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Visible‐Shortwave Infrared (VSWIR) Spectral Parameters for the Lunar Trailblazer High‐Resolution Volatiles and Minerals Moon Mapper (HVM 3 )

Abstract:
Plain Language Summary: The High‐resolution Volatiles and Minerals Moon Mapper (HVM3) is one of two science instruments on the Lunar Trailblazer smallsat mission, whose science goal is to understand the distribution, abundance, and form of water on the Moon, as well as the lunar water cycle. HVM3 uses patterns in infrared light reflection and absorption at different wavelengths to detect water and minerals in rocks and soils on the Moon's surface. In July 2025 the Lunar Trailblazer mission end was declared. Here, we detail the formulation and testing of algorithms for making water and mineral maps in preparation for the anticipated HVM3 returned data using existing Moon Mineralogy Mapper (M3) and Deep Impact spacecraft lunar data sets, which are similar types of instruments. We demonstrate that presented spectral parameters can distinguish lunar minerals of interest and therefore, capture lunar mineral diversity well. We also show that a newly developed water spectral parameter can be used as a reliable indication of lunar surface water presence, thereby demonstrating the value of expected HVM3 maps for the broader scientific community as well as planning future exploration of the Moon.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1029/2025ea004557

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Role:
Author
ORCID:
0000-0003-0343-7382
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Role:
Author
ORCID:
0000-0002-9151-6429
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Role:
Author
ORCID:
0000-0002-7149-7144
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Role:
Author
ORCID:
0000-0002-2745-3240
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Role:
Author
ORCID:
0000-0002-8096-9633



Publisher:
Wiley
Journal:
Earth and Space Science More from this journal
Volume:
13
Issue:
3
Article number:
e2025EA004557
Publication date:
2026-03-10
Acceptance date:
2025-12-03
DOI:
EISSN:
2333-5084
ISSN:
2333-5084


Language:
English
Pubs id:
2389552
Local pid:
pubs:2389552
Source identifiers:
3839831
Deposit date:
2026-03-10
ARK identifier:
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