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DOI | 10.1126/science.272.5266.1314 |
Type II supernova matter in a silicon carbide grain from the Murchison meteorite | |
Hoppe P.; Strebel R.; Eberhardt P.; Amari S.; Lewis R.S. | |
发表日期 | 1996 |
ISSN | 0036-8075 |
起始页码 | 1314 |
结束页码 | 1316 |
卷号 | 272期号:5266 |
英文摘要 | The circumstellar silicon carbide (SiC) grain X57 from the Murchison meteorite contains large amounts of radiogenic calcium-44 (20 times its solar system abundance) and has an anomalous silicon isotopic composition, different from other circumstellar SiC grains. Its inferred initial 44Ti/Si and 44Ti/48Ti ratios are 1.6 × 10-4 and 0.37. In addition, it contains radiogenic magnesium-26; the inferred initial 26Al/27Al ratio is 0.11. The isotopic and elemental data of X57 can be explained by selective mixing of matter from different zones of a typical type II supernova of 25 solar masses during its explosion. The high 44Ti/Si ratio requires contributions from the innermost nickel zone of the supernova to the SiC condensation site, as similarly suggested by astronomical observations. |
英文关键词 | carbonaceous chondrite; isotopic composition; Murchison meteorite; silicon carbide; supernova type II |
语种 | 英语 |
来源期刊 | Science
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/244057 |
作者单位 | Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland; Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, United States; McDonnell Center, Space Sci. and Physics Department, Washington University, St. Louis, MO 63130, United States |
推荐引用方式 GB/T 7714 | Hoppe P.,Strebel R.,Eberhardt P.,et al. Type II supernova matter in a silicon carbide grain from the Murchison meteorite[J],1996,272(5266). |
APA | Hoppe P.,Strebel R.,Eberhardt P.,Amari S.,&Lewis R.S..(1996).Type II supernova matter in a silicon carbide grain from the Murchison meteorite.Science,272(5266). |
MLA | Hoppe P.,et al."Type II supernova matter in a silicon carbide grain from the Murchison meteorite".Science 272.5266(1996). |
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