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

Труды ИПА РАН, вып. 8, 75–76 (2002)

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

Аннотация

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

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T. Yu. Galushina. The motion of asteroids at the 5:2 resonance with Jupiter // Труды ИПА РАН. — 2002. — Вып. 8. — С. 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 = {Труды ИПА РАН},
  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/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  - Труды ИПА РАН
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/library/paper/327/
ER  -