Details

Autor(en) / Beteiligte

• Willmes, Malte
• Reiss, Dennis
• Hiesinger, Harald
• Zanetti, Michael

Titel

Surface age of the ice–dust mantle deposit in Malea Planum, Mars

Ist Teil von

• Planetary and space science, 2012-01, Vol.60 (1), p.199-206

Ort / Verlag

Elsevier Ltd

Erscheinungsjahr

2012

Link zum Volltext

Quelle

Elsevier ScienceDirect Journals Complete

Beschreibungen/Notizen

• The mid- and high-latitudes of Mars are covered by a smooth young mantle that is interpreted as an atmospherically derived air-fall deposit of ice and dust related to recent climate changes. In order to determine relative and absolute ages of this surface unit within the southern hemisphere, a systematic survey of all available HiRISE and CTX images in the Malea Planum region from 55–60°S latitude and 50–70°E longitude was performed and the distribution and the morphology of small impact craters on the mantle deposit were investigated. Using crater size-frequency measurements, we derived absolute model ages of ∼3–5Ma for the surface of the mantle, immediately south of the Hellas basin rim. Morphologic observations of the mantle, its fresh appearance, very low number of craters, and superposition on older units support this very young Amazonian age. Nearly all observed craters on the smooth mantle in Malea Planum are small and show signs of erosion, evidence for the ongoing modification of the ice–dust mantle. However, this modification has not been strong enough to reset the surface age. Compared to the ice–dust mantle at higher latitudes in the northern and southern hemisphere, the surface of the mantle in Malea Planum is older and thus has been relatively stable during obliquity changes in the last ∼3–5Ma. This is consistent with the hypothesis that the ice–dust mantle is a complex surface deposit of different layers, that shows a strong latitude dependence in morphology and has been deposited and degraded at different times in martian history. ▶ The ice–dust mantle in Malea Planum has a surface age of ∼3–5Ma. ▶ The surface age is most likely connected to the last major deposition of the mantle. ▶ Small fresh craters <50m have been obliterated during recent mantle modification