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The Spitzer Space Telescope, formerly the Space Infrared Telescope Facility (SIRTF), was an infrared space telescope launched in 2003, that was deactivated when operations ended on 30 January 2020. [ 5 ] [ 9 ] Spitzer was the third space telescope dedicated to infrared astronomy, following IRAS (1983) and ISO (1995–1998).
The nebula is visible as a hazy patch in a small telescope, while a larger aperture will show a pair ... An infrared image of NGC 1333 by the Spitzer Space Telescope.
SOFIA had a larger aperture than Spitzer, but lower relative sensitivity. The Fermi Gamma-ray Space Telescope (FGRST), formerly known as the Gamma Ray Large Area Space Telescope, is a follow-on to Compton launched on 11 June 2008. [18]
Everyone has seen the incredible photos of space and the galaxies beyond thanks to the groundbreaking technology of the Hubble space telescope. The Hubble only views visible light, but there are ...
The Spitzer Space Telescope (formerly the Space Infrared Telescope Facility, SIRTF) is an infrared space observatory launched in 2003. It is the fourth and final of ...
Five-hundred-meter Aperture Spherical Radio Telescope: 2013 Duyun, Pingtang County, Guizhou Province, China Félix Aguilar Observatory: 1965 San Juan, Argentina: Fernbank Observatory: Atlanta, Georgia, US Fermi Gamma-ray Space Telescope: 2008 Low Earth orbit: Fick Observatory: 1966 Boone, Iowa, US Five College Radio Astronomy Observatory ...
Later, NASA designated IPAC as the U.S. science support center for the European Infrared Space Observatory (ISO), which ceased operations in 1998. About that same time, IPAC was designated as the science center for the Space Infrared Telescope Facility (SIRTF) -- renamed the Spitzer Space Telescope after launch.
This image from NASA Spitzer Space Telescope, shows the wispy filamentary structure of Henize 206 which is a small satellite galaxy gravitationally bound to the Milky Way galaxy. The SSPSF (stochastic self-propagating star formation) model of star formation was proposed by Mueller & Arnett [ 1 ] in 1976, generalized afterward by Gerola & Seiden ...