Seismic Velocity Variations in a 3D Martian Mantle: Implications for the InSight Measurements

نویسندگان

چکیده

We use a large data set of 3D thermal evolution models to predict the distribution present-day seismic velocities in Martian interior. Our show difference between maximum and minimum S wave velocity up 10% either below crust, where variations are largest, or at depth olivine wadsleyite phase transition, located around 1,000–1,200 km depth. Models with thick lithospheres on average have weak low-velocity zones that extend deeper than 400 uppermost 400–600 closely follow crustal thickness pattern. For these cases, crust contains more half total amount heat-producing elements. limited heat production thinner shallower but prominent incompatible Interior exploration using Seismic Investigations, Geodesy Heat Transport (InSight) observations. events suggested originate Cerberus Fossae indicate absence shadow 25°–30° epicentral distance. This result is compatible previous best fit require lithospheric containing bulk elements be geological geophysical constraints. Ongoing future InSight measurements will determine existence zone directly bear production.

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ژورنال

عنوان ژورنال: Journal Of Geophysical Research: Planets

سال: 2021

ISSN: ['2169-9100', '2169-9097']

DOI: https://doi.org/10.1029/2020je006755