
to Delay in the Eclipse or Immediately Begin to Return Again
to its Original State
The latitude of the Moon is subtracted from half of the two diameters. The result is
called the parts of the eclipse. Then they are examined. If the parts of the eclipse of
the Moon are equal to the diameter of the Moon, the whole Moon will be eclipsed
and immediately turn back. If the parts of the eclipse are greater than the diameter
of the Moon, the whole Moon will be eclipsed and will remain for a little while in the
eclipse. If the parts of the eclipse are less than the diameter of the Moon, a small
(part) of the Moon will be eclipsed.
If it is necessary to know how much of the Moon will be eclipsed, the parts of the
120
eclipse of the Moon are multiplied by twelve. The result is divided by the diameter
of the Moon. The result is the (number of) digits of the diameter of the Moon out
of the 12 digits of its diameter.
10.2.1.4 On the Hour of the Eclipse of the Moon
The latitude of the Moon is multiplied by itself. For example, if the latitude is
25, it is multiplied by 25 and so the square of the latitude of the Moon is found.
This is subtracted from the half of the (two) diameters. The multiplication of this
result is reckoned. What is found is said to be the parts of the eclipse of the Moon.
These (parts) are multiplied by 24, and the result is divided by the complete motion
(10.1.1) of the Moon in a nychthemeron. The result is the hour which is called the
falling hour of the eclipse^.
Then the time of the opposition is written in three places on the tablet. The
falling hour is subtracted from the hour of the opposition set down previously on
the tablet, and it is added to the (hour) set down in the third place. The result in
the first (place) is the hour of the beginning of the eclipse of the Moon. The result
in the second place is the middle hour of the eclipse of the Moon. The result in the
third place is the hour of the complete return of the Moon. That is the calculation
at a time when a part of the Moon is eclipsed.
10.2.1.5 (Duration of Totality)
When the whole Moon is eclipsed, the diameter of the Moon is subtracted from half
of the two diameters. The square of the latitude of the Moon is then subtracted from
the square of this result. The multiplication (by itself) of the remainder results, and
so the fractions of the duration^ are found. These are multiplied by 24, and the
^Neugebauer p. 18 under c5pa Tf]c; Tieaouarjc;
^Pingree: axdatc; is evidently the half-duration
121
result is divided by the complete motion (of the Moon) in a nychthemeron. The
result is the hours of the duration.
Then the hour of the opposition is set down in five places. The falling hour is
subtracted from the first hour^ and added to the fifth. The hours of the duration
are subtracted from the second hour and added to the fourth.
The first place of the five is the beginning of the eclipse of the Moon, the second
is the hour of the beginning of totality'', the third is the hour of the middle of the
eclipse, the fourth is the the beginning of the return of the Moon^, and the fifth
place is the final hour at which the Moon returns.
Then the falling hours are doubled. The result is the hour from the beginning of
the eclipse of the Moon until the complete return.
10.2.2 On the Eclipse of the Moon by Means of Tables
10.2.2.1 (Magnitude)
The latitude of the Moon is extracted for the time of the opposition of the Sun and
Moon and kept aside. Then entrance is made into the table of the velocitie(s) of
the Sun and Moon. The fractional parts of the true longitude are reckoned opposite
the latitude and examined. Then once again entrance is made into the table of the
observation of the Sun opposite the aforementioned latitude of the Moon for the
closer distance in the three tables. The digits of the falling hour are reckoned. The
hour of the duration and the correction for each are kept aside separately. Then the
correction for eachis multiplied by the fractional parts of the true longitude. The
result is added to each of the corrections kept aside separately. The result is final.
Then the digits of the eclipse are examined. If they are greater than twelve, the
^Pingree: reading here as elsewhere wpa^ instead of ^OLpa^
'^Pingree: middle of the eclipse (xf]^ [leoric, ExXeii^EC^c,) is wrong
^Neugebauer p. 6 under dTioxaxdaTaaLc;
122
eclipse of the Moon is total and it remains for (some) time in the eclipse. If there
are (exactly) twelve digits, the whole Moon is eclipsed, but it does not remain in the
eclipse. If the digits are less than twelve, a part of the Moon in proportion to the
digits of the diameter is eclipsed.
It is necessary to know how much of the Moon is (eclipsed). Entrance is made
into the table of the diameter of the Moon. The number of digits of the surface^ of
the Moon is reckoned opposite the digits. The result is the (number of digits) from
the surface in digits of the entire Moon.
10.2.2.2 On Knowing the Time of the Eclipse of the Moon
It is in the same way as was described in the fourth and fifth sections of the first
chapter (10.2.1.4, 10.2.1.5).
10.2.2.3 On the Time of a Eclipse of the Moon if a Part of it is Eclipsed
at Night and a Part in Daytime
If the eclipse occurs during the daylight, if the hour of the eclipseof the Moon is
greater than the (length of) daylight, the hour of daylight is subtracted from that
(hour of the eclipse). The result is during the night. If a total eclipse occurs at night,
the hour at night of the eclipse is greater than the hour of night which is subtracted
from that. The result is the hour during the day.
10.3 Third Calculation. On the Eclipse of the Sun
This is divided into three chapters.
^twelfths of area
123
10.3.1 On Obtaining the Best and (Most) Proper Table for
the Echpses of the Sun
The calculation of the eclipse of the Sun with a table should be made to be easy
because if there is a lot of calculation, this will extend (it )in length and it will
be difficult to apprehend. We have set down this table at length for the sake of
clarity. Three calculations are set in it. The first calculation: they are the hours
of distance^^ before mid-day and after mid-day. The second: the more and less of
visibility for the longitude. The third: the more and less of visibility for the latitude.
The construction of this table is completed^^ in three sections.
10.3.1.1 On the Construction of the Table of the More and Less of Vis-
ibility for the Latitude of the City for which there is no Table
in this Composition
This table is made from two tables. One is that for a latitude less than that of
that city, and the other is for a latitude greater (than that of the given city). This
calculation was described earlier in the second chapter of the ninth book (9.2.4). We
have set down this table for a latitude of 38 degrees.
10.3.1.2 On the Extraction of the More and Less of Visibility for the
Degree (of Longitude) of the Sun and the Moon when They are
in Conjunction
When this degree is not at the beginning of a zodiacal sign, the calculation is made
with two zodiacal signs. This calculation was described in the ninth book in the
second chapter (9.2.3).
^^Neugebauer p. 12 under \ifixoc,
iipingree: read TiXrjpouTaL
124
10.3.1.3 On the Correction of the More and Less of Visibility for the
Position of the Moon, that is, for its Proper Motion on the
Small Circle
This calculation was described in the second chapter of the ninth book along with
the others (9.2.5).
We calculated this table for the entrance of the Sun at 25 degrees of Leo. This
calculation was between zero (degree) of Leo and zero (degree) of Virgo. The Sun
was eclipsed after mid-day. This is the reason the table was for after mid-day since
there was no need to calculate a table for the time before mid-day just as when an
eclipse occurs before mid-day there is no need to calculate a table for after mid-day
The latitude of the city was 38 (degrees). This was extracted from the tables of
their two latitudes, 36 (and) 41 (degrees). The result was multiplied by the fractional
parts of its more and less. This result has been set down in this table.
o
o
a;
o
a;
m
First: The Beginning of
Leo and Virgo
Second: 25 De-
grees of Leo
The More and Less of Vi-
sion of the Anomaly of the
Moon
Hours
At the Beginning of Leo
At the Beginning of Virgo
Hours
EasyTable
36
41
38
36
41
38
8
36
a;
T3
'5b
a
o
a;
a;
T3
4^
'5b
a
o
a;
T3
a;
T3
'5b
o
T3
4^
a;
T3
4^
'5b
sn
o
T3
a;
T3
'5b
a
o
4^
a;
T3
4^
'5b
a
o
a;
T3
'5b
o
4^
a;
T3
4^
'5b
sn
o
T3
4^
7
7
6
6
5
5
4
4
3
3
2
2
1
1
Noon
3
14
4
18
3
15
8
20
9
23
8
21
7
20
8
23
O
O
<
1
8
16
6
20
6
17
2
24
27
2
29
3
24
1
4
28
2
17
20
15
24
17
21
12
29
9
31
11
30
12
28
2
14
33
3
24
24
22
28
24
25
19
33
16
36
18
34
19
32
3
22
37
4
31
28
27
32
30
29
24
37
21
39
23
38
24
36
4
28
42
5
35
33
30
35
33
34
27
40
24
42
26
41
27
40
5
31
42
6
34
37
31
38
32
33
28
42
27
43
27
43
28
42
6
33
49
7
33
40
28
42
31
40
28
43
28
45
28
44
28
43
7
34
50
Half of the table was not
calculated because the
eclipse occurred before
noon
10.3.2 On the Calculation of an Eclipse of the Sun by Means
of both a Table and Calculation
This is divided into three sections.
125
(Method of Computation)
When there is need for this method, first the true longitude(s) of the Sun, the Moon
and the ascending node are (calculated) daily for one year. Then all the conjunctions
are extracted. Then a conjunction is sought which occurs during the day or near the
day by so much that there is less than one hour from it until day. The latitude of
the Moon is extracted for the hour of the conjunction. If the latitude of the Moon is
southerly, it should be less than 35 minutes. If it is northerly, it should be less than
93 minutes. The eclipse will take place in this (interval). If it is more than this, the
eclipse will not take place.
Before entering into this calculation, it is necessary first to mention what methods
should be used. First, it is necessary to know that conjunction in which an eclipse is
going to take place, then the hours until the conjunction, then the degree at which
the conjunction takes place. The true longitude of the ascending node is apprehended
for that time. Then the diameter of the Sun and the motion of the Sun in one hour
are determined. The diameter of the Moon and its motion in one hour are extracted.
Then the complete motion of the Moon in one hour is apprehended, as well as the
hour of mid-day ^^. All these are apprehended and examined. Then is reckoned the
''fortune" for that time when the conjunction of the Sun and Moon takes place. Then
the zodiacal sign, degrees and minutes of the conjunction of the Sun and the Moon
are subtracted from the ''fortune" for (that) time. The result is the longitude of the
conjunction in degrees. This is kept aside and examined.
If this longitude is 90 degrees, the extracted hour of the conjunction is the middle
hour of the eclipse. The degree in which the Sun is in conjunction with the Moon is
the location of the visibility of the Moon. In this case there is no need for the hour
of the conjunction to be precise.
If this longitude is less than 90 degrees, that degree in which the Sun is in
12
Neugebauer p. 18 under wpa toO \iEao\j xf]^ fj^epa^
126
conjunction with the Moon is towards the east. If (this) longitude is greater than
90, the degree of the conjunction is towards the west.
Between these two it is is necessary to correct that hour, (by a method) which is
(given) in three (sections).
10.3.2.1 On the Correction of the Hour of the Mid-Eclipse
This is done in two (ways) — by calculation and by table. The calculation requires
five things.
The first is the reckoning of the hour of the conjunction. The ''fortune", the
tenth house, and the altitude of the tenth house should be reckoned from that hour.
This is examined. The second is the apprehension of the altitude of the Moon. The
third is the knowing of the more and less of visibility of the Sun and the Moon in
the circle of altitude. Then the more and less of visibility of the Sun is subtracted
from the (that) of the Moon. The result is reckoned. The fourth is the apprehension
of the angle of latitude and longitude. The fifth is the apprehension of the more and
less of visibility of the Moon in longitude and latitude.
We do not (have) need of these five for this calculation. These five ought to be
treated methodically in three.
The Calculation of an Eclipse of the Sun through the Table
The hour of the conjunction is examined and the hour of mid-day. If these two hours
are equal numerically, entrance is made into the hourly table^^ opposite mid-day and
the more and less of visibility in longitude is calculated. If the hour of the conjunction
is less than the hour of mid-day, that (first) is subtracted from that hour. The result
is the hour of distance before mid-day. If the hour of the conjunction is greater than
the hour of mid-day, the hour of mid-day is subtracted from that. The result is the
13
Neugebauer p. 18 under (bpatov xavovLov
127
hour of distance after mid-day. Whether this is before mid-day or after mid-day, it
is called the hour of the first distance. Then entrance is (made) into the hourly table
opposite this hour, and the more and less of visibility in longitude, which is called
the first more and less of visibility, is reckoned. This more and less of visibility is
divided by the complete motion of the Moon in one hour. The result is the hour of
the first more and less of visibility. This hour is always added to the hour of the
first distance and the hour of the second distance is found. Then the more and less
of visibility in longitude is reckoned opposite that hour of the second distance, and
this, in turn, is divided by the complete motion of the Moon in one hour. The result
is the hour of the more and less of visibility at the second distance. This hour added
to that hour of mid-day. The result is the hour of the third distance. Once again
entrance is (made) into the hourly table opposite this hour. This calculation occurs
frequently in this manner — four and even six times — until two (consecutive) more
and lesses of of visibility which are reckoned are equal numerically^^. The last more
and less of visibility is final, and that hour of the last distance is final.
Then is reckoned the degree in which the Sun is in conjunction with the Moon.
If it is in the East, the more and less of visibility of the distance which resulted last
is subtracted from that degree. If the (degree of conjunction) is in the West, it is
added to it. The result is the location of the sighting of the Moon at the middle
of the eclipse. If that degree (of conjunction) is in the East, the hour of the final
distance is subtracted from the hour of mid-day. If (the degree of conjunction) is in
the West, it is added to it. The result is the hour of the mid-eclipse.
14
i.e., until convergence is achieved
128
10.3.2.2 On Knowing of Whether or Not an Eclipse Will Occur and, if
it will, How Great it will be
When we wish to make this calculation, the true longitude of the descending node
is always subtracted from the place of the sighting of the Moon, and the degree of
latitude of the Moon results. Entrance is (made) into the table opposite the degree
of this latitude of the Moon, and the latitude of the Moon is reckoned. This is called
the final latitude.
Then it is examined whether (this final latitude) is northerly or southerly. This
(result) is kept aside. Then entrance is (made) into the hourly table opposite that
hour of the final distance, and the more and less of visibility for the latitude is
reckoned and kept aside. Then it is examined whether (this) is northerly or southerly.
If the final latitude of the Moon with the more and less of visibility for the latitude
is northerly or southerly, the two are added together. If one is northerly and the
other southerly, the smaller is subtracted from the larger. The result is the solid
latitude of the Moon. This is examined. Then the diameter of the Sun is added to
the diameter of the Moon, and the result is divided by two. The result is called the
half of the two diameters (p. 119). This is placed on the tablet, and the solid latitude
of the Moon is placed near it and examined. If the solid latitude of the Moon is equal
to the half of the two diameters or is greater than it, the eclipse does not occur. If
it is less, an eclipse occurs.
Then if it is necessary to know how much of the Sun will be eclipsed, that solid
latitude is subtracted from the half of the two diameters. The result is called the
fractional parts of the eclipse. Then an examination is made. If these fractional
parts of the eclipse are equal to the half of the two diameters, the eclipse of the
Sun is total. If the fractional parts of the eclipse are less than the half of the two
diameters, a part of the Sun is eclipsed.
Then that total eclipse with the diameters of the Sun and Moon is examined. If
129
the two diameters are equal, the Sun will be totally eclipsed and it will not have any
duration in the eclipse. If the diameter of the Moon is greater, the whole Sun will
be eclipsed and it will remain a sufficient time in the eclipse. If the diameter of the
Sun is greater, the center of the Sun will be eclipsed, but the periphery will not.
Then that partial and not total eclipse is examined, how many digits from the
diameter of the Sun will be eclipsed with this calculation, since the complete diameter
of the Sun is 12 digits. When it is necessary for this calculation to take place, the
fractional parts of the eclipse discovered earlier are multiplied by twelve. The result
is divided by the diameter of the Sun, and so the digits of the eclipse are discovered
from the diameter of the Sun.
10.3.2.3 On How Much of the Sun will be Eclipsed and the Knowing of
the Time by Means of a Table
Once the hour of the mid-eclipse together with the the solid latitude of the Moon has
been extracted, entrance is (made) into the table of the motion of the Sun and Moon
opposite the (proper) motion of the Moon or its velocity. The fractional parts of the
true longitude are reckoned from that and kept aside. Then entrance is made into
the table of the eclipse of the Sun opposite the solid latitude of the Moon. The digits
and their correction are reckoned and the falling hour with its correction. Each is
examined individually. Then the fractional parts of the true longitude are multiplied
by the correction of each. The result is lowered by one (sexagesimal) step. This
result is always added to the digits and the (falling) hour, and so the digits and the
falling hour become final.
Then an examination is made. If the digits are 12 or more, the whole Sun will
be eclipsed. If they are less than twelve, the whole (Sun) will not be eclipsed.
Then it is examined how much of the twelve digits will be eclipsed. Then the
calculation is from this. Those digits are the diameter of the Sun.
130
If it is necessary to reckon^^ the digits of the surface of the Sun^^ (that will be
eclipsed), entrance is made into the table opposite the digits of the diameter of the
Sun, and the number found is reckoned as of the surface of the Sun in digits. These
are the digits of the eclipse. When the final falling hour was clear, the hour of the
mid-eclipse is set down in three places on the tablet. The falling hour is subtracted
from the first and added to the third, and so the times of the eclipse are discovered
in the way described earlier (see page 120).
^^Pingree: read xaTaXir]cp6f]vaL
^^Neugebauer p. 8 under SdxTuXoL
BOOK 11
On Understanding When the
Moon Becomes New and When
the Planets Appear after
Conjunction with the Sun
Our observations about the Moon will be discussed. This computation is very diffi-
cult because the ancients made no mention of it. Why did they say nothing? (They
said nothing) because the beginning of the months of the Moon were reckoned from
the moment there was (some) distance of the Moon from the Sun after conjunction
(and not from the sighting of the lunar crescent).
When the Persians, however, had need for this because of (their) feast, fast and
great days, their great days become clear through the sighting of the new Moon. We
have therefore set down in this book that which those astronomers^ set down in their
books, along with computation and by a table, and some other things necessary for
these, not from those calculations which someone might suppose are easy, and from
ipingree: He (C) means the Persians
131
132
those calculations which do not seem to turn away faith, but which are most useful
for this (topic). It is therefore difficult to find such a calculation in other books
because of the loftiness of this (topic).
One would not find in another how this calculation was set down in this book.
Why have I put such a marvelous calculation in this book? Because the months of
the Moon are reckoned by the Persians through sighting the apparent new Moon,
not through a middling calculation. Whoever wants the benefit of this calculation
should know that the vision of all men is not the same, and the new Moon does not
always appear at the same place, and in each city it is viewed one way or another.
If the person searching for the sighting of the new Moon does not understand how
and where to search for it, he will be left behind completely empty. He will have
so much difficulty in looking towards the sky that his vision will be blinded, so that
even when the Moon does appear to all, he will not be able to see it before it sets.
In as much as the man is clever, with this calculation and understanding of the
altitude of the Moon at the time of its sighting and its point in heaven, it will appear
to him in one place as soon as he looks in the sky.
The method of this art is divided into five chapters.
11.1 On the Computations Necessary for this Method
This chapter is divided into eight (sections).
11.1.1 On the Apprehension of the True Longitude of the
Sun and Moon at that Time When the Degree of the
True Longitude of the Moon is Setting
Thus is the calculation: the motion of the Moon in one hour is apprehended and
subtracted from fifteen. The result is the fast motion of that hour. This is examined.
133
Then the true longitude of the Sun and Moon for mid-day of the 29th day in the
Arabic month is apprehended.
Then entrance is made into the table of the place of ''fortune" with a straight line
opposite each true longitude, and the number discovered for the place of ''fortune" of
each with the straight line is reckoned. Then the difference of each place of "fortune"
is examined and added to half the arc of the day^. The result is divided by the fast
motion. The result is the hour between (the middle) of that day and the setting of
the degree of the Moon.
Then the motion of the Sun and the Moon in one hour is sought and each (of
these) is multiplied by those hours (between) the middle of that day and the setting
(of the lunar degree). The result from the motion of each is added to the true
longitude of each for half of a day. The result is the true longitude of the Sun and
Moon for that hour when the degree of the Moon sets. The true longitude of the
descending node is extracted for that hour. Then when there is need to know the
true longitude of the Moon at the time of the setting of the Sun, the hour of mid-day
is multiplied by the motion of the Moon in one hour. The result is added to the true
longitude of the Moon at mid-day, and the true longitude of the Moon for the hour
when it sets is found.
11.1.2 On the Accurate Correction of the Location of the
Moon for the More and Less of Visibihty in Latitude
and Longitude
The location of the Moon is in the west when it sets. This is corrected. This is
an easy method arising from the tables of more and less of visibility along with the
fractional parts of the true longitude found in the table of the motion of the Sun and
^Neugebauer p. 17 under to^ov
134
Moon as was said previously in book nine.
11.1.3 On the Accurate Correction of the Location of the
Moon with the Equation of the Day
Entrance is made into the table of the equation of the day opposite the degree of the
Sun, and the fractional parts of the hour are reckoned. Entrance is made into the
table of hours for the months opposite this result, and the mean motion is reckoned.
This is subtracted from the true longitude of the Moon, and so this becomes final.
11.1.4 On the Degree Which Sets with the Moon
An examination is made. If the Moon^ does not have a latitude, it sets with that
degree (which is) together with the true longitude. If it does have a correct latitude,
its Sine is reckoned. This is multiplied by the Sine of the altitude of the location of
the ''highest point" . The result is divided by the completed Sine of the complement
of the altitude of the place of the ''highest point". The result is a Sine. Its arc is
taken. The result is a correction. It is examined. If ever there is need that this
computation be easier, through only one method, the degree of the Moon which was
found for the motion of the Moon is sought in the table of more and less for the
place of "fortune" for the third Mima. Entrance is made (into the table) opposite
that (degree), namely of the zodiacal signs there, for the desired klima and the city
closest to us. The number found there is reckoned in degrees and minutes. The
result is multiplied by the solid latitude of the Moon. The result is a correction.
Then that solid latitude is examined. If it is northerly, the correction is added
to the location of the Moon. If it is southerly, it is subtracted from that (location
of the Moon). The result is the degree setting with the Moon. If the calculation
3pingree: In Greek, p. 161 line 7, read EeXrjvr] for Tpaxir]XaLa
135
occurs through the degree setting with the Moon, it occurs in an opposite way to
that calculation, that is, where there was subtraction, there is addition with the
correction, and where there was addition, there is subtraction.
11.1.5 On the Arc of the Light
The solid latitude of the Moon is squared, that is, multiplied by itself, and is added
to the square of the distance (in latitude) between the Sun and the Moon. The
''multiplication" of this result is sought. The result is the arc of light, that is, the
shining of the Moon^.
11.1.6 On the Arc and the Time When the Moon is above
the Earth after the Setting of the Sun
The place of ''fortune" of the degree of the diameter of the Sun is reckoned for the
latitude of the city. Then it is examined. Then the place of "fortune" of the degree
of the diameter is reckoned along with the degree with which the Moon sets for the
latitude of the city. Then the place of "fortune" of the Sun is subtracted from the
place of "fortune" of the Moon. The result is that which was mentioned.
11.1.7 On the Arc of the Setting of the Sun Below the Earth
at the Time when the Moon Sets
When there is need for this calculation, the true longitude of the Sun is subtracted
from the location of the Moon which we corrected. The Sine of this result is then
reckoned. Then it is multiplied by the completed Sine of the altitude of the place of
the "highest points". The result is lowered by one (sexagesimal) step. The result is
^Neugebauer p. 17 under cpco^
136
a Sine. Then its arc is reckoned, and the setting of the Sun is found. We have set
up a table for the latitude of 37 degrees.
If there is need for this arc of time to be apprehended for the highest altitude of
the degree of the diameter of the Sun, entrance is made into the table of the setting
of the Sun and the altitude of the Moon opposite that altitude, at the number in
red for the altitude of the degree of the diameter of the Sun on the circle of mid-day,
and (at) the number, also in red, at the top of the table for the arc of the time of
the altitude of the Moon. Wherever the values from the distances come together,
the number found there is reckoned. The result in degrees and minutes is the arc of
the setting of the Sun .
11.1.8 On the Altitude of the Moon after the Setting of the
Sun from this Table
When it is necessary to know this method, the latitude of the Moon is extracted,
and it is determined whether it is southerly or northerly. This latitude is kept aside.
Then the highest altitude^ of the degree of the Moon is apprehended and examined.
If the latitude of the Moon is northerly, it is added to the altitude. If (the latitude
of the Moon) is southerly, it is subtracted from that (altitude). And the highest
altitude of the Moon is found. Then this (highest altitude) is sought in the table of
the setting of the Sun and the altitude of the Moon in the red numbers. The time
of the arc is sought opposite (the place) where this is found within the table. The
red number at the top of the table is reckoned opposite (the place) where it is found.
This is the altitude of the Moon when it appears new.
^Neugebauer p. 6 under dvdpaaL^
137
11.2 On the Apprehension of Arcs
It was investigated concerning the New Moon that appears after conjunction in the
books of the ancients. It was found that 4 arcs were set down by them (for its
determination). The first is the arc of time, the second is (the arc) of the rays,
another is (the arc) of altitude, and the other is the arc of setting. These four
arcs with the computation of the proper (place) of the Moon are corrected into the
computation that exists with us.
These four arcs are not straightforward in all (locations) Why? Because of the
excess and deficiency in the latitudes of cities and because there is excess and defi-
ciency in the arcs of the time of rising and setting. We have sought to extract this
so that the excess of each arc and (its) deficiency and quantity might be obtained.
11.2.1 On the Apprehension of the Arc from Ten Degrees
until Twelve
The arc^ of time is from eight until twelve, the arc of the altitude of the Moon from
six degrees until eight, and the arc of the setting'' of the Sun from eight degrees
until ten. When there is need to have the number of each, the diflFerence of each is
reckoned in excess and deficiency. This is multiplied by the fractional parts of the
true longitude. The result is lowered by one (sexagesimal) step. This is a correction.
It is added to each of the four arcs. The result from each of these (four additions) is
a limit of the visibility of the Moon.
When there are four arcs and four limits, and each of these four arcs is extracted
by calculation in the way mentioned (earlier), one by one (these arcs) are observed
opposite the number of the limit. If each is equal to or greater than the number of its
^Pingree: text, p. 165, 1. 12, read toO to^ou and om. second toO cpcoxo^
^Pingree: p. 165 1.15 read xaxapdaeco^
138
limit, the Moon is observed. If it is less, (the Moon) is not observed. It is possible to
see the Moon with the number of one of these 4 arcs, but it is not possible with the
other 3. Therefore the computation is for these 3. If it is possible to see (the Moon)
through the 3 numbers, it is not possible through these. Because of this there is no
way for this calculation to be avoided. There is another method (of determination
of visibility) which will be discussed next.
11.3 On the Complete Basis of Seeing the Moon
Know that the sighting of the New Moon when it appears is with respect to the
vision of the eyes. There are eyes sharing in more light, and there are others sharing
in less, and there are those participating in a middling of sight. For this (reason)
three numbers were set forth. The first calculation is large (and is) by means of
eyes having the least light, the second (number) is middling (and is) by means of
eyes having middling light, and the third number is small (and is) by means of eyes
having the most light. This, the middling number, is trusted by all.
When there is need for such a method, the true longitude (s) of the Sun and of
the Moon are extracted for that time when the Moon sets so that the arc of light
might be extracted with the setting of the Sun. These two — the arc and the setting
— are examined. Then entrance is made from the proper (motion) or the velocity
of the Moon into the tables of the sighting of the Moon, from its visibility.
The middling number found between the two marks, which is called the mean
number, is reckoned opposite these, the proper (motion) and the velocity. This
number is reckoned for one and for two separately. Then the number from one is
subtracted (from the number) from the second. The result is called a correction.
This result — the correction — is examined. There are two things in this number on
which it is necessary for the mind to dwell.
139
11.3.1 For the First Sighting
There is an investigation into the first sighting. If it is less than or equal to the first
arc, there is no sighting of the Moon. Why? Because the Moon is still hidden under
the light of the Sun. If it is equal to or greater than the second arc, the Moon has
come out from under the light of the Sun and appears before the Sun sets. (In this
case) there is no need for a calculation on the tablet. If the arc of light is greater
than the first arc and less than the second, the New Moon is or is not at the stage
of appearing^.
In this case there is absolutely a need of calculation for (whether) or not one sees
the Moon. When we want to make this calculation we do as follows: we subtract
the first arc from the arc of light. The result is called the excess. We multiply this
excess by the first arc. We divide the result by the correction which was kept aside.
This result is subtracted from the first arc, and the remainder is the arc of complete
visibility^.
11.3.2 On the Second Sighting
The setting of the Sun is examined. If it is equal to or greater than the arc of
complete visibility, the New Moon is visible.
If one wishes to examine this method without error with regard to the two other
ones — the first and the third — , it its necessary to do the work.
If the Moon appears with the number of this first table, we say that the Moon
ought to appear large so that even the blind see it. If the number comes out of the
second table, we say that the Moon ought to appear neither very dim nor large, so
that eyes middling in vision see it. If the number comes out of the third table, there
is no work because the Moon is then very dim, so that unless there is a cloud in the
^Neugebauer p. 7 under pa6^6^
^Neugebauer p. 16 under to^ov
140
horizon or a mist, (only those) eyes that see clearly see it, and the beginning of the
month is not reckoned from that time, but it is written at the beginning of the true
longitude that the Moon may perhaps appear.
11.4 On the Calculation so that the Moon is Shown
in Digits
If there is need for (this) calculation, four minutes are added to the location of the
Moon so that the location of the Moon may be found when the Sun sets up to an
eighth of one hour because the Sun has not set so much under the earth and the
light of the Sun does not yet let the Moon appear. Then the altitude of the Moon
is extracted in the way described earlier just as is the point of altitude^^ as was
described in the fifth chapter of the sixth book.
Then a plumbline is placed at the point of altitude with its demonstration so
that neither a hill nor a cloud comes in front of the direction of setting.
11.4.1
Then the astrolabe is hung on that plumbline and is aligned with the straight line
which is on the earth. Then the altitude of the Moon is examined, how much comes
out of the table of the setting of the Sun and the altitude of the Moon. The tip of
the ''beam"^^ of the astrolabe is placed against this number. Then with one eye,
with the other closed, one looks through the sighting holes of the ''beam" (to see) if
the Moon is visible. If the Moon does not appear through these sighting holes, that
location visible in the sky is where the Moon should be sought.
^^Neugebauer appendix 14.
iipingree: "beam" = diopter
141
11.5 Concerning the Five Planets, at what Time
They Come Out or Stand Out from under
the Light of the Sun, and at what Hour They
Enter under the Light of the Sun, in the
Morning or Evening
This calculation is the same as in the case of the Moon.
When there is need for this calculation, the degree rising with the star or the
degree setting with the star is determined in the way that was described earlier
(5.4). The arc of the time of the setting of the Sun should be extracted just as it was
extracted for the calculation of the apparent New Moon. The arc(s) for the visibility
of the planets are as follows according to the Indians: Saturn, 15; Jupiter, 11; Mars,
13; Venus, 9 , and Mercury, 13^^.
(The arcs for the visibility of the planets) are as follows according to Ptolemy,
with the calculation of the arc of the setting of the Sun for the time when the planet
sets or rises: Saturn, 11; Jupiter, 10; Mars 11;30 ; Venus, when it has direct motion,
60^^, and when it is in retrograde, 5; Mercury 10.
Then how much the distance of the planet from the Sun is is examined. If it is
opposite these arcs or greater, the planet is visible. If it is less, the planet is not
visible.
^^Pingree: should be 17.
^^ Should be 7 {I mistake for Q.
142
11.5.1 On the Knowledge of When the Planet May Appear
and When it May Set with a Table
We have set down a table (for this), and have put the arcs we need in this table with
the number (s) of the settings for the fourth klima at the beginnings of the zodiacal
signs. If the planet is at the beginning of a zodiacal sign, it is reckoned in the table.
If it is not at the beginning of a zodiacal sign, the number which is at the beginning
of the zodiacal sign is reckoned and examined as well as whatever is found at the
beginning of the following zodiacal sign. This is reckoned, and with the number(s) of
the two zodiacal signs is corrected as was described for the more and less of visibility.
The result is the arc of the sighting of the planet. Then the mean difference of the
true longitude (s) of the Sun and of the planet is reckoned and examined. If this
number is for (when) the planet appears, and if that difference is greater than the
arc of the (planet) when it appears, the planet is visible. If it is less, the planet is
not visible. If this number is for when the planet sets, if that difference is greater
than the arc of where we look, the planet has not yet set. If it is less, the planet has
set.
11.5.2 For Ascertaining at What Time the Planet Sets and
at What (Time) it Rises
The motion of the Sun and of that planet are apprehended and placed on the tablet.
Then they are examined. If the planet is retrograde, the two motions are added.
If the planet moves directly, the smaller (value) is subtracted from the larger. The
result is the final motion. This is examined. Then the difference is put down on the
tablet, and the apparent arc is placed alongside it. Then the smaller is subtracted
from the larger. The result is divided by that final motion. The result is the day
when the planet either sets or rises.
143
11.6 On the New Moon When it Appears with
the Calculations which were Combined with
Others Which Have Been Produced from the
Mind of KhazinI for an Easy Road without
the Difficulty of those Long Methods, Since
These are Worked out for Clarity and Brevity
This is in two sections.
11.6.1 On the Accurate Correction of the Arc of Time
The true longitude (s) of the Sun and of the Moon (are calculated) for the beginning
of the night which is of the morning following the thirtieth day (reckoned) in the
days of the Arabs. Then the arc of time, the arc of light, and the motion of the
Moon are calculated. Then the motion is put on the tablet and subtracted from
25;30. The result is the not final arc of sighting. It is examined. Then the arc of
light is placed alongside it and examined. If the two are equal, the arc of sighting is
final. If they are not equal, the smaller is subtracted from the larger. The result is
the excess. This is examined. If the arc of light is less than the arc of sighting, that
excess is added to the arc of sighting. If it is greater than the arc of sighting, this
final arc is placed on the tablet. The arc of time is placed alongside it and examined.
If the arc of time is equal to or greater than the arc of sighting, the Moon is visible.
If it is not, it is not visible. Then the arc of light is examined. If it is 25;30 or more,
the Moon comes out from under the light of the Sun and is visible before the Sun
sets. If it is less, it is not visible.
144
11.6.2 On the Accurate Correction of the Arc of the Setting
of the Sun and for the Extraction of the New Moon
with Other Calculations
The true longitude (s) of the Sun and of the Moon are (calculated) for the thirtieth
night of the month of the Arabs when the Moon sets. Then the arc of light, the
setting of the Sun and the motion of the Moon are examined. Then the motion of
the Moon is subtracted from 24:30. The result is the not final arc of sighting. This
is multiplied by the arc of light. If it is less than the arc of sighting, there is no need
of looking for the Moon. If it is equal to or greater than it, it is visible.
The Calculation
The arc of light and the arc of sighting are put in two places on the tablet. The
diflFerence of the two is reckoned and subtracted from the arc of light, and it becomes
final. This is put on the tablet. The (setting) of the Sun is placed alongside it.
Then the setting of the Sun is examined. If it is equal to or greater than the arc of
sighting, the Moon is visible. If it is less, it is not visible.
Then an examination is made. If the arc of light is 24;30 or more, the Moon is
visible before the Sun sets. If it is less than this, it is not visible before the Sun sets.
BOOK 12
On the Beginning of the Years and
Genethhalogical (Dates), and on
Ascertaining the Location(s) of the
Planets, the Motion of the
Degrees, and Ascertaining the
Location(s) of the Degrees
When we wish to know how much has passed of year(s) of the Sun with respect
to the genethhalogical (date), the year of the Persians when the birth occurred is
subtracted from the current year of the Persians, or the then year of the Romans
from the current year of the Romans. The result is (the number of) the complete
years of the Sun which have elapsed since the birth. This book is divided into four
chapters.
145
146
12.1 On the Beginning(s) of Complete Years, of
Genethlialogical Years, and of the Place of
^Tortune'' of Each
This calculation should be apprehended^ (as follows): if it is such that the true
longitude of the Sun at the time when the birth took place was complete with the
equation of day, the true longitude of the Sun for this time in which we are should
be complete with the equation of the day. If that is not complete, then neither is
this. This calculation should be reckoned enthusiastically.
12.1.1 On the Extraction of the Hours of the Beginning(s)
of the Years at the Time When the Sun is at the
Beginning of (one of) the Zodiacal Signs, or at the
Time When the Sun is at That Degree at which (it
was when) the Seeking of the Birth Occurred
This is called the location of the radix of the Sun for the calculation of the geneth-
lialogical (horoscope). This calculation will be described in this book with respect
to the distance of motion. If we wish to know the hour of the time when the Sun
arrives at that degree, the true longitude of the Sun is sought for the mid-day which
is close (st) to that degree for the longitude of the city where the birth (took place).
If the true longitude is equal to that degree, the hour of mid-day is the hour of (its)
entrance (into that degree). If it is not equal, the difference found between the two
of them is reckoned. This is multiplied by 24. The result is divided by the motion
of the Sun. The result is the hours of distance.
ipingree: text p. 176, line 12 read xaTaXir]cp6f]vaL
147
This is examined. If the true longitude of the Sun is less than that degree, the hour
of distance is added to the hour of mid-day. If it is greater, it is subtracted from that
degree. The calculation is made complete just as was described for the opposition
and conjunction of the Sun and the Moon. And the hours of the entrance are found
in the day or the night for the calculation of the genethlialogical (horoscopes) and
of the complete perceived years.
One thing should be considered in the case of a perceived year. If the true
longitude of the Sun was not complete with the equation of day, entrance is made
into the table of the equation of day opposite the true longitude of the Sun, and the
minutes and seconds of the hour are reckoned. These are added to the hour of the
entrance.
12.1.2 On The Entrance of the Place of "Fortune"
From what (ever calculation) the hour of entrance was ascertained^, from that hour
the ''fortune" is extracted as was described previously.
If we wish to extract the ''fortune" of the entrance with another calculation, that
calculation is the calculation of the excess of the years^. A search is made for how
many years have passed since the birth. Entrance is made into the table of excess of
the years opposite those years, and (the excess) is reckoned opposite it.
That excess is made final with the correction for the apogee. This is always
added to the place of the "fortune", that is, to the beginning of the birth. If the
result is greater than the circumference of a circle, 360 (degrees), the circumference
is subtracted from it until it becomes less than that. The result is the place of
"fortune" of the entrance. Entrance is made opposite this into the table of the place
^Pingree: p. 178, 9 read xaTaXrjcpGf]
^Neugebauer p. 14 under izEpiooEia
148
of ''fortune" for the latitude of that city^ in which the search for the genethlialogical
(horoscope) was made. And the ''fortune" is extracted opposite that in the way
described earlier.
12.1.3 On Ascertaining the "Fortune" of Middle of the In-
habited (Earth) in Longitude and Latitude
The difference between the longitude of the city and 90 is reckoned. The result is
an arc. If the longitude of our city is less than 90, that arc is added to the place
of "fortune" for our city. If it is greater than 90, it is subtracted. The result is the
place of "fortune" .
Entrance is made opposite this (result) into the table of the place of "fortune"
with the straight line whose beginning is from the beginning of Aries, and the "for-
tune" is extracted. If the beginning of this table with the straight line is from the
beginning of Capricorn, the "fortune" is extracted counting from that.
That place of "fortune" which is with us is more than 270. The result is the
place of "fortune" in that table. If we wish to extract the "fortune" from the middle
of the inhabited (world), where the latitude is 33 (degrees), that place of "fortune"
— not the one added to 270, but the one before it — is extracted from the place of
"fortune" in the table for the latitude of 33.
^oblique ascension of the ascendant
149
12.2 On Ascertaining the Location of the Light of
the Stars, or their Configuration with Each
Other
Before entering into this calculation, there are certain basic things which should be
known. Know that from the tenth (house) (and) the first until the fourth is the
half(-circle)^ of descent, from the fourth house (and) the seventh until the tenth is
the half (-circle) of ascent^.
12.2.1 On the Distance of the Stars from the Seventh (House)
- which is at the center- and the Fourth (until) the
Tenth — with the Calculation of Ptolemy
The place of ''fortune" of the stars is reckoned with the straight line. Then it is
examined. If the star is above the earth, the degree of the tenth house is reckoned
with the straight line. If the star is beneath the earth, the degree of the place of
''fortune" of the fourth house is reckoned with the straight line. Then an examination
is made. If the star is under the earth between the seventh and the fifth, the place
of "fortune" of the star is subtracted from the place of "fortune" of the tenth house.
The result is the distance from the tenth. If the star is between the tenth and the
first house of the place of "fortune" , the place of "fortune" of the tenth '' is subtracted
from the place of "fortune" of the star. The result is the distance of the star from the
tenth. If the star is under the earth, it is examined. If it is between the ascendant
and the fourth, the place of "fortune" of the star is subtracted from the place of
^Pingree: p. 180, line 8 read xaxapdaeco^
^Neugebauer p. 6 under dvdpaaL^
^Pingree: p. 181, line 2 toO for 6^
150
''fortune" of the fourth. The result is the distance of the star from the fourth. If the
star is between the fourth and the seventh, the place of ''fortune" of the fourth^ is
subtracted from the place of "fortune" of the star. The result is the distance of the
star from the fourth.
12.2.2 On the Latitude of the Circle of Motion, Namely, the
Latitude of Cities
When there is need (for) this calculation^, the distance of the planet from the center
of the tenth or the fourth is multiplied by the latitude of the city. The result is
examined. This is called a radix. Then this is examined. If the planet is above the
earth, that radix is divided by half the arc of the day^^ — the hayldj according to
the Indians. If the planet is beneath the earth, that radix is divided by half the arc
of the night — the hayldj. The result is the latitude of the circle of motion.
For this latitude there is a table of place (s) of "fortune" of the zodiacal signs so
that this might be the radix for the motion of the planets.
12.2.3 On the Place of Light of the Planets, that is, the
Configuration with Respect to Each Other of those
(Planets) which have a Latitude, with Calculation
and by Means of a Table
Know if a star has no latitude, the arcs of sextile, square, trine and opposition are
60, 90, 120, 180, 240, 270. If the planet has a latitude, these arcs greater and less,
are (ones) for which there is a need of correction.
Spingree: p. 181, line 8 toO for 6
^Neugebauer p. 15 under uXoltoc,
^^Neugebauer p. 16 under to^ov
151
The Sine of 30 is reckoned. It is multiplied by the completed Sine of the latitude
of the planet. The result is lowered by one (sexagesimal) step. The result is a Sine.
Its arc is reckoned. This is called the correction. It is examined. Then 90 is placed
in three places (on the tablet). Then that correction is subtracted from the first and
added to the third. The result from the first is the arc of the sextile, the ''diameter" ^^
of this is the trine. The second arc is of a square, the ''diameter" of this is again
square. The third arc is of a trine; the "diameter" of this is the arc of a sextile.
Calculation with the Table from which the Latitude of the Planet is Clear
Entrance is made into this table of the configurations of the planets opposite the
latitude of the planet, and (a value) is reckoned opposite that. Whatever is found
from the first and the second table and what is found from the two tables are ex-
amined. The true longitude of the planet is placed on the tablet in two places. The
number reckoned from the first table is subtracted from the true longitude of the
planet which was placed first on the tablet, and added to the true longitude which
was placed second. The result in the second (place) is the place of the light of the
sextile of the planet from the left, and its "diameter" is its right trine. The result
from the first is the right sextile and its "diameter" is its left trine.
The number (from) the second table is the latitude of the sextile in the direction
where is the latitude of the planet. This number is also the latitude of the trine in the
direction where there is no latitude of the planet. The square has no latitude. If it is
necessary to comprehend^^ the square, 90 degrees are added to the true longitude of
the planet, and the left square is found. The "diameter" of this is the right square.
The latitude of the opposition of the planet is opposite the latitude of the planet in
that direction where the planet is not.
^^The ^Ld^STpoc; of angle is here apparently 180 — 0, or the supplement of 0.
^^Pingree: p. 183, 15 read xaTaXir]cp6f]vaL
152
12.2 A On the Place of Light of the Planets with the Com-
bination of the Two Places of "Fortune" with the
Calculation of Ptolemy
When there is a need, an examination is made. If the planet is in the half(-circle) of
ascent of the sphere (12.2), entrance is made into the table of the place of ''fortune"
with the straight line opposite the degree of the planet, and the place is reckoned
from within the table. This is set down in 6 places on the tablet. 60 is added to
the first place. 90 is added to the second, 120 to the third; and 60 is subtracted
from the fourth, 90 from the fifth, 120 from the sixth. Then each of the six is sought
within the table of the place of ''fortune" with the straight line. The zodiacal sign is
reckoned above the table and the degrees along the side. The minutes are extracted
from between the two tables as was described earlier (2.1). The result is placed in
the same order in six places. The left sextile is found from the first place, the left
square from the second, the right trine from the third, the right sextile from the
fourth, the right square from the fifth, and the right trine from the sixth. These six,
namely the six configurations, are examined.
Then entrance is made opposite the true longitude of the planet into the table
of the place of "fortune" of the zodiacal signs for the latitude of the city where the
birth took place, and the place of "fortune" is reckoned from the middle of the table
and set down in six places. Then this number — as the first is set down in 6 places
opposite those six numbers, the first below the first, the second below the second,
and so on. Then it is examined whether, (concerning) these two numbers, each is
with the other opposite (it) or not, the first with the first and so on. If the two (rows)
are equal, the place of the six lights of the planets (that is, their configurations) is
correct.
If they are not opposite, they must be corrected. Once one is corrected, the rest
will be also. When it is necessary to extract the correction of each, the difference of
153
each (pair) is examined, that is, the (difference) found between the first and so on.
That (result) is multiplied by the distance of the planet from the tenth or the fourth
center. The result is called the basis. This is examined.
Again it is examined. If the planet is above the earth, the basis is divided by half
the arc of the day of the planet (A). If the planet is below the earth, the basis is
divided by half the arc of the night of the planet. The result is the correction. This
is multiplied by the three ray-castings of the planet, that is, by the three aspects
from the left, each of which came out from the two numbers so as to be close to the
planet. This correction is added to that which is closer. Then it is added to the
three ray-castings from the right to that which is farther, and the six configurations
are found.
If the planet is in the half(-circle) of descent of the sphere, these mentioned
calculations are made for the place of ''fortune" of the (opposite) point^^ of the
planet. The result is the opposite (point) of the light of the planet. 6 zodiacal signs
are always added to that opposite (point) and the light of the planet is found.
If we wish to perform this art in a different way, the latitude of the circle of
motion^^ is ascertained, and the table of the place of ''fortune" for that latitude that
is recognized so the computation may be easier.
When we wish to make the calculation, it is examined. If the planet is in the
half (-circle) of ascent of the sphere (12.2), the place of "fortune" of that degree is
reckoned from the table. If the planet is in the half(-circle) of descent of the sphere,
the place of opposition to the degree of the true longitude of the planet is reckoned
in the table of the place of "fortune" for the latitude of the city with the straight
line. The number of each ray-casting for that place of "fortune" is combined as was
^^Here and elsewhere opposite point is used to signify the point which is 180 degrees away from
the point in question
^^Neugebauer p. 15 under TiXdioc;
154
said (12.2.4), when there is addition and subtraction with the values 60, 90 and 120.
The other calculation is completed in the way described earlier. The result is the
diametrical point of the light of those planets. Six zodiacal signs are added to each,
and the light of the planets is found.
The Calculation by Means of another, Easier Method
When the calculation of this is (made) by means of one place of ''fortune" the table
of the place of ''fortune" along with the latitude of the circle of motion is brought to
(one's) hands, and these numbers are read from the table. There is no need of the
place of "fortune" with the straight line.
12.3 On the Motion of the Hayldj^ that which Ex-
ists from its Proper Purpose, and the Place
of that Degree
Know that the motion of the hayldj is one degree of the place of "fortune" for each
year of the Sun. Since one degree per year is (equivalent to) 5 minutes in one month,
and there are 6 days for one minute, and ten seconds are one day, and it is thus for
all calculations, this hayldj which moves with the planets and good and bad hours,
it moves so that from this it is ascertained^^ whether a man will live or die. Two
calculations are employed for this motion of the hayldj. One calculation is for when
the hayldj moves twice to that degree; this is the second, that the time ought ot be
ascertained, but not necessarily the degree. For this (reason) this chapter is divided
into two (sections).
^^Pingree: p. 188, 1.1 read xaTaXrjcpGf]
155
12.3.1 On the Calculation so that the Degree of the Un-
known Time may be Known
When it is necessary that this calculation occur, first the place of ''fortune" of the
hayldj together with the place of ''fortune" of the degree with the latitude of the
city are reckoned, and each is placed separately. Then the hayldj is examined. If
it is in a degree of the tenth or the fourth house, its place of "fortune" with the
straight line is subtracted from the place of "fortune" with the straight line of that
(hayldj). If the hayldj is in a degree of the seventh house, the place of "fortune"
of its opposite (point) together with the latitude of the city is subtracted from the
place of "fortune" of the opposite (point) of that degree together with the latitude
of the city. The result is the arc of motion.
One year is reckoned for each degree as was mentioned earlier (12.3), so that the
time of motion may be known. If the hayldj is between two cardines, correction
is made as follows: if the hayldj is in the half(-circle) of ascent of the sphere, the
difference between the place of "fortune" with the straight line of its degree for the
latitude of the city is reckoned and examined. This is multiplied by the distance of
the hayldj from the cardine. the result is a basis. This is examined. If the hayldj
is above the earth, that basis is divided by half the arc of day(light) of the hayldj.
If it is beneath the earth, it is divided by half the arc of night (of the hayldj). The
result is the correction. Then it is examined with the place of "fortune" (with) the
straight line. If it is greater than the place of "fortune" of the city, the correction
is subtracted from it. If it is less, it is added to it. The result is the final place of
"fortune" of the degree of the hayldj. This is examined. Then the difference between
the place of "fortune" with the straight line of that degree (compared) with the
place of "fortune" of that degree for that city is reckoned. This is multiplied by the
distance of the hayldj and divided by half the arc of day(light) or of night of the
hayldj. The second calculation is completed in the way described, so that the final
156
place of ''fortune" of that degree may be found.
Then the final place of ''fortune" of the hayldj is subtracted from the place of
"fortune" of that degree. The result is the arc of motion. If the hayldj is in the
half(-circle) of descent of the sphere, the place of "fortune" of the opposite (point)
of the hayldj is reckoned from that degree, and the calculation occurs so that the
arc of motion is found.
If we wish to make this computation easier, first the place of "fortune" of the
zodiacal sign together with the latitude of the circle of motion is obtained. Then
one place of "fortune" is reckoned, either that of the hayldj or (that) of its opposite
(point), and again its degree similarly. Then the place of "fortune" of the hayldj is
subtracted from the place of "fortune" of that degree so that the arc of motion may
be found. The degree of each is reckoned in the way described.
12.3.2 On the (Temporal) Subdivision of the Degree of the
Haylaj
When the time is known, even though the degree to which the hayldj is moving
is not known, when it is necessary that this calculation occur, the genethlialogical
(horoscope) is examined, how many years, months and days have elapsed from it.
Each year of the Sun is reckoned as one degree, each month is reckoned as 5 minutes,
and each day is reckoned as 10 seconds. The result is called the arc of motion or the
march. This is kept aside. Then it is investigated if the hayldj is in a degree of the
tenth or the fourth cardine, this arc of motion is added to the place of "fortune" with
the straight line (of the hayldj). The result is examined in the middle (of the table)
of the place of "fortune" with the straight line, and the zodiacal sign is reckoned
above, and the degrees along the side. The number of minutes is extracted from
between the two tables just as was described earlier (2.1).
The result is the location of the degree of the hayldj. If the hayldj is at the degree
157
of the ''fortune" , this calculation is made with the place of ''fortune" for the city. If
the hayldj is at the degree of the seventh house, this calculation is (made) with the
place of "fortune" of the opposite (point) of the hayldj for the place of "fortune" for
the city. The result is the opposite (point) of the degree of the portion of the hayldj.
Six zodiacal signs are added to this, and the degree of the portion of the hayldj is
found. If the hayldj is between the two cardines, the calculation should occur with
the two places of "fortune" (of the centers), (that is), with the place of "fortune"
(with) the straight line and (that for) the city. This is examined. If the hayldj is
in the half(-circle) of ascent of the sphere, this calculation occurs with the place of
the degree of the hayldj. If it is in the half(-circle) of descent of the sphere, this
calculation occurs with the opposite (point) of the degree of the hayldj. The result
from the two places of "fortune" in zodiacal signs, degrees and minutes — (is) that
the degree is the degree of (the) hayldj (made) with the number of each place of
"fortune". This is again examined. If the two (values) are equal in zodiacal signs,
degrees and minutes, that degree is the final degree of the hayldj. If they are not
equal, a correction occurs.
Its calculation is thus. The diflFerence between the two places of "fortune" is
reckoned. This is multiplied by the distance (from) the hayldj to the tenth or fourth
cardine. The result is a basis. Again, this is examined. If the hayldj is above the
earth, the basis is divided by half the arc of the day of the hayldj. If the hayldj is
beneath the earth, the basis is divided by half the arc of the night of the hayldj. The
result is the correction.
Then it is examined (in realtion) to the place of "fortune" with the straight line.
If it is greater than the place of "fortune" for the city, the correction is subtracted
from it. If it is less, the correction is added to it. The result is the place of "fortune"
158
of the degree, which degree^^ is of the hayldj^ with the straight line. The degree^''
of the hayldj is extracted from that place of ''fortune" . If the hayldj is in the half (-
circle) of descent of the sphere, this calculation occurs with the place of ''fortune" of
the opposite (point) of the hayldj. The result is the degree of the opposite (point)
of the degree of the hayldj. Six zodiacal signs are added to this. The result is the
degree of the hayldj.
This calculation with another order (is) easier, being with one place of "fortune" .
When there is need that this calculation occur, the place of "fortune" of the zodiacal
signs of the latitude (of the circle) of motion (12.2.2) is reckoned. Then it is examined.
If the hayldj is in the half (-circle) of ascent (of the sphere), this number occurs
together with the place of "fortune" of the degree of the hayldj from its table. If
it is in the half (-circle) of descent, this number occurs together with the place of
"fortune" of the opposite (point) of the hayldj from this table.
12.4 On Considering the Motion of the Degree of
the ^Tortune'' of the Genethhalogical (Horo-
scope) in a Year, in Months and Days
There are four sections for the motion of its "fortune" .
12.4.1 On Considering that Calculation that it Moves One
Zodiacal Sign in Each Year
When there is need of this calculation, the completed years of the Sun that have
passed from the genethlialogical (horoscope - date) are placed on the tablet. The
^^Pingree: p. 192, 10 read f] ^OLpd
^'^Pingree: p. 192, 11 read f] \ioipa[Tfic, ^oLpa^]
159
point of the zodiacal sign of the ''fortune" in the base genethlialogical (horoscope) ^^
is additional to those years. The result is divided by 12, that is, there is a subtraction
of those (years) by twelve. The result should be the zodiacal sign at which the the
motion of the ''fortune" has arrived at that year. That zodiacal sign is called the
intihd\ The degree and its minutes are the degree and minutes of the "fortune" in
the (horoscopic) diagram.
This motion is in three (ways) The first is that for each year^^, it moves one
zodiacal sign, for each month two and a half degrees, and for each day 5 minutes.
With this calculation the degree of the "fortune" moves together with the light of
the planets when there is a "fortune" of the base (horoscope) and a "fortune" of the
"entrance" .^° The second (type of motion) is that 13 zodiacal signs are counted for
each year, one degree and 4 minutes for each day, and for every 28 and one tenth of
a day it passes by one zodiacal sign. This is called the motion of the months.
The third (type of motion) is that 13 zodiacal signs are counted for every 28 days
and one tenth of a day, and 13 degrees and 53 minutes for every day (this is the
motion in that (way) of days). A table has been set up for each of these three so
that this calculation may be easily (found) there.
12.4.2 On the Calculations of the Motion of the "Fortune"
of the " Entrance"
Know that the degree of the "fortune" of the "entrance" and its houses and their
planets moves 12 zodiacal signs in a year and 59 minutes and 8 seconds in a day
— that (this) is the mean motion of the Sun — and they move with this number
along with the light of all the planets through a complete rotation of the sphere. The
^^Pingree: base horoscope = J^^l
i9pingree: p. 194, 3 read xpovov for C^^lov
20
Pingree: zlaiXzxjaiQ = sL^
160
second (type) is for the motion of the months. This is 12 degrees and 49 minutes for
one day. With this number one zodiacal sign is completed in so many days, minutes
of a day, and seconds: 30;26,12, in a month of the Sun.
12.4.3 On the March of the "Fortune" of the "Entrance" for
a Month with this Calculation
In so much time: 30;26,12 (days), 12 zodiacal signs are traversed so that a rotation
is completed. In each day are so many degrees (and) minutes: 11;50, so that in
one month the calculation of the ''fortune" of the months returns to their beginning
with all the ray-castings of the planets. Tables have been set up by means of these
calculations so that the computation is easy.
12.4.4 On the March of the "Fortune" of the "Entrance"
with another Calculation
The place of ''fortune" of the "entrance" is placed on the tablet. For one month
of the Sun 7 degrees and 13 minutes are additional. The result is sought within
the table of the place of "fortune" for the city. The zodiacal signs and degrees are
reckoned opposite that so that the degree for one month may be found.
The degree for each day is extracted there (in the table) with this calculation for
one year of the Sun. 86;44,4 (degrees) are additional to the place of "fortune" of the
"fortune" of the "entrance" ^^.
A table has been set up by means of the calculation so that the calculation is
easier.
Whatever was found by us from the beginning (of this work) and whatever we
have supplied beforehand in these twelve books and the chapters of each book and the
21
Pingree: place of "fortune" = JLLo; "fortune" = Jli?
161
sections of all these (chapters), we have brought this to an end with the will of God
as (our) helper. May God maintain that man who, going through this composition,
learns (the problems) worked out in it by us accurately as behoves (him).
Appendix A
First Scholium
Shams ( al-Bukharl) with respect to this.
Half the arc of that night and half the star's arc in the day are examined. If
these two are equal, that discovered arc when the star rises is of the beginning of the
night. If half the star's arc in the day is less than half the arc of the night, that is
subtracted from half the arc of the night. The result is added to the arc. The result
is the arc from the beginning of the night. If half the star's arc in the day is greater
than half the arc of the night, the smaller is subtracted from the larger. The result
is subtracted from the arc. The result is the arc of the beginning of the night, and
the desired hours of the night are apprehended from this.
162
PART III
Glossary
163
164
• Entries are given in alphabetical order
• Within the alphabetical order, entries are listed by order of appearance in the
text
• Nouns are given in the nominative
• Verbs are left in the finite form
• Adjectives and participles are given in the nominative
• Adjectives and participles are given in the masculine singular, unless used as
substantives
• the form of each entry is
- Greek word
- one or two corresponding Arabic words (if applicable)
- location in text (book, chapter, section, subsection)
- Greek lemma
- Arabic corresponding to the Greek lemma
- English translation of the Arabic
OL (^lyi) 12.2.1
6 daxrip \iioo\ xoO i xal xoO a OLXTQ^axoc; xoO xotiou xfjc; xu^iQ^
— ^JliaJlj jt\^\ (jiu UJ jIS^ jI _ ^^^\ if the star is between the tenth and
the ascendant
ApSoupax^av ( Jjl^li ) 7.0.0
6 ApSoupax^ocv 6 Xa^aviQc; — (Jj^' ^1 Khazinl
165
Map ( oUjIil ) 1.5.2
'A8dp — oLojIil Adhar-mah
TO ToO AtyoxspcoTOc; ( Oi^'>Li;Mi j^ioju ) 5.2
eav 6 daxrip sic; to eaxl xoO KapxLvou y] slc; to xoO Alyoxepcoxoc; —
ijiJ^LuMI ^Wg> (^As>l ^ (3^*^^ O^ in agreement with one of the two solstitial
points
atXaxC ( ^>Ui ) 12.2.2
TO alXax^ — /T^W^' the hayldj
atXaxC ( ^>Ui ) 12.3
Tiepl xfjc; XLVTQGSCOc; xoO alXax^ — /T^^' ^i^^' cJ ^^ ^'^^ prorogation of the
hayldj
atXaxC ( ^>Ui) 12.3.1
6 xoTioc; xfjc; xuxTjc; 6 xsXsloc; xoO alXdx^ — jL^a^l /T^^' ^Ua^ the resulting
rising time of the hayldj
atXaxC ( r%:k\) 12.3.1
x6 ^fjxoc; xoO alXdx^ olko xoO xevxpou
— JJ^I j^ /T^W^' -^ distance of the hayldj from the cardine
atXaxC ( ) 12.3.1
si he x6 alXdx^ [xeaov eaxl xcov 8uo xevxpcov — XjMI (jju jlS^ lil if it is
between the cardines
166
alXax^ ( ) 12.3.2
f) \xoipa ToO [ispouQ ToO aiXdxC — «Lo.4*i!l ^^yi location of the division
alXax^ ( ) 12.3.2
f) \xoipa eic, f]v xivstrai to alXdxC — io_^l ^^yo location of the division
diXoLT^ ( r->ai ) 12.3.2
ToO [jiepLa^iGU Tf]C, \ioipac, xou alXaxC — /T^^' iV* io-^l the division of the
haylaj
AlXouX ( J^J ) 1.1
AlXouX — jy^l Elul
alaGrjTOc; ( ) 12.1.1
Twv xpovcov Twv ala6T)TWv oXwv — jUI |^_^ years of the world
dxpov ( ) 2.2.1
sic; TO dxpov xfjc; dpxfjc; — ^yJa}\ i-U- ^^a^ ^j in the column of the numbers
of arcs
dxpov ( c^Ja5 ) 9.1.1
ToO Tojiou Ttov dxpcov Tf)(; acpatpac; xtov C^oSicov — /Tj-'i^' '^ (wJas the poles
of the sphere of the zodiacal signs
dxTLVopoXia ( ) 12.2.4
xdc; y dxxivopoXiac; xdq e'E, be^i&v — ^.^^ dexter (rays)
167
dxTLVopoXta ( f U^i ) 12.2.4
xac; y dxTLVopoXtac; xoO daxepoc; fjyouv xouc; xpsLc; axTj^axLa^ouc;
— ^r^.^1 pUJJI sinister ray
aXTL^ {jy^\) 11.2
a xo^ov xoO xatpoO exepov xcov dxxLvcov dXXo xfjc; dvapdaecoc; xal exepov
xo^ov xfjc; xaxapdaecoc;
— Jtf»lia^Mlj pUjjMIj JU5CIIj jyi\ ryy the arc of light; of duration; of altitude
and of declivity
'AXs^oivSprjvoc; ( J\jXs^>l\ jjl: ) 9.2
6 Bapdv exsLvoc; 6 AXe^avSprivoc; — ^(jXiC^^^I jjb^ Theon of Alexandria
dXXrjXouxta (J^ ) 8.3.1; 8.3.2
x/jv a xal P' dXXrjXouxLocv — :>AjJI ^^ia^ column of numbers
dvdpaaLc; ( ^j ) 1.3.4
dvdpaaLc; xcov xp^vcov xal xcov ^rivcov. — ijJt^S W'-^ iJlua^l ^^.^^ ^j ^
on the raising of the days summarized in years and months
dvdpaatc; ( 9\^j\ ) 3.1
xfjc; dvapdaecoc; xoO fiXlou sic; xov xuxXov xoO ^eaou xfjc; fj^epac; —
jlyJl cJLuaj 5yl:> ^ j^usJJl 9'^j^ '^^ limit of the altitude of the sun on the circle
of half the day
dvdpaatc; <^jyu^\ ) 3.1
168
dvdpaaLc; — jyi^] ascending
dvdpaat^ ( p liJjMi ) 3.3
dvdpaaLc; eaui xoO tiXlou y] toO daxepoc; — j^U' ♦^^^-^^ ^ f-UjjMI ijU- limit
of the altitude from the zenith
dvdpaaLc; ( <j^[juj\ ) 5.2
xfjc; ea^dxric; dvapdaecoc; — 4^Lfljjl ijU limit of its altitude
dvdpaaLc; ( pliJjMI ) 6.1.1
dvdpaaLc; xoO daxepoc; — SyljJl ^ plijjMI altitude from the circle
dvdpaaLc; ( ^^J ) 6.1.3
xfjc; dvapdaecoc; xoO xatpoO — c^S^I ^^j' altitude of the time
dvdpaaLc; ( ^^J ) 6.1.3
xfjc; dvapdaecoc; xoO ^eaou xuxXou xfjc; fj^epac; — jV^' cJLuaj ^li^jl altitude
of half the day
dvdpaaLc; ( ^[juj ) 6.5.2
xfjc; dvapdaecoc; — P UjjI altitude
dvdpaaLc; ( apL^ ) 8.3.1
dvdpaaLc; — A^L^ increasing
dvdpaaLc; ( ^i^^^uaJl ) 8.3.4
eiiei he xp2:La slSevaL x/jv dvdpaatv xal xaxdpaatv — ^yi^] ascending
169
dvdpaaLc; ( apL^ ) 8.3.4
dvdpaaLc; soti toO TiXdxouc; — 'ti A^L^ ^.^^^501 the star is ascending in it
dvdpaaLc; ( apL^ ) 8.3.4
si he eXaxTOV dvdpaaLc; — 'ti A^L^ jj^ it is increasing in it
dvdpaatc; ( apL^ ) 8.3.4
f) dvdpaaLc; voxta — c-;j-^l ^ A^L^ j-to it is increasing in the south
dvdpaaLc; ( ^^J ) 9.1.1
xfjc; dvapdaecoc; xoO xotiou xcov dxpcov xfjc; acpatpac; xcov ^coSlcov fjyouv xcov
dxpcov xfjc; xepxtSoc; 8l' fjc; XLVSLxaL f) acpatpa — /TJ^' ^^ c-JaS ^li^jl altitude of
the pole of the sphere of the zodiacal signs
dvdpaaLc; ( ^^J ) 9.1.1
xfjc; dvapdaecoc; xoO i olxiQ^axoc; xfjc; Tuyjiq xoO xatpoO — c^Sj^ll ^U ^^j\
altitude of the tenth of time (nonagesimal)
dvdpaaLc; ( ) 9.1.1
f) xpaxTjXaLa f) xexeXsLCO^evr) xfjc; dvapdaecoc; xou xotiou xcov dxpcov xfjc; xepxtSoc;
— '^^^J\ ^\ j^j^ ^^ V^ ^^^^ of the complement of the latitude of the place of
observation
dvdpaaL^ ( ^[juJ ) 9.1.1; 9.1.3
f) dvdpaaLc; eaxL xoO xotiou xcov dxpcov — /TJ^' ^^ c-JaS ^^j\ altitude
of the pole of the sphere of the zodiacal signs
170
dvdpaaLc; ( ^[juj ) 9.1.2
xfjc; dvapdaecoc; otac; pouXo^sGa ^OLpac; — Ju^y <^j^ '^} t^J^ altitude of
whatever degree we wish
dvdpaaLc; ( ^^J ) 9.1.2
xfjc; dvapdaecoc; xfjc; aeXrivriq fivLxa TiXdxoc; oOx exTl
— c-^^^^L j^j^ <) 03^. i 1->1 ^r«^l t^J^ the altitude of the moon when it has
no latitude approximately
dvdpaatc; ( ^^J ) 9.1.3
f) dvdpaoLc; sgxlv — ^^j' jIaIo measure of altitude
dvdpaatc; ( f li^ji ) 9.1.3
f) dvdpaoLc; xoO xotiou xcov dxpcov — /TJ^' ^^ c-JaS ^li'jl jIaIo measure
of the altitude of the pole of the sphere of the zodiacal signs
dvdpaatc; ( ^[juj ) 9.1.4
xfjc; xexeXsLCO^evrjc; dvapdaecoc; xoO tiXlou xal xfjc; aeXTQvric;
— jAJii\^ j^usJJl ^l^jl j»Lr complement of the altitude of the sun and moon
dvdpaatc; ( cu^ ) 9.2.5
xax' evavxLov xoO lSlou xfjc; aeXrivriq y] xfjc; dvapdaecoc; xauxTjc; — ^^1 C/^.
