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neutron star

美英

na.【天】中子星
网络成中子星；脉冲星中子星；中子星座

neutron star

英-汉英-英网络释义

neutron star

中子星

中子星(neutron star)，一名波霎(pulsar，脉冲星)。质量高於太阳数倍的恒星当核心的氢於核融合反应中耗尽，完全转变成铁时 …

成中子星

...，后来缩成白矮星体积变小质量变大，然后白矮星会坍塌成中子星（neutron star）；然后说超新星（supernova），超新星是 …

脉冲星中子星

中子星与脉冲星中子星（neutron star）是主要由中子和少量质子、电子组成的超密型恒星。

中子星座

双子电波球体是一个中子星座 (neutron star)，环绕另一中子星座的体系(system)。一般来讲，中子星的引力强度，是太阳的十 …

例句：

In the nebula 's very center lies a pulsar : a neutron star as massive as the Sun but with only the size of a small town.

在星云的正中心有一个脉冲星：一个中心星，它拥有和太阳类似的质量而只有一个小村庄那么大。

(Kusenko likens it to "a bullet passing through a cloud of vapor. " ) And if it runs into a neutron star ?

（Kusenko 把这比作 “一颗子弹穿过一层蒸汽 ”）那么它跑进中子星会发生什么呢？

And this really changed our whole concept of astronomy , the existence of these neutron star binaries.

对于天文学的概念，这些中子双星的，存在，现在一部分是。

And I take a little bit of matter m , and I drop it from a large distance onto the neutron star .

从很远的距离扔到，中子星上，那个小物体。

Astarquake is thought to be the tearing apart of the surface of a neutron star , much like an earthquake here on Earth .

恒星地震拒信可以撕裂中子星表面，其所能产生的破坏力很像地球上的地震。

It was the first time that astronomers have measured the rate of cooling of a young neutron star .

这是天文学家第一次测量到了年轻中子星的冷却速率。

If you had a clock on the surface of a neutron star , for example , it would tick at about 70% of the rate of a clock on Earth .

举个例子，假如你在中子星的表面有一个时钟，那么它的运行速度只有在地球的 70%。

A ten-gram object thrown onto a neutron star -- the reason being that this velocity becomes enormously high.

原因就在于 -，速度，变得无穷大，若扔到中子星的物体。

Smolin's predictions , including ideas about cosmological inflation and the mass of the heaviest stable neutron star , have held up so far.

Smolin 的预测，包括宇宙暴胀学说和最重稳定中子星的质量都有待验证。

In theory , the first step toward producing a millisecond pulsar is the formation of a neutron star when a massive star goes supernova .

理论上，形成一颗毫秒脉冲星的第一步，是一个大质量恒星在成为超新星而爆发后留下的中子星。

In other words, if you were there , the neutron star would pull at you with exactly the same force as the other star .

如果你在那里，中子星对你的引力，和另一颗星对你的，引力是相同的，这个点上你进退两难。

If the neutron star is too large , the gravitational forces overwhelm the pressure gradients and collapse cannot be halted .

如果中子星太大，吸引力胜过气压梯度，塌陷便不能被阻止。

At this point , a neutron star pair , or even a neutron star -black hole pair , is formed .

此刻，一个双中子星、甚至中子星 -黑洞对将形成。

Three years later , Salla's nav computer malfunctioned and deposited her vessel on a collision course with a neutron star .

三年后，萨拉的飞船因导航电脑故障，锁定航线向一颗中子星撞去。

And you don't really ; have to be infinitely far away; you just have to be much further away than the radius of the neutron star .

从无穷远处来，你只要在远大于；，中子星半径的地方，当物体撞到。

The only things more dense are black holes , as a teaspoonful of neutron star matter would weigh about 100 million tons.

比它密度再大的就只有黑洞了，只需要一勺匙中子星的质量就可以达到 100万吨。

Basically , a black hole is formed when a very , very large star has a supernova event which can result in a neutron star or a black hole .

基本上，黑洞都脱胎于恒星，如果这颗恒星爆发成一颗非常，非常硕大的超新星，那么就可能会产生中子星或黑洞。

In each case, the neutron star is orbiting within the outer atmosphere of its supergiant companion .

无一例外，中子星的轨道都在其巨星同伴的外层大气之中。

Since a 7-solar-mass is too large to be a white dwarf or neutron star , it must be a black hole .

因为有着 7 个太阳质量的星体不可能是白矮星或中于星，所以它一定是黑洞。

The most likely explanation for GRB050709 is that it was produced by a collision of two neutron stars, or a neutron star and a black hole .

对于 GRB050709 ，最可能的解释认为，它是两颗中子星，或者一颗中子星和一个黑洞碰撞的结果。

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