The Occurrence and Architecture of Exoplanetary Systems

被引：655

作者：

Winn, Joshua N. ^{[1
]}

Fabrycky, Daniel C. ^{[2
]}

机构：

[1] MIT, Dept Phys, Cambridge, MA 02139 USA

[2] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 53 | 2015年 / 53卷

关键词：

exoplanets; extrasolar planets; orbital properties; planet formation; SPIN-ORBIT MISALIGNMENT; KEPLER PLANET CANDIDATES; EXTRA-SOLAR PLANETS; MEAN MOTION RESONANCES; HUBBLE-SPACE-TELESCOPE; FALSE-POSITIVE RATE; IN-SITU FORMATION; R-CIRCLE-PLUS; GIANT PLANETS; HOT JUPITERS;

D O I：

10.1146/annurev-astro-082214-122246

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The basic geometry of the Solar System-the shapes, spacings, and orientations of the planetary orbits-has long been a subject of fascination as well as inspiration for planet-formation theories. For exoplanetary systems, those same properties have only recently come into focus. Here we review our current knowledge of the occurrence of planets around other stars, their orbital distances and eccentricities, the orbital spacings and mutual inclinations in multiplanet systems, the orientation of the host star's rotation axis, and the properties of planets in binary-star systems.

引用

页码：409 / 447

页数：39

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