Gregory, Olinthus Gilbert Lessons, Astronomical and Philosophical OLD CLASS S G8232kx BMED CA.L E^l^Senkler CKI.KSTIAI, HEMISPHERE LESSONS, ASTRONOMICAL AND PHILOSOPHICAL, FOR THE AMUSEMENT AND INSTRUCTION BEING AN ATTEMPT TO EXPLAIN AND ACCOUNT FOR THE MOST USUAL APPEARANCES IN NATURE IN A FAMILIAR MANNER, FROM ESTABLISHED PRINCIPLES. The Whole interspersed with MORAL REFLECTIONS. BY OLINTHUS GREGORY, LL.D. OF THE ROYAL MILITARY ACADEMY, WOOLWICH. -The glittering stars, By the deep ear of Meditation heard, Still in their midnight watches sing of HIM. He uods a culm; the tempests blow His wrath ; The thunder is His voice ; and the red flash His speedy sword of justice. At His touch The mountains flame. He shakos the solid earth, And rocks tlie nations. Nor in these alone, In every common instance GOD is seen. THOMSON, THE FIFTH EDITION, MUCH ENLARGED AND IMPROVED. LONDON: PRINTED FOR JOSIAH CONDER, 18. ST. PAUL'S CHURCH- YARH LONGMAN, Ht'RST, REES, ORME, AND BROWN, PATERNOSTER ROW; DARTON, HARVEY, AND DARTON, GRACECHURCH STREET ; SHERWOOD, NEELY, AND JONES, PATERNOSTER ROWJ AND LAW AND WHITAKER, A\E MARIA LANE. 1815. Etlettoo and lleoderton, Primers, Johnson's Court, London. TO THE RIGHT HON. JOHN JOSHUA PROBY, EARL CARYSFORT, EVER ZEALOUS IK THE PROMOTION AND ENCOURAGEMENT OF GOOD WORK.1j UNDER WHOSE PATRONAGE THE FORMER EDITIONS OP THIS PERFORMANCE MET WITH SO FAVOURABLE A RECEPTION; THE PRESENT IMPROVED EDITION IS RESPECTFULLY DEDICATED BT HIS LORDSHIP'S MOST OBEDIENT, AND MOST OBLIGED, HUMBLE SERVANT, OLTNTHLTS GREGORY. PREFACE. JL-T has been for a considerable time allowed by the majority of intelligent persons, that amongst a variety of studies there are none of greater utility, or that afford more real pleasure to a rational mind, than those on Philosophical Subjects. On mature delibe- ration it may be concluded, that this does not so much arise from any intrinsic value of Natural Philosophy, solely considered, as from the peculiar use to which it may be applied, and without which it hardly merits the name it has obtained : and this is no other, than regulating by it our observa- tions upon the numerous objects of the creation, whereby we may correct any erro- neous notions which we may have hitherto encouraged, either concerning them, or the a 2 OMNIPOTENT VI PREFACE. OMNIPOTENT BEING by whose Will they \vere formed. When it is considered how liable all our senses are to deception, and what wrong ideas are generally formed of the different parts of the universe from mere cursory ob- servation, the absolute necessity of the dis- 'semination of true philosophical principles will the more obviously appear. And if the rudeness and imbecility of the human mind in an uncultivated state of nature be taken into the consideration, it will be the more readily admitted, that every attempt to extend the sphere of human knowledge is laudable in its nature; and, if it be found to answer the intention, is deserving of encouragement. Being duly impressed with the force of these reflections, and also recollecting that it is the indispensable duty of every member of society, to render himself as serviceable to his fellow-creatures as his abilities will allow, I was induced to apply my leisure hours to the execution of a performance which might in some measure tend to the instruction PREFACE. Vll instruction of the Youth of Great Britain. And as iny principal design was to lay be- fore them some pages of the Volume of Nature, I judged that if this could be per- formed in such a manner as to be also a source of amusement, it would probably meet with a more welcome reception, and conse- quently have the better effect. I have likewise been cautious in checking any inclination to scepticism during the study of Natural Philosophy : and in guard- ing against a mischievous misapplication of the word Nature. I uniformly wish this word to be considered as an abridged form of expressing, sometimes the results of the laws to which the mechanism of the universe is subjected by the Supreme Being; some- times the collection of beings created by him. Nature viewed thus, in its true light, is no longer a subject of cold unproductive speculation, with regard to morality. The study of its productions and its phenomena not only enlightens the mind, but warms the heart, by exciting feelings of reverence and admiration, at the sight of so many wonders, bearing Vlll PREFACE. bearing such striking characters of unlimited power and matchless wisdom. Pursuant to these ideas 1 have divided the following work into easy lessons of various lengths, as the nature of the respective sub- jects would admit ; and have interspersed them with moral reflections, in prose and verse, in order to alleviate the mind of the student, and to lead him, by imperceptible degrees, to reflect seriously on the several objects around him. To the honour of our British Poets, it must be acknowledged, I was seldom at a loss for an Extract suitable to my purpose ; and if my acquaintance with their works had been more extensive, I be- lieve there would have been no occasion for those two or three little original pieces, which make so dim an appearance in such brilliant company. These Lessons may with propriety be in- troduced into Schools to be read before the master in greater or less proportions, as may be thought most proper : in which case they will answer a double purpose, — improving the Pupil in the Art of Reading, while they enlarge PREFACE. IX enlarge the bounds of his understanding. That they might be as much as possibly sub- servient to the former, without raising an impediment in the way of the latter, reflec- tions, attendant on the several subjects, are the more frequently introduced. To some persons it may perhaps appear necessary, that I should have given an ex- planation of all the technical terms which are found in the following pages : for in- stance, such as centre, or center, diaphanous, equinox, focus, glands, lacteal, peristaltic, &c. Here I would observe, that I have not neglected such explanation where it could be given without leading me too circuitous a course ; and even where it is otherwise, the omission will not afford an objection of great weight ; for there is scarcely a dic- tionary in which the requisite information may not be met with. Perhaps in schools this raay be productive of some advantage, as it may lead to inquiry ; but that this may have the better effect, it may be re- marked, that the preceptor does not pro- perly acquit himself in his duty towards his X PREFACE. his pupils, who does not indulge them in the liberty of asking every question, the solu- tion of which may have a tendency to in- crease their fund of learning. Masters, by acting thus, would undoubtedly be able to judge in what respects their scholars were most deficient; and could, of course, sup- ply those deficiencies from their own know- ledge, or from those helps which it may naturally be supposed they have at hand. In the composition of these Lessons, I have not scrupled to make a free use of the Works of several of the most esteemed Au- thors on Astronomy and Philosophy; and if I have not always acknowledged where the obligation lay, I may observe that such alterations were made, or the extracts taken in so detached a manner, as rendered it nearly, if not absolutely, impossible. When we remember that the improvements in these sciences were gradual aod not effected by one man, or by one age ; it must be allowed that every production (except those which boast of new inventions and discoveries) must be principally a compilation; and the chief merit PREFACE. xi merit to which the person who undertakes it can aspire, is that of arranging the mate- rials before him in a manner more suitable to his purpose, and making such reflections as may be best adapted to the subject. I am conscious, that in the present under- taking many imperfections will be met with : however, such as it is, I present it with cheer- fulness to the public view ; and if it meet with a favourable reception from the candid and ingenuous, I shall have but little to fear from the severe critic. Literary fame I want not to acquire : zeal for the welfare of the British Youth was the only motive which urged me to this performance ; and if it prove to be of service to- them, I shall think myself amply rewarded. As to the numerous defects, I must sue for indulgence by observing, that I am yet but a young man; and am wil- ling to hope that if health and leisure should permit, I may at some future period pro- duce something more worthy of public fa- vour. Yet, as I am desirous to make this Work as correct and useful as possible, I cannot but add, that those who will be so obliging Xli PREFACE. obliging as to furnish me with hints for its improvement, will confer a lasting obliga- tion upon me, and shall receive my grate- ful acknowledgments. O. G. GREGORY. Yaxley, May 20th 1793. ADVER- ADVERTISEMENT. GRATITUDE for the favourable reception which the first Edition of these LESSONS has experienced, has induced the Author to give them a careful revisal, in order that this New Edition may be found less un- worthy of public favour. In this revisal, he has been assisted by the polite suggestions of some of the Review- ers, (for whose testimonials in favour of his perform- ance he feels peculiarly obliged), and by many useful hints which have been communicated to him in letters from several of his literary friends ; to whom he can- not but acknowledge his obligations, and whose names would reflect honour upon his work, if he were per- mitted to mention them. He is in a particular man~ ner indebted to a Nobleman of distinguished worth and abilities, for condescending to point out several alttratious and emendations ; all of which were of so much importance, that his Lordship will find they have been universally attended to. The Author has taken care to incorporate into this Edition, all those improvements and discoveries that have been made since the first Edition was published, and that ap- peared to have any connection with the subjects on a 3 which XlV ADVERTISEMENT. which he has treated. Besides the numerous altera- tions which are to be met with in almost every Lesson, he has added three New Lessons, — one on Electricity, one on Fountains or Springs, and one on Plants and Vegetation. He humbly hopes that these corrections and additions will ensure to him a con* tinuation of that encouragement with which he ha* Heen already honoured by an indulgent Public. Cambridge, May 2<)th, 1799* Should any, who possess extensive philosophical knowledge, honour this work with a perusal, they will perceive that it is a juvenile production; being, indeed, written originally before the author was 20 years of age : but, as its success has shewn its fitness forjuveniTe minds, the Author should not think him- self justifiable in making any alterations in the plan ; but simply thinks himself bound to correct it as muck- as possible, and to supply omissions by notes of refer- ence, while the plan remains the same. The principal additions and changes in the fourth edition, were in the 15th, imti, (24th, 28(A, 29th, and SQth Lessons. Sevc,- ral minor corrections are made in thejlth edition. Ro} til Military Academy, Aug. 20tii, 1815. CONTENTS. Page INTRODUCTORY LESSON ••••• I View of the Heavens •«••• • %••• 5 On the Sun 9 Mercury • • ••• 15 Venus « 2O TheEarth .• - •> -•••• 2* Mars f 31 Jupiter . 34 Saturn ••- 38 Georgtum Sidus, or Herschel «.«• 41 TheMoon .-• 4S' Comets ••• « ••«• 51 Projection and' Gravity 55. Zclipses of the Sun and Moon 62: The Fixed Stars, with Reflections on the Immensity of the Universe G8 The Air and Atmosphere «•• , .... 77 Winds •• ••• 91 Sounds and Echoes ••*".*.• 98 Evaporation, Ruin, Hail, Snow, Mists, and Dew • • 108 Frostandlce 115- Electricity »«•• 122, Thunder and Lightning ••••• ••• •• 135 The Ignis Fatuus r 14* The Aurora Borealis 149 Light and Colours ••• 155- Tke Rainbow .» • • •_• •...„»• • • v •• • • • M • v.r • • • •_'• W* XVI CONTENTS. On Halos and Parhelia >•• 172 Fire 177 Water 190 Fountains or Springs 201 The Tide* 209 Days and Nights 214 The Seasons 218 Vegetables or Plants • • 226 Earthquakes 239 Volcanos 265 TheEje 278 Concoction • • • 286 The Circulation of the Blood 295 Concluding Lesson •••• 303 Appendix, containing Additional Remarks on Heat, Cold, aud Light 311 LESSON I. INTRODUCTION. Every object of Creation Can furnish hints to contemplation, GAY. you, my dear young friends, have no\v ar- rived at a period of life, in which the mental faculties are rapidly expanding and increasing in vigour, you will perceive an inquisitive curiosity, which has long remained dormant in your minds, hastily bursting forth : it will be of the utmost importance to your happiness, both present and future, that you be careful in directing this active principle into its proper course. Ever since you have been able to exercise the power of reasoning, you cannot but have observed, with wonder and admiration, the sun shining with astonishing splendour, dispensing light and heat around; — the moon, with majesty serene, gliding along the arched heavens, scattering her gentle rays, in the absence of the glittering luminary of day; — and the spacious canopy bespangled with iiumerous stars, like twinkling flames, adding to the beauty of the scene. You must have observed, B mih 2 INTRODUCTION. [Lesson r. with awful astonishment, the forked lightning in vivid motion glancing through the wide expanse; and have heard, with fear and anxiety, the tre- mendous thunder, shaking the firmest buildings with its pealing crash. When you reflect upon these and other appearances in nature, what im- pressions do you feel ? You who have considered these things attentively will ingeniously confess, that you are thereby led to conceive that there must be some First Cause which produced, governs, and regulates the whole. The most cursory obser- vation will have induced you to entertain a high opinion of the wisdom, power, and goodness of the ALMIGHTY DESIGNER ; but I can assure you, my young friends, that the more you reflect upon the universe, in the display of its wonders and beauties, and the better you are acquainted with it, so much the more will be increased your reverence and love of the Governor of all. Nature is but a name for an effect Whose cause is God. COWPER. Natural Philosophy is subservient to purposes of a high and noble kind, and is chiefly to be valued, as it lays a sure foundation for natural re- ligion and moral philosophy; by leading us, in a satisfactory manner, to the knowledge of the Au- thor and Governor of the universe. To study na- ture is to search into his workmanship : every new discovery opens to us a new part of his scheme. And while we still meet, in our inquiries, with hints of greater things yet undiscovered, the mind is Lesson I. INTRODUCTION. 3 is kept in a pleasing expectation of making a fur- ther progress ; acquiring, at the same time, higher conceptions of that great Being, whose works are so various, and hard to be comprehended. It is a melancholy consideration, that too many young persons, instead of being zealous of acquir- ing real and useful knowledge, suffer a kind of torpor to dwell upon their minds, and give way to such supineness as may, if they be not quickly roused from their lethargy, be attended with fatal consequences. If any such persons should peruse these Lessons, let me exhort them to shake off their carelessness, and endeavour to furnish their minds, ere it be too late, with a true knowledge of the works and wonders of the creation : let them be assured that such conduct will produce the hap- piest effects; for philosophical contemplations will form the safest bulwark against the insidious at- tacks of Atheists : because the principal intention, of such inquiries is, from a consideration of the effects produced, to correct our ideas with respect to the Great First Cause; or, as the poet has ex- pressed it, To look through Nature up to NATURE'S GOD. POPE, In these Lessons it shall therefore be my pro- vince to explain to you, in a concise and familiar manner, some of the wonders of the universe : I will first lead you to lake a survey of the heavenly bodies; and afterwards consider some of those objects and some of those appearances of na- B 2 ture, INTRODUCTION. [Lesson i. ture which relate to the earth we inhabit : thus shall we See through this vast extended theatre Of skill divine, what shining marks appear ! Creating power is all around exprest, The GOD discover'd, and his care confest : Nature's high birth her heav'nly beauties shew : By every feature we the parent know. Th' expanded spheres, amazing to the sight, Magnificent with stars, and globes of light; The glorious orbs which heav'n's bright host compose . Th' imprison'd sea, resistless ebbs and flows ; The fluctuating fields of liquid air, With all the curious meteors hov'ring there, And the wide regions of the land proclaim, The POW'R DIVINE that rais'd the mighty frame. BLACKMORE. LESSON LESSON II. VIEW OF THE HEAVENS. Heaven Is as the book of GOD before thee set Wherein to read his wond'rous works. MILTON. The heav'ns declare the glory of GOD. DAVID. AGREEABLY to my plan, I shall now endea- vour, in the first place, to describe to you the na- ture, size, and motion of the principal heavenly bodies; the beauty and variety of which have no doubt often filled you with astonishment: follow- ing the advice of Ovid, ' We, though from heaven remote, to heaven will move ' With strength of mind, and tread th' abyss above ; ' And penetrate with an interior light, ' Those upper depths which nature hid from sight. ' Pleas'd we will be to walk along the sphere * Of shining stars, and travel through the year." The science which teaches the knowledge of the celestial bodies, their magnitudes, motions, distances, periods, eclipses, order, &c. is called ASTRONOMY : the study of this has been pursued with avidity in all ages, and it is now arrived at a tolerable degree of accuracy. The hypotheses which have, been invented by astronomers, at different times and in different countries, are nu- ll 3 merous, VIEW OP THE HEAVENS. [LeSS07l II. nierous, and the greater part of them are too futile in their nature to d'eservea particular account : the only one which agrees with all the phenomena is that which was first invented by Pythagoras (who was born 577 years before Christ), and taught in Greece and Italy ; but this was soon buried in ob- livion, and was set aside from the time of Ptolemy, until it was restored about the year 1507» by Nicholas Copernicus. The discoveries of Kepler and Galileo tended greatly to prove its truth ; but it was much opposed, until at length the indefati- gable researches of Sir ISAAC NEWTON fixed it upon too firm a basis to be easily overthrown. It is now generally adopted by Astronomers, and is> with a few modifications, now called the Newtonian System ; an account of which I shall here proceed to lay before you. When we take a view of the heavenly bodies, our attention is first attracted by the sun and moon, which are distinctively named luminaries : the other beautiful spangles in the glorious canopy are called stars ; and of these a distinction is made into pla- nets or wandering stars, and fixed stars. The pla- nets, of which the earth we inhabit is one, move in regular and uninterrupted order aro'und the sun j some of these planets have attendants, usually called satellites, moving around them. Sometimes there are other stars seen, with blazing tails issu- ing from them : these pursue very eccentric irre- gular courses, and are called comets. The planets* them- * Correctly speaking, the Satellites are Planets, as well aa those round which they revolve: for planet is a Greek word, Lesson n.] VIEW OF THE HEAVENS. 7 themselves are frequently called primaries., and their satellites secondaries. Tfiere are two methods of discovering which are planets, and which are fixed stars : every fixed star twinkles, but a planet does not ; for the stars are to appearance only lu- cid poinis, and therefore any opaque particle float- ing in the air is sufficient to cause a momentary eclipse of them f; but ihe planets, though smaller, suffer very little apparent diminution. The pro- per criterion, however, is this : the planets are al- ways in motion from one part of the heavens to the other, whereas the other stars keep constantly the same relative distance. The names of the planets, beginning with that nearest the sun, are as follow : Mercury, Penus, the Earthy Mars, Jupiter, Saturn, and Georgium Sidus, or Herschel. These are all that are yet discovered, though there very probably may be signifying any thing that wanders. Agreeably to this accep- tation, the Sun itself is a Planet; as it, like the others, has a two-fold motion. And indeed, to complete the similarity, Dr. Herschel has (in a paper which will be presently more largely spoken of) asserted^ that his body is opaque, and that it is diversified with hills and valleys. t Although the above is the generally adopted method! of explaining the twinkling of the fixed stars, yet it is now thought to be inaccurate. Mr. Michell justly observes (in the " Philosophical Transactions,") that no object can hide & star from us, that is not large enough to exceed the apparent diameter of the star, by the diameter of the pupil of the eye> nay, it must be large enough to hide the star from both eyes at the same time. Perhaps the principal cause of this twinkling, is the unequal refraction of light, in consequence of inequalities and undulations in the atmosphere. » *• more : 8 VIEW OF THE HEAVENS. [LeSSOH II. more*: after describing to you the sun, I shall proceed to the rest in their order. * Since the commencement of the present century, four other Planets have been discovered. The first of these was discovered on the 1st of January, 1801, by M. Piazzi, of Palermo : its mean distance from the sun is not qtiite three times that of the earth (2.768): its revolution is performed in four years, seven months, and ten days; and its orbit is inclined to the ecliptic in an angle of about lOf degrees. This planet is much less in size than our moon : its discoverer has given it the name of Ceres, but most astronomers call it by the name of Piazzi. The second was discovered on the 20th of March 1802, by Dr. Olbers, of Bremen. Its distance from the sun, time of revolution, and magnitude, are nearly the same as Piazzi's planet; and the orbits of the two intersect each other; the latter being inclined to the ecliptic in an angle of about 34^ degrees. It is called by the names Pallas, and Olbers. The third was discovered on the 1st of September 1801, by M. Harding, of Lilienthal. Its mean distance from the sun is rather greater than that of the two former; and its size nearly equal to that of Ceres. Its inclination is 13 degrees. It appears like a star of the eighth magnitude. Harding has given to this planet the name of Juno. The- fourth was discovered by Dr. Olbers, early in 1807. It is nearer to Mars than either of the other newly discovered planets, its mean distance being rather more than 2| times that of the earth ; and the revolution through its orbit is performed in 1130 of our days. The inclination of that orbit to the ecliptic is 7 and l-7th degrees, being rather more than that of Mercury. The size of this planet is not known. Astronomers have given it the name of Vesta. LESSON LESSON III, ON THE SUN. Hail sacred source of inexhausted light ! Prodigious instance of creating might ! His distance man's imagination foils ; Numbers will scarce avail to-cotint the miles. His globous body how immensely great! How fierce his burnings ! how intense his heat! As swift as thought he darts liis radiance round. To distant worlds his system's utmost bound : Of all the planets the directing soul, That heightens and invigorates the whole. BROWN. wFTEN as you hfije beheld the mid-day sun shining in all his grandeur, disseminating his reful- gent beams around ; and often as you have felt the efficacy of his all -genial heat, you may never have entertained an idea of his vast size. When you are informed of the dimensions of this grand dispenser of light and heat, and when you coi)ne to be acquainted with some of the laws by which he is governed, you will consider it as one of the many irrefragable proofs, that the universe could not (as atheists assert) be jumbled together by chance ; but that the whole must have been formed by an all-wise, all-powerful, and adorable Creator ! The sun is a body very nearly in the form of that solid which is by mathematicians called. a B 5 sphere 10 • THE SUN. [Lesson in. sphere or globe, and the observations of astrono- mers have proved beyond a doubt, that its axis is nearly 883,210 miles, its circumference 2,774,692 miles, and its solidity in cubic miles 360,737,732, 256,5fi4,299 : viz. three hundred and sixty thou- sand seven hundred and thirty-seven billions, seven hundred and thirty-two thousand two hun- dred and fifty-six millions, five hundred and twen- ty-four thousand two hundred and ninety-nine » a number almost surpassing the powers of imagi- nation ! From a cursory observation you would perhaps be led to imagine that the sun moves round the earth once in twenty-four hours ; but this is not the case. The sun has two motions : the one is a peri- odical motion, in an elliptical or very nearly a cir- cular direction, round the common centre of all the planetary motions. As this common centre is found to be always exceedingly near the sun, and most commonly within it, I shall henceforward suppose this luminary to be the centre of the planetary system, for in such a supposition we shall not fall into any material error. The other mo- tion is a revolution upon its axis, which is com- pleted in about twenty-five days, as appears ob- viously by paying attention to the maculce and faculce, or spots upon his surface. The sun was supposed, by many of the ancients, to be the clearest image of his Maker, <( without *' spot, or wrinkle, or any such thing." To such a degree had this prejudice arisen, that when Gali- leo discovered several dark spots on the surface of the Lesson ill.] THE strir, 1 j the sun, and mentioned his discovery to another philosopher, he was told that the thing was utterly impossible, and that there must be some defect either in his glasses or his eyes : it was added also, as another proof of the assertor's candour and pe- netration, that as such a circumstance was not noticed by Aristotle, the pretended discovery could be nothing less than presumption or deception^ However, that there are spots on the sun, has since been indisputably confirmed, and is- now univer- sally admitted. Of these spots, the dark ones are ealled macula, to distinguish them from the others, which are of a brighter appearance than the rest of the sun's surface, and which have obtained the name offaculce. Concerning the nature of these spots, there have been various opinions entertained by different per- sons. Some have supposed maculae to be large portions of opaque matter moving up and down in the fiery fluid, of which the sun was thought to be composed or surrounded, revolving near its sur- face, and sometimes beyond it. Others have taken them for the smoke of volcanoes in the sun, or the scum floating upon a huge ocean of fluid matter, Faculae, on the contrary, have been called clouds of light, and luminous vapours j and, because ma- culae have been sometimes observed to change into- faculae, it has been conjectured, that the latter were the bright flames of volcanoes rapidly blazing out, after the dark smoky matter, which produced the maculae, became dissipated by combustion^ These are the opinions I hat have been commonly held 12 THE SUN. [Lesson in. held on the subject; but it does not appear to have been considered with much attention until very lately. The discoveries and observations of Dr. fierschel, have in a great measure supplied the de- fect, and afforded ample materials for forming a rational and plausible theory to explain and eluci- date the appearances we are now treating upon. This ingenious astronomer has assigned very forcible reasons for concluding, that the opinion commonly received, that the sun is a body of real fire, is futile and erroneous. He susposes, on the contrary, that it is an opaque body, surrounded by an atmosphere of a phosphoric nature, composed of various transparent and elastic fluids, by the decomposition of which, light is produced, and lu- cid appearances formed of different degrees and intensity. The doctor even goes so far as to assert, with much probability, that the suri is in reality an inhabitable world; but this assertion has no con- nection with our present inquiry, which we must confine, for the present, to maculae and faculae. Admitting, therefore, the precexling remarks, we will endeavour to deduce from them a satisfactory hypothesis to account for these appearances. The sun, it has been said, is an opaque body, surrounded by a lucid atmosphere : you will easily conceive, then, that maeulse are those parts of his surface which happen to be free from luminous decompo- sitions, or, in other words, which are but slightlyj if at all, covered by the shining matter, and are for that reason exposed to our view. In most cases the real body of the sun is supposed to be visible through Lesson in.] THE SUN. 13 through its transparent atmosphere, where the lu- cid substance is not very intense, or where it is removed by some temporary cause. As some of the spots appear below, and others above the sur- face of the shining fluid, it is reasonable to con- clude that the former are the lower parts of the sun's surface, and the latter his mountains, which project beyond the lucid part of his atmosphere. The former are found to vary in their situation, as they may be hidden or rendered visible by any cause which will accumulate or remove the shining matter : the latter are fixed, with respect to the sun's surface, and are those, by observations on which {lie sun's rotation upon his axis has been determined. From what has been here said, it is hoped you are tolerably well acquainted with the nature of maculae : we will now proceed to the consideration of faculae. Faculse, on this hypothesis, are those parts of the solar atmosphere which are brighter, and in general more elevated than the rest. These Dr. Herschel supposes to be " more copious mixtures " of such fluids as decompose each other;'* or they may be called, larger collections of the luminous fluids which form the solar atmosphere, according to the quantity, brightness, and depth of which, the faculce differ in magnitude and intensity. They are more frequently observed near ;he borders, than to- wards the middle of the sun's disc, because, as they are supposed to extend beyond the usual level of his atmosphere those which are near the middle of the disc become edgewise to our view, and are there- fore 14 THE SUN. [Lesson m. fore not so easily discernible as those which ap- proach nearer its circumference. If the hypothesis concerning the nature of the sun, which is recited in this lesson, be admitted, it will readily be acknowledged that that luminary differs but little in his nature from the planets j and perhaps we may be allowed to call the sun, in a popular way, the central planet, or the grand planet) to which all the others are intimately united, and from which, as from a copious fountain, flows all that is necessary to support, connect, and har- monize the various planets in the system : hence we may advert to the beautiful and instructive ob- servation of the poet, and say, The planets of each system represent Kind neighbours: mutual amity prevails; Sweet interchange of rays, received, retuHi'd : Enlight'ning and enlighten'd ! All at once Attracting and attracted ! Patriot like, None sins against the welfare of the whole: But their reciprocal, unselfish aid, Affords an emblem of millennial love. Nothing in nature, much less conscious being, Was e'er created solely for itself: Thus man his sov'reign duty learn* in this Material picture of be nucoltnce. Yousc, LESSON IV. ON MERCURY. First Mercury amidst full tides of light, Rolls next the Sun, through his small circle bright; All that dwell there must be refin'd and pure ; Bodies like ours, such ardour can't endure; Onr earth would blaze beneath so fierce a ray, And all its marble mountains waste away. BAKER. JlOWEVER ignorant we are of the nature of qualities, and how much soever their mode of ope- ration is concealed from us, if it be but admitted that they act in right lines, and that they are pro- pagated from a point, or body, as from a center, then it may be demonstrated in a strictly geome- trical manner, that their energy, or intensity, di- minishes in a duplicate proportion of the distance from that center. Thus, for instance, suppose a person whom I will call Thomas, stands at ten feet distance from a fire, and another, whom I will call James, stands twenty feet from the fire ; if they are similarly situated in all respects but that of distance, it may be demonstrated, that the fire will impart four times as much heat to Thomas as to James ; that is, Thomas's heat is to James's, as the square of James's distance from the fire is to the square of Thomas's distance from it. Considering the sun as the center from whence proceed those rays, or particles, which meeting with j6 MERCURY. [Lesson iv. with proper substances, produce light and heat at the planets, and calculating by the theorem above mentioned, it has been concluded, that if the earth were placed in the situation of Mercury, its medium of heat : would be sevca limes more intense than the greatest heat uf our torrid zone is in its present situation. And hence it has been asserted, that if the materials of which Mercury is com- posed were exactly of the same nature as those of the earth, they could not long remain without be- ing either melted into a fluid, and dissipated into vapour, or vitrified. Have we not then, in the formation o£ this planet, another proof of infinite wisdom ? For, if the world were formed by chance, or, as atheistical writers express it, by the fortui- tous concourse of atoms, whence comes it, that Mercury and the Earth should have the materials of which they are composed, so adjusted and ar- ranged as to make them so well adapted for their respective situations, as we have abundant reason to conclude they are? It will be necessary to premise, that, though the motions of the planets are tolerably uniform and regular, yet they are not exactly so :. nor are their orbits, or the tracks in which they describe their periodical motions, strictly circular, but rather elliptical j their bodies are not globes, but sphe- riods, being flatted at the ends of their axes, which are called poles, and more protuberant at their middle parts or equator? : their orbits are not all in the same plane, but are variously inclined to each other. However, as it is foreign from my design to Lesson iv.] MERCUHY. 17 to treat upon them in so particular a manner, I shall content myself with referring you to places where you may find abundant information in these respects. (See the books recommended towards the end of these Lessons.) Those planets which move in orbits within that of the earth, are called inferior, perhaps more properly Interior planets : those whose orbits en- close the earth's are called superior, or more pro- perly exterior planets. Mercury is the smallest of the inferior planets, and the nearest to the sun, about which he is car- ried with a very rapid motion. Hence it was that this planet was considered mythologically as the messenger of the gods : hev was repre- sented emblematically by the figure of a youth with wings at his head and feet, and his cadu- ceus entwined by winged serpents. The cha- racter $ in present use for this planet i» also de- rived from the mythological description. Though small, he has a bright appearance, with a light tinct of blue : he never departs 28° from the sun, and on that account is usually hid in the splen- dour of that luminary. The mean distance of Mercury from the sun, is to that of 'the earth from the sun, as 387 to 1000: hence his distance is about 37 millions of miles. The sun's diameter will appear at Mer- cury nearly three times as large as at the earth : and the sun's light and heat received there, is, as before observed, about seven times those at the earth. The 18 MERCURY. [Lesson iv. The diamtter of this planet is nearly one-third of the diameter of the eanh, or about 3000 miles. Hence the surface of Mercury is nearly 1-gth, and his magnitude or bulk l-27th of that of the earth. His period of revolution round the sun is 87 days, 23 hours, and l-4th : hence you may find that he moves in his orbit about the sun at the amazing rate of more than 95,OOO miles in an hour. His length of day, or time of rotation on his axis, inclination of axis to his orbit, &cc. are yet unknown. Mercury changes his phases in a manner simi- lar to the moon, according as he is differently stationed, with regard to the earth and sun : though we may observe that he never appears quite full, because his bright side is only turned directly to- wards us, when he is so near the sun as to be lost from our sight in his beams. These different phases of his make it obvious that he does not shine by any light of his own 5 for if he did, he would always appear round. As the orbit of this planet is between the earth's orbit and the sun, if it were in the same plane as the orbit of the earth, Mercury would fre- quently be seen to move across the face or diac of the sun. But as the planes of their orbits are not coincident, this appearance happens less com- monly ; it is denominated by astronomers, a transit of Mercury over the sun's disc, the planet then appearing like a black spot on the face of the sun. The last transit of Mercury happened in the year -Lesson iv.] .MKHOURY. 19 year 1802 : other transits will happen on the 12th of November in the present year 1815 ; Novem- ber 5th, 1822; May 5th, 1832; November 7th, 1835; May 8th, 1845; May 9th, 1S-18; No- vember 12th, 1861 ; November 5th, 1868 ; May 6th, 1878; November 8th, 1881; May 10th, 1891; and November 10th, 1894. These are all which wjfl occur hi the course of the present ceil', tury. LESSON LESSON V. ON VENUS. » Fair Venus next fulfils her larger round, With softer beams, and milder glory crown'd ; Friend to mankind, she glitters from afar, Now the bright evening, now the morning star. BAKER. VENUS, the second planet from the sun, is the next which comes under our consideration : the character by which she is denoted in astro- nomical performances is ? , which is the same as that which the chemists make use of to denote copper. The mean distance of this planet from the sun is about 69 millions of miles, and her magnitude is nearly the same as the earth's, her diameter be- ing something more than 7?900 miles. Astrono- mers have discovered mountains on her surface ; and some dark moveable spots, which have been observed on her disc, give us great reason to sup- pose she has an atmosphere. Her periodical course round the sun is completed in less than 225 days. The time of a complete rotation on her axis was by Bianchini assigned to be 24 days and 6 hours : but Cassi?ii, with a much stronger appearance of probability, says the rotation is performed in about 23 Lesson v.] VENUS. 2JL 23 hours ; and this assertion is supported by some late observations accurately made by Shroeter, from which he has determined the time of one ro- tation to be nearly 24 hours. Delamlre assigns it at 24 hours 5| minutes. Venus when viewed through a telescope, is rarely seen to shine with a full face ; but has phases changing in like manner with the moon : being now gibbous, now horned ; and her illumined part is constantly toward the sun. To the naked eye this planet is easily distinguishable, on ac- count ot her brightness and whiteness, which ex- ceeds that of any other planet ; nay, her lustre is so considerable, that when she is about 40 de- grees removed from the sun, it is hardly equalled by that of the moon, which is frequently a dull light when compared with the vigour and bright- ness of the beams of the planet. In this state she has been often mistaken for a comet, and is fre- quently seen in the day time when the sun shines : a phenomenon which is taken notice of by some of our philosophical poets. No stars besides their radiance can display In Phoebus' presence, the dread lord of day : Ev'n Cynthia's self, though regent of the night, Is quite obscur'd by his emergent light : But Venus only, as if more divine, With Phoebus dares in partnership to shine." This planet is a morning star, when she appears westward of the sun, for she then rises before himj at these times she is among poets called Phosphorus 22 VENUS. [Lesson v. Phosphorus or Lucifer; but when eastward of the sun, she shines in the evening after he sets, and then is called popularly the evening star ; but poets then give her the name Hesperus or Vesper. She retains each of these names in its turn about 290 days. Venus, as well as Mercury, is sometimes seen to transit the sun's disc, in form of a dark round spot. These transits of Venus happen but seldom. One was seen in England iir 1639 ; and two in the last century, viz. the one in 1761, and the other in 1/69: there will not happen another until December gth, 1874; and after that, only one more, namely, on December 7th, 1882, before the close of the present century. None of the wandering stars are more cele- brated and admired among the ancients, than the one we are now reflecting upon : they had a pro- digious veneration for her, making her their fa- vourite goddess, paying her adoration, and all that Deity could claim ; they even thought that her power supplied earth, air, and sea, and that clouds and tempests disappeared at her presence. But those who direct their contemplations into a proper channel will strip the planet of these ima- ginary honours, and place them where they are really due : we must consider her in all her va- ried and attendant beauties, as a part, a small part only, of the divine workmanship of HIM " who covers himself with light, as with a gar- *' nient, and has stretched out the heavens like a « curtain.'