Ultraviolet Astronomy - Research Article from World of Scientific Discovery

This encyclopedia article consists of approximately 2 pages of information about Ultraviolet Astronomy.

Ultraviolet Astronomy - Research Article from World of Scientific Discovery

This encyclopedia article consists of approximately 2 pages of information about Ultraviolet Astronomy.
This section contains 537 words
(approx. 2 pages at 300 words per page)
Buy the Ultraviolet Astronomy Encyclopedia Article

Optical telescopes use mirrors and lenses to gather light for magnification. They have been in use for nearly 400 years. But visible light is a small part of the overall spectrum of electromagnetic waves. Beyond the violet portion of visible light are high-energy ultraviolet rays, X-rays and cosmic rays. Each wavelength gives a different "picture" of the sky. Very hot stars produce more energy in the ultraviolet wavelengths than in visible light. Consequently, what astronomers see is just a small part of the star's total energy output. To get a better understanding of the nature of celestial objects, observations in other wavelengths than the visual are necessary.

The ozone layer of the earth's atmosphere absorbs high-energy radiation; the only way to detect ultraviolet radiation is by satellite. The first opportunity to do so presented itself following World War II. Herbert Friedman (1916-) launched several captured German V-...

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This section contains 537 words
(approx. 2 pages at 300 words per page)
Buy the Ultraviolet Astronomy Encyclopedia Article
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Ultraviolet Astronomy from Gale. ©2005-2006 Thomson Gale, a part of the Thomson Corporation. All rights reserved.