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contributor authorPhilip T. Metzger
contributor authorChristopher D. Immer
contributor authorCarly M. Donahue
contributor authorBruce T. Vu
contributor authorRobert C. Latta III
contributor authorMatthew Deyo-Svendsen
date accessioned2017-05-08T21:16:23Z
date available2017-05-08T21:16:23Z
date copyrightJanuary 2009
date issued2009
identifier other%28asce%290893-1321%282009%2922%3A1%2824%29.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/45140
description abstractThe erosion of lunar soil by rocket exhaust plumes is investigated experimentally. This has identified the diffusion-driven flow in the bulk of the sand as an important but previously unrecognized mechanism for erosion dynamics. It has also shown that slow regime cratering is governed by the recirculation of sand in the widening geometry of the crater. Scaling relationships and erosion mechanisms have been characterized in detail for the slow regime. The diffusion-driven flow occurs in both slow and fast regime cratering. Because diffusion-driven flow had been omitted from the lunar erosion theory and from the pressure cratering theory of the Apollo and Viking era, those theories cannot be entirely correct.
publisherAmerican Society of Civil Engineers
titleJet-Induced Cratering of a Granular Surface with Application to Lunar Spaceports
typeJournal Paper
journal volume22
journal issue1
journal titleJournal of Aerospace Engineering
identifier doi10.1061/(ASCE)0893-1321(2009)22:1(24)
treeJournal of Aerospace Engineering:;2009:;Volume ( 022 ):;issue: 001
contenttypeFulltext


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