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Collisions of stars by oscillating orbits of the second kind - MaRDI portal

Collisions of stars by oscillating orbits of the second kind

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Publication:4178538

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DOI10.1016/0094-5765(78)90066-8zbMath0395.70008OpenAlexW1999421217MaRDI QIDQ4178538

Christian Marchal

Publication date: 1978

Published in: Acta Astronautica (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0094-5765(78)90066-8

zbMATH Keywords

Delaunay Variables Three-Body Problem Oscillating Orbits Star Collisions Von Zeipel Transformation

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Collision of rigid or pseudo-rigid bodies (70F35)

Related Items (3)

Quasi‐Periodic Almost‐Collision Orbits in the Spatial Three‐Body Problem ⋮ Normalization through invariants in \(n\)-dimensional Kepler problems ⋮ A dynamic extremum seeking scheme for three-player attack-defense with unknown gradient

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