| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701514 | Icarus | 2011 | 11 Pages |
Abstract
⺠We compute the thermal- and condensation structure of the early Solar nebula. ⺠The snow line location depends on the accretion rate and the dust properties. ⺠The increase in solid matter by ice is substantially lower than currently assumed. ⺠There is a hot inner region with a thermostat at the dust evaporation temperature. ⺠In this region, sintering of materials will strongly influence grain growth.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
M. Min, C.P. Dullemond, M. Kama, C. Dominik,