The heat budget of rocky planets
The heat budget of rocky planets
复制标题
岩石行星的热量收支
DOI：
10.1088/2514-3433/abb4d9ch4
复制
发表时间：
2020
期刊：
影响因子：
--
通讯作者：
N. Tosi
中科院分区：
文献类型：
--
作者：
B. Foley;C. Houser;L. Noack;N. Tosi
内部热量向太空的损失驱动着行星体的内部动力学并控制着长期演化。它通过决定随着时间的推移火山释放气体和挥发物循环到行星内部的速率，塑造了行星的表面环境及其宜居性的前景。本章讨论了行星形成过程中如何获取热量以及随后的演化过程中如何损失热量，这些来源和汇如何影响行星的表面和内部结构，并探索太阳系和系外行星系统的潜在变化。
The loss of interior heat to space drives the internal dynamics of planetary bodies and governs long term evolution. This shapes a planet’s surface environment and its prospects of habitability by dictating the rates of volcanic outgassing and recycling of volatiles into the planet interior over time. This chapter addresses how heat is acquired during planet formation and lost during the subsequent evolution, how these sources and sinks influence the surface and interior structure of the planet and explores the potential variations through our solar system and exoplanet systems.