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Wilhelm Heinrich Walter Baade (March 24, 1893 – June 25, 1960) was a German astronomer who worked in the United States from 1931 to 1959.

Walter Baade
Born(1893-03-24)March 24, 1893
Schröttinghausen, German Empire
DiedJune 25, 1960(1960-06-25) (aged 67)
Göttingen, West Germany
NationalityGerman
CitizenshipGerman
Alma materUniversity of Göttingen
Known forCoined the term "supernova" and "neutron star" with Fritz Zwicky
AwardsBruce Medal 1955
Scientific career
FieldsAstronomy
InstitutionsHamburg-Bergedorf Observatory, Mt. Wilson, Palomar Observatory
Doctoral studentsHalton Arp
Allan Sandage

Biography


The son of a teacher, Baade finished school in 1912. He then studied maths, physics and astronomy at the universities of Münster and Göttingen. After receiving his PhD in 1919, Baade worked at Hamburg Observatory at Bergedorf from 1919 to 1931.[1] There in 1920 he discovered 944 Hidalgo, the first of a class of minor planets now called Centaurs which cross the orbits of giant planets.

He worked at Mount Wilson Observatory from 1931 to 1958.[2] There, during World War II, he took advantage of wartime blackout conditions (which reduced light pollution), to resolve stars in the center of the Andromeda Galaxy for the first time. These observations led him to define distinct "populations" for stars (Population I and Population II). The same observations led him to discover that there are two types of Cepheid variable stars. Using this discovery he recalculated the size of the known universe, doubling the previous calculation made by Edwin Hubble in 1929.[3][4][5] He announced this finding to considerable astonishment at the 1952 meeting of the International Astronomical Union in Rome.

Together with Fritz Zwicky, he identified supernovae as a new category of astronomical objects.[6][7] Zwicky and he also proposed the existence of neutron stars, and suggested supernovae might create them.[8]

Beginning in 1952, he and Rudolph Minkowski identified the optical counterparts of various radio sources,[9] including Cygnus A. He discovered 10 asteroids, including 944 Hidalgo, which has a long orbital period (it is actually the first centaur ever discovered, although they were not recognized as a distinct dynamical class until 1977); the Apollo-class 1566 Icarus, the perihelion of which is closer than that of Mercury; and the Amor-type 1036 Ganymed.


Honors


Asteroids discovered: 10[10]
930 WestphaliaMarch 10, 1920
934 ThüringiaAugust 15, 1920
944 HidalgoOctober 31, 1920
966 MuschiNovember 9, 1921
967 HelionapeNovember 9, 1921
1036 GanymedOctober 23, 1924
1103 SequoiaNovember 9, 1928
1566 IcarusJune 27, 1949
5656 OldfieldOctober 8, 1920
7448 PöllathJanuary 14, 1948

Awards

Named after him


See also



References


  1. Osterbrock, D. E. (Sep 2002). "Walter Baade, Dynamical Astronomer at Goettingen, Hamburg, Mount Wilson, and Palomar Observatories". Aas/Division of Dynamical Astronomy Meeting #33. Harvard Univ. 33: 10.03. Bibcode:2002DDA....33.1003O.
  2. "1955 Brude Medalist". Sonoma State University. Retrieved 4 March 2016.
  3. Baade W (1944) The resolution of Messier 32, NGC 205, and the central region of the Andromeda nebula. ApJ 100 137-146
  4. Baade W (1956) The period-luminosity relation of the Cepheids. PASP 68 5-16
  5. Allen, Nick. "Section 2: The Great Debate and the Great Mistake: Shapley, Hubble, Baade". The Cepheid Distance Scale: A History. Archived from the original on December 10, 2007.
  6. W. Baade, F. Zwicky, 1934, "On Super-Novae". Proceedings of the National Academy of Sciences of the United States of America, 254-259.
  7. Donald E. Osterbrock, Walter Baade – A Life in Astrophysics, Princeton und Oxford: Princeton University Press 2001. ISBN 0-691-04936-X.
  8. Osterbrock, D. E. (2001). "Who Really Coined the Word Supernova? Who First Predicted Neutron Stars?". Bulletin of the American Astronomical Society. 33: 1330. Bibcode:2001AAS...199.1501O.
  9. Baade, W. and Minkowski, R., 1954. Identification of the Radio Sources in Cassiopeia, Cygnus A, and Puppis A. Astrophysical Journal, Vol. 119, p. 206-214 (January 1954) ADS: 1954ApJ...119..206B
  10. "Minor Planet Discoverers (by number)". Minor Planet Center. 4 September 2016. Retrieved 7 September 2016.
  11. "Walter H.W. Baade (1893 - 1960)". Royal Netherlands Academy of Arts and Sciences. Retrieved 26 January 2016.

Further reading





Obituaries



На других языках


[de] Walter Baade

Wilhelm Heinrich Walter Baade (* 24. März 1893 in Schröttinghausen; † 25. Juni 1960 in Göttingen) war ein deutscher Astronom und Astrophysiker.
- [en] Walter Baade

[es] Walter Baade

Wilhelm Heinrich Walter Baade (Schröttinghausen, 24 de marzo de 1893-Gotinga, 25 de junio de 1960) fue un astrónomo alemán que emigró a los Estados Unidos en 1931. Entre otros aportes, definió el concepto de población estelar, descubrió diez asteroides y la existencia de dos tipos de Cefeidas, lo que llevó a una importante corrección en la escala de distancias extragalácticas.[1]

[it] Walter Baade

Walter Baade (Schröttinghausen, 24 marzo 1893 – Gottinga, 25 giugno 1960) è stato un astronomo tedesco, che emigrò negli Stati Uniti d'America nel 1931.

[ru] Бааде, Вальтер

Ва́льтер Ба́аде (нем. Walter Baade; 24 марта 1893, Шрёттингхаузен, Германская империя, — 25 июня 1960, Гёттинген, ФРГ) — немецкий астроном и астрофизик.



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