John Couch Adams (June 5 1819 – January 21, 1892), was a British
mathematician and astronomer. Adams was born in
Laneast, Cornwall and died in Cambridge. The Cornish name Couch is pronounced "cooch".
His most famous achievement was predicting the existence and position of Neptune, using only
mathematics. The calculations were made to explain discrepancies with Uranus's orbit and the laws of
Kepler and Newton. At the same time, but unknown
to each other, the same calculations were made by Urbain Le Verrier. Le Verrier would
assist Galle in locating the planet (September
1846); which was found within 1° of its predicted location, a point in Aquarius. (There was, and to some extent still is, some controversy over the apportionment of
credit for the discovery; see Discovery of Neptune.)
He was Lowndean Professor at the University of Cambridge for thirty-three years from 1859 to his death. He won the
Gold Medal of the Royal Astronomical Society in 1866. In
1884, he attended the International Meridian Conference as a delegate
for Britain.
A crater on the Moon is jointly named after him,
Walter Sydney Adams and Charles Hitchcock
Adams. Neptune's outermost known ring and the asteroid 1996 Adams are also named after him. The Adams Prize, presented by the University of Cambridge, commemorates his prediction of the position of
Neptune. His personal library is now in the care of Cambridge University
Library.
Early life
Adams was born at Lidcot, a farm at Laneast,[1] near Launceston, Cornwall, the eldest of seven children. His parents were Thomas Adams (1788–1859), a poor tenant farmer, and his wife, Tabitha Knill née Grylls (1796–1866). The family were devout
Wesleyans who enjoyed music and among John's brothers, Thomas
became a missionary, George a farmer, and William Grylls Adams, professor of natural philosophy and
astronomy at King's College
London. Tabitha was a farmer's daughter but had received a rudimentary education from John Couch, her uncle, whose small
library she had inherited. John was intrigued by the astronomy books from an early age.[2]
John attended the Laneast village school where he acquired some Greek and
algebra. From there, he went, at the age of twelve, to Devonport, where his mother's cousin, the Rev. John Couch Grylls, kept a private school. There he
learned classics but was largely self-taught in mathematics, studying in the Library of Devonport Mechanics'
Institute and reading Rees's Cyclopaedia and Samuel Vince's Fluxions. He observed Halley's comet in
1835 from Landulph and the following year started to make his own
astronomical calculations, predictions and observations, engaging in private tutoring to finance his activities.[2]
In 1836, his mother inherited a small estate at Badharlick
and his promise as a mathematician induced his parents to send him to the University of
Cambridge, and in October 1839 he entered as a sizar at St John's College. He graduated with a B.A. in
1843 as the senior wrangler and first Smith's prizeman of his year.[2]
Discovery of Neptune
-
In 1821, Alexis Bouvard had published astronomical tables of the orbit of Uranus, making predictions of future positions based on Newton's laws of motion and gravitation.[3] Subsequent observations revealed substantial deviations from the tables, leading Bouvard to
hypothesize some perturbing body.[4] Adams learnt of the
irregularities while still an undergraduate and became convinced of the "perturbation" theory. Adams believed, in the face of
anything that had been attempted before, that he could use the observed data on Uranus, and utilising nothing more than Newton's
law of gravitation, deduce the mass, position and orbit of the perturbing body On 3 July
1841, he noted his intention to work on the problem.[2]
After his final examinations in 1843, Adams was
elected fellow of his college and spent the summer vacation in Cornwall calculating the first of
six iterations. While he worked on the problem back in Cambridge, he tutored undergraduates, sending money home to educate his
brothers, and even taught Mrs Ireland, his bedmaker, to read.[2]
Supposedly, Adams communicated his work to James Challis, director of the Cambridge Observatory, in mid-September 1845 but there is some controversy as to how. On 21 October 1845,
Adams, returning from a Cornwall vacation and without appointment, twice called on Astronomer
Royal George Biddell Airy in Greenwich.
