THE THREE PRINCIPAL SECULAR RESONANCES v(5), v(6), and v(16) IN THE ASTEROIDAL BELT

被引:27
作者
Froeschle, Ch. [1 ]
Scholl, H. [1 ]
机构
[1] Observ Nice, F-06003 Nice, France
关键词
D O I
10.1007/BF00049260
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We review theoretical and numerical results obtained for secular resonant motion in the asteroidal belt. William's theory (1969) yields the locations of the principal secular resonances v(5), v(6), and v(16) in the asteroidal belt. Theories by Nakai and Kinoshita (1985) and by Yoshikawa (1987) allow us to model the basic features of orbital evolution at the secular resonances v(16) and v(6), respectively. No theory is available for the secular resonance v(5). Numerical experiments by Froeschle and Scholl yield quantitative and new qualitative results for orbital evolutions at the three principal secular resonances v(5), v(6), and v(16). These experiments indicate possible chaotic motion due to overlapping resonances. A secular resonance may overlap with another secular resonance or with a mean motion resonance. The role of the secular resonances as possible sources of meteorites is discussed.
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页码:231 / 251
页数:21
相关论文
共 36 条
  • [1] TROJAN ORBITS IN SECULAR RESONANCES
    BIEN, R
    SCHUBART, J
    [J]. CELESTIAL MECHANICS, 1984, 34 (1-4): : 425 - 434
  • [2] Brouwer D., 1961, METHODS CELESTIAL ME
  • [3] BROUWER D, 1950, ASTRON PAP AM EPHEME, V13, P85
  • [4] CBARLIER CVL, 1902, MECH HIMMELS, P421
  • [5] CHARLIER CVL, 1900, B ASTRON, V17, P209
  • [6] UNIVERSAL INSTABILITY OF MANY-DIMENSIONAL OSCILLATOR SYSTEMS
    CHIRIKOV, BV
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1979, 52 (05): : 263 - 379
  • [7] FERRAZMELLO S, 1987, ASTRON ASTROPHYS, V179, P304
  • [8] FROESCHLE C, 1988, CELESTIAL MECH, V43, P113
  • [9] FROESCHLE C, 1987, ASTRON ASTROPHYS, V179, P294
  • [10] FROESCHLE C, 1986, ASTRON ASTROPHYS, V166, P326