MOTION OF THE PERIHELION OF TROJAN ASTEROIDS

被引：17

作者：

ERDI, B

机构：

[1] Department of Astronomy, Eotvos University, Budapest

来源：

CELESTIAL MECHANICS | 1979年 / 20卷 / 01期

关键词：

D O I：

10.1007/BF01236608

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The problem is investigated by using the equations of Jupiter's main perturbations in the eccentricity and in the perihelion longitude of Trojan asteroids. The limits and the period of the variation of the eccentricity and of the perihelion longitude are calculated for 30 Trojans. The perihelion is shown to circulate in 20 cases and to librate for 10 asteroids. © 1979 D. Reidel Publishing Co.

引用

页码：59 / 67

页数：9

共 7 条

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[2]

CHEBOTAREV GA, 1974, STABILITY SOLAR SYST, P63

[3] 3-DIMENSIONAL MOTION OF TROJAN ASTEROIDS [J].

ERDI, B .

CELESTIAL MECHANICS, 1978, 18 (02) :141-161

[4] ASYMPTOTIC SOLUTION FOR TROJAN CASE OF PLANE ELLIPTIC RESTRICTED PROBLEM OF 3 BODIES [J].

ERDI, B .

CELESTIAL MECHANICS, 1977, 15 (03) :367-383

[5]

HERTZ HG, 1943, ASTRON J, V50, P121

[6]

Kevorkian J., 1970, Periodic orbits, stability and resonances, P286

[7]

VANHOUTEN CJ, 1970, ASTRON ASTROPHYS SUP, V2, P339

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