File:Hubble carina star births.jpg: Difference between revisions
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; <big><big>''About Hubble and the Hubble Imaging Team''</big></big> | ; <big><big>''About Hubble and the Hubble Imaging Team''</big></big> | ||
[[File:Hubble @25.png | link=http://www.stsci.edu/hst]] | [[File:Hubble @25.png | link=http://www.stsci.edu/hst]] | ||
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''STIS is a versatile imaging spectrograph, providing spatially resolved spectroscopy in the UV and optical, high spatial resolution echelle spectroscopy in the UV, solar-blind imaging in the UV, and direct and coronagraphic imaging in the optical.'' | ''STIS is a versatile imaging spectrograph, providing spatially resolved spectroscopy in the UV and optical, high spatial resolution echelle spectroscopy in the UV, solar-blind imaging in the UV, and direct and coronagraphic imaging in the optical.'' | ||
''http://www.stsci.edu/hst'' | ''* http://www.stsci.edu/hst'' | ||
''* http://www.greenpolicy360.net/w/Hubble'' | |||
[[File:Carina.jpg]] | |||
[[Category:Green Graphics]] | [[Category:Green Graphics]] | ||
[[Category:NASA]] | |||
[[Category:Origins of Life]] | |||
[[Category:Planetary Science]] | [[Category:Planetary Science]] | ||
[[Category:Space Science and Space Physics]] | [[Category:Space Science and Space Physics]] |
Latest revision as of 18:38, 26 June 2020
- About Hubble and the Hubble Imaging Team
Iconic Images Are Actually Black-and-White
https://www.youtube.com/watch?v=fDwkDZ5dx-c (video)
How Hubble's imaging goes from black-and-white to color
By analyzing the wavelengths of light that different elements emit in space, 'dull' pictures of our universe are turned into colorful masterpieces
About Zolt Levay of the Imaging Team at the Space Telescope Science Institute
The Space Telescope Imaging Spectrograph (STIS) was installed onboard HST during Servicing Mission (SM) 2 in 1997 and operated until an electronic failure in 2004. It resumed operations with all ultraviolet and optical channels in 2009 after it was successfully repaired...
STIS is a versatile imaging spectrograph, providing spatially resolved spectroscopy in the UV and optical, high spatial resolution echelle spectroscopy in the UV, solar-blind imaging in the UV, and direct and coronagraphic imaging in the optical.
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