弗里德里希·阿格兰德1799—1875

生平

阿格兰德1799年出生于东普鲁士的梅梅尔（今立陶宛的克莱佩达），父亲是德国人，母亲是芬兰人。阿格兰德曾师从德国著名天文学家贝塞尔，1822年在柯尼斯堡取得物理学博士学位。

1823年到1837年，阿格兰德在芬兰数个天文台担任领导人，后前往波恩。在那里他与普鲁士国王腓特烈·威廉四世建立了良好的私人友谊，成为波恩天文台的台长，进行了天体测量的工作。在他和同事们的努力下，1852年到1859年间，波恩天文台发表了波恩星表，记载了324,189颗恒星的位置，是照相术发明以前最完整的一份星表。阿格兰德还是早期研究变星的天文学家之一。

1863年他发起了德国天文学会。1875年阿格兰德在波恩去世。为纪念他，第1551号小行星以及月球上的一座环形山都以他的名字命名。

2006年，波恩大学成立了阿格兰德天文研究所。

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

Argelander was born in Memel in the Kingdom of Prussia (now Klaipėda in Lithuania), the son of a father of Finnish descent, Johann Gottlieb Argelander, and German (Prussian) mother, Dorothea Wilhelmina Grünhagen. He studied with Friedrich Bessel, whose assistant he became in 1820, and obtained his Ph.D. in 1822 at University of Königsberg. From 1823 until 1837, Argelander was the head of the Finnish observatory, first in Turku and then in Helsinki. He then moved to Bonn, Germany. There he designed and built a new observatory at the University of Bonn with funding approved directly by King Frederick William IV whom Argelander had become friends with in his childhood. This lifelong friendship had started when the then crown prince temporarily lived in Argelander's parents house after the Prussian royal family fled to Memel after the Battle of Jena–Auerstedt during the Napoleonic Wars.

Argelander developed practical methods for measuring stellar positions and magnitudes, contributing to the advancement of modern observational astronomy. He also measured stellar distances using heliometers. His work, together with that of his collaborators, included extensive star cataloguing and research on variable stars, made possible through the systematic use of newly developed observational techniques.

Argelander was the first astronomer to begin a careful study of variable stars. Only a handful were known when he began, and he was responsible for introducing the modern system of identifying them. He also made a rough determination of the direction in which the Sun was moving.

In 1842, he discovered that Groombridge 1830 had a very high proper motion. For many decades its proper motion was the highest known; today it still occupies third place. For a time, it was known as Argelander's Star.

Together with Adalbert Krüger and Eduard Schönfeld, Argelander was responsible for the star catalogue known as the Bonner Durchmusterung, published between 1859 and 1862, which gave the positions and brightness of more than 324,000 stars, although it did not cover much of the southern half of the sky. This was the last star map to be published without the use of photography.

In 1863, Argelander helped lead in the founding of an international organization of astronomers named the Astronomische Gesellschaft.

Honors and legacy

Elected a foreign member of the Royal Swedish Academy of Sciences in 1846.

Elected a Foreign Honorary Member of the American Academy of Arts and Sciences in 1855.

Elected Member of the Royal Academy of Science, Letters and Fine Arts of Belgium.

Was awarded the Gold Medal of the Royal Astronomical Society in 1863.

Orden Pour le Mérite für Wissenschaften und Künste (Order Pour le Mérite for Arts and Sciences - Civil class) in 1874.

The three astronomical institutes of the Bonn University were merged and renamed as the Argelander-Institut für Astronomie in 2006.

The crater Argelander on the Moon and the asteroid 1551 Argelander are named for him.