Explanation: 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.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: planetary nebula - dzhet - Planetarnaya tumannost' - belyi karlik Publikacii so slovami: planetary nebula - dzhet - Planetarnaya tumannost' - belyi karlik
Sm. takzhe: M27: eto ne kometa Porfirion: samyi dlinnyi dzhet ot chernoi dyry Dzhons-Emberson-1 Galaktika, dzhet i znamenitaya chernaya dyra Akkreciruyushaya chernaya dyra s dzhetom Kol'ca vokrug tumannosti Kol'co HFG1 i Eibell 6: planetarnye tumannosti Vse publikacii na tu zhe temu >>