Hubble Space Telescope
The Hubble Space Telescope is a telescope in orbit around the Earth. Its position outside the Earth's atmosphere allows it to take extremely sharp images, and since its launch in 1990, it has become one of the most important telescopes in the history of astronomy. It has been responsible for many ground-breaking observations and has helped astronomers achieve a better understanding of many fundamental problems in astrophysics.
Scientific results
Important discoveries
Hubble has helped to resolve some long-standing problems in astronomy, as well as turning up results that have required whole new theories to explain them. Among its primary mission targets was to measure distances to Cepheid variable stars more accurately than ever before, and thus constrain the value of the Hubble constant, the measure of the rate at which the universe is expanding, which is also related to its age. Before the launch of Hubble, estimates of the Hubble constant typically had errors of up to 50%, but Hubble measurements of Cepheid variables in the Virgo cluster and other distant galaxy clusters provided a measured value with an accuracy of 10%, which is consistent with other accurate measurements made since Hubble's launch using other techniques.
Related Topics:
Cepheid variable - Hubble constant - Error - Virgo cluster
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While Hubble helped to refine the age of the universe, it also threw doubt on its future. Astronomers using the telescope to observe distant supernovae uncovered evidence that far from decelerating under the influence of gravity, the universe may in fact be accelerating. This acceleration was later confirmed by other ground-based and space-based telescopes, but the cause of this acceleration is currently very poorly understood.
Related Topics:
Supernova - Gravity
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The collision of Comet Shoemaker-Levy 9 with Jupiter in 1994 was very fortuitously timed for astronomers, coming just a few months after Servicing Mission 1 had restored Hubble's optical performance. Hubble images of the planet were sharper than any taken since the passage of Voyager 2 in 1979, and were crucial in studying the dynamics of the collision of a comet with Jupiter, an event believed to occur once every few centuries.
Related Topics:
Comet Shoemaker-Levy 9 - Jupiter - 1994 - Voyager 2 - 1979
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Other major discoveries made using Hubble data include proto-planetary disks (proplyds) in the Orion Nebula; evidence for the presence of extrasolar planets around sun-like stars; and the optical counterparts of the still-mysterious gamma-ray bursts.
Related Topics:
Proplyd - Orion Nebula - Extrasolar planet - Gamma-ray burst
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Impact on astronomy
Many objective measures show the enormous impact of Hubble data on astronomy. Over 4,000 papers based on Hubble data have been published in peer-reviewed journals, and countless more have appeared in conference proceedings. Looking at papers several years after their publication, about one-third of all astronomy papers have no citations, while only 2% of papers based on Hubble data have no citations. On average, a paper based on Hubble data receives about twice as many citations as papers based on non-Hubble data. Of the 200 papers published each year which receive the most citations, about 10% are based on Hubble data {{ref|newsletter}}.
Related Topics:
Conference - Citation
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Although the HST has clearly had a significant impact on astronomical research, the financial cost of this impact has been very large. A study on the relative impacts on astronomy of different sizes of telescopes found that while papers based on HST data generate 15 times as many citations as a 4 m ground-based telescope such as the William Herschel Telescope, the HST cost about 100 times as much to build and maintain {{ref|Benn}}. The development of adaptive optics in recent years means that ground-based telescopes can take images approaching the sharpness of Hubble images, at much lower cost, and this has been a key consideration in the debate about the future of space telescopes (see below).
Related Topics:
William Herschel Telescope - Adaptive optics
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~ Table of Content ~
| ► | Introduction |
| ► | Conception, design and aims |
| ► | Flawed mirror |
| ► | Servicing missions and new instruments |
| ► | Scientific results |
| ► | Using the telescope |
| ► | Hubble data |
| ► | Outreach activities |
| ► | The future |
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