Matches in SemOpenAlex for { <https://semopenalex.org/work/W1995061945> ?p ?o ?g. }
- W1995061945 endingPage "99" @default.
- W1995061945 startingPage "83" @default.
- W1995061945 abstract "We have investigated secondary influences on the noble gas budget in rim and interior pairs of three Martian meteorites from Antarctica: the lherzolitic shergottites Y000027 and Y000097, and the nakhlite Y000593. Three factors have been found to influence the original Martian noble gas budget: shock metamorphic overprint, cosmic irradiation, and terrestrial weathering. The 3He/4He ratio of the shergottites is between 0.189 and 0.217, which indicates almost complete loss of radiogenic 4He. This is expected from the high shock pressure observed in the shergottite samples. The concentration of 4He in these shergottite samples ranges from 33.8 to 39.4 × 10−8 ccSTP/g. 22Ne in the shergottites is on the order of 14 × 10−9 ccSTP/g. The nakhlite has ∼800 × 10−8 ccSTP/g 4He and ∼26 × 10−9 ccSTP/g 22Ne. An indication for solar cosmic ray contribution to the neon budget can be found in the shergottites. As Y000027 and Y000097 are reported to be paired we conclude the cosmic ray exposure (CRE) age T(3+21) of this shergottite to be 4.41 ± 0.54 Ma. For the nakhlite Y000593 T(3+21) is 11.8 ± 0.3 Ma. Heavy noble gas concentrations show large differences between rim and interior samples with the rim samples having 1.3–2.9, 1.7–38, and 1.4–20 times as much 36Ar, 84Kr, and 132Xe, respectively. The enrichment of heavy noble gases in the rim samples indicates severe terrestrial contamination. The relation between 129Xe/132Xe and 84Kr/132Xe in the rim samples shows that the incorporation mechanism caused elemental fractionation of Kr and Xe to the extent that in the Y000027 shergottite samples any Martian signature is completely masked by terrestrial contamination, if the total is taken. Only the 1400 °C steps show clear evidence for Martian atmosphere. The Y000593 nakhlite interior sample, on the other hand, shows low 84Kr/132Xe in relation to 129Xe/132Xe, which is characteristic for fractionated Martian atmosphere observed in nakhlites." @default.
- W1995061945 created "2016-06-24" @default.
- W1995061945 creator A5035578260 @default.
- W1995061945 creator A5035584356 @default.
- W1995061945 creator A5047827998 @default.
- W1995061945 date "2009-09-01" @default.
- W1995061945 modified "2023-09-30" @default.
- W1995061945 title "Noble gases in two shergottites and one nakhlite from Antarctica: Y000027, Y000097, and Y000593" @default.
- W1995061945 cites W1964591408 @default.
- W1995061945 cites W1966383562 @default.
- W1995061945 cites W1967220311 @default.
- W1995061945 cites W1967719914 @default.
- W1995061945 cites W1974075852 @default.
- W1995061945 cites W1977024643 @default.
- W1995061945 cites W1980354234 @default.
- W1995061945 cites W1980705055 @default.
- W1995061945 cites W1981194876 @default.
- W1995061945 cites W1993062389 @default.
- W1995061945 cites W1995806863 @default.
- W1995061945 cites W2007683078 @default.
- W1995061945 cites W2009223269 @default.
- W1995061945 cites W2011135993 @default.
- W1995061945 cites W2014883840 @default.
- W1995061945 cites W2015527356 @default.
- W1995061945 cites W2022454680 @default.
- W1995061945 cites W2024430005 @default.
- W1995061945 cites W2024862469 @default.
- W1995061945 cites W2025516746 @default.
- W1995061945 cites W2027277943 @default.
- W1995061945 cites W2027519531 @default.
- W1995061945 cites W2033098842 @default.
- W1995061945 cites W2035947215 @default.
- W1995061945 cites W2038845141 @default.
- W1995061945 cites W2041522814 @default.
- W1995061945 cites W2048091267 @default.
- W1995061945 cites W2049711752 @default.
- W1995061945 cites W2060089231 @default.
- W1995061945 cites W2061138336 @default.
- W1995061945 cites W2065454174 @default.
- W1995061945 cites W2070810804 @default.
- W1995061945 cites W2077722287 @default.
- W1995061945 cites W2081538356 @default.
- W1995061945 cites W2089222214 @default.
- W1995061945 cites W2089923948 @default.
- W1995061945 cites W2089964740 @default.
- W1995061945 cites W2091767388 @default.
- W1995061945 cites W2141190941 @default.
- W1995061945 doi "https://doi.org/10.1016/j.polar.2009.06.001" @default.
- W1995061945 hasPublicationYear "2009" @default.
- W1995061945 type Work @default.
- W1995061945 sameAs 1995061945 @default.
- W1995061945 citedByCount "11" @default.
- W1995061945 countsByYear W19950619452012 @default.
- W1995061945 countsByYear W19950619452013 @default.
- W1995061945 countsByYear W19950619452017 @default.
- W1995061945 countsByYear W19950619452019 @default.
- W1995061945 countsByYear W19950619452020 @default.
- W1995061945 countsByYear W19950619452022 @default.
- W1995061945 countsByYear W19950619452023 @default.
- W1995061945 crossrefType "journal-article" @default.
- W1995061945 hasAuthorship W1995061945A5035578260 @default.
- W1995061945 hasAuthorship W1995061945A5035584356 @default.
- W1995061945 hasAuthorship W1995061945A5047827998 @default.
- W1995061945 hasConcept C111309251 @default.
- W1995061945 hasConcept C121332964 @default.
- W1995061945 hasConcept C121530826 @default.
- W1995061945 hasConcept C127313418 @default.
- W1995061945 hasConcept C130635790 @default.
- W1995061945 hasConcept C17409809 @default.
- W1995061945 hasConcept C178790620 @default.
- W1995061945 hasConcept C185592680 @default.
- W1995061945 hasConcept C192562407 @default.
- W1995061945 hasConcept C2778600265 @default.
- W1995061945 hasConcept C44870925 @default.
- W1995061945 hasConcept C57016615 @default.
- W1995061945 hasConcept C67236022 @default.
- W1995061945 hasConcept C83260615 @default.
- W1995061945 hasConcept C87355193 @default.
- W1995061945 hasConceptScore W1995061945C111309251 @default.
- W1995061945 hasConceptScore W1995061945C121332964 @default.
- W1995061945 hasConceptScore W1995061945C121530826 @default.
- W1995061945 hasConceptScore W1995061945C127313418 @default.
- W1995061945 hasConceptScore W1995061945C130635790 @default.
- W1995061945 hasConceptScore W1995061945C17409809 @default.
- W1995061945 hasConceptScore W1995061945C178790620 @default.
- W1995061945 hasConceptScore W1995061945C185592680 @default.
- W1995061945 hasConceptScore W1995061945C192562407 @default.
- W1995061945 hasConceptScore W1995061945C2778600265 @default.
- W1995061945 hasConceptScore W1995061945C44870925 @default.
- W1995061945 hasConceptScore W1995061945C57016615 @default.
- W1995061945 hasConceptScore W1995061945C67236022 @default.
- W1995061945 hasConceptScore W1995061945C83260615 @default.
- W1995061945 hasConceptScore W1995061945C87355193 @default.
- W1995061945 hasIssue "2" @default.
- W1995061945 hasLocation W19950619451 @default.
- W1995061945 hasOpenAccess W1995061945 @default.
- W1995061945 hasPrimaryLocation W19950619451 @default.
- W1995061945 hasRelatedWork W1488072048 @default.