Abstract
Periodic orbits of the first kind of the planar circular restricted three-body problem are linearly stable except in the neighbourhood of second order resonances, where an interval of unstable orbits appears when the mass parameter is not zero. Our main result is the estimation of the length of the instability interval. © 1994 Birkhäuser Verlag.
Original language | English |
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Pages (from-to) | 956-977 |
Journal | ZAMP Zeitschrift für angewandte Mathematik und Physik |
Volume | 45 |
DOIs | |
Publication status | Published - 1 Nov 1994 |