Seager Sara, Bains William
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. ; Rufus Scientific, Herts SG8 6ED, UK.
Sci Adv. 2015 Mar 6;1(2):e1500047. doi: 10.1126/sciadv.1500047. eCollection 2015 Mar.
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 mélange 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.
在过去二十年里发现的数千颗系外行星与我们太阳系中的行星大不相同,这对传统行星科学的许多领域都提出了挑战。然而,在这片充满各种可能的行星世界中,关于如何探测生命迹象的想法却滞后了,直到最近几年,才开始认真地对生命迹象可能如何出现在真正的外星世界进行建模。最近的研究结果表明,生物特征气体研究的前沿领域并不在于生物学本身的研究,因为生物学不可避免地扎根于地球的地球化学和进化特性,而在于化学与行星物理学的交叉领域。