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Story of Eclipses

<h2>CHAPTER XII.</h2> ECLIPSES OF THE SUN MENTIONED IN HISTORY.—MEDIÆVAL AND MODERN. One of the most celebrated eclipses of mediæval times was that of August 2, 1133, visible as a total eclipse in Scotland. It was considered a presage of misfortune to Henry I. and was thus referred to by William of Malmesbury[80]:— “The elements manifested their sorrow at this great man’s last departure from England. For the Sun on that day at the 6th hour shrouded his glorious face, as the poets say, in hideous darkness agitating the hearts of men by an eclipse; and on the 6th day of the week early in the morning there was so great an earthquake that the ground appeared absolutely to[146] sink down; an horrid noise being first heard beneath the surface.” This eclipse is also alluded to in the Anglo-Saxon Chronicle though the year is wrongly given as 1135 instead of 1133 as it certainly was. The Chronicle says:—“In this year King Henry went over sea at Lammas, and the second day as he lay and slept on the ship the day darkened over all lands; and the Sun became as it were a three-night-old Moon, and the stars about it at mid-day. Men were greatly wonder-stricken and affrighted, and said that a great thing should come hereafter. So it did, for the same year the king died on the following day after St. Andrew’s Mass day, Dec. 2, in Normandy.” The king did die in 1135, but there was no eclipse of the August new Moon, and without doubt the writer has muddled up the year of the eclipse and of the king’s departure from England (to which he never returned) and the year of his death. Calvisius states that this eclipse was observed in Flanders and that the stars appeared. Respecting the above-mentioned discrepancy Mrs. Todd aptly remarks:—“So Henry must have died in 1133, which he did not; or else there must have been an eclipse in 1135, which there was not. But this is not the only labyrinth into which chronology and old eclipses, imagination, and computation, lead the unwary searcher.” Professor Freeman’s explanation fairly clears up the difficulty:—“The fact that he never came back to England, together with the circumstances of his voyage, seems to have made a deep impression on men’s minds. In popular belief the[147] signs and wonders which marked his last voyage were transferred to the Lammas-tide before his death two years later.”[81] The central line of this eclipse traversed Scotland from Ross to Forfar and the eclipse was of course large in every part of the country. The totality lasted 4m. 20s. in Forfarshire. Hind has furnished some further information respecting this eclipse. It appears that during the existence of the Kingdom of Jerusalem created by the Crusaders an eclipse occurred which would appear to have been total at Jerusalem or in its immediate neighbourhood. No date is given and a date can only be guessed, and Hind guessed that the eclipse of 1133 was the one referred to. He found that after leaving Scotland and crossing Europe the central line of the 1133 eclipse entered Palestine near Jaffa and passed over Jerusalem where the Sun was hidden for 4¼ minutes at about 3h. p.m. From Nablous on the N. to Ascalon on the S. the country was in darkness for nearly the same period of time. The alternative eclipses to this one would be those of Sept. 4, 1187, magnitude at Jerusalem 9⁄10ths of the Sun’s diameter; or June 23, 1191, magnitude at the same place about 7⁄10ths; but these do not seem to harmonise so well with the accounts handed down to us as does the eclipse of 1133. In 1140, on March 20, there happened a total eclipse of the Sun visible in England which is thus referred to by William of Malmesbury[82]:—[148]“During this year, in Lent, on the 13th of the Calends of April, at the 9th hour of the 4th day of the week, there was an eclipse, throughout England, as I have heard. With us, indeed, and with all our neighbours, the obscuration of the Sun also was so remarkable, that persons sitting at table, as it then happened almost everywhere, for it was Lent, at first feared that Chaos was come again: afterwards, learning the cause, they went out and beheld the stars around the Sun. It was thought and said by many, not untruly, that the King [Stephen] would not continue a year in the government.” The same eclipse is also thus mentioned in the Anglo-Saxon Chronicle:—“Afterwards in Lent the Sun and the day