NUMERICAL EVIDENCE THAT THE MOTION OF PLUTO IS CHAOTIC

[1] THE OUTER SOLAR-SYSTEM FOR 200 MILLION YEARS [J]. ASTRONOMICAL JOURNAL, 1986, 92 (01) : 176 - 194

[2] APPLEGATE JH, 1985, IEEE T COMPUT, V34, P822, DOI 10.1109/TC.1985.1676638

[3] Arnol'd V.I., 1963, USPEHI MAT NAUK, V18, P85, DOI [10.1070/RM1963v018n06ABEH001143, DOI 10.1070/RM1963V018N06ABEH001143]

[4] BENETTIN G, 1980, MECCANICA MAR, P21

[5] UNIVERSAL INSTABILITY OF MANY-DIMENSIONAL OSCILLATOR SYSTEMS [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1979, 52 (05): : 263 - 379

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

[7] LIBRATION OF CLOSE APPROACHES OF PLUTO TO NEPTUNE [J]. ASTRONOMICAL JOURNAL, 1965, 70 (01) : 10 - &

[8] COWELL PH, 1910, GREENWICH OBSERVATIO

[9] MOTIONS OF THE PERIHELIONS OF NEPTUNE AND PLUTO [J]. CELESTIAL MECHANICS, 1984, 34 (1-4): : 203 - 217

[10] NOBILI A, 1987, FEW BODY PROBLEM, P147

[1] THE OUTER SOLAR-SYSTEM FOR 200 MILLION YEARS [J]. ASTRONOMICAL JOURNAL, 1986, 92 (01) : 176 - 194

[2] APPLEGATE JH, 1985, IEEE T COMPUT, V34, P822, DOI 10.1109/TC.1985.1676638

[3] Arnol'd V.I., 1963, USPEHI MAT NAUK, V18, P85, DOI [10.1070/RM1963v018n06ABEH001143, DOI 10.1070/RM1963V018N06ABEH001143]

[4] BENETTIN G, 1980, MECCANICA MAR, P21

[5] UNIVERSAL INSTABILITY OF MANY-DIMENSIONAL OSCILLATOR SYSTEMS [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1979, 52 (05): : 263 - 379

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

[7] LIBRATION OF CLOSE APPROACHES OF PLUTO TO NEPTUNE [J]. ASTRONOMICAL JOURNAL, 1965, 70 (01) : 10 - &

[8] COWELL PH, 1910, GREENWICH OBSERVATIO

[9] MOTIONS OF THE PERIHELIONS OF NEPTUNE AND PLUTO [J]. CELESTIAL MECHANICS, 1984, 34 (1-4): : 203 - 217

[10] NOBILI A, 1987, FEW BODY PROBLEM, P147