the daily velocity of the moon
dvdpaatc; {jy^ ) 9.2.5
xd xavovLa y] xoO lSlou y] xfjc; dvapdaecoc; xfjc; aeXTQvric; — ^jd^' ^i-^^ Jj^
171
table of the motions of the two luminaries
dvapdatc; ( ^^J ) 9.3.1
xfjc; dvapdaecoc; xoO l' OLXTQ^axoc; xfjc; Tuyjiq xoO xatpoO — ^LJI i^j^ ^^j'
altitude of the degree of the tenth
dvdpaat^ ( ^[juJ ) 10.3.2.1
f) dvdpaaLc; xfjc; aeXTQvric; — c-^^^^L ^^1 pUjjI jj^j pUi^^-MI ty*- ^^j' alti-
tude of the degree of the conjunction and it is the altitude of the moon approximately
dvdpaat^ ( ^J) 10.3.2.1
f) dvdpaoLc; xoO i olxiQ^axoc; — ^^jb ^^d its (the tenth's) altitude
dvdpaat^ ( f liJji ) 11.1.7
x/jv ea^dxriv dvdpaatv xfjc; SLa^expou xfjc; ^otpac; xoO tiXlou
— j^ujJJl ty>- jiJaj ^^j\ 'i}^ limit of the altitude of the opposite point of the
degree of the sun
dvdpaatc; ( ^pliuji ) 11.1.8
f) dvdpaoLc; xfjc; aeXrivriq fjVLxa vea cpavfj — 4^lijjl its altitude
dvdpaatc; ( ^[juj ) 11.1.8
f) ea^dxT) dvdpaoLc; xfjc; aeXTQvric; — ^^j' ^1^ limit of the altitude
dvdpaatc; ( f liiji ) 11.1.8
f) ea^dxT) dvdpaoLc; xfjc; ^otpac; xfjc; aeXTQvric; — ^"j-^ ^^j' h^ limit of the
altitude of the degree
172
dvdpaaLc; ( ^[juj ) 11.1.8
xfjc; dvapdaecoc; xfjc; aeXTQvric; ^exd xriv Suglv xoO tiXlou
— j^usJJl c-^wJl^ X^ ^^I t^J^ altitude of the moon at the setting of the sun
dvdpaat^ ( p liJjMi ) 11.2
a To^ov xoO xatpoO exepov xcov dxxLvcov dXXo xfjc; dvapdaecoc; xal exepov
xo^ov xfjc; xaxapdaecoc;
— Jtf»lia^Mlj pUjjMIj JU5Cilj jyi\ ryy the arc of light; of duration; of altitude
and of declivity
dvdpaat^ ( J^IWI) 11.2.1
x6 To'E.ov xfjc; dvapdaecoc; xoO tiXlou — j^ujJJl J^^Lia^'l j^^ arc of the de-
clivity of the sun
dvdpaatc; ( ^^J) 11.2.1
x6 TO^ov xfjc; dvapdaecoc; xfjc; aeXrivriq — jA2i\ ^^j\ ^y arc of the altitude
of the moon
dvdpaatc; ( f liiji) 11.4
dvdpaaLc; xfjc; aeXTQvric; — ^^1 ^^j' altitude of the moon
dvdpaatc; ( f li^;^!) 11.4.1
f) dvdpaaLc; xfjc; aeXTQvric; — ^^1 ^^j' altitude of the moon
dvdpaat^ ( iajUi ) 12.2
^£XP^ ^^'^ "^^^ ^'"^^ fj^LGU SGXL xfjc; OLVOL^OLOeCdC,
173
— iajlAI cJLuaJl the descending half
dvdpaaLc; ( apLJI ) 12.2
^£XP^ ^^'^ "^^^ TSTdpTOU YJ^LGU soTL xfjc; dvapdascoc; — A^LaJl cJLuaJl the
ascending half
dvdpaat^ ( apLJI ) 12.2.4
TO YJ^LGU xfjc; dvapdaecoc; xfjc; acpatpac; — A^LaJl cJLuaJl the rising half
dvapLpdCcov (y^j^l) 8.1.2
f) ^ear) XLvrjaLc; xoO dvapLpd^ovxoc; — ytij^\ Ja^j mean (motion) of the
node
dvapLpdCcov ( c^JJI) 8.1.3
xoO dvaptpd^ovxoc; — c-^jJl tail (node)
dvapLpdCcov (y^j^l) 8.3.1
f) [xeari XLvrjaLc; xoO dvapLpd^ovxoc; — ^j^l Ja^j mean (motion) of the
node
dvapLpdCcov ( ^1^1) 10.3.2
x6 aOGrj^epLvov xoO dvapLpd^ovxoc; — lT^J^ f y^ true position of the head
(node)
dvdXr)(];Lc; ( a^UjI ) 1.5.3
dvdXrjcJ^Lc; — ^LiJl resurrection
174
OLVOLToXri ( Jj^ ) 10.3.2
TO \xepoc, TTJc; dvaToXfjc; — ijj^ eastern
dvaxoXT^ ( [JJ, ) 10.3.2.1
zic; TO iiipoc, Tf]C, dvaToXf)(; — ^j-^ eastern
dvSTSlXsV ( OoJlip ) 1.2
dviTZikev 6 f^Xiot; — j^oJJl OjJlL? the sun rises
dviaxsL ( ^_^ ) 4.1
dvioy^ei — P" .3^ rising
dviaxsL ( <S^^ ) 5.5
oxav dviaxei xal 5uvr] — "^^J^J 's-^iSo oUjI ^^ in the times of its rising
and its setting
dviaxsL ( ^^ ) 11.5
ToO TO^ou Tf]<; xaxapdaecix; xoO fiXtou £L(; tov xaipov fivtxa 8uvt) 6 daxfip f]
dviaxT]
the arcs of the declivity of the sun at the time of the setting of the planet or its
rising which is called the arc of complete sighting
dviaxsL ( ^ ) 11-5.2
6 daxrip xaxd koIov xaipov 5uv£i xal xaxd koIov dviaxei — ^^ rise
dv63 ( ) 9.3.1
175
eav f) dvdpaaLc; xoO i olxTQ^axoc; dvco oOaa xfjc; xecpaXfjc; fj^cov voxta x6 tiXsov
xal eXaxxov xfjc; ocj^ecoc; xoO TiXdxouc; sic; x6 voxlov ^epoc;
we measure it (the parallax) by the altitude of the degree of the tenth. If it is
northerly from the zenith it (the parallax) is northerly. If it is southerly (from the
zenith) it (the parallax) is southerly
^Ati (c^Mi) 1.1
'Ati —^^\ al-Ab
dTioxaGLaTaxaL ( .>U'Mi) 10.2.1.5
f) xexeXsLCO^evT) oSpa xa6' y]v djioxaGLaxaxaL f) aeXTQvr) — t>L:^''^l >Lr ol^Lu
hours of the completion of the clearing
dTioxaxdaTaaLc; ( 5>^ ) 1.1
diioxaxdaxaaLc; — 'S^y^ return
dTioxaxdaTaaLc; ( f>U'Mi ) 10.2.1.4
f) oSpa xfjc; xeXe Lac; djioxaxaaxdaecoc; xfjc; aeXTQvric; — t>U^MI >Lr ol^Lu hours
of the completion of the clearing
dTioxaxdaxaaLc; ( f>U'Mi ) 10.2.1.5
oSpa eaxlv duo xfjc; dp^fjc; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; ^£XP^ '^^^ xeXetac;
diioxaxaaxdaecoc;
— t^U^'^l >Lr Jl tljJl /^ l3j-^I t ^3 ol^Lu hours of the occurrence of the
176
eclipse from the beginning to the completion of the clearing
dTioxaxdaTaaLc; ( f>U'Mi ) 10.2.1.5
hours of the beginning of the clearing
d7iCL)X£La ( ^>U ) 1.2
dcTiciXsLa xoa^ou — ^1 ^>U destruction of the world
dpLGTSpoc; (^^Mi) 12.2.3
6 TOTioc; eaxl xoO cpcoxoc; xoO e^aycivou xoO daxepoc; e'E, dpLaxepcov
— ^r^.^1 4^ .uJ jy ^yi the location of the illumination of its sinister sextile
dpLGTSpoc; (^^Mi) 12.2.4
xdc; y dxxLvopoXLac; xoO daxepoc; fjyouv xouc; xpsLc; axTj^axLa^ouc;
— j^^\ f UJJI sinister rays (aspects)
dpLGTSpo^ [j^^\) 12,2 A
x6 dpLGxepov xptycovov — ^H.^' JUitJl sinister trine
dpLGTSpoc; (^^Mi) 12.2.4
x6 dpLGxepov xexpdycovov — ^H.^' A^^' sinister quartile
dpLGTSpoc; (^^Mi) 12.2.4
x6 dpLGxepov e^dycovov — ^r*^.^' j^J^^I sinister sextile
dpxaioc; ( Oi^Aiill ) 2.2
177
ol dpxaioi exeivoi — (j^^^AZdl the predecessors
&9XA ( J3"^l ) 1-1
apx^O ( ^^^ ) 1-2
yjXloc; £c; xriv apx^Q^ "^^^O KptoO — ^5*:^^' JljI^MI iiaU j^usJJl cJi^ the sun
came to the point of the Spring equinox
o^PX^ ( >-^ ) 1-4
xfjc; xaxaXiQcJ^ecoc; xfjc; ocpx'^^ "^^^ XP^^^^ ^^'^ "^^^ ^tjvcov xouxcov xcov excov
xaxa TioLav fj^epav slaepxovxaL xfjc; fepSo^dSoc; — ^LuMI >U ^ jj-pJl J^Xo on
the entrance of the months in days of the week
apxr] ( ^ ) 1-4.1
f) dpxTQ '^c)^ xp6^<^^ — ^^^' ^>^Ilio beginning of the year
dpx>l (J30 4.4
xfjc; ocpxfjc; xoO KptoO sic; xd ^opeioL Z^cdhia — <JUJJI r^y^\ ^ J^' Jj' 0^
from the beginning of Aries in the northern zodiacal signs
apx^O ( ^"^^^^ ) 7.3.1
f) dpxT) xoO -/^povou — iL^I ?JIio beginning of the year
^9X^ (crL)7-4
£Lc; x/jv dpxTjv exdaxou ^rivoc; 6 yjXloc; slc; x/jv dpxTjv ytvexaL xoO ^coSlou
— ry- U^^J ^ J^ <f^J cJ J^' j^usJJl the sun alights at the beginning of every
178
month at the beginning of a zodiacal sign
apx-f] ( ) 9.1.3
£Lc; xriv dpxTjv ToO KpLoO y] ToO ZuyoO — (JjJIjIpMI ^Wg> ^u-J^j^j its location
is one of the two equinoctial points
apxri ( ) 9.1.3
xriv dpxTjv ToO KapxLvou y] ToO 'ALyoxepcoxoc; — (jju^luMI iiaU ^^s>\ ^ji^ya
its location is one of the two solstitial points
eiq xriv dpxiQ^ fexdaxou ^coSlou — /TJ^' lTJj cJ ^^ ^'^^ beginnings of the
zodiacal signs
^PX>1 (ctL) 9-2-3
xriv dpxTjv xoO ^coSlou — /T^' ^-^ j^L) cJ ^^ ^'^^ beginning of that zodiacal
sign
dpx>l ( ^^ ) 10.2.1.4
oSpa xfjc; dpxfjc; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; — lJ^^^\ t\ju ol^Lu hours of
the beginning of the eclipse
dpx>l ( ^^ ) 10.2.1.5
oSpa eaxlv duo xfjc; dp^fjc; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; ^£XP^ '^^^ xeXetac;
diioxaxaaxdaecoc;
— t>L:^MI >Lr Jl tIjJl j^ l3j-^I t y^ ol^Lu hours of the occurrence of the
eclipse from the beginning to the completion of the clearing
179
dpx>l ( ^^ ) 10.2.1.5
hours of the beginning of the clearing
dpx>l ( ^^ ) 10.2.1.5
dpxT) xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; — l3j-^I tijj ol^Lu hours of the begin-
ning of the eclipse
'H^SLc; xavovLov eGiQxa^ev xal xd xo^a diiep eSo^ev xeGsLxa^ev sic; sxslvo x6
xavovLov ^£xd xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xdc; dp^dc; xcov ^coSlcov
— ^^11 ^ ^^^J^^ oU^lia^^Uj r^j^^ ^^yr^ o^ ^3^^ ^jAs> jIaSI L«^j
We have set out the values of the limits of sighting in degrees of the zodiacal
signs and for the initial declivities (we have set them out) for the fourth clime at the
beginnings of the zodiacal signs
dpx>l ( ) 11.6.1
eiq x/jv dpxTjv xfjc; vuxxoc; — j^usJJl c-^^J*^ X^ at the setting of the sun
apXTQ ( Jb' ) 12.1.1
eiq exelvov xov xatpov oxl 6 tiXloc; ytvexaL sic; x/jv dpxTjv xcov ^coSlcov —
IAjlI] r^j)i\ J^ls' j^usJJl JjjP Al^ when the sun alights upon the beginnings of
the coming zodiacal signs
dpx>l ( J3i ) 12.1.3
180
KpLoO
— J^l J3' (V r^^^l dLiiJl ^JUa^ rising time in the right sphere from the first
of Aries
daTrjp ( c^yCJi ) 1.2
[xeaoii XLVTQGSLc; xcov daxepcov — ^.^^iCJl olS^ J^^LujI mean motions of the
planets
daxrjp ( c^y^) 1.5.1
Tcov dcTiXavcov sxslvcov daxepcov — <lI^I S^3^ fixed planets
daTrjp ( ^^) 3.2.1
ToO del cpaLvovToc; daxepoc; xal ^tqtiots Suo^evou — j>^' l^-^' V^S^ ^^"
ways visible star
daTrjp ( c^yCJi ) 5.0.0
Tcov diiXavcov daxepcov — tol^l ^.^JlSCJl fixed stars
daxrjp ( 'Sj\^\ ) 8.0.0
ToO aOGrj^epLvoO Tcov £ daxepcov — SjJlp^iII c y^^ correction of the planets
daTrjp ( c^yCJi) 8.1.4
Tcov £ daxepcov — SjjLpjil L^usil ^.^^iCJl the 5 moveable stars
daTrjp ( c^iyCJi ) 8.3.2
ToO TiXaxouc; xcov daxepcov xcov dvco xoO tiXlou — Si^J^' c-^^iCJl ^^ lat-
181
itude of the superior planets
daxrjp ( ) 8.3.4
6 daxrip xfjc; ^opeioiq xaxapdaecoc; — JUJJI ^ iajU jj^ it is decreasing in
the north
daxrip ( v^y^^ ) ll-O-O
ol daxepec; tioxs tva cpavcoaL ^exd x/jv auvoSov xoO tiXlou
— lyo^j Sjiipjil c-^^iCJl ^,j^ the rising of the planets and their setting
daxrip ( v^y^^ ) 11-5
exsLVT) f) ^oLpa f) e^ep^o^evr) ^exd xoO daxepoc; xrjpeLxaL y] exsLvr) f) ^otpa f)
^£xd xoO daxepoc; Suvouaa — V^. j' c-^^iCll <jco ^iiaj ^1 i^jjJl the degree
with which the planet rises or sets
daxrip ( v^y^^ ) 11-5
Kspi xcov e TiXavco^evcov daxepcov oxl xaxd tiolov xatpov e^ep^ovxat yjxol
UTie^LGxavxaL xoO cpcoxoc; xoO tiXlou xal xaxd TioLav oSpav slaepxovxaL Otio cpcoc; xoO
tiXlou xaxd x6 Tipcot y] x/jv saTiepav — [^^jyu^ oIa^^iII ^.^^iCJl (3:i^r^' ^ on the
rising of the moveable stars (planets) and their settings
daxrip ( ) 12.0.0
xoO xoTiou xcov daxepcov — ol^L«JJl rj^ casting of the rays
daxrip ( ) 12-2
xoO xoTiou xoO cpcoxoc; xcov daxepcov yjxol xoO Tipoc; aXX/jXa xouxcov axTj^axLa^oO
— ol^LiJl rj^ casting of rays
182
daxrjp ( ^^) 12.2.1
£L hz 6 daxrip ^eaov xoO 8' xal xoO C
— «jLJIj ^Ijl C^ U^ <^^\ jlT jl if the star is between the fourth and the
seventh
daxrjp ( ) 12.2.1
^fjxoc; eaxL xoO daxepoc; duo xoO 8' — «j|JI j^ oAju its (the star's) distance
from the fourth
daxrip ( v^^O 12.2.1
xoO xoTiou xfjc; xu^TQ^ ^^^ daxepoc; — ^>il^l <^^\ ^JUa^ rising time of
the star in right ascension
daxrjp ( ^^\) 12.2.1
6 daxrip ]^zqo\ xoO \, xal xoO a olxiQ^axoc; xoO xotiou xfjc; xu^iQ^
— ^JliaJlj ^LJI (jiu UJ jIS^ jI _ <^^\ if the star is between the tenth and
the ascendant
daxrjp ( ^^\) 12.2.1
xoTioc; xfjc; xu^iQ^ '^^^ daxepoc; — ^>il^l ^^^\ ^JUa^ rising time of the
star in right ascension (A2 / in marg Al)
daxrjp ( <^^\) 12.2.1
xoO ^TQXouc; xcov daxepcov — <^^\ x»j distance of the star
daxrjp ( <^^\ ) 12.2.2
183
TO ^fjxoc; ToO daxepoc; duo xoO xevxpou xoO l' y] xoO 8'
— «j|JI jl ^LJI (^Xj j^ c-^J^5CJI Aju the distance of the star from the tenth
or fourth cardine
daTrjp ( <^^\ ) 12.2.3
x6 TiXdxoc; xoO daxepoc; — ^^^\ ^J- latitude of the planet
daTrjp ( <^^\ ) 12.2.3
x6 aOGrj^epLvov xoO daxepoc; — <^^\ ^ yoj the true position of the planet
daTrjp ( ) 12.2.3
xavovLov xoSe xcov axTj^axLa^cov xcov daxepcov
— j^j»i\ c-^w^ pUJJI rj^ Jj-^ table of the casting of the rays by the
calculation of latitude
daTrjp ( ^^\ ) 12.2.3
x/jv xexeXsLCO^evriv xpaxTjXaLav xoO TiXdxouc; xoO daxepoc;
— c-^y^iCJl j^j^ j»Lr c-^w^ sine of the complement of the latitude of the planet
daTrjp ( ^^\ ) 12.2.3
xoO xoTiou xoO cpcoxoc; xcov daxepcov — i^^^\ ol^Li rj^ casting of rays
of the planet
daTrjp ( c^yCJi ) 12.4.2
xoO cpcoxoc; xcov daxepcov oXcov — iJb^^^l ol^L-JJlj ^.^^iCJl ^^^^woj^ with
all the stars and the aspects of revolution
184
daxpoXdpo^ ( ^^jL^^\ ) 11.4.1
6 daxpoXdpoc; — ^^Sj^a^S] astrolabe
dacpaXrjc; ( ^^-^sk^ ) 11.1.2
xfjc; dacpaXoOc; opGciaecoc; xoO totiou xfjc; aeXrivriq — jAJii\ »^yi ?^^^p^-u2J cor-
rection of the place of the moon
dacpaXrjc; ( ^^.^sk^ ) 11.1.3
xfjc; dacpaXoOc; opGciaecoc; xoO xotiou xfjc; aeXTQvric; ^exd xfjc; opGciaecoc; xfjc;
fj^epac; — UUb j>L>^(l Ju AaL ^^1 »^yi ?^^^p^-u2J correction of the place of the moon
with the equation of days with their nights
au6r)^£pLv6v ( ^^-^sk^ ) 5.1
xoO aOGrj^epLvoO xcov daxepcov — lf«^lj^ ^^-^^"^ correction of their (the
planets') places
au6r)^£pLv6v ( i^j^ ) 5.2.1
xoO aOGrj^epLvoO xoO daxepoc; — ^.^i^iCJl <^j^ degree of the star
au6r)^£pLv6v ( a*^ ) 5.3
xoO aOGrj^epLvoO xoO daxepoc; — ^.^i^iCJl Aju distance of the star
au6r)^£pLv6v ( ^y> ) 6.3
x6 aOGrj^epLvov xoO tiXlou — j^usJJl iy> degree of the sun
au6r)^£pLv6v { r^ yu) 7.4
x6 aOGrj^epLvov xoO xaxapLpd^ovxoc; — ytijy^\ ^ yoj true position of the
185
node
TO a06T)[jiepLv6v — f y'^ true position
au0r)[ispLv6v ( r>^0 8-0.0
ToO a06T)[jiepLvou xtov daxepcov — ^3^' true position
au9r)[ji£pLv6v ( ^yo) 8.0.0
ToO aOGrj^epLvoO xoO xaxapLpd^ovToc; — j^L^' f y^ ^^^^ position of the
head (node)
au6r)^£pLv6v ( ^yu ) 8.0.0
ToO aOGrj^epLvoO xcov e daxepcov — oIa^^iII c^' true position of the
planets
au6r)^£pLv6v ( ^yu ) 8.1
ToO aOGrj^epLvoO xoO tiXlou xal xfjc; aeXr]vr](; — ^j:!^' f y^ true position
of the two luminaries
au6r)^£pLv6v (^^•) 8.1.1
ToO aOGrj^epLvoO xoO tiXlou — j^usJJl c y^^ true position of the sun
au6r)^£pLv6v (^^5^) 8.1.1
PouXo^evcov fj^cov TioLfjaaL aOGrj^epLvov xou tiXlou
— j^ujJJl j5^ c-?L^> J^' jl b:>jl lil if we wish to calculate the center of the
sun
186
au6r)^£pLv6v (^^•) 8.1.1
xal aOGic; exelvo to aOGrj^epLvov xoO tiXlou
— r^j)i\ illaLo ^ j^usJJl c yi^ true position of the sun in the zone of the
zodiacal signs
au6r)^£pLv6v (^^•) 8.1.2
TO aOGrj^epLvov xfjc; p ' acpatpac; xfjc; aeXr]vr](; — JuLlI dliiJl ^ j^\ ^ yu
true position of the moon in the inclined sphere
au6r)^£pLv6v (^^•) 8.1.2
Tcp aOGrj^epLvcp xfjc; aeXrivriq — jA2i\ ^ yij true position of the moon
au6r)^£pLv6v (^^•) 8.1.2
TO aOGrj^epLvov ToO xaxapLpd^ovTOc; — j^L^' f y^ true position of the head
(node)
au6r)^£pLv6v (^^•) 8.1.3
ToO aOGrj^epLvoO xoO xaxapLpd^ovTOc; xal xoO dvapLpd^ovxoc; —
^jJlj ^\J\ ^,yaj true positions of the head and tail (nodes)
«^/o
au6r)^£pLv6v (^^•) 8.1.3
aOGrj^epLvov xoO xaxapLpd^ovxoc; — j^L^' f y^ true position of the head
(node)
au6r)^£pLv6v (^^•) 8.1.3
aOGrj^epLvov xoO dvapLpd^ovxoc; — c-^jJl c yj true position of the tail
187
(node)
ToO a06T)[jiepLvou xtov e daxepcov — 5ji?*dll L.*oji-l ^_^_^l rj-aJ" true po-
sition of the 5 moveable stars
au9r][i£pLv6v ( r>fl^) 8.1.4
auGr][ji£pLv6v ToO daxepoc; — <_^^\ c y^ true position of the planet
au9r][i£pLv6v ( r>fl^) 8.3.1
TO aOGrj^epLvov ToO xaxapLpd^ovTOc; — j^L^' /^>^' true position of the head
(node)
au6r)^£pLv6v ( ^^•) 8.3.1
ToO aOGrj^epLvoO xfjc; aeXTQvric; — ^^1 X'^^' true position of the moon
au6r)^£pLv6v ( \^^y^ ) 9.3
TO aOGrj^epLvov — 'U^j^ its location
au6r)^£pLv6v ( ^y^ ) lO.l.l
TO aOGrj^epLvov toO tiXlou xal ttjc; ozkr\\r\<:^ eyevovTO TsXeioL [xeTOL ttjc; opGciaecoc;
TTJc; fj^epac; — V^W^ j*^.^' Jd-^ ^Iajco ^^I »^yi location of the moon corrected
with the equation of the day and its night
au6r)^£pLv6v ( ju«Ji ) lO.l.l
el he TO aOGrj^epLvov ttjc; aeXr]vr](; iikeov eoTi toO aOGrj^epLvoO toO tiXlou —
jAJi\i AjtJl jir jl if there is distance to the moon
188
au9r)[ji£pLv6v ( -uJI ) lO.l.l
sav oOv TO auGr][ji£pLv6v xfjc; asXrivT)^ IXaxxov i] xoO auGr][ji£pLvou xoO rjXiou
— j^oJJJ A*JI jlS' jl if there is distance to the sun
au0r)[i£pLv6v ( ^j*^y> ) lO.l.l
x6 au6T]^i£:piv6v xoO f)Xiou xal a£:XTJVT]<; — (ji-^' is*^y longitudes of the
two luminaries
au9r)[ji£pLv6v ( r>fl^) 10.2.2.1
xa Xeuxa xoO au6T)[i£pivou — i^_^il)l JjjUi minutes of the true position
au0r)[i£pLv6v { ^yu) 10.3.2
TO aOGrj^epLvov ToO dvapLpd^ovTOc; — lT^J^ f y^ true position of the head
(node)
au6r)^£pLv6v ( cy^) 10.3.2
TO aOGrj^epLvov — f" y^ true position
au6r)^£pLv6v ( cy^) 10.3.2.2
TO aOGrj^epLvov ToO xaTaptpd^ovTOc; — j^L^' f y^ true position of the head
(node)
au6r)^£pLv6v ( cy^\) 10.3.2.3
Td \zKiQL ToO aOGrj^epLvoO — ^ yL]\ ^^^ minutes of the true position
au6r)^£pLv6v ( ^y^ ) ll.l.l
189
aOGrj^epLvov xfjc; aeXTQvric; — yi2i\ ^ya place of the moon
au6r)^£pLv6v ( r^') ll.l.l
Elc; xriv xaxdXricJ^Lv xoO aOGrj^epLvoO xoO tiXlou xal xfjc; aeXrivriq eiq exelvov x6
xatpov oxL f) ^oLpa xoO aOGrj^epLvoO xfjc; aeXTQvric; xaxepx^xaL Suvouaa
— ^^1 ty»" V^:^*^ -^-*^ Od^' /^>^' the true position of the of the two luminaries
at the setting of the degree of the moon
au6r)^£pLv6v ( ^j^ ) 11.1.3
xoO aOGrj^epLvoO xfjc; aeXrivriq — yi2i\ »^yi place of the moon
au6r)^£pLv6v ( c^i) 11.2.1
:a XsTixa xoO aOGrj^epLvoO — ^^^1 (3^^-> minutes of true position
xa
au6r)^£pLv6v ( ) 11.6.1
FLvexaL x6 aOGrj^epLvov xoO tiXlou xal xfjc; aeXTQvric; — <jd^' ^y ^^ rectify
(the position of) the two luminaries
au6r)^£pLv6v ( ) 11.6.2
yLvexaL aOGrj^epLvov xoO tiXlou xal xfjc; aeXrivriq — (jd^' ^y ^^ rectify
(the position of) the two luminaries
au6r)^£pLv6v ( ^j^ ) 12.1
x6 aOGrj^epLvov xoO fiXlou — ^ jlilll ^ j^usJJl ^ya the position of the
sun in true positions
au6r)^£pLv6v ( ^y^ ) 12.1.1
190
eav f) ouTCOc; otl to aOGrj^epLvov xoO tiXlou tsXslov oOx eyevexo ^exa xfjc;
opGciaecoc; xfjc; fj^epac;
— lAUb j>lj^l Jd-^ lgg< j^usJJl ^«^j^ jiC J li>l if the location of the sun is
not corrected by the equation of the days with their nights
au6r)^£pLv6v ( cy^) 12.1.1
x6 aOGrj^epLvov xoO tiXlou — ^^3^' its (the sun's) true position
au6r)^£pLv6v ( cy^) 12.2.3
x6 aOGrj^epLvov xoO daxepoc; — ^.^i^iCJl ^ yu the true position of the planet
au^SL ( SjtT) 1.2
f) aeXTQvr) au^SL xal ^SLoOxaL — SJLa'^I <M^3j '^-^ multitude of their sight-
ings of the lunar crescent
dcpaLpsiiaL ( j^\ ) 2.1
dcpaLpsLxaL — \s>-\ take
dcpaLpsiiaL ( ^^ ) 2.2.2
dcpaLpoOvxaL — l^^g> we subtract
dcpaLpSLxaL ( rj^) 12.1.2
f) TiepLcpopd dcpaLpsLxaL £^ exsLvou — jlj:>MI L^ L>.^ we cast off from it
cycles
dcpatpsaLc; ( ^b ) 2.1
£V£ua£ Tipoc; dcpaLpsGLV — ^y2S)\j y (it is ) decreasing
191
dcpaLpSGLC; ( jLaiJl ) 4.2.1
xriv dcpaLpsGLV — jLaiJi subtraction
dcpaLpSGLc; ( l^iil ) 12.4.1
el XL eOpsGrj sxslvo slc; xa lP ^epL^exat fjyouv dva i^ ytvexaL xouxcov dcpaLpsGLc;
— j^ L$^^ /^*^' 0^ ^-^' ^^ ^^^^ off twelve from the result
PaG^oc; ( Oi^ ) 4.2
Tiap' £va Pa6^6v xpaxsLxaL — Oi^ ^^ ^^r^ multiply by 60 (see A pll. Line
17) first occurrence in 4.2
PaG^oc; ( o<^ ) 4.2
Tiap' £va Pa6^6v xpaxsLxaL — Oy^ ^ aM^' Lo-^ we divide the results by
60 (second occurrence in 4.2)
PaG^oc; ( Cj<^) 5.2.1
xpaxsLxaL eXaxxov evoc; paG^oO — ijw/ ^^^ L<s-^ we divide it by 60
paG^o^ ( Oil-) 6.1.3;9.1.1
d XL e^eXGr] nap' eva pa6^6v eXaxxov xpaxsLxaL — iJC^ ^ i«Lll L<s-^ we
divide the result by 60
Pa0[i6^ ( ) 6.7
d XL eOpsGrj nap' eva pa6^6v eXaxxov xpaxsLxaL — ^ ^.^^\ ^ oL<s-^ we
divide the result by the total sine
192
paG^o^ ( ) 10.3.2.3
xal el XL e^eXQj] nap' eva pa6^6v eXaxxov xpaxsLxaL. — Oy^ ^ aM^' LU-^
we divide the result by 60
paG^o^ ( ) 11.3.1
f) ozkT\\T\ veoi yevo^evT) sic; sxslvov sgxl xov pa6^6v xoO cpavfjvaL y] ou —
IfC-LHolj ^.J^^ *^>^J ij^ l}^3 oLLii^ll ^ ^ J^UI the crescent is within the limit
of uncertainty and on the edge of necessity (of seeing it) or of abstention (from seeing
it)
P6p£L0^ ( iJLc^ ) 8.3.2
PopsLov — ^y^ northern
PpaSuvSL ( oXo St ) 10.3.2.2
6 r\kioc, TsXeiov ixkz'v]^zi xal ou PpaSuvsi sv xfj £xX£1(J;£l
— aJ ^^a^ Mj ,_JSJ| l3^.^*5CJI the ecUpse is total and there is no duration to it
rdcpip Oil!) 1.5.1
rdcpip — jkjii\ al-Ghafr
YsvsGXiaXoYLxd ( jJljII ) 7.0.0
Twv ysveGXiaXoyixcov — -Uljll nativities
YsvsGXiaXoYLxd ( jJljII ) 7.2.1
xa ysveGXiaXoyixd — aJIjII nativities
YSvsGXiaXoYLxd ( jjy.i ) 12.0.0
193
Tcov yeveQXiaXoyixcdv — jJljil nativities
ysveGXtaXoyLxd (jJl3li)l2.l
Kspi xfjc; eiaeXeuaecdq xcov xpovcov oXcov xal xcov xpovcov xcov yevsGXLaXoyLXCov
— jjljllj JLJI ^^^ Jd^^" cJ ^^ ^'^^ revolution of the years of the world and
of the nativities
ysveGXtaXoyLxo^ ( ^%1\) 12.1.2
eiq x6 xavovLov xoO xotiou xfjc; Tuyjiq eiq x6 TiXdxoc; xfjc; tioXscoc; exsLvrjc; ev fj
yLvexaL xrjVLxaOxa f) ^TQxriaLc; xoO yevsGXLaXoyLXoO
— ^>m j^j^ r3^^ ^Ua^ Jj-^ (^ ill the table of rising times of the zodiacal
signs for the latitude of the nativity
ysvsGXtaXoyLxoc; ( ) 12.4.1
x6 arj^SLov xoO ^coSlou xfjc; Tuyjiq xoO Gs^eXlou xoO yevsGXLaXoyLXoO Kspi-
aaeuexaL sic; xouc; )(p6vouc; exsLvouc;
— «JliaJl 'ijy^ jl c-^y^iCJl 'ti ^M\ rj)}\ Ijy^ ^ \j ^j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
ysvsGXtaXoyLxoc; ( ^^^\) 12.4.1
o\ xexeXsLCO^evoL xpovoL xoO tiXlou o\ TiapeXGovxec; duo xoO yevsGXLaXoyLXoO
— j^^jll ^ ^\ ^ll)l OiL^I the complete years which have passed for the
native
ysvvTTjaLc; ( jJljII ) 12.1
xaxd xov xatpov fjVLxa eyevexo f) yevvrjaLc; — jJljII nativities
194
yswrjat^ ( ^>Lli ) 12.1.1
elq TO ^fjxoc; xfjc; tioXscoc; exeLvrjc; £v6a xal f) yevvrjaLc; — ->MJ»1 Jj-!^ (^ for
the longitude of the nativity
yf] ( v^ji ) 1.2
[xeyiGTOV epyov xcov xfjc; yfjc; — V^j' oLo>U j^ ioJa^ <j:>U" great occur-
rence of earthly signs
yfi ( ) 4.1
del Otio yfjv sgxlv — tliil (^-^1 always hidden
yf] ( ^^^fl ) 12.2.1
Otio yfjv — j^j^^ <^^ below the earth
yf] ( ^^^fl ) 12.2.1
UTiep yfjv — j^j^^ <Jy above the earth
ypa^^rj cf. suGsta ypa^^rj
ypa^^rj ( ia^;^ ) 6.6
xfjc; ypa^^fjc; xoO [xeaou xfjc; fj^epac; xfjc; yfjc; — jV^' cJLuaj iai- line of half
the day
ypa^^rj ( Ja:^ ) 6.6
f) ypa^^f) xoO \ieao\j xfjc; fj^epac; — j[^\ cJLuaj iai- line of half the day
195
ypa^^rj ( 1^\ ) 6.6
ypa^^T) xfjc; dvaxoXfjc; xal xfjc; Suaecoc; — JIjI^^^I Jail line of the equinoctial
points
ypa^^rj ( Ja:^ ) 6.7
xfjc; ypa^^fjc; xoO [xeaou xfjc; fj^epac; — J'jj;^' ^^ line of noon
ycovLa ( ^Ujji) 9.1.3
xcov y ycovLCOv — JiJliil ^^Jjj^' three angles
ycovLa ( ijjij ) 9.1.3
f) ycovLa xoO ^tqxouc; xexeXsLCO^evr) sic; xa 9 — u):^*^ ^\ ^^^ j^j^^ ^Ijb
the angle of latitude and its complement to 90
ycovLa ( h^\j ) 9.1.3
xal xoOxo f) ycovLa xoO TiXdxouc; — Jj^aJl h3[j single of longitude
ycovLa ( <jjij ) 9.1.3
el XL eOpsGrj ycovta xoO TiXdxouc; eaxlv xal x6 TiXiQpco^a xauxrjc; ycovla eaxl xoO
[iTiXouq — j^j^^ ^Ijb ^ngl^ of latitude
ycovLa ( h^\j ) 9.1.3
el XL eOpsGrj ycovla eaxl xoO TiXdxouc;. xal xoOxo sgxlv f) xexeXsLCO^evr) ycovla
xoO TiXdxouc; — Jj^aJl h3[j W^^j (J^^' ^Ijb V^ J^*^*^^^ the result is the sine
of the angle of latitude and its complement is the angle of longitude
ycovLa ( .Ujj ) 10.3.2.1
196
f) ycovLa ToO TiXdxouc; xal xoO ^tqxouc; — ^^Ij Jj-!^1 ^^Jjj t'^^ angles of
longitude and latitude
SdxTuXo^ ( ^[^^\) 2.2.3
Touc; SaxTuXouc; — *jL^MI fingers
SdxTuXo^ ( ^L^i) 10.2.1.3
SdxTuXoL — ^L^l fingers
SdxTuXo^ ( ^L^i) 10.2.2.1
Tcov SaxTuXcov xfjc; STiLcpavsLac; xfjc; aeXTQvric; — 4^Ja^ j^ l3j-^I /^^' digits
of the eclipse on its surface
SdxTuXo^ ( ^L^i) 10.2.2.1
exXeiKSi [xepoq xfjc; aeXrivriq oaov dvacpavrj eiq xouc; SaxxuXouc; xfjc; SLa^expou
— Ojias «jL^I j^ jjJu l3j-^I 03^. the eclipse is in the measure of the digits of
its diameter
SdxTuXo^ ( ^L^i) 10.2.2.1
ol SdxxuXoL xfjc; exXsLcJ^ecoc; — l3j-^I ^.^^ digits of the eclipse
SdxTuXo^ ( ^UMi) 10.2.2.1
ol SdxxuXoL xfjc; Ksaouariq oSpac; — Jg>j^.Jl ol^Luj «jL^MI the digits and
the hours of half-duration
SdxTuXo^ ( ^UMi) 10.3.2.3
ol SdxxuXoL xal opGcoatc; sxslvcov — UtIAjJj «jL^MI digits and their equa-
197
tion
SdxTuXo^ ( c^\ ) 11.4
Kspi ToO (J^TQcpou TOUTOU Ivoi SslxQtj f) asXT^vT) Sloc SaxTuXcov
— jL^^j J^iAl ^\ SjLiiMI ^ on the pointing out of the crescent by fingers
heix% ( SjUMI ) 11.4
Tiepl ToO (J^TQcpou TOUTOU tva SsLxQrj f) aeXTQvr) Sloc SaxxuXcov
— jL^^j J^UI Jl SjLiiMI ^ on the pointing out of the crescent by fingers
Ssxaxov {jtj^\ ) 6.4
Sexaxov — ^^^1 the tenth
helio^ ( jxMi ) 12.2.3
e^dycovov eaxL Ss^lov — J^.^' 'U^.uJ its dexter sextile
Ss^LO^ ( O^'^i ) 12.2.3
f) SLd^expoc; xouxou xptycovov sgxl Ss^lov — J^.^' JUitJl '^^.j ^^^ oppo-
site to it ( the sinister sextile ) is the dexter trine
hzlioq ( ^y\ ) 12.2.4
xdc; y axxLvopoXtac; xdc; e'E, Ss^lcov — J^.^' C^^^JJl) dexter (rays)
hzlioq ( ^^fi ) 12.2.4
x6 Se^Lov xptycovov — JUiiJl 0^^' dexter trine
hzlioq ( ^^fi ) 12.2.4
198
TO Ss^Lov Tsxpdywvov — ^.J^^ 0^"^^ dexter quartile
hzlioq ( ^^fi ) 12.2.4
TO Se^Lov e^dycovov — j^ J^^l 0^^' dexter sextile
hfiko^ (jiALlli) 1.2
SfjXaL xal [ieyiGTOLi fj^epaL — ^hLALjdl >[j\ famous days
SfjXoc; ( 'Sjy^\ ) 1.2
al SfjXaL fj^epaL — Sj^y^JII (O^^Jj their famous days
SfjXoc; ( 'Sjy^\ ) 1.2
xd STT) SfjXa — Sjjyiil ^ jl^^l famous epochs
Std^STpoc; {Jos ) 2.2
xriv Std^STpov — ^^ diameter
Std^STpoc; ( jikj ) 5.5
^eaov ToO tiXlou xal xfjc; SLa^expou TOUTOU — UjjJaj Jl j^usJJl <^j^ Oj^ UJ
in what is between the degree of the sun up to its opposite point
Std^STpoc; {Jos ) 8.4
xfjc; SLa^expou toutcov — U^^^^ their diameters
Std^STpoc; ( Jos ) 8.4.1
xriv SLd^expov xoO tiXlou — Ia^ its (the sun's) diameter
199
Std^STpoc; ( J^ ) 8.4.2
xfjc; SLa^expou xoO axLda^axoc; — JJaJl Ja3 diameter of the shadow
Std^STpo^ (jliaSMi) 8.4.3
xfjc; SLa^expou xouxcov — jliaSMI the diameters
Std^STpoc; (Jfi5) 8.4.3
Std^expoc; sgxl xoO axLda^axoc; xeXeta — JajJI JJaJl ^^ the equated di-
ameter of the shadow
Std^STpOC; ( Cj^\JuJ^\ ) 10.1
xfjc; auvoSou xoO tiXlou xal xfjc; ozkr^tf, xal xfjc; SLa^expou xouxcov xal xoO
^TQXouc; xfjc; xouxcov ^exapdaecoc;
— C/Y^lj AjcJL o^^Lfil^^^lj oU-Ul>^ll conjunctions and oppositions in dis-
tance and daily velocity
Std^STpo^ ( JLiiu^Mi ) 10.1.1
xaxd auvoSov f\ xoltol Std^expov — JLil^MI opposition
Std^STpo^ ( JLiiu^Mi ) 10.2.1.1
Std^expoc; tiXlou xal aeXrivriq — JLil^MI opposition
Std^STpO^ ( J^) 10.2.1.2
f) Std^expoc; xoO tiXlou xal xfjc; aeXrivriq xal x6 axlaa^a
— JLil^^^l CC/^j) J^b j^^ L$j^ the diameters of the moon and the shadow
(at the time of) opposition
200
Std^STpo^ ( J^) 10.2.1.3
TTJ SLa^expcp xfjc; aeXTQvric; — yi2i\ Ja3 diameter of the moon
Std^STpo^ ( JLiiu^Mi ) 10.2.1.4
oSpa xfjc; SLa^expou — JLil^MI ol^Lu hours of opposition
Std^STpo^ ( JLiiu^Mi ) 10.2.1.5
d)paL SLGL xfjc; axdaecoc; — JLil^MI ol^Lu hours of opposition
Std^STpoc; ( Lij-uJti ) 10.2.2.1
x6 xavovLov xfjc; SLa^expou xfjc; ozkr^tf, — ^j^^ l3j-^I Jj-^ table of
the lunar eclipse
Std^STpO^ ( J^) 10.2.2.1
exXsLTiSL ^epoc; xfjc; aeXTQvric; oaov dvacpavfj sic; xouc; SaxxuXouc; xfjc; SLa^expou
— 0^^ fJ\jJ\ ^ jAij l3j-^I 03^. the eclipse is in the measure of the digits of
its diameter
Std^STpoc; ( cij-uJli ) 10.2.2.1
xov xatpov xfjc; SLa^expou tiXlou xal ozkr^tf, — l3j-^I Ja^j middle of the
eclipse
Std^STpoc; (Jfi5) 10.3.2
f) Std^expoc; xfjc; ozkr^tf, — ^^1 Jas the moon's diameter
Std^STpoc; (Jfi5) 10.3.2
f) Std^expoc; xoO tiXlou — j^ujJJl Job diameter of the sun
201
Std^STpo^ ij^) 10.3.2.2
YJ^LGU XeyexaL xcov p Sta^expcov — jjjiali] cJLuaj half of the two diameters
Std^STpo^ (J^O 10.3.2.2
f) SLd^expoc; xoO tiXlou svoOxaL xrj SLa^expcp xfjc; aeXTQvric;
— ^^Ij j^usJJl ^j^ Lit^ we add the diameters of the sun and the moon
Std^STpO^ ( J^ ) 10.3.2.3
xal oOxoL ol SdxxuXoL Std^expoc; xoO tiXlou ytvovxaL — j^ diameter
Std^STpoc; ( jikj ) 11.1.7
x/jv eaxdxriv dvdpaaLV xfjc; SLa^expou xfjc; ^otpac; xoO tiXlou
— j^usJJl ty>- jjJaj ^li^jl 'ij}^ limit of the altitude of the opposite point of the
degree of the sun
Std^STpoc; ( ) 12.1.1
£Lc; x/jv Std^expov xal auvoSov tiXlou xal aeXrivriq — ol^Ul^MI ^ in the
case of conjunctions
Std^STpo^ ( <Llij ) 12.2.3
f) Std^expoc; xouxou xplycovov sgxl Ss^lov — J^.^' JUJltJl '^^.J ^^d oppo-
site to it ( the sinister sextile ) is the dexter trine
Std^STpoc; ( o>l^llo ) 12.2.3
f) Std^expoc; sxslvou aOGic; xexpdycovov — o^^jI^ opposites
202
Std^STpo^ ( ) 12.2.3
f) SLd^expoc; exeivou xptycovov
— JUitJl ^y M^iis^Ci 0^L«-^' ^J-^ Cj^.-^-^0 ^^-^j we add it (the sextile) to 90
and the sum is the arc of trine
Std^STpoc; ( jikj ) 12.2.4
6 TOTioc; xfjc; SLa^expou xfjc; ^otpac; xoO aOGrj^epLvoO xoO daxepoc; — ojjJaj ^JUa^
rising time of its opposite point
Std^STpO^ {J[]hJ ) 12.2.4
Std^expoc; sgxl xoO cpcoxoc; xoO daxepoc; — ol^L«JJl y[iaj the opposite points
of the rays (aspects)
Std^STpoc; ( jikj ) 12.2.4
x6v xoTiov xfjc; xuxtjc; xfjc; SLa^expou xoO daxepoc; — '^j^ ^?^ ^Ua^ the
rising time of the opposite point of its degree
Std^STpoc; ( jikj ) 12.3.1
xfjc; SaL^expou — j\^aj opposite point
Std^STpoc; (jikJi ) 12.3.1
6 xoTioc; xfjc; xu^iQ^ '^^^ SLa^expou exeivou — jiJaJl ^JUa^ rising time of the
opposite point
Std^STpoc; ( jikj ) 12.3.2
Std^expoc; — j\^ opposite point
203
Sta^STpcov ( JLiiu^Mi ) 10.1.1
Sta^expcov — JLZL^MI opposition
StdaTaaLc; ( a*^ ) 4.1
f) SLdaxaaLc; — Aju distance
StdaTaaLc; ( a*^ ) 5.0.0
xfjc; hioLGTOiaecdq sxslvcov olko toO xuxXou toO xaxa to vu^QiQ^epov xlvou^svou
— jV^' Jajco j^ :>UjI distances from the equalizer of the day
SLTiXaatdCsTaL ( I'Jl^-j^J ) 1.2
SLTiXaaLd^exaL — Li«^l we double (IV)
huikOLGlOLoQfl ( cJl«^ ) 4.2
huikoLGioLaQfi — ULiitJ? we double it
5U£L ( ^^J- ) 4.1
8u£L — VJ^ setting
5ur) ( c^vj^) 11.4
oxav 8ur] 6 yjXloc; — j^usJJl c-^^Jl^ Aju after the setting of the sun
SOvat ( c^vJi^ ) 11.3.1
f) aeXTQvr) OTie^eaxri xoO cpcoxoc; xoO tiXlou xal Tipo xoO SOvat xov yjXlov cpatvexaL
auxT)
— j^usJJl c-^wJl^ JuS IjL^ (^^^ jl 0"^^^ pL«JJl j^ J^' j^ the crescent has come
into view from under the (sun's) rays and it is possible to see it in daylight before
204
the setting of the sun
SUVSL ( ^^i) 11.5.2
6 doTTip xaxa nolov xaipbv Suvei xal xaxa jioiov dvtaxei — t^^^' disappear
SUVTJ ( Cj^wJ^ ) 11.3
£L(; Tov xaipov exeivov f)vixa 8uvt) f) aeXTJVT] — ^^1 ^_,vJc« X^ at the time
of the setting of the moon
5uvr) ( c^w.^ ) 11.5
ToO To^ou xfjc; xaxapdaswc; xoO rjXiou sic; xov xaipov rjvixa 6uvt) 6 daxT)p f]
dviaxT]
the arc of the declivity of the sun at the time of the setting of the planet or its rising
which is called the complete arc of sighting
5uvr) ( ,[ju^^ ) 11.5.1
£L 8' eaxlv oOxoc; 6 (J;fjcpoc; tva 8uvr] 6 daxTQp — tUli">U J^\ jlS^ jU if the
computation is for the disappearance
5uvr) ( .liLi^Mi) 11.5.1
oxav cpavrj 6 daxrip xal oxav Suvr] — tUli-Mlj jj^gWII appearance and dis-
appearance
5uvr) ( v-iuo) 11.6.2
oxav SuvT) f) aeXr]vr] — yJii\ c^>^ Al^ at the setting of the moon
205
Suvouaa ( ^..vjuo ) 11.1.1
Elc; xriv xaxdXricJ^Lv xoO aOGrj^epLvoO xoO tiXlou xal xfjc; aeXTQvric; sic; sxslvov x6
xatpov oxL f) ^oLpa xoO aOGrj^epLvoO xfjc; aeXTQvric; xaxepx^xaL Suvouaa
— ^^1 ty»" V^:^*^ ^^^ Od^' /^>^' ^'^^ ^^^^ position of the two luminaries at
the setting of the degree of the moon
Suvouaa ( ^ju^ ) 11.5
exsLVT) f) ^oLpa f) e^ep^o^evr) ^exa xoO daxepoc; xrjpeLxaL y] exsLvr) f) ^otpa f)
^£xd xoO daxepoc; Suvouaa — V^. j' c-^^jiCJl ^u^ ^iiaj ^1 i^jjJl the degree
with which rises the planet or sets
SUGLC; ( ^^J^ ) 1.1
SuGLc; xoO tiXlou — j^usJJl <^^j^ setting of the
sun
SUGL^ ( J> ) 10-3.2
x6 ^epoc; xfjc; Suaecoc; — ^ji western
SUGL^ ( L>) 10.3.2.1
£Lc; x6 ^epoc; xfjc; Suaecoc; — L^ western
SUGL^ ( ^vJ^) 11.1.6
Ilepl xoO xo^ou £X£Lvou xal xoO xatpoO oxl eaxlv buep yfjv f) aeXTQvr) ^exd x/jv
SuGLv xoO tiXlou
— j^usJJl c-^wJLo Aju ^j^l 3y JU5Cil j^^S arc of duration above the earth af-
ter the setting of the sun
SUGL^ ( ^vJ^) 11.1.8
206
xfjc; dvapdaecoc; xfjc; aeXTQvric; ^exd xriv Suglv xoO tiXlou
— j^usJJl c-^wJl^ X^ ^^I ^^j' altitude of the moon at the setting of the sun
syyu^ ( ) 3.2.1
oxav UTiapxT) syyuc; — J^^lia^ I declivity
syyuTSpov ( c-^yl ) 1.4.2
(J;fjcpoc; eyyuxepov — v^' closest
sSuvsv ( ^^i) 11.5.1
6 daxrip eSuvev — ^5^^' ^ it has already disappeared
sGrjxa^sv ( Il«^j ) 11.5.1
'H^SLc; xavovLov eGiQxa^ev xal xd xo^a omep eho\iev xeGsLxa^ev sic; exelvo x6
xavovLov ^£xd xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xdc; dp^dc; xcov ^coSlcov
— ^^11 ^ ^^^J^^ oU^lia^^Uj /TJ^^ ^!>^^ 0^ '^'^J^ ^jAs> jljil LitJpj
We have set out the values of the limits of sighting in degrees of the zodiacal signs
and for the initial declivities in the fourth clime at the beginnings of the zodiacal
signs
zlozXzyjGic, ( ) 1.2
f) eiaeXeuaiq xoO tiXlou eiq xov Kptov
— J^l ^ <^-> Jj' ^ j^ujJJl the sun is in the first degree of Aries
zlozXzyjoic, ( Jl^" ) 1.2
f) eiaeXexjGic, xoO tiXlou sic, xov Kptov
207
— ^5*^^' JIjI^^^I 'iialj j^ujJJl Jl^" jI when the sun enters the point of the
Spring equinox
zlozXzyjGic, ( ) 1.4.1
ehoi xax' evavTLov xcov xaxaXsLcpGevxcov yLvexaL eiaeXeuaiq eiq xa xavovta —
4jj^ ^ <JUI LJdtf* we seek the result in its table
zlozXzyjoic, ( J^^ ) 2.2.1
yLvexaL elaeXeuaLc; — \:^£>^ we enter
SLasXsuaLc; ( JujUdl ) 7.0.0
xfjc; eiaeXeuaecdq — JujU^l)! revolution
zlozXzyjoic, ( J^-> ) 7.0.0
xfjc; eiaeXeuaecdq xcov aouXxavLXCov y^povcdv — ^JiiaLJl j^LiOl ^J^^ dy^^
the beginning of the sultanic intercalary years
zlozXzyjGic, ( J^xo ) 7.3
xfjc; SLaeXeuaecoc; — Jci-Xo entrance
SLasXsuat^ ( Ju^" ) 12.0.0
xfjc; eiaeXeuaecdq xcov xpovcov — JLJI ^^^u^ Jd^^" revolution of the years of
the world
zlozXzyjGic, ( Ji^" ) 12.1
Tiepl xfjc; SLaeXeuaecoc; xcov xpovcov oXcov xal xcov xpovcov xcov yevsGXLaXoyLXCov
— -^JljJ^lj iLJl ^J^ Jd3^" cJ ^^ ^'^^ revolution of the years of the world and
208
of the nativities
SLasXsuaLc; ( Ju^^l ) 12.1.1
al &>poii xfjc; eiaeXeuaecdq olko xfjc; fj^epac; y] xfjc; vuxxoc;
— jL^ jl JJ ^ Jjy>Ci\ CaSj ol^Lu hours of the time of turning of night or
day
SLasXsuaLc; ( Ju^" ) 12.1.1
oSpa eaxl xfjc; eiaeXeuaecdq — J:! 3^" ol^Lu hours of turning
SLasXsuaLc; ( Ju^" ) 12.1.1
Kspi xfjc; expoXfjc; xcov (bpcov xfjc; elaeXeijaecoc; xcov xpovcov oXcov —
JLJI ^^^u^ Jd^^" olSjl ry>^^^\ ^ on the extraction of the times of the revolutions
of the years of the world
SLasXsuaLc; ( Ju^^l ) 12.1.2
f) oSpa xfjc; SLaeXeuaecoc; — Ju^^^l C^Sj ol^Lu hours of the time of the
revolution
SLasXsuaLc; ( Ju^^l ) 12.1.2
Tiepl xfjc; SLaeXeuaecoc; xoO xotiou xfjc; i\)jr\^ — Jd>^' /^^ Isj^Ji ^ on the
knowledge of the ascendant of the revolution
SLasXsuaLc; ( Ju^" ) 12.4.2
f) ^OLpa xfjc; xu^TQ^ "^"H^ SLaeXeuaecoc; — iL^I Jd^^" ^UaJl i^j^ degree of
the ascendant of the revolution of the year
209
SLasXsuaLc; ( Ju^" ) 12.4.2
Tiepl xfjc; XLVTQGSCoc; xcov (J;7]cpcov xfjc; xuxiQ^ "^"H^ elaeXeuaecoc;
— iL^I Jd3^" ^^-^^ ^Oi^^' cJ ^^ ^'^^ motion of the indicators of the revolution
of the year
zlozXzyjGic, ( ) 12.4.3
Tiepl xfjc; eXdaecoc; xfjc; xuxtjc; xfjc; elaeXeuaecoc; xoO ^rivoc;
— ^y^\ ^i^^j jjt^' J:! 3^" cJ ^^ ^'^^ revolution of the months and the motion
of their indicators
zlozXzyjGlC, ( Jj^y^' ) 12.4.4
6 xoTioc; xfjc; xuxTjc; xfjc; elaeXeuaecdq — iL^I Jd3^" /^^ ascendant of the
revolution of the year
zlozXzyjoic, ( Ji^" ) 12.4.4
Kspi xfjc; eXdaecoc; xfjc; elaeXeuaecoc; xfjc; Tuyjiq
— iL^I ik^^ /^^ ^'Jhi-^' L-f ^^ ^'^^ motion of the ascendant of the revolution
of the year
SLaspx^vxat ( c^.^' ) 11.5
Kspi xcov e TiXavco^evcov daxepcov oxl xaxd tiolov xatpov e^ep^ovxat yjxol
UTie^LGxavxaL xoO cpcoxoc; xoO tiXlou xal xaxd TioLav oSpav slaepxovxaL Otio cpcoc; xoO
tiXlou xaxd x6 Tipcot y] x/jv saTiepav — Lp:>^j oIa^^iII ^.^^iCJl ^,ji»^ ^ on the
rising of the moveable stars (planets) and their settings
sxpdXXsxaL ( ) 11.3
sxpdXXexaL x6 aOGrj^epLvov xoO tiXlou xal xfjc; aeXTQvric; — ^jd^' ^3^ ^^
210
find the true positions of the two luminaries
sxpoXrj ( o^^ ) 1.4
xal xfjc; expoXfjc; xoO evbq enouq olko toO enepou hia xcov xavovLCOv
— JjAi-L j}2ju ^ Lp^ ^ jb^' i^^^jco the knowledge of the calendars from
each other via table
sxPoXt^ ( ^jc^\ ) 1.4.2
Kspi xfjc; expoXfjc; — t-^^J-^I ^ on the extraction
SxPoXt^ ( J.^^" ) 10.3.1.2
Kspi xfjc; expoXfjc; xoO tiXslovoc; xal eXdxxovoc; xfjc; ocj^ecoc;
— ^Lll L3>lli-I Jd3^" cJ ^^ ^'^^ conversion of parallax
sxpoXrj ( ^>^i) 12.1.1
Tiepl xfjc; expoXfjc; xcov (bpcov xfjc; elaeXeijaecoc; xcov xpovcov oXcov —
JLJI ^^^ Jd^^" olSjl T-^pJ^I ^ on the extraction of the times of the revolutions
of the years of the world
sxsLVOc; ( ) 12.3.1
f) iiepiaaeioL f) [xeay] xoO xotiou xfjc; xu^iQ^ "^"H^ ^otpac; exsLvou
— /tM^I ^j-^ ^^Ua^ Oju iLia3 the excess of what is between the rising times
of the degree of the hayldj
SXXSLTISL ( cij-uJli ) 10.2.2.1
exXsLTiSL ^epoc; xfjc; aeXTQvric; oaov dvacpavfj sic; xouc; SaxxuXouc; xfjc; SLa^expou
— Oj^ /^^' 0^ j^ l33-^I 03^. the eclipse is in the measure of the digits of
211
its diameter
SXXSLTISL ( Ul.^ ) 10.2.2.1
f) aeXTQvr) kolgol exXsLTiSL dXX' oO^ taxaxaL sic; x/jv exXslcJ^lv
— JU5Co 4J 035C Mj 4JS^ lJlu^^^ the eclipse is entire and it has no duration
SXXSLTISL ( cJlu^' ) 10.3.2.2
[xepoc, exXsLTiSL xoO tiXlou — V^^ lJl^JCj part of it (the sun) is eclipsed
£XX£L(];£L ( ) 10.3.2.2
x6 [isaov xoO tiXlou exXslcJ^sl f) Se TiepLcpepsLa oOx exXslcJ^sl
— j^ iiJb" j^usJJl >y>- ^ jAJii\ ^y> around the moon in the body of the sun
is a ring of fire
£XX£L(];£L ( Lij-ujCJi) 10.3.2.2
oXoc; exXei(\)ei xal xatpov Ixavov axaGiQaexaL ev xrj exXslcJ^sl. —
JU5Co ^ ^ l3j-uJCJI the eclipse is total with duration
£XX£L(];£L ( Lij-ujCJi) 10.3.2.2
6 yjXloc; xeXsLov exXslcJ^sl xal oO PpaSuvsL ev xrj exXslcJ^sl
— 4J cU5Co "^j (J^' l33-uJCJI the eclipse is total and there is no duration to it
£XX£L(];£L ( Lij-ujCJi) 10.3.2.3
6 yjXloc; oXoc; exXslcJ^sl — ^JS""^ i^j-^JCJI the eclipse is total
£XX£L(];£L ( Lij-ujCJi) 10.3.2.3
dcTio xoO tiXlou tiogov exXslcJ^sl — l3j-uJCJI jIaIo amount of the eclipse
212
£xX£L(];lc; ( oUj-u^l ) 8.4.1
Sloc xriv £xX£L(J;lv — oUj-^JCJI ^ during eclipses
£xX£L(];lc; ( oUj-u^l ) 9.1.4
xriv £xX£L(J;lv toO tiXlou — oUj-^JCJI eclipses
£xX£L(];lc; ( i^^c^i oUj-uJll ) 10.2
xfjc; exXsLcJ^ecoc; xfjc; aeXrivriq — Si^*^' oUj-^l lunar eclipses
exXei(\)i^ ( Lij-uJli ) 10.2.2.1
TsXeioi yLvexaL exXslcJ^lc; xfjc; aeXrivriq xal Tipoc; xatpov sic; x/jv exXslcJ^lv taxaxat
— cU5Co 4jj JS^ l33-^I the eclipse is total and it has duration
£xX£L(];l^ ( oUj-uJCJI) 10.3
xfjc; £xX£L(J;£coc; xoO tiXlou — i^-^ujJJl oUj-^JCJI solar eclipses
£xX£L(];L^ ( ) 10.3.2
xal £v xouxcp yLvexaL f) exXslcJ^lc; — pUIj*-'^! dL)i> ^ '^.jj J^' there is a
possibility of its (an eclipse's) sighting in this conjunction
£xX£L(];l^ ( oUj-uJCJI) 10.3.2
xfjc; exXsLcJ^ecoc; xoO tiXlou — ^^co^dll oUj-^JCJI solar eclipses
£xX£L(];L^ ( cJluJCj ) 10.3.2.2
xeXsLa yLvexaL exXslcJ^lc; xoO tiXlou — Ur lJl^JCjJ L^U all of it (the sun) is
eclipsed
213
£xX£L(];L^ ( Lij-ujCJi ) 10.3.2.2
el yevTiTOLi exXslcJ^lc; y] ou — lJ^^.mS^\ jISCoI possibility of the eclipse
sxiXfjcpL ( lJ^^S\) 9.1.5
exxXfjcpL ^avSap yjtol to tiXsov xal eXaxxov xfjc; ocj^ecoc; — ^^klll l3M^^1
difference in vision (parallax)
sXaaL^ ( ) 12.4.3
Kspi xfjc; eXdaecoc; xfjc; Tuyjiq xfjc; elaeXeijaecoc; xoO ^rivoc;
— L^.^->1 ^'Jhi-^J jj-p^^ J^.3^ lJ ^^ ^'^^ revolution of the months and the motion
of their indicators
eXoLGl^ ( ) 12.4.4
Kspi xfjc; eXoLoecdq xfjc; eiaeXeuaecdq xfjc; xuxtjc;
— iL^I ik^^ /^^ ^'Jhi-^' L-f ^^ ^^^ motion of the ascendant of the revolution
of the year
sXdxTCOv ( Jii ) 1.4.2
(J;fjcpoc; eXdxxcov — Jil less
£XXd^(];L^ {jyi\) 11.1.5
x6 e^eXGov xo^ov eaxl xoO cpcoxoc; fjyouv xfjc; eXXd^cJ^ecoc; xfjc; aeXTQvric;
— jj^l J^3^ ^^^ ^f light
SXXSLCJ^L^ ( L^Ui) 8.1.4
eXXsLTicJ^Lc; — iuaSUI decreasing
214
s^cpdvsta ( ooi^ ) 1.2
£^cpdv£La TipocpiQTOU — ^ ctot^ Sending of a prophet
svap^!-^ ( ^'^^^^ ) 7.0.0
xriv evap^LV — ?Jlio beginning
svoOvxat ( br, ) 1.2
svoOvxaL — b>j we add
svoOxaL ( ^ ) 3.2.1
svoOvxaL — Uj^Liti?" we add them
SVCOGL^ ( T^bloi ) 12.2.4
xfjc; evciaecoc; xcov p xoticov xfjc; xuxtjc; — ij^LjJLiall r\ji<i\ a mixture of the two
rising times
s^o^ycovov ( ^.J-uJ ) 12.2.3
e^dycovov sgxl Ss^lov — J^^' 'U^.uJ its dexter sextile
s^o^ycovov ( ^.J-uJ ) 12.2.3
6 xoTioc; eaxl xoO cpcoxoc; xoO e^aycivou xoO daxepoc; e'E, dptaxepcov
— ^r^.^1 4^ .uJ jy ^yi the location of the illumination of its sinister sextile
s^o^ycovov ( ^^JuuJJi ) 12.2.3
\oi(:>\ eaxl xoO e^aycivou — j^ J^' j^3^ ^^^ ^f ^^^ sextile
215
s^o^ycovov ( ^^JuuJJi ) 12.2.4
TO Se^Lov e^dycovov — j^^uJJl 0^."^' dexter sextile
s^o^ycovov ( ^^JuuJJi ) 12.2.4
TO dpLGTspov e^dycovov — ^r*^.^' j^J^^I sinister sextile
s^o^ycovoc; ( ^^j^uJ)! ) 12.2.3
TO TiXdTOc; ToO e^aycivou — j^ J^^l ^^ latitude of the sextile
zi,Z^yp\lZ\T\ ( ^JlaJ ) 11.5
exsLVT) f) ^oLpa f) z\z^yp\iz\T\ \iz\h toO doTspoc; TripeiraL f\ exsLvr) f) ^otpa f)
^£Td ToO doTspoc; Suvouaa — V^. j' c-^^jiCJl ^u^ ^iiaj ^1 i^jjJl the degree
with which rises the planet or sets
zi,Z^Yp\\QL\ ( Ji^' ) 11.5
Tiepl Tcov z TiXavco^evcov doTspcov otl xaTd tiolov xatpov e^ep^ovTat yjtol
UTie^LGTavTaL toO cpcoTOc; toO tiXlou xal xaTd Tiotav oSpav slaepxovTaL Otio cpcoc; toO
tiXlou xaTd to Tipcot f\ t/jv saTiepav — \^jiu^ Ij^^^cW <^^^\ ^^j^ ^ on the
rising of the moveable stars (planets) and their settings
i^i]P)(Z^QLi ( ^ ) 1.5.1
e^T^px^TO — m\]a> rise
ziiao\)\iZ'\)o^ ( JJU ) 9.2.1
e^LGOu^evov — Jlo equal
s^i-cyoOvTaL ( ) 1.2
216
ol ^fjvec; s^LGoOvxaL [xeTOL xcov 8 xatpcov
— iL^I Jj-^ ^ jjr^ ^'^^ months (are fixed) with the seasons of the year
Z'E.IG 0)01)0 Oi\^ ( ^J^ ) 1.2
e^LaciGrjaav — ^^ corresponds
STiavaxuxXoOvxaL ( Sjj^ a*^ Sjj^ ) 1.2
STiavaxuxXoOvxaL — Sjj:> Aju Sjj:> cycle after cycle
STiLcpdvsta ( 4^j ) 6.6
xfjc; STiLcpavsLac; xfjc; yfjc; — ^^Ml o»"j area of earth
STlLCpdvSta ( ^Ja-u. ) 10.2.2.1
xcov SaxxuXcov xfjc; STiLcpave Lac; xfjc; aeXTQvric; — 4^Ja^ j^ l3j-^I /^^' digits
of the eclipse in its surface
STiLcpdvsta ( ^Ja-u. ) 10.3.2.3
xfjc; STiLcpavsLac; — ?tWM> surface
spyov ( <:^U ) 1.2
^eytaxov epyov xcov xoO oOpavoO — ^jjIa oL'J j-o ioJa^ <j:>U" great oc-
currence of atmospheric marvels
spyov ( <:->U ) 1.2
^eytaxov epyov xcov xfjc; yfjc; — V^j' oLo>U ^ ioJa^ <j:>U" great occur-
rence of earthly signs
217
eoy^oLTOC, ( <jIp ) 11.1.7
xriv saxaTTiv dvdpaaLV xfjc; SLa^expou xfjc; ^OLpac; xoO tiXlou
— j^usJJl ty>- j^ ^^j' h^ limit of the altitude of the opposite point of the
degree of the sun
saxaTOc; ( <jIp ) 11.1.8
f) eaxoLTy] dvdpaaLc; xfjc; aeXTQvric; — ^^j' h^ limit of the altitude
eoy^oLTOC, ( <jIp ) 11.1.8
f) ea^dxT) dvdpaoLc; xfjc; ^OLpac; xfjc; aeXTQvric; — ^j-^ t^J^ '^-^ limit of the
altitude of the degree
STsGrjaav ( <z^ju ) 1.2
exsGrjaav — cJl^ are transferred
£T£X£LCL)6r) ( ^' ) 1.2
exeXsLciGr) — ^' completed
£To^ ( g.ji>:)i ) 1.2
xd exT) SfjXa — Sj^yill '^j\yi\ famous epochs
£TO^ ( iLu. ) 1.4.2
x6 xavovLov xcov diiXcov excov — i^j-^l ^^^ Jj-^ table of simple years
SToq ( '^j\: ) 1.4.2
xoO exouc; xcov Apdpcov — S^^l J^jl^' epoch of the hij
ra
218
£TO^ ( g^jUl) 7.2.1
dcTio ToO STOUc; — ^ jlx)l calendar
£TO^ ( g,jUl) 7.2.1
xal opGoOxaL to stoc; opGcoatv neXeioiv — ^^t^ ^j^'^i^. the calendar
becomes corrected
£TO^ ( ^^Jyi\ ) 7.4
xa STT) — '^j\y:}\ calendar (dates)
suGsta ypa^^rj ( ) 3.0.0
[iSTOL xfjc; eOGsLac; ypa^^fjc; — ^vil^l dliiJl right sphere
suGsta ypa^^rj ( ) ll.l.l
ToO TOTiou xfjc; TUXTjc; ^exa eOGsLac; ypa^^fjc; — ^vil^l dLiiJl JUa^ rising
time of the right sphere
suGsta ypa^^rj ( ^sjllA] ) 12.1.3
ToO TOTiou xfjc; TUXTjc; [xsTOi xfjc; eOGsLac; ypa^^fjc; fjc; f) apxiQ o^^^ "^"H^ ^PX'H^ "^^^
KpLoO
— J^l Jj' 0-^ ^vSl^l dliiJl JUa^ rising time in the right sphere from the
beginning of Aries
suGsta ypa^^rj ( ^sjllA] ) 12.3.1
xoO xoTiou xfjc; xuxTjc; exeivou ^exa xfjc; eOGsLac; ypa^^fjc;
— ^>il^l dUliJl ^JUa^ rising time in the right sphere
219
suGsta ypa^^rj ( ^viiuil ) 12.3.2
Tov TOTiov xfjc; TUXTjc; TOUTOU ^exa xfjc; eOGsLac; ypa^^fjc; — ^vZLoil 'LJUa^ its
rising time in the right (sphere)
suxaxaXrjTiTOTSpov ( ) 9.2
OKsp eaxlv eOxaxaXriTixoxepov — c-^^^^l ^ 9 y <Jj in it there is a kind
of approximation
SUpsGf] ( rj^ ) 1.2
d XL eOpsGrj — rj^ there results
SUpsGf] ( fj^^^i ) 1.2
d XL eOpsGrj — P jus^l the sum
£9dvr) {j^) 11.5.1
6 daxrip ecpdvr) — j^ it appears
Zou^Tipd ( o^Ji ) 1.5.1
Zou^Tipd — '^J.i)^ al-Zubra
CcpStaxoc; ( r^j^\ <^ ) 1.1
^cpSLaxoc; xuxXoc; — /TJ^' ^ sphere of the zodiacal signs
C^SlOV ( r^j^\ ) 1.2
ox£ 6 yjXloc; duo ^coSlou ^sxapaLvsL sic; ^6)8lov — /TJ^' J^-ls' j^usJJl J^^^
the entrance of the sun into the beginnings of the zodiacal signs
220
C^Slov ( ^j^i ) 4.4
£Lc; xa voTLa ^cpSta — ^^jlj-l ^3^^ cJ ^^ ^^^ southern zodiacal signs
C^Slov ( rj)i\) 11.5.1
xal ^exa xoO (J;7]cpou xcov p ^coSlcov opGoOxat
— iji^^l ijiu U J^Jaij oUa^ we equate it with the excess of what is between
two zodiacal signs
C^Slov ( r^j\i\) 11.5.1
'H^SLc; xavovLov eGiQxa^ev xal xa xo^a omep eho\iev xeGsLxa^ev sic; sxslvo x6
xavovLov ^£xa xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xac; OLpy^oiq xcov ^coSlcov
— ^^11 ^ ^J^^ oU^lia^^Uj /TJ^^ ^hr!*^ 0^ ^3^^ ^j-V^ jIaSI LitJpj
we have set out the values of the limits of sighting in degrees of the zodiacal signs
and for the initial declivities in the fourth clime at the beginnings of the zodiacal
signs
C^SlOV ( ^j^i) 12.1.1
eiq exelvov xov xatpov oxl 6 tiXloc; ytvexaL sic; x/jv apx^Q^ "^^^ ^coSlcov —
IAjlI] r^j)i\ J^ls' j^usJJl ^^y Xs- when the sun alights upon the beginnings of
the coming zodiacal signs
C^Slov ( r^j^\ ) 12.2.2
xoO xoTiou xfjc; xuxTjc; xcov ^coSlcov — /TJ^' ^Ua^ rising time of the zodiacal
signs
C^Slov ( rj^\) 12.4.1
221
TO arj^SLov xoO ^coSlou xfjc; xuxiQ^ ^o\j Qe\ieXio\j xoO yeveBXiaXoyixoxj TiepL-
oaeueTOii eiq xouc; xpovouc; exsLvouc;
— ^JLUJI Sjj-i^ jl «^^i^j5CJl 'ti (^a)I /^^I Ojy^ ^J^ l3:>j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
C^SlOV ( 04^ ) 12.4.1
Tiepl xfjc; evGu^TQaecoc; exeivou xoO (J;7]cpou oxl xa6 ' exaaxov xpovov a ^6)8lov
XLVSLXaL
— O'biu-^j V^^S^ *^-^ J^cJ LiY^' cJ ^^ ^'^^ intihd^ in every house and star
and its motions
^63Vr) ( ) 3.1
xfjc; xeXsLac; xfjc; fj^epac; ^(ivrjc; — jV^' Jajco equalizer of the day
fikioq ( ^^.oJJl) 1.1
SuGLc; xoO tiXlou — j^usJJl i^^ji- setting of the sun
fjXtO^ ( ^^.ccJJi ) 1.2
ox£ 6 yjXloc; dcTio ^coSlou [xenoi^oiivei eiq ^6)8lov — /TJ^' J^-ls' j^usJJl J^^^
the entrance of the sun into the beginnings of the zodiacal signs
fjXtoc; ( ^^.ccJJi ) 1.2
OLveTSikev 6 yjXloc; — j^usJJl Ca^JJ^* the sun rises
fjXto^ ( ^^.ccjji ) 1.2
yjXloc; £c; x/jv apx^Q^ "^^^^ KpLoO — ^y^,J^ JljI^MI iial5 j^usJJl cJi^ the sun
222
came to the point of the Spring equinox
fjXtO^ ( ^^.ccJJi ) 1.2
f) eiaeXeuaiq xoO tiXlou eiq xov Kptov
— J^\ ^ ^^-^ J3' cJ j^*^*-*^' the sun is in the first degree of Aries
fjXtoc; ( ^^.ccJJi ) 1.2
f) elaeXeuaLc; xoO tiXlou sic, xov Kptov
— ^y^,J\ JIaI^MI iiaU j^usJJl Jl^" jI when the sun enters the point of the
Spring equinox
fjXtoc; ( L-uccJJi ) 1.2
XpovoL xoO tiXlou — i^-^usJJl ijj^ solar years
fjXto^ ( ) 8.0.0
6 yjXloc; xal f) aeXTQvr) — jbj^l the two luminaries
fjXtO^ ( ^^.ccJJi ) 10.3.2.2
x6 [isaov xoO tiXlou exXslcJ^sl f) Se TiepLcpepsLa oux exXslcJ^sl
— j^ 'il\s> j^usJJl >^ j^ ^^1 J^^ around the moon in the body of the sun
is a ring of fire
fiklOCi ( ) 10.3.2.2
6 fikioc, Tzkziov £xX£i(J;£L xal ou PpaSuvsL iv xfj ix'kzi'.\)ei
— 4J i±Jia Sj i_^^ l3^.^*5CJI the eclipse is total and there is no duration to it
fikioq ( ^^.oJJl) 11.1.7
223
TO^ov eaxl xfjc; xaxapdaecoc; xfjc; tiXlou — j^ujJJl J^^lia^'l ^yi arc of the
declivity of the sun
f]kloq ( ^^.ccJJi) 12.4.2
f) XLvrjaLc; sgxlv f) ^ear) xoO tiXlou — j^usJJl '^j> motion of the sun
f)^£pa ( jl^i ) 1.1
x6 \iiao\ xfjc; fj^epac; — j[^\ cJLuaj dlU sphere of half of the day
f)^£pa ( >y^\ ) 1.1
fj^epa xaL vu^ — CLL >^l day with its night
f)^£pa ( >U ) 1.2
SfjXaL xal ^syLGxaL fj^epaL — ^hLALjdl >\j\ famous days
f)^£pa ( >U ) 1.2
al SfjXaL fj^epaL — Sj^y^JII (O^^Jj its famous days
f)^£pa ( ) 1.2
xXoTiL^ataL fj^epaL — il^JLo ( ^-^usJi-O (five days) are added
f)^£pa ( ) 1.2
xXoTiL^ataL fj^epaL — SjjI^I additional (days)
f)^£pa ( ) 1.2
xXoTiL^ataL fj^epaL — iS^L^.^ stolen (days)
224
f][ispa ( >y^ ) 1.2
\ieaov xfjc; fwiepaq — >y__ <Js^ half of the day
f][ispa ( >^\ ) 1.4.2
Tc5v TiapeX6ouac5v f)[jiepc5v — <us ^y^ ^_^jJl »^l the day which we are in
f][ispa ( >U ) 1.5
Tc5v StjXcov xal ^leytaxcov f)[ji£p(ov — Oj^^cil l^U their famous days
f][ispa ( ) 6.1
jipo Tou [jieaou Tf)(; f)[jiepa(; — Jbj;'' -*^ after noon
rjjispa ( >Li ) 7.3
Twv r][ji£pwv xfjc; fepSofidSoc; — ol*oJ-l >L1 days of the week
TjjiSpa (jLjAli) 10.2.2.3
rjjispa (jLj; ) ll.l.l
TW f)[iLa£L To^cp xfjc; f)[ji£pa(; — ^j*o-:lH tjs>- Jif ^^ L-i-aJ half the arc of
day of the degree of the sun
f)[ispa (jl^ ) 12.2.2
TO f][jiiau TO^ov Tf)(; f]\iepa.<:; — ^_,J^X)I Jif ^yi t-a.uaj half the arc of the
day of the star
f)[ispa (jl^ ) 12.2.4
225
TO YJ^LGU TO^ov xfjc; fj^spac; xoO daxepoc; — OjL^ j^3^ cJLuaj the half arc of
its day
fj^LV ( b ) 2.2.2
£v fj^LV — Lico with us
fj^LGU ( cJLuaJi ) 8.0.0
YJ^LGU u(J;co^a xfjc; acpatpac; — ^J^"^' cJLuaJl upper half
fj^LGU ( cJLuaJi ) 8.0.0
YJ^LGU xfjc; xaxG) Gcpatpac; — jLi-^^^l cJLuaJl lower half
fj^LGU ( cJLuaJ ) 10.2.1.2
YJ^LGU XeyexaL xcov p Sta^expcov — ^^^^iaiJl cJLuaj half of the two diameters
fj^LGU ( cJLuaJ ) 10.3.2.2
YJ^LGU XeyexaL xcov p Sta^expcov — ^^^Wgll cJLuaj half of the two diameters
fj^LGU ( cJLuaJ ) 11.1.1
xcp fj^LGSL xo^cp xfjc; fj^epac; — j^usJJl iy> jL^ J^3^ cJLuaj half the arc of
day of the degree of the sun
fj^LGU ( cJLuaJi ) 12.2
^£XP^ ^^'^ "^^^ ^'"^^ fj^LGU £GXL xfjc; dvapdGSCOc;
— iajlAI cJLuaJl the descending half (C mistranslates)
fj^LGU ( cJLuaJi ) 12.2
226
^£XP^ ^^'^ "^^^ TSTdpTOU YJ^LGU soTL xfjc; dvapdascoc; — A^LaJl cJLuaJl the
ascending half
fj^LGU ( cJLuaJ ) 12.2.2
TO YJ^LGU TO^ov xfjc; vuxTOc; — iL) j^^^ cJLuaj half the arc of night
fj^LGU ( cJLuaJ ) 12.2.2
TO YJ^LGU TO^ov xfjc; fj^spac; — i^^\ j[^ ^y cJLuaj half the arc of the
day of the star
fj^LGU ( Ul^\ ) 12.2.4
TO YJ^LGU TTJc; OLVOL^OLoecdq TTJc; Gcpatpac; — A^LaJl cJLuaJl the rising half
fj^LGU ( cJLuaJ ) 12.2.4
6 dcGTrip eiq to yj^lgu ttjc; xomoi^oiaeoyq sgtl ttjc; Gcpatpac; — iajlAI cJLuaj the
half of descent
fj^LGU ( cJLuaJ ) 12.2.4
TO YJ^LGU TO^ov TTJc; fj^spac; ToO doTspoc; — OjL^ ^y cJLuaj the half arc of
its day
fj^LacpatpLOV ( cJLuaJi ) 8.3.3; 8.3.4
TO dvco fj^LacpaLpLov — ^J^^^ cJLuaJl upper half (of the sphere)
fj^LacpatpLOV ( cJLuaJi ) 8.3.3; 8.3.4
TO xdTCO fj^LacpaLpLov — jLiL^"^! cJLuaJl lowcr half (of the sphere)
227
f]V63[iSVaL ( %^) 1.2
f)vw[ji£vai — >loJ* summarily
Bapdv ( oy ) 9.2
6 ©a^av exelvoc; 6 'AXe^avSpTjvot; — ^\jXjL^^\ tjy Theon of Alexandria
GdXaaaa (^_ ) 7.0.0
Tf]<; axpat; 8uTixf)<; 6aXdTTT]<; — i^ji\.\ j^ J**"^ shore of the western ocean
0£^isXlov ( il^Sti) 1.2
ol ^if]V£(; Tou Bz\ieXio\j — tJL«>MI jj-(^Jl months of the base-horoscope
Gs^sXtov ( Jl^MI ) 4.2
Gs^sXlov — J^^"^' base-horoscope
Gs^sXtov (jLJ.i) 6.7
Qe\ieXiov — jLcJ.1 measure
Gs^sXlOV {jyi^^ ) 7.4
Tiepl ToO Gs^eXlou toO aOGrj^epLvoO xoO tiXlou sic, eva xp^vov xoO tiXlou —
i^-uj:^ iL^ >^^l j^^:> <^^j ^ on the computation of the rule of the rectifier for
the solar year
Gs^sXlov ( Jj-^i ) 7.4
Gs^sXlov xfjc; ocpx'H^ "^^^Ci j^6\o\^ — -^CZjui ^yJ\ bases of the beg
mnms
Gs^sXtov ( o^^O 11-3
228
ToO Qe\ieXio\j xfjc; Gecoptac; xfjc; aeXr]vr](; oXou —
il^MI 'L/^j ii^^jco ^ (j^^ j^liJl the entire rule on the knowledge of the sighting
of the crescent
Gs^sXlOV ( <^Alo ) 12.2
ToaaOxd eiai Qe\ieXi(x a xpiQ eiSevaL — <^a1o premises
Gs^sXtov ( ) 12.4.1
TO arj^SLov xoO ^coSlou xfjc; Tuyjiq xoO Gs^eXlou xoO yevsGXLaXoyLXoO Kspi-
oaeueTOii eiq xouc; xpovouc; exeivouq
— ^JLUJI 'Sjy^ jl «^^i^j5CJl 'ti (^a)I /^^I Sjj-i^ ^J^ l3:>j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
Gscopta ( ^jl\ ) 10.3.2; 10.3.2.1
6 xoTioc; eaxl xfjc; Gecoptac; xfjc; aeXTQvric; — ^^\ j^\ ^ya place of the visible
moon
Gscopta ( kiJ^) 11-2.1
xpuxdvr) xfjc; Gecoptac; xfjc; aeXrivriq — h3j^ jW*^ measurement of sighting
Gscopta ( i^JJi ) 11.3
xd xavovLa xfjc; Gecoptac; xfjc; aeXrivriq olko xfjc; ocj^ecoc; — h3j^ ^^J^=> Jj-^
table of the limits of vision
0£63pLa ( Y^J\ ) 11.3
f) Gecopia xfjc; a£XT)VT)(; vsaq cpavsiarjc; — Slj^' :>3A2> jIa^ measure of the
229
limits of sighting
Gscopta ( <ijj ) 11.3
ToO Gs^eXlou xfjc; Qecdpioiq xfjc; aeXrivriq oXou —
il^MI 'L^j o^^jco ^ (j^^ j^liJl the entire rule on the knowledge of the sighting
of the crescent
Gscopta ( <ijj ) 11.3.1
Gecopta oOx eaxL xfjc; aeXTQvric; — J^UI <jjj ^ «iaj M we do not aspire to
sighting of the crescent
Gscopta (jln^^fi) 11.3.1
£Lc; x/jv Tipcixriv Gecoptav — Mjl jLl^MI ^ on consideration first
Gscopta (jln^^fi) 11.3.2
Tiepl xfjc; Seuxepac; Gecoptac; — Ljb^ jLl^MI ^ on consideration secondly
Gscopta ( kiJ^) 11-5.1
xo^ov xfjc; Gecoptac; xoO daxepoc; — h3j^ ^j^y ^^^3 ^^ ^^^^ it the arc of
vision
Gscopta ( <d3Ji) 11.6.1
£X£Lvo TO^ov XeyexaL xfjc; Gecoptac; 00^1 xsXslov — iiiiall '^,^J\ ^y arc of
general sighting
Gscopta ( i^JJi ) 11.6.2
xoO xo^ou xfjc; Gecoptac; xoO xeXsLou — iiiiall <:ij^l j^^^ arc of general
230
sighting
Gscopta ( i^JJi ) 11.6.2
TO TO^ov xfjc; Gecoptac; — iiiiall 'ij,^J\ ^y arc of general sighting
Gupa ( c-^L ) 2.1
6upa TLc; — LL door
l' ( .U^i J^j ) 12.2
OLKO TOO l' TOO TipcixOU ^^XP^ ^^'^ "^^^ TSTapTOU
— ^\J\ ^\ JliaJl Jl glo^cJl ]a^^ ja from the mid-heaven to the ascendant to
the fourth
'laaSaxspSr) ( ^j>^y, ) 1.2
xpaxoOvxaL ol xpovoL TSTsXeLCO^evoL xoO exouc; xoO 'laaSaxepSr)
— ^bl ^^>;;:i ^^5>-^ ljAfli"l we take the completed years of Yazdijird
tSta ( <i^U ) 8.1.2
f) ISta — 'CL^U- its anomaly
tSta ( L^U ) 8.1.4
f) ISta — ii^U" anomaly
tSta ( L^l^l ) 8.1.4
f) ISta xeXsLa — iJAjJl S^li for the equated anomaly
ISlov ( L^l^li ) 8.1.4; 8.3.3; 8.3.4
231
ToO i5lou TsXeiou — iJ-uIl L^lil equated anomaly
ISlov ( <^\^\) 8.3.3; 8.3.4
TO iSlov — 'LsU-l anomaly
ISlov ( ■i^\^\)9.1A
ToO lSlou xfjc; aeXrivriq — L^lil anomaly
ISlov ( l^\}l\) 9.2.5
xax' evavTLov xoO lSlou xfjc; aeXTQvric; fjxfjc; dvapdaecoc; xauxTjc; — ^JajJII L^lil
equated anomaly
ISlov ( Ji-^ ) 9.2.5
xd xavovLa y] xoO lSlou y] xfjc; dvapdaecoc; xfjc; aeXTQvric; — ^jd^' ^i-^^ Jj^
table of the motion of the two luminaries
ISlov ( l^\^\) 10.3.2.3
xoO lSlou xfjc; aeXrivriq — <^lil anomaly
ISlov ( L^U ) 11.3
xoO lSlou y] xfjc; ^exapdaecoc; xfjc; aeXTQvric; — C^ jl ^^1 S^U- anomaly of
the moon or its daily velocity
LVT££ ( ^j^\) 12.4.1
el XL xaxaXsLcpGfj exelvo ^6)8lov ocpsLXsL slvaL ecp' & f) XLvrjaLc; xfjc; xu^iQ^ ^^o^"^'
£X£Lvov xov xpovov £cp6aa£v. £X£Lvo x6 ^6)8lov Lvxee xaXsLxat. —
iL^I dlij ^ (^5Y^' r^^ Ijy^ y^ jts- ^\ jj:> ^^ Lo what remains less than 12
232
is the image of the zodiacal sign of the muntahd in that year
Igoc, ( ijjLJu ) 2.2
[xsTOi ToO dcXXou laov — <j jLJu equal
laxd^svoc; ( <i^p\ ) 1.2
laxd^evoc; — ^.^^^ fixed
laxaxaL ( 'ir\s ) 6.4
laxaxaL — irlS standing
taxaxaL ( ^ ) 8.2
6 daxrip taxaxat fjyouv axripL^SL — ? y>-JS ^vlo standing for the retrogres-
sion
loTOLTOil ( oXo ) 10.2.2.1
f) aeXTQvr) Tiaaa exXemei dXX' oO^ taxaxat sic; x/jv exXslcJ^lv
— JU5Co 4J 035C Mj 4JS^ lJlu^^^ the eclipse is entire and it has no duration
taxaxaL ( 0X0 ) 10.2.2.1
TsXeioL yLvexaL exXslcJ^lc; xfjc; aeXTQvric; xal Tipoc; xatpov sic; x/jv exXslcJ^lv taxaxat
— JU5Co 4jj JS^ l3j-^I the eclipse is total and it has duration
LXVOHoSa ( ^ISSti ) 2.2.3
xa IxvoTioSa — »I5MI feet
xdGsToc; ( JyjJi ) 6.6
233
xdGsTOc; — J^^iJJl plumbline
xatpoc; ( Jj-uai ) 1.2
ol [xfiveq s^LGoOvxaL [xstol tcov 8 xatpcov
— iL^I Jj-^ ^ jJt^ ^'^^ months (are fixed) with the seasons of the year
xatpoc; ( Sxo ) 8.2.1
xatpoc; OTL dcpx^L OtiotioSl^slv 6 daxTQp — ? y>-J\ ^\ iolil^MI 'Sxa the period
of time from direct to retrograde motion
xatpoc; ( oi^i ) 9.1.1
xfjc; dvapdaecoc; xoO i OLXTQ^axoc; xfjc; Tuyjiq xoO xatpoO — c^S^I ^U ^^j\
altitude of the tenth of time
xatpoc; ( ) 9.1.1
x/jv xpaxTjXaLav xoO xo^ou exeivou yjxlc; eaxlv ^exa^u xoO i olxiQ^axoc; xal
xfjc; Tuyjiq xoO xatpoO — 'uJl^j ^LJI (jju ^1 j^>^' the arc which is between the
tenth and its ascendant
xatpo^ ( ) 10.2.2.1
xov xatpov xfjc; SLa^expou tiXlou xal aeXTQvric; — l3j-^I \z^^ middle of the
eclipse
xatpo^ ( o^j\) 10.2.2.2
xov xatpov xfjc; exXsLcJ^ecoc; xfjc; aeXrivriq — l3j-^I O^;' time-degrees of the
eclipse
234
xatpo^ ( ) 10.3.2
f) TUXTQ ^o\j xatpoO — JliaJl ascendant
xatpo^ ( ) 10.3.2.2
oXoq exXei(\^ei xal xatpov Ixavov axaGiQaeTaL ev xfj exXslcJ^sl. —
JU5Co ^ ^^^ l3j-uJCJI the eclipse is total with duration
xatpo^ ( C)^j\) 10.3.2.3
ol xatpoL — jLojl time-degrees
xatpoc; ( oXli ) 11.1.6
Ilepl ToO To^ou £X£Lvou xal ToO xatpoO otl eaxlv Oiiep yfjv f) aeXTQvr) ^exa xriv
SuGLv xoO tiXlou
— j^usJJl c-^wJLo Aju ^j^l (3^^ JU5Cil ^y arc of duration above the earth af-
ter the setting of the sun
xatpo^ ( <zXl\) 11.2
a To^ov xoO xatpoO exepov xcov dxxLvcov dcXXo xfjc; dvapdaecoc; xal exepov
TO^ov xfjc; xaxapdaecoc;
— Jtf»lia^''^lj pliJj'^lj ctJCllj jjJl j^^ the arc of light; of duration; of altitude
