Cited by 490Planetary Science and ExplorationAstro and Planetary ScienceHistory and Developments in Astronomy

Temporal and Spatial Variability of Lunar Hydration As Observed by the Deep Impact Spacecraft

Sunshine, Jessica M., Farnham, Tony L., Feaga, Lori M., Groussin, Olivier, Merlin, Frédéric, Milliken, Ralph E., A’Hearn, Michael F.·2009·Science

Abstract

Lunar Water: The Moon has been thought to be primarily anhydrous, although there has been some evidence for accumulated ice in permanently shadowed craters near its poles (see the Perspective by Lucey , published online 24 September). By analyzing recent infrared mapping by Chandrayaan-1 and Deep Impact, and reexamining Cassini data obtained during its early flyby of the Moon, Pieters et al. (p. 568 , published online 24 September), Sunshine et al. (p. 565 , published online 24 September), and Clark et al. (p. 562 , published online 24 September) reveal a noticeable absorption signal for H 2 O and OH across much of the surface. Some variability in water abundance is seen over the course of the lunar day. The data imply that solar wind is depositing and/or somehow forming water and OH in minerals near the lunar surface, and that this trapped water is dynamic.

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Crossref · 10.1126/science.1179788

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  • Global remote sensing observations have revealed that the lunar surface is distributed with abundant non-metal elements (e.g., O and Si), metal elements (e.g., Fe, Ti, Mg, Ca, and REE), volatile (e.g., H2O, C, and N), thick regolith, and lava tube.

    “The global remote sensing observations have revealed that lunar surface is distributed with abundant non-metal elements (e.g., O and Si), 231 metal elements (e.g., Fe, Ti, Mg, Ca, and REE), 231,232 volatile (e.g., H 2 O, C, and N), 233 thick regolith, 234 and lava tube. 235”

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Authors
Sunshine, J. M., Farnham, T. L., Feaga, L. M., Groussin, O., Merlin, F., Milliken, R. E., & A’Hearn, M. F.
Affiliations
  • University of Maryland, College Park (US)
  • Laboratoire d’Astrophysique de Marseille (FR)
  • Jet Propulsion Laboratory (US)
Corresponding author
Sunshine, Jessica M.
Venue
Science
Published
2009-10-23
Volume
326
Issue
5952
Pages
565-568
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2028837562
Cited by
490
References
17
Citations by year
2026: 31 · 2025: 36 · 2024: 39 · 2023: 39 · 2022: 32 · 2021: 33 · 2020: 20 · 2019: 20 · 2018: 27 · 2017: 24 · 2016: 18 · 2015: 30 · 2014: 29 · 2013: 23 · 2012: 23
FWCI
14.60
Type
journal article
Language
en
Open access
closed
Locations
  • Science (publishedVersion)
  • PubMed (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
Keywords
lunar water, hydroxyl absorption, water absorption, diurnal variation, lunar poles, lunar mare basalts, lunar highlands, solar wind, near-infrared spectroscopy, lunar surface
MeSH terms
Extraterrestrial Environment, Spectrum Analysis, Sunlight, Temperature, Time Factors, Water, Moon, Hydroxyl Radical, Spacecraft

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