Regolith formation on Phobos and Deimos

M. Banaszkiewicz; W. H. Ip

doi:10.1016/b978-0-08-040787-6.50020-3

Regolith formation on Phobos and Deimos

M. Banaszkiewicz, W. H. Ip

Graduate Institute of Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

Regolith formation on the Martian satellites is considered as a stochastic process. Each cratering event is further divided into five elementary processes: impact cratering, launching of ejecta, blanket formation and recapturing of ejecta from circum-Mars orbits. Peculiarities of the blanket shape for Phobos and Deimos ejecta, found from calculations, are indicated. The possible scenario of the regolith development on the satellites is discussed. -Authors

Original language	English
Pages (from-to)	109-112
Number of pages	4
Journal	Unknown Journal
DOIs	https://doi.org/10.1016/b978-0-08-040787-6.50020-3
State	Published - 1991

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title = "Regolith formation on Phobos and Deimos",

abstract = "Regolith formation on the Martian satellites is considered as a stochastic process. Each cratering event is further divided into five elementary processes: impact cratering, launching of ejecta, blanket formation and recapturing of ejecta from circum-Mars orbits. Peculiarities of the blanket shape for Phobos and Deimos ejecta, found from calculations, are indicated. The possible scenario of the regolith development on the satellites is discussed. -Authors",

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AU - Banaszkiewicz, M.

AU - Ip, W. H.

PY - 1991

Y1 - 1991

N2 - Regolith formation on the Martian satellites is considered as a stochastic process. Each cratering event is further divided into five elementary processes: impact cratering, launching of ejecta, blanket formation and recapturing of ejecta from circum-Mars orbits. Peculiarities of the blanket shape for Phobos and Deimos ejecta, found from calculations, are indicated. The possible scenario of the regolith development on the satellites is discussed. -Authors

AB - Regolith formation on the Martian satellites is considered as a stochastic process. Each cratering event is further divided into five elementary processes: impact cratering, launching of ejecta, blanket formation and recapturing of ejecta from circum-Mars orbits. Peculiarities of the blanket shape for Phobos and Deimos ejecta, found from calculations, are indicated. The possible scenario of the regolith development on the satellites is discussed. -Authors

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DO - 10.1016/b978-0-08-040787-6.50020-3

M3 - 期刊論文

AN - SCOPUS:0026288078

SP - 109

EP - 112

JO - Unknown Journal

JF - Unknown Journal

ER -

Regolith formation on Phobos and Deimos

Abstract

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