Results by Neukum et al.(2001) and Ivanov (2001) are combined with crater counts to
estimate ages of Martian surfaces. These results are combined with studies of Martian …

This paper reviews and refines the technique of dating martian surfaces by using impact-
crater isochrons (defined as size distributions of impact craters on undisturbed martian …

The HiRISE camera features a 0.5 m diameter primary mirror, 12 m effective focal length,
and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data …

The Context Camera (CTX) on the Mars Reconnaissance Orbiter (MRO) is a Facility
Instrument (ie, government‐furnished equipment operated by a science team not …

The large-scale volcanic lineaments in Iceland are an axial zone, which is delineated by the
Reykjanes, West and North Volcanic Zones (RVZ, WVZ, NVZ) and the East Volcanic Zone …

We review the radiometric ages of the 16 currently known Martian meteorites, classified as
11 shergottites (8 basaltic and 3 lherzolitic), 3 nakhlites (clinopyroxenites), Chassigny (a …

More than 3 years of high‐resolution (1.5–20 m/pixel) photographic observations of the
surface of Mars have dramatically changed our view of that planet. Among the most …

Layered and massive outcrops on Mars, some as thick as 4 kilometers, display the
geomorphic attributes and stratigraphic relations of sedimentary rock. Repeated beds in …

Over the past 30 years, the water-generated landforms and landscapes of Mars have been
revealed in increasing detail by a succession of spacecraft missions. Recent data from the …

If the large Late Hesperian outflow channels were eroded by extensive floods, as appears
likely, then large bodies of water must have once occupied the northern plains during that …