Each golden record displays the location of our solar system with respect to fourteen pulsars.

每个金唱片都显示着我们太阳系相对于14个的位置。

Pulsars provide little light or heat and would bathe these worlds in intense radiation.

上几乎没有阳光和热量，到处都强辐射。

A pulsar is the rapidly rotating ultra-dense remnant of a collapsed massive star.

快速转动的超高密度残骸，来自毁灭的大型恒。

You too can lend your spare computer power to the pulsar hunt.

你也可以将你的空闲电脑力量用于寻找。

Telltale tweaks to the spins of dead stars called pulsars scattered throughout the Milky Way.

散布在河系中的、被称为“”的死亡恒，其自转发生了微妙的变化。

And we time an array of pulsars will look for gravitational wave signals.

我们计算阵列寻找引力波信号所用的时间。

Pulsars have such extreme gravity because they're made of incredibly dense matter.

之所以有如此强劲的引力，因为构成它的物质非常致密。

And the second big thing is pulsars and things going bang in the sky.

第二件大事和空中爆炸的物体。

Some of them we see as pulsars, flashing in brightness as they spin.

其中些在我们看来，在旋转时闪烁着明亮的光芒。

" We think this new signal could be a magnetar or pulsar on steroids, " Michilli said.

“我们认为这个新信号可能大型磁或发出的。”

They also used it to find an unusual kind of star system, a binary pulsar, in 1967.

1967年，科学家还用该望远镜找到了个罕见的恒系统，即双。

In 1992, astronomers found the first planets outside our solar system, which were orbiting an older pulsar.

1992年，天文学家首次发现太阳系外的些行，它们都在围绕个年纪更大的飞行。

The research was based on pulsar timing observations carried out with the Five-hundred-meter Aperture Spherical Telescope (FAST).

这项研究基于500米口径球面望远镜(FAST)进行的计时观测。

Pulsars, or fast-spinning neutron stars, originate from the imploded cores of massive dying stars through supernova explosions.

，或快速旋转的中子，起源于巨大的垂死恒通过超新爆炸的内爆核心。

(A pulsar is the dead, ultra-dense remnant left over after a supernova.) A trickle of subsequent discoveries followed.

（在超新阶段后超高密度的死亡残余。）随后小发现接踵而来。

The second way that we've learned to detect gravitational waves is by using these exotic stars called pulsars.

我们探测引力波的第二方法利用这些奇特的恒，叫做。

The discovery of a planet forming disk around a younger pulsar makes this likely.

在我们发现某行在年级更小的附近形成圆盘后，就更加确信了这点。

Discovered in 1967, pulsars spin very rapidly, often hundreds of times per second.

于1967年被发现，它们的转速极快，往往每秒钟能旋转数百周。

And what we're looking for very tiny changes in timing of those pulsars that Chiara mentioned.

我们正在寻找的，基娅拉提到的的时间微小变化。

When the beams sweep across the Earth, they can be heard as regular pulses, so we call them pulsars.

当它们扫过地球时，我们会接收到有规律的，因此它们被称作。