J.D. Harrington
Headquarters, Washington
202-358-5241
j.d.harrington@nasa.gov
Nicholas A. Veronico / Huong Nguyen
Ames Research Center, Moffett Field,
Calif.
650-604-4589/650-604-4789
nveronico@sofia.usra.edu /
huong.nguyen@nasa.gov
MOFFETT FIELD, Calif. -- The
Astrophysical Journal, a leading professional astronomy research publication,
will issue a special edition of its Letters volume on April 20 with papers
about observations made with NASA's Stratospheric Observatory for Infrared
Astronomy (SOFIA) airborne telescope.
SOFIA is a highly modified Boeing 747SP
aircraft that carries a telescope with a 100-inch (2.5-meter) diameter
reflecting mirror that conducts astronomy research not possible with
ground-based telescopes. By operating in the stratosphere at altitudes up to
45,000 feet, SOFIA can make observations above the water vapor in Earth's lower
atmosphere.
"This is really SOFIA's debut on
the world scientific stage," said Chris Davis, SOFIA program scientist at
NASA Headquarters in Washington. "World-class observatories such as the
Hubble, Chandra and Spitzer space telescopes had their Astrophysical Journal
special editions, and now SOFIA joins their prestigious ranks."
The eight SOFIA papers featured in the
special edition cover diverse research on topics including SOFIA's capabilities
as a flying observatory and its study of star formation in our galaxy and
beyond.
"Studies of star and planet
formation processes are one of SOFIA's 'sweet spots,'" said SOFIA Science
Mission Director Erick Young. "SOFIA's infrared instruments can see into
the dense clouds where stars and planets are forming and detect heat radiation
from their construction material. By getting above the Earth's atmospheric
water vapor layer that blocks most of the infrared band, SOFIA's telescope can
view the glow from forming stars at their strongest emission wavelengths."
The infrared images analyzed in these
papers were obtained with the FORCAST (Faint Object Infrared Camera for the
SOFIA Telescope) instrument during SOFIA's first science observations in
December 2010. Papers based on observations with SOFIA and the GREAT spectrometer
(German Receiver for Astronomy at THz Frequencies) will be published in a May
2012 special volume of the European journal Astronomy and Astrophysics.
SOFIA is a joint project of NASA and the
German Aerospace Center and is based and managed at NASA's Dryden Aircraft
Operations Facility in Palmdale, Calif. NASA's Ames Research Center at Moffett
Field, Calif., manages the SOFIA science and mission operations in cooperation
with the Universities Space Research Association, headquartered in Columbia,
Md., and the German SOFIA Institute at the University of Stuttgart.
For more information about SOFIA, visit http://www.nasa.gov/sofia
or www.sofia.usra.edu.
To view The Astrophysical Journal
Letters containing the SOFIA papers, visit http://iopscience.iop.org/2041-8205/749/2.
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