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 …

Bright radar reflections observed beneath the south polar layered deposits (SPLD) by the
Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument were …

Abnormally bright radar reflections below the Martian south polar layered deposit were
originally interpreted as evidence of subglacial liquid water. However, unlike on Earth …

NATURE ASTRONOMY deposit, potentially resulting in stronger subsurface reflections. The
region where bright reflectors were originally mapped 4 is not located below the south polar …

In recent decades, extensive research has led to the understanding that Mars once hosted
substantial liquid-water reserves. While the current Martian landscape boasts significant …

The planet Mars is the most probable among the terrestrial planets in our solar system to
support human settlement or colonization in the future. The detection of water ice or liquid …

The seismometer deployed by the InSight lander measured the seismic velocity of the
Martian crust. We use a rock physics model to interpret those velocities and constrain …

We expand on previous studies of the South Polar Layered Deposits'(SPLD) basal interface
using data acquired by the Mars Advanced Radar for Subsurface and Ionospheric Sounding …

The flexure of the lithosphere under stresses imposed by the geologically young south polar
cap is one of the few clues we have regarding the south polar cap composition and the …

Strong radar reflections have been previously mapped at the base of the Martian South
Polar Layered Deposits. Here, we analyze laboratory measurements of dry and briny …