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Hubble Space Telescope |
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Hubble Space Telescope![]() Successive observations with Hubble's wide-field and planetary camera (WFPC) produced this image of the Bubble Nebula (NGC 7635). The spherical boundary region is formed as an expanding shell of particles thrown off by the star within. ![]() The Hubble wide-field planetary camera was used to capture this image of planetary nebula NGC 6751, in the constellation of Aquila. The gases were ejected by the central star several thousand years ago. ![]() The Hubble Space Telescope photographed shortly after its release from the space shuttle Discovery's robot arm, following its third servicing mission (STS-103) in December 1999. The telescope's failed gyroscopes were replaced, its computer upgraded, and other new components installed. Space-based astronomical observing facility, orbiting the Earth at an altitude of 610 km/380 mi. It consists of a 2.4 m/94 in telescope and four complementary scientific instruments, is roughly cylindrical, 13 m/43 ft long and 4 m/13 ft in diameter, and has two large solar panels. HST produces a wealth of scientific data, and allows astronomers to observe the birth of stars, find planets around neighbouring stars, follow the expanding remnants of exploding stars, and search for black holes in the centre of galaxies. HST is a cooperative programme between the European Space Agency (ESA) and the US space agency NASA, and is the first spacecraft specifically designed to be serviced in orbit as a permanent space-based observatory. It was launched in 1990. It will re-enter the Earth's atmosphere some time after 2010 and be destroyed unless more servicing missions are flown to it – missions that are currently in doubt following the Columbia shuttle disaster. By having a large telescope above Earth's atmosphere, astronomers are able to look at the universe with unprecedented clarity. Celestial observations by HST are unhampered by clouds and other atmospheric phenomena that distort and attenuate starlight. In particular, the apparent twinkling of starlight, caused by density fluctuations in the atmosphere, limits the clarity of ground-based telescopes. HST performs at least ten times better than such telescopes and can see almost back to the edge of the universe and to the beginning of time (see Big Bang). Before HST could reach its full potential, a flaw in the shape of its main mirror, discovered two months after the launch, had to be corrected. In 1993, as part of a planned servicing and instrument upgrade mission, NASA astronauts aboard the space shuttle Endeavour installed a set of corrective lenses to compensate for the error in the mirror figure. COSTAR (corrective optics space telescope axial replacement), a device containing ten coin-sized mirrors, now feeds a corrected image from the main mirror to three of the HST's four scientific instruments. HST is also being used to detail the distribution of dust and stars in nearby galaxies, watch the collisions of galaxies in detail, infer the evolution of galaxies, and measure the age of the universe.
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Prof Brown's lecture, Our Magical Cosmos and How We Reveal its Tricks - From Freddy Flintstone to the Hubble Telescope and Beyond, promises to be both very informative and very entertaining. The students have also corresponded with a NASA astronaut and spoken with an engineer working to repair the Hubble telescope. One of the most important telescopes in the history of astronomy, the Hubble telescope has allowed observers to peer farther into space than any previous telescope. |
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