[HTML][HTML] Mars seismology
P Lognonné, WB Banerdt, J Clinton… - Annual Review of …, 2023 - annualreviews.org
For the first time, from early 2019 to the end of 2022, Mars' shallow and deep interiors have
been explored by seismology with the InSight mission. Thanks to the performances of its …
been explored by seismology with the InSight mission. Thanks to the performances of its …
Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation
LV Posiolova, P Lognonné, WB Banerdt, J Clinton… - Science, 2022 - science.org
Two> 130-meter-diameter impact craters formed on Mars during the later half of 2021. These
are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter …
are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter …
Surface waves and crustal structure on Mars
We detected surface waves from two meteorite impacts on Mars. By measuring group
velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal …
velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal …
Geophysical evidence for an active mantle plume underneath Elysium Planitia on Mars
A Broquet, JC Andrews-Hanna - Nature Astronomy, 2023 - nature.com
Although the majority of volcanic and tectonic activity on Mars occurred during the first 1.5
billion years of its geologic history, recent volcanism, tectonism and active seismicity in …
billion years of its geologic history, recent volcanism, tectonism and active seismicity in …
An overview of sedimentary volcanism on Mars
Extensive fields of sub-kilometre-to kilometre-scale mounds, cones, domes, shields, and
flow-like edifices cover large parts of the martian lowlands. These features have been …
flow-like edifices cover large parts of the martian lowlands. These features have been …
Crustal anisotropy in the Martian lowlands from surface waves
The largest seismic event ever recorded on Mars, with a moment magnitude of 4.7±0.2, is
the first event to produce both Love and Rayleigh wave signals. We measured their group …
the first event to produce both Love and Rayleigh wave signals. We measured their group …
Structure along the Martian dichotomy constrained by Rayleigh and love waves and their overtones
Using seismic recordings of event S1222a, we measure dispersion curves of Rayleigh and
Love waves, including their first overtones, and invert these for shear velocity (VS) and radial …
Love waves, including their first overtones, and invert these for shear velocity (VS) and radial …
Liquid water in the Martian mid-crust
Large volumes of liquid water transiently existed on the surface of Mars more than 3 billion
years ago. Much of this water is hypothesized to have been sequestered in the subsurface …
years ago. Much of this water is hypothesized to have been sequestered in the subsurface …
High‐frequency receiver functions with event S1222a reveal a discontinuity in the Martian shallow crust
J Shi, M Plasman, B Knapmeyer‐Endrun… - Geophysical …, 2023 - Wiley Online Library
The shallow crustal structure of Mars records the evolutionary history of the planet, which is
crucial for understanding the early Martian geological environment. Until now, seismic …
crucial for understanding the early Martian geological environment. Until now, seismic …
Investigation of Martian regional crustal structure near the dichotomy using S1222a surface‐wave group velocities
Abstract Knowledge of Martian crust and uppermost mantle aid us studying the planet's
evolution. NASA's InSight mission provides seismic data being used to reveal the interior …
evolution. NASA's InSight mission provides seismic data being used to reveal the interior …