A Tectonic Origin for the Largest Marsquake Observed by InSight

Author:

Fernando Benjamin1ORCID,Daubar Ingrid J.2ORCID,Charalambous Constantinos3ORCID,Grindrod Peter M.4ORCID,Stott Alexander5ORCID,Al Ateqi Abdullah6ORCID,Atri Dimitra6ORCID,Ceylan Savas7ORCID,Clinton John7ORCID,Fillingim Matthew8ORCID,Hauber Ernest9ORCID,Hill Jonathon R.10ORCID,Kawamura Taichi11ORCID,Liu Jianjun12,Lucas Antoine11ORCID,Lorenz Ralph13ORCID,Ojha Lujendra14ORCID,Perrin Clement15ORCID,Piqueux Sylvain16ORCID,Stähler Simon7ORCID,Tirsch Daniela9ORCID,Wilson Colin17ORCID,Wójcicka Natalia18ORCID,Giardini Domenico7ORCID,Lognonné Philippe11ORCID,Banerdt W. Bruce16ORCID

Affiliation:

1. Department of Physics University of Oxford Oxford UK

2. Department of Earth, Environmental, and Planetary Sciences Brown University Providence RI USA

3. Department of Electrical and Electronic Engineering Imperial College London London UK

4. Natural History Museum London UK

5. ISAE‐SUPAERO Toulouse France

6. Center for Space Science New York University Abu Dhabi UAE

7. Department of Earth Sciences ETH Zurich Zurich Switzerland

8. Space Sciences Laboratory University of California Berkeley Berkeley CA USA

9. Institute of Planetary Research German Aerospace Center (DLR) Berlin Germany

10. School of Earth and Space Exploration Arizona State Univeristy Tempe AZ USA

11. Institut de Physique du Globe de Paris CNRS Université Paris Cité Paris France

12. National Astronomical Observatories Chinese Academy of Sciences Beijing China

13. Applied Physics Laboratory Johns Hopkins University Baltimore MD USA

14. Department of Earth and Planetary Sciences Rutgers University New York NY USA

15. Laboratoire de Planétologie et Géosciences Nantes Université Nantes France

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

17. European Space Agency Noordwijk The Netherlands

18. Department of Earth Science and Engineering Imperial College London London UK

Abstract

AbstractThe S1222a marsquake detected by InSight on 4 May 2022 was the largest of the mission, at 4.7. Given its resemblance to two other large seismic events (S1000a and S1094b), which were associated with the formation of fresh craters, we undertook a search for a fresh crater associated with S1222a. Such a crater would be expected to be ∼300 m in diameter and have a blast zone on the order of 180 km across. Orbital images were targeted and searched as part of an international, multi‐mission effort. Comprehensive analysis of the area using low‐ and medium‐resolution images reveals no relevant transient atmospheric phenomena and no fresh blast zone. High‐resolution coverage of the epicentral area from most spacecraft are more limited, but no fresh crater or other evidence of a new impact have been identified in those images either. We thus conclude that the S1222a event was highly likely of tectonic origin.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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