When the extrasolar planets around KIC 05807616 were initially discovered in December, their location near the star surprised astronomers.
它将继续其前身的工作,寻找系外行星来增加我们的数据库。
It will continue its predecessor's work, searching for exoplanets to add to our database.
很多时候,系外行星距离地球有数百上千光年远,因此研究人员很难判断宜居性。
In many cases, extrasolar planets are hundreds of thousands of light years away from the Earth, making it difficult for researchers to determine livability.
它的行星HD83443b是由米歇尔·麦耶领导的日内瓦系外行星探测小组于2000年发现的。
The planet HD 83443b was discovered in 2000 by the Geneva Extrasolar Planet Search Team led by Michel Mayor.
这颗恒星和它的行星盘还有一个有趣之处--它可能拥有系外行星。
This star and its disk are interesting for another reason:the likelihood that it hosts extrasolar planets.
系外行星的径向速度测量,未包括在本文中,刚刚单独公布并证实了这一结论。
(Radial velocity measurements of the exoplanets, not included in this paper, have just been separately published and confirm this conclusion.).
研究人员然后比较了所有十种已知系外行星,其直径小于地球精确测量质量的2.7倍。
The researchers then compared all 10 known exoplanets with a diameter less than 2.7 times Earth's that had accurately measured masses.
Beaulieu相信这一发现帮助天文学家更为接近了寻找可居住系外行星的目标。
Beaulieu believes that the findbrings astronomers ever-closer to discovering habitable extrasolar planets.
它也被证明是探测系外行星和描述其大气的有力工具。
It also proved to be a powerful tool for detecting exoplanets and characterizing their atmospheres.
这颗恒星和它的行星盘还有一个有趣之处--它可能拥有系外行星。
This star and its disk are interesting for another reason:the possibility that it could host extrasolar planets.
该小组希望这种探测系外行星的新方法将为了解系外行星的栖息地开辟新的途径。
The group expects this new method of detecting exoplanets will open up a new way of understanding the environment of exoplanets.
这种“第一光”科学图像捕获了大量的恒星和其他物体,包括以前已知有系外行星的系统。
This“first light” science image catches an abundance of stars and different objects,including systems that are previously known to have exoplanets.
Astrophysicist Dr Markus Mugrauer of Friedrich Schiller University Jena, Germany, has discovered andcharacterised many new multiple star systems that contain exoplanets.
虽然一些基本的算法用来对数据进行分类和过滤,但人类的大脑仍然是识别系外行星的主要工具。
Though some basic algorithms were used to sort and filter the data,human brains were still the primary workhorses for identifying exoplanets.
这种“第一光”科学图像捕获了大量的恒星和其他物体,包括以前已知有系外行星的系统。
The"first light" science image captures a wealth of stars and other objects,including systems previously known to have exoplanets.
它有多种科学上的角色,其中包括取得邻近星系、大型星云、个别恒星和系外行星的图片。
It has many scientific roles, including obtaining images of nearby galaxies orlarge nebulae as well as individual stars and exoplanets.
这样的事件被称为过境,并已被用于检测迄今为止编目的许多系外行星。
Such an event is called a transit,and has been used to detect many of the exoplanets catalogued to date.
他们模拟了两种理想化的,贫氧的地球系外行星的大气:富氢和富二氧化碳的大气。
They simulated the atmospheres of idealised, oxygen-poor, terrestrial exoplanets of two types: hydrogen-rich and carbon dioxide-rich atmospheres.
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