Eric E. Becklin (born 1940) is an American astrophysicist, best known for his pioneering study of infra-red sources at the center of our galaxy.
Becklin received his Ph.D. in physics from the California Institute of Technology. A faculty member since 1989, Becklin is a Professor Emeritus of Physics and Astronomy at UCLA. Named SOFIA Chief Scientist in 1996, he was the first director of the NASA Infrared Telescope Facility (IRTF) at Mauna Kea, Hawaii and a principal investigator on the Kuiper Airborne Observatory (KAO). Becklin is internationally recognized for his expertise and research in infrared astronomy.
The primary focus of Becklin's research is infrared imaging and spectroscopy, including the search for brown dwarfs, the detection of circumstellar dust rings, the dynamics and composition of the center of the Milky Way galaxy, and the nature of luminous infrared galaxies.[1]
Becklin is Chief Scientist and Director Designate of the Stratospheric Observatory for Infrared Astronomy (SOFIA), which is a 2.7m infrared telescope installed in a modified Boeing 747-SP.
Becklin is widely known for his discovery with Gerry Neugebauer in 1966 of an exceptionally bright infrared source within Orion known today as the Becklin-Neugebauer Object.[2]
Educational background
- B.S., Physics, University of Minnesota, 1963
- Ph.D., Physics, California Institute of Technology, 1968
Notes
- ^ "Eric Becklin,". UCLA Department of Physics and Astronomy faculty profile. http://personnel.physics.ucla.edu/directory/faculty/index.php?f_name=becklin. Retrieved on 2009-02-15.
- ^ "Becklin-Neugebauer Object". The Internet Encyclopedia of Science. http://www.daviddarling.info/encyclopedia/B/Becklin-Neugebauer_Object.html.
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