[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 …
Geophysical evidence for an enriched molten silicate layer above Mars's core
The detection of deep reflected S waves on Mars inferred a core size of 1,830±40 km (ref.),
requiring light-element contents that are incompatible with experimental petrological …
requiring light-element contents that are incompatible with experimental petrological …
First observations of core-transiting seismic phases on Mars
We present the first observations of seismic waves propagating through the core of Mars.
These observations, made using seismic data collected by the InSight geophysical mission …
These observations, made using seismic data collected by the InSight geophysical mission …
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 …
Focal Mechanism Determination of Event S1222a and Implications for Tectonics Near the Dichotomy Boundary in Southern Elysium Planitia, Mars
Abstract On 4 May 2022 the InSight seismometer SEIS‐VBB recorded the largest marsquake
ever observed, S1222a, with an initial magnitude estimate of 4.6. Understanding the depth …
ever observed, S1222a, with an initial magnitude estimate of 4.6. Understanding the depth …
Constraints on the martian crust away from the InSight landing site
The most distant marsquake recorded so far by the InSight seismometer occurred at an
epicentral distance of 146.3±6.9 o, close to the western end of Valles Marineris. On the …
epicentral distance of 146.3±6.9 o, close to the western end of Valles Marineris. On the …
Crustal structure constraints from the detection of the SsPp phase on Mars
The shallowest intracrustal layer (extending to 8±2 km depth) beneath the Mars InSight
Lander site exhibits low seismic wave velocity, which is likely related to a combination of …
Lander site exhibits low seismic wave velocity, which is likely related to a combination of …
A positive feedback between crustal thickness and melt extraction for the origin of the Martian dichotomy
A North/South difference in crustal thickness is likely at the origin of the Martian dichotomy in
topography. Recent crustal thickness maps were obtained by inversion of topography and …
topography. Recent crustal thickness maps were obtained by inversion of topography and …
Estimating primary magmas from Mars with PRIMARSMELT: Implications for the petrogenesis of some Martian rocks and the thermal evolution of Mars
Primary magmas form by partial melting in the mantle of a terrestrial planet and represent
the starting material for building its crust. The compositions of primary magmas are critical for …
the starting material for building its crust. The compositions of primary magmas are critical for …
Prussian blue analogue-derived high-entropy alloy nanoarchitectonics for efficient Fenton-like catalysis
Y Yao, S Wang, C Wang, Z Wu, C **ao… - Journal of Materials …, 2024 - pubs.rsc.org
The selective distribution of reactive oxygen species originating from the optimized
activation of peroxymonosulfate (PMS) offers opportunities to achieve the effective …
activation of peroxymonosulfate (PMS) offers opportunities to achieve the effective …