darkened about the noontide of the day, when men were eating, and they lighted candles to eat by; and that was the 13th of the Calends of April, March 20. Men were greatly wonder-stricken.” The greatest obscuration at London took place at 2h. 36m. p.m., but it is not quite clear whether the line of totality did actually pass over London. It was long supposed that this eclipse was total at London, an idea which seems to have arisen from Halley having told the Royal Society anent the total eclipse of May 3, 1715, that he could not find that any total eclipse had been visible at London since March 20, 1140. In consequence of this statement of Halley’s, Hind carefully investigated the circumstances of this eclipse, and found that it had not been total at London. The central line entered our island at Aberystwith, and passing near Shrewsbury, Stafford, Derby,[149] Nottingham, and Lincoln, reached the German Ocean, 10 miles S. of Saltfleet. The southern limit of the zone of totality passed through the South Midland counties, and the nearest point of approach to London was a point on the borders of Northamptonshire and Bedfordshire. For a position on the central line near Stafford, Hind found that the totality began at 2h. 36m. p.m. local mean time, the duration being 3m. 26s., and the Sun’s altitude being more than 30°. The stars seen were probably the planets Mercury and Venus, then within a degree of each other, and 10° W. of the Sun, and perhaps the stars forming the well-known “Square of Pegasus.” Mars and Saturn were also, at that time, within a degree of each other, but very near the western horizon. It is therefore necessary to look further back than 1140 to find a total solar eclipse visible in London.[83] A solar eclipse seems to have been alluded to by certain historians as having happened in A.D. 1153. We have the obscure statement that “something singular happened to the Sun the day after the Conversion of St. Paul.” A somewhat large eclipse having been visible at Augsburg in Germany, on January 26, this may have been the “something” referred to. It would seem that about 11⁄12ths of the Sun’s diameter was covered. On May 14, A.D. 1230, there happened a great eclipse of the Sun, thus described by Roger of Wendover[84]:—“On the 14th of May, which was[150] the Tuesday in Rogation Week, an unusual eclipse of the Sun took place very early in the morning, immediately after sunrise; and it became so dark that the labourers, who had commenced their morning’s work, were obliged to leave it, and returned again to their beds to sleep; but in about an hour’s time, to the astonishment of many, the Sun regained its usual brightness.” This eclipse, as regards its total phase, is said by Johnston to have begun in the horizon, a little to the N. of London, in the early morning. On June 3, A.D. 1239, and October 6, 1241, there occurred total eclipses of the Sun, which have been very carefully discussed by Professor Celoria of Milan, with the view of using them in investigations into the Moon’s mean motion.[85] The second of these eclipses is mentioned by Tycho Brahe.[86] He states that “a few stars appeared about noonday, and the Sun was hidden from sight in a clear sky.” The eclipse was total in Eastern Europe. Dr. Lingard,[87] the well-known Roman Catholic historian, speaking of the battle of Cressy, which was fought on August 26, 1346, says:—“Never, perhaps, were preparations for battle made under circumstances so truly awful. On that very day the Sun suffered a partial eclipse: birds in clouds, precursors of a storm, flew screaming over the two armies; and the rain fell in torrents, accompanied[151] with incessant thunder and lightning. About 5 in the afternoon, the weather cleared up, the Sun in full splendour darted his rays in the eyes of the enemy; and the Genoese, setting up their shouts, discharged their quarrels.” This was not an eclipse, for none was due to take place; and the phenomenon could only have been meteorological—dense clouds or something of that sort in the sky. On June 16, 1406, there was a large eclipse of the Sun, 9⁄10ths of its diameter being covered at London; but on the Continent it seems to have been total. It is stated that the darkness was such that people could hardly recognise one another. One of the most celebrated eclipses during the Middle Ages was undoubtedly that of June 17, 1433. This was long remembered in Scotland as the “Black Hour,” and