尘埃是老年恒星风暴和超新星的产物。
Dust is produced from the winds of aging stars and from the aftermath of supernovae.
研究队伍用定位距离地球最远的超新星的办法来绘制宇宙地图。
The research teams raced to map the Universe by locating the most distant supernovae.
在这个地址正不断上传着这颗不断演化的超新星的照片。
这一发现可以帮助我们了解中子星如何从超新星的剧烈爆炸中诞生.
“This discovery helps us understand how neutron stars are born in violent supernova explosions,” astrophysicist Craig Heinke of the University of Alberta said in a press release.
由于形成Ia型超新星的特殊环境，它们也是显著同一的。
They're also remarkably uniform, thanks to the special circumstances that engender them.
超新星的残骸位于银河系的平面内，距离地球2600光年。
The supernova remnant is within the plane of our Milky way Galaxy and is 2,600 light-years away.
不论裘德·洛演出生涯的下一步将是什么，这颗新星的未来肯定灿烂眩目。
Whatever Jude Law's next career move may be, the future certainly looks bright for the rising young star.
银幕上，米高梅通过给她配备最好的摄影师和造型师来增加这位新星的神秘感。
On screen, MGM enhanced the mystique of its new star by teaming her with the best photographers and designers.
然而，如果超新星的残核大于三个太阳质量，按常规物理法则来说，就将成为黑洞。
However, if the supernova remnant exceeds three solar masses, conventional physics suggests a black hole should be left behind.
该星云是超新星的遗迹，是一个大质量的恒星死亡爆炸时的扩散云气形成的。
The nebula is a large supernova remnant, an expanding cloud born of the death explosion of a massive star.
这些记录被后人加以分析，找到了准确的位置，并发现了一颗超新星的残骸。
Then those findings were later reviewed, the old location pinpointed, and the remnants of a supernova found.
由于其质量亏损而产生的能量辐射可用来解释超新星的爆发等一些天文现象。
Energy radiation produced by mass defect can be used to explain some astronomical astronomical phenomena such as the eruption of supernova.
换句话说，基于现有的宇宙模型，超新星的实际距离要比其红移显示的距离远。
In other words, the supernovae were further away than their red-shifts indicated they should be, based on the existing model of the universe.
这个出乎意料的发现是因为发现超新星的亮度(表示距离)和以前的理论不相符。
That unexpected finding was the result of studies of supernovas whose apparent brightness (and therefore distance) did not match the previous theory.
有关超新星的研究使科学家了解到，追溯到90亿前暗能量就已经开始影响星系。
Supernovae studies have allowed scientists to see that dark energy has been impacting galaxies since as far back as nine billion years ago.
在二十世纪五十年代，这个超新星的残骸依然可以借助天文望远镜的帮助观测到。
In the 1950s, the remnants of the supernova could be seen again with the help of telescopes.
第三，新星的高重量值可能意味着它由铁组成，正好适合用火神并且是一名铁匠来命名。
Third, its high mass probably means it is made of iron, an appropriate material for a planet named after a divine Smith.
同样，此事件引发对这个二十八岁的，正在亚洲影界冉冉上升的新星的公众的强烈反应。
There was also a huge public backlash against the 28-year-old who has been one of the rising young stars of Asia cinema.
在一则流言中，曼联被指是格策潜在的买家之一，而尤文图斯得到这位新星的可能性最大。
United have been mentioned among potential suitors, but this report says Juventus lead the pack.
在确定这是一颗超新星后又过了近半个世纪，天文学家终于弄清楚了这颗超新星的演变过程。
Then almost a half-century after determining that it was a supernova, astronomers figured out how the supernova proceeded.
这幅由哈勃空间望远镜摄于1991年的图像捕捉到了天鹅座Loop超新星的一小段残骸。
This 1991 image from NASA's Hubble Space Telescope captures a small section of the Cygnus Loop supernova remnant.
他们注意到新星的行为不像以往那样千篇一律和不灵活，而是表现出一种对大自然探索的愉悦。
They all watched as his behavior changed from stereotypic and inactive behavior to a beautiful exhibition of natural exploratory behavior and delight.
在任一给定的星系中观测到Ia型超新星的机会是很小的，每个星系每千年预期只有一到两次。
The chance of observing a type Ia supernova in any given galaxy is low. Only one or two are expected to pop off per galaxy per millennium.
在那个星系的中心，新星的诞生比我们银河系的新星诞生速度要快10倍，集合了一大堆的新星。
In the galaxy's centre, young stars are being born 10 times faster than they are inside our Milky Way galaxy, resulting in a huge concentration of young stars.
正如电视观众所设计的梦幻球队一样，新星的创始人约翰•杜费尔德网罗了他认为业内最佳的基金经理。
Rather like the fantasy sports teams devised by armchair fans, its founder, John Duffield, recruited people he believed to be the best fund managers in the business.
如果得到证实，新发现的超新星的研究可以在早期宇宙中的恒星形成重大影响的计算机模型，纽金特说。
If confirmed, studies of the newfound supernova could have major implications for computer models of star formation in the early universe, Nugent said.
如果这种双星系统就是这类罕见的亚型超新星的起源，我们将会发现这类奇异的双星系统和超新星具有相同的频率。
If this is the progenitor of these rare subclass of supernova, we expect to be finding these exotic pairs at the same frequency as the supernova.
通过对比遥远的超级新星和附近超级新星的亮度，科学家们发现遥远的超级新星相对而言比近的要暗淡25%左右。
By comparing the brightness of distant, far-away supernovae with the brightness of nearby supernovae, the scientists discovered that the far-away supernovae were about 25 percent too faint.
通过对比遥远的超级新星和附近超级新星的亮度，科学家们发现遥远的超级新星相对而言比近的要暗淡25%左右。
By comparing the brightness of distant, far-away supernovae with the brightness of nearby supernovae, the scientists discovered that the far-away supernovae were about 25 percent too faint.
应用推荐