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个脉冲星的位置。

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

脉冲星上几乎没有阳光和热量，到处都是强辐射。

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

脉冲星是一种快速转动的超高密度残，毁灭的大型恒星。

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脉冲星。

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“脉冲星”的死亡恒星，其转发生了微妙的变化。

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

我们计算脉冲星阵列寻找引力所用的时间。

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

脉冲星之所以有如此强劲的引力，是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.

第二件大事是脉冲星和空中爆炸的物体。

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

其中一些在我们看是脉冲星，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.

“我们认为这个新可能是大型磁星或脉冲星发出的。”

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一个罕见的恒星系统，即脉冲双星。

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一些行星，它们都在围绕一个年纪更大的脉冲星飞行。

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

这项研究是基于500米口径球面望远镜(FAST)进行的脉冲星计时观测。

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

脉冲星，或快速旋转的中子星，起源于巨大的垂死恒星通过超新星爆炸的内爆核心。

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

（脉冲星是在超新星阶段后超高密度的死亡残余。）随后小发现接踵而。

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

我们探测引力的第二种方法是利用这些奇特的恒星，叫做脉冲星。

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

在我们发现某行星在年级更小的脉冲星附近形成圆盘后，就更加确了这一点。

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

脉冲星于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，是基娅拉提到的脉冲星的时间微小变化。

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脉冲，因此它们被称作脉冲星。