its circumstances were fully investigated some years ago by Hind. It was a remarkable eclipse in that the Moon was within 13° of perigee and the Sun only 2° from apogee. The central line traversed Scotland in a south-easterly direction from Ross to Forfar, passing near Inverness and Dundee. Maclaurin[88] who lived in the early part of the last century mentions that in his time a manuscript account of this eclipse was preserved in the library of the University of Edinburgh wherein the darkness is said to have come on at about 3 p.m., and to have been very profound. The duration of the totality at Inverness was 4m. 32s.; at Edinburgh 3m. 41s. The central line passed from Britain to the N. of Frankfort-on-the-Maine, through[152] Bavaria, to the Dardanelles, to the S. of Aleppo and thence nearly parallel to the river Euphrates to the N.-E. border of Arabia. In Turkey, according to Calvisius, “near evening the light of the Sun was so overpowered that darkness covered the land.” In 1544, on Jan. 24, there occurred an eclipse of the Sun which was nearly but not quite total. The chief interest arises from the fact that it was one of the first observed by professed astronomers: Gemma Frisius saw it at Louvain. Kepler says[89] that the day became dark like the twilight of evening and that the birds which from the break of day had been singing became mute. The middle of the eclipse was at about 9 a.m. In 1560 an eclipse of the Sun took place which was total in Spain and Portugal. Clavius who observed it at Coimbra says[90] that “the Sun remained obscured for no little time: there was darkness greater than that of night, no one could see where he trod and the stars shone very brightly in the sky: the birds moreover, wonderful to say, fell down to the ground in fright at such startling darkness.” Kepler is responsible for the statement that Tycho Brahe did not believe this, and wrote to Clavius to that effect 40 years afterwards. In 1567 there was an annular eclipse visible at Rome on April 9. Clavius says[91] that “the[153] whole Sun was not eclipsed but that there was left a bright circle all round.” This in set terms is a description of an annular eclipse, but Johnston who calculated that at Rome the greatest obscuration took place at 20m. past noon points out that the augmentation of the Moon’s semi-diameter would almost have produced totality. Tycho tells us that he saw this eclipse on the shores of the Baltic when a young man about 20 years of age. The total eclipse of February 25, 1598, long left a special mark on the memories of the people of Scotland. The day was spoken of as “Black Saturday.” Maclaurin states[92]:—“There is a tradition that some persons in the North lost their way in the time of this eclipse, and perished in the snow”—a statement which Hind discredits. The central line passed from near Stranraer, over Dalkeith, and therefore Edinburgh was within the zone of totality. Totality came on at Edinburgh at 10h. 15m. and lasted 1m. 30s. From the rapid motion of the Moon in declination, the course of the central line was a quickly ascending one in latitude on the Earth’s surface, the totality passing off within the Arctic circle. Kepler in his account of the new star in the constellation Ophiuchus[93] refers to the total eclipse of the Sun of October 12, 1605, as having been observed at Naples, and that the “Red Flames” were visible as a rim of red[154] light round the Sun’s disc: at least this seems to be the construction which may fairly be put upon the Latin of the original description. The partial eclipse of the Sun of May 30, 1612, is recorded to have been seen “through a tube.” No doubt this is an allusion to the newly-invented instrument which we now call the telescope. Seemingly this is the first eclipse of the Sun so observed, but it is on record that an eclipse of the Moon had been previously observed through a telescope. This was the lunar eclipse of July 6, 1610, though the observer’s name has not been handed down to us. The eclipse of April 8, 1652, is another of those Scotch eclipses, as we may call them, which left their mark on the people of that country. Maclaurin[94] speaks of it in his time (he died in 1746) as one of the two central eclipses which are “still famous among the populace in this country” [Scotland], and “known amongst them by the appellation of Mirk Monday.” The central line passed over the S.E. of Ireland, near Wexford and Wicklow, and reaching Scotland near Burrow Head in Wigtownshire, and passing not far from Edinburgh, Montrose and Aberdeen, quitted Scotland at Peterhead. Greenock and Elgin were near the northern limit of the zone of totality, and the Cheviots and Berwick upon the southern limit. The eclipse was observed at Carrickfergus by Dr. Wyberd.