* By thus examining with attention the Lesson v.J VENUS, 23 the separate parts of his wonderful performances, we shall reflect with greater pleasure on the whole, and be induced to exclaim, These are thy glorious works, Parent of Good, Almighty ; thine this universal frame, Thus woaderous fair ! THYSELF how vvond'rous then ! MILTON. LESSON LESSON vi. ON THE EARTH. More distant still our earth comes rolling on, And forms a wider circle round the sun ; With her the moon, companion ever dear ! Her course attending through the shining year. BAKER. IN the earliest ages of the world the generality of mankind entertained very strange notions con- cerning the form and dimensions of the earth we inhabit : and even in the present enlightened age it is not unusual to meet with persons whose ideas in this respect are very far from the truth. Those who have not been in the habit of considering this subject in an astronomical point of view, look upon the earth as a very extensive plane, here and there interspersed with hills and vales ; they have also a confused notion of its being fixed firmly upon something ; but upon what, or in what man- ner, it is impossible for them to tell. But I would wish you, my young friends, to re- flect upon the subject in a more correct manner. To you 1 must therefore observe, that the earth is in form nearly globular, and partakes of two con- stant motions; the one about its axis, and the other through its orbit round the sun, like the other planets. To this perhaps some of you may ob- ject, Lessonvi.] THE EARTH. 23 ject, and you may advance several reasons for the objection, the principal of which will be like the following: — l.'It is repugnant to our senses, which represent the earth to be flat and immove- able ', and 2. It is contrary to the words of Scrip- ture. The first of these reasons may be obviated with ease, if the subject be considered with a proper attention. Thus, the roundness of the Earth is con- firmed by recollecting that it has been frequently circumnavigated : that it is round is also proved by considering that its shadow, as projected upon the Moon in a lunar eclipse, always appears nearly circular, which would not happen if the Earth were not nearly spherical j — but the most mani- fest proof is derived from the considerations di- rectly following. If we stand upon the sea shore and notice a ship sailing from us, we shall first lose sight of the hull or body of the vessel, then of the lower pajts of the masts and rigging, and as she goes farther off, the upper parts of the masts disappear : so again, when a ship comes towards port, the steeples and highest buildings are first seen by the sailors ; as the vessel comes nearer, they per- ceive the houses and lower buildings ; and pre- sently after the surface of the ground "appears. Thus it is obvious that the earth is nearly spheri- cal : and the diversifications of its surface with mountains and valleys have no sensible effect in destroying its sphericity; for the greatest hills, when compared with its magnitude, bear no greater proportion to the whole, than the little protu- c berances 3<> THE EAKTH. [LeSSOH VI. — - — i—f- — • . beranccs on the coat of an orange to the bulk thereof. The argument alleged against the earth's mo- tion, " that no such motion is evident to our semises,-" 03 too weak and frivolous to deserve a particular answer ; for it is well known that we meet with deceptions in the sense of vision, in a variety of instances where the objects viewed are quite familiar to us ; and when the fallacy is dis- covered, we have been surprised that we should be so easily deceived. As to the second reason before advanced, those who oppose the astronomical principles concern- ing the shape and motion of the Earth, because they think them contrary to Revelation, would do well to consider for what purpose the holy Scriptures were written. Were they written as a measure of faith, or as a rule to regulate our phi- losophical opinions ? Gassendus does not give a direct answer to the question ; but he has made some very pertinent observations on the subject, with which I shall here present you. " There are," says he, " two sacred volumes ; the one written, " called the Bible, — the other Nature, or the " World; GOD having manifested himself by two " lights, the one of revelation, and the other of "demonstration: accordingly the interpreters of *' the former are divines, of the latter mathemati- ** cians. As to matters of natural knowledge, *' the mathematicians are to be consulted, — and " as to objects of faith, the prophets j the for- «• aaer being no less interpreters, or apostles, from " God Lesson vu] THE EARTH. 27 " God to men than the latter. And as the ma- " thematician would be judged to wander out of " his province, if he should pretend to controvert, " or set aside any article of faith from principles " of geometry ; so it must be granted, the divines ft are no less out of their limits, when they ven- " lure to pronounce on a point of natural know- *' ledge, beyond the reach of any ftot versed in " geometry and optics, merely from holy Scrip- " ture, which does not pretend to teach any thing " of the matter." I shall now proceed to exhibit to you the Earth in an astronomical point of view; for I am con- vinced, that the more attentively you consider it in this light, the more willingly you will throw aside the common prejudices, and place the true result of philosophical reasoning in their stead. The earth, considered as an element, after the manner of Aristotle, is called Terra: but amongst astronomers it has obtained the name Tellus, and is denoted by the character ® ; it is the third pla- net from the Sun, its mean distance from him being 95 millions of miles; and its diameter is found to be 7970 miles*. It is nearly 365| days in completing a revolution through its orbit, is the length of our year : and a complete rof upon its axis is performed in the compass of a:na- * Strictly speaking, the Earth, and indeed all toe planets are spheroids formed by the rotation of ellipses of small ellrpticity upon their minor axes ; but their deviation from the spherical form is too minute to need any particular spe- cification in a populai work like this. "e 2 tural 28 THE EARTH. \LesSOH VI. tural day, or 24 hours. From mathematical prin- ciples it has been demonstrated that the length of the day is somewhat different at different parts of the year, but the difference is very inconsider- able ; one day when the Sun is in the equinoctial being shorter by 40 seconds than when he is in the tropics. There is also another motion of the Earth, which occasions the precession of the equi- noxes; but it is of too abstruse a nature to be explained to you in a satisfactory manner, until you have gained a better acquaintance with astro- nomy. Here let us pause, and contemplate with humi- lity, mingled with satisfaction, the abundant good- ness of HIM " who hangeth the earth upon if nothing," to us his creatures. He compels the huge mass of inert matter on which we dwell, to travel with wonderful regularity through the abyss of space ; and in its progress the various parts thereof are, by means of the diurnal rotation, made to feel the. effects of the invigorating foun- tain of light and heat. Were it not for this we should sensibly feel the want of the returning sea- Sons : no more should we see the valleys standing thick with com ; nor should we behold the beau- tiful verdure of the fertile meadow ; — no more would the trees spread forth their foliage, nor would the plants be ornamented with flowers. Or as it is expressed in the lang|tege of inspiration, — " No longer would the fig-tree blossom, nor " fruit be in the vine : the labour of the olive " would fail, and the fields could yield no meat : "the Lesson v*.] THE EARTH. " the flocks must be cut off from the fold, and " there would be no herd in the stalls/' Consider this, ye perverse mortals! who argue against conviction : consider, and tell us, if the above gloomy picture would not be realized, were the chance, which you so blindly extol, to preside over us. But thanks to the beneficence of the all- wise PROTECTOR of erring men, the evils which would be brought upon us under the dominion of chance, are averted : directed by an ALMIGHTY command, the earth is carried gradually along^ and its motions are regulated in such a manner as are most conducive to the general design : the varied seasons of the year and the vicissi- tudes of day and night follow each other in pleas- ing gradations : the whole move on with astonish- ing harmony; and through every part of their pro- gress, the omnipotent Conductor is administering to our wants, and bestowing upon us additional blessings. " Oh ! that men would praise the Lord " for his goodness, and for his wonderful works " to the children of men * 1" The * It has been customary, when speaking of the benefits we enjoy, to mention the convenient situation of the earth in the system, with respect to light and heat : and in particular, with regard to heat, it has been said that were we nearer the sun, the earth would be burnt ; and were it farther off, we should be frozen. This method of reasoning might be applied with propiiety, when it was thought that the sun was a globe of fire ; but as modern discoveries have led philosophers to dis- pute the truth of such an opinion, it was thought better to omit the argument here hinted at. However, I have in some parts of these Lessous spoken of the dcgreesof light and heat, C3 m THE EARTH. [Lesson VI. The Earth is attended with a satellite, which adds greatly to our comforts and greatly to our pleasures : I dare say you will wish to be ac- quainted with its nature and size, when I tell you that this satellite is no other than the Moon, which with a — - — pleasing light Shadowy sets off the face of things. MILTO.V. But as this heavenly body is of such importance as to deserve a separate description, I shall gratify your curiosity in a future Lesson. iu a manner conformable to the most generally received opi- nion : I have also, in those places where I have spoken of the heat produced by the action of the Sun's rays, generally called it the solar heat; as it would not be right to alter the mode of expression most commonly used, until the premises upon which such alteration is grounded, are entirely acceded to. LESSON LESSON VII. ON MARS, In larger circuit rolls the orb ot" Mars, Guiltless of stern debate, and wasteful wars, As some have erring taught: he journeys on, ImpelPd and nourish'd by the attractive sun ; Like us, his seasons and his day he owes To the vast bounty which from Phoebus flows . Bnowx. 1 HE next planet which falls under our consi- deration, is called by the same name as Mars, the heathen god of war ; and very probably, because he appears with a ruddy fiery countenance : among astronomers he is characterised by this mark », that all the various appearances which we behold flow from a few very general and subordi- nate causes, which more immediately depend upon the ascendant power of the INK SUPREME CAUSE, the Author and Governor of the Universe ! whose existence and influence are manifested by every the most obvious effect ; and of whose power, wis- dom, and goodness we acquire higher and more enlarged conceptions in proportion as we obtain a more complete knowledge of his works. The laws of nature being discovered, as above- mentioned, by analysis, particular phenomena are explained synthetically, by shewing their con- formity to these laws. Thus, to shewthat the Moon is retained in its orbit by the force of gravity, is to shew the agreement between that force and the force by which a stone, or any heavy body, lends lo the centre of the earth : that the Moon is con- tinually bent from the tangent of its orbit, in the same manner as a body near the surface of the •earth is turned from its rectilinear motion into a curve : that both these motions are directed to the same GRAVITY, WEIGHT, &C. $9 same point, and agree in quantity : that, if the Moon were to approach to ihe surface of the E th, the force, by which it is retained in its or- bit, would make it descend « ,waids .he centre of the Earth, through ihe same space which a heavy body, falling by its gravity, would descend through in the same time : and that if a stone or a bullet could be carried to the distance of the Moon, and there projected with a sufficient velocity, it would revolve round the Earth like a Moon, for the same reason by which it is bent into a curve, when pro- jected near the surface of the earth. By pursuing these methods Sir Isaac Newton demonstrated the universal gravitation of matter ; and it is now pretty generally allowed that the same principle of gravity, by which we see all bodies tend towards the centre of the Earth, is a general law of na- ture, extended to all distances, and to every body in the universe. Thus it is agreed, that the pri- mary and secondary planets in our system, as also the Sun, are mutually attracted by each other. But since all attractions are mutual, it will follow, that if one or more bodies revolve about another, which is also attracted by them, that other body will not be at rest ; but together with them will revolve round the common centre of gravity of the whole system. Hence, then, and from the proportions of the quantities of matter of the Sun and the planets, it is found that the common centre of gravity of • {he solar system is never far removed from the body of the Sun, and is generally within its surface. Round this point the Sun itself is continually, moved 6o GRAVITY, WEIGHT, &c. [Lesson xin. moved in various directions, approaching or re- ceding according to the different positions of the planets. Since, then, all bodies, terrestrial and celestial, on which experiments or observations can be made, arc found to gravitate towards each other, what has been before said of the universal extension of Gravity will be the more willingly acceded to j I hope, therefore, I may now quit this part of the subject, without giving any additional arguments in support of the opinion. Before I conclude this Lesson, I cannot avoid adding a few words to explain the difference be- tween Gravity, freight, and Heaviness ; which appear to me the more necessary, because I am aware that the notions commonly entertained are not very correct. In order to form an exact idea of the weight of a body, it must be recollected, that Gravity im- presses, or has a tendency to impress, on every particle of bodies, in an instant, a certain velocity, with which they would fall, if they were not sup- ported ; and that, abstracting the influence of the air, this velocity would be the same for each of the particles of bodies, whatever be their substance. This being observed, we must understand by the weight of a body, the effort necessary to prevent it from falling ; and, it is evident, that in order to this, it is necessary to destroy the velocity which gravity has impressed on every particle. This ef- fort must, therefore, be equal to the sum of the velo- cities of all the particles. Hence it may be naturally con- Lesson XIII.] GRAVITY, WEIGHT, Sec. 6l concluded that bodies the most compact, and which consequently contain a greater number of particles in the same bulk, will weigh more than others; be- cause the weight being the sum of the velocities impressed on all the particles, that sum must be so much the greater, as there are more material par- ticles contained in the mass of the body. From what is here said, I would observe with M. de Condorcet, that we may see " the necessity " of carefully distinguishing between the effect of " Gravity, and that of Weight : the former is the t( power of transmitting, or a tendency to trans- " tnit, into every particle of matter a certain velo- nd degree of that quality which we cannot as- certain but by comparison. We say absolutely, and in an undetermined sense, that a thing is heavy ; but relatively, and in a determined man- ner, that it is of such a weight ; for example, of two, three, or four pounds. A thousand circum- stances prove the heaviness of the air, for instance; but the mercury in the barometer determines its exact weight* LESSON LESSON XIV. ON ECLIPSES OF THE SUN AND MOON. Give me the ways of wandering stars to know, The depths of heav'n above and earth below ; Teach me the various labours of the Moon, And whence proceed th' eclipses of the Sun. VIRG. GEORG. ir. 1 DOUBT not but that several of you, my young friends, will heartily join in Virgil's petition above cited : and though you, perhaps, may never have either leisure or opportunity enough to acquire a very great astronomical knowledge; yet I can as- sure you it is no difficult mailer to attain such an acquaintance with the science, as to understand the reason of Eclipses of the Sun and Moon. You will observe, then, that an Eclipse of the Jfloon is a privation of the light of tht Moon, oc- casioned by an interposition of the body of the Earth (as she revolves in her orbit) directly be- tween the Sun and Moon j by which mean, the Sun's rays are so intercepted that they cannot illuminate the Moon : then - — The silver Moon is all o'er blood, A settling crimson stains her beauteous face. LEE. It is at the lime of full Moon that lunar eclipses happen 5 Lesson xiv.] ECLIPSES. 63 happen ; because it is only then that the Earth is between the Sun and Moon : neither do they hap- pen every full Moon (as they would do if the orbits of the Earth and Moon were coincident) because of the obliquity of the Moon's path with respect to the Earth's ; but only in such full Moons as happen at the intersections of those two paths, called the Moon's nodes; or at least on those full Moons which happen but a little distance from the nodes. The chief circumstances in lunar eclipses, as they are given by Dr. Hutlon in his Mathemati- cal and Philosophical Dictionary, are as follow: — 1. All lunar eclipses are universal, or visible in all parts of the earth which have the Moon above the horizon ; and are every where of the same magnitude, with the Fame beginning and end. — 2. In all lunar eclipses, the eastern side is what first immerges and emerges again; i.e. the left side of the Moon as we look toward her from the north ; for the proper motion of the Moon being swifter than that of the Earth's shadow, the Moon approaches it from the west, overtakes it and passes through it with the Moon's east side fore- most, leaving the shadow behind, or to the west- ward.— 3, Total eclipses, and those of i he-longest duration, happen in the very nodes of the eclip- tic ; because the section of the Earth's shadow^ then falling on the Moon, is considerably larger than her disc. There may, however, be total eclipses within a small distance of the nodes ; but their duration is the less as they are farther from 64 ECLIPSE*. [Lesson xiv. from them ; till they become only partial ones, and at last not at all. — 4. The Moon, even in the middle of an eclipse, has usually a faint appear- ance of light, resembling tarnished copper; which Gassendus, Ricciolus, and Kepler, attribute to the light of the Sun, refracted by the Earth's atmos- phere, and so transmitted thither. — Lastly, she grows sensibly paler and dimmer before entering into the real shadow; owing to a penumbra which surrounds that shadow to some distance. In addition to these circumstances, some astro- nomers observe, and it is here added, that no eclipse of the Moon can last above 5| hours, from' the Moon's first touching the Earth's penumbra, to its last leaving it : but an eclipse of the Moon, by the Earth's shadow, perhaps never lasts above 3| hours; nor when total, above If hours. An Eclipse oj the Sun is an occultation or hiding of the Sun's body from our sight, occasion- ed by an interposition of the Moon between the Earth and Sun. .• — Shorn of his beams, the Sun In dim eclipse disastrous twilight sheds, MILTON. It is by several considered and called an Eclipse of the Earth, since the light of the Sun is hid from the Earth by the Moon, whose shadow involves a part of the Earth. The manner of a solar eclipse may be conceived by imagining a small part near the vertex of the Moon's conical shadow, travel- ling over a part of the earth's surface, and making a com- Lesson xiv.] ECLIPSES. 63 a complete eclipse to all the inhabitants residing within that track; but no where else ; for in the large space around, within the limits of the fainter shade called the penumbra, the eclipse will only be partial. It will not be difficult to understand that solar eclipses can only happen about the time of New Moon, when the Moon is in conjunction with the Sun, In the nodes, when the Moon has no visible latitude, the eclipses are total : out cf the nodes, but near them, the eclipses are partial : the limits are about 17 degrees on each side the nodes:— but much also depends upon the Moon's latitude, for it must in these cases be always less than the apparent semi- diameters of the Sun and Moon added together. Some circumstances of solar eclipses, as de- scribed by the very ingenious author before-men- tioned in this Lesson, are, 1. That none of them are universal ; that is, none of them are seen throughout the whole hemisphere which the Sim is then above : the Moon's disc being much too little, and much too near the Earth, to hide the Sun from the whole disc of the Earth. Commonly the Moon's dark shadow covers only a spot on the Earth's surface, about 180 miles broad, when the Sun's distance is greatest, and the Moon's least. But her partial shadow or penumbra, may thea cover a circular space of 4900 mites in diameter, within which the Sun is more or less eclipsed as the places are nearer to or farther from the centre of the penumbra. In this case the axis of the shade passe 06 ECLIPSES. [Lesson xiv. passes through the centre of the Earth, or the New Moon happens exactly in the node, and then it is evident that the section of the shadow is circular j but in every other case the conical shadow is cut obliquely by the surface of the Earth, and the sec- tion will be an oval, and very nearly a true ellipsis. —2. Nor does the eclipse appear the same in all parts of the Earth, where it is seen ; but when in one place it is total, in another it is only partial. Farther, when the Moon appears much less than the Sun, as is chiefly the case when she is in Apoge, and he in Perige *; the vertex of the lunar shadow is then too short to reach the Earth, and though she be in a central conjunction with the Sun, is yet not large enough to cover his whole disc, but lets his ring appear as a lucid ring or bracelet, and so causes an annular eclipse. — 3. A solar eclipse does not happen at the same time in all places where it is seen j but appears more early to the western parts, and later to the eastern j as the motion of the Moon, and consequently of her shadow, is from west to east. — 4. In most solar eclipses the Moon's disc is covered with a faint light, which is attributed to the reflection of the light from the illuminated part of the Earth.— Lastly, in total eclipses of the Sun, the Moon's limb is seen surrounded by a pale circle of light j which some astronomers consider as an indication of an atmosphere of the Sun, because it has been * Apoge is that place in which the Sun or a planet primary or secondary, is at its greatest distance from the Karlh : Perige. is when either of these is at Us neatest possible distance from us. observed f.esson xiv.] ECLIPSES. 67 observed to move equally with the Sun, and not with the Moon. In addition to these circumstances we may observe, that though a solar eclipse may last from beginning to end (at one place on the earth) more than two hours ; yet the duration of total dark- ness can never, in the greatest eclipse he more than four minutes, and very commonly not more than two. We may also observe, with regard to eclipses of both luminaries, that in general, as many eclipses happen of the Sun as of the Moon : but in any particular place there are more eclipses of the Moon than of the Sun. Again, that though in lunar eclipses the eastern side is first eclipsed, and the eclipse ends on the western sidej yet in solar eclipses, the western side is first eclipsed, and ends on the eastern. As to the number of eclipses both solar and lunar, it may be observed that there cannot in any year be less than two, nor more than seven : the most usual number is four, and it is very sel- dom that there are more than six. The satellites of some of the superior planets frequently undergo eclipses and occultations j Hut as these are unobservable by the naked eye, it would not agree with my design to say more about them. Some of the fixed stars, Aldeba- ran for instance, is frequently hidden behind the Moon ; Jupiter also experiences occultations of this kind: but of these the bare mention may- suffice. LESSON LESSON XV. ON THE FIXED STARS, WITH REFLECTIONS ON THE IMMENSITY OF THE V*lllr£KSE. ——Who turns bis eye on Nature's midnight face Rut must inquire — " What hand behind tin1. s cc-nv, •' What arm Almighty, put these wheeling globes " In motion, and wound up the vjxst machine ? " Who rounded in his palm those spacious orb.1! ? " Who bowl'd them flaming through the dark profound, "And set the bosom of old night on lire?" Nature's Controulcr, Author, Guide, mid End ! YOUNG. V\HEN you, my young friends, consider the unwieldy size of those celestial bodies on which we have already descanted, and reflect upon the asto- nishing rapidity of some of their motions j surely you must entertain very high ideas of the GREAT POWER which first launched them in the illimi- table void, and causes their motions to continue through the flux of so many thousand years ; none having yet mistaken their way, or wandered from their destined paths :— on the contrary, their ro- tations still proceed in such exquisite regularity and harmony as is best adapted to the perfection of the whole. What awful power and adorable goodness is here displayed ! But our reflections on tke Lesson xv.] FIXED STARS, Sec. 69 the heavens must be carried infinitely farther than we have yet extended them. The gems in the brilliant canopy which remain to be contemplated, are the fixed stars; which are chiefly distinguishable, as was suggested in the Second Lesson, from their never changing their relative situation with regard to each other. The heavens are divided into three regions, called the Northern and Southern Hemispheres, and the Zodiac. The Fixed Stars were classed by the ancients under the outlines of certain figures of birds, beasts, fishes, and other animals j and these were called Constellations. The number of which is, in the Northern Hemisphere, 36 j in the Southern, 32; and in theZodiac,12. Stars not com- prehended in any of these ancient constellations, are called Unformed Stars; and others, of a cloudy appearance, are called Nebula:. Of this number are the Magellanic clouds near the south pole, which resemble two whitish spots in the heavens, and are well known to sailors *. The • The Plate which is »;iven as a Frontispiece, is a projec- tion of the northern and southern CELESTIAL HEMISPHERES on the plans of the llqxator. The centre of the first projec- tion is the North Pole of the Equator, aroand which are de- scribed two circles ; the smaller is the Arctic circle, the larger, the Tropic of Cancer: a little above the centre of the first pro- jection is the North Poll of the Ecliptic, where all the Circles of latitude drawn through every tenth degree of each Sign of the Zodiac, meet and intersect each other. The centre of the second projection is the South Pole of the Equator; the first of the two circles, which are described about it, is the An- tarctic circle, the other is the Tropic of Capricorn : a little below the 70 FIXED STARS, &c. [Lesson XV. The last star in the tail of Ursa Minor, or the Less Bear, is called the Polar Star, and serves for a guide to mariners ; because, on account of its nearness to the north pole, its apparent situa- tion, with regard to the Earth, varies but very little throughout the period of the Earth's annual revolution. Two of the stars in the constellation of Ursa Major) or the Greater Bear, are called the centre of the second projection is the South pole of the Ecliptic, where all the Circles of Latitude meet and intersect, as in the Southern Hemisphere. From the Poles of the Ecliptic as centres, the Circles of Longitude are drawn at every tenth degree: that circle which is described at 90* from each pole of the Ecliptic, is the Ecliptic itself ; of this, half appears in the one projection, and half in the other; it interests the Equator in the fiist points of Arits(«¥») and Libra (•£:). The diameter of each projection which crosses it from top to bottom, is called the Solstitial Colure, because it passes through the solstitial points, Cancer (25) and Capricorn (Vf} '• the diameter that crosses each projection from right to left denotes the Equinoctial Colure, so called be- cause it passes through the equinoctial points. Ariet and Libra. These four points of the Ecliptic which are crossed by the Colures are called Cardinal Points; and when the Sun enters one or other of these points, one of the four Seasons of the year commenc( s. The Stars are given in this plate as they appear on the sur- face of the Celestial Globe, with this difference, that the figures of the Constellations are omitted, as they would only tend to create confusion when the Hemispheres arc projected on so small a scale. The Stars of different magnitudes are so distinguished, that with little difficulty they may be reckoned in many instances : Thus, in Ursa Minor, or the Less Hear, it is easy to reckon two stars of the second, one of the third, three of the fourth, one of the fifth, and three of the sixth magnitude. Again, in Cunicula, or the Little Dog, you may discover ten stars, whereof one, called Procyon, is of the first magnitude. the Lesson xv.J FIXED STARS, 8cc. 71 the Pointers, because they always point very nearly to the polar star. Those of the fixed stars which are nearest to us seem largest, and are therefore said to be of the first magnitude ; those of the second magnitude, being at a greater distance, seem lessj and thus they proceed by regular gradations unto the sixth magnitude, which includes all the rest of the fixed stars that are visible without a telescope. With regard to their number, a common observer might be led to suppose that even to the unas- sisted eye they are innumerable : but this arises from their being observed in a confused manner : for it may be proved, that when they are divided into proper classes, and reckoned up, those in the visible hemisphere,seen without a telescope, amount not to many more than a thousand. Since the introduction of telescopes into astro- nomical observations, the number of fixed stars has been very justly considered as immense ; for, to the greater perfection our glasses are carried,, the more stars we discover. The astonishingly immense distance of the fixed stars from one ano- ther, and from the earth we inhabit, is one of the most proper considerations for elevating our ideas of the works of GOD. Astronomers have com- puted from indubitable principles, that the distance of Sirius or the Dog Star (which is the nearest fixed star) from us, is considerably more than two mil- lions of millions of miles ! A distance almost in- conceivable ! A cannon-ball flying from thence at FIXED STARS. [Lesson xv. at the rate of 400 miles in an hour, would not reach us in 570,000 years. The stars being at such great distances from the* sun, cannot possibly receive from him so strong a light as they shine with: hence, on mature re* flection, it will appear that they shine with their own native lustre, in like manner with the sun ; and since each star is confined to a particular por- tion of space, we must reasonably conclude that each fixed star is in reality a sun *. It is not at ail probable that the ALMIGHTY, whose actions all evince infinite wisdom j and who does nothing in vain, should create so many glo- rious suns for no other purpose than to add to our pleasure, and give us an additional glimmering of light. Those who are so fond of arrogating Divine favours to themselves have but a mean opi- nion of Infinite Wisdom : since, by a considerably • " That stars arc suns will scarcely admit of a doubt. Their immense distance would perfectly exclude them from our view, if the light they sent us were not of the solar kind. Besides the analogy may be traced much farther. The sun turns on its axis ; so does the star Algol ; so do the stars called $ Lyra-, S Cephet, ij Antinoi, -e Ccti, and many more; most probably all. From what other catise can we so probably account for their periodical changes ? Again, our fun has spots on its surface ; so has the star Algol: and- so have the stars already named; and probably every star iu the heavens. On our sun those spots are changeable ; so they are on the star o Ceti ; as evidently appears from the irregularity of its changeable lustre, which is often broken in upon by acciden- tal changes, while the general period continues unaltered. The same little deviations have been observed in other pe- riodical stars, and ought to be ascribed to the same cause." HERSCHEL. less XV.] FIXRD, STAHS, &C. f3 less degree of creating power, our earth would have received much more light from only one ad^ ditional moon. And canst then think, poor worm, these orbs of ligkt, In size immense, in number infinite, Were made for thee alone, to twinkle in thy sight? Presumptuous mortal! can thy nerves descry, How far from thee they roll, from thee how high? With all thy boasted knowledge canst thon see Their various beauty, order, harmony? If not— then sure they were not made for thee. BASER Instead, then, of one sun and one world only in the universe, as the unscientific suppose, our contemplations induce us to acknowledge that there must be an inconceivable number of suns and of systems of planets revolving round them, dispersed through the infinitely wide expanse of boundless space; insomuch that were our sun, with all the planets about it, annihilated, they would be no more missed by an eye that could take in the whole creation, than a drop of water from the wide ocean- M Our single system is asuougfct in estimate " When balaoc'd with the heatr*ns : greater the specfc M Which on the sun-beam dances, when compar'd " With Taurus, or the Alps, or Caucasus ; 14 Or on the blade the dew-drop to the »ea." These reBections tend to excite a deep con- sciousness of our own inferiority. Who can help exclaiming with David after a similar contempla- JK t 74 FIXBD STARS, &c. [Lesson xv. tion-— " Lord, what is man, lhat thou art mindful "of him?" As there is a. general analogy running through and connecting every part of the creation, into one grand whole : and as there is undoubtedly an absolute similarity between the earth we inhabit and the other planets in our system ; can it be un- reasonable to suppose that they and the planets of ether systems have plants, and trees, herbs, fruits, &c. &c. as we have? Or is it repugnant to na- ture to imagine that they are inhabited by animals and rational creatures ? Among numberless argu- ments which might be adduced, a very good one to shew the great probability of the planets being inhabited, is derived from the following conside- ration. . There is no part of matter that we are ac- quainted with, which lies waste and useless : seas, lakrs,and rivers,teem with living creatures; moun- tains and vallies; trees and herbs; grasses and the animals which feed upon them; nay, even the blood and:humours of the animals themselves, all have their respective inhabitants. Surely, then, t-he most numerous and large bodies in the uni- verse, are furnished with beings adapted to their several situations. What an august conception does this give of the works of the CREATOR ! Almost more than the human imagination is able to con- ceive. Millions of --suns at immense distances from each other; attended by tens of millions of worlds moving round them, all in rapid motion, yet re- gular and calm: and these, we may safely infer, are Letion xv.] FIXED STARS, fcc. are inhabited -by millions of millions of rational creatures formed for endless felicity; - Hail ! Source of being ! universal Son! Of' heaven and earth ! essential Presence hail ! To THEE I bend the knee, to THEE my thoughts Continual climb, who with a master-hand Hast the great whole into perfection touch'd! THOMSON, When an innumerable multitude of bodies of enormous bulk, are all set in motion, and keep travelling through their extensive orbits with such beauteous regularity and order, by means of the attraction of the suns to which they respectively belong; without having their motions either de- stroyed or directed into other courses ; how can we express our conceptions of the greatness, wis- dom, and goodness of HIM who made and go- verns the whole ? " By the word of the LOHD were the heavens " made, and ail the host of them by the Ireatk " of his mouth." (DavidJ What an amazing in- stance of Omnipotence ! How inconceivably great do these his marvellous works evince him to be : then Since the great Sovereign sends ten thousand worlds, To tell us he resides above them all, In glory's unapproachable recess : YOUH&. how can we forbear venting our adoration in hymns of praise ? — Previous to my closing this Lesson I shall therefore insert a hymn indited by E £ inspiration, 7* FIXED STARS, See. [Lesson XT. inspiration, and translated into our language by no less a Christian and poet than Mr. Addison. HYMN. PSALM XIX. THE spacious firmament on high, With all the blue ctlit rial sky, And spangled heavens, a shining frame, Their great Original proclaim. Th' unwearied sun from day to day Does his Creator's power display, And publishes to every land The work of an Almighty hand. Soon as the evening shades prevail, The moon takes up the wondrous tale, And nightly, to the listening earth, Repeats the story of her birth ; While all the stars that round her bum, And all th* planets, in their turn, Confirm the tidings as they roll, And spread the truth from pole to pole. What though in solemn silence all Move round the dark terrestrial ball ? What though nor real voice, nor sound, Amid their radiant orbs are found ? In reason's ear they all rejoice, And utter forth a glorious voice; For ever singing, as they shine, The HAND that made vs is divine! END OF THE ASTRONOMICAL PART. U36 ON LESSON XVI. ON THE ATMOSPHERE. Diffusing gently its enlivening pow'r, The genial Air we all around us feel Cheering — though unexplor'd by human sight. we have now finished our survey of the hea- venly bodies, our inquiries may naturally descend to the Earth we inhabit : and here the first thing which attracts our attention is, that thin, transpa- rent, and fluid body, called Air, which surrounds this terraqueous globe, and covers it to a consider- able height. Or, if we include in our definition the whole of the fluid mass, consisting of air, electric matter, aqueous and other vapours, which surrounds the Earth, and partakes of all its motions; we then make use of the word Atmosphere, as a term comprising the whole. Beside the different kinds of air, it is manifest that the whole mass of the atmosphere contains a considerable quantity of water, together with an heterogeneous collec- tion of particles exhaled from all solid or fluid bodies on the surface of the Earth. These, how- ever, are transformed into a fluid mass called Atmospheric Air, which is that transparent, colour- less fluid which every where invests this elobe, possessing permanent elasticity and gravity. It is composed of four gases, but principally of 78 parts of nitrogen and 22 of oxygen gas in bulk ; and in- E 3 weigh U 78 , ATMOSPHERE, [LesSWl XVI. ':. I" —— '• - '.. I I ' P I weight of about 74 nitrogen, and 26 oxygen ; and is soluble in about 30 times its bulk of water : 10O cubic inches weigh 3 1 grains. On the surface of the earth it is compressed by the weight of the superincumbent atmosphere: its density, therefore, diminishes according to its height above the earth. It is dilatable by heat : at 60° of temperature, its bulk is increased about its l-82d part. The con- st^ituent principles of atmospheric air are rendered evident by the following experiment: quicksilver being enclosed in a proper vessel of atmospheric air, on heat being applied the air will be diminish- ed, and the quicksilver will lose its splendour, and gradually change to a reddish powder ; acquiring, at the same time, an augmentation of weight. When neither the air nor the quicksilver suffers any farther change, the separation of the princi- ples has taken place : the one, the gas remaining in the receivers, is now unfit for supporting flame,, or maintaining respiration, and is nitrogen gas : the other is absorbed by the quicksilver, while re- ducing to the state of an oxide, and may be ex- tricated from it on the application of heat ; when the powder, to which the quicksilver is reduced, will be restored to its metallic state> but will have lost the weight it had gained during its oxidation } this deficiency being exactly equal to the weight of the evolved gas, which is oxygen gas. These separated gases, thus differing in their properties from each other, and, from atmospheric air being again mix,ed, form atmospheric air of the or^i- nary degree of purity. The- Lesson xvi.] ATMOSPHERE. 