Studies of many objects in petrographic thin section, such as melt inclusions in igneous rocks, chondrules and Ca-Al rich inclusions in chondritic meteorites, or clasts in lunar and other breccias, require or can benefit from knowledge of their bulk compositions. Given the scarcity of these materials, the reluctance of curators to provide more abundant material, and the extreme difficulty of cleanly separating such objects from their rock matrices, geochemical and cosmochemical studies need the ability to determine their bulk compositions from in situ methods, such as defocused beam analysis, or quantitative chemical mapping by electron beam methods
NASA Lunar Sample Educational Set is a valuable source for planetary petrology education. Using the ...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
National audienceWe discuss if the detection of aqueous alteration depends on the techniques that ar...
Petrologic investigation of the shergottites has been hampered by the fact that most of these meteor...
We report a large database of bulk meteorite elemental abundances, compiled to aid in the interpreta...
This paper looks at two ways to estimate the bulk mineralogy of the rocks for assay intervals. The a...
73rd Annual Meeting of the Meteoritical-Society, New York, NY, July 26-30, 2010International audienc...
Classification of meteorites is most effectively carried out by petrographic and mineralogic studies...
Methods and Petrographic Descriptions of Selected Chondrules. Petrographic data on each of ten Allen...
A detailed electron microprobe (EMP) study was performed on chondrules of various textural types in ...
The petrologic components of carbonaceous chondrites each contain a distinct set of physical, chemic...
Chondrules and matrix are the major components of chondritic meteorites and represent a significant ...
Chondrules are microscopic, recrystallized melt droplets found in chondritic meteorites. High-resolu...
Numerous geosciences samples display a multi-scale mineralogical heterogeneity for which it is chall...
Twenty-four refractory inclusions (40-230 micrometers, with average of 86 +/- 40 micrometers) were f...
NASA Lunar Sample Educational Set is a valuable source for planetary petrology education. Using the ...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
National audienceWe discuss if the detection of aqueous alteration depends on the techniques that ar...
Petrologic investigation of the shergottites has been hampered by the fact that most of these meteor...
We report a large database of bulk meteorite elemental abundances, compiled to aid in the interpreta...
This paper looks at two ways to estimate the bulk mineralogy of the rocks for assay intervals. The a...
73rd Annual Meeting of the Meteoritical-Society, New York, NY, July 26-30, 2010International audienc...
Classification of meteorites is most effectively carried out by petrographic and mineralogic studies...
Methods and Petrographic Descriptions of Selected Chondrules. Petrographic data on each of ten Allen...
A detailed electron microprobe (EMP) study was performed on chondrules of various textural types in ...
The petrologic components of carbonaceous chondrites each contain a distinct set of physical, chemic...
Chondrules and matrix are the major components of chondritic meteorites and represent a significant ...
Chondrules are microscopic, recrystallized melt droplets found in chondritic meteorites. High-resolu...
Numerous geosciences samples display a multi-scale mineralogical heterogeneity for which it is chall...
Twenty-four refractory inclusions (40-230 micrometers, with average of 86 +/- 40 micrometers) were f...
NASA Lunar Sample Educational Set is a valuable source for planetary petrology education. Using the ...
A study of the compositional and textural variations between Fe-Ni sulphides in a suite of pristine ...
National audienceWe discuss if the detection of aqueous alteration depends on the techniques that ar...