and of declivity
xatpo^ ( <zXl\) 11.2.1
x6 TO^ov xoO xatpoO — JU5Cil ^y arc of duration
xatpoc; ( ) 11.3
£Lc; xov xatpov sxslvov fivLxa Suvr] f) aeXTQvr) — ^^1 v^:^«^ -^^ ^t the time
235
of the setting of the moon
xatpoc; ( oXli ) 11.5
TO To^ov ToO xatpoO xfjc; xaxapdaecoc; xoO tiXlou — J^^lia^'lj JU5CII J^^^ the
arc of duration and declivity
xatpoc; ( oXli ) 11.6.1
TO TO^ov ToO xatpoO — JU5CII ^y arc of duration
xatpoc; ( oXli ) 11.6.1
xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xoO xatpoO — JU5CII ^y Jd-^' equa-
tion of the arc of duration
xatpoc; ( ) 12.1
xaxd xov xatpov fivLxa eyevexo f) yevvrjaLc; — jJljII nativities
xatpo^ ( olli ) 12.3.2
6 xatpoc; — SjII period of time
xaxoc; ( j^^^i ) 12.3
xcov (bpcov xcov xaXcov xal xaxcov — j^^^b •^^^«-^' ^tJ?j^ place of benefic
and malefic (planets)
xaXo^ ( ^y^\ ) 12.3
xcov (bpcov xcov xaXcov xal xaxcov — (r^^b •^^^«-^' ^tJ?j^ place of benefic
and malefic (planets)
236
xavovLov ( JjaJ^I ) 1.2
xavovLov — Jj-^' table
xavovLov ( JjaJ^I ) 1.2
eiq TO xavovLov — Jj-^' ^ ^^ the table
XaVOVLOV ( Jj^ ) 4.2
xavovLov STsGr) — MjJ^ L«^j we have made a table
XaVOVLOV ( Jj^ ) 6.2.1
ToO xavovLou ToO TOTiou xfjc; TUXTQ^ '^^^ TiXdxouc; xcov tioXscov —
jJlJl ^ r3^^ ^Ua^ Jj-^ table of the rising times of the zodiacal signs in the city
xavovLOV ( Jj^ ) 7.3.1
TO xavovLov Tcov SLXoaaexripLScov xal xcov aiiXcov excov
— i^j-^lj ipjus^l cJj-^ two tables of collected and simple (years)
xavovLOV ( Mj^ ) 7.4
KavovLov £Ti:oL7]6ri — MjJ^ L«^j we have made a table
xavovLOV ( Jj^ ) 8.4
Sloc tcov xavovLCOv — Mj^ by table
xavovLOV ( Jj^ ) 9.2.5
xa xavovLa y] xoO lSlou y] xfjc; dvapdaecoc; xfjc; aeXTQvric; — ^jd^' ^i-^^ Jj^
table of the motion of the two luminaries
237
xavovLOV ( JjaJ^I ) 10.3.2
ToO xavovLou TOUTOU — LJzJai)! JjaJ-I easy table
xavovLOV ( ) 11.1.3
yLvexaL elaeXeuaLc; eiq to Otio touc; ^fjvac; xavovLov xcov (bpcov
— ipLu ^ jA2i\ '^j> ^ OjAij bAfli-l we take the its measure from the motion
of the moon in an hour
XaVOVLOV ( JjA^ ) 11.1.4
TO xavovLov ToO TiXsLovoc; xal eXaxxovoc; xoO xotiou xfjc; xu^iQ^ ^'^^ "^^^ t' xXt^a
— <^ ^j^\ L3>ti"l Jj-^ table of western difference (in vision)
XaVOVLOV ( JjA^ ) 11.3
xa xavovLa xfjc; Gecoptac; xfjc; aeXTQvric; duo xfjc; ocj^ecoc; — Slj^' ^^So JjAc*-
table of the limits of vision
XaVOVLOV ( JjA^ ) 12.1.2
£Lc; x6 xavovLov xoO xotiou xfjc; xu^iQ^ ^k "^o TiXdxoc; xfjc; tioXscoc; exsLvrjc; ev fj
yLvexaL xrjVLxaOxa f) ^TQxriaLc; xoO yevsGXLaXoyLXoO
— ^%^S j^j^ r^^^ ^Ua^ Jj-^ ^ ill the table of rising times of the zodiacal
signs for the latitude of the nativity
xaTiLad ( j^,^\ ) 1.2
xaTiLad — j^LiCJl intercalary
xaTiLad ( l^yj3.\ ) 1.2
xaTiLad — 'L^yXl\ intercalary
238
xaTiiad ( jJLXll ) 7.3
xauiad — j^lXll intercalary
xaTiiad ( A-ooX)! ) 7.3.2
xauiad — iL*xXJl intercalary
TO ToG KapxLvou ( ov^^^*^^ ^s^ ) 5-2
edv 6 doTTip zlc, to eaxl xoO Kapxivou f] £l<; to xoO ALYOX£pcoTO(; —
(j^HjiJ*^! (J^-^ L^-^^' i_i (3^"*^L; jlS' in agreement with one of the two solstitial
points
xaxdpaaLc; ( is»^i ) 3.1
xaxdpaaiq — lgyJ>\ descending
xaxdpaaLc; ( iajU ) 8.3.1
xaxdpaan; — iajU descending
xaTdpaaic; ( is»^i ) 8.3.4
Ejiel he XP^^*^ elSevai Tf)v dvdpaaiv xal xaxd^aaLV — lfyJ>\ descending
xaxdpaaLc; ( iajU ) 8.3.4
ei 8' eXaxTOV xaxd^aaK; — kJ JajU it is descending in it
xaxdpaaLc; ( iajU ) 8.3.4
edv i] nkeov xaxdpaaic; eaxiv — <Li iajU <_^^\ the star is descending in
it
239
xaxdpaaLc; ( ^^vj^o ) 11.1.1
oSpa eaxl [xeaov xfjc; fj^epac; exsLvrjc; xal ^eaov xfjc; xaxapdaecoc; xfjc; ^otpac;
xfjc; aeXTQvric;
— jA2i\ ty>- c-^wJl^ Jl jV^' cJLuaj ijiu Lo ol^Lu the hours between the half of
the day up to the setting of the degree of the sun
xaxdpaaL^ ( J^IWI ) 11.1.7
TO^ov eoTi xfjc; xaxapdaecoc; xfjc; tiXlou — j^usJJl J^^lia^'l ^y arc of the
declivity of the sun
xaxdpaaL^ ( JpIWMI ) 11.1.7
xfjc; xaxapdaecoc; xoO tiXlou Otio yfjv — Jtf»lia^''^l declivity (of the sun)
xaxdpaaL^ ( JpIWMIj ) 11.2
a xo^ov xoO xatpoO exepov xcov dxxLvcov dXXo xfjc; dvapdaecoc; xal exepov
TO^ov xfjc; xaxapdaecoc;
— Jtf»lia^Mlj pUjjMIj JU5Cilj jyi\ ryy the arc of light; of duration; of altitude
and of declivity
xaxdpaaL^ ( J^IWI ) 11.3
xfjc; xaxapdaecoc; xoO tiXlou — j^usJJl J^^lia^'l declivity of the sun
xaxdpaaL^ ( J^IWI ) 11.3.2
f) xaxdpaaLc; xoO tiXlou — j^usJJl J^^lia^ I declivity of the sun
xaxdpaaL^ ( J^IWI ) 11.5
240
ToO To^ou xfjc; xaxapdaswc; xoO rjXiou sic; xov xaipov rjvixa 6uvt) 6 daxT)p f]
dviaxT]
the two arcs of the declivity of the sun at the time of the setting of the planet or its
rising which is called the complete arc of sighting
xaxdpaaLc; ( J^IWI ) 11.5
TO TO^ov ToO xatpoO xfjc; xaxapdaecoc; xoO tiXlou — J^^lia^ Ij JU5CII J^^^ the
arc of duration and declivity
xaxdpaaL^ ( JpIWMI ) 11.5.1
'H^SLc; xavovLov eGiQxa^ev xal xa xo^a ocTiep eSo^ev xeGsLxa^ev sic; exelvo x6
xavovLov ^£xa xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXi\i(x sic, xdc; dpx^c; xcov ^coSlcov
— ^^11 ^ ^^^J^^ oU^lia^^Uj /TJ^^ ^hr!*^ 0^ ^3^^ ^jAs> jljil LitJpj
We have set out the values of the limits of sighting in degrees of the zodiacal signs
and for the initial declivities in the fourth clime at the beginnings of the zodiacal
signs
xaxdpaaL^ ( J^IWI ) 11.6.2
xaxdpaaLc; xoO tiXlou — j^ujJJl J^^lia^'l declivity of the sun
xaxdpaaL^ ( J^IWI ) 11.6.2
Ilepl xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xfjc; xaxapdaecoc; xoO tiXlou —
j^usJJl Jtf»lia^ I ^y Jd-^' equation of the arc of the declivity of the sun
xaxdpaaL^ ( iajUl ) 12.2.4
241
6 daxrip sic; to yj^lgu xfjc; xaxapdaecic; soti xfjc; acpatpac; — iajlAI cJLuaj the
half of descent
xaxaptpdCcov (y^j^i)7.4
TO aOGrj^epLvov xoO xaxaptpd^ovTOc; — ^j^l X'^^' ^^^^ position of the
node
xaxaptpdCcov ( ^1^1 ) 8.0.0
ToO aOGrj^epLvoO xoO xaxaptpd^ovToc; — j^L^' /^>^' ^^^^ position of the
head (node)
xaxaptpdCcov ( ^\J\ ) 8.1.2
TO aOGrj^epLvov ToO xaxaptpd^ovTOc; — j^L^' /^>^' true position of the head
(node)
xaxaptpdCcov ( ^1^1 ) 8.1.3
ToO xaxaptpd^ovTOc; — j^L^' head (node)
xaxapipd^cov ( ^--1^1 ) 8.3.1
To aOGrj^epLvov xoO xaxaptpd^ovTOc; — j^L^' /^>^' ^^^^ position of the
head (node)
xaxaptpdCcov ( ^\J\) 10.3.2.2
TO aOGrj^epLvov ToO xaxaptpd^ovTOc; — lT^J^ f y^ true position of the head
(node)
xaxaptpdCcov (y^j^l ) 11.1.1
242
ToO xaxapLpd^ovTOc; — ytij^\ node
xaxaXsLcpGsvTSc; ( iU^I ) 1.2
xaxaXsLcpGevTSc; ^fjvec; — iio^l jj-^l neglected months
xaxaXsLcpGr] ( rj^^^ ) l.l
xaxaXsLcpGrj — rj^ (there) results
xaTaXsLcpGr] ( jUI ) 2.2.2
d XL oOv xaxaXsLcpGrj — (j^ the remainder
xaTdXr)(];Lc; ( o^ ) 3.1
x/jv xaxdXri(J>LV — ii^^ for knowing
xaTdXr)(];Lc; ( jIaIo ) 8.0.0
x/jv xaxdXri(J>LV xfjc; SLa^expou xouxcov — U^^^^ jIaIo measure of their di-
ameters
xaxaXL^TidvsTaL ( LJiJi ) 1.2
xaxaXt^TidvexaL — LuiJi we cast out
XOLTZpX^TOil ( c^vJu ) 11.1.4
Ilepl xfjc; ^oLpac; exeLvrjc; yjxlc; xaxepx^xaL ^exd xfjc; aeXTQvric;
— j^\ "LfUi i^^wJu (^a)I tji-l the degree with which the moon sets
XSVTpOV ( ^bjMi ) 6.4
xevxpov xoO I OLXTQ^axoc; — :>bjMI the cardines
243
XSVTpOV {ifj^) 6.6; 8.3.3
TO xsvxpov — -fjA center
XSVTpOV [-J'JS ) 7.4
TOUTO xevxpov xaXeixai — ,3^^' l/^^ general center
XSVXpOV ( i-a> ) 7.4
TO xevxpov xal to a06T)^i£piv6v tou f)Xiou — ij:__yj^ j^oJJI Las.- argument
of the sun and its correction
XSVTpOV ( J'j» ) 7.4
TO xsvTpov — -fjA center
XSVTpOV ( L^i-I ) 8.1.1
xevTpov TOU rjXiou — o-lLiail L^il general argument
XSVTpOV ( LaJ-I ) 8.1.1
TO xsvTpov — 2Lail argument
xsvxpov ( A*^ ) 8.1.2
TO xevTpov Tf]<; ozkv^vf, — L-ajuJaU oAju; its doubled distance
xsvxpov {'jy^) 8.1.4
TO xevTpov — i^^JKJI ^J^liail •J'ys general center of the planets
xsvxpov {'jy^) 8.1.4
244
TO xevxpov — ^jUall •J'JS general center
XSVTpOV ^'/^S ) 8.1.4; 8.3.3; 8.3.4
ToO xeXsLou xevxpou — Jaj«II -J'ys equated center
XSVTpOV ^'/)S) 8.1.4
Tcp TsXsLcp xevxpcp — JajcII 'J'y\ equated center
XSVTpOV ['J'^\ ) 8.2
ToO xeXsLou xevxpou xoO daxepoc; exsLvou — ^.^^^5^1) JajJI j5^l equated
center for the planet
XSVTpOV ^'/)S) 8.3.2
xo xevxpov xo xsXslov — Jaj«II •J'J^\ equated center
XSVTpOV ^'/)S) 8.3.2
xevxpov — 'J'y\ center
XSVTpOV ^'/)S) 8.3.3
xoO xeXsLou xevxpou — -J'^s center
XSVTpOV ( io>U ) 8.3.4
£Lc; xo xdxco fj^LacpaLpLov xo xevxpov p — <^>U mark
XSVTpOV ( L.a^ ) 8.4.3
xax' evavxLov xoO xevxpou exsLvou — La> argument
245
XSVTpOV ( JJj ) 12.2.1
ToO xevxpou ToO 8' xal xoO i — ^}J^3 ^UJI (jXj the tenth and the fourth
cardines
XSVTpOV ( JJj ) 12.2.2
TO ^fjxoc; ToO OLGTspoq OLKO ToO xevxpou ToO l' y] toO 8'
— «j|JI jl ji>[jti\ (^Xj j^ c-^y^iCJl Aju the distance of the star from the tenth
or fourth cardine
XSVTpOV ( JJj ) 12.3.1
TO ^fjxoc; ToO alXax^ olko toO xevxpou
— JJ^I j^ /T^W^' -^ distance of the hayldj from the cardine
XSVTpOV ( ^bjMi) 12.3.1
si he TO alXax^ [xeaov eaxl xcov 860 xevxpcov — XjMI ijju jlS^ lil if it is
between the cardines
XLVSLXat ( ) 8.2
6 daxrip xax' 6p66v XLVSLxaL — ^^jlL^ i^^^\ the planet in direct (motion)
XLVSLXat ( ) 8.2.1
fivLxa XLvsLxaL xax' 6p66v 6 daxrip xal oxav 0Ti:oTi:o8L^r]
— i^lil^^llj 9^ y>-J\ oXa the time of retrogression and of direct (motion)
XLVSLXat ( ) 8.2.1
edv 6 daxrip XLvfjxaL xax' 6p66v — U^^Sl^.^ i^^^\ jlS^ lil if the planet is in
direct motion
246
XLVSLXaL ( >[ju^\ ) 8.2.1
xiveiTOLi xax' 6p66v 6 daxTQp — >lil^l direct motion
XLVSLXaL ( >[ju^>l\ ) 8.2.1
xiveiTOLi xax' 6p66v 6 daxTQp — >lil^MI direct motion
XLVSLXaL ( ^viluJ ) 8.2.2
XLvrjOiQaexaL xax' 6p66v — r^^^. it (the planet) is in direct motion
XLVSLXaL ( ) 12.3.2
f) ^OLpa eiq y]v XLVSLxaL x6 alXdx^ — i<s-^l »^yi location of the division
XLVSLXat ( ) 12.4.1
Kspi xfjc; evQuycfiaecdq exeivou xoO (J;7]cpou oxl xa6 ' exaaxov xpovov a ^6)8lov
XLVSLXaL
— <jljiu-^j V^^S^ *^-^ J^cJ LiY^' cJ ^^ ^'^^ intihd^ in every house and star
and its progrogations
XLVTTjaLc; ( <5^ ) 1.1
^ear) XLvrjaLc; xoO tiXlou — j^usJJl iia^j i5^ mean motion of the sun
XLVTTjaLc; ( <5^ ) 1.1
[xeay] XLvrjaLc; xfjc; aeXTQvric; — ^^1 iia^j i5^ mean motion of moon
XLVTTjaLc; ( olS^ ) 1.2
[xeaoLi XLVTQGSLc; xcov daxepcov — ^.^^iCJl Cj^j=> J^^LujI mean motions of the
247
planets
XLVTTjaLc; ( cj^j> ) 7.0.0
Tcov [xeacdv xlvtqgscov tcov daxepcov xaxa xpsLc; ^sGoSouc; —
^^^501 olS^ Jtf»Lujl mean motions of the planets
XLVTjaL^ ( ia^jMi ) 7.0.0
[isar] XLvrjaLc; xfjc; tioXscoc; — ^-^1 i^u.j'^l mean (motion) for the city
XLVTjaL^ ( ia^jMi ) 7.0.0
f) [xeay] XLvrjaLc; ^exa xfjc; opGciaecoc; xfjc; fj^epac; opGoOvxat
— L^JLJ^ i*^.^' Jd-^ (3^^^ Ja-u/jMI the mean (motion) corrected by the equa-
tion of the day with its night
XLVTjaL^ ( JpUjMI ) 7.0.0
xcov [xeacdv xlvtqgscov xcov daxepcov — ^.^^iCJl J^^L^jMI mean (motions) of
the planets
XLVTTjaLC; ( Cj^j^ ) 7.1
xcov ^eacov xlvtqgscov xcov daxepcov — ^.^^iCJl olS^ J^^LujI mean motions
of the planets
XLVTTjaLc; ( Afj^ ) 7.1
f) XLvrjaLc; — <5^ motion
XLVTTjaLC; ( ia-^j ) 7.1
xfj [xeari xlvtqgsl — Ja^j mean (motion)
248
XLVTTjaLc; ( <5^ ) 7.1.1
xfjc; ^earjc; xlvtqgscoc; — ol^j^^l '^J^ motion of the apogees
XLVTTjaLc; ( <5^ ) 7.2
f) ^ear) XLvrjaLc; xoO daxepoc; exsLvou — ^.^^^501 i5^ motion of the planet
XLVTjaL^ ( jbCJi J^jMi ) 7.2
TTJ dcTio xfjc; auvxd^ecoc; ^ear] xlvtqgsl — (J^^^ Ja-u^jMI mean in the text
XLVTTjaLc; ( Ja-^jMi ) 7.2
sOpLGxexaL f) ^ear) XLvrjaLc; xfjc; tioXscoc; exeLvrjc;
— OjJjiaJl (jiu Lo jLiiaij ^^-P^-uall Ja^j^l the mean corrected by the difference of
what is between the two longitudes
XLVTTjaLc; ( Ja-^ji ) 7.2
xfjc; \izoT\c, XLVTQGSCOc; xoO tiXlou — j^usJJl Ja-u/jl mean (motion) of the sun
XLVTTjaLc; ( Ja-^jMi ) 7.2
xfjc; \izoT\c, XLVTQGSCOc; xfjc; tioXscoc; — ^-^1 Ja^jl mean (motion) of our city
XLVTTjaLc; ( Ja-^jMi ) 7.2
f) xeXsLa opGcoGLc; xfjc; ^SGrjc; xlvtqgscoc; xfjc; tioXscoc; exsLvrjc; — ^J^^l Sa^^\
the corrected mean
XLVTTjaLc; ( <5^ ) 7.4
x/jv XLvrjGLV xcov dcGxepcov — <^^\ '^j> motion of the planets
249
XLVTTjaLc; ( Ja-^ji ) 7.4
al ^saaL XLVTQGSLc; Tcov daxepcov — i^^^^\ Ja^jl mean motions of the planet
XLVTTjaLc; ( Li^U ) 7.4
xriv IStav XLvrjaLV — Li^^U- proper (motion)
XLVTTjaLc; ( l^lilu/i ) 8.0.0
xfjc; xax' 6p66v xlvtqgscoc; xcov daxepcov — L^lil^l their (the planets') direct
(motion)
XLVTTjaLc; ( <5^ ) 8.0.0
f) XLvrjaLc; xouxcov sic; x6 tiXsov xal eXaxxov — iiilpJl [&^j=> their differing
motion
XLVTTjaLc; ( Ja-^ji ) 8.1.1
f) ^ear) XLvrjaLc; xoO tiXlou — l^ia^jl its (the sun's) mean (motion)
XLVTTjaLc; ( Ja-^ji ) 8.1.2
f) [xeari XLvrjaLc; — ^^1 Ja^jl mean (motion) of the moon
XLVTTjaLc; ( Ja-^j ) 8.1.2
f) ^ear) XLvrjaLc; xoO dvapLpd^ovxoc; — ^j^l Ja^j mean (motion) of the
node
XLVTjaL^ ( l^\^\ ) 8.1.2
f) ihioL TsXeioL XLvrjaLc; — ^Jajco L^lil equated anomaly
250
XLVTTjaLc; ( l^\^\ ) 8.1.2
IhioL TsXeioL XLvrjaLc; — iJAjJll 'L^[ji^\ equated anomaly
XLVTTjaLc; ( Ja-^ji ) 8.1.2
f) [xeay] XLvrjaLc; xoO dvapLpd^ovxoc; — ytij^\ \z^^\ mean (motion) of the
node
XLVTTjaLc; ( Ja-^ji ) 8.1.4
f) ^ear) XLvrjaLc; — Ja^jl mean (motion)
XLVTTjaLc; ( l^\^\ ) 8.1.4
TTJ lSloc xlvtqgsl — i^^lil anomaly
XLVTTjaLc; ( l^\^\ ) 8.1.4
xfjc; IStac; xeXsLac; xlvtqgscoc; — i^^lil anomaly
XLVTTjaLc; ( l^[jiL^\ ) 8.2
xfjc; xax' opGfjc; xlvtqgscoc; xcov daxepcov — SjjLpjil ^lil^l direct (motion) of
the planets
XLVTTjaLc; ( L^U ) 8.2
f) ISta xeXsLa XLvrjaLc; — ^JajJI L^U- equated anomaly
XLVTTjaLc; ( l^\^\ ) 8.2.1
f) ihioL TsXeioL XLvrjaLc; — i^^lil anomaly
251
XLVTTjaLc; ( 'k^j> ) 8.2.1
xriv xaxa to vu^QiQ^epov IStav XLvrjaLV xoO daxepoc; —
iiJj >^^ ^ 4J L^lil i5^ the motion of its (the planet's) anomaly in a day and
night
XLVTTjaLc; ( L^l}ti ) 8.2.1
xfjc; IStac; xeXsLac; xlvtqgscoc;. — iJAjJl L^lil equated anomaly
XLVTTjaLc; ( 'k^j> ) 8.2.1
x/jv IStav XLvrjaLv xoO daxepoc; exsLvou y]v XLvsLxaL xa6' ev vu^QiQ^epov
— iiJj >^^ ^ 'kjJK^\ '^y> motion of the anomaly in a day and a night
XLVTTjaLc; ( L^l}li ) 8.2.2
f) ISta izkziQL XLvrjaLc; — L^lil anomaly
XLVTTjaLc; ( L^l}li <5^ ) 8.2.2
x/jv IStav XLvrjaLv y]v XLvsLxaL 6 daxrip xaxd x6 vu^QiQ^epov — L^lil i5^
motion of the anomaly
XLVTjaL^ ( 'L^\:l\) 8.2.2
xfjc; IStac; xeXetac; xlvtqgscoc; — iJAjJl i^^lil equated anomaly
XLVTjaL^ ( <5^i) 8.2.2
f) ISta XLvrjaLc; xoO xaxd vu^QiQ^epov xlvou^svou daxepoc; — <^lil i5^l
motion of the anomaly
XLVTTjaLc; ( Ja-^j ) 8.3.1
252
f) [xeay] XLvrjaLc; xoO dvapLpd^ovxoc; — ytij^\ Ja^j mean (motion) of the
node
XLVTTjaLc; ( ji-uoo ) 8.4
f) XLvrjaLc; Tcov daxepcov £Lc; TO aOGrj^epLvov — ^^^1 ^ i^^^^\ j^^^^ motion
of the planet in true position
XLVTTjaLc; ( L^U ) 8.4.3
xfjc; ihioiq xlvtqgscoc; xfjc; aeXrivriq — '<L^\£> anomaly
XLVTjaL^ ( ) 10.3.1.3
xfjc; £v xcp ^Lxpcp xuxXcp lSloc xal lSloc xauxTjc; xlvtqgscoc;
— ^.j-vl)l dlU ^ j^\ j^ the being of the moon in the sphere of (its) epicycle
XLVTTjaLc; ( ji^' ) 12.0.0
xfjc; XLVTQGSCOc; xcov ^OLpcov — UjwJj ol^^Jl intihd^ and their prorogations
XLVTTjaLc; ( ji^i ) 12.2.2
TiXdxoc; eaxl xoO xuxXou xfjc; xlvtqgscoc; — ^Jhi-^' v'-^ J^J^ latitude of the
circle of the prorogation
XLVTTjaLc; (j^u^i ) 12.2.2
Kspi xoO TiXdxouc; xfjc; xlvtqgscoc; xoO xuxXou
— c-^^^^L jju-^1 5y !:> j^j^ 'isjji^ ^ on the knowledge of the latitude of the
circle of prorogation approximately
XLVTTjaLc; (jju^i ) 12.2.4
253
TO TiXdxoc; xfjc; xlvtqgscoc; toO xuxXou — ^i^^' 5y '-^ <y^J^ latitude of the
circle of prorogation
XLVTTjaLc; ( ji^' ) 12.3
Tiepl xfjc; XLVTQGSCOc; xoO alXax^ — /T^^' ^i^^' cJ ^^ ^'^^ prorogation of the
haylaj
XLVTTjaLc; ( O'La^' ) 12.4.1
xal f) XLvrjaLc; exsLvr) sic; xpta xLvd sgxlv — ^^ '^ ^ ^^^..y^ its pro-
rogations are in three types
XLVTTjaLc; ( j^' ) 12.4.2
Seuxepov sic; x/jv XLvrjaLv xcov ^rivcov
— jj-pJl tM:>l ^Jhi-^' J-^J Jd^^' c5Y^ cJ cJ^' second: on the muntahd^ of
the revolution which is the prorogation of the indicators of the month
XLVTjaL^ ( i5^ ) 12.4.2
f) XLvrjaLc; sgxlv f) ^ear) xoO tiXlou — j^usJJl '^j> motion of the sun
XLVTTjaLc; ( j^' ) 12.4.2
Tiepl xfjc; XLVTQGSCoc; xcov (J;7]cpcov xfjc; xuxtjc; xfjc; elaeXeuaecoc;
— iL^I Jd^^" ^^-^^ ^i^^' cJ ^^ ^'^^ prorogation of the indicators of the revolu-
tion of the years
xXfjpoc; ( ) 6.2
6 xXfjpoc; xfjc; xuxTjc; — JUJI ascendant
254
xXt^a ( ^^^\ ) 9.2
xavovLov TsQeixev sic, xa ^ xXt^axa — ^Ml region
xXt^a ( ^xiiMi) 11.5.1
'H^SLc; xavovLov eGiQxa^ev xal xa xo^a ocTiep eSo^ev xeGsLxa^ev sic; sxslvo x6
xavovLov ^£xa xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xac; OLpy^oiq xcov ^coSlcov
— ^^11 ^ ^^^J^^ oU^lia^^Uj /TJ^^ ^!>^^ ij^ ^O^^ ^jAs> jljil LitJpj
We have set out the values of the limits of sighting in degrees of the zodiacal signs
and for the initial declivities in the fourth clime at the beginnings of the zodiacal
signs
xXoTiL^atoc; ( aI^kL^ ) 1.2
xXoiii\iQd(xi fj^epaL — il^JLo L^usil five days are added
xXoTiL^atoc; ( Sjjyi ) 1.2
xXoiii\iQd(xi fj^epaL — '6ju\J\ additional (days)
xXoTiL^atoc; ( oJL^ ) 1.2
xXoiii\iQd(xi fj^epaL — 'isJL^^ stolen (days)
xoxxLvoc; ( ^y^ ) 8.3.2
Sloc xoxxlvou — tl^ red
xo^Tioc; ( OAip ) 10.2.1.1
xcov xo^Ticov — oAip its (the moon's) node
255
x6o[ioc, ( Ia\ ) 1.2
dcTiciXsLa xoa^ou — ^1 ^>U destruction of the world
xpaxsLxaL ( ) 11.1.4
TO TO^ov TauTTjc; xpaxsLxaL — 'L^^ we take its arc
xpaxoOvTaL ( bj^l ) 1.2
xpaxoOvxaL ol xpovoL xexeXsLCO^evoL xoO exouc; xoO 'laaSaxepSr)
— ^bl ^^>;;:i ^J^^ [jJ^\ we take the completed years of Yazdijird
xpaxoOaLV ( J.<UiJ ) 1.1
xpaxoOaLV — Jl<s.*1^I employ
xps^axat ( lliip ) 11.4.1
6 daxpoXdpoc; sic; x/jv xdGsxov exsLvriv xpe^axat — ^^Sj^a^S] LiUl^ we hang
the astrolabe
f) dpXTT) TOO KpLOO ( ^^^,J\ ^\Xis^>l\ iiai; ) 1.2
yjXloc; £c; x/jv dpxTjv xoO KptoO — ^y^.J^ JljI^MI iial5 j^usJJl cJi^ the sun
came to the point of the Spring equinox
KpLo^ ( ^^^J\ ^\j^"^\ iiai; ) 1.2
f) eiaeXexjGic, xoO tiXlou sic, xov Kptov
— ^y^,J\ JIjI^MI iiaU j^usJJl Jl^" jI when the sun enters the point of the
Spring equinox
XpU(];L^ ( Lij-uJli) 10.2.2.1
256
TO xavovLov xfjc; xpucj^ecoc; xfjc; aeXTQvric; — ^j^\ l3j-^I Jj-^ table of the
lunar eclipse
xuxXoc; ( ^^ ) 1.1
^cdhioixbq xuxXoq — /TJ^' ^ sphere of the zodiacal signs
XUXXO^ ( SJijJi ) 2.2
xuxXoc; — SyljJl circle
XUXXO^ ( Syi:) ) 3.0.0
Tov xuxXov ToO ^eaou xfjc; fj^epac; — jl^Jl cJLuaj oJ\^ circle of half the day
xuxXo^ ( .^ ) 3.1
ToO ^cpStaxoO xuxXou — /TJ^' ^^ sphere of the zodiacal signs
6 TsXsLOc; xuxXoc; xfjc; fj^spac; ( jLjAll Ja^ ) 3.3
ToO TeXsLou xuxXou xfjc; fj^epac; — jV^' Jajco equalizer of the day (equator)
6 TsXsLOc; xuxXoc; xfjc; fj^spac; ( ) 4.1
£Lc; Tov TsXsLov xuxXov SLGL xfjc; fj^epac; xal TiXdxoc; dvaxoXfjc; oOx e-z^ouaiv —
JIjI^^I iiaU lJl^ ^^^ ^iiaj it rises on the point of the equinox itself
xuxXoc; xfjc; opGc^ascoc; xfjc; fj^spac; ( jl^i Ja^ ) 5.2
ToO xuxXou xfjc; opGciaecoc; xfjc; fj^epac; — jV^' Jajco the equalizer of the
day (equator)
xuxXoc; ( 'SJ\^ ) 6.6
257
xuxXoc; — oJ\^ circle
xuxXo^ (jj-^0 8.0.0
6 (J;fjcpoc; xoO xuxXou ( yjtol xfjc; acpatpac; ) TSTsXeLCO^evou — jjjJl >Lr com-
pletion of the rotation
XUXXO^ ( Syi:) ) 9.1.3
elq Tov xuxXov ToO \ieao\j xfjc; fj^epac; — jV^' cJLuaj Syl:> ^^ on the circle
of half the day
xuxXoc; ( 'SJ\^ ) 9.1.4
TOV xuxXov xfjc; dvapdaecoc; — pUjjMI Syl:> circle of altitude
xuxXoc; (^^jjJi ) 9.2.4
TO ucj^co^a ToO ^LxpoO xuxXou — ji.^^^ '^^j^ apogee of the epicycle
xuxXo^ ( ^.jJdi <^ ) 10.3.1.3
xfjc; £v Tcp ^Lxpcp xuxXcp lSloc xal lSloc TauTTjc; xlvtqgscoc;
— jj^^^\ <^ ^ j(^\ 03^ the being of the moon in the sphere of its epicycle
XUxXo^ ( lj\^ ) 12.2.2
TiXdxoc; eaxl xoO xuxXou xfjc; xlvtqgscoc; — ^i^^' '^J^^ c^j^ latitude of the
circle of the prorogation
XUxXo^ ( lj\^ ) 12.2.2
Tiepl xoO TiXdxouc; xfjc; xlvtqgscoc; xoO xuxXou
— c-^^^^L jju-^1 5y !:> c^j^ 'isjjui ^ on the knowledge of the latitude of the
258
circle of the prorogation approximately
XUxXo^ ( 'SJ\:> ) 12.2.4
TO TiXdxoc; xfjc; xlvtqgscoc; toO xuxXou — ^i^^' v'-^ J^j^ latitude of the
circle of the prorogation
XaxpsuovTSc; xcp TiupL ( ) 1.2
ol XaxpeuovTSc; xcp Tiupt — i^^^^l ^.> Mazdaism
XsTixd ( J!U^ ) 2.1
XenTOL — ^^^ minutes
XsTlxd ( 'ilJ:> ) 4.2; 8.3.2; 8.3.3; 8.3.4
XsTixd yevLxd — ^.^^^1 ^^-^ minutes of proportion
XsTixd (^) 7.3.1
SKeiTOi TTipehoii eiq xd XsTixd xcov fj^epcov xfjc; fepSo^dSoc;
— ol^tdjll jyj^ ^\ \jj^ we look at the fractions of weeks
XsTixd (^^i) 7.3.2
xd XsTixd xcov fj^epcov xfjc; fepSo^dSoc; — oL«^l ^^\ ^ j^jJl ^^^JCJI fractions
which are with the days of the week
XsTlxd ( J^U^ ) 8.1.2; 8.3.4
xd yevLxd XsTixd — ^.^^^1 (3^^-> minutes of proportion
XsTixd ( ^\3^ ) 8.3.3
259
xa yevLxa XsTixd — jJll ^.^^ ^^^ minutes of proportion of declination
XsTixd ( ^\s^) 9.1.4
xa XsTixa xoO aOGrj^epLvoO — ^^^1 (3^^-> minutes of true position
XsTlxd ( J^U:) ) 9.2.1
XsTixd — 3^^-> minutes
XsTixd ( J^U^ ) 9.2.5
xd XsTixd xd ebpsQevTOi ev xcp xavovLcp xoO tiXslovoc; xal eXdxxovoc; xoO lSlou
xfjc; aeXTQvric; — j.^^^ l3>Ii^I (3^^-> minutes of difference of the epicycle
XsTixd ( ^\s^ ) 10.2.1.3
XsTixd xfjc; exXsLcJ^ecoc; — l3j-^I (3^^-> minutes of the eclipse
XsTixd ( ^\s^ ) 10.2.1.4
£X£Lva XsTixd XeyovxaL xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; — X^yuA] ^\s^ minutes
of half duration
XsTixd ( j:U^ ) 10.2.1.5
xd XsTixd xfjc; axdaecoc; — JU5CII (3^lS:> minutes of duration
XsTixd ( j:U^ ) 10.2.2.1
xd XsTixd xoO aOGrj^epLvoO — ^ yi:}] ^\s^ minutes of the true position
XsTixd ( J5U^ ) 10.3.2.2
XsTixd XeyovxaL xfjc; exXsLcJ^ecoc; — l3j-uJCJI (3^l5:> minutes of the eclipse
260
XsTixd ( J^Uj ) 10.3.2.3
xa XeTixa ToO au6T)[i£pivou — i^_^il)l JjjUi minutes of the true position
XsTixd ( J^UjJI) 11.1.4
dTio [jioipcov xal Xetitwv — ^ISaJIj /Tj-^I ^ in degrees and minutes
XsKxd ( J.'U^ ) 11.2.1
xa Xejixa ToO au6T]^i£pivou — o_^2JI J^\Js:> minutes of true position
XsKxd (jsS) 12.1.1
xa Tiptoxa xal P' XcTixd — j^ fractions
XSKTOV ( Jl^ili ) 2.2
Seuxepov Xejixov — ijl?^' seconds
[iaxpdv ( i.U ) 3.2.1
oxav SitaxaxL xf)(; Yf)(; [jiaxpdv — 9- liujl iiU- limit of the altitude
}jiZYioi:oc, ( ) 1.2
SfjXai xal [isyiaxai r][ji£pai — ^aaUiII j»IjI famous days
}JiZYioi:oc, ( ioJafr ) 1.2
[isyiaxov Ipyov xwv xoO oupavoO — Z^[a oIjJ ^ *-»i)^^ ^:>\s- great oc-
currence of atmospheric marvels
[xeyioToc, ( loJas- ) 1.2
261
^syLGTOV gpyov xcov xfjc; yfjc; — V^j' oLo>U j^ ioJa^ <j:>U" great occur-
rence of earthly signs
[iiOoho<^ ( oLoAlli ) 10.3.2
SsL SLTiSLv TLGL ^sGoSoLc; ^9"^^^^^^^ XP*"! — oLoAllI premiscs
^SLoOxaL ( ) 1.2
f) aeXTQvr) au^SL xal ^SLoOxaL — IIaS] (O-^jj Sjt^ multitude of their sight-
ings of lunar crescents
[liXoiC, ( ^^y^ ) 8.3.2
Sloc ^eXavoc; — t\^y^ black
^sptCsTaL ( ) 12.4.1
el XL eOpsGrj exeivo eiq xa lP ^epL^exat fjyouv dva lP ytvexat xouxcov ac^oiipeaiq
— jLs^ (jbM iJLlI ^ LuiJi we cast off twelve from the result
^sptCovxaL ( Lc^ ) 1.1
^spL^ovxaL — Ld-^ we divide
^spLG^oc; ( Ic^u^i ) 12.3.2
xoO ^epLG^oO xfjc; ^otpac; xoO alXdx^ — /T^^' 0^ io-^l the division of the
hayldj
[lZpO(^ ( ^j> ) 10.2.1.4
fivLxa exXsLTiSL ^epoc; xfjc; aeXTQvric; — ^j^^ j^ cJ ^J-^' o^ 1->1 when
the eclipse is in part of (its) body
262
[XZpOCi ( ) 10.3.2
TO \xepoc, TTJc; Suaecoc; — ^^i- western
[iSpOC ( ) 10.3.2
TO \xepoc, TTJc; dvaToXfjc; — ijj^ eastern
[ispoc; ( ) 10.3.2.1
zic; TO iiipoc, Tf]C, Suaecot; — L^ western
[ispoc; ( ) 10.3.2.1
zic; TO iiipoc, Tf]C, dvaToXf)(; — ^j-^ eastern
[ispoc; ( ^^ ) 10.3.2.2
Iiipoc, exXeiTiei toO f)Xiou — V'^ lJl^JCj part of it (the sun) is eclipsed
[iSpOC ( ip. ) 12.2.3
TO [ispoc; — ip- direction
[iSpOC ( ) 12.3.2
f) [jioipa ToO [jiepouc; toO aiXdcTC — <u-^l f^Jpyo location of the division
[XZOOV ( jljAli cJLuaJ <^ ) 1.1
TO [xzaov Tfjc; rjfjiepac; — jV^' i-i-aj i^ sphere of half of the day
[XeOOV ( cJiuaJ ) 1.2
[isaov TTJc; fiiiepaq — >y_ L-i-aJ half of the day
263
}JiZGO\^ ( ) 8.4
>^^ J I >^^ ^ from day to day
[IZGOV ( ia^j ) 10.3.2.1
TO [xeaov xfjc; exXsLcJ^ecoc; — l3j-uJCJI Ja^j ol^Lu hours of the middle of the
eclipse
[lioo^ ( Jijji) 10.3.2.1
xax' evavTLov xoO ^eaou xfjc; fj^epac; ytvexaL eiaeXeuaic,
— Jljj;)! tljL Lo Aci"Lli we take whatever is opposite noon
[IZGOV ( ) 10.3.2.2
x6 [xeaov xoO tiXlou exXslcJ^sl f) Se TiepLcpepsLa oOx exXslcJ^sl
— j^ iiW j^usJJl >js>- ^ yi2i\ ^y> around the moon from the body of the
sun is a ring of light
[IZGOM ( cJLuaJ ) 12.1.1
f) oSpa xoO [xeaou xfjc; fj^epac; — jV^' cJLuaj ol^Lu hours of half the day
}JiZGO\^ ( Ja-^j ) 12.1.3
xfjc; xuxTjc; xoO ^eaou xfjc; olxou^evric; — 5jju^j«II Ja^j /^^J ^' /^^ ^^"
cendant of the cupola and the ascendant of the middle of the inhabited world
[IZGOM ( Oi^ UJ ) 12.2.1
si he 6 daxfip [xeaov xoO 8' xal xoO C
264
— «jLJIj 9u\J\ ijiu UJ c-^i^5CJl jir jl if the star is in what is between between
the fourth and the seventh
[izao^ ( Oi^ UJ ) 12.2.1
eav \iioo\ xfjc; tuxtq^ ^^o^^- '^^^ S' — /^L^ls ^UJI ijju UJ jlS^ it (the planet)
is in what is between the ascendant and the fourth
[izaov ( Oi^ UJ ) 12.2.1
6 daxrip \iioo\ xoO i xal xoO a OLXTQ^axoc; xoO xotiou xfjc; xuxtjc;
— ^JliaJlj ^LJI ijiu UJ o^ jl - c-^i^iCJl if the star is in what is between the
tenth and the ascendant
\izaov ( Oi^ ) 12.3.1
£L hz x6 alXax^ ^eaov eaxl xcov Suo xevxpcov — XjMI ij^u jlS^ lil if it is
between the cardines
[iZaOq ( iia-^j ) 1.1
^ear) XLvrjaLc; xoO tiXlou — j^usJJl aWm>j <5^ mean motion of the sun
[iZaOq ( iia-^j ) 1.1
\iior\ XLvrjaLc; xfjc; aeXTQvric; — ^^1 iia-^^j i5^ mean motion of the moon
[izaoq ( JpUjI ) 1.2
^saaL XLVTQGSLc; xcov daxepcov — ^.^^iCJl Cj^j> J^^LujI mean motions of the
planets
\izaoq ( J^jMi ) 1.2
265
6 [isaoq (J>fjcpoc; — ]a^^S\ jIaIo measure of the mean
[l£GO^ ( J^jMi ) 11.3
6 [leooci (J;fjcpoc; — ^^'j cJ3^' ^^ Ja1«II Ja-^jMI jJ-l the mean equated
limit of the first and second arcs
[IZGOC, ( 0\j ) 12.3.1
f) iiepiaaeioL f) ^ear) xoO totiou xfjc; tuxtjc; xfjc; [xoipoLc, exeivou
— /T^^' ^J-^ ^^Ua^ Oju iLiai the excess (of what is) between the rising times
of the degree of the hayldj
[lZGO(^ ( ) 12.4.2
f) XLvrjaLc; eaxLV f) \iear] xoO tiXlou — j^ujJJl 'i^j=> motion of the sun
^saoupdvTTj^a ( ia-^^i: ) 5.3
6 daxrip oOxoc; Tipoxepov xfjc; IStac; ^oLpac; cpGdvsL sic; x6 ^eaoupdvri^a —
JuS glo^cJl lg,c.>^^ 4jU if it reaches the midheaven beforehand
^sxapaLVSL ( J^-> ) 1.2
ox£ 6 yjXloc; duo ^coSlou [xenoi^oiivei eiq ^6)8lov — /TJ^' J^-ls' j^usJJl J^^^
the entrance of the sun into the beginnings of the zodiacal signs
^sxdpaaLc; ( cu^ ) 8.4
xfjc; ^exapdaecoc; tiXlou xal aeXr]vr](; — ^jd^' ^^ the daily velocity of the
sun and moon
^sxdpaaLc; ( ^^\ cu^ ) 8.4
266
f) XLvrjaLc; xcov daxepcov sic; to aOGrj^epLvov duo xoO \ieao\j xfjc; fj^epac; ^^XP^
xal ToO STspou ^eaou xfjc; fj^epac; [xeTOi^oiaiq Xeyenoii — i^^^\ C/^ daily velocity
of the planet
^sxdpaaLc; (jj.uoo)8.4
xriv ^STdpaaLV xoO daxepoc; sic; x/jv ^Lav oSpav
— ipLu ^ L-iilpcll ojiu^.^ its varying motion in an hour
^sxdpaaLc; ( cu^ ) 8.4.1
f) ^sxdpaaLc; exsLvou — C/^. daily velocity
^sxdpaaLc; (j^lu^o ) 8.4.1
f) ^sxdpaaLc; xoO tiXlou xrjpeLxaL sic; x/jv ^Lav oSpav sic; xd vy' XsTixd —
ipLu ^ Uj\-u.^ its motion in an hour
^sxdpaaLc; ( j^-u^o ) 8.4.3
xfjc; [xsTOi^oiaecdq xoO tiXlou xal xfjc; aeXrivriq — ^j:!^' iSj"*^ motions of the
two luminaries
^sxdpaaLc; ( ^l^ / cu^ ) 8.4.3
f) ^sxdpaaLc; xoO tiXlou slc; x6 £v vu^QiQ^epov xal sic; x/jv ^lav oSpav —
ipLu ^ Uj^u^.^j j^usJJl C/^. the daily velocity of the sun and its motion in an hour
^sxdpaaLc; ( jy^ / cu^ ) 8.4.3
f) ^sxdpaaLc; xfjc; aeXTQvric; sic; x6 £v vu^QiQ^epov xal sic; x/jv ^lav oSpav —
ipLu ^ oj\-ucoj ^;^l C/^ the daily velocity of the moon and its motion in an hour
267
^sxdpaaLc; ( cu^ ) 9.1.4
xfjc; [iSTOL^OLaecdc, aeXTQvric; — C^ its (the moon's) daily velocity
^sxdpaaLc; ( j^-u^o ) 9.1.4
xfjc; [xsTOi^oiaecdq fikiou xal aeXrivriq — (jd^' ^i-^^ motion of the two lumi-
naries
^sxdpaaLc; ( cu^i ) 10.1
xfjc; auvoSou xoO tiXlou xal xfjc; aeXTQvric; xal xfjc; SLa^expou xouxcov xal xoO
^TQXouc; xfjc; xouxcov ^exapdaecoc;
— C/Y^lj AjcJL o^JLil^^Jlj ol^Ul5»"MI conjunctions and oppositions in dis-
tance and daily velocity
^sxdpaaLc; ( J^ ) 10.1.1
x/jv xeXelav exsLvriv ^sxdpaaLV — yi2i\ 3^^ i^j-^^ extension of the prece-
dence of the moon
^sxdpaaLc; ( J^ ) 10.1.1
£X£Lvo ^sxdpaaLc; XeyexaL xeXela — jA2i\ 3^^ precedence of the moon
^sxdpaaLc; ( cu^ ) 10.1.1
STiSLxa f) ^sxdpaaLc; xoO fiXlou dcpaLpsLxaL duo xfjc; ^exapdaecoc; xfjc; aeXTQvric; —
^r«^l C/^ j-o j^usJJl C/^ Luaij we subtract the daily velocity of the sun from the
daily velocity of the moon
^sxdpaaLc; ( cu^ ) 10.1.1
f) ^sxdpaaLc; fiXlou xal aeXTQvric; — C/^ daily velocity
268
[ence
^sxdpaaLc; ( J^ ) 10.2.1.4
xriv TsXeioLv ^sxapaaLv xfjc; aeXTQvric; xriv xaxa x6 vu^QiQ^epov —
'^J r^^. cJ J^^ <3^^ precedence of the moon in a day and its night
^sxdpaaLc; ( J^ ) 10.2.1.5
x/jv xeXsLav ^sxdpaaLV xoO vuxQTj^epou — 4JLJ5 >^^ ^ yjii] J.^^ preced
of the moon in a day and its night
^sxdpaaLc; ( cu^ / ^l^ ) 10.2.2.1
x6 xavovLov xfjc; ^exapdaecoc; tiXlou xal aeXTQvric;
— ^^1 ♦^^^^Y^ Od^' ^i-^^ Jj^ table of the motion of the two luminaries with
the daily velocity of the moon
^sxdpaaLc; ( J^ ) 10.3.2
f) TsXeioL [iSTOL^oLGic, xfjc; aeXTQvric; sic; ^tav oSpav — i^Lu ^ ^^1 3^^ the
precedence of the moon in an hour
^sxdpaaL^ ( <5^ ) 10.3.2
f) ^sxdpaaLc; aOxfjc; eiq x/jv ^Lav oSpav — ipLu ^ ^5^ its (the moon's)
motion in an hour
^sxdpaaLc; ( <5^ ) 10.3.2
f) ^sxdpaaLc; xoO tiXlou (baauxcoc; sic; ^Lav oSpav — ipLu ^ ^^J^ its (the
sun's) motion in an hour
^sxdpaaL^ ( J^ ) 10.3.2.1
269
xriv TsXeioLv ^sxapaaLv xfjc; aeXTQvric; sic; [xLolv oSpav — ipU ^ ^^1 ^J^^
precedence of the moon in an hour
^sxdpaaLc; ( cu^ ) 10.3.2.3
xfjc; [xsTOi^oiaecdq exsLvrjc; — ^^1 C/^. daily velocity of the moon
^sxdpaaLc; ( cu^ ) 11.1.1
x/jv ^sxdpaaLV xfjc; aeXTQvric; sic; x/jv ^Lav oSpav — yi2i\ C/^ daily velocity of
the moon
^sxdpaaLc; ( J^ ) 11.1.1
f) ^sxdpaaLc; xfjc; aeXrivriq eiq [xioiv oSpav — ol^Lu ^ ^^1 3^^ precedence
of the moon in hours
^sxdpaaLc; ( L^U / cu^ ) 11.3
xoO lSlou y] xfjc; ^exapdaecoc; xfjc; aeXTQvric; — C^ jl ^^1 ^.^U- anomaly of
the moon or its daily velocity
^sxdpaaLc; ( cu^ ) 11.5.2
x/jv xeXsLav ^sxdpaaLV — i^^^\^ j^usJJl ijju CU^)! JlJi^ excess of the daily
velocity between the sun and the planet
^sxdpaaLc; ( cu^i ) 11.5.2
'H [iSTOL^oLGic, xoO tiXlou xal exeivoxj xoO daxepoc;
— c-^y^iCJlj j^usJJl ijju <z^\ the daily velocity between the sun and the planet
^sxdpaaLc; ( cu^ ) 11.6.1
270
f) [ieTOL^OLGiq xfjc; aeXfjvric; — y^\ cu^. the daily velocity of the moon
^sxdpaaLc; ( cu^ ) 11.6.2
f) [xsTOi^oiaiq xfjc; aeXfjvric; — ^^1 cu^. the daily velocity of the moon
^sxdpaaLc; ( cu^ ) 12.1.1
xriv ^sxdpaaLV xoO tiXlou — j^usJJl C/^. the daily velocity of the sun
[IZTCixXlGlC, ( Ju^ ) 3.0.0
[xsTOixXiaiq — Jl^ declination
[IZTCixXlGlC, ( JJi ) 3.1
f) [isyaXr] [iSTOLxXiaiq — p]as^S\ Jul I the greatest declination
[IZTCixXlGlC, ( jJi ) 3.4
xfjc; xexeXsLCO^evrjc; ^exaxXLaecoc; — jJ,! >Lc complement of the declination
^sxaxXtaLc; ( Ju^ ) 6.5
f) ^exdxXLGLc; xoO tiXlou — j^ujJJl Ju^ declination of the sun
[IZHOixXlOlC, ( Ju^ ) 7.4
x/jv ^exdxXLGLV xoO tiXlou — j^usJJl Ju^ declination of the sun
[iznoixXioic, ( jJi ) 9.1.3
eiq x/jv ^exdxXLGLV xoO oXou xoO ycfixouq xfjc; ycovtac; xexeXsLCO^evrjc; xoO TiXdxouc;
(...) xfjc; ycovLac;
— Jjia)l h3^j 0?e«-^' (J' W^^j J^^^ '^'3^J ^ J^' r^ jIaI/ the measure of
271
the complement of the declination is the angle of latitude and its complement to 90
is the angle of longitude
^STpOV ( ) 8.0.0
[xenpov — :>AjJI ^^Wm> two columns of numbers
^STpOV ( ) 8.1.4
ToO [iSTpoxj — :>AjJI (^^r^ two columus of numbers
[iflXO^ ( J> ) 1.2
TO ^fjxoc; Tcov 9 — i^l Jj-U longitude of the Cupola
[ifixo^ ( ^^ ) 3.0.0
ToO ^TQXouc; xfjc; tioXscoc; — jJJl j^y- latitude of the city
^fjxoc; ( Juio ) 3.1
ToO [xrixouq xoO daxepoc; fjyouv xfjc; xcov daxepcov SLaaxdaecoc; duo xfjc; neXeioiq
^(ivrjc; xfjc; fj^epac; — jV^' Jajco js^ i^^^^\ Aju distance of the star from the equal-
izer of the day
[ifixoc, ( Ju«Ji ) 3.3
x6 ^fjxoc; xoO daxepoc; olko xoO xeXsLou xuxXou xfjc; fj^epac;
— jLpJl Jajco j^ c-^y^iCJl Aju distance of the star from the equalizer of the day
^fjxoc; ( Ju«Ji ) 3.3
x6 ^fjxoc; — AjcJI distance
272
[iflXOC, ( A*j ) 5.2
ToO [iTJxouc; ffioi TTJc; biaaxdaecxic, twv daxspcov duo xoO xuxXou xoO xaxd x6
vux6TJ[jiepov xivou[jievou — jV^' Jajc« rjS- a*j its distance from the equalizer of the
day
[ifixOC; { Xmj) 5.2
x6 [jifjxoc; xoO daxepoc; duo xfjc; opGwaswc; xoO xuxXou — jV^' jAjt« ^^ oa*j
distance from the equahzer of the day
[iYJXOC; ( A*j ) 6.5.2
x6 [jif)xo<; xou doTSpoc; — t^^J^^I Aju; distance of the star
[xfixo<; ( ^^ ) 6.5.2
TO ^TQXouc; xfjc; tioXscoc; — (j^^ latitude
[xfixo<; ( J_^ ) 6.7
xou [xrixouc, xou Maxxd — iC« JjAs longitude of Mecca
}J.f]XOC, ( J_^ ) 7.0.0
[ifjxoc; — Jjis longitude
[iYJXOC; ( A*Ji ) 8.1.4
x6 eyyuxepov [jifjxoc; — s-"^*^' -^' closest distance
[ifixoc, ( A*Ji ) 8.1.4
x6 Tioppco [jif)xo<; — JjuSlI A*JI the furthest distance
273
[lfiXO<^ ( J^O 9.1.5;9.2.1
TO ^fjxoc; xal TiXdxoc; — Jj^aJl longitude
^fjxoc; ( Juio ) 9.3
TO ^fjxoc; xfjc; aeXrivriq olko xfjc; Tuyjiq — ^JUJI j^ ^^1 Aju distance of the
moon from the ascendant
[lfiXO(^ ( J^i ) 9.3
TO TiXeov xal eXaxxov xfjc; ocj^ecoc; exsLvrjc; sic; xo ^fjxoc;
— JjiaJl ^ jiaLa l3M^1 difference in vision in longitude
^fjxoc; ( JL«Ji) 10.1
xfjc; auvoSou xoO tiXlou xal xfjc; aeXrivriq xal xfjc; Sta^expou xouxcov xal xoO
^TQXouc; xfjc; xouxcov ^exapdaecoc;
— C/Y^lj AjcJL o^^Lfil^^^lj oU-Ul>^ll conjunctions and oppositions in dis-
tance and daily velocity
^fjxoc; ( Ju«Ji ) 10.1.1
x6 ^fjxoc; x6 [xeaov fjXLOu xal aeXrivriq — Aj«JI i^j-^^ extension of the
distance
^fjxoc; ( JL«Ji) 10.1.2
x6 [xeaov xouxcov ^fjxoc; — U^vo Aj«JI the distance between the two
^fjxoc; ( JL«Ji) 10.1.3
x6 ^fjxoc; oKsp £xpax7]6ri [xeaov xoO fjXLou xal aeXTQvric; — ^jd^' 0^. -W^'
distance between the two luminaries
274
^fjxoc; ( Juio ) 10.3.2
£X£Lvo oOv TO ^fjxoc; eijiep eaxl eXaxxov xcov 9 ^otpcov
— O^ji^ ^ Jil ^liaJl ^ tjJ^\ Aju the distance of the degree from the ascen-
dant is less than 90
^fjXOC; ( Juio ) 10.3.2
^fjxoc; eaxL xcov ^OLpcov xfjc; auvoSou — pUi^*-"^! ty>- Aju distance of the
degree of the conjunction
^lyjxo*; ( ^y ) 11.5
x6 ^fjxoc; xoO daxepoc; olko xoO tiXlou tiogov svl
— i^LlI Jtf»lia^'^l jl i>^Lll JU5CII j^^^ the taken arc of duration or the taken
(arc) of declivity
[lflXO(^ ( J^ ) 12.1.1
£Lc; x6 ^fjxoc; xfjc; tioXscoc; exeLvrjc; £v6a xal f) yevvrjaLc; — ->MJ*1 Jj-!^ (^ for
the longitude of the nativity
^fjxoc; ( Juio ) 12.2.1
^fjxoc; eaxL xoO daxepoc; duo xoO 8' — ^jI^I j^ oAju its (the star's) distance
from the fourth
^fjxoc; ( JL«Ji) 12.2.1
^fjxoc; eaxL duo xoO i — ^LJI j^ c-^i^5CJl AjJI the distance of the star
from the tenth
275
^fjxoc; ( jLio ) 12.2.1
ToO ^TQXouc; Tcov daxepcov — i^^^^\ Aju distance of the star
^fjxoc; ( jLio ) 12.2.2
TO ^fjxoc; ToO daxepoc; olko toO xevxpou xoO l' y] toO 8'
— «j|JI jl ^LJI (^Xj j^ c-^y^iCJl Aju the distance of the star from the tenth
or fourth cardine
^fjxoc; ( jLio ) 12.3.1
TO ^fjxoc; ToO alXax^ OLub xoO xevxpou
— JJ^I j^ /T^W^' -^ distance of the hayldj from the cardine
[xriv ( ) 1.1
^riv TipoaTLGsxaL — j^^ intercalate
^TTJV (j^t^i) 1.1
^7] V — J j-pJ ' months
^TTJV (j^t^i) 1.2
iU^I jjr^' neglected months
[X-flV {jy^\) 1.2
ol ^fjvec; ToO Gs^eXlou — ^Jl^^^I jytr^^ months of the base
^>^V ijy^) 1.2
ol [xfiveq s^LGoOvxaL [xstol xcov 8 xatpcov
— iL^I Jj-^ ^ jjr^ ^^^ months (are fixed) with the seasons of the year
276
^rjv {jy^\) 12.4.2
SeuTspov £Lc; xriv XLvrjaLv xcov ^rivcov
— jj-pJl tM:>l ^Jhi-^' J-^J Jd^^' c5Y^ cJ cJ^' second: on the muntahd^ of
the revolution which is the prorogation of the indicators of the month
^rjV {jy^\) 12.4.3
Tiepl xfjc; eXdaecoc; xfjc; xuxtjc; xfjc; eiaeXe^aecdc, xoO ^rivoc;
— L^.^->1 ^Jhi-^J jjt^' J:! 3^" cJ ^^ ^^^ revolution of the months and the pro-
rogation of their indicators
^La ( ) 7.3
^La fj^epa ytvexaL xexeXsLCO^evr) — >UIS^ U^^ ^i^. it becomes one full day
^OLpa ( i;;^ ) 2.2
^OLpac; — \y>- degree
^OLpa ( i^j^ ) 5.0.0
xfjc; ^oLpac; exsLvrjc; yjxlc; dmb xoO ^coSlou exeivou ^exa xoO daxepoc; o^oO sic; xov
xuxXov yLvexaL xoO ^eaou xfjc; fj^epac; — l^.^ tU-^l i^^^' ^1 V^J-^ ^^^ degree
with which it reaches the middle of the sky
^OLpa ( ) 5.0.0
xfjc; ^oLpac; fjxLc; ^exd xoO daxepoc; dvLax^L xal xfjc; ^otpac; fjxLc; ^exd xoO
daxepoc; huei — v^j A^ ^^ ^V^j-^^ [its degree] with which it rises and sets
^OLpa ( '<L^2^ ) 5.2
277
f) ^OLpa ToO [iTiXouq — AjiJI '^^2^ portion of distance
^OLpa ( 'i^j^ ) 5.3
[xsTOi xfjc; ^OLpac; xoO lSlou aOGrj^epLvoO — L^i ^ ^\ ^j-^ /^*^ with the
degree in which it is
^OLpa ( i^j^ ) 5.3
^oLpd eaxLv otl [xeTOL xoO daxepoc; o^oO cpGdvsL sic; x6 ^eaoupdvri^a —
Ifico glo^cJl c-^y^iCJl lg,c.>^^ ^1 0^^ ^"j'^ t'^^ degree of its transit with which the
star reaches midheaven
^OLpa ( <^j^ ) 5.3
xfjc; IStac; ^OLpac; — '^j^ its degree
^OLpa ( i^j^ ) 5.4
xfjc; ^OLpac; exsLvrjc; yjxlc; dvLax^L ^£xd xoO daxepoc;
— 4jj^j c-^y^iCJl ^^JJ^ cJ^J"^ ^^^ degrees of the star's rising and setting
^OLpa ( 'i^j^ ) 5.4.1
xfjc; ^£xd daxepoc; Suvouarjc; ^otpac; — i^^^\ [^jui c-^^Ju ^\ i^j^ the de-
gree with which the star sets
^OLpa ( ^y> ) 6.2.1
xcov ^OLpcov xoO I OLXTQ^axoc; — ^LJI ty*- the degree of the tenth
^OLpa ( ^y> ) 6.4
al ^OLpaL xcov (bpcov xal al ^otpaL xfjc; xuxtjc; — ^JUJI ty>- ol^Lu t\y>-\ the
278
degrees of the hours of the degree of the ascendant
^OLpa ( '<L^2^ ) 8.1.2
^OLpa ToO TiXaxouc; xfjc; aeXrivriq — ^^jS^ 'L^2j> argument of its (the moon's)
latitude
^OLpa ( Lu^ ) 8.3.1
f) ^OLpa ToO TiXaxouc; — c^j^^ 'L/2j:> argument of latitude
^OLpa ( ) 9.1.3
^OLpav ToO ( olxr\\iQLio<^ — ^LJI ^ in the tenth
^OLpa ( ^y> ) 10.1.3
xfjc; ^oLpac; exsLvrjc; £v fj auvep^ovxaL 6 yjXloc; xal f\ ozkr\\r\ f\ xqliql a6vohov y]
xaxa Std^expov — JL2JMI ty>- degree of approach
^OLpa ( ) 10.2.1.5
f) TieaoOaa oSpa olko xfjc; a ^OLpac; dcpaLpsLxaL
— J3^^ u^ Sj^^Jul Jg>j^gM>H oU-Lu LuaiJ we subtract the mentioned hours of
cadence from the first (place)
^OLpa ( i^j^ ) 10.3.1.2
x/jv ^OLpav xoO tiXlou xal xfjc; aeXrivriq fjVLxa yLvcovxat xaxd auvoSov —
pUIj»"MI i^j^ degree of conjunction
^OLpa ( iua^ ) 10.3.2.2
f) ^OLpa xoO TiXdxouc; xfjc; aeXTQvric;. — j^j^^ 'L^^2s> argument of the latitude
279
^OLpa ( ^;^ ) 11.1.1
Elc; xriv xaxdXricJ^Lv xoO aOGrj^epLvoO xoO tiXlou xal xfjc; oz\t^t\<:, slc; sxslvov
xov xatpov oxL f) ^oLpa xoO aOGrj^epLvoO xfjc; ozkr^tf, xaxepx^xaL Suvouaa
— jijiS\ iy> c-^wJl^ Al^ ijd^' f y^ ^^^ ^^^^ position of the two luminaries at
the setting of the degree of the moon
^OLpa ( ^y> ) 11.1.3
xfjc; ^OLpac; xoO tiXlou — j^usJJl iy> degree of the sun
^OLpa ( ^jAJi) 11.1.4
dcTio ^OLpcov xal Xstixcov — ^^UjJIj rj^^ ^ i^ degrees and minutes
^OLpa ( ^y> ) 11.1.4
Ilepl xfjc; ^oLpac; exeLvrjc; yjxlc; xaxepx^xaL ^exa xfjc; aeXTQvric;
— j^\ "LfUi i^^wJu (^a)I tji-l the degree with which the moon sets
^OLpa ( ^y> ) 11.1.7
x/jv saxaTTiv dvdpaaLV xfjc; SLa^expou xfjc; ^otpac; xoO tiXlou
— j^usJJl ty>- j\^aj ^^j\ <j}^ limit of the altitude of the opposite point of the
degree of the sun
^OLpa ( i^j^ ) 11.1.8
f) eaxoLTy] dvdpaaLc; xfjc; ^otpac; xfjc; aeXTQvric; — '^j^ t^J^ '^-^ limit of the
altitude of the degree
^OLpa ( i^jjJi ) 11.5
280
exsLVT) f) ^oLpa f) e^ep^o^evr) ^exa xoO daxepoc; xrjpeLxaL y] exsLvr) f) ^otpa f)
[xsTOi xoO daxepoc; Suvouaa — <^j*i. 3^ c-^^jiCJl ^u^ ^iiaj ^\ i^jjJl the degree
with which rises the planet or sets
^OLpa ( ) 12.0.0
xoO xoTiou xcov ^OLpcov — id-^l ^\yi locatioHS of the divisions
^OLpa ( ) 12.0.0
xfjc; XLVTQGSCOc; xcov ^OLpcov — UjwJj ol^^Jl miz/ia^ and their prorogations
^OLpa ( ikiJi) 12.1.1
fivLxa cp6dv£L 6 yjXloc; eiq x/jv ^otpav exeivriv —
'<ijp^yii\ iialJl j^usJJl JjjP Al^ at the alighting of the sun at the determined point
^OLpa ( ) 12.2.4
6 xoTioc; xfjc; xu^iQ^ '^^^ ^otpac; — /T^^' ^Ua^ rising time of the hayldj
[lolpoi ( i^j^ ) 12.3
^La ^OLpa xoO xotiou xfjc; xuxtjc; — ^iJUa^ '^j^ degree of rising time
^OLpa ( ) 12.3
xoO xoTiou xfjc; ^OLpac; exsLvrjc; — i<j-^l »^yi location of the division
^OLpa ( ) 12.3.1
xoO xoTiou xfjc; xuxTjc; xfjc; ^oLpac; exsLvrjc; — jL^a^l <JI ^ju-^1 ^JUa^ the
resulting rising time of the motion towards it
281
^OLpa ( i^j^ ) 12.3.1
f) iiepiaaeioL f) [xeay] xoO totiou xfjc; tuxtq^ "^"H^ [xoipoLc, exeivou
— /T^^' ^J-^ ^^Ua^ Oju iLiai the excess (of what is) between the rising times
of the degree of the hayldj
[lolpoi ( M^y^ ) 12.3.2
f) ^OLpa ToO [xepoxjc, xoO alXax^ — i<s-^l ^ya location of the division
^OLpa ( ^y^ ) 12.3.2
f) ^OLpa £Lc; y]v XLVSLxaL TO alXax^ — i<s-^l ^tJ?j^ location of the division
^OLpa ( ) 12.3.2
ToO ^epLG^oO xfjc; ^otpac; xoO alXdx^ — /T^^' 0^ io-^l the division from
the hayldj
[lolpOi ( i^j^ ) 12.4.2
f) ^oLpa xfjc; xuxTjc; xfjc; elaeXeuaecdq — iL^I Jd3^" ^UaJl <^j^ degree of
the ascendant of the revolution of the year
[lOMOil ( JjLo ) 1.5.1
xcov ^ovcov xfjc; aeXrivriq — ^^1 Jj^ mansions of the moon
vsoq ( ) 1.1
aeXTQvric; veac; cpaveLarjc; — J>UI <jjj sighting of the crescent
V£0^ ( ) 11.0.0
oxL f) aeXTQvr) tioxs tva cpavfj vea — il^MI <j jj the sighting of the crescents
282
V£0^ ( ) 11.6
xfjc; aeXTJvrjc; veaq (pav£iaT)(; — Ha^] 'L^j sighting of the crescents
V£U£L ( ii^U ) 6.4
veusL — iijU incUning
NlVSUt {yJJ ) 1.5.3
Niveu'i — yjJ Nineveh
VOTLOC; ( <-)y^ ) 3.2
jip6(; TO voTLOv — VJ^ south
VOTLOC; ( ^,y^ ) 8.3.2
VOTLOV — Siiy^ southern
vu5 ( cLL ) 1.1
fj^iepa xai vu^ — -CLL >^\ day with its night
VU5 ( JJllI) 10.2.2.3
dTio TTJc; vuxTOQ SGTLV — J^' J^' j-« '*j^j its time is in the next night
VU5 ( ) 11.6.1
sic; TT)v dpxT)v xfjc; vuxtoq — j-^oJJl <-r*i*-« -^^ at the setting of the sun
vu5 ( <iJ ) 12.2.2
TO f][jiiau To^ov Tfjc; vuxtoq — iJJ jj-^^ i-^waj half the arc of night
283
oIxTTj^a ( ) 6.3
ToO I OLXTQ^axoc; — JUJI ascendant
oIxTTj^a ( o^^i ) 6.4
Tcov lP OLXTQ^axcov — O^^l houses
oIxTTj^a ( ) 9.1.2
[xsTOi'E.b xfjc; TUXTjc; xal xoO l' olxTQ^axoc; — ^LJI tenth
olxri[ioL ( ) 10.3.2.1
TO I oIxTj^a — ^LJI the tenth
olxrj^a ( ) 12.2.1
6 daxrip ^eaov xoO i xal xoO a olxiQ^axoc; xoO xotiou xfjc; Tuyjiq
— ^JliaJlj ji>[jti\ J\j U^ jlS^ jl i^^$^\ if the star is in what is between the
tenth and the ascendant
olxrj^a ( ) 12.2.1
xoO xoTiou xfjc; xu^TQ^ '^^^ ^' olxiQ^axoc; — ^>il^l ^LJI ^JUa^ rising time of
the tenth in right ascension
oIxTTj^a ( <ZJj ) 12.4.2
xa OLXTQ^axa xauxTjc; — ^"3^ its houses
OLXOU^SVTT) ( Ojj^i ) 12.1.3
xfjc; xu^iQ^ "^oO ^eaou xfjc; oLXou^evrjc; — Sjju^jcll \z^^ ^^3 ^' ^^ ^^~
284
cendant of the cupola and the ascendant of the middle of the inhabited world
oXo^ ( JS") 10.3.2.2
oXoc; exXei(\^ei xal xatpov Ixavov axaGiQaeTaL ev xfj exXslcJ^sl. —
JU5Co ^ ^ l3j-uJCJI the eclipse is total with duration
OKOC, ( JS") 10.3.2.3
6 yjXloc; oXoc; exXslcJ^sl — ^JS""^ i^j-^JCJI the eclipse is total
oKoc, ( ) 12.1
Tiepl xfjc; SLaeXeuaecoc; xcov xpovcov oXcov xal xcov j^6\<sy^ xcov yevsGXLaXoyLXCov
— jjljllj JLJI ^^^ Jd^^" cJ ^^ ^'^^ revolution of the years of the world and
of nativities
oKoc, ( ) 12.1.1
Tiepl xfjc; expoXfjc; xcov (bpcov xfjc; elaeXeijaecoc; xcov j^6\<sy^ oXcdv —
JLJI ^^^u^ Jd^^" olSjl T-^pJ^I ^ on the extraction of the times of the revolution
of the years of the world
6Xo<^ ( ^ ) 12.4.2
xoO cpcoxoc; xcov daxepcov oXcov — SJu^^^l ol^L-JJlj c-^^iCll ^^^^woj^ with
all the planets and the aspects of a revolution
OKiaGsv ( Jl^i J^ ) 5.3
OKioQev xoO KapxLvou y] xoO Alyoxepoxoc; — cJl^^' cJ^ c-;H^^l AWg> j^
from the solstitial point in the direction of the following signs
285
6p66v ( LcJiiuoo ) 11.5.2
si he xiveiTOLi 6 daxrip e'E, 6p6o0 — U^^ZLo^ jlT lil if (the planet) has direct
motion
opGoOxaL ( Uap ) 8.1.1
opGoOxaL — Ua^ we equate
opGoOxaL ( Uap ) 11.5.1
xal ^exa xoO (J;7]cpou xcov p ^coSlcov opGoOxat
— J\f>j)i\ ^^ U J^Jaij oUa^ we equate it with the excess of what is between
two zodiacal signs
opGcoGLc; ( JuA*: ) 2.1
xfjc; opGciaecoc; xoO ^eaou (J;7]cpou xcov p xavovLCOv — ^^^^ia^l (jju U JuAjJ
equation of what is between 2 columns
opGcoGLc; ( JuA*: ) 3.1
xfjc; dpQ(i>aecdq xfjc; fj^epac; — ^j^ Jd-^' equation of its day
opGcoGLc; ( JuA*: ) 4.0.0
xfjc; opGciaecoc; xfjc; fj^epac; — jV^' Jd-^' equation of day
opGcoGLc; ( JuA*: ) 4.2
x/jv opGcoGLV x/jv xexeXsLCO^evriv xfjc; fj^epac; — ^j^' jV^' Jd-^' equation of
the entire day
opGcoGLc; ( Ja^ ) 5.2
286
xfjc; opGciaecoc; xoO xuxXou — j[^\ Jajco the equalizer of the day
opGcoGLc; ( Ja^ ) 5.4
xfjc; opGciaecoc; xoO xuxXou xfjc; fj^epac; — jV^' Jajco equalizer of the day
OpGcOGLC; ( <jj^' ) 6.0.0
xfjc; opGciaecoc; xcov lP OLXTj^dxcov — O^^l hy^ equalization of the houses
OpGcOGLC; ( <jj^' ) 6.4
xfjc; opGciaecoc; — ^ij-^' equalization
opGcoGLc; ( JuA*: ) 6.4
opGcoGLc; TipcixT) — Jj^' J:!-^' fi^^t equation
opGcoGLc; ( JuA*: ) 6.4
opGcoGLc; Seuxepa — ^li)l Ju AjJ)I second equation
opGcoGLc; ( JuA*: ) 6.5
opGcoGLc; xoO arj^SLOu — C/o-^l Jd-^' equation of the azimuth
opGcoGLc; ( JuA*: ) 6.5.1
'H opGcoGLc; xoO arj^SLOu — C/o-^l Jd-^' equation of the azimuth
opGcoGLc; ( Ja^ ) 7.0.0
xfjc; opGciaecoc; xcov p ^rixcov — O^j-S^l Oj^ L« J^*^ Jaico equated by the
difference of what is between the two longitudes
287
opGcoGLc; ( ^^^^^^^ ) 7.1.1
xfjc; opGciaecoc; xoO OcJ^ci^axoc; — ^^^\ oU-jl ?^^p^-u2j correction of the
apogees of the planets
opGcoGLc; ( JuA*: ) 7.2
xfjc; opGciaecoc; xcov ^eacov xlvtqgscov xcov daxepcov — ^J:^"^ Ja^jMI ?^^^p^-u2J
the correction and rectification of the mean
opGcoGLc; ( ^jJiJ ) 7.2
xfjc; opGciaecoc; xfjc; fj^epac; ytvexaL xeXeta — V^W^ j^L^^I Jd-^ <3:^" cor-
rection with the equation of the days with their nights
opGcoGLc; ( ^jJiJ ) 7.2
x/jv opGcoGLV xfjc; ^earjc; xlvtqgscoc; xfjc; tioXscoc; exsLvrjc;
— ^J^\ Ja^jl (3:^^ the correction of the mean of our city
opGcoaL^ ( JuJuJ ) 8.1.1
xfjc; opGciaecoc; xoO tiXlou — j^usJJl J^i^jJ equation of the sun
opGcoaL^ ( JuA*:Ji) 8.1.1
f) opGcoGLc; dcTio xfjc; ^earjc; xlvtqgscoc; — JajJI JuAjJ)! equated equation
opGcoGLc; ( JuA*: ) 8.1.2
xcov opGciaecov xfjc; aeXTQvric; — ^^1 Jd-^' equation of the moon
opGcoGLc; ( Ja^ ) 8.1.2
o\)y\ izkziQL opGcoGLc; — Jajco jii- not equated
288
opGcoaic; ( JjJu; ) 8.1.4
Twv opGcoaecov twv daxepwv — ^_^^^\ JjAjJ equation of the planets
opGcoaic; ( Jj.*^ ) 8.1.4
o\)y\. TsXeia Xeyexai opGcoaiq — Ja*^ jji- not equated
Op063aL^ ( J::A*X)i) 8.1.4
XT] P' 6p6c5a£L — ij^' Ji"**^' second equation
Op063aL^ ( J::A*X)i) 8.1.4
f) P' opScoan; xeXeta — Ja*!! ^Jlill JjAjJI the second equated equation
OpGcOGLC; ( JjAjJ ) 8.3.1
Tf]<; 6p6c5a£CO(; if\c, azki]\r\c, — ^^1 JjAjJ equation of the moon
opGcoaic; ( JjJu; ) 8.3.2
Tc5v 6p6(oaecov xtov daxepcov — t_^^5CJl JjAjJ equation of the planets
opGcoaic; ( JjJu; ) 8.4.3
xfjc; opGwaswc; xoO axidafiaxoc; — JJaJl JjAjJ equation of the shadow
opGcoaic; ( JjJu; ) 9.2.3
xfjc; opGcoaecoc; xwv [ioipwv xwv ^wSicov — /TJ^' ^W"j-^ Ji-^-^ equation of
the degrees of the zodiacal signs
opGcOGLc; ( JjAjJ ) 9.2.4
289
xfjc; opGciaecoc; xcov p TiXaxcov — ^j^^Jp^m}] J\j U JuAjJ the equation of what
is between the two latitudes
opGcoaL^ ( JuJuJ ) 10.2.2.1
f) opGcoGLc; exdaxou — Ut^AjJ their equation
opGcoaL^ ( JuJuJ ) 10.3.2.3
f) TieaoOaa oSpa ^exa xfjc; opGciaecoc; xauxrjc; — UV-AjJj X^yuJ] ol^Lu hours
of the half duration and their equation
opGcoaL^ ( JuJuJ ) 10.3.2.3
ol SdxxuXoL xal opGcoatc; sxslvcov — UtIAjJj «jL^MI digits and their equa-
tion
OpGcOGLC; ( ^^.^SK^ ) 11.1.2
xfjc; dacpaXoOc; opGciaecoc; xoO xotiou xfjc; aeXTQvric; — yi2i\ ^yo ^^^^skj^ cor-
rection of the place of the moon
opGcoGLc; ( JuA*: / ^^.^sk^ ) 11.1.3
xfjc; dacpaXoOc; opGciaecoc; xoO xotiou xfjc; aeXrivriq [xstol xfjc; opGciaecoc; xfjc;
fj^epac; — lALL j>L>^(l J^i-^^ ^^1 ^«^j^ t^.^^^^ correction of the place of the moon
with the equation of days with their nights
opGcoGLc; ( JuA*: ) 11.3
£X£Lvo opGcoGLc; XsysxaL. — Ju AjJ)I ^y the arcs of the equation
opGcoGLc; ( JuA*: ) 11.6.1
290
xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xoO xatpoO — JU5CII ^y Jd-^' equa-
tion of the arc of duration
opGcoGLc; ( JuA*: ) 11.6.2
Ilepl xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xfjc; xaxapdaecoc; xoO tiXlou —
j^ujJJl Jtf»lia^'l j^^ Jd-^' equation of the arc of declivity of the sun
OpGcOGL^ ( JuJuJ ) 12.1
xeXsLov eyevsTO [xstol xfjc; opGciaecoc; xfjc; fj^epac;
— ^yJLJ^ i*^.^' Jd-^ ^^^ 03^. o' V^ ^^ (^'^^ position of the sun) should be
corrected with the equation of the days with their nights
oupavoc; ( 'C^\jt, ) 1.2
^eytaxov epyov xcov xoO oOpavoO — <jjIa Cj^\ ^ ioJaP <j:>U" great oc-
currence of atmospheric marvels
oupavoc; ( tU^I) 11.4.1
£v xcp oOpavcp — glo^cJl sky
oc]; ( c^' ) 11.4.1
Std xcov OTicov xoO TiTix^oq — iLill ^^^^ two holes of the block
6(\)ic, cf. TiXsov xal sXaxxov xfjc; ocj^scoc;
o(];l^ ( ii^Ji ) 11.3
xd xavovLa xfjc; Gecoptac; xfjc; aeXTQvric; duo xfjc; ocj^ecoc; — h3j^ ^^J^s>^ JjAc*-
table of the limits of vision
291
o(];l^ ( kiJ^) 11-3.1
TO^ov eaxl xfjc; xeXsLac; ocj^ecoc; — ^^^JSCJl <:i3^' lT^^ ^^^ of complete sighting
o(];l^ ( i^JJi ) 11.3.2
Tcp TO^cp xfjc; TsXsLac; ocj^ecoc; — ^^^JSCJl <:ij^l ^y arc of complete sighting
Tiapa^ovrj ( ) 1.2
Tiapa^ovTQ — ^ j-J' ^rp' month of shift
TiapsXGovTSc; ( oJl ) 12.4.1
ol TSTsXeLCO^evoL xpovoL ToO tiXlou ol TiapeXGovTSc; duo xoO yevsGXLaXoyLXoO
— :>yjll ^^ oJI (jJl ^bl C^^' the complete years which have passed for the
native
7iapf]X6oV ( ^^via^ ) 6.0.0
TiapfjXGov — ^j''^^ pass by
Tia^ ( JT) 10.2.2.1
f) aeXTQvr) Tiaaa exXsLTiSL dXX' oO^ taxaxaL sic; x/jv £xX£L(J;lv
— cU5Co 4J 035C S^ ^ (-ig,c.c^ all of it is eclipsed and it has no duration
TiaaLxd ( ik^ ) 1.2
TiaaLxd — ^^^i-^ ordinary
TiaaLxd ( ik^i ) 7.3.2
TiaaLxd — iia^^-^l iL^I ordinary year
292
Tidaxa ( j^\ ) 1.5
ToO Tidaxa exdaxou IGvouq — jo-«Sll -Uf-I festivals of the nations
Tidaxa (^ ) 1.5.3
Tidaxa — ^^iaj breaking of a fast
KSKT63XSV ( ^\j ) 6.4
jiETiTCOxev — iJulj falling
Kspiaasta ( Jja*; ) 2.0.0
Tf]C, TiepLaaeia(; — ^v^^ia^l {j\j U Jj A*j" the equation of what is between
two columns
HZplOOZioi ( Ju^lidl ) 2.1
f) Tiepiaaeia — J^LalJl difference
HZplOOZioi ( iLa5 ) 4.2
Tispiaaeia xfjc; rjfjiepac; — jV^' ^^J'-^ remainder of the day
KSpiOOeiOi ( OyljJl J^wa5 ) 6.1
jiepiaaeia Tf]<; Tiepicpopdt; — 5y IjJl Jui»9 excess of the circle
KSpiOOeiOi ( J.Ja5 ) 6.1.1
jiepiaaeta Tf]<; aaYtTaa(; — oyljJl J-i»s ^^^ versine of the excess of the circle
KSpiOOeiOi ( J.Ja5 ) 7.2
293
iiepiaaeioL — J^Jas excess
TispLaasta ( Juia^ ) 7.2
xfjc; Kepiaaeioiq xcov p ^rixcov — C^j-S^l C^ L« J^^ difference of what is
between the two longitudes
TispLaasta { 0\j U ) 7.2
f) TiepLaasLa f) ^ear) xcov p xfjc; tioXscoc; fjc; pouXo^sGa xal xoO ^tqxouc; xcov 9
— ij\jL^^ b jJb Jj-U (jiu Lo what is between the longitude of our city and 90
TispLaasta ( Ju^lidi ) 8.1.1
Kepiaaeioi — JlJ^Ui)! excess
TispLaasta ( Ju^liJ ) 9.2
£Lc; x/jv TiepLaasLav xfjc; fi\iiaeioiq oSpac; — ipLu cJLuaj JlJ^Uj ^^^ in accor-
dance with a difference of half an hour
TispLaasta ( J^ ) 9.2.4
x/jv TiepLaasLav xcov p TiXaxcov — ijjui?^! Oju U JuJai excess of what is be-
tween the two latitudes
TispLaasta ( ^^jJ^\) 11.2.1
f) TiepLaasLa exdaxou — :>jjJ"l limits
TispLaasta ( iLiiiJi ) 11.3.1
TiepLaasLa — iLiaiJi excess
294
TispLaasta ( ju«Ji ) 11.5.1
exsLVT) f) iiepiaaeioL eav tiXslcov toO cpavevxoc; xo^ou
— ^Ij^' 1^3^ 0^ ^^ "^' O^ the distance is greater than the arc of vision
TispLaasta ( ju«Ji ) 11.5.1
f) [xeari xoO aOGrj^epLvoO xoO tiXlou xal xoO daxepoc; TiepLaasLa
— AjtJl j^ c-^y^iCJlj j^usJJl c^' u)j ^ whatever distance is between the true
position of the sun and the planet
TispLaasta ( iLiiiJi ) 12.1.2
f) Kepiaaeioi exsLvr) [xstol xfjc; opGciaecoc; xoO OcJ^ci^axoc; neXeioi ytvexaL —
T-j'^L iJAjJl 'i\<ha\\ excess equated by the apogee
TispLaasta ( <L;a5 ) 12.1.2
xfjc; iiepiaaeioLc, xcov xpovcov — C^^l ^^J^^ excess of the years
TispLaasta ( iLiiiJi ) 12.3.1
f) Kepiaaeioi f) ^ear) xoO xotiou xfjc; Tuyjiq xfjc; ^otpac; exsLvou
— /T^^' ^J-^ ^^Ua^ Oju iLia3 the excess (of what is) between the rising times
of the degree of the hayldj
TispLaasusxaL ( ) 1.4.1
£v iiepiaae^eTOLi — As>lj [j^j we add one
TispLaasusxaL ( ) 4.2.1
£Lc; xa ^ TiepLaaeuexaL — ij\l^ ^ \j^j we add (it) to 60
295
TispLaasusxaL ( ) 12.4.1
TO arj^SLov xoO ^coSlou xfjc; xuxiQ^ ^o\j Qe\ieXio\j xoO yeveBXiaXoyixoxj TiepL-
oaeueTOii eiq xouc; xpovouc; exeivouq
— ^JLUJI 'Sjy^ jl «^^i^j5CJl 'ti (^a)I /^^I Sjj-i^ ^J^ l3:>j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
TlZpiGGOC, ( Ju\j ) 2.1
TiepLGGOc; — Ju\j increasing
TispLcpspsta ( Ja^) 6.6
x/jv TiepLcpepsLav — Jac^ circumference
TlSpLCpSpSta ( iiJb^ ) 10.3.2.2
x6 [isaov xoO tiXlou exXslcJ^sl f) Se TiepLcpepsLa oOx exXei(\^ei
— jy iiW j^usJJl >y>- ^ jAJii\ ^y> around the moon from the body of the
sun is a ring of light
TlSpLCpOpd ( jjAJi ) 1.2
TiepLcpopd — jjjJl cycle
TlSpLCpOpd ( ijjjJi ) 1.4.1
TiepLcpopaL — IjjjJl cycle
TispLcpopd ( SyijJi ) 5.5
TiepLcpopd eaxLv olko xfjc; ocpx'^^ '^^^ fj^epac; exsLvrjc; oxav avia'/^ei 6 daxiQp —
j^ujJJl ^^ jjJ jA dliiJl j^ SyljJl the arc on the zodiacal circle since sunrise
296
TispLcpopd ( SyijJi ) 5.5
TiepLcpopd eaxLv dmb xfjc; ocpx'^^ "^"H^ vuxxoc; ^^XP^ "^"^^ oSpac; xa6' y]v dvLax^L 6
daxTQp — L-^^jiCJl ^^ii^ Jl V^^*^ ^"^ 0^ ^Ia)I the arc since the setting of it (the
sun) till the rising of the star
TlSpLCpOpd ( SyijJi ) 6.1
xfjc; TiepLcpopac; xoO tiXlou oxav dvLaxT)
— j^usJJl ^^i^ jaJ ^ dliiJl ^ SyljJl arc on the zodiacal circle since sunrise
TlSpLCpOpd ( SyijJi ) 6.1
Tiepcpopd — dliiJl ^ SyljJl arc on the (zodiacal) circle
TispLcpopd ( JijJi ) 6.3
xfjc; TiepLcpopdc; xcov (bpcov — ol^LJlj y\ji\ arc and hours
TlSpLCpopd ( jij^Mi ) 12.1.2
f) TiepLcpopd dcpatpsLxaL £^ exeivou — jlj:>MI L^ L>.^ we cast off from it
cycles
TiSpLcpopd ( JijJi) 12.1.3
el XL eOpsGfj TiepLcpopd sgxlv — y\ji\ ll^j we call it an arc
TiSpLcpopd (jjAJi ) 12.4.2
xfjc; Gcpatpac; TiXrjpcoGeLaric; xfjc; jiepLcpopdc; — jj jJl ^" the cycle is completed
Tifix^q ( iJJi) 11.4.1
297
Sia Twv oTiwv ToO Tirixzoq — ilJJl ,j>ii" two holes of the block
KfJXU^ ( iJJl) 11.4.1
ToO TiTQXs^oc; — ilJl)! block
7iXavcL)^£VOc; ( oj\^\ ) 11.5
Tiepl Tcov e TiXavco^evcov daxepcov otl xaxa tiolov xatpov s^ep^ovxaL yjtol
OTie^LGTavxaL xoO cpcoxoc; xoO tiXlou xal xaxa Tiotav oSpav slaepxovxaL Otio cpcoc; xoO
tiXlou xaxa x6 Tipcot y] x/jv saTiepav — [^^j^^u^ SjJlp^iII ^.^^iCJl ^,j^ ^ on the
rising of the moveable stars (planets) and their setting
TiXdxoc; ( ^j. ) 3.2
xoO TiXdxoc; exdaxric; tioXscoc; — aJJI ^^ the latitude of the city
TiXdxoc; ( ^j. ) 3.3
xcp xexeXsLCO^evcp TiXdxsL — jJlJl j^j^ j*Lr complement of the latitude of
the city
TiXdxoc; ( 'U^ ) 4.1
xoO TiXdxouc; xfjc; dvaxoXfjc; — (3y^l i«-^ rising amplitude
TiXdxoc; ( ^^ ) 4.1
xoO xeXsLou TiXdxouc; xfjc; tioXscoc; — Aj«JI ^^ j»Lr complement of the lati-
tude of the city
TiXdxoc; ( ^j^ ) 5.2
TiXdxoc; — c^j^ latitude
298
TiXdxoc; ( ^j. ) 6.7
TO TSTsXeLCO^evov xfjc; tioXscoc; xfjc; ^riTou^evric; TiXdxoc; — aL ^j- j»Lc com-
plement of the latitude of the city
TiXdxoc; ( ^j. ) 7.4
TO TiXdxoc; xfjc; ozkr^tf, — ^^1 ^j^ latitude of the moon
TiXdxoc; ( ^j. ) 7.4
xd TiXdxT) xcov daxepcov — SjJlp^iII ^J- latitude of the planets
TiXdxoc; ( ^j. ) 8.3
xoO TiXdxouc; xcov daxepcov — ^.^^iCJl ^J^ latitude of the planets
TiXdxoc; ( ^j. ) 8.3.1
xoO TiXdxouc; xfjc; ozkr^tf, — jaj^\ ^J- latitude of the moon
TiXdxo^ ( jJi ) 8.3.3
xal xpaxsLxaL x6 TiXdxoc; — jJkl declination
TiXdxo^ ( jJi ) 8.3.3
STiSLxa x6 TiXdxoc; xoOxo xrjpeLxaL sic; xd yevLxd XsTixd
— jJkl declination
TiXdxoc; ( ikj-ucu ) 8.3.3
elxa xouxou x6 TiXdxoc; sic; xd yevLxd XsTixd xouxou xpaxsLxat
— l3|^ ^\ «^^ ^\s)^ ^ 'iSg>yjjSA ^,j^ we multiply the extension by the min-
299
utes of proportion of the inclination
TiXdxoc; ( ^j^ ) 8.3.3
£L hz QfXko \iz\ TiXdxoc; £Lc; voTLOv — ^J^ latitude
TiXdxoc; ( 4^^ ) 8.3.4
TO TsXsLov TiXdxoc; — (J^^ 'Ui?^ its second latitude
TiXdxo^ ( Lii^'Mi) 8.3.4
TO y' TiXdxoc; — l3I^MI inclination
TiXdxo^ ( Lii^'Mi) 8.3.4
toOto TiXdxoc; o\^y\ tsXslov — Jajco jji- l3|^ Ml unequated inclination
TiXdxoc; ( ^^ ) 8.3.4
xal eOpLGxexaL to TiXdxoc; to tsXslov — JUii^l 'Ui?^ its third latitude
TiXdxoc; ( 4^^ ) 8.3.4
edv (boL xal Td p arj^SLa e^Laou^eva to TiXdToc; popsLov
— ^J^'' ^^^^ JU)li)l 'Ui?^ Jl.^U"U The result is the third latitude. Its (the
latitude's ) direction is northerly.
