Extrasolar planets: Constraints for planet formation models

被引:38
作者
Santos, NC [1 ]
Benz, W
Mayor, M
机构
[1] Univ Lisbon, Ctr Astron & Astrofis, Observ Astron Lisboa, P-1349018 Lisbon, Portugal
[2] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
[3] Observ Geneva, CH-1290 Sauverny, Switzerland
关键词
D O I
10.1126/science.1100210
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
Since 1995, more than 150 extrasolar planets have been discovered, most of them in orbits quite different from those of the giant planets in our own solar system. The number of discovered extrasolar planets demonstrates that planetary systems are common but also that they may possess a large variety of properties. As the number of detections grows, statistical studies of the properties of exoplanets and their host stars can be conducted to unravel some of the key physical and chemical processes leading to the formation of planetary systems.
引用
收藏
页码:251 / 255
页数:5
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