skip to primary navigation skip to content
 

 

You are not currently logged in

SPRI library catalogue

View a record

Please note: You are viewing the legacy database of the Scott Polar Research Institute Library catalogue. It is no longer being updated, so does not reliably reflect our current library holdings.

Please search for material in iDiscover for up-to-date information about the library collection.


Record #112065:

Exospheric transport restrictions on water ice in lunar polar traps / R. Richard Hodges, Jr.

Title: Exospheric transport restrictions on water ice in lunar polar traps / R. Richard Hodges, Jr.
Author(s): Hodges, R. Richard,
Date: 1991.
In: Geophysical Research Letters. (1991.), Vol. 18(11) (1991)
Abstract: At least 10¹⁷ g water has accreted on Moon by reduction of ferric iron by solar wind protons, vapourization of chondrites, and comet impacts. Most is probably there now. If water were to have migrated to permanently shaded cold traps near lunar poles, ice deposits with densities >1000 g cm⁻² would cover traps, providing accessible resources. However, exospheric transport considerations suggest that actual amount of water ice in cold traps is probably too small to be of practical interest. Alternative is global assimilation of most of water into regolith, which must account for about 30 μmol water per gram of soil.
Notes:

Geophysical Research Letters. Vol. 18(11) :2113-2116 (1991).

Keywords: 551.32 -- Glaciology.
523.3 -- Moon.
556 -- Hydrology.
E13 -- Glaciology: glacioastronomy.
SPRI record no.: 112065

MARCXML

LDR 01360naa#a2200000#a#4500
001 SPRI-112065
005 20240419004014.0
007 ta
008 240419s1991####xx####|##|###|0||#0|eng#d
035 ## ‡aSPRI-112065
040 ## ‡aUkCU-P‡beng‡eaacr
100 1# ‡aHodges, R. Richard,‡cJr.
245 10 ‡aExospheric transport restrictions on water ice in lunar polar traps /‡cR. Richard Hodges, Jr.
260 ## ‡a[S.l.] :‡b[s.n.],‡c1991.
300 ## ‡ap. 2113-2116.
500 ## ‡aGeophysical Research Letters. Vol. 18(11) :2113-2116 (1991).
520 3# ‡aAt least 10¹⁷ g water has accreted on Moon by reduction of ferric iron by solar wind protons, vapourization of chondrites, and comet impacts. Most is probably there now. If water were to have migrated to permanently shaded cold traps near lunar poles, ice deposits with densities >1000 g cm⁻² would cover traps, providing accessible resources. However, exospheric transport considerations suggest that actual amount of water ice in cold traps is probably too small to be of practical interest. Alternative is global assimilation of most of water into regolith, which must account for about 30 μmol water per gram of soil.
650 07 ‡a551.32 -- Glaciology.‡2udc
650 07 ‡a523.3 -- Moon.‡2udc
650 07 ‡a556 -- Hydrology.‡2udc
650 07 ‡aE13 -- Glaciology: glacioastronomy.‡2local
773 0# ‡7nnas ‡tGeophysical Research Letters. ‡gVol. 18(11) (1991) ‡wSPRI-1033
917 ## ‡aUnenhanced record from Muscat, imported 2019
948 3# ‡a20240419