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The motion of asteroids at the 5:2 resonance with Jupiter

Transactions of IAA RAS, issue 8, 75–76 (2002)

Keywords: Very Long Baseline Interferometry (VLBI), celestial mechanics, motion of asteroids, resonance

Abstract

The present work is devoted to investigation of Near-Earth asteroids (NEAs) motion at the 5:2 resonance with Jupiter. The motion of these objects has some peculiarities such as close approaches to the inner major planets and Jupiter, large eccentricities and so on. These features render the motion of many considered asteroids unstable

Citation

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T. Yu. Galushina. The motion of asteroids at the 5:2 resonance with Jupiter // Transactions of IAA RAS. — 2002. — Issue 8. — P. 75–76.

@article{galushina2002,
  abstract = {The present work is devoted to investigation of Near-Earth asteroids (NEAs) motion at the 5:2 resonance with Jupiter. The motion of these objects has some peculiarities such as close approaches to the inner major planets and Jupiter, large eccentricities and so on. These features render the motion of many considered asteroids unstable},
  author = {T.~Yu. Galushina},
  issue = {8},
  journal = {Transactions of IAA RAS},
  keyword = {Very Long Baseline Interferometry (VLBI), celestial mechanics, motion of asteroids, resonance},
  pages = {75--76},
  title = {The motion of asteroids at the 5:2 resonance with Jupiter},
  url = {http://iaaras.ru/en/library/paper/327/},
  year = {2002}
}

TY  - JOUR
TI  - The motion of asteroids at the 5:2 resonance with Jupiter
AU  - Galushina, T. Yu.
PY  - 2002
T2  - Transactions of IAA RAS
IS  - 8
SP  - 75
AB  - The present work is devoted to investigation of Near-Earth asteroids
(NEAs) motion at the 5:2 resonance with Jupiter. The motion of these
objects has some peculiarities such as close approaches to the inner
major planets and Jupiter, large eccentricities and so on. These
features render the motion of many considered asteroids unstable
UR  - http://iaaras.ru/en/library/paper/327/
ER  -