Detection of Mars Normal Modes From S1222a Event and Seismic Hum

Author:

Lognonné P.1ORCID,Schimmel M.2ORCID,Stutzmann E.1ORCID,Davis P.3,Drilleau M.4ORCID,Sainton G.1ORCID,Kawamura T.1ORCID,Panning M. P.5ORCID,Banerdt W. B.5ORCID

Affiliation:

1. Université Paris Cité Institut de physique du globe de Paris CNRS Paris France

2. Geosciences Barcelona—CSIC Barcelona Spain

3. University of California CA Los Angeles USA

4. Institut supérieur de l’Aéronautique et de l’Espace, Sup Aéro Toulouse France

5. Jet Propulsion Laboratory California Institute of Technology CA Pasadena USA

Abstract

AbstractWe present the first detection of normal modes on Mars using the vertical records from InSight's broad‐band seismometer following the marsquake that occurred on sol 1222. The proposed catalog lists 60 potential eigenfrequencies between 3 and 12 mHz. Due to their low signal‐to‐noise ratio, these normal modes were detected using the phasor walkout approach. The normal modes amplitudes are consistent with the upper limit of the S1222a magnitude and with high quality factors. Additionally, we provide the first detection of a Martian hum before the quake for several of these frequencies. The proposed frequencies are at about 1‐sigma of those predicted by published models based on body wave travel time inversions. Our detection of normal modes is the first made on a terrestrial planet other than Earth and opens the way for future interior models that incorporate both normal modes frequencies, surface waves velocities and body wave travel times.

Funder

Agence Nationale de la Recherche

Centre National d’Etudes Spatiales

National Aeronautics and Space Administration

Jet Propulsion Laboratory

California Institute of Technology

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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