Don't drink the water

被引:9
作者
Reed, GW [1 ]
机构
[1] Argonne Natl Lab, Div Chem, Argonne, IL 60439 USA
来源
METEORITICS & PLANETARY SCIENCE | 1999年 / 34卷 / 05期
关键词
D O I
10.1111/j.1945-5100.1999.tb01394.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
If water exists in permanently shadowed terrain on the Moon as suggested by a number of investigators (Watson et al., 1961; Arnold, 1979; Hedges, 1980; Nozette et al., 1996; Duke and Whittaker, 1997) and strongly supported by the Lunar Prospector neutron flux measurements (Feldman et al., 1998), the results of studies on another volatile, namely Hg, are quite relevant. Whereas water has not been positively found, a large number of studies have established the presence of Hg in lunar samples. Its presence and volatile behavior are important when considering water as probably the most important in situ lunar resource. Here we show that the amount of Hg in lunar cold traps may be comparable to the amounts of water.
引用
收藏
页码:809 / 811
页数:3
相关论文
共 34 条
[1]  
ARNOLD JR, 1979, J GEOPHYS RES, V84, P5649
[2]  
BERNATOWICZ T, 1982, LUNAR PLANET SCI, V13, P39
[3]  
BOGARD DD, 1972, APOLLO 15 LUNAR SAMP, P342
[4]  
DUKE MB, 1997, LUNAR PLANET SCI, V28, P311
[5]   Fluxes of fast and epithermal neutrons from lunar prospector: Evidence for water ice at the lunar poles [J].
Feldman, WC ;
Maurice, S ;
Binder, AB ;
Barraclough, BL ;
Elphic, RC ;
Lawrence, DJ .
SCIENCE, 1998, 281 (5382) :1496-1500
[6]   A spectroscopic survey of metallic species abundances in the lunar atmosphere [J].
Flynn, BC ;
Stern, SA .
ICARUS, 1996, 124 (02) :530-536
[7]  
HEIKEN G, 1973, P LUNAR PLANET SCI C, P191
[8]  
Hodges Jr R. R., 1973, GEOCHIM COSM SUPPL, V4, P2855
[9]  
Hodges R.R., 1981, LUNAR PLANETARY I SC, P451
[10]  
Hodges R. R., 1980, Lunar and Planetary Science Conference, V11, P2463