FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4210362967> ?p ?o ?g. }

• W4210362967 endingPage "449" @default.
• W4210362967 startingPage "435" @default.
• W4210362967 abstract "Abstract NorthWest Africa 10628 (NWA 10628) is a shergottite found in Tindouf (Algeria) in 2014. Little is known on this meteorite apart from the Meteoritical Bulletin report. In this work, original and altered mineral phases of NWA 10628 were characterised by micro‐Raman spectroscopy assisted with micro‐energy dispersive X‐ray fluorescence imaging. The matrix of the meteorite is dominated by high‐Ca pyroxenes, augite ((Ca,Na)(Mg,Fe,Al,Ti)(Si,Al) 2 O 6 ) and diopside (CaMgSi 2 O 6 ). Olivine and feldspars appeared as small crystals all along the matrix. Merrillite (Ca 9 NaMg(PO 4 ) 7 ) was found as big crystals in inclusions. As whitlockite (Ca 9 NaMg(PO 4 ) 6 (HPO 4 )) can be transformed into merrillite at high temperature and pressure, we suggest that merrillite in the meteorite was originally whitlockite, before its ejection from Mars. Gypsum (CaSO 4 ·2H 2 O) was found as small crystals and in fractures; this last one could come from terrestrial weathering because it was associated with calcite (CaCO 3 ). Small anhydrite (CaSO 4 ) crystals are shown in the bulk together with gypsum, probably from the partial dehydration of original Martian gypsum by the high‐pressure/temperature of ejection. Pyrite and marcasite (FeS 2 polymorphs) minerals were detected, as well as their oxidation products, goethite (α‐FeO (OH)) and rozenite (FeSO 4 ·4H 2 O), due to their terrestrial weathering. The identification of hematite (Fe 2 O 3 ), magnetite (Fe 3 O 4 ), ilmenite (FeTiO 3 ) and anatase (TiO 2 ) suggested that ulvospinel (Fe 2 TiO 4 ) was the precursor on Mars, because ulvospinel is transformed into ilmenite by pressure and later ilmenite can be altered to magnetite/hematite and anatase by oxidative weathering on Earth. This non‐destructive analytical methodology provides deep mineralogical characterisation adequate for scarce samples like those returning from the Mars Sample Return mission." @default.
• W4210362967 created "2022-02-08" @default.
• W4210362967 creator A5006312958 @default.
• W4210362967 creator A5009847049 @default.
• W4210362967 creator A5014133800 @default.
• W4210362967 creator A5047633922 @default.
• W4210362967 creator A5064120053 @default.
• W4210362967 creator A5078978971 @default.
• W4210362967 creator A5087361975 @default.
• W4210362967 creator A5060060168 @default.
• W4210362967 date "2022-01-27" @default.
• W4210362967 modified "2023-10-09" @default.
• W4210362967 title "Original and alteration mineral phases in the NWA 10628 Martian shergottite determined by micro‐Raman spectroscopy assisted with micro‐energy dispersive X‐ray fluorescence imaging" @default.
• W4210362967 cites W1566788261 @default.
• W4210362967 cites W1898254927 @default.
• W4210362967 cites W1969417208 @default.
• W4210362967 cites W1997618648 @default.
• W4210362967 cites W1999771813 @default.
• W4210362967 cites W2015856769 @default.
• W4210362967 cites W2018642420 @default.
• W4210362967 cites W2031578559 @default.
• W4210362967 cites W2035129310 @default.
• W4210362967 cites W2044160398 @default.
• W4210362967 cites W2046944925 @default.
• W4210362967 cites W2050041941 @default.
• W4210362967 cites W2055493473 @default.
• W4210362967 cites W2057927816 @default.
• W4210362967 cites W2085142070 @default.
• W4210362967 cites W2101223042 @default.
• W4210362967 cites W2101226812 @default.
• W4210362967 cites W2114057247 @default.