79 The following is Mr. Dalton's table of the weights of the different gases constituting the at- mosphere : — Incites of Mercury • Azotic 6as 23.36 Oxygenous Gas •• ' 6.18 Aqueous Vapour • -14 Carbonic Acid Gas «•• .02 30.00 Table of the proportional weights of the dif- ferent gases in a given volume of atmospheric air, taken at the surface of the earth :— • Azotic Gas • Oxygenous Gas • • • • Aqueous Vapour • • Carbonic Acid Gas 100.00 The uses of the Atmosphere are so many and great, that it is absolutely necessary, not only to the comfort and convenience of mankind, but even to the existence of all animal and vegetable life. Ex.- periments which have been frequently made with an instrument called an air pump, place it beyond doubt that without the air or atmosphere, no. animal could exist, or even be produced : with- out its aid all vegetation would cease, neither would there be any great degree of either inflam- mation or combustion. Sound could not be pro- duced without it, nor would there be either rains or dews to moisten the ground : in short, all our S 4 reflections *O ATMOSPHERE. [LeSWH XVf. reflections on the atmosphere will tend more clearly to convince us that we continually stand in need of the superintendance of our allwisc CREATOR. Besides other innumerable conveniences which we receive from the atmosphere, one great advan- tage is, that while the Sun shines, it makes the face of the heavens appear lucid and bright: but, on> the contrary, if there were no atmosphere surrounding the Earth, only that part of the sky would appear light in which the Sun was placed: if a person should turn his back to the Sun, he •would directly perceive it as dark as night, and the least stars would be seen to shine, as in th« clearest night. For in that case there would be no substance to reflect the rays of the sun to our eyes ; and of course, those which did not fall upon the Earth would be thrown out into infinite space, and would never be reflected back to us. But since there is an atmosphere covering the Earth, which is strongly illuminated by the Sun, it, by its power of reflection, turns the light towards us, and makes the whole heavens to shine with such splendour as to render the light of the stars invisi- ble in ttie day-time. * By means of the atmosphere it happens, thai though after the Sun has set, we receive no direct Kcrht from the Sun, yet we enjoy its reflected and refracted light for some time; so that the dark- ness of the night docs not come on suddenly (as it would otherwise do) but by degrees. For, after the Earth "by revolving on its axis has withdrawn us Lesson xvj.] TWILIGHT. 8T, us from seeing the Sun ; the atmosphere (whose reflecting part reaches to the height of about sixty miles) will still be illuminated by that luminary : so that for a while the whole heaven will have some of his light imparted to it. But as the Earth pursues its revolution, the Sun retires farther below the horrzon ; and so much the less is the atmosphere illustrated by him : until trie Sun is about eighteen degrees below the horizon^ w O when he no longer enlightens our atmosphere, and then all that part thereof which is over us be- comes dark. Likewise in the morning, as soon as the Sun comes within eighteen degrees of the horizon, he begins again to enlighten the atmosphere, and to diffuse his light over the sky : so tbat its bright- ness does still increase, till the Sun rises and makes - full day. This kind of illumination between day and night, which is observed' in the morning be- fore the Sun's rising, and 'in the evening after his settihg, is called Crespusculum or Twilight. It is - longest in England, from May 24th to July 23d; during which period there is " no real night;" and shortest on March 2d and October 1 2th, when its duration at London is about 1 hour 55 minutes. The terrestrial atmosphere also refracts those rays which fall upon it from the Sun and Stars, and changes their directions, by propagating the light in other lines, and thus making the apparent places of the celestial bodies different from their true places. This refraction causes the Sun to be yisible before he has risen above the horizon., and i E 5. io ATMOSPHERE. [Lesson xvt. to protract his stay with us after he is set in the evening. This is an admirable contrivance to shorten the long and dismal nights in the frigid zones, and thus to add to the comfort of the in- habitants of those forlorn regions. Varenius re- lates in his geography, that " to those Hollanders " who wintered in Nova Zemlla, the Sun was " visible, in a clear sky, sixteen days before it ac- (t tually rose above the horizon, being yet four de- ** grees below it." And Hook, speaking of the same circumstance, says, — " The night in that *' place shortened no less than a whole month j ^•which must needs be a very great comfort, to *' all such people as live very far towards the «* North and South poles, where length of night, t( and want of seeing the Sun, cannot but be very for bulk, the higher it rises : and therefore must also decrease in density; and the law of diminu- tion is such, that when the heights increase in arithmetical progression, the densities decrease in geometrical progression. 4. It is of an elastic or springy nature : and the law it observes in this respect is, that the force of the spring is equal to its weight, or the density is alway§ proportional to the force by which it is compressed. We may also observe that heat increases and cold diminishes the elasticity of the air : or heat expands and cold condenses it. The weight or pressure of the atmosphere upon any base at the surface of the earth, is equal to the weight of a column of quicksilver of the sarn« base, and its height between twenty-eight and thirty-one inches: Lesson X.VL] PRESSURE OF AIR. 85 inches : or equal to the weight of a column of water of the same base and height, betw.een thirty- two and thirty-five feet. The first part of this is proved by observations on the Barometer, an in- strument which measures the pressure of the air: tor the limit of barometrical variation is between twenty-eight and thirty-one inches. And the latter part is proved by the sucking pump, which will never raise water higher than thirty. five feet, and sometimes not higher than thirty-two. This va- riation in the weight of the atmosphere depends in great measure on the different degrees of heat in the air near the surface of the earth ; but, perhaps it depends in a much greater degree, on the commotions and changes in the atmosphere from wind, vapours, and other causes. From the foregoing account of the weight of the atmosphere, it will not be difficult to infer, that, at a medium, there is a pressure equal to nearly fifteen pounds avoirdupois upon every square inch : this entirely, arises from its weight and fluidity. By the combination of these two qualities, which bind down all bodies on the earth with such great force, many wonderful effects are produced: it is this which prevents the arterial vessels of animals and plants from being too much distended, by the impetus of the circulating juices, or by the. elastic foice of the air so copiously abounding in them :. it is this also which hinders the fluids from transpir- at. ing in. too great a degree through the pores of their containing vessels, which would otherwise destroy the 66 ATMOSPHERE. [Lesson xvi. the animal by a debility gradually brought on : to this are also owing many natural phenomena by far too numerous to be mentioned in this place. Another property of air, and which indeed is its chief criterion, is its elasticity or springiness ; it is by virtue of this quality that it dilates itself, after the removal of any pressure ; or contracts itself into a less space when it has to sustain a greater pressure. A familiar instance of this qua- lity you may often have observed ; namely, by 'having a fresh bladder filled with air ; for when squeezed in the hand the air makes a sensible resistance, but when the hand is taken away, the parts which were compressed, directly restore themselves to their former state. I have before observed that th« air presses on a square inch with the weight of J5lbs. on a me- dium. Now if we suppose the surface of a full- sized human body to be ten square feet, which is not too much, we shall find, (as it is the nature of the air to press equally in all directions,) that a mart who probably supposes he bears no weight, sustains a pressure of no less than -21,601) Ibs. When we consider that the greater part of us are surrounded with such an astonishing pressure, and that this pressure may in the course of a very few hours be either increased or diminished by more than a thousand pounds weight ; are we never led to reflect upon that POWER who keeps us from utler destruction! Let the Atheist consider what* he Lesson xvi.] PRESSURE OF AIR. 87' he has to expect, for his blasphemous denial of so wise and mighty a Being. Another remarkable property of air, which ought to fill our hearts with thankfulness to the adorable CREATOR, is its transparency : let us recollect in what a dreary and disconsolate situation we should be if the air were visible. What would then be the use of that noble instrument the eye? Or how should we discern those diversified and variegated prospects of distant towns, green woods, flowery meado.ws, fields of corn, 8cc. which now so often give us pleasure ? Alas ! how dismal and gloomy would be the reverse ! Surely our hearts must overflow with gratitude to the DIVINE AUTHOR of our existence, for such unbounded goodness to us his creatures. Before we terminate this Lesson, we cannot for- bear recurring to the use of the air in respiration ; but shall point out one or two striking instances which it furnishes of exquisite contrivance for the most beneficent purposes. ' Animal heat is preserved enfirely by the in- spiration of atmospheric air ! The lungs, which imbibe the oxygen gas from the air, impart it to the blood ; and the blood, in its circulation, gives out the caloric to every part of the body. No- thing can afford a more striking proof of creative wisdom, than this provision for the preservation of an equable animal temperature. By the de- composition of atmospheric air, caloric is evolved, and this caloric is taken up by the arterial blood, without its temperature being at all raised by the addition, ATMOSPHERE. [Lesson xvi. addition. When it passes to the veins, its capacity for caloric is diminished, as much as it had been before increased in the longs: the caloric, there- fore, which had been absorbed, is again given out fc and this slow and constant evolution of caloric in the extreme vessels over the whole body, is the source of that uniform temperature which we have so much occasion to admire. Dr. Crawford asr certained, that whenever an animal is placed in a medium, the temperature of which is considerably high, the usual change of arterial into venous blood does not go on j consequently, no evolution of caloric will take place, and the animal heat will not rise much above the natural standard. How pleasing it is to contemplate the arrange- ments which the Deity has made for the preservat- ion and felichy of his creatures, and to observe .that he has provided for every possible exigency ! Lavoisier has shewn, that in respiration there is a constant combination of the oxygen of the at- mbsphere with the hydrogen and carbon of the blood. Thus Itfe discordant elements arrests, Rejects the noxious and tire pure digests ; Combines with heat the fluctuating mass, And gives a while solidity to gas, DARTHH.. A postulatutn has been assumed by some atheists, that the organs of the body have been formed by •what they call appetency, i. e. endeavours per- petuated, and imperceptibly working its effects through a long series of generations : hut I. would ask-, PRESStfRE OF AIK. ask any one, whether he would venture to assert that he believes this to be the way in which the lungs acquired the faculty of decomposing atmos- pheric air; and that he believes that this hypothesis is sufficient to account for the composition of this air, which so exactly suits the operation of these lungs, and which contains that exact portion of caloric which the animal ceconomy requires ! It is worthy of remark, that cold-blooded animals, which are not furnished with this breathing ap- paratus, are so constituted that their temperature changes with every change of the temperature of the surrounding medium. Frogs have been abso- lutely frozen so as to chip like ice, and then when carefully and gradually thawed, have been com- pletely re-animated. Lastly, it may be remarked, that the interval which there is between every inspiration seems to have been designed to allow time for the nitrogen gas which is throwirout of the lungs to mount in the air above the head, in order that a fresh por- tion of air might be taken in, and that the same air might not be repeatedly breathed. During that remarkable interval that always occurs in breathing, there is sufficient time al- lowed for the noxious fluids to separate; the first to ascend, while the other preponderates, leaving a. space for a fresh current of uncontaminated atmospheric air. Thus every thing is prepared by Divine Goodness, without any care or forethought ,of purs, for a new inspiration. " The go ATMOSPHERE. [Lesson XVT. The air inhaled is not the gas That from a thousand lungs reek back to thine, Sated with exhalations rank and fell, Which, drunk, would poison the balsamic blood, And rouse the heart to ev'ry fever's rape- But air that trembling floats from hill to hill, From vale to mountain, with inccstai.t change Of purest element. LESSON LESSON XVII, ON WINDS. Trade-winds, observing well their stated course,' To human good employ their powerful force : The loaded ships across the ocean fann'd By steady galen, spread commerce through the land. These you observe— but have you no desire The hidden Spring of such effects t'inqnire? Or, when contending winds around you blow, Do you ne'er wish the cause of them to know ? XlITHERTO our reflections have carried us no farther than to consider the air in a motionless state ; but as this fluid mass is frequently in motion, and that too sometimes in a violent degree, it would be almost unpardonable to pass by such an obvious effect without paying some attention to it, Air in a current-like motion is known by the nam« of wind. Though the winds in a temperate zone of the earth are very inconstant and change- able, yet this is not the case in every part of the terrestrial globe j for in the torrid zone and some other parts, the winds are generally very uniform and constant in their directions, as will appear from the following facts relative to them : — 1. Over the Atlantic and Pacific oceans, parli- ' ~ cularly between thirty degrees of North and thirty degrees of South latitude, the Trade-winds, as they are 0$ WINDS. [Lesson xvir. are called, blow uniformly from east to west, all the year round, with a small variation in the different seasons. — 2. When the sun is on the equator, the Trade-winds in sailing northward, veer more and more from the east towards the north; so that about their limit they become nearly north-east: and vice versa in sailing southward, they become at last nearly south-east. — 3. When the sun is near the Tropic of Cancer, the Trade-winds north of the equator, become more nearly east than at other times, and those south of the equator more nearly south ; and vice versa, when the sun is near the Tropic of Capricorn.— 4. The Trade- winds are not due east upon the equator, but about four de- grees to the north of it. To account for these facts relative to the winds is a most curious and important, though mysterious inquiry ; having employed the pens of several very eminent philosophers : but amongst all the expla- nations I have seen, there is none in my opinion more agreeable to nature than one given by Mr. John Dallon, of Manchester, in his " Meteoro- logical Observations and Essays." The method of reasoning applied to the subject in that work, I shall here adopt. The inequality of heat in the different climates and places, and the earth's rotation on its axis, appear to be the principal causes of all winds, re- gular and irregular. It may be observed, that whenever the heat is greatest, there the air will ascend, and a supply of colder air will be received from Lessen xvn.] WINDS. 93 from the neighbouring parts : it will be willingly allowed that the heat is at all times greatest in the torrid zone, and decreases gradually in proceeding; northward or southward ; also that the poles may at all times be considered as the centres of cold. Hence it manifestly results, that, abstracting from accidental circumstances, there will be a constant ascent of air over the torrid zone, which air will afterwards fall northward and southward, whilst the colder air below is determined by a continual impulse towards the equator. When the effects of the earth's rotation are takea into consideration, our reasoning must be as fol- lows :-— The air over any part of the earth's surface, when apparently at rest or calm, will have the same rotatory Telocity as that part ; but if a quan- tity of air in the northern hemisphere receive an impulse in the direction of the meridian, either northward or southward, its rotatory velocity will be greater in the former case, and less in the latter, than that of the air into which it moves ; con- sequently, if it move northward, it will have a greater velocity eastward than the air, or surface of the earth over which it moves, and will there- fore become a south-west wind, or a wind be- tween the south and west.' And vice versa, if it move southward, it becomes a north-east wind. From similar considerations it will appear, that in the southward hemisphere the winds will be north- west and south-east respectively. The Trade-winds may therefore be explained thns : The two general masses of air proceeding from Q4 TRA»E-wiNCi»__ [Lesson XVII. from both hemispheres towards the equator, as they advance, are constantly deflected more and more towards the east, by reason of the earth's rotation j that from the southern hemisphere originally a south wind, is made to veer more and more towards the east : in like manner, that from the northern hemisphere is made to change its direction from the north towards the east. These two masses meeting near the equator, their velocities south and north destroy each other, and they proceed afterwards with their common velocity from east to west round the torrid zone, excepting the irregularities produced by the continents. The equator is not in reality the place of concourse, but the northern, parallel of four degrees : because the centre of heat is thereabouts, the sun being no longer on the north side of the equator than on the south side. More- over, when the sun is near one of the tropics, the centre of heat upon the earth's surface is then nearer that tropic than usual, and therefore the winds about the tropic are more nearly east at that time, and those about the other tropic more nearly north and south. If all the terrestrial globe were covered with water, or, if the variations of the earth's surface in heat were regular and constant, so that the heat was the same in every part of the same parallel of latitude, the winds would then be very nearly re- gular also. But this is not the case : for we find the irregularities of heat, arising from the interspersion of land and sea, are such, that though all the1 parts of the atmosphere in some measure conspire to produce Lesson XVH.j TRADE-WIrfDS. 95 produce regular winds about the torrid zone, yet very striking irregularities are often found to take place. A remarkable instance we have in Mon- soon$t which are winds that in the Indian ocean, &c. blow for six months together one way, and the next six months the contrary way : these with sea and land breezes do not seem easily accounted for on any other principle than that of rarefaction. Perhaps some persons may be led to suppose that the winds in the northern temperate zone should be between the north and east towards the poles, and between the south and west nearer the equator, almost as regular as the Trade-winds: but when the changes of seasons, the different capacities of land and water for heat, the interference and op- position of the two general currents are considered, it might be concluded almost next to impossible that the winds in the temperate zone should exhibit any thing like regularity. However, notwithstand- ing this, observations sufficiently evince, that the winds therein are, for the most part, in the direc- tion of one of the general currents : namely, some- where between the south and west, or almost as commonly between the north and east j and that winds in other directions happen only as acci- dental varieties, chiefly in unsettled weather. We may have frequently taken notice, that several winds, particularly stormy ones, are at- tended with a cloudy sky. To this it may be added, that we have more winds than usually occur in rather less latitudes, where the atmosphere is gene- rally more serene: these considered make it exceed- ingly WINDS, ingly probable, that the aqueous vapours which are sustained by the air, from whence come clouds and rains may be one great cause of irregular winds. It has been determined, from very accurate experiments, that one inch of water when evapo- rated, will fill more than 2000 inches of space : from hence it appears that the water which falls in drops of rain, &c. possessed more than 2000 times the space when it floated in the atmosphere in vapours j the condensation thereof must therefore occasion vacuities of such a nature as will cause winds of different kind and degrees, according to the deficiency which is to be supplied. The oeconomy of winds, an illustration of which has been here attempted, is admirably adapted to the various purposes of nature, and to the general intercourse of mankind : — if the earth had been fixed, and the sun had revolved about it, the air over the torrid zone, and particularly about the. equator would have been almost always stagnant : and in the other zones the winds would have had little variation either in direction or strength; in this case navigation would have been greatly impeded, and a communication between the two hemispheres by sea rendered impracticable. Oil the present system of things, however, the irregu- larity of winds is of the happiest consequence, by being subservient to navigation : and a general circulation of air constantly takes place between the eastern and western hemispheres, as well as between the polar and equatorial regions ; by reason of which, that diffusion and intermixture of Lesson xvn.] WINDS. 97 of the different aerial fluids, so necessary for the life, health, and prosperity of the animal and vege- table kingdoms, is accomplished : — such is the transcendant wisdom and providential care of the beneficent FATHER OF ALL ! LESSON LESSON XVIII. ON SOUNDS AND ECHOES. • - • Sweet music breathe, Above, about, or underneath, Sent by some spirit to mortals good. MILTON. ANOTHER peculiar motion of the air remains yet to be considered, which is, that by means of which sounds are rendered audible or sensible to us, under all their different affections and circum- stances. Of the philosophy of sounds, Music is un- doubtedly the essential and most refined part ; and we find that persons in general are exceedingly fond of musical sounds, being thereby affected with the most agreeable and ravishing sensations. It is my province in this place to give no more of the science of Music than what relates to the production of musical sounds, and indeed of sounds in general, to which I shall now proceed*. Experiments * Though it be somewhat foreign to the subject immedi- ately under discussion, yet I cannot pass by an opportunity of suggesting an obvious improvement in the practice of Mu- sic ; the use of which has been frequently urged, though it be not yet generally acceded to. This improvement is no other than the substitution of proper characters to denote the dif- ferent kinds and velocities of musical time, instead of those vague, Lesson xvm.J SOUND. 99 Experiments on the air-pump prove to us, that without the assistance of air, sounds cannot be produced : they also evince, that the nature of sounds depends entirely upon a certain motion of the aerial particles. This motion is a pulsive or vibratory one, carrying these particles forward and backward through the very same space : and it results from, or depends upon, the spring or elasticity of the air. It is by means of this power that, when any one particle is by any cause urged forward, it must necessarily propel the particle next before it : this second particle, in the same vague, indefinite ones, which are now in use. What is the in- formation we can obtain from casting our eyes upon the cha- racters f > T> T> ¥, &c. ? Why truly, no more than can be learn- ed from reckoning up the Crotchets, Minims, Quavers, &c. in the first complete bar in the tune. The characters for the several rates of common time ; and the terms Adagio, Largo, Allegro, Presto, &c. &c. are also of very little avail in ascer- taining with precision the point the musician wishes to dis- cover. Every composer of musical airs, &c. would be of real iervice to the practitioner, if he would point out the absolute rate at which his music is to be performed : this would be no difficult task ; as he would only have to mention the length of a pendulum which would make one complete vibration in the time that part of a bar called a beat was performing. Thus, for instance, suppose I set a tune in triple time, and wish to have each bar performed in a second and a half, the cha- racter I must make use of is iV for from this it might be con- cluded that there were three beats in a bar, and each of these beats must be performed in the time a pendulum 10 inches long made one vibration. To explain this method clearly, much more room is requisite; but the present would not be a proper place for it : however, Jthosc who understand what improvement i: intended, from this short account, will, I hope, excuse me for exhorting them to use their best endeavours to make it general. F 2 manner, 100 SOUND. [Lesson •XVIIT. manner, moves a third, and so on, successively: and by these means the motion is propagated in the several particles, through a certain space in a direction forward : but, on the other hand, when the force which was first impre>t upon the elastic particles of air ceases to act, those particles return again, by the action of the air's elasticity, through the same space. It is evident, that if the producing force be continued on these elastic par- ticles, there must necessarily be produced in them a mutual vibratory motion of each particle, so long as the repercussive force continues to act : and this motion of the aerial particles being continued until it reaches the ear, the different parts, nerves, &c. belonging to and contiguous to the organ of hearing, being exquisitely adapted to the purpose, convey the sensation to the Irain, and so produce the idea or perception of sound. The waves in water, and the pulses in aif which produce sound, though brought about by two dif- ferent causes, gravity and elasticity, are yet some- what similar : if a stone be dropped into the water, it will cause waves to be propagated in a circular direction upon the water's surface all round the point where the stone was thrown in ; in like manner, the motion of a sounding body is propa- gated around it in regular gradations : but the aqueous waves differ from the aerial pulses in this, that the former are circular, being generated on a plane surface ; but the latter are of a spherical form, because they are produced in the lody of an elastic fluid. The Lesson xvin.] SOUND. 101 The kind of motion which produces sound must be understood to be that which is brought about by means of the elastic particles of which sonorous bodies consist; for without such an elastic dispo- sition of parts they could not by any means be ren- dered sonorous, or capabje of emitting sounds ; be- cause the stroke being made externally, affects the particles of such a body but with one single act: the particles of the body could therefore, in such a case, be moved only through a certain small space, and would there be made to stop by the resistance of, the parts beyond : thus without an elastic force, the particles would remain at rest, after the percu- tient body was removed ; and therefore, from a single stroke the parts of unelastic bodies could emit but a kind of blunt, short sound : in such, cases, it is common to say we hear the stroke, as when we strike with a hammer on a piece of lead. But when we consider the stroke impressed on bodies whose parts are in any considerable degree elastic, they not only yield to the stroke and go forward through a small space, but, after the strik- ing body is removed, those elastic parts, by their renilent force, return again with a velocity equal to that by which they were displaced ; and thus a vibratory motion being produced, will continue a perceptible time, and produce successive impulses on the contiguous air; hence, the air being thus agitated by the elastic particles of the body, trans- mits its impulses successively to ^he ear, and there produces a sensation of sound of some duration. Thus amongst sonorous bodies, we notice a wire F 3 when 102 SOUND. [Lesson xvur. when stretched and properly struck : also a bell and a glass, which are some of the fittest instru- ments for musical modulations. Much more might be said on the causes of sound in general j but for a general notion, what has been already mention- ed may suffice. To determine the nature and effect of different bodies in conducting sound, Mr. George Sounder s made a variety of experiments : some of his con- clusions and remarks are as follow : — Earth may be supposed to have a two-fold pro- perty with respect to sound. Being very porous, it absorbs sound, which is counteracted by its property of conducting it, and occasions it to pass on a plane, in an equal proportion to its progress in air, unencumbered by any body. If a sound be sufficiently intense to impress the earth in its tremulous quality, it will be carried to a con- siderable distance, as when the earth is struck with any thing hard, as by horses' feet, or the motion of a carriage. Plaister is proportionally better than loose earth for conducting sound, as it is more compact. Clothes of every kind, but particularly wool- len ones, are very prejudicial to sound ; their absorption of sound, may be compared to their absorption of water, which they greedily imbibe. A number of people seated before others (as in the gallery of a chapel or theatre) considerably pre- vent the voice reaching those behind ; and hencs it is that we hear so much better in the front of the galleries, Lesson xvin.] SOUND. 103 galleries, than behind others. Our seats, rising so little above each other, occasion this defect j which would be remedied, could we have the seats to rise their whole height above each other, as iu the ancient theatres. Water has been little noticed with respect to its conducting of sound ; but it has been lately- found to conduct sound more than any other body whatever. A conversation delivered- in no very loud tone, has been distinctly heard, on water, at the distance of a mile ; and a whisper has been heard at the distance of more than two hundred yards. Stone is sonorous, but gives a harsh disa- greeable tone, unfavourable to music. Brick, in respect to sound, has nearly the same properties as stone. Wood is sonorous, conductive, and vibrative. Of all materials, it produces a tone the most agreeable and melodious; and it is, therefore, the fittest for musical instruments, and for lining rooms and theatres. Paint has been generally thought unfavourable to sound, from its being so to musical instruments, whose effects it entirely destroys. Musical instru- ments mostly depend on the vibrative or tremulous property of the material, which a body of colour hardened in oil must very much alter : but we should distinguish that this regards information of sound, which may not altogether be the case in the progress of it. A remarkable circumstance in the nature of F 4 sounds, 104 SOUND. f Lesson xvm. souuds, which well deserves the attention of my young readers, is, that every substance whatever, whose parts are so connected as to be capable of an uniform vibration, may have that vibration pro- duced in it by the sounding of a certain musical note or tone, with which it is in unison. Thus Kircher speaks of a large stone that would tremble at the sound of one particular organ-pipe. Mr. Eoyle states the fact of seats trembling at the sound of organs ; he tells us also, that he has felt his hat to shake under his hand at certain notes, both of organs and other instruments ; and he was told by an experienced builder, that any well- built vault will answer some determinate note. JEven liquids, when so suspended as to be capable of vibration (for example, water in a glass), are observed, not only to vibrate when a particular note is struck or sounded, but actually sound themselves in concord. That water suspended in a glass becomes in reality a sonorous body, is proved by the mode of tuning a set of musical glasses, which become the graver in tone, the more water is poured into them ; for, were it only the empty part of the glass that sounded, the sound would become more acute, as more water is pour- ed in ; but, as the contrary is the fact, it is thence evident that the water and glass together form one compound sonorous substance, of which the greater the quantity or volume, the deeper is its musical tone. From what has been already stated, it will ap- pear manifest; that when the producing cause of any Lesson xvnf.] SOUND. 