While the processes and products of lunar space weathering are reasonably well-studied, their accumulation rates in lunar soils are poorly constrained. Previously, we showed that the thickness of solar wind irradiated rims on soil grains is a smooth function of their solar flare particle track density, whereas the thickness of vapor-deposited rims was largely independent of track density [1]. Here, we have extended these preliminary results with data on additional grains from other mature soils.


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    Titel :

    Rates of Space Weathering in Lunar Regolith Grains


    Beteiligte:
    Zhang, S. (Autor:in) / Keller, L. P. (Autor:in)

    Kongress:

    75the Annual Meeting of the Meteroritical Society ; 2012 ; Cairns, Australia


    Erscheinungsdatum :

    2012-08-12


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




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