• W4210362967 cites W2130253237 @default.
• W4210362967 cites W2138853606 @default.
• W4210362967 cites W2160811744 @default.
• W4210362967 cites W2266253915 @default.
• W4210362967 cites W2317330103 @default.
• W4210362967 cites W2329234523 @default.
• W4210362967 cites W2338492782 @default.
• W4210362967 cites W2341462518 @default.
• W4210362967 cites W2462664897 @default.
• W4210362967 cites W2594277300 @default.
• W4210362967 cites W2623640619 @default.
• W4210362967 cites W2757044229 @default.
• W4210362967 cites W2792447901 @default.
• W4210362967 cites W3004112162 @default.
• W4210362967 cites W3096843802 @default.
• W4210362967 cites W4230493275 @default.
• W4210362967 cites W4250870406 @default.
• W4210362967 doi "https://doi.org/10.1002/jrs.6305" @default.
• W4210362967 hasPublicationYear "2022" @default.
• W4210362967 type Work @default.
• W4210362967 citedByCount "4" @default.
• W4210362967 countsByYear W42103629672022 @default.
• W4210362967 countsByYear W42103629672023 @default.
• W4210362967 crossrefType "journal-article" @default.
• W4210362967 hasAuthorship W4210362967A5006312958 @default.
• W4210362967 hasAuthorship W4210362967A5009847049 @default.
• W4210362967 hasAuthorship W4210362967A5014133800 @default.
• W4210362967 hasAuthorship W4210362967A5047633922 @default.
• W4210362967 hasAuthorship W4210362967A5060060168 @default.
• W4210362967 hasAuthorship W4210362967A5064120053 @default.
• W4210362967 hasAuthorship W4210362967A5078978971 @default.
• W4210362967 hasAuthorship W4210362967A5087361975 @default.
• W4210362967 hasConcept C113196181 @default.
• W4210362967 hasConcept C116862484 @default.
• W4210362967 hasConcept C120665830 @default.
• W4210362967 hasConcept C121332964 @default.
• W4210362967 hasConcept C127313418 @default.
• W4210362967 hasConcept C130635790 @default.
• W4210362967 hasConcept C185592680 @default.
• W4210362967 hasConcept C191897082 @default.
• W4210362967 hasConcept C192562407 @default.
• W4210362967 hasConcept C199289684 @default.
• W4210362967 hasConcept C2776283581 @default.
• W4210362967 hasConcept C2776342828 @default.
• W4210362967 hasConcept C2776432453 @default.
• W4210362967 hasConcept C2776567116 @default.
• W4210362967 hasConcept C2777018398 @default.
• W4210362967 hasConcept C2777156721 @default.
• W4210362967 hasConcept C2779181077 @default.
• W4210362967 hasConcept C2779870107 @default.
• W4210362967 hasConcept C2780191791 @default.
• W4210362967 hasConcept C2780364934 @default.
• W4210362967 hasConcept C2780375929 @default.
• W4210362967 hasConcept C40003534 @default.
• W4210362967 hasConcept C43617362 @default.
• W4210362967 hasConcept C87355193 @default.
• W4210362967 hasConceptScore W4210362967C113196181 @default.
• W4210362967 hasConceptScore W4210362967C116862484 @default.
• W4210362967 hasConceptScore W4210362967C120665830 @default.
• W4210362967 hasConceptScore W4210362967C121332964 @default.
• W4210362967 hasConceptScore W4210362967C127313418 @default.
• W4210362967 hasConceptScore W4210362967C130635790 @default.
• W4210362967 hasConceptScore W4210362967C185592680 @default.
• W4210362967 hasConceptScore W4210362967C191897082 @default.
• W4210362967 hasConceptScore W4210362967C192562407 @default.
• W4210362967 hasConceptScore W4210362967C199289684 @default.
• W4210362967 hasConceptScore W4210362967C2776283581 @default.

• next