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Friedrich Wilhelm August Argelander (22 March 1799 – 17 February 1875) was a German astronomer. He is known for his determinations of stellar brightnesses, positions, and distances. Life and work [ edit ]
- 17 February 1875 (aged 75), Bonn, Germany
- Prussian
Friedrich Wilhelm August Argelander (born March 22, 1799, Memel, East Prussia—died Feb. 17, 1875, Bonn) was a German astronomer who established the study of variable stars as an independent branch of astronomy and is renowned for his great catalog listing the positions and magnitudes of 324,188 stars. He studied at the University of ...
- The Editors of Encyclopaedia Britannica
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May 23, 2018 · Argelander, Friedrich Wilhelm August. ( b. Memel, Prussia, 22 March 1799; d. Bonn, Germany, 17 February 1875) astronomy. Argelander’s father, Johann Gottlieb Argelander, was a wealthy merchant from Finland; his mother, Dorothea Wilhelmine Grünlingen, was German. The boy grew up in the easternmost corner of Prussia, and the Napoleonic Wars ...
Friedrich Wilhelm August Argelander has 13 books on Goodreads with 0 ratings. Friedrich Wilhelm August Argelander’s most popular book is Mittlere Oerter ...
Argelander, Friedrich Wilhelm August. Born Memel (Klaipeda, Lithuania), 23 March 1799. Died Bonn, Germany, 17 February 1875. Friedrich Argelander was an observatory director who confirmed solar motion from stellar proper motions; he later produced the Bonner Durchmusterung. Argelander was the son of merchant and shipowner Johann Gottfried ...
Friedrich Wilhelm August Argelander. 1799-1875. German astronomer who completed a survey of the heavens that included data on the positions and brightnesses of over 324,000 stars. His catalog, called the Bonner Durchmusterung, included more precise data on the brightnesses of stars than previous catalogs, aiding astronomers who studied ...
A Dictionary of Astronomy (2 rev) (1799–1875)Germanastronomer, born in modern Lithuania. From a study of the proper motions of several hundred stars he confirmed F. W. Herschel's calculated position of the Sun's apex. His main achievement, begun in 1852, was a survey of all stars down to 9th magnitude in the northern hemisphere.