The importance of the study of igneous rocks and compositions to constrain the martian planetary evolution

A. Udry, J. Filiberto, J. Gross, M. Schmidt, D. Rogers, Libby Hausrath, R. Wiens, N. Lanza
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Abstract

This white paper summarizes the scientific importance of studying igneous compositions in meteorites, surface samples, and through orbital analyses to better constrain the geology of Mars as a whole and better understand the geological processes that have shaped Mars in the past and present. In support of martian igneous studies, we strongly advocate for the following in the upcoming decade: 1. To sustain funding for meteorite recovery in order to have continued access to martian samples; 2. To support the return of igneous samples from Jezero crater; 3. To support funding for detailed analyses of igneous rocks at the martian surface; 4. To support laboratories and collaborations between sample, remote-sensing, and mission scientists; 5. To support curation facilities needed for not only meteorite samples, but also Mars sample return. The study of martian igneous compositions is crucial to the entire planetary community as it will help us to resolve questions about the formation and evolution of planetary interiors, climate and atmospheres, as well as habitability throughout the entire solar system.
火成岩及其组成研究对约束火星行星演化的重要性
这份白皮书总结了研究陨石、地表样本中的火成岩成分,以及通过轨道分析来更好地约束火星的整体地质,更好地理解过去和现在塑造火星的地质过程的科学重要性。为了支持火星火成岩研究,我们在未来十年强烈主张以下几点:继续为陨石回收提供资金,以便继续获得火星样本;2. 为了支持从耶泽罗陨石坑带回的火成岩样本;3.为火星表面火成岩的详细分析提供资金支持;4. 支持实验室和样本、遥感和任务科学家之间的合作;5. 支持管理设施,不仅需要陨石样本,也需要火星样本返回。对火星火成岩成分的研究对整个行星群落至关重要,因为它将帮助我们解决有关行星内部、气候和大气的形成和演化以及整个太阳系的可居住性的问题。
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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