阿波罗下一代样品分析(ANGSA):阿波罗参与科学家计划,为阿耳特弥斯计划准备月球样品群。

IF 9.1 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Space Science Reviews Pub Date : 2024-01-01 Epub Date: 2024-08-20 DOI:10.1007/s11214-024-01094-x
C K Shearer, F M McCubbin, S Eckley, S B Simon, A Meshik, F McDonald, H H Schmitt, R A Zeigler, J Gross, J Mitchell, C Krysher, R V Morris, R Parai, B L Jolliff, J J Gillis-Davis, K H Joy, S K Bell, P G Lucey, L Sun, Z D Sharp, C Dukes, A Sehlke, A Mosie, J Allton, C Amick, J I Simon, T M Erickson, J J Barnes, M D Dyar, K Burgess, N Petro, D Moriarty, N M Curran, J E Elsila, R A Colina-Ruiz, T Kroll, D Sokaras, H A Ishii, J P Bradley, D Sears, B Cohen, O Pravdivseva, M S Thompson, C R Neal, R Hana, R Ketcham, K Welten
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引用次数: 0

摘要

作为准备阿耳特弥斯计划从月球返回样品的第一步,美国航天局启动了阿波罗下一代样品分析计划(ANGSA)。阿波罗下一代样本分析计划的目的是作为一项低成本的样本返回任务,对阿波罗 17 号任务以前返回的样本进行整理和分析,这些样本在 50 年的时间里一直未被打开或储存在独特的条件下。这些样本包括先前密封在月球表面的双驱动管的下部、该驱动管一直未打开的上部,以及在零下 27 ℃ 保存了约 50 年的各种阿波罗 17 号样本。ANGSA 是 50 多年来月球 "样本返回任务 "的第一个初步检查阶段。它还模仿了阿耳特弥斯地面探测任务的同一阶段,其设计包括通过自阿波罗以来收集的新的轨道观测数据以及阿波罗 17 号宇航员哈里森-施密特提供的额外的新的 "实地 "观测数据、数据综合和解释,将样本置于当地和区域地质的背景下。ANGSA 使用新的保存技术来准备、记录和分配这些新的月球样本,开发了新的工具来打开和提取容器中的气体,并应用了以前在阿波罗计划中无法使用的新的分析仪器来揭示这些样本的新信息。参与此次任务的 90 名科学家、工程师和馆员中的大多数人在阿波罗计划期间都不在世,而在美国宇航局联合空间中心的阿波罗馆藏设施中处理最后一个阿波罗核心样本距今已有 30 年之久。ANGSA 有许多与阿耳特弥斯直接相关的 "第一"。ANGSA 是第一个打开以前封存在月球表面的岩心样品的机构,是第一个提取和分析在原地收集的月球气体的机构,是第一个检查穿透月球滑坡沉积物的岩心的机构,也是第一个在零下 20 ℃ 的手套箱中处理原始阿波罗样品的机构。ANGSA的所有活动都有助于阿耳特弥斯一代为未来做好准备。该计划的时间安排、团队的组成以及未打开的阿波罗样本的保存,促进了从阿波罗到阿耳特弥斯的代际交接,为阿耳特弥斯和月球样本科学界取得更多成功奠定了基础。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Apollo Next Generation Sample Analysis (ANGSA): an Apollo Participating Scientist Program to Prepare the Lunar Sample Community for Artemis.

As a first step in preparing for the return of samples from the Moon by the Artemis Program, NASA initiated the Apollo Next Generation Sample Analysis Program (ANGSA). ANGSA was designed to function as a low-cost sample return mission and involved the curation and analysis of samples previously returned by the Apollo 17 mission that remained unopened or stored under unique conditions for 50 years. These samples include the lower portion of a double drive tube previously sealed on the lunar surface, the upper portion of that drive tube that had remained unopened, and a variety of Apollo 17 samples that had remained stored at -27 °C for approximately 50 years. ANGSA constitutes the first preliminary examination phase of a lunar "sample return mission" in over 50 years. It also mimics that same phase of an Artemis surface exploration mission, its design included placing samples within the context of local and regional geology through new orbital observations collected since Apollo and additional new "boots-on-the-ground" observations, data synthesis, and interpretations provided by Apollo 17 astronaut Harrison Schmitt. ANGSA used new curation techniques to prepare, document, and allocate these new lunar samples, developed new tools to open and extract gases from their containers, and applied new analytical instrumentation previously unavailable during the Apollo Program to reveal new information about these samples. Most of the 90 scientists, engineers, and curators involved in this mission were not alive during the Apollo Program, and it had been 30 years since the last Apollo core sample was processed in the Apollo curation facility at NASA JSC. There are many firsts associated with ANGSA that have direct relevance to Artemis. ANGSA is the first to open a core sample previously sealed on the surface of the Moon, the first to extract and analyze lunar gases collected in situ, the first to examine a core that penetrated a lunar landslide deposit, and the first to process pristine Apollo samples in a glovebox at -20 °C. All the ANGSA activities have helped to prepare the Artemis generation for what is to come. The timing of this program, the composition of the team, and the preservation of unopened Apollo samples facilitated this generational handoff from Apollo to Artemis that sets up Artemis and the lunar sample science community for additional successes.

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来源期刊
Space Science Reviews
Space Science Reviews 地学天文-天文与天体物理
CiteScore
19.70
自引率
3.90%
发文量
60
审稿时长
4-8 weeks
期刊介绍: Space Science Reviews (SSRv) stands as an international journal dedicated to scientific space research, offering a contemporary synthesis across various branches of space exploration. Emphasizing scientific outcomes and instruments, SSRv spans astrophysics, physics of planetary systems, solar physics, and the physics of magnetospheres & interplanetary matter. Beyond Topical Collections and invited Review Articles, Space Science Reviews welcomes unsolicited Review Articles and Special Communications. The latter encompass papers related to a prior topical volume/collection, report-type papers, or timely contributions addressing a robust combination of space science and technology. These papers succinctly summarize both the science and technology aspects of instruments or missions in a single publication.
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