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The James Webb Space Telescope builds on the
success of NASAs Great Observatories, a series of
orbiting telescopes that NASA began building in the 1980s as a way
of
seeing the cosmos at all wavelength bands. Each of these large, highly
sophisticated space telescopes looks at a specific window of the electromagnetic
spectrum from gamma rays to infrared. Webb is part of NASA's Origins program, which seeks to answer fundamental questions about the universe.
Chandra
X-Ray Telescope
The Chandra X-Ray Observatory formerly known as the
Advanced X-Ray Astrophysics Facility (AXAF) was deployed on
July 23, 1999. Chandra is looking at some of the most energetic objects
in the universe.
Hubble Space Telescope
Named after American astronomer Edwin P. Hubble, the Hubble
Space Telescope was launched in 1990 and has since found never-before-seen
stars and galaxies exceeding astronomers expectations.
With its suite of onboard instruments, Hubble is capable of seeing objects
emitting ultraviolet, visible, and infrared radiation.
Spitzer Space Telescope
Launched in August 2003, this infrared-detecting telescope is answering fundamental
questions about the birth and evolution of the universe. It can study
fetal stars, detect other solar systems, and examine ancient, distant
galaxies toward the edge of the universe. The primary Spitzer mission will continue until 2009, when the cryogens that cool the telescope -- essential for instruments that look for infrared radiation -- will be expended.
Compton Gamma Ray Observatory
The second of NASA's Great Observatories looked at
astronomical objects that emit gamma rays, the most
energetic form of light. Compton, whose mission
ended in June 2000 in a fiery reentry into Earth's
atmosphere, was at 17 tons the heaviest astrophysical
payload flown to date. Over 700 scientists used the
satellite and its instruments to survey the surrounding
universe. |