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See also: British astronomer, was See also: born in See also: London on the 28th of See also: February 1831
.
Educated at the City of London School, he obtained a studentship at See also: King's
See also: College, London, and in 1856 a scholarship at See also: Queen's College, Cambridge, graduated as fifth wrangler in 1859, and was immediately elected See also: fellow of his college
.
The following See also: year he succeeded the Rev
.
R
.
See also: Main as chief assistant at the Royal See also: Observatory, See also: Greenwich, and at once undertook the fundamental task of improving astronomical constants
.
The most important of these, the See also: sun's mean See also: parallax, was at that See also: time subject to considerable uncertainty
.
From a discussion of the observations of See also: Mars made in 186o and 1862 at Greenwich and See also: Williams-See also: town (near Melbourne), See also: Stone deduced for it a value of 8.932" (Mon
.
Not
.
R.A.S.
See also: xxiii
.
183), and in a further investigation in which he included the observations made in 1862, at the Cape of See also: Good Hope, he obtained 8.945" (Mein. of R.A.S., vol. xxxiii.)
.
Confirmatory results were afforded by his discussion of the observations of the transit of See also: Venus in 1769 which yielded the figure 8.91" (Mon
.
Not
.
R.A.S. See also: xxviii
.
255)
.
In 1865 he contributed a memoir to the Royal Astronomical Society on the See also: constant of lunar parallax
.
He also deter-See also: mined the mass of the See also: moon, and from a discussion of the Greenwich transit circle observations between 1851 and 1865 he found for the constant of See also: nutation the value 9.134"
.
These services were recognized by the award of the Royal Astronomical Society's gold medal in 1869, and on the resignation of See also: Sir See also: Thomas Maclear in 1870 he was appointed Her Majesty's astronomer at the Cape
.
His first task on taking up this
See also: post was the reduction and publication of a large mass of observations See also: left by his predecessor, from a selected portion of which (those made 1856-186o) he compiled a See also: catalogue of 1159 stars
.
His See also: principal See also: work was, however, a catalogue of 12,441 stars to the 7th magnitude between the See also: South See also: Pole and 25° S. declination, which was practically finished by the end of 1878 and published in 1881
.
Shortly after the See also: death of Main on the 9th of May 1878, Stone was appointed to succeed him as See also: Radcliffe Observer at See also: Oxford, and he left the Cape on the 27th of May 1879
.
At Oxford he extended the Cape observations of stars to the 7th magnitude from 25° S. declination to the equator, and collected the results in the Radcliffe Catalogue for 189o, which contains the places of 6424 stars
.
Stone observed the transit of Venus of 1874 at the Cape, and organized the See also: government expeditions for the corresponding event in 1882
.
He was elected president of the Royal Astronomical Society (1882-1884), and he was the first to recognize the importance of the old observations accumulated at the Radcliffe Observatory by Hornsby, See also: Robertson and See also: Rigaud (Mon
.
Not
.
R.A.S., vol. lv.) . He successfully observed the See also: total solar eclipse of the 8th of See also: August 1896 at Novaya Zemlya, and purposed a voyage to See also: India for the eclipse of 1898, but died suddenly at the Radcliffe Observatory on the 9th of May 1897
.
The number of his astronomical publications exceeds 150, but his reputation depends mainly on his earlier work at Greenwich and his two See also: great See also: star catalogues— the Cape Catalogue for 188o and the Radcliffe Catalogue for 1890
.
See Proc
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See also: Roy
.
Society, Ixii
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10; See also: Month
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Not
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Roy
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Ast
.
See also: Soc. lviii
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143; The Times, loth of May 1897; Observatory, xx.234; Astr
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Nach . No . 3426; Roy . Soc . See also: Cat
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Scient
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Papers
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(A M
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