The search for signs of life on exoplanets at the interface of chemistry and planetary science

被引:49
|
作者
Seager, Sara [1 ,2 ]
Bains, William [1 ,3 ]
机构
[1] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[2] MIT, Dept Phys, Cambridge, MA 02139 USA
[3] Rufus Sci, Royston SG8 6ED, Herts, England
来源
SCIENCE ADVANCES | 2015年 / 1卷 / 02期
关键词
EARTH-LIKE PLANETS; TRANSMISSION SPECTRUM; HABITABLE ZONE; ATMOSPHERIC RETRIEVAL; SYNTHETIC SPECTRA; MASS; TERRESTRIAL; EVOLUTION; BIOSIGNATURES; EMISSION;
D O I
10.1126/sciadv.1500047
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
The discovery of thousands of exoplanets in the last two decades that are so different from planets in our own solar system challenges many areas of traditional planetary science. However, ideas for how to detect signs of life in this melange of planetary possibilities have lagged, and only in the last few years has modeling how signs of life might appear on genuinely alien worlds begun in earnest. Recent results have shown that the exciting frontier for biosignature gas ideas is not in the study of biology itself, which is inevitably rooted in Earth's geochemical and evolutionary specifics, but in the interface of chemistry and planetary physics.
引用
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页数:11
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