Add to ORKGCrater size–frequency distribution is one of the powerful techniques to estimate the ages of planetary surfaces, especially from remote sensing studies. This has been applied to images of the Moon obtained from Clementine mission in 1994. Simple techniques of measurement of the diameter of the craters (in pixels) are used and converted into linear dimensions. Among the several maria studied, the results of Mare Humorum and the central region of Mare Imbrium are reported. The results are compared with age estimates from other sources. 1
Determining the ages of young planetary surfaces relies on using populations of small, often sub-km ...
Knowledge of regolith depth structure is important for a variety of studies of the Moon and other bo...
Context. In December 2020, China’s Chang’e-5 spacecraft successfully returned 1731 g of lunar sample...
The analysis of the impact crater size-frequency distribution (CSFD) is a well-established approach ...
[1] Accurate estimates of mare basalt ages are necessary to place constraints on the duration and th...
Several characteristics of very small impact craters of lunar surface have recently been improved by...
Tsiolkovskiy is a ~200 km diameter crater presenting one of the few mare deposits of the lunar far s...
A research program was designed (1) to map regional lithological units of the lunar surface based o...
Tsiolkovskiy is a ~200 km diameter crater presenting one of the few mare deposits of the lunar far s...
Crater size-frequency distributions were studied (100-500 m) and are shown to provide significant in...
A comparison of the optical and topographic data based analysis helps to identify craters down to ab...
Accurate estimates of mare basalt ages are necessary to place constraints on the duration and the fl...
Previous studies have estimated the ages of lunar lobate scarps, some of the youngest tectonic landf...
Accurate estimates of mare basalt ages are necessary to place constraints on the duration and the fl...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
Determining the ages of young planetary surfaces relies on using populations of small, often sub-km ...
Knowledge of regolith depth structure is important for a variety of studies of the Moon and other bo...
Context. In December 2020, China’s Chang’e-5 spacecraft successfully returned 1731 g of lunar sample...
The analysis of the impact crater size-frequency distribution (CSFD) is a well-established approach ...
[1] Accurate estimates of mare basalt ages are necessary to place constraints on the duration and th...
Several characteristics of very small impact craters of lunar surface have recently been improved by...
Tsiolkovskiy is a ~200 km diameter crater presenting one of the few mare deposits of the lunar far s...
A research program was designed (1) to map regional lithological units of the lunar surface based o...
Tsiolkovskiy is a ~200 km diameter crater presenting one of the few mare deposits of the lunar far s...
Crater size-frequency distributions were studied (100-500 m) and are shown to provide significant in...
A comparison of the optical and topographic data based analysis helps to identify craters down to ab...
Accurate estimates of mare basalt ages are necessary to place constraints on the duration and the fl...
Previous studies have estimated the ages of lunar lobate scarps, some of the youngest tectonic landf...
Accurate estimates of mare basalt ages are necessary to place constraints on the duration and the fl...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
Determining the ages of young planetary surfaces relies on using populations of small, often sub-km ...
Knowledge of regolith depth structure is important for a variety of studies of the Moon and other bo...
Context. In December 2020, China’s Chang’e-5 spacecraft successfully returned 1731 g of lunar sample...