- 1EHU, Bilbao, Spain (alexander.stott@ehu.eus)
- 2ISAE-Supaero, Université de Toulouse, France
- 3Institut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, France.
- 4IPGP, Paris, France
- 5University of Bristol, UK
- 6Imperial College London, UK
Over the 1440-sol mission of the NASA InSight lander, more than 1900 seismic events (marsquakes) were recorded and catalogued by the Marsquake service [1]. These events have enabled the determination of both the bulk interior structure [e.g. 2,3,4] and hinted at more curious aspects, for example, a basal mantle layer [5,6], mantle plumes/dynamics [e.g. 7] and crustal heterogeneities [e.g. 8]. Much evidence for such features has come from a small select group of events, owing to their superior signal quality or magnitude. On top of this, only a handful of events have generated deep mantle phases [9].
Given that InSight is only a single station, it is necessary to develop methods that extract information from a broader range of marsquakes to further develop our understanding of event origins and interior structure. To this end, we propose a clustering approach for the P-wave coda of events. This method targets the relatively underused high frequency energy of events, typically dominated by scattering [8] and more affected by environmental noise [10]. The clustering approach effectively acts as a selective event stacking to improve signal to noise ratios, identifying only the most similar events to create the stack. Using this method, we identify a set of P-wave coda features and track their evolution over distances.
We will explore the obtained families of P-waves morphology to infer the potential range of event sources and help improve marsquake classifications [1]. This is of interest to probe questions on whether they are generated from tectonic or impact sources [1], with recent research proposing the possibility of a swarm source for certain events [11]. This interpretation, in turn, has implications for the variability of Mars’s crustal structure. Furthermore, the signal to noise ratio improvement highlights delayed energy arrivals, providing new characteristics to infer structural complexities from scattering behaviour [8].
References
[1] Ceylan, Savas, et al. "The marsquake catalogue from InSight, sols 0–1011." Physics of the Earth and Planetary Interiors 333 (2022): 106943.
[2] Knapmeyer-Endrun, Brigitte, et al. "Thickness and structure of the Martian crust from InSight seismic data." Science 373.6553 (2021): 438-443.
[3] Khan, Amir, et al. "Upper mantle structure of Mars from InSight seismic data." Science 373.6553 (2021): 434-438.
[4] Stähler, Simon C., et al. "Seismic detection of the martian core." Science 373.6553 (2021): 443-448.
[5] Samuel, Henri, et al. "Geophysical evidence for an enriched molten silicate layer above Mars’s core." Nature 622.7984 (2023): 712-717.
[6] Khan, Amir, et al. "Evidence for a liquid silicate layer atop the Martian core." Nature 622.7984 (2023): 718-723.
[7] Broquet, Adrien, and Jeffrey C. Andrews-Hanna. "Geophysical evidence for an active mantle plume underneath Elysium Planitia on Mars." Nature Astronomy 7.2 (2023): 160-169.
[8] Menina, S., et al. "Stratification of heterogeneity in the lithosphere of Mars from envelope modeling of event S1222a and near impacts: Interpretation and implications for very‐high‐frequency events." Geophysical Research Letters 50.7 (2023): e2023GL103202.
[9] Horleston, Anna C., et al. "The far side of Mars: Two distant marsquakes detected by InSight." The seismic record 2.2 (2022): 88-99.
[10] Stott, Alexander E., et al. "Machine learning and marsquakes: a tool to predict atmospheric-seismic noise for the NASA InSight mission." Geophysical Journal International 233.2 (2023): 978-998.
[11] Dahmen, Nikolaj L., et al. "Analysis of high frequency Marsquake swarms informed by deep learning." Journal of Geophysical Research: Planets 131.1 (2026): e2025JE009229.
How to cite: Stott, A., Margerin, L., Calvet, M., Garcia, R., Drilleau, M., Fuji, N., Horleston, A., and Kim, D.: Identification of new Marsquake clusters from P-wave coda analysis and implications for crustal structure and seismicity, Europlanet Science Congress 2026, The Hague, The Netherlands, 7–11 Sep 2026, EPSC2026-592, https://doi.org/10.5194/epsc2026-592, 2026.