Vannah Sara, Stiehl Ian D, Gleiser Marcelo
Atmospheric and Environmental Research, Inc., Lexington, MA 02421, USA.
Department of Physics and Astronomy, Dartmouth College, Hanover, NH 03755, USA.
Entropy (Basel). 2025 Apr 4;27(4):385. doi: 10.3390/e27040385.
In the past, measures of the "Earth-likeness" of exoplanets have been qualitative, considering an abiotic Earth, or requiring discretionary choices of what parameters make a planet Earth-like. With the advent of high-resolution exoplanet spectroscopy, there is a growing need for a method of quantifying the Earth-likeness of a planet that addresses these issues while making use of the data available from modern telescope missions. In this work, we introduce an informational-entropic metric that makes use of the spectrum of an exoplanet to directly quantify how Earth-like the planet is. To illustrate our method, we generate simulated transmission spectra of a series of Earth-like and super-Earth exoplanets, as well as an exoJupiter and several gas giant exoplanets. As a proof of concept, we demonstrate the ability of the information metric to evaluate how similar a planet is to Earth, making it a powerful tool in the search for a candidate Earth 2.0.
过去,系外行星“类地性”的衡量标准一直是定性的,要么考虑无生命的地球,要么需要自行决定哪些参数能使一颗行星具有类地性。随着高分辨率系外行星光谱学的出现,越来越需要一种量化行星类地性的方法,这种方法既能解决上述问题,又能利用现代望远镜任务获取的数据。在这项工作中,我们引入了一种信息熵度量,利用系外行星的光谱直接量化该行星的类地程度。为了说明我们的方法,我们生成了一系列类地和超级地球系外行星以及一颗类木行星和几颗气态巨行星的模拟透射光谱。作为概念验证,我们展示了信息度量评估一颗行星与地球相似程度的能力,使其成为寻找候选“地球2.0”的有力工具。