neutron stars发音

意思翻译

n.[天]中子星

相似词语短语

stars───v.点缀；成辐射状开裂；使担任主角（star的第三人称单数）；abbr.specializedtrainingandreassignmentstudents经过专门训练后再分配的学生；stationaryautomotiveroadstimulator(Toyota)汽车公路固定刺激物（丰田汽车）；n.明星类，明星（star的复数形式）

neutron star───n.[天]中子星；n.中子星

fallen stars───陨星

try stars───试试星星

dark stars───[天]暗星

famous stars───著名明星

dying stars───垂死的星星

zero stars───零星

party stars───派对明星

双语使用场景

Neutron stars are, after all, a little less extreme than black holes, Big Bangs and supernovae...───毕竟中子星并没有黑洞、大爆炸、超新星等等那么极端。

So instead of looking at many neutron stars, researchers needed to look at only this one.───因此，不同于以往观察许多中子星，研究人员们只需要观测这一个中子星即可。

Neutron stars are created when massive stars run out of fuel and collapse.───中子星是在大型恒星耗尽燃料后崩溃而产生的。

One of the best possible sources for gravitational waves would be a merger between compact binary neutron stars.───观测引力波的最佳时机之一就是两颗中子星互相吞噬的过程。

A third topic is that of the high-density colour superconductive state of matter, which may be present in the core of neutron stars.───第三个议题是，在高密度色超导物质的状态，这可能是在中子星的核心存在。

He said the neutron stars can be no larger than about 20. 5 miles (33 kilometers) across.───他指出，这些中子星的直径不可能超过20.5英里（33公里）。

To find out how strong the crusts of neutron stars really are, Horowitz and a colleague created a computer simulation of a star's surface.───为了发现中子星的地壳到底有多么硬，Horowitz和一位同事建立了一颗星球表面的计算机模拟程序。

Strong gravitational waves are thought to be produced by the collision of two neutron stars.───在两颗中子星星体之间的作用被认为会产生很强的重力波动。

One of the neutron stars is a pulsar; it emits radio pulses at regular intervals as it spins 45 times per second.───其中一颗为脉冲星，该脉冲星以每秒45周的旋频率向宇宙中发射有规律的无线电波。

英语使用场景

Though the maximum masses and corresponding radii are similar, bare strange quark stars and normal neutron stars could be distinguished in the regime of low masses.

Before the two neutron stars collide, they would orbit each other as a binary system.

Neutron stars are the second exhibit in the gallery of stellar corpses.

Pulsars, neutron stars and quark stars are then created based on their mass.

Moreover, because of their intense density, neutron stars exert strong gravitational force on their binary companion.

They were therefore called neutron stars.

They are massively compressed neutron stars that intermittently sendout bursts of radio waves that can last for as few as two milliseconds withdark gaps lasting as long as three hours.

Supernovae remnants can leave behind pulsars or spinning neutron stars that may produce gravitational waves.

The onset of superfluidity in materials on Earth occurs at extremely low temperatures near absolute zero, but in neutron stars, it can occur at temperatures near a billion degrees Celsius.