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 to the right. 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 it to glow. The Bubble Nebula, pictured above in scientifically mapped colors to bring up contrast, 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 the Queen of Aethiopia (Cassiopeia).

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

Publikacii s klyuchevymi slovami: Bubble nebula - NGC 7635 - molecular cloud - tumannost' Puzyr' - Molekulyarnye oblaka Publikacii so slovami: Bubble nebula - NGC 7635 - molecular cloud - tumannost' Puzyr' - Molekulyarnye oblaka
Sm. takzhe: Ruka pomoshi v Kassiopee NGC 7635: tumannost' Puzyr' Temnyi Morskoi konek v Cefee IC 5146: tumannost' Kokon Tumannost' "Temnaya shtuchka" Temnaya tumannost' Lindsa LDN 1251 NGC 6188: drakony v Zhertvennike Vse publikacii na tu zhe temu >>