The source craters of the martian meteorites: Implications for the igneous evolution of Mars

CDK Herd, JS Hamilton, EL Walton, LL Tornabene… - Science …, 2024 - science.org
Approximately 200 meteorites come from~ 10 impact events on the surface of Mars, yet their
pre-ejection locations are largely unknown. Here, we combine the results of diverse sets of …

Automated precision counting of small lunar craters-A broader view

PH Cadogan - Icarus, 2024 - Elsevier
An automated system for counting small craters at lunar landing sites has been expanded to
include selected locations on the Moon's far side and high latitudes. Highland areas were …

Slopes of Lunar Crater Size‐Frequency Distributions at Copernican‐Aged Craters

A Oetting, N Schmedemann… - Journal of …, 2023 - Wiley Online Library
Craters on the lunar surface can provide valuable information about the timing and
sequence of surface‐forming processes on the Moon. A commonly used method for age …

[HTML][HTML] Effect of Target Properties on Regolith Production

M Xie, Y Li - Remote Sensing, 2024 - mdpi.com
Based on the measurements of regolith thicknesses on the lunar maria (basalts), the lunar
regolith was determined to have accumulated at a rate of about 1 m/Gyr since the era of the …

Estimation of the Rate of Slope Processes and Morphological Variability of Kilometer-Sized Impact Craters on the Moon

X Kochubey, MA Ivanov - Solar System Research, 2024 - Springer
In order to estimate the rate of slope processes on the Moon, we studied the morphology
and topographic configuration of 24 craters in the diameter range of 5–15 km. These craters …

Оценка темпа склоновых процессов и морфологической изменчивости километровых ударных кратеров на Луне

К Кочубей, К Кочубей, МА Иванов… - Astronomičeskij …, 2024 - cardiosomatics.orscience.ru
Для того чтобы оценить темп склоновых процессов на Луне, мы изучили морфологию и
топографическую конфигурацию 24-х кратеров в интервале диаметров 5–15 км …