TiXdxoc; ( ^j. ) 8.3.4
Td y TiXdTT) — <^l^l (j^^ three latitudes
TlXdxo^ ( ^^i) 9.1.5; 9.2.1
TO ^fjxoc; xal TiXdTOc; — (j^^' latitude
300
TiXdxoc; ( ^j. ) 9.2.4
Tcp TiXaxsL xfjc; tioXscoc; fjc; pouXo^sGa — b aL ^^ latitude of our city
TiXdxoc; ( ^j. ) 9.3.1
£X£Lvo TiXdxoc; xfjc; ocj^ecoc; xfjc; aeXTQvric; XeyexaL y] xal TiXdxoc; axepeov —
^y\ <j^jS^ jl CpcII j(^\ ^j- the precise latitude of the moon or its visible lati-
tude
TiXdxo^ ( ^J. ) 10.2.1.1
x6 TiXdxoc; xfjc; ozkr^tf, — \j^j^ its (the moon's) latitude
TiXdxo^ ( ^J. ) 10.2.1.3
x6 TiXdxoc; xfjc; ozkr^tf, — jaj^\ ^jS- latitude of the moon
TiXdxo^ ( ^j. ) 10.3.2
x6 TiXdxoc; xfjc; ozkr^tf, — j^\ j^j^ latitude of the moon
TiXdxo^ ( jk>j^\ ) 10.3.2.2
x6 axepeov TiXdxoc; xfjc; azkr\\r\c^ — CpJI ^j^^ the exact latitude
TiXdxo^ ( ^j. ) 10.3.2.2
TiXdxoc; eaxl xfjc; azkr\\r\c^ axepeov — CpJI 'Ui?^ jl l^^' ^^I (J^^ t'^^
visible latitude of the moon or its exact latitude
TiXdxo^ ( jk>js. ) 10.3.2.3
xoO axepeoO TiXdxouc; — ^^^ y^^ J^j^ visible latitude of the moon
301
TiXdxoc; ( ^j. ) 11.1.4
TO GTspeov TiXdxoc; xfjc; oz\t^t\<:, — CSj^^ J^"^ J^j^ ^^^ visible latitude of
the moon
TiXdxoc; ( ^j^ ) 11.1.4
TiXdxoc; dacpaXec; — ^jn ^J- visible latitude
TiXdxoc; ( ^j. ) 11.1.4
edv f) TpoL-zrikoiloi TiXdxoc; oOx exTl — J^j^ '^ 0^. i o' j^^ if the moon
does not have a latitude
TiXdxoc; ( ji^jS^ ) 11.1.5
x6 axepeov TiXdxoc; xfjc; aeXTQvric; ytvexaL xexpdycovov — C$^^ j^^ J^j^ ^.j^
the square of the visible latitude of the moon
TiXdxoc; ( ^^ ) 11.1.8
x6 TiXdxoc; xfjc; aeXrivriq — ^^1 j^j^ latitude of the moon
TiXdxoc; ( ^^ ) 12.1.2
£Lc; x6 xavovLov xoO xotiou xfjc; xu^iQ^ ^'^^ "^^ TiXdxoc; xfjc; tioXscoc; exsLvrjc; ev fj
yLvexaL xrjVLxaOxa f) ^TQxriaLc; xoO yevsGXLaXoyLXoO
— ^MJ»1 (J^^ r^^^ ^Ua^ Jj-^ (^ i^ the table of rising times of the zodiacal
signs for the latitude of the nativity
TiXdxo^ ( ^^ ) 12.2.2
TiXdxoc; eaxl xoO xuxXou xfjc; xlvtqgscoc; — ^Jhi-^' v'-^ J^J^ latitude of the
302
circle of prorogation
TiXdxo^ ( ^j. ) 12.2.2
TO TiXdxoc; xfjc; tioXscoc; — aJJI ^^ latitude of the city
TiXdxo^ ( ^j. ) 12.2.2
Tiepl ToO TiXaxouc; xfjc; xlvtqgscoc; xoO xuxXou
— c-^^^^L jju-^1 Sy !:> (j^^ o^^jco ^ on the knowledge of the latitude of the
circle of prorogation approximately
TiXdxo^ ( ^j. ) 12.2.3
x6 TiXdxoc; eaxl xoO xpLycivou — JUitJl ^^ latitude of the trine
TiXdxo^ ( ^j. ) 12.2.3
x6 TiXdxoc; xoO daxepoc; — <^^\ ^^ latitude of the planet
TiXdxo^ ( ^j. ) 12.2.3
x6 TiXdxoc; xoO e^aycivou — j^ J^^l ^^ latitude of the sextile
TiXdxo^ ( ^j. ) 12.2.3
x/jv xexeXsLCO^evriv xpaxTjXaLav xoO TiXdxouc; xoO daxepoc;
— <^^\ j^jS- j»Lr c-^w^ sine of the complement of the latitude of the planet
TiXdxo^ ( j}pj. ) 12.2.4
x6 TiXdxoc; xfjc; xlvtqgscoc; xoO xuxXou — ^i^^' v'-^ C^j^ latitude of the
circle of prorogation
303
TlXsov ( J5l) 2.2.2
TiXeov — JS\ greater
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^io L3>l::^i ) 9.0.0
ToO TiXsLovoc; xal eXaxxovoc; duo xfjc; ocj^ecoc; — ^^klo L3>ti"l difference in
vision (parallax)
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ ciM::^! ) 9.1.3
xoO TiXsLovoc; xal eXdxxovoc; xal xfjc; ocj^ecoc; — ^Lll L3>ti"l difference in
vision
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ ciM::^! ) 9.1.4
xoO TiXsLovoc; xal eXdxxovoc; xfjc; ocj^ecoc; — ^jd^' J^^ l3M^1 difference in
vision of the two luminaries
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ L3>l::^i ) 9.1.4
x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; xfjc; aeXTQvric; eaxlv sic; xov xuxXov xfjc;
dvapdaecoc; — pUjjMI Syl:> ^ j(^\ ^^klo L3>ti"l difference in vision of the moon
on the circle of altitude
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ L3>l::^i ) 9.1.4
x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; xoO fiXlou — j^usJJl JaLu ^yc^\ difference
in vision of the sun
TiXsov xal sXaxTOV xfjc; ocj^scoc; {J^^ lJ%^\ ) 9.1.4; 9.1.5
xoO TiXsLovoc; xal eXdxxovoc; xfjc; ocj^ecoc; xfjc; ozkr\\r\<:^ — ^^1 ^^kLo L3>ti"l
difference in vision of the moon
304
TiXsov xal sXaxTOV xfjc; ocj^scoc; {J^^ lJ%^\ ) 9.1.5
TO TiXeov xal eXaxxov xfjc; ocj^ecoc; xfjc; aeXTQvric; xexeXsLCO^evov eaxlv oO xp^^o^
Sloc x/jv £xX£L(J;lv xoO tiXlou — L-^usJJl l3j-uJCJI CaSj JajJI 4i>lli"l its (the moon's)
equated difference at the time of a solar eclipse
TiXsov xal sXaxTOV xfjc; ocj^scoc; {J^^ lJ%^\ ) 9.2.2
x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; — ^^kLo L3>ti"l difference in vision
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ L3>l::^i ) 10.3.2.1
x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; sic; x6 ^fjxoc; — Jj^aJl ^ ^^1 l3M^1 dif-
ference in vision in longitude
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( J^:^ L3>l::^i ) 10.3.2.1
TiXeov xal eXaxxov xfjc; ocj^ecoc; a' — Jj^' L3>ti"MI the first difference (in
vision)
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( Ji^ L3>l:::^i ) 10.3.2.1
xoO TiXsLovoc; xal eXdxxovoc; xfjc; ocj^ecoc; xfjc; ozkr\\r\<:^ sic; x6 ^fjxoc; xal TiXdxoc;
— j^y^\^ Jj-!^1 ^ y^^ ^^kLo L3>ti"l difference in vision of the moon in longitude
and latitude
TiXsov xal sXaxTOV xfjc; ocj^scoc; {Ji^ lJ%^\ ) 10.3.2.1
x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; xoO fiXlou — j^usJJl ^^kLo L3>ti"l difference
in vision of the sun
TiXsov xal sXaxTOV xfjc; ocj^scoc; ( Ji^ L3>l:::^i ) 10.3.2.1
305
TO TiXeov xal eXaxxov xfjc; ocj^ecoc; xoO tiXlou xal xfjc; aeXTQvric; sic; xov xuxXov
xfjc; dvapdaecoc; — pUjjMI 5yl:> ^ ijd^' ^^klo L3>ti"l difference in vision of the
two luminaries on the circle of altitude
TiXsov xal sXaxTOV xfjc; ocj^scoc; {J^:^ lJ'>^\ ) 11.1.4
x6 xavovLov xoO tiXslovoc; xal eXdxxovoc; xoO xotiou xfjc; xu^iQ^ ^'^^ "^^ t' xXt^a
— <^^j^\ L3>ti"l Jj-^ table of difference (in vision) in the west
TiXsovaa^oc; ( SjjJI) 4.2.1
xov TiXeovaa^ov — Sjjj^)! addition
TiXsovaa^oc; ( ojjyi) 8.1.4
TiXeovaa^oc; — '6ju\J\ increasing
TiXrjpcoGsLarjc; ( ^' ) 12.4.2
xfjc; acpatpac; TiXrjpcoGeLaric; xfjc; jiepLcpopac; — jj jJl ^" the cycle is completed
TiXrjpco^a ( >Lr ) 9.1.3
x6 Tikr]pcd\ioL xauxTjc; ycovta eaxl xoO ^tqxouc; — JjiaJl <j jlj l^Lr its comple-
ment is the angle of longitude
TIOLSL ( J^^ ) 8.1.1
PouXo^evcov fj^cov TioLfjaaL aOGrj^epLvov xou tiXlou
— j^usJJl j5^ c-;L^> J^ jl b:>jl lil if we wish to accomplish the calculation
of the center of the sun
TiOLTJaLc; ( ^^-^SK^ ) 9.3
306
Tiepl xfjc; dacpaXoOc; tioltqgscoc; toO totiou xfjc; aeXTQvric; sic; to ^fjxoc; xal TiXdxoc;
— ^^Ij Jj-!^1 ^^ ^^1 ^tJ?j^ ?^;P^-uaj ^ on the correction of the location of the
moon in longitude and latitude
TiOLTJaLc; ( ^^.^SK^ ) 9.3.1
Tiepl xfjc; GTspeac; TioLiQaecoc; xoO totiou xfjc; aeXTQvric; sic; x6 TiXdxoc; —
j^j^^ ^ 'U^j^ ?^^^p^-u2j the correction of its (the moon's) location in latitude
TlOLTTjaLC; ( CjmLup ) 10.3.1
TiOLTjaLc; — CjcL^ (its) making
tioXl^ ( aL ) 12.2.2
x6 TiXdxoc; xfjc; tioXscoc; — aJJI ^^ latitude of the city
TioXuTiXaataa^oc; ( ) 10.2.1.4
d XL xaxaXsLcpGrj 6 TioXuTiXaaLaa^oc; xouxou xpaxsLxaL — ^\^\ j'^£> the root
of the result
TioXuTiXaataa^oc; ( ) 10.2.1.5
xoO xaxaXsLcpGsvxoc; 6 TioXuTiXaaLaa^oc; — ^^^ j'^ the root of the remain-
der
TioXuTiXaataa^oc; ( ) 11.1.5
d XL eOpsGrj 6 TioXuTiXaaLaa^oc; exsLvou ^rixsLxaL
— iicll J J^ the square of the remainder
lioaoq (jIaIo ) 10.2.2.1
307
Tioaov eaxlv OLub xfjc; aeXTQvric; — 4^Ja^ /^^' J^ OjIaIo its measure is in
digits of its surface
Tioao^ (jIaIo) 10.3.2.2
Tioaov £xX£L(J;£L ToO tiXlou — l3j-uJCJI jIaIo measure of the eclipse
Tioaoc; ( OjIaIo ) 10.3.2.2
xal £L yevriTaL noay] [xeXXei ehoLi — OjIaIo its measure (that of an eclipse)
Tioao^ (jIaIo) 10.3.2.3
dcTio ToO tiXlou Tioaov exXslcJ^sl — l3j-uJCJI jIaIo amount of the eclipse
Tipoasuxrj ( ) 6.0.0
TipoaeuxTQ — ^ qibla
Tipoasuxrj ( ) 6.7
f) ^Lapa Kpoaew/j] xcov daepcov — iLiJi l3|^'I inclination of the qibla
TipoaTLGsvxaL ( LiJ^I ) 1.2
KpoaniQevTOii — Lii-I we add
TipoaTiGsTaL ( ^^^) 1.1
[xriv TipoaTLGsxaL — j^4^ intercalate
TipoacoTia {jy^ ) 1.5.1
xa TipoacoTia — j>^ forms
308
Kpo(^r]Tr](; ( ^ ) 1.2
£^cpav£La TipocpiQTOU — ^ ctot^ sending of a prophet
TipcoTOc; ( ) 12.2
— ^}J\ ^\ «JliaJl Jl glo^cJl Ja-u/j j^ from the mid-heaven to the ascendant to
the fourth
IlToXs^aLOC; ( j^^^cdiaJ ) 11.5
Tov IlToXe^aLov — j^^^^wJliaj Ptolemy
TlOp ( ) 1.2
ol XaxpeuovTSc; xcp Tiupt — i^^^^l ^.> Mazdaism
aaytxa ( >l^i ) 2.0.0
xfjc; aayLxac; — j^LpJl arrow (versine)
aaytxa ( ^o^l ) 2.2
aayLxa ^eydXr) — (O-pJ' ^b ^^ f^^ the arrow
aaytxa ( ^o^x. ) 4.2.1
aayLxa xfjc; fj^epac; — jV^' (O-r" arrow of the day
aaytxa ( ^o^x. ) 6.1.1
xfjc; aayLxac; xfjc; fj^epac; — jV^' (O-p' arrow of the day
asXrjvr) (^i) 1.0.0
309
f) aeXr]vr] — yJii\ moon
asXrjvTT) ( ) 1.1
aeXrivriq veaq cpaveLarjc; — J^UI Z^j sighting of the crescent
asXrjvTT) ( <i^i ) 1.2
ol xpovoL xfjc; aeXTQvric; — ^i^r«^' jj-L^I lunar years
asXrjvTT) ( ) 1.2
f) aeXTQvr) au^SL xal ^SLoOxaL — <JLaMI (^^j 5jt5^ multitude of their sight-
ings of the lunar crescents
asXrjvr) ( ) 10.2.1
OTL f) aeXTQvr) ^sXXsl sxXltislv y] ou — 4jLojIj 4jISCoI position and duration (of
a lunar eclipse)
asXrjvr) ( ) 10.2.1.1
'H aeXTQvr) otl exXslcJ^sl y] ou — 4jIsCoI the possibility of it (a lunar eclipse)
asXrjvr) ( ) 10.2.1.2
f) aeXTQvr) ^sXXsl exXslcJ^slv y] oO — l33-^I ^3^J ^yT3 ^^^ preconditions
for the occurrence of an eclipse
asXrjvr) ( ) 10.2.1.3
Tioaov xfjc; aeXrivriq exXslcJ^sl — l3j-^I /^^' digits of the eclipse
asXrjvr) ( ) 10.2.1.3
310
oXtyov xfjc; aeXTQvric; exXsLTiSL — 'Uiaju lJl^^^^ a part of it (the moon) is
eclipsed
asXrjvr) ( ) 10.2.1.3
f) aeXTQvr) Tiaaa exXsLTiSL xal oXiyriv oSpav taxaxaL sic; x/jv exXslcJ^lv —
cU5Co 4J 035C J 4JS^ lJlu^^^ C^r«^0 all of it (the moon) is eclipsed and there is a
duration to it
asXrjvr) (^i) 10.2.1.3
f) aeXTQvr) xeXeta exXsLTiSL xal euQbq STiavaaxpecpexaL
— 4i-u^ ^ JU5Co 035C Mj 4JS^ lJlu^^^ ^^I the entire moon is eclipsed and
there is no duration in its eclipse
asXrjvr) ( ) 11. 0.0
oxL f) aeXTQvr) tioxs Ivol cpavrj vea — il^MI <jjj the sighting of the lunar
crescent
asXrjvTT) (^c^i ) 11.1.1
aOGrj^epLvov xfjc; aeXTQvric; — ^^1 ^«-J?j^ place of the moon
asXrjvTT) ( ) 11.2
Kspi xfjc; aeXTQvric; veac; cpaLvo^evrjc; [xstol auvoSov — ilA^II 'ij^^j JU^I ^ on
the computations for the sighting of the crescent
asXrjvTT) ( ) 11.3
xoO Qe\ieXio\j xfjc; Gecoptac; xfjc; aeXr]vr](; oXou —
ilA^^I 'L^j 'is^^ ^ c> ' j^liJl the complete rule for the knowledge of the sight-
311
ing of the crescent
asXrjvTT) ( ) 11.4
Kspi ToO (J^TQcpou TOUTOU Ivoi SslxQtj f) asXT^vT) Sloc SaxTuXcov
— jL^^j J^iAl ^Jl SjLiiMI ^ on the pointing out of the crescents by fingers
asXrjvTT) ( ) 11.6
xfjc; aeXr]vr](; veac; cpaveLarjc; — iU^^I 'ij^'^j sighting of the crescent
asXrjvr) ( ) 11.6.2
f) aeXr]vr] cpaLvexaL — ^j^ J>U1 the crescents are visible
asXrjvr)^ ( ) 10.3.2.3
ToO lSlou xfjc; aeXTQvric; — L^lil anomaly
arj^SLOV ( oj:- ) 6.0.0
arj^SLOv — C/wT" azimuth
arj^SLOV ( oj:- ) 6.0.0
ToO arj^SLOu exdaxric; dvapdaecoc; — ^^j' JS^ C/^T" azimuth of every alti-
tude
arj^SLOV ( <zj:^ ) 6.0.0
ToO ar]\ieio\j xfjc; Tipoaeuxfjc; — iLiJi cur^ azimuth of the qibla
arj^SLOv ( cuc^ ) 6.5
xcov arj^SLCOv xfjc; dvapdaecoc; — ^^j' J^ *^^^^^^ azimuth of every altitude
312
arj^SLOv ( cuc^i ) 6.5
TO arj^SLOv soti xfjc; ^OLpac; xfjc; dvapdaecoc; — cUo-^l La> portion of the
azimuth
arj^SLOV ( oj:- ) 6.7
TO arj^SLOv xfjc; ^tapac; sOxfjc; aOxcov — iLiJi C/wC*' azimuth of the qibla
arj^SLOv ( cuc^ ) 6.7
TO arj^SLOv xfjc; Qeoanuyouq sO^fjc; — iLiJi c^s^ azimuth of the qibla
arj^SLOV ( io>U ) 8.3.3
TO arj^SLOv — ^>U mark
arj^SLOV ( oj:- ) 11.4
TO arj^SLOv ttjc; dvapdaecoc; — ^^1 Sy !:> ^ Cc*' its (the altitude's) azimuth
on the circle of the horizon
arj^SLOV ( 'Sjy^ ) 12.4.1
TO arj^SLov toO ^coSlou ttjc; Tuyjiq toO Gs^eXlou toO yeveOXioiXoyixou Kspi-
aae^eTOLi sic, touc; xpovouc; exsLvouc;
— «JliaJl Sjj..^ jl c-^y^iCJl <J (^jJl /f^l Sjj..^ ^^^ [j^j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
GXi6lg[10L ( jy i ) 2.0.0; 8.4.2
ToO GXLda^aTOc; — JJaJl shadow (tangent)
313
Sou^Tidx ( JpLi ) 1.5.2
Sou^Tidx — Jtf»LJ; Shubat
axaGrjasTaL ( oXo ) 10.3.2.2
oXoc; £xX£L(J;£L xal xatpov Ixavov axaGiQaeTaL £v xfj exXslcJ^sl. —
JU5Co ^ ^^^ l3j-uJCJI the eclipse is total with duration
onoiOK^ ( oXli) 10.2.1.5
xa XsTixa xfjc; axdaecoc; — JU5CII ^\s^ minutes of duration
onoiOK^ ( oXli ) 10.2.2.1
f) oSpa xfjc; axdaecoc; — JU5CII ol^Lu hours of duration
axaupcoGLc; ( ojJlJI ) 1.5.3
axaupcoGLc; — o^JL^aJl crucifixion
axspso^ ( CJi ) 10.3.2.2
x6 Gxepeov TiXdxoc; xfjc; aeXTQvric; — CpJI ^^1 the exact latitude
axspso^ ( CJi ) 10.3.2.2
TiXdxoc; eoTi xfjc; aeXTQvric; axepeov — CpJI 'Ui?^ jl l^^' ^^I j^j^ ^^^
visible latitude of the moon or its exact latitude
axspso^ ( ^jl\ ) 10.3.2.3
xoO axepeoO TiXdxouc; — ^^^ j^^ J^j^ visible latitude of the moon
314
axspso^ ( ^J,\ ) 11.1.4
TO GTspeov TiXdxoc; xfjc; aeXTQvric; — C$^^ j^^ J^j^ ^^^ visible latitude of
the moon
axspsoc; ( ^J.\ ) 11.1.5
TO GTspeov TiXdxoc; xfjc; azkr\\r\c^ yLvexaL xexpdycovov — l?^' y^^ c^j^ r^.j^
the square of the visible latitude of the moon
axrjpLy^oc; ( >li]i ) 8.2
6 a GxripLy^oc; — Jj^' z*^' first station
axrjpLy^oc; ( iollo ) 8.2
6 P' GxripLy^oc; — ^li)l 'kAjm second station
axrjpLy^oc; ( >llli ) 8.2
xax' evavxLov xoO ^ axripLy^oO — ^li)l >llll second station
axrjpLCsL ( cfj^ ) 8.2
6 daxrip axripL^SL xal ^sXXsl XLvrjGfjvaL xax' 6p66v — ^lil^M ^vlo stationary
for direct motion
axpscpsxaL ( ns>j^ ) 8.2.1
GxpecpexaL — ^J, returns
auvoSsuar) ( f Ui>i ) 1.1
auvoSeuGT] — ^^^»^' conjunction
315
auvoSsucov ( pUi^MI ) lO.l.l
auvoSeucov — pUi^*-"^! conjunction
auvoSoc; ( ^Ui>i ) 1.1
auvoSoc; — ^^^»^' conjunction
auvoSo^ ( f UJ^i) 1.5.2
xfjc; auvoSou xoO tiXlou — ^^^»^' conjunction
auvoSo^ ( p Ui^Mi ) 9.2
oSpa xfjc; auvoSou — pU^MI conjunction
auvoSo^ ( o^fLaJi ) 10.0.0
xfjc; auvoSou xou tiXlou xal xfjc; aeXr]vr](; — ^jd^' o^tL2j1 approach of the
two luminaries
auvoSo^ ( oUUi^^fi) 10.1
xfjc; auvoSou xou fjXLOu xal xfjc; aeXT^vrjc; xal xfjc; Sta^expou xouxcov xal xou
^TQXouc; xfjc; xouxcov ^exapdaecoc;
— C/Y^lj AjcJL o^^Lfil^^^lj oU-Ul>^ll conjunctions and oppositions in dis-
tance and daily velocity
auvoSo^ ( f Ui^^fi) 10.1.1
xaxa auvoSov y] xaxa Std^expov — pUi^^-MI conjunction
auvoSo^ ( pUi^MI ) 10.3.1.2
x/jv ^OLpav xou fjXLOu xal xfjc; aeXT^vrjc; fjVLxa ylvcovxat xaxd auvoSov —
316
pUl5»"MI i^j^ degree of conjunction
auvoSo^ ( f Ui^i ) 10.3.2
al auvoSoL — ^^^»^' conjunction
auvoSo^ ( pUi^MI ) 10.3.2.1
f) oSpa xfjc; auvoSou — pUi^^-MI ol^Lu hours of conjunction
auvoSo^ ( oUUi^^fi ) 12.1.1
eiq xriv SLd^expov xal auvoSov tiXlou xal aeXTQvric; — ol^Ul^^tl ^ in the
case of conjunctions
acpatpa ( Ais ) 8.1.2
xfjc; p ' acpatpac; xfjc; aeXTQvric; — JuLlI dliiJl the inclined sphere
acpatpa ( Ais ) 8.1.2
x/jv a acpatpav — /TJ^' ^^ sphere of the zodiacal signs
acpatpa ( Ais ) 8.1.2
xfjc; acpatpac; xcov i^ ^coSlcov — /TJ^' ^^ sphere of the zodiacal signs
acpatpa ( A]s ) 9.1.1
xfjc; acpatpac; xcov ^coSlcov — /TJ^' ^^ the zodiacal sphere
acpatpa ( jjaJI ) 12.4.2
xfjc; acpatpac; TiXrjpcoGeLaric; xfjc; jiepLcpopac; — jj jJl ^" the cycle is completed
317
axTTj^axLa^oc; ( ) 12.2
ToO TOTiou ToO cpcoTOc; Tcov daxspcov YJTOL ToO Tipoc; dcXXriXa toutcov axTj^axLa^oO
— ol^LiJl f'^r^ casting of rays
axTTj^axLa^oc; ( ) 12.2.3
xavovLov ToSe xcov axTj^axLa^cov xcov daxepcov
— (j^^' c^^^.^^ pUJJI ^^r^ Jj-^ the table of the casting of the rays by the
calculation of latitude
axTTj^axLa^oc; ( ) 12.2.4
xdc; y axxLvopoXtac; xoO daxepoc; fjyouv xouc; xpsLc; c/rwioiTiayiOuq
— jy^^^\ f UJJI sinister rays (aspects)
xaxsia XLVTTjaLc; ( J^ ) 11.1.1
x/jv xax^Locv XLvrjaLV — ipLu 3^^ precedence of an hour
xaxsia XLVTTjaLc; ( J^ ) 11.1.1
£X£Lvo xax^Loc XLvrjaLc; sgxl xfjc; oSpac; exsLvrjc; — ipLu 3^^ precedence of an
hour
TsGsLxaaLV ( oJii3 ) 1.1
TsQeixoLGiv — cJllJ are transferred
TsXsLOc; ( JjuJi ) 2.1
xeXsLoc; — JajJI equated
TsXsLOc; ( Ja^ ) 8.1.2;
318
TsXeioL — Jajco equated
TsXsLOc; ( Ja^ ) 8.1.4
ToO xeXsLou xevxpou — Jaj«II ^^\ equated center
TsXsLOc; ( J^}Xm^ ) 8.1.4
yLvovxaL al p tsXslol — (JjJajco ^^^^ they become equated
TSXSLO^ ( JjuJi ) 8.3.4
TO TiXdxoc; yLvexaL tsXslov — Jaj«II equated
TSXSLOC; ( UUap ) 9.2.1
yLvexaL tsXslov — IaUa^ we equate them (minutes)
TSXSLO^ ( JT) 10.2.2.1
TsXsLa yLvexaL exXslcJ^lc; xfjc; aeXTQvric; xal Tipoc; xatpov sic; xriv exXslcJ^lv taxaxaL
— JU5Co 4jj JS^ l3j-^I the eclipse is total and it has duration
TSXSLO^ ( JS^i ) 10.3.2.2
6 yjXloc; xeXsLov exXslcJ^sl xal oO PpaSuvsL ev xrj exXslcJ^sl
— 4J cU5Co "^j ^^\ l33-uJCJI the eclipse is total and there is no duration to it
TSXSLO^ ( JT) 10.3.2.2
TsXeioL yLvexaL exXslcJ^lc; xoO tiXlou — Ur lJl^JCjj L^U all of it (the sun) is
eclipsed
TSXSLO^ ( ^/^\) 10.3.2.2
319
£X£Lvo TiXdxoc; XeyexaL tsXslov — '^^^j l?^:^' j^^ J^j^ ^^^ corrected
latitude of the moon and its direction
TsXsLOc; ( C;\ij<^ ) 10.3.2.3
xal yLvovxaL ol SdxTuXoL neXeioi xal f) TieaoOaa oSpa xeXsLa — ^jOajco j^-^^
so they become equated
TSXSLO^ ( JaJI) 11.1.3
xal yLvexaL toOto tsXslov — JajJII equated
TSXSLO^ ( iiCJi) 11.3.1
To^ov eoTi xfjc; xeXsLac; ocj^ecoc; — ^^^JSCJl <:i3^' lT^^ ^^^ of complete sighting
TSXSLO^ ( iiCJi ) 11.3.2
Tcp TO^cp xfjc; TsXeioiq ocj^ecoc; — ^^^JSCJl '^^^J^ ^y arc of complete sighting
TSXSLOC; ( Juia^ ) 11.5.2
xriv TsXsLav ^sxapaaLV — i^^^\^ j^usJJl ij^u c^y^I JlJi^ excess (under-
stood as ''superiority") of the daily velocity between the sun and the planet
TSXSLOC; ( iJA^ ) 11.6.1
£X£Lvo To^ov XsysxaL xfjc; 6£CL)pLac;[oOxl] xsXslov — JJajco iiiiall 'ij,^J\ ^y
equated arc of general sighting
TSXSLOC; ( [11^) 12.1
xeXsLov eyevexo ^exd xfjc; opGciaecoc; xfjc; fj^epac;
— lyJLJL; j^L/^l Jd-^ lgg< 03^. o' v^ ^t (t'^^ position of the sun) should be
320
corrected by the equation of days with their nights
TSXSLO^ ( iJJLJi ) 12.1.2
f) Kepiaaeioi exsLvr) [xstol xfjc; opGciaecoc; xoO OcJ^ci^axoc; xeXsLa ytvexaL —
T-jML iJAjcll iLiaiJi excess equated with the apogee
TSXSLO^ ( Jua^i) 12.3.1
6 xoTioc; xfjc; xu^iQ^ ^ xsXsloc; xoO alXax^ — Jlu^pcII /T^^' ^Ua^ the resulting
rising time of the hayldj
TsXsLCoaLc; ( a:^*) 7.0.0
xeXsLCOGLV — ^Uj^ ending
TSXO^ Oi) 1.2
x6 xeXoc; — ^1 the end
TSXO^ Oi) 1.4.2
£Lc; x6 xeXoc; — ^1 ^ at the end
TS^^dxLOV ( j^UjMi ) 1.4.1
xe^^dxLoc — (*^j^' numerals
TS^^dxLOV ( ^ ) 2.2
xe^^dxLoc — LoLJI divisions
TS^^dxLOV ( fi;;^! ) 4.3.1
xd xe^^dxLoc xfjc; ^T) opGfjc; oSpac; xfjc; fj^epac; — ^>«J»' V^J;^' jV^' ol^Lu ti^l
321
parts of the seasonal (and) crooked hours of the day
TS^^dxLOV ( ^y>\ ) 4.3.1
xa TS^^dxLoc xfjc; [xt] opGfjc; oSpac; xfjc; vuxxoc; — JuUl ol^Lu t\y>-\ parts of
the hours of night
TS^^dxLOV ( jj-uJ^) 7.2
xe^^dxLov xfjc; oSpac; — jj-^ fractions
xe^^dxLoc — jj-uJCJI fractions
TSTapTTTj^OpLOV ( ^j ) 6.6
exaaxov oOv xoO xuxXou xexapxTj^opLov — L^ ^j ^\ each quarter of it
TSxapTO^ ( ^i^i) 12.2
OLKO xoO l' xoO Tipcixou ^^XP^ ^^'^ "^^^ xsxdpxou
— ^}J\ ^\ «JliaJl Jl glo^cJl Ja-u/j j^ from the mid-heaven to the ascendant to
the fourth
TSTsXsLCO^svoc; ( >Lr ) 1.0.0
xexeXsLCO^evoc; — >Lr the complement
TSTSXSLCO^SVOC; ( A^Ui ) 1.2
xpaxoOvxaL ol xpovoL xexeXsLCO^evoL xoO exouc; xoO 'laaSaxepSr)
obi ^^>;;:i ^^y*-^ bj^l we take the completed years of Yazdijird
'Ul
322
TSTSXSLCO^SVOC; ( O^yi^ ) 9.2.5
ebpsQev to iikeov xal eXaxxov xfjc; ocj^ecic; eaxLv xexeXsLCO^evov — C^^^
fundamental (elements)
TSTSXSLCO^SVOC; ( A^Ui ) 12.0.0
XpovoL eiai xoO tiXlou xexeXsLCO^evoL — i^-^usJJl ^bl jjl^l complete solar
years
TSTsXsLCO^svoc; ( >Lr ) 12.2.3
x/jv xexeXsLCO^evriv xpaxTjXaLav xoO TiXdxouc; xoO daxepoc;
— c-^y^iCJl j^j^ j»Lr c-^w^ sine of the complement of the latitude of the planet
TSTSXSLCO^SVOC; (a^UI) 12.4.1
ol xexeXsLCO^evoL xpovoL xoO tiXlou ol TiapeXGovxec; duo xoO yevsGXLaXoyLXoO
— ^^^\ ^ c^\ ^\ ^bl OiL^I the complete years which have passed for the
native
TSTpdycovov ( ^^ ) 11.1.5
xoO xexpaycivou xoO ^tqxouc; ^eaov tiXlou xal aeXTQvric; — (jd^' 0?^ ^ /^^
the square of what is between the two luminaries
TSTpdyCOVOV ( ^^ ) 11.1.5
x6 axepeov TiXdxoc; xfjc; aeXTQvric; ytvexaL xexpdycovov — C$^^ j^^ J^j^ r^-j^
the square of the visible latitude of the moon
TSTpdycovov ( ^ji)i ) 12.2.3
f) Std^expoc; exsLvou aOGic; xexpdycovov — ^,J^^ quartile
323
TSTpdycovov ( ^,J0\ ) 12.2.4
TO M^iov Tsxpdywvov — ^.J^^ O^-'^^ dexter quartile
TSTpdycovov ( ^,J0\ ) 12.2.4
TO apiaxepbv TSTpdywvov — ^r*J*^' ^.^^ sinister quartile
TTjpSLTaL ( <-)j^ ) 1.3.4
TT)p£LTai — <-r'j^ multiply
TO^OV ( ^j^\ ) 2.0.0
TOO TO^OU ij^'
arcs
TO^ov ( oL^y ) 3.4
TO TO^ov Tf)(; TpaxT)Xaia(; ex£ivT]<; xpaTEiTai — oL^y we take its arc
TO^OV ( ^y ) 4.2
TO f][jiiau TO^ov Tf]C, f]iJiipac, — jV^' iry L-a.uaJ half of the arc of day
t65ov ( ) 4.3
TETeXsLWfjievov to to^ov Tfjc; f)[i£pa(; — jV^' *^-^ determination of the day
TO^OV ( ^y ) 4.3
ToO To^ou ToO vux6r)[i£pou — JJJl ij^y^ jV^' ij^^ ^"^^ *^f *^^y ^"^"^ ^"^^ *^f
night
TO^OV ( j^-y ) 4.3
324
TO YJ^LGU TO^ov xfjc; fj^spac; — jL^I ^yi cJLuaj half of the arc of day
TO^OV ( ^y ) 4.3
TO TO^ov xfjc; fj^epac; — j{^\ ^yi arc of day
TO^OV ( ^^i) 9.1.1
\T\\ TpaxTjXaLav xoO xo^ou exsLvou yjxlc; eaxlv ^exa^u xoO l' olxiQ^axoc; xal xfjc;
xuxTjc; xoO xatpoO — 'uJl^j ^LJI (jju (jjJl j^^^l the arc which is between the
tenth and its ascendant
TO^OV ( ^y ) 11.1.1
xcp fj^LasL xo^cp xfjc; fj^epac; — j^usJJl iy> jL^ ryyi cJLuaj half of the arc of
day of the degree of the sun
TO^OV ( 4^^ ) 11.1.4
x6 lo^ov xauxTjc; xpaxsLxaL — ^^yhj we take its arc
TO^OV ( ^y ) 11.1.5
x6 e^eXGov lo^ov eaxl xoO cpcoxoc; fjyouv xfjc; eXXd^cJ^ecoc; xfjc; ozkr\\r\<:^
— jj-Jl (^3^ ^^c of light
TO^OV ( j^y ) 11.1.5
xoO xo^ou xoO cpcoxoc; — jyi\ ^yi arc of light
TO^OV ( ^y ) 11.1.6
Ilepl xoO xo^ou £X£Lvou xal xoO xatpoO oxl eaxlv Oiiep yfjv f\ ozkr\\r\ \iz\ql if\\
SUGLV XOO fjXLOU
325
— j^usJJl c-^wJLo Aju j^j^\ 3y JU5Cil ^y arc of duration above the earth af-
ter the setting of the sun
TO^OV ( ^y ) 11.1.7
TO^ov eoTi xfjc; xaxapdaecoc; xfjc; tiXlou — j^usJJl J^^lia^ I ^yi arc of the
declivity of the sun
TO^OV ( ^y ) 11.2
a To^ov ToO xatpoO exepov xcov dxxLvcov dXXo xfjc; dvapdaecoc; xal exepov
TO^ov xfjc; xaxapdaecoc;
— Jtf»lia^''^lj pliJj'^lj ctJCllj jjJl ^y the arc of light; of duration; of altitude
and of declivity
TO^OV ( ^y) 11.2.1
x6 xo^ov xfjc; dvapdaecoc; xoO tiXlou — j^usJJl J^^Liarf I j^3^ ^^^ ^f t'^^ d^"
clivity of the sun
TO^OV ( j^^i ) 11.2.1
x6 TO^ov xfjc; dvapdaecoc; xfjc; aeXTQvric; — ^^1 ^^j' lT^^ ^^^ of the altitude
of the moon
TO^OV ( ^y ) 11.2.1
x6 xo^ov xoO xatpoO — JU5Cil j^^^ arc of duration
TO^OV ( ^y ) 11.3
x6 xo^ov xoO cpcoxoc; — jy^\ ^y arc of light
326
TO^OV ( ^y ) 11.3.1
To^ov saxl xfjc; xeXsiac; o(|»£W(; — '\^^ '^..3J^ Cf^ arc of complete sighting
TO^ov ( j-y ) 11.3.1
ToO TO^ou ToO (pcoT6(; — jyi\ ^ys arc of light
To56v ( ^y ) 11.3.1
TO TiptOTOV TO^OV (^3*^' if 3^^ ^^^ ^^^^ ^^^
TO^OV ( ^y ) 11.3.2
T& TO^Cf) Tf]<; xeXetat; 6'\)Z(x>c, — <JSOI i;3^' (^"3^ ^^^ ^^ complete sighting
TO^OV ( ^y ) 11.5
ToO To^ou xfjc; xaxapdaecoc; xoO rjXiou sic; xov xaipov rjvixa 5uvr] 6 daxT)p f]
dviaxn
the arcs of the declivity of the sun at the time of the setting of the planet or of its
rising which is called the arc of complete sighting
TO^OV ( ) 11.5
TO To^ov eiq xriv Gecoptav xcov daxepcov
— JU5CII ^3^ if=^ rjA iJL^^II '^,^J\ J>jAs> limits of the initial sighting from the
direction of the arc of duration
TO^OV ( ^y ) 11.5
TO TO^ov ToO xatpoO xfjc; xaxapdaecoc; xoO tiXlou — J^^lia^ Ij JU5CII J^^^ the
arc of duration and declivity
327
TO^OV ( J.y ) 11.5.1
exsLVT) f) iiepiaaeioL eav tiXslcov toO cpavevxoc; xo^ou
— '^^^J\ ^y ^ jt5l AjtJl jlSj the distance is greater than the arc of vision
TO^OV ( ^y ) 11.5.1
TO^ov xfjc; Qecdpioiq xoO daxepoc; — h3j^ ify ^-^"j ^^ ^^^^ it the arc of
vision
TO^OV ( ) 11.5.1
'H^SLc; xavovLov eGiQxa^ev xal xa xo^a omep eho\iev xeGsLxa^ev sic; exelvo x6
xavovLov ^£xa xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xdc; dcpx^c; xcov ^coSlcov
— ^^11 ^ ^^^J^^ oU^lia^^Uj /TJ^^ ^!>^^ 0^ '^'^J^ ^jAs> jljil LitJpj
We have set out the values of the limits of sighting in degrees of the zodiacal signs
and for the initial declivities in the fourth clime at the beginnings of the zodiacal
signs
TO^OV ( ^y ) 11.5.2
x6 TO^ov x6 cpavev — h3j^ ify ^^^ ^f vision
TO^OV ( ^y ) 11.6.1
£X£Lvo To^ov XeyexaL xfjc; Gecoptac; ouyl xsXslov — iiiiall '^,^J\ ^y arc of
general sighting
TO^OV ( ^y) 11.6.1
x6 TO^ov xoO cpcoxoc; — jyi\ ^y arc of light
328
TO^OV ( ^^ ) 11.6.1
TO TO^ov ToO xatpoO — JU5CII j^^^ arc of duration
TO^OV ( j^^i ) 11.6.1
xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xoO xatpoO — JU5CII ^yi Ju AjJ equa-
tion of the arc of duration
TO^OV ( ^y ) 11.6.2
xoO xo^ou xfjc; Gecoptac; xoO xeXsLou — iiiiall '<i,'^J\ j^3^ ^^^ ^^ general
sighting
TO^ov ( ^y ) 11.6.2
x6 xo^ov xfjc; Gecoptac; — iiiiall <:ij^l ^y> arc of general sighting
TO^OV ( ^^5 ) 11.6.2
x6 \oE,o\ xoO cpcoxoc; — jy]\ ^yi arc of light
TO^OV ( ^^5 ) 11.6.2
Ilepl xfjc; dacpaXoOc; opGciaecoc; xoO xo^ou xfjc; xaxapdaecoc; xoO tiXlou —
j^ujJJl Jtf»lia^'l j^^ Jd-^' equation of the arc of declivity of the sun
TO^OV ( ^y ) 12.2.2
x6 YJ^LGU lo^ov xfjc; vuxxoc; — iL) ^^ cJLuaj half of the arc of night
TO^OV ( ^y ) 12.2.2
x6 YJ^LGU xo^ov xfjc; fj^epac; — ^_^^\ jl^ j^^ cJLuaj half of the arc of the
329
day of the star
TO^OV ( ^y ) 12.2.3
To^ov eaxl xoO e^aycivou — j^ J^' j^3^ ^^^ ^f t'^^ sextile
TO^OV ( ^35 ) 12.2.4
TO YJ^LGU TO^ov xfjc; fj^spac; xoO daxepoc; — OjL^ j^3^ cJLuaj the half of the
arc of its day
TOTioc; cf. TOTioc; xfjc; tuxttjc; ( ) 4.1
Tcov TOTicov Tcov ^coSlcov £lc; Tidvxa xd xki\iQLiQL — (3^^^ (^ /TJ^' ^Ua^ rising
times of the zodiacal signs in the horizons
TOTioc; cf. TOTioc; xfjc; tuxttjc; ( ^lia^ ) 4.4
TCOV TOTICOV TCOV ^CoSlCOV £Lc; xd TlXdTT) TCOV xXt^dxCOV TldvTCOV
— (3^^^ ik r 3^^ ^LU^ rising times of the zodiacal signs in the horizons
TOTIO^ ( ) 9.1.1;9.1.3
ToO TOTiou Tcov dxpcov — /Tj^' ^^ V^ poles of the sphere of the zodiacal
signs
TOTIOC; ( ^y^ ) 9.2
6 TOTioc; xfjc; aeXTQvric; fjyouv to aOGrj^epLvov — ^^1 ^yn location of the
moon
TOTioc; ( ^y^ ) 9.3
6 TOTioc; eaxl xfjc; ocj^ecoc; xfjc; aeXTQvric; — l^^' ^^I ^yi position of the
330
visible moon
TOTIO^ ( ^y^ ) 10.3.2; 10.3.2.1
6 TOTioc; eoTi xfjc; Gecoptac; xfjc; aeXTQvric; — l^^' C/w<^iJl ^tJ?j^ position of the
visible moon
TOTIOC; ( M^y^ ) 11.1.4
Tcp TOTicp xfjc; aeXTQvric; — ^^1 ^ya place of the moon
TOTioc; ( ^j^ ) 11.4
Tov TOTiov xfjc; aeXTQvric; — yi2i\ ^ya place of the moon
TOTIOC; ( ^ij^ ) 12.0.0
ToO TOTiou Tcov ^OLpcov — i<s-^l ^\yi placcs of the division
TOTIO^ ( ) 12.0.0
ToO TOTiou Tcov daxspcov — ol^L«JJl rj^ casting of the rays
TOTIO^ ( ) 12.2
ToO TOTiou ToO cpcoTOc; Tcov OLGTspcdv Y]TOL ToO Tipoc; ocXXriXa TOUTCOv axTj^axLa^oO
— ol^LiJl rj^ casting of rays
TOTioc; ( M^y^ ) 12.2.3
6 TOTioc; eaxl xoO cpcoxoc; xoO e^aycivou xoO daxepoc; £^ dpLaxepcov
— ^r^.^1 4^.uJ j^ ^tJ?j^ the location of the light of its sinister sextile
TOTIO^ ( ) 12.2.3
331
ToO TOTiou ToO cpcoTOc; Tcov daxspcov — i^^^\ ol^Li rj^ casting of rays
of the planet
TOTioc; cf. TOTIOC; TTJc; TUX^O^ ( ) 12.2.4
6 TOKoq xfjc; SLa^expou xfjc; [xoipoiq xoO aOGrj^epLvoO xoO daxepoc; — ojjJaj ^JUa^
rising time of its opposite point
TOTIO^ ( ) 12.2.4
xoO xoTiou xoO cpcoxoc; xcov daxepcov — pUJJI rj^ casting of the rays
TOTioc; ( ^y^ ) 12.3
xoO xoTiou xfjc; ^OLpac; exsLvrjc; — i<s-^l »^yi location of the division
TOTioc; xfjc; tux^O^ ( /^^ ) 3.0.0
xoO xoTiou xfjc; Tuyjiq — JUa^ rising time
TOTioc; xfjc; tux^O^ ( /^^ ) 3.4
xoO xoTiou xfjc; Tuyjiq xcov ^coSlcov — /TJ^' ^Ua^ rising time of the zodiacal
signs
TOTioc; xfjc; tux^O^ ( ) 4.4
xoO xoTiou xfjc; Tuyjiq xcov ^coSlcov ^exd xfjc; euQeioiq ypa^^fjc; —
^vSl^l dliiJIj 'LJUa^ its rising time in right sphere
TOTioc; xfjc; tux^O^ ( /^^ ) ^-4
xoTioc; xfjc; xu^iQ^ "^^^ ^OLpcov eaxL ^£0' d)v dvLax^L 6 daxiQp
— Ifico ^iiaj ^\ 'Cs>-j^ ^JUa^ the rising time of its degree with which it rises
332
TOTioc; TTJc; TUX^O^ ( /^^ ) 5-5
6 TOTioc; xfjc; tuxtjc; tcov ^otpcov xoO tiXlou sic, to TiXdxoc; xfjc; tioXscoc; —
aJJI ^ j^usJJl ty>- ^JUa^ the rising time of the degree of the sun in the city
TOTioc; xfjc; tux^O^ ( /^^ ) ^-^
ToO TOTiou xfjc; TUXTjc; Tcov ^oLpcov Tcov dvLGXovTCOv ^exd ToO tiXlou —
i^^y^iCJl ^^JJ^ ^j-^ ^Ua^ rising time of the degree of the rising of the star
TOTioc; xfjc; tux^O^ ( /^^ ) ^-^
6 TOTioc; xfjc; tuxtjc; tcov ^otpcov xfjc; SLa^expou xoO tiXlou — Ia^ j^ JUa^
the rising time of the opposite point of its degree
TOTioc; xfjc; tux^O^ ( /^^ ) 6. 2
xcp xoTicp xfjc; xuxTjc; xoO aOGrj^epLvoO xoO tiXlou slc; x6 TiXdxoc; xfjc; tioXscoc; —
aJJI ^ j^usJJl ty»" ^JUa^ rising time of the degree of the sun in the city
TOTioc; xfjc; tux^O^ ( /^^ ) 6. 2
xcp xoTicp xfjc; xu^Tjc; xfjc; SLa^expou xou auGrj^epLvou xou tiXlou slc; x6 TiXdxoc;
xfjc; KoXecdq — aJJI ^ Ia^ j\^ ^JUa^ rising time of the opposite point of its degree
in the city
TOTioc; xfjc; tux^O^ ( /^^ ) 6.2.1
6 xoTioc; xfjc; xu^iQ^ [iSTOL xfjc; euGsLac; ypa^^fjc; — ^vil^l dliiJIj 'uJUa^ its
rising time in the right sphere
TOTioc; xfjc; tux^O^ ( /^^ ) 6. 3
333
6 TOTioc; xfjc; tuxtq^ aOGrj^epLvoO xoO tiXlou [xeTOL xoO dmb xoO TiXdxouc; xfjc;
TioXecoc; — aJJI ^ j^usJJl ty*- ^JUa^ rising time of the degree of the sun in the city
TOTioc; xfjc; tux^O^ ( /^^ ) 6. 3
xoO xoTiou xfjc; Tuyjiq xoO TiXdxouc; xfjc; tioXscoc; — aJJI ^ ^JUJI ty*- JUa^
rising time of the degree of the ascendant in the city
TOTioc; xfjc; tux^O^ ( /^^ ) 6.3
6 xoTioc; xfjc; Tuyjiq xfjc; SLa^expou xoO tiXlou — j^usJJl ty>- j\^ ^JUa^ rising
time of the opposite point of the degree of the sun
TOTioc; xfjc; tux^O^ ( /^^ ) 6. 3
xoO xoTiou xfjc; xu^TQ^ "X-^'^ '^^^ TiXdxouc; xfjc; tioXscoc; — «JUtf» ^JUa^ rising time
of the ascendant
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
6 xoTioc; xfjc; Tuyjiq xal x6 TiXdxoc; xfjc; tioXscoc; — aJlJIj «JUtf» ^JUa^ rising time
of the ascendant in the city
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
xoTioc; xfjc; xu^iQ^ "^^^Ci evSexdxou olxiQ^axoc; — jls^ ^^^^ ^Ua^ rising time
of the eleventh
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
xoTioc; xfjc; Tuyjiq xoO ScoSexdxou olxiQ^axoc; — jLs^ ^li)l ^JUa^ rising time
of the twelfth
334
TOTioc; TTJc; TUX^O^ ( /^^ ) 6.4
6 TOTioc; xfjc; tuxtjc;. — ^JUJI ^JUa^ rising time of the ascendant
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
6 TOTioc; xfjc; Tuyjiq xoO Seuxepou olxiQ^axoc; — ^liJl ^JUa^ rising time of the
second
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
6 xoTioc; xfjc; xuxtjc; xoO xpLxou olxiQ^axoc; — JU)li)l ^Ua^ rising time of the
third
TOTioc; xfjc; tux^O^ ( /^^ ) 6.4
x6 xexapxov oIxTj^a xoO xotiou xfjc; Tuyjiq — ^}J^ ^Ua^ rising time of the
fourth
TOTioc; xfjc; tux^O^ ( /^^ ) H-l-l
xoO xoTiou xfjc; xuxTjc; ^exa eOGsLac; ypa^^fjc; — ^vil^l dliiJl JUa^ rising
time of the right sphere
TOTioc; xfjc; tux^O^ ( /^^ ) 12.1
xoO xoTiou xfjc; Tuyjiq exdaxou — /^b^ ascendants
TOTioc; xfjc; tux^O^ ( /^^ ) 12.1.2
£Lc; x6 xavovLov xoO xotiou xfjc; Tuyjiq eiq x6 TiXdxoc; xfjc; KoXecdq exsLvrjc; ev fj
yLvexaL xrjVLxaOxa f) ^TQxriaLc; xoO yevsGXLaXoyLXoO
— ^MJ»1 (J^^ r^^^ ^Ua^ Jj-^ (^ in the table of rising times of the zodiacal
signs for the latitude of the nativity
335
TOTIOC; TTJC; TUX^O^ ( /^^ ) 12.1.2
Tiepl xfjc; elaeXeuaecoc; xoO totiou xfjc; tuxtjc; — Ju^^^l «JUtf» o^^jco ^ on the
knowledge of the ascendant of the revolution
TOTioc; xfjc; tux^O^ ( /^^ ) 12.1.3
ToO TOTiou xfjc; TUXTjc; [xsTOi xfjc; eOGsLac; ypa^^fjc; fjc; f) apxiQ o^^^ "^"H^ ^PX'H^ "^^^
KpLoO
— J^l Jj' 0-^ ^vSl^l dliiJl JUa^ rising time in the right sphere from the
beginning of Aries
TOTioc; xfjc; tuxttjc; ( Jlia^ ) 12.1.3
d XL eOpsGrj xotioc; xfjc; xuxtjc; sgxlv — JUtf» JUa^ J^^^' the result is the
rising time of the ascendant
TOTioc; xfjc; tuxtt)^ ( ^U^ ) 12.2.1
6 xoTioc; xfjc; xuxtjc; 6 8' — ^>il^l /^.[J^ ^Ua^ rising time of the fourth in
right (ascension)
TOTioc; xfjc; tux^O^ ( /^^ ) 12.2.1
xoO xoTiou xfjc; xuxTjc; xoO 8' — ^vZlJ.1 ^\J\ JUa^ rising time of the fourth
in right (ascension)
TOTioc; xfjc; tux^O^ ( /^^ ) 12.2.1
xoO xoTiou xfjc; xuxTjc; xoO daxepoc; — ^>il^l i^^S^\ ^JUa^ rising time of
the star in right (ascension)
336
TOKOc; TYJc; Tuxrjc; ( Jlia^ ) 12.2.1
6 TOTioc, xfjc; Tuyr()q b i — ^vZlJ.1 jLj>i\ JLL^a rising time of the tenth in
right (ascension)
TOTIOC; TTJC; TUXTQC; ( ^Uaw ) 12.2.1
C 5 V
O OLOTTlp [iSaOV TOU L XaL TOU a OLXTQ^aXOc; XOU TOTIOU TTjc; TUXTjc;
^JliaJlj ^LJI ijiu UJ jIS^ jI c-^y^iCJl if the star is in what is between the
tenth and the ascendant
TOTIOC; TTJc; TUX^O^ ( /^^ ) 12.2.1
ToO TOTiou xfjc; TUXTQ^ "^^^Ci l' OLXTQ^axoc; — ^>il^l ^LJI ^JUa^ rising time of
the tenth in right (ascension)
TOTioc; xfjc; tux^O^ ( /^^ ) 12.2.1
TOTioc; xfjc; tuxtq^ "^^^C; daxepoc; — ^>il^l i^^S^\ ^JUa^ rising time of the
star in right (ascension)
TOTIOC, xfjc; TUX^O^ ( /^^ ) 12.2.2
ToO TOTiou xfjc; TUXTjc; Tcov ^coSlcov — /TJ^' ^Ua^ rising time of the zodiacal
signs
TOTioc; xfjc; tux^O^ ( /^^ ) 12.2.4
6 TOTioc; xfjc; tuxtjc; xfjc; [xoipoLC, — /T^^' ^Ua^ rising time of the hayldj
TOTIOC, xfjc; TUX^O^ ( /^^ ) 12.2.4
Tov TOTiov xfjc; TUXTjc; xfjc; SLa^expou xoO daxepoc; — '^j-^ ^?^ ^Ua^ the
rising time of the opposite point of its degree
337
TOTioc; TTJc; TUX^O^ ( /^^ ) 12.2.4
xfjc; evciaecoc; xcov p toticov xfjc; tuxtjc; — ij^LjJLiall r\jifi\ a mixture of the two
rising times
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3
^La ^OLpa ToO TOTiou xfjc; Tuyjiq — SlJUa^ '^j^ degree of rising time
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3.1
ToO TOTiou xfjc; TUXTjc; xfjc; ^oLpac; exsLvrjc; — jL^a^l <JI ^'ju-^l ^JUa^ the
resulting rising time of the motion towards it
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3.1
6 TOTioc; xfjc; xuxtjc; 6 xsXsloc; xoO alXax^ — jL^a^l /T^^' ^Ua^ the resulting
rising time of the hayldj
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3.1
f) TiepLaasLa f) ^ear) xoO xotiou xfjc; Tuyjiq xfjc; ^OLpac; exeivou
— ry^\ ^j-> i^U^ O^, iJLiiai the excess (of what is) between the two rising
times of the degree of the hayldj
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3.1
6 xoTioc; xfjc; Tuyjiq xfjc; SLa^expou exeivou — j\^\ ^JUa^ rising time of the
opposite point
TOTioc; xfjc; tux^O^ ( /^^ ) 12.3.1
xoO xoTiou xfjc; xu^TQ^ exeivou [xeTOL xfjc; eOGsLac; ypa^^fjc;
338
^viJLall dUliJl ^JLU^ rising time in right sphere
TOTioc; TTJc; TUX^O^ ( /^^ ) 12.3.2
Tov TOTiov xfjc; TUXTjc; TOUTOU ^exa xfjc; eOGsLac; ypa^^fjc; — ^vZLoIl 'LJUa^ its
rising time in right (ascension)
TOTioc; xfjc; tux^O^ ( /^^ ) 12.4.4
6 TOTioc; xfjc; xuxTjc; xfjc; elaeXeuaecdq — iL^I J:! 3^" ^^ ascendant of the
revolution of the year
TpaxTTjXaLa ( ^^\ ) 2.0.0
xfjc; xpaxTjXaLac; — c-;^^! sines
TpaxTTjXaLa ( ^^^\ ) 2.2
f) ^eydXr) xpaxTjXaLa — ^Ja^MI c-^^J-l the greatest sine
TpaxTTjXaLa ( c^v^ ) 2.2.2
f) xexeXsLCO^evT) xoO xo^ou exeivou xpaxTjXaLa — >Lc c.^^^ sine of the com-
plement
TpaxTTjXaLa ( ^..v^ ) 5.3
f) xpaxTjXaLa xoO xexeXsLCO^evou TiXdxouc; — ^.^^^501 ^^ j»Lr c.^^^ sine of
the complement of the latitude of the planet
TpaxTTjXaLa ( c^v^ ) 5.3
£Lc; x/jv xpaxTjXaLav xoO ^tqxouc; xoO daxepoc; duo xfjc; dp^fjc; xoO KapxLvou
y] xfjc; dpxfjc; xoO Alyoxepcoxoc; olov duo xouxcov xcov ^coSlcov eaxlv eyyuxepov xoO
339
daxepoc; — <JI c-?^^ll c-^H^^^l AWg> ^ oAju «^^^^ the sine of its distance from
the point of the solstice closest to it
TpaxTTjXaLa ( c^v^ ) 6.5.1
xriv TpaxTjXaLav \t\\ TSTsXeLCO^evriv xfjc; dvapdaecoc; — pUjjMI >Lr c-^wc>
the sine of the complement of the altitude
TpaxTTjXaLa ( <^^^^ ) 6.5.1
TpaxTjXaLd eaxL xoO arj^SLOu — C/w<s-^l v^ ^^^^ ^f the azimuth
TpaxTTjXaLa ( <^^^^ ) 6.5.2
TpaxTjXaLd eaxL xfjc; dvapdaecoc; exsLvrjc; xfjc; ^r) zyp\^oT\c, arj^SLov. —
4J C/wC*' ^ j^jJl plijj^l *^^^ si^^ of the altitude which has no azimuth
TpaxTTjXaLa ( c^v^ ) 6.7
x/jv xpaxTjXaLav x/jv xexeXsLCO^evriv xoO TiXdxouc; xoO Maxxd
— i5Co ^^ j»Lc c-^w^ sine of the complement of the latitude of Mecca
TpaxTTjXaLa ( <^^^^ ) 6.7
f) xpaxTjXaLa xoO ^tqxouc; xoO xeXsLou
— JajJI JjJJl c-^w^ sine of the equated longitude
TpaxTTjXaLa ( c^v^ ) 6.7
x/jv xpaxTjXaLav x/jv xexeXsLCO^evriv xoO xeXsLou ^tqxouc;
— JajcII JjJJl >Lr c-^w^ sine of the complement of the equated longitude
TpaxTTjXaLa ( <^^^^ ) 6.7
340
TpaxTjXaLa xoO TSTsXeLCO^evou ^tqxouc; [xeaov xfjc; ^riTou^evric; tioXscoc; xal xoO
Geo^Laouarjc; Maxxa — oLoIl >Lc c.^^^ sine of the complement of the distance
TpaxTTjXaLa ( c^v^ ) 9.1.1
f) TpaxTjXaLa f) TSTeXeLCO^evr) xfjc; dvapdaecoc; xou totiou tcov dxpcov xfjc; xepxtSoc;
— 'i,'^J\ ^\ j^y- ^^ v:^ ^^^^ of the complement of the latitude of the clime of
the sighting
TpaxTTjXaLa ( c^v^ ) 9.1.3
xriv xpaxTjXaLav xfjc; xexeXsLCO^evrjc; dvapdaecoc; xfjc; aeXTQvric;
— j^\ ^^j\ j>Lr «^^w^ sine of the complement of the altitude of the moon
TpaxTTjXaLa ( ^..v^ ) 11.1.4
x/jv xpaxTjXaLav x/jv xexeXsLCO^evriv xfjc; dvapdaecoc; xoO xotiou xcov dxpcov —
<jj^l ^1 (j^^ ^^ V:^ ^^^^ ^f ^'^^ complement of the latitude of the clime of
the sighting
TpaxTTjXaLa ( c^v^ ) 11.1.4
x/jv xpaxTjXaLav xfjc; dvapdaecoc; xoO xotiou xcov dxpcov
— '^^^J\ ^\ j^j^ V^ ^^^^ ^f ^^^ latitude of the clime of the sighting
TpaxTTjXaLa ( c^v^ ) 11.1.7
x/jv xpaxTjXaLav x/jv xexeXsLCO^evriv xfjc; dvapdaecoc; xoO xotiou xcov dxpcov —
<j j^l Ajii\ j^jS- j>Lr «^^w^ sine of the complement of the latitude of the clime of
the sighting
TpaxTTjXaLa ( c^v^ ) 12.2.3
341
xriv TSTsXeLCO^evriv TpaxTjXaLav xoO TiXdxouc; xoO daxepoc;
— c-^y^iCJl ^^ ?^ V^ ^i^^ of the complement of the latitude of the planet
TpLycovov ( oJitJi ) 12.2.3
x6 TiXdxoc; eaxl xoO xpLycivou — JUitJl ^^ latitude of the trine
TpLycovov ( oJitJi ) 12.2.3
f) Std^expoc; xouxou xptycovov sgxl Ss^lov — J^.^' JUitJl '^l^.j and oppo-
site to it ( the sinister sextile ) is the dexter trine
TpLycovov ( oJitJi ) 12.2.3
f) Std^expoc; exsLvou xptycovov
— cUitJl ^^ ^t<jl>l5 QjLR-uJ ^ Cj^^uJJl) ob>j we add it (the sextile) to 90
and the sum is the arc of trine
TpLycovov ( C^^\ ) 12.2.4
x6 Se^Lov xptycovov — JUiiJl 0^^' dexter trine
TpLycovov ( C^^\ ) 12.2.4
x6 dpLGxepov xptycovov — ^H.^' JUitJl sinister trine
TpUTdvTT) ( jL^ ) 11.2.1
xpuxdvT) xfjc; Gecoptac; xfjc; ozkr^tf, — '^S^J^ jW^ measurement of the sight-
ing
TUX^O cf. TOTIOC; TTJC; TUX^O^
342
Tuxr) ( JliJi) 6.2.1
xfjc; TUXTjc; — JUaJl ascendant
TUxr) (^liJi)6.3
xfjc; Tuyjiq ToO 8' — ^JUJI ascendant
TUX^l ( ^liaJi) 9.1.2
xfjc; TUXTQ^ '^^^ xatpoO — ^JUJI ascendant
TUX^l ( ^liaJi) 9.1.2
^exa^u xfjc; Tuyjiq xal xoO l' olxiQ^axoc; — ^JUJI ascendant
TUxr] (^lk!i)9.3
x6 ^fjxoc; xfjc; aeXr]vr](; oltio xfjc; xuxtjc; — JUJI ja yjii\ a*j distance of the
moon from the ascendant
TUX^l ( ^^) 10.1.3
x/jv xu^TQ^ '^^^ auvoSou y] xfjc; SLa^expou — JL2JMI c^Sj ^Utf» ascendant at
the time of approach
TUX^l ( ^liaJi) 10.3.2
f) xuxT) xoO xatpoO — JUJI ascendant
TUX^l ( ^liaJi) 10.3.2.1
f) xuxT) — JliaJl the ascendant
TUxr) (^1>)12.1
343
ToO TOTiou xfjc; TUXTQ^ exdaxou — /^b^ ascendants
TUX^l ( ^liaJi) 12.1.2
f) TUXT) — «JLiaJl ascendant
TUX^l ( ^^) 12.1.2
Tiepl xfjc; elaeXeuaecoc; xoO totiou xfjc; xuxtjc; — Ju^^^l «JUtf» i^^^jco ^ on the
knowledge of the ascendant of the revolution
TUX^l ( ^^) 12.1.3
d XL eOpsGrj xotioc; xfjc; xuxtjc; sgxlv — JUtf» JUa^ J^^^' the result is the
rising time of the ascendant
Tuxr) ( ^Up) 12.1.3
xfjc; xuxTjc; xoO ^eaou xfjc; olxou^evric; — 5jj.o>.icU Ja^j /^^3 ^' /^^ ^^"
cendant of the cupola and the ascendant of the middle of the inhabited world
TUX^l ( ^liaJi) 12.2.1
eav [isaov xfjc; xu^iQ^ xal xoO 8' — ^.\J^3 ^UJI ijju UJ jlT it (the planet)
is in what is between the ascendant and the fourth
TUX^l ( ^liaJi) 12.2.1
C 5 V
o aaxrip [xeaov xou l xat xou a OLXTj^axoc; xou xotiou xtjc; xuxtjc;
— ^JliaJlj ji>[jti\ J\j UJ jIS^ jI i^^y^iCJl if the star is in what is between the
tenth and the ascendant
TUX^l ( ^liaJi) 12.4.
344
TO arj^SLov xoO ^coSlou xfjc; xuxiQ^ ^o\j Qe\ieXio\j xoO yeveBXiaXoyixoxj TiepL-
oaeueTOii eiq xouc; xpovouc; exsLvouc;
— ^JLUJI Sjj-i^ jl «^^i^j5CJl 'ti (^a)I /^^I Ojy^ ^J^ l3:>j we add them (the com-
pleted years) to the image of the zodiacal sign in which the planet is or to the image
of the ascendant
TUX^l ( ^liaJi) 12.4.2
f) ^oLpa xfjc; xu^iQ^ ^y]^ elaeXeuaecdq — iL^I Jd3^" ^UaJl <^j^ degree of
the ascendant of the revolution of the year
TUX^l ( ) 12.4.2
Kspi xfjc; XLVTQGSCOc; xcov (J^TQcpcov xfjc; xuxTjc; xfjc; eiaeXeuaecdq
— iL^I ik^^ ^^-^^ ^'Jhi-^' L-f ^^ ^'^^ prorogation of the indicators of the revolu-
tion of the year
TUxr) ( ) 12.4.3
Kspi xfjc; eXoLoecdq xfjc; Tuyjiq xfjc; elaeXeuaecoc; xoO ^rivoc;
— ^y^\ J}::^^^ jytr^^ J:! 3^" cJ ^^ ^'^^ revolution of the months and the pro-
rogation of their indicators
TUX^l ( ^^ ) 12.4.4
6 xoTioc; xfjc; Tuyjiq xfjc; eiaeXeuaecdq — iL^I J:! 3^" ^^ ascendant of the
revolution of the year
TUX^l ( ^^ ) 12.4.4
Tiepl xfjc; eXdaecoc; xfjc; elaeXeuaecoc; xfjc; xuxtjc;
— iL^I Jd3^ /^^ ^i^^' cJ ^^ ^'^^ prorogation of the ascendant of the revolu-
345
tion of the year
(jTlz'iZGi:!] {jjj ) 11.3.1
f) aeXTQvr) OTie^eaxri xoO cpcoxoc; xoO tiXlou xal Tipo xoO SOvat xov yjXlov cpatvexaL
auxT)
— j..^] c^.^ Ju5 IjL^ ^^, jl j5Co^ ^L^l jj^ J>UI j^
the crescent has come into view from under the rays and it is possible to see it in
daylight before the setting of the sun
UTlsSscyTTT) ( j^ ) 11.6.1
f) aeXTQvr) OTie^eaxr) xoO cpcoxoc; xoO tiXlou xal upb xoO SOvat xov yjXlov cpatvexaL
— jLaj>U pUJJI j^ j^ Ji it (the moon) has emerged from under the rays for
sighting
UTis^^axavTaL ( ) 11.5
Tiepl xcov £ TiXavco^evcov daxepcov oxl xaxa tiolov xatpov e^ep^ovxat yjxol
UTie^LGxavxaL xoO cpcoxoc; xoO tiXlou xal xaxa Tiolav oSpav slaepxovxaL Otio cpcoc; xoO
tiXlou xaxa x6 Tipcot y] xtjv saTiepav — Lp:>^j oIa^^iII ^.^^iCJl ^,j^ ^ on the
rising of the moveable stars (planets) and their settings
UTisp ( 3y ) 12.2.1
UTiep yfjv — c^j^^ <Jy above the earth
UTisppatvsL ( jU ) 1.5.2
UTiepPaLVSL — J3^ S^ beyond
UTIO ( Oc^" ) 12.2.1
346
UTio yfjv — j^j^^ '•^^ below the earth
ukokoSl^sl ( ^\j ) 8.2
6 daTf)p OjiOTioSiCei — /*^!j retrograding
ukokoSl^sl ( ^\j ) 8.2.1
'Eav 6 daTf)p utiojioSiCt] — ^*^|j tw-^^^^OI jlS' jlj if the planet is retrograd-
ing
utiotio5l^£l ( «^j ) 8.2.2
UTioTioSiCsi. — ^j retrograde
ukokoSl^T) ( \^\j ) 11.5.2
sdv 6 daTf)p utiotioSlCt) — ^*^!j O'^ '-^^ if the star is retrograding
UKOKoSiajioc; ( iffr_^j ) 8.0.0
Tou UTiojioSLa^ioO aOxcov — \^ y>j their (the planets') retrogression
UKOKoSiajioc; ( ^^^Ji ) 8.2
TOU UTiojioSLa^ioO — ? y^y^ retrogression
U(J;cu)[jia ( oUjl ) 7.0.0
Tc5v ut|;co[jidTCOv — olaj-jl apogees
u();(0[jia ( rp^\) 7.1.1
u(|»w[id eaxi xfjc; opGcoaecoc; — JajJ.1 r ^^ equated apogee
347
U();63[ia ( rj,\ ) 7.4
xa u(J;(0[jiaTa — oU-jl apogees
U();63[ia ( r^\ ) 8.1.1
TO ut|;co[jia xou f)Xiou — W=fj' its (the sun's) apogee
U();63[ia ( r^\ ) 8.1.1
TO Tzkeiov ut|;co[jia — ^j-.oJJl J Ajc« ?-jI equated apogee of the sun
U();63[ia ( rj,\ ) 8.1.4
TO ut|;co[jia — ^-jl apogee
U(J;CO[jia ( Sjji ) 9.2.4
TO u(J;w[jia ToO [jiixpoO xuxXou — jij-^' Sjji apogee of the epicycle
u();(0[jia ( r-j^fl ) 12.1.2
f) Tispiaasia exeivT) [iSTOc Tfjc; opGcoaswq toO ()'i^<i>\xaToq TsXeia yivsTai —
?-jML; iljjtll iLaill excess equated by the apogee
cpaivsTai (j_^) 1.5.1
OTiOTav dnb tou fiXtou SuoTa^ievou cpatvcovTai — pL«JJl o^" j>« Iaj_5^ its
appearance from under the rays
cpaivsTai (^ ) 11.5
6 daTT)p cpaivsTai — j^ Ai <_^^\ the star has already appeared
cpaLVSxaL ( ^_^ ) 11.6.2
348
f) aeXr]vr] cpaLvexaL — ^^^ J>U1 the crescent is visible
cpatvo^svoc; ( ijjj ) 11.2
Kspi xfjc; aeXrivriq veaq cpaLvo^evrjc; [xstol auvoSov — ilA^II 'ij^^j JU^I ^ on
the computations for the sighting of the crescent
cpavsLc; ( 'C^j ) 1.1
gsXtqvc; veac; cpaveLarjc; — J>UI <jjj sighting of the crescent
cpavsL^ ( <::3Ji) 11.5.1
exsLVT) f) TiepLaasLa eav tiXslcov toO cpavevToc; xo^ou
— '^^^J\ ^y ^ J^ AjtJl jlSj the distance is greater than the arc of vision
cpavsL^ ( <ijji ) 11.5.2
TO TO^ov TO cpavev — h3j^ iT^ ^^^ ^f vision
cpavsLc; ( i^Jj ) 11.6
TTJc; aeXrivriq veaq cpaveLarjc; — il^MI <jjj sighting of the crescent
CpaVT] ( i^jj ) 11.0.0
OTL f) aeXTQvr) tiots tva cpavrj vea — ilA^II <j jj the sighting of the crescent
CpaVT] {jyi^\ ) 11.5.1
OTav cpavrj 6 daTiQp xal OTav Suvr] — tUli-Mlj j^^l appearance and dis-
appearance
cpavfjvaL ( jyi^ ) 11.5.1
349
eav oOv 6 (J;fjcpoc; oOxoc; sic; to cpavfjvaL xov daxepa — j^-^^ J^' 0^0^
if the computation is for the appearance
^apoux ( <5jjliJi ) 1.5.3
3>apoiJx — iSjjliJl Faruqa
cpGdvsL ( JjjP ) 12.1.1
fivLxa cp6dv£L 6 yjXloc; sic, xriv ^otpav exsLvriv —
i^^yii] iialJl j^usJJl Jjj3 Al^ at the alighting of the sun at the determined point
cpcoc; (jjJi ) 11.1.5
TO e^eXGov to^ov soti toO cpcoxoc; fjyouv xfjc; eXXd^cJ^ecoc; xfjc; aeXTQvric;
— jj-Jl j^3^ ^^c of light
cpcoc; (jjJi) 11.1.5
xoO xo^ou xoO cpcoxoc; — jyi\ ^yi arc of light
CpCO^ {jyi\) 11.3
x6 TO^ov xoO cpcoxoc; — jy^\ ^y arc of light
cpco^ {jyi\) 11.3.1
xoO xo^ou xoO cpcoxoc; — jyi\ ^y arc of light
cpco^ ( pU^I) 11.3.1
f) aeXTQvr) OTie^eaxr) xoO cpcoxoc; xoO tiXlou xal Tipo xoO SOvat xov yjXlov cpatvexaL
auxT)
350
the crescent has come into view from under the rays and it is possible to see it in
daylight before the setting of the sun
cpco^ ( pU^I) 11.3.1
f) aeXTQvr) £tl Otio to cpcoc; eaui xoO tiXlou xexpu^^evr) — pUjJI c^ under
the rays
cpco^ {jyi\) 11.6.1
TO TO^ov ToO cpcoTOc; — jyi\ ^y arc of light
CpCO^ {jyi\) 11.6.2
TO TO^ov ToO cpcoTOc; — jyi\ ^y arc of light
CpCO^ ( pU^I) 12.2
ToO TOTiou ToO cpcoTOc; Tcov dcGTspcov Y]TOL ToO Tipoc; ocXXriXa TOUTCOv axTj^aTLG^oO
— ol^L«Jjl rj^ casting of rays
CpCO^ {jy ) 12.2.3
6 TOTioc; eoTL toO cpcoToc; toO e^aycivou toO daTspoc; e'E, dpLGTspcov
— ^r^.^1 4^.uJ jy ^yi the location of the light of its sinister sextile
CpCO^ ( pU^I) 12.2.3
ToO TOTiou ToO cpcoTOc; Tcov dcGTspcov — <^^\ ol^l^ ^ J^^ castiug of rays
of the planet
CpCO^ ( pU^I) 12.2.4
Std^STpoc; SGTL ToO cpcoTOc; ToO dcGTspoc; — ol^L«JJl ^UaJ the opposite points
351
of the rays (aspects)
963^ ( ^UJJl) 12.2.4
ToO TOTiou Tou (pcoT6(; Ttov daxEpcov — pLuJJI /»-^,ia« casting of the rays
963^ ( ^UJJl) 12.4.2
TOU (pcoT6(; Ttov daxepcov oXcov — LLj^l ols-l*-jJlj ^_^^X)I >«;woji: by all
the stars and the aspects of the revolution
Xa^avf] ( J j 1:^0 11.6
ToO Xa^avfj — (^j^^ >Lo^[| ^k^ Shaykh Imam al-Khazinl
Xpovoc; ( iLJi ) 1.1
Xpovoc; — iL^I year
Xpovoc; ( iLu/ ) 1.2
xpaxoOvxaL ol xpovoL TSTsXeLCO^evoL xoO enouq xoO 'laaSaxepSr)
— ^bl ^y>-^y, ^j^ \jJ^\ we take the completed years of Yazdijird
Xpovo^ ( 0^ ) 1.2
XpovoL ToO tiXlou — i^-uusJJl ijj^ solar years
Xpovoc; ( oj^i ) 1.2
ol xpovoL xfjc; aeXTQvric; — ^i^r«^' jj-L^I lunar years
Xp6vo<; ( ) 1.4.1
xavovLa xcov xpovcov xcov fivco^evcov xal xcov aiiXcov —
352
i^j-^lj ipjuj^l cJ3^ ^^^ ^^^ tables of the collected and simple (years)
Xpovoc; ( iLu/ ) 1.4.1
ol OLTsXelq y^povoi xoO enouq exeivou — i^aSUI ^ jUl ^J^^ incomplete years
of the calendar
Xpovoc; ( iLu. ) 1.4.2
ol TSTsXeLCO^evoL xpovoL — ^bl ^J^^ complete years
Xpovoc; ( 'Ll^ ) 7.1
ol dxeXsLc; xpovoL — <^UI iJLu diminished years
Xpovo^ ( Ju^ ) 7.3
yvcopL^cov xpovcov — JLJI ^^^u^ years of the world
TCOV
Xpovo^ ( ) 7.3
Xpovcov Tcov aouXxavLXCOv — iJliaLJl Sultanic (years)
Xpovoc; ( iLJi ) 7.3
xpovoc; ToO tiXlou — i^-^usJJl iL^I solar year
Xpovo^ ( ) 7.3
6 xpovoc; Tcov 'Pco^aLCOv — *^j^' Roman (year)
Xpovoc; ( iLJi ) 7.3
ToO xpovou xfjc; aeXTQvric; — ^i^r«^' 'iL^] lunar year
353
Xpovo^ {J^)7.3
ol xpovoL ol alaGriTol — JLJI ^^^ years of the world
Xpovo^ ( l^ ) 7.3
Tcov TSTsXeLCO^evcov aouXxavLXCov xpovcov — iobi L^JL^ its complete years
Xpovoc; ( jjJlJI ) 12.0.0
XpovoL eiai xoO tiXlou TSTsXeLCO^evoL — L-^usJJl iobi jjJL^I complete solar
years
Xpovoc; ( iLu. ) 12.0.0
xfjc; SLaeXeuaecoc; xcov xpovcov — JLJI ^^^u^ Jd3^ revolution of the years of
the world
Xpovoc; ( iLu/ ) 12.1
Kspi xfjc; SLaeXeuaecoc; xcov xpovcov oXcov xal xcov xpovcov xcov yevsGXLaXoyLXCov
— -^JljJ^lj iLJl ^J^ ^.y^' ^ on the revolution of the years of the world and
of nativities
Xpovoc; ( iLu/ ) 12.1.1
Kspi xfjc; expoXfjc; xcov (bpcov xfjc; eiaeXeuaecdq xcov xpovcov oXcov —
JLJI ^^^u^ Jd^^" olSjl ry>^^^\ ^ on the extraction of the times of the revolutions
of the years of the world
Xpovoc; ( 0^^ ) 12.4.1
ol xexeXsLCO^evoL xpovoL xoO tiXlou ol TiapeXGovxec; duo xoO yevsGXLaXoyLXoO
— ^^^\ ^ oJI (jJl ^bl C^^' the complete years which have passed for the
354
native
XpOVO^ ( ) 12.4.1
Kspi xfjc; evQ\j\iriaecdq exeivou xoO (J;7]cpou otl xa6 ' exaaxov xpovov a ^6)8lov
XLVSLXaL
— O'biu-^j V^^S^ *^-^ J^cJ LiY^' cJ ^^ ^'^^ muntahd^ in every house and
the star and its prorogations
XCOpSL ( ) 2.1
Tipoc; TO eXaxTOV x^P^i^ — LaSb decreasing
XCOpSL ( ) 2.1
Xcoprj Tipoc; to tiXsov — JjIj increasing
(];f]cpoc; ( jIaIo ) 1.2
6 \iiao^ ^ff^o^ — ]a^^H\ jIaIo measure of the mean
(];f]cpoc; (^.J^i ) 1.4.2
ToO ^eaou exsLvou (J;7]cpou — ]a^^H\ ^.Ail)l mean estimate
();fi90^ ( ) 2.1
6 (J;fjcpoc; xaxa xriv apx^Q^ "^^^O xavovLou — 'LJ\s> (number in) the margin
();fi90^ ( ) 2.1
ToO xpaxou^ievou jiap' f)[jic5v t|;TJcpou — JsjJlpJ,! set aside
();fi90c; ( ) 2.1.1
355
ToO dcTio ToO [xeaoxj xavovLou (J;7]cpou — Jj-^' jJl> ^ (number) in the
interior of the table
(];f]cpoc; {j^J^ ) 7.1
ToO ^eaou (J;7]cpou — Ja^jl ^.-^' mean estimate
(];f]cpoc; ( ) 8.1.4
ToO (J^TQcpou ToO eOpsGevToc; ^eaov xcov p xavovLCOv — 4Jb AjJ its equalization
(];f]cpoc; ( c-^Lo^ ) 8.4
[iSTOL ToO (J^TQcpou — [jLms> by calculation
(];f]cpo^ ( J^ ) 10.3.2
Tiepl ToO (J^TQcpou — Jl^ ^ on the calculation
();fi90^ ( ) 11.3
6 [leooci (J;fjcpoc; — ^^'j cJ3^' c5^3^ Ja1«II Ja-^jMI jJ-l the mean equated
limit of the first and second arcs
();f]cpo^ ( J«*)l) 11.5.1
si 8' eaxlv oOxoc; 6 (J;fjcpoc; tva Suvr] 6 daxTQp — tUli-^U Ju^jJI jIT jU if the
computation is for the disappearance
^fic^oq ( Jo^l) 11.5.1
eav oOv 6 (J;fjcpoc; oOxoc; sic; x6 cpavfjvaL xov daxepa — jj^gWU Ju^*)! j^ j^i
if the computation is for the appearance
356
(];f]cpoc; ( ) 12.4.1
Tiepl xfjc; evGu^TQaecoc; exeivou xoO (J;7]cpou otl xa6 ' exaaxov xpovov a ^6)8lov
XLVSLXaL
— <jljiu-^j V^^S^ *^-^ J^cJ LiY^' cJ ^^ ^'^^ muntahd^ in every house and
the star and its prorogations
63pa ( oUUi) 4.3.1
xfjc; opGfjc; oSpac; — ij^^l^l ol^LJl equal hours
63pa ( oUU) 4.3.1
f) oSpa xfjc; vuxxoc; Tidarjc; — jV^\ ol^Lu hours of the daytime
63pa ( oUji ) 5.0.0
xfjc; oSpac; exsLvrjc; xfjc; xaxa if\\ dvdpaaLV xal xaxdpaaLV xouxcov xaxd if\\
fj^epav f\ if\\ vuxxa — J^ j' J^ 0^ V:J^ 3^ [^^^ olSjl the times of its rising
or setting in the night or day
63pa ( ) 6.0.0
duo xfjc; fj^epac; hoooli d^pat TiapfjXGov — JJl)I jI jV^' J-^ c-f-^^ ^ what has
passed of the day or of the night
63pa ( oUUi) 6.1
x/jv 6p6fiv oSpav xal x/jv ^f) opGiQv — i^^^lj <j^jl^l ol^LJl equal and
seasonal hours
c5pa (^lk)l)6.2
xfjc; oSpac; ex xfjc; jiepLcpopdc; — SyljJl j^ ^JUJI ascendant from the arc
357
63pa ( oij ) 6.3
xfjc; oSpac; xoO xatpoO — j^^' C^Sj time under consideration
IdpOL ( oUUi) 7.4
xac; oSpac; xfjc; dvapdaecoc; — ol^li^j^dj ol^LJl hours and altitudes
63pa ( ipU) 8.4; 8.4.1
x/jv oSpav — ipLu an hour
63pa ( ipU ) 9.2
xfjc; oSpac; xoO ^tqxouc; xoO [xeaou xfjc; fj^epac; — J'jj/Jl j^ -^1 ol^Lu hours
of distance from noon
63pa ( ) 9.2
oSpa xfjc; auvoSou — ^t<sl5»"MI (hour) of conjunction
63pa ( oUL. ) 9.2
f) oSpa xoO ^eaou xfjc; fj^epac; — j[^\ cJLuaj ol^Lu hours of half the day
63pa ( ipU ) 9.2
f) oSpa xoO ^TQXouc; ^exd x6 [xeaov xfjc; fj^epac; sgxlv. — J'jj;^' J^ -W^' ol^Lu
hours of distance from noon
63pa ( ipU ) 9.2
f) oSpa xoO ^TQXouc; Tipo xoO \ieao\j xfjc; fj^epac; sgxlv — J'jj/Jl j^ -^1 ol^Lu
hours of distance from noon
358
63pa ( ) 10.1.1
xal yLvexaL oSpa TsXeioL — [lls> JL2JMI j}:^^ the approach becomes complete
Idpoi ( oUU) 10.1.1
oSpa eaxl xfjc; auvoSou y] xfjc; SLa^expou duo xfjc; TiapeXGouarjc; vuxxoc; —
i^LlI iLUl ^ iiiiall JluqjMI ol^Lu the hours of the general approach of the night
just passed
63pa ( oUL. ) 10.1.1
oSpa eaxl xfjc; auvoSou y] xfjc; SLa^expou dmb xfjc; £p)(o^£vric; vuxxoc; —
iLllI <Jl)I j^ (jUall JluqjMI ol^Lu the hours of the general approach of the coming
night
63pa ( oUL. ) 10.1.1
oSpa eaxl xfjc; auvoSou y] xfjc; Sta^expou sic; exsLvriv x/jv fj^epav —
>yj\ dJi j^ i^LlI (jUall JUajMI ol^Lu the hours of the general approach that
have passed of that day
Idpoi ( oUU) 10.1.1
xcov (bpcov xfjc; fj^epac; exsLvrjc; Tidarjc; — 4JS^jlyJl ol^Lu hours of the whole
day
63pa ( oUU) 10.1.1
f) oSpa eaxl xou ^tqxouc; — Aj«JI ol^Lu hours of distance
63pa ( oUU) 10.2.1.1
359
f) oSpa xfjc; ^earjc; exXsLcJ^ecoc; — lJ^^^\ ]a^^ ol^Lu hours of the middle of
the eclipse
63pa ( oUL.) 10.2.1.1
f) oSpa xfjc; auvoSou — JLajMI ol^Lu hours of the approach
63pa ( oUL.) 10.2.1.4
f) c5pa xfjc; TsXe Lac; dTioxaTaaxdaecoc; xfjc; aeXTQvric; — t>U^MI >Lr ol^Lu hours
of the completion of the clearing
63pa ( oUL.) 10.2.1.4
f) ^ear) oSpa xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; — l3j-^I Ja^jl ol^Lu hours of
the middle of the eclipse
63pa ( oUL.) 10.2.1.4
oSpa xfjc; dpx'H^ "^"H^ exXsLcJ^ecoc; xfjc; aeXTQvric; — l3j-^I tijj ol^Lu hours of
the beginning of the eclipse
63pa ( oUL.) 10.2.1.4
oSpa xfjc; SLa^expou — JLil^MI ol^Lu hours of opposition
63pa ( oUL.) 10.2.1.4
oSpa TieaoOaa — Jg>j^.Jl ol^Lu hours of the falling (half duration)
63pa ( o*^jO 10.2.1.4
xfjc; oSpac; xfjc; £xX£L(J;£COc; xfjc; aeXTQvric; — ^y^\ jUjI duration of the eclipse
360
63pa ( oUU) 10.2.1.5
oSpa eaxlv duo xfjc; ocp^fjc; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; ^^XP^ '^^^ xeXetac;
dcTioxaxaaxdaecoc;
— t>L:^'^l >Lr Jl tljJl j^ l3j-^I t ^3 ol^Lu hours of the occurrence of the
eclipse from the beginning to the completion of the clearing
63pa ( oUU) 10.2.1.5
al Keaouaoii &>poii — Jg>j)gM> ol^Lu hours of the falling
63pa ( oUU) 10.2.1.5
f) xexeXsLCO^evT) oSpa xa6' y]v djioxaGLaxaxaL f) aeXTQvr) — t^U^MI >Lr ol^Lu
hours of the completion of the clearing
63pa ( ) 10.2.1.5
f) dpxT) xfjc; oSpac; xfjc; duoxaxaaxdaecoc; xfjc; aeXTQvric; — t>U"MI tijj (hours)
of the beginning of the clearing
63pa ( oUU) 10.2.1.5
f) oSpa xfjc; ^earjc; exXsLcJ^ecoc; — l3j-^I Ja^jl ol^Lu hours of the middle of
the eclipse
63pa ( oUU) 10.2.1.5
oSpa xfjc; xeXsLac; exXsLcJ^ecoc; — JU5CII tijj ol^Lu hours of the beginning of
the duration
63pa ( oUU) 10.2.1.5
d)paL SLGL xfjc; Gxdaecoc; — JLil^MI ol^Lu hours of opposition
361
63pa ( oUU) 10.2.2.1
f) oSpa xfjc; axdaecoc; — JU5CII ol^Lu hours of duration
IdpOi ( oUU) 10.2.2.1
ol SdxTuXoL xfjc; Tieaouaric; oSpac; — ^^yuJ] ol^Luj «jL^MI the digits and
the hours of the falling
IdpOi ( oUU) 10.2.2.3
f) oSpa xfjc; vuxxoc; xfjc; exXsLcJ^ecoc; tiXslcov eaxlv duo xfjc; oSpac; xfjc; vuxxoc;
— JJJI ol^Lu ^^^ ^«^ljll As>l ol^Lu j}2ju Cj^\j some of the hours of one of the
places is greater than the hours of night
63pa ( oUU) 10.2.2.3
edv f) oSpa xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; duo xfjc; fj^epac; tiXslcov f) —
jlyJl oU-Lu ^J^ Sj^Ail ^«^ljil J<£>\ oU-Lu o^Ij the hours of one of the mentioned
places is greater than the hours of the day
63pa ( oUU) 10.3.1
al &>poii eiai xoO ^tqxouc; Tipo xoO [xeaou xfjc; fj^epac; xal ^exd x6 [xeaov xfjc;
fj^epac; — ^^Ij Jj-!^1 ^^ oAjuj Jljj;)! J^ ol^Lu the hours before noon and
after it in longitude and latitude
63pa ( oUU) 10.3.2
x/jv oSpav xfjc; auvoSou opGiQv — ^^1^1 pUi^^-MI ol^Lu JuAjJ equation of
the correct hours of the conjunction
362
63pa ( oUU) 10.3.2
f) [isar] cdpoL eoTi xfjc; exXsLcJ^ecoc; — lJ^^.mS^\ ]a^^ ol^Lu hours of the middle
of the eclipse
63pa ( oUU) 10.3.2
oSpa ToO ^eaou xfjc; fj^epac; — j{^\ cJLuaj ol^Lu hours of half the day
63pa ( oUU) 10.3.2.1
oSpa eaxl xfjc; ^earjc; exXsLcJ^ecoc;. — l33-uJCJI i^^^j ol^Lu hours of the middle
of the eclipse
63pa ( oUU) 10.3.2.1
f) oSpa xoO P' ^TQXouc; — ^li)l pUIj»"MI ol^Lu the hours of the second con-
junction
63pa ( oUU) 10.3.2.1
oSpa xoO TiXsLovoc; xal eXdxxovoc; xfjc; ocj^ecoc; xoO a — Jj^' L3>ti"MI ol^Lu
hours of the first difference (in vision)
63pa ( oUU) 10.3.2.1
xfjc; oSpac; xoO \iioo\j xfjc; fj^epac; — j[^\ cJLuaj ol^Lu hours of half of the
day
63pa ( oUU) 10.3.2.1
f) oSpa xoO ^TQXouc; eaxl ^exa x6 \iioo\ xfjc; fj^epac;
— Jljj;)! Aju ol^LJl ^ AjtJl c-Jliaj we seek the distance in the hours after
noon
363
IdpOL ( oUU) 10.3.2.1
f) oSpa ToO ^TQXouc; eaxl upb xoO ^eaou xfjc; fj^epac;
— Jljj;)! Jl^ ol^LJl ^ AjtJl L-Jliaj we seek the distance in the hours before
noon
IdpOi ( oUU) 10.3.2.1
f) oSpa ToO ^eaou xfjc; fj^epac; — jV^' cJLuaj ol^Lu hours of half of the day
IdpOi ( oUU) 10.3.2.1
f) oSpa xfjc; aovoSou — pUi^^-MI ol^Lu hours of conjunction
63pa ( oUU) 10.3.2.1
f) oSpa xfjc; auvoSou — pUj^MI ol^Lu hours of conjunction
63pa ( oUU) 10.3.2.3
f) TieaoOaa oSpa ^exa xfjc; opGciaecoc; xauxTjc; — UtIAjJj Jg>j^.Jl ol^Lu hours
of the falling and their equation
63pa ( oUL. ) 11.1.1
f) oSpa xoO ^eaou xfjc; fj^epac; — j^usJJl 'is>-j^ j[^ cJLuaj ol^Lu hours of half
of the day of the degree of the sun
63pa ( oUU) 11.1.1
oSpa eaxl ^eaov xfjc; fj^epac; exsLvrjc; xal [xeaov xfjc; xaxapdaecoc; xfjc; ^otpac;
xfjc; aeXTQvric;
— ^;^l ty>- «^^wJl^ Jl jV^^ cJLuaj ijiu Lo o^-Lu the hours between the half of
364
the day to the setting of the degree of the moon
63pa ( oUU) 12.1.1
al &>poii xfjc; eiaeXeuaecdq olko xfjc; fj^epac; y] xfjc; vuxxoc;
— jL^ j' J^ 0^ Jd^^' C/^j ol^Lu hours of the time of the revolution at
night or in the day
63pa ( oUU) 12.1.1
oSpa eaxl xfjc; eiaeXeuaecdq — J:! 3^" ol^Lu hours of the revolution
63pa ( oUU) 12.1.1
f) oSpa xoO [xeaou xfjc; fj^epac; — jV^' cJLuaj ol^Lu hours of half of the day
63pa ( oUji) 12.1.1
Tiepl xfjc; expoXfjc; xcov (bpcov xfjc; elaeXeijaecoc; xcov xpovcov oXcov —
JLJI ^J^^ Jd>^ olSjl T-^pJ^I ^ on the extraction of the times of the revolutions
of the years of the world
63pa ( oUU) 12.1.2
f) oSpa xfjc; eiaeXeuaecdq — Ju^^^l C^Sj ol^Lu hours of the time of the
revolution
63pa ( ) 12.3
xcov (bpcov xcov xaXcov xal xaxcov — j^^^b •^3^«-^' ^ya place of the
benefices and malefices
(bpat ( oUUi) 9.2.1
365
al S^poLi ToO ^TQXOUc; — jV^' eJLuaJ ^ yiJii] Aju L^ ^ ^1 ol^LJl hours
by which there is a distance of the moon from half of the day
6paLO^ ( cJzJalJi) 10.3.2.1
TO (bpaLov xavovLov — LJzJaUl Jj^i-I the easy table
PART IV
Greek Text
366
9
12
367
yApyji ToO PlPXlou toO Savx^apfj fssv, f273vv
MoLpa a . Ilepl xcov yvcopt^cov excov.
