Overview of the habitability of exoplanets several factors of habitability

Boya Zhang, Mengduo Wang, Xiaohang Xu
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Abstract

By analyzing the data of the earth and the sun, we get some of the factors of a planets habitability, such as the distance from the star to the planet, the atmosphere, and the tidal locked effect. We use the equation of radiative equilibrium and get the orbital semi-major axis in terms of the stars radius and the planets temperature and albedo. Then, according to the data of the planet and the definition of habitat zone, we can get the range of the habitat zone. We find that the relationship between the radius of the star and the planets radius is the radius of the stars surface, the temperature of the planets surface, and the albedo. We also discussed how the albedo, the star mass, the composition of the atmosphere, and the tidal lock influence the planets habitability. In conclusion, the only factor of the habitability of a planet is not the distance from the sun to the planet, we need to consider more factors and re-examine the habitability of the planets.
系外行星的可居住性概述 可居住性的几个因素
通过分析地球和太阳的数据,我们得到了行星宜居性的一些因素,如恒星到行星的距离、大气层和潮汐锁定效应。我们利用辐射平衡方程,根据恒星半径、行星温度和反照率得到轨道半长轴。然后,根据行星的数据和栖息区的定义,我们可以得到栖息区的范围。我们发现恒星半径和行星半径之间的关系是恒星表面半径、行星表面温度和反照率。我们还讨论了反照率、恒星质量、大气成分和潮汐锁定如何影响行星的宜居性。总之,影响行星宜居性的唯一因素并不是太阳到行星的距离,我们需要考虑更多的因素,重新审视行星的宜居性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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