[95] Hind found that its duration there was but 44s. This short duration, he suggested,[155] may partly explain the curious remark of Dr. Wyberd that when the Sun was reduced to “a very slender crescent of light, the Moon all at once threw herself within the margin of the solar disc with such agility that she seemed to revolve like an upper millstone, affording a pleasant spectacle of rotatory motion.” Wyberd’s further description clearly applies to the Corona. A Scotch account says that “the country people tilling, loosed their ploughs. The birds dropped to the ground.” The eclipse of November 4, 1668, visible as a partial one in England, was of no particular interest in itself but deserves notice as having been observed by Flamsteed,[96] who gives a few diagrams of his observations at Derby. He states that the eclipse came on much earlier than had been predicted. It was well known at this time that the tables of the Sun and Moon then in use were very defective, and it was a recognition of this fact which eventually led to the foundation of the Greenwich Observatory in 1675. On September 23, 1699, an eclipse of the Sun occurred which was total to the N. of Caithness for the very brief space of 10-15 secs. At Edinburgh, about 11⁄12ths of the Sun’s diameter was obscured. In the Appendix to Pepys’s Diary[97] there is a letter from Dr. Wallis mentioning that his daughter’s attention was called to it by noticing “the light of the Sun look somewhat[156] dim” at about 9 a.m., whilst she was writing a letter, she knowing nothing of the eclipse. An eclipse of the Sun occurred on May 12, 1706, which was visible as a partial eclipse in England and was total on the Continent, especially in Switzerland. A certain Captain Stannyan who made observations at Berne, writes thus to Flamsteed[98]:—“That the Sun was totally darkened there for four and a half minutes of time; that a fixed star and a planet appeared very bright; and that his getting out of his eclipse was preceded by a blood-red streak of light from its left limb, which continued not longer than six or seven seconds of time; then part of the Sun’s disc appeared all of a sudden as bright as Venus was ever seen in the night; nay, brighter; and in that very instant gave a light and shadow to things as strong as the Moon uses to do.” On this communication Flamsteed remarks:—“The Captain is the first man I ever heard of that took notice of a red streak preceding the emersion of the Sun’s body from a total eclipse, and I take notice of it to you [the Royal Society], because it infers that the Moon has an atmosphere; and its short continuance, if only six or seven seconds’ time, tells us that its height was not more than five or six hundredths part of her diameter.” On the whole, perhaps, the most celebrated eclipse of the Sun ever recorded in England was that of May 3, 1715. The line of totality passed right across England from Cornwall to Norfolk, and the phenomenon was carefully observed and[157] described by the most experienced astronomer of the time, Dr. Edmund Halley. The line of totality passed over London amongst other places, and as the maximum phase took place soon after 9 a.m. on a fine spring morning, the inhabitants of the Metropolis saw a sight which their successors will not see again till many generations have come and gone. Halley has left behind him an exceedingly interesting account of this event, some allusions to which have already been made. He seems to have seen what we call the Corona, described by him however as a “luminous ring,” “of a pale whiteness, or rather pearl colour, a little tinged with the colours of the Iris, and concentric with the Moon.” He speaks also of a dusky but strong red light which seemed to colour the dark edge of the Moon just before the Sun emerged from totality. Jupiter, Mercury, Venus, and the stars Capella and Aldebaran were seen in London, whilst N. of London, more directly under the central line, as many as twenty stars were seen. The inhabitants of England who lived in the reign of George I. were singularly fortunate in their chances of seeing