EGU25-13152, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-13152
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
PICO | Thursday, 01 May, 10:59–11:01 (CEST)
 
PICO spot 1, PICO1.8
The Marsquake Service Reference Catalogue
John Clinton1, Nikolaj Dahmen2, Savas Ceylan2, Simon Stähler2, Domenico Giardini2, Cecilia Duran2, Geraldine Zenhausern2, Fabian Euchner1, Anna Horleston3, Taichi Kawamura4, and Doyeon Kim5
John Clinton et al.
  • 1ETHZ, Swiss Seismological Service, Zurich, Switzerland (jclinton@sed.ethz.ch)
  • 2ETHZ, D-EAPS, Zurich, Switzerland
  • 3U. Bristol, Bristol, United Kingdom
  • 4IPGP, Paris, France
  • 5Imperial College, London, United Kingdom

The Marsquake Service (MQS) [1] is finalizing the release of the reference catalogue of Martian seismicity recorded by NASA’s InSight mission. Previous catalogue versions [2] listed over 1300 events classified by their observed frequency content into i) low frequency (LF) and broadband (BB) - the key events for constraining interior structure, ii) 2.4 Hz and high frequency (HF) -  representing the majority of events with weak signals and enigmatic origin,  and iii) very high frequency (VF) events, including several nearby impacts [3].

Since the last release in April 2023, directly following the mission end, MQS has reviewed the entire data set, also using denoised data sets [4,5] to refine phase picks, back azimuths, and ensuring consistency across the catalogue. 

For distance computation, MQS has adopted an updated suite of interior models, now applied to all event types [6, 7]. Previously 2.4 Hz, HF, and VF events were located using constant crustal velocities. However,  new insights from observations of impacts and surface waves [8,9,10] suggest these events propagate through deeper interior layers, leading to significantly larger distances.

MQS has revised the frequency-based event classification, incorporating spectral analysis [11] and other parameters such as distance and seasonality to improve event characterization. Events are grouped into three interpretation types:

  • i) Tectonic events, mostly located ~30° east of InSight in Cerberus Fossae and in few other regions with deeper sources, include most LF and BB events with low corner frequencies.
  • ii) Swarm events are a subset of HF and 2.4 Hz events clustered in ~44° distance with shallow seasonal sources, though their source region remains speculative; this group has been significantly expanded through deep learning techniques [5].
  • iii) Meteorite impacts, characterized by high corner frequencies, encompass VF events, several large BB events, and HF/2.4Hz events located outside of the swarm region.

The reference catalogue includes over 1900 events with improved locations and new interpretation types, providing a more comprehensive view of Martian seismicity observed by InSight.

[1] Clinton et al (2018), 10.1007/s11214-018-0567-5

[2] Ceylan et al. (2022), 10.1016/j.pepi.2022.106943

[3] Garcia et al (2022), 10.1038/s41561-022-01014-0

[4] Scholz et al (2020), 10.1029/2020EA001317

[5] Dahmen et al. (2024), 10.1093/gji/ggae279

[6] Khan et al. (2023), 10.1038/s41586-023-06586-4

[7] Samuel et al. (2023), 10.1038/s41586-023-06601-8

[8] Posiolova et al. (2022), 10.1126/science.abq7704

[9] Panning et al. (2023), 10.1029/2022GL101270

[10] Charalambous et al. (in press)

[11] Stähler et al. (in prep.)



How to cite: Clinton, J., Dahmen, N., Ceylan, S., Stähler, S., Giardini, D., Duran, C., Zenhausern, G., Euchner, F., Horleston, A., Kawamura, T., and Kim, D.: The Marsquake Service Reference Catalogue, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13152, https://doi.org/10.5194/egusphere-egu25-13152, 2025.