MoLpa P' . Ilepl xcov xaxaXiQcJ^ecov xcov (J^iQcpcov xcov xaxa tioXu XuglxeXouvxcov
£Lc; x/jv spyaaLav xfjc; auvxd^ecoc; fjyouv xfjc; TiepLaasLac;, xfjc; xpaxTjXaLac; xoO
5 xo^ou, xfjc; aayLxac; xal xoO axLda^axoc;.
MoLpa Y ' Ilepl xfjc; TipcixTjc; xal Seuxepac; ^exaxXtaecoc; xfjc; popetac; xal
voxlac; xal xoO TiXdxouc; xcov tioXscov xal xfjc; dvapdaecoc; xcov daxepcov sic; xov
xuxXov xoO \ieao\j xfjc; fj^epac; xal xoO xotiou xfjc; xu^iQ^ t^s:xd xfjc; eOGsLac;
ypa^L^ifjc;.
10 I MoLpa 8' . Ilepl xfjc; opGciaecoc; xfjc; fj^epac; ^exd xoO xo^ou xfjc; fj^epac; xal fsivL
xfjc; vuxxoc; xal xcov 6p6cov (bpcov ^exd xcov ^oLpcov xcov ^f) 6p6cov (bpcov xal
xcov xoTicov xcov ^coSlcov £lc; Tidvxa xd xXl^axa ^exd xoO TiXdxouc; xfjc; dvaxoXfjc;.
MoLpa £ . Ilepl xfjc; xlvtqgscoc; xcov diiXavcov daxepcov olko xcov aOGrj^epLvcov
exsLvcov xal xoO ^tqxouc; yjxol xfjc; Staaxdaecoc; sxslvcov olko xoO xuxXou xoO
15 xaxd x6 vu^QiQ^epov xlvou^svou xal xfjc; dvapdaecoc; xcov diiXavcov sic; xov
xuxXov xoO ^eaou xfjc; fj^epac; xal xfjc; ^olpac; exsLvrjc; yjxlc; duo xoO ^coSlou
I £X£Lvou ^£xd xoO doxspoc; o^oO £Lc; xov xuxXov xoO ^eaou xfjc; fj^epac; f274rv
ylvexaL xal xfjc; ^olpac; yjxlc; dvlax^L ^£xd xoO daxepoc; xal xfjc; ^olpac; xfjc;
1 Tit. diff. lectu V || 2 TipcoTir] v || i5 tov om. v
368
[xeTOL ToO daxepoc; Suvouarjc; xal xfjc; xaxaXiQcJ^ecoc; xfjc; oSpac; exsLvrjc; xfjc; xaxa
x/jv dvdpaaLV xal xaxdpaaLV xouxcov xaxd x/jv fj^epav y] x/jv vuxxa.
MoLpa q . Ilepl xfjc; xaxaXiQcJ^ecoc; exsLvrjc; oxl duo xfjc; fj^epac; jioaaL &>poii
TiapfjXGov xal TioaaL ^otpaL olko xfjc; ^f) opGfjc; oSpac; xal sic; xdc; oSpac; xfjc; Tuyjiq
5 xal xfjc; opGciaecoc; xcov i^ OLXTj^dxcov, xal xfjc; xaxaXiQcJ^ecoc; xoO arj^SLOu xfjc;
exdaxric; dvapdaecoc; xal xoO arj^SLOu xfjc; jipoaeuxfjc; fexdaxric;.
MoLpa C • Ilepl xfjc; expoXfjc; xcov [xeacdv xlvtqgscov xcov ^ daxepcov xal xcov
lSlcov I xouxcov XLVTQGSCov xal xcov OcJ^co^dxcov xal xcov opGciaecov exdaxric; xal fssvv
xfjc; xaxaXiQcJ^ecoc; xfjc; dp^fjc; xoO aouXxavLXoO xpovou xaxd Tiolav fj^epav eaxlv
10 duo xcov fj^epcov xfjc; 8:p|8o^d8oc; duo xcov ^rivcov xal xcov xpovcov xcov excov xal f82L
xoO xeXouc; xouxou xal xfjc; opGciaecoc; ^exd xoO Gs^eXlou oxl x6 aOGrj^epLvov
duo xfjc; auvxd^ecoc; olko xouxou xoO Gs^eXlou sxpdXXexaL sic; a xp^vov xoO
fjXLou Std x6 aOGrj^epLvov.
MoLpa y] . Ilepl xfjc; expoXfjc; xcov ^ daxepcov xoO aOGrj^epLvoO xal xoO dva-
15 pLpd^ovxoc; xal xfjc; xax' 6p66v xlvtqgscoc; xal xoO OtiotioSlg^oO xcov daxepcov
xal xoO TiXdxouc; sxslvcov xal xfjc; ^exapdaecoc; exdaxou xal xcov Sta^expcov
xouxcov.
MoLpa 6'. Ilepl xoO tiXslovoc; xal eXdxxovoc; olko xfjc; ocj^ecoc; xfjc; Gecoplac;
xfjc; aeXTQvric; xal xfjc; opGciaecoc; xoO xotiou exeivou sic; x6 ^fjxoc; xal TiXdxoc;.
6 Tipoaex'n^ V II 9 xf]^ o^PX'H^ ^^P- ^i^- L | auXxavLXoO v || 14-15 dvapLpdCovTO^]
U Vv,r) L II 19 exsLvou quia^^l masc.
369
MoLpa l'. Ilepl xfjc; xaxaXiQcJ^ecoc; xcov auvoScov xal Sta^expcov tiXlou xal
aeXTQvric; ^exa xoO ^tqxouc; xal xfjc; ^exapdaecoc; sxslvcov xal xcov exXelcJ^ecov
tiXlou xal aeXrivriq. f) l' Se auxr) ^otpa sic; xpla SLaLpsLxaL.
MoLpa La'. Ilepl xfjc; aeXrivriq veaq cpaLvo^evrjc; xal xcov e daxepcov.
5 MoLpa i^\ Ilepl xfjc; Tuyjiq xcov y^povcdv xal xcov 8 xatpcov xal xfjc;
SLaeXeuaecoc; xfjc; xu^iQ^ "^^^Ci xp^^ou exsLvou xal xoO yevsGXLaXoyLXoO xal xfjc;
axxLvopoXlac; xcov daxepcov.
3 Y L
370
MoLpa Tipcixr). Ilepl xcov yvcopt^cov excov. xaOxa sic; £ xecpaXata exsGrjaav
KecpdXaLov a . Ilepl xfjc; fj^epac; xal vuxxoc; xal xoO ^rivoc; xal xoO xpovou,
xLva xaOxa.
KecpdXaLov P' . Ilepl xoO exouc; xl sgxl xal koIol sxt) slc; xov fj^exepov xpovov,
5 SfjXa.
IKscpdXaLov y'. Ilepl xfjc; xaxaXiQcJ^ecoc; xfjc; ocp^fjc; xoO xpovou xax' exoc; xal f82vL
xcov ^rivcov xaxd Tiolav fj^epav elal xfjc; fepSo^dSoc; | xal xfjc; expoXfjc; xoO evoc; f39rv
exouc; OLKO xoO exepou ^exd xoO (J;7]cpou.
KecpdXaLov 8'. Ilepl xfjc; dp^fjc; xcov y^povcdv xal xcov ^rivcov xaxd Tiolav
10 fj^epav SLGspxovxaL xfjc; fepSo^dSoc; xal xfjc; expoXfjc; xoO evoc; exouc; duo xoO
exepou Std xcov xavovlcov.
KecpdXaLov £ . Ilepl xcov eopxcov xal xcov ^eydXcov fj^epcov xal StqXcov xcov
xax' sQvoq xeXou^evcov xal Std (J^iQcpcov xal Std xavovlcov.
KecpdXaLov ol . Ilepl xfjc; fj^epac; xal vuxxoc; xal xoO ^rivoc; xal xoO xpovou
15 xLc;.
1 ^OLpa TipcoTiT] iter, in marg. v^ || 2 -3 Ilepl xfjc;. . . xLva TaOxa] Tiepl toutou* fj^epa tlc; eaxL
xal vu^ tlc; xal ^ttjv tlc; xal xpovoc; tlc; L || 4 Ilepl toO stouc;] Tiepl xaTaXir](|>£(j)c; toutou otl
TO ETOc, L 4-5 SfjXa post ETT] transpoH. L || 6 xal + tcov apx^v L || 9 Ilepl . . . ^rjvcov]
Tiepl Tf]^ xaTaXir](|>£co^ toutou otl f] apx^^ xou xpovou xaT' sto^ xal dpxal tcov ^rjvcov L || is
(|>ir]cpou L II 14 fj^epa^ + tt]^ L | xal^ + tt]^ L || i5 tl^ om. L
371
'H^epa xal vu^ yjtol vu^QiQ^epov exelvo eaxLv f) xfjc; acpatpac; XLvou^evrjc;
dcTio ToO auToO arj^SLOu sic; to aOxo TidXtv dTioxaxdaTaaLc;, o xal 8l' (bpcov
TsXeiomoii x8. xriv dpxTjv Se toutou exaaxov sGvoc; lSloc TioLSLxaL. ol 'Apapec;
xriv dpxTjv xoO vuxQTj^epou duo xfjc; Suaecoc; xpaxoOat xoO tiXlou. STieLSr)
5 xouc; ^fjvac; aOxcov duo xfjc; aeXTQvric; veaq cpaveLarjc; xpaxoOaLV, ol xal Std xfjc;
XLVTQGSCoc; xauxTjc; dpiG^oOvxaL. f) Se aeXTQvr) ^exd Suglv fjXLou cpalvexaL ved. ol
MouGOuX^dvoL x/jv dpxTjv xfjc; fj^epac; Tipo xoO dvaxelXaL xov yjXlov xpaxoOaL
^£XP^ ^^'^ "^"^^ SuGSCOc; Sloxl xal x/jv vrjaxsLav xouxcov ouxcoc; xsXoOglv. ol
daxpovo^oL x/jv dpxTjv xoO vuxQTj^epou duo xoO ^eaou xfjc; fj^epac; xpaxoOaL
10 Sloxl | xal ol (J;fjcpoL xcov daxepcov sic; xo [xeaov exsGrjaav xfjc; fj^epac;. si ydp fssL
xaxd x/jv dpxTQv, STiel f) fj^epa au^SL xal ^SLoOxaL, oOx e\ieXXev ehoLi 6 (J;fjcpoc;
opGoc;. xal fj^epa he e'E, exeivou Xoyl^exaL, dii' dvaxoXfjc; fjXLou ^^XP^ Suaecoc;,
xal vu^ f) ^£xd SuGLV fjXLOu ^^XP^ TidXLV xfjc; xouxou dvaxoXfjc;. xal Tiepl xoO
Xpovou xLc;.
15 Xpovoc; exsLvoc;* f) xoO fjXLOu XLvrjaLc; 8Ld xoO ^cpSLaxoO xuxXou duo xoO
aOxoO ^coSlou xal xfjc; ^olpac; sic; xo aOxo ^6)8lov xal ^otpav duoxaxdaxaaLc;,
xal f) xcov 8 xaLpcov xeXslcoglc;, xal f) xcov x^e fj^epcov xal 8' Tiapd xl nepi-
cpopd. oOxoc; 6 xpovoc; xoO fjXLOu. xfjc; he aeXrivriq oOxoc;* f) ^ear) XLvrjaLc; xoO
I 'H^epa . . . vuxSrj^epov om. L | eoti + vuxSrj^epov L | acpatpa^ + exsLvr]^ sed del.
V II 3 Trjv . . .TOUTOu] ToO vuxSrj^spou oOv TOUTOU Trjv dtpx^^^ L || 4 STiSLSr]] ^La tl otl L
II 5 auTCOv] exsLvcov L | cpaLvo^evr]^ L || 6 f] Se aeXrjvr]] auTr] Se L || 9 dTio + xfj^
dpxf]^ Vv II 12 xal + f] L II 13 Tiepl + Se L || i4 tl^ om. Vv || i7 f]^ om. Vv
II 18 xf]^ aeXrjvr]^ he Vv
372
tiXlou dcpaLpsLxaL | dmb xfjc; ^earjc; xlvtqgscoc; xfjc; aeXTQvric;. el tl xaxaXsLcpGrj, f39vv
al T^ ^oLpaL ^spL^ovxaL sic; sxslvo. el xl e^eXGrj, sxslvo fj^epaL eiai xoO
evoc; ^rivoc; xfjc; aeXrivriq. eiq x/jv auvxa^Lv oOv xauxrjv ecJ^rjcpLaGr) xoOxo xal
sOpeGrjaav fj^epaL xoaat x6 Xa v'' fj^epaL xal Tipcoxa xal Seuxepa XsTixd* xaOxa
5 £xrip7]6riaav sic; xd i^ xal dvecpavrjaav al fj^epaL xfjc; aeXTQvric; xoaat xoO evbq
Xpovou* xv8 xP' P'' fj^epaL xal XsTixd Tipcoxa xal Seuxepa. omb xouxou dvecpdvr)
oxL f) aeXTQvr) Std xcov fj^epcov xouxcov xd i^ SLspx^xaL ^(pSta. exepoL xouc; p
xouxouc; )(p6vouc; svoOglv. xov oOv xpovov sxslvov Std xfjc; xlvtqgscoc; dpLG^oOaL
xoO fjXLOu, xal xov ^fjva Std xfjc; xlvtqgscoc; xfjc; aeXTQvric;, xal xdc; ^eydXac;
10 fj^epac; xal xd Tidaxa xouxcov Std xoO (J;7]cpou xfjc; aeXTQvric; dpLG^oOaLV. sic; y
he xpovouc; | TioXXdxLc; xal Suo, ^eaov xcov Suo fjXLOu xal aeXTQvric; tiXslgxtic; tssvl
ylvexaL eXXslcJ^lc; xal TiXsLovaa^oc;. sic; yoOv ^fiv TipoaxlGsxaL oticoc; jidXtv
e^LacoGcoGLv. sic; xov y^povov exelvov eiq ov oOx eyevexo TiXeovaa^oc; xv8
fj^epaL SLGLV, £Lc; ov he xpovov eyevexo | TiXeovaa^oc; xoO ^rivoc;, fj^epaL xoaat f275rv
15 XTlS.
01 'EPpaLOL Se xal 'IvSol xoOxov xov xpovov xpaxoOatv. ol ^ev 'EPpatoL
x/jv dpxTjv xoO xp^vou xpaxoOaLV fjVLxa 6 yjXloc; yevrixaL xaxd auvoSov xfj
aeXTQVT] £Lc; xov Zuyov, duo xcov x8 xoO 'Ati ^^xP^ ^^'^ "^^^ ^^ "^^^ AlXouX, ol
3 oOv] 5e: V, om. v || 4 a XsTixa L | [J L || 5 xal dvecpavrjaav ] 6^ av dvacpavcoatv
L 5-6 xf]^ . . -xpovou] ToO evo^ XP^^^^ ^"H^ aeXrjvr]^ eupsGr] xoaov L | xoaaL + al V || 6
x^ ] L^ Vv I a' L I p Lv II 7 ^LS^epxexaL v || 8 f]vcoaav L || ii 5uo^ ] p LV
I 5uo^] p Lv II 13 XP^^^^ + 5e: V II 16-17 ePpaloL^. . .xpaxoOaLV om. Vv || is C^yov
+ xpaxoOaL Trjv dpxir]v toO xpovou Vv
373
he 'IvSol fivLxa auvoSeuar] 6 yjXloc; ttj aeXTQvr] sic; xov Kptov.
KecpdXaLov P'. Ilepl xoO exouc;, xoO ^rivoc; xal xoO xp^vou, xl slglv, tioGsv
syvciaGriaav xal Sloc xl eyevovxo.
01 dpxocLOL £X£LVOL dcGxpovo^oL STisl slSov oxL f) asXT^vT) au^SL xal ^SLoOxaL,
5 xov (J;fjcpov xcov ^rivcov xal xouc; xpovouc; olko xouxou eyvcoaav, oxl ol xeaaapec;
oOxoL xatpol del Tipoc; eauxouc; STiavaxuxXoOvxaL dcp' d)v xaxeXTQcpGr) 6 y^povoq
£XL x£ xal duo xfjc; TioLoxrjxoc; xal ^exapoXfjc; aOxcov — xfjc; Gep^oxrixoc; Tipoc; x/jv
(J;uxp6xrixa, xal dvajiaXtv xfjc; xaxd xov aOxov xal eva xatpov fjyouv xp^vov
au^PaLvouarjc;. T^pouXT^Grjaav oOv lSslv xaxd tiolov xatpov ylvexat xoOxo. sksi
10 oOv al ^syLGxaL xcov fj^epcov | xal al Tipd^SLc; TidaaL | sic; xouc; xatpouc; ylvovxat, f84rL, f40rv
Std xoOxo exsGr) nap' aOxcov xo exoc; xal xpaxsLxaL.
Xpecbv oOv SLTiSLv xal xl sgxlv exoc;. exoc; xoOxo dcp' oO ol XP^^^^
dpiG^oOvxaL, OXL xrjVLxaOxa ^syLaxov epyov eyevexo olko xcov xoO oOpavoO
y] xfjc; yfjc;, olov e^cpdvsLa TipocpiQxou y] eOxu^La xlvoc; y] djiciXsLa xoa^ou y]
15 XLvrjaLc; yfjc; xal xaxanovxLa^oc; y] exXslcJ^lc; fjXLOu xal aeXTQvric; xeXela y] exepa
o^oLa xouxoLc; d ylvovxaL xpovcov tiXslgxcov TiapcpxTjXoxcov.
I auvoSeuar]] yevcovxaL xaxa auvoSov L || 2 -3 toO-*- . . . eyevovTO ] sxslvou otl tl eaxL to
STOc; xal Sta tl eyevsTO xal tioGsv syvcoaGr] 6 ^ttjv xal 6 xpovoc; L || 5 eyvcov Vv | 5 L
II rauTCOv + diio L || 8 xal eva in marg. v || 9 toOto om. L || lo {liyioTOi codd.
II 11 STsGr] in marg. L || i5 TsXela om. Vv
374
Ola oOv eoTi yeved, to stoc; TauTTjc; lSloc, xal 6 xpovoc; (baauxcoc;. ol xpovoL
TOLVUV £X£LVOL [XeTOL TCOV 8TC0V SXSLVCOV SLGL aUVTiy^SVOL SlOC TTIV XaTdXTjCj^LV TOO
TOTS xatpoO, (be; prjOTQaexaL. lSloc oOv exsGriaav xaOxa.
Ilepl xfjc; xaxaXiQcJ^ecoc; xcov excov xcov yevo^evcov StqXcov xal xaxd xov
5 fj^exepov xatpov. ^ he eiaiv. ev sxslvcov x6 xcov Apdpcov. f) dpxT) Se xoO
exouc; xouxou duo xfjc; dp^fjc; xoO xpovou exelvou expaxT^Gr) fivlxa 6 Mcod^sG
duo xoO Maxxd diifjXGev sic; x/jv MaStvalav, xal ol xpovoL xfjc; aeXTQvric; ^exd
xoO exouc; xouxou eSea^euGriaav, xal ol ^fjvec; oOxol olko xfjc; aeXrivriq veaq
cpaveLarjc; dpiG^oOvxaL xal Tidvxec; ol MouaouX^dvoL xcp (j>W9 "^^S^ XP^^"^^^-
10 xal f) dpxT) xoO exouc; xouxou fj^epa f)v c;'. al fj^epaL he xal ol ^fjvec; xoO
exouc; xouxou oOx s^LaoOvxaL. xal tj^slc; Se | x^P^v eOxoXlac; xoOxov xov f84vL
^fjva ^£xd xoO [xeaoxj (J;7]cpou xpaxoO^ev, xcov X SrjXovoxL xal xcov x6 ^^XP^
xeXsLciaecoc; xoO xp^vou. Std xl; Sloxl xo xe^^dx^ov xfjc; fj^epac; tiXsov xoO
^eaou xfjc; fj^epac; ov, ^la fj^epa xpaxelxaL. Std xl oOv eyevexo ouxcoc;; Sloxl
15 f) XLvrjaLc; xcov daxepcov ev xfj pipXcp xauxr] sic; xo exoc; xoOxo exsGr). edv ydp
al fj^epaL xcov ^rivcov oOx f)aav SfjXaL, 6 (J;fjcpoc; xcov daxepcov ticoc; dv e\ieXXe
5 exsLvcov + TO £TO^ L, exsLvo Vv II 6 6 + daepr]^ Vv | ^cod^eS L || 8 -9 cpavsLar]^
vea^ aeXrjvr]^ L || 9 Tidvxe^ + Se L || lo dpxir] + Se L || 12 tcov^ om. L || 13 XP^^^^
sed linea strictum, toO sup. lin. v | xfj^ + ^Ld^ L || 14 ^eaou in marg. L
375
XeveoQoLi; \ xal xa stt) he xaOxa e'E, sxslvcov ticoc; e^eXXov sxpXrjGfjvaL; sic; xriv f275vv
auvxa^LV xauxrjv xa ovo^axa xcov ^rivcov sic; xoOxo x6 exoc; sic; xa xavovta
exsGrjaav ouxcoc;, oxl al fj^epaL | xcov ^rivcov sxslvcov slglv sxsl xal fivco^evaL f 40vv
xal SLaxex^P^^t^^^o^L-
5 Aeuxepov exoc; duo xcov excov sxslvcov, x6 xoO McoxaSlx.
01 xp^voL £X£Lvou xoO sxouc; ol xpovoL xcov 'Pco^alcov. xal ol ^fjvec; ^exd
xoO (J^TQcpou xal xcov ovo^dxcov xcov Hepacov. xal f) dpxT) xoO exouc; xouxou f)
La' xoO A^updv. xal al xXoTiL^ataL e fj^epaL sic; x6 xeXoc; xoO 'Aiidv [xrivbq
xlGevxaL. Std xl; oxl xal ol dp^atoL sxslvol ol Xaxpeuovxec; xcp Tiupl ouxcoc;
10 sGrixav xauxac;.
Tplxov. To exoc; xcov 'Pco^alcov.
01 xp^voL xouxou ol xp^voL xoO fiXlou SLGLV. xal ol ^fjvec; xouxou | ^exd fssr l
SupLxfjc; StaXexxou. f) dpxT) Se xoO exouc; xouxou fj^epa P'. xal exaaxoc;
Xpovoc; xouxcov, fj^epaL x^e 8'. xo 8' oOv sxslvo fivlxa yevrixaL tiXsov xoO
15 ^eaou xfjc; fj^epac;, ^la fj^epa xpaxelxaL. exsLvr) 88 f) TiepLxxr) fj^epa sic; xo
1 £xpXir]6f]vaL + izepi tcov (|>ir]cpcov Se toutcov. tico^ eyevsTO e^ sxslvou pir]6ir]a£TaL otl xf]^
aeXrjvr]^ vea^ cpavsLar]^ 6 (J^ficpo^ TauTr]^ tico^ ocpsLXsL xpaTir]6f]vaL; L || 5 Seuxepov sto^]
STspov L I exsLvcov + p sto^ L || 6 XP^^^^ + ^Sv L || i4 TiXeov YevrjiaL v
376
TsXoc; TipoaTLGsxaL xoO Su^Tiax ^rivoc;. xal 6 xp^voc; sxslvoc; fj^epaL xoaaL*
x^c; . dcTio xcov y^povcdv oOv xoO tiXlou xcov (be; Gs^sXlov xpaxou^evcov xaxa
pL xp^vouc; ^La fj^epa TiepLxxeusL. exsGrjaav oOv xa ovo^axa xal al fj^epaL
xcov ^rivcov £Lc; 8uo xotiouc; TiXrjaLov xcov ^rivcov sxslvcov xal fivco^evaL xal
5 8Lr]pri^£vaL. XP^^^^ xolvuv yevo^evrjc;, £X£l6£v ^rixoOvxaL xal ol ^fjvec; xal al
fj^epaL.
Texapxov. To exoc; xcov Hepacov.
ToOxo exsGr) sic; x/jv fj^epav xoO 'laaSaxepSr) Saptdp. f) dpxiQ '^c)^ exouc;
£X£Lvou fj^epa y - "^^ S'^<^^ S^ xoOxo xaxd p xpoTiouc; exsGr). sic; exelvoq Std
10 x6 ae^oLc, sxslvcov, OTiep eaxl TiaaLxd. xal xa6' exaaxov xp^vov x^e fj^epac;
xpaxoOaLV oOxol del, xal xa6' exaaxov ^fjva fj^epac; X. al xXoTiL^ataL he
e fj^epaL sic; x6 xeXoc; xoO Ajidv xlGevxaL. xd ovo^axa he xcov ^rivcov xal
xcov fj^epcov xoO enouq exeivou exsGrjaav sic; x6 xavovLov. xal x6 exepov Se
enoq eneQri hia xdc; epyaalac; xcov 8 xatpcov xal xfjc; dpxfjc; xcov spyaaLCOv,
15 OTiep XeyexaL xaiiLad. x6 exoc; xoOxo | sic; TioXXd xLva xlGsxaL. ev exelvo' fssvL
oxL exaaxoc; \iy]v X e^^^ fj^epac;, xal exdaxr) fj^epa ISlov ex^^ ovo^a. xal al
xXoTiL^ataL e fj^epaL sic; x6 xeXoc; | xoO xp^vou xlGevxaL. Seuxepov Se xoOxo* f4ir v
OXL del f) fj^epa xfjc; eiaeXeuaecdq xoO fiXlou sic; xov Kptov, fjyouv f) vea duo
3 ^La] a L II 4 p LV II 17 he om. L || is f]^ sup. lin. v
377
Tcov fj^epcov, eoTi xoO exouc; toutou xfjc; ocpx'^^ "^^^Ci 3>apPa(p)8Lv ^rivoc;. to
xpLTOv OTL oxav ysvTiTaL 6 xp^voc; xaiiLad, ^La fj^epa sic; to tsXoc; exeivou
(oO) TipoaTLGsxaL. sic; xouc; px he xpovouc; xcov fj^epcov toutcov auvriy^evcov
sic; [xriv yLvexaL Kspiaaoq. hia tl; otl f) Kepiaaeioi xoO xp^vou xoO tiXlou slc;
5 Tov xpovov xfjc; aeXTQvric; | xaxa xoOxov xov xatpov eyyuc; xcov X fj^epcov sgxlv. f276rv
01 ^fjvec; oOv xoO exouc; xouxou sic; Suo hvripeQriaoLv x^P^-v epyaatac;. ev
£X£Lvo* oxL ol ^fjvsc; xouxou s^LGoOvxaL [xeTOL xcov 8 xatpcov. xal f) apxiQ '^c)^
Xpovou £X£Lvou 6 3>apPa(p)8Lv, xal sic; xo xeXoc; xouxou 6 'lacpavxapS^dS. xal
al xXoTiL^ataL e fj^epaL sic; xo xeXoc; xoO 'lacpavxapS^dS xlGevxaL. (baauxcoc;
10 xal al fj^epaL al ^eydXat xcov eopxcov xal al SfjXat sic; xouxouc; xoOc; ^fjvac;
xoO xaTiLad. xo Seuxepov oxl ol ^fjvec; xaxd xouc; 8 xatpouc; sic; eva xotiov oO
xlGsvxaL. xal sic; xouc; px[8] XP^^^^^ ^l^ t^iQ^ ^'^^ "^^^ xotiov xoO Tipcixou ^rivoc;
xlGsxaL. f) xd^Lc; Se xouxou ouxcoc; eaxlv oxl oloc; ^riv xaxd x/jv dpxTjv xoO
eapoc; TidXtv uaxepov xoO x^^t^^voc; TipoaxlGsxaL xal xaxd ^ Y'\ Y xp6^<^^^
15 Tipcoxoc; \iy]v 6 3>apPap8lv TidXtv sic; xov ISlov xotiov sOplaxexaL. xal f) dpxT) xfjc;
TipcixTjc; fj^epac; xoO 3>apPap8lv f) slaeXeuaLc; xoO fiXlou sic; xov Kptov fjyouv
ouxco ylvexaL.
'ExsLvoc; xoLvuv 6 dvGpcoTioc;, oq neQeixe xoOxo xo exoc;, ouxco cprjaLv
O f86r L
3 ou] M Ar. II 4 TiepLTTO^ L I hioTi L II 6 p L II 8 XPOVOU ] ^rjvo^ LVv,iLSJI Ar.
II 11 p L II 12 a L II 15 cpapPaSlv L || i6 cpapPaSlv L | cpapPapSlv + nakiv elc,
TOV ISlov totiov ebpiaxETai sed cancell v | f] om. L || is to sto^ toOto L
378
OTL xaxa xriv apx^Q^ "^^^ Tipcixcov dvGpciTicov sxslvcov fivLxa eyevexo 6
xaxaxXua^oc;, xal ol 8uo ^fjvec; xoO 3>apPap8Lv 6 sic; exelvoc, 6 sic; xov
ISlov xoTiov laxd^evoc;, xal 6 enepoq 6 duo xotiou slc; xotiov xlvou^svoc; xax'
evavxLov. xal xaxd x/jv fj^epav xfjc; dp^fjc; xoO ^rivoc; exsLvou 6 yjXloc; eiq
5 x/jv dpxTjv f)v xoO KpLoO. xal dii' exsLvou he xoO xatpoO ^^XP^ "^"^^ ^PX'H^
xoO exouc; xcov Hepacov xogol TiapfjXGov xP^vol* iTr"\. sic; xov xp^vov Se f4ivv
xfjc; paaLXelac; xcov Hepacov xaxd xov ASSep ^fjva 6 yjXloc; slc; xov Kptov
elaTQpxsTO. xal sxslvoc; 6 ASSep [xriv xax' evavxlov f)v xoO 3>apPap8lv xoO
laxa^evou. xal al e fj^epaL al xXoTiL^ataL sic; xo xeXoc; xoO Aiidv ^rivoc;
10 xlGevxaL xax' evavxlov xoO 'lacpavxapS^dS xoO laxa^evou. xal xaxd x/jv
dpxTjv xoO exouc; xoO 'laaSaxepSr) 6 Nxd'i \iy]v xax' evavxlov f)v xfjc; dpxfjc;
xoO laxa^evou 3>apPap8LV. oOxoc; he 6 ^fiv XeyexaL Tiapa^oviQ.
Xpecov oOv slSevaL xoOxov xov ^fjva ^exd xoO (J;7]cpou. xpaxoOvxat ol
xexeXsLCO^evoL | xpovoL xoO exouc; xoO 'laaSaxepSr), xal evoOvxat xouxolc; del fsevL
15 pxy P'' . el XL eOpsGfj, SLTiXaaLd^exaL. xal aOGic; el xl eOpsGfj, ^spl^exaL sic;
xd G[iB. el XL e^eXGr], ^fjvec; slgl xoO xaiiLad. sxslvo xaxaXL^TidvexaL duo
xoO ASSep ^rivoc;. £v6a oOv xaxaXiQ^SL 6 (J;fjcpoc;, xal al e xXoTiL^ataL fj^epaL
TipoaxlGevxaL xcp xsXsl xoO ^rivoc; xouxou. STiSLxa xrjpeLxaL oloc; ^tqv sgxl Tipo
£X£Lvou. exsLvoc; diiep s^LaoOxaL xouxcp, oOxoc; ^fiv XeyexaL xfjc; Tiapa^ovfjc;.
2 cpapPa^LV L | b^ om. L || 3 6^ om. v || 4 evavTLOv + f]aav L || 7 toO paatXecoc;
Vv II 8 cpapPaSlv L || ii laahaxip^ Vv || 12 cpapPa^LV L || 17 ahtp Vv
379
oOtoc; oOv 6 prjGelc; (J;fjcpoc; xaxa to tsXoc; f)v xfjc; xcov Hepacov sOtuxlocc;. tcov
Apdpcov Se UTiepLax^advTCOv toutcov xaxeXeLcpGr) f) xd^Lc; toutou, xal al xXoti-
L^ataL he kevts fj^epaL xaTsXeLcpGrjaav sic; to tsXoc; toO Ajidv ^rivoc; ^^XP^ "^^^
Xpovou £X£Lvou Tcov Hspacov ToO rvS OLKO ToO STOuc; ToO 'laaSaxepSr). exsLvr) f276vv
5 oOv f) TiepLcpopd eneXeio^Qri TrivLxaOxa, tots xal 6 yjXloc; slc; xriv dpxTjv eyeveno
ToO KpLoO xaxd xriv dpxTjv xoO 3>apPa(p)8LV ovxoc; xouxou xax' evavxLov xoO
laxa^evou ^rivoc;. exsLvac; oOv xdc; £ xXoTiL^atac; fj^epac; xlvsc; xcov Hepacov sic;
xo xeXoc; xoO 'lacpavxapS^dS xsGsLxaaLV. dXXoL he xauxac; sic; xo xeXoc; xoO
Ajidv xaxeXsLcJ^av. Std xl; Sloxl ol Xaxpeuovxec; xcp Tiupl TipoaeSoxriaav (be;,
10 dXXcoc; I yevo^evou | xal xcov fj^epcov ^sxaxeGsLacov, xo aepac; sxslvcov ^sXXsl f42rv, fsrrL
xaxaaxpacpfjvaL, OTiep oOx f)v Tipoc; dXT^GsLav.
'fie; yoOv dvexsLXev 6 yjXloc; slc; xo cp' exoc; xcov Hepacov, 6 yjXloc; f)v sic;
x/jv dpxTjv xoO KpLoO, £Lc; xo ^fjxoc; xcov 9, xaxd x/jv dpxTjv xoO 'ApSe^Tieeax
^rivoc; xoO ^r) laxa^evou. xal sxsLvaL al e al xXoTiL^alaL fj^epaL xaxd xo
15 xeXoc; xoO ^r) laxa^evou 3>apPap8lv exsGrjaav oxl e^LaciGrjaav 6 Tipcoxoc; xal
[XT] laxd^evoc; [xriv 6 ApSe^Tieeax ^exd xfjc; TipcixTjc; xoO laxa^evou 3>apPap8lv
[xrivoq. xaxd Tidvxa he xpovov, oc; eam Tiapd xcov xsGsvxcov xp^vcov sic; xoSe
1 oOv om. L I xf]^ £UTUXLO(^ f]v tcov Tiepacov L || 3 e L | to] toO V 3-4 sxslvou
ToO xpovou V II 4 r£Y L | laahaxip^ LVv || 5 STeXsLCoGr] ] £TiXir]pco6ir] L || 9 hioTi]
hi exsLvo OTL L I 6c;] otl L || 11 Tipoc;] slc; L || 12 -13 slc; Trjv otpx^^^ "^^^ v || 14 ^r]
om. Vv I al^ om. L || 15 paSlv L, cpap sup. lin. L^ | a L || 16 a L | cpapPaSlv
L, cpap^aSlv v || 17 Tiapa] Tipo L
380
TO xavovLov, exsLvoc; 6 xpovoc; eaxl xoO xaiiLaa ^rivoc; Ly', xal 6 3>apPa(p)8Lv
\iy]v sic, Tov xpovov sxslvov P' au^paLvsL, 6 sic; sic; xriv apx^Q^ "^^^O X9^^^^^
I xal 6 STspoc; sic; to tsXoc;. eiq exeivov oOv tov uaTspov 3>apPa(p)8Lv oO f277rv
TiGevTaL al SfjXat xal ^syLOTaL fj^epaL tcov eopTCOv. exelvoq 6 y^povoq TY S
5 fj^epaL SGTLV. OTav oOv e^LaciGrjaav | f) apx^Q '^c)^ [xt] laTa^evou ApSe^TieeaT f42v v
xal f) apxTQ '^c)^ laTa^evou 3>apPa(p)8lv, fj^epa fepSo^r) f)v lP' toO ^rivoc; toO
'Pa^TiLaXax^Lp, XP^^^^ Apdpcov SYS. xaT' exsLvriv t/jv fj^epav 6 yjXloc; slc; t/jv
dpxTjv ToO KpLoO. OLKO ToO STOuc; oOv ToO xaTaxXua^oO ^^XP^ tots TiapfjXGov
XpovoL i''Ar"\. xal ^£XP^ "^^^ ^"^^^^ "^^^ 'laaSaxepSr) xpovoL ToaoL'Soo. xal fssrL
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(J^eOSoc; 8l' exelvo otl f) euTUxia sxslvcov ^eTSTpaTir), oOtoc; 6 (J>fjcpoc; xaTsXeLcpGr)
xevoc;.
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Qe\ieXio\j. xal ol xaTaXsLcpGevTSc; ^fjvec; xdxsLvoL STeGrjaav exsL sic; toOto
15 he TO xavovLov xal 8uo stt) STeGrjaav ev stoc; tcov 'Pco^alcov, xal to STspov
Tcov Hepacov. XP^^^^^ dTsXsLc;.
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x/jv eOxoXlav x6 aOGrj^epLvov sic; xoOxo x6 exoc; xlGsxaL. xal f) dpxT) xoO
exouc; xouxou fj^epa ol f)v duo xoO ^rivoc; xoO Sa^Tidv XP^^9 ^''"^^ ^^^ "^^^
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5 ^rivcov xouxcov xcov excov xaxd Tiotav fj^epav slaepxovxaL xfjc; fepSo^dSoc; xal
xfjc; expoXfjc; xoO evoc; exouc; olko xoO exepou ^exd xoO (J;7]cpou. xoOxo oOv sic;
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fj^epav SLGspxovxaL xfjc; fepSo^dSoc; ^exd xoO (J;7]cpou.
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elxa xax' evavxlov xcov xexeXsLCO^evcov sxslvcov ^rivcov xpaxoOvxat al auv-
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'H y'. f) £Lc; Tov gxotslvov xdcpov elaeXeuaLc; xoO aae^ouq ev xfj olxloc xfjc;
5 aOxoO ya^rixfjc;.
'H y] . f) £Lc; x/jv MaStvatav dcpt^Lc; xoO daepoOc;.
'H l' xa6' y]v e^Lyr) xrj xupta aOxoO xrj Xa8[8]Lx^a.
'H lP'. f) yevvrjaLc; xoO daepoOc;.
'H l8'. 6 Gdvaxoc; xoO 'la^Lx.
10 'Pa^TiLaXdx^Lp
'H y'. (fj) xaxdxauGLc; Tiapd xoO Avx^dx xoO Maxxd.
'H l8'. f) Kpoaew/j] xcov djiep^o^evcov dc; xLva xotiov y] ^evovxcov oIxol.
Nxa^^dx ouXe
'H T)'. f) yevvrjaLc; xoO 'AXfj xoO A^TiLxaXfj.
15 'H IS . 6 Std xa^T^Xcov tioXs^oc;.
Nx^a^dv dXdx^ip
'H Y ' 6 Qdvaxoc; xfjc; Guyaxpoc; xoO daepoOc; xfjc; 3>ax^dc;.
3 euaepoO^ sup. daepoO^ L^ || 4 f]^ sup. lin. v | axoxsLvov om. Vv | cpcoTauye:^
sup. axoTSLVov L^ | euaepoO^ sup. daepoO^ L^ || 5 \iaxapiac, au^pLir]^ sup. ya^rjif]^ L^
II 6 euaepoO^ sup. daepoO^ L^ || 7 xo^'^^^^ot L || 8 euaepoO^ sup. daepoO^ L^ || 9
LaCir]T Vv II 11 xaxdxauaLc;] e^Tiprja^oc; Vv || 12 diiepxo^evcov + f] SLaepxo^evcov Vv
I TLva om. Vv | f] ^svovtcov oIxol om. Vv || 16 dXXdxetp L || 17 euaepoO^ sup.
daepoO^ L
408
'H 6'. 6 Gdvaxoc; xoO 'A^TiouTidxr).
'H IS . f) xaxapoXr) xfjc; Tipoaeuxfjc; aOxcov Tiapd xoO uloO xoO ZouTidxr).
'Pavx^dTi
'H a . f) xoO daepoOc; xaxaTioXe^rjaLc; xoO Mapxou^.
5 I 'H 8' xa6' y]v 6 AXfjc; xal 6 Aptd auvfj(J>av dXXiQXoLc; tioXs^ov slc; x6 SLcpiQ. f98rL
I 'H xc;'. f) xoO daepoOc; Ssl^lc; Tipoc; xouc; daepsLc; oxl TipocpTQxric; sgxlv. f48vv
'H xC- TQ vu^ xa6' y]v STiopeuGr) 6 daeprjc; sic; x6 ^aayfjSLv X^P^t^^ ^^'^ ^^^
xouxou (be; aOxol cpXuapoOaLV dvfjXGsv sic; xov oOpavov. xal f) dXT^GsLa oxl eiq
xov olxov xoO Tiaxpoc; aOxoO xoO StapoXou STiopeuGr).
10 SaTidv
'H y'. f) yevvrjaLc; Xoadriv xoO uloO xoO AXfj.
'H £ . f) yevvrjaLc; xoO Xaadv xoO uloO xoO AXfj.
'H Ly' , f] l8' ,7) L£ . al Xeuxal fj^epaL.
Tfjc; L£ f) vu^ f) ^Lapd xouxcov TipoaeuxT) f] Xeyo^evr) TiapdxLv, xal xaxd x/jv
15 aOxriv f) Tipoc; x6 Maxxd STiavaaxpocpr) xfjc; ^tapdc; Tipoaeuxfjc; aOxcov.
'Pa^aSdv
'H a', f) xaxdpaaLc; (be; aOxol cpXuapoOaL xfjc; xoO Appad^ PlPXou oOpavoGsv.
'H q . f) M(oua£oc; PlPXou xaxdpaatc; oOpavoGsv.
4 daepoO^ L, corr. in euaepoO^ L^ || 6 daepoO^ L, corr. in euaepoO^ L^ | otl Tipocprjir]^
sail Tipo^ Tou^ daepsL^ L || 7 xC- i^ vu^] vu^ tcov xC L || 8 xal] xdv v || i4 Tfj^ le
f] vu^] f] vu^ Tcov IE L 14-15 xaxd Trjv auTrjv om. Vv || i5 ^axxd^ L
409
'H l'. 6 Gdvaxoc; xfjc; XaSivx^a, yuvaLXoc; xoO daepoOc;.
'H i^\ f) Tipoc; xov AaulS xaxdpaaLc; xfjc; ^i^Xou oOpavoGsv.
'H lC- 6 TioXe^oc; xoO MiidxpL hia xcov l xoO aae^ouq xpoTicoaa^evou x^XtdSac;
5 'H IT] . f) xoO EOayyeXLOu (be; cpXuapoOaL xaxdpaatc;.
'H l6'. diioxaxdaxaaLc; xoO Maxxd.
'H xa . 6 Gdvaxoc; xoO AXfj xoO uloO xoO MouxaXfj, xal 6 Gdvaxoc; xoO
AXtpriSd, uloO aOxoO.
'H x^\ f) yevvrjaLc; xoO AXfj.
10 I'H x8'. f) xoO KoupavLou (be; cpXuapoOaL xaxdpaatc; Tipoc; xov daepfj. xpsLxxov f98vL
8' SLTiSLV f) duo xoO Tiaxpoc; aOxoO xoO StapoXou dvoSoc; xouxou Tipoc; aOxov.
'H xc;'. f) sxPoXt) xoO nepxouL
'H xC- TQ vu^ exsLVT) f) TipoaxuvrjaLc; x(ov SevSpcov.
SaoudX
15 I'H a . x6 Tidaxoc xfjc; ^Lapdc; vrjaxsLac; aOx(ov. 28ivv
'H P'. f) a x(ov c; fj^epoiv xfjc; ^tapdc; jipoaeuxfjc; aOx(ov.
'H 8'. f) StdXe^Lc; xoO aae^ouq [xstol x(ov XptaxLavoiv.
'H lC- 6 TioXe^oc; xoO Xoux, xal f) cpoveuaLc; xoO Gslou xoO daepoOc;.
10 -11 xpsLTTOV . . .auTOv] 6 Tiapa toO Tiaxpoc; auxoO toO ^LapoXou £Ti£xopir]Yir]6ir] auxcp Vv
11 12 TiepxoL L II 13 vu^. . .TipoaxuvrjaL^] TipoaxuvrjaL^ Sta xfj^ vuxto^ Vv || 15 Tidaxot
+ xf]^ dvoL^eco^ L || le a ] TipcoTr] Vv | fj^epcov om. Vv
410
'H x^\ f) ToO 'Icova Tiapa xoO xtqtouc; xaxaPpoxQiaLc;.
AouXxdx
'H l8'. (fj) sxPoXt) toO 'Icova duo xoO xtqtouc;.
'H L£ . f) xaxdpaaLc; xoO Kaiia oOpavoGsv (be; aOxol cpXuapoOaLV, xal f)
5 GuyxcipTiaLc; xoO 'A8d^.
'H x6'. f) I dvapXaaxTjaLc; xfjc; xoXoxuvrjc; 'Icovd. f49rv
AouXx^vx^a
'Ha. f) xfjc; 3>ax^dc; Soglc; Tipoc; xov AXfj. Tipo xouxou (xoO) \n]\b^ l
fj^epaL XeyovxaL xoO yvcopLa^axoc;. sic; xauxac; xdc; fj^epac; f) ^Lapd TipoaeuxT)
10 aOxcov, dXXd f\ dmb xcov l tj' dvdxpa^Lc; ^syLaxr) xfjc; ^Lapdc; jipoaeuxfjc; aOxcov.
'H 6'. f) fj^epa fjVLxa yu^voOvxat xal TipoaeuxovxaL StovuGLaxcoc;.
'H l'. f) KOLC/^oiXioi xouxcov, YJxLc; XeyexaL TipoacpayiQ.
'H La', f) fj^epa xfjc; dpiiayfjc;.
'H i^\ f) cpuyf) Tidvxcov duo xfjc; jipoaeuxfjc; aOxcov.
15 I 'H Ly'. f) xaGsSpa fj^epac; y. f99rL
'H lC- acpayf) xcov guvtqGcov xoO daepoOc; xoO Ax^dv.
'H x£ . acpayf) xoO A^dpr) Xaxdii.
'H xC- TQ sic, xfjv MaStvatav TiXsLaxr) Gep^iQ, xal olko xouxou xcov tioXXcov
3 lS'. ] S'. L II 7 5oXx£vtCo( Vv II 8 Sexa L | ^rjvo^] fj^epa^ codd. || lo t] om.
Vv II 11 Tipoaeux^VTaL V || 12 Tipoacpayr] ] Tipopdxcov acpayr] v || 13 if om. L || 16
auvrjGcov] auvxpocpcov L || 17 ^dpr] L, corr. L^
411
GvfJGLc;.
AioLipeaic, z . HaaxocXLaL xcov Hepacov xal al ^eydXat fj^epaL sxslvcov ot
dpLG^oOaL TipcoTOV xal xdc; fj^epac;, elxa xdc; vuxxac;.
3>apap8Lv
5 'H a . fj^epa f) vea.
'H i , f) vea fj^epa xoO MsXl^S.
'H lC- Soupcoc;.
'H l6'. 3>apPavxLvdv, f) KOLc/^oiXioi sxslvcov.
ApSe^Tieeax
10 'H y'. ApSe^TiLaxdv, TiaaxocXLa sxslvcov.
'H c;'. f) a Xapx^dv Aaouxx.
'H xc;'. f) a Kouou^Tidc;- fj^epaL e.
Xopvxdx
'H q . f) KOLC/^oiXioi xoO Xopvxaxdv. f) a Nataavx^ Souxx.
15 ('H) xc;'. f) a Kou^dx.
Tip
'H c;'. Nx^davL VLXoucpdp.
2 Tie^TiTiT] V I [lEYCikai] [lEYiGTOi L I ot] oItlvsc; L || 3 a L | elxa] xal STieLxa
L II 4 cpapPa^LV L || 5 f]^ om. L || 6 (;. + fj^epa L || 7 EoOp 63^ codd. || 9
dpSe^TiesTC L || lo dpSee^TiLa^av v || ii daouxY(?) L || i4 vatadv T^aouxT Vv,
vaLaavT^aouxT L || i7 vxCaavLVLXoucpd v
412
'H Ly'. TiaaxocXLa xoO Ttpyav Mtxpa.
('H) vf] . TiaaxocXLa xoO Ttpyav MeydXr).
MoupvTdx
'H q . Euvax^VT Souxx.
5 'H C- TiaaxocXta MoupvTaxxdv.
Sapepdp
'H 8'. TiaaxocXLa xcov SaxpipSv xal 'Eaxta xdvL.
'H c;'. Mlx^lxocv Souxx.
'H Lc;'. f) a xoO cpGLvoTicipou. exsLvr) f) fj^epa olko xcov £ Kou^Tidx, at eiai e.
10 M^eep
'H a cpGLvoTicipou Seuxepa.
'H c;'. Bayxdv Souxx.
'H Lc;'. M^eepxdv KOLc/^oiXioi.
('H) xa . M^eepxdv ^eydXr).
15 Ajidv
'H c;'. Ajiavx^ou Souxx.
'H l'. Tidaxoc xoO Ajiavxav.
3 ^oupidT L II 4 auvaxSevT Vv || 5 ^oupxax xav L || 7 eaxLa V, corr. in laxta
V, laxLa L, elaxLa v || 8 [iut^ixolv Vv || 9 a om. Vv | xou^TiaC L | at SLat] xal
sxsLvaL fj^epaL L || lo ^^X^P L || n ^ L || 12 payxaaouxx V, paaxouaouxx v
II 16 dTidv VT^ou aouxT L, diidv T^ouaouxT Vv
413
I ('H) Xa . f) a — al xXoiii[icdoii s fj^epaL aOxat. Kou^Tiax XeyexaL exxov. f99vL
xal eiq xouc; laxa^evouc; ^fjvac; al e fj^epaL sic; x6 uaxepov xoO Scpavxap 8^d8
I SLGLV. f49vV
5 'A8dp
'H a . f) xapaXXtxeuGLc; xoO IlavoO. HaxocpxeS XeyexaL fjyouv 6 BepaLXTjc;.
'H 6'. 'A8dp x^davL.
NxdL
'H a . Xopo^ 'Poc;.
10 'H y] . Tidaxoc sxslvcov.
'H lOL . f) TipcixT) xoO Kou^Tidx xal f) xcov l£ vu^ Tidaxa xoO KaxexeX.
('H) xy'. TiaaxaXLa.
Ilax^dv
I 'H a'. Zari^avxav(d)x^ Souxx. 282rv
15 ('H) P'. Ilax^dv x^Lvd TiaaxaXLa.
'lacpavxdp 8^d8
'H a'. AoudX Xouaou^ou Souxx.
'H £ . TiaaxaXLa 'lacpavxdp 8^d8 xdv.
1 f]^ om. L II 2 aou^Tiax codd. || 6 xapaXtxeuat^ L. | Tiax^pxey Vv || 7 T^aovi]
VT^avL L. II 9 To^] Tipo^ codd. || ii TipcoTir]] a L | ^axeXex L, xaxeXex Vv || is
^Tiax^av Vv II 14 CotTTj^av xaxxC codd. || i5 ^Tiax^otv Vv | vx^Lva Vv
414
'H La . f) a Kou^Tidc; P'. fj^epaL e.
'H (l)c; \ MouaxouTiaxa fjyouv xatpoc; xoO eapoc;.
('H) xc;'. ZapxapoT sic; to 'l{o)ii(r/by auvaycoyiQ.
AtaLpeaLc; Sxtt). Ta ovo^axa xcov fj^epcov xal xcov ^rivcov xcov Hepacov.
5 'H a xoO ^rivoc;, Xoup^ouC
'H y'. ApSe^Tieeax.
'H 8'. Sapepdp.
'H £ . 'lacpavxdp 8^d8.
10 'H c;'. Xopxdx.
^HC. Mouxdcx.
'H x]. T£^Ti:a8x7]c;.
^HG'. A8dp.
'H l'. Ajidv.
15 'H La . Xodp.
^H Lp'. Mdv.
^H Ly . Tip.
1 fj^epa Vv II 3 LTiaxotv LV, LTiaaxotv v || 4 ^' L || 5 x^^P^^^^^ L || lo )(op^\JTQiT
V, xop^xdx V II 11 -13 'H C . . . 'A5dp om. Vv || i6 ^dp V
415
^H l8'. Koq.
'H Lc;'. M\ieep.
5 'H IT] . 'PdavL.
'H l6'. 3>apPap8Lv.
'H x'. Mjiaxpa^^.
'H xa . 'Pd^.
'H XP'. I Mjldx. flOOrL
10 'H xy'. Ntstitlv.
^HxS'.Ntlv.
'H x£ . 'Apx.
'H xc;'. 'I(a)Td8.
'H xC- Aa^dv.
15 'H XT)'. 'Fa^LdS.
'H x& . M\ieep acpdv.
'HX'. AvLpdv.
Td ovo^axa xcov e fj^epcov xcov xXoTiL^atcov.
1 xoL Vv II 2 Tia^^eaap Vv || 3 \i\iEp Vv || 4 aoOp 63^ L || 6 cpapPa^LV L || 7
^Tiaxpaar] Vv || i7 X' ] S' codd.
416
^Hp'. AavouS.
'H 8'. Kaadx.
'H £ . OOaaaxouc;.
5 AtaLpeaLc; fepSo^r). Elc; xdc; KOLC/^oiXioiq xcov XptaxLavcov, al [xeyoiXoii fj^epaL,
xd ovo^axa xcov ^rivcov.
TaaLpriv doudX
'H 6'. Moupxdx [xriv MaxaStx.
TaaLpriv dXXdx^ip
10 'H y] . Sapepdp ^d MaxaStx.
('H) x^\ TiaaxocXLa xoO Xavaxd.
KavoOv doudX
('Ha) KOLc/^oiXioi xoO Su^ovL
'H y] . M\ieep [xol MaxaStx.
15 (...)
Ouxoc; 6 \iy]v Xe fj^epaL, xal elc; xov xpovov xoO xaiiLad fj^epaL Xc;.
Sou^Tidx
3 yaadx L || 7 xaatplv Vv || 8 Moupxax] v sup. p V, ^oupviax v | \iaTahhu: codd.
II 9 xaaLplv Vv || 14 \iaTahhu: L
417
'H P'. f) UTiaTiavTr).
'H C- TQ o^PX'H "^"^^ ^^^ '^^^ y^^ Gep^Tjc;.
'H La . 'A8ap [xol MaxaSLx. oOxoc; XaXtcpac; f)v xal exsGr) x6 exoc; xouxou sic;
xoOxo.
5 'H l8'. f) dcTio I xfjc; yfjc; Seuxepa Gep^r). fsorv
'H L£ . f) apxTQ "^"H^ pXaaxTjc; xcov cpuxcov.
'H XOL . al y Qep\i(xi al duo xfjc; yfjc;.
'H xq . al TipcoxaL fj^epaL xoO TiaXaLoO (J;uxouc;, fj^epaL C
'A8dp
10 ('H T)') f) xcov x^XlSovcov xal TieXapycov cpavepcoaLc;.
'H Ly'. Nxdl ^d MaxaStx.
Ntaadv
('H) i^\ Ilax^dv [xriv MaxaStx.
('H) x8'. Aou[X]xpdvri \ir]v T^ou(p)x^ac;.
15 ('H) x£ . f) yevvrjaLc; xoO Icova.
'Idp
I 'H i^\ 'lacpavxdp 8^d8 MaxaStx. fioovL
'H Ly'. f) TiXiQ^upa xoO NslXou.
'H vf] . (fj) TiapeXeuGLc; xoO Gepouc; xal xcov dve^cov XLvrjaLc;, fj^epaL ^.
3 ^aMaxa^LT] \iaxaTahhiT L, \iaxaTahu: Yv \\ 7 al^ om. v || is f]^ om. Vv | TiXrj^^upa
codd. II 19 GepTiou^ v
418
'H La . f) a 3>apPap8LV [xol MaxaSLx.
('H) xa . f) yevvrjaLc; xoO HpoSpo^ou.
('H) x8'. Kveuaiq xoO Xtpa.
5 ('H) xC- xeXsLCOGLc; xcov [x fj^epcov.
'H y \ Aouxpdvr) ^dp Tou^d.
'H La . ApSe^Tieeax ^d[L] MaxaStx.
'H l6'. f) a' fj^epa xcov xuavoxau^dxcov, fj^epaL C
'H a', f) vrjaxsLa xfjc; Beoxoxou.
'H q . f) ^exa^opcpcoGLc;.
'H l'. Xopxdx ^d MaxaSLx.
'H L£ . x6 Tidaxa xfjc; Beoxoxou.
15 'H x8'. f) cpoveuGLc; xoO EpoSpo^ou.
AlXouX
'H P' xa6' y]v STiLxeXXsL 6 Alpdx daxiQp.
^H 6'. Tip ^d MaxaSLx.
'H Ly'. f) TiaaxaXLa xfjc; OcJ^ciaecoc; xoO axaupoO.
10
2 TipcoTiT] Vv I cpapPaSlv L || 7 y] Ly' codd. || is x^P^^^^tT Vv || i5 f]^ om. Vv
II 19 ToO + TL^LOU xal Z(x>01lOlO\J Vv
419
I MoLpa SeuTspa. Ilepl xfjc; xaxaXiQcJ^ecoc; xcov (J^rjcpcov, xfjc; TiepLaasLac;, 282vv
xfjc; xpaxTjXaLac;, xoO xo^ou, xfjc; aaytxac; xal xoO axLda^axoc; xaxa tioXu
XuGLxeXouvxcov xouxcov eiq x/jv xfjc; Suvxd^ecoc; ^sxax^LpaLV. auxr) f) ^otpa sic;
xpta StaLpeLxaL x^iQ^axa.
5 T^fj^a a . Ilepl xfjc; opGciaecoc; xoO [xeaou (J;7]cpou xcov p xavovLCOv.
AsL slSevaL oxl olov xal eaxL xavovLov, sxslvoc; 6 xsGelc; (J;fjcpoc; xax' dpx^c;
xcov xavovLCOv olov 6ijpa xlc; sgxlv sic; xov (J;fjcpov sxslvov xoO xavovlou. sxslvoc;
oOv 6 (J;fjcpoc; oloc; xal eam [xeaov xcov | xavovlcov | xal 6 xaxd x/jv dpxiQ^ f^ovv, fioirL
xoO xavovLou, del opGoc; sgxlv slc; x/jv TiepLaasLav, exsLvr) Se f) Kepiaaeioi f)
10 ^eaov xcov Suo xavovlcov Tidaa oOSe au^palvsL opGiQ. edv oOv f) ^eaov xoO
xavovLou auxT) TiepLaasLa eypdcpr) sic; xo xavovLov, xal xd ^cpSta duo xcov dvco
xaxepxovxaL, f) TiepLaasLa xax' evavxlov exsLvou xoO (J;7]cpou xpaxsLxaL. el Se
xd ^(iSta OLKO xcov xdxco dvep^ovxat, f) TiepLaasLa duo xoO P' (J;7]cpou xpaxsLxaL.
£L 8' oOx eypdcpr) f) TiepLaasLa ev xcp xavovlcp, ylvexaL ^TQxriaLc; sic; xov (J;fjcpov
15 £X£Lvov 8l ' oO eyevexo elaeXeuaLc;. 6 (J;fjcpoc; yoOv 6 ^ex' sxslvov xrjpeLxaL xal 6
eXdxxcov dcpatpsLxaL xoO tiXslovoc;. eliiep 6 P' tiXslcov, sxslvoc; 6 (J;fjcpoc; Xeyexat
I -3 xfjc; TiepLaasLac;. . .[lETax^ipoiv] tcov xaxa tioXu XuaLxeXouvTCOv slc; Trjv ^STdxeipaLV xfjc;
auvxd^ecoc; f] xfjc; TiepLaasLac; xfjc; Tpaxir]XaLac; toO to^ou xfjc; aayLxac; xal toO axLda^axoc; L
II 5 TipcoTov V I Tiepl xf]^ opGcoaeco^ ] f] 6p6coaL^ L | (J;ir]cpou post xavovLCOv Vv || 8 oloc,]
OTioLO^ Vv I Tcov + [lEoov Tcov V | 6^ ] OTL Vv || 10 P L | ouSsv codd. II 11 xd
xavovLa v || 13 Seuxepou Vv || 16 Seuxepo^ Vv
420
TiepLGGOc;. si he 6 a tiXslcov, 6 (J;fjcpoc; eveuae Tipoc; dcpaLpsGLv. oOxoc; oOv 6
(J;fjcpoc; Tcov ^eacov xavovLCOv eaxLv, enei 6 xfjc; ocpx'^^ ^^i- Tipoc; iikeov x<^9^^'
'Eksi xps^a yeveaQoii xriv spyaaLav xauxriv, dnep Xsktol oOx sIglv slc;
xov (J;fjcpov xoOxov xov nap' fj^cov xpaxrjGevxa, XP^^^^ ^^^ ^^"^^ "^"H^ xoLauxrjc;
5 spyaaLac;. xax' evavxLov he xoO (J;7]cpou exsLvou, d xl eOpsGrj, xpaxsLxaL. el Se
eiai XenTOL sic, xov (J;fjcpov fj^cov, xax' evavxLov xcov ^otpcov xoO xpaxou^evou
Tiap' fj^cov (J^TQcpou dcTio xfjc; ocpx'^^ "^^^Ci xavovLou ytvexat elaeXeuaLc;, xal duo
xfjc; [xeariq xoO xavovLou xpaxsLxaL 6 eOpsGelc; | (J;fjcpoc; xal xrjpeLxaL. STiSLxa fioivL
f) TiepLaasLa xouxou cpavepoOxaL, xal exsLvr) f) TiepLaasLa sic; xd Xsktol xoO
10 xpaxou^evou nap' fj^cov (J;7]cpou xrjpeLxaL. el xl eOpsGfj, ^spl^exaL sic; x/jv
TiepLaasLav xfjc; dp^fjc; xoO xavovlou. d xl e^eXGr], edv 6 (J;fjcpoc; 6 duo xfjc;
[xeariq xoO xavovLou xoO xpaxrjGsvxoc; xal xrjpriGevxoc; | x^PTl ^P^^ "^^ tiXsov, fsirv
£X£Lvo x6 e^eXGov svoOxaL xouxcp. el Se Tipoc; x6 eXaxxov, dcpaLpsLxaL tva
yevrixaL 6 (J;fjcpoc; sxslvoc; xsXsloc; [xeaov xoO (J;7]cpou xcov p xavovLCOv.
15 ALalpsGLc;
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1 TipCOTO^ Vv II 4 TOUTOV OHl. Vv || 9 £X£LVir] OHl. Vv || 14 TOO ] TCOV V || 17 OtTIO
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5 eaxlv eXdxxcov xal eyyuxepov. eha xax' evavxLov exsLvou xpaxsLxaL 6 (J;fjcpoc; 6
xaxd x/jv dpxTjv xoO xavovLou xal xrjpeLxaL. eneiioL 6 (J;fjcpoc; 6 eOpsGelc; [xeaov
xoO xavovLou dcp' oO xax' evavxlov eyevexo elaeXeuaLc;, duo xoO xpaxou^evou
I Tiap' fj^cov (J^TQcpou dcpaLpsLxaL. d xl oOv xaxaXsLcpGrj, exelvo xrjpeLxaL sic; x/jv fio2rL
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10 x/jv iiepiaaeioLv xfjc; ^earjc; xoO xavovlou. el xl oOv eOpsGfj duo xcov Tipcixcov xal
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xoO xavovLou (be; dv yevrixaL 6 (J;fjcpoc; sxslvoc; 6 xpaxrjGelc; duo xfjc; dp^fjc; xoO
xavovLou xeXsLoc;.
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15 aayLxcov.
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x^ e^epLaav, sic; x6 yeveaQoii exaaxov ^exd xoO dXXou laov, xal xd xe^^d^La
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10 \iEa(x>v L II 11 p L II 14 P L II 16 xuxXo^ post apa L
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d)v exaaxov Seuxepov Xstixov exdXeaav. xal ^exd xfjc; xd^ecoc; xauxrjc; eyevexo
f) SLalpsGLc; xcov xaGs^fjc; Xstixcov ^^xP^ "^^^ ^' Xstixcov.
5 AsL slSevaL oxl f) xpaxTjXaLa Gs^sXlov sgxlv slc; x/jv xaxaXTjcJ^Lv xfjc; xd^ecoc;
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^. olov oOv I xo^ov xal eaxLv, hel eihevoii x/jv xpaxTjXaLav exsLvou. el x6 fio2vL
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10 Se TiXeov xcov 9 xal eXaxxov xcov pii, f) TiepLaasLa xfjc; ^earjc; xoO xo^ou exsLvou
pTi xpaxsLxaL, fjyouv x6 eXaxxov dcpatpsLxaL xoO tiXslovoc;. el xl xaxaXsLcpGfj
£^ £X£Lvou, xax' svavxLov xpaxsLxaL f) xpaxTjXaLa. xal el x6 xo^ov sxslvo
TiXeov eaxl xcov pii ^otpcov, exeivo dcpatpsLxaL olko xcov x^ [xoipcdv. el xl oOv
xaxaXsLcpGfj, xax' evavxlov exeivou xpaxsLxaL f) xpaxTjXaLa.
15 El yevrixaL xp^^a xax' evavxLov xoO xo^ou xpaxrjGfjvaL x/jv aaylxav, edv
x6 xo^ov eXaxxov sgxl xcov pii ^oLpcov, xax' evavxLov exeivou sxpdXXexaL f)
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Vv II 15 edv + oOv L || 19 ^oLpat post elai L
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I AtaLpeaLc;. Ilepl xoO slSevaL x/jv xpaxTjXaLav duo xoO xo^ou, xal x6 to^ov 283vv
dcTio xfjc; xpaxTjXaLac;.
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5 xoO xo^ou £Lc; x6 dxpov xfjc; ocp^fjc; xfjc; xpaxTjXaLac;. xal xax' evavxLov
£X£Lvou dcTio ^SGOU xoO xavovLou f) xpaxTjXaLa | sxpdXXexaL. stisl oOv ^exd f52rv
xoO xo^ou oO dxo^ev f)aav XsTixd, exsLvr) f) xpaxTjXaLa xeXeta ytvexaL | ^exd fiosrL
xfjc; opGciaecoc; xoO ^eaou xcov p xavovLCOv. ouxcoc; (be; eppsGr) sic; x/jv dpxTjv
xoO a x^TQ^axoc;. d xl eOpsGfj, xpaxTjXaLd sgxlv exslvou xoO xo^ou. xal dv
10 yevrixaL X9^^^ yeveaGaL x/jv xpaxTjXaLav exsLvou xoO xo^ou xexeXsLCO^evriv,
x6 xo^ov dcpatpsLxaL duo xcov 9. [sxslvo] el xl xaxaXsLcpGfj, xexeXsLCO^evov
eaxl x6 to^ov xal f) xpaxTjXaLa exsLvou xpaxsLxaL. d xl eOpsGfj, xpaxTjXaLd
eaxL xexeXsLCO^evT) exeivou xoO xo^ou.
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15 xfjc; xpaxTjXaLac; ^rixsLxaL, xal xax' evavxLov exeivou duo xfjc; dp^fjc; xoO
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xecpaXaLou.
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5 f) xexeXsLCO^evT) xoO xo^ou exsLvou xpaxTjXaLa dcpaLpsLxaL duo xcov ^. el xl oOv
xaxaXsLcpGfj, aaytxa eaxl xoO xo^ou exsLvou. xal edv x6 xo^ov sxslvo 9 ^otpaL,
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exeivou 9. d xl oOv xaxaXsLcpGfj, f) xpaxTjXaLa exsLvou xpaxsLxaL xal svoOxaL
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el XL xaxaXsLcpGfj, to^ov eaxl xfjc; aaylxac; exsLvrjc;. ei he f) aaylxa ^ ^otpaL,
15 opQfi eoTi xal x6 to^ov exsLvrjc; 9 ^otpal slglv. ei he f) aaylxa tiXslcov xcov ^,
dcpaLpoOvxaL £^ exsLvrjc; ^. d xl xaxaXsLcpGfj, xpaxTjXaLa sgxlv. x6 to^ov oOv
exsLvrjc; xpaxsLxaL. d xl eOpsGfj, svoOvxaL xolc; 9, xal eOplaxexaL x6 to^ov xfjc;
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xal xd LxvoTioSa. xax' evavxLov oOv xfjc; dvapdaecoc; ytvexaL elaeXeuaLc; xal
xpaxsLxaL x6 axtaa^a.
426
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^eaou xfjc; fj^epac; | xal xoO xotiou xfjc; Tuyjiq [xstol xfjc; eOGsLac; ypa^^fjc;. auxr) f284r
Se f) ^oLpa £Lc; 8 StaLpeLxaL xecpaXata.
5 KecpdXaLov a'. Ilepl xfjc; a xal P' ^exaxXlaecoc;.
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10 dvapdaecoc; xoO fjXLOu sic; xov xuxXov xoO ^eaou xfjc; fj^epac; xal xfjc; opGciaecoc;
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daxepoc;, fjyouv xfjc; [dii' dXXi^Xcov] xcov daxepcov SLaaxdaecoc; duo xfjc; xeXelac;
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15 xpaxsLxaL 6 (J;fjcpoc; xfjc; ^exaxXlaecoc;. | el oOv -/^peioi slSevaL x/jv ^sxaxXtaLV fssrv
xauxriv, si popela y] voxla y] xal sic; x/jv dvdpaaLV sgxlv y] x/jv xaxdpaaLV,
ylvexaL xT^prjaLc; sic; xd ^cpSta exsLva. dnep eXaxxov eiai xaOxa xcov c;, popela
4 he om. L II 5 a ^ om. L | a^] TipcoTir]^ Lv || 6 tolvuv om. Vv || 9 a ^] TipcoTir]^ Vv
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Vv
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dvdpaaLc; sgxlv. £l Se ^eaov xcov y, c; xal 6 slglv, xaxdpaaLc; sgxlv.
KecpdXaLov P'. Ilepl xfjc; xaxaXiQcJ^ecoc; xoO TiXdxouc; exdaxric; KoXecdq.
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5 Xa^pdvexaL, xal xax' evavxlov xcov ^OLpcov xoO tiXlou xpaxsLxat f) a'
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dcpatpsLxaL | omb xcov 9, xal x6 xaxaXsLcpGsv TiXdxoc; eaxl xfjc; noXscdq. fio4vL
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10 OLKO xoO xeXsLou xuxXou xfjc; fj^epac;, f) ^sGoSoc; o^olcoc; (be; sxsl xdvxaOGa
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cpalvovxoc; daxepoc; xal ^tqtioxs Suo^evou.
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15 p xaLpouc;, oxav SLLaxaxaL xfjc; yfjc; ^axpdv, xal oxav UTidp^T) syyuc;. elxa
2 EiGiv om. Vv II 3 SeuTspov LV || 5 TipcoTr] Vv || 9 totiov] xuxXov codd. |
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+ \ifixoc, Trjv £Tioxir]v SrjXoL toO dTiXavoO^ daxepo^ in marg. L^
428
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xaxd x6 [xeaov xfjc; fj^epac; xoO tiXlou. olko xouxou x8 dcpatpoOvxaL. el xl
5 xaxaXsLcpGrj, iiXdxoc; eaxl xfjc; tioXscoc; exsLvrjc;, £v6a expaxT^Gr) f) dvdpaatc;. el
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I dcpaLpsGLv y] Svcoglv xcov x8 x6 xaxaXsLcpGsv del dcpatpsLxaL duo xcov 9 xal fssvv
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429
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xu^TQ^ xoOxov. xal f) xd^Lc; xoO xavovLou | exsLvou duo xfjc; dp^fjc; xoO ^coSlou fiosvL
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5 IKscpdXaLov a'. Ilepl xoO TiXdxouc; xfjc; dvaxoXfjc; xdv xs voxlov soti xoOxo fioerL
xdv x£ popsLov
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xuxXou xfjc; fj^epac; Tipoc; x6 ^opeiov ^epoc; tiXsov eaxl xoO xeXsLou TiXdxouc;
xfjc; TioXecoc;, sxslvoc; oOv 6 daxfip del cpaviQc; sgxl xal oO huei (jko x/jv yfjv. el
10 he f) ^exdxXLGLc; exsLvou y] x6 ^fjxoc; Tipoc; x6 voxlov ^spoc;, sxslvoc; 6 daxfip
del bub yfjv sgxlv. slc; xaOxa oOv xal xd p TiXdxoc; dvaxoXfjc; oOx eaxLV.
£L he f) ^exdxXLGLc; exsLvou y] xo ^fjxoc; xax' evavxlov elalv exdxepov xoO
xexeXsLCO^evou TiXdxouc; xfjc; tioXscoc;, xo TiXdxoc; xfjc; dvaxoXfjc; 9 ^otpal slglv.
£L Se f) ^exdxXLGLc; y] xo ^fjxoc; eXaxxov eiai xoO xolouxou TiXdxouc; xfjc; tioXscoc;,
15 exsLvoc; 6 daxfip dvlax^L xal aOGic; h6ei xal xo TiXdxoc; svl xfjc; dvaxoXfjc;.
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5 'Edv f) ^exdxXLGLc; popeta, xal xoOxo. si he voxla, xal xo TiXdxoc; xoOxo
VOXLOV. £L Se 6 yjXloc; ^exdxXtaLV oOx e^^^ "H ^ daxfip ^fjxoc;, | xrjVLxaOxa sic; fioevL
xov xeXsLov xuxXov elal xfjc; fj^epac; xal TiXdxoc; dvaxoXfjc; oOx e-z^ouaiv.
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10 'Edv 6 yjXloc; ^exdxXtaLV oOx exTl ^ ^ daxfip ^fjxoc;, opGcoatv fj^epac;
oOx £x^^^^^5 ^^'^ "^^ YJ^LGU TO^ov xfjc; fj^spac; 9 ^otpal slglv. £l Se 6 yjXloc;
xal 6 daxfip exo\Joi ^exdxXtaLV xal ^fjxoc;, xrjpeLxaL exdaxou xpaxTjXaLa
£Lc; x/jv xpaxTjXaLav xoO TiXdxouc; xfjc; tioXscoc;. d xl eOpsGfj, ^spl^exaL sic;
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15 XeyexaL.
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f) xpaxTjXaLa xfjc; opGciaecoc; xfjc; fj^epac; sOpLaxexaL. elxa x6 to^ov exsLvrjc;
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5 fj^cov Sta xoOxo fjyouv x/jv opGcoatv x/jv xexeXsLCO^evriv xfjc; fj^epac;. xax'
evavxLov oOv xoO TiXdxouc; otac; pouXo^sGa tioXscoc; f) xpaxTjXaLa xfjc; opGciaecoc;
xpaxsLxaL xfjc; fj^epac;. xal xax' evavxlov xcov ^OLpcov xoO fjXLOu XsTixd yevLxd
xpaxoOvxaL. xaOxa oOv xd XsTixd xrjpoOvxaL sic; x/jv xpaxTjXaLav xfjc; opGciaecoc;
xfjc; fj^epac;. d xl eOpsGfj, nap' eva pa6^6v xpaxsLxaL oticoc; eOpsGfj f) xpaxTjXaLa
10 I xfjc; opGciaecoc; xfjc; fj^epac;. elxa xpaxsLxaL x6 to^ov xfjc; xpaxTjXaLac; xauxTjc; 285vv
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x/jv fj^epav. £L Se f) opQcdoiq xfjc; fj^epac; SLTiXaaLaaGfj, sOplaxexaL Kepiaaeioi
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15 'Edv oOv f) ^exdxXLGLc; y] x6 ^fjxoc; popsLov, f) xpaxTjXaLa xfjc; opGciaecoc;
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xpaxTjXaLa xfjc; opGciaecoc; xfjc; fj^epac; duo xcov ^ dcpatpsLxaL, xal sOplaxexaL f)
aaylxa xfjc; fj^epac; y] slc; xov TiXeovaa^ov y] slc; x/jv dcpalpeaLV.