103 any sound is at a distance, there must be an inter, val of time elapse before the sound itself can arrive tt the ear j and, indeed, this may often have been manifested to us by our own observations. Thus, for instance, when a gun has been fired at a dis- tance, we may have taken notice, that after we have seen the flash, sometime has elapsed previous to our hearing the report : or again, when a wood- man, remote from us, has been felling trees, we may have observed that an interval of time passes away after we have seen the action performed before we hear the stroke. The experiments which have been made to determine the velocity of sound, have neither been so numerous nor so accurate as could be wished ; and on this account it is, that opinions differ concerning the nature of its pro- gressive motion. Because the intensity of sound diminishes as the distance increases, some persons suppose that the velocity does also : they therefore imagine that the velocity is inversely as the dis- tance, and consequently the time will be directly as the distance : but an opinion which meets with more advocates, and may now bt regarded as con- firmed, is, that sound moves uniformly in common, atmospheric air, at the rate of 1 142 feet in one se- cond of lime, or about an English mile in 4f se- conds ; and this rate of motion being allowed, it will not be any way difficult to determine the time for the passage of sound, the distance being given, and vice versa, in a variety of cases. A curious phaenomenon with regard to sounds, is an echoy which is caused by the vibrating air r 5 being 106 ECHO. [Lesson XVHI being interrupted in its passage. For as the air tmdulates forward like a wave, it often meets with various objects, and by striking against them is reflected back to us, and causes new vibrations, xvhich, if the object lie in a proper situation, return to us and repeat the same sound, tone, or word, as was first given : and this, it sometimes happens, not only once but several times. From this short account of the nature of echoes, it will not be difficult to conceive that they also may be applied to the measuring of inaccessible distances : thus, Dr. Derham, standing upon the bank of the Thames opposite to Woolwich, ob- served that the echo of a single sound was reflected back from the houses on the opposite bank in 3 seconds ; consequently the sum of the direct and reflex rays must have been 1142 multiplied into 3, or 3126 feet, and the half of it, viz. 17 13 feet, the breadth of the river in that place. But to treat upon the nature of sounds in such a manner as the importance of the subject demands ' would fill a volume : I must therefore now desist. From what little has been here mentioned, the •contemplative young reader will with pleasure draw this inference : that even in the nature and production of sounds the goodness of the CRE- ATOR to his creatures is conspicuously shewn: for, if bodies had no degree of elasticity, or if the air were not so fluid as to be easily put in motion, there would be an end of all the melody and har- mony which now so much delight us. What praise does that benevolent BEING require from us, Lesson xvin.] ECHO. 107 us, who not only administers to us what is neces- sary for our welfare, but has contrived all around us in so admirable a manner as to be subservient to our pleasures ! " On the1 contrary, had God wished our misery, or even had he been indifferent to our happiness, he might have formed our senses to be so many pains and sores to us, as they now are instruments of gratification and enjoyment : or have placed us amidst objects so ill surted to our perceptions as to have continually offended us, instead of mi- nistering to our refreshment and delight. He might have made, for example, every thing we tasted, bitter ; every thing we saw, loathsome ; every thing we touched, a sting ; every smell, a stench j and every sound, a discord." LESSON LESSON XIX. ON ErAPORATION, RATN, HAIL, SNOW, MISTS, AND DEW. • Th' effusive south Warms the wide air, and o'er the void of heav'A Breathes the big clouds with vernal show'rs distent, At first a dusky wreath they seem to rise, Scarce staining aether; but by swift degrees, In heaps on heaps, the doubling vapour sails Along the clouded sky. THOMSON. t\ OUR next business is to reflect upon the means by which the most usual meteors, as Rain, Hail, Snow, and the all-enlivening Dew, are produced : and in order to this, the first thing we are to con- sider is the process of Evaporation. To have a precise idea of evaporation, some persons distin- guish it from exha ation, and say that the former is the act of dissipating the humidity of a body in fumes or vapour ; while the latter, they say, is' properly a dispersion of dry particles issuing from a body. Others say there is no need of any such distinction, exhalation (properly signifying a Ireathing forth) being applicable to all bodies "capable of being respired, whether moist or dry. The term commonly used by chemists for the wising of the minute panicles of bodies in a dry form* Lesson xix.] EVAPORATION, &c. 109 form, is sublimation. Evaporation is by them ge- nerally applied to bodies in a state of humidity; and precipitation is the falling down ot any body> dry or humid, which has been held in solution ia any other body. There are, indeed, few subjects of philosophi- cal investigation that have occasioned a greater variety of opinions than the theory of Evapo- ration : as such a diversity of opinions yet exist, it is almost next to impossible to advance one, but what may be contradicted, and, in some respect, refuted : however, be this as it will, among the various theories I shall make use of the following. Dr. Hamilton, late Professor of Philosophy in the University of Dublin, supposes that Evaporation is nothing more than a gradual solution of water in air produced and promoted by attraction, heat, and motion, just as other solutions are effected. To account for the ascent of aqueous vapours into the atmosphere, this ingenious author ob- serves, that the lowest part of the air being pressed by the weight of the upper against the surface of the water, and continually nibbing upon it by its motion, attracts and dissolves those particles which it is in contact with, and separates them from the rest of the water. And since the cause of solution in this case is the stronger attrac- tion of the particles of water towards the air, than towards each other, those that are already dissolved and taken up, will be still farther raised bv the at- traction of the dry air that lice over them, and thus will 110 EVAPORATION, 8cc. [Lesson xix. will diffuse themselves, rising gradually higher and higher, and so leave the lowest air not so much satu- rated but that it will still be able to dissolve and take up fresh particles of water; which process is greatly promoted by the motion of the wind. When the vapours are thus raised and carried by the winds into the higher and colder regions of the atmosphere, some of them will coalesce into small particles, which slightly attracting each other, and being intermixed with air, will form clouds; and these clouds will float at different heights (varying from less than half a mile to somewhat more than two miles) according to the quantity of vapour borne up, and the degree of heat in the upper part of the atmosphere: and thus, clouds are generally higher in summer than in winter. When the clouds are much increased by a con- tinual addition of vapours, and their particles are driven close together, by winds, cold, and other causes, then will they run into drops heavy enough to fall down in Rain : —The clouds consign their treasures to the fields, And, softly shaking on the dimpled pool Prelusive drops, let all the moisture flow In large effusion o'er the fresLen'd world. THOMSON. In the winter, when the air is disposed for freez- ing, it is not unlikely that the atoms of vapour which are near the earth are congealed, whereby they become more opaque, and form those ob- scure fogs which constitute a hoar frost. At this time Lesson xix.] SNOW, HAIL, 8cc. 1 1 1 time the clouds are probably frozen before their particles are gathered into drops : small pieces of them being condensed and made heavier by the cold, fall down in Snow :— Then from aerial treasures downward pours Sheets of unsullied snow in lucid showers ; Flake after flake, through air, thick wav'ring flie», Till one vast shining waste all natnre lies. Then the proud hills a virgin whiteness shed A dazzling brightness glitters from the mead ; The hoary trees reflect a silver show, And groves beneath the lovely burden bow. BROOME, On a close examination, Snow is found to be composed of icy darts or stars united to each other, as crystals of water commonly are, whether they compose ice, snow, or hoar frost, at angles of 60 or 120 degrees. Its whiteness is owing to the small particles, into which it is divided, re- fracting and reflecting, instead of transmitting, all the rays of light that fall upon it. Ice, when pounded, becomes equally white. If drops of rain in their falling pass through a region of cold air, they become congealed in their passage, and fall in Hailstones: but Signior Beccana supposes that Hail is formed in the higher regions of the air, where ihe cold is intense, and where the electric matter is very copious. In the months of October and November, Fogs or Mist 9 are more frequent and thicker than at any other period of the year. If we consider the cause of llf EVAPORATION, Sec. [Lesson xix. of Fogs, the reason of this will appear evident. There is, besides the evaporation from the seas, lakes, and rivers, a constant and very large exha- lation from the surface of the earth, at all seasons, of water in the form of vapour ; and the warmer the ground the greater will be the evaporation. When the air is waum-r, or even but a little colder than the earth, the ascent of vapour is not per- ceptible to the eye : but when the temperature of the air is considerably lower, the vapour as soon as it rises is deprived of part of its heat, the watery particles are brought more into union, and they become visible in the form of steam. It is also essential to the formation of Fog, that there should be little or no wind stirring, in order that the rising exhalations may have full opportunity to condense. The heat of the middle of the days in autumn is stiil sufficient to warm the earth and cause a large ascent of vapour, which .the chill- ing frosty nights, which are also generally very calm, condense into Fogs. When vapour is condensed into small drops upon the surface of bodies on the ground, it is called Dew ; the most apparent difference between Dew and Rain is, that the condensation of vapour, in the one case, is made at or near the surface of the body receiving it, and in the other the drops fall a considerable space before thev reach the earth : the cause is the same in both cases, namely, cold operating upon vapoury air. At first view, 4t will appear improbable that a condensation of vapour should take place in the air resting upon the earth's surface, Lesson xrx.] FOGS, DEWS, &c. H3f surface, which is generally supposed to be warmer than that above; but it is an incontestible fact, that after sun-set, and during the night, in serene weather, the air is coldest at the earth's surface, and grows warmer the higher we ascend, till a certain moderate height, commonly between 2O and 100 yards : accordingly we find, that Dews and Hoar Frost are more copious in valleys than in elevated situations. When we recollect that winds in great measure prevent the accumulation of Dew, it can scarcely be doubted but that it depends upon the abovexircumstance. It would be nearly inexcusable to conclude this Lesson, without calling the attention of my young readers, for a moment, to the beneficent and wise laws established by the AUTHOR OF NATURE to provide for the various exigencies of the sublunary creation, and to make the several parts so depend- ant upon each other, as to form one well-regulated whole. In the torrid zone, and, it may be added, in the temperate and frigid zones also, in summer, the heat produced by the action of the solar rays would be insupportable, were not a large portion of it absorbed, in the process of Evaporation, into the atmosphere, without increasing its tempe- rature. This heat is again given out in winter, when the vapour is condensed, and mitigates the severity of the cold. The dry spring months are favourable to agriculture, and the Evaporation, which then begins to be considerable, absorbs a portion of the heat imparted to the earth by the sun, and thus renders the transition from cold to heat 114 EVAPORATION, &C. [Lesson XIX. heat slow and gradual. Jn autumn, the sun's in- fluence fails apace, but ihe condensation of vapour contributes to keep up the temperature and pre- vent too rapid a transition to winter. Thus have you another page of the volume of nature opened to your view ; and though de- scanted upon in a concise manner, I have no doubt but that it will be an additional incentive for you to increase in gratitude, reverence, and love for the adorable AUTHOU of ail good. LESSON LESSON XX. ON FROST. What art thou, Frost! and whence are thy keen stores Deriv'd, thou secret, all-invading power, Whom even th' illusive fluid cannot fly? THOMSON. XlOW admirably wonderful and diversified are the opejations of Frost ! The thronging mulii- tudes of the stars with peculiar brilliancy glitter through the fair expanse, while the Frost pours its subtle and penetrating influence all around ; and sharp and intensely severe throughout th^ long night continues its rigid operations. Loud rings the frozen earth, and hard reflect* A double noise : while at the evening watch The village dog deters the nightly thief: The heifer lows ; the distant water-fall Swells in the breeze ; and with the hasty tread Of traveller, the hollow sounding plain Shakes from afar. THOMSON. When, late and slowly, the morning opens her pale eye, in what a curious and amusing disguise is nature dressed ! The icicles, jagged and un- even, hang pendant from the eves, and a whitish film encrusts the windows, where mimic landscapes rise, and fancied figures swell. The once fruitful fields are hardened as iron, and the moistened mea- dows 116 rnosr. [Leston xx. dows are firmly congealed. The limpid stream is arrested in its career, and its formerly flowing sur- face chained to the banks. The fluid paths become a solid road ; and where the finny shoals were wont to rove, the sportive youths slide, or with rapid /motion skate along the crystal pavement. When these and other wonders brought about by freez- ing, are considered, surely it is not unnatural to ask — how are they occasioned ? This, perhaps, cannot be answered with the wi?hed-for accuracy : however, though the following observations do not entirely determine the point under consideration, they may yet be somewhat amusing. The fixing of a fluid body into a firm or solid mass by the action of cold, is called freezing, or congelation ; in which sense the terms are applied to water when it freezes into Ice. By what mean it is that fluid bodies should thus be rendered solid by cold, the learned have not yet been able to dis- cover. It would seem, however, that it arises from the air then abounding with nitrous and saline par- ticles, which insinuate themselves into the pores of water, &c.by which mean they become hard. This is the more probable when it is considered that zmongfreezing mixtures, all kinds of salts, whether alkaline or acid, are the principal ingredients. The process of congelation is always attended with the emission of heat : it is also observed, that water loses of its weight by freezing, being found lighter after thawing again, than before it was frozen. And indeed it evaporates almost as fast when frozen, as when it is fluid : iiay, it has been observed, Lesson xx.] FROST. 117 observed, that, in Frost, the greater the cold the greater the evaporation; and this, by the bye, fur- nishes us with areason why there should generally be more rain fall in February than in any other month. The manner in which congelation is effected, is now generally thus explained. When water is exposed to , some evil spirit attends,) Hovering, aud blazing with delusive light, Misleads th' amaz'd night-wanderer from his way Through bogs and mire. MILTOV 1 OO numerous by far are the stones of ghosts and apparitions, hobgoblins and spectres, which are handed down from one generation to another, by the great vvtakness and folly of some parents and nurses, who?e whole in'ention, one would imagine, is to make tueir children chiefly suscepti- ble of the impn sions of fear. When we consider how difficult it is to eradicate prejt.d cts which were imbibed in th Idhood, we shall not be greatly surprized at the avidity with which tales of the mischievous feats performed by Jack o' Lanterns, and Will u 1th a Wisps, are swallowed, even by up- grown people, of mature judgment in otb. r con- cerns. For instance, a child njay have been told by his father, that once, when he was going over a piece of marihy land in a dark night, he was sud- denly 144 IGNIS PATUUS. [Lesson xxm. denly startled with the appearance of a spirit wrap- ped up in fire, which kept dancing round him, and dazzled his eyes to such a degree, that he became dismally frightened, and so the fiery spirit led him out of his road, and then left him. This misfortune of the father would be remembered by the child when he arrived at years of maturity, when he would, perhaps, hear several similar tales from other persons, which the credulous youth would look upon as so many corroborating testimonies of the reality of such ghostly appear- ances ; and, of course, the prejudice would be the more rooted in his mind. Should any persons who have been thus mise- rably misinformed, peruse these Lessons, I hope they will be quickly convinced that these horrible Jack 61 Lanterns are far from having any thing supernatural about them : on the contrary, their cause, and the effects they produce, may be ac- counted for in a very natural and easy manner. The meleor vulgarly known by the names before mentioned, is among philosophers called Ignis Fa- tuus : it is chiefly seen about marshes, meadows, and other moist places, also in burying grounds that lie flat and low, and sometimes near dunghills. The appearances of it usually observed, sufficiently evince that it is an ignited vapour: for inflam- mable air has been found to be the most common of all the factitious airs in nature; and as it is known to be frequently produced from the putre- faction and decomposition of vegetable substances in water, with which marshes, bogs, 8cc. abound, it Lesson XXIIK] IGNIS FATUUS. it may be reasonably inferred that when this in- flammable air arises, it will be speedily kindled, and, being wafted about near the surface of the earth, will cause the appearances which create so much unnecessary alarm. Dr. Skaiv has described a singular Ignis Fatuus which he saw in the Holy Land, when the atmos- phere had been thick and hazy, insomuch that the dew on the horses' bridles was remarkably clammy and unctuous. This meteor was sometimes globular, then in the form of a flame of a candle; presently afterwards it spread itself so much as to involve the whole company in a pale harmless light, and then it would contract itself and suddenly disappear. But in less than a minute it would be- come visible as before, or, running along from one place to another, with a swift, progressive motion, would expand itself at certain intervals over niote than two or three acres of the adjacent mountains. In the plains in the territory of Bologna, these meteors are very often seen : sometimes they vary. in figure and situation in a very uncertain manner; but commonly they are very large, and give light equal to a torch. Even in England they are frequently seen in dif- ferent numbers, from two or three to upwards of twenty together in one field, running here and there with great rapidity; sometimes mixed to- gether and crossing each other's paths, as though ' they were danciig: then all at once several of them disappear, which may, perhaps, be occasioned by their striking against each other, or some cori- H tisruoii* 146 IGNIS FATUUS. [LeSSOH XXIH. tiguous object. In many places, one may be almost sure of seeing them every dark night. That persons should be ltd out of the way by these meteors is more to be attributed to their own unreasonable fears, raised by prejudices instilled into their minds in their infantile years, than any other cause. For when the Ignis Fatuus happens to overtake or approach them, ihcy are struck with fear and surprize at so shining a light, and dismal a spectre, as they imagine it to be; whence they, in their fright, immediately run out of the direct pathway, and by such deviation very probably lose their road entirely : more especially, if (as will most frequently be the case) the meteor be attracted after them in iheir flight. From a consideration of what has been here ad- vanced, the great importance of being educated without having any superstitious or childish pre- judices engrafted in the mind, is exceedingly ob- vious : to the elder part of my readers I would therefore take the liberty of recommending a pe- culiar attention that no idle trash be insinuated into the minds of their children j for in this, as well as other cases, Children, like tender osiers, take the bow, And as they first are fashiou'd always grow. To those who have, unfortunately, been badly educated in this respect, a friendly act would be, to endeavour with sound reasoning to convince them of their error, and dissuade them from giving hoed, in future,-to idle, superstitious, or inconsistent stories Lesson xxm.} IGNIS FATUUS. 147 stories of any kind ; advising them to furnish themselves with such knowledge, as may have a tendency to produce true pleasur.|e and happiness through life, and which when dying they can re- flect upon without uneasiness*. * " The natural offspring of prevailing superstition is infi- delity. Of the truth of this, the present times afford as a lamentable example. Where ignorance and fear once ruled supreme, there has rash philosophy but too successfully planted presumption and atheism. Tis the diffusion of pure and solid knowledge, which alone can preserve us from the dominion of these opposite tyrants. How should this consi- deration increase our zeal and stimulate our endeavours! The immediate sphere of our action may be circumscribed, but our exertions trill not on that account be entirely lost. In that circumscribed sphere let us labour to root out every superstitious lying vanity, and plant pure religion and unso- phisticated truth in its stead. " How charming, how enlivening to the soul, to gaze upon the dawning beams of opening light, to behold them irradiate that dismal gloom of intellectual darkness which long over- whelmed the millions of mankind! How supremely pleasing, to view them wider and wider spreading their invigorating influence ! How rapturously transporting, to contemplate the spleadescent prospect of pure and perfect day ! " Power supreme ! " O everlasting King! to thee we kneel, " To thee we lift our voice ;" " () spread thy benign, thy vivifying light over the iJvrefl;- iiiit> of the sons of men; dispel the yet impending mists of ignorance and superstition: and, O preserve us from the dismal gulph of infidelity and atheism; let thy truth run and prevail gloriously, let pure, celestial wisdom over- spread thp earth as the waters cover the sea! — Then shall millions kneel before thee with grateful and enrap- tured hearts; then shall they rejoice to sing the praises of thee, their Benefactor, their Father, and their Gad: then H 2 >uall 148 1SN1S FATUUS. [f.fSKOn XXHI. shall this val« of tears be filled with the mansions of joy and gladness, and become a blissful foretaste of those regions, where the saints, crowned with unfading glory and felicity, surround thy throne with never-ceasing hallelujahs !" See Sermons on " The Iwmty and Mischitf of Vitlgar Superstitions," by the Kev, M..J. Naylor. LESSON LESSON XXIV. ON THE AURORA BOREALIS. Silent from the north, A blaze of meteors shoots : cnsweeping first The lower skies, they all at once converge High to the crown of heav'n, nnd all at once Relapsing quick, as quickly reascend, And mix «ml thwart, extinguish and renew, All aether emu sing in a maze of light. THOMSON. 1 HERE are, perhaps, but few appearances in* nature which are more curious than those known by the appellations, Aurora B&realis, Northern- lights, or Streamers. The radiant streams, )ikfi legions rushing to the engagement, meet and mingle, insomuch that the air seems to be con- flicting fire; — presently they start from one ano- ther, and, like armies in precipitate flight, each marching a different way, they are thrown into a quivering motion : — the whole horizon is illumi- nated with the glancing flames j and, with an aspect partly awful, and partly ludicrous, they re- present extravagant and antic vagaries, The villagers, assembled together, gaze at the spectacle, first with astonishment, then with horror, H 3 150 NORTHERN LIGHTS. [Lesson XXIV. From look to look, contagious through the crowd The panic runs, and into woudroas shapes Th' appearance throws; armies in meet array, Throng'd with aerial spears and steeds office, Till the long lines of full extended war, In bleeding fight commixt, the sanguine flood Rolls a broad slaughter o'er the plains of heav'u. As thus they scaii the visionary scene, On all sides swell the superstitious diii, Incontinent; and bnsy frenzy talks Of blood and battle, cities overturn'd, And late at night in swallowing earthquakes sunk, Or hideous wrapt in fierce ascending flame ; Of sallow famine, inundation, storm ; Of pestilence, and very great distress; Empires subvers'd, when ruling fate has struck Th' unalterable hour: ev'n Nature's self Is deem'd to totter on the brink of time. THOMSON. Though this waving brightness, which plays so innocently over our heads, causes such astonish- ment in ihe gazing throng, it has a very different effect upon the philosopher: he feels stimulated to inquire how so curious, and in great measure pleasing, an appearance may be occasioned. In order to arrive at the result of such inquiry, it will be necessary to consider with attention the various phenomena of this meteor, as they have been ac- curately observed. It may be remarked, then, that the appearances of the Aurora come under four different descrip- tions : — First, a horizontal light, like the morning Aurora, or break of day; which horizontal light tends to the magnetic east and west, and is bisected by the magnetic meridian. — Secondly, fine, splen- did, Lesson xxtv.] NORTHERS LIGHTS* 751 did, luminous beams, well defined, and of dense light; these continue i, £, or 1 minute, sometimes apparently at rest, but more frequently with a quick •lateral motion. These beams appear at all places alike, to be arches of great circles of the sphere, with the eye in the centre ; and these arches, it* prolonged upwards, would all meet in one point. This converging point is the same as that to which the south pole of the dipping needle points, at the place where the observation is made. — Thirdly, flashes pointing upward, or in the same direction as the beams, which they always succeed. These arc only momentary, and have no lateral motion, but they are generally repeated many times in a mi- nute : they appear much broader, more diffuse, and of a weaker light than the beams: they become gradually fainter till they disappear ; but they sometimes continue for hours, flashing at inter- vals.— Fourthly, arches nearly in the form of rain- bows. These, when complete, go quite across the heavens, tending to the magnetic east and west, and crossing the magnetic meridian at right angles. When an Aurora takes place, the appearances above described generally succeed one another in the following order:— first, the faint, rainbow-like arches; second, the beams; third, the flashes. As for the horizontal light, it is found to consist of au abundance of flashes or beams, blended together, owing to the situation of the observer relative to them. These phenomena have been accounted for on various suppositions, i. It has been supposed to H 4 he 152 NORTHERN LIGHTS. [LffSSOn XXIV. be a fianie arising from a chemical effervescence of combustible exhalations from the earth. 2. It has been thought lo be inflammable air, fired by elec- tricity. 3. It has been imagined to be occasioned by the zodiacal light. 4. It has been conjectured, that it is caused by the reflection of the sun's •beams on large bodies of ice floating near the po- lar regions. But all these suppositions will admit t)f objections, being utterly inadequate to account .for the appearances. Lastly, it has been supposed electric light itself; and this opinion has met with many advocates since the identity of lightning and the electric matter has been determined : for we know that discharges of the electric fluid in the atmosphere do exhibit light; and for this, and other reasons which might be advanced, it is considered almost beyond a doubt, that the light of the Au- rora Borealisas-we]] as \hatof falling stars, and the large meteors, is electric light solely, and that there is nothing of combustion in any of these phae- nomena. M. Libes has lately proposed a new theory of the Aurora Borealis, which has already been adopted by most of the northern philosophers, and may be concisely stated thus : the production of hydro- genous gas is next to nothing at the poles ; there- tore, so often as the electricity is put into an equi- librated state in the atmosphere, the spark, instead of passing through a mixture of hydrogenous and oxygenous gas, as in our climates, passes through a mixture of oxygenous and azotic gas : it must therefore cause a production of nitrous gas, nitrous acid, Lesson xx i v.] NORTHBR-N LIGHTS.. 153 acid, and nitric acid, which give birlh to ruddy vapours, whose red colour will vary according to ihe quantity and proportion of those different sub- stances, which are generated. These vapours are carried towards the south, where the air is most dilated, so that they approach more and more to- wards the spectator; and it is probable their mo- tion may be assisted by a north wind. Sometimes they rise as if to the zenith of the spectator, and then descend again towards the south; and a great number of causes may carry the vapour towards the different points of the heavens, whence origi- nate the different motions taken by the Aurora Borealis, or its several parts. Lastly, the slight detonations which are sometimes heard, depend upon the small quantity of hydrogenous gas, which is found in the upper regions of the atmos- phere, and .which combines with the oxygen to form water. These principles, at the same time that they ac- count in. M. L'bcs's estimation, for all thephaeno- mena accompanying the Aurora Borealis, explain also why it is so common towards the poles^ and so rare in the temperate regions; while thunder, which is frequent in the torrid zone, is scarcely eve.*1 heard in the polar. regions. The disengagement of hydrogenous gas is considerable near the equa- tor, and very little towards the poles: and svhea we excite the electric spark in a mixture of hydro- gen, oxygen, and azote, it combines in preference the bases of the two former gases;, the electric spark ought, therefore, to occasion thunder solely H .•> in 134 NORTHERN XIGHTS. [LeSSOn XXIV. r.— .. — ^f^ft^ff^tt - • -_. ^.- . ^. ^ — _-~ — in hot countries, and to produce Aurora Boreales alone in cold countries. This theory, though plausible, is not, however, entirely free from objections. Mr John Dalton, whose name I mentioned in the Seventeenth Lesson, has advanced a new theory of the Aurora Borealis, in which he has endeavoured to shew, that the luminous beams of this phenomenon are cylindrical, and parallel to each other at least over a moderate extent of country, — that these cylindrical beams are all magnetic, and parallel to the dipping-needle at ihe places over which they appear, — that the distance of these beams from the earth is nearly equal to their len receive so much heat from the sun in the day time, as to continue warm, in some degree, through the night, and thereby preserve the fruit from frosts, or forward its growth ? With sundry other parti« culars of less or greater importance, that will occur from time to time to attentive mindsr" Many other properties of bodies of different Colours may be found in various parts of Sir Isaac Newton's Optics. The subject of Light and Colours has been lately consider- ed with much acuteness and attention by Mr. Delavel. From a variety of well-conducted experiments this gentleman con- cludes, that Colours are exhibited, not by reflected, but by transmitted Light. For an ample investigation of this curious and interesting subject, the reader must be referred to the Memoirs of the Manchester Society, Vol. II. Hack 164 LIGHT AND COLOURS. [Lesson XXV. black cannot with propriety be called a Colour, it being a deprivation of all Light, because the sub- stance stifles all the rays : but white, on the con- trary, is comprehended of all the primary Colours in one, as may be proved experimentally, by tak- ing a small wheel with a broad rim, which let be divided into 360 equal parts; then let 45 of these parts be painted red; 37, orange; 48, yellow; 5O, green; 60, blue; 40, indico ; and 80 of violet ; making in all 360 : if this wheel be whirled swiftly round, the rim will appear as though it were painted of the purest while. It is pretty generally admitted, that the whiteness of the sun's Light is owing to a mixture of all the original Colours in a clue proportion; and hence it is naturally con- cluded, that whiteness in other bodies is a dispo- sition to reflect all the rays of Light in the same proportion and order as they come from the sun. My young readers will, I doubt not, after at- tending to what has been advanced in this Lesson, readily unite with me in acknowledging, with gratitiule and joy, the great utility and benefit of Light. For by the help of this admirable, this first-made creature of the Deity ', we are enabled (•as before suggested) to behold many other of his glorious works : we can view with admiration and pleasure the beauties of the flowery fields, the gay attire of the feathered tribes, the exquisite and well-adapted proportions of many insects, qua- drupeds, and other creatures; we can dwell with rapture in the coiUemplaiion of extensive land- scapes Lesson xxv.] LIGHT AND COLOURS. 165 scapes and diversified prospects j we can trace enough to be convinced of the great harmony and beauty of the lower part of creation j and we can extend our views to the heavens, and thus survey God's wonderful skill and contrivance, so clearly manifested in every region of his glorious works. LESSON XXVI. ON THE RAINBOW. •• " Refracted from yon eastern clout! , Bestriding earth the grand etheriel bow Shoots up immense, and every hue unfolds, In fair proportion running from the red, To where the violet fades into the sky. THOMSON. DOUBTLESS you have frequently beheld thai beautiful appearance known by the appellation of the Rainbow, or Iris, bending gracefully and majestically across the sky, painting the arched vault with a pleasing variety of beautiful colours : when this is viewed by the philosophic eye, it immediately excites an inclination to explore the cause of so curious and pleasing a phenomenon. Not so the playful boy ; He wondering views the bright enchantment bend, Delightful, o'er the radiant fields, and runs To catch the falling glory ; but, amazed, Behold t h' amimve arch before him fly, Then vanish quite away. THOMSON. By a perusal of holy writ you will discover, that the Rainbow was first placed, and is still at times seen Lesson xxvi.J RAINBOW. 167 «een in the clouds, as a pledge of inviolable- fidelity and infinite mercy j assuring us, that, " while the "earth remaineth, seed-time and harvest, and " cold and heat, and summer and winter, and day (t and nigh*, shall not cease." How gracious and benevolent that BEING, who so often renews a covenant of kindness and mercy to his creatures; and that too, in such a manner as to raise pleas- ing sensations in every heart, and charm every beholder ! To account for the production of the Rainbotv, we are in the first place (o consider, that it is never seen but in the time of rain, or near it, and when the sun shines. You will understand, then, that when a ray from the sun falls upon a drop of rain in a cloud, if it enter the^ upper part of the drop in a proper situation, it will, by refraction, be thrown upon the inner surface of the back part of 'the drop; from thence it will be reflected to the lower part of the drop, at which place undergoing a second refraction, it will be bent towards the earth : and thus rays of the sun, after one re- flection, and two refractions, may come to the eye of a spectator, whose back is towards the sun, and his face towards the drop. When rays which are effectual, emerge from the drop after one re- flection and two refractions, those which are most refrangible, will, at their emersion, make angles with the incident rays, different from. those which are least refrangible; by which means the rays that produce the sensations of different colours will 168 IJAINBOW. [Lesson xxvi. will be separated from one another. Hence it may be easily perceived, that some of the falling globules may be in that position which will cause the rays that produce a red colour to fall upor the eye, — others next to them below will send forth orange-making rays, — the drops next to them will cast the yellow-making rays, — and those suc- cessively in order below them, will refract the blue, indico, and violet-making rays to the eye;— • and thus, in a certain space in the cloud, all the colours will appear ; and since, under the same angles, the same phcenomena will be produced, therefore an arch of this various-coloured light must necessarily be produced in the clouds. The different sizes of the Rainbows depend en- tirely upon the height of the sun at the time : for when the sun is in the meridian, or at his highest altitude, the bow will then be least to our sight, being but a small segment of a circle; but as the sun gets lower and lower, the bow will increase in height; and when the sun is in the horizon, or just setting, a bow at that time is as large as it can be, being very nearly semi-circular. It may also be ob- served that at all those places and times when the altitude of the sun is more than 42° no primary Rainbow can appear ; and when his altitude ex- ceeds 54l° no secondary bow can appear. With regard to the part of the sky in which a Rainbow appears, when I say that it is always opposite to the sun, I present you with an invariable rule where to find it ; and this is anadditional reason for Lesson xxvi.] RAINBOW. 169 for concluding, that the appearance is occasioned by the rays of the sun shining upon the falling drops of rain. There is also often seen a fainter coloured bow, commonly called a water-gall, above the Rainbow; and here it will be found, that the colours are in a contrary position to what they are in the bow it- self: hence it is evident that this is a kind of re- flection from the Rainbow, or a double reflection from the drops of rain ; and as a considerable quantity of light is lost at each reflection, it is plain that the colours in the superior bow will be more dilute and faint than those in the lower. The nature of the Rainbow, as here explained, may be illustrated and confirmed by experiment in several different ways. Thus, for example, hang up a glass globe, full of water, in the sun-shine, and view it in such a posture, that the rays which come from the globe to the eye may make an angle of about 42- with the sun's direct rays, and you will see a full red colour in that side of the globe opposite to the sun : and by varying the position so as to make that angle gradually less, the other colours, yellow, green, and blue, will appear very distinctly, in succession, on the same side of the globe. But if, by raising the globe, the angle be made about 50 , there will appear a red colour in that side of the globe which is toward the sun, though somewhat faint ; and if, by raising the globe still higher, the angle be made greater, x this 170 RAINBOW. [Lesson xxvi. this red will change successively to the other co- lours, yellow, green, ajid blue. Or, the appearances of the Rainbow may be exhibited, in a very natural and beautiful manner, any day when the sun shine?, with the assistance of an artificial fountain, or jet d'eau, which is an instrument expressly intended to throw up streams of water to a great height. These streams, spreading very wide in their upper part, when falling, form a delightful shower of artificial rain. When the fountain is playing, move between it and the sun, at a proper distance from the fountain, until your shadow points directly towards it : then looking at the shower, you will observe the colours of the Rainbow, very vivid and strong — those of the water-gall very languid and faint — the gradations of the colours of each in an inverted order : and, what forcibly shews the deceitfulness of vision, the bows appear, notwithstanding the nearness of the artificial shower, to be as far off, and as large, as those which we really see in a natural shower of rain. A similar bow is often observed among the waves of the sea, the upper parts of the waves being blown about by the wind and so falling down in drops : this is called the Marine Rainbow. This appearance is also sometimes seen by moon-light, though it is seldom vivid enough to render the difFert-nt colours distinguishable: it is then called the Lunar Rainbow. Rainbows are even sometimes seen on the ground, when the sun shines on a very thick Lesson xxvi.] RAINBOW. . IJL thick dew. All these are of the same nature, an they could not separate the metal from the ore, nor by any means make those instruments- for agricul- ture, arts, and manufactures, which we now have in such abundance ? For the sake of a supposition, let us imagine, that we were in a state, continually without light> without warmth, without any method of preparing raw food for sustenance, without all the conve- niencies, which metals (and principally iron) now afford Lesson xxvm.] F'RE* 179 afford us : let us suppose, I say, that in such a situation we received information that a person had invented something by the help of which all these defects and wants might be supplied : I would only ask, if we should not, under such circumstances, entertain very high ideas of the wisdom of the inventor ? The ingenious young reader will know how to apply this conjecture and question, without any farther comment upon them. By Fire is here to be understood, that subtile in- visible cause by which bodies are made hot to the touch, and expanded or enlarged in bulk ; by which fluids are rarefied into vapour; or solid bodies be- come fluid, and at last either dissipated and carried off in vapour, or else melted into glass. It seems also to be the chief agent in nature, on which animal and vegetable life have an immediate de- pendence. Among philosophers, Fire is now usually de- nominated CALOKIC, which appears to be a highly elastic and imponderable substance ; and it is so very subtile, that neither has its gravity been yet ascertained, nor its existence, in a simple and uncombined state, been shewn. There can be very1 little doubt that it radiates with light from the sun : and experiments shew, that, like light, its absorption is affected by the difference of colour and of surface possessed by different bodies. It combines chemically with all bodies, in a quantity proportioned to their affinity with it. By its elastic power, or power of repulsion, it constantly tends to 180 FIRE. [Lesson xxvnr. to separate the particles of matter ; in which it is opposed by the attraction of cohesion : hence at- traction of cohesion predominating, the body ex- ists in a solid form : caloric existing in such a pro- portion as to weaken the attraction of cohesion to a certain degree, the body assumes a liquid form j and when the quantity of caloric is increased still farther, the body takes a gaseous form. That heat moves, like light, with vast velocity, is inferred from caloric being always found to ac- company the rays of light. Dr. Herscheli has dis- covered that the coloured rays of light are pos- sessed of a heating power, and that the least re- frangible rays possess this power in the highest degree : this power diminishing as the refrangi- bility increases j the red rays possessing, therefore, the greatest, and the violet the smallest power. This property is directly opposite, in this respect, to the property which the rays of light possess, of deoxidizing substances exposed to their action 5 this property existing in the rays of light, in pro- portion to their degrees of refrangibility. It i* likewise remarkable, that as the deoxidizing power exists, in the highest degree of all, at a certain distance beyond the violet ray, and out of the spectrum, so the calorific power is found to exist, at its maximum, at about half an inch beyond the termination of the spectrum, by the red rays. These calorific rays, and which are even regarded as rays of caloric itself, suffer refraction and reflec- tion, similar to the rays of light ; possessing ge- nerally, however, less refrangibility than the rays of -Lesson XXVIIK] FIRE. 181 of light j and having the angle of their reflection equal to the angle of their incidence. This is supposed to be the case, not merely with the caloric immediately derived from the sun, but with that which proceeds from our common fires, candles, and even hot water, and iron heated not so much as to become lucid. It appears, by the experiments of Professor Pictet, that ihe radiation of heat, and even its reflection, takes place inde- pendent of light : thus a piece of iron heated, but not so high as to emit any light, being placed in the focus of a concave mirror, will very sensibly affect a thermometer, placed in the focus of another mirror opposed to the former. On the same principle, if ice be employed instead of heated iron, the thermometer will be affected in a contrary direction. From this latter experiment it has been conjectured that cold, as a body, is emitted from the ice, and reflected by the mirror. This opinion, however, appears to be entirely un- founded. On a lighted candle being thus em- ployed, and a plate of clear glass being placed be- tween the mirrors, the caloric appeared to be in- tercepted, although the light passed with its usual facility ; the thermometer sinking 14°, in nine minutes, and rising 12°, in seven minutes after its removal. Caloric is transmitted through some bodies with unabated rapidity, whilst its passage through others is very considerably retarded ; and hence bodies have been named either good or lad cojiductors. The cause of this difference has never yet been satisfactorily ascertained, All bodies appear 18« FIRE. [Lesson xxvin. appear to be capable of conducting caloric, and fluids also possess the property of conducting it slowly. Heat constantly tends to form an equilibrium, by passing from bodies of an higher and diffusing itself through bodies of a lower temperature. Two bodies of the same nature, unequally heated, on being brought into contact, soon arrive at an equal temperature, the caloric becoming equally divided between them. But when two bodies, differing in their nature, aad differing in * ^ w the quantity of caloric they possess, are thus al- lowed to form one common temperature, by com- munication, this will not be found to be an arith- metical mean between the two original tempera- tures ; but the one will be found to have required a greater or less quantity of caloric than the other, to render it of the common temperature. In this way it is found that the quantity of ca- loric which raises mercury 38', raises water only 12°; consequently the caloric which raises the temperature of water 1°, will raise that of the same weight of mercury 3.16°. The quantity of caloric which a body thus requires to heat it to a given temperature, is called the specific caloric of that body. Thus the quantity of caloric which heats water 1°, heats the same quantity of mercury 3.16' ; the specific caloric of water is, therefore, 3.16 times greater than that of mercury ; and, con- sequently, if the specific caloric of water be = 1, that of mercury must be = 0.31. It is fully established that the specific caloric is different in* different Tesson xxvin.] FIRE. 18* different bodies : as when bodies manifest the same temperature by the test of the thermometer* the relative quantity of caloric which they contain is, we discover, very different. Much ingenuity and acute investigation have been employed toj ascertain the absolute quantity of caloric which* they contain. These endeavours have not, per- haps, been as yet completely successful. Dr. Black discovered, that whenever a solid le- romes a fluid, a great portion of heat enters into it, which does not affect the thermometer j and that, on its again becoming solid, this portion of heat quits it, without a diminution of its temperature taking place. Snow at 32°, being mixed with an equal quantity of water at 172°, the snow melts, and the mixture is only 32"> j so that the water has parted with 14O1, which has disappeared, and has combined with the snow, shewing that snow or ice, during its change into water, absorbs, and, in- deed, combines with 140°, of caloric. It also ap- pears that water, though cooled down to 32", does not freeze until it has given out 140° of caloric : on the absorption, or the parting with this dose of caloric, depends therefore the fluidity or solidity of water. Not only the fluidity of such bodies as liquify, but the softness of such bodies as acquire this state by heat, depends also on the quantity of heat which thus combines with them> The mal» leability and ductility of metals likewise depends on the same cause. The quantity of heat thus im- bibed, Dr. Black calls latent heat ; since it does not manifest itself by its effects on the thermo- meter. 