Failing to find him at home, Adams reputedly left a manuscript of his solution, again without the detailed calculations. Airy
responded with a letter to Adams asking for some clarification.[5] It appears that Adams did not regard the question as "trivial", as is often alleged, but he
failed to complete a response. Various theories have been discussed as to Adams's failure to reply, such as his general
nervousness, procrastination and disorganisation.[5]
Meanwhile, Urbain Le Verrier, on 10 November
1845, presented to the Académie des
sciences in Paris a memoir on Uranus, showing that the pre-existing
theory failed to account for its motion.[1] On reading
Le Verrier's memoir, Airy was struck by the coincidence and initiated a desparate race for English priority in discovery of the
planet.[6] The search was begun by a laborious method on 29
July.[2] Only after the discovery of Neptune on 23
September 1846 had been announced in Paris did it become apparent that Neptune had been observed on 8 and 12 August but because Challis lacked an up-to-date star-map it was not
recognized as a planet.[1]
A keen controversy arose in France and England as to the merits of the two astronomers. As the facts became known, there was
wide recognition that the two astronomers had independently solved the problem of Uranus, and each was ascribed equal
importance.[2][1] However, there have been subsequent assertions that "The Brits Stole Neptune"
and that Adams's British contemporaries retrospectively ascribed him more credit than he was due.[5]
Adams held no bitterness towards Challis or Airy[2] and acknowledged his own failure to convince the astronomical world:[5]
I could not expect however that practical astronomers, who were already fully occupied with important labours, would feel as
much confidence in the results of my investigations, as I myself did.
Adams's style of working
His lay fellowship at St John's College came to an end in 1852, and the existing statutes did
not permit his re-election. However, Pembroke College, which possessed
greater freedom, elected him in the following year to a lay fellowship which he held for the rest of his life. Despite the fame
of his work on Neptune, Adams also did much important work on gravitational astronomy and terrestrial magnetism. He was
particularly adept at fine numerical calculations, often making substantial revisions to the contributions of his
predecessors.[1] However, he was "extraordinarily
uncompetitive, reluctant to publish imperfect work to stimulate debate or claim priority, averse to correspondence about it, and
forgetful in practical matters".[2] It has been
suggested that these are symptoms of Asperger
syndrome which would also be consistent with the "repetitive behaviours and restricted interests" necessary to perform the
Neptune calculations, in addition to his difficulties in personal interaction with Challis and Airy.[7]
In 1852, he published new and accurate tables of the moon's parallax, which superseded Johann Karl Burckhardt's, and
supplied corrections to the theories of Marie-Charles Damoiseau,
Giovanni Antonio Amedeo Plana, and Philippe Gustave Doulcet.[1]
He had hoped that this work would leverage him into the vacant post as superintendent of HM Nautical Almanac Office but John Russell Hind
was preferred, Adams lacking the necessary ability as an organiser and administrator.[2]
Secular acceleration of the Moon
It had been observed since ancient times that the Moon's position in the sky was drifting over
time. In 1693, Edmond Halley had shown that the rate of the
drift was increasing by approximately 11" per century, an effect known as the secular acceleration of the Moon.
Pierre-Simon Laplace had given an explanation in 1787
in terms of changes in the eccentricity of the Earth's orbit. He considered only the
radial garviational force on the Moon, from the Sun and
Earth but obtained close agreement with the historical record of
observations.[8]
In 1820, at the insistence of the Académie des
sciences, Damoiseau, Plana and Francesco Carlini revisited Laplace's work,
investigating quadratic and higher-order perturbing terms, and obtained similar results, again
addressing only a radial, and neglecting tangential, gravitational force on the Moon. Hansen obtained similar results in
1842 and 1847.[9]
In 1853, Adams published a paper[10] showing that, while tangential terms vanish in the first-order tneory of Laplace, they become
substantial when quadratic terms are admitted. Small terms integrated in time come to have
large effects and Adams concluded that Plana had overestimated the secular acceleration by approximately 1.66" pre
century.[9]
At first, Le Verrier rejected Adams's results.[11] In 1856, Plana admitted Adams's conclusions, claiming to have
revised his own analysis and arrived at the some results. However, he soon recanted, publishing a third result different both
from Adams's and Plana's own earlier work. Delaunay in 1859 calculated the fourth-order term and
duplicated Adams's result leading Adams to publish his own calculations for the fifth, sixth and seventh-order terms. Adams now
calculated that only 5.7" of the observed 11" was accounted for by graviational effects.[9]
Later that year, Philippe Gustave Doulcet, Comte de Pontécoulant published a claim that the tangential force could have no
effect though Peter Andreas Hansen, who seems to have cast himself in the role of
arbitrator, declared that the burden of proof
rested on Pontécoulant, while lamenting the need to discover a further effect to account for the balance. Much of the controversy
