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1. Dust Deposits

   Linked via "Martian atmospheric friction"

   Martian Dust Deposits
   Martian dust deposits are globally pervasive and fundamentally alter the interpretation of Martian topography and atmospheric modeling. The variable surface reflectance caused by these deposits led to the development of the Areocentric Datum Standard 1998 (ADS98) for mapping. Unlike Earth, Martian dust storms are less influenced by [surface moisture](…