登录注册
Quick Links : Mindat手册The Rock H. Currier Digital LibraryMindat Newsletter [Free Download]
主页关于 MindatMindat手册Mindat的历史版权Who We Are联系我们于 Mindat.org刊登广告
捐赠给 MindatCorporate Sponsorship赞助板页已赞助的板页在 Mindat刊登 广告的广告商于 Mindat.org刊登广告
Learning CenterWhat is a mineral?The most common minerals on earthInformation for EducatorsMindat ArticlesThe ElementsThe Rock H. Currier Digital LibraryGeologic Time
搜索矿物的性质搜索矿物的化学Advanced Locality Search随意显示任何一 种矿物Random Locality使用minID搜索邻近产地Search Articles搜索词汇表更多搜索选项
搜索:
矿物名称:
地区产地名称:
关键字:
 
Mindat手册添加新照片Rate Photos产区编辑报告Coordinate Completion Report添加词汇表项目
Mining Companies统计会员列表Mineral MuseumsClubs & Organizations矿物展及活动The Mindat目录表设备设置The Mineral Quiz
照片搜索Photo GalleriesSearch by Color今天最新的照片昨天最新的照片用户照片相集过去每日精选照片相集Photography

Rai, V. K. (2005) Photochemical Mass-Independent Sulfur Isotopes in Achondritic Meteorites. Science, 309 (5737). 1062-1065 doi:10.1126/science.1112954

Advanced
   -   Only viewable:
Reference TypeJournal (article/letter/editorial)
TitlePhotochemical Mass-Independent Sulfur Isotopes in Achondritic Meteorites
JournalScience
AuthorsRai, V. K.Author
Year2005 (August 12)Volume309
Page(s)1062-1065Issue5737
PublisherAmerican Association for the Advancement of Science (AAAS)
DOIdoi:10.1126/science.1112954Search in ResearchGate
Mindat Ref. ID2576752Long-form Identifiermindat:1:5:2576752:8
GUID6a1d04f9-a624-4a77-a25c-ee72e618dffc
Full ReferenceRai, V. K. (2005) Photochemical Mass-Independent Sulfur Isotopes in Achondritic Meteorites. Science, 309 (5737). 1062-1065 doi:10.1126/science.1112954
Plain TextRai, V. K. (2005) Photochemical Mass-Independent Sulfur Isotopes in Achondritic Meteorites. Science, 309 (5737). 1062-1065 doi:10.1126/science.1112954
In(2005, August) Science Vol. 309 (5737) American Association for the Advancement of Science (AAAS)

References Listed

These are the references the publisher has listed as being connected to the article. Please check the article itself for the full list of references which may differ. Not all references are currently linkable within the Digital Library.

There have been numerous presolar oxide grains with anomalous oxygen identified but their abundance is far too small and of the wrong isotopic composition to account for oxygen isotopic anomalies known to be present at the bulk meteorite level [( 2 ) and references therein].
Not Yet Imported: Accounts of Chemical Research - journal-article : 10.1021/ar960224f

If you would like this item imported into the Digital Library, please contact us quoting Journal ID 470
M. H. Thiemens, in Treaties on Geochemistry, R. F. Keeling, Ed. (Elsevier, Oxford, 2003), vol. 4, pp. 159–175.
Sulfide extractions were done by using the procedure described in ( 13 ); also see online Materials and Methods for more details. The typical errors of δ 33 S δ 34 S and δ 36 S measurements are 0.010 0.010 and 0.200 (in ‰) respectively.
We calculated 33 S and 36 S enrichment with the following equation: Δ 33 S = δ 33 S – 1000[(1 + δ 34 S/1000) 0.515 – 1] and Δ 36 S = δ 36 S – 1000[(1 + δ 34 S/1000) 1.91 – 1].
Y. N. Chin, C. Henkel, J. B. Whiteoak, N. Langer, E. B. Churchwell, Astron. Astrophys.305, 960 (1996).
As a result of its small abundance δ 36 S is sensitive to contaminations at any stage from chemical extraction or gas chromatography or during measurements. The reported error on δ 36 S is only measurement error; the actual uncertainty due to contamination might be higher.
A. N. Krot, B. Fegley, K. Lodders, H. Palme, in Protostars and Planets IV, V. Mannings, A. P. Boss, S. S. Russell, Eds. (Univ. of Arizona, Tucson, AZ, 2000), pp. 1019–1054.
NASA Cosmochemistry program is gratefully acknowledged for support of this research.


See Also

These are possibly similar items as determined by title/reference text matching only.

 
and/or  
Mindat Discussions Facebook Logo Instagram Logo Discord Logo
版权所有© mindat.org1993年至2024年,除了规定的地方。 Mindat.org全赖于全球数千个以上成员和支持者们的参与。
隐私政策 - 条款和条款细则 - 联络我们 - Report a bug/vulnerability Current server date and time: 2024.5.8 20:01:20
Go to top of page