NASA's SOFIA Captures Images of the Planetary Nebula M2-9

Researchers using NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) have captured infrared images of the last exhalations of a dying sun-like star.

The object observed by SOFIA, planetary nebula Minkowski 2-9, or M2-9 for short, is seen in this three-color composite image. The SOFIA observations were made at the mid-infrared wavelengths of 20, 24, and 37 microns. The 37-micron wavelength band detects the strongest emissions from the nebula and is impossible to observe from ground-based telescopes.

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SOFIA Featured in Video Series

SOFIA is the subject of the new "Destination Innovation" video series produced at NASA Ames. Episode 2, "Window to the Hidden Universe," was produced by the Ames Video team with support from the Dryden Public Affairs video staff. The video is available on YouTube and VMIX.

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NASA Unveils Second Round of Women@NASA Honorees in Celebration of Women's History Month

To inspire and encourage young girls to enter science, technology, engineering and mathematics professions, NASA has expanded the Women@NASA program with a second round of honorees to showcase at its website.

The SOFIA team is proud to recognize SOFIA Project Scientist Pamela Marcum having been selected as a Women@NASA Honoree. Get to know Pamela Marcum here.

Learn more about Women@NASA here.

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Educators Selected to Fly on NASA's SOFIA Airborne Observatory

Release 12-027

Twenty-six educators from the United States have been selected for research flights aboard SOFIA, NASA's Stratospheric Observatory for Infrared Astronomy. As participants in the Airborne Astronomy Ambassadors program, the educators will partner with professional astronomers using SOFIA for scientific observations in 2012 and 2013.

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SOFIA Image of the Newborn Star Cluster W3A

Researchers using NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) have captured new images of a recently born cluster of massive stars named W3A. The cluster is seen (inset) lurking in the depths of the large gas and dust cloud from which it formed. The larger image shows the overall structure of the W3 region, lying 6,400 light years away in the direction of the constellation Perseus, as seen at near-infrared wavelengths by the Spitzer Space Telescope.

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SOFIA Peers in to the Heart of the Orion Nebula

A new image from NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) shows a complex distribution of interstellar dust and stars in the Orion nebula. Interstellar dust, composed mostly of silicon, carbon and other heavy elements astronomers refer to generically as “metals,” plus some ice and organic molecules, is part of the raw material from which new stars and planets are forming.

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Nov. 9/10: The Battle to Observe Betelgeuse

“SOFIA Flight 86 must rank as the most exciting observing nights that I have ever done!” said Graham M. Harper, an astrophysicist from the School of Physics, Trinity College, Dublin, Ireland, after his all-night expedition on Nov. 9/10. That's an impressive statement from a researcher who focuses on stellar activity in cool stars and routinely uses a variety of ground-based and space telescopes to capture energy ranging from the ultraviolet to centimeter radio wavelengths.

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SOFIA Flying Telescope Visits NASA Ames

The Stratospheric Observatory For Infrared Astronomy (SOFIA) landed at NASA's Ames Research Center for tours by NASA employees, members of the media and the general public. Housing a 17-ton telescope assembly, the highly modified Boeing 747SP aircraft is the largest flying telescope in the world. More than 6500 people visited SOFIA during her visit.

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SOFIA Heads Home

Deployment Update

NASA's Stratospheric Observatory for Infrared Astronomy, SOFIA, departed Joint Base Andrews, Md., on Sept. 23, 2011 at 3:15 p.m. local time, en route to its home base at the Dryden Aircraft Operations Center in Palmdale, Calif. The flight to Palmdale concludes SOFIA's first international deployment.

SOFIA is a highly modified Boeing 747SP aircraft that carries a telescope with a 100-inch (2.5-meter) reflecting mirror that conducts astronomy research not possible with ground-based telescopes.

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SOFIA on Display at Stuttgart, Germany

Deployment Update

SOFIA was flown from Cologne, Germany, home of the German Aerospace Center, to the Stuttgart Airport, home of the nearby German SOFIA Institute located at the University of Stuttgart on the morning of Sept. 19, 2011. No science was conducted during the short flight, approximately 290 km (180 miles) between the two cities.

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SOFIA Begins First International Deployment

SOFIA Mission Manager’s Update

On Sept. 16, at 10:10 a.m. local time, NASA’s Stratospheric Observatory for Infrared Astronomy, SOFIA, lifted off from its base at Palmdale, Calif., flying east en route to Cologne, Germany, for its first international deployment. After conducting astronomical research during the flight, SOFIA landed at the Cologne-Bonn Airport, shortly before 7 a.m. local time.

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NASA Flying Observatory Undergoes Mirror Inspections, Prepares for Deployment

SOFIA Mission Manager’s Update

The Stratospheric Observatory for Infrared Astronomy (SOFIA) has completed an avionics upgrade and is currently undergoing inspection and maintenance of its telescope assembly. Should the observatory’s mirror be cleared for flight and preflight operations proceed with no anomalies this week, SOFIA will depart for the German Aerospace Center’s annual open house to be held Sept. 18, in Cologne, Germany.

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SOFIA Successfully Observes Challenging Pluto Occultation

On June 23, NASA’s Stratospheric Observatory for Infrared Astronomy (SOFIA) observed the dwarf planet Pluto as it passed in front of a distant star. This event, known as an “occultation,” allowed scientific analysis of Pluto and its atmosphere by flying SOFIA at the right moment to an exact location where Pluto’s shadow fell on Earth.

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SOFIA HIPO & FDC observations of a stellar occultation by Pluto

On June 23, 2011 SOFIA observed an occultation by dwarf planet Pluto of a comparably bright (V ~ +14) star using two instruments simultaneously: HIPO (High Speed Photometer for Occultations; P.I. = Ted Dunham, Lowell Observatory) and FDC (Fast Diagnostic Camera; P.I. = Jürgen Wolf, DSI). The results were published in Person et al. 2013, Astrophysical Journal 146, 83.

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