PLANETARY ACCRETION RATES - ANALYTICAL DERIVATION

被引：58

作者：

GREENBERG, R ^{[1
]}

BOTTKE, WF ^{[1
]}

CARUSI, A ^{[1
]}

VALSECCHI, GB ^{[1
]}

机构：

[1] IAS,REPARTO PLANETOL,I-00185 ROME,ITALY

来源：

ICARUS | 1991年 / 94卷 / 01期

关键词：

D O I：

10.1016/0019-1035(91)90143-H

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Analytic formulae for estimating planetary accretion rates have long been available for conditions where random motion of planetesimals controls velocities relative to a growing planet. Recent Monte Carlo studies have explored a wider range of conditions, but gave impact rates only for the specific conditions under which those numerical experiments were performed. Now analytical formulae, which are valid even when keplerian shear controls the approach velocity, and which accurately reproduce the Monte Carlo results, give accretion rates over a wide range of conditions relevant to the problem of planet formation. © 1991.

引用

页码：98 / 111

页数：14

共 26 条

[1]

BURNS JA, 1989, CASSINI MISSION ANNO, V13

[2]

Danby J, 1988, FUNDAMENTALS CELESTI

[3] THE DYNAMICS OF TADPOLE AND HORSESHOE ORBITS .1. THEORY [J].