The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system

We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Abreu, N.M. [verfasserIn] Aponte, J.C. [verfasserIn] Cloutis, E.A. [verfasserIn] Nguyen, A.N. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Schlagwörter:	CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra

Systematik:	VA 1120

Übergeordnetes Werk:	Enthalten in: Chemie der Erde - München : Elsevier, 2002, 80
Übergeordnetes Werk:	volume:80

DOI / URN:	10.1016/j.chemer.2020.125631

Katalog-ID:	ELV005217202

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520			\|a We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed.
650		4	\|a CR chondrites
650		4	\|a Carbonaceous chondrites
650		4	\|a Aqueous alteration
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650		4	\|a CR chondrite petrology
650		4	\|a CR chondrite mineralogy
650		4	\|a CR chondrite spectra
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700	1		\|a Cloutis, E.A. \|e verfasserin \|4 aut
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author_variant	n a na j a ja e c ec a n an
matchkey_str	article:16115864:2020----::hrnzoieabncoshnrtsseoretudrtntergnvltoa
hierarchy_sort_str	2020
bklnumber	38.32
publishDate	2020
allfields	10.1016/j.chemer.2020.125631 doi (DE-627)ELV005217202 (ELSEVIER)S0009-2819(20)30032-5 DE-627 ger DE-627 rda eng 550 DE-600 VA 1120 rvk (DE-625)rvk/146972: 38.32 bkl Abreu, N.M. verfasserin aut The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed. CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra Aponte, J.C. verfasserin aut Cloutis, E.A. verfasserin aut Nguyen, A.N. verfasserin aut Enthalten in Chemie der Erde München : Elsevier, 2002 80 Online-Ressource (DE-627)350638489 (DE-600)2082649-7 (DE-576)104345101 1611-5864 nnns volume:80 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-GGO GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 VA 1120 Zeitschriften Chemie und Pharmazie Referateorgane, Zeitschriften, Handbücher Zeitschriften (DE-625)rvk/146972: (DE-576)206609647 38.32 Geochemie AR 80
spelling	10.1016/j.chemer.2020.125631 doi (DE-627)ELV005217202 (ELSEVIER)S0009-2819(20)30032-5 DE-627 ger DE-627 rda eng 550 DE-600 VA 1120 rvk (DE-625)rvk/146972: 38.32 bkl Abreu, N.M. verfasserin aut The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed. CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra Aponte, J.C. verfasserin aut Cloutis, E.A. verfasserin aut Nguyen, A.N. verfasserin aut Enthalten in Chemie der Erde München : Elsevier, 2002 80 Online-Ressource (DE-627)350638489 (DE-600)2082649-7 (DE-576)104345101 1611-5864 nnns volume:80 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-GGO GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 VA 1120 Zeitschriften Chemie und Pharmazie Referateorgane, Zeitschriften, Handbücher Zeitschriften (DE-625)rvk/146972: (DE-576)206609647 38.32 Geochemie AR 80
allfields_unstemmed	10.1016/j.chemer.2020.125631 doi (DE-627)ELV005217202 (ELSEVIER)S0009-2819(20)30032-5 DE-627 ger DE-627 rda eng 550 DE-600 VA 1120 rvk (DE-625)rvk/146972: 38.32 bkl Abreu, N.M. verfasserin aut The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed. CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra Aponte, J.C. verfasserin aut Cloutis, E.A. verfasserin aut Nguyen, A.N. verfasserin aut Enthalten in Chemie der Erde München : Elsevier, 2002 80 Online-Ressource (DE-627)350638489 (DE-600)2082649-7 (DE-576)104345101 1611-5864 nnns volume:80 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-GGO GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 VA 1120 Zeitschriften Chemie und Pharmazie Referateorgane, Zeitschriften, Handbücher Zeitschriften (DE-625)rvk/146972: (DE-576)206609647 38.32 Geochemie AR 80
allfieldsGer	10.1016/j.chemer.2020.125631 doi (DE-627)ELV005217202 (ELSEVIER)S0009-2819(20)30032-5 DE-627 ger DE-627 rda eng 550 DE-600 VA 1120 rvk (DE-625)rvk/146972: 38.32 bkl Abreu, N.M. verfasserin aut The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed. CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra Aponte, J.C. verfasserin aut Cloutis, E.A. verfasserin aut Nguyen, A.N. verfasserin aut Enthalten in Chemie der Erde München : Elsevier, 2002 80 Online-Ressource (DE-627)350638489 (DE-600)2082649-7 (DE-576)104345101 1611-5864 nnns volume:80 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-GGO GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 VA 1120 Zeitschriften Chemie und Pharmazie Referateorgane, Zeitschriften, Handbücher Zeitschriften (DE-625)rvk/146972: (DE-576)206609647 38.32 Geochemie AR 80
allfieldsSound	10.1016/j.chemer.2020.125631 doi (DE-627)ELV005217202 (ELSEVIER)S0009-2819(20)30032-5 DE-627 ger DE-627 rda eng 550 DE-600 VA 1120 rvk (DE-625)rvk/146972: 38.32 bkl Abreu, N.M. verfasserin aut The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system 2020 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed. CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra Aponte, J.C. verfasserin aut Cloutis, E.A. verfasserin aut Nguyen, A.N. verfasserin aut Enthalten in Chemie der Erde München : Elsevier, 2002 80 Online-Ressource (DE-627)350638489 (DE-600)2082649-7 (DE-576)104345101 1611-5864 nnns volume:80 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-GGO GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 VA 1120 Zeitschriften Chemie und Pharmazie Referateorgane, Zeitschriften, Handbücher Zeitschriften (DE-625)rvk/146972: (DE-576)206609647 38.32 Geochemie AR 80
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topic_facet	CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra
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author	Abreu, N.M.
spellingShingle	Abreu, N.M. ddc 550 rvk VA 1120 bkl 38.32 misc CR chondrites misc Carbonaceous chondrites misc Aqueous alteration misc Primitive meteorites misc CR chondrite petrology misc CR chondrite mineralogy misc CR chondrite spectra The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
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topic_title	550 DE-600 VA 1120 rvk (DE-625)rvk/146972 38.32 bkl The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system CR chondrites Carbonaceous chondrites Aqueous alteration Primitive meteorites CR chondrite petrology CR chondrite mineralogy CR chondrite spectra
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title	The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
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title_full	The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
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title_sort	the renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
title_auth	The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
abstract	We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed.
abstractGer	We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed.
abstract_unstemmed	We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. This paper summarizes these investigations, their similarities, and differences with other chondritic groups, their relationships to asteroids, and the questions yet to be addressed.
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title_short	The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system
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up_date	2024-07-06T17:12:51.141Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV005217202</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230524165846.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230503s2020 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.chemer.2020.125631</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV005217202</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0009-2819(20)30032-5</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">550</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">VA 1120</subfield><subfield code="2">rvk</subfield><subfield code="0">(DE-625)rvk/146972:</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">38.32</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Abreu, N.M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2020</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">We present here a review of the characteristics of CR carbonaceous chondrite meteorites. Over the past three decades, our knowledge and understanding of the scientific value of the CR chondrites have increased dramatically, as more samples from cold and hot deserts have become available for analysis. Based on a variety of compositional, mineralogical, isotopic, and spectroscopic studies, we have come to understand that CR chondrites are excellent samples of asteroidal meteorites to look for virtually unaltered solar nebula material and to observe asteroidal processes in progress. 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The Renazzo-like carbonaceous chondrites as resources to understand the origin, evolution, and exploration of the solar system

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