Origin and thermal evolution of Mars [PDF]
The thermal evolution of Mars is governed by subsolidus mantle convection beneath a thick lithosphere. Models of the interior evolution are developed by parameterizing mantle convective heat transport in terms of mantle viscosity, the superadiabatic ...
Drake, M. J. +4 more
core +1 more source
Quantifying crustal stress in the Sinai Peninsula caused by gravitational potential energy and its tectonic implications. [PDF]
Jallouli C, Abdelfattah AK, Alzahrani H.
europepmc +1 more source
Groundwater production from geothermal heating on early Mars and implication for early martian habitability. [PDF]
Ojha L +3 more
europepmc +1 more source
Subaerial crust emergence hindered by phase-driven lower crust densification on early Earth. [PDF]
Tang M, Chen H, Lee CA, Cao W.
europepmc +1 more source
Gravitational spreading of Danu, Freyja and Maxwell Montes, Venus [PDF]
The potential energy of elevated terrain tends to drive the collapse of the topography. This process of gravitational spreading is likely to be more important on Venus than on Earth because the higher surface temperature weakens the crust.
Smrekar, Suzanne E., Solomon, Sean C.
core +1 more source
Least squares collocation method in Moho depth determination in Iran using gravity gradient data. [PDF]
Heydarizadeh Shali H +6 more
europepmc +1 more source
Rapid Quaternary subsidence in the northwestern German North Sea. [PDF]
Arfai J +5 more
europepmc +1 more source
Northern Scandinavian mountains supported by a low-grade eclogitic crustal keel. [PDF]
Kahraman M +5 more
europepmc +1 more source
Volcanic processes within the Petavius crater, nearside of the Moon. [PDF]
Satyakumar AV, Patel S, Patel DD.
europepmc +1 more source
Weakened continental lithosphere beneath the northern Red Sea inferred from elastic thickness. [PDF]
Jallouli C +3 more
europepmc +1 more source

