TRIAXIALITY OF HALLEY COMET

被引:1
作者
BURSA, M
KOPAL, Z
VANYSEK, V
机构
[1] UNIV MANCHESTER,INST ASTRON,MANCHESTER M13 9PL,LANCS,ENGLAND
[2] CHARLES UNIV,DEPT ASTRON & ASTROPHYS,CS-11636 PRAGUE 1,CZECHOSLOVAKIA
来源
EARTH MOON AND PLANETS | 1992年 / 57卷 / 01期
关键词
D O I
10.1007/BF00115414
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
There are many aspects of observational evidence that cometary nuclei have irregular or nonspherical shape. Tbe triaxial figure of the Halley's Comet nucleus is a well known fact. Therefore, the nucleus shape plays a significant role in consideration of the formation and evolution of comets and several attempts have been made to explain their nonsphericity. These studies were mainly based on the random-walk schemes for the aggregation processes. Although some results indeed lead to irregularities and deviation from sphericity, the spherical or irregular shape seem to be prevailing results. On the other hand the triaxial figure can be formed by the tidal and rotational forces. Thus, the assumption that the shape of the cometary nucleus due to some of these effects is in principle acceptable. In here assumed scenario already evolved cometary nucleus is situated as a satellite in the gravitation field of a planetary-like body. Since the rigidity of the nucleus is low, it may be easily transferred in the state of a synchronous satellite and in its shape could be imprinted the dynamical effects from this epoch. Here presented results indicate, that such a possibility should be seriously considered. The theory of this process is applied to the nucleus of comet Halley. It is shown, that the nucleus might be synchronously orbiting around a planetary-like hypothetical body with a period of 0.7 days. The minimal bulk tensile strength of the cometary material of about 10(2) N m-2 is estimated.
引用
收藏
页码:65 / 73
页数:9
相关论文
共 16 条
[1]   ROCHE LIMIT OF A SOLID BODY [J].
AGGARWAL, HR ;
OBERBECK, VR .
ASTROPHYSICAL JOURNAL, 1974, 191 (02) :577-588
[2]  
BELTON MJS, 1991, COMETS POST HALLEY E, V2, P691
[3]   TIDAL DISRUPTION OF INVISCID PLANETESIMALS [J].
BOSS, AP ;
CAMERON, AGW ;
BENZ, W .
ICARUS, 1991, 92 (01) :165-178
[4]   THE ACCRETION OF COSMIC DUST - A COMPUTER-SIMULATION [J].
DANIELS, PA ;
HUGHES, DW .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 195 (03) :1001-1009
[5]   TIDAL DISRUPTION OF SOLID BODIES [J].
DOBROVOLSKIS, AR .
ICARUS, 1990, 88 (01) :24-38
[6]  
DONN B, 1991, COMETS POST HALLEY E, V2, P335
[7]  
DONN B, 1986, ESA SP, V250, P523
[8]  
Hughes D.W., 1991, COMETS POSTHALLEY ER, Vsecond, P825
[9]   OPTICAL-PROPERTIES OF COMETARY NUCLEI AND A PRELIMINARY COMPARISON WITH ASTEROIDS [J].
JEWITT, DC ;
MEECH, KJ .
ASTROPHYSICAL JOURNAL, 1988, 328 (02) :974-&
[10]  
KELLER HU, 1987, ESA SP, V278, P447