Rocks around the InSight lander were measured in lander orthoimages of the near field (<10 m), in panoramas of the far field (<40 m), and in a high-resolution orbital image around the lander (1 km2). The cumulative fractional area versus diameter size-frequency distributions for four areas in the near field fall on exponential model curves used for estimating hazards for landing spacecraft. The rock abundance varies in the near field from 0.6% for the sand and pebble-rich area to the east within Homestead hollow to ∼3–5% for the progressively rockier areas to the south, north, and west. The rock abundance of the entire near field is just over 3%, which falls between that at the Phoenix (2%) and Spirit (5%) landing sites. Rocks in the far fi...
Multispectral measurements in the visible and near infrared of rocks at Meridiani Planum by the Mars...
Because Mars lacks a global magnetic field or protective ozone layer, its surface is unshielded to h...
The Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecra...
Rocks around the InSight lander were measured in lander orthoimages of the near field (<10 m), in pa...
We present preliminary work to characterize surface rock abundance at ExoMars Rover landing site can...
[1] The cumulative fractional area covered by rocks versus diameter measured at the Pathfinder site ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95449/1/jgre1686.pd
Researchers mapped the surface materials at the Viking landing sites on Mars to gain a better unders...
This paper presents the abundances and the size-frequency distributions (SFD) of boulders identified...
Thermal Emission Spectrometer (TES) are well suited for determining the subpixel abundance of rocks ...
The surface materials on Mars were extensively studied using a variety of spacecraft and Earth-based...
Rock heights and three-dimensional shapes around the InSight lander in Homestead hollow, Mars, provi...
International audienceMany boundary layer processes simulated within a Mars General Circulation Mode...
Rocky ejecta craters (RECs) at the Interior Exploration using Seismic Investigations, Geodesy and He...
During the Phoenix mission landing site selection process, the Mars Reconnaissance Orbiter (MRO) Hig...
Multispectral measurements in the visible and near infrared of rocks at Meridiani Planum by the Mars...
Because Mars lacks a global magnetic field or protective ozone layer, its surface is unshielded to h...
The Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecra...
Rocks around the InSight lander were measured in lander orthoimages of the near field (<10 m), in pa...
We present preliminary work to characterize surface rock abundance at ExoMars Rover landing site can...
[1] The cumulative fractional area covered by rocks versus diameter measured at the Pathfinder site ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95449/1/jgre1686.pd
Researchers mapped the surface materials at the Viking landing sites on Mars to gain a better unders...
This paper presents the abundances and the size-frequency distributions (SFD) of boulders identified...
Thermal Emission Spectrometer (TES) are well suited for determining the subpixel abundance of rocks ...
The surface materials on Mars were extensively studied using a variety of spacecraft and Earth-based...
Rock heights and three-dimensional shapes around the InSight lander in Homestead hollow, Mars, provi...
International audienceMany boundary layer processes simulated within a Mars General Circulation Mode...
Rocky ejecta craters (RECs) at the Interior Exploration using Seismic Investigations, Geodesy and He...
During the Phoenix mission landing site selection process, the Mars Reconnaissance Orbiter (MRO) Hig...
Multispectral measurements in the visible and near infrared of rocks at Meridiani Planum by the Mars...
Because Mars lacks a global magnetic field or protective ozone layer, its surface is unshielded to h...
The Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecra...