Extrasolar planets - Direct detection at last

被引:2
|
作者
Burrows, A [1 ]
Angel, R
机构
[1] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
关键词
D O I
10.1038/45401
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Astronomers have previously inferred the existence of giant extrasolar planets from the wobble they generate in their parent star. Now, the shadow caused by a planet passing in front of its star, and the probable detection of reflected light from a planet orbiting a very bright star, provide direct evidence for their existence. Such studies offer a way to probe the chemical composition and atmospheres of extrasolar planets.
引用
收藏
页码:732 / 733
页数:2
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