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31 grudnia 1997

NGC 5307: A Symmetric Planetary Nebula
Źródło: H. Bond (STScI) & R. Ciardullo (Penn State), WFPC2, HST, NASA

Opis: Some stellar nebulae are strangely symmetric. For example, every major blob of gas visible on the upper left of NGC 5307 appears to have a counterpart on the lower right. This picture taken by the Hubble Space Telescope was released last week. NGC 5307 is an example of a planetary nebula with a spiral shape. Spiral planetary nebulae are thought to be caused by a bright central white dwarf star expelling a symmetric wobbling jet of rapidly moving gas. It takes light about 10,000 years to reach us from NGC 5307, and about 6 months just to go from one side to the other. In contrast, light takes only about 8 minutes to reach Earth from the Sun.

Jutro: The Largest Rock Known


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Autorzy i wydawcy: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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