On the aerodynamic redistribution of chondrite components in protoplanetary disks
On the aerodynamic redistribution of chondrite components in protoplanetary disks
复制标题
原行星盘中球粒陨石成分的气动重新分布
DOI:
10.1016/j.icarus.2012.04.022
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发表时间:
2012
期刊:
影响因子:
3.2
通讯作者:
S. Fromang
中科院分区:
文献类型:
--
作者:
E. Jacquet;M. Gounelle;S. Fromang
Despite being all roughly of solar composition, primitive meteorites (chondrites) present a diversity in their chemical, isotopic and petrographic properties, and in particular a first-order dichotomy between carbonaceous and non-carbonaceous chondrites. We investigate here analytically the dynamics of their components (chondrules, refractory inclusions, metal/sulfide and matrix grains) in protoplanetary disks prior to their incorporation in chondrite parent bodies. We find the dynamics of the solids, subject to gas drag, to be essentially controlled by the “gas–solid decoupling parameter”S≡St/α, the ratio of the dimensionless stopping time to the turbulence parameter. The decoupling of the solid particles relative to the gas is significant when S exceeds unity. S is expected to increase with time and heliocentric distance. On the basis of (i) abundance of refractory inclusions, (ii) proportion of matrix, (iii) lithophile element abundances, and (iv) oxygen isotopic composition of chondrules, we propose that non-matrix chondritic components had S<1 when carbonaceous chondrites accreted and S>1 when the other chondrites accreted. This suggests that accretion of carbonaceous chondrites predated on average that of the other chondrites and that refractory inclusions are genetically related to their host carbonaceous chondrites.
影响因子:
2.2
作者:
Hezel, Dominik C.;Russell, Sara S.;Kearsley, Anton T.
通讯作者:
Kearsley, Anton T.
影响因子:
5
作者:
A. Stracke;H. Palme;M. Gellissen;C. Münker;T. Kleine;Karin Birbaum;D. Günther;B. Bourdon;J. Zipfel
通讯作者:
A. Stracke;H. Palme;M. Gellissen;C. Münker;T. Kleine;Karin Birbaum;D. Günther;B. Bourdon;J. Zipfel
影响因子:
5.3
作者:
D. Hezel;H. Palme
通讯作者:
D. Hezel;H. Palme