Noble gases and Earth's accretion

被引:109
作者
Harper, CL
Jacobsen, SB
机构
[1] Harvard Ctr. for Isotope Geochem., Dept. of Earth and Planet. Sciences, Harvard University, Cambridge, MA 02138
关键词
D O I
10.1126/science.273.5283.1814
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Earth probably accreted in two stages corresponding to conditions before and after the removal of gas from the nebular disk. Helium and neon in the mantle primarily record a solar like component likely incorporated during the first stage by solution into a magma ocean blanketed under a massive protoatmosphere of molecular hydrogen and helium. The heavier noble gases primarily reflect a meteoritic (planetary) component trapped in accreted planetesimals. This model provides a possible explanation for the reduced and oxidized accretion stages inferred from siderophile elements and may explain why the present mantle appears to be too oxidized to be in equilibrium with the core.
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页码:1814 / 1818
页数:5
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