Gallet Florian, Charbonnel Corinne, Amard Louis
Department of Astronomy, University of Geneva, Chemin des Maillettes 51, 1290, Versoix, Switzerland.
IRAP, UMR 5277, CNRS and Université de Toulouse, 14, av. E. Belin, F-31400, Toulouse, France.
Orig Life Evol Biosph. 2016 Nov;46(4):395-401. doi: 10.1007/s11084-016-9491-4. Epub 2016 Apr 6.
With about 2000 exoplanets discovered within a large range of different configurations of distance from the star, size, mass, and atmospheric conditions, the concept of habitability cannot rely only on the stellar effective temperature anymore. In addition to the natural evolution of habitability with the intrinsic stellar parameters, tidal, magnetic, and atmospheric interactions are believed to have strong impact on the relative position of the planets inside the so-called habitable zone. Moreover, the notion of habitability itself strongly depends on the definition we give to the term "habitable". The aim of this contribution is to provide a global and up-to-date overview of the work done during the last few years about the description and the modelling of the habitability, and to present the physical processes currently includes in this description.
随着在距离恒星的不同距离、大小、质量和大气条件的大范围不同配置中发现了约2000颗系外行星，宜居性概念再也不能仅依赖于恒星有效温度了。除了宜居性随恒星固有参数的自然演化外，潮汐、磁和大气相互作用被认为对行星在所谓宜居带内的相对位置有强烈影响。此外，宜居性概念本身在很大程度上取决于我们赋予“宜居”一词的定义。本文的目的是提供一个关于过去几年在宜居性描述和建模方面所做工作的全面且最新的概述，并介绍目前该描述中包含的物理过程。
