Observed Properties of Extrasolar Planets

被引：115

作者：

Howard, Andrew W. ^{[1
]}

机构：

[1] Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA

来源：

SCIENCE | 2013年 / 340卷 / 6132期

关键词：

PERIOD DISTRIBUTION; HOST STARS; MASS; SYSTEMS; ARCHITECTURE; CONSTRAINTS; EXOPLANETS; FREQUENCY; MIGRATION; RADII;

D O I：

10.1126/science.1233545

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：

Observational surveys for extrasolar planets probe the diverse outcomes of planet formation and evolution. These surveys measure the frequency of planets with different masses, sizes, orbital characteristics, and host star properties. Small planets between the sizes of Earth and Neptune substantially outnumber Jupiter-sized planets. The survey measurements support the core accretion model, in which planets form by the accumulation of solids and then gas in protoplanetary disks. The diversity of exoplanetary characteristics demonstrates that most of the gross features of the solar system are one outcome in a continuum of possibilities. The most common class of planetary system detectable today consists of one or more planets approximately one to three times Earth's size orbiting within a fraction of the Earth-Sun distance.

引用

页码：572 / 576

页数：5

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