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EVIDENCE FOR THERMAL FATIGUE ON MARS FROM ROCKFALL PATTERNS ON IMPACT CRATER SLOPES

Authors :
Tesson, P.-A.
Conway, S. J.
Mangold, N.
Ciazela, J.
Lewis, S. R.
Mège, D.
Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG)
Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST)
Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Space Research Centre of Polish Academy of Sciences (CBK)
Polska Akademia Nauk = Polish Academy of Sciences (PAN)
The Open University [Milton Keynes] (OU)
Conway, Susan
Source :
50th Lunar and Planetary Science Conference, 50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, Texas, United States, The Open University (ORO-Open Research Online)
Publication Year :
2019
Publisher :
HAL CCSD, 2019.

Abstract

International audience; Introduction: Individual block falls are one of the currently active surface processes on Mars. Similarly to Earth, clasts detach from upslope outcrops roll or bounce downslope, leaving a track on the substratum (Fig. 1). The trails show that the rockfalls are recent, as aeolian processes would infill topographic lows over time. Using rover-track erasure rates, these tracks are likely

Details

Language :
English
Database :
OpenAIRE
Journal :
50th Lunar and Planetary Science Conference, 50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, Texas, United States, The Open University (ORO-Open Research Online)
Accession number :
edsair.dedup.wf.001..0f5c6f3611c33aefbc8f440c70b5529e