CHAOTIC EVOLUTION OF THE SOLAR-SYSTEM

被引：218

作者：

SUSSMAN, GJ ^{[1
]}

WISDOM, J ^{[1
]}

机构：

[1] MIT,DEPT EARTH ATMOSPHER & PLANETARY SCI,CAMBRIDGE,MA 02139

来源：

SCIENCE | 1992年 / 257卷 / 5066期

关键词：

D O I：

10.1126/science.257.5066.56

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The evolution of the entire planetary system has been numerically integrated for a time span of nearly 100 million years. This calculation confirms that the evolution of the solar system as a whole is chaotic, with a time scale of exponential divergence of about 4 million years. Additional numerical experiments indicate that the Jovian planet subsystem is chaotic, although some small variations in the model can yield quasiperiodic motion. The motion of Pluto is independently and robustly chaotic.

引用

页码：56 / 62

页数：7

共 29 条

[1]

ABELSON H, UNPUB

[2]

[Anonymous], 1978, MATH METHODS CLASSIC, DOI [DOI 10.1007/978-1-4757-1693-1, 10.1007/978-1-4757-1693-1]

[3]

APPLEGATE J, 1985, IEEE T COMPUT C, V34

[4] THE OUTER SOLAR-SYSTEM FOR 200 MILLION YEARS [J].

APPLEGATE, JH ;

DOUGLAS, MR ;

GURSEL, Y ;

SUSSMAN, GJ ;

WISDOM, J .

ASTRONOMICAL JOURNAL, 1986, 92 (01) :176-194

[5]

Cohen C. J., 1973, ASTR PAP AM EPHEMERI, VXXII, P1

[6] THE REDUCING TRANSFORMATION AND APOCENTRIC LIBRATORS [J].

HENRARD, J ;

LEMAITRE, A ;

MILANI, A ;

MURRAY, CD .

CELESTIAL MECHANICS, 1986, 38 (04) :335-344

[7] MOTIONS OF THE PERIHELIONS OF NEPTUNE AND PLUTO [J].

Kinoshita, H ;

Nakai, H .

CELESTIAL MECHANICS, 1984, 34 (1-4) :203-217

[8] A NUMERICAL EXPERIMENT ON THE CHAOTIC BEHAVIOR OF THE SOLAR-SYSTEM [J].

LASKAR, J .

NATURE, 1989, 338 (6212) :237-238

[9] THE CHAOTIC MOTION OF THE SOLAR-SYSTEM - A NUMERICAL ESTIMATE OF THE SIZE OF THE CHAOTIC ZONES [J].

LASKAR, J .

ICARUS, 1990, 88 (02) :266-291

[10] CONFIRMATION OF RESONANT STRUCTURE IN THE SOLAR-SYSTEM [J].

LASKAR, J ;

QUINN, T ;

TREMAINE, S .

ICARUS, 1992, 95 (01) :148-152

← 1 2 3 →