On the origin and evolution of the material in 67P/Churyumov-Gerasimenko

International audiencePrimitive objects like comets hold important information on the material that formed our solar system. Several comets have been visited by spacecraft and many more have been observed through Earth- and space-based telescopes. Still our understanding remains limited. Molecular abundances in comets have been shown to be similar to interstellar ices and thus indicate that common processes and conditions were involved in their formation. The samples returned by the Stardust mission to comet Wild 2 showed that the bulk refractory material was processed by high temperatures in the vicinity of the early sun. The recent Rosetta mission acquired a wealth of new data on the composition of comet 67P/Churyumov-Gerasimenko (hereafter 67P/C-G) and complemented earlier observations of other comets. The isotopic, elemental, and molecular abundances of the volatile, semi-volatile, and refractory phases brought many new insights into the origin and processing of the incorporated material. The emerging picture after Rosetta is that at least part of the volatile material was formed before the solar system and that cometary nuclei agglomerated over a wide range of heliocentric distances, different from where they are found today. Deviations from bulk solar system abundances indicate that the material was not fully homogenized at the location of comet formation, despite the radial mixing implied by the Stardust results. Post-formation evolution of the material might play an important role, which further complicates the picture. This paper discusses these major findings of the Rosetta mission with respect to the origin of the material and puts them in the context of what we know from other comets and solar system objects

Characterization of selected strains of mucorales using fatty acid profiles Caracterização de linhagens de mucorales através do perfil de ácidos graxos

The fatty acid profiles of several fungi of the order Mucorales (Zygomycetes), including Backusella lamprospora (Lendner) Benny and R.K. Benj., Benjaminiella youngii P.M. Kirk, Circinella simplex van Tieghem, Cunninghamella blakesleeana Lendner, Mortierella ramanniana (Möller) Linnem., Mucor circinelloides f. janssenii (Lendner) Schipper, Mycotypha microspora Fenner, Rhizomucor miehei (Cooney and R. Emerson) Schipper and Rhizomucor pusillus (Lindt) Schipper, and of Volutella sp. Fr., from the class Ascomycetes, were qualitatively analysed by gas-liquid chromatography in order to determine the taxonomic value of these chemotaxonomic markers. The fatty acids present in all strains were palmitic (16:0), oleic (18:1), linoleic (18:2) and <FONT FACE="Symbol">g</FONT>-linolenic (18:3) acid, with the exception that the latter was not found in Volutella sp. Chemotaxonomic markers for some species and genera were obtained, including a non-identified fatty acid, FAME8 (minimum and maximum retention times of 27.92 and 28.28 minutes) for Rhizomucor miehei CCT 2236 and Rhizomucor pusillus CCT 4133, and FAME3 (minimum and maximum of 16.53 and 16.61 minutes) for Benjaminiella youngii CCT 4121. The chemotaxonomic marker of the order Mucorales was the fatty acid 18:3<FONT FACE="Symbol">w</FONT>6, confirming previous data from literature. The results of the present study suggest that qualitative fatty acid analysis can be an important chemotaxonomic tool for the classification of fungi assigned to the order Mucorales (Zygomycetes).<br>O perfil de ácidos graxos de Backusella lamprospora (Lendner) Benny e R.K. Benj., Benjaminiella youngii P.M. Kirk, Circinella simplex van Tieghem, Cunninghamella blakesleeana Lendner, Mortierella ramanniana (Möller) Linnem., Mucor circinelloides f. janssenii (Lendner) Schipper, Mycotypha microspora Fenner, Rhizomucor miehei (Cooney e R. Emerson) Schipper e Rhizomucor pusillus (Lindt) Schipper, da ordem Mucorales (Zygomycetes), e Volutella sp. Fr., da classe Ascomycetes, foram analisados qualitativamente por cromatografia gás-líquida, tendo como objetivo determinar o valor taxonômico destes marcadores quimiotaxonômicos. Os ácidos palmítico (16:0), oléico (18:1), linoléico (18:2) e <FONT FACE="Symbol">g</FONT>-linolênico (18:3) foram encontrados em todas as linhagens, com exceção do último, o qual não foi encontrado na linhagem de Volutella analisada. Foram obtidos marcadores quimiotaxonômicos para algumas espécies e gêneros estudados, incluindo um ácido graxo não-identificado, FAME8 (tempos de retenção mínimo e máximo de 27,92 e 28,28 minutos) para Rhizomucor miehei CCT 2236 e Rhizomucor pusillus CCT 4133 e FAME3 (tempos de retenção mínimo e máximo de 16,53 e 16,61 minutos) para Benjaminiella youngii CCT 4121. Para a ordem Mucorales, o marcador quimiotaxonômico obtido foi o ácido graxo 18:3<FONT FACE="Symbol">w</FONT>6, confirmando dados da literatura. Os resultados do presente estudo sugerem que a análise qualitativa do perfil de ácidos graxos pode ser uma ferramenta importante na classificação de fungos da ordem Mucorales (Zygomycetes)