Quick Views of Big Advances
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Maps of the Ice Favorability Index (IFI) in the northern (left) and southern (right) polar regions of the Moon. The IFI is based on modeling a source term (where the H2O comes from), a capture term (the nature of polar cold traps), and a retention term (how H2O is preserved in polar regolith). The white squares on the south polar map indicate the locations of Cabeus crater (left) and Shackleton crater (lower right), which Cannon and Britt discuss in detail. |
(pdf version)
See Reference:
· Cannon, Kevin M. and Britt, Daniel T. (2020) A Geologic Model for Lunar Ice Deposits at Mining Scales, Icarus, v. 347, 113778, doi: 10.1016/j.icarus.2020.113778. [article]
See also:
· Martel, L. M. V. (November 2019) Refueling Space Exploration, PSRD, www.psrd.hawaii.edu/CosmoSparks/Nov19/lunar-propellant-production.html.
· Martel, L. M. V. (October 2010) An Icy Treat—Water ice Confirmed on the Moon, PSRD, www.psrd.hawaii.edu/CosmoSparks/Oct10/Moon-surfacewater.html.
· Spudis, P. D. (December 1996) Ice on the Bone Dry Moon, PSRD, www.psrd.hawaii.edu/Dec96/IceonMoon.html.
· Taylor, G. J. and Martel, L. M. V. (April 2018) New Age for Lunar Exploration, PSRD, www.psrd.hawaii.edu/April18/lunar-exploration.html.
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