- 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.