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Hubble is a long-term, space-based observatory. Observations are carried out in visible, infrared and ultraviolet light. Hubble's orbit above the Earth's distorting atmosphere allows astronomers to make the very high resolution observations that are essential to open new windows to planets, stars and galaxies. |
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Named after Edwin Powell Hubble (1889-1953), one of the great pioneers of modern astronomy |
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| Type | Three-axis stabilised Space Observatory.Attitude control by four (of six) gyros at any one time plus three fine guidance sensors | ||
| Mass | Launch mass 11110 kg. | ||
| Size | Length: 15.9 m, diameter: 4.2 m. Two solar panels each 2.4 x 12.1 m |
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| Telescope | 2.4 m f/24 Ritchey-Chretien | ||
| WFPC2 | Wide Field/Planetary Camera 2 is an electronic camera working at two magnifications. It has four CCD detectors with 800 x 800 pixels. | ||
| STIS | Space Telescope Imaging Spectrograph provides images and spectra. It is sensitive to a wide range of light from UV to Infrared | ||
| NICMOS | Near Infrared Camera and Multi-Object Spectrometer provides images and spectra in the infrared. NICMOS uses cooled HgCdTe detectors. | ||
| FOC | FOC -The Faint Object Camera is a very high resolution camera built by ESA | ||
| Date | Cape Canaveral, 24 April, 1990, deployment 26 April | ||
| Vehicle | Space Shuttle Discovery (STS-31 ) | ||
| Circular, 593 km inclined at 28.5 degrees to the Equator. The time for one orbit is between 96 and 97 minutes | |||
| Daily on-orbit operations at NASA's Goddard Space Flight Center (GSFC) in Greenbelt.Science operations are co-ordinated by the Space Telescope Science Institute (STScI) in Baltimore. | |||