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超級氣泡
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超級氣泡

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thumb|220x220px|The superbubble Henize 70, also known as N70 or DEM301, in the [[Large Magellanic Cloud]] In astronomy a superbubble or supershell is a cavity which is hundreds of light years across and is populated with hot (106 K) gas atoms, less dense than the surrounding interstellar medium, blown against that medium and carved out by multiple supernovae and stellar winds. The winds, passage and gravity of newly born stars strip superbubbles of any other dust or gas. The Solar System lies near the center of an old superbubble, known as the Local Bubble, whose boundaries can be traced

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超級氣泡是天文學的術語,用來描述橫越數百光年,被數顆超新星和恆星風充滿了106 K氣體的空洞。太陽系就位在一個古老的,被稱為本地泡的超級氣泡的中心,它的邊界在數百光年的距離之外,可以追蹤使恆星消光的塵埃突然增加的區域來界定。

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