5 Trjv 6p6coaLv Trjv TeTeXeLCO^evrjv ] Trjv TeTeXeLCO^evrjv opGcoatv Vv || 6 -7 xpaxeLxaL xfj^
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annotationem primam | dcpatpeaLV ] £XX£L(|>lv Vv
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I 01 dpxocLOL £X£LvoL ouxcoc; sQrixev oxl x6 ev vu^QiQ^epov x^ xatpoL slglv. fiorvL
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x/jv xaxdXri(J>Lv sxslvcov exsGr). edv oOv f) ^sxaxXtaLc; y] x6 ^fjxoc; popeta, f)
opQcdoiq xfjc; fj^epac; svoOxaL xolc; 9 . el Se voxta xaOxa, dcpaLpsLxaL olko xcov
9 . el XL eOpsGfj, x6 yj^lgu to^ov eaxl xfjc; fj^epac;. xoOxo SLTiXaaLd^exaL, xal
xexeXsLCO^evov x6 to^ov xfjc; fj^epac; sOplaxexaL. xal dXXcoc; edv f) ^exdxXtaLc;
10 y] x6 ^fjxoc; I popsLov, f) TiepLaasLa xfjc; fj^epac; svoOxaL xatc; pji ^olpaLc;. el fssvv
he voxLa xaOxa, dcpatpsLxaL | f) ^exdxXtaLc; y] x6 ^fjxoc; omb xcov pii ^OLpcov, f286rv
xal f) fj^epa xoO xo^ou sOplaxexaL. edv Se x6 xo^ov xfjc; fj^epac; olko xcov x^
dcpaLpsGfj, x6 to^ov xfjc; vuxxoc; sOplaxexaL.
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15 To TO^ov xfjc; fj^epac; ^spl^exaL sic; xd l£, xal f) opGf) oSpa xfjc; fj^epac; Tidarjc;
2 Ilepl ] elc, TO yvcopLa^a L || 4 to om. L || 9 xal om. Vv || 10 popeta LVv |
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xaOxa £L dcpaLpsGcoGLV duo xcov X, xd xe^^dxioc xfjc; ^f) opGfjc; oSpac; xfjc; vuxxoc;
5 xaxaXa^pdvovxaL.
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xd 8, xd xe^^dxLoc xfjc; ^f) opGfjc; oSpac; sOpLaxovxaL. xal edv xd xe^^d^La xfjc;
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oSpa f) opGf) sOplaxexaL.
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15 ^fjxoc;, xd ♦ ^ OLKO xcov xp^vcov xcov Apdpcov dcpaLpsLxaL. d xl xaxaXsLcpGfj,
^spl^exaL £Lc; xd ^r). d xl | e^eXGr], ^otpal slglv. aOxat xrjpoOvxaL sic; xd vy 286vv
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437
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xouxcov
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xuxXou. £L Se 6 daxfip ey^ei \ TiXdxoc;, f) Seuxepa ^sxaxXtaLc; exsLvr) xpaxsLxaL fsevv
10 xal xripsLxaL. eneiTOL xrjpeLxaL si popela eaxlv y] voxta (baauxcoc; xal xo TiXdxoc;
dx£ popsLov eaxLv dxe voxlov.
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15 si 8' oOx s^LGoOvxaL, xo eXaxxov dcpatpsLxaL xoO tiXslovoc;. el xl xaxaXsLcpGfj,
xripsLxaL. edv xo tiXsov eiq xo popsLov f), xoOxo popsLov sgxlv. £l Se xo voxlov
1 TO + ^eya v || 2 to ^fjxoc; xal om. L | post to stoc; LVv habent annotationem
secundam || 9 [J L || 10 TrjpeiTaL-'- om. Vv | voTLa + xaTXa^pdvovTat Vv || 11 eIte^ ]
el Vv I sIts^] f] Vv II 12 STiSLTa TrjpeiTaL om. Vv | eav (bat] sl ^ev oOv slaL Vv | f]^
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438
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E eaxl ToO KapxLvou, y] slc; to E toO AlyoxepcoToc;, d tl sxpaTT^Gr), to ^fjxoc;
SGTL I £X£LVOU OLKO TOO XUxXoU TTJc; fj^Spac;. £L Ss 6 daTTlp oOx SaTLV £Lc; TaUTa fl09vL
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5 Tiap' fj^cov, £X£Lv6 SGTLV f) ^oLpa ToO ^TQXouc; duo ToO xuxXou TTJc; dpQ(i>aecdq
TTJc; fj^epac;.
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ToO xuxXou TTJc; fj^epac;
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10 TpaxTjXaLav ttjc; TeTeXeLCO^evrjc; ^STaxXLaecoc; ttjc; ^eyLaTrjc;. d tl eOpsGrj,
[xepi'C.eTOLi sic, t/jv TSTsXeLCO^evriv P' ^STaxXtaLv toO aOGrj^epLvoO toO doTspoc;
£X£Lvou. xal f) TpaxTjXaLa toO ^tqxouc; sOpLaxsTaL duo ttjc; opGciaecoc; toO
xuxXou TTJc; fj^epac;. | el Se to aOGrj^epLvov toO doTspoc; [xeTOixXiaiv oOx 287rv
eX^^ s'^ TL eOpsGrj duo ttjc; xpouaecoc; ttjc; TpaxTjXaLac; ttjc; TeTeXeLCO^evrjc;
15 ^STaxXLaecoc;, xpaTSiraL sXaTTOv evoc; paG^oO. d tl eOpsGrj, f) TpaxTjXaLa toO
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exsLvo^ Vv II 4 f] + xal L | dXXa dXXaxoO om. Vv || lo ^exaxXLaeco^ xf]^ {leyioTric,]
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daxepoc; yLvo^evcov elc; xov xuxXov xoO ^eaou xfjc; fj^epac;
5 Oloc; daxrip TiXdxoc; oOx sx^^^ sxslvoc; 6 daxrip ^exd xfjc; ^otpac; xoO lSlou
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eX^L TiXdxoc;, sxslvoc; 6 daxiQp, el eaxL [xeaov xoO KapxLvou, xoO ZuyoO xal
xoO Alyoxepcoxoc;, xo TiXdxoc; exelvo voxlov, xal 6 daxfip oOxoc; | jipoxepov fiiorL
xfjc; ihioiq ^OLpac; cp6dv£L elc; xo ^eaoupdvri^a. el Se 6 daxfip [xeaov eaxl xoO
10 Alyoxepcoxoc;, xoO KptoO xal xoO Kapxlvou, xo TiXdxoc; exeivou popsLov xal
6 daxfip Tipo xfjc; ISlac; ^olpac; elc; xov [xeaov xfjc; fj^epac; ylvexat xuxXov.
xpaxsLxaL f) xpaxTjXaLa xoO xexeXsLCO^evou TiXdxouc;, xat xrjpeLxaL elc; x/jv
xpaxTjXaLav xoO ^tqxouc; xoO daxepoc; duo xfjc; dp^fjc; xoO Kapxlvou y] xfjc;
dpxfjc; xoO Alyoxepcoxoc; olov duo xouxcov xcov ^coSlcov eaxlv eyyuxepov
15 xoO daxepoc;. el xl eOpsGfj, ^spl^exaL elc; x/jv xexeXsLCO^evriv xpaxTjXaLav
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E ToO KapxLvou y] slc; to E toO Alyoxepcoxoc; [xstol xfjc; eOGsLac; ypa^^fjc;. el tl
5 eOpsGrj, xax' evavxLov exeivou ytvexaL elaeXeuaLc; sic; xd xavovta xoO xotiou
xfjc; xu^iQ^ t^s:xd xfjc; eOGsLac; ypa^^fjc;. xal xax' evavxLov exsLvou (J;7]cpou
xpaxoOvxaL xd ^cpSta dvco xal al ^otpat ex xoO TiXaylou. xal 6 (J;fjcpoc; 6
exepoc; 6 [xeaov xcov p xavovlcov | TiXrjpoOxaL (be; eppsGr). d xl e^eXGr], sxslvo fsrvv
^oLpd eaxLv oxl ^exd xoO daxepoc; o^oO cpGdvsL sic; xo ^eaoupdvri^a.
10 KecpdXaLov 8'. Ilepl xfjc; ^olpac; exsLvrjc; yjxlc; avia'/^ei [xenoi xoO daxepoc;
'Edv 6 daxfip TiXdxoc; oOx e^^i^ exelvoq 6 daxfip ^exd xfjc; ^olpac; xoO
aOGrj^epLvoO | dvlax^L. el §£ 6 daxfip e^^^ TiXdxoc;, 6 xotioc; xfjc; xu^iQ^ xouxou fiiovL
^£xd xfjc; eOGelac; ypa^^fjc; xaxaXa^pdvexat, xal f) dp^T) xouxou duo xfjc; dp^fjc;
xoO Alyoxepcoxoc;. el xl eOpsGfj, xpaxsLxaL. STiSLxa xrjpeLxaL. edv xo ^fjxoc; xoO
15 daxepoc; olko xfjc; opGciaecoc; xoO xuxXou xfjc; fj^epac; popsLov f), f) opGcoatc; xfjc;
fj^epac; dcpatpsLxaL | duo xoO xotiou xfjc; xu^iQ^- ^'^ S^ voxlov sgxl xo ^fjxoc; f287vv
xoO daxepoc;, evoOxat xcp xotico xfjc; xu^iQ^- ^'^ "^^ eOpsGfj, duo xouxou del 9
2 f]] T] V II 8 h6o Vv II 10 Ilepl] elc, to yvcopta^a L
441
dcpaLpoOvxaL. el tl xaxaXsLcpGrj, totioc; xfjc; tuxtq^ "^^^ ^otpcov soti [xsQ^ &>v
dvLGX^L 6 daxTQp. xax' evavxLov toutou slc; to xavovLov xoO totiou xfjc; tuxtjc;
yLvexaL elaeXeuaLc;. £v6a eOpsGrj [xeaov xoO xavovLou 6 (J;fjcpoc;, xax' evavxLov
xouxou xpaxoOvxaL dvco xd ^cpSta xal ex TiXayLou al [xolpoii^ xal xd XsTixd
5 [xeaov xcov p xavovLCOv xrjpoOvxaL (be; eppsGr).
AtaLpeaLc;. Ilepl xfjc; ^exd xoO daxepoc; Suvouarjc; [xoipoLc,
'Eiiei xpeioL (J;7]cpou, x6 to^ov xoO daxepoc; xfjc; fj^epac; svoOxaL xfj ^otpa
xoO xoTiou xfjc; Tuyjiq fjxLc; dvLax^L ^s:t' sxslvov. d xl eOpsGfj, sic; x6 xavovLov
xoO xoTiou xfjc; Tuyjiq xoO TiXdxouc; xfjc; tioXscoc; exsLvrjc; duo ^coSlcov xal ^OLpcov
10 £^ exsLvrjc; xrjpeLxaL (be; eppsGr). d xl eOpsGfj, c; ^(bSta svoOxaL xouxo), xal
sOplaxovxaL al ^otpaL sxelvaL al ^exd xoO daxepoc; SuvouaaL.
KecpdXaLov £ . Ilepl xoO daxepoc; oxav dvlax^L xal Suvr] y] xaxd x/jv vuxxa y]
x/jv fj^epav
I TripsLxaL f) ^olpa exsLvr) f) dvlaxouaa | ^exd xoO daxepoc;. edv f) ^eaov fssrv, fiiirL
15 xoO fjXLOu xal xfjc; SLa^expou xouxou, xaxd x/jv fj^epav avia'/^ei 6 daxiQp. el
1 post xaTaXsLcpGf] v add et cancell 6 || 4 al ^oLpat ex TiXayLou Vv || 6 Ilepl] elc, to
yvcopLa^a L | [ietol om. Vv || 7 xfj ^OLpa in marg. v || 8 tco totico v || lo eppsGr]]
SLpsLxaL L I C^^^cp V II 12 Ilepl] slc; Trjv xaTdXir](|>LV L | xaxa Trjv vuxxa] diio xfjc; fj^epac;
L II 13 Trjv fj^epav] xfj^ vuxto^ L
442
he f) ^oLpa eOpsGrj [xeaov xfjc; SLa^expou xoO tiXlou xal aOxoO xoO tiXlou, xaxa
x/jv vuxxa. eav dvLax^L 6 daxrip xaxd x/jv fj^epav, 6 xotioc; xfjc; xu^iQ^ "^^^
^OLpcov xoO tiXlou £lc; x6 TiXdxoc; xfjc; tioXscoc; exsLvrjc; dcpaLpsLxaL duo xoO xotiou
xfjc; xu^TQ^ "^^^ ^OLpcov xcov dvLG^ovxcov ^£xd xoO fjXLOu. d XL eOpsGfj, sxslvo
5 TiepLcpopd eaxLv olko xfjc; dp^fjc; xfjc; fj^epac; exsLvrjc; oxav avia'/^ei 6 daxiQp. el Se
dvLGX^L 6 daxfip xaxd x/jv vuxxa, 6 xotioc; xfjc; xuxtjc; xcov ^OLpcov xfjc; SLa^expou
xoO fjXLOu £Lc; x6 TiXdxoc; xfjc; tioXscoc; dcpatpsLxaL duo xoO xotioO xfjc; xu^iQ^ "^^^Ci
daxepoc;. d xl xaxaXsLcpGfj, iiepLcpopd sgxlv duo xfjc; dp^fjc; xfjc; vuxxoc; [isXP^
xfjc; oSpac; xa6' y]v dvLGX^t 6 daxiQp. xal sic; xoOxov xov (J;fjcpov xov prjGevxa
10 si pouXri6co^£v eihevoLi oxav Suvr] 6 daxiQp, exsLvr) f) ^otpa f) Suvouaa ouxcoc;
xpaxsLxaL oxl dvLax^t xal o^olcoc; ylvexaL f) [xeBohoc^.
2 xaxa Trjv fj^epav sup. lin v
443
MoLpa c, . Ilepl xfjc; xaxaXiQcJ^ecoc; exsLvrjc; otl duo xfjc; fj^epac; TioaaL d^pat
TiapfjXGov xal TioaaL ^otpaL duo xfjc; ^r) opGfjc; oSpac; xal xcov (bpcov xfjc; xu^iQ^ ^^o^^-
xfjc; opGciaecoc; xcov lP OLXTj^dxcov xal xfjc; xaxaXiQcJ^ecoc; xoO arj^SLOu exdaxric;
dvapdaecoc; xal xoO arj^SLou xfjc; jipoaeuxfjc;
5 AuxT) f) ^OLpa £Lc; ^ StaLpsLxaL xecpaXata.
KecpdXaLov a'. Ilepl xfjc; xaxaXiQcJ^ecoc; | xfjc; jiepLcpopdc; xoO fjXLOu oxav dvLaxT) f288rv, fiiivL
I xa6' ov xatpov pouXo^sGa slSevaL xoOxo fjyouv x/jv 6p6fiv oSpav xal | x/jv ^f) fssvv
opGiQv
'EtisI y^^zioL £Lc; x6 yvcovat xal spydaGaL x/jv stilgxtq^tiv xauxriv, Tipcoxov
10 xpaxsLxaL Std xoO daxpoXdpou f) dvdpaaLc; xoO fjXLOu xa6' ov xatpov
PouXo^sGa, xal xoOxo Xeyexat dvdpaaLc; xoO xatpoO. STiSLxa f) eaxdxr)
dvdpaaLc; xoO fjXLOu sic; exsLvriv x/jv fj^epav xaxaXa^pdvexat (baauxcoc;, xal
aaylxa xfjc; fj^epac; ^rixsLxaL xal sOplaxexaL. pouXo^evcov 8' fj^cov TioLfjaat
(J;fjcpov TioLoO^ev ouxcoc;* xrjpeLxaL f) xpaxTjXaLa xfjc; dvapdaecoc; exsLvrjc; sic; x/jv
15 aaylxav xfjc; fj^epac;. d xl eOpsGfj, ^spl^exaL sic; x/jv xpaxTjXaLav xfjc; eaxaxTjc;
dvapdaecoc;. d xl eOpsGfj, sxslvo xpaxTjXaLa sgxlv. xoOxo del dcpatpsLxaL
duo xfjc; aaylxac; xfjc; fj^epac;. d xl xaxaXsLcpGfj, sxslvo aaylxa sgxlv. duo
1 exTiT] V II 2 63pa^ om v || 7 TOUTO add et cancell v || i4 outco^] otico^ v
444
TauTTjc; ^riTSLTaL to to^ov exsLvrjc;. el tl eOpsGrj, sxslvo nepiaaeioL XeyexaL
xfjc; TiepLcpopac;. STiSLxa TTipelioLi 6 xatpoc; xfjc; dvapdaecoc;. dnep eaxl Tipo xoO
^eaou xfjc; fj^epac;, f) TiepLaasLa auxr) dcpaLpsLxaL duo xoO yj^lgu xo^ou xfjc;
fj^epac;. el Se ^exd x6 [xeaov xfjc; fj^epac;, svoOxaL xouxcp xal ebpiaxsTOii f)
5 TiepLcpopd dii' exsLvrjc; xfjc; oSpac; oxav dvLGX^t 6 yjXloc; ^£XP^ ^^'^ "^^^ xatpoO
£X£Lvou, fjVLxa yLvsxaL f) ^TQxriaLc;. duo xouxou oOv sxpdXXovxaL al d^pat.
AtaLpeaLc;. | Elc; x6 yvcipLa^a xfjc; dvapdaecoc; xoO daxepoc; xaxd xov xatpov fii2rL
ov pouXexaL xlc; olko xfjc; jiepLcpopdc;
XpsLac; yevo^evrjc; jiepl xoO (J;7]cpou xouxou xaxaXa^pdvexat f) TiepLaasLa
10 xfjc; aayLxac; xal dcpatpsLxaL duo xfjc; aaytxac; xfjc; fj^epac;. el xl xaxaXsLcpGfj,
xpaxTjXaLd sgxlv. exsLvr) f) xpaxTjXaLa xrjpeLxaL elc; x/jv xpaxTjXaLav xfjc; ea^dxric;
dvapdaecoc; elc; xov xuxXov xoO \ieao\j xfjc; fj^epac;. d xl eOpsGfj, | ^epL^exat f59rv
£Lc; x/jv aayLxav xfjc; fj^epac;. xo xaxaXsLcpGsv xpaxTjXaLd sgxl xfjc; dvapdaecoc;
£X£Lvou xoO xatpou.
15 AtaLpeaLc;. Elc; xo elSevat d xl TiapfjXGsv duo xfjc; vuxxoc;
'H dvdpaaLc; xoO diiXavoOc; daxepoc; xpaxelxaL. xal o^olcoc; ^sGoSeuexaL
1 XeyexaL] dvaXeyexaL L || 3 ami]] outco L || is to xaxaXsLcpGev] d tl supeGfj L
445
(be; xal eid xoO tiXlou xal 6 aOxoc; dcTiapdXXaxToc; (J;fjcpoc;. xdvxaOGa ydp f)
TpaxTjXaLa xfjc; dvapdaecoc; exsLvrjc; sic; xriv aayLxav xfjc; fj^epac; xrjpeLxaL, xal
xaGs^fjc; ytvexaL (J;fjcpoc; (be; exeu xal sOplaxexaL f) TiepLcpopd dii' exsLvrjc; xfjc;
oSpac; oxav dvlaxT) 6 daxrip ^^XP^ ^^'^ "^"^^ oSpac; fivlxa ylvexaL f) ^TQxriaLc;.
5 ALalpsGLc;. Elc; x/jv xaxdXrjcJ^Lv exeivou kogoli &>poii TiapfjXGov xfjc; fj^epac; olko
x(ov ^f) 6p6(ov (bp(ov
'ExsLvo xaxaXa^pdvexaL duo xfjc; dvapdaecoc; xoO xatpoO xal xfjc;
dvapda£(oc; xoO | ^eaou xuxXou xfjc; fj^epac;. xal ydp f) xpaxTjXaLa xfjc; f59vv
dvapda£(oc; xoO xatpoO elc; x/jv xpaxTjXaLav xfjc; ea^dxTjc; xfjc; dvapdaecoc;
10 ^spl^exaL. el xl eOpsGfj, nap' eva pa6^6v eXaxxov xpaxsLxaL. el xl eOpsGfj,
xpaxTjXaLd sgxlv. x6 xo^ov xauxTjc; xpaxsLxaL xal ^spl^exaL elc; xd le. el xl
eOpsGfj, f) ^f) op67] eaxLv oSpa. ei oOv f) dvdpaatc; exsLvr) f) xpaxsLGsLaa Tipo
xoO ^eaou xfjc; fj^epac; sgxlv, exsLvr) f) ebpeQelaoi oSpa f) ^f) 6p67] sgxlv duo xfjc;
dpxfjc; xfjc; fj^epac; ^£XP^ xoxe. el Se sgxlv f) dvdpaatc; auxr) ^exd x6 [xeaov
15 xfjc; fj^epac;, exsLvr) f) oSpa | dcpatpsLxaL duo x(ov tp. d xl xaxaXsLcpGfj, f) oSpa fiisrL
f) ^f) 6p67] eaxLv duo xfjc; dp^fjc; xfjc; fj^epac; ^£XP^ xoxe. ei pouXri6(o^£v duo
x(ov ^f) 6p6(ov (bp(ov slSevaL x/jv dvdpaatv, xrjpoOvxaL al d^pat sxsLvaL elc; xd
3 6^ om Vv II 4 post f] CV]xir]aL^ LVv habent annotationem tertiam || 5 Trjv xaTdXir](|>LV
exsLvou] TO SL^evaL Vv || 8 toO [iego\j xuxXou xfj^ fj^epa^] toO xuxXou xfj^ fj^epa^ ^eaou
L II 10 xpaxsLTaL eXaxxov L || ii -12 d tl eupsGrj] to xaTaXsLcpGsv Vv || 12 oOv] yoOv
V II 14 ^£Ta] xaTa Vv
446
L£. el XL eOpsGrj, f) TpaxTjXaLa exsLvr) xripeLTaL sic; xriv TpaxTjXaLav xfjc; eaxaTTjc;
dvapdaecoc;. d tl e^eXGr], nap' eva pa6^6v eXaxxov xpaxsLxaL. d xl eOpsGrj,
xpaxTjXaLd sgxlv xfjc; dvapdaecoc; xoO xatpoO.
KecpdXaLov P'. Elc; x/jv xaxdXrjcJ^LV xfjc; oSpac; ex xfjc; jiepLcpopdc; xal £^ dXXcov
5 XLVCOV
'Eiiei xpeioL xeveoQoLi x/jv spyaaLav xauxriv, el (eaxLv)/) TiepLcpopd duo xfjc;
fj^epac;, svoOxaL xcp xotico xfjc; xu^iQ^ "^^^Ci aOGrj^epLvoO xoO fjXLOu elc; x6 TiXdxoc;
xfjc; KoXecdq. el 8' eaxlv f) TiepLcpopd xfjc; vuxxoc;, svoOxaL exsLvr) f) TiepLcpopd
xcp xoTicp xfjc; Tuyjiq xfjc; SLa^expou xoO aOGrj^epLvoO xoO fjXLOu elc; x6 TiXdxoc;
10 xfjc; TioXecoc;. el xl eOpsGfj, xax' evavxLov exsLvrjc; ytvexaL elaeXeuaLc; ^eaov
xoO xavovLou xoO TiXdxouc; xcov tioXscov, onep eaxl xal xotioc; xfjc; xu^iQ^^
xal xpaxoOvxaL £X£l6£v ^cpSta xal ^otpaL xal XsTixd ^exd xfjc; ^sGoSou xoO
TioXXdxLc; eipri\ievo\j (J;7]cpou. el xl eOpsGfj, ^cpSta, ^otpaL | xal XsTixd eiai xfjc; feorv
Tuyjiq eiq xov xatpov exelvov fjVLxa expaxT^Gr) f) dvdpaatc;. ei he eam yvcipL^oc;
15 f) TiapeXGoOaa oSpa duo xfjc; fj^epac; y] xfjc; vuxxoc;, [edv] f) oSpa exsLvr) | duo f289rv
xcov 6p6cov £Lc; xd le xrjpeLxaL. ei he sgxlv duo xcov ^f) 6p6cov, exsLvr) elc; xd
6 'Etisl xp^^of yeveaGaL Trjv epyaatdv TauTrjv] STiav yevrjiaL xp^^o^ xfjc; epyaatac; xauTrjc; Vv
I £l] eav L || 7 xfj^ tuxtt]^ + xfj^ ^La^expou L || 8 -lo el 5' eaxlv . . .xfj^ tioXsco^ om. L
II 446 .16 -447.1 TOL te\i\i6lxiol] Tir]v Tpaxir]XaLav V
447
T£^^d)(Loc xfjc; ^T) opGfjc; oSpac; TTipelioLi. el tl eOpsGrj, iiepLcpopd eaxLv acp' fjc;
sxpdXXsTaL I 6 xXfjpoc; xfjc; tuxtq^- fusrL
AtaLpeaLc;. Elc; xriv xaxdXricJ^Lv xfjc; xuxtjc; duo xcov ^otpcov xoO l' olxiQ^axoc;
'O xoTioc; xfjc; Tuyjiq [xstol xfjc; eOGsLac; ypa^^fjc; xpaxsLxaL olko xouxcov xcov
5 ^oLpcov, xal f) dpxT) xouxou duo xfjc; dp^fjc; xoO Alyoxepcoxoc;. el xl eOpsGfj,
xax' evavxLov xouxou ytvexaL elaeXeuaLc; elc; x6 [xeaov xoO xavovLou xoO xotiou
xfjc; xu^TQ^ "^^^Ci TiXdxouc; xcov tioXscov, xal £X£l6£v xpaxoOvxat xd ^cpSta xal al
^oLpaL xaxd x/jv prjGeLaav ^sGoSov. xal el xl e^eXGr], sxslvo sgxlv f) xu^iQ-
KecpdXaLov y'. Ilepl xfjc; xaxaXiQcJ^ecoc; xfjc; jiepLcpopdc; xcov (bpcov olko xfjc; xu^iQ^
10 ZrjxeLxaL xal xpaxsLxaL x6 aOGrj^epLvov xoO fjXLou xal al ^otpaL xfjc; Tuyjiq^
xal xrjpoOvxaL. edv x6 aOGrj^epLvov xoO fjXLou ^eaov xoO ^' xal l' olxiQ^axoc;
eaxLV, 6 xotioc; xfjc; xu^iQ^ aOGrj^epLvoO xoO fjXLOu ^exd xoO duo xou TiXdxouc;
xfjc; TioXecoc; olko xoO xotiou xfjc; xu^iQ^ '^^^ TiXdxouc; xfjc; tioXscoc; dcpaLpsLxaL.
el XL xaxaXsLcpGfj, iiepLcpopd sgxlv olko xfjc; dp^fjc; xfjc; TiapeXGouarjc; fj^epac;
15 exsLvrjc;. el Se x6 aOGrj^epLvov xoO fjXLou ^eaov xcov oLxrj^dxcov xfjc; xu^iQ^ "^^^Ci
8' xal C eaxLV, 6 xotioc; xfjc; xu^iQ^ "^"H^ SLa^expou xoO fjXLOu duo xoO xotiou xfjc;
3 I Om. V II 9 XpLTOV V || 12 TOO OtTIO TOU ] TOUTOU L
448
TUXTQ^ "X-^'^ '^^^ TiXdxouc; xfjc; tioXscoc; dcpaLpsLxaL. el tl xaxaXsLcpGrj, TiepLcpolpd feovv
eaxLV dcTio xfjc; dp^fjc; xfjc; vuxxoc; [isXP^ '^^^ oSpac; xoO xatpoO xouxou. | octi' fii4rL
exeLvrjc; xfjc; jiepLcpopac; sxpdXXexaL f) oSpa f) opGf) xal ^f) opGiQ.
KecpdXaLov 8' . Ilepl xfjc; xaxaXiQcJ^ecoc; xcov i^ OLXTj^dxcov fjyouv xfjc; opGciaecoc;
5 auxcov.
'Etisl xp2:Loc xeveoQoLi x/jv ^sGoSov xauxrjv, al ^otpaL xcov (bpcov xal al ^otpaL
xfjc; xuxTjc; yLvciaxovxaL xal SLTiXaaLa^ovxaL. el xl eOpsGfj, xoOxo opGcoatc;
TipcixT) eaxLv, OTiep del dcpatpsLxaL olko xcov ^. xal Seuxepa ylvexaL opQcdoiq.
xaOxa oOv xal xd p xrjpoOvxaL. STiSLxa xpaxsLxaL 6 xotioc; xfjc; xu^iQ^ ^^o^^- "^^
10 TiXdxoc; xfjc; tioXscoc; exsLvrjc;. xouxcp exsGr) ovo^a Sexaxov. oOxoc; 6 (J;fjcpoc;
exsGr) sic; x6 Sexaxov olxrj^a. elxa f) Tipcixr) opGcoatc; svoOxaL xouxcp. el xl
eOpsGfj, xoOxo xotioc; xfjc; Tuyjiq xoO evSexdxou olxiQ^axoc;. xal aOGic; f) Tipcixr)
opGcoGLc; svoOxaL xcp xolouxco xotico xfjc; Tuyjiq xoO evSexdxou olxiQ^axoc;. d
XL oOv eOpsGfj, xoTioc; xfjc; xu^iQ^ "^^^Ci ScoSexdxou olxiQ^axoc; sgxlv. six' aOGLc;
15 f) TipcixT) opGcoGLc; svoOxaL xcp ScoSexdxcp olxiQ^axL, xal eOplaxexaL 6 xotioc;
xfjc; Tuyriq. eha f) Seuxepa opGcooLc; svoOxaL xcp xolouxco xotico xfjc; Tuyjiq^ xal
ylvexaL 6 xotioc; xfjc; Tuyjiq xoO Seuxepou olxiQ^axoc;. xal aOGLc; f) Seuxepa
14 oOv omVv I supeGfj] e^eXGr] Vv || i7 P' Vv
449
opGcoGLc; £Lc; xov totiov xfjc; tuxtq^ "^^^C; Seuxepou olxTQ^axoc; iiepiaae^eTOLi. xal
6 TOTioc; xfjc; tuxtjc; toO xpLxou olxTQ^axoc; sOpLaxexaL. xal aOGic; | f) Seuxepa fii4vL
opQcdoiq svoOxaL xcp xotico xfjc; Tuyjiq xoO xpLxou olxiQ^axoc;. | xal x6 xexapxov f289vv, feirv
oIxTj^a I sOplaxexaL xoO xotiou xfjc; Tuyjiq. eha 6 xotioc; xfjc; xu^iQ^ "^^^Ci l'
5 OLXTQ^axoc; eladyexaL sic; x6 xavovLov xoO xotiou xfjc; xu^iQ^ '^^^ [xstol xfjc;
eOGsLac; ypa^^fjc; duo xfjc; dp^fjc; xoO Alyoxepcoxoc;. xal xax' evavxlov xoO
eOpsGsvxoc; (J;7]cpou ^eaov xoO xavovlou xpaxoOvxat xd ^cpSta dvco xal al ^otpaL
ex TiXayLou ^exd xoO (J;7]cpou eOpsGsvxoc; ^eaov xcov 8uo xavovlcov. el xl eOpsGfj,
xevxpov eaxl xoO l' olxiQ^axoc;. (baauxcoc; 6 xotioc; xfjc; xu^iQ^ "^^^Ci La' olxiQ^axoc;
10 xripsLxaL £Lc; x6 xavovLov xoO xotiou xfjc; xu^iQ^ "^^^Ci ^exd xfjc; eOGsLac; ypa^^fjc;.
xal ylvexaL sic; xoOxo xal ev xolc; Xoltiolc; olxiQ^aaL ^^XP^ ^^'^ "^^^ ^' ^^ sppsBr)
xal em xoO l' olxiQ^axoc;. xal sOplaxovxaL xd xevxpa xouxcov.
Elxa al ^OLpaL xoO e' olxiQ^axoc; xax' evavxlov elal xoO La', xal al ^otpaL
xoO c;' oLXTQ^axoc; xax' evavxLov xoO lP'. xal al xoO C (baauxcoc; xcov ^OLpcov
15 xoO a' OLXTQ^axoc;, xal al xoO rj' xcov xoO P' xal al xoO evdxou olxiQ^axoc;
^OLpaL xax' evavxLov xcov xoO y olxiQ^axoc; xal ouxco xeXsLoOvxaL al dpQ(i>aeiq
xcov lP OLXTj^dxcov xal sOplaxovxaL xd xevxpa Tidvxcov.
2 xal a06L^] o^oLCO^ Vv || 3 y' L || 4 ebpiaxETai] yLvexaL Vv || 8 tcov 5uo xavovLCOv ]
Tcov xavovLCOv Tcov p L II 13 Tie^TiTOU L II 14 al om. L | tcov ^OLpcov] xax' evavxlov
Vv II 15 al^ om. L | Seuxepou v | G' L | olxrj^aTO^^ om. Vv
450
Tpuxavr) xoO (J;7]cpou toutou
'Eav &ai ol (J;fjcpoL xoO C olxTQ^axoc; xal xoO 8' e'E,iao6\ievoi xaxa xac;
^oLpac; xal xa XsTixd, 6 (J;fjcpoc; 6p66c; sgxlv. | xal aOGic; eav 6 xotioc; xfjc; fiisrL
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15 £X^^5 "^^ ^^ ^^^ Xfjyov Tipoc; o^u.
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x(ov xp6v(ov xal ^riv(ov xpaxrjGeLaaLc; fj^epaLc;. elxa ^rixoOvxaL al xpaxrjGeLaaL
fj^epaL xoO ^rivoc; sic; x6 xavovLov x(ov fj^epGiv. £v6a sOpsGoiaLv, xax' evavxlov
£X£LV(ov ylvexaL elaeXeuaLc; sic; x6 xavovLov x(ov fj^epGiv | xoO daxepoc; exelvou. fesrv
el XL oOv eOpsGrj, | xlGsxaL bub xov (J;fjcpov x(ov [xriv&v — xd ^(bSta bub xd ^(bSta fii9vL
15 xal ecpe^fjc; 6^ol(oc; xal em xolc; dXXoLc;.
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6 (J;fjcpoc;, dvd ^ ylvexaL xouxou dcpalpeaLc;. el xl STiSLxa xaxaXsLcpGrj, edv
s^LGoOvxaL xaLc; Tipoxepov xpaxrjGeLaaLc; fj^epaLc; xoO ^rivoc;, 6 (J;fjcpoc; opGoc;. ei
2 XsTripL^cov L II 4 -5 XsTripL^cov L II 9 -10 b\ioi(x>c, . . . aOxaL ] d tl eupsGf] omaQev anb
Tcov fj^epcov xf]^ epSo^dSo^ xpaxsLTaL xal L || ii xal ^rjvcov om L
460
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Se xoO (J^TQcpou 6p6o0, evoOvxat ol (J;fjcpoL Tidvxec; xcov ^eacov xlvtqgscov. edv oOv
£Lc; xd Seuxepa Xsktol UKsp^fi 6 (J;fjcpoc; xd ^, xd ^ dcpatpoOvxaL e^ sxslvcov, xal
a TipoaxiGexaL sic; xd a XsTixd. xal aOGic; edv 6 (J;fjcpoc; xcov a Xstixcov Oiiep xd
5 ^ yevrixaL, xd ^ dcpatpoOvxaL duo xcov xolouxcov Xstixcov, xal a TipoaxlGsxaL sic;
xdc; ^olpac;. si he 6 (J;fjcpoc; xcov ^OLpcov xd X UTiepPrj, xd X duo xcov auvaxQeiacov
^OLpcov dcpatpoOvxaL, xal a TipoaxlGsxaL sic; xd ^(pSta. si he TidXtv 6 (J;fjcpoc; xcov
^coSlcov xov lP UKsp^fi dpLG^ov, xd i^ xaxaXt^TidvovxaL, xal x6 ev djioXsLcpGev
xpaxsLxaL. el xl oOv eOpsGrj, duo ^coSlcov, ^otpcov, xal Xstixcov f) [xeari XLvrjaLc;
10 eaxL xoO daxepoc; exeivou eic, x/jv ^eariv XLvrjaLv xfjc; auvxd^ecoc; sic; sxslvo x6
[xeaov xfjc; fj^epac; sic; x6 ^fjxoc; xcov 9 . el 8' eaxl ^£0' fj^cov xe^^dx^ov xfjc;
oSpac;, xax' evavxlov | xfjc; oSpac; xauxTjc; ylvexaL eiaeXeuaiq eiq x6 xavovLov xcov fi20rL
(jKO xouc; ^fjvac; (bpcov. xal f) XLvrjaLc; xoO daxepoc; exeivou xpaxsLxaL, | xal fesvv
svoOxaL xfj [xeari xlvtqgsl xfj Tipoxepov xpaxrjGeLar].
15 ALalpsGLc;. Ilepl xfjc; opGciaecoc; xoO OcJ^ci^axoc;
I KpaxrjGeLaric; xfjc; ^earjc; xlvtqgscoc; xax' evavxlov xoO exouc; exsLvou duo 292vv
xcov xpovcov, xcov ^rivcov, xal xcov fj^epcov ylvexat elaeXeuaLc;, xal xpaxsLxaL f)
4 TipCOTa Vv I TipCOTCOV Vv II 5 dllO TCl)V TOLOUTCOV XSTITCOV ] £^ SXSLVWV TCl)V TipCOTCOV XSTITCOV
Vv II 7-8 £L 5e: TidXLv . . . UTiepPf] ] edv Tov LIT]' UTiepPcoaLv L || 8 ScoSexaxov v | ScoSexa v
II 16 exsLvoul exsLvcov v
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Otio touc; ^fjvac; ucj^co^a xoO daxepoc; exeivou to xaxd xriv dpxTjv xoO xpovou
xcov Apdpcov eOpsGev svoOxaL xrj xoLauxr] xlvtqgsl xoO OcJ^ci^axoc;. d xl oOv
eOpsGrj, ucj^co^d sgxl xfjc; opGciaecoc;.
5 KecpdXaLov P' . Ilepl xfjc; opGciaecoc; xcov ^eacov xlvtqgscov xcov daxepcov
ToOxo xaxd p ytvexaL xpoTiouc;. sic; sxslvoc;, oxl duo xfjc; Kepiaaeioiq xcov p
^rixcov 6 (J>fjcpoc; xfjc; ^earjc; xlvtqgscoc; xfjc; auvxd^ecoc; sic; x6 ^fjxoc; xfjc; exepac;
TioXecoc; StapLpd^exaL. Seuxepoc; sxslvoc;* auxr) f) ^ear) XLvrjaLc; f) ^exd xoO
^TQXouc; xfjc; tioXscoc; opGcoGsLaa ^exd xfjc; opGciaecoc; xfjc; fj^epac; ytvexaL xeXeta.
10 6 OLKO xcov p Tipcoxoc; (J;fjcpoc; xpaxsLxaL - f) TiepLaasLa f) ^ear) xcov p xfjc; tioXscoc;
fjc; pouXo^sGa xal xoO ^tqxouc; xcov 9. d xl oOv eOpsGfj, sxslvo ^epL^exat sic;
xd L£ I y] xripsLxaL sic; xd 8 XsTixd. d xl eOpsGfj, oSpa eaxlv sxslvo y] xe^^d^iov fi20vL
xfjc; oSpac;. elxa xax' evavxLov xcov (bpcov xouxcov ytvexaL elaeXeuaLc; sic; x6 bub
xouc; ^fjvac; xavovLov xcov (bpcov, xal xpaxsLxaL f) ^ear) XLvrjaLc; xoO daxepoc;
15 £X£Lvou, xal xripsLxaL. STiSLxa xrjpeLxaL sic; x6 ^fjxoc; xfjc; tioXscoc; exsLvrjc;. dnep
eXaxxov sgxl xoOxo xcov 9, exsLvr) f) [xeay] XLvrjaLc; f) duo xcov (bpcov xpaxrjGeLaa
svoOxaL xfj duo xfjc; auvxd^ecoc; [xeari xlvtqgsl. £l he tiXsov xcov 9, dcpatpsLxaL
I TipcoTCOv Vv I SeuTspcov Vv II 5 5' V II 6 p^ ] h6o V II 10 p^ ] 5uo V I p^ ] h6o V
II 16 EOTi post eXaxTov L | f] ^ear] om Vv
462
£^ £X£Lvou, xal ebpiaxsTOLi f) [xeay] XLvrjaLc; xfjc; tioXscoc; exsLvrjc; - TiepLaasLa
I £Lc; xriv opGcoGLv xfjc; ^earjc; xlvtqgscoc; xfjc; tioXscoc; exsLvrjc; ^exa xfjc; opGciaecoc; feerv
xfjc; fj^epac;. xax' evavxLov xfjc; [xeariq xlvtqgscoc; xoO fjXLOu ytvexaL elaeXeuaLc;
£Lc; xa xavovLa xfjc; opGciaecoc; xcov fj^epcov, xal xpaxsLxaL x6 xe^^dxiov xfjc;
5 oSpac;. STiSLxa xax' evavxLov xoO xe^^axiou xouxou ytvexaL elaeXeuaLc; sic; xa
bub xouc; ^fjvac; xavovLa xcov (bpcov, xal f) [xeay] XLvrjaLc; xoO daxepoc; exsLvou
xpaxsLxaL. el xl eOpsGfj, dcpaLpsLxaL del duo xfjc; ^earjc; xlvtqgscoc; xfjc; tioXscoc;
exsLvrjc;, xal sOplaxexaL f) xeXela opGcoatc; xfjc; ^earjc; xlvtqgscoc; xfjc; tioXscoc;
exeLvrjc;.
10 ALalpsGLc;. 'Edv f) ^sGoSoc; auxr) xcov aOGrj^epLvcov Std xd yevsGXLaXoyLxd
yevrixaL, xrjpeLxaL x6 ^fjxoc; xfjc; noXscdq. edv f) eXaxxov xcov 9, exsLvr) f) oSpa | f) fi2irL
e^eXGoOaa duo xcov p ^rivcov svoOxaL xcp exsL exsLvcp sic; o eyevexo f) yevvrjaLc;.
£L 8' eaxl TiXeov xcov 9 | x6 ^fjxoc; xfjc; tioXscoc;, exsLvr) f) oSpa dcpatpsLxaL olko xoO f293rv
exouc; £X£Lvou. STiSLxa x6 xe^^dxiov xfjc; opGciaecoc; xcov fj^epcov del dcpatpsLxaL
15 duo xoO exouc;, xal opGoOxat x6 exoc; opGcoatv xeXelav. elxa xax' evavxlov
xoO exouc; xouxou ylvexat elaeXeuaLc; sic; xd xavovta xcov [xeacdv xlvtqgscov xcov
daxepcov, xal xpaxoOvxat ol (J;fjcpoL xouxcov olko xfjc; auvxd^ecoc;. al [xeaoii oOv
10 auTiT] + xf]^ xexviT]^ L || 11 f] sup lin v || 12 5uo Vv || 13 ante toO \ifixoc, v add
et cancell dcpaLpeixaL e^ sxslvou || 14 STiSLxa] elxa Vv
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KecpdXaLov y' . Ilepl xfjc; elaeXeijaecoc; xcov yvcopt^cov XP^^^^ "^^^ SouX-
xavLXCOv xaTiLaa
'IgGl (be; sic; y^povoq xoO tiXlou eaxl xoaov x^e l8 x^ x Xc; ^^ . 6 y^povoq
5 xcov 'Pco^aLCOv xoaoc; xal xoaa xe^^dxia slglv slc; sxslvov TiepLaaasLa duo
xoO xp^vou xoO tiXlou E E Xp X6 xy ty . xd xe^^dxioc xaOxa sic; xouc; pt
Xpovouc; ^La fj^epa ytvexat xexeXsLCO^evr). 6 y^povoq xcov Hepacov eXdxxcov
eaxl xoO xpovou xoO tiXlou xoaov E l8 x^ x Xc; ^^ . 6 y^povoq xfjc; aeXTQvric;
I xoaoc;* xv8 xp a Xc; va . 6 xp^voc; xoO tiXlou duo xou xp^vou xfjc; aeXT^vrjc; feevv
10 TiXsLCOv Toaov L vp X£ ^y ^£ v£ . f) TiepLcpopd xfjc; fepSo^dSoc; iiepiaay] yLvexaL
fj^epav ^Lav sic; xov | xpovov xou fjXLOu sic; xe^^d^La xoaa oxl 6 xpovoc; xcov fi2ivL
Hepacov eXdxxcov xou xpovou xou fjXLou. sic; xouxo exsGr) xavovLov 8Ld xo exoc;
xo SouXxavLXov £v d) exsGrjaav ol xpovoL dvd x xou fjXLou.
ALaLpeaLc;. Elc; xo yvcipLa^a sxslvo oxl ol X9^^^^ ^'^ aLaGrjxoL fjyouv ol
15 yvcipL^OL ol aouXxavLXOL xaxd TioLav fj^epav slaep^ovxaL duo xcov xpLCOv
xouxcov excov xal xcov fj^epcov xfjc; fepSo^dSoc;
1 aOxaL om Vv || 2 Ilepl] elc, to yvcopta^a L || 6 E E SpXGxyLy v
464
FLvexaL eiaeXeuaic, xax' evavxLov xcov xexeXsLCO^evcov aouXxavLXCov xpovcov
£Lc; x6 xavovLov xcov elxoaaexripLScov xal xcov aiiXcov excov. d xl oOv eOpsGrj,
xax' evavxLov xcov p xavovLCOv, xpaxsLxaL duo xcov y^povcdv xcov y sxslvcov
excov. (baauxcoc; xal al fj^epaL ex TiXayLou xcov xpovcov xal xd a' xal Seuxepa
5 XsTixd. elxa xrjpoOvxaL xal al fj^epaL xfjc; fepSo^dSoc; al xaxd x6 xeXoc; xcov
xavovLCOv xal xd xouxcov ol xal P' XsTixd, xal (be; eaxLV f) xd^Lc; xrjpoOvxaL. edv
oOv 6 (J;fjcpoc; xcov P' Xstixcov tiXslcov xcov ^, xd ^ dcpatpoOvxaL £^ sxslvcov, xal
a TipoaxlGsxaL sic; xd a XsTixd. el Se xaOx' aOGic; TiXelova xcov ^, olko xouxcov
dcpatpoOvxaL xd ^, xal a TipoaxlGsxaL xatc; fj^epaLc;. el he al fj^epaL aOxat
10 TiXsLovec; xcov fj^epcov xoO xp^^ou, al fj^epaL xoO xp^^ou xaxaXt^TidvovxaL,
xal a TipoaxlGsxaL xolc; xpovoLc;. STiSLxa xrjpeLxaL sic; xd XsTixd xcov fj^epcov xfjc;
I fepSo^dSoc; I xd xpaxrjGevxa. edv &aiv eXaxxov xcov ls, f) dpxT) xoO xpovou duo fi22rL, ferrv
xcov I xpaxrjGevxcov fj^epcov sgxl xfjc; fepSo^dSoc;. el Se tiXsov xcov ls, f) dpxT) f293vv
xoO xp^vou duo xfjc; aXXirjc; fj^epac;* ^la fj^epa TipoaxlGsxaL xatc; ebpsQeiaoLic,
15 fj^epaLc; xal sic; [xa6'] exaaxov exoc; duo xcov y ^la fj^epa TipoaxlGsxaL.
ALalpsGLc;. Ilepl xoO yvcovat oxl oOxoc; 6 elaepxo^evoc; xpovoc; TiaaLxd sgxlv
y] xaTiLad
3 xpLCOv Vv II 4 TipcoTa Vv II 5 TrjpoOvTaL ] xpaxsLTaL L II 6 TipcoTa Vv I SeuTspa
Vv II 7 SeuTspcov V II 8 Tipcoxa Vv || i5 xpLCOv Vv II 16 Ilepl ToO yvcovat] sl^ to
yvcopLa^a sxslvo L || it xaiiLaa + f]TOL pLae^xo^ Vv
465
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eXaxxov xcov xoacov E ^£ Xe , oOxoc; 6 elaepxo^evoc; xp^voc; TiaaLxd sgxlv,
xal fj^epaL xoO -/^povou exeivou xoaaL* x^e. el Se exsLva xd XsTixd TiXsLovd
SLGL xcov E ^£ Xe , oOxoc; 6 elaepxo^evoc; xpovoc; xaiiLad sgxl. fj^epaL xouxou
5 xoaaL* x^c; . oOxoc; 6 (J;fjcpoc; sic; x6 ^fjxoc; xcov 9, ou-/} eiq x6 ^fjxoc; xcov exepcov
TioXecov.
KecpdXaLov 8'. Ilepl xoO Gs^eXlou xoO aOGrj^epLvoO xoO tiXlou sic, eva xpovov
xoO tiXlou
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10 tiXlou xal sic; xouc; ^fjvac; xoO xpovou exsLvou. xal oOxol ol ^fjvec; sic; exeivo
exsGrjaav oxl slc; x/jv dpxTjv exdaxou ^rivoc; 6 yjXloc; slc; x/jv dpxTjv ylvexaL xoO
^coSlou. STiSLxa acp' oO e^eXGr] f) dp^T) xoO xpovou xoO tiXlou xaxd Tiolav fj^epav
I eaxl xal tiolov ^fjva xal tiolov xpovov duo xou exouc; xcov Apdpcov, £^ sxslvou fi22vL
xou xp^vou xal xou ^rivoc; xal xfjc; fj^epac; ylvexaL SLaeXeuaLc;, xal al ^saaL
15 XLVTQGSLc; xcov doxspcov xpaxouvxaL xal xd ucj^ci^axa xouxcov sxpdXXovxaL. | xal fervv
al ISLaL XLVTQGSLc; xal sxsLvaL al ^saaL xlvtqgslc; ^exd xfjc; TiepLaasLac; xcov p
^rixcov opGouvxaL (be; eppsGr). xal xo ucj^co^a exdaxou daxepoc; duo xfjc; ^earjc;
4 TOUTOU om Vv II 7 Ilepl] sl^ Trjv xaTdXir](|>Lv xfj^ TioLrjaeco^ L || 9 a L || 15
xpaxoOvTaL tcov daxepcov Vv || 16 5uo Vv || 17 opGoOxaL Vv
466
XLVTQGSCoc; TOUTOU oLc^oLipelioLi. sl XL xaxaXsLcpGrj, toOto xevxpov xolXsItoli. xaOxa
oOv Tidvxa xa expXrjGsvxa ev ovo^a exo\Joiv - Qe\ieXiov xfjc; ocpx'^^ "^^^Ci xp^vou.
xaOxa oOv Tidvxa xiGevxaL sic; x/jv dpxiQ^ "^^^O 3>apPap8LV ^rivoc; xaxd x6 enoq
x6 SouXxavLXov - exaaxov sic; xov ISlov xotiov xaQoyoKsp f)v f) xd^Lc; xouxou
5 - xal eiq x6 xavovLov OTiep eyevexo 8l' sxslvo.
Xpr) oOv SLTiSLv xal Tiepl xcov xavovLCOv tiogcov sgxl xp^^a. Std xd exr) £
xavovLa exsGrjaav xal Std xdc; fj^epac; xfjc; fepSo^dSoc;, xal p xavovta Std x6
xevxpov xal x6 aOGrj^epLvov xoO tiXlou, xavovta £ Std x/jv aeXTQvriv xal x/jv
[xeariv XLvrjaLv exsLvrjc; xal x/jv ISlav XLvrjaLv xal x6 xevxpov xal x6 aOG^epLvov
10 xoO xaxapLpd^ovxoc;. xal exaaxoc; xcov e daxepcov y xavovta £x^^* ^^ Std x6
xevxpov, a Std x/jv ISlav XLvrjaLv, xal a Std x6 aOGrj^epLvov. xal exepa
I xavovLa exsGrjaav ev Std |xriv ^exdxXtaLv xoO tiXlou, ev Std x6 TiXdxoc; xfjc; f294rv, fi23rL
aeXTQvric;, xal £ Std xd TiXdxr) xcov daxepcov. xal exepa p exsGrjaav Std xdc;
oSpac; xfjc; dvapdaecoc;.
15 'EtisI yoOv exsGrjaav xd xavovta Tidvxa xexeXsLCO^eva, exelvo x6 Gs^sXlov,
f) ^ear) XLvrjaLc; xal f) ISla xal xd exepa, sic; x/jv dpxTjv xoO 3>apPap8lv ^rivoc;
ypdcpexaL. STiSLxa ylvexat eiaeXeuaiq eiq x6 xavovLov xfjc; xlvtqgscoc; xcov ^
daxepcov xal xoO xaxapLpd^ovxoc; sic; xouc; ^fjvac; xoO SouXxavLXoO Svexa xoO
Xpovou xoO fjXLOu. xal xax' evavxlov exdaxou ^rivoc; f) XLvrjaLc; xcov daxepcov
3 oOv om Vv II 6 XP^] XP^^^ ^^ II 9 XLvrjaLv om Vv | to auGrj^epLvov + xal to
auGrj^epLvov L || lo TpLCOv L | ey^^i xavovia Yv || 12 a Vv | a Vv || is TaTiXdTr]]
TO TlXdTO^ L
467
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Tcp Ge^eXLcp exsLvcp xcov daxepcov, exaaxov exdaxcp - f) XLvrjaLc; xoO tiXlou xcp
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5 6 (J;fjcpoc; 6 e^ep^o^evoc; xax' evavxLov exdaxou [xrivbq olko xcov xlvtqgscov xcov
daxepcov del svoOxaL xcp Ge^eXLcp exeivou xoO daxepoc;. xal x6 e\jpiax6\ievov
xiGsxaL £Lc; x/jv dpxTjv xoO aOGrj^epLvoO. STiSLxa ytvexaL elaeXeuaLc; sic; xd
xavovLa xcov fj^epcov. xal 6 (J;fjcpoc; xfjc; ^lac; fj^epac; duo xcov p xpaxsLxat.
xal 6 (J;fjcpoc; xcov £ fj^epcov duo xcov c;. xal 6 (J;fjcpoc; xcov l fj^epcov olko xcov
10 La xpaxsLxaL. xal 6 (J;fjcpoc; xcov l£ fj^epcov duo xcov lc; xpaxsLxaL. xal £v
exaaxov | sic; x6 Qe\ieXiov exdaxou ^rivoc; svoOxaL, xal 6 (J;fjcpoc; xfjc; fj^epac; fi23vL
exsLvrjc; ypdcpexat dii' exsLvou xoO ^rivoc;.
'EtisI yoOv eyevexo dSeta xoO (J;7]cpou xfjc; ^earjc; xlvtqgscoc; xal duo xcov
^rivcov xal xcov fj^epcov, STiSLxa ev ev aOGrj^epLvov sxpdXXexaL exdaxou daxepoc;
15 £Lc; x6 ^fjxoc; xal x6 TiXdxoc;* xal sic; x6 TiXdxoc; xfjc; ^earjc; xlvtqgscoc; ypdcpexat
£Lc; x6 xavovLov xoO aOGrj^epLvoO. xouxou Se yevo^evou, STiSLxa 6 (J;fjcpoc; xoO
aOGrj^epLvoO xa6' exdaxriv fj^epav ^spl^exaL dvxLX7](J>£L BeoO.
4 cpapPaSlv L || 6 toO daxepo^] tcov daxepcov v. post quod v add et cancell exaaxov
txaoTCx) XLvrjaL^ toO fjXLou tco Ge^eXLcp toO auGrj^epLvoO toO fjXLou xal xaGs^fj^ || is a Std
L II 17 dvTLXir](|>£L 0£oO] ^exd xfj^ toO GeoO porjGeLa^ xal ev tl Xstitov L
468
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Xal STSpCOV TLVCOV
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TauTa* 6 yjXloc; xal f) aeXTQvr) xal f) XLvrjaLc; toutcov slc; to tiXsov xal sXaTTOv,
5 xal eiq t/jv xaTaXTjcJ^Lv ttjc; Sta^STpou | toutcov xal toO aOGrj^epLvoO toO fesvv
xaTaptpd^ovToc; xal toO aOGrj^epLvoO tcov e daTspcov, xal sic; t/jv xaTaXTjcJ^Lv
TTJc; xaT' 6p66v xlvtqgscoc; tcov doTspcov xal toO OtiotioSlg^oO auTCOv.
'ExsLvcov he tcov doTspcov d)v sxpdXXsTaL to aOGrj^epLvov olko toO TiXaTouc;,
f) aeXTQvr) sgtI xal ol e daTspec; &>v to TiXdToc; | sxpdXXsTaL y] slc; to popsLov 294vv
10 ^epoc; y] £lc; to votlov. TrjpriGevTa he TauTa TidvTa eypdcpriaav sic; Td xavovta
TTJc; opGciaecoc; tcov doTspcov. xaT' evavTLov oOv toutcov slc; t/jv dpxTjv tcov
xavovLCOv I p dXXrjXouxLaL STeGrjaav. xal TauTatc; Tate; Sualv ovo^a STsGr) fi24rL
^STpov. xal 6 (J;fjcpoc; toO xuxXou ( yjtol ttjc; acpalpac; ) TSTsXeLCO^evou evTaOGa
STsGr).
15 'H OL oOv dXXrjXouxLa sic; tov (J;fjcpov tcov ^coSlcov duo toO E y-^XP^ "^^^ ^
^coSlcov, xal 6 (J;fjcpoc; tcov ^otpcov duo ttjc; ^lac; ^olpac; ^^XP^ ^^'^ "^^^ P^- "^"^^
SeuTspac; Se dXXrjXouxLac; 6 (J;fjcpoc; dvTSGTpa^^evoc; duo tcov xdTCO Koio6\ievoq
T/jv dpxTjv Tipoc; Td dvco. f) evap^Lc; exsLvrjc; duo tcov c; ^coSlcov ^^xP^ "^^^ KptoO,
8l' d)v TiXrjpoOTaL xal 6 (J;fjcpoc; ttjc; acpalpac; Tidarjc;. ^STd Se toO (J;7]cpou tcov
1 Ilepl ToO auGrj^epLvoO] sl^ to yvcopta^a tcov auGrj^epLvcov L || 3 Se om. Vv || 8 he
om L II 12 5uo L II 17 5e: om. Vv
469
^oLpcov f) evap^Lc; sxslvcov dmb xcov pnoL [isx9^ "^^^ "^^ ^otpcov sic; xov (J;fjcpov
toOtov xfjc; acpatpac;. xal exepoc; (J;fjcpoc;, el yLvexaL 6 (J;fjcpoc; sic; xa ^cpSta, duo
xfjc; ocpxfjc; xcov 6 ^coSlcov ^exd xfjc; xd^ecoc; xouxcov ^^XP^ "^^^ ^ fjyouv xoO
KpLoO xal xfjc; dp^fjc; xcov y. exeivo yj^lgu Xeyexat ucj^co^a xfjc; acpatpac;, xal
5 ^£xd xoO (J^TQcpou xcov ^OLpcov OLKO xcov GO ^OLpcov Scoc; xcov x^ xal ^^XP^ "^^^
9. xal duo xcov y he ^coSlcov ^^xP^ "^^^ ^ ^coSlcov xal xfjc; dpxfjc; xcov 6 exelvo
XeyexaL yj^lgu xfjc; xdxco acpalpac;, | xal ^exd xoO (J;7]cpou xcov ^OLpcov duo xcov f69rv
9 ^OLpcov ^^XP^ "^^^ P^ ^^'^ ^'^^ '^'^^ ^^ ^olpac;. auxr) f) ^otpa sic; 8 xecpdXata
SLaLpsLxaL.
10 KecpdXaLov a'. | Ilepl xfjc; xaxaXiQcJ^ecoc; xoO aOGrj^epLvoO xoO fjXLOu xal xfjc; fi24vL
aeXTQvric; xal xcov £ daxepcov xal xoO xaxapLpd^ovxoc;. xoOxo x6 xecpdXaLov
£Lc; 8 SLaLpsLxaL.
ALalpsGLc; a'. Ilepl xoO aOGrj^epLvoO xoO fjXLou
BouXo^evcov fj^cov TioLfjaat aOGrj^epLvov xou fjXLou, tioloO^sv ouxcoc;* f)
15 [xeay] XLvrjaLc; xoO fjXLOu £v 8ual ^speaL xlGsxaL xfjc; xauXac;, xal x6 ucj^co^a xoO
4 exsLvo + TO V I u(|>co^a et fi\iio\j transpon. Vv || 6 xpLCOv Vv || 7 XeyexaL + to v
II 14 ToO fjXLOu om. V II 15 TiGsTaL om. Vv
470
tiXlou dcpaLpsLxaL dmb xoO evoc; [xepouc, xfjc; ^earjc; xlvtqgscoc;. el tl xaxaXsLcpGrj,
xevxpov eaxl xoO tiXlou. STiSLxa xax' evavxLov xoO xevxpou xouxou ytvexaL
elaeXeuaLc; sic; x6 xavovLov xfjc; opGciaecoc; xoO tiXlou, xal ^rixsLxaL x6 xevxpov
xoOxo eiq xa p xavovta xfjc; a xal P' dXXriXouxLocc;. £v6a eOpsGfj xax'
5 evavxLov xouxou sic; x/jv y' dXXriXouxLocv, f) opGcoatc; xpaxsLxat, xal olko xfjc;
8' dXXriXouxLac; f) TiepLaasLa xpaxsLxaL* xal xlGevxaL xal xd p sic; x/jv xaOXav.
edv oOv exTl "^^ xevxpov XsTixd ^exd xoO (J;7]cpou xcov p xavovlcov, opGoOxat 6
(J;fjcpoc; xfjc; opGciaecoc;, xal ylvexaL f) xeXela opQcdoiq. STiSLxa xrjpeLxaL. edv x6
xevxpov £v xfj a' dXXrjXouxLa , f) opGcoatc; duo xfjc; [xeariq xlvtqgscoc; dcpatpsLxaL,
10 edv Se sic; x/jv Seuxepav dXXrjXouxLav, svoOxaL x6 xevxpov xfj [xeari xlvtqgsl,
I xal sOpLGxexaL x6 aOGrj^epLvov xoO fjXLou. el he f) opGcoGLc; dcpatpeGfj duo xoO 295rv
xevxpou y] fevcoGfj xouxcp, STiSLxa x6 xsXslov ucj^co^a evcoGfj | xcp xevxpcp xouxcp f69vv
I xcp eOpsGsvxL UGxepov tiXsov y] eXaxxov duo xfjc; ev(i>aecdq y] dcpatpsGecoc;, xal fi25rL
aOGic; £X£Lvo x6 aOGrj^epLvov xoO fjXLou.
15 AtaLpsGLc; P'. Ilepl xoO aOGrj^epLvoO xfjc; gsXtqvtic;
TlGevxaL f) ^SGr) XLvrjGLc; xal f) ISla xal x6 xevxpov xfjc; gsXtqvtic; slc; x/jv
xaOXav xal f) ^SGr) XLvrjGLc; xoO dvapLpd^ovxoc;, iidvxa ISla. STiSLxa xax'
1 a L II 3 xa xavovLa L || 4 TipcoTTTjc; Vv | Seuxepac; Vv || 5 TpLTrjv Vv || 6
TSTdpTir]^ Vv II 7 h6o v || 9 TipcoTir] V || i4 fjXLou + Iv' f] L II 15 SeuTspa V | Ilepl]
£L^ TO yvcopLa^a L || i7 dvapLpdCovTO^] xaxapLpdCovTO^ Vv
471
evavTLov xoO xevxpou yLvexaL eiaeXeuaic, sic, xa xavovta xcov opGciaecov xfjc;
aeXTQvric;, xal ^rixsLxaL exel x6 xevxpov sic; x/jv a xal P' dXXriXouxLocv. £v6a
eOpsGrj xax' evavxLov exsLvou, ytvexaL eiaeXeuaiq eiq x/jv y' dXXriXouxLocv,
xal f) a opGcoGLc; xfjc; aeXrivriq xpaxsLxaL [xstol xoO ^sgou xcov p xavovLCOv
5 (J^TQcpou £X£Lvou. shoi xrjpeLxaL. edv x6 xevxpov sic; x/jv a eOpsGrj dXXriXouxLocv,
f) opGcoGLc; f) a svoOxaL xrj lSloc xlvtqgsl. sl he sic, x/jv P' dXXriXouxLocv,
dcpatpsLxaL xauxTjc;, xal sOpLGxexaL f) ISla xeXela XLvrjGLc;. auxr) xrjpeLxaL. elxa
xax' evavxLov xoO xevxpou ylvexat f) SLGsXeuGLc; sic; x6 xavovLov xfjc; xexapxTjc;
dXXrjXouxLac;, xal xpaxoOvxat xd yevLxd XsTixd xal xlGevxaL sic; ev ^epoc; xfjc;
10 xauXac;. eneiioL xax' evavxlov xfjc; ISlac; xeXelac; xlvtqgscoc; ylvexat SLGsXeuGLc;
£Lc; x6 xavovLov xcov opQo^aecdv xfjc; gsXtqvtic;, xal ^rixsLxaL f) ISla XLvrjGLc;
£Lc; x/jv oi xal P' dXXrjXouxLav | xoO xevxpou. £v6a eOpsGfj, xax' evavxlov fi25vL
£X£Lvou ylvexaL SLGsXeuGLc; sic; x6 xavovLov xfjc; to^tixtic; dXXrjXouxLac;, xal f)
P ' opGcoGLc; xfjc; gsXtqvtic; xpaxsLxat ^£x' exsLvou xoO (J;7]cpou xoO eOpLGXo^evou
15 [xeaov xcov p xavovlcov, xal xlGsxaL sic; ev ^epoc; xfjc; xauXTjc;. auxr) Se sgxlv
f) oO^l xeXela opGcoGLc;. gjiSLxa xax' evavxlov xfjc; ISlac; | xeXelac; xlvtqgscoc; frorv
ylvexaL SLGsXeuGLc; sic; x6 xavovLov xcov dpQ(i>aecdv xfjc; gsXtqvtic; slc; x/jv a' xal
P' dXXrjXouxLav. £v6a eOpsGfj, xax' evaxlov exeivou ylvexat SLGsXeuGLc; sic; x6
I tcl)v opGcoaecov om Vv || 2 TipcoTrjv V | Seuxepav Vv || 3 TpLTrjv Vv || 4 TipcoTr]
Vv II 5 TipcoTTrjv V II 6 TipcoTiT] Vv | SsuTspav Vv II 8 xevxpou + TrjpsLTaL xal V II
12 TipcoTTrjv Vv I SeuTspav Vv || 14 Seuxepa Vv || 15 [liaov om v || 17 TipcoTrjv Vv
II 18 SeuTspav Vv
472
xavovLov xfjc; c^ Qi\\r\ko\jy}QL<^^ xal to eyyuxepov ^fjxoc; xpaxsLxaL — ^otpaL xal
XsTixd. £X£Lvo £Lc; xoc ysvLXoc XsTixa xripsLxaL. d xl eOpsGrj, sxslvo del svoOxaL
xrj P' opGciasL, xal ytvexaL f) P' opGcoatc; xeXeta.
''EjiSLxa xripsLxaL. edv f) ISta xeXeta XLvrjaLc; sic; x/jv a 6XkT\ko\jyiaL\
5 sOpLGxrixaL, f) P' auxr) xeXeta opGcoatc; dcpaLpsLxaL duo xfjc; [lioTf^ xlvtqgscoc;.
£L Se £Lc; x/jv P' Qik\r\ko\jy}QL\ svoOxaL auxr) xrj ^ear] xlvtqgsl, xal sOplaxexaL
x6 aOGrj^epLvov xfjc; P' acpalpac; xfjc; ozkr\\r\<^. si hz pouXriGco^ev TioLfjaat
aOGrj^epLvov sic; x/jv ol acpatpav xfjc; aeXTQvric;, f) \iioT\ XLvrjaLc; xoO
dvapLpd^ovxoc; svoOxaL xcp aOGrj^epLvcp xfjc; aeXTQvric;. d xl eOpsGfj, sxslvo
10 ^oLpd eaxL | xoO TiXdxouc; xfjc; ozkr\\r\<^. si hz x6 aOGrj^epLvov xoO f295vv
xaxapLpd^ovxoc; dcpatpeGfj | duo xoO aOGrj^epLvoO xfjc; aeXTQvric;, xal aOGic; f\ fi26rL
^OLpa exsLVT) eaxl sxslvo xoO TiXdxouc; xfjc; ozkT\\T\<^. STiSLxa xax' evavxlov
£X£Lvou ylvexaL elaeXeuaLc; sic; x6 xavovLov xcov opGciaecov xfjc; aeXTQvric;, xal
^rixsLxaL xoOxo sic; if\\ P' Qik\r\ko\jy}QL\ . svQol eOpsGfj, xax' evavxlov exeivou
15 ylvexaL eiaeXeuaic, sic; x6 xavovLov xfjc; epSo^rjc; dXXrjXouxLac; xfjc; aeXTQvric;,
xal xpaxoOvxaL xd XsTixd xfjc; y opGciaecoc; xfjc; aeXrivriq xal xrjpoOvxaL.
STiSLxa xrjpoOxaL f) ^otpa xoO TiXdxouc; xfjc; aeXrivriq. edv f) eXdxxcov xcov 7
^coSlcov xal TiXecov xcov c; ^coSlcov - eXdxxcov he xcov 6 ^coSlcov, exsLvr) he f) y'
1 exTiT]^ V II 3 SeuTspa Vv | Seuxepa Vv || 4 TipcoTrjv Vv || 5 Seuxepa V || 6
SeuTspav V || 7 Seuxepac; Vv || 8 TipcoTrjv Vv || 9 dvapLpd^ovTOc;] xaxapLpdCovTOc;
Vv II 12 exsLvo om Vv || 14 Seuxepav Vv || 16 TpLTir]^ Vv || 17 f] ] oOv Vv || is
TpLTlT] Vv
473
opGcoGLc; dcpaLpsLxaL dmb xoO aOGrj^epLvoO xfjc; P' acpatpac; xfjc; aeXTQvric;. el 8'
eaxl TiXecov xcov y | ^coSlcov xal eXdxxcov xcov c; y] tiXsov xcov 6 ^coSlcov, auxr) f) frovv
Y opQcdoiq svoOxaL xcp aOGrj^epLvcp xfjc; aeXTQvric;, xal ytvexaL x6 aOGrj^epLvov
xfjc; a acpatpac; xfjc; aeXTQvric;. f) a oOv auxr) xfjc; aeXTQvric; acpatpac; 6p67] sgxl
5 ^£xd xfjc; Gcpatpac; xcov i^ ^coSlcov.
AtaLpeaLc; y'. Ilepl xoO aOGrj^epLvoO xoO xaxapLpd^ovxoc; xal xoO
dvapLpd^ovxoc;
Mexd x6 sxpXrjGfjvaL x/jv ^eariv XLvrjaLv xoO xaxapLpd^ovxoc; (be; eppsGr),
exsLVT) duo xcov i^ ^coSlcov dcpatpsLxaL. d xl xaxaXsLcpGfj, x6 aOGrj^epLvov sgxl
10 xoO xaxapLpd^ovxoc;. c; oOv ^(iSta svoOxaL exsLvcp, xal x6 aOGrj^epLvov xoO
dvapLpd^ovxoc; ylvexaL.
ALalpsGLc; 8'. Ilepl xfjc; xaxXiQcJ^ecoc; xoO aOGrj^epLvoO xcov £ daxepcov
TlGevxaL sic; x/jv xaOXav ISla xal ISla f) ^ear) XLvrjaLc;, f) ISla, xal x6 ucj^co^a
xoO daxepoc;. gjiSLxa x6 ucj^co^a del dcpatpsLxaL olko xfjc; ^earjc; xlvtqgscoc;, xal
15 sOpLGxexaL x6 xevxpov. elxa x6 xevxpov xoOxo ^rixsLxaL sic; xd xavovta xcov
opGciaecov xcov daxepcov sic; x/jv ol y] x/jv P' dXXrjXouxLav xoO ^expou. £v6a
1 SeUTSpa^ Vv || 3 TpiTT] Vv II 4 TipCOTlT]^ Vv | TipCOTlT]^ Vv || 6 TpLTlT] V || 12 xf]^
xaTaXir](|>£co^ om Vv || i6 TipcoTrjv Vv | Seuxepav Vv
474
oOv eOpsGrj, xax' evavxLov exeivou yLvexaL eiaeXeuaic, sic, to xavovLov xfjc; y '
dXXriXouxLocc;, xal xpaxsLxat f) a opGcoatc; — ^otpaL xal XsTixd — ^exd xoO
(J^TQcpou xoO eOpsGsvxoc; [xeaov xcov p xavovLCOv.
''EjiSLxa xripsLxaL x6 xevxpov. edv f) olko xfjc; a dXXriXouxLocc;, f) a opGcoatc;
5 svoOxaL xrj lSloc xlvtqgsl xal dcpaLpsLxaL duo xoO xevxpou. el 8' eaxl x6 xevxpov
duo xfjc; P' dXXrjXouxLocc;, f) a opGcoatc; svoOxaL xcp xevxpcp xal dcpatpsLxaL duo
xfjc; ISlac; xlvtqgscoc;. xal ylvovxaL al p xsXslol. STiSLxa ylvexat eiaeXeuaic, xax'
evavxLov xoO xeXsLou xevxpou sic; x6 xavovLov xfjc; xexapxTjc; dXXrjXouxLac;, xal
xpaxoOvxaL xd yevLxd XsTixd. edv oOv (batv exelvoi yeypa^^eva Std xoxxlvou,
10 TiXeovaa^oc; sgxlv, £l Se Std ^eXavoc;, eXXslcJ^lc;. xaOxa xlGevxaL sic; ev ^epoc;
xfjc; xauXac;. eneiioL \ xax' evavxlov xoO lSlou xeXslou ylvexat elaeXeuaLc; sic; xd frirv
xavovLa xcov opGciaecov sic; x/jv a' xal P' dXXrjXouxLav. £v6a oOv eOpsGfj, xax'
I evavxLov exeivou ylvexat elaeXeuaLc; sic; x6 |xav6vLov xfjc; c; dXXrjXouxLac;. xal f296rv, fi27rL
f) P' opGcoGLc; xpaxsLxaL — ^otpaL xal XsTixd — xal 6 [xeaov xcov p xavovlcov
15 (J;fjcpoc;. auxT) oOv oO^l xeXela Xeyexat opGcoatc;. gjiSLxa TidXtv xax' evavxlov xfjc;
ISlac; xeXelac; xlvtqgscoc; ylvexat eiaeXeuaiq. edv xd yevLxd XsTixd TiXeovaa^oc;
(baLV, xax' evavxLov xoO xavovlou xfjc; ^ ' dXXrjXouxLac; xal xpaxsLxat x6
eyyuxepov ^fjxoc;. el Se xd yevLxd XsTixd eXXslcJ^lc; slglv, slc; x6 xavovLov
1 TpLTlT]^ Vv II 2 TipCOTlT] Vv || 4 TipCOTlT]^ Vv | TipCOTlT] Vv || 6 SsUTSpa^ Vv | TipCOTlT]
Vv II 12 TipcoTTrjv Vv I SeuTspav Vv || 13 exTir]^ v || 14 [J ] Seuxepa V || 17 epSo^r]^
Vv II 18 eyyuTspov] exepov v
475
yLvexaL eiaeXeuaic, xfjc; e dXXriXouxLocc;, xal xpaxsLxaL x6 Tioppco ^fjxoc;. exelvo
oOv x6 e^eXGov del xrjpeLxaL sic; xd yevLxd XsTixd. el xl eOpsGrj, edv xd
yevLxd XsTixd Std xoxxlvou, xoOxo svoOxaL xrj P' opGcoasL. el Se Std ^eXavoc;,
dcpatpsLxaL e'E, exsLvou, xal ytvexaL f) P' opGcoatc; xeXeta. STiSLxa xrjpeLxaL. edv
5 f) ISta xeXsLa sic; x/jv a dXXrjXouxLocv f), t] P auxr) xeXeta opGcoatc; xcp xeXsLcp
xevxpcp svoOxaL. el Se sic; x/jv Seuxepav dXXrjXouxLocv eOpsGrj, dcpatpsLxaL e^
£X£Lvou. STiSLxa svoOxaL del xouxcp x6 ucj^co^a, xal sOplaxexaL x6 aOGrj^epLvov
xoO daxepoc;. f) aOxr) ^sGoSoc; xal sic; xouc; Xomobq daxepac;.
10 KecpdXaLov P'. Ilepl xfjc; xax' opGfjc; xlvtqgscoc; xcov daxepcov xal xoO
OtiotioSlg^oO aOxcov
I 'Eksi xpsLa slSevaL xoOxo, xax' evavxlov xoO xeXsLou xevxpou xoO daxepoc; fi27vL
£X£Lvou ylvexaL eiae\ke\jaic, sic, xd xavovta xfjc; opGciaecoc; xoO daxepoc; sic; frivv
x/jv a' y] P' dXXrjXouxLav. £v6a oOv eOpsGfj, xax' evavxlov exeivou ylvexat
15 elaeXeuaLc; sic; x6 xavovLov xfjc; rj' dXXrjXouxLac;, xal xpaxsLxaL 6 a' axripLy^oc;
xal cpuXdxxexaL. STiSLxa oOxoc; dcpatpsLxaL olko xcov lP ^coSlcov, xal 6 P' ylvexat
axripLy^oc;. elxa xrjpeLxaL f) ISla xeXela XLvrjaLc;. edv s^LaoOxaL xcp a' axripLy^cp,
1 Tie^TiTiT]^ Vv II 3 SeuTspa Vv || 4 SeuTspa Vv || 5 TipcoTrjv Vv | Seuxepa Vv ||
14 TipcoTTrjv Vv I SeuTspav Vv || i5 TipcoTOc; v || i7 Tipcoxcp Vv
476
6 daxrip Igtoltoli fjyouv axripL^eL. xal eneiioL [xeXXei buonohiaoLi. si he f) ihioL
XLvrjaLc; f) TsXeioL tiXslcov toO a axripLy^oO xal eXaxxcov xoO p ' axripLy^oO, 6
daxrip OtiotioSl^sl. £l 8' eaxlv f) ISta auxr) xeXeta XLvrjaLc; xax' evavxLov xoO P'
axripLy^oO, 6 daxrip auripi^ei xal ^sXXsl XLvrjGfjvaL xax' 6p66v. el Se tiXslcov
5 xoO P' axripLy^oO xal eXdxxcov xoO a' axripLy^oO, 6 daxrip xax' 6p66v XLvsLxaL.
ALalpsGLc;. Ilepl xoO eihevoLi fivlxa XLvsLxat xax' 6p66v 6 daxrip xal oxav
OtiotioSl^T]
'Edv 6 daxrip XLvfjxaL xax' 6p66v, xal pouXo^sGa eihevoii kots axpecpexaL, f)
ISla xeXela XLvrjaLc; dcpatpsLxaL olko xoO a' axripLy^oO. d xl xaxaXsLcpGrj, sxslvo
10 ^spl^exaL £Lc; x/jv xaxd x6 vu^QiQ^epov ISlav XLvrjaLv | xoO daxepoc;. d xl e^eXGr], fi28rL
£X£Lv6 eaxL xatpoc; oxl dpx^L OtiotioSl^slv 6 daxiQp. xal edv pouXci^sGa slSevaL
Tioaac; fj^epac; XLVSLxaL xax' 6p66v 6 daxiQp, 6 p ' axripLy^oc; dcpatpsLxaL duo xfjc;
ISlac; xeXelac; xlvtqgscoc;. el xl xaxaXsLcpGrj, ^spl^exaL sic; x/jv ISlav XLvrjaLv xoO
daxepoc; exeivou y]v XLvsLxaL xa6' ev vw/^drwiepov . el xl oOv e^eXGr], exelvoq 6
15 xaLpoc; oaac; fj^epac; XLVSLxaL | xax' 6p66v 6 daxiQp. f296vv
ALalpsGLc;. 'Edv 6 daxrip OtiotioSl^t], xal ^rjxfjxaL tioxs XLvrjOiQaexaL xax'
2 TipCOTOU Vv II 3 SeUTSpOU Vv II 5 SsUTSpOU Vv | TipCOTOU Vv || 9 TipCOTOU Vv |
exsLvo om Vv || lo -13 elc, Trjv . . . [lepi'^eTai om Vv || 11 pouXco^sGa corr.in pouXo^sGa
L II 16 ^LaLpeaL^ + xal L | C>lxf]TaL] hefioei yeviaQai hfikov L
477
6p66v, f) ihioL TsXeioL XLvrjaLc; dmb xoO Seuxepou axripLy^oO dcpaLpsLxaL. d xl
xaxaXsLcpGrj, sic; x/jv | IStav XLvrjaLv y]v XLvsLxaL 6 daxrip xaxd x6 vu^QiQ^epov f72rv
^spL^exaL. d xl xaxaXsLcpGrj, xatpoc; sgxlv oxl 6 daxrip TiXrjpou^evou xouxou
XLvrjOiQaexaL xax' 6p66v. el Se xal Tioaac; fj^epac; OtiotioSl^sl 6 daxrip PouXsl
5 slSevaL, 6 a axripLy^oc; dcpatpsLxaL duo xfjc; IStac; xeXetac; xlvtqgscoc;. d xl
xaxaXsLcpGrj, sxslvo ^epL^exat sic; OTiep TioXXdxLc; dprjxaL. el xl eOpsGrj, sxslvo
xatpoc; eaxLV oxl 6 daxrip OtiotioSl^sl. xal exsLvr) he f) ISta XLvrjaLc; xoO xaxd
vu^QiQ^epov XLVou^evou daxepoc; xoO Kpovou xoarj-E v^, xoO Aloc; xoarj* E
v8, xoO 'Apeoc; xoarj* E xr), xfjc; AcppoSLXTjc; xoarj* E X^, xoO 'Ep^oO xoarj* y
10 c;.
KecpdXaLov y'. Hepl xoO TiXdxouc; xcov daxepcov xoO popsLou xal xoO voxlou fi28vL
ToOxo xpL^coc; SLrjpsGrj.
ALalpeaLc; a . Ilepl xoO TiXdxouc; xfjc; aeXiQvrjc;
To aOGrj^epLvov xoO dvdpLpd^ovxoc; dcpaLpsLxaL duo xoO aOGrj^epLvoO xfjc;
15 aeXiQvrjc;, xal fj ^otpa xoO TiXdxouc; xaxaXL^TidvexaL, y] svoOxaL fj ^earj XLvrjaLc;
3 xaipoc, eaxLv] f] wpa Vv | TiXrjpou^evr]^ Tauxr]^ Vv || 4 PouXsl] hefioei yeviaQai
hfikov L II 5 TipcoTO^ Vv II 14 xaTapLpd^ovTO^ L
478
ToO dvapLpd^ovToc; xcp aOGrj^epLvcp xfjc; aeXTQvric;, xal f) [xolpoL xoO TiXdxouc;
yLvexaL StqXt). STiSLxa xax' evavxLov xfjc; ^otpac; xoO TiXdxouc; ytvexaL elaeXeuaLc;
£Lc; xd xavovLa xfjc; opGciaecoc; xfjc; aeXTQvric; sic; x/jv a xal P' dXXrjXouxLocv. £v6a
oOv eOpsGfj f) ^OLpa xoO TiXdxouc;, xax' evavxLov exsLvrjc; ytvexaL elaeXeuaLc; sic;
5 x6 xavovLov xfjc; rj' dXXrjXouxLocc;, xal x6 TiXdxoc; xpaxsLxaL xfjc; aeXrivriq [xstol
xoO eOpsGsvxoc; (J;7]cpou [xeaov xcov p xavovlcov. STiSLxa xrjpeLxaL f) ^otpa xoO
TiXdxouc;. eliiep eaxlv sic; x/jv a' dXXrjXouxLav x6 TiXdxoc; popsLov, el he sic; x/jv
P' x6 TiXdxoc; £Lc; x6 | voxlov ^epoc;. xal si eaxLV duo xoO E t^^XP^ "^^^ T ^^S^cov f72vv
Popela eaxlv dvdpaatc;, el he olko xcov y ^^XP^ "^^^ ^ Popela xaxdpaatc;, el Se
10 duo xcov c; ^coSlcov eaxl ^^XP^ ^^'^ "^^^ ^ voxla xaxdpaatc;, el he duo xcov 6
^coSlcov eaxl ^^XP^ "^^^ ^ voxla dvdpaatc;.
ALalpsGLc; P'. I Ilepl xoO TiXdxouc; xcov daxepcov xcov dvco xoO fjXLOu — xoO fi29rL
Kpovou, xoO Aloc;, xal xoO 'Apeoc;
To xevxpov x6 xsXslov ^rixsLxaL sic; xd xavovta xcov opGciaecov xcov daxepcov
15 £Lc; x/jv a' xal x/jv P' dXXrjXouxLav sic; xov Kpovov xal xov Ala. edv oOv x6
xevxpov eOpsGfj sic; x/jv ol dXXrjXouxlav, xax' evavxlov xfjc; 6' dXXrjXouxlac;
ylvexaL elaeXeuaLc;, xal xpaxoOvxat xd yevLxd XsTixd. ei he x6 xevxpov sic; x/jv
3 TipcoTTrjv Vv I SeuTspav Vv || 5 oySorjc; Vv || 7 TipcoTrjv Vv || 8 Seuxepav Vv
II 11 sail om Vv || i4 to tsXslov xevxpov Vv || i5 TipcoTrjv Vv | Seuxepav Vv || i6
TipcoTTrjv Vv I svdTir]^ Vv || 478 .17 -479.2 el he to xevxpov . . .xa yevLxa XsTixa in marg v
479
P' dXXriXouxLocv eOpsGrj, xax' evavxLov xoO xavovLou xfjc; l' dXXriXouxLocc; ytvexaL
elaeXeuaLc;, xal xpaxoOvxat xd yevLxd XsTixd. STiSLxa xfjpsLxaL. edv xd yevLxd
XsTixd Std xoxxLvou x6 TiXdxoc; popsLov, el he Std ^eXavoc; x6 TiXdxoc; voxlov.
