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红矮星

与 红矮星 相关的网络例句 [注:此内容来源于网络,仅供参考]

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。

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

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。

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。

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

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。

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。

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。。。。

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。

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。

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他是我知道的人中最值得注意的人。

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