|Asteroids discovered: 8|
|42 Isis||May 23 1856|
|43 Ariadne||April 15 1857|
|46 Hestia||August 16 1857|
|67 Asia||April 17 1861|
|80 Sappho||May 2 1864|
|87 Sylvia||May 16 1866|
|107 Camilla||November 17 1868|
|245 Vera||February 6 1885|
By the time he was 18 years old, he had computed the orbits of two comets. He became an assistant at Radcliffe Observatory in Oxford, England in 1851. In 1860 he travelled to Madras, India, becoming the government astronomer. At the Madras Observatory he produced the Madras Catalogue of 11,015 stars. He also discovered five asteroids and six variable stars.
His most notable contribution was to note that in the stellar magnitude system introduced by the Greek astronomer Hipparchus, stars of the first magnitude were about a hundred times as bright as stars of the sixth magnitude. His suggestion in 1856 was to make this a standard, so each decrease in magnitude represented a decrease in brightness equal to the fifth-root of 100 (or about 2.512). The Pogson Ratio became the standard method of assigning magnitudes.
The magnitude relation is given as follows:
where m is the stellar magnitude and L is the luminosity, for stars 1 and 2.
In 1868 and 1871, Pogson joined the Indian solar eclipse expeditions.
During his career he discovered a total of eight asteroids and 21 variable stars. He headed the Madras Observatory for 30 years until his death.
Publication No. WO/2010/018746 Published on Feb. 18, Assigned to NTT DOCOMO for User Device, Radio Base Station, Method (Japanese Inventors)
Feb 19, 2010; GENEVA, Feb. 23 -- Akihito Morimoto, Motohiro Tanno, Yoshihisa Kishiyama and Mamoru Sawahashi, all from Japan, have developed a...