BLAST (telescope)
From Wikipedia, the free encyclopedia
The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) is a submillimeter telescope that hangs from a high altitude balloon. It has a 2 meter primary mirror that directs light into bolometer arrays operating at 250, 350, and 500 µm. The project is being carried out by a multi-university consortium headed by the University of Pennsylvania and the University of Toronto which also includes Brown University, the University of Miami, the University of British Columbia, JPL, INAOE, and Cardiff University.
BLAST's primary science goals are (from the BLAST Public Webpage):
- Measure photometric redshifts, rest-frame FIR luminosities and star formation rates of high-redshift starburst galaxies, thereby constraining the evolutionary history of those galaxies that produce the FIR/submillimeter background.
- Measure cold pre-stellar sources associated with the earliest stages of star and planet formation.
- Make high-resolution maps of diffuse galactic emission over a wide range of galactic latitudes.
- Observe solar system objects including planets, large asteroids, and trans-Neptunian objects.
BLAST's first flight was an engineering (test) flight. BLAST launched at approximately 15:10 UTC September 28 2003 from the Columbia Scientific Balloon Facility base in Fort Sumner, New Mexico, and landed approximately 26 hours later in north western New Mexico.
BLAST's second flight was its first scientific flight. BLAST launched at 1:10 UTC June 12 2005 from Esrange, near Kiruna, Sweden and landed at 6:15 UTC June 16 2005 on Victoria Island, Northwest Territories, Canada.
BLAST's third flight was its second scientific flight. BLAST launched at 1:54:10 UTC December 21 2006 from McMurdo Station, Antarctica and landed at 1:05 UTC January 2 2007 756 km southwest of McMurdo.
Filmmaker Paul Devlin is making a documentary film about BLAST. A preview can be seen here.
