FORMATION MODELS OF COMETARY ICES IN PROTOPLANETARY DISKS

被引：0

作者：

Chaparro Molano, G. ^{[1
]}

Kamp, I. ^{[2
]}

机构：

[1] Univ Sergio Arboleda, Observat Astron, Calle 74 14-14, Bogota 110221, Colombia

[2] Kapteyn Astron Inst, NL-9747 AV Groningen, Netherlands

来源：

XIV LATIN AMERICAN REGIONAL IAU MEETING | 2014年 / 44卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We set out to constrain the chemical conditions in the early Solar System by analyzing chemical evolution models of protoplanetary disks and comparing them to our current knowledge of Solar System bodies, such as comets. We propose that the region located at 10 AU <= r <= 30 AU is ideal for the formation of ice mantles that match observed cometary abundances. The growth of an ice mantle contributes to increase significantly the size of dust grains, which will impact the midplane temperature and the efficiency of dust coagulation.

引用

页码：5 / 5

页数：1

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