冰巨大气科学

E. Dahl, S. Brueshaber, R. Cosentino, C. Palotai, N. Rowe-Gurney, R. Sankar, K. Sayanagi, S. Aslam, K. Baines, E. Barth, N. Chanover, L. Fletcher, S. Guerlet, H. Hammel, M. Hofstadter, A. Hyder, E. Leonard, T. Livengood, T. Momary, G. Orton, I. Pater, K. Retherford, J. Sinclair, K. Soderlund, L. Spilker, L. Sromovsky, M. Wong
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引用次数: 2

摘要

这份白皮书是为支持NASA的2023-2032年行星年代际调查而写的,概述了10个主要问题,重点关注天王星和海王星大气的起源、演化和当前过程。在接下来的十年里优先考虑这些问题将大大提高我们对这类独特行星的理解,自从旅行者号飞掠以来,这类行星在很大程度上仍未被探索过。研究冰巨星的大气层将极大地帮助我们了解整个太阳系的起源和演化,以及越来越多的包含海王星质量行星的系外行星系统。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ice Giant Atmospheric Science
This white paper, written in support of NASA's 2023-2032 Planetary Decadal Survey, outlines 10 major questions that focus on the origin, evolution, and current processes that shape the atmospheres of Uranus and Neptune. Prioritizing these questions over the next decade will greatly improve our understanding of this unique class of planets, which have remained largely unexplored since the Voyager flybys. Studying the atmospheres of the Ice Giants will greatly inform our understanding of the origin and evolution of the solar system as a whole, in addition to the growing number of exoplanetary systems that contain Neptune-mass planets.
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