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NEVIL See also:MASKELYNE (1732-1811)
, See also:English astronomer-royal, was See also:born in See also:London on the 6th of See also:October 1732
.
The
See also:solar See also:eclipse of 1748 made a deep impression upon him; and having graduated as seventh wrangler from Trinity See also:College, See also:Cambridge, in 1754, he determined to devote himself wholly to See also:astronomy
.
He became intimate with See also:
He continued during the See also:remainder of his See also:life the superintendence of this invaluable annual
.
He further induced the government to See also:print his observations annually, thereby securing the prompt dissemination of a large See also:mass of data inestimable from their continuity and accuracy
.
Maskelyne had but one assistant, yet the See also:work of the See also:observatory was perfectly organized and methodically executed
.
He introduced several See also:practical improvements, such as the measurement of See also:time to tenths of a second; and he prevailed upon the government to replace See also:Bird's mural quadrant by a repeating circle 6 ft. in See also:diameter
.
The new See also:instrument was constructed by E
.
See also:Troughton; but Maskelyne did not live to see it completed
.
In 1972 he suggested to the Royal Society the famous Schehallion experiment for the determination of the See also:earth's See also:density and carried out his See also:plan in 1774 (Phil
.
Trans
.
1
.
495), the apparent difference of See also:latitude between two stations on opposite sides of the See also:mountain being compared with the real difference of latitude obtained by triangulation
.
From Maskelyne's observations See also: Maskelyne also took a See also:great See also:interest in various geodetical operations, notably the measurement of the length of a degree of latitude in See also:Maryland and See also:Pennsylvania (ibid. lviii . 323), executed by See also:Mason and See also:Dixon in 1766-1768, and later the determination of the relative longitude of See also:Greenwich and See also:Paris (ib. lxxvii . 151) . On the See also:French See also:side the work was conducted by See also:Count See also:Cassini, See also:Legendre, and Mechain; on the English side by See also:General See also:Roy . This triangulation was the beginning of the great trigonometrical survey which has since been extended all over the See also:country . His observations appeared in four large See also:folio volumes (1776-1811) . Some of them were reprinted in S . Vince's Astronomy (vol. iii.) . (A . M . |
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