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超高密度残骸，来自毁灭恒星。

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

你也可以将你空闲电脑力量用于脉冲星。

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

散布在河系中、被称为“脉冲星”死亡恒星，其自转发生了微妙变化。

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

我们计算脉冲星阵引力波信号所用时间。

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

脉冲星之所以有如此强劲引力，是因为构成它物质非常致密。

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

第二件事是脉冲星和空中爆炸物体。

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

其中一些在我们看来是脉冲星，在旋转时闪烁着明亮光芒。

" 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是磁星或脉冲星发出。”

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到了一个罕见恒星系统，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一些行星，它们都在围绕一个年纪更脉冲星飞行。

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，或快速旋转中子星，起源于巨垂死恒星通过超新星爆炸内爆核心。

(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.

我们探测引力波第二种方法是利用这些奇特恒星，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脉冲星附近形成圆盘后，就更加确信了这一点。

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，是基娅拉提到脉冲星时间微小变化。

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脉冲，因此它们被称作脉冲星。