钱德拉太太已经收到了发给她5个孩子每人一件的毛衫，并且说这样一来冬天就不会那么难过了。
Mrs. Chandra has received one sweater for each of her five children and says that the winter will not be so hard now.
当一颗白矮星以这种方式增长到足够的质量时，它将达到钱德拉·塞卡极限。
When a White Dwarf takes on enough mass in this manner, it reaches a level called the chandrasekhar limit.
钱德拉能检测和成像数十亿光年之遥的X射线源。
Chandra detects and images X-ray sources that are billions of light years away.
这项钱德拉的研究要比先前的X射线观测深入很多。
This Chandra study is much deeper than previous X-ray observations.
这项钱德拉的研究要比先前的X射线观测深入很多。
ThisChandra study is much deeper than previous X-ray observations.
钱德拉X射线天文台能观测到堕落黑洞之前的微粒。
Image above: the Chandra X-ray Observatory can observe particles right before they fall into a black hole! Credit: NASA.
钱德拉X射线天文站正在庆祝它探索未知宇宙10周年。
Chandra X-ray Observatoryis celebrating 10 years of exploring the invisible universe.
美国宇航局的钱德拉X射线天文台本月迎来十周年庆典。
Nasa's Chandra X-ray Observatory celebrates its 10th anniversary this month.
钱德拉镜面是有史以来最大、排列最精确、最平稳的镜面。
The mirrors on Chandra are the largest, most precisely shaped and aligned, and smoothest mirrors ever constructed.
想要进一步了解NASA的钱德拉X射线天文台，请访问。
For more information about NASA's Chandra X-ray Observatory, visit.
最近有一个新的，天文站建成了，它叫做，钱德拉x射线观察站。
A very new observatory was launched only recently, and that is called the Chandra X-ray observatory.
钱德拉最近做了个，蟹状星云的图，中子星的图，我现在给你们看。
And Chandra made a picture very recently of the Crab Nebula, of the pulsar, and that's what I want to show you now.
普拉昌达的竞争对手拉姆·钱德拉·鲍德尔是尼泊尔国会党的领导人。
His rival is Ram Chandra Poudel, who heads the Nepali Congress party, which was in the coalition government that succeeded Prachanda's.
钱德拉岛（图像右中部）的沿海生态系统处于浮油的威胁之列。
Among the coastal ecosystems threatened by the spill are the Chandeleur Islands (image right center).
如果地球表面和钱德拉镜面一样平滑，那么所谓最高山峰也不足6英尺！
If the surface of Earth was as smooth as the Chandra mirrors, the highest mountain would be less than six feet tall!
但是我觉得这一演示引人注意的是，我从未见过仙人·钱德拉与人直接的互动。
But what I found notable about the demo was that I never saw Rishi Chandra actually interacting with anything directly.
钱德拉高敏度性能，使得我们想了解黑洞、超新星、暗物质更多细节成为可能。
Chandra's improved sensitivity is making possible more detailed studies of black holes, supernovas, and dark matter.
钱德拉X射线观测被用于查找和表述那个质量超过300万个太阳的惊人黑洞。
Chandra X-ray observations were used to find and characterise the whopping black hole with a mass of more than 3 million SUNS.
在这个图像中，钱德拉的X射线以蓝色显示并且以哈勃望远镜的光学成像为背景。
In this image, X-rays from Chandra are shown in blue and are overlaid on an optical image from the Hubble Space Telescope.
杀害马诺基和巴布里的凶手在很大程度上是有新郎的母亲。钱德拉帕提坚持追捕。
The killers of Manoj and Babli were pursued largely at the insistence of the groom's mother, Chandrapati.
杀害马诺基和巴布里的凶手在很大程度上是有新郎的母亲.钱德拉帕提坚持追捕。
The killers of Manoj and Babli were pursued largely at the insistence of the groom’s mother, Chandrapati.
2002年，钱德拉提供的数据推动了两个相距仅3,000光年的合并黑洞的发现。
In 2002, Chandra data led to the discovery of two merging black holes, which are a mere 3,000 light years apart.
2002年，钱德拉提供的数据推动了两个相距仅3,000光年的合并黑洞的发现。
In 2002, Chandra data led to the discovery of two merging black holes, which are a mere 3, 000 light years apart.
当电子通过被磁化的星云时释放出能量，造就出“钱德拉”望远镜所看到的精致的星云。
As the electrons move through the magnetized nebula, they radiate away their energy and create the elaborate nebula seen by Chandra.
美国宇航局钱德拉X射线天文台(紫)以及光学数据：哈勃空间望远镜(红，绿，蓝)。
Data from NASA's Chandra X-ray Observatory (purple) are shown here along with optical data from the Hubble Space Telescope (red, green, blue).
这张照片是多张钱德拉天文台的照片合成的，显示的是130光年远的银河系的中心部分。
This image was produced by combining a dozen Chandra observations made of a 130-light-year region in the center of the Milky Way.
钱德拉探测到环绕M 87的星团充斥着炙热的气体所发出的X射线(在图像中呈蓝色)。
The cluster surrounding M87 is filled with hot gas glowing in X-ray light (and shown in blue) that is detected by Chandra.
组成这幅猫眼星云图像的数据来自NASA的两个伟大的观察站-钱德拉和哈勃太空望远镜。
This image of the Cat's Eye Nebulawas made by combining data from two of NASA's GreatObservatories — Chandra and the Hubble Space Telescope.
这幅仙王座B的合成图像结合了来自钱德拉X射线观测站和斯皮茨太空望远镜所获得的数据。
This composite image of Cepheus B combines data from the Chandra X-ray Observatory and the Spitzer Space Telescope.
当一颗白矮星以这种方式增长到足够的质量时，它将达到一个称为钱德拉·塞卡极限的质量标准。
When a White Dwarf takes on enough mass in this manner it reaches a level called the chandrasekhar limit.
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