Literature DB >> 19779149

Temporal and spatial variability of lunar hydration as observed by the Deep Impact spacecraft.

Jessica M Sunshine1, Tony L Farnham, Lori M Feaga, Olivier Groussin, Frédéric Merlin, Ralph E Milliken, Michael F A'Hearn.   

Abstract

The Moon is generally anhydrous, yet the Deep Impact spacecraft found the entire surface to be hydrated during some portions of the day. Hydroxyl (OH) and water (H2O) absorptions in the near infrared were strongest near the North Pole and are consistent with <0.5 weight percent H2O. Hydration varied with temperature, rather than cumulative solar radiation, but no inherent absorptivity differences with composition were observed. However, comparisons between data collected 1 week (a quarter lunar day) apart show a dynamic process with diurnal changes in hydration that were greater for mare basalts (approximately 70%) than for highlands (approximately 50%). This hydration loss and return to a steady state occurred entirely between local morning and evening, requiring a ready daytime source of water-group ions, which is consistent with a solar wind origin.

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Year:  2009        PMID: 19779149     DOI: 10.1126/science.1179788

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  19 in total

1.  Solutes determine the temperature windows for microbial survival and growth.

Authors:  Jason P Chin; Julianne Megaw; Caroline L Magill; Krzysztof Nowotarski; Jim P Williams; Prashanth Bhaganna; Mark Linton; Margaret F Patterson; Graham J C Underwood; Allen Y Mswaka; John E Hallsworth
Journal:  Proc Natl Acad Sci U S A       Date:  2010-04-19       Impact factor: 11.205

2.  Nominally hydrous magmatism on the Moon.

Authors:  Francis M McCubbin; Andrew Steele; Erik H Hauri; Hanna Nekvasil; Shigeru Yamashita; Russell J Hemley
Journal:  Proc Natl Acad Sci U S A       Date:  2010-06-14       Impact factor: 11.205

3.  Space Weathering on Airless Bodies.

Authors:  Carle M Pieters; Sarah K Noble
Journal:  J Geophys Res Planets       Date:  2016-09-09       Impact factor: 3.755

4.  Understanding the origin and evolution of water in the Moon through lunar sample studies.

Authors:  Mahesh Anand; Romain Tartèse; Jessica J Barnes
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2014-09-13       Impact factor: 4.226

5.  The negligible chondritic contribution in the lunar soils water.

Authors:  Alice Stephant; François Robert
Journal:  Proc Natl Acad Sci U S A       Date:  2014-10-06       Impact factor: 11.205

6.  Untangling the formation and liberation of water in the lunar regolith.

Authors:  Cheng Zhu; Parker B Crandall; Jeffrey J Gillis-Davis; Hope A Ishii; John P Bradley; Laura M Corley; Ralf I Kaiser
Journal:  Proc Natl Acad Sci U S A       Date:  2019-05-20       Impact factor: 11.205

7.  Detection of solar wind-produced water in irradiated rims on silicate minerals.

Authors:  John P Bradley; Hope A Ishii; Jeffrey J Gillis-Davis; James Ciston; Michael H Nielsen; Hans A Bechtel; Michael C Martin
Journal:  Proc Natl Acad Sci U S A       Date:  2014-01-21       Impact factor: 11.205

8.  Lunar soil hydration constrained by exospheric water liberated by meteoroid impacts.

Authors:  M Benna; D M Hurley; T J Stubbs; P R Mahaffy; R C Elphic
Journal:  Nat Geosci       Date:  2019-04-15       Impact factor: 16.908

9.  Remotely distinguishing and mapping endogenic water on the Moon.

Authors:  Rachel L Klima; Noah E Petro
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2017-05-28       Impact factor: 4.226

10.  Evidence of water on the lunar surface from Chang'E-5 in-situ spectra and returned samples.

Authors:  Jianjun Liu; Bin Liu; Xin Ren; Chunlai Li; Rong Shu; Lin Guo; Songzheng Yu; Qin Zhou; Dawei Liu; Xingguo Zeng; Xingye Gao; Guangliang Zhang; Wei Yan; Hongbo Zhang; Lihui Jia; Shifeng Jin; Chunhua Xu; Xiangjin Deng; Jianfeng Xie; Jianfeng Yang; Changning Huang; Wei Zuo; Yan Su; Weibin Wen; Ziyuan Ouyang
Journal:  Nat Commun       Date:  2022-06-14       Impact factor: 17.694

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