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Volumn 317, Issue 5846, 2007, Pages 1900-1903

Late archean biospheric oxygenation and atmospheric evolution

Author keywords

[No Author keywords available]

Indexed keywords

OXYGEN;

EID: 34848904580     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1138700     Document Type: Article
Times cited : (326)

References (38)
  • 5
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    • Details of the new scientific core, methods of analysis and calculations, a brief review of S isotope variations through the geological record, and time-series data from a broadly equivalent South African core are available (along with data tables) as supporting material on Science Online.
    • Details of the new scientific core, methods of analysis and calculations, a brief review of S isotope variations through the geological record, and time-series data from a broadly equivalent South African core are available (along with data tables) as supporting material on Science Online.
  • 9
    • 34848893987 scopus 로고    scopus 로고
    • A. D. Anbar et al., Science 317, 1903 (2007).
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  • 17
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    • A. Bekker et al., Nature 427, 117 (2004).
    • (2004) Nature , vol.427 , pp. 117
    • Bekker, A.1
  • 18
    • 34848857242 scopus 로고    scopus 로고
    • 36S, respectively.
    • 36S, respectively.
  • 19
    • 34848837535 scopus 로고    scopus 로고
    • 33S = -0.54 (±0.17).
    • 33S = -0.54 (±0.17).
  • 20
    • 34848849371 scopus 로고    scopus 로고
    • Atmospheric photochemistry is presently the only known mechanism that can account for the nonzero Δ33S data and their relationship to Δ36S values in the Archean record (1-4, 17, The principal source of S in the Archean atmosphere was volcanic (although biogenic sources may have also existed, Gas-phase photochemistry involving sulfur dioxide or sulfur monoxide has been shown in closed-cell photochemical experiments (2) to result in NMD sulfate (SO42, with negative, and in some cases positive, Δ33S values) and elemental S (S8, with positive Δ33S values, These reactions are sensitive to the wavelength of available ultraviolet radiation, and this parameter depends on, among other things, atmospheric O2 concentrations. The transfer pathways of S from the atmosphere to Earth's surface also depend on O2 concentration. An atmospheric model (4) cons
    • 2, the two S reservoirs homogenize in the atmosphere, and the photochemical signal is not preserved.
  • 23
    • 34848831354 scopus 로고    scopus 로고
    • This interpretation is based on the assumption that S metabolisms operating at the Archean/Proterozoic boundary are similar to those of today. At present, we see no other realistic environmental scenario that could account for the unusual S isotope compositions of the upper Mount McRae Shale
    • This interpretation is based on the assumption that S metabolisms operating at the Archean/Proterozoic boundary are similar to those of today. At present, we see no other realistic environmental scenario that could account for the unusual S isotope compositions of the upper Mount McRae Shale.
  • 25
    • 28544449263 scopus 로고    scopus 로고
    • D. T. Johnston et al., Science 310, 1477 (2005).
    • (2005) Science , vol.310 , pp. 1477
    • Johnston, D.T.1
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    • 27644562800 scopus 로고    scopus 로고
    • I. McDonald, A. J. Boyce, I. B. Butler, R. J. Herrington, D. A. Polya, Eds, Geol. Soc. London Spec. Pub, London
    • J. Farquhar, B. A. Wing, in Mineral Deposits and Earth Evolution, I. McDonald, A. J. Boyce, I. B. Butler, R. J. Herrington, D. A. Polya, Eds. (Geol. Soc. London Spec. Pub., London, 2005), vol. 248, pp. 167-177.
    • (2005) Mineral Deposits and Earth Evolution , vol.248 , pp. 167-177
    • Farquhar, J.1    Wing, B.A.2
  • 28
    • 34848888227 scopus 로고    scopus 로고
    • 33S reservoir. Ultimately, the balance of sources and sinks maintained generally low sulfate concentrations that allowed for spatial isotopic heterogeneities.
    • 33S reservoir. Ultimately, the balance of sources and sinks maintained generally low sulfate concentrations that allowed for spatial isotopic heterogeneities.
  • 33
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    • H. Ohmoto et al., Nature 442, 908 (2006).
    • (2006) Nature , vol.442 , pp. 908
    • Ohmoto, H.1
  • 35
    • 34848816979 scopus 로고    scopus 로고
    • 33S slopes.
    • 33S slopes.
  • 38
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    • We thank the NASA Astrobiology Institute and the Geological Survey of Western Australia for drilling of the ABDP-9 core; the NSF for scientific funding for the project; J. S. R. Dunlop, L. C. Bonser, M. van Kranendonk, A. Hickman, and the Geological Survey of Western Australia for assisting with core recovery; B. Runnegar and R. Grymes for launching the Astrobiology Drilling Program; A. H. Knoll for long-term support of the project; J. Kasting, B. Simonson, and anonymous reviewers for their comments and suggestions; and the Gas Source Mass Spectrometry research staff at the University of Maryland, including N. Collins, K. Yokoyama, B. Williams, and A. Shrestha for their analytical efforts. Samples from the AD-5 core were provided to N. Beukes, C. Klein, and A.J.K. by Griqualand Exploration and Finance Company in South Africa
    • We thank the NASA Astrobiology Institute and the Geological Survey of Western Australia for drilling of the ABDP-9 core; the NSF for scientific funding for the project; J. S. R. Dunlop, L. C. Bonser, M. van Kranendonk, A. Hickman, and the Geological Survey of Western Australia for assisting with core recovery; B. Runnegar and R. Grymes for launching the Astrobiology Drilling Program; A. H. Knoll for long-term support of the project; J. Kasting, B. Simonson, and anonymous reviewers for their comments and suggestions; and the Gas Source Mass Spectrometry research staff at the University of Maryland, including N. Collins, K. Yokoyama, B. Williams, and A. Shrestha for their analytical efforts. Samples from the AD-5 core were provided to N. Beukes, C. Klein, and A.J.K. by Griqualand Exploration and Finance Company in South Africa.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.