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Updated: Oct 22, 2025

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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Thickness and structure of the martian crust from InSight seismic data
Brigitte Knapmeyer-Endrun1, Mark P Panning2, Felix Bissig3
1Bensberg Observatory, University of Cologne, Vinzenz-Pallotti-Str. 26, 51429 Bergisch Gladbach, Germany. bknapmey@uni-koeln.de.
Summary
Scientists measured Mars's crust thickness using seismic data from the InSight lander. The Martian crust is estimated to be between 24 and 72 kilometers thick on average.
Area of Science:
- Planetary Science
- Seismology
- Geophysics
Background:
- The crust records a planet's formation and evolution.
- Mars lacked absolute measurements of crustal thickness prior to this study.
Purpose of the Study:
- To determine the crustal thickness beneath the InSight lander site on Mars.
- To provide the first absolute measurement of Martian crustal thickness.
Main Methods:
- Analysis of seismic phases reflected and converted at subsurface interfaces.
- Utilizing both marsquake recordings and the ambient wavefield.
- Extrapolation of point measurements using global gravity and topography maps.
Main Results:
- Seismic data suggest at least two, possibly three, subsurface interfaces.
- Crustal thickness estimates range from 20 ± 5 km (second interface) to 39 ± 8 km (third interface).
- Average Martian crustal thickness is estimated between 24 and 72 kilometers.
Conclusions:
- The findings provide crucial data for understanding Martian geological evolution.
- Geodynamic and compositional constraints favor thicker crust models with concentrated heat-producing elements at depth.
- This study establishes a new baseline for Martian crustal studies.
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