Evidence for Water Ice Near Mercury's North Pole from MESSENGER Neutron Spectrometer Measurements

被引:143
作者
Lawrence, David J. [1 ]
Feldman, William C. [2 ]
Goldsten, John O. [1 ]
Maurice, Sylvestre [3 ]
Peplowski, Patrick N. [1 ]
Anderson, Brian J. [1 ]
Bazell, David [1 ]
McNutt, Ralph L., Jr. [1 ]
Nittler, Larry R. [4 ]
Prettyman, Thomas H. [2 ]
Rodgers, Douglas J. [1 ]
Solomon, Sean C. [4 ,5 ]
Weider, Shoshana Z. [4 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Planetary Sci Inst, Tucson, AZ 85719 USA
[3] Univ Toulouse 3, CNRS, Observ Midi Pyrenees, Inst Rech Astrophys & Planetol, F-31062 Toulouse, France
[4] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA
[5] Columbia Univ, Lamont Doherty Earth Observ, Palisades, NY 10964 USA
关键词
LUNAR PROSPECTOR; MOON; SURFACE; REGOLITH; HYDROGEN; DEPOSITS; ELEMENTS; RAY;
D O I
10.1126/science.1229953
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Measurements by the Neutron Spectrometer on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft show decreases in the flux of epithermal and fast neutrons from Mercury's north polar region that are consistent with the presence of water ice in permanently shadowed regions. The neutron data indicate that Mercury's radar-bright polar deposits contain, on average, a hydrogen-rich layer more than tens of centimeters thick beneath a surficial layer 10 to 30 cm thick that is less rich in hydrogen. Combined neutron and radar data are best matched if the buried layer consists of nearly pure water ice. The upper layer contains less than 25 weight % water-equivalent hydrogen. The total mass of water at Mercury's poles is inferred to be 2 x 10(16) to 10(18) grams and is consistent with delivery by comets or volatile-rich asteroids.
引用
收藏
页码:292 / 296
页数:5
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