Abstract
The main goal of this paper is to show that the elliptic restricted three-body problem has ejection-collision orbits when the mass parameter μ is small enough. We make use of the 'blow up' techniques. Moreover, we describe the global flow of the elliptic problem when μ = 0 taking into account the singularities due to collision and to infinity. © 1990 Kluwer Academic Publishers.
Original language | English |
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Pages (from-to) | 319-345 |
Journal | Celestial Mechanics and Dynamical Astronomy |
Volume | 48 |
DOIs | |
Publication status | Published - 1 Dec 1990 |