Add to ORKGNASA\u27s Phoenix Lander uncovered two types of ice at its 2008 landing site on the northern plains of Mars: a brighter, slab-like ice that broke during Robotic Arm operations; and a darker icy deposit. Spectra from the Phoenix Surface Stereo Imager (SSI) are used to demonstrate that the brighter material consists of nearly pure water ice, which probably formed by migration and freezing of liquid water. The darker icy material consists of similar to 30 +/- 20 wt% ice, with the remainder composed of fine-grained soil, indicating that it probably formed as pore ice. These two types of ice represent two different emplacement mechanisms and periods of deposition
The discovery of buried carbon dioxide (CO2) ice between water (H2O) ice layers within the martian s...
Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of p...
Ground-ice exists widely on Mars and has been observed directly - the Phoenix Mars Lander revealed i...
NASA\u27s Phoenix Lander uncovered two types of ice at its 2008 landing site on the northern plains ...
International audienceIce buried beneath a thin layer of soil has been revealed by neutron spectrosc...
The combination of ground observations from the Mars Phoenix Lander and orbital data from the Compac...
The water cycle is critically important to understanding Mars system science, especially interaction...
Includes bibliographical references (pages 35-36)The discovery of a network of channels on the surfa...
The condensation, evolution, and sublimation of seasonal water and carbon dioxide ices were characte...
Experiments demonstrate for the first time the deposition of subsurface ice directly from atmospheri...
Near-surface perennial water ice on Mars has been previously inferred down to latitudes of about 45°...
Mars’s mid-latitudes, corresponding approximately to the 30°–60° latitude bands in both hemispheres,...
At the Mars Phoenix landing site and in much of the Martian northern plains, there is ice-cemented g...
The interface between certain geological and atmospheric phenomena on Mars was studied by examining ...
This repository contains: 1. Calculated spectra of snow-dust mixtures from Khuller and Christensen ...
The discovery of buried carbon dioxide (CO2) ice between water (H2O) ice layers within the martian s...
Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of p...
Ground-ice exists widely on Mars and has been observed directly - the Phoenix Mars Lander revealed i...
NASA\u27s Phoenix Lander uncovered two types of ice at its 2008 landing site on the northern plains ...
International audienceIce buried beneath a thin layer of soil has been revealed by neutron spectrosc...
The combination of ground observations from the Mars Phoenix Lander and orbital data from the Compac...
The water cycle is critically important to understanding Mars system science, especially interaction...
Includes bibliographical references (pages 35-36)The discovery of a network of channels on the surfa...
The condensation, evolution, and sublimation of seasonal water and carbon dioxide ices were characte...
Experiments demonstrate for the first time the deposition of subsurface ice directly from atmospheri...
Near-surface perennial water ice on Mars has been previously inferred down to latitudes of about 45°...
Mars’s mid-latitudes, corresponding approximately to the 30°–60° latitude bands in both hemispheres,...
At the Mars Phoenix landing site and in much of the Martian northern plains, there is ice-cemented g...
The interface between certain geological and atmospheric phenomena on Mars was studied by examining ...
This repository contains: 1. Calculated spectra of snow-dust mixtures from Khuller and Christensen ...
The discovery of buried carbon dioxide (CO2) ice between water (H2O) ice layers within the martian s...
Ice sheets, such as the polar layered deposits (PLDs) of Mars, are of great interest as records of p...
Ground-ice exists widely on Mars and has been observed directly - the Phoenix Mars Lander revealed i...