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10.1134/S1069351319040025

We analyze nonhydrostatic stress field in the Martian interior for two types of heterogeneous elastic models: the ones with a lithosphere and the ones with a lithosphere and probable melting zones within it.

Nonhydrostatic Stress State in the Martian Interior for Different Rheological Models

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10.1016/b978-0-12-804191-8.00002-7

Therefore in order to understand the concentrations of volatiles in the crust, it is vital to first constrain the volatile budget of the Martian interior, the preeruptive volatile content of Martian magmas, and evidence within the Martian meteorites for magmatic degassing.

Volatiles in Martian Magmas and the Interior

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10.1007/978-3-319-97670-9_27

To evaluate the stress field in the Martian interior a static-state approach is applied.

Non-hydrostatic Stresses Under the Local Structures on Mars

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Martian Interior - We analyze nonhydrostatic stress field in the Martian interior for two types of heterogeneous elastic models: the ones with a lithosphere and the ones with a lithosphere and probable melting zones within it. [1] Therefore in order to understand the concentrations of volatiles in the crust, it is vital to first constrain the volatile budget of the Martian interior, the preeruptive volatile content of Martian magmas, and evidence within the Martian meteorites for magmatic degassing. [2] To evaluate the stress field in the Martian interior a static-state approach is applied. [3]