Jump to content

Gerry Neugebauer: Difference between revisions

From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
minor typo
Added significant publication
Line 2: Line 2:
{{More footnotes|date=April 2013}}
{{More footnotes|date=April 2013}}
{{Use dmy dates|date=May 2021}}
{{Use dmy dates|date=May 2021}}
'''Gerhart "Gerry" Neugebauer'''<ref>Neugebauer's first name is pronounced ''Gary'', not ''Jerry''.</ref> (3 September 1932 – 26 September 2014) was an [[United States of America|American]] [[astronomer]] known for his pioneering work in [[infrared astronomy]].
'''Gerhart "Gerry" Neugebauer'''<ref group=Note name=Note01/> (3 September 1932 – 26 September 2014) was an [[United States of America|American]] [[astronomer]] known for his pioneering work in [[infrared astronomy]].


Neugebauer was born in [[Göttingen]], [[Weimar Republic|Germany]] and was the son of [[Otto E. Neugebauer|Otto Neugebauer]], an Austrian-American [[mathematician]] and [[History of science|historian of science]], and Grete Bruck. After moving to the United States at age seven, he received his B.A. in [[physics]] from [[Cornell University]] in 1954 and his Ph.D. in physics from [[California Institute of Technology|Caltech]] in 1960, with a thesis on the photoproduction of negative and positive [[pions]] from [[deuterium]].
Neugebauer was born in [[Göttingen]], [[Weimar Republic|Germany]] and was the son of [[Otto E. Neugebauer|Otto Neugebauer]], an Austrian-American [[mathematician]] and [[History of science|historian of science]], and Grete Bruck. After moving to the United States at age seven, he received his B.A. in [[physics]] from [[Cornell University]] in 1954 and his Ph.D. in physics from [[California Institute of Technology|Caltech]] in 1960, with a thesis on the photoproduction of negative and positive [[pions]] from [[deuterium]].


After completing his doctorate degree, he was commissioned a second lieutenant in the [[United States Army]] he was stationed at the [[Jet Propulsion Laboratory]] where he worked for the [[Ordnance Corps (United States Army)|Ordnance Corps]] until 1962. He joined the Caltech faculty in 1962 as an assistant professor, becoming a full professor of physics in 1970. He was named [[Howard Hughes]] Professor in 1985 and Chairman of the Division of Physics, Math and Astronomy in 1988. At the time of his death, he was the [[Robert Andrews Millikan]] Professor of Physics, Emeritus and an adjunct faculty member of the University of Arizona's Steward Observatory.
After completing his doctorate degree, he was commissioned a second lieutenant in the [[United States Army]] he was stationed at the [[Jet Propulsion Laboratory]] where he worked for the [[Ordnance Corps (United States Army)|Ordnance Corps]] until 1962. He joined the Caltech faculty in 1962 as an assistant professor, becoming a full professor of physics in 1970. He was named [[Howard Hughes]] Professor in 1985 and Chairman of the Division of Physics, Math and Astronomy in 1988. In 1993 he published together with [[Reinhard Meinel]] a complete analytical solution to the field equations of [[Albert Einstein]]'s [[General Relativity|Theory of gravity]] in the case of a rigidly rotating disk of dust.<ref>{{cite journal|title=The Einsteinian Gravitational Field of the Rigidly Rotating Disk of Dust|doi=10.1086/187005}}></ref>At the time of his death, he was the [[Robert Andrews Millikan]] Professor of Physics, Emeritus and an adjunct faculty member of the University of Arizona's Steward Observatory.


Neugebauer served as the director of the [[Palomar Observatory]] from 1980 to 1994.
Neugebauer served as the director of the [[Palomar Observatory]] from 1980 to 1994.
Line 23: Line 23:


==Notes==
==Notes==
{{reflist|group=Note|refs=
<ref name=Note01>Neugebauer's first name is pronounced ''Gary'', not ''Jerry''.</ref>
}}

==References==
{{reflist}}
{{reflist}}


Revision as of 07:11, 16 December 2021

Gerhart "Gerry" Neugebauer[Note 1] (3 September 1932 – 26 September 2014) was an American astronomer known for his pioneering work in infrared astronomy.

Neugebauer was born in Göttingen, Germany and was the son of Otto Neugebauer, an Austrian-American mathematician and historian of science, and Grete Bruck. After moving to the United States at age seven, he received his B.A. in physics from Cornell University in 1954 and his Ph.D. in physics from Caltech in 1960, with a thesis on the photoproduction of negative and positive pions from deuterium.

After completing his doctorate degree, he was commissioned a second lieutenant in the United States Army he was stationed at the Jet Propulsion Laboratory where he worked for the Ordnance Corps until 1962. He joined the Caltech faculty in 1962 as an assistant professor, becoming a full professor of physics in 1970. He was named Howard Hughes Professor in 1985 and Chairman of the Division of Physics, Math and Astronomy in 1988. In 1993 he published together with Reinhard Meinel a complete analytical solution to the field equations of Albert Einstein's Theory of gravity in the case of a rigidly rotating disk of dust.[1]At the time of his death, he was the Robert Andrews Millikan Professor of Physics, Emeritus and an adjunct faculty member of the University of Arizona's Steward Observatory.

Neugebauer served as the director of the Palomar Observatory from 1980 to 1994.

Neugebauer was active in infrared astronomy, and played a leading role in infrared studies of the planets. In addition—and largely through his activities with the Infrared Astronomical Satellite (IRAS) and the Infrared Processing and Analysis Center (IPAC)—he led both ground- and space-based infrared studies of the stars, the Milky Way and other galaxies. Observations by him and his colleagues at Mount Wilson and Palomar observatories revealed thousands of infrared sources in the sky, and afforded the first infrared view of the galactic center. Together with Robert B. Leighton, he completed the Two-Micron Sky Survey, the first infrared survey of the sky, which cataloged more than 5,000 infrared sources. Together with Eric Becklin, he discovered the Becklin–Neugebauer Object, an intense source of infrared radiation in the Orion Nebula that is one of the brightest objects in the sky at wavelengths less than 10 micrometres.

Neugebauer played a role in the design and construction of the W. M. Keck Observatory in Hawaii. Among Neugebauer's numerous awards are two NASA Exceptional Scientific Achievement Medals (1972, 1984), the 1985 Space Science Award of the American Institute of Aeronautics and Astronautics, the 1985 Richmyer Lecture Award, the 1986 Rumford Prize, the 1996 Henry Norris Russell Lectureship, the 1998 Herschel Medal, and the 2010 Bruce Medal. He was named California Scientist of the Year for 1986 by the California Museum of Science and Industry, and he was elected to the National Academy of the Sciences, the American Philosophical Society, the American Academy of Arts and Sciences and the Royal Astronomical Society.

Neugebauer was married to the geophysicist Marcia Neugebauer, a pioneer in solar wind research at the Jet Propulsion Laboratory, and the two resided in Tucson, Arizona. He died on 26 September 2014 in Tucson, due to spinocerebellar ataxia.[2]

Prizes

Notes

  1. ^ Neugebauer's first name is pronounced Gary, not Jerry.

References

  1. ^ "The Einsteinian Gravitational Field of the Rigidly Rotating Disk of Dust". doi:10.1086/187005. {{cite journal}}: Cite journal requires |journal= (help)>
  2. ^ Martin, Douglas (3 October 2014). "Gerry Neugebauer, Pioneer in Space Studies, Dies at 82". The New York Times.
Retrieved from "https://en.wikipedia.org/w/index.php?title=Gerry_Neugebauer&oldid=1060557284"