£X£Lvo xiGsxaL lSloc £lc; £v ^epoc; xfjc; xauXac;. STiSLxa f) ISta xeXeta XLvrjaLc;
5 ^rixsLxaL £v xolc; xavovLOLc; xcov opGciaecov | sic; x/jv a xal [3 dXXrjXouxLocv. £v6a 297rv
eOpsGrj, xax' evavxLov exsLvou ytvexaL elaeXeuaLc;, xal xpaxsLxaL x6 TiXdxoc; x6
VOXLOV.
Elc; he xov 'Apea xax' evavxlov xoO xeXelou xevxpou ylvexat eiaeXeuaiq eiq
xo xavovLov xfjc; 6' dXXrjXouxLac;, xal xpaxoOvxat xd yevLxd XsTixd. edv &ai
10 hioL XOXXLVOU xo TiXdxoc; popsLov, ei he Std ^eXavoc; xo TiXdxoc; voxlov. STiSLxa
xax' evavxLov xoO lSlou | xeXslou ylvexat eiaeXeuaici. edv xd yevLxd XsTixd frsrv
Std XOXXLVOU, £Lc; xo xavovLov xfjc; i \ dXXrjXouxLac;, xal xo popsLov xpaxsLxat fi29vL
TiXdxoc;. ei he hia ^eXavoc;, xauxa elc; xo xavovLov xfjc; La' dXXrjXouxLac;, xal
xpaxsLxaL £X£l6£v xo voxlov TiXdxoc;. eneiioL xd yevLxd XsTixd xrjpouvxaL elc; xo
15 TiXdxoc;, xal euplaxexaL xo xsXslov TiXdxoc; dxe voxlov elie popsLov sgxlv.
El he xal heriaei SfjXov yeveaGaL oxl dvdpaalc; sgxlv y] xaxdpaoLc;, xrjpeLxaL.
edv xo ISlov xsXslov eXaxxov xcov c; ^coSlcov xal xo TiXdxoc; popsLov, sxslvo
dvdpaalc; eaxL popela. ei he xo TiXdxoc; voxlov, xaxdpaaLc; voxla. ei he xo
ISlov xsXslov tiXsov xcov c; ^coSlcov xal xo TiXdxoc; popsLov, xaxdpaalc; sgxl
I p ] SeuTspav V | toO xavovLou om v | SexdTir]^ V || 5 TipcoTrjv Vv | Seuxepav Vv
II 9 ff om. Vv II 12 SexdTir]^ Vv 12-13 xal to popsLov. . .xfj^ La' dXXrjXouxLa^ in marg
V II 13 evSexaTiT]^ V
480
PopsLa. si he to TiXdxoc; votlov, dvdpaaLc; voxta.
AioLipeaic, TpLxr). Ilepl xoO TiXdxouc; xfjc; AcppoSLxrjc;
AuxT) xpta TiXdxT) £x^^-
nXdxoc; a . FLvexaL elaeXeuaLc; sic; xd xavovta xfjc; AcppoSLXTjc; (be; eppsGr)
5 dvco. xal xax' evavxLov xoO xeXsLou xevxpou ytvexaL eiaeXeuaiq eiq x6
xavovLov xfjc; Ly' dXXrjXouxLocc;, xal xpaxoOvxat xd XsTixd xoO TiXdxouc;. xoOxo
Se x6 TiXdxoc; del popsLov. xal xrjpoOvxaL sic; ev ^epoc; xfjc; xauXac;.
nXdxoc; P'. ''EjiSLxa xax' evavxlov xoO lSlou xeXslou ylvexaL eiaeXeuaiq
eiq xd xavovLa xfjc; 6' dXXrjXouxLac;, xal xd yevLxd XsTixd xpaxoOvxat xal
10 xrjpoOvxaL sic; ev ^epoc; xfjc; xauXac;. xal x6 arj^SLOv xouxou xpaxsLxaL ouxcoc;*
edv x6 xevxpov sic; x/jv a' dXXrjXouxLav eaxl x6 arj^SLov sxslvo a, el Se sic;
x/jv P' I dXXrjXouxLav | x6 xevxpov x6 arj^SLov exelvo p. sxslvo x6 arj^SLov f73vv,fi30rL
xpaxsLxaL. STiSLxa xax' evavxlov xoO lSlou xeXslou ylvexat elaeXeuaLc; eiq x6
xavovLov xfjc; l' dXXrjXouxLac;, xal xpaxsLxaL x6 TiXdxoc;.
15 Elxa xal xoOxo xpaxsLxaL ouxcoc;* edv x6 ISlov slc; x6 dvco fj^LacpaLpLov x6
arj^SLov £X£Lvou a, si he sic; x6 xdxco fj^LacpaLpLov x6 arj^SLov exeivou p.
x6 arj^SLOv xoOxo xpaxsLxaL. STiSLxa x6 TiXdxoc; xoOxo xrjpeLxaL eiq xd yevLxd
9 svdTir]^ Vv II 10 post xal v add et cancell uXoltoc, \\ ii TipcoTrjv Vv || 12 Seuxepav
V II 14 l' ] SexaTiT]^ Vv || 15 xal om. Vv
481
XenTOL xa xpaxriGevTa 8l' aOxo, xal ebpiaxsTOLi to TiXdxoc; x6 xsXslov. xal
£X£Lvo cpuXdxxexaL | xal xrjpeLxaL. STiSLxa edv xd Suo arj^SLa pp y] xal xd Suo 297vv
aa x6 TiXdxoc; popsLov, el Se x6 ev p xal x6 exepov a x6 TiXdxoc; voxlov.
nXdxoc; Y' Kaxd x6 y' ylvexaL eiaeXeuaiq xax' evavxlov xoO xeXsLou
5 xevxpou £Lc; x6 xavovLov xfjc; La' aXXriXouxtac;, xal xd yevLxd XsTixd
xpaxoOvxaL. xal x6 arj^SLov exsLvou - edv sic; x6 dvco fj^LacpaLpLov - a, si
he sic, x6 xdxco fj^LacpaLpLov p. xaOxa xrjpoOvxaL. eneiioL xax' evavxlov xoO
lSlou xeXsLou ylvexat elaeXeuaLc; sic; x6 xavovLov xfjc; lP' aXXriXouxtac;, xal
x6 TiXdxoc; xpaxsLxaL. x6 arj^SLov exeivou xoOxo. edv x6 ISlov eiq x/jv a'
10 dXXriXouxLav eaxl a, el Se sic; x/jv P' p.
Elxa xouxou x6 TiXdxoc; sic; xd yevLxd XsTixd xouxou xpaxsLxaL. xal x6
xeXsLov I sOplaxexaL TiXdxoc;. STiSLxa xrjpeLxaL. edv xd p arj^SLa s^LaoOvxaL x6 fisovL
TiXdxoc; £Lc; x6 popsLov ^spoc;, el 8' oOx s^LaoOvxaL x6 TiXdxoc; sic; x6 voxlov.
Elxa xal xd y TiXdxr) xlGevxaL ISla xal ISla sic; x/jv xaOXav. edv oOv &ai xal
15 xd y popsLa, xal xd y evoOvxat. xal | sOplaxexaL xo TiXdxoc; xfjc; AcppoSLXTjc;. el f74rv
he dXXo [xev TiXdxoc; sic; voxlov, dXXo he popsLov, xpaxsLxaL ISla xoO popelou
xal ISla xoO voxlou. STiSLxa xrjpeLxaL. otiolov sgxlv eXaxxov dcpaLpsLxaL xoO
TiXsLovoc;. el xl xaxaXsLcpGfj, iiXdxoc; eaxl xfjc; AcppoSLXTjc; eiq exelvo xo ^epoc;
£v6a f)v xo TiXdxoc; tiXsov. ei 8' elal xal xd Suo e^Laou^eva y] popeta y] voxta,
2 p VL II 4 xpLTOv Vv II 5 evSexaTiT]^ Vv || 9 TipcoTTrjv Vv II 10 SeuTspav Vv
12 h6o Vv II 14 xpta Vv || i5 xpta Vv | xpta Vv
482
f) 'AcppoSLTTjc; TiXdxoc; oOx ex^^-
AioLipeaic, y'. Ilepl xoO TiXdxouc; xoO 'Ep^oO
OOxoc; xpta TiXdxr) £x^^-
nXdxoc; a . Kax' evavxLov xoO xeXsLou xevxpou ytvexaL eiaeXeuaiq eiq x6
5 xavovLov xcov opGciaecov xoO 'Ep^oO. xal £v6a eOpsGrj sic; x/jv P' y] x/jv a
dXXriXouxLocv, xax' evavxLov exsLvou ytvexaL elaeXeuaLc; sic; x6 xavovLov xfjc; ty'
dXXrjXouxLocc;, xal xpaxoOvxat xd yevLxd XsTixd xoO TiXdxouc; xal cpuXdxxovxaL.
xaOxa del sic; x6 voxlov ^epoc; eiaiv.
nXdxoc; P'. Kax' evavxlov xoO xeXsLou xevxpou ylvexat elaeXeuaLc; sic; x6
10 xavovLov xfjc; 6' dXXrjXouxLac;, xal xpaxoOvxat xd yevLxd XsTixd xal xrjpoOvxaL.
xal x6 arj^SLov exsLvou | xoOxo* edv x6 xevxpov sic; x/jv a' dXXrjXouxLav p, fisirL
£L Se £Lc; x/jv P' dXXrjXouxLav a. xaOxa xrjpoOvxaL. STiSLxa xax' evavxlov xoO
lSlou xeXsLou ylvexat eiaeXeuaiq eiq x6 xavovLov xfjc; i dXXrjXouxLac;, | xal f298rv
xpaxsLxaL x6 TiXdxoc;. x6 arj^SLov exeivou xoOxo* edv x6 ISlov eiq x6 dvco
15 fj^LGcpaLpLov a, si he sic; x6 xdxco fj^LacpaLpLov p. eneiioL x6 TiXdxoc; sic; xd
yevLxd XsTixd xouxou xrjpeLxaL, xal sOplaxexaL x6 xsXslov TiXdxoc;.
Elxa xripsLxaL. edv xal xd p arj^SLa s^LaoOvxaL x6 TiXdxoc; popsLov, el 8' oOx
2 Tiepl + ToO yvcopLa^axoc; L || 5 Seuxepav Vv | TipcoTrjv Vv || 9 ^ ] xaxa to [I L
II 10 EVOLTTlC, Vv II 11 TipCOTTrjV Vv || 12 SsUTSpaV Vv II 13 SexaTlT]^ Vv II 14 TOUTO
om. V II 16 XsTixa post toutou V || i7 5uo Vv 17-483. i TO TiXdTOc; . . . e^LaoOvTat to
in marg v
483
s^LGoOvxaL TiXdxoc; votlov.
nXdxoc; y'. AOGlc; yLvexaL elaeXeuaLc; xax' evavxLov xoO xeXsLou xevxpou | f74vv
eiq x6 xavovLov xfjc; La dXXriXouxLocc;, xal xd yevLxd XsTixd xpaxoOvxat. x6
arj^SLov £X£Lvo* edv sic; x6 dvco fj^LacpaLpLov a, el Se sic; x6 xdxco fj^LacpaLpLov
5 x6 xevxpov p. xaOxa xpaxoOvxat. STiSLxa xaxd x6 P' xax' evavxLov xoO lSlou
xeXsLou yLvexaL elaeXeuaLc; sic; x6 xavovLov xfjc; lP' dXXrjXouxLocc;, xal xpaxsLxaL
x6 y'jiXdxoc; xoO 'Ep^oO. xoOxo TiXdxoc; 00^1 xsXslov XeyexaL.
'Eksi he -/^peioi eihevoii x/jv opGcoatv xouxou, sxslvo x6 TiXdxoc; sic; p ^epr)
xiGsxaL, xal x6 ev xrjpeLxaL. x6 he enepov xrjpeLxaL sic; xd c; XsTixd. el xl eOpsGrj,
10 opGcoGLc; eoTi xoO TiXdxouc; exeivou. eneiioL xrjpeLxaL. edv x6 xsXslov xevxpov
xoO 'Ep^oO £Lc; x6 dvco fj^LacpaLpLov, f) opGcoatc; auxr) duo xoO xplxou xouxou
TiXdxouc; xoO | xrjpriGevxoc; dcpaLpsLxaL. ei he eiq x6 xdxco fj^LacpaLpLov, svoOxaL fisivL
xouxcp, xal x6 TiXdxoc; ylvexat xsXslov eiq x/jv opGcoatv xauxriv.
ToOxo x6 TiXdxoc; xrjpeLxaL. elxa xrjpeLxaL. edv x6 ISlov eic, x/jv a'
15 dXXrjXouxLav x6 arj^SLov xouxou p, ei he eic, x/jv P' dXXrjXouxLav a. STiSLxa
xoOxo x6 TiXdxoc; xrjpeLxaL eiq xd yevLxd XsTixd xouxou, xal sOplaxexaL x6
TiXdxoc; x6 xeXsLov.
TripsLxaL he STiSLxa. edv (bat xal xd p arj^SLa e^Laou^eva x6 TiXdxoc; popsLov,
3 evSexaTiT]^ Vv || 5 Seuxepov Vv || 6 SuoSexdTir]^ Vv || 7 xpLxov Vv || 8 slSevaL
Trjv opGcoaLv] xfjc; opGcoaecoc; Vv | 5uo Vv || 9 to ht exepov TrjpsLTaL om Vv || 12
Tir]pir]6£VTO^ ] prjGsvTO^ Vv || 14 TipcoTrjv Vv || 15 Seuxepav Vv || 16 -17 to tsXslov
TiXdTO^ Vv II 18 h6o Vv
484
si 8' oOx s^LGoOvxaL to TiXdxoc; votlov. aOGic; Se xal xa y TiXaxr) xiGevxaL lSloc
£Lc; x/jv xaOXav xal xrjpoOvxaL. eav xal xa y &ai voxta, svoOxaL xa y, xal
ebpiaxsTOii x6 xsXslov TiXdxoc; xoO 'Ep^oO sic; x6 voxlov [xepoq. el 8' sgxl xl
eiq x6 popsLov ^epoc; xal xl eiq x6 voxlov, olov sgxlv eXaxxov dcpaLpsLxaL xoO
5 TiXsLovoc;, xal sOpLGxexaL xo TiXdxoc; xoO 'Ep^oO eiq xo tiXsov ^epoc;. | el 8' frsrv
s^LGoOvxaL xo popsLov xal xo VOXLOV, 6 'Ep^fjc; oXcoc; TiXdxoc; oOx ex^^-
'Eiiei he xp^loc £L8£vaL x/jv dvdpaGLv xal xaxdpaGLv xfjc; 'Acppo8Lxric; xal xoO
'Ep^oO £Lc; xo TiXdxoc;, xo TiXdxoc; sxslvcov sxpdXXexaL eiq [xioiv oSpav. STiSLxa
dii' exsLvrjc; xfjc; fj^epac; ^exd TiapeXeuGLv Ixavcov fj^epcov aOGLc; sxpdXXexaL
10 xo TiXdxoc; xouxcov. edv oOv xo TiXdxoc; popsLov xal xo expXrjGsv STiSLxa tiXsov
dvdpaGLc; sgxl xoO TiXdxouc;, el 8' eXaxxov xaxdpaGLc;. ei he xo | TiXdxoc; voxlov, fi32rL
I xo ex^XQev eiq xo P' edv f) tiXsov xaxdpaGLc; sgxlv, ei he eXaxxov dvdpaGLc;. ei 298vv
88 xo expXrjGsv a TiXdxoc; popsLov xal xo expXrjGsv STiSLxa voxlov 6 dGxrip xfjc;
Popelac; xaxapdGSCOc;, ei he xo expXrjGsv Tipoxepov voxlov xal xo p ' popsLov f)
15 dvdpaGLc; voxla.
KecpdXaLov 8' . Ilepl xfjc; xaxaX7](J>£C0c; xfjc; ^sxapdGSCOc; fjXLOu xal gsXtqvtic; xal
xfjc; 8La^£xpou - xouxcov ^exd xoO (J;7]cpou xal 8Ld xcov xavovLCOv
1 xpta Vv II 2 xpta Vv | voxLa] c; sup o v | xpta Vv || 7 'Eiid ht xp^^ot SL^evaL]
Xpeta^ yevo^evr]^ elc, to slSevaL Vv || 12 Seuxepav Vv || 13 Tipcoxov Vv || 14 Seuxepov
Vv
485
'H XLvrjaLc; xcov daxepcov sic; to aOGrj^epLvov duo xoO \ieao\j xfjc; fj^epac;
^£XP^ ^^'^ "^^^ STspou ^eaou xfjc; fj^epac; [iSTOL^oiaic, XeyexaL. el yoOv SsTQasL
x/jv ^sxdpaaLV xoO daxepoc; sic; x/jv ^Lav oSpav xaxaXrjcpGfjvaL, ^epL^exat f)
xoLauxT) xoO daxepoc; ^exdpaatc; sic; xd x8.
5 AtaLpeaLc;. 'Eksi xp^^v slSevaL x/jv Std^expov xoO tiXlou Std x/jv exXslcJ^lv, f)
^sxdpaaLc; exsLvou xrjpeLxaL sic; xd vr). d xl eOpsGrj, ^epL^exat sxslvo slc; xd
p£ YJyouv I a ^£ ^oLpac; xal XsTixd. el xl e^eXGr], Std^expoc; sgxl xoO tiXlou. frsvv
dXXcoc;* f) ^exdpaoLc; xoO tiXlou xrjpeLxaL sic; x/jv ^tav oSpav sic; xd vy' XsTixd.
el XL eOpsGrj, ^spL^exaL sic; xd 8 xal f) SLd^expoc; yLvexaL xoO tiXlou.
10 ALaLpsGLc;. Elc; x/jv aeXTQvriv
'Eiiei hel eihevoLi x/jv SLd^expov xfjc; aeXTQvric; 8Ld xdc; exXslcJ^slc;, f) ^sxdpaaLc;
xauxTjc; xripsLxaL elc; xd e. el xl eupsGfj, ^spL^exaL elc; xd pxa fjyouv p a
^oLpac; xal XsTixd, xal f) SLa^expoc; xfjc; aeXrivriq ylvexaL. el Se pouXco^ev | olko fi32vL
xfjc; SLa^expou xauxrjc; elc; xaxaXTjcJ^LV eXQeiv xfjc; SLa^expou xou axLaa^axoc;,
15 f) SLa^expoc; xfjc; aeXTQvric; xrjpeLxaL elc; xd Ly. el xl eupsGfj, ^spl^exaL elc; xd £,
xal supLGxexaL f) SLa^expoc; xou axLda^axoc;. xouxo he elc; x/jv exXei(\)iv xfjc;
5 'Etisl xp^<j^v SL^evaL Trjv ^Ld^expov] Tiepl xfj^ ^La^expou Vv || 6 sxslvo om Vv || ii
'Etisl hei SL^evaL Trjv ^Ld^expov] xP^^o^^ yevo^evr]^ xfj^ ^La^expou Vv
486
aeXr]vr](; XuaiieXel.
AtaLpeaLc;. Elc; xriv xaxdXricJ^Lv xfjc; ^exapdaecoc; xoO tiXlou xal xfjc; aeXTQvric;
xal xfjc; SLa^expou xouxcov omb xoO xavovLou Std xov yjXlov
FLvexaL eiaeXeuaiq xax' evavxLov xoO xevxpou exeivou eiq x6 xavovLov xfjc;
5 [xsTOi^oiaecdq fjXLOu xal aeXTQvric; xal xfjc; SLa^expou xal xoO axtda^axoc;, xal
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xax' evavxLov exeivou xpaxsLxaL f) ^sxdpaaLc; xoO fjXLOu elc; x6 £v vu^QiQ^epov
xal £Lc; x/jv ^lav oSpav, xal f) Std^expoc; exsLvou ^exd xfjc; opGciaecoc; xoO
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487
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5 xecpdXaLa.
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acpatpac; xcov ^coSlcov fjyouv xcov dxpcov xfjc; xepxtSoc; 8l' fjc; XLVSLxaL f) acpatpa.
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xal dcpaLpsLxaL xoOxo olko xcov 9 . el xl xaxaXsLcpGfj, f) dvdpaalc; sgxl xoO xotiou
xcov dxpcov.
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488
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5 xoO xo^ou £X£Lvou fjxLc; eaxl ^exa^u xfjc; Tuyjiq xal xoO l' olxiQ^axoc;. el xl
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ALalpsGLc; y'. Ilepl xfjc; xaxaXiQcJ^ecoc; xcov y ycovLCOv duo xoO tiXslovoc; xal
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10 xal f) xu^TQ "^oO xatpoO xoOxo* c; E E , f) dvdpaalc; eaxL E duo xoO Kapxlvou
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15 f) ycovla xoO TiXdxouc;. el Se f) xu^iQ "^oO xatpoO oOx eaxLV sic; x6 E xoO KptoO
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5 Sexdiou V II 6 e'^eXQji + f] Vv || 7 xfj^ xaTaXir](|>£co^ om Vv | xptcov Vv
Tipcoxf]^ Vv
489
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xoO I OLXTQ^axoc;. xal x6 ^fjxoc; x6 ^exa^u y] xoO KptoO y] xoO ZuyoO xal
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10 xpaxTjXaLa xcov p ^rixcov. elxa f) xpaxTjXaLa xoO xotiou xfjc; xuxtjc; ^epL^exat
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5 xou xavovLou
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10 Std x/jv aeXTQvriv duo xfjc; y' xal 8' dXXrjXouxLac;. xal xlGevxaL Tidvxa elc;
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15 xfjc; 8' dXXrjXouxLac;. d xl oOv eOpsGfj, evoOxat elc; sxslvov xov (J;fjcpov xov
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10 pa6^6v eXaxxov xpaxsLxaL, xal x6 xaxaXsLcpGsv xpaxTjXaLa xoO tiXslovoc; xal
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f)v exsLVT), xal xoOxo xoO TiXdxouc;.
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12 f] om. Vv II 15 SeuTspov v
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6 yjXloc; xpaxsLxaL xal xlGsxaL sic; x/jv xaOXav. STiSLxa f) oSpa xfjc; auvoSou xal
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eXdxxcov dcpatpsLxaL xfjc; tiXslovoc;. d xl oOv xaxaXsLcpGfj, sxslvo f) oSpa eaxl
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14 xf]^ 6(|>£co^ om. Vv I Tico^] Tiepa L || i7 5uo Vv
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fj^epac; sgxlv.
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£X£Lvo x6 xavovLov ^rixsLxaL x6 ^6)8lov ev d) sgxlv f) aeXTQvr). xal xax' evavxlov
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exsGrjaav arj^SLa axLy^at* o o oo. exel oOv £v6a | sOpsGcoaLV al axty^al aOxat f79rv
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xal x6 exepov sic; xd XsTixd xoO ^tqxouc; xfjc; oSpac; exsLvrjc; xfjc; TipcixTjc; ^eaov
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edv f) e^LGOu^evov exsLvcp xcp ^epsL xcp cpuXaxxo^evcp, fjSr) cpavepov eyevexo
10 oxL TiXeov xal eXaxxov xfjc; ocj^ecoc; oOx eaxLv el Se oOx s^LaoOxaL, f) ^ear) xcov
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15 xoO ^coSlou £X£lvou £lc; x6 xavovLov xoO tiXslovoc; xal eXdxxovoc; xfjc; ocj^ecoc;,
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1 xaxa TioXu om Vv || 5 h6o Vv | h6o Vv || 9 tco [lipei tco cpuXaTTO^evcp ] tco
cpuXaTTO^evcp [lipei L || ii 5uo v || 494 .13 -495.9 AtaLpeaL^. . . tvomai toutco om Vv
495
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xal eXaxxov xfjc; ocj^ecoc; x6 duo xoO ol ^coSlou tiXsov eaxl xoO P' tiXslovoc; xal
eXdxxovoc;, f) opQcdoiq auxr) dcpatpsLxaL £^ exsLvou* el 8' eXaxxov, f) opGcoatc;
I svoOxaL xouxco. fisrrL
10 ALalpsGLc;. Ilepl xfjc; opGciaecoc; xcov p TiXaxcov
'Edv x6 TiXdxoc; xoO xavovlou xouxou xoO tiXslovoc; xal eXdxxovoc; xfjc;
6(J;£Cl)c; s^LaoOxaL xcp TiXdxsL xfjc; tioXscoc; fjc; pouXo^sGa, 6 (J;fjcpoc; duo xoO
xavovLou xouxou xpaxsLxaL* el 8' oOx s^LaoOxaL x6 TiXdxoc; xoO xavovlou ^exd
xoO TiXdxouc; xfjc; tioXscoc;, ^rixsLxaL TiXdxoc; sic; x6 xavovLov xoOxo eXaxxov xfjc;
15 TioXecoc; xal eyyuxepov xauxTjc;. elxa ^rixsLxaL £v xcp xavovlcp exepov TiXdxoc;
TiXsLov xoO TiXdxouc; xoO a', xal f) ^ear) xcov 860 TiXaxcov xoO tiXslovoc; xal
eXdxxovoc; Kepiaaeioi xpaxsLxaL. STiSLxa xpaxsLxaL xal f) ^ear) xoO TiXdxouc; xfjc;
KoXecdq xal xoO eXdxxovoc; TiXdxouc; xoO xavovlou TiepLaasLa yjxlc; xal xrjpeLxaL
10 h6o Vv II 11 TOO TOUTOU V II 16 TipCOTOU Vv
496
£Lc; £X£Lvriv xriv nepiaaeioLv. el tl oOv eOpsGrj, ^spL^exaL sic; xriv TiepLaasLav xcov
P TiXaxcov xcov xavovLCOv. d xl xaxaXsLcpGrj, opGcolatc; sgxlv. STiSLxa duo xcov p f79vv
TiXaxcov xcov £v xcp xavovLcp xpaxrjGevxcov dcp' &>v expaxT^Gr) f) TiepLaasLa exsLvr),
edv f) 6 (J;fjcpoc; | xoO a TiXdxouc; tiXsov xoO P' , f) opGcoatc; auxr) dcpatpsLxaL duo fsoirv
5 xoO a TiXdxouc;* el 8' eaxlv x6 a TiXdxoc; eXaxxov xoO P', f) opGcoatc; svoOxaL
xouxcp, xal x6 ebpsQev tiXsov xal eXaxxov xfjc; ocj^ecic; sgxlv. 6 (J;fjcpoc; Se oOxoc;
eaxLv oxav f) aeXTQvr) sic; x6 u(J;co^a xoO ^LxpoO xuxXou exsLvou f).
AtaLpeaLc;. Ilepl xfjc; opGciaecoc; xoO tiXslovoc; xal eXdxxovoc; xfjc; ocj^ecoc; ^exd
xoO xoTiou xfjc; aeXTQvric;
10 I FLvexaL eiaeXeuaic, sic; x6 xavovLov xfjc; ^exapdaecoc; fjXLOu xal aeXTQvric; xfjc; fisrvL
SLa^expou xal xoO axtda^axoc;. xal xax' evavxlov xoO lSlou xfjc; aeXTQvric; y]
xfjc; dvapdaecoc; xauxTjc; ylvexaL eiaeXeuaic, sic; xd xavovta y] xoO lSlou y] xfjc;
dvapdaecoc; xfjc; aeXTQvric;, xal xax' evavxlov exeivou xpaxoOvxat xd XsTixd xd
eOpsGevxa ev xcp xavovlcp xoO tiXslovoc; xal eXdxxovoc; xoO lSlou xfjc; aeXrivriq.
15 d XL oOv eOpsGfj, sic; xoOxo xrjpeLxaL x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; xal
xoO ^TQXouc; xal xoO TiXdxouc; ISla xal ISla. eneiioL x6 eOpsGev x6 tiXsov xal
eXaxxov xfjc; ocj^ecic; sgxlv xexeXsLCO^evov. xoOxo cpuXdxxexaL Std x/jv exXslcJ^lv
2 5U0 Vv I h6o Vv II 4 TipCOTOU Vv I SeUTSpOU V II 5 TipCOTOU Vv I TipCOTOV Vv
I SeuTspou Vv II 7 fi] eaxLV L || lo xa xavovta Vv
497
ToO tiXlou.
KecpdXaLov y'. Ilepl xfjc; dacpaXoOc; tioltqgscoc; toO totiou xfjc; aeXTQvric; sic; to
^fjxoc; xal TiXdxoc;
'Eiiei xpeioL xeveoQoLi spyaaLav, TTipelioLi. edv to ^fjxoc; xfjc; aeXTQvric; duo
5 xfjc; Tuyjiq eXaxxov xcov 9 ^oLpcov, evoOxat xo tiXsov xal eXaxxov xfjc; ocj^ecoc;
exeLvrjc; sic; xo ^fjxoc;, sic; xo aOGrj^epLvov exeLvrjc; fjyouv xfjc; aeXTQvric;- el Se
TiXeov, dcpatpsLxaL e^ exsLvou xoO aOGrj^epLvoO. d xl eOpsGfj, 6 xotioc; | eaxl fsorv
xfjc; 6(J;£C0c; xfjc; aeXTQvric;.
AtaLpeaLc;. Ilepl xfjc; axepedc; tioltqgscoc; xoO xotiou xfjc; aeXrivriq eiq xo TiXdxoc;
10 IIpo xoO spydaaaGaL x/jv xsxvtjv xauxriv Set yvcovat xo tiXsov xal eXaxxov
xfjc; 6(J;£Cl)c; dxe popsLov dxe voxlov. exelvo oOv duo xfjc; dvapdaecoc; xoO l '
OLXTQ^axoc; xfjc; xu^iQ^ "^^^Ci xatpoO xaxaXa^pdvexaL ouxcoc;. edv f) dvdpaatc; xoO
l' OLXTQ^axoc; dvco oOaa xfjc; xecpaXfjc; fj^cov voxla, xo tiXsov xal eXaxxov xfjc;
6(J;£Cl)c; xoO TiXdxouc; sic; xo voxlov ^epoc;* el he \ popela, sic; xo popsLov ^epoc;. fissrL
15 'AXXcoc; xo aOxo 8l' exepac; ^sGoSou. xrjpeLxaL xo TiXdxoc; xfjc; tioXscoc; fjc;
PouXo^sGa. eliiep eaxl tiXsov xfjc; ^exaxXlaecoc;, oXcoc; xo tiXsov xal eXaxxov
498
xfjc; 6(J;£Cl)c; toO TiXdxouc; exelvo del votlov sl Se to TiXdxoc; xfjc; TioXecic; eaxL
Toaov OTL f) ^STaxXtaLc; oXr) ^exd xoO TiXdxouc; xfjc; aeXTQvric; svcdQelaoL e'E.iaomoLi
xcp TiXdxsL xfjc; TioXecoc;, x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; xoO TiXdxouc; eaxLV
ox£ popsLov UTiapx^L xal dXXoxe voxlov.
5 Elc; £X£Lvriv oOv x/jv tioXlv yjxlc; £)(£l ouxcoc; xrjpeLxaL x6 tiXsov xal eXaxxov
xfjc; 6(J;£Cl)c; xoO TiXdxouc; xal x6 TiXdxoc; xfjc; aeXTQvric;. dnep eaxl ouxcoc; oxl xal
xd p £Lc; x6 ^epoc; x6 popsLov y] slc; x6 voxlov slglv, evoOxat xal xd p* si he sgxl
xo £v popsLov xal xo exepov voxlov, xo eXaxxov dcpatpsLxaL xoO tiXslovoc;. el
XL xaxaXsLcpGfj, sxslvo TiXdxoc; xfjc; ocj^ecoc; xfjc; aeXTQvric; XeyexaL | y] xal TiXdxoc; fsoiw
10 Gxepeov. hel xcp pouXo^evcp tiolslv aOGrj^epLvov tiolslv xavovLa 8Ld xo tiXsov
xal eXaxxov xfjc; ocj^ecoc; xfjc; aeXTQvric; elc; xo TiXdxoc; xfjc; tioXscoc; exsLvrjc; ev fj
eyeveno xo | aOGrj^epLvov. fsovv
Ouxco xaGcbc; tj^slc; STioLiQaa^ev xoOxo. xfjc; KoXecdq fj^cov xo TiXdxoc; f)v
xoaov Xt). xoOxo noQev e'E.e^XfiQy] nap' fj^cov duo xcov p xavovLCOv dcp' &>v xoO
15 evoc; xo TiXdxoc; f)v xoaov Xc;, xal xoO exepou xo TiXdxoc; xoaov ^a.
6 TO TiXdioc;] ToO TiXdiouc; LVv || 7 5uo Vv | to \iipoc, to popsLov] to popsLov ^epoc;
Vv I elaiv om L | h6o Vv || 9 -lo f] xal TiXdTO^ aTspeov om. L || is fj^SL^ STioLrjaa^ev
TOUTo] £TioLir]6ir] TOUTO Tiap' fj^cov Vv II 14 5uo Vv
499
MoLpa I . Ilepl xfjc; xaxaXiQcJ^ecoc; xfjc; auvoSou xoO tiXlou xal xfjc; aeXTQvric; xal
xfjc; SLa^expou xouxcov
ToOxo £Lc; xpsLc; (J^iQcpouc; exsGr).
^fjcpoc; a . Ilepl xfjc; auvoSou xoO tiXlou xal xfjc; aeXrivriq xal xfjc; SLa^expou
5 I xouxcov xal xoO ^tqxouc; xfjc; xouxcov ^exapdaecoc; fissvL
TripsLxaL x6 aOGrj^epLvov xoO fjXLou xal aeXTQvric; oxl xaxa Tiolav fj^epav
GUvepxovxaL y] xaxa auvoSov y] xaxa Std^expov sic; ev ^6)8lov xal ^lav ^otpav
xal £v XsTixov. edv oOv eOpsGfj ouxcoc;, xaxd x/jv oSpav xoO ^eaou xfjc; fj^epac;
exsLvrjc; eyevexo y] xaxd auvoSov y] xaxd Std^expov xal xaxd x/jv ^otpav
10 £X£Lvriv £v fj eaxL xrjVLxaOxa 6 yjXloc; Sta^expcov y] auvoSeucov xfj aeXTQvr].
El he x6 aOGrj^epLvov xoO fjXLOu xal xfjc; aeXTQvric; oOx dat xax' evavxlov
£Lc; x6 [xeaov exsLvrjc; xfjc; fj^epac; p xrjpoOvxaL [xeaoL xfjc; fj^epac; tva xaxd x6
£v ^eaov xfjc; fj^epac; x6 aOGrj^epLvov xfjc; aeXTQvric; eXaxxov f) xoO aOGrj^epLvoO
xoO fjXLOu, £Lc; he x6 ^£x' sxslvo [xeaov xfjc; fj^epac; tiXsov xoO aOGrj^epLvoO
15 xoO fjXLOu. STiSLxa xripsLxaL tiolov ^eaov xfjc; fj^epac; eaxl eyyuxepov. xax'
£X£Lvo oOv x6 [xeaov xfjc; fj^epac; xpaxoOvxat xal d^cpoxepcov xoO fjXLOu xal
xfjc; aeXrivriq xd ^tqxt) xal xrjpoOvxaL. elxa olko xcov | p ^eacov xfjc; fj^epac; fsirv
sxpdXXexaL exdaxou f) ^exdpaatc; fjXLOu xal aeXrivriq. eKeiia f) ^exdpaatc; xoO
1 auvoSou] auvSou ut videtur V || 4 (J;f]cpo^] ^OLpa LVv || 12 exsLvr]^] sxslvo V | h6o
Vv II 17 5uo Vv
500
tiXlou dcpaLpsLxaL dmb xfjc; ^exapdaecoc; xfjc; aeXTQvric;. el xl xaxaXsLcpGrj, sxslvo
^sxdpaaLc; XeyexaL xeXeta.
Elxa £X£Lvo x6 ^fjxoc; x6 [xeaov fikiou xal aeXrivriq xrjpeLxaL sic; xd x8. el xl
e^eXGr], [xepi^eTOii eiq x/jv xeXetav exeivriv ^sxdpaaLv. d xl oOv xaxaXsLcpGrj,
5 f) oSpa eaxl xoO ^tqxouc;. auxr) cpuXdxxexaL. elxa xrjpeLxaL x6 aOGrj^epLvov
xoO tiXlou xal xfjc; aeXTQvric; sic; sxslvo x6 [xeaov xfjc; fj^epac;. edv oOv x6
aOGrj^epLvov xfjc; aeXTQvric; eXaxxov | f) xoO aOGrj^epLvoO xoO fjXLou, f) oSpa xoO fi39rL
[xrixouq [xenoi xfjc; oSpac; xoO ^eaou xfjc; fj^epac; svoOxaL. el xl eOpsGfj, dnep eaxlv
eXaxxov xcov (bpcov xfjc; fj^epac; exsLvrjc; Tidarjc;, exsLvr) f) oSpa f) oSpa eaxl xfjc;
10 auvoSou y] xfjc; SLa^expou sic; exeivriv x/jv fj^epav el 8' eaxl iikeov x6 eOpsGev
xfjc; oSpac; Tidarjc; xfjc; fj^epac;, f) oSpa auxr) xfjc; fj^epac; dcpaLpsLxaL e'E, exeivou. el
XL svaTioXsLcpGfj, f) oSpa eaxl xfjc; auvoSou y] xfjc; SLa^expou duo xfjc; epxo\ievriq
vuxxoc;. £L Se x6 aOGrj^epLvov xfjc; aeXTQvric; tiXsov eaxl xoO aOGrj^epLvoO xoO
fjXLOu, xripsLxaL f) oSpa xoO ^tqxouc;. dnep eaxl eXdxxcov xfjc; oSpac; xoO [ieaou xfjc;
15 fj^epac;, exsLvr) dcpaLpsLxaL duo xfjc; oSpac; xauxTjc; | xoO ^eaou xfjc; fj^epac;. el xl f302rv
xaxaXsLcpGfj, oSpa eaxl xfjc; auvoSou y] xfjc; SLa^expou sic; exeivriv x/jv fj^epav.
ei he f) oSpa xou ^tqxouc; tiXslcov eaxl xfjc; oSpac; xou ^eaou xfjc; fj^epac;, svouvxaL
xal al p, xal xo ebpeQev dcpaLpsLxaL duo xcov x8.| el xl xaxaXsLcpGfj, oSpa eaxl fsivv
xfjc; auvoSou y] xfjc; SLa^expou duo xfjc; TiapeXGouarjc; vuxxoc;.
9 if om. Vv II 12 f] om. Vv || is h6o Vv || i9 auvoSou et ^La^expou transpond L
501
OOtoc; oOv 6 (J;fjcpoc; xoxetv' f) dvsTiLacpaXric; fivLxa to aOGrj^epLvov xoO tiXlou
xal xfjc; aeXrivriq eyevovTO xeXsLa ^exa xfjc; opGciaecoc; xfjc; fj^epac;. el Se oOx
eyevovxo xeXeta, xax' evavxLov xoO aOGrj^epLvoO xoO tiXlou ytvexaL eiaeXeuaiq
5 £Lc; x6 xavovLov xfjc; opGciaecoc; xcov fj^epcov, xal xpaxsLxaL f) opGcoatc; xfjc;
fj^epac; xaxa xa a xal xa P' XsTixa xfjc; oSpac;. d xl oOv eOpsGfj,, sxslvo del sic;
x/jv oSpav xfjc; auvoSou y] xfjc; SLa^expou svoOxaL, xal ylvexaL f) oSpa xeXela.
I ALalpsGLc;. El pouXriGco^ev xov (J;fjcpov xoOxov XsTixoxepov TioLfjaat, ylvexat x6 fi39vL
aOGrj^epLvov xoO fjXLou xal xfjc; aeXrivriq eiq exeivriv x/jv oSpav fjVLxa ylvexat f)
10 auvoSoc; y] f) Std^expoc;. edv &ai xaxd xdc; ^olpac; xal xd XsTixd e^Laou^eva
xal d^cpoxepa xaOxa, f) oSpa exsLvr) 6p67] eaxLv el 8' oOx s^LaoOvxaL, aOGic; x6
[xeaov xouxcov ^fjxoc; xpaxsLxaL, xal ylvexat (be; eppsGr) sic; xov a' (J;fjcpov oticoc;
eOpsGfj f) oSpa opGiQ.
ALalpsGLc;. Ilepl xfjc; xaxaXiQcJ^ecoc; xfjc; ^olpac; exsLvrjc; ev fj auvep^ovxaL 6 yjXloc;
15 xal f) aeXTQvr) y] xaxd auvoSov y] xaxd Std^expov
'ExsLvo xo ^fjxoc; oTiep expaxT^Gr) ^eaov xoO fjXLou xal aeXTQvric; xlGsxaL sic;
3 oux difficile visu v || 6 xaxa] f]TOL Vv | Tipcoxa Vv | Seuxepa Vv || 7 f] om v
II 11 exsLvr] difficile visu v || 12 Tipcoxov Vv || 15 f] om L
502
P TOTlOUc; £V TTJ XauXoC* TO £V TTlpSLTaL OCGCpaXcOc; Xal TO STspov TTipsLTaL £Lc;
Toc £ XsTiTd. d TL oOv sOpsGrj, opGcoGLc; sgtl TTJc; ^otpac; toO tiXlou. exelvo
TTipsLTaL lSloc, xal toOto aOGic; svouTaL tc5 TTjpriGevTL | dacpaXcoc; ^tqxsl. el tl f82rv
eOpsGrj, opGcoatc; sgtl ttjc; ^otpac; ttjc; aeXTQvric;.
5 ''EjiSLTa TO aOGrj^epLvov tiXlou xal aeXrivriq - ocTLva eOpeGrjaav sic; to
[xeaov exsLvrjc; ttjc; fj^epac; - TiGevTaL sic; t/jv TaOXav lSloc xal ISla. xal bub
TauTa TLGsTaL sxaTspa f) opGcoatc;. elTa TripeiraL. edv to aOGrj^epLvov ttjc;
aeXTQvric; sXaTTOv toO aOGrj^epLvoO toO tiXlou, f) opGcoatc; ttjc; ^olpac; ttjc;
aeXrivriq svouTaL tc5 TauTTjc; aOGrj^epLvcp, xal f) opQcdoiq (baauTCOc; toO tiXlou
10 svouTaL Tcp TOUTOU auGrj^spLvcp. edv he to auGrj^epLvov ttjc; aeXTQvric; iikeov
Tou auGrj^epLvou tou tiXlou, | sxaTspou f) opGcoaLc; dcpaLpeiraL duo tou lSlou fi4o fl
auGrj^epLvou.
EI TL oOv STiSLTa xaTaXsLcpGrj, TripeiraL. edv s^LaouvTaL xal d^cpoTspa
xaTd Tdc; ^olpac; xal Ta XsTiTa, 6 (J;fjcpoc; ttjc; aeXTQvric; opGoc; saTLv ei 8' oux
15 s^LGOuvTaL, oux soTLv 6p66c;. ei oOv opGoc; sgtlv 6 (J;fjcpoc; sic; t/jv guvoSov
y] T/jv fj^epav y] t/jv vuxTa, f) ^otpa exsLvr) del ^la sgtlv sxslvoc; 6 (J;fjcpoc;
ypdcpsTaL sic; to auGrj^epLvov. ei 8' sgtI SLa^STpoc; sic; t/jv fj^epav f) ^otpa
TOU tiXlou xpaTSiraL, xal t/jv vuxTa f) ^otpa ttjc; gsXtqvtic;. £l yevriTaL xp^^a
sxpXrjGfjvaL t/jv tu^tq^ I '^^^ guvoSou y] ttjc; SLa^STpou, 6 (J;fjcpoc; toloutoc; f302vv
1 h6o Vv II 3 TTrjprjGevTL] prjGsvTL Vv || 6 exsLvr]^] sxslvo L || 7 exaxepa + A v |
f] sup lin V II 15 6p66^ eaxLv 6 (|>f]cpo^] 6 (J^ficpo^ 6p66^ eaxLv Vv
503
oloc; eppsGr) Tipoxepov.
^fjcpoc; P'. Ilepl ToO (J;7]cpou xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; xal ^exa xoO (J;7]cpou
xal Sloc xoO xavovLou. xoOxo sic; p StaLpeLxaL xecpaXata.
KecpdXLov a . Ilepl xoO eihevoLi oxl f) aeXTQvr) ^sXXsl sxXltislv y] ou, xal ^exa
5 xoO (J^TQcpou. xoOxo £Lc; e hioiipeaeiq exsGr).
I AtaLpeaLc; a . ''Oxl f) aeXTQvr) exXslcJ^sl y] ou f82vv
'EvxaOGd slgl xoaa d ocpsLXouaL xpaxrjGfjvaL. ev sxslvo, oxl f) SLd^expoc;
tiXlou xal aeXTQvric; xaxd vuxxa ocpsLXsL slvaL y] eyyuc; xfjc; vuxxoc; ouxcoc; oxl p
d)paL y] eXaxxov tv' cbaL ^eaov xfjc; fj^epac; xal xfjc; vuxxoc; xfjc; dp^fjc; xal xfjc;
10 TsXeioyaecdq fjVLxa SLa^expsL 6 yjXloc; x/jv aeXTQvriv. P' Se sxslvo, oxl [xeaov xcov
xo^Ticov xal xcov ^OLpcov xfjc; aeXTQvric; eXaxxov ocpelXsL slvaL | xcov lP ^OLpcov, y] fi40vL
xo TiXdxoc; xfjc; aeXTQvric; SLjiep eaxlv eXaxxov xcov ^y Xstixcov y] slc; xo popsLov y]
£Lc; xo voxLov ^spoc;, f) aeXTQvr) exXsLTiSL* el he tiXsov xouxcov, oOx exXsLTiSL. si
oOv ^eXXsL £xX£L(J;£Lv f) aeXTQvr), f) oSpa xfjc; auvoSou f) oSpa xfjc; ^earjc; exXsLcJ^ecoc;
3 h6o Vv II 6 Tiepl xf]^ aeXrjvr]^ £xX£L(|>£l f] ou Vv || 7 xpaTrjGfjvaL ] XrjcpGfjvaL Vv || 8
5uo V II 10 ^La^STpsL] ^La^STpf] V I SeuTspov Vv I exsLvo om Vv
504
XeyexaL.
AioLipeaiq P'. Ilepl xoO elhevoLi otl f) aeXTQvr) [xeXXei exXslcJ^slv y] oO ^exa xoO
(J^TQcpou
'Etisl xP^^o^ ^£xa xoO (J;7]cpou sltislv Tiepl xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric;, f)
5 Std^expoc; xoO tiXlou xal xfjc; aeXrivriq xal x6 axtaa^a — xal xa y sxpdXXovxaL.
eneiTOL f) Std^expoc; xoO tiXlou svoOxaL xrj SLa^expcp xfjc; aeXTQvric;. d xl eOpsGfj,
^spL^exaL £Lc; p. x6 xaxaXsLcpGsv sxslvo yj^lgu XeyexaL xcov p Sta^expcov.
xoOxo xripsLxaL. STiSLxa x6 TiXdxoc; xfjc; aeXTQvric; xaxd x/jv oSpav xfjc; SLa^expou
xripsLxaL. diiep oOv sgxl xoOxo s^lgou^svov xouxcp xcp fj^LasL xcov p Sta^expcov
10 y] TiXeov, f) aeXTQvr) oOx exXsLTiSL* el he eXaxxov, exXsLTiSL.
AtaLpeaLc; y'. Ilepl xoO slSevaL oxl tiogov xfjc; aeXTQvric; ^sXXsl sxXltislv, ^epoc;
xauxTjc; y] djiaaa, xal el ^epoc; xauxrjc; ^sXXsl exXmelv noaoi SdxxuXoL, xal si
£xX£L(J;£L Tiaaa ^sXXsl Tiepl x/jv exXslcJ^lv dpyfjaat y] sOGuc; jidXtv dp^aaGaL Tipoc;
x/jv xauxTjc; STiavaaxpecpsLV duoxaxdaxaaLV.
15 AcpaLpsLxaL I x6 TiXdxoc; xfjc; aeXTQvric; duo xfjc; fj^LasLac; xcov p Sta^expcov. fssrv
4 £Tid . . . aeXrjvr]^ om V || 5 xpta Vv || 7 5uo Vv | xaxaXsLcpGev] eupsGev L | sxslvo
om Vv I h6o Vv || 8-9 STiSLxa ...xfj^ ^La^expou TrjpsLTaL om Vv || 9 h6o Vv || ii
exXsLTiSLV V II 13 TidXtv] TidXaL V I dp^aaGat] dp^rjiaL L || i4 £TiavaaTpocpir]v xal Vv
505
el XL xaxaXsLcpGrj, exelvoL XsTixa XeyexaL xfjc; exXsLcJ^ecoc;. STiSLxa xrjpeLxaL. eav
xa XsTixa xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric; s^LaoOvxaL xfj SLa^expcp xfjc; aeXTQvric;, | f) fi4irL
aeXTQvr) xeXeta exXsLTiSL xal euQbq STiavaaxpecpexaL.
El Se xa Xsktol xfjc; exXsLcJ^ecoc; jiXsLovd slgl xfjc; SLa^expou xfjc; aeXTQvric;, f)
5 aeXTQvr) Tiaaa exXsLTiSL xal oXiyriv oSpav taxaxat sic; x/jv £xX£L(J;lv. sl Se xa
XsTixa xfjc; exXsLcJ^ecoc; eXdxxovd slgl xfjc; SLa^expou xfjc; aeXTQvric;, oXtyov xfjc;
aeXTQvric; exXsLTiSL.
'Etisl oOv xpiQ siMvoii Koaov xfjc; aeXTQvric; exXslcJ^sl, xd XsTixd xfjc; exXsLcJ^ecoc;
xfjc; aeXrivriq xrjpoOvxaL sic; xd i^. el xl eOpsGfj, ^epL^exat exeivo eiq x/jv
10 Std^expov xfjc; aeXTQvric;. el xl e^eXGr], SdxxuXoL eiai xfjc; SLa^expou xfjc; aeXTQvric;
duo xcov lP SaxxuXcov xfjc; SLa^expou xauxTjc;.
AtaLpeaLc; 8' . Ilepl xfjc; oSpac; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric;
To TiXdxoc; xfjc; aeXTQvric; xrjpeLxaL aOGic; sic; exelvo. olov edv f) xu^ov X£
x6 TiXdxoc;, xaOxa xrjpoOvxaL sic; xd xe TidXtv, xal sOplaxexaL x6 xexpdycovov
15 xoO TiXdxouc; xfjc; aeXTQvric;. | sxslvo duo xoO TiXdxouc; xcov yj^lgu Sta^expcov sosrv
dcpaLpsLxaL. el xl xaxaXsLcpGfj, 6 TioXuTiXaaLaa^oc; xouxou xpaxsLxat, xal x6
eOpsGev exelva XsTixd Xeyovxat xfjc; exXelcJ^ecoc; xfjc; aeXTQvric;. xaOxa xrjpoOvxaL
£Lc; xd x8 , xal xo e^eXQbv ^spl^exaL sic; x/jv xeXelav ^exdpaatv xfjc; aeXTQvric;
1 XeyexaL] XeyovxaL Vv
506
xriv xaxa to vuxQiQ^epov. el tl yevriTaL, oSpa eaxlv yjtlc; XeyexaL oSpa TieaoOaa.
Elxa f) oSpa xfjc; | SLa^expou xiGsxaL sic; xpsLc; xotiouc; xfjc; xauXac;. exsLvr) fssvv
oOv f) TieaoOaa oSpa duo xfjc; oSpac; xfjc; SLa^expou xfjc; neQeiariq Tipoxepov £v
xfj xauXa dcpaLpsLxaL xal svoOxaL xfj xsGsLar] ev xcp xptxcp xotico. d xl oOv
5 xaxaXsLcpGfj, olko xoO a f) oSpa xfjc; dp^fjc; xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric;. | d xl fi4ivL
he eOpsGfj, sic; xov P' xotiov f) ^ear) oSpa xfjc; exXsLcJ^ecoc; xfjc; aeXTQvric;. x6 he
yevo^evov sic; xov y' xotiov f) oSpa xfjc; xeXetac; djioxaxaaxdaecoc; xfjc; aeXTQvric;.
oOxoc; 6 (J;fjcpoc; xoxe ytvexat fjVLxa exXsLTiSL ^epoc; xfjc; aeXTQvric;.
AtaLpeaLc; e. ''Oxav exXsLTir] f) aeXTQvr) Tidaa, f) Std^expoc; xfjc; aeXTQvric;
10 duo xoO fj^LGSoc; xcov p Sta^expcov dcpatpsLxaL. d xl xaxaXsLcpGfj, duo xoO
xexpaycivou exsLvou xo xexpdycovov xoO TiXdxouc; xfjc; aeXTQvric; dcpatpsLxaL, xal
xoO xaxaXsLcpGsvxoc; 6 TioXuTiXaaLaa^oc; xpaxsLxaL, xal sOplaxovxaL xd XsTixd
xfjc; axdaecoc;. exsLva xrjpoOvxaL sic; xd x8, xal xo yevo^evov ^spl^exaL sic;
x/jv xeXelav ^exdpaatv xoO vuxQTj^epou. d xl oOv STiSLxa eOpsGfj, d^pal eiai
15 xfjc; axdaecoc;. elxa f) oSpa xfjc; Sta^expou sic; e xotiouc; xlGsxaL. xal f) neaoxjooL
oSpa duo xfjc; a' ^olpac; dcpatpsLxaL xal xfj e svoOxaL. xal aOGic; al d^pat xfjc;
axdaecoc; olko xfjc; P' ^olpac; dcpatpoOvxat xal xfj 8' svoOxaL.
I xaxa TO vuxSrj^epov ] toO vuxSrj^epou Vv || 5 Tipcoxou Vv 5-6 d. . . aeXrjvric; in marg
V II 6 SeuTspov V II 7 xpLTOv Vv II 9 ExXiiiji Vv || 10 h6o V II 11 aeXrjvr]^ om v
II 16 TipCOTlT]^ Vv I Tie^TITlT] V || 17 SsUTSpa^ V | TETOLpTJl V
507
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oSpac; xfjc; dcTioxaxaaxdaecoc; xfjc; aeXTQvric;, xal 6 £ xotioc; f) xexeXsLCO^evr) oSpa
xa6' y]v dcTioxaGLGxaxaL f) aeXTQvrj.l STiSLxa al Keaouaoii &>poii SLTiXaaLd^ovxaL. f84rv
5 el XL oOv eOpsGfj, oSpa eaxlv olko xfjc; dpx'^^ "^"H^ exXsLcJ^ecoc; xfjc; aeXTQvric; ^£XP^
xfjc; xeXsLac; dcTioxaxaaxdaecoc;.
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To TiXdxoc; xfjc; aeXTQvric; sxpdXXexaL | sic; xov xatpov xfjc; SLa^expou fjXLOu fi42rL
xal aeXrivriq xal cpuXdxxexaL. STiSLxa ylvexaL eiaeXeuaiq eiq x6 xavovLov xfjc;
10 ^exapdaecoc; fjXLOu xal aeXTQvric;. xal xax' evavxlov xoO TiXdxouc; xpaxoOvxat
xd XsTixd xoO aOGrj^epLvoO xal xrjpoOvxaL. elxa aOGic; ylvexat eiaeXeuaic, xax'
evavxLov xoO eipri\ievo\j TiXdxouc; xfjc; aeXTQvric; sic; x6 xavovLov xfjc; xpucj^ecoc;
xfjc; aeXrivriq eiq x6 Tioppcixepov ^fjxoc; sic; xd y xavovta, xal xpaxoOvxat ol
SdxxuXoL I xfjc; Tieaouaric; oSpac;. exsLvr) oOv f) oSpa xfjc; axdaecoc; xal f) opGcoatc; fsosw
15 exdaxou ISla xal ISla cpuXdxxovxaL. elxa f) opGcoatc; exdaxou sic; xd XsTixd xoO
aOGrj^epLvoO xrjpeLxaL. d xl eOpsGfj, svoOxaL sic; exaaxov xcov cpuXaxQevxcov
opGciaecov sxslvcov ISla xal ISla. OTiep oOv eOpsGfj ylvexat xsXslov.
1 TipcoTO^ Vv I SeuTspo^ V II 2 xpLTO^ Vv | TSxapTO^ V II 3 Tie^TiTO^ V II 13 xpta
Vv
508
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lP, TsXeioL yLvexaL exXslcJ^lc; xfjc; aeXTQvric;, xal Tipoc; xatpov sic; x/jv exXslcJ^lv
taxaxaL. el he i^ SdxxuXoL slglv, f) aeXTQvr) Tiaaa exXsLTiSL dXX' oO^ taxaxat
£Lc; x/jv £xX£L(J;lv. sl he ol SdxxuXoL eXdxxovec; xcov i^ exXemei [xepoq xfjc;
5 aeXrivriq oaov dvacpavrj sic; xouc; SaxxuXouc; xfjc; SLa^expou.
'ExsLvo xoLvuv xpiQ eihevoLi tiogov eaxlv duo xfjc; aeXTQvric;. ytvexaL
elaeXeuaLc; sic; x6 xavovLov xfjc; SLa^expou xfjc; aeXTQvric;. xal xax' evavxLov
xcov SaxxuXcov xpaxelxaL 6 (J;fjcpoc; xcov SaxxuXcov xfjc; | sjiLcpavsLac; xfjc; aeXrivriq. f84vv
d XL oOv eOpsGfj, exel SdxxuXoL eiaiv olko xfjc; sjiLcpavsLac; xcov SaxxuXcov xfjc;
10 aeXTQvric; Tidarjc;.
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Ouxcoc; eaxlv (be; eppsGr) | £v xfj 8' xal e hioLipeaei xoO ol xecpaXaLou. fi42vL
AtaLpeaLc;. Ilepl xoO xatpoO xfjc; exXsLcJ^ecoc; xfjc; aeXrivriq dnep ^epoc; xauxTjc;
exXsLTiSL xaxd x/jv vuxxa xal ^epoc; xaxd x/jv fj^epav
15 El yLvexaL f) exXslcJ^lc; xaxd x/jv fj^epav, edv f) oSpa xfjc; exXsLcJ^ecoc; xfjc;
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2 -3 SLc; Trjv £xX£L(|>LV laxaxaL ] exXsLTiouaa yLvexaL L || 3 Tiaaa post ixkeuiEi V || 12
TETapTji Vv I Tie^TTir] Vv I TipcoTou Vv II 13 TauTiT]^ om L II 15 yLvsTat] yevrjiaL L
II 16 dTio xf]^ fj^epa^ tiXslcov f]] f] wpa L
509
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vuxxoc; YJxLc; xal dcpaLpsLxaL £^ exsLvrjc;. el xl xaxaXsLcpGfj, oSpa eaxlv olko xfjc;
fj^Lspac;.
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£XX£L(J;£C0C; xou fjXLOU
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10 £XX£xaxaL sic; ^fjxoc;, xal eaxLV SuaxaxdXrjTixoc;. tj^slc; he xo xavovLov xouxo
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[xeaov xfjc; fj^epac;, 6 P' - xo tiXsov xal eXaxxov xfjc; ocj^ecoc; sic; xo ^fjxoc;, xal
6 y' - xo TiXeov xal eXaxxov xfjc; ocj^ecoc; sic; xo TiXdxoc;. f) TioLTjaLc; oOv xouxou
15 xou xavovLou sic; xdc; y TiXrjpouvxaL hioLipeaeic^.
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eaxL auvxd^SL.
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15 xauxTjc; XLVTQGSCOc;
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15 ^sGoSoLc; xpfjaGaL xpiQ- Tipcoxov hel eihevoLi x/jv auvoSov exsLvriv xa6' y]v ^sXXsl
3 xpsL^ Vv II 5 dd om Vv || 6 xal^ om. Vv | eva Vv || 7 xal om. Vv || 12
ocpsLXsL slvaL om. Vv || is toutcov] toutou Vv
514
XeveoQoLi f) exXslcJ^lc;, eha xal xac; ^^XP^ '^^^ auvoSou oSpac;, STiSLxa xaxa Tiotav
^oLpav yLvexaL f) auvoSoc;. xal x6 aOGrj^epLvov xoO dvapLpd^ovxoc; xrjVLxaOxa
xaxaXa^pdvexaL. xouxcov he xaxaXrjcpGevxcov xaxaXa^pdvexat xal f) Std^expoc;
xoO tiXlou xal f) ^sxdpaaLc; xoO tiXlou (baauxcoc; sic; ^lav oSpav. xal f) Std^expoc;
5 xfjc; aeXrivriq xal auxr) sxpdXXexaL xal f) ^sxdpaaLc; aOxfjc; eiq x/jv ^lav oSpav.
eneiTOL xal f) xeXela ^sxdpaaLc; xfjc; aeXTQvric; sic; ^lav oSpav xaxaXa^pdvexat
xal f) oSpa xoO \ieao\j xfjc; fj^epac;.
TaOxa Tidvxa xaxaXa^pdvovxat xal xrjpoOvxaL. elxa xal f) xu^iQ "^oO xatpoO
£X£Lvou fjVLxa yLvsxaL f) auvoSoc; fjXLOu xal aeXrivriq xpaxsLxat. elxa x6 ^6)8lov,
10 al ^OLpaL xal xd XsTixd xfjc; auvoSou fjXLOu xal aeXTQvric; dcpatpoOvxaL duo xfjc;
xu^TQ^ "^^^Ci xatpoO. d xl oOv | xaxaXsLcpGfj, ^fjxoc; sgxl xcov ^OLpcov xfjc; auvoSou. fi44vL
Touxo cpuXdxxexaL. STiSLxa xrjpeLxaL. edv xo ^fjxoc; sxslvo 9 ^otpat (bat,
exsLVT) f) oSpa f) expXrjGsLaa xfjc; auvoSou f) ^ear) oSpa eaxl xfjc; exXelcJ^ecoc;.
exsLVT) he f) ^otpa xa6' y]v 6 yjXloc; auvoSeusL xfj aeXTQvr] 6 xotioc; eaxl xfjc;
15 Gecoplac; xfjc; aeXTQvric;. evxauGa he ou X9^^^ xauxrjc; yeveaQoLi x/jv oSpav xfjc;
auvoSou opGiQv. sxslvo oOv xo ^fjxoc; dnep eaxl eXaxxov xcov 9 ^otpcov, exsLvr)
f) ^OLpa xa6' y]v 6 yjXloc; auvoSeusL xfj aeXTQvr] sic; xo ^epoc; xfjc; dvaxoXfjc;* el he
I xo ^fjxoc; TiXeov xcov 9, exsLvr) f) ^otpa xfjc; auvoSou sic; xo ^epoc; xfjc; Suaecoc;. fsevv
Meaov oOv xcov p xouxcov eaxl xp^^a xfjc; opGciaecoc; xfjc; oSpac; exsLvrjc; oTiep
1 f] sup lin V II 2 auGrj^epLvov + Se L || 9 f] auvoSo^ sup lin v || 19 h6o Vv |
Xpeta + ^exa LVv
515
eaxlv £Lc; y hioLipeaeici.
AioLipeaic, ol . Ilepl xfjc; opGciaecoc; xfjc; oSpac; xfjc; ^earjc; exXsLcJ^ecoc;
'ExsLvo oOv £Lc; Suo xLvd eaxLv £v ^exa xoO (J;7]cpou xal ev Sloc xoO xavovLou.
x6 yoOv Sloc xoO (J;7]cpou £ xlvcov SsLxaL. ev exelvo Iva xaxaXsLcpGrj f) oSpa xfjc;
5 auvoSou* dcTi' exsLvrjc; he xfjc; oSpac; f) xu^iQ ocpetXeL xaxaXsLcpGfjvat xal x6 l'
oIxTj^a xal f) dvdpaaLc; xoO i olxiQ^axoc;. xoOxo xrjpeLxaL. P' f) dvdpaaLc;
xfjc; aeXTQvric; xaxaXa^pdvexat. xplxov x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; xoO
fjXLOu xal xfjc; aeXrivriq eiq xov xuxXov xfjc; dvapdaecoc; | yLvciaxexaL. STiSLxa sosrv
dcpatpsLxaL x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; xoO fjXLOu olko xfjc; aeXTQvric;. x6 oOv
10 xaxalXsLcpGsv xpaxsLxaL. 8' sic; exelvo oticoc; xaxaXsLcpGfj f) ycovla xoO TiXdxouc; fi45rL
xal xoO ^TQXouc;. x6 £ f) xaxdXrjcJ^Lc; xoO tiXslovoc; xal eXdxxovoc; xfjc; ocj^ecoc;
xfjc; aeXTQvric; sic; x6 ^fjxoc; xal TiXdxoc;. sic; xoOxov he xov (J;fjcpov tj^slc; duo
xcov e xouxcov oOx ea^ev ev XP^^9^- oOxol Se ol e (J;fjcpoL dvd xptcov ocpelXouaL
[xeQoheuQfivoii.
15 'O (J>fjcpoc; xfjc; exXsLcJ^ecoc; xoO fjXLOu Std xoO xavovlou. xrjpsLxaL f) oSpa xfjc;
aovoSou xal f) oSpa xoO [ieaou xfjc; fj^epac;. edv oOv e^LaoOvxat xal al p xaxd
xouc; (J^TQcpouc;, sic; xo (bpatov xavovLov xax' evavxlov xoO [xeaou xfjc; fj^epac;
1 xpsL^ Vv II 3 oOv om. V || 4 TievTS Vv II 6 SeuTspa v || 7 toO om. v
xf]^ om. Vv II 10 TSxapTOV Vv || ii tis^titov v || 16 h6o V
516
yLvexaL elaeXeuaLc;, xal xpaxsLxaL to tiXsov xal eXaxxov xfjc; | ocj^ecoc; sic; x6 fsrrv
^fjxoc;. eav oOv f) oSpa xfjc; auvoSou duo xfjc; oSpac; xoO ^eaou xfjc; fj^epac;
eXdxxcov, exsLVT) dcpaLpsLxaL duo xfjc; oSpac; xauxTjc;. el xl xaxaXsLcpGfj, f) oSpa
xoO ^TQXouc; eaxl Tipo xoO ^eaou xfjc; fj^epac;. el he f) oSpa xfjc; auvoSou tiXslcov
5 xfjc; oSpac; xoO [xeaou xfjc; fj^epac;, f) oSpa xoO ^eaou xfjc; fj^epac; e^ exsLvrjc;
dcpaLpsLxaL. d xl xaxaXsLcpGfj, f) oSpa xoO ^tqxouc; eaxl ^exd x6 [xeaov xfjc;
fj^Lspac;.
ToOxo oOv dx£ Tipo xoO [xeaou elie [xenoi x6 ^eaov xfjc; fj^epac; sgxlv, f) oSpa
xoO Tipcixou ^TQXouc; XeyexaL. STiSLxa xax' evavxLov xfjc; oSpac; exsLvrjc; ytvexaL
10 elaeXeuaLc; sic; x6 (bpatov xavovLov, xal xpaxsLxaL x6 iikeov xal eXaxxov xfjc;
6(J;£Cl)c; slc; x6 ^fjxoc;, oTiep XeyexaL iikeov xal eXaxxov xfjc; ocj^ecoc; a'.
ToOxo oOv I x6 TiXeov xal eXaxxov xfjc; ocj^ecoc; ^spl^exaL sic; x/jv xeXelav fi45vL
^sxdpaaLV xfjc; aeXrivriq eiq [xioiv oSpav. el xl eOpsGfj, sxslvo oSpa xoO tiXslovoc;
xal eXdxxovoc; xfjc; ocj^ecoc; xoO a' . auxr) f) oSpa ^exd xfjc; oSpac; xoO ^tqxouc; xoO
15 OL del svoOxaL, xal f) oSpa xoO P' ^tqxouc; sOplaxexaL. STiSLxa xax' evavxlov
xfjc; oSpac; xauxTjc; xoO P' ^tqxouc; xpaxsLxaL x6 tiXsov xal eXaxxov xfjc; ocj^ecoc;
£Lc; x6 ^fjxoc;, xal xoOxo aOGic; sic; x/jv xeXelav ^sxdpaaLV xfjc; aeXrivriq eiq x/jv
^lav oSpav ^spl^exaL. el xl oOv eOpsGfj, oSpa eaxl xoO tiXslovoc; xal eXdxxovoc;
xfjc; 6(J;£Cl)c; slc; x6 ^fjxoc; x6 P'. xal auxr) f) oSpa ^exd xfjc; oSpac; exsLvrjc; xoO
3 exsLvr] + f] V || 4 xfj^ iter, v || ii Tipcoxov Vv || i4 Tipcoxou Vv || i5 Tipcoxo^
Vv I SeuTspou Vv II 16 SeuTspou Vv || is oO om. Vv || i9 Seuxepov Vv
517
[xeaoxj xfjc; fj^epac; evomoLi. xal el tl e^eXGr], sxslvo oSpa eaxl xoO y' ^tqxouc;.
xal aOGic; xax' evavxLov xfjc; oSpac; xauxrjc; ytvexaL elaeXeuaLc; sic; x6 (bpatov
xavovLov.
Kal yLvexaL 6 (J;fjcpoc; TioXXdxLc; ouxcoc; | xal xexpdxLc; xal e^dxLc; ^^XP^ ^^ ^^'^^^
5 xd p TiXsLova xal eXdxxova xfjc; ocj^ecoc;, diiep expaxT^Grjaav, s'E.iacdQcdai xaxd
xouc; (J^TQcpouc;. exsLvo oOv x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; x6 uaxepov xsXslov
eaxLv, xal exsLvr) f) oSpa xoO Oaxepou ^tqxouc; xeXela. STiSLxa xrjpeLxaL f) ^otpa
exsLVT) fjVLxa ylvexat 6 yjXloc; xaxd auvoSov xfjc; aeXrivriq. edv f) sic; x6 ^epoc;
xfjc; dvaxoXfjc;, xoOxo x6 tiXsov xal eXaxxov | xfjc; ocj^ecoc; xoO ^tqxouc; oTiep fsosw
10 e^fjXGsv uaxepov dcpaLpsLxaL | duo xfjc; ^olpac; exsLvrjc;* si he sic; x6 ^epoc; xfjc; fi46rL
Suaecoc;, svoOxaL exsLvr]. el xl oOv eOpsGfj, xotioc; eaxl xfjc; Gecoplac; xfjc; aeXTQvric;
£Lc; x6 [xeaov xfjc; exXelcJ^ecoc;. gjiSLxa edv f) ^otpa exsLvr) sic; x6 ^epoc; f) xfjc;
dvaxoXfjc;, exsLvr) f) oSpa xoO neXeiou ^tqxouc; dcpatpsLxaL duo xfjc; oSpac; xoO
^eaou xfjc; fj^epac;* ei he Tipoc; x6 ^epoc; xfjc; Suaecoc;, svoOxaL xauxr]. d xl
15 eOpsGfj, oSpa eaxl xfjc; ^earjc; exXelcJ^ecoc;.
ALalpsGLc; P'. Ilepl xoO slSevaL el yevrixaL exXslcJ^lc; y] ou, xal el yevrixaL noay]
^eXXsL slvaL
'EtisI pouXo^sGa TioLfjaat xov (J;fjcpov xoOxov, x6 aOGrj^epLvov xoO xaxa-
1 xpLTOU Vv II 4 5 ' L, TSTSTpdxL^ V || 5 h6o Vv II 12 f] post dvaxoXf]^ V II 16
SeuTspa V
518
Ptpd^ovToc; ex xoO totiou xfjc; Gecoptac; xfjc; aeXTQvric; dcpaLpsLxaL dsL, xal
s^epX^xaL f) ^OLpa xoO TiXdxouc; xfjc; aeXTQvric;. xax' evavxLov oOv xfjc; ^otpac;
xoO TiXdxouc; xouxou xfjc; aeXTQvric; ytvexaL eiaeXeuaiq eiq x6 xavovLov, xal
xpaxsLxaL x6 TiXdxoc; xfjc; aeXrivriq. xal exelvo TiXdxoc; XeyexaL xsXslov.
5 Elxa xripsLxaL el popsLov sgxl y] voxlov. sxslvo cpuXdxxexaL. STiSLxa xax'
evavxLov xfjc; oSpac; exsLvrjc; xoO xeXsLou ^tqxouc; ylvexaL eiaeXeuaic, sic; x6
(bpaLov xavovLov, xal x6 tiXsov xal eXaxxov xfjc; ocj^ecoc; xoO TiXdxouc; xpaxsLxaL
xal cpuXdxxexaL. STiSLxa xrjpeLxaL el ^opeiov y] voxlov. edv oOv xo xsXslov
TiXdxoc; xfjc; aeXTQvric; ^exd xoO tiXslovoc; xal eXdxxovoc; xouxou xfjc; ocj^ecoc; xoO
10 TiXdxouc; popsLa | y] voxta, evoOvxat xal xd p. el he xo £v popsLov xal xo exepov fi46vL
VOXLOV, xo eXaxxov dcpatpsLxaL xoO tiXslovoc;. el xl xaxaXsLcpGfj, TiXdxoc; eaxl
xfjc; aeXrivriq anepeov. xoOxo xrjpeLxaL. STiSLxa f) | Std^expoc; xoO fjXLOu evoOxat fssrv
xfj SLa^expcp xfjc; aeXTQvric;, xal xo eOpsGev ^spl^exaL eiq p. el xl eOpsGfj, sxslvo
YJ^LGU XeyexaL xcov p Sta^expcov. xoOxo xlGsxaL sic; x/jv xaOXav. xal sxslvo
15 xo Gxepeov TiXdxoc; xfjc; aeXTQvric; TiXrjaLov xouxou xlGsxaL xal xrjpeLxaL. edv
xo axepeov TiXdxoc; s^LaoOxaL xcp fj^LasL xcov p Sta^expcov y] tiXsov xouxou,
£xX£L(J;lc; oO ylvexaL* ei 8' eXaxxov, exXsLTiSL.
''EjiSLxa ei yevrixaL xp^^o^ slSevaL tiogov exXslcJ^sl xoO fjXLou, xo axepeov
£X£Lvo TiXdxoc; duo xoO fj^Laeoc; xcov p Sta^expcov dcpaLpsLxaL. el xl xaxaXsLcpGfj,
2 -4 xax' . . . aeXrjvr]^ om Vv || 5 -8 sxslvo . . . votlov om. Vv || lo h6o V || is h6o
Vv I eupeefj] e^eXer] Vv || i4 5uo V || le 5uo V || i9 5uo V
519
£X£Lvo XenTOL XsyovxaL xfjc; exXsLcJ^ecoc;. ehoL TTipelioLi. eav xa XsTixa xaOxa xfjc;
exXsLcJ^ecoc; s^LaoOvxaL xcp fj^LasL xcov p Sta^expcov, xeXeta ytvexaL exXslcJ^lc; xoO
tiXlou* £l 8' eXdxxova xa XsTixa xfjc; exXsLcJ^ecoc; xoO fj^Laeoc; xcov p Sta^expcov,
^epoc; exXsLTiSL xoO tiXlou.
5 ''EjiSLxa xripsLxaL f) xeXeta exsLvr) exXslcJ^lc; ^exa xfjc; SLa^expou fjXLou xal
aeXTQvric;. eav oOv xal al p Std^expoL laaL, 6 yjXloc; xsXslov exXslcJ^sl xal oO
PpaSuvsL £v xfj exXei(\)ei. si he f) Std^expoc; xfjc; aeXTQvric; tiXslcov, 6 yjXloc; oXoc;
£xX£L(J;£L xal xatpov Ixavov axaGiQaexaL £v xfj exXslcJ^sl. sl he f) Std^expoc; xoO
fjXLou TiXsLCOv, x6 ^eaov xoO fjXLou exXslcJ^sl, f) Se TiepLcpepsLa | oOx exXslcJ^sl. fi47rL
10 Elxa xripsLxaL f) exXslcJ^lc; exsLvr) f) xaxd ^epoc; yLvo^evr) xal oO^l xeXela
TioaoL SdxxuXoL slglv duo xfjc; SLa^expou xoO fjXLou ^exd xoO (J;7]cpou exsLvou,
xfjc; xeXelac; SLa^expou xoO fjXLou lP SaxxuXcov ouarjc;. stisI oOv xps^ia yeveaGaL
xov (J;fjcpov xoOxov, xd XsTixd exeiva xfjc; exXelcJ^ecoc; xd eOpsGevxa Tipo xouxou
xrjpoOvxaL | sic; xd i^. el xl eOpsGfj, exelvo elq x/jv Std^expov xoO fjXLou fssvv
15 ^spl^exaL, xal sOplaxovxaL ol SdxxuXoL xfjc; exXelcJ^ecoc; duo xfjc; SLa^expou xoO
fjXLOU.
ALalpsGLc;. Ilepl exeivou oxl duo xoO fjXLou tiogov exXslcJ^sl xal xfjc;
xaxaXiQcJ^ecoc; xoO xatpoO Std xoO xavovlou
2 5uO V II 3 5uO Vv II 6 5uO V
520
I ''Oxav f) oSpa xfjc; ^earjc; exXsLcJ^ecoc; expXrjGrj ^exa xoO axepeoO TiXdxouc; fsoerv
xfjc; aeXTQvric;, STiSLxa xax' evavxLov xoO lSlou xfjc; aeXTQvric; y] xfjc; ^exapdaecoc;
exsLvrjc; ytvexaL elaeXeuaLc; sic; x6 xavovLov xfjc; ^exapdaecoc; fjXLOu xal aeXTQvric;,
xal xd XsTixd xoO aOGrj^epLvoO xpaxoOvxat £X£l6£v xal cpuXdxxovxaL. STiSLxa
5 xax' evavxLov xoO axepeoO TiXdxouc; xfjc; aeXTQvric; ytvexaL elaeXeuaLc; sic; x6
xavovLov xfjc; exXsLcJ^ecoc; xoO fjXLOu, xal xpaxoOvxat ol SdxxuXoL xal opGcoatc;
exsLvcov xal f) TieaoOaa oSpa ^exd xfjc; opGciaecoc; xauxTjc;. xal xrjpeLxaL exaaxov
ISla xal ISla. STiSLxa xd XsTixd xoO aOGrj^epLvoO xrjpoOvxaL sic; x/jv opGcoatv
exdaxou. xal el xl e^eXGr], nap' eva pa6^6v eXaxxov xpaxsLxaL. xal exeivo
10 del svoOxaL sic; exelvoL sic; xouc; SaxxuXouc; xal sic; x/jv oSpav, xal ylvovxaL ol
SdxxuXoL xeXsLOL xal f) | TieaoOaa oSpa xeXela. fi47vL
Elxa xripsLxaL. edv ol SdxxuXoL exelvoi i^ y] tiXslovsc;, 6 yjXloc; oXoc; exXsLcJ^SL*
£L Se eXaxxov xcov lP, oXoc; oOx exXslcJ^sl. xrjpeLxaL oOv tiogov duo xcov i^
SaxxuXcov £xX£L(J;£L. elxa e'E, exeivou ylvexaL 6 (J;fjcpoc;. xal oOxol ol SdxxuXoL
15 Std^expoc; xoO fjXLOu ylvovxat.
El oOv -/^peioi xaxaXsLcpGfjvat xouc; SaxxuXouc; xfjc; sjiLcpavsLac; xoO fjXLOu xax'
evavxLov xcov SaxxuXcov xfjc; Sta^expou xoO fjXLOu, ylvexat eiaeXeuaiq eiq xo
xavovLov, xal xpaxsLxaL 6 eOpsGelc; (J;fjcpoc; xfjc; sjiLcpavsLac; xcov SaxxuXcov xoO
fjXLou. xal xoOxo sgxlv ol SdxxuXoL | xfjc; exXelcJ^ecoc;. enei oOv f) TieaoOaa oSpa f89rv
12 TiXsLove^] TiXeov he v || is sl ht...o\)x ixXeii^ei in marg v || i6 xaxaXsLcpGfjvaL
Xpeta Vv
521
f) TsXeioL eyevsTO StqXt), f) oSpa xfjc; ^earjc; exXsLcJ^ecoc; sic; y totiouc; xLOexaL ev
TTJ xauXa. xal f) TieaoOaa oSpa duo xoO a dcpaLpsLxaL xal xcp xpLxcp svoOxaL,
xal sOpLGXovxaL ol xatpol xfjc; exXsLcJ^ecoc; (be; eppsGr) Tipo xouxou.
1 XpSL^ Vv II 2 TipCOTOU Vv
522
MoLpa La . Ilepl xfjc; xaxaXiQcJ^ecoc; exsLvrjc; otl f) aeXTQvr) hots Ivol cpavrj vea
(baauTCOc; xal ol daxepec; tiots tva cpavcoaL [xeTOL xriv auvoSov xoO tiXlou
'ExsLvo TOLvuv pTjOTQasTaL Tiepl xfjc; aeXrivriq o GecopsLxaL nap' fj^cov. xal
6 (J;fjcpoc; Se oOxoc; Xtav eaxl Suax^pTjc; Sta xoOxo oxl ol dpxaloL sxslvol Tiepl
5 xouxou oOx sItiov XL. Std xl oOv oOx sIkov xl; 8l' sxslvo oxl f) dpxiQ "^^^
^rivcov duo xfjc; aeXTQvric; duo xoO xatpoO expaxelxo exelvou nap' aOxolc; | fivlxa fi48rL
^£xd auvoSov eyevexo f) SLdaxaaLc; xfjc; aeXTQvric; duo xoO fiXlou. enei oOv
Xpsla f)v xcov Hepacov sic; xoOxo Std x/jv vrjaxsLav xal xd Tidaxa xal xdc;
^eydXac; xouxcov fj^epac;, aOxat he al ^eydXat xouxcov fj^epaL Std xfjc; Gecoplac;
10 xfjc; aeXTQvric; veac; ylvovxat SfjXat, tj^slc; xolvuv xeGelxa^ev £v xfj pipXcp xauxr]
OTiep ol daxpovo^oL exelvoi ev xalc; pipXoLc; xouxcov xsGelxaaLV. xal ^exd xoO
(J^TQcpou xal Std xoO xavovlou xal dXXa xLvd &>v f)v xouxolc; xP^^^^^ ^^^ ^^'
exsLvcov xcov (J^iQcpcov d)v lacoc; UTioXdpoL dv xlc; oO Suax^pcov, dXX' e'E, sxslvcov
xcov (J^TQcpcov oO^l Tcov Soxouvxcov dTioxpoTialcov xfjc; TiLGxecoc;, dXXd xcov xaxd
15 TioXu XuGLxeXouvxcov £Lc; x/jv xauxriv. Suax^pec; oOv sOpsGfjvaL xoloOxov (J;fjcpov
£V xaLc; pipXoLc; xcov dXXcov Std xo U(J;oc; | xouxou. fsoew
Kal (be; exsGr) Se | oOxoc; 6 (J;fjcpoc; sic; xo ^i^Xiov xoOxo £v dXXcp oOx dv f89vv
xlc; eupoL. Std xl oOv eycoye xoloOxov (J;fjcpov Gau^daLov £v xouxcp xsGrixa xcp
PlPXlco; 8l' £X£lvo oxl ol ^fjvec; xfjc; aeXTQvric; Tiapd xcov Hepacov 8Ld xfjc; Gecoplac;
1 evSexdTir] Vv || 5 Sta . . . otl ] hioLTi. 5l6tl Vv || 7 ^LdaxaaL^] StdpaaL^ cum ^xa sup
P V II 8 vrjaxsLav + toutcov Vv
523
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15 xoOxo xo xecpdXaLov sic; oxxco StaLpeLxaL .
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15 aeXTQvric;.
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525
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eOpsGfj, £Lc; x6 aOGrj^epLvov xfjc; aeXTQvric; xoO ^eaou xfjc; fj^epac; svoOxaL, xal
sOplaxexaL x6 | aOGrj^epLvov xfjc; aeXTQvric; sic; x/jv oSpav oxav xaxepxTjxaL. f90vv
ALalpsGLc; P'. Ilepl xfjc; dacpaXoOc; opGciaecoc; xoO xotiou xfjc; aeXTQvric; sic; x6
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10 ToTioc; he xfjc; aeXTQvric; exelvoc, oxav xaxepxTjxaL Tipoc; Suglv oOxoc; oOv
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£v xcp xavovLcp xfjc; ^exapdaecoc; fjXLOu xal aeXTQvric; xaGcbc; eppsGr) Tipoxepov
£Lc; x/jv 6' MoLpav.
15 ALalpsGLc; y' . Ilepl xfjc; dacpaXoOc; opGciaecoc; xoO xotiou xfjc; aeXTQvric; ^exd xfjc;
opGciaecoc; xfjc; fj^epac;
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526
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xax' evavxLov xouxou ytvexaL eiaeXeuaiq eiq x6 Otio xouc; ^fjvac; xavovLov xcov
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5 xfjc; aeXTQvric;, xal ylvexaL xoOxo xsXslov.
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eaxLV.
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xripsLxaL. ei oOv xp^^a yevrixaL 8Ld ^Ldc; ^£668ou yeveoQai xov (J;fjcpov xoOxov
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8 a\ia post £XD L I xaxepxexaL toO auGrj^epLvoO Vv || i4 YevrjiaL xp^^o^ L | Sta
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xal £X£Lvo TO eOpsGev xripeLTaL sic; to axepeov TiXdxoc; xfjc; aeXrivriq. el xl oOv
eOpsGrj, opQcdoiq sgxlv.