total eclipses of the Sun, for only nine years after[99] the one just described, namely, on May 22, 1724, another total eclipse occurred. The central line crossed some of the southern countries, and the phenomenon was well seen and reported on by Dr. Stukeley,[100] who stationed himself on Haraden Hill, near Salisbury. The Doctor says of the darkness that he[158] seemed to “feel it, as it were, drop upon us ... like a great dark mantle,” and that during the totality the spectacle presented to his view “was beyond all that he had ever seen or could picture to his imagination the most solemn.” He could with difficulty discern the faces of his companions which had a ghastly startling appearance. When the totality was ending there appeared a small lucid spot, and from it ran a rim of faint brightness. In about 3½ minutes from this appearance the hill-tops changed from black to blue, the horizon gave out the grey streaks previous to morning dawn, and the birds sprang joyously into the air. This eclipse seems to have had royal observers. It was watched at Kensington apparently by the King or some of the royal family of England, and at Trianon (Paris) by the King of France,[101] under the competent guidance of Maraldi, Cassini and De Louville. It was the last which was visible as a total one in any part of England. On May 2, 1733, there was an eclipse of the Sun, which was total in Sweden and partial in England. In Sweden the total obscuration lasted more than 3 minutes. Jupiter, the stars in Ursa Major, Capella, and several other stars were visible to the naked eye, as also was a luminous ring round the Sun. Three or four spots of reddish colour were also perceived near the limb of the Moon, but not in immediate contact with it. These so-called red “spots” were doubtless the[159] Red Flames of the present century, and the luminous ring the Corona. On March 1, 1737, a good annular eclipse was observed at Edinburgh by Maclaurin.[102] In his account he says:—“A little before the annulus was complete a remarkable point or speck of pale light appeared near the middle of the part of the Moon’s circumference that was not yet come upon the disc of the Sun.... During the appearance of the annulus the direct light of the Sun was still very considerable, but the places that were shaded from his light appeared gloomy. There was a dusk in the atmosphere, especially towards the N. and E. In those chambers which had not their lights westwards the obscurity was considerable. Venus appeared plainly, and continued visible long after the annulus was dissolved, and I am told that other stars were seen by some.” Lord Aberdour mentions a narrow streak of dusky red light on the dark edge of the Moon immediately before the ring was completed, and after it was dissolved. No doubt this is a record of the “Red Flames.” In 1748 Scotland was again favoured with a central eclipse, but it was only annular. The Earl of Morton[103] and James Short, the optician, who observed the phenomenon at Aberdour Castle, 10 miles N.-W. of Edinburgh, just outside the line of annularity, saw a brown coloured light stretching along the circumference of the[160] Moon from each of the cusps. A “star” (probably the planet Venus) was seen to the E. of the Sun. The annular eclipse of April 1, 1764, visible as such in North Kent, was the subject of the following quaint letter by the Rev. Dr. Stukeley:— <div class="blockquot">“To the Printer of Whitehall Evening Post,— “In regard to the approaching solar eclipse of Sunday, April 1, I think it advisable to remark that, it happening in the time of divine service, it is desired you would insert this caution in your public paper. The eclipse begins soon after 9, the middle a little before 11, the end a little after 12. There will be no total darkness in the very middle, observable in this metropolis, but as people’s curiositys will not be over with the middle of the eclipse, if the church service be ordered to begin a little before 12, it will properly be morning prayer, and an uniformity preserved in our duty to the Supreme Being, the author of these amazing celestial movements,— Yours, Rector of St. Geo., Q.S.”[104] </div> The year 1766 furnishes the somewhat rare case of a total eclipse of the Sun observed on board ship on the high seas. The observers were officers of the French man-of-war the Comte d’Artois. Though the total obscuration lasted only 53 secs., there was seen a luminous ring about the Moon which had four remarkable expansions, situate at a distance of 90° from each[161] other.