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Close Up of the Bubble Nebula
<< Yesterday 18.11.1998 Tomorrow >>
Close Up of the Bubble Nebula
Credit & Copyright: Hubble Heritage Team (AURA/ STScI/ NASA)
Explanation: It's the bubble versus the cloud. NGC 7635, the Bubble Nebula, is being pushed out by the stellar wind of massive central star BD+602522. Next door, though, lives a giant molecular cloud, visible above to the upper left. At this place in space, an irresistible force meets an immovable object in an interesting way. The cloud is able to contain the expansion of the bubble gas, but gets blasted by the hot radiation from the bubble's central star. The radiation heats up dense regions of the molecular cloud, causing the orange glow seen above. The Bubble Nebula is about 10 light-years across and part of a much larger complex of stars and shells. The Bubble Nebula can be seen with a small telescope towards the constellation of Cassiopeia.

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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.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: HII region - emission nebula - massivnye zvezdy - Molekulyarnye oblaka - oblasti ionizovannogo vodoroda
Publikacii so slovami: HII region - emission nebula - massivnye zvezdy - Molekulyarnye oblaka - oblasti ionizovannogo vodoroda
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