GEOLOGIC MAPPING TO CONSTRAIN THE SOURCES AND TIMING OF FLUVIAL ACTIVITY IN WESTERN LADON BASIN, MARS
There are fifteen geologic units that we have identified and mapped: Middle Noachian Mountainous Unit (Nm), Late Noachian to Early Hesperian Terra Unit (HNt), Late Noachian to Early Hesperian Channel Units (HNch1 and HNch2), Late Noachian through Hesperian Basin Fill Units (HNb1, HNb2, Hb3), Late Hesperian to Early Amazonian Alluvial Fans Unit (AHf), Hesperian Light-toned Layered Units (Hl1 and Hl2), Hesperian Light-toned Altered Unit (Ha), Amazonian Volcanic Unit (Av), and Crater Units (C1, C2, and C3). The geologic history includes: (i) Formation of Ladon and Holden impact basins in the middle Noachian, producing mountainous unit Nm; (ii) Landscape degradation and infilling during the Midde/Late Noachian with the terra unit HNt; (iii) Formation of Ladon Valles in the Late Noachian to Early Hesperian by catastrophic flooding to produce channel units HNch1 and HNch2; (iv) In the Late Noachian to Early Hesperian, Ladon basin floor accumulated sediments that resulted in units HNb1 and HNb2; (v) Deposition of light-toned layered deposits (Hl1 and Hl2) during the Hesperian within Ladon Valles, Ladon basin, and other smaller valley networks along the western uplands, as well as aqueous alteration along some crater floors (Ha); (vi) Deposition of unit Hb3 within Ladon basin and Ladon Valles; (vii) Eruption of volcanic unit Av in the Amazonian. Craters formed throughout the geologic history of the mapping region.