Science Enabling Exploration: Using LRO to Prepare for Future Missions

Discoveries from LRO have transformed our understanding of the Moon, but LRO's instruments were originally designed to collect the measurements required to enable future lunar surface exploration. A high lunar exploration priority is the collection of new samples and their return to Earth for c...

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Main Authors: Stopar, J. D., Jolliff, B. L., Petro, N. E., Speyerer, E. J., Lawrence, S. J.
Format: Other/Unknown Material
Language:unknown
Published: 2016
Subjects:
Online Access:http://hdl.handle.net/2060/20160012278
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:20160012278 2023-05-15T18:22:58+02:00 Science Enabling Exploration: Using LRO to Prepare for Future Missions Stopar, J. D. Jolliff, B. L. Petro, N. E. Speyerer, E. J. Lawrence, S. J. Unclassified, Unlimited, Publicly available December 12, 2016 application/pdf http://hdl.handle.net/2060/20160012278 unknown Document ID: 20160012278 http://hdl.handle.net/2060/20160012278 Copyright, Distribution as joint owner in the copyright CASI Lunar and Planetary Science and Exploration JSC-CN-37518 American Geophysical Union (AGU) Fall Meeting; 12-16 Dec. 2016; San Francisco, CA; United States 2016 ftnasantrs 2019-07-20T23:44:35Z Discoveries from LRO have transformed our understanding of the Moon, but LRO's instruments were originally designed to collect the measurements required to enable future lunar surface exploration. A high lunar exploration priority is the collection of new samples and their return to Earth for comprehensive analysis. The importance of sample return from South Pole-Aitken is well-established [Jolliff et al., this conference], but there are numerous other locations where sample return will yield important advances in planetary science. Using new LRO data, we have defined an achievability envelope based on the physical characteristics of successful lunar landing sites. Those results were then used to define 1km x 1km regions of interest where sample return could be executed, including: the basalt flows in Oceanus Procellarum (22.1N, 53.9W), the Gruithuisen Domes (36.1N, 39.7W), the Dewar cryptomare (2.2S, 166.8E), the Aristarchus pyroclastic deposit (24.8N, 48.5W), the Sulpicius Gallus formation (19.9N, 10.3E), the Sinus Aestuum pyroclastic deposit (5.2N, 9.2W), the Compton-Belkovich volcanic complex (61.5N, 99.9E), the Ina Irregular Mare Patch (18.7N, 5.3E), and the Marius Hills volcanic complex (13.4N, 55.9W). All of these locations represent safe landing sites where sample returns are needed to advance our understanding of the evolution of the lunar interior and the timescales of lunar volcanism. If LRO is still active when any future mission reaches the surface, LRO's capability to rapidly place surface activities into broader geologic context will provide operational advantages. LRO remains a unique strategic asset that continues to address the needs of future missions. Other/Unknown Material South pole NASA Technical Reports Server (NTRS) Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) Dewar ENVELOPE(-21.158,-21.158,-80.534,-80.534) South Pole
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic Lunar and Planetary Science and Exploration
spellingShingle Lunar and Planetary Science and Exploration
Stopar, J. D.
Jolliff, B. L.
Petro, N. E.
Speyerer, E. J.
Lawrence, S. J.
Science Enabling Exploration: Using LRO to Prepare for Future Missions
topic_facet Lunar and Planetary Science and Exploration
description Discoveries from LRO have transformed our understanding of the Moon, but LRO's instruments were originally designed to collect the measurements required to enable future lunar surface exploration. A high lunar exploration priority is the collection of new samples and their return to Earth for comprehensive analysis. The importance of sample return from South Pole-Aitken is well-established [Jolliff et al., this conference], but there are numerous other locations where sample return will yield important advances in planetary science. Using new LRO data, we have defined an achievability envelope based on the physical characteristics of successful lunar landing sites. Those results were then used to define 1km x 1km regions of interest where sample return could be executed, including: the basalt flows in Oceanus Procellarum (22.1N, 53.9W), the Gruithuisen Domes (36.1N, 39.7W), the Dewar cryptomare (2.2S, 166.8E), the Aristarchus pyroclastic deposit (24.8N, 48.5W), the Sulpicius Gallus formation (19.9N, 10.3E), the Sinus Aestuum pyroclastic deposit (5.2N, 9.2W), the Compton-Belkovich volcanic complex (61.5N, 99.9E), the Ina Irregular Mare Patch (18.7N, 5.3E), and the Marius Hills volcanic complex (13.4N, 55.9W). All of these locations represent safe landing sites where sample returns are needed to advance our understanding of the evolution of the lunar interior and the timescales of lunar volcanism. If LRO is still active when any future mission reaches the surface, LRO's capability to rapidly place surface activities into broader geologic context will provide operational advantages. LRO remains a unique strategic asset that continues to address the needs of future missions.
format Other/Unknown Material
author Stopar, J. D.
Jolliff, B. L.
Petro, N. E.
Speyerer, E. J.
Lawrence, S. J.
author_facet Stopar, J. D.
Jolliff, B. L.
Petro, N. E.
Speyerer, E. J.
Lawrence, S. J.
author_sort Stopar, J. D.
title Science Enabling Exploration: Using LRO to Prepare for Future Missions
title_short Science Enabling Exploration: Using LRO to Prepare for Future Missions
title_full Science Enabling Exploration: Using LRO to Prepare for Future Missions
title_fullStr Science Enabling Exploration: Using LRO to Prepare for Future Missions
title_full_unstemmed Science Enabling Exploration: Using LRO to Prepare for Future Missions
title_sort science enabling exploration: using lro to prepare for future missions
publishDate 2016
url http://hdl.handle.net/2060/20160012278
op_coverage Unclassified, Unlimited, Publicly available
long_lat ENVELOPE(-44.516,-44.516,-60.733,-60.733)
ENVELOPE(-21.158,-21.158,-80.534,-80.534)
geographic Aitken
Dewar
South Pole
geographic_facet Aitken
Dewar
South Pole
genre South pole
genre_facet South pole
op_source CASI
op_relation Document ID: 20160012278
http://hdl.handle.net/2060/20160012278
op_rights Copyright, Distribution as joint owner in the copyright
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