Eric E. Becklin (born 6 April 1940) is an American astrophysicist. 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]
On August 23, 2012, in a ceremony held at Dryden Flight Research Center (now the Armstrong Flight Research Center), Becklin received the NASA Exceptional Public Service Medal “for excellence as a pioneer in the infrared astronomy field and providing key leadership for the scientific success of the Stratospheric Observatory for Infrared Astronomy.”[3] He was awarded the Henry Norris Russell Lectureship by the American Astronomical Society in 2017.[4]
In 1988, while returning home from an observing run on Mauna Kea, Becklin was a passenger on Aloha Airlines Flight 243, which underwent explosive decompression and had to make an emergency landing in Maui.[7]
Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation. The wavelength of infrared light ranges from 0.75 to 300 micrometers, and falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.
An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy, astrology, climatology/meteorology, geophysics, oceanography and volcanology are examples of disciplines for which observatories have been constructed. Historically, observatories were as simple as containing an astronomical sextant or Stonehenge.
The W. M. Keck Observatory is an astronomical observatory with two telescopes at an elevation of 4,145 meters (13,600 ft) near the summit of Mauna Kea in the U.S. state of Hawaii. Both telescopes have 10 m (33 ft) aperture primary mirrors, and, when completed in 1993 and 1996, they were the largest optical reflecting telescopes in the world. They are currently the third and fourth largest.
Marc Aaronson was an American astronomer.
The Mauna Kea Observatories (MKO) are a group of independent astronomical research facilities and large telescope observatories that are located at the summit of Mauna Kea on the Big Island of Hawaiʻi, United States. The facilities are located in a 525-acre (212 ha) special land use zone known as the "Astronomy Precinct", which is located within the 11,228-acre (4,544 ha) Mauna Kea Science Reserve. The Astronomy Precinct was established in 1967 and is located on land protected by the Historical Preservation Act for its significance to Hawaiian culture. The presence and continued construction of telescopes is highly controversial due to Mauna Kea's centrality in native Hawaiian religion and culture, as well as for a variety of environmental reasons.
The Gerard P. Kuiper Airborne Observatory (KAO) was a national facility operated by NASA to support research in infrared astronomy. The observation platform was a highly modified Lockheed C-141A Starlifter jet transport aircraft with a range of 6,000 nautical miles (11,000 km), capable of conducting research operations at altitudes of up to 48,000 feet (14 km).
Andrea Mia Ghez is an American astrophysicist, Nobel laureate, and professor in the Department of Physics and Astronomy and the Lauren B. Leichtman & Arthur E. Levine chair in Astrophysics, at the University of California, Los Angeles. Her research focuses on the center of the Milky Way galaxy.
NASA's series of Great Observatories satellites are four large, powerful space-based astronomical telescopes launched between 1990 and 2003. They were built with different technology to examine specific wavelength/energy regions of the electromagnetic spectrum: gamma rays, X-rays, visible and ultraviolet light, and infrared light.
The Stratospheric Observatory For Infrared Astronomy (SOFIA) was a 80/20 joint project of NASA and the German Aerospace Center (DLR) to construct and maintain an airborne observatory. NASA awarded the contract for the development of the aircraft, operation of the observatory and management of the American part of the project to the Universities Space Research Association (USRA) in 1996. The DSI managed the German parts of the project which were primarily science-and telescope-related. SOFIA's telescope saw first light on May 26, 2010. SOFIA was the successor to the Kuiper Airborne Observatory. During 10-hour, overnight flights, it observed celestial magnetic fields, star-forming regions, comets, nebulae, and the Galactic Center.
Submillimetre astronomy or submillimeter astronomy is the branch of observational astronomy that is conducted at submillimetre wavelengths of the electromagnetic spectrum. Astronomers place the submillimetre waveband between the far-infrared and microwave wavebands, typically taken to be between a few hundred micrometres and a millimetre. It is still common in submillimetre astronomy to quote wavelengths in 'microns', the old name for micrometre.
An infrared telescope is a telescope that uses infrared light to detect celestial bodies. Infrared light is one of several types of radiation present in the electromagnetic spectrum.
Gerhart "Gerry" Neugebauer was an American astronomer known for his pioneering work in infrared astronomy.
Ian Gatley was the former Provost and Senior Vice President for Academic Affairs of New Jersey Institute of Technology (NJIT) in Newark, New Jersey. He is also a Distinguished Professor of Physics in the department of Physics at the College of Science and Liberal Arts in NJIT. He is a prolific scholar well known in Astronomy and Imaging Science.
The Onizuka Center for International Astronomy, also known as Hale Pōhaku, is a complex of support facilities for the telescopes and other instruments that comprise the Mauna Kea Observatory atop Mauna Kea, on Hawaiʻi island.
A balloon-borne telescope is a type of airborne telescope, a sub-orbital astronomical telescope that is suspended below one or more stratospheric balloons, allowing it to be lifted above the lower, dense part of the Earth's atmosphere. This has the advantage of improving the resolution limit of the telescope at a much lower cost than for a space telescope. It also allows observation of frequency bands that are blocked by the atmosphere.
Hawaii's first aeronautical event was on 2 March 1889, when Emil L. Melville hung from a trapeze in a balloon. Hawaii's first aircraft flight was on 31 December 1910 by a Curtiss Biplane.
James Richard Houck was the Kenneth A. Wallace Professor of Astronomy at Cornell University.
Joan T. Schmelz is the Associate Director for Science and Public Outreach at the Stratospheric Observatory for Infrared Astronomy (SOFIA) for the Universities Space Research Association (USRA). Previously, Schmelz was the Deputy Director of Arecibo Observatory and the Director of USRA Operations at Arecibo from 2015 through 2018. Before joining USRA, Schmelz was an NSF Program Director in the Astronomical Sciences Division, where she oversaw the Astronomy & Astrophysics Postdoctoral Fellowship program, and a professor of physics at the University of Memphis from 1996 to 2017. Schmelz's research focus is heliophysics, specifically investigating the coronal heating problem as well as the properties and dynamics of the solar atmosphere. She uses spectroscopic and image data in the X-ray and ultraviolet wavelength ranges obtained from NASA satellites and rockets. She has published over 80 refereed scientific journal articles and authored three books.
Giovanni Fazio is an American physicist at Center for Astrophysics | Harvard & Smithsonian. He is an astrophysicist who has initiated and participated in multiple observation programs.
Frederick Carl Gillett was an American astronomer who was a pioneer of infrared astronomy. He was based successively at the University of California, San Diego, Kitt Peak National Observatory, and the International Gemini Observatory. His discoveries include the Vega phenomenon and the first unidentified infrared emission bands.
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