[HTML][HTML] SEIS: Insight's seismic experiment for internal structure of Mars
By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars,
InSight will deploy onto Mars' surface the SEIS (S eismic E xperiment for I nternal S tructure) …
InSight will deploy onto Mars' surface the SEIS (S eismic E xperiment for I nternal S tructure) …
Impact-seismic investigations of the InSight mission
Impact investigations will be an important aspect of the InSight mission. One of the scientific
goals of the mission is a measurement of the current impact rate at Mars. Impacts will …
goals of the mission is a measurement of the current impact rate at Mars. Impacts will …
Updated lunar cratering chronology model with the radiometric age of Chang'e-5 samples
Z Yue, K Di, W Wan, Z Liu, S Gou, B Liu, M Peng… - Nature …, 2022 - nature.com
Lunar chronology models are built by associating the radiometric ages of samples returned
by the Apollo and Luna missions measured in the laboratory with compiled crater …
by the Apollo and Luna missions measured in the laboratory with compiled crater …
Martian dunes indicative of wind regime shift in line with end of ice age
Orbital observations suggest that Mars underwent a recent 'ice age'(roughly 0.4–2.1 million
years ago), during which a latitude-dependent ice-dust mantle (LDM), was emplaced. A …
years ago), during which a latitude-dependent ice-dust mantle (LDM), was emplaced. A …
Seismically detected cratering on Mars: Enhanced recent impact flux?
Seismic observations of impacts on Mars indicate a higher impact flux than previously
measured. Using six confirmed seismic impact detections near the NASA InSight lander and …
measured. Using six confirmed seismic impact detections near the NASA InSight lander and …
A tectonic origin for the largest marsquake observed by InSight
B Fernando, IJ Daubar… - Geophysical …, 2023 - Wiley Online Library
The S1222a marsquake detected by InSight on 4 May 2022 was the largest of the mission,
at 4.7. Given its resemblance to two other large seismic events (S1000a and S1094b), which …
at 4.7. Given its resemblance to two other large seismic events (S1000a and S1094b), which …
A two‐step K‐Ar experiment on Mars: Dating the diagenetic formation of jarosite from Amazonian groundwaters
PE Martin, KA Farley, MB Baker… - Journal of …, 2017 - Wiley Online Library
Following K‐Ar dating of a mudstone and a sandstone, a third sample has been dated by the
Curiosity rover exploring Gale Crater. The Mojave 2 mudstone, which contains relatively …
Curiosity rover exploring Gale Crater. The Mojave 2 mudstone, which contains relatively …
An estimate of the impact rate on Mars from statistics of very-high-frequency marsquakes
The number density of impact craters on a planetary surface is used to determine its age,
which requires a model for the production rate of craters of different sizes. On Mars …
which requires a model for the production rate of craters of different sizes. On Mars …
Transverse aeolian ridges in the landing area of the Tianwen-1 Zhurong rover on Utopia Planitia, Mars
S Gou, Z Yue, K Di, C Zhao, R Bugiolacchi… - Earth and Planetary …, 2022 - Elsevier
The enigmatic transverse aeolian ridges (TARs), with distinct morphology and albedo, are
among the key geological features investigated by China's Tianwen-1 Zhurong rover on …
among the key geological features investigated by China's Tianwen-1 Zhurong rover on …
A new chronology from debiased crater densities: Implications for the origin and evolution of lunar impactors
The giant planets are believed to experience dynamic instability, delivering numerous
impactors (asteroids, comets and leftover planetesimals) to the Moon. Dynamic simulations …
impactors (asteroids, comets and leftover planetesimals) to the Moon. Dynamic simulations …