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SIR GEORGE BIDDELL AIRY (1801-1892)

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Originally appearing in Volume V01, Page 447 of the 1911 Encyclopedia Britannica.
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SIR See also:GEORGE BIDDELL See also:AIRY (1801-1892)  , See also:British Astronomer Royal, was See also:born at See also:Alnwick on the 27th of See also:July 18oi . He came of a See also:long- See also:line of Airys who traced their descent back to a See also:family of the same name residing at Rentmere, in See also:Westmorland, in the 14th See also:century; but the See also:branch to which he belonged, having suffered in the See also:civil See also:wars, removed to See also:Lincolnshire, where for several generations they lived as farmers . See also:George See also:Airy was educated first at elementary See also:schools in See also:Hereford, and afterwards at See also:Colchester See also:Grammar School . In 1819 he entered Trinity See also:College, See also:Cambridge, as a See also:sizar . Here he had a brilliant career, and seems to have been almost immediately recognized as the leading See also:man of his See also:year . In 1822 he was elected See also:scholar of Trinity, and in the following year he graduated as See also:senior wrangler and obtained first See also:Smith's See also:prize . On the 1st of See also:October 1824 he was elected See also:fellow of Trinity, and in See also:December 1826 was appointed Lucasian See also:professor of See also:mathematics in See also:succession to See also:Thomas See also:Turton . This See also:chair he held for little more than a year, being elected in See also:February 1828 Plumian professor of See also:astronomy and director of the new Cambridge See also:observatory . Some See also:idea of his activity as a writer on mathematical and See also:physical subjects during these See also:early years may be gathered from the fact that previous to this See also:appointment he had contributed no less than three important See also:memoirs to the Philosophical Transactions of the Royal Society, and eight to the Cambridge Philosophical Society . At the Cambridge observatory Airy soon gave See also:evidence of his remarkable See also:power of organization . The only See also:telescope erected in the See also:establishment when he took it in See also:charge was the transit See also:instrument, and to this he vigorously devoted himself . By the See also:adoption of a See also:regular See also:system of See also:work, and a careful See also:plan of reduction, he was able to keep his observations reduced practically up to date, and published them annually with a degree of punctuality which astonished his contemporaries .

Before long a mural circle was installed, and regular observations were instituted with it in 1833 . In the same year the See also:

duke of See also:Northumberland presented the Cambridge observatory with a See also:fine See also:object-See also:glass of 12 in. See also:aperture, which was mounted according to Airy's designs and under his superintendence, although the erection was not completed until after his removal to See also:Greenwich in 1835 . Airy's writings during this See also:time are divided between mathematical physics and astronomy . The former are for the m6st See also:part concerned with questions See also:relating to the theory of See also:Tighe, arising out of his professorial lectures, among which may be specially mentioned his See also:paper " On the Diffraction of an Object-Glass with Circular Aperture." In 1831 the See also:Copley See also:medal of the Royal Society was awarded to him for these researches . Of his astronomical writings during this See also:period the most important are his investigation of the See also:mass of See also:Jupiter, his See also:report to the British Association on the progress of astronomy during the 19th century, and his memoit On an Inequality of Long Period in the Motions of the See also:Earth and See also:Venus . One of the sections of his able and instructive report was devoted to " A Comparison of the Progress of Astronomy in See also:England with that in other Countries," very much to the disadvantage of England . This reproach was subsequently to a See also:great extent removed by his own labours . Airy's See also:discovery of a new inequality in the motions of Venus and the earth is in some respects his most remarkable achievement . In correcting the elements of See also:Delambre's See also:solar tables he had been led to suspect an inequality overlooked by their constructor . The cause of this he did not long seek in vain: Eight times the mean See also:motion of Venus is so nearly equal. to thirteen times that of the earth that the difference amounts to only the 210th of the earth's mean motion, and from the fact that the See also:term depending on this difference, although very small in itself, receives in the integration of the See also:differential equations a multiplier of about 2,200,000, Airy was led to infer the existence of a sensible inequality extending over 240 years (Phil . Trans. cxxii . 67) .

