McSween Harry Y, Hamilton Victoria E, Farley Kenneth A
Department of Earth, Environmental, and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1526.
Solar System Science and Exploration Division, Southwest Research Institute, Boulder, CO 80302.
Proc Natl Acad Sci U S A. 2025 Jan 14;122(2):e2404248121. doi: 10.1073/pnas.2404248121. Epub 2025 Jan 6.
Mars Sample Return (MSR) has been the highest flagship mission priority in the last two Planetary Decadal Surveys of the National Academies of Science, Engineering, and Medicine (hereafter, "the National Academies") and was the highest priority flagship for Mars in the Decadal Survey that preceded them. This inspirational and challenging campaign, like the Apollo program's returned lunar samples, will potentially revolutionize our understanding of Mars and help inform how other planets are explored. MSR's technological advances will keep the NASA and European Space Agency at the forefront of planetary exploration, and data on returned samples will fill knowledge gaps for future human exploration. Investigations of the ancient rocks collected in and around Jezero crater, as well as samples of the regolith and atmosphere, will be fundamentally different in scope, depth, and certainty from what is achievable with spaceborne observations. Returned Mars samples can address critical science issues including the discovery and characterization of ancient extraterrestrial life, prebiotic organic chemistry, the history of habitable planetary environments, planetary geological, geochemical, and geophysical evolution, orbital dynamics of bodies in the early Solar System, and the formation and evolution of atmospheres.
火星样本返回(MSR)一直是美国国家科学院、工程院和医学院(以下简称“美国国家科学院”)过去两次行星十年调查中最高优先级的旗舰任务,并且在之前的十年调查中也是火星探测的最高优先级旗舰任务。这项鼓舞人心且具有挑战性的任务,就像阿波罗计划带回月球样本一样,有可能彻底改变我们对火星的理解,并为其他行星的探索提供参考。MSR的技术进步将使美国国家航空航天局(NASA)和欧洲航天局处于行星探索的前沿,而返回样本的数据将填补未来人类探索的知识空白。对在杰泽罗陨石坑及其周围收集的古老岩石以及风化层和大气样本的研究,在范围、深度和确定性方面将与通过太空观测所能达到的情况有根本不同。返回的火星样本可以解决关键的科学问题,包括古代外星生命的发现与特征描述、益生元有机化学、宜居行星环境的历史、行星地质、地球化学和地球物理演化、早期太阳系天体的轨道动力学以及大气的形成与演化。