centred around the convergence of the power series
expansion used and, in 1860, Adams duplicated his results without using a power series. Sir
John Lubbock also duplicated Adams's results and Plana finally concurred. Adams's view was
ultimately accepted and further developed, winning him the Gold
Medal of the Royal Astronomical Society in 1866.[11][9] The unexplained drift is now known to be due to tidal
acceleration.[2]
In 1858 Adams became professor of mathematics at the University of St Andrews, but lectured only for a session, before returning to Cambridge for
the Lowndean professorship of astronomy and geometry. Two years later he succeeded Challis as director of the Observatory, a post
Adams held until his death.[1]
The Leonids
The great meteor shower of November 1866 turned his attention to the Leonids, whose probable path and period had already been discussed and predicted by Hubert Anson Newton in 1864. Newton had asserted that the
longitude of the ascending node, that marked where the shower would
occur, was increasing and the problem of explaining this variation attracted some of Europe's leading astronomers.[2]
Using a powerful and elaborate analysis, Adams ascertained that this cluster of meteors, which belongs to the solar system,
traverses an elongated ellipse in 33.25 years, and is subject to definite perturbations from the larger planets, Jupiter, Saturn
and Uranus. These results were published in 1867.[1]
Some experts consider this Adams's most substantial achievement. His "definitive orbit" for the Leonids coincided with that of
the comet 55P/Tempel-Tuttle and
therefore suggested the, later widely accepted, close relationship between comets and meteors.[2]
Later career
Ten years later, George William Hill described a novel and elegant method for
attacking the problem of lunar motion. Adams briefly announced his own unpublished work in the same field, which, following a
parallel course had confirmed and supplemented Hill's.[1]
Over a period of forty years, he periodically addressed the determination of the constants in Carl Friedrich Gauss's theory of terrestrial magnetism. Again, the calculations involved great
labour, and were not published during his lifetime. They were edited by his brother, William Grylls
Adams, and appear in the second volume of the collected Scientific Papers. Numerical computation of this kind might
almost be described as his pastime.[1] He calculated
the Euler–Mascheroni constant, perhaps somewhat eccentrically, to 236
decimal places[2] and evaluated the Bernoulli numbers up to the
62nd.[1]
Adams had boundless admiration for Newton and his writings and many of his papers bear the cast of Newton's thought.[1] In 1872, Isaac Newton Wallop, 5th Earl of Portsmouth donated his private collection of Newton's papers to Cambridge
University. Adams and G. G. Stokes took on the task or arranging the material,
publishing a catalogue in 1888.[12][13]
The post of Astronomer Royal was offered him in 1881, but he preferred to pursue his
peaceful course of teaching and research in Cambridge. He was British delegate to the International Meridian Conference at Washington in 1884, when he also attended the meetings of the British
Association at Montreal and of the American Association at Philadelphia.[1]
Honours
- He is reputed to have been offered a knighthood on Queen Victoria's 1847 Cambridge
visit but to have declined, either out of modesty,[1]
or fear of the financial consequences of such social distinction;[2]
- Copley medal of the Royal Society,
(1848);[1]
- Adams Prize, founded by the members of St John's College, to be given biennially for the
best treatise on a mathematical subject (1848);[1]
- President of the Royal Astronomical Society, (1851-1853 and
1874-1876).[1]
Family and death
Five years later his health gave way, and after a long illness he died at the Cambridge Observatory on 21 January 1892, and was buried in St Giles's cemetery, near his home. In 1863
he had married Miss Eliza Bruce, of Dublin, who survived him.[1] His wealth at death was £32,434 (£2.6 million at 2003 prices[14]).[2]
Memorials
References
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y [Anon.] (1911) "John Couch Adams, Encyclopaedia Britannica
- ^ a b c d e f g h i j k l m n o p
- ^ A. Bouvard (1821), Tables astronomiques publiées par le Bureau des Longitudes de France, Paris, FR:
Bachelier
- ^ [Anon.] (2001) "Bouvard, Alexis", Encyclopaedia Britannica, Deluxe CDROM edition
- ^ a b c d
- ^ Smart (1947) p.59
- ^ Sheehan & Thurber (2007)
- ^ Roy, A. E. (2005). Orbital Motion. London: CRC Press, 313. ISBN 0750310154.
- ^ a b c d de la Rue (1866)
- ^ Adams, J. C. (1853). "On the secular
variation of the Moon's mean motion". Philosophical Transactions of the Royal Society of London 143:
397-406.
- ^ a b Kushner (1989)
- ^ Introduction to the Newton Manuscripts Catalogue. The Newton Project. Retrieved on
2007-08-24.
- ^ A Catalogue of the Portsmouth Collection of Books and Papers written by
or belonging to Sir Issac Newton, the Sceintific Part of which has been Presented by the Earl of Portsmouth to the University of
Cambridge, drawn up by the Syndicate appointed 6th November 1982, Cambridge: Cambridge University Press, 1888
- ^ O‘Donoghue, J. et al. (2004).
"Consumer Price Inflation
since 1750". Economic Trends 604: 38-46, March.
- ^ Kollerstrom, N. (2001). Eggen
takes the papers. The British Case for Co-prediction. University College London. Retrieved on 2007-08-23.
