Nowadays, Walter Baade is a topic that is on everyone's lips and that does not go unnoticed in today's society. Its importance and relevance become increasingly evident as its analysis deepens. Walter Baade has generated a wide range of opinions and positions, both for and against, which has provoked constant debate in various areas. In this article, we will fully explore the impact Walter Baade has had on our daily lives, as well as its implications for the present and future. In addition, we will analyze the different perspectives that exist around Walter Baade, with the aim of providing a comprehensive and contrasted vision of this enigmatic topic.
Walter Baade | |
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Born | |
Died | June 25, 1960 | (aged 67)
Citizenship | German |
Alma mater | University of Göttingen |
Known for | Coined the term "supernova" and "neutron star" with Fritz Zwicky |
Awards | Bruce Medal 1955 |
Scientific career | |
Fields | Astronomy |
Institutions | Hamburg-Bergedorf Observatory, Mt. Wilson, Palomar Observatory |
Doctoral students | Halton Arp Allan Sandage |
Wilhelm Heinrich Walter Baade (March 24, 1893 – June 25, 1960) was a German astronomer who worked in the United States from 1931 to 1959.
Baade was born the son of a teacher in North Rhine-Westphalia, Germany. He finished school in 1912. He then studied maths, physics and astronomy at the universities of Münster and Göttingen. He received his PhD in 1919.[1]
Baade worked at Hamburg Observatory at Bergedorf from 1919 to 1931.[1] In 1920 he discovered 944 Hidalgo, the first of a class of minor planets now called Centaurs which cross the orbits of giant planets.
From 1931 to 1958, he worked at Mount Wilson Observatory[2]
In 1937, the University of Hamburg wanted Baade as successor of Richard Schorr for the Hamburg Observatory, but he refused.[3]
At Mount Wilson Observatory, 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.[4][5][6] 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.[7][8] Zwicky and he also proposed the existence of neutron stars, and suggested supernovae might create them.[9]
Beginning in 1952, he and Rudolph Minkowski identified the optical counterparts of various radio sources,[10] 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.
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He died in 1960 in Göttingen, West Germany.
930 Westphalia | March 10, 1920 |
934 Thüringia | August 15, 1920 |
944 Hidalgo | October 31, 1920 |
966 Muschi | November 9, 1921 |
967 Helionape | November 9, 1921 |
1036 Ganymed | October 23, 1924 |
1103 Sequoia | November 9, 1928 |
1566 Icarus | June 27, 1949 |
5656 Oldfield | October 8, 1920 |
7448 Pöllath | January 14, 1948 |
Awards
Named after him
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: CS1 maint: multiple names: authors list (link)