184 FIRE. [Lesson xxvm. meter. It has been called by others the caloric of fluidity. At the moment of the chemical union of two different substances, the new compound, not, per- haps, having the same capacity for caloric as its constituents, must either yield a part to neigh- bouring bodies, or receive it from them: pro- ducing thereby a change in their temperature, which is increased in the former, and diminished in the latter case. Ice, we have seen, imbibes the caloric of sur- rounding bodies, until it has imbibed sufficient to render it fluid j the temperature of those bodies descending proportionally. On this principle may be explained the effects of freezing mixtures, of snow and different salts, but particularly muriate of lime. During the liquefaction of these mix- tures, so rapidly and so considerably is the caloric absorbed, as to produce a most extraordinary de- gree of cold, such as even to solidify quicksilver. Another change in bodies is effected by the presence of heat. All liquids, and many solids,, assume a gaseous form, when heated to a certain temperature : thus water is made to assume the form of vapour, and become 1800 times more bulky than water itself. This change Dr. Black discovered also to depend on a certain portion of heat combining with the liquid, without producing any increase of temperature. The latent heat of steam was ascertained to be at least 940°. The Doctor proved that all liquids, during their change into vapour, combine with a portion of heat, with- out Lesson xxviii.] FIRE. 185 out undergoing a change of temperature ; and that on their reduction to a liquid state, a portion of heat is givtn out, and likewise without mani- festing any change of temperature. Thus it appears, that by a certain dose of caloric solid bodies become liquid, and that by a farther dose they acquire a gaseous form. Hence the ge- neral law discovered by Dr. Black ; Whenever a lody changes its state, it either combines with caloric, rr separates from caloric. Dr. Irvine admitted the importance of the facts discovered by Dr. Black ; but supposed, that the quantity of heat absorbed by different substances depended on the capacities which those sub- stances possessed for heat: and which he ascer- tained was different, in different substances ; and, in the same substances, under different forms. He also believed that the heat thus absorbed does not exist in any peculiar state : he therefore objected to the term latent heat, when intended to imply such a circumstance. It has been likewise ascertained, that on salts, which contain much water in their composition, as muriate of lime, &c. being dissolved in waier, the temperature sinks considerably ; but if previously deprived of their water, the temperature rises. This is to be explained by this law — that when the compound, formed by the union of two bodies, is more dense or fluid than the mean density or fluidity of the two bodies before mixture, then the temperature is diminished : but when the fluidity or 186 FIUF. [Lesson xxvm. or density becomes less, then the temperature is increased. Thus when the solution of a mixture of salt and snow is completed, the temperature rises. The whole of these phaenomena, as Dr. Thomson observes, as well as the evolution of heat during putrefaction or fermentation, are readily explained by Dr. Black's theory of latent heat. Setting aside certain particularities of a very few bodies, it may be assumed, that every addition of caloric to a body is succeeded by the expansion of that body : and every abstraction of caloric by a diminution of bulk. Gaseous bodies in general expand most : common air expands eight times more than water, and liquids expand more than solids : thus the expansion of water is about forty- five times greater than that of iron. Mr. Dalton, of Manchester, has ascertained, by a simple apparatus ; consisting of a graduated glass tube, open at one end, at which end mercury is in- troduced to a given point, the rest of the tube being filled by gaseous matter, the dilation of which is measur-ed by the quantity of mercury, which is forced out by the application of heat to the gas j that all gaseous bodies suffer the same degree of expansion from the same addition of caloric, under the same circumstances : and the increase of bulk it J- part, for 1° elevation of the mercury in the thermometer. M.GayLausac also made a series of experiments, the result of which coincided with that of Mr. Dal ton's. From these experiments Lesion xxvin.] FIRE. )&7 experiments it appears, that the expansion of all elastic fluids, including steam of water, vapour of ether, Jcc. is equal and uniform, and nearly equable. Fire, in a sensible or collective state, is well known to be one of the grandest agents of nature ; and for this very reason, perhaps, was regarded amongst most nations, in an early period of the world, cither as the creator and productive cause of all things, or, at least, as the substance from which the Creator produced all things. Hence the Persians, Ethiopians, Scythians, andCarthaginians, in the Old World, and the Mexicans and Peruvians in the New, paid divine honours to fire itself, or to the sun, which was esteemed the sublimest re- presentation of this element. Zoroaster ordained the erection of pyrea, or temples dedicated to fire, throughout all Persia. And even the Hebrews imagined fire to be the grandest proof of the pre- sence of the Deity. Under this symbol, He ap- peared to Moses on Mount Horeb ; and to the Hebrews at large on Mount Sinai, on the promul- gation of the sacred law ; and under this symbol He evinced his protective presence every night, by assuming the form of a fiery pillar. And, im- pressed with this idea, the Jews were ever anxious to preserve it in a pure and active flame, upon the national altar. When, therefore, the Jews were borne away in captivity to Persia, the priests took the sacred fire of the altar and concealed it in a dry cave, with which none but themselves were acquainted, and where, on their restoration to li- berty, 188 FIRE. [Lesson xxvnr. berty, the posterity of those priests found it on their return 10 Judea. (2 Mac-cab, i. 18.) Fire was regarded wiih an equal degree of veneration throughout Greece and Rome. Temples in every city were erected to the goddess Vesta — a name importing fire, whether derived from the Grecian grrja, or the Hebrew : and in every temple a lam- bent flame was perpettially burning over the altar. And even so late as in the third century of the Christian sera, when Heliogabalus anticipated his own apotheosis, and instituted the worship of himself over all the Roman empire, having erected a magnificent temple to his own divinity, he supplied its altar \\ith sacred fire from the temple of Vesta, which he plundered for this purpose. The frequent reference to fire in the Holy Scriptures, as emblematical and typical, and its frequent introduction either to add dignity or so- lemnity to occurrences, suggests important re- flections. Sacrifices were consumed by fire, to signify that wrath from Heaven is due to sin, and would fall upon the sinful offerer himself, if the victim did not receive it for him by sub- stitution. When the law was given on Mount Sinai, the heavens flamed with fire, and the moun- tain burned below, to give the people a sense of the terrors of Divine judgment. With allusion to which exhibition, and other examples of the ac- tual effects of his wrath, God is said to be " a con- suming fire " to his enemies, while he is as " « wall ef fire" about those who trust in him, to de- fend Lesson xxvni.] FIRE. 189 fend them. Elijah was taken up to heaven " in a chariot of fire ;" and the destruction of the world by fire, is a positive doctrine of Scripture. This doctrine, indeed, is perfectly consistent with the most correct philosophy. All bodies contain ca- loric, and this substance, by its expansive forre, tends constantly to ex1 end its energy to surround- ing substances. The matter which produces light- ning also, whatever it may be, is now found to be universally diffused through the system of nature : so that the heavens which, according to the lan- guage of Peter, are to " melt with fervent heat," want no foreign matter to convert them into fire. So, likewise, " the earth and the works that are therein," carry with them the seeds of their own destruction, and will, in the appointed time, be burnt up by that element which now r sides within them, and is only waiting for the word from its Creator. LESSON XXIX. ON WATER. Ye, whose vital moisture yields Life's pwrple stream, and fresh supply Sweet waters, wand'ring through the flow'ry fields, Or dropping from the sky ; Confess the Power whose all-snfficient name, Nor needs your aid to build, nor to support our frame. WATTS. IF any such person as an Atheist should peruse these Lessons, if he be not yet convinced of the existence of a DEITY, let him pass on with me to the contemplation of Water : and here I may ven- ture to say, that he will at least agree with me when I assert, that if there had been no such thing as water in the world, all mankind, and almost all living creatures, even in the midst of a super- fluity of air and other food, would certainly perish in a very short time ; since thirst, if it be not ex- tinguished, is soon fatal, all men and the greater part of the animal kingdom being unable to exist without drink. But it may be also observed, that even if it were possible that men and other creatures could exist without drinking, their condition would still be very XXIX.] WATER. 191 very miserable deprived of Water : for without its nourishment, neither grass, nor plants, nor trees, would be able to spring out of the earth ; the con- sequence of which would be, that animals, and consequently mankind would be deprived of food, as well as drink, whence death must speedily fol- low. From these passages I would not wish to have it inferred, that it is not in the power of the ALMIGHTY to furnish us with a substitute for Water: this the reader may easily judge is not my intention : my only design is, to ask, if these things be produced by chance, as Atheists assert, how it comes about that this same chance is always en our side ? For it must appear very strange, that it is owing to mere chance, that creatures in general have the faculty of supporting their lives by Water, and likewise that Water has, by a very lucky hit, acquired the properties which are neces- sary for that purpose ! From the Mosaic account of the creation of the world, we learn, that the division and partition of the Water into proper channels and courses, was part of the workmanship of the second and third days: we there also learn, that the business of the creation was completed in six days. GOD could certainly have spoken the whole world into exist- ence in an instant ; but his love for his creatures led him to consult their happiness, to make their felicity flow from their duty : for the regular man- ner in which HE has pleased to create all things, points out to us a lesson which should never be forgotten, namely, that we should so regulate the manner WATER. [Lesson xxix. manner of spending our time in this world, that the performance of one duty may not interfere with or obstruct another. Water is an uninflammable fluid, and, when pure, is transparent, colourless, and void both of tasst bodies, will cohere firmly with some others^ and bind them together in the most solid masses : as in the tempering of earth or ashes, clay or pow- dered bones, with water, and then causing them to be dried and burnt, when the masses become hard as stones; though, without the Water, they would have become mere dust or powder. Indeed, it appears wonderful, that Water, which is an almost universal dissolvent, should nevertheless be, in many instances, a great coagulator. It has been imagined by some that Water is In- compressible, and therefore non-elastic : but Mr. Canton has proved, by accurate experiments, that Water is actually compressed, even by the weight of the atmosphere. Besides, the diminution of size which Water suffers when it passes to a less degree of heat, sufficiently shews that the par- ticles of this fluid are, like those of all other known substances, capable of approaching nearer together. But the most remarkable property of Water is, that which has been already spoken of in the Twentieth Lesson : the discovery o£ which, as it ap- pears to be one of the most curious and important which modern times can boast of, I must again recur to. For this discovery we are indebted to Count Rumford; and it is given in his Essays. After proving, in a very satisfactory way, that the par- ticles of fluids are incapable of imparting heat to K. 2 e&ch 196 WATER. [Lesson xxix. each other, and that when their temperature is undergoing any change, an intestine faction is kept up in them, by a successive alteration taking place in the specific gravity of their particles, he proceeds to shew, that " all bodies are condensed (f by cold without limitation, Water only excep led," and describes the wonderful effects produced in consequence of this particular fact*. " Though in temperatures above blood-heat (says the Count), " the expansion of Water with " heat is very considerable, yet in ihe neighbour- " hood of the freezing point it is almost nothing. tl And what is still more remarkable, as it is an ex- tl ception to one of the most general laws of nature t( with which we are acquainted, when in cooling " it comes within eight or nine degrees of Fahren- * The circnmstances of this remarkable anomaly have been for some time believed to be the following: — When heat is applied to water, ice cold, or at a tempera- ture not far distant, it causes a diminution of the fluid. The water contracts, and continues to contract, with the tempe- rature, till it reaches the 10th or 41st degree. Between this point and the 42d or 43d, it suffers scarcely any perceptible change ; but when heated beyond the last-mentioned degree, it begins to expand, and increases in volume with every sub- sequent rise of temperature. During the abstraction of heat, the peculiarity in the con- stitution of water equally appears. Warm water, as it cools, shrinks, as other bodies do, till it arrives at the temperature of 43r or 42°. It then suffers a loss of two degrees without any alteration of density. But when farther cooled, it begins to dilate, and continues to dilate, as the temperature falls, till congelation actually commences, whether this occurs as soon as the water reaches the 32°, or after it has descended auy number of degrees'below it. « belt's Lesson xxix.] WATER. 197 " heit's scale of the freezing point, instead of going « on to he farther condensed, as it loses more of its " heat, it actually expands, as it grows colder, " and continues to expand more and more as it is " more cooled." After enlarging upon this subject, he proceeds thus : — " As nourishment and life are conveyed " to all living creatures through the medium of "Water; liquid, living Water; to preserve life, " it was absolutely necessary to preserve a great " quantity of Water in a fluid state, in winter as " well as in summer. But in cold climates the «'• temperature of the atmosphere, during many " months in the year, is so much below the " freezing point, that had not measures been taken " to prevent so fatal an accident, all the water " must inevitably have been changed to ice, which " would infallibly have caused the destruction of •" every living thing/' Count Rumford then shews how very powerfully this wonderful contrivance tends to retard the cooling of 'Water, when it is exposed in a cold atmosphere, and its consequent tendency to pre- vent all those dreadful evils which must have ne- cessarily ensued, had it not been for this remark- able property : but instead of making farther ex- tracts, which, as they must be short, would be in. adequate to the purpose, I must refer my young reader to the Essays themselves, for the time be- stowed on the perusal of which he will find him- self amply repaid. K. 3 Water, 198 WATER. [Lesson xxix. Water, as a fluid, is governed by several laws peculiarto itself, to notice all of which would require a volume : one of its most curious properties is, that its pressure, or force, varies in the proportion, of its depth, without any regard to its breadth : if it were not for this remarkable property, it would be impossible for ships, or any other vessels, to put out to sea, — for if the lateral pressure varied with the breadth, it is evident that every sailing vessel would be forced against the nearest shore with great violence, and, of course, there would be an insuperable bar in the way of navigation. As it would be absolutely impossible to mnke a calculation of the quantity of subterraneousWaters, I shall not attempi it ; but as it is a much easier matter to have an idea of the enormous quantity of Water on the earth's surface contained in seas, we will here set about it. It is a reasonable sup- position that of the earth's surface two-thirds are seas : now if we suppose one common depth to be the tenth part of a mile, we shall find that there is Water sufficient to cover the whole globe to the height of six hundred feet ; and if this Water were reduced into one mass, it would form a globe of more than sixty miles diameter. In reflecting upon the various changes of Water, we have a curious kind of perpetual motion placed in view : — Vapours are raised from the ocean, by means of the sun and other agents in the process of evaporation ; and these are transported by the winds,. 8cc. through every climate. The progress of these Lesson xxix.] WATER. 199 these vapours is interrupted by the tops of moun- tains, and other causes, whence they accumulate into clouds, and descend in the form of rain, snow, &c. as explained in the Nineteenth Lesson: after having refreshed the surface of the earth, the sur- plus proceeds, by virtue of its intrinsic gravity, to steer its course through rivulets, &c. to the lower parts, where it meets with rivers, which conduct it to the sea; from whence it again undergoes a si- milar process, and so on continually. Here I cannot help adverting to the great utility and ad- vantage of the distribution of the Waters and the D dry land; which, although it may seem rude and undesigned to a careless view, yet is admirably adapted to our benefit and convenience. The Earth and Waters are so placed about the globe, as to minister to one another's uses. The great oceans, with the seas and the lakes, are so exten- sive, and so situated as to produce sufficient va- pours for clouds and rains, to mitigate the heats, and to refresh the earth with fertile showers. The mountains and the smaller hills are distributed in such a manner as to afford proper situations for fountains, and the sources of rivers; and this, whether they are supplied from the condensation of vapours, or from subterraneous channels. Nay, so abundant is this great blessing which the most indulgent Creator hath bestowed upon us, by means of the distribution of the Earth and Waters, that there is more than a scanty, bare sufficiency, even a surplus and plenty, of this most K 4 necessary 20O WATER. [Lesson xxix. necessary article afforded to the world : this, too, is so well ordered, by means of the hills and vales on the surface of the earth, as not to suffer a sufficient quantity to remain stagnant at one time, to be of any material injury to mankind. How ought our hearts to overflow with gratitude and praise, for 'such beneficence and wisdom as ar« here made manifest \ LESSON LESSON XXX. FOUNTAINS OR SPRINGS. Tell by what paths, what subterranean ways, Back to the fountain's head the sea conveys The r,efluent rivei's, and the land repays : Tell what superior, what controuling cause, Makes waters, in contempt of Nature's law#, Climb up, and gain the aspiring mountain's height, Swift and forgetful of their native weight. BLACKMORE. 1 KE conjectures of philosophers, concerning the origin of Fountains, have been various : and though the subject has been discussed frequently for more than two thousand years, it is to be lamented that it is yet attended with considerable difficulty. Aristotle, whose thoughts on the matter have reached us, was of opinion, that the air contained in the caverns of the earth, being condensed by cold near its surface, was thereby changed into water, and, making its way through, formed foun- tains or springs. Most of the ancient philosophers after him, embraced this opinion j- but the mo- derns have entirely rejected it, as they have no ex- perience of any such transmutation of air into water. Among the hypotheses which have lately been proposed to account for the formation of Springs, K 5 I 802 FOUNTAINS. [Lesson xxx. I shall describe to you only three, they being the only ones which in my opinion carry with them any degree of probability. The first hypothesis is, that Springs are owing to rain and melted snow. The water penetrates the earth till it meets with a soil, or stratum of earth, of a nature sufficiently solid to sustain it, and pre- vent it from descending lower in such minute quantities. It then glides gently along in that way which the stratum declines, and in its passage meets with fresh quantities which have been fil- tered through in the same manner : these gradually descend together till they arrive at an aperture in the surface, through which they escape and form a spring, and perhaps the source of a brook or rivulet. Another hypothesis, so nearly allied to that just mentioned that it is almost unnecessary to dis- tinguish them in a work of this kind, is that of the ingenious Dr. Halley. When this gentleman made his celestial observations upon the tops of the mountains at St. Helena, he found that the quan- tity of vapour which fell there (even when the sky was clear) was so great, that his observations were thereby much impeded: his glasses were so covered with water through the condensation of the Vapours, that he was obliged to wipe them every ten minutes. In reflecting upon this, he was led to suppose that the water raised by evaporation from the seas and large rivers might afford a sufficient supply for the water discharged by Fountains. In order to deter- mine, with some degree of accuracy, how much water would be raised in vapour in any space of time, Lesson xxx.j SPRINGS, f03 time, he took a vessel of water salted to the same degree with that of sea-water, in which he placed a thermometer, and by means of a pan of coals brought the water to the same degree of heat as would be produced by the sun in summer : he then affixed the vessel of water with the thermo- meter in it, to one end of a pair of scales, and exactly counterpoised it with weights on the other. Then, at the end of two hours, he found by the alteration in the weight of the vessel, that a six- tieth part of an inch in the depth of the water was gone off in vapour; and therefore, in twelve hours, one tenth of an inch would have gone off. From this experiment the Doctor calculates (in as accurate a manner as the subject will admit) the quantity of water raised by evaporation from the Mediterranean Sea, to be at least five thousand two hundred and eighty millions of tuns of water in a day ; and from the River Thames twenty mil- lions three hundred thousand tuns per day, on the average. If, as it appeared reasonable to conclude, other seas and rivers should afford vapour in the same proportion, when they are acted upon by the sun in a similar degree; or in greater or less pro- portions as they are acted upon in a greater or less degree; this was thought, by the Doctor, a source abundantly sufficient for the supply of Fountains. The waters thus raised by evaporation, he ima- gined would keep rising, and float in extremely fcmall and light bubbles, till, being condensed by the cold, they become specifially heavier than the air when they would descend, or being driven by the wind* SPRINGS. [Lesson xxx. winds against the sides of mountains (some of which surpass the usual height to which the va- pours would of themselves ascend) are compelled by the stream of air to mount up with it to their tops; and, being presently precipitated, enter the crannies of the mountains, and glide down, as described in the former hypothesis. Jn the third hypothesis it is imagined, that the water is conveyed from the sea to the places where there are Fountains, by some subterranean passage; either by ascending in very small portions in capil- lary tubes, or by being conveyed in larger portions by means of Charyldes. Charybdis is a name given to an opening which is supposed to be in the bottom of the sea. The Fluxus moschonicus or MaalstromCf on the coast of Norway, is supposed to be owing to some such subterranean indraught; and it is asserted also, by several, that the Mediter- ranean Sea could not be emptied of the vast quan- tities of water which it receives, but would over- flow its boundaries, unless part were taken off by such a charybdis, which is either in some part of the bason of that sea, or near the mouth of it. In support of this supposition may be mentioned that strong under-current, described by all those who have treated of this sea. A large charybdis, placed near the strait's mouth, may be hid under the immensity of waters therej and as it would con- tinually draw in the lower waters in large quantities, it would necessarily cause such an under-current. If it be admitted, that there are such orifices as these eharybdes at the bottoms of some seas, it Lesson xxx.] SPRINGS. it is natural to inquire of what use they are. A«d perhaps none will offer a more probable answer to this inquiry, than those who say the waters of the sea are by such means conveyed through subterra- nean channels to the sides of mountains and hills, whence they gush out at convenient apertures, and form springs. Each of the hypotheses here advanced admits of objections. To the first two it is objected that they are not the only ways in which Springs are pro- duced: for as causes may always be measured by their effects, it is unphilosophical to conclude, that an inconstant cause will produce a constant effect— and therefore Springs which constantly send forth the same, or nearly the same quantities of water, cannot be supplied in the manner pointed out under the two first hypotheses, where the causes, as pain, snow, or vapours, are inconstant or variable. Suppose the truth of this remark be allowed, it does not follow from this, that all Springs are pro- duced in some other way. Perhaps, if the nature of Springs, and the nature of the hypothesis be compared, we shall, by such comparison, be brought to a very different conclusion. Let us consider the first hypothesis. Neither rain nor snow continues without intermission : but there are intervals between the showers, during which neither rain nor snow descends. Is it not probable, that those Springs which flow and stop alternately, and are therefore called intermitting Springs, are caused by these showers ? It may, perhaps, be objected, that in such Springs, the- time J00 SPRINGS. [Lesson xxx. time of flowing does not seem at all connected with the time of the shower. But in answer to this, I would observe, that it is not an easy matter to judge of this, as it cannot be determined which was the shower that caused the flowing of the Spring. Those showers which cause the Spring to flow may perhaps fall at a great distance from it j while those which fall near it may have an effect upon some Spring at a distance. Or there may be four or five showers fall in the interval, between the flowing o£ the Spring and that shower which caused it to flow. But perhaps it may be said, that this hypothesis will not satisfactorily account for those Springs which ebb and flow every six hours, or some such short period. It will not: we must therefore have recourse to the third hypothesis, and suppose that Springs which ebb and flow thus regularly are sup- plied by charybdes, placed in some parts of the sea of such a depth as to cause their discharges to be effected by the tide, and when the tide ebbs and flows at periods similar to those of the Spring. The second hypothesis will assist us in account- ing for reciprocating Springs, or those which flow constantly with a stream subject to increase and de^ crease. If these are supplied by condensed vapours, their streams will increase or decrease in propor- tion as the vapour which supplied them was pro- duced in a greater or less degree by the union of heat, wind, and other causes. As to those Springs which are constant and regular in their discharge, we may suppose, that they are supplied from ckaryldes) situated at such a depth Lesson xxx.] SPRINGS. 207 depth as to be not at all affected by the ebbing and flowing of the sea ; but convey the water always in equal portions in equal times, and, of course, supply the Springs with regularity. Against this hypothesis of charybdes, T imagine two objections will be opposed ; but I think neither of them will overset it. And first, it may be said, that if many of the Springs are supplied in this way, the charybdes must be numerous, and therefore it js surprising that not more of them are discovered. Here I would reply, that if there are many, suppose a charybdis to a Spring, it follows that they must, comparatively speaking, be very small, and of course, their effects may not be perceptible upon so large and deep a body of water. A hole a quarter of an inch in diameter, would let out much liquor from a full hogshead, though it would not disturb the tranquillity of the liquor at the surface. But, in the second place, it may be said, that I cannot explain the way in which water is con- ducted so high above its source. I cannot j. but this is no proof that it is not so conducted — no more than it would be a proof that a man was lifeless, because he could not account for his own existence. The properties of various kinds of matter have been determined j but only in such circumstances as would admit of experiments being tried : in those cases wheje we can only form a judgment by analogy, we are always liable to fall into error, though we may sometimes escape it. Since the late discoveries in Electricity and Mag- netism, matter has been found to possess qualities which 208 SPRINGS. [Lesson xxx. which philosophers of an earlier period were not aware of: and in all probability, matter differently modified, or under different circumstances, may possess properties which, are yet undiscovered. Let this stimulate us to fresh exertions in the cause of philosophy ; and if, after all, we are obliged to confess ourselves purblind and ignorant in a great degree, let us not despair ; for Religion points out a cheering prospect : she directs us to a period when all our faculties shall be expanded, and all our inquiries satisfied : " When GOD'S almighty hand shall lift the curtain high, And all creation's wonders open to our eye." LESSON LESSON XXXI. ON THE TIDES. Now the mighty mass of water swells Resistless, heaving on the broken rocks, And the full river turning, till again The tide revertive, unattracted leaves A yellow waste of idle sands behind. THOMSON. 'PHILOSOPHERS in every age of the world have been greatly puzzled to explain and account for the Tides of the sea, which ebb and flow twice in twenty-four hours ; but in despite of every attempt, the doctrine of them remained in obscurity, until the great Sir Isaac Newton developed the mystery. This eminent philosopher having demonstrated that there is a principle in all bodies, by which they mutually draw or attract each other in certain pro- portions according as their distances or size vary, proved that as fluids are very easily put in motion by any force acting upon them, those parts of the sea which are immediately below the moon, must be attracted towards it, and consequently wherevec the moon is nearly vertical, the sea will be raised, which occasions the flowing of the Tide there. A similar reason occasions the flowing of the Tide likewise in those places where the moon is in the nadir, CIO TIDES. [Lesson xxxi. nadir, and which must be diametrically opposite to the former : for in the hemisphere farthest from the moon, the parts in the nadir being less attracted by her than the other parts which are nearer to her, gravitate less towards the earth's centre, and con- sequently must be higher than the rest. Those parts of the earth, on the contrary, where the moon appears on the horizon, will have low water: for as the waters in the zenith and nadir rise at the same time, the waters in their neighbourhood will press towards those places to maintain the equilibrium ; to supply the place of these, others will move the same way, and so on, to the places ninety degrees distant from the zenith and nadir, where the water will be the lowest. Let the diurnal rotation of the earth be now taken into the consideration, and it is evident, that every portion will pass twice through the elevated, and twice through the depressed parts, so as to produce two Tides in the day. But the places of high and low water are now altered ; for the impressed motions of rising and falling are retained for some time after the forces which produce them are greatest: and the greatest elevation happens about three hours after the meridian of the place has passed under the luminary, when it points about half a quadrant to the east of it : and the water continues to descend for 90 degrees hence, or till the meridian points about half a quadrant to the east of the next quarter. But in shallow seas, and in the mouths of rivers, the Tides are retarded till the fourth, fifth, or perhaps, sixth hour, after the meridian Lesson xxxi.] TIDES. 211 meridian of the place has passed under the lumi- nary. The force of the sun to raise the Tides, is about a third that of the moon : but it is evident, that when the forces of both conspire,"so as to elevate and depress the water in the same places, then the Tides are greatest, and are called Spring Tides, which happen about the new and full moon. When the moon is in her quarters, she elevates the water most where it is most depressed by the sun, and the contrary ; and the Tides, being raised by the difference of their forces, are least, or Neap Tides. But because of the continuation of motion, these effects are greatest and least, some time after the forces are : so .that the greatest Spring Tides commonly happen three days after the new and full moons; and the least Neap Tides three days after the first and third quarters. By the action of the sun the time of high water is also changed, being sometimes sooner, and sometimes later than it would happen by the action of the moon alone. For in the transit of the moon from new or full to a quarter, when the tide raised by the sun alone would precede that raised by the moon alone, the high water which is produced by their united actions, will happen at an interme- diate time, nearer to, but yet before, the time at which it would be raised by the action of the moon. But when the moon is passing from her quarters to the new or full moon, since the sun alone would produce TIDES. [Lesson xxxi. produce a greater tide, the time of high water is retarded. The greatest Spring Tide will happen when the moon is in perige, if other things are the same : and the succeeding Spring Tide, when the moon is in apogc, will be least. But because the. earth is nearer the sun in winter than in summer ; and the effect of a luminary is also greater, the nearer it ap- proaches to the plane of the equator ; the greatest Spring Tides, and the least Neap Tides, will gene- rally happen immediately after the autumnal and before the vernal equinox. In places remote from the equator, the two im- mediately succeeding Tides are unequal, whenever the luminary declines from the equator. Thus it is observed, that the evening tides in summer exceed the morning Tides ; and the contrary, in winter. For, if the greatest elevation immediatelyunder the luminary points to one side of the equator, the op- posite greatesfelevation points as much to the other side. And those places, which are on the same side of the equator with the luminary, approach nearer to the greatest elevation, when the luminary is above the horizon, than to the greatest opposite elevation, when the luminary is below the horizon. This inequality is greatest, when the sun and moon have the greatest declination. It is also greatest in places most remote from the equator. The nearer the place approaches to the poles, the farther it is removed from the greatest elevation on the opposite side of the equator. Thus the less Tide Lesson xxxi.] TIDES. Tide is continually diminished, til! at last it en- tirely vanishes, and leaves only one Tide in the day. Hence it is found by observation, that, when the moon has declination, there is only one Tide in twenty-four hours in all places in the polar regions, in which the moon is either always above or al- ways below the horizon, during a whole rotation of the earth about its axis. These things would happen uniformly in the manner above described, if the whole surface of the earth were covered with water ; but since there is a multitude of islands, continents, &c. which inter- rupt the natural course of the water, varieties of appearances are to be met with in different places, which cannot be explained without regarding the situation of shores, straits, and other objects : and as this would lead me too great a length, with- out oeing of much utility, I shall here take my leave of the subject, with remarking, that the most correct popular view of it with which I am ac- quainted is given by Laplace in his Exposition du Systems du Monde. LESSON LESSON XXXIT. ON DAYS AND NIGHTS. My God, all nature owns thy sway : Thou giv'st the Night, and Thou the Day ! When all thy lov'd creation wakes, When Morning, rich in lustre, breaks, And bathes in dew the opening llow'r, To Thee we owe her fragrant hour; And when she pours her choral song, Ker melodies to Thee belong ! Or when, in paler tints array'd, The Evening slowly spreads her shade ; That soothing shade, that grateful gloom, Can more than Day's enliv'ning bloom, Still ev'ry fond and vain desire, And calmer, purer thoughts inspire; From eartli the pensive spirit free, And lead the soften'd heart to Thee Miss WILLIAMS. PjlEVIOUSLYto the dawn of thetruepbilosnphy, when several erroneous opinions were entertained by philosophers, the principal one with regard to the form of the earth was, that it was a vastly wide extended plain ; lhat the visible horizon bounded the earth, and the ocean bounded the horizon. To account for Day and Night, it was then imagined that thesun in the morning emerged from the eastern ocean, and, after pursuing his daily Lesson XXKII.] DAYS AND NIGHTS. 