What photometric space telescopes can tell us about extrasolar giant planets

被引：0

作者：

Seager, S ^{[1
]}

Hui, L ^{[1
]}

机构：

[1] Inst Adv Study, Princeton, NJ 08540 USA

来源：

PLANETARY SYSTEMS IN THE UNIVERSE OBSERVATION, FORMATION AND EVOLUTION | 2004年 / 202期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Within the next few years three microsatellites with part-per-million photometric capability (MOST, MONS, COROT) will be launched. These space telescopes, which were designed for asteroseismology, as well as other proposed or planned space telescopes to detect Earth-like transiting planets (Kepler and Eddington), will be able to observe the reflected light curves of the close-in extrasolar giant planets (CEGPs). The CEGPs are 0.05 AU from their parent star and are potentially bright in reflected light. For a transiting planet (at any orbital distance) moons and planetary rings may be detected.

引用

页码：468 / 470

页数：3

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