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
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.
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页码:98 / 111
页数:14
相关论文
共 26 条
[11]  
Hill G. W., 1978, AM J MATH, V1, P5, DOI DOI 10.2307/2369430
[12]  
HILL GW, 1878, AM J MATH, V1, P5, DOI DOI 10.2307/2369430
[13]  
Hill GW., 1878, AM J MATH, V1, P245, DOI [10.2307/2369313, DOI 10.2307/2369313]
[14]  
IDA S, 1989, ASTRON ASTROPHYS, V220, P293
[15]   COLLISIONAL PROCESSES OF PLANETESIMALS WITH A PROTOPLANET UNDER THE GRAVITY OF THE PROTO-SUN [J].
NISHIDA, S .
PROGRESS OF THEORETICAL PHYSICS, 1983, 70 (01) :93-105
[16]   RUNAWAY PLANETARY GROWTH WITH COLLISION RATE IN THE SOLAR GRAVITATIONAL-FIELD [J].
OHTSUKI, K ;
IDA, S .
ICARUS, 1990, 85 (02) :499-511
[17]  
Opik E.J., 1951, PRIAA, V54, P165
[18]   SATELLITE ENCOUNTERS [J].
PETIT, JM ;
HENON, M .
ICARUS, 1986, 66 (03) :536-555
[19]  
Roy A.E., 1988, ORBITAL MOTION, Vthird
[20]  
SAFRONOV VS, 1972, NASA TTF677