The Large Magellanic Cloud is about 15, 000 light-years across.
大麦哲伦星云的直径大约为 15000 光年。
It was seen in 1987 amid vast billows of gas in the Tarantula Nebula within the Large Magellanic Cloud.
1987年科学家们在大麦哲伦星云里的蜘蛛星云的波涛滚滚的巨大气云中观测到这颗超新星。
Stars a hundred times more massive than the sun Pierce the roiling haze of the Tarantula Nebula in the Large Magellanic Cloud.
那些比太阳大一百多倍的恒星穿过大麦哲伦星云里的蜘蛛星云中翻滚的烟雾。
The Small Magellanic Cloud, and its companion galaxy the Large Magellanic Cloud, are the two galaxies where this type of study is possible.
小麦哲伦星云和其伴生的大麦哲伦星云，是在可能进行这种研究的两个星系。
This infrared portrait of the Small Magellanic Cloud, taken by NASA's Spitzer Space Telescope, reveals stars and dust in this galaxy as never seen before. T.
美国宇航局的斯皮策太空望远镜拍摄的小麦哲伦星系的红外图像，揭示了这个星系中前所未见的恒星和尘埃。
The two bright objects that look like car headlights are a pair of stars in the Large Magellanic Cloud.
两个看上去像车灯的明亮的物体是在大麦哲伦星云中的一对恒星。
SN 1987A is sited in the nearby Large Magellanic Cloud, a dwarf galaxy adjacent to our own Milky Way Galaxy.
SN 1987A位于邻近的大麦哲伦星云，一个毗连我们银河系的矮星系。
The Small Magellanic Cloud isn't much to look at with the naked eye, even for visitors to the International Space Station.
小麦哲伦星云甚至对国际空间站的访客来说也不能用肉眼看清。
This tiny, bleak and diamond-shaped constellation, not far on the sky from the Large Magellanic Cloud, is often overlooked.
这个小而黯淡、在天球上离大麦云不远的钻石状星座，常常被人小瞧了。
Identified as E0102-72, the supernova remnant lies about 190,000 light-years away in our neighboring galaxy, the Small Magellanic Cloud.
名为e0102- 72的超新星遗骸，位在邻近的小麦哲伦星系内，离我们约有190,000光年远。
On February 23, 1987, astronomers got the next best thing: a supernova in one of the Milky Way's satellite galaxies, the Large Magellanic Cloud.
在1987年2月23日，天文学家获得了次佳的机会：银河系的卫星星系“大麦哲伦云”中，发生了一次超新星爆发。
On February 23, 1987, astronomers got the next best thing: a supernova in one of the Milky Way 's satellite galaxies, the large Magellanic cloud.
在1987年2月23日，天文学家获得了次佳的机会：银河系的卫星星系大麦哲伦云中，发生了一次超新星爆发。
Glowing visible filaments, shown in yellow, and X-ray hot gas, shown in blue, span about 30 light-years in our neighboring galaxy, the Large Magellanic Cloud.
可见光波段的发光丝状物，用黄色显示，X射线波段热气体，用蓝色显示，宽30光年，在我们的近邻星系大麦哲伦云中。
As Olsen's team will report in a future issue of the Astrophysical Journal, the Large Magellanic Cloud probably stole 5% of its stars from its smaller sibling.
奥尔森的研究小组在将要出版的一期《天体物理学杂志》上报道说，大麦哲伦星云很可能从它较小的兄弟星云那里偷窃了5%的恒星。
The new observations not only tell us what elements are being recycled into the Large Magellanic Cloud, but how it changes its environment on human time scales.
新的观察结果不仅告诉我们什么元素正在循环进入大麦哲伦星云，而且告诉我们按人类的时标它如何改变自己的环境。
Located in the Large Magellanic Cloud, a small satellite galaxy orbiting our Milky Way galaxy, the region's spidery appearance is responsible for its popular name, the Tarantula nebula.
该区域位于围绕我们所在的银河系旋转的一个卫星星系——大麦哲伦星云之中，其蛛网状的样子得来了这个人尽皆知的名字，蜘蛛星云。
Located in the Large Magellanic Cloud, a small satellite galaxy orbiting our Milky Way galaxy, the region's spidery appearance is responsible for its popular name, the Tarantula nebula.
该区域位于围绕我们所在的银河系旋转的一个卫星星系——大麦哲伦星云之中，其蛛网状的样子得来了这个人尽皆知的名字，蜘蛛星云。
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