Updating the Planetary Time Scale: Focus on Mars

Authors

  • Kenneth L. Tanaka Astrogeology Science Center, U.S. Geological Survey, 2255 N. Gemini Dr., Flagstaff, AZ 86001, USA
  • Cathy Quantin-Nataf Laboratoire de Géologie de Lyon, Université Claude Bernard Lyon 1 / CNRS/ ENS Lyon, Bâtiment GEODE, 2 rue Raphaël Dubois, 69622 Villeurbanne, France

Abstract

Formal stratigraphic systems have been developed for the surface materials of the Moon, Mars, Mercury, and the Galilean satellite Ganymede. These systems are based on geologic mapping, which establishes relative ages of surfaces delineated by superposition, morphology, impact crater densities, and other relations and features. Referent units selected from the mapping determine time-stratigraphic bases and/or representative materials characteristic of events and periods for definition of chronologic units. Absolute ages of these units in some cases can be estimated using crater size-frequency data. For the Moon, the chronologic units and cratering record are calibrated by radiometric ages measured from samples collected from the lunar surface. Model ages for other cratered planetary surfaces are constructed primarily by estimating cratering rates relative to that of the Moon. Other cratered bodies with estimated surface ages include Venus and the Galilean satellites of Jupiter. New global geologic mapping and crater dating studies of Mars are resulting in more accurate and detailed reconstructions of its geologic history. Keywords: planets, chronology, stratigraphy, geologic mapping, craters, Mars

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Published

2013-07-26

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Articles