[105] These expansions are doubtless those rays which we now speak of as “streamers” from the Corona. Curiously enough the next important total eclipse deserving of notice was also observed at sea. This was the eclipse of June 24, 1778. The observer was the Spanish Admiral, Don Antonio Ulloa, who was passing from the Azores to Cape St. Vincent. The total obscuration lasted 4 minutes. The luminous ring presented a very beautiful appearance: out of it there issued forth rays of light which reached to the distance of a diameter of the Moon. Before it became very conspicuous stars of the 1st and 2nd magnitudes were distinctly visible, but when it attained its greatest brilliancy, only stars of the 1st magnitude could be perceived. “The darkness was such that persons who were asleep and happened to wake, thought that they had slept the whole evening and only waked when the night was pretty far advanced. The fowls, birds, and other animals on board took their usual position for sleeping, as if it had been night.”[106] On Sept. 5, 1793, there happened an eclipse which, annular to the N. of Scotland, was seen and observed in England by Sir W. Herschel[107] as a partial eclipse. He made some important observations on the Moon on this occasion measuring the height of several of the lunar[162] mountains. Considerations respecting the shape of one of the Moon’s horns led him to form an opinion adverse to the idea that there the Moon had an atmosphere. <div class="footnotes">Footnotes: <div class="footnote">[79] Historiarum Sui Temporis, Lib. iv., cap. 9. </div> <div class="footnote">[80] Historia Novella, Lib. i., sec. 8. </div> <div class="footnote">[81] Norman Conquest, vol. v. p. 239. </div> <div class="footnote">[82] Historia Novella, Lib. ii., sec. 35. </div> <div class="footnote">[83] Letter in the Times, July 28, 1871. </div> <div class="footnote">[84] Rogerus de Wendover, Flores Historiarum, vol. ii. p. 535, Bohn’s ed. </div> <div class="footnote">[85] Sugli Eclissi Solari Totali del 3 Giugno 1239, e del 6 Ottobre 1241 in the Memorie del R. Istituto Lombardo di Scienze e Littere, vol. xiii. p. 275. </div> <div class="footnote">[86] Historia Cœlestis, vol. i. p. 38. </div> <div class="footnote">[87] Hist. Engl., vol. iii. chap. xviii. p. 50, 4to. ed. </div> <div class="footnote">[88] Phil. Trans., vol. xl. p. 194, 1737. </div> <div class="footnote">[89] Astronomiæ Pars Optica, c. viii. sec. 3; Opera Omnia, vol. ii. p. 315. Ed. Frisch, 1859. </div> <div class="footnote">[90] Quoted by Kepler, as above, at p. 315. </div> <div class="footnote">[91] Commentarius in Sacroboscum, cap. iv.; quoted in Kepler’s Astronomiæ Pars Optica, c. viii. sec. 3; Opera Omnia, vol ii. p. 316. Ed. Frisch, 1859. </div> <div class="footnote">[92] Phil. Trans., vol. xl. p. 193; 1737. </div> <div class="footnote">[93] De Stellâ Novâ in Pede Serpentarii, p. 115; Pragæ, 1606. </div> <div class="footnote">[94] Phil. Trans., vol. xl. p. 193; 1737. </div> <div class="footnote">[95] V. Wing, Astronomia Britannica, p. 355. </div> <div class="footnote">[96] Historia Cœlestis, vol. i. pp. 7 and 21. </div> <div class="footnote">[97] Diary of Samuel Pepys, vol. vi. p. 208; Ed. M. Bright, 1879. </div> <div class="footnote">[98] Phil. Trans., vol. xxv. p. 2240; 1706. </div> <div class="footnote">[99] Being half a Saros period (see p. 20, ante). </div> <div class="footnote">[100] Itinerarium Curiosum, 2nd ed., vol. i. p. 180. </div> <div class="footnote">[101] Mem. de Mathématique et de Physique de l’Acad. des Sciences, 1724, p. 259. </div> <div class="footnote">[102] Phil. Trans., vol. xl. pp. 181, 184. 1737. </div> <div class="footnote">[103] Phil. Trans., vol. xlv. p. 586. 1750. This is the man who under the designation of “Lord Aberdour” observed the eclipse of 1737 (ante). </div> <div class="footnote">[104] Rev. W. Stukeley, Rector of St. George’s, Queen’s Square, London, Diary, vol. xx. p. 44, ed. “Surtees Soc.,” vol. lxxvi. p. 384. </div> <div class="footnote">[105] Le Gentil, Voyage dans les Mers de l’Inde, vol. ii. p. 16. Paris, 1769. </div> <div class="footnote">[106] Phil. Trans., vol. lxix. p. 105. 1779. </div> <div class="footnote">[107] Phil. Trans., vol. lxxxiv. p. 39. 1794. </div> </div> <div style="break-after:column;"></div>

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