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 …
Dating very young planetary surfaces from crater statistics: A review of issues and challenges
Determining the ages of young planetary surfaces relies on using populations of small, often
sub‐km diameter impact craters due to the higher frequency at which they form. Smaller …
sub‐km diameter impact craters due to the higher frequency at which they form. Smaller …
Evidence for geologically recent explosive volcanism in Elysium Planitia, Mars
Volcanic activity on Mars peaked during the Noachian and Hesperian periods but has
continued since then in isolated locales. Elysium Planitia hosts numerous young, fissure-fed …
continued since then in isolated locales. Elysium Planitia hosts numerous young, fissure-fed …
A catalogue of impact craters larger than 200 m and surface age analysis in the Chang'e-5 landing area
M Jia, Z Yue, K Di, B Liu, J Liu, G Michael - Earth and Planetary Science …, 2020 - Elsevier
Abstract Chang'e-5 (CE-5) is the first sample-return mission of China's lunar exploration and
will be launched in 2020. The planned landing area is near Mons Rümker in Oceanus …
will be launched in 2020. The planned landing area is near Mons Rümker in Oceanus …
Relative depths of simple craters and the nature of the lunar regolith
We assessed the morphologies of more than 930 simple impact craters (diameters 40 m–10
km) on the Moon using digital terrain models (DTMs) of a variety of terrains in order to …
km) on the Moon using digital terrain models (DTMs) of a variety of terrains in order to …
[HTML][HTML] The equilibrium size-frequency distribution of small craters reveals the effects of distal ejecta on lunar landscape morphology
Small craters of the lunar maria are observed to be in a state of equilibrium, in which the rate
of production of new craters is, on average, equal to the rate of destruction of old craters …
of production of new craters is, on average, equal to the rate of destruction of old craters …
Morphological characteristics of impact craters with diameters of 5–20 km on the Moon
The morphology of impact craters on the Moon plays an important role in understanding
impact cratering process, surface and subsurface properties, and their evolutions. In this …
impact cratering process, surface and subsurface properties, and their evolutions. In this …
Automatic map** of small lunar impact craters using LRO‐NAC images
Impact craters are the most common feature on the Moon's surface. Crater size–frequency
distributions provide critical insight into the timing of geological events, surface erosion …
distributions provide critical insight into the timing of geological events, surface erosion …
Small crater modification on Meridiani Planum and implications for erosion rates and climate change on Mars
A morphometric and morphologic catalog of~ 100 small craters imaged by the Opportunity
rover over the 33.5 km traverse between Eagle and Endeavour craters on Meridiani Planum …
rover over the 33.5 km traverse between Eagle and Endeavour craters on Meridiani Planum …
Polar science results from Mars Reconnaissance Orbiter: Multiwavelength, multiyear insights
Abstract Mars Reconnaissance Orbiter (MRO), with its arrival in 2006 and nearly continuous
operation since, has provided data for the study of martian polar processes spanning nine …
operation since, has provided data for the study of martian polar processes spanning nine …