کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
9522596 | 1634957 | 2005 | 12 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
A short timescale for changing oxygen fugacity in the solar nebula revealed by high-resolution 26Al-26Mg dating of CAI rims
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
علوم زمین و سیاره ای (عمومی)
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چکیده انگلیسی
Most rocky objects in the solar system, including the primitive chondrites and the terrestrial planets themselves, formed at oxygen fugacities (fO2) near that of the Iron-Wüstite (IW) fO2 buffer. Conversely, the most ancient rocky objects of the solar system, the calcium aluminum-rich inclusions (CAIs), formed at fO2 values 5 orders of magnitude lower than the IW buffer in an environment more closely resembling a solar gas. High-resolution Mg isotope data and estimates for fO2 for rims on CAIs show that this shift from â¼solar to protoplanetary (chondritic) fO2 occurred in 100,000 to 300,000 yr for these objects. Magnesium isotopes show further that the rise in fO2 was accompanied by a rise in the partial pressure of Mg. These results establish that CAIs entered a region resembling where planet progenitors formed within 3Â ÃÂ 105 yr of their formation in the solar nebula.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 238, Issues 3â4, 15 October 2005, Pages 272-283
Journal: Earth and Planetary Science Letters - Volume 238, Issues 3â4, 15 October 2005, Pages 272-283
نویسندگان
Justin I. Simon, Edward D. Young, Sara S. Russell, Eric K. Tonui, Kathryn A. Dyl, Craig E. Manning,