Infrared diffuse reflectance spectra (2.53-25μm) were measured for several Antarctic carbonaceous chondrites. Thermally metamorphosed carbonaceous chondrites with CI-CM affinities (Belgica (B)-7904,Yamato (Y)-793321,Y-82162,and Y-86720), which were recently found in the Antarctic collection, show weaker absorption bands near 3μm due to hydrous minerals, compared with the Murchison (CM) carbonaceous chondrite. These results show that hydrous minerals are dehydrated as a result of thermal metamorphism, consistent with the results of chemical, mineralogical, and petrologic studies. B-7904,Y-793321,and Y-86720 show weaker absorption bands near 6.9μm due to carbonates than those of Murchison. For Y-82162,the 1450cm^ (6.9μm) band is relatively st...
Carbonaceous chondrite meteorites are so far the only available samples representing carbon-rich ast...
We obtained mid-infrared reflectance spectra of powdered size fractions (0–25 μm, 25–63 μm, 63–125...
International audienceIn this work, infrared transmission spectra (2-25 μm range, 5000-400 cm-1) of ...
Reflectance spectra (0.3-2.6μm) of the C, G, B, and F asteroids and carbonaceous chondrites are comp...
The presence and intensity of absorption band near 3μm in the reflectance spectra are due to the pre...
International audienceIn order to determine the controls on the reflectance spectra of hydrated carb...
Mid-infrared absorption spectra were obtained for 6 carbonaceous chondrites and 6 Antarctic micromet...
In order to determine the controls on the reflectance spectra of hydrated carbonaceous chondrites, r...
Infrared (IR) absorption spectra of major types of carbonaceous matter in four Antarctic carbonaceou...
第8回極域科学シンポジウム/個別セッション:[OA] 南極隕石12月6日(水)国語研究所 2階講堂The Eighth Symposium on Polar Science/Ordinary sess...
We have examined mineral grains and matrix of new Antarctic carbonaceous chondrites Yamato (Y)-86029...
Antarctic carbonaceous chondrite (CC) meteorite chip samples in the Japanese and US collections have...
International audienceIR spectroscopy is one of the few techniques that can directly probe water mol...
Carbonaceous chondrite meteorites are so far the only available samples representing carbon-rich ast...
We obtained mid-infrared reflectance spectra of powdered size fractions (0–25 μm, 25–63 μm, 63–125...
International audienceIn this work, infrared transmission spectra (2-25 μm range, 5000-400 cm-1) of ...
Reflectance spectra (0.3-2.6μm) of the C, G, B, and F asteroids and carbonaceous chondrites are comp...
The presence and intensity of absorption band near 3μm in the reflectance spectra are due to the pre...
International audienceIn order to determine the controls on the reflectance spectra of hydrated carb...
Mid-infrared absorption spectra were obtained for 6 carbonaceous chondrites and 6 Antarctic micromet...
In order to determine the controls on the reflectance spectra of hydrated carbonaceous chondrites, r...
Infrared (IR) absorption spectra of major types of carbonaceous matter in four Antarctic carbonaceou...
第8回極域科学シンポジウム/個別セッション:[OA] 南極隕石12月6日(水)国語研究所 2階講堂The Eighth Symposium on Polar Science/Ordinary sess...
We have examined mineral grains and matrix of new Antarctic carbonaceous chondrites Yamato (Y)-86029...
Antarctic carbonaceous chondrite (CC) meteorite chip samples in the Japanese and US collections have...
International audienceIR spectroscopy is one of the few techniques that can directly probe water mol...
Carbonaceous chondrite meteorites are so far the only available samples representing carbon-rich ast...
We obtained mid-infrared reflectance spectra of powdered size fractions (0–25 μm, 25–63 μm, 63–125...
International audienceIn this work, infrared transmission spectra (2-25 μm range, 5000-400 cm-1) of ...