envelope star 中文意思是什麼
envelope star
解釋
氣殼星-
At the point c, the star develops a convection zone extending from near the surface deep into the extended envelope.
在C點，星體產生一個對流區，從表面附近向內擴展到廣袤的包層。 -
In this model, the resulting implosion and ensuing explosion would blow off the outer envelope of the star and leave behind the core as a neutron star.
按此模型，引起的突然壓縮和隨后的爆發會把恆量的外部包層吹跑，留下的核成為一顆中子星。 -
Not all parts of the star exhibit continued shrinkage; sometimes the stellar core will continue to shrink while the envelope expands, and vice versa.
並非星體每個部分都收縮，有時星核不斷收縮而殼層卻在膨脹，或者相反。 -
At the end of the process a carbon core of the star will be surrounded by a shell where helium is still being fused into carbon, which in turn is surrounded by and envelope where hydrogen is converted into helium
該過程結束時碳的星核會被一層仍然在進行氦聚變為碳的殼層包圍，而在這個氦-碳聚變層的外面還包圍著一層由氫-氦聚變層。 -
The helium core of the star starts to collapse. this gravitational contraction will heat up the hydrogen envelope surrounding the core. fusion therefore begins in the envelope and the star expands
剩下的氦核心便會開始塌縮並產生熱，緊鄰核心的氫外殼會被加熱而開始有熱核反應恆星亦同時膨脹。 -
When helium burning takes over the main burden of energy generation in the star, the core expands somewhat, and the envelope contracts somewhat.
當氦燃燒成為星體能量產生的主要來源時，核心略微膨脹，而包層略微收縮。 -
At the point c, the star develops a convection zone extending from near the surface deep into the extended envelope
在c點，星體產生一個對流區，從表面附近向內擴展到廣袤的包層。
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