Literature DB >> 20966247

Hydrogen mapping of the lunar south pole using the LRO neutron detector experiment LEND.

I G Mitrofanov1, A B Sanin, W V Boynton, G Chin, J B Garvin, D Golovin, L G Evans, K Harshman, A S Kozyrev, M L Litvak, A Malakhov, E Mazarico, T McClanahan, G Milikh, M Mokrousov, G Nandikotkur, G A Neumann, I Nuzhdin, R Sagdeev, V Shevchenko, V Shvetsov, D E Smith, R Starr, V I Tretyakov, J Trombka, D Usikov, A Varenikov, A Vostrukhin, M T Zuber.   

Abstract

Hydrogen has been inferred to occur in enhanced concentrations within permanently shadowed regions and, hence, the coldest areas of the lunar poles. The Lunar Crater Observation and Sensing Satellite (LCROSS) mission was designed to detect hydrogen-bearing volatiles directly. Neutron flux measurements of the Moon's south polar region from the Lunar Exploration Neutron Detector (LEND) on the Lunar Reconnaissance Orbiter (LRO) spacecraft were used to select the optimal impact site for LCROSS. LEND data show several regions where the epithermal neutron flux from the surface is suppressed, which is indicative of enhanced hydrogen content. These regions are not spatially coincident with permanently shadowed regions of the Moon. The LCROSS impact site inside the Cabeus crater demonstrates the highest hydrogen concentration in the lunar south polar region, corresponding to an estimated content of 0.5 to 4.0% water ice by weight, depending on the thickness of any overlying dry regolith layer. The distribution of hydrogen across the region is consistent with buried water ice from cometary impacts, hydrogen implantation from the solar wind, and/or other as yet unknown sources.

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Year:  2010        PMID: 20966247     DOI: 10.1126/science.1185696

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


  7 in total

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Authors:  Erwan Mazarico; Michael K Barker; Joseph B Nicholas
Journal:  Adv Space Res       Date:  2018-08-25       Impact factor: 2.152

2.  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

3.  Lunar true polar wander inferred from polar hydrogen.

Authors:  M A Siegler; R S Miller; J T Keane; M Laneuville; D A Paige; I Matsuyama; D J Lawrence; A Crotts; M J Poston
Journal:  Nature       Date:  2016-03-24       Impact factor: 49.962

4.  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

5.  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

6.  Moonshine: Diurnally varying hydration through natural distillation on the Moon, detected by the Lunar Exploration Neutron Detector (LEND).

Authors:  T A Livengood; G Chin; R Z Sagdeev; I G Mitrofanov; W V Boynton; L G Evans; M L Litvak; T P McClanahan; A B Sanin; R D Starr; J J Su
Journal:  Icarus       Date:  2015-07-15       Impact factor: 3.508

7.  Human habitats: prospects for infrastructure supporting astronomy from the Moon.

Authors:  C Heinicke; B Foing
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2020-11-23       Impact factor: 4.226

  7 in total

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