[1] Streamlined forms and longitudinal grooving seen in Mars Orbital Camera (MOC) images indicate recent aqueous flooding occurred downslope (south) of the southern-most Cerberus Fossae fissure. Topography from the Mars Orbital Laser Altimeter (MOLA), in conjunction with the absence of fluvial features in MOC images immediately to the north of the Fossa, substantiate the idea that floods emanated from this fissure. The floodwater flowed southward onto the western Cerberus Plains, where it probably percolated into existing lava flows. Thus, shallow ice may still be extant beneath young lava flows in this equatoria
Mars Orbiter Laser Altimeter (MOLA) topographic data, High Resolution Imaging Science Experiment (Hi...
Summary. The four youngest megaflood channels on Mars – Mangala Valles, Marte Vallis, Grjotá Valles ...
The Elysium Volcanic Province consists of numerous overlapping flow units and may include the younge...
The geomorphology and topography of the Cerberus Plains region of Mars show three spatially and temp...
Mars Orbiter Camera (MOC) images and Mars Orbiter Laser Altimeter (MOLA) data on the Mars Global Sur...
The Cerberus Fossae fissures on Mars are the source of both lava and water floods 2-10 million year...
This work examines the relative chronology of geologic units within the Cerberus Plains of Mars with...
In a number of recent publications (e.g., Burr et al., Geophys. Res. Lett. 29/1, 2002), volcanic and...
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water flood...
The Mangala Valles system is an ∼ ∼900 km fluvially carved channel system located southwest of the T...
In order to investigate sources of lava and water to the Cerberus plains of Mars, geomorphological m...
Abstract. The Mangala Valles system is an ~900 km fluvially carved channel system located southwest ...
Mangala Valles has always been viewed as the typical outflow channel formed by catastrophic floods o...
Previous studies noted the close association of geologically very recent lava flows and fluvial chan...
It is by now widely accepted that Mars had a wet and periodically warm past in the Noachian e.g., bu...
Mars Orbiter Laser Altimeter (MOLA) topographic data, High Resolution Imaging Science Experiment (Hi...
Summary. The four youngest megaflood channels on Mars – Mangala Valles, Marte Vallis, Grjotá Valles ...
The Elysium Volcanic Province consists of numerous overlapping flow units and may include the younge...
The geomorphology and topography of the Cerberus Plains region of Mars show three spatially and temp...
Mars Orbiter Camera (MOC) images and Mars Orbiter Laser Altimeter (MOLA) data on the Mars Global Sur...
The Cerberus Fossae fissures on Mars are the source of both lava and water floods 2-10 million year...
This work examines the relative chronology of geologic units within the Cerberus Plains of Mars with...
In a number of recent publications (e.g., Burr et al., Geophys. Res. Lett. 29/1, 2002), volcanic and...
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water flood...
The Mangala Valles system is an ∼ ∼900 km fluvially carved channel system located southwest of the T...
In order to investigate sources of lava and water to the Cerberus plains of Mars, geomorphological m...
Abstract. The Mangala Valles system is an ~900 km fluvially carved channel system located southwest ...
Mangala Valles has always been viewed as the typical outflow channel formed by catastrophic floods o...
Previous studies noted the close association of geologically very recent lava flows and fluvial chan...
It is by now widely accepted that Mars had a wet and periodically warm past in the Noachian e.g., bu...
Mars Orbiter Laser Altimeter (MOLA) topographic data, High Resolution Imaging Science Experiment (Hi...
Summary. The four youngest megaflood channels on Mars – Mangala Valles, Marte Vallis, Grjotá Valles ...
The Elysium Volcanic Province consists of numerous overlapping flow units and may include the younge...