|Birthname||Friedrich Wilhelm Bessel|
|born on||21 June 1784 at 16:00 (= 4:00 PM )|
|Place||Minden, Germany, 52n17, 8e55|
|Timezone||LMT m8e55 (is local mean time)|
|Astrology data||00°44' 13°37 Asc. 11°58'|
German mathematician, astronomer, and systematizer of the Bessel functions. He was a contemporary of Carl Gauss, also a mathematician and physicist. Bessel came to the attention of a major figure of German astronomy at the time, Heinrich Wilhelm Olbers, by producing a refinement on the orbital calculations for Halley's Comet. Within two years Bessel had left Kulenkamp and become an assistant at Lilienthal Observatory near Bremen. There he worked on James Bradley's stellar observations to produce precise positions for some 3,222 stars. This work attracted considerable attention, and in January 1810, at the age of 25, Bessel was appointed director of the Königsberg Observatory. There he published tables of atmospheric refraction based on Bradley's observations. Bessel was able to pin down the position of over 50,000 stars during his time at Königsberg.
With this work under his belt, Bessel was able to achieve the feat for which he is best remembered today: he is credited with being the first to use parallax in calculating the distance to a star. Astronomers had believed for some time that parallax would provide the first accurate measurement of interstellar distances—in fact, in the 1830s there was a fierce competition between astronomers to be the first to measure a stellar parallax accurately. In 1838 Bessel won the race, announcing that 61 Cygni had a parallax of 0.314 arcseconds; which, given the diameter of the Earth's orbit, indicated that the star is 10.4 ly away. If the currently accepted figure of 11.4 ly is correct, Bessel's figure had an error of 8.8%. He narrowly beat Friedrich Georg Wilhelm Struve and Thomas Henderson, who measured the parallaxes of Vega and Alpha Centauri in the same year.
As well as helping determine the parallax of 61 Cygni, Bessel's precise measurements allowed him to notice deviations in the motions of Sirius and Procyon, which he deduced must be caused by the gravitational attraction of unseen companions. His announcement of Sirius's "dark companion" in 1844 was the first correct claim of a previously unobserved companion by positional measurement, and eventually led to the discovery of Sirius B.
Despite lacking a university education, Bessel was a major figure in astronomy during his lifetime. He was elected a fellow of the Royal Society, a foreign member of the Royal Swedish Academy of Sciences in 1823, and the largest crater in the Moon's Mare Serenitatis is named Bessel after him. Bessel's work in 1840 contributed in some degree to the discovery of Neptune. In 1832, he was elected a Foreign Honorary Member of the American Academy of Arts and Sciences.
He died in the spring of 1846 in Königsberg from cancer.
The asteroid 1552 Bessel was named in his honour.
- Work : Gain social status 6 January 1810 (became director of Königsberg observatory, and professor of astronomy)
chart Placidus Equal_H.
Taeger IHL quotes Arno Müller, vol. 2, birth registry (?)
- Vocation : Science : Astronomy
- Vocation : Science : Mathematics/ Statistics