第119期: Brown Dwarf 褐矮星
日期:2023-05-14 13:36

(单词翻译:单击)

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A brown dwarf is a type of celestial object that can’t be classified as a planet or a star.

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褐矮星是一种天体,但它不能被归类为行星或恒星zpdE[R36!6Wh^_zI[whL

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Although brown dwarfs look more like planets, they form the same way stars do.

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虽然褐矮星看起来更像行星,但它们的形成方式与恒星相同dy4N8dp,fnx

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A star is created when a cloud of gas and dust begins to compress.

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当气体云和尘埃云开始收缩时,恒星就产生了A_v9-B[1d8^7Gu|

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The intense force of gravity causes the star’s core to fuse atoms together, producing helium.

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强烈的引力使恒星的核心将原子融合在一起,并产生氦MI3Z|7t5jS3y=A-wspFn

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Fusion is what causes a star to shine.

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聚变是恒星发光的原因vo+D011E|+7F|^B3fF

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Early in its life, a star fuses atoms of deuterium.

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在恒星生命的早期会发生氘原子聚变*IU#.Ogr+VPT

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It begins to use regular hydrogen as its core gets hotter.

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随着核心温度的升高,氢原子聚变就开始了+NK4NKHKEO

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However, brown dwarfs never reach this stage.

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然而,褐矮星从未达到这一阶段AAHCP3XCLx

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They stay at low temperatures and fuse deuterium until they run out.

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它们在低温下熔化氘,直到耗尽K2D_=eHOlBi&E

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Brown dwarfs produce very little light, which makes them hard to find.

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褐矮星发出的光很微弱,这使得它们很难被发现w3w[QBr7,#W2HfM-Bd|

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Scientists first theorized about brown dwarfs in 1963, but didn’t observe any until 1995.

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科学家在1963年首次提出了有关褐矮星的理论,但直到1995年才观测到褐矮星7]0NGv6YhJKNL|Eix^pw

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