Open-basin lake outlet valleys are incised when water breaches the basin-confining topography and overflows. Outlet valleys record this flooding event and provide insight into how the lake and surrounding terrain evolved over time. Here we present a study of the paleolake outlet Licus Vallis, a >350 km long, >2 km wide, >100 m deep valley that heads at the outlet breach of an approx.30 km diameter impact crater. Multiple geomorphic features of this valley system suggest it records a more complex evolution than formation from a single lake overflow flood. This provides unique insight into the paleohydrology of lakes on early Mars, as we can make inferences beyond the most recent phase of activity.
A number of martian outflow channels were carved by discharges from large dilational fault zones. Th...
To inspect past environmental changes and potential habitability, the growing interests for the anci...
Gale crater is a ~154-km-diameter impact crater formed during the Late Noachian/Early Hesperian at t...
Numerous observations from both orbital remote sensing [1-3] and Mars Curiosity [4] suggest that lak...
Martian valley networks (VNs) have been viewed as one of the most compelling pieces of evidence for ...
There is conflicting evidence for an ancient ocean which occupied the northern hemispheric basin on ...
The problems of how warm and wet Mars once was and when climate transitions may have occurred are no...
Jezero crater is a site of prime scientific interest because it was a lake early in Mars history. Pr...
There is conflicting evidence for an ancient ocean which occupied the northern hemispheric basin on ...
High Resolution Stereo Camera (HRSC) data , with their stereo capabilities, allow the investigation ...
Using the new High Resolution Stereo Camera (HRSC) data and other Martian data sets, we reconstructe...
Pronounced global volcanism as well as fracturing and erosion along the highland/lowland boundary (H...
long) that each formed distributary fans as they entered an ancient 40-km diameter impact crater. An...
McLaughlin crater is a 92-kmdiameter Martian impact crater that contained an ancient carbonate- and ...
The ~150 km wide Holden crater lies in an area characterized by high density of valley networks impl...
A number of martian outflow channels were carved by discharges from large dilational fault zones. Th...
To inspect past environmental changes and potential habitability, the growing interests for the anci...
Gale crater is a ~154-km-diameter impact crater formed during the Late Noachian/Early Hesperian at t...
Numerous observations from both orbital remote sensing [1-3] and Mars Curiosity [4] suggest that lak...
Martian valley networks (VNs) have been viewed as one of the most compelling pieces of evidence for ...
There is conflicting evidence for an ancient ocean which occupied the northern hemispheric basin on ...
The problems of how warm and wet Mars once was and when climate transitions may have occurred are no...
Jezero crater is a site of prime scientific interest because it was a lake early in Mars history. Pr...
There is conflicting evidence for an ancient ocean which occupied the northern hemispheric basin on ...
High Resolution Stereo Camera (HRSC) data , with their stereo capabilities, allow the investigation ...
Using the new High Resolution Stereo Camera (HRSC) data and other Martian data sets, we reconstructe...
Pronounced global volcanism as well as fracturing and erosion along the highland/lowland boundary (H...
long) that each formed distributary fans as they entered an ancient 40-km diameter impact crater. An...
McLaughlin crater is a 92-kmdiameter Martian impact crater that contained an ancient carbonate- and ...
The ~150 km wide Holden crater lies in an area characterized by high density of valley networks impl...
A number of martian outflow channels were carved by discharges from large dilational fault zones. Th...
To inspect past environmental changes and potential habitability, the growing interests for the anci...
Gale crater is a ~154-km-diameter impact crater formed during the Late Noachian/Early Hesperian at t...