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与 星云的 相关的网络例句 [注:此内容来源于网络,仅供参考]

In fact, the Carina Nebula is one of our galaxy's largest star-forming regions and home to young, extremely massive stars, including the still enigmatic variable Eta Carinae , a star with well over 100 times the mass of the Sun.

事实上,船底座星云也是银河系最大恒星诞生区域的一部分,也是年轻、极大质量恒星的家园,其中含有仍处于神秘变换中的船底座η星,其质量是太阳质量的100多倍。

The more famous nebula is M78, near the image center, cataloged over 200 years ago.

二者中较著名的星云是位在影像中央的M78,早在二百多年前就被登录了,位在影像左上角的则是较不出名的NGC 2071。

The most plausible explanation is that the cluster contains a distinct ring of dark matter without any accompanying ordinary matter.

最大似是而非的解释是星云包含了一个分离的暗物质的环没有任何相邻的普通物质。

The greater nebula, also known as M8 and NGC 6523, is named "Lagoon" for the band of dust seen to the left of the open cluster's center.

更大的星云,像M8和已知的星系6523,名为&乐园&,可以看到的疏散星团的中心有尘埃带。

Of course , in this well-studied example of a planetary nebula , the glowing material does not come from planets .

当然,在这个被细致地研究过的行星状星云样本中,炽热的物质并非来自行星,而是一颗正在死亡的太阳型恒星向外扩散的气壳。

The inner filaments visible above are being ejected by strong wind of particles from the central star. The outer disk contains unusual light-year long orange filaments.

影像中清楚可见的星云内层丝状结构,是强烈恒星风所抛出的的中心星物质,而外层碟状区,有许多长度有一光年长的奇特橘色指状物。

The long exposure used to create the above photograph makes the light from the left, reflected from Phoenix, Arizona, USA, appear like a sunset. Far in the distance, however, are star clouds from the disk of our Milky Way Galaxy.

亚利桑那州凤凰城的灯光从云层反射,造成类似日落时分的景象;遥远的后方则为我们银河系盘面上的星云。

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。

The Carina Nebula is home to young, extremely massive stars, including the still enigmatic variable Eta Carinae, a star with well over 100 times the mass of the Sun.

船底座星云是极大质量年轻恒星的家园,范例之一为神秘莫测的变星海山二星(船底座η,Eta Carina),该星的质量为太阳的百倍以上。

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