Effects of gravitational interactions on asteroid spin states

被引:85
作者
Scheeres, DJ [1 ]
Ostro, SJ
Werner, RA
Asphaug, E
Hudson, RS
机构
[1] Univ Michigan, Dept Aerosp Engn, Ann Arbor, MI 48109 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Univ Calif Santa Cruz, Dept Earth Sci, Santa Cruz, CA 95064 USA
[4] Washington State Univ, Sch Elect Engn & Comp Sci, Pullman, WA 99164 USA
关键词
D O I
10.1006/icar.2000.6443
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We demonstrate that mutual gravitational interactions between an asteroid and a planet or another asteroid can play an important role in shaping an asteroid's spin state. We focus on two situations that asteroids may encounter during their lifetimes. The first is the environment after creation from a disrupted parent asteroid, when there may be many asteroid fragments interacting gravitationally with each other before their mutual escape. The other is the interaction between an asteroid and a planet during a hyperbolic flyby. In each case the mutual gravitational interaction can alter the asteroid's spin state. We derive analytical descriptions of the effects and perform numerical simulations to explore the interactions and to give examples, The net effect of many small interactions, taken in isolation, is to cause the asteroid to spin at a faster rate-although this must be balanced against all other effects that influence spin rates. Conversely, the effect of a single, strong interaction can fundamentally change an asteroid's spin state, causing it to tumble and significantly increasing or decreasing its overall angular momentum. We simulate interactions of a sphere of arbitrary mass with Toutatis and find that these types of gravitational interactions can provide partial explanations for the current Toutatis rotational state. (C) 2000 Academic Press.
引用
收藏
页码:106 / 118
页数:13
相关论文
共 21 条
[1]   Deconstructing Castalia: Evaluating a postimpact state [J].
Asphaug, E ;
Scheeres, DJ .
ICARUS, 1999, 139 (02) :383-386
[2]  
Binzel R.P., 1989, ASTEROIDS, VII, P416
[3]   On a possible rotation state of (433) Eros [J].
Black, GJ ;
Nicholson, PD ;
Bottke, WF ;
Burns, JA ;
Harris, AW .
ICARUS, 1999, 140 (01) :239-242
[4]  
BORDERIES N, 1990, ASTRON ASTROPHYS, V233, P235
[5]  
Brouwer D., 1961, METHODS CELESTIAL ME, P595
[6]   ASTEROID NUTATION ANGLES [J].
BURNS, JA ;
SAFRONOV, VS .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 165 (04) :403-411
[7]   ASTEROID COLLISIONAL EVOLUTION .1. ANGULAR-MOMENTUM SPLASH - DESPINNING ASTEROIDS THROUGH CATASTROPHIC COLLISIONS [J].
CELLINO, A ;
ZAPPALA, V ;
DAVIS, DR ;
FARINELLA, P ;
PAOLICCHI, P .
ICARUS, 1990, 87 (02) :391-402
[8]   PLANAR ORBITS ABOUT A TRIAXIAL BODY - APPLICATION TO ASTEROIDAL SATELLITES [J].
CHAUVINEAU, B ;
FARINELLA, P ;
MIGNARD, F .
ICARUS, 1993, 105 (02) :370-384
[9]   PLANAR NONDISSIPATIVE SPIN-ORBIT-COUPLING [J].
CHAUVINEAU, B ;
METRIS, G .
ICARUS, 1994, 109 (01) :191-203
[10]   ANGULAR-MOMENTUM DRAIN - A MECHANISM FOR DESPINNING ASTEROIDS [J].
DOBROVOLSKIS, AR ;
BURNS, JA .
ICARUS, 1984, 57 (03) :464-476