As Viking Lander 1 touched down on Mars one of its footpads fully penetrated a patch of loose fine-grained drift material. The surrounding landing site, as observed by VL-1, was found to exhibit a complex terrain consisting of a crusted surface with an assortment of rocks, large dune-like drifts and smaller patches of drift material. We use a temperature sensor attached to the buried footpad and covered in fine-grained material to determine the thermal properties of drift material at the VL-1 site. The thermal properties are used to investigate the microstructure of the drift material and understand its relevance to surface-atmosphere interactions. We obtained a thermal inertia value of 103 ± 22 tiu. This value is in the upper range...
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Albedo and thermal property correlations of the topography of Mars were conducted with emphases upon...
The thermal interia of the surface of Mars varies spatially by a factor of eight. This is attributab...
As Viking Lander 1 touched down on Mars one of its footpads fully penetrated a patch of loose fine-g...
A semiquantitative appreciation for the physical properties of the Mars surface materials and their ...
The north polar layered deposits on Mars appear to be the source of the dark material that comprises...
Current data indicate that Mars, like the Earth and Moon, will have a soil-like layer. An understand...
f Viking infrared thermal mapping (IRTM) and bistatic radar data suggest that the bulk density of th...
We study the Martian fine-grained dark material by focussing on a global selection of impact craters...
Abstract Measurements from the InSight lander radiometer acquired after landing are used to characte...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
Presently the landing site for Mars Pathfinder will be constrained to latitudes between 0 deg and 30...
<p>The most significant mobility challenges that planetary rovers encounter are compounded by loose,...
The present work reviews the information on mineralogy and chemistry of Martian soils from the data ...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Albedo and thermal property correlations of the topography of Mars were conducted with emphases upon...
The thermal interia of the surface of Mars varies spatially by a factor of eight. This is attributab...
As Viking Lander 1 touched down on Mars one of its footpads fully penetrated a patch of loose fine-g...
A semiquantitative appreciation for the physical properties of the Mars surface materials and their ...
The north polar layered deposits on Mars appear to be the source of the dark material that comprises...
Current data indicate that Mars, like the Earth and Moon, will have a soil-like layer. An understand...
f Viking infrared thermal mapping (IRTM) and bistatic radar data suggest that the bulk density of th...
We study the Martian fine-grained dark material by focussing on a global selection of impact craters...
Abstract Measurements from the InSight lander radiometer acquired after landing are used to characte...
Thesis Summary: Surface energy budget and thermal inertia are two major thermophysical parameters t...
Presently the landing site for Mars Pathfinder will be constrained to latitudes between 0 deg and 30...
<p>The most significant mobility challenges that planetary rovers encounter are compounded by loose,...
The present work reviews the information on mineralogy and chemistry of Martian soils from the data ...
[1] Thermal inertia values at 100 m per pixel are determined using nighttime temperature data from t...
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Albedo and thermal property correlations of the topography of Mars were conducted with emphases upon...
The thermal interia of the surface of Mars varies spatially by a factor of eight. This is attributab...