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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

### Цитирование

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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 -