Bibliography
Obituaries
About Adams and the discovery of Neptune
- Airy, G. B. (1847). "Account of some
circumstances historically connected with the discovery of the planet exterior to Uranus". Memoirs of the Royal Astronomical
Society 16: 385–414.
- Airy, W. (ed.) (1896). The Autobiography of Sir George Biddell Airy. Cambridge University
Press.
from Project Gutenberg
- [Anon.] (1911) "John Couch
Adams, Encyclopaedia Britannica
- Baum, R. & Sheehan, W. (1997). In Search of Planet Vulcan: The Ghost in
Newton's Clockwork Universe. Plenum.
- Chapman, A. (1988). "Private research and public duty: George Biddell Airy and the search for
Neptune". Journal for the History of Astronomy 19(2): 121-139.
- de la Rue, W. (1866). "Address on award of RAS
gold medal for work on secular acceleration of the Moon". Monthly Notes of the Royal Astronomical Society 26:
157.
- Doggett, L. E. (1997) "Celestial mechanics", in Lankford, J. (ed.) (1997).
History of Astronomy, an Encylopedia, 131–40.
- Dreyer, J. L. E. & Turner, H. H. (eds) [1923] (1987). History of the
Royal Astronomical Society [1]: 1820–1920, 161–2.
- Grosser, M. (1962). The Discovery of Neptune. Harvard University Press.
ISBN 0674212258.
- — (1970). "Adams, John Couch". Dictionary of Scientific Biography 1. New York: Charles Scribner's Sons.
53-54. ISBN 0684101149.
- Harrison, H. M (1994). Voyager in Time and Space: The Life of John Couch Adams, Cambridge Astronomer. Lewes: Book
Guild, ISBN 0-86332-918-7
- Hughes, D. W. (1996). "J. C. Adams, Cambridge and Neptune". Notes and Records of the Royal
Society 50: 245–8.
- Hutchins, R. (2004) "Adams, John
Couch (1819–1892)", Oxford Dictionary of National Biography,
Oxford University Press, accessed 23 August 2007 (subscription or UK/ Ireland public library membership required)
- J. W. L. G. [J. W. L. Glaisher] (1882–3). "James Challis". Monthly Notices of the Royal
Astronomical Society 43: 160–79.
- Kollerstrom, Nick (2001). Neptune's Discovery. The British Case for Co-Prediction.. Unuiversity College London.
Archived from the original on
2005-11-11. Retrieved on 2007-03-19.
- Kushner, D. (1989). "The controversy surrounding the secular acceleration of the moon's mean
motion". Archive for History of Exact Sciences 39(4): 291-316.
- Moore, P. (1996). The Planet Neptune: An Historical Survey before
Voyager. Praxis.
- Sampson, R.A. (1904). "A description of Adams’s manuscripts on the perturbations of Uranus".
Memoirs of the Royal Astronomical Society 54: 143-161.
- Sheehan, W. & Thurber, S. (2007). "John Couch Adams's Asperger syndrome and the British
non-discovery of Neptune". Notes and Records of the Royal Society 61(3): 285-299.
- Sheehan, W. et al. (2004). The Case of the Pilfered Planet - Did the British steal Neptune? Scientific
American
- Smart, W. M. (1946). "John Couch Adams and the discovery of Neptune". Nature 158: 829-830.
- — (1947). "John Couch Adams and the discovery of Neptune". Occasional Notes of the Royal
Astronomical Society 2: 33–88.
- Smith, R. W. (1989). "The Cambridge network in action: the discovery of Neptune". Isis
80(303): 395-422.
- Standage, T. (2000). The Neptune File. Penguin Press.
By Adams
- Adams, J. C., ed. W. G. Adams & R. A. Sampson (1896-1900 The Scientific Papers of John Couch Adams, 2 vols,
London: Cambridge University Press, with a memoir by J. W. L. Glaisher:
- Vol.1 (1896) Previously published writings;
- Vol.2 (1900) Manuscripts including the substance of his lectures on the Lunar Theory.
- A collection, virtually complete, of Adams's papers regarding the discovery of Neptune was presented by Mrs Adams to the
library of St John's College, see: Sampson (1904), and also:
- "The collected papers of Prof. Adams", Journal of the British Astronomical Association, 7 (1896–7)
- Monthly Notices of the Royal Astronomical Society, 53 184;
- Observatory, 15 174;
- Nature, 34 565; 45 301;
- Astronomical Journal, No.254;
- R. Grant, History of Physical Astronomy, p.168; and
- Edinburgh Review, No.381, p.72.
- The papers were ultimately lodged with the Royal Greenwich Observatory and evacuated to Herstmonceux Castle during World War II. After the war, they
were stolen by Olin J. Eggen and only recovered in
1998, hampering much historical research in the subject.[15]
External links
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