- 更多网络例句与红矮星相关的网络例句 [注：此内容来源于网络，仅供参考]
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Aurelia is the planet of a red dwarf, a star much cooler than our own sun.
"奥里里亚"是一颗红矮星的行星。
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But how do relatively rare titans such as Betelgeuse emerge from the same stuff that usually yields batches of sun-sized orbs and even more common red dwarfs?
但是象参宿四那样相对稀少的巨型恒星是如何出现的呢？同样多的物质材料通常可以产生一批象太阳大小的天体，甚至可以产生更多的普通红矮星。
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This allowed the host star to be identified as a red dwarf star located 19,000 light-years away .
这一发现终于确定了主要恒星--发出光线的那个恒星--的身份，就是红矮星，距离我们19000光年。
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The rising red dwarf star shows expected stellar magnetic activity which includes dramatic and violent prominences .
上升中的红矮星有著可预期的磁场活动，包含了激烈的日珥现象。
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Even at that, it'd be a red dwarf star. These red dwarfs are thought to make up 75% of the Milky Way galaxy's stars, but these stars are so small and faint that not a single one can be seen with the unaided eye!
人们认为75%银河系是由红矮星构成的，但是由于它们是那么的小且发出光也不强，所以很难直接用肉眼识别出一颗红矮星。
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They found that the cool stars, both the M-dwarf stars and browndwarfs, showed no hydrogen cyanide at all, while 30 percent of thesun-like stars did.
他们发现所有的寒冷恒星，无论是M型红矮星还是棕矮星，全都没有HCN分子踪迹，而类太阳恒星周围，只有30%左右的没有发现HCN。
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They found that the cool stars, both the M-dwarf stars and brown dwarfs, showed no hydrogen cyanide at all, while 30 percent of the sun-like stars did.
他们发现所有的寒冷恒星，无论是M型红矮星还是棕矮星，全都没有HCN分子踪迹，而类太阳恒星周围，只有30%左右的没有发现HCN。
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Spectral type is O ﹑ B ﹑ A dwarf star known as the blue dwarf star (such as Vega ﹑ Sirius), spectral type is F ﹑ G dwarf star known as the yellow dwarf star, spectral type as K and later the dwarf star called red dwarf star (such as the South Gate diethylamino star )...
光谱型为O﹑B﹑A的矮星称为蓝矮星﹐光谱型为F﹑G的矮星称为黄矮星﹐光谱型为K及更晚的矮星称为红矮星。。。。
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The researchers detected hydrogen cyanide molecules in disks circling yellow stars like our sun -- but found none around cooler and smaller stars, such as the reddish-colored "M-dwarfs" and "brown dwarfs" common throughout the universe.
研究人员在类似太阳的黄色恒星周围的星云盘中检测到了HCN，但在更冷更小的恒星——比如遍布宇宙的M型红矮星和棕矮星——周围却没有找到HCN踪迹。
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The researchers detected hydrogen cyanide molecules in disks circlingyellow stars like our sun -- but found none around cooler and smallerstars, such as the reddish-colored "M-dwarfs" and "brown dwarfs" commonthroughout the universe.
研究人员在类似太阳的黄色恒星周围的星云盘中检测到了HCN，但在更冷更小的恒星——比如遍布宇宙的M型红矮星和棕矮星——周围却没有找到HCN踪迹。
- 更多网络解释与红矮星相关的网络解释 [注：此内容来源于网络，仅供参考]
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red dwarf star：红矮星
原来这颗灰暗的'太阳' 就在我们不远处, 就我看到的资料, 这暗淡无光的红矮星(red dwarf star) 就在我们太阳的一至三光年的距离左右, 但近这几年, 这颗星已迈向她的死亡边沿, 在始踏入棕色矮星(brown dwarf) 的行列.
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swell：膨胀
据推断,有些星星老化时会膨胀(swell)成为一个红巨星(red giant star), 然后它的外层(outer layer)脱落,剩下一个走向消亡的矮星(dwarf star). 不过,这个矮星仍会经过几十亿年才最终从人类的视野内淡出(fade).
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red giant：红巨星濒临死亡的低温恒星,直径已经膨胀到太阳的几十倍甚至上百倍
red dwarf红矮星低质量的主序星,比太阳小得多,冷得多,也... | red giant红巨星濒临死亡的低温恒星,直径已经膨胀到太阳的几十倍甚至上百倍. | red supergiant红超巨星濒临死亡的大质量恒星,温度很低,直径为太阳的上百倍...