SOFIA
The Stratospheric Observatory for Infrared Astronomy

The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint U.S. and German project to develop and operate a 2.5 meter infrared airborne telescope in a Boeing 747-SP. SOFIA is designed to make sensitive infrared measurements of a wide range of astronomical objects. It will fly at and above 12.5 km, where the telescope collects radiation in the wavelength range from 0.3 micrometers to 1.6 millimeters. First science flights will begin in 2008 and the observatory is expected to operate for over 20 years.

UCLA has a significant and diverse role in SOFIA development and operations. The SOFIA Chief Scientist, Prof. Eric Becklin leads the team at UCLA and will become the first observatory director during the telescope's operational phase. UCLA Infrared Detector Laboratory has recently completed FLITECAM, a SOFIA first-light instrument that will be used for telescope testing and scientific research.

 

SOFIA Images: (click on any image below to view a full-size version)

sofia-thumb.jpg (9788 bytes)  The SOFIA aircraft, the "Clipper Lindbergh" currently undergoing modifications

sm-sofia2.jpg (12496 bytes)  The SOFIA primary mirror (lightweighted and polished)

flitecam-thumb.jpg (8849 bytes)  The FLITECAM Instrument installed on SOFIA co-mounted with HIPO

sm-sofia4.jpg (6519 bytes)  Results from FLITECAM tests at Lick Observatory (object S106)

1stflight-thumb.jpg (6519 bytes)  FLITECAM's 1st flight on SOFIA on October 13, 2011

 

The UCLA SOFIA team:

Faculty

Graduate Students

Administrative

Project Staff

Select Publications:

Contact the SOFIA Office at UCLA for a copy of one of the above publications

Links