Detection of earth-sized planets with the COROT space mission

被引：0

作者：

Deleuil, M ^{[1
]}

Barge, P ^{[1
]}

Leger, A ^{[1
]}

Schneider, J ^{[1
]}

机构：

[1] CNRS, Astron Spatiale Lab, F-13376 Marseille 12, France

来源：

PLANETS BEYOND THE SOLAR SYSTEM AND THE NEXT GENERATION OF SPACE MISSIONS | 1997年 / 119卷

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：

The frequent occurrence of disks around pre-main sequence stars, as well as the recent detections of massive extra-solar planets suggest planetary formation is common. The next challenge is the detection of Earth-like planets. Their detection from the ground is problematic due to their very low masses and brightnesses, but space observations could enable these detections. The French space mission COROT (COnvection & ROTation), originally devoted to asteroseismology, is also well-adapted for the detection of low-mass objects using the method of stellar occultation. Due to its high photometric accuracy, a few tens of detections can be expected over the mission lifetime, assuming that about 50% of stars possess an Earth-like planet.

引用

页码：259 / 262

页数：4

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