News release
From:
Springer Nature
Mars InSight lander records impact of meteoroids
Seismic waves produced by meteoroid impact events on Mars have been detected by NASA’s InSight lander and traced to the associated, newly formed impact craters by NASA’s Mars Reconnaissance Orbiter, according to a study published in Nature Geoscience. The study presents the first detections of seismic and acoustic waves from impacts on another planet that have been linked to the source craters.
The atmospheric entry and surface collision of a meteoroid at high speeds generates shock waves. These decay into seismic and acoustic waves that can be detected by seismometers. Such waves have been recorded for airburst events — where the impactor breaks up before reaching the surface — in Earth’s atmosphere, and for the formation of a single small impact crater on Earth. However, geophysical observations of new crater formation on other planets have been limited.
Raphael Garcia and colleagues analysed seismometer data from the InSight lander and identified seismic and acoustic waves from four events. The authors used the arrival times of the waves to calculate the location of each of these four events, and then requested imaging from the Mars Reconnaissance Orbiter to confirm the impact sites for three of them (the fourth was a seismic event associated to an impact previously detected by imaging). With the source craters known, the impact-induced waves can be used to provide information about the cratering process and the properties of the Martian atmosphere and crust.
The authors conclude that these findings demonstrate the value of planetary seismology for studying impact processes on other worlds.
Journal/
conference:
Nature Geoscience
Organisation/s:
Curtin University, Université de Toulouse, France
Funder:
This study is InSight contribution number 241 and LA-UR-22-25144. The French
authors acknowledge the French Space Agency CNES and ANR (ANR-14-CE36-0012-02
and ANR-19-CE31-0008-08) for funding the InSight Science analysis. I.J.D. was
supported by NASA grant 80NSSC20K0971. P.L., Z.X., S.M., M.F., T.K. and M. Plasman
acknowledge IdEx Université de Paris ANR-18-IDEX-0001. N.W. and G.S.C. are funded
by the UK Space Agency (Grants ST/S001514/1 and ST/T002026/1). N.A.T. and A.H. are funded by the UK Space Agency (grants ST/R002096/1 and ST/W002523/1). M.F. is
funded by the Center for Space and Earth Science of Los Alamos National Laboratory.
S.C.S., N.L.D., C.D. and G.Z., acknowledge support from ETHZ through the ETH+
funding scheme (ETH+2 19-1: ‘Planet MARS’). A.R., K.M., E.K.S. and T.N. are funded
by the Australian Research Council (DE180100584, DP180100661 and DP180100661).
W.B.B., M. Panning, and L. Martire were supported by the NASA InSight mission
and funds from the Jet Propulsion Laboratory, California Institute of Technology,
under a contract with the National Aeronautics and Space Administration (grant
80NM0018D0004). N.C.S. was supported by funds from the National Aeronautics
and Space Administration (grant 80NSSC18K1628). The authors thank CALMIP
(Toulouse, France, project #p1404) computing centre for HPC resources. We
acknowledge NASA, CNES, their partner agencies and institutions (UKSA, SSO, DLR,
JPL, IPGP-CNRS, ETHZ, IC and MPS-MPG) and the flight operations team at JPL,
SISMOC, MSDS, IRIS-DMC and PDS for providing SEED SEIS data. We are grateful to
the CTX and HiRISE operations teams who planned and acquired the orbital images of
the new impacts.