The Cerberus Fossae fissures on Mars are the source of both lava and water floods 2-10 million years old. Evidence for resulting lava plains has been identified in eastern Elysium, but seas and lakes from these fissures and previous flooding events were presumed to have evaporated and sublimed away. HRSC images from the ESA Mars Express spacecraft indicate that they may still be there. We present evidence consistent with a presently-existing frozen body of water, with surface pack-ice, around +5º latitude and 150º east longitude in southern Elysium. It measures about 800 km x 900 km and averages up to 45 metres deep: similar in size and depth to the North Sea. Its age from crater counts is 5 ±2 Ma. If our interpretation is confirme...
The geomorphology and topography of the Cerberus Plains region of Mars show three spatially and temp...
A review of the evidence concerning the original and current water budgets of Mars is presented. Pre...
There is now widespread agreement that the surface of Mars underwent some degree of fluvial modifica...
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water flood...
[1] Streamlined forms and longitudinal grooving seen in Mars Orbital Camera (MOC) images indicate re...
Ten new passes have been made of the frozen sea area of Elysium imaged near the equator of Mars earl...
In order to investigate sources of lava and water to the Cerberus plains of Mars, geomorphological m...
This work examines the relative chronology of geologic units within the Cerberus Plains of Mars with...
It is by now widely accepted that Mars had a wet and periodically warm past in the Noachian e.g., bu...
Liquid water is generally only meta-stable on Mars today; it quickly freezes, evaporates or boils in...
The Elysium Volcanic Province consists of numerous overlapping flow units and may include the younge...
The first HiRISE images of Elysium Planitia (Mars) show areas both near the centreand the edges of t...
Mars Orbiter Camera (MOC) images and Mars Orbiter Laser Altimeter (MOLA) data on the Mars Global Sur...
It is suggested that certain landforms in the Elysium region of Mars provide strong evidence for gla...
Along a 500 km-wide belt extending between 202 deg and 180 deg W and lying astride the martian equat...
The geomorphology and topography of the Cerberus Plains region of Mars show three spatially and temp...
A review of the evidence concerning the original and current water budgets of Mars is presented. Pre...
There is now widespread agreement that the surface of Mars underwent some degree of fluvial modifica...
It is thought that the Cerberus Fossae fissures on Mars were the source of both lava and water flood...
[1] Streamlined forms and longitudinal grooving seen in Mars Orbital Camera (MOC) images indicate re...
Ten new passes have been made of the frozen sea area of Elysium imaged near the equator of Mars earl...
In order to investigate sources of lava and water to the Cerberus plains of Mars, geomorphological m...
This work examines the relative chronology of geologic units within the Cerberus Plains of Mars with...
It is by now widely accepted that Mars had a wet and periodically warm past in the Noachian e.g., bu...
Liquid water is generally only meta-stable on Mars today; it quickly freezes, evaporates or boils in...
The Elysium Volcanic Province consists of numerous overlapping flow units and may include the younge...
The first HiRISE images of Elysium Planitia (Mars) show areas both near the centreand the edges of t...
Mars Orbiter Camera (MOC) images and Mars Orbiter Laser Altimeter (MOLA) data on the Mars Global Sur...
It is suggested that certain landforms in the Elysium region of Mars provide strong evidence for gla...
Along a 500 km-wide belt extending between 202 deg and 180 deg W and lying astride the martian equat...
The geomorphology and topography of the Cerberus Plains region of Mars show three spatially and temp...
A review of the evidence concerning the original and current water budgets of Mars is presented. Pre...
There is now widespread agreement that the surface of Mars underwent some degree of fluvial modifica...