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中子星

n.neutron star
网络neutron stars; pulsar; space.com

中子星

中子星

英-汉网络释义

中子星

n.

1.neutron star

1

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。

2

(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？

3

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。

5

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。

6

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

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

7

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。

8

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。

9

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）。

11

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%。

12

13

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。

14

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。

15

17

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。

18

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。

20

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。

21

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。

23

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。

24

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。

26

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。

27

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。

28

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。

29

30

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。

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