NASA’s “flying” telescope, the Stratospheric Observatory for Infrared Astronomy (SOFIA) aboard a highly modified Boeing 747SP jetliner, began its fourth series of science flights on Feb. 3, 2016.
This operational period, known as “Cycle 4,” is a one-year-long observing period in which SOFIA is scheduled for 106 flights between now and the end of January 2017.
“The Cycle 4 program will make more than 550 hours of observations,” said Pamela Marcum, NASA’s SOFIA Project Scientist. “We’ll be studying objects spanning the full gamut of astronomical topics including planets, moons, asteroids and comets in our solar system; star and planet formation; extrasolar planets and the evolution of planetary systems; the interstellar medium and interstellar chemistry; the nucleus of the Milky Way galaxy, and nearby normal and active galaxies.”
SOFIA’s instruments observe infrared energy – one part of the electromagnetic spectrum, which includes visible light, x-rays, radio waves and others. Many objects in space, for example newborn stars, emit almost all their energy at infrared wavelengths and are undetectable when observed in ordinary visible light. In other cases, clouds of gas and dust in space block visible light objects but allow infrared energy to reach Earth. In both situations, the celestial objects of interest can only be studied using infrared facilities like SOFIA.
“During the February third flight, the target objects ranged from a young planetary system around the naked-eye star Vega, only 25 light years from us, to an infant star 1,500 light years away in the Orion star forming region,” said Erick Young, SOFIA’s Science Mission Operations Director, describing the science conducted on Cycle 4’s inaugural flight. “We also observed a supermassive black hole hidden behind dense dust clouds in the center of a galaxy 170 million light years away.”
Scientists from the University of Georgia, University of Arizona, University of Texas at San Antonio, and the Space Telescope Science Institute in Baltimore, plus their collaborators from institutions in the United States and Europe, obtained data using the Faint Object Infrared Camera for the SOFIA Telescope (FORCAST) mounted on SOFIA’s telescope for imaging and spectroscopic observations during the flight.
Later in Cycle 4, the SOFIA observatory is scheduled to deploy to the Southern Hemisphere for seven weeks in June and July 2016, with 24 science flights planned from a base at Christchurch, New Zealand. There, scientists will have the opportunity to observe areas of interest such as the Galactic Center and other parts of the Milky Way that are not visible or difficult to observe from the Northern Hemisphere.
The far-infrared High-resolution Airborne Wideband Camera-plus (HAWC+) will be added to SOFIA’s suite of seven cameras, spectrometers, and high-speed photometers during the latter part of Cycle 4. HAWC+’s optics, state-of-the art detector arrays, and upgradability will permit a broad range of important astrophysical investigations, including the unique and powerful capability of mapping magnetic fields in molecular clouds.
SOFIA is a joint project of NASA and the German Aerospace Center (DLR). NASA’s Ames Research Center in Moffett Field, California, manages the SOFIA program. The aircraft is based at NASA’s Armstrong Flight Research Center’s facility in Palmdale, California. NASA Ames manages the SOFIA science and mission operations in cooperation with the Universities Space Research Association (USRA) headquartered in Columbia, Maryland, and the German SOFIA Institute (DSI) at the University of Stuttgart.
For a list of science programs selected for Cycle 4, visit:
For more information about SOFIA, visit:
For information about SOFIA’s science mission, visit:
http://www.sofia.usra.edu • http://www.dsi.uni-stuttgart.de/index.en.html
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