Standard

Planetary dynamics in the α Centauri system : Lyapunov spectra and long-term behaviour. / Popova, E. A.; Shevchenko, I. I.

From Interacting Binaries to Exoplanets: Essential Modeling Tools. ред. / Mercedes Richards; Ivan Hubeny. S282. ред. 2011. стр. 450-451 (Proceedings of the International Astronomical Union; Том 7, № S282).

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › Рецензирование

Harvard

Popova, EA & Shevchenko, II 2011, Planetary dynamics in the α Centauri system: Lyapunov spectra and long-term behaviour. в M Richards & I Hubeny (ред.), From Interacting Binaries to Exoplanets: Essential Modeling Tools. S282 изд., Proceedings of the International Astronomical Union, № S282, Том. 7, стр. 450-451. https://doi.org/10.1017/S1743921311028031

APA

Popova, E. A., & Shevchenko, I. I. (2011). Planetary dynamics in the α Centauri system: Lyapunov spectra and long-term behaviour. в M. Richards, & I. Hubeny (Ред.), From Interacting Binaries to Exoplanets: Essential Modeling Tools (S282 ред., стр. 450-451). (Proceedings of the International Astronomical Union; Том 7, № S282). https://doi.org/10.1017/S1743921311028031

Vancouver

Popova EA, Shevchenko II. Planetary dynamics in the α Centauri system: Lyapunov spectra and long-term behaviour. в Richards M, Hubeny I, Редакторы, From Interacting Binaries to Exoplanets: Essential Modeling Tools. S282 ред. 2011. стр. 450-451. (Proceedings of the International Astronomical Union; S282). https://doi.org/10.1017/S1743921311028031

Author

Popova, E. A. ; Shevchenko, I. I. / Planetary dynamics in the α Centauri system : Lyapunov spectra and long-term behaviour. From Interacting Binaries to Exoplanets: Essential Modeling Tools. Редактор / Mercedes Richards ; Ivan Hubeny. S282. ред. 2011. стр. 450-451 (Proceedings of the International Astronomical Union; S282).

BibTeX

@inproceedings{092d8ac525b44ab4bb7803430ce63565,
title = "Planetary dynamics in the α Centauri system: Lyapunov spectra and long-term behaviour",
abstract = "The stability of planetary motion in the binary system α Cen A-B is studied. Lyapunov spectra of the motion of the system with a single massive planet are computed on a fine grid of the initial data, and, by means of statistical analysis of the obtained data arrays, chaotic domains are identified in the pericentric distance - eccentricity initial data space for the planetary orbit. Association with the initial data domains for the orbits exhibiting close encounters with central stars and for the orbits exhibiting long-term escape is investigated.",
keywords = "Celestial mechanics, methods: numerical, planetary systems",
author = "Popova, {E. A.} and Shevchenko, {I. I.}",
year = "2011",
month = jul,
day = "1",
doi = "10.1017/S1743921311028031",
language = "English",
isbn = "9781107019829",
series = "Proceedings of the International Astronomical Union",
number = "S282",
pages = "450--451",
editor = "Mercedes Richards and Ivan Hubeny",
booktitle = "From Interacting Binaries to Exoplanets",
edition = "S282",

}

RIS

TY - GEN

T1 - Planetary dynamics in the α Centauri system

T2 - Lyapunov spectra and long-term behaviour

AU - Popova, E. A.

AU - Shevchenko, I. I.

PY - 2011/7/1

Y1 - 2011/7/1

N2 - The stability of planetary motion in the binary system α Cen A-B is studied. Lyapunov spectra of the motion of the system with a single massive planet are computed on a fine grid of the initial data, and, by means of statistical analysis of the obtained data arrays, chaotic domains are identified in the pericentric distance - eccentricity initial data space for the planetary orbit. Association with the initial data domains for the orbits exhibiting close encounters with central stars and for the orbits exhibiting long-term escape is investigated.

AB - The stability of planetary motion in the binary system α Cen A-B is studied. Lyapunov spectra of the motion of the system with a single massive planet are computed on a fine grid of the initial data, and, by means of statistical analysis of the obtained data arrays, chaotic domains are identified in the pericentric distance - eccentricity initial data space for the planetary orbit. Association with the initial data domains for the orbits exhibiting close encounters with central stars and for the orbits exhibiting long-term escape is investigated.

KW - Celestial mechanics

KW - methods: numerical

KW - planetary systems

UR - http://www.scopus.com/inward/record.url?scp=84887339772&partnerID=8YFLogxK

U2 - 10.1017/S1743921311028031

DO - 10.1017/S1743921311028031

M3 - Conference contribution

AN - SCOPUS:84887339772

SN - 9781107019829

T3 - Proceedings of the International Astronomical Union

SP - 450

EP - 451

BT - From Interacting Binaries to Exoplanets

A2 - Richards, Mercedes

A2 - Hubeny, Ivan

ER -

ID: 45987846