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\begin{document}

\title{DISCUSSION ON SEISMICALLY TRIGGERED AVALANCHES ON MARS}



\author[1]{Antoine Lucas}%
\author[2]{I J Daubar}%
\author[3]{M Le Teuff}%
\author[4]{L V Posiolova}%
\author[3]{G Sainton}%
\author[3]{A Mangeney}%
\author[5]{C Perrin}%
\author[3]{T Kawamura}%
\author[6]{D Giardini}%
\author[3]{P Lognonné}%
\affil[1]{Affiliation not available}%
\affil[2]{Univ of AZ-Planetary Sciences}%
\affil[3]{Université Paris Cité, IPGP, CNRS}%
\affil[4]{Malin Space Science Systems}%
\affil[5]{Laboratoire de Planétologie et Géosciences, CNRS, Université}%
\affil[6]{Department of Earth Sciences, Institute of Geophysics, ETH Zurich}%


\vspace{-1em}



  
  \date{May 07, 2024}


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\begin{abstract}
Motivation: On May 5, 2022, the martian SEIS seismometer recorded an
unprecedented M Ma W 4.7 Marsquake. The epicenter is located at 3.0 * S,
171.9 * E. The areas is barely flat with only a few N-S tectonic-like
features. Most unfilled impact craters and ridges show dust avalanches
(a.k.a. Slope streaks). We investigate the post-seismic outcomes in
terms of avalanche triggering under today's Mars conditions in the
framework of the s1222a event.%
\end{abstract}%



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\includegraphics[width=0.70\columnwidth]{figures/LPSC-s1222a-POSTER-2023-(3)/LPSC-s1222a-POSTER-2023-(3)}
\caption{{LPSC Poster
{\label{502108}}%
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