215 daily track, was immerged inio the western ocean, whence, in the course of the Night, he travelled on to the eastern in order to perform his next di- urnal journey : an absurd doctrine, which is now entirely laid aside ; except, indeed, by the most illiterate. But as my young readers will readily admit the near approach of the earth to a spherical form, I must endeavour to explain to them the occasion of Day and Night in a more rational manner. — On account of the immense distance of the earth from the sun, and the earth's minute size when compared with him, it is evident that the rays of light emitted from that luminary (setting aside the effects of the atmosphere) will fall upon the earth in parallel directions, and will always illuminate a hemisphere of the earth, whilst the other hemisphere remains in darkness. Hence then, so long as any parti- cular place on the earth continues in the darkened hemisphere, it will be night at that place : but, as soon as that place, by the diurnal rotation of the earth from west to east, is brought to the verge of the enlightened hemisphere, then \sDay-lreak; and The morn, in russet mantle clad, Walks o'er the dew of you high eastern hill. SHAKESPEARE. When the meridian of that place is, by the rotatory motion, brought directly beneath the sun, it is then Noon there, and at every place in the enlightened part of the same meridian : but in the darkened part of the same meridian it is 21() ' DAYS AND NIGHTS. [LesSOH XXJ is then midnight. As the place is carried for- ward, the afterhoon hours keep wasting, until it arrive at the edge of the darkened hemisphere, and then approaches sober Evening, shedding her dusky influence round : that part of the globe which is directly opposite., is, at the same moment, just emerged from darkness into Day-light : and thus, by the earth's rotation, the whole is obviously accounted for. When to the western main the Sun descends, To other lands a rising day he lends ; The spreading dawn another region spies, And e'er the Antipodes* begins to rise: While we in Sleep's embraces waste the night, The climes oppos'd enjoy meridian light ; And when those lands the busy sun forsakes, With us again the rosy Morning wakes. GAY. To explain the reason of the different lengths of Days and Nights will be part of the subject of the next Lesson : but I shall first present you with an agreeable method of shewing all those places of the earth which are enlightened by the sun at any time. In order to this, let a terrestrial globe be taken from its several appendages, and placed upon a pedestal in the sun-shine, in such a manner that its north pole may point directly towards the north pole of the heavens, and that the meridian of the place where you are may be directly toward the south. Then the sun will * Those people are called Antipodes, who, living on the other side of the earth, have their feet directly opposite to ours. shine XXXII.] DAYS AND NIOHYS. shine upon ail the like places or the globe, as 4ie does really on the earth, rising to some when he is setting to others: as you may perceive by noticing where the enlightened hair" of the globe is divided from the half in the shade ; all those places, on which the sun shines at any time, having day, — and all those on which he dues not shine, having night : also, when any pL.ce is near the middle of the enlightened part, it is then nearly noon there ; and those places which ar$ about the middle of the darkened part, have then, midnight. The vicissitudes of Days and Nights have raised in the minds of several prose and poetical writers very serious and excellent reflections concerning the sublunary state : with one of which this Lesson day be concluded. For ever running an enchanted ronnd, Passe* the Day, deceitful, vain, and void ; Af* fleets the vision o'er the formful brain, This moment hurrying wild th* impassion'd soul, The next in nothing lost. Tis so to Itim The dreamer of this earth, an idle blank; A tight of horror to the cruel wretch, Who all day long in sordid pleasure roli'd, Himself an useless load, has squauder'd vilsj Upon his scoundrel train, what might have chcer'd A drooping family of modest worth : But to the generous still-improving mind, That gives the hopeless heart to sing for joy, Diffusing kind beneficence around, Boastlcss as now descends the silent dew; To him the long review of order'd life la inward rapture only to be felt. LfcSSON LESSON XXXIII. ON THE SEASONS. Observe the circling year; how unperceiv'd H«r Seasons change! behold, by slow degrees, Stern Winter tam'd into a ruder Spring ; The ripeii'd Spring a milder Summer glows; Departing Summer sheds Pomona's store; And aged Autumn brews the Winter's storm. ARMSTRONG. 1 THINK there is scarcely one of the youthful perusers of these pages, but must have an inclina- tion (if he be not already acquainted with it) to be made sensible in some measure of the reason and cause of that agreeable succession of the Seasons which constitute the year. 'Here we meet with a variety, the limits of which are not ascertainable. With pleasure we behold the varied appearances of nature : whether Spring arrays herself in her spotted robe; or Summer scorches with his sultry beams j or Autumn pours forth her exuberant stores j or Winter with his howling tempest drives us to our habitations; — still we are admirers of na- ture, and disposed -" To mark the mighty Hand That, ever busy, wheels the silent spheres; Works in the secret deep ; shoots streaming thence The fair profusion that o'erspreads the Spring ; Flings Lest on xxxm.] SEASONS. Flings from the sun direct the flaming day; Feeds ev'ry creature ; hurls the tempest forth : And as on earth this grateful change revolves, With transport touches all the springs of life." It may have been observed that, when explain- ing the nature of the tides, I said, " The earth is nearer the sun in Winter than in Summer." This may to many persons appear improbable, but it is absolutely fact : for the apparent diameter of the sun is about 32' 48" on the shortest day, and only 31 30" on the longest : whence it is manifest that his distance from us must be less in the former case than in the latter. But the effects occa- sioned by the difference of distance are more than counterbalanced to the inhabitants of the earth's northern hemisphere : for, though the sun in Summer be farther from us ; yet, on account . of his being more nearly in a vertical position, his rays fall more directly on any part, and of course are denser and thicker; and this, not •nly because the same quantity of rays fell on a less space of the earth, but because they are not so much refracted and attenuated by the at- mosphere, as when they fall upon it more ob- liquely. The diversity of seasons is occasioned by the earth's annual motion in her orbit ; and in this motion two peculiar circumstances must be well understood, because on their combination the whole phaenomena depend. " 1. The earth's axis does not always keep the same relative situation with regard to the sun as the centre of its orbit ; L 2 but. 220 SEASONS. [Lesson t>ut, on the contrary, it always keeps very nearly in a parallel position, or points always towards the same part of the heavens. 2. The axis of the earth is inclined to the plane of the earth's orbit, which may be conceived by supposing a spindle put 'through a ball, with one end of it touching the ground, oj table; then by moving the ball directly forwards whilst the one end of the «,pindlto describe. Let two large circular hoops nearly of «qin the centre of the hoops, and a small terrestrial globe must be taken from its ap- pendages, having a string tied to its north pole, from which string the globe may be suspended. In this experiment, the candle flame must be sup- posed to represent the sun, and the inclined hoop the earth's orbit: just on the inside of this hoop, the globe suspended from the string must be car- tied gently round in a direction from west to east ; then JLesson xxxni.] SEASONS. then its axis will always be parallel to itself, and the various seasons will be represented in the different parts of the path. Thus, when the globe is at one of the places where the hoops intersect, its poles are equally illuminated, and the days are every where of the same length : then Spring commences to the inhabitants of the northern hemisphere; being about the 9Oth of March. As the globe is carried onrthe days keep increas- ing, until it has arrived at the lowest part of thft hoops ; when the north pole will appear a con- siderable way in the illuminated hemisphere, and the south pole as much in the darkened one ; then is our beginning of Summer and their beginning of Winter ; and here it may be perceived that any parallel of latitude toward the north pole is considerably more in the enlightened hemisphere than in the darkened one; while, on the con- trary, in the southern hemisphere, a far greater part of the parallel of latitude is darkened than enlightened: hence, our days are then longest* and theirs shortest; which happens about the 21st of June. The globe being carried on until it arrive at the intersection of the hoops on the other side; each. of. its poles is again illuminated, and the days every, where of equal length^ because each parallel of latitude is half in the enlightened and half in- the darkened part^ then 'Commence* Autumn with us, being about the 22el. of Sep- tember. As the globe is- carried oa> the days with us shorten, until it has-arrived at the highest part of the hoop : then the north pok is in th« fc.-3 darkened 222 SEASONS. [Lessen xxxw. darkened hemisphere, and the southern one in the enlightened part; our day is at the shortest, while in the southern hemisphere the clay is lon- gest; our Winter commences and their Summer; . being about the 21st of December. As the mo- tion of the globe is continued, our days lengthen ;. and when it has again arrived at the intersection of the hoops, we have Spring, and the inhabitants of the southern hemisphere have Autumn. In the course of this experiment it will be found, that •ach of thepoles continues enlightened half through the annual revolution, and darkened through the other half: consequently, at the poles of the earth, there is but one day and one night through the year. At the equator the sun's rays fall perpendicu- larly on the earth, and therefore act more powerfully; whence arises the great heat* of the torrid zone. On advancing towards both poles,, the rays fall more and more obliquely, and therefore act with less force and less; whence this -space is occupied, first by the temperate .zones extending on each side the tropics, and then by the frigid zones extending from these to the poles. So weak is the sun's power in these last owing to the great obliq-uity with which its rays strike the earth, that they are buried in almost •perpetual snow and ice. But these are merely the differences of climate: the differences of Season depend not upon these causes merely, but also upon the length of time that any por- iion of the earth is exposed to the solar rays. During Lesson xxxin.] SEASONS. 223 During the short days, the sun's influence it less, both with respect to the intensity of its rays and the time of their continuance, which there- fore produces \yinter: during the long days, it is greater in both respects, and therefore causes Summer. The middle seasons of Spring and Au- tumn correspond with the equality of nights and days. It is to be remarked, however, that this correspondence is not perfectly exact ; for the severest frosts usually take place afier the days hare begun to lengthen, and the most oppres- sive heats are found to happen when the days are decreasing : the reason of which is, that the earth, having imbibed more heat than it gave out during the summer months, is not exhausted of its superabundant warmth till about the close of the year: in like manner, because the waste of the earth's heat is greater in Winter than its supply, it continues to imbibe heat during the Spring, and is not saturated till after the Summer Solstice. Hence also arises the differ- ence between the Spring and Autumn, though the position of the sun,, in respect to the earth, is in both the same. The heat, "of- the Spring is inferior to that of Autumn, both in point of regularity and degree; for, on account of the deficiency of warmth in the earth, it is con- stantly imbibing heat from the lower part of the atmosphere; hence originates a large collec- tion of cloud.-?, which, intercepting the solar rays, combines, together with the absorption of the earth, to .deprive the air of much of its heat: • L.4 whereas 224 REASONS. [Lesson xxxu:> •whereas in Autumn, the earth being holier thaiu ' the air, gives out regularly a large portion of •warmth, which, naturally tending to disperse the clouds, affords a free passage to the solar rays. Thus Autumn ought in general to be hotter than Spring, far these two reasons : first, that the earth itself- gives out a considerable quantity of heat ^and, se- condly, that the rays of the sun meet with fewer interruptions in passing thence to the earth. At the equator there is no proper difference of Sea- sons except as occasioned by rainy or windy pe- riods, which proceed from other causes ; and the. case is much the same on each side of it for some, distance. Several of the British poets have presented us •with a variety of descriptions of the Seasons ; some Serious, some humorous and comic. As an in- stance of thff latter, we have a droll account of Winter's effects, in a song in Shakespeare's play of (< Love's labour lost" But the obvious simi- larity between infancy, youth, manhood, and old age of human life, and the Spring, Summer,. Autumn,.and Winter of the year, suggests a subject for the most sublime reflections. The excellence o£ those which Mr. Thomson has made on this heady will supersede the necessity of my apologizing for giving them insertion here. -Behold, fond roan ! See here ihy pictur'd life: pass some few years, Thy flowering Spring, thy Summer's ardent strength, Tliy sober Autumn fading into age, And pale concluding Winter conaf t sit last And- JE«SOH XXXI11.] SEASONS. 225 And shuts the scene. Ah! whither now are fled Those dreams of greatness ; those unsolid hepes Of happiness ; those" longings after fame; Those restless cares ; those busy bustling days ; Tliose gay-spent festive'nights ; those veering thoughts, Lost between good and ill, that shar'd thy life ? All now are vanished! Virtue sole survives, Immortal never-failing friend of man ; His guide to happiness on high.' Ami set ! 'Tis come, the glorious morn ! the second birth Of heav'n and earth! Awakening nature hears The new-creating word, and starts to life, In every heighten'd form, from paift and death For ever free*. The great eternal scheme, Involving all, and in a perfect whole Uniting, as the prospect wider spreads, To reason's eye refin'd clears up apace. Ye vainly wise! ye blind presumptuous! now, Confounded in the dust, adore that POWER And WISDOM oft arpaign'd : see now the cans* "Why unassuming worth in secret liv'd, And died neglected'; why tfte good man's sbarfe In life, was gall and bitterness of soul ; Why the lone widow and her orphans pin'd In starving solitude ; while luxury, In palaces, lay straining her low thought, • To form unreal wants ; why heav'h-born truth, And moderation fair, wore the red m;trks Of superstition's scourge; why liceu&'d paiuy That cntel spoiler, that embosora'd'foe, Imbitter'd all our-blissr. Ye good distrest ! Ye noble few! who-here imbelidirrg stand Bt-ueath life's pressure, yet bear up a while, And what your bounded view, which only sa-w A little part, deem'd evil, is no more : The storms of wintry time will quickly pass, Aiul ou« unbounded spring encircle all! THOMSON'S WiNftn. LESSON XXXIV. VEGETABLES OR PLANTS. Your contemplations farther yet pursue; The wondrous world of Vegetables view: Observe the forest oak, the mountain pine, The tow'ring cedar, and the humble vine, The bending willow that o'ershades th« flood, And each spontaneous offspring of the wood. BLACKMOHEV IVlY young readers having undoubtedly expe- rienced delight in viewing the beauties of the Ve- getable Creation, I am in hopes of contributing to their satisfaction, while I endeavour to explain the nature of Vegetables and Vegetation. A Vegetable or Plant is an organized body, con- sisting of various parts, taking in its nourishment usually by a root, and increasing its dimensions by growth. Vegetables may be divided into three classes; namely, herbs, shrubs, and trees. Herbs are those sorts of Vegetables whose stalks are soft, and have no wood in them ; as parsley, lettuce, violets, grass, thistles, and an infinite number of others. Shrubs are those Plants which, though woody, never grow into trees, but bow down their branches Lesson xxxiv-.J VEGETATION. 827 branches near the earth's surface: such are those Planrs which produce roses/honeysuckles, goose- berries', raspbcrres, and the like. But trees shoot up in one great stem or body, and rise to a consi- derable distance from the ground before they spread their branches : as the oak, the ash, the dm, the beach, the fir, the walnut tree, the pear tree, and many others. The most considerable parts of Plants are the root, the stalk or stem, the kaves, the flowers, and the seed. Most Plants have these several parts; though there are some that have not all of them : the alot, for instance, has no htalk ; the savine has no leaves ; the fern has no flowers. The uses of most of the parts of Plants are very obvious: thus, the root evidently serves as a ba- lance or counterpoise to the head, and by that means enables the Plant to stand firmly in the ground. In what other way could enormous oaks be kept upright and fixed, but by the counter- balance of their extensive, turgid roots? The fibrous par's of the roots of Plants, like so many mouths, absorb nutritious juices from the earth, and thus convey to the Plants the chief of their nourishment. The root also discharges the office of a parent, by preserving the embryo Plants jn her bosom, during the severity of the winter, in form of bulbs or buds. The trunk, or stem of plants, consists of various parts, as bark, wood, pith, sap vessels, &c. The bark of Plants performs the same offices to them that the skin does to animals : it clothes and de- fendi VBGETATioy. [Lemn xxxiv. jfrnds them from injuries, inhales the moisture of the air and conveys from the Plant the superfluous humid particles. The bark (as well as the wood) is supplied with innumerable vessels, which. convey the fluids to and from every part of the Plant: the wood aUo is furnished with others,. which contain air,, ami are distributed through its- substance. The stability of trees and shrubs con- sists in the wood, which corresponds with the bones of animals. The pith, which is a fine tissue of vessels originating in the centre of the stem, is supposed to be the seat of life. The fluids of Plants are : the sap, analogous to the blood of animals, — and the proper juice, which is of various colours and consistence, in different individuals ; as white or milky in the dandelion, resinous in the fir, and producing gum in cherry or plum trees » The leaves contribute both to the benefit and the ornament of the plant : they are supposed to answer the purpose of lungs ; and by their readi- ness to be moved by the wind, they may in some measure act the part of muscles. They are very porous on both their surfaces, and inhale and ex- hale freely. In some Plants (as Venus's Fly-trap), the leaves are armed with long teeth, like the an* tenna of insects : they are so irritable, that when an insect creeps up them, they fold1 up, and crush or pierce it to death. The uses of th« flowers and seed, are too evident to need enumeration. The most general method of propagating Plants is XXXIV.] VEGETATIONS is by seed : some, however, are raised by a part of the root of the old plant set in the ground, as po- tatoes f otheFS-, by new roots propagated from the old one», as hyacinths and tulips; others by cutting off branches and putting them into the ground which will there take root and grow, as vines; and others are propagated by grafting, and budding, or inoculation* What is most difficult with respect to Plants (and what has been the subject of much controversy, though yet undetermined), is to explain the man- ner in which they receive tlieir nourishment. The earth has not so much to do in this business as has been commonly supposed. This is known from the experiments of Mr. Boyle and Dr. Woodward. These gentlemen raised several Plants in earth- watered with rain or spring water, and even distil- led water; and upon weighing the dry earth, both before and after the product! an of the Plants, they found that very little of it was diminished or takem up by the Plant- Jf the earth contributes so little towards the production and nourishment of Plants, it seems natural to apprehend that water must be much concerned; and that this is the case in great mea- sure is evident, from the quantity of water which- most plants require to keep them in a state of health and vigour. But there is some other agent besides water; else, how can the growth of Plants in sandy desarts where it seldom rains be account- ed for, and these Plants such as cuntain juices i» great abundance ? Dr. Hunter^ ISO VEGETATION. [LesSOH XXXIV. Dr. Hunter, so well known and so justly cele- brated both as an anatomist and a naturalist, is in- duced, by a number of experiments accurately con* ducted, to believe, ttfat all Vegetables receive their principal nourishment from oily particles incor- porated with water by means of an alkaline salt$ or absorbent earth. Till oil is made miscibk-, it cannot enter the radical vessels of Vegetables! and on that account, Providence has bountifully supplied all natural soils with chalkv or other ab-> sorbent particles : and those soils which are as- sistfd by art are full of materials for that purpose;. as lime, marl, and the volatile alkaline salt of pu- trid dunghills. The argument in favour of oil being the prin- cipal food of Plants is confirmed by the observa- tion, that all Vegetables, whose seeds are of an oily nature, are found to be remarkable impoverish- ers of the soil ; as hemp, rape, and flax : and the best manures for lands worn out by these crops are such as have a good deal of oil in their com- position, provided that they are laid on with lime, chalk, marl, or soap-ashes, so as to render the oily part f les miscible with water. But Plants not only receive nourishment by. their roots, but also by their leaves. Vegetables- that have a succulent leaf, such as peas, beans, and buck wheat, draw much of their nourishment from the air; and on that account impoverish the soil less than wheat, oats, barley, or rye, the leaves of which are of a firmer texture. The leaves of al] kinds of grain are succulent for a time, during which . Lesson xxxiv.] VEGETATION. 231 which the Plants lake little from the earth ; but as soon as the ear begins to be formed, thty lose their softness, and diminish in thtir attractive power. The radical fibres are then more vigorously employed in extracting the oily particles from the tarth, for the nourishment of the plant. The leaves of Plants serve not only to imbibe the dew and rain, which contain salt, sulphur, &c. but they serve also as excretory ducts to separate and carry off ihe redundant watery fluid, which by being long detained in the Plants, would turn rancid and prejudicial to them. The annual sun- flower is an extraordinary instance of this fact : it is said to perspire nineteen times as much as a man in twenty-four hours. Fine weather encou- rages the perspiration of Vegetables; but in htavy, moist, and wet weather the inhalation is greatest. The effluvia of Plants is thought unwholesome to persons of delicate constitutions; but particularly so at night, and in a dull state of the atmosphere : the matter perspired by the yew tree, in particular, is said to be very noxious. Let us now endeavour to illustrate the subject of Vegttation, by taking a view of what happens to a bean after it has been committed to the earth. In a few days, sooner or later, according to the tem- perature of the weather and disposition of the soil, the external coverings open at one end, and dis- close to -.he naked eye part of the body of the grain. This substance consists of two lobes, between which the seminal Plaut is securely lodged. Soon after VEGETATION. [Lesson xxxir. after the opening of the membranes, a sharp pointed body appears, which is the root. By a kind of instinctive principle (if the expression may be allowed), it seeks a passage downward, and fixes itself into the soil. At this period the root is a smooth and polished- body, and has, perhaps, bub- little power to absorb any thing from the earth for the nutriment of the germ. The two lobes next begin to separate; and the germ, with its leaves, may be plainly discorered. As the germ increases- insize, the lobes are farther separated, and the ten- der leaves, being closely joined, push themselves- forward in the form of a wedge* These leaves* take a contrary direction tcrthat of th* root: they seek a passage upward; which having obtained, they lay aside their wedge-like form, and spread- themselves in an horizontal direction, as being the best adapted for receiving the rains and dew. The radicle, every hour increasing in size and vigour, pushes itself deeper into the earth, from- which it now draws some nutritive particles. At the same- time the leaves of the germ, being of a succulent- nature, assist the Plant by attracting from the at- mosphere such particles as the tender vessels are* fit to convey. These particles, however, are of a watery kind, and have not in their own nature a*- sufficiency of nutriment for the increasing Plant. Vegetables, a& well as animals, during their tender state, require a large share of balmy nourishment. As soon as an animal is brought to life, the milk of its mother is supplied i& a liberal stream : but, at LlSM-Jl XXXIV.] VFCETAT10N. this period, the tender germ seems only to have the crude and watery juices of the earth for its support* This, however, is not the case ; for the Vegetable lives upon a similar fluid, though differently sup- plied. For its use the farinaceous lobes are melted down into a milky juice, which, as long as it lasts, i& conveyed to the tender Plant, by means of innu- merable small vessels which are spread through the substance of the lobes ; and which, uniting into one common trunk, enter the body of the germ, and thus supply that balmy liquor, without which the Plant must inevitably ha\ e perished, its root being then too small to absorb a sufficiency of food, and its body too weak to assimilate it into nourishment, Thus admirable and well contrived is the method of Providence, in supporting the Plant in its earliest and tenderest stages ! As the plant increases in size, the almy juice diminishesrtill at last itisq^uite exhausted. The trunk of small vessels then dries up, and the external covering of the seed appear* connected with the root in the form of a shrivelled bag. In the process of vegetation there is no mor« lalityt from the moment that the seed is lodged in its parent eapth, the vegetative soul begins its- operations, and,, in the whole successive gradation of them-, illustrates the wisdom, power, and bounty of Him who created and rules the UNIVERSE. These attributes of the ALMIGHTY are also strikingly manifested, in the provision which he has afforded them against the winter season to secure them from the effects of cold. Those called her- I'aceous, which die down to the root every autumn, are 234 VEGETATION. [Lesson xxxiv. are now safely concealed under ground, preparing their new shoots to burst forth when the earth is softened in spring. Shrubs and trees which are ex- posed to the open air have all their soft and ten- der parts closely wrapt up in buds, which by their firmness resist all the power of frosts ; the larger kind of buds, and those which are almost ready to expand, are farther guarded by a covering of resin or gum, such as the horse-chesnut, the sycamore, and the lime. Their external covering, however, and the closeness of their internal texture, are of themselves, as some say, not adequate to resist the intense cold of a winter's night : a bud detached from its stem, enclosed in glass, and thus protected from all access of internal air, if suspended from a tree during a sharp frost, will be entirely penetrated and its parts deranged by the cold, while the buds on the same tree will not have sustained the slight- est injury: either the detached bud must have been injured by reason of the cold entering it at the part where it was broken from the stalk; or we must attribute to the living principle in Vegetables, the power of resisting cold to a very considerable degree ; — probably each of these is true in »ome measure; but how Vegetables require this latter- mentioned property, must be left for future obser- vations to determine. After the frost is moderated, and the earth suffi- ciently thawed, the first vital function in trees is the ascent of the sap, which is taken up by the ab- sorbent vessels composing the inner bark of the tree, and reaching to the extremity of the fibres of the Lesson xxxiv.j VEGETATION. 23 "i the roots. The water and oil, thus imbibed by the roots, is there mfxed with a quantity of saccharine matter, and formed into sap, whence it is distri- buted in great abundance to every individual bud. The amazing quantity of sweet liquid sap provided for the nourishment of some trees, is evident from a prevalent custom in this country, of tapping the birch in the early part of spring; thus obtaining from each tree more than a quart of liquor, which is fermented into a species of wine. This great accession of nourishment, by means of the ascent of the sap, causes the bud to swell, to break through its covering, and to spread into blossoms, or length- en into a shoot bearing leaves. This is the first process, and, properly speaking, is all that belongs to the springing or elongation of trees j and, in many Plants, namely, all those which are annual or deciduous, there is no other process. The Plant absorbsjuices from the earth, and, in proportion to the quantity of these juices, increases in size; it ex- pands its blossoms, perfects its fruit; and when the ground is incapable, by drought or frost, of yield- ing any more moisture, or when the vessels are not able to draw it up, the Plant perishes. But in trees though the beginning and end of the first process is exactly similar to what takes place in annuals, yet there is a second process, which at the same time that it adds to their bulk, enables them to go on increasing through a long series of years. This second process begins soon after the first, in this way. At the base of the foot-stalk of each leaf a small bud is gradually formed; but the absorbent vessels 936 VESETATION. [Lesson xxxtv. vessels of the leaf, having exhausted themselves in the formation of the bud, are unable to bring it nearer to maturity. In this state it exactly resem- bles a seed, containing within itself the rudiments of vegetation, but destitute of absorbent vessels to nourish and evolve the embryo. Being surround*- ed, however, by sap, like a seed in moist earth, it is in a proper situation for growing ; the influence of the sun sets in motion the juices of the bud,, and of the seed ; and the first operation in both of. them, is to send forth the roots downwards a cer* tain depth, cor the purpose of obtaining the. neces- sary moisture. The bud, accordingly, shoots down- its root-? upon the inner bark of the tree, till they reach the part covered by the earth. Winter now arriving, the cold and defect of moisture, owing t»- the clogged condition of the absorbent vessels,. cause the fruit and leaves to fall ; so that, except, the. provision of buds with; roots, the remainder of the tree, like an annual plant, i« entirely dead : the. leaves, the flowers, and fruit, are gone ;. and what was the inner bark is no longer organized, while the roots of the buds form a new inner bark ; and thus the buds with their roots contain all that re- mains alive of the whole tree. It is owing to this annual renovation- of. the inner bark, that the tree increase.? in bulk j and a new coating being added every year, we are iience furnished with an easy and exact method qf ascertaining the age of a tree,, by counting the number of concentric circles of which the trunk is composed. A tree, therefore, properly speaking, is rather a congeries of a mul- titude. Lesson xxx!v.] VEGETATION. titiule of annual Plants, than a perennial indi- vidual. The sap in trees always rises as soon as the frost is abated, that when the stimulus of the warm weather in the spring acts upon the bud, there should be at hand a supply of food for its nourishment; and if, by any means, the sap is prevented from ascending in proper time, the tree inevitably perishes, as has been very frequently observed. Before I conclude this Lesson, I cannot forbear paying a few words on the different manners in which Plants disseminate their seed. Having gone through the progressive stages of springing, flower- ing, and seeding, fhey liave at length brought to maturity the rudiments of a future progeny, which are>now to be deposited in thefostering bosom of the earth. Seeds are scattered by the hand of nature in various ways. Those of them which are furnish- ed with plumes, or wings, are dispersed about by the high winds which blow soon after the Autumnal Equinox, the time of dissemination. Hence Plants with such seeds are, of ail others, the most generally to be met wkh: as dandelion, groundsel, thistles, &c. Others by means of hooks, with which they are furnished, lay hold of passing animals, and are thus carried to distant places •: the common burs are examples of this contrivance, Several when ripe are thrown out with considerable force, from their receptacle, by means of a strong spiral elastic spring; of this the impatiens,or touch-me- not, and all the species of cardamine, or cuckoo- flower, are instances. Many are co; tamed in berries, 238 VEGETATION. [Lesson berries, which being eaten by birds, the seeds are discharged again uninjured, and grow wherever they happen to fall. In these, and in many other ways, is the distribution of various kinds of Vege- tables provided for. The shedding of the seed . being finished, the parent Vegetable, if of the herbaceous kind, either totally perishes or withers down to the root; if a shrul, or tree, it casts all those tender leaves that in the Spring and Summer it had put forth. Thus it continues until the fol- lowing Spring, when These naked shoots, Barren as lances, among which the wind Makes wintry music, sighing as it goes, Shall put their graceful foliage on again, And more aspiring, a*nd with ampler spread, Shall boast new charms, and more than they have lost. LESSON LESSON XXXV. EARTHQUAKES. The earth shook and trembled; the foundations also oftht hills moved, and were shaken, because He was wroth. DAVID. HISTORIANS relate innumerable instances of the dreadful and various effects of those tremend- ous phenomena called Earthquakes : from which I shall select two only. The first is the description of the Earthquake at Calabria, in the year 1638 :. it happened whilst the celebrated Father Kircher was on his journey to visit Mount JEtna; and I shall present it in the language of that great pro- digy of learning. egan to shake most dreadfully, so that, being un- able Less«n XXXV.} EARTHftUAKES. 