A field campaign was organized in September 2006 by Centro de Astobiologica (Spain) and Washington University (St Louis, USA) for the geological study of the Rio Tinto river bed sediments using a suite of in-situ instruments comprising an ASD reflectance spectrometer, an emission spectrometer, panoramic and close-up color imaging cameras, a life detection system and NASA's CheMin 4 XRD/XRF prototype. The primary objectives of the field campaign were to study the geology of the site and test the potential of the instrument suite in an astrobiological investigation context for future Mars surface robotic missions. The results of the overall campaign will be presented elsewhere. This paper focuses on the results of the XRD/XRF instrument deplo...
The Mars Science Laboratory (MSL) Curiosity rover is equipped with CheMin, the first x-ray diffracti...
The mineralogy of a planetary surface can be used to identify the provenance of soil or sediment and...
The legacy of planetary X-ray Diffraction (XRD) and X-ray Fluorescence (XRF) began in 1960 when W. P...
The Rio Tinto, located in southwest Spain, exhibits a nearly constant, acidic pHvalue along its cour...
Recently reported results from latest Mars Orbiters and Rovers missions are transforming our opinion...
To obtain detailed mineralogy information, the Mars Science Laboratory rover Curiosity carries CheMi...
Exploration by the NASA rover Opportunity has revealed sulfate- and hematite-rich sedimentary rocks ...
The Mars Science Laboratory (MSL) rover will land in Gale Crater on Mars in August 2012. The planned...
By employing an integrated x-ray instrument on a future Mars mission, data obtained will greatly aug...
In situ analysis of rock chemistry is a fundamental tool for exploration of planets. To meet this ne...
The Mars Science Laboratory Curiosity landed in Gale crater in August 2012 with the goal to identify...
A principal goal of the Mars Science Laboratory (MSL) rover Curiosity is to identify and characteriz...
OMEGA recently identified spectral signatures of kieserite, gypsum, and other polyhydrated sulfates ...
The Portable Test System (PTS), designed & developed by Charles Rivers Laboratories, Inc. (Charlesto...
The recent discovery of abundant sulfate minerals, particularly Jarosite by the Opportunity Rover at...
The Mars Science Laboratory (MSL) Curiosity rover is equipped with CheMin, the first x-ray diffracti...
The mineralogy of a planetary surface can be used to identify the provenance of soil or sediment and...
The legacy of planetary X-ray Diffraction (XRD) and X-ray Fluorescence (XRF) began in 1960 when W. P...
The Rio Tinto, located in southwest Spain, exhibits a nearly constant, acidic pHvalue along its cour...
Recently reported results from latest Mars Orbiters and Rovers missions are transforming our opinion...
To obtain detailed mineralogy information, the Mars Science Laboratory rover Curiosity carries CheMi...
Exploration by the NASA rover Opportunity has revealed sulfate- and hematite-rich sedimentary rocks ...
The Mars Science Laboratory (MSL) rover will land in Gale Crater on Mars in August 2012. The planned...
By employing an integrated x-ray instrument on a future Mars mission, data obtained will greatly aug...
In situ analysis of rock chemistry is a fundamental tool for exploration of planets. To meet this ne...
The Mars Science Laboratory Curiosity landed in Gale crater in August 2012 with the goal to identify...
A principal goal of the Mars Science Laboratory (MSL) rover Curiosity is to identify and characteriz...
OMEGA recently identified spectral signatures of kieserite, gypsum, and other polyhydrated sulfates ...
The Portable Test System (PTS), designed & developed by Charles Rivers Laboratories, Inc. (Charlesto...
The recent discovery of abundant sulfate minerals, particularly Jarosite by the Opportunity Rover at...
The Mars Science Laboratory (MSL) Curiosity rover is equipped with CheMin, the first x-ray diffracti...
The mineralogy of a planetary surface can be used to identify the provenance of soil or sediment and...
The legacy of planetary X-ray Diffraction (XRD) and X-ray Fluorescence (XRF) began in 1960 when W. P...