¹Zahia Djouadi,²Vassilissa Vinogradoff,¹Zelia Dionnet,²Coline Serra,³Douchka Dimitrijevic,⁴Alexandra Malnuit,¹Cateline Lantz,⁵Philippe Claeys,⁵Steven Goderis,²Louis Le Sergeant d’Hendecourt
Meteoritics & Planetary Science (in Press) Open Access Link to Article [https://doi.org/10.1111/maps.70017]
¹CNRS, Institut d’Astrophysique Spatiale, Université Paris-Saclay, Orsay, France
²UMR CNRS 7345, PIIM, Université Aix-Marseille, Marseille, France
³École Centrale de Lyon, Écully, France
⁴Université Paris-Saclay, Orsay, France
⁵Archaeology, Environmental Changes & Geo-Chemistry, Vrije Universiteit Brussel, Brussels, Belgium
Published by arrangement with John Wiley & Sons

Carbonaceous chondrites are meteorites originating from undifferentiated objects of the Solar System, which may retain signatures of primitive matter. Here, we present a comparative study between two CM chondrites Asuka 12236 and Paris, both considered among the most primitive in the carbonaceous chondrite meteorite collection. This work is based on the combination of infrared and Raman micro-spectroscopy, aiming to compare the spectral characteristics of these two peculiar chondrites. We present an average infrared spectrum from the mid to far infrared of Asuka 12236, which has never been reported yet in the literature. Contrary to the average spectrum of Paris, the Asuka 12236 spectrum shows signatures of anhydrous minerals (olivine and or pyroxene) as well as the presence of amorphous phases. These findings are in agreement with the low degree of alteration reported for Asuka 12236. Aromatic primary amines and imines are also detected in Asuka 12236, heterogeneously distributed within the meteorite. In addition, the comparison of the Raman signatures of the two meteorites highlights different carbon structuration and thus thermal histories. Our spectroscopic investigations confirm that Asuka 12236 can be considered more primitive than the Paris carbonaceous chondrite.