The investigation that brought about this result was probably the most laborious that had been made up to Airy's time in planetary theory, and represented the first specific improvement in the solar tables effected in England since the establishment of the theory of See also:

gravitation . In recognition of this work the medal of the Royal Astronomical Society was awarded to him in 1833 . In See also:June 1835 Airy was appointed Astronomer Royal in succession to See also:John See also:Pond, and thus commenced that long career of wisely directed and vigorously sustained See also:industry at the See also:national observatory which, even more perhaps than his investigations in abstract See also:science or theoretical astronomy, constitutes his See also:chief See also:title to fame . The See also:condition of the observatory at the time of his appointment was such that See also:Lord See also:Auckland, the first lord of the See also:Admiralty, considered that " it ought to be cleared out," while Airy admitted that " it was in a queer See also:state." With his usual See also:energy he set to work at once to reorganize the whole management . He remodelled the volumes of observations, put the library on a proper footing, mounted the new (See also:Sheepshanks) See also:equatorial and organized a new magnetic observatory . In 1847 an altazimuth was erected, designed by Airy to enable observations of the See also:moon to be made not only on the See also:meridian, but whenever she might be visible . In 1848 Airy invented the reflex See also:zenith See also:tube to replace the zenith sector previously employed . At the end of 185o the great transit circle of 8 in. aperture and 11 ft . 6 in. See also:focal length was erected, and is still the See also:principal instrument of its class at the observatory . The mounting in 1859 of an equatorial of 13 in. aperture evoked the comment in his See also:journal for that year, " There is not now a single See also:person employed or instrument used in the observatory which was there in Mr Pond's time "; and the transfcrmation was completed by the inauguration of spectroscopic work in 1868 and of the photo-graphic See also:registration of See also:sun-spots in 1873 . The formidable undertaking of reducing the accumulated planetary observations made at Greenwich from 1750 to 183o was already in progress under Airy's supervision when he became Astronomer Royal . Shortly afterwards he undertook the further laborious task of reducing the enormous mass of observations of the moon made at Greenwich during the same period under the direction, successively, of J .

See also:

Bradley, N . See also:Bliss, N . See also:Maskelyne and John Pond, to defray the expense of which a large sum of See also:money was allotted by the See also:Treasury . As the result, no less than 8000 lunar observations were rescued from oblivion, and were, in 1846, placed at the disposal of astronomers in such a See also:form thatthey -could be used directly for comparison with the theory and for. the improvement of the tables of the moon's motion . For this work Airy received in 1848 a testimonial from the Royal Astronomical Society, and it at once led to the discovery by P . • A . See also:Hansen of two new inequalities in the moon's motion . After completing these reductions, Airy made inquiries, before engaging in any theoretical investigation in connexion with them, whether any other mathematician was pursuing the subject, and learning that Hansen had taken it in See also:hand under the patronage of the See also:king of See also:Denmark, but that, owing to the See also:death of the king and the consequent lack of funds, there was danger of his being compelled to abandon it, he applied to the admiralty on Hansen's behalf for the necessary sum . His See also:request was immediately granted, and thus it came about that Hansen's famous Tables de la Lune werededicated to La Haute Amiraute de sa Majeste la Reine de la Grande Bretagne et d'Irlande . One of - the most remarkable of Airy's researches was his determination of the mean See also:density of the earth . In 1826 the idea occurred to him of attacking this problem by means of pendulum- experiments at the t9p and bottom of a deep mine . His first See also:attempt, made in the same year, at the Dolcoath mine in See also:Cornwall, failed in consequence of an See also:accident to one of the pendulums; a second attempt in 1828 was defeated by a flooding of the mine, and many years elapsed before another opportunity presented itself .

