Analyzing the density of impact craters on planetary surfaces is the only known technique for
learning their ages remotely. As a result, crater statistics have been widely analyzed on the …

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 …

We present a new catalog of 205 candidate closed-basin lakes contained within impact
craters across the surface of Mars. These basins have an inlet valley that incises the crater …

The acquisition of high-resolution imagery for the surface of Mars has enabled map** of
spatially limited (order of< 10 3 km 2) landforms such as alluvial fans, deltas, and lacustrine …

The High Resolution Imaging Science Experiment (HiRISE) on the Mars Reconnaissance
Orbiter (MRO) acquired 8terapixels of data in 9137 images of Mars between October 2006 …

The cratered highlands located northwest of Isidis Planitia have been recognized as one of
the best preserved Noachian (~ 3.7–4.1 Ga; Nimmo and Tanaka, 2005) landscapes …

The new, post-Viking generation of Mars orbital imaging and topographical data provide
significant higher-resolution details of surface morphologies, which induced a new effort to …

Abstract The 90.5-km Occator crater, with its peculiar and unique bright spots, is one of the
most prominent and renowned feature on Ceres. Occator attracted broad public attention in …

The small crater populations (diameter smaller than 1km) are widely used to date planetary
surfaces. The reliability of small crater counts is tested by counting small craters at several …

Abundant evidence exists for valley network‐related fluvial activity near the Noachian‐
Hesperian transition on Mars, and areally significant quantities of volcanic ridged plains …