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svoOxaL xcp xoTicp xfjc; aeXTQvric;* el Se voxlov, dcpaLpsLxaL e'E, exeivou. el
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ylvexaL (J;fjcpoc; | Std x/jv ^otpav exeivriv x/jv ^exd xfjc; aeXrivriq xaxep^o^evriv, fisovL
dvxeaxpa^^evcoc; xcp (j>W9 "^ouxcp ylvexat, fjyouv £v6a eyevexo dcpalpeaLc;
10 £vxa06a Svcoglc; Std xfjc; opGciaecoc;, xal £v6a Svcoglc; evxaOGa dcpalpsGLc;.
ALalpsGLc; £ . Ilepl xoO xo^ou xoO cpcoxoc;
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svoOxaL. el xl eOpsGfj, 6 TioXuTiXaGLaG^oc; exeivou ^rixsLxaL, xal xo e^eXQbv
15 TO^ov £Gxl xoO cpcoxoc; YJyouv xfjc; eXXd^cJ^ecoc; xfjc; gsXtqvtic;.
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GeXTQvri ^£xd x/jv Suglv xoO fjXLou
13 eauTol auTO Vv
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^OLpac; exsLvrjc; xfjc; SLa^expou [xstol xfjc; ^oLpac; ^£0' fjc; xaxepx^xaL f) aeXTQvr)
£Lc; x6 TiXdxoc; xfjc; KoXecdq. STiSLxa 6 xotioc; xfjc; xuxTjc; xoO fjXLOu dcpaLpsLxaL duo
5 xoO xoTiou xfjc; Tuyjiq xfjc; aeXTQvric;. d xl xaxaXsLcpGfj, exelvo eaui x6 prjGev.
AtaLpeaLc; C • Hepl xoO xo^ou xfjc; xaxapdaecoc; xoO fjXLOu Otio yfjv xaxd xov
xatpov fjVLxa xaxepx^xaL f) aeXTQvr)
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xoO opGcoGsvxoc; jiap' fj^cov exeivou xotiou xfjc; aeXTQvric; dcpaLpsLxaL. el xl
10 xaxaXsLcpGfj, f) xpaxTjXaLa exsLvr) STiSLxa xpaxsLxaL. | xal exsLvr) xrjpeLxaL sic; fisirL
x/jv xpaxTjXaLav x/jv xexeXsLCO^evriv xfjc; dvapdaecoc; xoO xotiou xcov dxpcov.
x6 yoOv eOpsGev sxslvo nap' eva pa6^6v eXaxxov xpaxsLxaL. o xl eOpsGfj,
xpaxTjXaLd sgxlv. eha x6 to^ov exeivou xpaxsLxaL, xal f) xaxdpaoLc; xoO fjXLOu
sOpLGxexaL. | nap' fj^cov Se exsGr) xavovLov sic; x6 TiXdxoc; xcov XC f92rv
15 El oOv hefiaei x6 xo^ov sxslvo xoO xaLpoO xaxaXrjcpGfjvaL sic; x/jv ea^dxriv
dvdpaoLV xfjc; SLa^expou xfjc; ^oLpac; xoO fjXLOu, xax' evavxLov xfjc; xoLauxTjc;
dvapdaecoc; yLvexaL SLaeXeuaLc; sic; x6 xavovLov xfjc; xaxapdaecoc; fjXLOu xal
dvapdaecoc; xfjc; aeXrivriq eiq xov 8Ld xoxxlvou (J;fjcpov xfjc; dvapdaecoc; xfjc;
529
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xov (J;fjcpov xoO xo^ou xoO xaLpou xfjc; dvapdaecoc; xfjc; aeXTQvric; dvco xoO
xavovLou, ovxa xal xoOxov 8l' xoxxlvou. £v6a oOv auvSpd^coatv ol (J;fjcpoL ex
SLaaxTj^dxcov xpaxsLxaL 6 eOpsGelc; (J;fjcpoc; exeu d xl eOpsGfj olko [xoipcdv xal
5 XsTixcov, £X£Lvo xo^ov SGxl xfjc; xaxapdaecoc; xfjc; fjXLOu.
ALalpsGLc; {y]). Ilepl xfjc; dvapdaecoc; xfjc; aeXTQvric; ^exd x/jv Suglv xoO fjXLOu
duo xoO xavovLou xouxou
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aeXTQvric;, xal xrjpeLxaL elie voxlov elie ^opeiov sgxlv. sxslvo oOv x6 TiXdxoc;
10 cpuXdxxexaL. eneiioL xaxaXa^pdvexat f) ea^dxr) dvdpaatc; xfjc; ^olpac; xfjc;
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xfj dvapdasL* si he voxlov, dcpatpsLxaL e'E, exeivou. xal sOplaxexaL f) ea^dxr)
dvdpaoLc; xfjc; aeXTQvric;. elxa auxr) ^rixsLxaL sic; xo xavovLov xfjc; xaxapdaecoc;
xoO fjXLOu xal dvapdaecoc; xfjc; aeXrivriq eiq xov Std xoxxlvou (J;fjcpov. £v6a
15 oOv eOpsGfj xax' | evavxlov xouxou [xeaov xoO xolouxou xavovlou, 6 xatpoc; fsosrv
I ^rixsLxaL xoO xo^ou. £v6a eOpsGfj, xax' evavxlov xouxou 6 dvco (J;fjcpoc; xoO 92vv
xavovLou 6 Std xoxxlvou xpaxsLxaL. xal sxslvo sgxlv f) dvdpaatc; xfjc; aeXrivriq
fjVLxa vea cpavfj.
7 TOUTOU om. Vv II 11 TauTiT]] TOUTcp codd.
530
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£Lc; xov Tiap' fj^cov 88 yLvo^evov (J;fjcpov.
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£Lc; xd xo^a xfjc; dvapdaecoc; xal xfjc; xaxapdaecoc; xoO xatpoO nepiaaeioL xal
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15 xfjc; aeXrivriq olko xcov c; ^oLpcov ecdq xcov r), xo xo^ov xfjc; dvapdaecoc; xoO fjXLOu
3 \iETa auvoSov om. L || 5 xeaaapa Vv || 6 yLvo^evov om. Vv || is xal om. Vv
II 14 xal om. Vv
531
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xoO (J^TQcpou £X£Lvou xfjc; xpuxdviTjc; GecopsLxaL xax' evavxLov. ei oOv exaaxov
10 s^LGoOxaL xcp (j>W9 "^"^^ L8Lac; xpuxdvirjc; y] tiXsov eaxl xouxou, f) aeXTQvr)
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15 xLc; oQev 6 (J;fjcpoc; oOxoc; xaxaXL^TidvexaL. xal exepoc; ^£6o8£ij£xaL (be; STiSLxa
prjOiQaexaL.
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-9 6^. . . ToO (|>ir]cpou in marg v || 12 xpLCOv Vv || 13 y^ ] p Lvv
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15 XOLVUV 6 (J;fjcpoc; 6 duo xoO evoc; xal xcov Suo ISla xpaxsLxaL. STiSLxa 6 duo xoO
evoc; (J;fjcpoc; dcpatpsLxaL olko xoO Seuxepou. d xl xaxaXsLcpGfj, sxslvo opQcdoiq
XeyexaL. xal xoOxo fjyouv f) opGcoatc; xrjpeLxaL. sic; xov (J;fjcpov Se xoOxov Suo
xLvd SLGLV £cp' olc; )(pfi STiLaxfjaaL xov voOv.
3 EiC, Vv I (J^fjcpo^ + 6 Vv II 4 EiC, Vv || 5 eIc, Vv II 10 5U0 V II 15 /3 L W 17
f] om. V
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FLvexaL TTQpriaLc; elc; xriv Tipcixriv Gecoptav. dnep eaxlv eXdxxcov dmb xoO
a'xo^ou y] lar), Gecopta oOx eaxL xfjc; aeXTQvric;. Sloc xl; oxl f) aeXTQvr) £xl Otio x6
cpcoc; eaxL xoO tiXlou xexpu^^evr). | el 8' s^LaoOxaL xcp P' xo^cp y] tiXsov sgxlv, f) f94rv
5 aeXTQvr) OTie^eaxr) xoO cpcoxoc; xoO tiXlou xal Tipo xoO SOvat xov yjXlov cpatvexaL
auxT). xal xps^a (J;7]cpou oOx eaxLv ev xauXa. el Se x6 to^ov xoO cpcoxoc; tiXsov
xoO a xo^ou xal eXaxxov xoO P' , f) aeXTQvr) vea yevo^evr) elc; sxslvov sgxl
xov pa6^6v xoO cpavfjvaL y] ou.
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10 pouXo^evcov oOv fj^cov TioLYJaaL xov (J^fjcpov xoOxov tioloO^sv ouxcoc;* xo Tipcoxov
To^ov duo xoO xo^ou xoO cpcoxoc; dcpaLpoO^ev. el xl xaxaXsLcpOfj, sxslvo
Kepiaaeioi XeyexaL. xauxriv oOv Kepiaaeioiv \ xrjpoO^ev elc; xo a to^ov. el fissvL
XL sOpeGfj, ^epL^o^ev elc; x/jv cpuXaxQ^Laav exsLvriv opGcoaLv. el xl e^eXGr],
£X£Lvo dcpaLpsLxaL duo xoO a' xo^ou, xal sxslvo xo xaxaXsLcpGsv to^ov eaxl
15 xYJc; xeXelac; ocj^ecoc;.
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TripsLxaL f) xaxdpaoLc; xoO tiXlou. edv f) e^Laou^evr) auxr) xcp xo^cp xfjc;
3 TipCOTOU Vv II 4 SeUTSpcp V II 7 TipCOTOU Vv | SsUTSpOU V | yLVO^SVir] V II 10
PouXo^evcov ...TOUTOV om. Vv | tioloO^sv + oOv Vv || 12 Tipcoxov V || 14 Tipcoxou
Vv I xal exsLvo to] to yoOv Vv
534
TsXeioLc, 6(J;£Cl)c; y] tiXslcov, f) aeXTQvr) cpaLvexaL yevo^evr) vea.
El he pouXexaL tlc; dacpaXcoc; xripfjaaL xriv ^sGoSov xauxriv ^exa xcov Suo
XoLTicov, xoO a xal xoO y', XP'H "^"n^ spyaatav TioLfjaaL. eav oOv ^exa xoO
(J^TQcpou xoO a xouxou xavovLou cpavrj f) aeXTQvr), | Xeyo^ev oxl f) aeXTQvr) ^eydXr) f309rv
5 ocpsLXsL cpavfjvaL oSaxe xal xouc; d^pXucoTioLoOvxac; lSslv aOxiQv. el Se e^eXGr]
6 (J;fjcpoc; dmb xoO P' xavovLou, Xeyo^ev oxl f) aeXTQvr) ouxe Tidvu d^uSpd ouxe
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x/jv 6(J;lv. £l Se e^eXGr] 6 (J;fjcpoc; duo xoO y' xavovLou, epyaoLa oO yLvexaL 8l6xl
f) aeXTQvr) Tidvu eaxl xrjVLxaOxa d^uSpd xoLauxr) | oxl sl oOx eaxL vecpoc; sic; xov f94vv
10 oOpavov y] o^lxXt) xlc;, ol ocpGaX^ol ol pXsTiovxec; xaGapcoc; ^Xenouai xauxriv.
xal f) dpxT) xoO ^rivoc; oO Xoyl^exaL duo xoxe, dXXd ypdcpexaL sic; x/jv dpxTjv
xoO aOGrj^epLvoO ouxcoc; oxl | lacoc; tva cpavrj f) aeXTQvr). fi54 fl
KecpdXaLov 8'. Ilepl xoO (J;7]cpou xouxou tva SsLxQfj f) aeXTQvr) 8Ld SaxxuXcov
'Etisl -/^peioi xouxou xoO (J;7]cpou, TiepLaaeuovxaL sic; xov xotiov xfjc; aeXTQvric;
15 8 XsTixd OTicoc; eOpsGrj 6 xotioc; xfjc; aeXrivriq oxav Sur] 6 yjXloc; sic; STioySoov
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I -3 Yevo^evrjv. . .noifioai] el 5' eXaxTov ou cpaLvexaL sl 5e: eyevsTO f] {liQohoc, xal epyaata
^La ToO a xal y xavovlou Vv || s oOv om. Vv | ^exa ] Sta Vv || 4 toutou om. Vv
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II 9 TrjVLxauTa Tidvu sail Vv || ii apx^jv] axprjv L || 12 laco^] av xuxr] L || 14 (J^rjcpou
TOUTOU Vv II 16 Toaov om Vv
535
tiXlou £tl oOx ea xriv aeXTQvriv cpavfjvaL. eneiioL sx^oiXXeTOLi f) dvdpaaLc; xfjc;
aeXTQvric; xaGcbc; eppsGr) Tipoxepov (baauxcoc; xal x6 arj^SLov xfjc; dvapdaecoc;
xaGcbc; eppsGr) eiq x6 £ xecpdXatov xfjc; q ^otpac;.
Elxa exel xiGsxaL xdGsxoc; sic; x6 arj^SLOv xfjc; dvapdaecoc; ^exd xfjc;
5 djioSsL^ecoc; xauxTjc; tva sic; x6 ^epoc; xfjc; Suaecoc; ^tqxs pouvoc; ^tqxs vecpoc;
STiLTipoaGoOv.
AtaLpeaLc;.
''EjiSLxa 6 daxpoXdpoc; sic; x/jv xdGsxov exsLvriv xpe^dxat, xal s^LaoOxaL
^£xd xfjc; £v xfj yfj yevo^evrjc; eOGsLac; ypa^^fjc;. xal xrjpeLxaL f) dvdpaatc; xfjc;
10 aeXTQvric; Tioar) f) e^eXGoOaa duo xoO xavovlou xfjc; xaxapdaecoc; xoO fjXLOu
xal xfjc; dvapdaecoc; xfjc; aeXTQvric;. xal xlGsxaL x6 dxpov xoO titqxs^oc; xoO
daxpoXdpou sic; xov xoloOxov (J;fjcpov. eneiioL Std xoO evoc; 6cp6aX^oO xoO
exepou xa^^uaavxoc; GecopsLxaL Std xcov oticov xoO titqxs^oc; d ticoc; cpavfj f)
aeXTQvr). el he oO cpavfj Std xcov xolouxcov oticov, sxslvoc; 6 cpavelc; ev xcp oOpavcp
15 xoTioc; I £X£Lv6c; | eaxLv £v d) f) aeXTQvr) £v6a ocpsLXsL auxr) ^rjxriGfjvaL. fi54vL, f95rv
3 Tie^TiTov Vv I exTiT]^ V II 11 TO axpov] f] axpa L || 12 STiSLxa] elxa v
536
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e^epXovxaL yjtol OTie^LaxavTaL xoO cpcoxoc; xoO tiXlou, xal xaxd Tiotav oSpav
SLGspxovxaL Otio cpcoc; xoO tiXlou xaxd x6 Tipcot y] x/jv saTiepav
Kal oOxoc; 6 (J;fjcpoc; ouxcoc; eaxl xaQoyoKsp xal em xfjc; aeXTQvric;.
5 'Eksi oOv xps^a xoO (J;7]cpou xouxou, exsLvr) f) ^otpa f) e^ep^o^evr) ^exd xoO
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veaq cpaLvo^evrjc; x6 to^ov xoO xatpoO xfjc; xaxapdaecoc; xoO fjXLOu xal evxaOGa
ouxcoc; I ocpsLXsL sxpXrjGfjvaL. x6 xo^ov sic; x/jv Gecoplav xcov daxepcov xaxd f309vv
10 xouc; 'IvSouc; eaxL togov xoO Kpovou l£, xoO Aloc; La, xoO 'Apeoc; ty, xfjc;
AcppoSLXTjc; 6 xal xoO 'Ep^oO ty.
Kaxd xov IIxoXe^aLov ^exd xoO (J;7]cpou xoO xo^ou xfjc; xaxapdaecoc; xoO
fjXLOu £Lc; xov xatpov fjVLxa Suvr] 6 daxfip y] dvlaxT) saxl togov xoO Kpovou
La, xoO Aloc; l, xoO 'Apeoc; La X', xfjc; AcppoSLXTjc; oxav XLvfjxaL xax' 6p66v
15 ^, xal oxav OtiotioSl^T] e, xfjc; 'Ep^oO l.
''EjiSLxa xripsLxaL oxl xo ^fjxoc; xoO daxepoc; olko xoO fjXLOu tiogov svl. edv
fl xax' evavxLov xcov xo^cov xouxcov y] tiXsov, 6 daxfip cpalvexaL* el 8' eXaxxov,
6 daxfip oO cpalvexaL.
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I ToO^] 6 L I xf]^] f] L II 11 ToO] 6 L || is toO] 6 L || i4 toO^ ] 6 L | toO^] 6 L
I xf]^] f] L I £^ 6p6oO L II 15 xf]^] f] L
537
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xavovLou
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x6 xavovLov [xstol xoO (J;7]cpou xcov xaxapdaecov sic; x6 8' xXt^a sic; xdc; dcpx^c;
5 xcov ^coSlcov. edv oOv 6 daxrip sic; x/jv dpxTjv xcov ^coSlcov d xl svl, | slc; x6 f95vv
xavovLov xpaxsLxaL* el Se sic; x/jv dpxTjv xoO ^coSlou oOx eaxLv, 6 (J;fjcpoc; ogxlc;
£VL £Lc; x/jv dpxTjv xoO ^coSlou xpaxsLxaL, xal xrjpeLxaL (baauxcoc; xal el xl eOpsGrj
£Lc; x/jv dpxTjv xoO ^£x' aOxo ^coSlou. xal xoOxo xpaxsLxaL, xal ^exd xoO (J;7]cpou
xcov p ^coSlcov opGoOxaL (be; eppsGr) sic; x6 kXsov xal eXaxxov xfjc; ocj^ecoc;. d xl
10 oOv eOpsGrj, to^ov xfjc; Gecoplac; xoO daxepoc; sgxlv. elxa xpaxsLxaL f) [xeay] xoO
aOGrj^epLvoO xoO tiXlou xal xoO daxepoc; TiepLaasLa xal xrjpeLxaL. edv oOv 6
(J;fjcpoc; oOxoc; sic; x6 cpavfjvaL xov daxepa, exsLvr) f) TiepLaasLa edv tiXslcov xoO
cpavevxoc; xo^ou, 6 daxrip ecpdvr)* el 8' eXdxxcov, 6 daxrip oO cpalvexaL. el 8'
eaxlv oOxoc; 6 (J;fjcpoc; tva 8ijvr] 6 daxiQp, exsLvr) f) TiepLaasLa edv tiXslcov xoO
15 xo^ou oO d8o^£v, 6 daxrip sxl oOx £8uv£v sl 8' eXdxxcov, 6 daxrip ehuvev.
ALalpsGLc;. Elc; x/jv xaxaXTjcJ^Lv exsLvriv oxl 6 daxrip xaxd tiolov xaLpov 8ijv£l
3 xavovLov] xavova v || 9 5uo Vv
538
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'H [iSTOL^oLGic, ToO tiXlou xal exeivoxj xoO daxepoc; xaxaXa^pdvovxaL xal
I xiGevxaL sic; x/jv xaOXav. STiSLxa xrjpoOvxaL. edv 6 daxrip OtiotioSl^t], evoOvxat fissvL
xal al p ^exapdasLc;. el Se XLvsLxaL 6 daxrip e'E, 6p6o0, x6 eXaxxov dcpatpsLxaL
5 OLKO xoO TiXsLovoc;. d XL eOpsGrj, sxslvo ^sxdpaaLc; sgxl xeXela. xoOxo xrjpeLxaL.
eneiTOL exsLVT) f) TiepLaasLa xlGsxaL sic; x/jv xaOXav, xal x6 to^ov x6 cpavev sic;
x6 TiXdyLov xauxTjc; xlGsxaL. xal x6 eXaxxov dcpatpsLxaL xoO tiXslovoc;. d xl
xaxaXsLcpGrj, exelvo ^spl^exaL sic; exeivriv x/jv | xeXelav ^sxdpaaLv. el xl fsiorv
e^eXGr], fj^epaL elal oxl y] Suvsl y] dvlax^L 6 daxiQp.
10 KecpdXaLov c;'. | Ilepl xfjc; aeXTQvric; veac; cpaveLarjc; ^exd xcov (J^iQcpcov o'ixlvsc; f96rv
fivciGrjaav ^exd exepcov dXXcov ot xal eyevvT^Griaav duo xoO vooc; xoO Xa^avfj
£Lc; x/jv 686v x/jv euXriTixov Sl^a huc/^epeioiq xcov ^axpcov sxslvcov (J^iQcpcov,
[xeQoheuQevTCdv xouxcov Tipoc; aacpiQveLav xal Ppa^iixrixa. xoOxo sic; Suo exsGr)
SLaLpeasLc;.
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4 5uo Vv II 5 dTio om. V || ii \iETa + tcov V I x^^^^^'n ^ II 12 euXrjTiTov] euxoXov
L II 15 opGcoaeco^] opGco^axo^ L
539
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YJxLc; eaxl xfjc; STiLouarjc; Tipcotac; sic; x/jv X' fj^epav sic; xac; fj^epac; xcov Apdpcov.
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5 dcpaLpsLxaL duo xoO xoaou* x£ X' . d xl xaxaXsLcpGfj, sxslvo xo^ov XeyexaL
xfjc; Gecoplac; o\)y\ xsXslov. sxslvo xrjpeLxaL. STiSLxa x6 xo^ov xoO cpcoxoc; sic; x6
TiXdyLov exsLvrjc; xlGsxaL xal xrjpeLxaL. edv s^LaoOvxaL xal xd p, sxslvo x6 io^ov
xfjc; Gecoplac; xsXslov eaxLV zl 8' oOx s^LaoOvxaL, x6 eXaxxov dcpatpsLxaL xoO
TiXsLovoc;. d XL xaxaXsLcpGfj, sxslvo TiepLaasLa sgxlv. xoOxo xrjpeLxaL. STiSLxa
10 edv x6 lo^ov xoO cpcoxoc; eXaxxov f) xoO xo^ou xfjc; Gecoplac;, exsLvr) f) TiepLaasLa
£Lc; x6 lo^ov xoOxo xfjc; Gecoplac; svoOxaL. si eaxL tiXsov oticoc; yevrixaL x6 lo^ov
xfjc; Gecoplac;, xsXslov xoOxo slc; x/jv xaOXav xlGsxaL. xal x6 \oE,o\ xoO xatpoO
£Lc; x6 TiXdyLov xouxou xlGsxaL xal xrjpeLxaL. zl x6 xo^ov xoO xatpoO s^LaoOxaL
xcp xo^cp xfjc; Gecoplac; f\ iikeov^ f) aeXTQvr) cpalvexaL* el 8' oOx, oO cpalvexaL.
15 STiSLxa xripsLxaL x6 to^ov xoO cpcoxoc;. edv f) xoaov X£ X' y] tiXsov, f) aeXTQvr)
UTie^eaxri xoO cpcoxoc; xoO fjXLou xal Tipo xoO 80vaL xov yjXlov cpalvexaL* el 8'
eXaxxov, oO cpalvexaL.
1 TO om L II 2 f]TL^. . .fj^epav] xfj^ X' fj^epa^ Vv || 3 oOv om L || 7 5uo Vv
540
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tiXlou xal £Lc; x/jv expoXriv xfjc; aeXTQvric; veac; yevo^evrjc; ^exd xcov exepcov
FLvexaL aOGrj^epLvov xoO tiXlou xal xfjc; aeXrivriq eiq x/jv vuxxa x/jv X' duo xoO
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5 xal f) xaxdpaaLc; xoO fjXLOu xal f) ^exdpaatc; xfjc; aeXfjvrjc;. elxa dcpatpsLxaL f)
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eaxl xfjc; Gecoplac; oO^l xsXslov. xoxs xrjpeLxaL sic; x6 to^ov xoO cpcoxoc;. edv f)
eXaxxov xoO xo^ou xfjc; Gecoplac;, oOx £vl xp^^a xfjc; Gecoplac; xfjc; aeXTQvric;* el
8' s^LGoOxaL xouxcp y] TiXeov, cpalvexaL.
10 'O (J>fjcpoc;.
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cpcoxoc;, xal ylvexaL xsXslov. xoOxo xlGsxaL sic; x/jv xaOXav. xal f) xaxdpaatc;
xoO fjXLOu £Lc; x6 TiXdytov xouxou xlGsxaL. elxa xrjpeLxaL f) xaxdpaatc; xoO fjXLOu.
15 edv s^LGoOxaL ^exd xoO xo^ou xfjc; Gecoplac; xoO xeXsLou y] tiXsov xouxou, f)
aeXTQvr) cpalvexaL* el 8' eXaxxov, oO cpalvexaL. elxa xrjpeLxaL. el x6 xo^ov xoO
cpcoxoc; eaxL xoaov x8 X' y] tiXsov xouxou, f) aeXTQvr) Tipo xoO 80vaL xov yjXlov
II 18 ToO dacpaXoO^ opGco^axo^ L 8 svl] eoti L \\ 9 cpaLvexaL] sXtil^ lSslv auTrjv L || ii
5uo Vv II 12 5uo Vv
541
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542
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xal xfjc; xaxaXiQcJ^ecoc; xoO xotiou xcov ^OLpcov
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duo xoO eveaxcoxoc; exouc; xcov 'Pco^alcov dcpaLpsLxaL. el xl xaxaXsLcpGfj, X9^^^^
eiai xoO fjXLou xexeXsLCO^evoL ol TiapeXGovxec; duo xfjc; yevviQaecoc;. f) ^otpa Se
auxT) £Lc; 8 StaLpeLxaL xecpaXata.
10 KecpdXaLov ol . Ilepl xfjc; elaeXeijaecoc; xcov xpovcov oXcov xal xcov xpovcov xcov
yeveGXtaXoyLXCOv xal xoO xotiou xfjc; xu^iQ^ fexdaxou
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fj^epac;* el 8' exelvo xsXslov oOx eaxLv, oO he xoOxo. oOxoc; 6 (J;fjcpoc; ocpelXsL
xpax£La6aL sic; evGu^rjaLv.
1 huohexaTTi v || 3 ^OLpcov] ^epta^cov L || 8 f] om. L
543
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xatpov £X£Lvov OXL 6 yjXloc; ytvexaL sic; x/jv ^otpav exsLvriv xa6' y]v eyevexo | f) hstvl
^TQxrjaLc; xfjc; yevviQaecoc;
5 I ToOxo 6 TOKoq xoO Gs^eXlou xoO tiXlou xaXsLxaL sic; xov (J;fjcpov xoO f97vv
yeveGXtaXoyLXoO. oOxoc; 6 (J;fjcpoc; sic; xoOxo xo PlPXlov sic, xo ^fjxoc; xfjc;
^exapdaecoc; prjOiQaexaL. stisl pouXo^sGa slSevaL x/jv oSpav xoO xatpoO exsLvou
fjVLxa cp6dv£L 6 yjXloc; eiq x/jv ^otpav exsLvriv, xo aOGrj^epLvov xoO fjXLou
^rixsLxaL £Lc; xo ^eaov xfjc; fj^epac; oTiep eaxlv eyyuc; xfjc; ^oLpac; exsLvrjc; xo
10 xal yeyovoc; sic; xo ^fjxoc; xfjc; tioXscoc; exsLvrjc; | £v6a xal f) yevvrjaLc;. el fsiirv
oOv eaxL xo aOGrj^epLvov sxslvo s^lgou^svov ^exd xfjc; ^otpac; exsLvrjc;, f) oSpa
xoO ^eaou xfjc; fj^epac; oSpa eaxl xfjc; elaeXeijaecoc;* si 8' oOx s^LaoOxaL, f)
ebpsQelaoi Kepiaaeioi [xeaov xcov p xpaxsLxaL. xal xrjpeLxaL auxr) sic; xd x8. el
XL eOpsGfj, ^spL^exaL sic; x/jv ^sxdpaaLv xoO fjXLou. el xl e^eXGr], al &>poii eiai
15 xoO ^TQXouc;. eneiTOL xrjpeLxaL. edv xo aOGrj^epLvov xoO fjXLou eXaxxov f) xfjc;
^OLpac; exsLvrjc;, f) oSpa xoO ^tqxouc; evoOxat xfj oSpa xoO [ieaou xfjc; fj^epac;*
£L Se TiXeov, dcpaLpeixaL duo xfjc; ^otpac; exsLvrjc;. xal TiXrjpoOxaL 6 (J;fjcpoc; (be;
eppsGr) £Lc; x/jv Std^expov xal auvoSov fjXLou xal aeXTQvric;. xal sOplaxovxaL
8 cpGdvr] V II 13 h6o Vv
544
al S^poLi xfjc; eiaeXe^aecdc, dmb xfjc; fj^epac; y] xfjc; vuxxoc; sic; xov (J;fjcpov xcov
yevsGXLaXoyLXCov xal xcov xpovcov xcov alaGrixcov oXcov.
Elc; xov alaGrixov he xpovov Sv xl ocpsLXsL xrjpeLaGaL. eav f) ouxcoc; oxl | x6 fissrL
aOGrj^epLvov xoO tiXlou xsXslov oOx eyevexo ^exa xfjc; opGciaecoc; xfjc; fj^epac;,
5 xax' evavxLov xoO aOGrj^epLvoO xoO fjXLou ytvexaL elaeXeuaLc; elc; x6 xavovLov
xfjc; opGciaecoc; xfjc; fj^epac;, xal | xpaxoOvxat xa Tipcoxa xal P' XsTixa xfjc; oSpac;. fgsrv
xal £X£Lva svoOvxaL elc; x/jv oSpav xfjc; elaeXeijecoc;.
ALalpsGLc;. Ilepl xfjc; eiaeXeuaecdq xoO xotiou xfjc; Tuyjiq
Acp' oO xaxaXsLcpGfj f) oSpa xfjc; elaeXeijaecoc;, dTi' exsLvrjc; xfjc; oSpac; f) xu^iQ
10 sxpdXXexaL ouxcoc; xaGcbc; eppsGr) Tipoxepov.
'EtisI Se pouXo^sGa xfiv xuxiQv xfjc; elaeXeijaecoc; ^£0' exepou (J;7]cpou
expaXsLV, sxslvoc; 6 (J;fjcpoc; 6 (J;fjcp6c; sgxl xfjc; TiepLaasLac; xcov XP^^^^-
ylvexaL xolvuv ^TQxriaLc; oxl olko xfjc; yevviQaecoc; tiogol xP^vol TiapfjXGov. xal
xax' evavxLov xcov y^povcdv sxslvcov ylvexat eiaeXeuaiq eiq xo xavovLov xfjc;
15 iiepiaaeioLc, xcov xp^^cov, xal xax' evavxlov exeivou xpaxsLxaL. f) TiepLaasLa
exsLVT) ^£xd xfjc; opGciaecoc; xoO OcJ^ci^axoc; xeXela ylvexaL. xal exsLvr) del
svoOxaL xcp xoTicp xfjc; Tuyjiq exsLvrjc; fjyouv xfj dp^fj xfjc; yevviQaecoc;. d
XL eOpsGfj, edv f) tiXsov xfjc; jiepLcpopdc; xoO xuxXou xcov x^, f) TiepLcpopd
6 SeuTspa Vv || ii STid] STiSLxa Vv || 12 post xpovcov add et cancell xal xax' evaviLov
V
545
dcpaLpsLxaL e'E, exeivou [isx9^ ^^ yevriTaL eXaxxcov exsLvrjc;. d tl xaxaXsLcpGrj,
6 TOTioc; xfjc; tuxtjc; eaxl xfjc; elaeXeuaecoc;. xax' evavxLov exeivou ytvexaL
elaeXeuaLc; sic; x6 xavovLov xoO xotiou xfjc; Tuyjiq eiq x6 | TiXdxoc; xfjc; tioXscoc; fissvL
exsLvrjc; ev fj ytvexaL xrjVLxaOxa f) ^TQxriaLc; xoO yevsGXLaXoyLXoO. xal xax'
5 evavxLov exeivou f) xu^iQ sxpdXXexaL (be; eppsGr) Tipoxepov.
AtaLpeaLc;. Ilepl xfjc; xaxaXiQcJ^ecoc; xfjc; xu^iQ^ "^^^Ci \ieao\j xfjc; oLXou^evrjc; sic; x6
^fjxoc; xal TiXdxoc;
KpaxsLxaL f) Kepiaaeioi xfjc; ^earjc; xoO ^tqxouc; xfjc; tioXscoc; xal xfjc; ^earjc;
xcov 9. I el XL eOpsGfj, iiepLcpopd sgxlv. sl Se x6 ^fjxoc; xfjc; fj^exepac; tioXscoc; fsiiw
10 eXaxxov saxi xcov 9, exsLvr) f) TiepLcpopd sic; xov | xotiov xfjc; xu^iQ^ "^"H^ fj^exepac; fgsvv
TioXecoc; svoOxaL* si he tiXsov xcov 9, dcpaLpsLxaL. el xl eOpsGfj, xotioc; xfjc; xu^iQ^
eaxLV. xax' evavxlov exeivou sic; x6 xavovLov xoO xotiou xfjc; xu^iQ^ ^£xd xfjc;
euQeiaq ypa^^fjc; fjc; f) dp^T) olko xfjc; dp^fjc; xoO KptoO ylvexat eiaeXeuaiq^ xal
sxpdXXexaL f) xu^iQ- ^'^ S^ iQ ^PX'H "^^^ xavovlou exsLvou xoO ^exd xfjc; euQeiaq
15 ypa^^fjc; duo xfjc; dp^fjc; eoTi xoO Alyoxepcoxoc;, e'E, exeivou expdXXexat f) xu^iQ-
'ExsLvoc; oOv 6 xotioc; xfjc; xu^iQ^ ^ t^^Q' fj^cov TiepLaaeuexaL togov go. el
XL eOpsGfj, xoTioc; xfjc; xu^iQ^ eaxlv sic; x6 xavovLov sxslvo. £l pouXo^sGa x/jv
xu^TQ^ expaXsLV duo xoO [xeGOU xfjc; oLXou^evrjc; oxl x6 TiXdxoc; exsLvrjc; eaxl
546
Toaov Xy, exelvoc, 6 totioc; xfjc; tuxtq^ ^^^x'- ^ fevcoGslc; ^exa xcov ao, dXX' 6
Tipo auToO dcTio ToO TOTiou xfjc; TUXTjc; ToO £v Tcp xavovLcp ToO TiXdxouc; Tcov Xy
sxpdXXsTaL.
I KecpdXaLov P'. Ilepl xfjc; xaxaXiQcJ^ecoc; xoO xotiou xoO cpcoxoc; xcov daxepcov fi59rL
5 YJxoL xoO Tipoc; dXXrjXa xouxcov axTj^axLa^oO
IIpo xoO SLaeXGsLv sic; xov (J;fjcpov xoOxov xoaaOxd eiai Qe\ieXi(x d xpiQ
slSevaL. laQi oxl duo xoO l', xoO Tipcixou ^^XP^ ^^'^ "^^^ xexdpxou yj^lgu sgxl
xfjc; dvapdaecoc;, olko he xoO 8', xoO C t^^XP^ ^^'^ "^^^ ^'"^^ tj^lgu sgxl xfjc;
dvapdaecoc;.
10 AtaLpeaLc;. Ilepl xoO ^tqxouc; xcov daxepcov duo xcov ^ oloc; xal eaxLV duo xoO
xevxpou xoO 8' xal xoO l' ^exd xoO (J;7]cpou xoO IIxoXe^aLou
KpaxsLxaL 6 xotioc; xfjc; xuxtjc; xcov daxepcov ^exd xfjc; eOGsLac; ypa^^fjc;. elxa
xripsLxaL. £L eaxLV 6 daxfip UKsp yfjv, xpa|x£LxaL f) ^otpa xoO l' olxiQ^axoc; ^exd f99rv
xfjc; euQeioiq ypa^^fjc;* el 8' Otio yfjv 6 daxiQp, xpaxsLxaL f) ^otpa xoO xotiou
15 xfjc; xuxTjc; xoO 8' olxiQ^axoc; ^exd xfjc; eOGsLac; ypa^^fjc;. elxa xrjpeLxaL. edv 6
daxfip UTiep yfjv ^eaov xcov C xo^l "^^v £ , 6 xotioc; xfjc; xuxtjc; xoO daxepoc; duo
7 Sexdiou V, L
547
ToO TOTiou xfjc; TUXTQ^ '^^^ ^' OLXTQ^axoc; dcpaLpsLxaL. d tl xaxaXsLcpGrj, ^fjxoc;
eaxL dcTio xoO l'. £l Se 6 daxrip ^eaov xoO l' xal xoO a olxiQ^axoc; xoO xotiou
xfjc; xuxTjc;, 6 xotioc; xfjc; Tuyjiq 6 l' duo xoO xotiou xfjc; xuxtjc; xoO daxepoc;
dcpaLpsLxaL. el xl xaxaXsLcpGfj, ^fjxoc; sgxl xoO daxepoc; duo xoO l'. £l 8' eaxlv
5 6 daxfip (jKO yfjv, xrjpeLxaL. edv ^eaov xfjc; xu^iQ^ ^^o^^- '^^^ S' ^ ^ xotioc; xfjc; Tuyjiq
I xoO daxepoc; dcpatpsLxaL duo xoO xotiou xfjc; xuxtjc; xoO 8'. d xl xaxaXsLcpGfj, fi59vL
^fjxoc; eaxL xoO daxepoc; | duo xoO 8'. si he 6 daxfip ^eaov xoO 8' xal xoO C, f3i2rv
6 xoTioc; xfjc; xu^iQ^ ^ S ' ^^^ "^^^Ci xotiou xfjc; xuxTjc; xoO daxepoc; dcpatpsLxaL. d
XL xaxaXsLcpGfj, ^fjxoc; sgxl xoO daxepoc; duo xoO 8'.
10 AtaLpeaLc;. Ilepl xoO TiXdxouc; xfjc; xlvtqgscoc; xoO xuxXou fjyouv xoO TiXdxouc;
xcov TioXecov
'Eiiei xpeioL xeveoQoLi xov (J;fjcpov xoOxov, x6 ^fjxoc; xoO daxepoc; duo xoO
xevxpou xoO l' y] xoO 8' xrjpeLxaL sic; x6 TiXdxoc; xfjc; tioXscoc;. d xl eOpsGfj,
xripsLxaL. xoOxo Qe\ieXiov xaXsLxaL. STiSLxa xrjpeLxaL. edv 6 daxfip UKsp yfjv,
15 £X£Lvo x6 Qe\ieXiov ^spL^exaL sic; x6 yj^lgu to^ov xfjc; fj^epac; - 1 x6 alXdx^ xax' f99vv
'Iv8oijc;. £L 8' bub yfjv sgxlv 6 daxiQp, exelvo x6 Qe\ieXiov ^spL^exaL sic; x6
YJ^LGU TO^ov xfjc; vuxxoc; - x6 alXdxC d xl e^eXGr], iiXdxoc; eaxl xoO xuxXou
xfjc; XLVTQGSCOc;.
2 post eaxL V add et cancell toO daxepo^ || 7-9 d 5' ... 5 in marg v || i6 t6^ iter.
V
548
Elc; toOto to TiXdxoc; xavovLov xoO totiou xfjc; tuxtq^ "^^^ ^coSlcov yLvexaL (be;
OCV £X£LVO f) TO Gs^sXlOV £Lc; to XLVrj^a TCOV dcGTspcov
AtaLpeaLc;. Ilepl toO totiou toO cpcoTOc; tcov daTspcov yjtol toO Tipoc; dXXriXa
TOUTCOv axTj^aTLG^oO o'lnep e^^^^^ TiXdTOc; [xstol toO (J;7]cpou xal hia toO
5 xavovLou
'IgGl* edv 6 daTrip TiXdToc; oOx e^Tl^ '^'^ To^a toO e^aycivou xal TSTpaycivou
xal TpLycivou xal ttjc; Sta^STpou Toaa * ^, 9, px, pii, a^, ao. edv exTl
TOLVuv 6 doTTip TiXdTOc;, Td TO^a I TauTa tiXsov xal sXaTTOV ylvovTat &>v -/^peioi fieorL
dpQ(i>aecdq.
10 KpaTSLTaL oOv f) TpaxTjXaLa X. exsLvr) TrjpeLTaL elc; t/jv TSTsXeLCO^evriv
TpaxTjXaLav toO TiXdTouc; toO doTspoc;. d tl eOpsGrj, nap' eva paG^ov sXaTTOv
xpaTSLTaL. eneiTOL el tl eOpsGrj, exelvo TpaxTjXaLd sgtlv. to to^ov exsLvrjc;
xpaTSLTaL* £X£Lvo opGcoGLc; XeysTaL. toOto TripeiraL. SKeiioi Td 9 elc; TpsLc;
TOTiouc; TiGevTaL. elTa f) opGcoatc; exsLvr) duo toO ol dcpaLpeiraL xal tc5 y'
15 svouTaL. d TL eOpsGrj duo toO a' to^ov sgtI toO e^aycivou, f) Std^STpoc;
£X£LVOU TplyCOVOV TO P' TO^OV SGtI TOO TSTpaycivOU, f) Std^STpOc; £X£LVOU
aOGic; TSTpdycovov to y' to^ov sgtI toO TpLycivou, f) Std^STpoc; toutou to^ov
£gtI toO e^aycivou.
2 f] Om V, L II 6 £X^^ ^ II 14 TipCOTOU V I XpLTCp Vv II 15 TipCOTOU V || 16
SeUTSpOV V II 17 XpLTOV Vv
549
^fjcpoc; [xsTOi ToO xavovLou dcp' oO yLvexaL SfjXov to TiXdxoc; xoO daxepoc;
Kax' evavxLov xoO | TiXdxouc; xoO daxepoc; ytvexaL elaeXeuaLc; sic; x6 xavovLov fioorv
xoSe xcov axTj^axLa^cov xcov daxepcov, xal xpaxsLxat xax' evavxLov exeivou. el
XL eOpsGrj olko xoO a xal P' xavovLou xal x6 olko xcov p eOpsGev xavovlcov
5 xripsLxaL. STiSLxa x6 aOGrj^epLvov xoO daxepoc; xlGsxaL sic; x/jv xaOXav sic; p
xoTiouc;. exsLvoc; oOv 6 xpaxrjGelc; (J>fjcpoc; duo xoO a' xavovlou dcpatpsLxaL duo
xoO aOGrj^epLvoO xoO daxepoc; xoO xsGsvxoc; sic; x/jv xaOXav a', xal svoOxaL xcp
xsGsvxL aOGrj^epLvcp P'. d xl oOv eOpsGrj sic; x6 P' | 6 xotioc; [eaxl xoO cpcoxoc; fieovL, f3i2vv
xoO e^aycivou xoO daxepoc; £^ dptaxepcov, xal f) Std^expoc; xouxou xplycovov
10 eaxL Se^Lov. d xl he ebpeQfi dmb xoO a' e^dycovov sgxl Ss^lov, xal f) Std^expoc;
xouxou xplycovov sgxl dpLaxepov.
'O (J>fjcpoc; Se xoO P' xavovlou x6 TiXdxoc; xoO e^aycivou sic; exelvo x6 ^epoc;
£v6a eaxl x6 TiXdxoc; xoO daxepoc;. xal TidXtv oOxoc; 6 (J;fjcpoc; x6 TiXdxoc; eaxl
xoO xpLycivou eiq exelvo x6 ^epoc; £v6a oOx eaxL x6 TiXdxoc; xoO daxepoc;. x6
15 xexpdycovov TiXdxoc; oOx e^^^- £l yoOv SsTQasL xaxaXsLcpGfjvaL x6 xexpdycovov,
9 ^oLpaL svoOvxaL xcp aOGrj^epLvcp xoO daxepoc;, xal x6 xexpdycovov x6
dpLGxepov sOpLGxexaL. xal f) Std^expoc; xouxou x6 he^iov eam xexpdycovov.
I YevrjiaL Vv || 4 Tipcoxou Vv | Seuxepou Vv | 5uo Vv || 5 5uo Vv || 6 Tipcoxou
Vv II 7 TipCOTOU Vv I TCp OHl V || 8 SsUTSpcp Vv | SsUTSpOV V || 10 TipCOTOU V
II 12 SeuTspou Vv II 17 EOTi post TSTpdycovov L
550
xal TO TiXdxoc; xfjc; SLa^expou xoO daxepoc; xax' evavxLov eaxl xoO TiXdxouc;
xoO daxepoc; sic; x6 ^epoc; sxslvo £v6a oOx eaxLv 6 daxiQp.
AtaLpeaLc;. Ilepl xoO xotiou xoO | cpcoxoc; xcov daxepcov ^exd xfjc; evciaecoc; xcov fioovv
P xoTicov xfjc; Tuyjiq [xstol xoO (J;7]cpou xoO IIxoXe^aLou
5 XpsLac; yevo^evrjc;, xrjpeLxaL. edv 6 daxfip sic; x6 yj^lgu xfjc; dvapdaecic; sgxlv
duo xfjc; Gcpatpac;, xax' evavxLov xfjc; ^oLpac; xoO daxepoc; ytvexaL eiaeXeuaic, sic;
x6 xavovLov xoO xotiou xfjc; xu^iQ^ ^£xd xfjc; eOGsLac; ypa^^fjc;, xal duo ^eaou
xoO xavovLou 6 xotioc; xpaxsLxaL. xoOxo sic; c; xotiouc; xiGsxaL sic; x/jv xaOXav.
£Lc; xov a oOv xotiov evoOvxat ^, sic; xov P' 9, sic; xov y' px* xal duo xoO 8'
10 I dcpatpoOvxaL ^, duo xoO £ 9, xal duo xoO c;' px. STiSLxa exaaxov duo xcov c; fieirL
^rixsLxaL [xeaov xoO xavovlou xoO xotiou xfjc; xu^iQ^ ^£xd xfjc; eOGsLac; ypa^^fjc;.
'AvcoGsv oOv xoO xavovlou xpaxsLxaL x6 ^coSlov, xal ex TiXaylou al ^otpaL.
xal xd XsTixd aOGic; sxpdXXovxaL olko [xeaou xcov p xavovlcov (be; eppsGr)
Tipoxepov. d XL oOv e^eXGr], xaxd x/jv xd^Lv exeivriv eiq q xotiouc; xlGsxaL,
15 xal sOplaxexaL duo xoO ol xotiou x6 dptaxepov e^dycovov, xal duo xoO P' x6
dpLGxepov xexpdycovov, xal duo xoO y' x6 dptaxepov xplycovov, xal duo xoO
8' x6 Se^Lov e^dycovov, xal olko xoO £ x6 Ss^lov xexpdycovov, xal duo xoO c;'
4 5uo Vv II 7 post diio L add et cancell toO || 9 TipcoTov Vv | Seuxepov Vv | xpLxov
Vv I TSTdpTOU Vv II 10 Tie^TITOU Vv II 13 5U0 Vv II 15 TipCOTOU Vv | SsUTSpOU Vv
II 16 XpLTOU Vv I XpLyCOVOv] TSTpdyCOVOV V II 17 TSTdpTOU Vv I Tie^TITOU Vv I eXTOU
V
551
TO Se^Lov xpLycovov. xaOxa oOv xa c; fjyouv ol c; axTj^axLa^ol xrjpoOvxaL.
''EjiSLxa aOGic; xax' evavxLov xoO aOGrj^epLvoO xoO daxepoc; ytvexaL
elaeXeuaLc; sic; x6 xavovLov xoO xotiou xfjc; xu^iQ^ "^^^ ^coSlcov | slc; x6 TiXdxoc; fioirv
xfjc; KoXecdq exsLvrjc; £v6a f) yevvrjaLc;, xal 6 xotioc; xfjc; xu^iQ^ xpaxsLxaL duo
5 [xeaou xoO xavovLou xal sic; c; xotiouc; xiGsxaL. | xal ylvexat 6 (J;fjcpoc; oOxoc; fsisrv
(be; 6 a' xsGslc; sic; c; xotiouc; xax' evavxlov xcov c; sxslvcov (J^iQcpcov, 6 ol bub
xov a', 6 P' Otio xov P', xal xaGs^fjc;. STiSLxa xrjpeLxaL, oxl ol p oOxol (J;fjcpoL,
exaaxoc; ^exd xoO exepou, xax' evavxlov elalv y] ou, 6 ol [xstol xoO a' xal
I xaGs^fjc;. edv oOv &ai xal ol p s^lgou^svol, 6 xotioc; xcov c; cpcoxcov xcov fieivL
10 daxepcov fjyouv xcov axTj^axLa^cov opGoc; sgxlv.
El he xax' evavxlov oOx datv, X9^^^ '^^^ xouxcov opGciaecoc;. opGcoGsvxoc; he
xoO evoc; xal xd exepa opGoOvxat. enei yoOv xp^^a sxpXrjGfjvaL x/jv opGcoatv
exdaxou, f) Kepiaaeioi exdaxou xpaxsLxaL fjyouv f) ebpeQelaoi [xeaov xoO a'
xal xaGs^fjc;. sxslvo xrjpeLxaL sic; xo ^fjxoc; xoO daxepoc; duo xoO i y] xoO 8'
15 xevxpou. el xl oOv eOpsGrj, exelvo Qe\ieXiov XeyexaL. xoOxo xrjpeLxaL.
ndXtv he xripsLxaL. edv 6 daxrip bnep yfjv, sxslvo xo Qe\ieXiov ^spl^exaL sic;
xo YJ^LGU TO^ov xfjc; fj^spac; xoO daxepoc;. ei he (jko yfjv 6 daxiQp, exelvo xo
Gs^sXlov ^spl^exaL sic; xo yj^lgu xo^ov xfjc; vuxxoc; xoO daxepoc;. el xl eOpsGfj,
opGcoGLc; eaxLv. xal aOGic; xrjpeLxaL sic; exelvac; xdc; y dxxLvopoXlac; xoO daxepoc;,
6 TipCOTO^ Vv I TipCOTO^ Vv || 7 TipCOTOV Vv | SsUTSpO^ Vv | SsUTSpOV Vv | h6o
Vv II 8 TipCOTO^ Vv I TipCOTOU Vv || 9 h6o Vv II 13 TipCOTOU Vv || 19 XpSL^ Vv
552
YJyouv Touc; xpsLc; axTj^axLa^ouc; xouc; £^ dpLaxepcov, dcp' d)v exaaxoc; duo xcov
P (J^TQcpcov e^fjXGsv oxl tioloc; sgxlv eyyuc; xoO daxepoc;. exsLvr) oOv f) opGcoatc;
svoOxaL £Lc; sxslvo x6 eyyuxepov. | xal sic; xdc; y dxxLvopoXtac; xdc; e^ Ss^lcov fioivv
eiq x6 Tioppcixepov svoOxaL, xal eOptaxovxaL ol c; axTj^aaxLa^oL
5 El he 6 daxrip sic; x6 yj^lgu xfjc; xaxapdaecic; sgxl xfjc; acpatpac;, oOxol ol
prjGevxec; (J;fjcpoL sic; xov xotiov xfjc; xu^iQ^ "^"H^ SLa^expou xoO daxepoc; ylvovxat.
el XL oOv eOpsGrj, Std^expoc; sgxl xoO | cpcoxoc; xoO daxepoc;. c; ^cpSta del fi62rL
svoOvxaL xrj SLa^expcp xauxr], xal sOplaxexaL x6 cpcoc; xoO daxepoc;.
El oOv pouXri6co^£v xal dXXcoc; spydaaaGaL x/jv xsxvtjv xauxriv, x6 TiXdxoc;
10 xfjc; XLVTQGSCOc; xoO xuxXou xaxaXa^pdvexat, xal x6 xavovLov xoO xotiou xfjc;
xu^TQ^ "^^^ ^coSlcov £lc; sxslvo x6 TiXdxoc; yLvciaxexaL (be; dv yevrixaL 6 (J;fjcpoc;
eOXriTixoxepoc;. stisI yoOv pouXo^sGa TioLfjaat (J;fjcpov, xrjpeLxaL. edv 6 daxfip
£Lc; x6 YJ^LGU xfjc; dvapdaecoc; xfjc; acpalpac; eaxLV, 6 xotioc; xfjc; Tuyjiq xfjc; ^olpac;
exsLvrjc; xpaxsLxaL duo xoO xavovlou exsLvou. el Se 6 daxfip sic; x6 yj^lgu
15 xfjc; xaxapdaecoc; xfjc; acpalpac; eaxLV, 6 xotioc; xfjc; SLa^expou xfjc; ^olpac; xoO
aOGrj^epLvoO xoO daxepoc; xpaxsLxaL sic; x6 xavovLov xoO xotiou xfjc; xu^iQ^ ^'^^
x6 TiXdxoc; xfjc; KoXecdq \ [xenoi xfjc; euQeiaq ypa^^fjc;. xal 6 (J;fjcpoc; exdaxric; fsisw
dxxLvopoXlac; sic; exelvov xov xotiov xfjc; Tuyjiq evoOxat (be; eppsGr) £v xolc; ^
xal 9 xal px, dcpaLpeaecoc; xal TipoaGsaecoc; yLvo^evrjc;. xal 6 (J;fjcpoc; 6 exepoc;
1 Tcov om Vv II 2 5uo Vv || 3 xpsL^ Vv II 4 xal iter, v
553
ouTCO TiXrjpoOTaL (be; eppsGr) Tipoxepov. el tl eOpsGrj, SLd^expoc; soti toO cpcoxoc;
Tcov daxepcov sxslvcov. slc; exaaxov c; ^(iSta Ti:poa|TL6£VTaL, xal ebpiaxsTOLi to fio2rv
cpcoc; Tcov daxepcov.
'O (J>fjcpoc; oOtoc; 8l' ocXXtjc; ^sGoSou eOXriTiTOTepac;
5 'Eksi hi evbq totiou xfjc; Tuyjiq yLvexaL 6 (J;fjcpoc; toutou outcoc;, to xavovLov
ToO TOTiou xfjc; TUXTQ^ ^exd | xoO TiXdxouc; xoO xuxXou xfjc; xlvtqgscoc; cpepexaL fi62vL
dvd x^^Lpocc;, xal ol Xex^evxec; oOxol (J;fjcpoL duo xoO xavovLou xouxou yLvovxat.
xal -/^peioi oOx eaxL xoO xotiou xfjc; xu^iQ^ ^£xd xfjc; euQeioiq ypa^^fjc;.
KecpdXaLov y - Hepl xfjc; xlvtqgscoc; xoO alXdx^ fjyouv xoO £^ ISlac; | StavoLac; fiesrL
10 yevo^evou xal xoO xotiou xfjc; ^olpac; exsLvrjc;
'IgGl oxl f) XLvrjaLc; xoO alXdx^ xa6' exaaxov xp^vov xoO fjXLOu ^la ^otpa
xoO xoTiou xfjc; Tuyjiq eaxLV. stisI yoOv ^la ^otpa xov xp^vov £ XsTixd slglv
£Lc; xov a ' ^fjva, xal c; fj^epaL sic; xo £v Xstixov, xal Sexa Seuxepa XsTixd
fj^epa ^la. xal sic; oXouc; xouc; (J;7]cpouc; ouxco ylvexat, xoOxo xo alXdx^ OTiep
15 XLVSLxaL ^£xd xcov I daxepcov xal xcov (bpcov xcov xaXcov xal xaxcov XLVSLxaL fio2vv
2 TO om V II 12 post ^OLpa V add et cancell toO totiou xfj^ tuxtt]^ eaxl || is eva LV
I L p L II 15 XLVoOaL LV | XLVoOaLV LV
554
OTL dcTio TOUTOutva xaxaXsLcpGrj otl 6 dcvGpcoTioc; sxslvoc; ^TQaexaL y] xeXeuTTQasL.
evxaOGa Se sic; xriv XLvrjaLv xauxriv xoO alXax^ p (J;fjcpoL slaepxovxaL. sic; (J;fjcpoc;
exelvoq oxl slc; x/jv ^otpav exeivriv x6 alXax^ Sl^coc; XLvsLxaL Seuxepov sxslvo,
oxL ocpsLXsL xaxaXrjcpGfjvaL 6 xatpoc;, f) Se ^otpa oOx £^ dvdyxric;. Std xoOxo
5 oOv x6 xecpaXaLov xoOxo sic; p SLaLpsLxaL.
AtaLpeaLc; a . Ilepl xoO (J;7]cpou exsLvou tva yLvciaxrixaL f) ^otpa xoO xatpoO
dyvoou^evou
'Etisl xps:Loc yeveaGaL | xov (J;fjcpov xoOxov, iipcoxov 6 xotioc; xfjc; xu^iQ^ "^^^Ci f3i4rv
alXdx^ ^£xd xoO xotiou xfjc; Tuyjiq xfjc; ^OLpac; exsLvrjc; ^exd xoO TiXdxouc; xfjc;
10 TioXecoc; xpaxsLxat, xal exaaxov lSloc xiGsxaL. elxa xrjpeLxaL x6 alXdxC sdv f)
£Lc; x/jv ^OLpav xoO l ' OL|x7]^axoc; y] xoO 8' , 6 xotioc; xfjc; xu^iQ^ exsLvou ^exd xfjc; fiesvL
eOGsLac; ypa^^fjc; duo xoO xotiou xfjc; xu^iQ^ exsLvou ^exd xfjc; eOGsLac; ypa^^fjc;
dcpaLpsLxaL* el Se x6 alXdx^ sic; x/jv ^otpdv sgxl xoO C olxiQ^axoc;, 6 xotioc; xfjc;
xuxTjc; xfjc; SLa^expou exeivou [xstol xoO TiXdxouc; xfjc; tioXscoc; duo xoO xotiou
15 xfjc; xu^TQ^ "^"H^ SLa^expou exsLvrjc; xfjc; ^oLpac; ^exd xoO TiXdxouc; xfjc; tioXscoc;
dcpaLpsLxaL. d xl xaxaXsLcpGfj, x6 to^ov eaxl xfjc; xlvtqgscoc;.
Elc; exdaxriv oOv ^otpav sic; )(p6voc; xpaxsLxaL ouxcoc; (be; dprjxaL Tipoxepov
(be; dv 6 xatpoc; xfjc; xlvtqgscoc; yv(opLa6fj. el he x6 alXdx^ ^eaov eaxl x(ov
2 5uo Vv II 3 XLVouaL LV II 4 xaxaXsLcpGfjvaL ut videtur L || 5 h6o Vv
555
Suo xevxpcov, exel opGcoatc; yLvexaL ouxcoc;. eav to alXax^ sic; to yj^lgu xfjc;
dvapdaecoc; xfjc; | acpatpac;, f) TiepLaasLa f) ^ear) xoO xotiou xfjc; xu^iQ^ "^"H^ ^OLpac; fiosrv
£X£Lvou [xsTOi xfjc; sOGsLac; ypa^^fjc; sic; xo TiXdxoc; xfjc; tioXscoc; xpaxsLxaL xal
xripsLxaL. £X£Lvo £Lc; xo ^fjxoc; xoO alXdx^ olko xoO xevxpou xrjpeLxaL. el xl
5 eOpsGfj, Qe\ieXi6v sgxlv. STiSLxa xrjpeLxaL. edv Oiiep yfjv sgxl xo alXdx^, exelvo
xo Gs^sXlov £lc; xo yj^lgu xo^ov xfjc; fj^epac; xoO alXdx^ ^spL^exaL* el 8' bub
yfjv, £Lc; xo yj^lgu to^ov xfjc; vuxxoc;. d xl e^eXGr], opGcoGLc; sgxlv. STiSLxa
xripsLxaL ^£xd xoO xotiou xfjc; Tuyjiq xfjc; euQeioiq ypa^^fjc;. edv tiXsov xoO
xoTiou xfjc; Tuyjiq xfjc; tioXscoc;, f) opGcoGLc; e^ exsLvou dcpaLpsLxaL* el 8' eXaxxov,
10 svoOxaL £X£Lvcp. I d XL eOpsGfj, 6 xotioc; xfjc; xu^iQ^ '^^^ ^OLpac; xoO alXdx^ sgxl fi64rL
xeXsLoc;. xoOxo xrjpeLxaL. f) TiepLGGSLa [xeaov xoO xotiou xfjc; xu^iQ^ ^£xd xfjc;
euQeioiq ypa^^fjc; exsLvrjc; xfjc; ^oLpac; ^exd xoO xotiou xfjc; Tuyjiq xfjc; tioXscoc;
exsLvrjc; xfjc; ^oLpac; xpaxsLxaL. sxslvo slc; xo ^fjxoc; xoO alXdx^ xrjpeLxaL, xal
£Lc; xo YJ^LGU TO^ov xfjc; fj^epac; y] xfjc; vuxxoc; xoO alXdx^ ^spL^exaL. xal 6
15 exepoc; (J;fjcpoc; TiXrjpoOxaL (be; eppsGr) tva 6 xotioc; xfjc; xu^iQ^ exsLvrjc; xfjc; ^olpac;
eOpsGfj xeXsLoc;.
''EjiSLxa 6 xoTioc; xfjc; Tuyjiq 6 xsXsloc; xoO alXdx^ olko xoO xotiou xfjc; Tuyjiq
xfjc; ^oLpac; exsLvrjc; dcpaLpsLxaL. el xl xaxaXsLcpGfj, to^ov sgxI xfjc; xlvtqgscoc;. ei
he xo alXdx^ sic; xo yj^lgu xfjc; xaxapdGSCOc; xfjc; Gcpalpac;, 6 xotioc; | xfjc; xu^iQ^ fiosvv
4 TTipeiTai iter. L
556
xfjc; SLa^expou xoO alXax^ xpaxsLxaL duo xfjc; ^oLpac; exsLvrjc;, | xal ytvexaL f3i4v
oOxoc; 6 (J;fjcpoc; tva x6 xo^ov xfjc; xlvtqgscoc; eOpsGrj. el Se QeXo\iev xov (J;fjcpov
xoOxov XsTixoxepov TioLfjaaL, Tipcoxov 6 xotioc; xfjc; Tuyjiq xcov ^coSlcov ^exd xoO
TiXdxouc; xoO xuxXou xfjc; xlvtqgscoc; [xenoi'/^eipi^eTOii. STiSLxa sic; xotioc; xfjc; Tuyjiq
5 xpaxsLxaL xoO alXdx^ y] xfjc; SLa^expou xouxou, xal TidXtv f) ^otpa exsLvr) xouxou
(baauxcoc;. STiSLxa 6 xotioc; xfjc; xu^iQ^ "^^^Ci alXdx^ duo xoO xotiou xfjc; xu^iQ^ "^"H^
^OLpac; exsLvrjc; dcpatpsLxaL tva eOpsGfj x6 to^ov xfjc; xlvtqgscoc;. xal exdaxou
^oLpa xpaxsLxaL (be; eppsGr).
I ALalpsGLc;. Ilepl xoO ^epLa^oO xfjc; ^olpac; xoO alXdx^ fi64vL
10 'EtisI syvciaGr) 6 xatpoc;, dnep oO yLvciaxexaL f) ^otpa sic; y]v XLVSLxaL
x6 alXdx^, XP^^^^ yevo^evrjc; yeveaGaL xov (J;fjcpov xoOxov, xrjpeLxaL x6
yeveGXtaXoyLXov noaoi xpovoL xal ^fjvec; xal fj^epaL ex xouxou TiapfjXGov.
xal exaaxoc; xpovoc; xoO fjXLOu ^la ^otpa xpaxsLxaL, xal exaaxoc; [xriv e XsTixd,
xal exdaxT) fj^epa Sexa Seuxepa XsTixd. el xl eOpsGfj, exeivo to^ov Xeyexat
15 xfjc; XLVTQGSCOc; fjyouv xfjc; eXdaecoc;. xoOxo cpuXdxxexaL. eneiioL xrjpeLxaL. edv
x6 alXdx^ £Lc; x/jv ^otpav xoO l' xal 8' xevxpou sgxlv, x6 to^ov xoOxo xfjc;
XLVTQGSCOc; svoOxaL £Lc; xov xoTiov xfjc; xu^iQ^ xouxou ^exd xfjc; euQeiaq ypa^^fjc;.
el XL eOpsGfj, sxslvo xrjpeLxaL sic; xo [xeaov xoO xotiou xfjc; Tuyjiq [xenoi xfjc;
12 xP^^o^ o^ L II 13 TievTS V II 14 Sexa] l L
557
eOGsLac; ypa^^fjc;, xal xpaxsLxaL to ^6)8lov dcvcoGsv xal al ^otpaL ex TiXayLou.
xal 6 (J;fjcpoc; xcov Xstitcov duo ^eaou xcov p xavovLCOv sxpdXXsTaL ouxcoc; | (be; fio4rv
dprjTaL TipoTspov.
EI XL eOpsGrj, 6 totioc; xfjc; [xoipoiq eaui xoO alXaxC £l Se x6 alXdx^ sic;
5 x/jv ^OLpdv eaxL xfjc; Tuyjiq^ oOxoc; 6 (J;fjcpoc; ^exd xoO xotiou xfjc; xu^iQ^ "^"H^
TioXecoc; yLvexat* el Se x6 alXdx^ sic; x/jv ^otpav xoO C olxiQ^axoc;, oOxoc; 6
(J;fjcpoc; ^£xd xoO xotiou xfjc; xuxTjc; xfjc; SLa^expou xoO alXdx^ ytvexaL sic; xov
xoTiov xfjc; xuxTjc; xfjc; KoXecdq. el xl eOpsGfj, Std^expoc; xfjc; ^oLpac; xoO ^epouc;
xoO alXdx^ eaxLV. | c; ^(iSta xouxcp TipoaxiGevxaL, xal sOpLaxexaL f) ^otpa xoO fiesrL
10 ^epouc; xoO alXdxC £l Se x6 alXdx^ [xeaov xcov p xevxpcov sgxlv, 6 (J;fjcpoc;
^£xd xcov p xoTicov xfjc; xuxTjc; oc^eiXei xeveaQoLi [xeTOL xoO xotiou xfjc; xu^iQ^ "^"H^
eOGsLac; ypa^^fjc; xal xfjc; KoXecdq. eKeiia xrjpeLxaL. edv x6 alXdx^ sic; x6 yj^lgu
eoTi xfjc; dvapdaecoc;, oOxoc; 6 (J;fjcpoc; ^exd xoO xotiou xfjc; ^olpac; xoO alXdx^
ylvexaL* ei he sic; x6 yj^lgu sgxl xfjc; xaxapdaecoc; xfjc; acpalpac;, | oOxoc; 6 (J;fjcpoc; fsisrv
15 ^£xd xfjc; SLa^expou xfjc; ^olpac; xoO alXdx^ ylvexaL. el xl eOpsGfj duo xcov Suo
xoTicov xfjc; Tuyjiq olko ^coSlcov, ^olpcov xal Xstixcov, exsLvr) f) ^otpa f) ^otpd sgxl
xoO alXdx^ ^£xd xoO (J;7]cpou exdaxou xotiou xfjc; xu^iQ^- ^^o^^- aOGic; xrjpeLxaL.
edv xal xd p xaxd xd ^(iSta, xdc; ^olpac; xal xd XsTixd s^LaoOvxaL, exsLvr) f)
^oLpa f) ^oLpa xoO alXdx^ xeXela* ei 8' oOx s^LaoOvxaL, ylvexat opGcoatc;.
I f] ^oLpa Vv II 2 5uo Vv II 10 h6o Vv || ii h6o Vv || is Tfj^^+TUxiT]^ f] LV
II 15 post YLvexaL add et cancell el he elc, to fi\iio6 eoti xfj^ xaxapdaeco^ xfj^ acpatpa^ v ||
18 5uo Vv
558
'O (J>fjcpoc; TOUTOU ouTCOc;* f) nepiaaeioL xcov p toticov xfjc; tuxtq^ xpaxsLxaL,
xal exsLVT) sic; to ^fjxoc; xoO alXax^ sic; to xevxpov to i y] 8' TTipelioLi. el tl
eOpsGrj, | Qe\ieXi6v eauiv. kolXiv TTipehoii. eav to alXocT^ Oiiep yfjv sgtlv, to fio4vv
Gs^sXlov toOto ^spL^STaL £Lc; TO YJ^LGU To^ov TTJc; fj^epac; toO alXdT^* el Se
5 TO alXocT^ Otio yfjv sgtlv, ^spL^STaL toOto eiq to yj^lgu to^ov ttjc; ^OLpac; toO
alXaT^ ^l TL eOpsGrj, exelvo opGcoGLc; sgtlv.
''EjiSLTa I TTipsLTaL £Lc; Tov TOTiov TTJc; TUXTjc; ^£Ta TTJc; eOGsLac; ypa^^fjc;. eav fiesvL
f) TiXeov ToO TOTiou TTJc; Tuyjiq TTJc; TioXecoc;, f) opGcoGLc; e^ exsLvou dcpaLpeiraL*
£L 8' sXaTTOv, f) opGcoGLc; £X£Lvcp svouTaL. d TL eOpsGrj, 6 totioc; ttjc; Tuyjiq
10 TTJc; ^oLpac; f) ^otpd sgtl toO alXocT^ ^stoc ttjc; eOGsLac; ypa^^fjc;. octi' exslvou
ToO TOTiou TTJc; TUXTjc; f) ^OLpa TTJc; ^OLpac; toO alXocT^ sxpdXXsTaL. si he to
alXocT^ £Lc; TO yj^lgu TTJc; xomoi^oiaecdq ttjc; Gcpatpac;, oOtoc; 6 (J;fjcpoc; ^stoc toO
TOTiou TTJc; Tuyjiq TTJc; 8La^£Tpou ToO alXocT^ yLvsTaL. d tl eOpsGrj, ^otpa ttjc;
8La^£Tpou TTJc; ^oLpac; sgtl toO alXaT^ ^ ^(pSLa toutco TipoGTLGsvTaL. el tl
15 eOpsGrj, f) ^otpd sgtl toO alXaT^
OOtoc; 6 (J;fjcpoc; [xenoi ocXXtjc; Td^ecoc; eOXriTiTOTepac; yLvo^evoc; [xenoi evbq
TOTIOU TTJc; TUXTjc;
El yevriTaL xp^^o^ yevsGGaL tov (J;fjcpov toOtov, 6 totioc; ttjc; Tuyjiq tcov
^coSlcov toO TiXdTouc; ttjc; xlvtqgscoc; xpaTSiraL. eneiioL TripeiraL. edv to alXocT^
1 5uo Vv II 5 ^OLpa^] sup lin fj^epa^ add et cancell V || 8 sxslvou] sxslvcov v
559
£Lc; TO YJ^LGU xfjc; dvapdaecoc;, oOxoc; 6 (J;fjcpoc; ^exd xoO xotiou xfjc; xu^iQ^ "^"H^
^oLpac; xoO alXdx^ duo xoO xavovLou xouxou yLvexat* el Se sic; x6 yj^lgu xfjc;
xaxapdaecoc;, oOxoc; 6 (J;fjcpoc; ^exd xoO xotiou xfjc; xuxtjc; xfjc; SLa^expou x6
alXdx^ I yLvexaL duo xouxou xoO xavovLou. fsisw
5 I KecpdXaLov 8' . Ilepl xfjc; evGu^iQaecoc; xfjc; xlvtqgscoc; xfjc; ^oLpac; xfjc; xu^iQ^ "^^^Ci fiosrv
yeveOXioiXoyixou eiq xov xpovov, sic; xouc; ^fjvac; xal xdc; fj^epac; xal sic; x/jv
XLvrjaLV xfjc; Tuyjiq \ xouxou xeaaapec; SLaLpeasLc; eiaiv. fieerL
AtaLpeaLc; a . Ilepl xfjc; evQuycfiaecdq exeivou xoO (J;7]cpou oxl xa6 ' exaaxov
Xpovov a ^6)8lov XLvsLxaL
10 'Etisl x9^^^ "^^^ (J>7]cpou xoOxou, ol xexeXsLCO^evoL XP^^^^ "^^^ fjXLou
ol TiaprjXGovxec; duo xoO yevsGXLaXoyLXoO xiGevxaL sic; x/jv xaOXav. xal
x6 arj^SLov xoO ^coSlou xfjc; xuxtjc; xoO Gs^eXlou xoO yeveGXtaXoyLXoO
TiepLaaeuexaL sic; xouc; )(p6vouc; exsLvouc;. d xl eOpsGfj, exelvo sic; xd i^
^spL^exaL, YJyouv dvd lP ytvexat xouxcov dcpatpeaLc;. d xl xaxaXsLcpGfj, exelvo
15 ^6)8lov ocpsLXsL ehoii ecp' d) f) XLvrjaLc; xfjc; Tuyjiq xax' sxslvov xov y^povov
£cp6aa£v. sxslvo xo ^6)8lov Ivxee xaXsLxaL.
5 evGu^TTjaeco^ + eXdaeco^ sup lin V || 7 toOto LV || 9 XLvoOaLv LV
560
'H ^oLpa oOv xal xa XsTixa exelvoL exsLvr) f) [xolpoL xal xa XsTixa xfjc; xu^iQ^
xoO Gs^eXlou slglv.
Kal f) XLvrjaLc; exsLvr) sic; xpta xLvd sgxlv. Sv oxl slc; exaaxov ^6)8lov ev
^6)8lov XLvsLxaL, xal xa6' exaaxov ^fjva 8uo ^otpaL xal yj^lgu, xal xa6'
5 exdaxriv fj^epav £ XsTixd. xal ^exd xouxou xoO (J;7]cpou f) ^otpa XLvsLxaL xfjc;
xu^TQ^ ^£xd xoO cpcoxoc; xcov daxepcov oxl f) xu^iQ ^axl xoO Gs^eXlou xal f) xuxt)
xfjc; elaeXeuaecoc;. Seuxepov oxl slc; exaaxov xp^vov Ly ^cpSLa dpLG^oOvxaL,
xal £Lc; exdaxriv fj^epav a ^otpa xal 8 XsTixd slglv, xal sic; xdc; xr) fj^epac;
xal STiLSexaxov xfjc; fj^epac; a ^coSlov Tiapepx^TaL. auxr) f) XLvrjaLc; XeyexaL xcov
10 ^rivcov. I xpLxov £X£Lvo OXL £Lc; xdc; XT) fj^epac; xal IsTiLSexaxov xfjc; fj^epac; Ly fiosvv, fieevL
^cpSLa dpLG^ouGLv, xal xa6' exdaxriv fj^epav togov Ly ^otpaL vy X£Ti:xd(auxri
£v xouxcp xcov fj^epcov f) XLvrjaLc;). xal sic; exaaxov olko xcov y xavovLov exsGr)
OXL 6 (J;fjcpoc; oOxoc; exelQev tva yevrixaL 8Ld xo euXriTixov.
ALalpsGLc; P' . Ilepl xfjc; xlvtqgscoc; xcov (J^iQcpcov xfjc; Tuyjiq xfjc; SLaeXeuaecoc;
15 'IgGl Tipcoxov OXL f) ^OLpa xfjc; xu^iQ^ "^"H^ SLaeXeuaecoc; xal xd olxiQ^axa
xauxTjc; xal ol daxepec; xouxcov sic; eva xpovov lP ^cpSLa xlvoOglv, xal sic; ^lav
fj^epav v6 XsTixd xal r) P' XsTixd - oxl f) XLvrjaLc; sgxlv f) ^ear) xoO fjXLou, xal
£Lc; £va xpovov ^exd xoO (J;7]cpou xouxou ^exd xoO cpcoxoc; xcov daxepcov oXcov
I exsLva difficile visu v || 5 tisvts Vv || lo stilSsxtov ut videtur v || 12 xpLCOv Vv
II 17 SeuTspa Vv
561
I XLvoOvxaL Sloc xfjc; acpatpac; TiXrjpcoGeLaric; xfjc; TiepLcpopac;. Seuxepov sic; x/jv fsier
XLvrjaLv xcov ^rivcov. exelvo sic, [xLolv fj^epav i^ [xolpoLi xal ^6 XsTixd. ^exa
xoO (J^TQcpou xouxou £Lc; xoaac; fj^epac; xel XsTixa xfjc; fj^epac; xal P' XsTixd* X
xq lP ^6)8lov a TiXrjpoOxaL sic; xov ^fjva xoO tiXlou.
5 AtaLpeaLc; y' . Ilepl xfjc; eXdaecoc; xfjc; xu^iQ^ "^"H^ eiaeXeuaecdq xoO ^rivoc; ^exd
xoO (J^TQcpou xouxou
Elc; xoaov xatpov X xc; i^ Z^cdhioL i^ eXauvovxat tva TiXrjpcoGfj f) TiepLcpopd.
xa6' exdaxriv eaxl xoaov ^otpat XsTixd* La v oSaxe elc; a ^fjva ol (J;fjcpoL xfjc;
xu^TQ^ "^^^ ^rivcov STiavaxuxXoOvxaL ^£0' oXcov xcov ocxxlvoPoXlcov xcov daxepcov.
10 xal Std xouxouc; xouc; (J;7]cpouc; xavovLa exsGrjaav oticoc; 6 (J;fjcpoc; euXriTixoc; f).
I ALalpsGLc; 8'. Ilepl xfjc; eXdaecoc; xfjc; elaeXeijaecoc; xfjc; xu^iQ^ t^^Q' fexepou fierrL
(J^TQcpou
'O xoTioc; xfjc; xu^iQ^ I '^^^ eiaeXeuaecdq xlGsxaL elc; x/jv xaOXav. xal elc; xov fioerv
a ^fjva xoO fjXLou KepiaaeueTOil togov ^ ly ^otpat xal XsTixd. el xl eOpsGfj,
15 £X£Lvo £Lc; xo [iSGOV xoO xavovLou xoO xoTiou xfjc; xu^TQ^ '^^^ TioXecoc; ^rixsLxaL.
xal xax' evavxLov exsLvou ^cpSta xal ^otpat xpaxoOvxat tva eOpsGfj f) ^otpa
3 SeuTspa Vv || 8 a^ ] eva Vv || i4 eva Vv
5 \
562
sic; Tov a ^fjva.
Kal f) ^oLpa exdaTrjc; fj^epac; £X£l6£v sxpdXXsTaL ^exd xoO (J;7]cpou toutou
£Lc; TOV a -/^povov xoO tiXlou. slc; tov totiov xfjc; Tuyjiq xfjc; eiaeXeuaecdq
KepiaaeueTOiiToaov' tic; ^8 8 xal SloctoOtov tov (J;fjcpov xavovLov STsGr) (be; dv
5 6 (J;fjcpoc; £X£l6£v suXtititoc; yevriTaL. el tl eOpsGrj nap' fj^cov e'E, dp^fjc; xal OTiep
UTieax^QTi^ev Tipoxepov sic; xauxac; xdc; i^ ^otpac; xal sic; xd xecpdXata exdaxTjc;
^OLpac; xal xdc; hioLKxpeaeic, xouxcov Tidvxcov, xoOxo sic; xo xeXoc; dpiQyovxoc; xoO
BeoO TQydyo^ev auv TipoGu^la. 6 Beoc; he StaxripTQaoL xov dvGpcoTiov sxslvov
oq x/jv auvxa^Lv xauxriv SlsXGcov ^d6oL dv (be; Set xd TiovrjGevxa nap' fj^oiv ev
10 aOxrj Tipoc; dxpipsLav.
1 £va Vv II 3 £va V | xf]^^ + xf]^ tuxtt]^ LV
563
First Appendix
S)(6Xlov toO Bpdva TiapaSsLy^axoc; x^P^-v
'O (J>fjcpoc; eiq y^povouq xcov 'Pco^atcov ^'\A louX lc; toO tiXlou slc; to ^ xoO
AeovToc; xal X6 ^otpac; Tiepl xfjc; opGciaecoc; xfjc; fj^epac; xax' evavxLov xoO
TiXdxouc; xfjc; tioXscoc; ^£. eyevexo eiaeXeuaic, sic, x6 xavovLov xfjc; opGciaecoc;
5 xcov fj^epcov, xal eOpsGr) (J>fjcpoc; xc; La. expaxT^Grjaav xax' evavxLov xfjc; STioxfjc;
xoO fjXLou yevLxd XsTixd x/jv dpxiQ^ xolouxcov xcov ^otpcov duo xoO a ^^XP^ ^^'^
xoO 9 , xal TidXtv STiavaaxpecpo^evcov. eOpeGrjaav oOv vl. xaOxa £xrip7]6riaav
£Lc; x/jv xpaxTjXaLav xfjc; opGciaecoc; xfjc; fj^epac; xd xc; La. SrjXovoxL xal e^fjXGov
xa vy Xa v.
10 TaOxa expaxT^Grjaav nap' eva pa6^6v xdxco xal eyevovxo x vy Xa v.
xal eOpsGr) f) xpaxTjXaLa xfjc; opGciaecoc; xfjc; fj^epac; xaOxa. xax' evavxlov
xfjc; xpaxTjXaLac; xauxTjc; expaxT^Gr) x6 to^ov 66. xal xoOxo f)v f) 6p6cL)aLc;
xfjc; fj^epac; sic; xdc; ^olpac; xoO fjXLOu. xrjVLxaOxa exelvoL he xd x vy Xa v
I eyevovxo xa xal fiv636riaav xolc; 9 xal eyevexo x6 yj^lgu to^ov xfjc; fj^epac; fiorvL
15 xauxTjc;. £8LTi:XaaLda6ri xauxr] xal eyevexo x6 to^ov xfjc; fj^epac; Tidarjc; yjxol
axp. £^£pLa6riaav sic; xd le. xaOxa xal £^fjX6ov al oSpat Tidarjc; xfjc; fj^epac;.
1 ToO Bpdva TiapaSsLY^axo^ x^P^^ ] ^'^^ TiapaSsLy^aTO^ + toO Ppdva in marg L || 2
\^A ] \^h V \x^ L I i-^ om L | toO fjXLOu ] exsLvr] Se toO fjXLOu L || 6 toloutcov ]
TioLouvTCOv V, L || 8 SrjXovoTL ] SfjXa L II 9 xalyXal v || lo xlyXal v || 13
xlyXal V II 14 xal om V || 15 TauTir] om V || 16 Tidarjc; ] TiaaaL v
564
Second Appendix
'AXXcoc; OLKO cpcovfjc; xoO Sd^cJ;
01 ♦ ^ -/^povoi dcpaLpoOvxaL olko toO enouq xcov 'Apdpcov. el tl xaxaXsLcpGrj,
d eoTi kXsov tcov ^, xd ^ dvdpaatc; ^La xpaxoOvxaL. d xl oOv eOpsGrj, duo
xcov dvapdaecov, o XeyexaL | xaxd Ilepaac; ^opcpoO, xal duo xcov xp^vcov sic; fio9rL
5 xd vy Seuxepa XsTixd del xrjpeLxaL. el xl eOpsGrj, duo ^otpcov xal Xstixcov
svoOxaL xcp eOpsGsvxL ev xcp xavovLcp (j>W9 "^^^ aOGrj^epLvoO xcov daxepcov xal
x6 aOGrj^epLvov xcov daxepcov sOplaxexaL sic; exelvo x6 exoc;.
1 dTio cpcovf]^ om. Vv || 2 tl] xLva v
565
Third Appendix
ToO Sa^cJ; elq toOto
TripsLTaL TO yj^lgu to^ov xfjc; vuxxoc; exsLvrjc; xal to yj^lgu to^ov toO
oLGTspoq xfjc; fj^epac;. el s^LaoOvxaL xal d^cpoxepa, exsLvr) f) sOpeGsLaa
TiepLcpopa oxav dvLaxT) 6 daxrip |xfjc; dp^fjc; | sgxl xfjc; vuxxoc;. si he xo f288vv, fii2vL
5 TO^ov xoO daxepoc; xfjc; fj^epac; eXaxxov duo xoO fj^Laecoc; xo^ou xfjc; vuxxoc;,
dcpatpsLxaL xouxo duo xou fj^Laecoc; xo^ou xfjc; vuxxoc;. el xl xaxaXsLcpGfj,
£X£Lvo svouxaL xfj TispLcpopd. d XL eupsGfj, TiepLcpopd eaxLv olko xfjc; dp^fjc;
xfjc; vuxxoc;. ei he xo yj^lgu to^ov xou daxepoc; xfjc; fj^epac; iikeov duo xou
fj^LGSCOc; xo^ou xfjc; vuxxoc;, xo eXaxxov dcpatpsLxaL (duo) xou tiXslovoc;. d
10 XL xaxaXsLcpGfj, sxslvo dcpatpsLxaL olko xfjc; jiepLcpopdc;. el xl xaxaXsLcpGfj,
TiepLcpopd eaxLV olko xfjc; dp^fjc; xfjc; vuxxoc;. xal olko xouxou xaxaXa^pdvovxaL
al ^rixou^evaL d^paL xfjc; vuxxoc;.
1 ToO Ea^(|> SLc; toOto] 6 'ApSoupax^o^vrjc; ^expov toOtov dprjxe xal 6 e^oc; bibaoxakoc,
TOvSe Tov ^expov TipoaeGrjxev L || 5 f]^Lau ut vid. v || 6 f]^Lau ut vid. v || 8
xf]^ fj^epa^ ToO daxepo^ L || lo d tl xaTaXsLcpGfj] to xaxaXsLcpGev Vv
566
Fourth Appendix
Xpr) eihevoLi otl eav dmb xoO KapxLvou xpaxriGrj 6 (J;fjcpoc; ev xcp xavovLcp xoO
a , xal 6 STspoq (J;fjcpoc; aOGic; duo xoO KapxLvou xoO £v xcp exepcp xavovLcp.
xal xaGs^fjc; ouxco xal ski xcov dXXcov ^coSlcov.
1 TOO^ Om V II 2 TipCOTOU Vv
567
Fifth Appendix
olov eav &ai X xal Xc; eiq xriv Kepiaaeioiv toutcov, xa c;.
1 £L^. . .xa ^ om. V