242 able to stand, my companions and I caught hold of whatever shrub grew next to us, and supported ourselves in that manner." " After some time, this violent paroxysm ceas- ing, we again stood up, in order to prosecute our voyage to Euphasmia, which lay within sight. In. the mean time, while we were preparing for this purpose, I turned my eyes towards the city, but could see only a frightful dark cloud, that seemed to rest upon the place. This the more surprised us, as the weather was so very serene. We waited, therefore, till the cloud had passed away : then turning to look for the city, it was totally sunk. Wonderful to tsll ! nothing but a dismal and pu- trid lake was seen where it stood. We looked about to find some one that could tell us of its sad catastrophe, but could see no person. All was be- come a melancholy solitude; a scene of hideous desolation. Thus proceeding pensively along, in quest of some human being that could give us a little information, we at length saw a boy sitting by the shore, and appearing stupified with terror. Of him, therefore, we inquired concerning the fate of the city ; but he could not be prevailed on to give us an answer. We entreated him, with every expression of tenderness and pity, to tell us ; but his senses were quite wrapt up in the contempla- tion of the danger he had escaped. We offered him some victuals; but he seemtd to loath the sight. We still persisted in our offices of kindness ; but he only pointed to the place of the city, like one out of his senses, and then, running up into the M 2 woods 244 EARTHQUAKES. [LesSOJl XXXV. woods, was never heard of after. Such was the fate of the city of Euphsemia: and as we conti- nued our melancholy course along the short, the whole coast, for the space of two hundred miles, presented nothing but the remains of cities; and men scattered, without a habitation, over the fields. Proceeding; thus along, we at length C7 O * C1 ended our distressful voyage, by arriving at Na- ples, after having escaped a thousand dangers both at sea and land." The great and almost universal Earthquake which happened on the 1st of November, 1755, affords a dreadful example of the chief attendants of these striking phaenomena, on which account the young reader shall be presented with the fol- lowing description of it. ' At Lisbon its effects were most severe. In 1750, there had been a sensible trembling of the earth felt in that city : for four years afterwards, there had been an excessive drought ; insomuch that some springs, formerly very plentiful of water, were dried and totally lost. The predomi- nant winds were north and north-east, accompa- nied with various, though very small, tremors of the earth. The year 1755 proved very wet and rainy; the summer cooler than usual; and for forty days before the earthquake, the weather was clear, but not remarkably so. The last day of October, the Bun was obscured, with a a singular gloominess in the atmosphere. The-lst of Novem- ber, early in the morning, ;i thick fog arose, which was soon dissipated by the heat of the sun; no wind Lesson xxxv.] EARTHQUAKES. wind was stirring ; the sea was calm, and the weather as warm as in June or July in this coun- try. At 35 minutes after nine, without the least warning, except a rumbling noise not unlike the artificial thunder in our theatres, a most dreadful earthquake shook, by short but quick vibrations, the foundations of all the city, so that many build- ings instantly fell. Then, with a scarce precepti- b!e pause, the nature of the motion was changed, and the houses were tossed from side to side, with a motion like that of a waggon violently driven over rough stones. The second shock laid almost the whole city in ruins, with prodigious slaughter of the people. The earthquake lasted in all about six minutes. At the moment of its beginning, some persons on the river, near a mile from the city, heard their boat make a noise as if it had run aground, though they were then in deep water; and at the same time they saw the houses falling on both sides of ihe river. .The bed of the river Tag us was in many places raised to its surface. Ships were driven from their anchors, and jostled together with great violence ; nor did their masters know whether they were afloat or aground. A large new quay sunk to an unfathomable depth, with several hundreds of people who were upon it ; nor was one of the dead bodies ever found. The bjr was at fmt seen dry from shore : but suddenly the sea came ruling in like a mountain; anci dboi.t fielem Castle the water rose 50 feet aim -t u <ck las't-d about ten minutes, but they felt^maller ones for the space of 24 hours. Such were the phaenomena of this very remark- able and destructive earthquake, which extended over a tract of at least four millions of square miles. There have been various hypotheses entertained "with regard to the production of Earthquakes ; nor does it appear an easy task to account for them with great precision. Those which are only felt at small distances are probably occasioned by the action of subterraneous fires, and the explosion of volcanoes. But there have been Earthquakes which are felt at great distances, and have shaken an extensive tract of country : this kind of Earth- quakes is by some persons accounted for in the following manner. To understand properly what .may be the cause of these ; hoeuomcua, it must be remembered, that all inflammable matters capable of explosion pro- duce, like gunpowder, by inflammation, a great quantity of air j that this air produced by fire is in a state of very great rarefaction j and that, by a state of compression in which 'it is found in the bowels of the earth, it must produce very violent "fetTects. It is then conjectured, that at a consider- able depth, as at about one or two hundred fa- thoms, pyrites and other sulphureous matters are to be met with ; and that by the fermentation pro- duced £6-2 EARTHQUAKES. [Lesson xx xv. not even appear to have been exposed to a great heat. The Indians, indeed, assert that they sometimes arrive alive at the foot of the mountain. Sometimes these animals are ejected from the mouth of the crater, sometimes they are vomited forth at the lateral cavities; but always at from 24 to 26OO yards above the neighbouring plains. M. HumL'olilt thinks that they live in the lakes situated at this height in the inside of the crater : and S76 VOLCANOS. [Lesson xxxvr. and what confirms this opinion is, that the same species is found in the rivulets which run at the foot of these mountains. It is the only species of fish which lives at the height of 2800 yards in the realm of Quito. This species is new to our naturalists. M. Humloldt has delineated it on the spot, and given it the name of Pimelodrus Cyclopum, which signifies thrown up ly the Cyclops — a name in some respects analogous to their origin. Dr. Woodward mentions the existence of Vol- canos as a special favour of Providence, and says— " There are scarcely any countries that are much " annoyed with earthquakes that have not one of " these fiery vents. And these are constantly all *' in flames whenever any earthquake happens ; tf they disgorging that fire which, whilst under- " neath, was the cause of the disaster. Indeed," says he, " were it not for these diverticula (t whereby it thus gaineth an exit, it would rage " in the bowels of the earth much more furiously, " and make greater havoc than it doth now. So> t( that though those countries, where there are " such xolcanos, are usually more or less trou- ** bled with earthquakes; yet, were these Volca- " nos wanting, they would be much more annoyed " with them than they now are j yea, in all proba- " bility to that degree, as to render the earth, for " a vast space around them, perfectly uninhabit- " able, In one word, so beneficial are these to» " the territories where they are, that there do not (f want instances of some which have been res- " cued Lesson XXXYI.] VOI.CANOS. 277 " cued from earthquakes by the breaking forth of " a new Volcano there j this continually discharg- " ing that matter, which being till then barricaded " up, and imprisoned in the bowels of the earth, <{ was the occasion of very great and frequent ca- " lamities." Let me then be permitted to observe in this place, that though we cannot, in every case, see the beneficent tendency of particular creatures and things in the universe, we ought to attribute this to our limited capacities ; and not arraign AL- MIGHTY SOVEREIGNTY, as is the custom with too many carping sciolists of the present day. How- ever dreadful and destructive subterraneous fires may appear : on proper reflection it may be in- ferred, that they are as necessary in promoting and sustaining the operations of this part of the uni- verse, as the natural heat in men's bodies is to the preservation and support of their being. As every body possesses inherently the princi- ples of its own dissolution, it is by many wise and learned men imagined that the general conflagra- tion may at last be brought about by means of these fires. Amongst the natural means of causing it we are acquainted with, some persons embrace the opinion here mentioned, whilst others are in- clined to think the effect will be produced by co- mets : but though finite creatures may conjecturfc on this subject, it is most probable that it will ne- ver be ascertained by mortals-. Such knowledge is J D not necessary for us ; and may be withheld for the wisest and most beneficent reasons. LESSON LESSON XXXVII. ON THE EYE. In the materials of the human frame, What num'rous wonders might we quickly name : Let it suffice that I describe a few, And treat my readers with a short review. VvE will now direct our contemplations to the human jabric : and here the science of Anatomy discovers to us ten thousand beauties which the narrow limits I have prescribed mystlf preclude my mentioning : indeed it would not be possible, in a performance of this kind, to explain adequate- ly the geometrical and mechanical accuracy with which the AUTHOR OF NATURK has constructed every part of the body, to carry on the animal economy, and answer the various purposes of life. All I propose to perform in this and the two fol- lowing Lessons is, by touching upon the nature and wonders of the Eye, of Concoction, and of the Circulation of the Blood, to give my young readers some little insight into these matters, as an, inducement for them to set apart a portion of their leisure time for the purpose of acquiring a farther acquaintance with Anatomy. And Lesson xxxvu/J THE EYE. 279 And first, for a short description of the organ of Sight, that noble instrument which O ' Takes in at once the landscape of the world, At a small inlet which a grain might close, And half creates the woudrous world we see. YOUNG. The Eye is in form nearly globular: it consists of three coats and -hree humours. The part of the outward coat hid from our sight is called the Sole" rotica : the front part, which rather projects out, the Cornea : the next within this coat is that called the Choroides, which serves, as it were, for a lining to the- other; in the front it joins with that part known by the name of the Iris, because it is in different persons of different colours, as blue, brown, green, &c. The iris is composed of two sets of muscular fibres ; the one, of a circular form, which contracts the hole in the middle called the Pupi1, when the light would otherwise be too strong for the E\e; and the other, of radial fibres, tend- ing every where from the circumference of the iris towards the middle of the pupil: these, by their contraction, dilate and enlarge the pupil, when the Irght is wi-ak, in order to admit more rays. The third coat is only a fine expansion of the optic nerve, which spreads like net work all over the in- side of the~choroides, and is therefore called the Retina : upon it are in a manner painted the images of all visible objects, by the rays of light which cither flow or are reflected from them. Immediately under the cornea is a fine transpa- rent S80 THE EYE. [Lesson xxxvn. rent fluid, like water, which is therefore called the aqueous humour : it gives a protuberant figure to the cernea, and has the same limpidity and refrac- tive power as water. At the back of this lies a humour transparent like crystal, and much of the consistenca of hard jelly : it is shaped like a double convex glass, and is a little more convex on the back than on the fore part : it is named the crystalline humour) and is of service in converging the rays which pass through it, to its focus at the bottom of the Eye. This humour is enclosed in a fine transparent membrane from which proceed ra- dial fibres, called the ligamentum ciliare^ all around its edge, joining to the circumference of the im. These fibres have a power of dilating and contract- ing occasionally, by which means the convexity of the crystalline humour is altered ; and it is also thereby shifted a little backward or forward in the Eye, so as to adapt its focal distance at the bottom of the Eye to the different distances of objects : .a provision without which we could only see objects distinctly at one particular distance from the Eye.. At the back of the crystalline, lies the vitreous humoitr, which is transparent like glass, as its name denotes, and is largest of all in quantity ; filling the rest of the Eye, and giving it a globular shape : h is much of the consistence of the white of an egg, its refractive power very little exceeding that of water. As rays are emitted or reflected from every point of an object; some of these from the side next ihe Eye will fait upon ihe cornea, and, by passing on through Lesson xxxvn.] THE EYE. f Si through thep*pzV and different humours, will be converged to various points on the retina at the bottom or' the Eye, and will form upon it an in- VTted picture of the object J or, if this inverted image be not formed, the object cannot be seen : when, unfortunately, any of the parts of the Eye are so injured as to lose their transparency, the person becomes blind. But it is not sufficient, in order to our seeing objects, that their images should be painted on the retina : some persons, it is said, are blind, though this takes place. Hence it should seem, that images painted on the retina are not the immediate object of vision, and that the perception of the soul is communicated some other way. The small nerves of the retina (it is now generally admitted) are agitated by the rays of light which form the image at the bottom of the Eye j and this agita-. tion is transmitted by the optic nerve to the brain. It is there the mental perception is formed ; but the nu»t dextrous anatomist is unable to pursue these nerves 10 their source: the union of the soul with the body will probably for ever remain a mystery. There is an astonishing apparatus of muscles, with which the Eye is furnished, to produce all the necessary and convenient motions : among these I cannot help alluding to that admirable contrivance by which the pupil is contracted or dilated, ac- cor.-iing as vision requires. This variability of the pupil is essentially necessary to vision : for, if an involuntary contraction were not to take place when the Eye was brought into a very enlight- ened 362 THF. EYE. [LfSSOJl XXXVlf. ened situation, the great number of rays which would enter, would probably much injure the fine contexture of nerves at the bottom of the Eye, or* which the image* of objects are pourtrayed; and if the pupil did not expand when ihe eye was in a dark place, the few feeble rays which would enter the Eye, would not form any impression on the retina. Hence it is a very remarkable and pro- vidential circumstance, that the change in ihe pu- pil should take place almost spontaneously and independent of any act of the will. The five following associated circumstances w seem to have some influence on our judgment con- cerning distance : the number of objects which intervene, the degree of distinctness in which the minute parts are seen, the degree of brightness, the inclination of the optic axes, and the confor- mation of the Eye. Thus, distance is chiefly con- ceived from experience j and the more distant an, object is, the less it appears : when therefore, from certain circumstances, we cannot form a just con- ception of distance, and when we cannot judge of objects but by the image which is pourtrayed in our Eyes, we are then necessarily deceived as to their size. Thus every person must be aware how liable we are, in travelling by night, to mistake a distant tree for a bush that is near, or a bush near at hand for a tree at a distance. In the same manner if we do not distinguish objects by their shape, and by it also judge of distance, the fallacy is likely to continue: in this case, a fly, which may pass before us slowly, will seem to be a bird at Lesson xxxvn.] THE EYE. 283 at a considerable distance j and a horse, which may be in the middle of a plain, not moving, and in an attitude similar, for instance, to that of a sheep, may in the dusk appear in every sense like a sheep. If, therefore, we are benighted in a strange place, where no judgment of distance can be formed, we are every moment liable to deceptions of vision. Hence originate niost of the dreadful stories of spectres, and of those wonderful, hideous and gigantic figures, which many persons speak of hav- ing seen. Though it is commonly asserted, that such figures exist solely in the imagination ; yet it is highly probable, that they might appear to the Eye in every respect as described. This remark will be allowed to have the greater force, when it is considered, that if the size of an object be in grekt measure estimated by the angle which it forms in the Eye, it is magnified according to its propinquity : of course, if it seemed at first to the spectator (who is equally incapable of distinguish- ing what he sees, and of judging at what distance it is,) a few feet high, when at the distance of thirty or forty yards from him : it must look to him, when, he is within a. few feet of it, of a size stupendously increased. At this he will naturally be terrified, unless he touch and 'hus distinguish the seemingly enormous object j for in* the instant he has an actual perception of what it is, the enormity will diminish, and the object will appear in its real state: if, on the other hand, he be afraid to ap- proach it, and flee from the spot with precipita- lion, f 84 THE ETE. [LeSSOH XXXVlf. tion, the only idea remaining of what was present- ed to his view, will be that of an image, gigantic in its size, and horrible in its form. The preju- dice about spectres and hobgoblins, therefore, in some degree originates from nature, and such vi- sionary objects depend not entirely on the imagi- nation alone, as has been frequent!) supposed. If room would permit, it would be a pleasing employment to point out many advantages which arise from the form, the size, ihe motion, and the situation of the Eye, each of which haa a tendency to evince the wisdom and goodness of the Omnipo- tent Creator. But this has been well done by Dr. Derham and Dr. Paley; to whose works I must refer you. The celebrated Euler, in his " Letters to a German Princtss," points out an astonishing difference between tht human Eye, and any arti- ficial eye which can be constructed : he then makes some admirable reflections, part of which I now lay before you. " The Eye which the Creator has *l formed, is subject to no one of all the imperfec- " tions under which the imaginary construction of 61 the free thinker labours. In this we discover the .*' true reason, why Infinite Wissdom has employed " several transparent substances in the formation " of the Eye : it is thereby secured against all the f( defects which characterize every work of man. «* What a noble subject of contemplation ' He who " formed the Eye, shall he not see ? and he who "planted the ear, shall he not hear? The Eye " alone being a master-piece that far transcends •ts the human understanding, what an exalted idea " must Lesson xxxvii.] THE EYE. 285 " must we form of Him, who has bestowed this " wonderful gift, and in the highest perfection, not " on man only, but on the brute creation, nay, " on the vilest of insects !" Indeed, if we do but reflect upon the many diver- sified and beautiful scenes which are made visible to us by means of the organ of Sight, and consider the deplorable state, and the many inconveniences those persons lie under, who are deprived of this blessing, our hearts ought to overflow with thank- fulness to that kind BEING who has bestowed so useful an instrument as the Eye upon us, to add to our convenience and delight j and whose superin- tendency protects it from those injuries to which ii is continually exposed. LESSON LESSON XXXVIII. ON CONCOCTION. -The concoctivc powers, with various ait, Subdue the cruder aliments to chyle ; The chyle to blood ; the foamy purple tide To liquors, which thro' finer arteries To different parts their winding course pursue. AKMSTKONG. AMONG all the wise contrivances observed in the human fabric, none can excite our attention and admiration more than the disposition and me- chanism of those parts, by which our aliment is concocted, or fitted for our daily support and nou- rishment. To have a clear idea of the manner in which Concoction is performed, we must distinguish it into three stages : the first of which is performed in the progress of the aliment from the mouth down to the lacteals; which are vessels that receive the chyle from the intestines ; the second is per- formed in the passage of the milky liquor called chyle, through the lacteal vessels to the loins, and then up under the collar bone, where it mingles with the blood : the third, or ultimate stage of Concoction, is performed by the. circulation of the blood and chyle together through the lungs, and the whole arterial system. In all these stages the Lesson xxxvin.j CONCOCTION; 287 the design of the SUPREME CONTRIVER has evidently been to grind and dissolve the aliment, and to incorporate it with a large quantity of animal juices already prepared, in such a manner as to reduce it at last to the very same substance with our blood and humours. • How wonderfully and completely this design has been executed, my young readers will presently be able to judge. In the first stage of Concoction, by a curious configuration of parts, and action of muscles, adapted to their respective functions, our food is ground small by the teeth, and moistened by a copious saliva in the mouth. It is in the next place swallowed, and conveyed down the gullet, where it is farther mollified and lubricated by a viscid unctuous humour, distilled from the glands of that canal. From thence it slips into the stomach, where several causes concur towards its complete dissolution. It is diluted by the juices, swelled and subtilized by the internal air, and it is macerated and dissolved by iheheat which it meets with in the cavity, ft is also agitated and attenu- ated by the perpetual friction of the coats of the stomach, and the pulsation of the arteries there; by the alternate -elevation and depression of the diaphragm or midriff in breathing; and hy the compression of the strong muscles of the belly. After a proper stay, it is gradually propelled into the intestines, in- the form pf a thick, smooth, uniform, ash-coloured fluid. When our aliment, thus prepared, arrives at the intestines,, it is there mixed with three different sorts •288 CONCOCTION. [Lesson xxxvn T- ' ' ' — =f= sorts of liquors. It receives two kinds of bile the one, thick, yellow, and extremely bitter, from the gall-bladder; the other, scarcely bitter, or yel- low, but in a much larger quantity, from the liver. The third liquor that falls here upon the food, issues plentifully from a large glandular substance, called the Pancreas or sweet-bread, and is a limpid mild fluid, like the saliva, which serves to dilute and sweeten what may be too thick and acrimo- nious. The two saponaceous biles resolve and attenuate viscid substances; incorporate oily fluids with aqueous ones, making the whole mixture homogeneous ; and by their penetrating and deter- gent qualities render the chyle fit to enter the lacteal veins, into which it is conveyed, partly by their absorbent nature, and partly by the peristaltic motion of the intestines. If we now consider the change which our ali- ment has undergone, in the mouth, gullet, and stomach, together with the large quantity of bile, and pancreatic juice poured upon it in the intes- tines : and if we reflect also on the incessant ac- tion of the muscles, blending, churning, and incorporating the whole, we shall readily perceive that their united agency must alter the flavours and properties of the different kinds of food, in such a manner as to bring the chyle nearer in its nature to our animal juices, than to the original substances from which it was formed. Our food, thus changed into chyle, constitutes the first stage of Concoction; and we shsll find the same assi- milation carried on through the second. Th« Wesson xxxvin.] CONCOCTIOX. 23f The next stage begins with the slender lacteat veins, where they arise from the intestines by an innumerable multitude of invisible pores, through which the fine, while, fluid part of the chyle is strained or absorbed; while, at the same time, the gross, yellow,, fibrous part, conveyed slowly for- ward, and further attenuated in the long intestinal tube, 15 perpetually pressed and drained of its re- maining chyle, until the dregs, becoming at last useless, are ejected out of the body. These lacteal veins issue from the intestines in various directions, now. straight and then oblique, often uniting and growing larger, but presently separating again. They frequently meet at acute •angles, and enter into soft glands dispersed through the mesentery, from which they proceed larger than before, and more turgid, with a fine lymph- atic fluid : in most places also they run contiguous •to the mesenteric arteries, by whose pulsation their load is pushed forward. And thus, after various communications, separations, and protru- sions, the lacteal veins pour their chyle into a sort of cistern or reservoir formed for that purpose, between the lowest portion of the diaphaygm and highest vertebre of the loins. It is very remark- able, that these veins are furnished with proper valves, which permit the chyle to move forward, but effectually stop its return j and that a great number of veins purely lymphatic, as well as the lacteal ones, empty themselves into the same cistern. In all this contrivance it is evident^ that the <» chyle CONCOCTION. [Lesson xxxvm.( cnyle, being more and more diluted and blended \viih abundance of lymph from the glands through which it passes, and from other sources, approaches still nearer to the nature of our animal juices, and consequently becomes more fit for nutrition. The chyle is pushed from its reservoir into a narrow transparent pipe, called the thoracic duct, which climbs in a perpendicular direction by the side of the back-bone, from the loins up to the collar-bone, and opens into the subclavian vein : where, by the peculiar arrangement of several small valves, the chyle mingles gently with the blood after it has been thoroughly elaborated ; and attenuated with lymph from every part of the thorax, or great cavity of the breast, and is from thence soon conveyed to the heart. Thus we may perceive, that by a wonderful me- chanism, a large quantity of chyle and lymph is forced upwards, in a perpendicular course, through a thin slender pipe ; but lo render this more plain, the following pariiculars must be attended to: — First, to the progress of the chyle, urged forward and continued from the ante edent action of the intestines, and the beating of the mesenteric arte- ries. Secondly, to the motion of the diaphragm and lungs, in respiration, pressing the thoracic duct that lies under them, whilst the thorax, rising and falling:, resists their action, whereby the duct is squeezed between two contrary forces, and the liquor which it contains pushed upwards. Thirdly, this duct runs close by the side of the great artery (called by anatomists, the superior portion of the descending Lesson xxxvm.] CONCOCTION. 291 descending aorta) whose strong pulsation presses its yielding sides, and compels the chyle and lymph to mount in an upright ascent. Fourthly, it must be observed, that this duct is accommodated with valves, which permit its contents to move upwards by every compression, hut never to fall back again. Thus terminates the second stage of Concoc- tion, when the chyle falls into the heart. And it may be seen that in the progress through these two stages, our aliment has been mixed accurately with all the nourishing juices and with all the sub- stances or principles which compose the blood, viz. saliva, mucus, lymph, bile, water, salts, oil, and spirits. But here it will be proper to take notice, that .he most fluid and subtile parts of our aliment, before and after it is elaborated into chyle, pass into the blood by certain absorbent veins dispersed all over the mouth, gullet, stomach, and intestines: when we consider how quickly refreshment and strength are communicated to weary, faint, and hungry people, immediately upon drinking a glass of good wine, or eating any cordial spoon-meat, this remark will appear ihe more obvious. The thiid stage begins where ihe chyle mingles with the blood, and, falling soon in;o the right ven- tricle of the heart, is from thence propelled into the lungs. It will appear that the lungs are the principal instruments of converting the chyle into the blood ; especially if we consider their struc- ture, first with regard to the air-vessels of which they are composed, and secondly with regard to o 3 their CONCOCTION. [Lesson xxrvni. their blood-vessels : for we shall then clearly per- ceive the change which their fabric and actjon. must produce on the chyle. The windpipe is composed of segments of car- tilaginous rings on the fore part, to giv.e a free passage to the air in respiration j and of a strong membrane on its back part, to bend with the neck, and give way to the gullet in deglutition. This pipe is lined throughout with an infinity of glands, which perpetually distil an unctuous dense humour to lubricate and anoint the passages of the air. Soon after the windpipe has descendecl into the cavity of the breast, it is divided into two great branches ; and these two are subdivided into innumerable ramifications called bronchia, which become smaller in their progress (not much unlike a bushy tree inverted), until at last they ter- minate in millions of Jittle bladders which hang in clusters at their extremities, and are inflated by their admission of air, and subside at its ex- pulsion. The plusters constitute the lobes of the lungs, The blood-vessels of the lungs next deserve^ur attention. The branches of the pulmonary artery run along with those of the windpipe, and are ul- timately subdivided into an endle.ss number of capillary ramifications, which are spread, like a fine net work, over the surface of every individual air- bladder ; and the pulmonary vein, whose extreme branches receive the blood and chyle from those of the arteries, run likewise in form of a net over all the air-bladders of the brpnchia. From Lesson xxxvm.] CONCOCTION. From this admirable structure of the lungs, it is obvious, that the crude mixture of the blood and chyle, passing through the minute ramifications o£ the pulmonary artery and vein, is compressed and ground by two contrary forces, viz. by that of the heart^ driving the mixture forward against the sides of the bronchia and air-bladders; and by the elastic force of the air equally repelling this mixture from the contrary side. By these two opposite forces the chyle and blood are more intimately blended and incorporated 5 and by the admission and expulsion of the air in respiration, the vessels are alternately inflated and compressed (and probably some subtile air of aether is received into the blood) by which means the mixture is still farther attenuated and dis- solved; and after various circulations through the lungs and heart, and the whole arterial system, is at last perfectly assimilated with the blood, being fitted to nourish the body, and answer the different purposes of animal life. When the blood thus prepared from the aliment, is, by repeated circulations, gradually drained of all its bland and useful parts, and begins to acquire too great a degree of acrimony, it is carried oft' by both sensible and insensible evacuations, through the several channels and distributions of nature. By these evacuations the body is made languid, and requires a fresh supply of aliment; while at the same time the saliva, and juices of the sto- mach and intestines, becoming thin and acrid by multiplied circulations, vellicate the nerves of © 3 thos 29* CONCOCTION'. [Lesson xxxvin those passages, and excite hunger, as a faithfi monitor, to remind us of that refreshment which is now become necessary. And here I close my account of the process of Concoction ; in the consideration of which the young reader will find abundant cause for astonishment and ad- miration. LESSON LESSON XXXIX. ON THE CIRCULATION OF THE BLOOD. The Blood, the fountain whence the spirits flow ; The pen'rous stream that waters ev'ry part, And motion, vigour, and warm life conveys To tv'ry particle that moves or lives. ARMSTRONG. 1 HOUGH it be common to talk familiarly of the Circulation of the Bloody yet perhaps very few of my young readers are well acquainted with it : I shall therefore appropriate this Lesson to the purpose of giving them a brief, though I hope in- .telligible, description of the manner in which the Circulation is performed. This important secret was brought to light by William Harvey, an Eng- lish physician, a little before the year 1600: and when it is considered thoroughly, it will appear to be one of the most stupendous works of matchless To form a distinct judgment of the mechanism and importance of the Circulation, it will be necessary to describe the structure of the arteries, veins, and nerves ; and take notice of some expe- riments made upon them; and then must be con- o 4 sidered CIRCULATION [Lesson xxxix. sidered the cavities of the heart, by means of which the Blood is propelled through the body. To these I now proceed. The arteries are blood-vessels consisting of a close texture of strong elastic fibres, woven in rarious webs, laid in different directions, and inter- spersed with an infinity of delicate nerves, veins, and minuter arteries. They are divided and sub- divi^jd into numberless branches and ramifica- tions, that become smaller and smaller as they recede from the heart, until at last their extremi- ties are found much more slender than the hairs of our heads, (and are therefore called capillary arteries), which either unite in continued pipes with the beginnings of the veins, or terminate in •mall receptacles, from which the veins derive their origin. The arteries have ,no valves, but only have their trunks spring from the heart : they throb and beat perpetually whilst life remains j their extremities differing in the thickness of their coats and some other particulars, according to the nature of the part which they pervade. All the arteries in the lungs (except the small ones that convey nourishment to them) are derived from the great pulmonary artery, which issues from the right ventricle of the heart. And all the arteries in the rest of the body proceed from the aorta, (which obtained this name, because the ancients thought it contained air only), whose trunk springs from the left ventricle of the heart. The veins resemble the arteries in their figure and distribution $ but their cavities are larger, and thier Lesson xxxix.] OF THE BLOOD. 29-7 their bnmches, perhaps, more numerous. Their coats are much weaker and more slender than those of the arteries. They are furnished with several vdlves, contrived in such a manner as to permit the Blood 10 pass freely from the smaller into the larger branches, but to stop its retrogres- sion. They neither throb nor beat. Their begin- nings form continued pipes with the extremities of the arteries, or arise horn some gland or recep- tacle where the arteries terminate. All the veins in the lungs, from their capillary beginnings grow- ing still larger, unite at last and dischaige their Blood into the left auricle of the heart: and all those in the rest of the body empty themselves in like manner, into the vena cava, which opens into the right auricle of the heart. The nerves deduce their origin from the brain, or its appendages, in several pairs, ofacylindric form, (like so many skeins of thread with their respective sheaths;, which in their progress de- crease by endless divisions and subdivisions, until at last they spread themselves into a texture of filaments, so slender, and so closely interwoven with each other over the whole body, that the point of a needle can hardly be put upon any part of it, without touching the delicate branch of some nerve. It has been found by many trials, that when an artery is laid bare, and a ligature made upon it, if it be opened with a lancet between the ligature and the heart, the Blood will rush out with great •violence j and a rapid, jerking stream will coa- O 5 298 CIRCULATION. [Lesson xxxix. tinue (if it be not stopped by art) until, through loss of Blood, the animal faints or dies. But if the same artery be opened between the ligature and extremities, a few drops only will ooze out from the wounded coats. On the other hand, when a vein is laid bare, and a ligature made upon it, if it be opened be- tween the ligature and the extremities, the Blood will gush out, as we see in common venesection. But if the same vein be opened between the bind- ing and the heart, no Blood will appear. From these experiments it is obvious to the slightest attention, that the Blood flows from the heart, through the arteries, to the extreme parts of the body; and returns again through the veins to the heart.' For the regular performance and continuation of this motion of the Blood through all the dif- ferent parts of the body, the heart, which is the primitm mobile, giving the first impulse, is fur- nished with four distinct muscular cavities, that is, with an auricle and a ventricle on the right side, and an auricle and a ventricle on the left. Through these cavities, curiously adapted to their * respective offices, the Blood circulates in the fol- lowing order : — it is received from the veins, first into the right auricle, which, contracting itself, pushes the Blood into the right ventricle at that instant dilated. The moment this ventricle is filled, it contracts itself with great force, and im- pels the Blood into the pulmonary artery, which passing through the lungs, and returning by the pulmonary Lesson xxxix.] OF THE BLOOD. 299 pulmonary veins, is received into the left auricle of the heart, and from thence it is pushed into the left ventricle 5 which, being thus filled, con- tracts itself, and drives the Blood with great rapi- dity to all the parts of the body, and from them it returns again through the veins into the right auricle of the heart, as before. It is very remarkable, that we have here a dou- ble Circulation : one, from the right ventricle, through the lungs, to the left auricle of the heart, in order to convert the chyle into Blood, and finally prepare it for the nourishment of the ani- mal ; the other, from the left ventricle, through the whole body, to the right auricle of the heart, which serves to apply that nourishment to every part, besides various other purposes. But to proceed — Of these four muscular cavi- ties, the two auricles are contracted at the same instant, while the two ventricles are dilated j the ventricles, in their turn, are contracting them- selves at the very instant that the auricles are di- lating. The arteries, in like .manner, beat in alternate time with the ventricles of the heart. The nerves, as well as the veins and arteries, act their part in this rotation of the Blood; for if the eighth pair of nerves which proceeds from the brain to the heart be bound up, the motion of the heart immediately languishes, and soon ceases entirely. Thus we have a species of perpetual motion, •which none but a Being of infinite wisdom and power 300 CIRCULATION [Lesson xx xix power could produce j yet whose continuation requires the constant aid of the same hand that first gave it existence. The brain transmits ani- mal spirits to the heart, to give it a vigorous con- traction. The heart, at the same time, pushes the Blood into the brain to supply it with new spirits; by which means the head and the heart give continual mutual support to each other. But this is not all ; the action of the heart sends the Blood and other vital humours over the whole body by the arteries, and distributes nourishment and rigour to every part (while perhaps the animal spirits, from the extremities of the nerves, return again into the Blood), and the whole refluent mass is conveyed back through the veins into the heart, which enables it, without intermission, to persi&t in rolling this tide of li/e. But here it must not be supposed, that the arte- ries pass on to the extremities of the limbs, before they communicate wivh the returning veins : for upon this supposition, after an amputation has been performed, whatever Blood might be brought to the stump by the arteries, it is certain, none of it could be carried back again to ihe heart; be- cause the intercourse between the heart and the limbs would, in this case, be entirely cut off. But the all-wise AUTHOR of our being has provided for this exigency, by forming a great number of less branches from the larger arteries, which constantly communicate with corresponding branches of the r«turning veins. And hence, it is easy to conceive Lesson xxxix.] OF THE BLOOD. 