The Kepler telescope obtained data on two such transits.

望远镜获得了两次这样的凌日数据。

The planet Kepler 69c follows a Venus-like orbit around a sunlike star.

69c围绕一颗类太阳恒星运转，其轨道类似于金星围绕太阳公转的轨道。

Kepler is accredited with revolutionizing understanding of the universe.

因变革了人类对宙的认识而为世人认可。

Astronomers using NASA's Kepler space telescope analyzed a giant star called Kepler 56, about 3,000 light-years from Earth.

天文学家利用 NASA 的宙望远镜分析了距地约3000光年的巨星“56”。

But Kepler went even further than just pontificating about the sun.

但并没有止步于对太阳的推测。

This is where the Kepler Space Telescope focused for many years.

太空望远镜在这里聚焦了很多年。

And we have well over 3000 more candidates from Kepler awaiting confirmation.

我们还有3000多名被所探测的候选星等待确认。

A NASA spacecraft called Kepler has found thousands of exoplanets this way.

美国航局一艘名为的宙飞船以这种方式发现了数千颗系外行星。

It began in 2009 with the launch of NASA's Kepler mission.

故事始于 2009 年， NASA 启动了计划。

Kepler has discovered around 2,600 exoplanets- those that orbit stars other than the sun.

发现了约2600颗外星行星—那些围绕恒星而非太阳运行的行星。

No, but still, it is supposedly in or near the habitable zone of Kepler 16.

但它仍然位于16号的适居区内或附近。

This blob is where NASA's Kepler space telescope stared at for about four whole years.

美国国家航空航天局用太空望远镜观察这里大约四年。

The data came from NASA's Kepler telescope and the European Space Agency's Gaia telescope.

这些数据来自美国航空航天局的太空望远镜和欧洲航天局的盖亚太空望远镜。

NASA's Kepler spacecraft has discovered three new planets that are close to earth's size.

美国国家航空航天局的“”宙飞船发现了与地球大小接近的三颗新行星。

But the Kepler Space Telescope, launched in 2009 was literally above all that.

但是，2009年发射的太空望远镜在这一切之上。

Kepler's second law deals with the speed of planets orbiting the Sun.

第二定律研究的是行星绕太阳运行的速度。

Kepler's data reveals planets' sizes as well as their distance from their parent star.

Kepler的數據揭示了行星的大小以及它们与直系恒星之间的距离。

It flags likely looking reductions as “candidate planets”, of which Kepler 22b was one.

观测者会发现恒星表面上出现疑是“候选行星”的小黑点。“22b”就是这些候选行星之一。

Spotting such tiny flickers is on the edge of Kepler's capabilities.

探测到如此微小的闪烁，探测器可能无能为力。

Kepler made it possible for us to measure stellar brightness much more precisely than we had before.

让我们可以以前所未有的精度测量恒星亮度。