Phoenix-squares

The experiments eventually took See also:

place at the See also:Hatton See also:pit near See also:South See also:Shields in 1854 . Their immediate result was to show that gravity at the bottom of the mine exceeded that at the See also:top by 19 li 8 6th of its amount, the See also:depth being 1256 ft . From this he was led to the final value of 6.566 for the mean density of the earth as compared with that of See also:water (Phil . Trans. cxlvi . 342) . This value, although considerably in excess of that previously found by different methods, was held by Airy, from the care and completeness with which the observations were carried out and discussed, to be " entitled to compete with the others on, at least, equal terms." In 1872 Airy conceived the idea of treating the lunar theory in a new way, and at the See also:age of seventy-one he embarked on the prodigious toil which this See also:scheme entailed . A See also:general description of his method will be found in the Monthly Notices of the Royal Astronomical Society, vol. xxxiv, No . 3 . It consisted essentially in the adoption of Delauny's final numerical expressions for See also:longitude, See also:latitude and See also:parallax, with a symbolic term attached to each number, the value of which was to be determined by substitution in the equations of motion . In this mode of treats See also:ing the question the See also:order of the terms is numerical, and though the amount of- labour is such- as might well have deterred a younger man, yet the details were easy, and a great part of it might be entrusted to a See also:mere computer . The work was published in 1886, when its author was eighty-five- years of age . For some little time previously he had been harassed by a suspicion that certain errors had crept into the computations, and accordingly he addressed himself to the task of revision .

But his See also:

powers were no longer what they had been, and he was never able to examine sufficiently into the See also:matter . In 18go he tells us how a grievous See also:error had been committed in one of the first steps, and pathetically adds, " My - spirit in the work was broken, and I have never heartily proceeded- with it since." In188r See also:Sir George' Airy resigned the See also:office of Astronomer Royal and resided at- the See also:White See also:House, Greenwich, not far from the Royal Observatory, until his death, which took place on the . 2nd of See also:January 5892: A See also:complete See also:list of Airy's printed papers, numbering no less than 518, will be found in his Autobiography, edited in 1896 by his son, See also:Wilfrid Airy, B . A., M . Inst.C.E . Amongst the most important of his See also:works not already mentioned may be named the following:—Mathematical Tracts (1826) on the Lunar Theory, Figure of the Earth, Precession and See also:Nutation, and Calculus of See also:Variations, to which, in the second edition of 1828, were added` tracts on the Planetary Theory and the Undulatory Theory of See also:Light; Experiments on See also:Iron-built See also:Ships, instituted for the purpose of discovering a correction for the deviation of the See also:Compass produced by the Iron of the Ships (1839); On the Theoretical Explanation of an apparent new See also:Polarity in Light (1840); Tides and Waves (1842)• He was elected a fellow of the Royal Society in 1836, its See also:president in 1871, and received both the Copley and Royal medals . He was five times president of the Royal Astronomical Society, was correspondent of the See also:French See also:Academy and belonged to many other See also:foreign and See also:American See also:societies . He was D.C.L. of See also:Oxford and LL.D. of Cambridge and See also:Edinburgh . In 1872 he was made K.C.B . In the same year he was nominated a See also:Grand See also:Cross in the Imperial Order of the See also:Rose of See also:Brazil; he also held the Prussian Order " Pour le Write," and belonged to the See also:Legion of See also:Honour of See also:France and to the Order of the See also:North See also:Star of See also:Sweden and See also:Norway . See also Prot . See also:Roy .

Society, li . 1 (E . J . See also:

Routh) ; See also:Month . Notices Roy . Astr . Society, lii . 212; Observatory, xv . 74 (E . Dunkin); Nature, 31st of Oct . 1878 (A . Winnecke), 7th of See also:Jan .

1892; The Times, 5th of Jan . 1892; R . See also:

Grant's Hist. of Phys . Astronomy; R . P . See also:Graves's See also:Life of Sir W . Rowan See also:Hamilton . (A . A .

End of Article: SIR GEORGE BIDDELL AIRY (1801-1892)
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