Four areas fit within the elevation and latitude constraints: Chryse, Elysium, Amazonis, and Isidis. There is geomorphic evidence that all have supported standing water. In some cases it would be difficult to pick a landing site that had no hope of teaching us about the climatic history of Mars. The southeast Elysium Basin provides an optimal target in which a variety of materials may be accessible in a near-shore environment. The albedo of the region is moderately low, and the thermal inertia is indicative of moderate rock coverage or some consolidation of fines, arguing that the site has not been covered with eolian dust deposits
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Along a 500 km-wide belt extending between 202 deg and 180 deg W and lying astride the martian equat...
The present engineering constraints imposed on the Mars Pathfinder mission leave only three broad re...
A Mars Pathfinder landing site in Melas Chasma (Valles Marineris) would yield significant science re...
The northwest Isidis Basin offers a unique opportunity to land near a fretted terrain lowland/upland...
The Mars Pathfinder Meteorological Package (ASI/MET) will measure the local pressure, temperature, a...
The Mars '94 spacecraft will still be operational when Mars Pathfinder begins its observations. Whil...
Presently the landing site for Mars Pathfinder will be constrained to latitudes between 0 deg and 30...
The problems that now confront Mars Pathfinder are much the same as those that confronted Viking, bu...
In addition to a better understanding of the geological evolution of Mars, new techniques for proces...
Potential landing sites are confined to latitudes between 0 deg and 30 deg N and surfaces below 0 km...
Several of the most fundamental issues about the geology of Mars can be addressed using information ...
The proposed site is the northernmost occurrence of the Medusae Fossae Formation (MFF), and lies at ...
A strategy for Pathfinder site selection must be developed that is fundamentally different from most...
Terrain studies of candidate landing sites for a future rover/sample-return mission to Mars are bein...
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Along a 500 km-wide belt extending between 202 deg and 180 deg W and lying astride the martian equat...
The present engineering constraints imposed on the Mars Pathfinder mission leave only three broad re...
A Mars Pathfinder landing site in Melas Chasma (Valles Marineris) would yield significant science re...
The northwest Isidis Basin offers a unique opportunity to land near a fretted terrain lowland/upland...
The Mars Pathfinder Meteorological Package (ASI/MET) will measure the local pressure, temperature, a...
The Mars '94 spacecraft will still be operational when Mars Pathfinder begins its observations. Whil...
Presently the landing site for Mars Pathfinder will be constrained to latitudes between 0 deg and 30...
The problems that now confront Mars Pathfinder are much the same as those that confronted Viking, bu...
In addition to a better understanding of the geological evolution of Mars, new techniques for proces...
Potential landing sites are confined to latitudes between 0 deg and 30 deg N and surfaces below 0 km...
Several of the most fundamental issues about the geology of Mars can be addressed using information ...
The proposed site is the northernmost occurrence of the Medusae Fossae Formation (MFF), and lies at ...
A strategy for Pathfinder site selection must be developed that is fundamentally different from most...
Terrain studies of candidate landing sites for a future rover/sample-return mission to Mars are bein...
Critical to the assessment of potential sites for the 1997 Pathfinder landing is estimation of gener...
Along a 500 km-wide belt extending between 202 deg and 180 deg W and lying astride the martian equat...
The present engineering constraints imposed on the Mars Pathfinder mission leave only three broad re...