From Solar System to Exoplanets:What can we learn from Planetary Spectroscopy?

作     者：Therese Encrenaz Therese Encrenaz

作者机构：LESIAParis Observatory-PSL UniversitéCNRSSorbonne UniversitéUniversitéde ParisParisFrance 

出 版 物：《Research in Astronomy and Astrophysics》 (天文和天体物理学研究（英文版）)

年 卷 期：2022年第22卷第12期

页      面：1-14页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：funded by Paris Observatory and the Centre National de la Recherche Scientifique 

主　　题：planets and satellites:atmospheres planets and satellites:composition (stars:)planetary systems 

摘      要：The purpose of this paper is to address the question:Using our knowledge of infrared planetary spectroscopy,what can we learn about the atmospheres of exoplanets?In a first part,a simplified classification of exoplanets,assuming thermochemical equilibrium,is presented,based on their masses and their equilibrium temperatures,in order to propose some possible estimations about their atmospheric *** the second part,infrared spectra of planets are discussed,in order to see what lessons can be drawn for exoplanetary *** the last part,we consider the solar system as it would appear from a star located in the ecliptic *** first appears that the solar system(except in a few specific cases)would not be seen as a multiple system,because,contrary to many exoplanetary systems,the planets are too far from the Sun and the inclinations of their orbits with respect to the ecliptic plane are too *** transit synthetic spectra of solar system planets are used to discuss the relative merits of transmission and direct emission spectroscopy for probing exoplanetary atmospheres.