A new approach to calculation of secular frequencies in the dynamics of near-Earth object in orbits with large eccentricities | Izvestiya vuzov. Fizika. 2020. № 1. DOI: 10.17223/00213411/63/1/57

A new approach to calculation of secular frequencies in the dynamics of near-Earth object in orbits with large eccentricities

A modified method for identifying and studying secular resonances in the dynamics of near-Earth objects is described. Unlike the traditionally used approach, based on approximate analytical formulas for calculating secular frequencies that are valid only for small eccentricities, the proposed method uses exact values obtained in the process of numerical simulation of motion from the Newton-Euler equations. This technique can be used in the analysis of the dynamics of objects with any eccentricities of the orbits, but its application to the study of motion along orbits with large or rapidly growing eccentricities is most interesting. This fact is clearly demonstrated by the above examples.

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Keywords

численное моделирование, околоземные объекты, вековые резонансы, уточненная методика исследования, результаты применения, numerical modeling, near-Earth objects, secular resonances, refined research technique, application results

Authors

NameOrganizationE-mail
Aleksandrova A.G.National Research Tomsk State Universityaleksann@sibmail.com
Bordovitsyna T.V.National Research Tomsk State Universitytvbord@sibmail.com
Popandopulo N.A.National Research Tomsk State Universitynikas.popandopulos@gmail.com
Tomilova I.V.National Research Tomsk State Universityirisha_tom@mail.ru
Всего: 4

References

Breiter S. // Celest. Mech. Dyn. Astr. - 2001. - V. 80. - P. 1-20.
Breiter S. // Celest. Mech. Dyn. Astr. - 2001. - V. 81. - P. 81-91.
Rosengren A.J. et al. // MNRAS. - 2015. - V. 449. - Iss. 4. - P. 3522-3526.
Daquin J. et al. // Celest Mech. Dyn Astr. - 2016. - Publ. online 02 January 2016.
Rossi A. // Celest. Mech. Dyn. Astr. - 2008. - V. 100. - P. 267-28.
Бордовицына Т.В., Томилова И.В. // Изв. вузов. Физика. - 2016. - T. 59. - № 3. - С. 41-48.
Бордовицына Т.В., Авдюшев В.А. Теория движения искусственных спутников Земли. Аналитические и численные методы. - Томск: Изд-во Том. ун-та, 2007. - 220 с.
Бордовицына Т.В., Томилова И.В. // Изв. вузов. Физика. - 2014. - T. 57. - № 4. - С. 84-91.
Александрова А.Г., Бордовицына Т.В., Томилова И.В. // Астрон. вестн. - 2018. - Т. 52. -№ 5. - С. 447-462.
Александрова А.Г., Бордовицына Т.В., Александров В.Б. // Изв. вузов. Физика. - 2019. - Т. 62. - № 3. - С. 86-91.
Александрова А.Г., Бордовицына Т.В, Чувашов И.Н. // Изв. вузов. Физика. - 2017. - Т. 60. - № 1. - C. 69-76.
Мюррей К., Дермотт С. Динамика Солнечной системы. - М.: Физматлит, 2009. - 588 с.
Morbidelli A. Modern Celestial Mechanics: Aspects of Solar System Dynamics. - London: Taylor & Francis, 2002. - 380 p.
Томилова И.В., Блинкова Е.В., Бордовицына Т.В. // Астрон. вест. - 2019. - Т. 53. - № 5. - С. 323-338.
Лидов М.Л. // Искусственные спутники Земли. - 1961. - Т. 8. - С. 5-45.
Kozai Y. // Astron. J. - 1962. - V. 67. - P. 591-598.
Shevchenko I.I. The Lidov - Kozai Effect - Applications in Exoplenet Research and Denamical Astronomy. - Springer, 2017. - 194 р.
 A new approach to calculation of secular frequencies in the dynamics of near-Earth object in orbits with large eccentricities | Izvestiya vuzov. Fizika. 2020. № 1. DOI: 10.17223/00213411/63/1/57

A new approach to calculation of secular frequencies in the dynamics of near-Earth object in orbits with large eccentricities | Izvestiya vuzov. Fizika. 2020. № 1. DOI: 10.17223/00213411/63/1/57