Biradical character of D-rich carriers in the insoluble organic matter of carbonaceous chondrites: A relic of the protoplanetary disk chemistry

2011 ◽  
Vol 75 (1) ◽  
pp. 326-336 ◽  
Author(s):  
Olivier Delpoux ◽  
Didier Gourier ◽  
Hervé Vezin ◽  
Laurent Binet ◽  
Sylvie Derenne ◽  
...  
2010 ◽  
Vol 300 (3-4) ◽  
pp. 321-328 ◽  
Author(s):  
F.-R. Orthous-Daunay ◽  
E. Quirico ◽  
L. Lemelle ◽  
P. Beck ◽  
V. deAndrade ◽  
...  

2004 ◽  
pp. 333-357
Author(s):  
Laurent Binet ◽  
Didier Gourier ◽  
Audrey Skrzypczak ◽  
Sylvie Derenne ◽  
François Robert

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Alexander Zherebker ◽  
Yury Kostyukevich ◽  
Dmitry S. Volkov ◽  
Ratibor G. Chumakov ◽  
Lukas Friederici ◽  
...  

AbstractDespite broad application of different analytical techniques for studies on organic matter of chondrite meteorites, information about composition and structure of individual compounds is still very limited due to extreme molecular diversity of extraterrestrial organic matter. Here we present the first application of isotopic exchange assisted Fourier transform ion cyclotron resonance mass spectrometry (FTICR MS) for analysis of alkali extractable fraction of insoluble organic matter (IOM) of the Murchison and Allende meteorites. This allowed us to determine the individual S-containing ions with different types of sulfur atoms in IOM. Thiols, thiophenes, sulfoxides, sulfonyls and sulfonates were identified in both samples but with different proportions, which contribution corroborated with the hydrothermal and thermal history of the meteorites. The results were supported by XPS and thermogravimetric analysis coupled to FTICR MS. The latter was applied for the first time for analysis of chondritic IOM. To emphasize the peculiar extraterrestrial origin of IOM we have compared it with coal kerogen, which is characterized by the comparable complexity of molecular composition but its aromatic nature and low oxygen content can be ascribed almost exclusively to degradation of biomacromolecules.


2021 ◽  
Vol 7 (18) ◽  
pp. eabd3575
Author(s):  
Yoshihiro Furukawa ◽  
Yoshinari Iwasa ◽  
Yoshito Chikaraishi

Solvent-soluble organic matter (SOM) in meteorites, which includes life’s building molecules, is suspected to originate from the cold region of the early solar system, on the basis of 13C enrichment in the molecules. Here, we demonstrate that the isotopic characteristics are reproducible in amino acid synthesis associated with a formose-type reaction in a heated aqueous solution. Both thermochemically driven formose-type reaction and photochemically driven formose-type reaction likely occurred in asteroids and ice-dust grains in the early solar system. Thus, the present results suggest that the formation of 13C-enriched SOM was not specific to the cold outer protosolar disk or the molecular cloud but occurred more widely in the early solar system.


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