Characterizing the Structure of Giant Planets

被引：8

作者：

Fortney, J. J. ^{[1
]}

机构：

[1] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA

来源：

CONTRIBUTIONS TO PLASMA PHYSICS | 2013年 / 53卷 / 4-5期

关键词：

Giant planets; exoplanets; equation of state; EXTRASOLAR PLANETS; JUPITER; EVOLUTION; HYDROGEN; INTERIORS; EQUATION; HELIUM; STATE; ATMOSPHERES; SATURN;

D O I：

10.1002/ctpp.201300001

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

Advances in understanding the structure of giant planets are happening quickly on multiple fronts. New first-principles equations of state calculations and cutting edge experiments for hydrogen, helium, water, and other planetary materials, are dramatically changing our view of the interior structure and thermal evolution of Jupiter, Saturn, Uranus, and Neptune. The field of transiting exoplanets has led to the addition of over 200 giant planets that can be studied is some detail, as their masses, radii, and bulk densities can be measured. This opens up the possibility of comparing and contrasting our own giant planets to these exoplanets, to better understand giant plants as a class of astrophysical object. ((c) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

引用

页码：385 / 391

页数：7

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