Direct evidence of surface exposed water ice in the lunar polar regions

Significance We found direct and definitive evidence for surface-exposed water ice in the lunar polar regions. The abundance and distribution of ice on the Moon are distinct from those on other airless bodies in the inner solar system such as Mercury and Ceres, which may be associated with the unique formation and evolution process of our Moon. These ice deposits might be utilized as an in situ resource in future exploration of the Moon. Water ice may be allowed to accumulate in permanently shaded regions on airless bodies in the inner solar system such as Mercury, the Moon, and Ceres [Watson K, et al. (1961) J Geophys Res 66:3033–3045]. Unlike Mercury and Ceres, direct evidence for water ice exposed at the lunar surface has remained elusive. We utilize indirect lighting in regions of permanent shadow to report the detection of diagnostic near-infrared absorption features of water ice in reflectance spectra acquired by the Moon Mineralogy Mapper [M (3)] instrument. Several thousand M (3) pixels (∼280 × 280 m) with signatures of water ice at the optical surface (depth of less than a few millimeters) are identified within 20° latitude of both poles, including locations where independent measurements have suggested that water ice may be present. Most ice locations detected in M (3) data also exhibit lunar orbiter laser altimeter reflectance values and Lyman Alpha Mapping Project instrument UV ratio values consistent with the presence of water ice and also exhibit annual maximum temperatures below 110 K. However, only ∼3.5% of cold traps exhibit ice exposures. Spectral modeling shows that some ice-bearing pixels may contain ∼30 wt % ice that is intimately mixed with dry regolith. The patchy distribution and low abundance of lunar surface-exposed water ice might be associated with the true polar wander and impact gardening. The observation of spectral features of H2O confirms that water ice is trapped and accumulates in permanently shadowed regions of the Moon, and in some locations, it is exposed at the modern optical surface.

[1]  A. Hunter,et al.  The Planets: Their Origin and Development , 1952 .

[2]  Roger N. Clark,et al.  Detection of Adsorbed Water and Hydroxyl on the Moon , 2009, Science.

[3]  Joseph W. Boardman,et al.  The Moon Mineralogy Mapper (M3) imaging spectrometer for lunar science: Instrument description, calibration, on‐orbit measurements, science data calibration and on‐orbit validation , 2011 .

[4]  Carl de Boor,et al.  A Practical Guide to Splines , 1978, Applied Mathematical Sciences.

[5]  Michael J. Hoffmann,et al.  Surface water-ice deposits in the northern shadowed regions of Ceres , 2016, Nature Astronomy.

[6]  S. Maurice,et al.  Sensitivity of orbital neutron measurements to the thickness and abundance of surficial lunar water , 2011 .

[7]  Kurt D. Retherford,et al.  Evidence for exposed water ice in the Moon’s south polar regions from Lunar Reconnaissance Orbiter ultraviolet albedo and temperature measurements , 2015 .

[8]  B. Hapke Bidirectional reflectance spectroscopy: 1. Theory , 1981 .

[9]  James R. Arnold,et al.  Ice in the lunar polar regions , 1979 .

[10]  David C. Slater,et al.  Far???ultraviolet reflectance properties of the Moon's permanently shadowed regions , 2012 .

[11]  Carle M. Pieters,et al.  Optical effects of space weathering: The role of the finest fraction , 1993 .

[12]  P. Lucey,et al.  Proton flux and radiation dose from galactic cosmic rays in the lunar regolith and implications for organic synthesis at the poles of the Moon and Mercury , 2013 .

[13]  R. S. Miller,et al.  Lunar true polar wander inferred from polar hydrogen , 2016, Nature.

[14]  W. Augustyniak,et al.  Low energy cosmic ray erosion of ice grains in interplanetary and interstellar media , 1978, Nature.

[15]  Engen Libowitzky,et al.  Correlation of O-H stretching frequencies and O-H…O hydrogen bond lengths in minerals , 1999 .

[16]  N. Thomas,et al.  Sublimation of water ice mixed with silicates and tholins: Evolution of surface texture and reflectance spectra, with implications for comets , 2016 .

[17]  David A. Paige,et al.  Thermal Stability of Volatiles in the North Polar Region of Mercury , 2013, Science.

[18]  Lori M. Feaga,et al.  Temporal and Spatial Variability of Lunar Hydration As Observed by the Deep Impact Spacecraft , 2009, Science.

[19]  A. Schriver,et al.  IR reflection–absorption spectra of thin water ice films between 10 and 160 K at low pressure , 2000 .

[20]  B. Hapke Bidirectional reflectance spectroscopy , 1984 .

[21]  A. Vasavada,et al.  Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits☆ , 1999 .

[22]  Roger N. Clark,et al.  Water frost and ice - The near-infrared spectral reflectance 0.65-2.5 microns. [observed on natural satellites and other solar system objects , 1981 .

[23]  D. Paige,et al.  The global surface temperatures of the Moon as measured by the Diviner Lunar Radiometer Experiment , 2017 .

[24]  Shuai Li,et al.  Water on the surface of the Moon as seen by the Moon Mineralogy Mapper: Distribution, abundance, and origins , 2017, Science Advances.

[25]  D. Lawrence,et al.  Two‐dimensional distribution of volatiles in the lunar regolith from space weathering simulations , 2012 .

[26]  Bruce C. Murray,et al.  The behavior of volatiles on the lunar surface , 1961 .

[27]  M. D. Dyar,et al.  Character and Spatial Distribution of OH/H2O on the Surface of the Moon Seen by M3 on Chandrayaan-1 , 2009, Science.

[28]  R. Milliken,et al.  An empirical thermal correction model for Moon Mineralogy Mapper data constrained by laboratory spectra and Diviner temperatures , 2016 .

[29]  J. Head,et al.  New evidence for surface water ice in small‐scale cold traps and in three large craters at the north polar region of Mercury from the Mercury Laser Altimeter , 2017 .

[30]  David E. Smith,et al.  IJ Constraints on the volatile distribution within Shackleton crater at the lunar south pole , 2012 .

[31]  David E. Smith,et al.  Bright and Dark Polar Deposits on Mercury: Evidence for Surface Volatiles , 2013, Science.

[32]  Andrew P. Ingersoll,et al.  Stability of polar frosts in spherical bowl-shaped craters on the Moon, Mercury, and Mars , 1992 .

[33]  H. J. Melosh,et al.  The global albedo of the Moon at 1064 nm from LOLA , 2014 .

[34]  David E. Smith,et al.  Evidence for surface water ice in the lunar polar regions using reflectance measurements from the Lunar Orbiter Laser Altimeter and temperature measurements from the Diviner Lunar Radiometer Experiment. , 2017, Icarus.

[35]  C. Russell,et al.  The Putative Cerean Exosphere , 2017 .

[36]  Fraser P. Fanale,et al.  Near-Surface Ice on Mercury and the Moon: A Topographic Thermal Model , 1994 .