Abstract The Heat Flow and Physical Properties Package HP 3 for the InSight mission will
attempt the first measurement of the planetary heat flow of Mars. The data will be taken at the …

Abstract The Interior exploration using Seismic Investigations, Geodesy, and Heat Transport
(InSight) Mission will focus on Mars' interior structure and evolution. The basic structure of …

A planet's crust bears witness to the history of planetary formation and evolution, but for
Mars, no absolute measurement of crustal thickness has been available. Here, we …

For 2 years, the InSight lander has been recording seismic data on Mars that are vital to
constrain the structure and thermochemical state of the planet. We used observations of …

Vera Rubin ridge (VRR) is an erosion‐resistant feature on the northwestern slope of Mount
Sharp in Gale crater, Mars, and orbital visible/shortwave infrared measurements indicate it …

Analyses of seismic data from the InSight mission have provided the first in situ constraints
on the thickness of the crust of Mars. These crustal thickness constraints are currently limited …

Petrologic investigations of martian rocks have been accomplished by mineralogical,
geochemical, and textural analyses from Mars rovers (with geologic context provided by …

The present‐day thermal state, interior structure, composition, and rheology of Mars can be
constrained by comparing the results of thermal history calculations with geophysical …

The Eridania region in the southern highlands of Mars once contained a vast inland sea with
a volume of water greater than that of all other Martian lakes combined. Here we show that …

The first in situ Martian heat flux measurement to be carried out by the InSight Discovery‐
class mission will provide an important baseline to constrain the present‐day heat budget of …