30-1 conceive how the Circulation is carried on after amputation has been performed*. From what little has been advanced in this and the two preceding Lessons, the unprejudiced young reader will rind a striking di-play of the wisdom and goodness of our CKEATOR. To those who still hold to the negation of such a Being, I scarce- ly know what to say: for thev who live, move, think, and act, must be left without excuse, if they deny or forget GOD, or refuse to honour or be thankful to "him. Those who withstand the evi- dence of the works of nature, when properly ob- served, are not likely to be convinced by rational deductions ; but will probably continue infidels (unless their hearts be changed by Divine Grace) untH they are convinced of their fatal mistake, by experiencing the indignation of that ALMIGHTY B. ING, whose existence they have so impiously denied. * But this, I sincerely hope, will not be the case with any of the youthful perusers of these Lessons. However, in this sceptical age, when every part of Divine Truth is questioned, opposed, and, alas ! too frequently holden in derision, it becomes us to be * With respect to the velocity of the circulating Blood, and the time in which the whole quantity thereof has undergone a complete circulation; although several computations have been made, the matter is not decisively settled. Dr. Jurin and Dr. Keill have most distinguished themselves in inquiries of this nature; but they are far from agreeing in their con- clusions. The substance of their calculations and experi- ments may be seen in Dr. Reel's improved edition of CHAM- CYCLOPAEDIA, under the articles Blood and Heart. wary j •302 CIRCULATION, &.c, [Lesson xxxix. wary j and not only so, but to join in a general endeavour to persuade those who are deflating from the true path, speedily to return thereto. Come! all ye nations ! bless the LORD, To him your grateful homage pay : Your voices raise with one accord, JEHOVAH'S praises to display. From clay our complex frames he moulds. And succours us in time of need : Like sheep when wandering from their folds He calls us back, and does us feed. Then through the world let's shout his praise, Ten thousand million tongues sliould join, To Heaven their thankful incense raise, And sound their MAKER'S love divine. When rolling years have ceas'd their rounds, Yet shall his goodness onward tend : For his great mercy has no bounds; His truth and love shall never end ! LESSON LESSON XL. CONCLUDING REMARKS AND ADVICE. Ye guardian Powers! who make mankind your care, Give me to know wise Nature's hidden depths, Trace each mysterious cause, with judgment read Th' expanded Volume, and submiss adore That great creative. VV ill, who at a word Spoke forth this wondrous scene. SOMERVILLE. WHEN we consider the contracted and confined nature of human knowledge, even in its present improved state, we must not anticipate to our- selves the pleasure of obtaining such a degree of philosophic skill, as is described in the above- cited lines of the poet : for it may be recollected that, when endeavouring to elucidate the causes of some of the grand phenomena of nature, we more fre- quently proceeded upon conjecture ami hypotheses than upon any real and permanent foundation. However, though this be admitted, it need not be thence concluded that we should be entirely inat- tentive to philosophic speculations: for contempla- tions of this kind, when properly regulated, have a 304 CONCLUDING ADVICE. [LeSSQH XL. a tendency to correct wrong ppinions, which we might otherwise entertain of the wisdom and goodness of that BEING who created the uni- verse. It is in conformity to this sentiment, that I have, in the foregoing Lessons, attempted to describe to you the nature and supposed causes of some few of the numerous objects and appearances in crea- tion: and I hope that, even from the descriptions which I have given, faint and imperfect as they must be acknowledged to be, I shall be justified in adopting the language of Mr. Cotes, when he says, " That man must be blind, who from the most *' wise and excellent disposal of things, cannot " immediately perceive tke infinite wisdom and " goodness of tbf Almighty Creator; and he " must be mad, svho refuses to acknowledge « them." I have, in the course of these Lessons, fre- quently referred you to such works of eminent writers, as may be consulted with advantage : I shall now, previous to drawing a conclusion, men- tion some other authors in whose works you may meet with more information; not only on the subjects treated upon in this performance, but oa several,, which the narrow limits I am confined to have hindered me from even mentioning. On Anatomy, I would recommend 'he works of Borellif Harvey, Hunter., Jurin, Keill, Motherby, Monro, and Nieuuuentyt. On Astronomical sub- jects, Bonny castle 3 Bryan^ Emerson, Fergusvn Gregory Lessen XL.]' CONCLUDING ADVICE. 305 Gregory, Ktill, Long, Maskelyne, Vince, and Wales, are writers of distinguished reputation. The best writers on Electricity, are Brooks, Caval- lo, Ferguson, Frank in, Morgan, and Priestley. On Optics, the performances of Harris, Martin, NKWTON, Smith, and Wood, will particularly merit your attention. Various other parts of Philosophy, or Natural Philosophy in general, may be found treated on, either in a popular or scientific way, in the works of Adams, Cavallb* Desaguliers, Emerson, Enfield, Ferguson, Gregory, Keill, Martin, Mariotte, NEWTON, Nicfiolsont Nieuiuentyt, Rowning, Rutherforth, and Ryland. There has also been lately issued into the world, a Dictionary, by my highly esteemed friend, Dr. Charles Hutton, in which abundant information; on astronomical, mathematical, and philosophical subjects may be met with. I would also recom- mend to your notice the periodical publications in which philosophical and mathematical questions are discussed: the principal of these are, the Ladies' Diary and Supplement, Gentleman's Diary, and Mathematical Repository $ besides monthly pro- ductions, several of which are worth notice. Nor tan I here omit pointing out, Maclaurins Piew oj Sir Isaac Newton's Phiosophical Discoveries; and, to those who are acquainted with th<^ French lannuage, the Traitc Elcmentaire de Physique, par M. R. J. Hauy, as works which will amply repay tlie student for any attention he ma\ pay them. And, since the author of a book commonly wishes it 306 CONCLUDING ADVICE. [Lesson XL. it to be read, and generally thinks it will be found worthy a perusal, it would be a mere affectation of modesty, were I not to recommend to the notice of my readers, the treatises on Astronomy and Mechanics advertised at the end of this volume. Finally, I must entreat my young readers early to imbibe correct religious principles*; for it is religion only that can regulate the heart, — it causes it to melt in sympathy at another's distress, or to glow with pleasure at another's happiness, — it is this alone that can harmonize the mind, " Attuning all its passions into peace." The astronomer, if enlightened by it, must con- template, with wonder and admiration, those lumi- naries on which his eye so often gazes with plea- sure. The philosopher too, when the wonders of nature are open to his view, with what adoration and gratitude must he look to that great Source . . from whence they flow ! Nay, in all professions how imperfect is man, unless illumined by the bright rays of Religion, which, like that glorious fountain of light, the sun, will enlighten all our paths. Let me beg of you, therefore, to study, with par- * " With the talents of an angel, a man may be a fool; if " he judge amiss in the supreme point, judging aright in all « else but aggravates his folly— as it shews him wrong, though " Llest with the best capacity of being right." DR. YOLIVG. ticular Lesson XL.] CONCLUDING ADVICF. 307 ticular attention, that much-negiected book the BIBLE; where energy of language, sublimity of sentiment, and the most exquisite beauties of oriental poetry, are among the least of its perfec- tions* ; from reading this book, and from con- templating the works of nature, we may learn that GOD is a supreme, eternal, self-existent, ne- cessary, and independent Being: that he is also invisible, immortal, incomprehensible, omnipotent, omniscient, omnipresent, ami supremely good. We may also thence deduce, that He manages the world in wisdom and goodness, and governs it in justice, truth, and holiness; that " not a sparrow " falls to the ground without HIM;" that " even * The Bible, on account of the precepts it contains, and the consolations which may be derived from it, is above all praise. But before it can be of advantage to a reader, he ought to be convinced of the truth of Revelation. Young persons should assent to the doctrines in this Divine Book ; not because they were born in a country where they have been told that they were true ; nor merely because they have been assented to, and defended, by very eminent men ; but because the evidences, accompanying the various parts of the volume, have CONVINCED them, that it has GOD for its author, TRUTH for its matter, and SALVATION for its end. I cannot help adding, that when youth make these evidences the subject of their pursuit, they should bear in mind a pre- cept, which ought always to accompany them when pursuing truth : namely, " As far as possible get rid of old prejudices, and watch continually against new ones." For more on this most interesting of all subjects, I trust the reader may advantageously consult my " Letters on the Evidences, Doctrines, and Duties of the Christian Reli. gion." "the 308 CONCLUDING ADVICE. [LeSSOH XL, " the hairs of our head are all numbered j" and that all second causes derive their origin, perma- nency, and efficacy from HIM alone. Since, then, THE LOKD GOD is himself the Source and Perfection of all beauty and excellency the Author of our existence, and the bountiful Giver of all good g'fts ; we undoubtedly ought to love him with our whole heart, and to serve him with all our powers ; we ought to reverence his majesty and authority, and endeavour above all things to obtain his favour} we ought to devote ourselves entirely to his service, and make all out actions tend to the advancement of his glory. And as his mercy.and goodness are unbounded, so , should be our gratitude and praise. JEHOVAH reigns : let ev'ry nation hear, And at his footstool bow with holy fear ; . Let heav n'^ high arches echo with his name, And the wide peopled earth his praise proclaim ; Then send it down to hell's deep gloom wsoundmg, Through all her caves in dreadful murmurs sounding. He rules with wide and absolute command, O'er the broad orean and the stedfast land : JEHOVAH reigns unbounded and alone, And all creation hangs beneath his throne : He reigus alone ; let no inferior nature Usurp or share the throne of the Creator. He saw the struggling beams of infant light Shoot lhron«h the massy gloom of ancient night j His Spirit hush'd the elemental strife, And brooded o'er the kindling seeds of life ; Seasons and months began the long procession, And ineasur'd o'«r the year IK bright succesnion. ThV coNctuDiNct ADVICE. The joyful sun sprung up th' ethereal way. Strong as a giant, as a bridegroom gay : And the pale moon diffus'd her shadowy light Superior o'er the dusky brow -of night ; Ten thousand glittering lamps the skies adorning, Numerous as dew-drop» from the wemb of morning. Earth's blooming face with rising flow'rs he dress'd, And spread a verdant mantle o'er her breast ; Then from the hollow of his hand he pours The circling waters round her winding shores,— The new-born world in their cool arms embracing, And with soft murmurs still her banks caressing. At lengthshe rose complete in finish'd pride, All fair and spotless like a vkgin bride ; Fresh with untai uish'd lustre as she stood, Her MAKER bless'd his work, and call'd it good ; The morning stars, with joyful acclamation, Exulting sung, and hail'd the new creation. Yet this fair world, the creature of a day, Though built by God's right hand, must pass away < And long oblivion creep o'er mortal things, The fate of empires, and the pride of kings .: Eternal night shall veil their proudest story, And drop the curtain o'er all human glory. The sun himself, with weary clouds opprest, Shall in his silent, dark pavilion rest; His golden urn shall broke and useless lie, Amidst the common ruins of the sky ! The stars rush headlong in the wild commotion, And bathe their glittering foreheads in the ocean. / But fix'd, O COD ! for .ever stands thy throne ; JEHOVAH reigns, a universe alone; Th' eternal fire that feeds each vital flame, Collected or diffused is still the same, He dwells within his own nnfathom'd essence, Aujl fills all space with his unbounded presence. , But CONCLUDING ADVICE. [LtiSSIM Xf.. But oh ! our highest notes the theme debase, Ari'd silence is our least injurious praise : Cease, cease your songs, the daring flight controul, — Revere him in the stillness of the soul j With silent duty meekly bend before him, And deep within your inmost hearts — adore him. MRS. BA.RBAULU, APPENDIX APPENDIX CONTAINING SOME ADDITIONAL REMARKS ON HEAT, COLD, AND LIGHT. J HERE is but little probability of our arriving at any great degree of accuracy in our opinions con- cerning these subjects, if in our reasonings upon them we only consider them separately j for there are several cases in which they have a dependence upon each other, which can only be tracrd out by considering them together. To answer this pur- pose, the following pages are written. As in the course of our discussion, the degrees of heat and cold will be spoken of, it appears ne- cessary to premise a little with regard to the instru- ment by which they are. usually (though not always) measured. This instrument is called a thermo- meter : to describe it with a nice particularity is not requisite, since more may be learnt from five minutes' examination of one, than could be ga- thered from a description which micht fill half a dozen pages. In order that thermometers of dif- ferent sizes may produce exactly the same conr chmon in determining the heat or cold of bodies applied • 12 APPENDIX. applied thereto, it is necessary to fix upon two certain points at some distance, of each of which we can judge by unvarying criteria. These ii Fahrenheit's Tliermometer (the one most generally used in England) are the boiling and freezing points of water. With regard to the former of these, it should be recollected as observed in the Twenty-ninth Lesson, that the degree of heat at which water bolls, is varied by the difference4 of the pressure of the atmosphere. The boiling heat is therefore taken at some certain degree of pres- sure : the degree now used is such as makes the mercury in a barometer stand at 29| inches. As to the latter of these points, it does not appear to be a proper criterion ; or at least, if it be, it has a wrong name affixed to it ; for it is well known that,' though fluids always thaw at the same de- gree of heat, yet the degree at which they freeze is liable to be varied with circumstances. It would therefore be better, if in future this latter point wene :laid aside^ and instead thereof the thawing point made use of. The different degrees of heat and cold are gene- rally estimated by their distance either above or below the, freezing point. Those above may be denoted by the affirmative sign : those below by the negative one ; though sometimes the words at length are used ; and at others, the expressions alove or below nothing are made use of j but this latter method seems somewhat absurd. Those who purchase thermometers ready made should pay particular attention to the tube and corresponding HEAT, COLD, AND LIGHT. 313 corresponding divisions : it is frequently found that the tubes, instead of being cylindrical, are smallest in the middle, and widen gradually to- wards each end, like two conic frustrums joined at their less bases. When this is the case, it is proper that the divisions, instead of being equal, should be longest in the middle, and decrease by regular gradations toward each end, so that the cavity in the tube shall contain the same quantity of fluid between every two division!. We now proceed to the more immediate objects of this Appendix, namely, Heat, Cold, and Light: The two latter of these will not be considered very attentively; only as they are connected with the former, which will be handled more at large. Heat and Cold are to be considered either as particular sensations, or as the causes of powers which bodies possess of exciting those sensations. Thus, we say that we ourselves are hot or cold, and that the fire or ice which heats or cools us is likewise hot or cold : though the sensations we experience are certainly very different things from that which enables those bodies to excite them. It must be observed that the sensations of Heat and Cold are very fallacious ones, in so far as they are effected by the temperature of the body in which they are excited : for we may feel a sub- stance hot when it is in the same circumstances in which we should feel it cool at another time. To elucidate this, we may observe that when we have been accustomed to live in an atmosphere of be- twixt 4- 60? and + 70°, if the Heat fall to + 60? p \vc 314 APPENDIX. we feel it cold : but, on the contrary, if we have lived in an atmosphere of between. + 40" and -}- 5O°, if the Heat rise to -f- 6()u we feel it very hot. Again, let two basons of water be taken, one heated only to -f- 35°. the other to -f- no°, and put one hand into the one, the other into the other bason, for some time: if we then immerse both hands in water 'heated to + 60Q} we shall with one hand feel this Cold, with the other Hot. Hence it may be reasonably inferred, that we can- not judge with precision of Heat or Cold by the Sensations they excite in us. In the next place, we are to consider Heat and Cold as the cause of powers which bodies possess of exciting particular sensations. As to Cold, it Is seldom supposed to be either matter itself or a quality: it is more commonly looked upon as a deprivation of Heat ; for the less the heat, found in a body, the greater the Cold, and vice versa. — There are particular cases in which Cold may be produced. i. When some particular chemical attraction takes place, Cold is produced. 2. The conversion of solids into liquids, and of liquids into vapour, produces Cold, as is shewn by chemists. And 3. Cold may be produced by animal powers. It is not intended to relate experiments by which these may be proved : but the grand question which we most wish to determine, is, with respect to Heat, whether it be matter under some parti- cular form, or only a quality. That our reason- ings on this important subject may have the better *ffect, we must first reflect upon the various means of HEAT, COLD, AND LIGHT. 315 of producing Heat. There are several ways by which Heat may be generated. 1. By means of the sun's rays. 2. By exciting vibrations in solids. 3. By the taking place of certain chemical attractions. 4. By conversion of vapours into fluids, and of fluids into solids. 5. By animal powers. 6. In volcanos. And first, if a cold body be exposed to the rays of the sun, it will be heated. It has been frequently conjectured that the sun is fire, burning and heating ocher bodies in like manner as a culinary fire: but the celebrated Dr. Fordyce has asserted, that the sun is probably not at all hot in itself; neither are the solar rays hot, but have only a power of producing Heat on being applied to other bodies. An opinion very little different from this is also entertained by Dr. tVil- liam Herschel, and supported with the authority of demonstration. As a farther consideration of this subject may tend to correct our notions con- cerning Light, it is here attempted. It is a constant rule, with regard to hot bodies that they heat ail colder bodies which are brought near them. Though it must be allowed (as will b« hereafter seen) that some bodies will receive Heat with more readiness than others: however, thi* will not easily form an objection to what imme- diately follows. Now, if we take a 'large burning glass, and hold a piece of iron in its focus, such Heat will be pro- duced as to melt the iron. But the glass through which all the rays passed is scarcely heated at all : and when they fell on the iron they were n.Q hotter pg than 31$ APPENDIX. than water when it is poured on vitriolic acid* But if we place water j which is perfectly transpa- rent, in the focus, no heat will be produced : nay, if spirits of wine were placed in the focus, they would scarcely be heaied. But the same Heat which melts iron, would more than suffice to make water boil. From this experiment, then, without advancing farther arguments, it appears that the rays in themselves have no Heat ; and there is no reason to suppose that the sun is hotter than the earth we inhabit. It is a question that has been much agitated, whether the solar rays be matter, or only an ar- rangement of matter; but their materiality is now pretty generally admitted: but a question which has not yet been answered satisfactorily, is, " If f* Light be matter, what becomes of it ? " Perhaps there is a distinction between Light and the solar rays, which has not yet been properly attended to. The sun's rays heat bodies only when they are lent or destroyed. (The term absorbed does«not in our opinion exactly answer the purpose.) Hence they do not heat water if perfectly transparent ; neither do they heat the air above the clouds: at least, as very little bending takes place in these cases, the heat is so trifling as to be scarcely worth mentioning. The upper regions of the air, then, are extremely cold, though exposed to the direct action of the sun. When a ray of Light is reflected, it does not touch the body reflecting it; but is thrown back before it arrives at the surface : therefore the more white HEAT, COLD, AND LIGHT. 317 white bodies are, or the more highly they are polished, the less they are heated, because they reflect more of the rays : and when a body is per- fectly white it reflects all the light, and is not heated at all. Bodies, in proportion as they deviate from whitea destroy the more solar rays, and a perfectly black ?Jody would destroy them all : hence bodies are more heated, ccet. par. as they are darker coloured, by this cause of Heat. When a body is rough, asi f we make a piece of glass so (which may have no colour) it destroys part of the rays, or, at least, suffers them to ap- proach' so near its surface before it reflects thein that they cause it to be heated. Thus far our reasonings induce us to suppose that Heat i8 a quality: but Heat, as a quality, cannot exist without a substance to exist in. So that, if it were possible to produce a perfect va- cuum, there could be no Heat therein. This also leads us to conclude, that tiie denser a body is, the more Heat may be therein produced ; other circumstances being: the same. Heai, it is affirmed, can only be produced by the solar rays at the surfaces of bodies : conse- quently the interior parts can only be heated by communication. And if we ketp in mind that Heat is more rtadily transmitted, communicated, and received, by some bodies than others ; it will then appear that, as a' body receives Heat with. more facility, it will be the mere heated by the sun's 318 APPENDIX. sun's rays ; as a piece of iron will be more heated than a piece of wood. We have seen, then, — that the solar rays are not hot in themselves, — that they produce Heat only when they are bent or destroyed, — that therefore they do not heat transparent bodies, nor do they heat in passing through them, but only at tha» entrance and passing out again. It is evident^ since the rays of the sun have a power of producing Heat, that they will heat a .body more, the greater the quantity is that falls on it. From this principle, combined with some particular circumstances, arises the different Heat and Cold of the seasons, and of the different parts of the earth. For instance, the Heat about the equator has been known to arise to -f- 1 10° : and it is said, that the Cold in Siberia has been as low as + 160°; but the accuracy of this may be doubted, for I do not see how so great a degree of Cold can be precisely measured. The Heat produced by the solar rays is increased also by reflection of them : if they be frequently reflected, a greater Heat is produced than even if they be all destroyed. Thus we find that, if we re- ceive them into a box so constructed as to reflect them frequently from side to side, more Heat will be produced than in a box made black, so as to destroy them almost all. Hence, in vallies, even in temperate climates, where the rays are reflected frequently, very great Heal is also produced. The different distances of the planets from the sun. MEAT, COLD, AND LIGHT. sun, it is imagined, makes a great difference in the number of the rays and in the momentum with which they fall on them. So that it has been. thought that Mercury is exceedingly hot, and Georgium Sidus cold beyond conception : but since the Heat produced in- bodies depends on their disposition to receive it, the several planets may be so composed as to- have but a very trifling difference in the Heat produced by the solar rays. Hence, then, what has been hitherto said concern- ing the Heat of the planets as calculated on the -supposition of the sun being the source of Heat, may be called in question : and, perhaps the New- tonian opinion concerning comets (recited in the astronomical part of this work) may in time be entirely abandoned, and some later hypothesis become generally received. Thus much for the first method of producing Heat. The next method of producing Heat is by ex- citing vibration in solids. Whether fluids can be thus heated, we do not know : there is no clear instance of Heat being produced by their vibration. We may excite vibration in solids, by friction or by collision. If we rub together or strike two bodies, if they have any elasticity they will vibrate. The rougher bodies are which are rubbed together, the greater vibration is produced, and therefore the greater heat. The vibration is also, cat. par. in proportion to the elasticity of bodies. Li Count Rumford's ninth Essay, which is an inquiry 3*0 APPENDIX. inquiry into the source of the Heat that is excited by friction, many interesting experiments are re- lated. From these experiments it appears, that sufficient Heat was produced by the friction of two metallic surfaces (when the access of atmosphe- rical air was entirely prevented) to make water actually boil. It appeared that a very considerable .quantity of Heat was excited by the friction, and given off in a constant stream in all directions^ without interruption or intermission, and without any signs of diminution or exhaustion. This ingenious philosopher, when reasoning on these experiments, gives satisfactory reasons to prove that the Heat could not be furnished either by the air, or by the water which surrounded the machinery. And, considering that the source of the Heat generated in these experiments, appeared evidently to be inexhaustible, he naturally con- cluded, that Heal could not be matter: for, says he, " It is hardly necessary to add, that any thing «* which any insulated body, or system of bodies, ft can continue to furnish without limitation, can- "-not possibly le a material substance." Another method of producing Heat is by the taking place of chemical attractions. Every che- mical attraction, as far as we know, in taking place, produces either Heat or Cold : whether it be simple combination, elective attraction, or com- pound elective attraction. Some of the chemical attractions are attended, besides the production of Heat, with another striking phenomenon, namely, HEAT, COLD, AND LIGHT. 321 namely, the producing of Light. For instance, this is produced by the combination of resp. air with phlogiston; and other instances might be adduced. This strikes out an interesting subject of philosophical inquiry. The fourth and fifth methods of producing Ileat might be descanted upon very copiously j but perhaps this would have but little tendency to- wards determining what Heat is. Lastly, Heat is produced in volcanos. This has commonly been supposed to be by burning of fuel. But it is evident that it cannot be produced by this cause, or by any other known means of the production of Heat. The burning of fuel, it is known, destroys a proportionate quantity of air : to produce a very great degree of Heat requires (till more to be applied than is naturally combined with phlogiston. Now the whole island Santalina is a mass of iron ore very difficult of fusion, which was fused and thrown up from the bottorn, of the sea in the midst betwixt two shore?, by this Heat ; where no air could therefore possibly come. And if it could, it would have required more in quantity than would have exhausted the whole atmosphere, to animate fuel enough to have pro- duced the Heat. In Friesland, some time ago, there was a tract of country 100 miles across, the whole of which (wiih men, animals, trees, and whatever was on it) was melted into one common mass. This Heat then cannot be produced by the burning of fuel ; much less can it be by the decomposition of pyrites, which is indeed the burning 322 APPENDIX. burning of sulphur. And by what means such intense Heat is produced, we are at a loss to de- termine. Having spoken of the various methods of pro- ducing Heat, we must next observe, that bodies may be heated by communication. And several experiments might be described to shew, that some bodies will both communicate and receive Heat more readily than, others. It is the same with re- spect to Cold as to heat : for those bodies which receive Heat most readily, most readily part with it ; and if they do this, they must also suffer it to pass through them (speaking of it as though it were a body) from one substance to another, or •onduct it most readily, and vice versa. Iron is a good conductor of Heat : on the con- trary, wood is one of the best non-conductors of Heat known. That the former is a conductor, and' the lattera non-conductor, of Heat, is evident from the following simple experiment; if you take a nail or a small piece of iron, and hold in the flame of a fire or candle,, it will speedily become so hot all over, as to oblige you to relinquish your hold ; but if you take a small piece of wood and hold in the flame, you may keep hold of it till it is nearly all consumed by the fire, without being incommoded by the heat of the wood. Hence heat passes with case in iron, and with difficulty in wood. From the results of various experiments, Count Rumjord * concludes that water , oil, mercury, and * In the Essays of this philosopher, very ingenious princi- ples are applied to practical uses in the great art qf living. That my HEAT, COLD, AN7D LIGHT. 32.T and air, are non-conductors of Heat : indeed, he thinks it essential to all fluids, that they should be non- conductors my young readers may have an idea of the advantages which aiay arise, from applying philosophical- principles to s«eh purposes, I present them with the following extracts :— In Essay VI. the Count says, " Among all the various " substances of which coverings may be formed for confining" " Heat none can be applied with greater advantage than at- " mospheric air. It is what Nature employs for that purpose ; " and we cannot do better than imitate her. " The warmth of tke wool and fur of beasts, and of the fea- " thers of birds, is undoubtedly owing to the air in their in- " terstices ; which air, being strongly attracted by these " substances, is confined, and forms a barrier, which not only " prevents the cold winds from approaching the body of th« " animal, but which opposes an almost insurmountable ob- " stacle to the escape of the Heat of the animalinto the at- " mosphere. And in the same manner, the air in snow serves u to preserve the Heat of the earth in wioter. The warmth, 44 of all kinds of artificial clothing may be shewn to depend " on the same cause ; and were this circumstance more ge- " nerally known, and more attended to, very important im- " provemeuts in the management of Heat could not fail to " result from it. A great part of our lives is spent in guard- " ing against the extremes of Heat and of Cold, and in ope- " rations in which the use of Fire is indispensable ; and yet " how little progress has been made in that most useful and " most important of the Arts — the management of Heat! " Double windows have been in use many years in most of " the northern parts of Europe, and their great utility, in * rendering the houses furnished with them warm and com- " fortable in winter, is universally acknowledged, — but I " have never heard that any body has thought of employing l< them in hot countries to keep their apartments cool in sum- " mer;— yet how easy and natural is this application of so "simple and so useful an invention! — If a double window " can prevent the Heat which is in a room from passing out. 334 APPENDIX. non-conductors of Heat ; or that all interchange and communication of Heat among their particles, as from one of them to the other, is absolutely impossible. Glass, when rendered of a loose tex- ture, conducts Heat with very great difficulty j insomuch that the lava of a volcano has, sixteen years after an eruption, been found red hat a foot under the surface of such glass, though this was quite cool. This circumstance might very pro- bably give the hint for the assertion (paradoxical as it may seem without proper deliberation) that it, would be no difficult matter to convey an iron ball red hot from London to Lincoln: to perform this, it must be inclosed in pumice stone, which is very porous glass, formed by volcanos, and then co- vered over with fur, It is also easy, by covering a room with (he to preserve the air in it of the same 14 of it, one would imagine it would require no great effort of " genius to discover that it would be equally efficacious for " preventing the Heat without from coming in. But natural " as this conclusion may appear, I believe it has never yet " occurred to any body ; at least I am quite certain that I " have never seen a double window, either in Italy, or in any " other hot country, I have had occasion to visit." A little farther on, he says, — " There is no communication of Heat between one particle of air and anotiter particle of air* From hence it follows, that though air may, and undoubt- edly does, curry off Heat, and transport it from one place, or from one body to another, yet a mass of air in a quiescent state, or with all its particles at rest, could it remain in that state, would be totally impervious to Heat; or such a mass (l of air would be a perfect non-conductor," Much curious and valuable information on this subject may be found in Professor LESLIE'S Experimental Inquiry init (lie Naiun and Propagation qf Heat, lately published. HEAT, COLD, AND LIGHT. 325 same temperature, without bringing any thing into it eiiher hot or cold, fora very great length of time. As to the effects produced by Heat, it is known to expand bodies ; and some late chemists affirm, that it tends to diminish every attraction we are acquainted with: they produce experiments to evince that Heat diminishes the attraction — of gravitation, — of cohesion, — of magnetism, — of electricity, and chemical attractions. But though it may be the case in particular instances, it will be better not to be too sanguine in imagining that such effects will take place universally. The asser- tion may be disputed with regard to the attraction of gravitation, and that of electricity. However, those who allow that Heat universally diminishes the electrical attraction, will strongly contend in. support of their opinion, because they may thereby explain with facility the reason of the frequency of thunder-storms in summer. From a review of what has been here advanced, we shall find that there are few, or, perhaps, we may confidently say, no appearances, but what will admit of as easy an explanation, by conjec- turing that Heat is a quality, as by supposing that it is a substance. Nay, some of the phenomena, particularly those which attend the production of Heat by friction, or vibration in solids, will (as must appear from what has been previously ob- served) induce us to incline mose to the former hypothesis than to the latter. Besides, whether Heat be a substance, or a quality, it is manifest, thai 326 APPENDIX. that it may be created and annihilated. Now, we have no idea of matter being created and anni hilated by any natural cause, (for under all its variety of forms, matter is matter still) ; then what kind of a substance must Heat be, to be produced and destroyed by so many causes ? Why, truly, nobody can tell : for it must have a property which matter has not. Heat is, then, probably a quality: for qualities we know can easily be created and annihilated. And, if Heat be a quality, it must have matter to exist in ; so that, if we apply any of the causes producing Heat, no Heat is produced unless there be some matter to receive it. This, therefore, is the result of our inquiries into the -nature of Heat. We have also seen, that Light may be produced by particular means, the solar rays for instance : it may likewise be destroyed, as has been previously shewn. The method of reasoning just applied to Heat, may with equal propriety be used here : and this will induce us to conclude that Light, instead of being a fluid per sr, as has been sometimes conjectured, is a quality, and can no more exist independently of matter than Heat can. Whether these conclusions may be safely relied on, is not for us to determine : the great myste- rious BEING who made and governs the universe, has set a part only of the chain of causes in our view ; and we find that as HK himself is too high for our comprehension, so His more immediate instruments are also involved in an obscurity that ©ur feeble endeavours are not able to dissipate. However, MEAT, COLD, AND LIGHT. 39f However, as Mr. Maclaurin has observed,— " From what we are able to understand of nature, " we may entertain the greater expectations of t( what will be discovered to us, if ever we shall " be allowed to penetrate to the FIRST CAUSE " himself, and see the whole scheme of his works •" as they are really derived from HIM, when our 4( imperfect philosophy shall bejcompleted." 1C. Jilli i ton and Henderson, Printeis, Johnson's Court, London. The following Works have leen lately published ly the Author of these Lessons, And may be had of J. CONDEK, 13, St. Paul's Church-yard. COURSE OF NATURAL AND MATHEMATICAL PHILOSOPHY. Just published, to be had, either together or in separate Parts, as follows : 1. AN ELEMENTARY TREATISE ON NATURAL PHILOSOPHY; Translated from the French of M. R. J, Haiiy, with Notes, critical, illustrative, and historical, by OLINTHUS GJIEGORY, L. L. D. of the Royal Military A ca-i demy, Woolwich, in two Volumes octavo, with twenty-four folding Plates, price I/. 4s. boards.' %* In this Work are treated the Subjects of Extension, Impenetrability, Divisibility, Mobility, Velocity, Inertia, Hardness, Elasticity, Ductility, Gravity, Accelerated Mo- tion, Specific Gravity, Crystallization, Heat, Dilatations by Heat, Thermometers, Combustion, Water in the States of Liquidity, Ice, and Vapour, Capillary Attraction, Congela- tion of Mercury, Steam-Engines, Air, Barometers, Syphons, Pumps, Evaporation, Winds, Air Balloons, Theory of Mu-» sical Sounds, Electricity, Galvanism, Magnetism, Light and Vision, with Descriptions of Electrical, Magnetical, and Optical Instruments, &c. Testimonies in favour of this Treatise. " We have not yet seen a Treatise on Natural Philoso- phy which approached so nearly to a systematic form; no one completed with so much care, comprehending such a variety of details, finished with more philosophical accu- racy." Crit. Rev. Series 3. vol. i. App. " There is more originality of maneer and more vigour of intellect discoverable in the Traite" de Physique of M. Haiiy, than in any ether elementary treatise of Natural Philosophy which has for many years made its appearance in Britain. The Translator has executed his task with fide- lity and skilh the public are well acquainted with his ta- lents, and will doubtless feel much indebted to him for- presenting so valuable a production to their notice : as well as for having considerably increased its utility by the fre- quent interspersion of copious notes." Eclec. Rev. vol. iv. No. 2. - " Mr. Gregory has dene justice to theauthor in his trans- lation, and has, we think, rendered a service to the public-' by giving this treatise in an English dress. He has not, Works by Dr. Gregory, published by J. Conder. however, confined himself to a bare translation, but has given many valuable notes, which add considerably to the utility of the work." Phil. Mag. Dec. 1307. 2. Dll. GREGORY'S TREATISE ON ASTRONOMY >• in which the Elements of the Science aie deduced in a na- tural Order from the Appearances of the Heavens to an Ob- server on the Eajth; demonstrated on Mathematical Prin.r ciples, and explained by an Application to the various Phenomena: one large octavo volume,, with nine folding plates, price 15s. in hoards. For testimonies in faveur of this Treatise, see Monthly Review, Aug. 1802; Phil. Mag. Feb. 1802; and Mathema- tical Repository and Review, Sept. 1802. 3 DR. 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S. .and Mr. NEWTON BOSWORTH, PANTOLOGIA : a General Dictionary of Arts, Sciences, and Words: now re-publishing in Monthly Parts, and completed in 12 vols. Royal octavo. 6. LETTERS TO A FRIEND ON THE EVIDENCES, DOCTRINES, AND DUTIES OF THE CHRISTIAN RELIGION. In 2'vels. crown' 8vo. 3d edition. 14s. boards. This work is intended to guard young persons of liberal edu- cation against infidelity and heterodoxy ; and to evince the peculiar importance and reasonableness of Christianity, a» manifested in its distinguishing doctrines^ and in their powet> ful tendency to influence The foUowing Works are likewise Sold by JosiAir CONDER, No. 18, St. Paul's Church-yard. 1. THE COMPLETE WORKS of the Rev. ISAAC WATTS, D. D. in 9 Vols. 8vo. 4/. 14*. 6d. boards; fin* paper, 6/. 6s. 2. The COMPLETE WORKS of the Rev. STEVHEK CHARNOCK, D. D. in 7 Vols. 8vo. price *2s. per Vol. Edited by the Rev. Edward Parsons, of Leeds. 3. THE ASSOCIATE MINSTRELS. The Second Edition; with additional Poems. 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