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Seismic detection of a deep mantle discontinuity within Mars by InSight
Quancheng Huang1,2, Nicholas C Schmerr1, Scott D King3
1Department of Geology, University of Maryland, College Park, MD 20742.
Scientists detected a seismic discontinuity in Mars' mantle, revealing its thermal and compositional state. This finding helps decipher the planet's formation and evolution, suggesting a more iron-rich mantle than Earth's.
Area of Science:
- Planetary Science
- Seismology
- Mineral Physics
Background:
- Understanding Mars' mantle temperature and composition is key to its formation and evolution.
- A seismic discontinuity is predicted in Mars' deep mantle due to olivine phase transformations.
- The depth of this boundary is sensitive to mantle temperature and composition.
Purpose of the Study:
- To seismically detect and characterize a mid-mantle discontinuity on Mars.
- To constrain the thermal and compositional state of the Martian mantle.
- To test models of Mars' thermochemical evolution.
Main Methods:
- Analysis of seismic data from NASA's InSight Mission.
- Observation of triplicated P and S waves from five teleseismic events.
- Waveform modeling to constrain the depth and characteristics of the discontinuity.
Main Results:
- Detection of a mid-mantle discontinuity at a depth of 1,006 ± 40 km.
- Inferred mantle potential temperature of 1,605 ± 100 K.
- Evidence for a more iron-enriched Martian mantle compared to Earth's.
- Identification of two compatible Martian composition models out of five proposed.
- Simulations indicate a relatively cold Martian mantle in the past (1,720–1,860 K) and a present-day surface heat flow of 21–24 mW/m².
Conclusions:
- The detected discontinuity aligns with the predicted postolivine transition.
- The findings provide crucial constraints on Mars' thermal and compositional evolution.
- The Martian mantle is likely more iron-rich and was cooler in its early history than previously thought.
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