✦ LIBER ✦

The rectilinear restricted problem of three bodies

✍ Scribed by Joerg Waldvogel

Publisher: Springer Netherlands
Year: 1973
Tongue: English
Weight: 705 KB
Volume: 8
Category: Article
ISSN: 1572-9478
DOI: 10.1007/bf01231413

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Stability of the periodic solutions of t

Stability of the periodic solutions of the restricted three-body problem representing analytic continuations of Keplerian rectilinear periodic motions

✍ Abdul Ahmad 📂 Article 📅 1995 🏛 Springer Netherlands 🌐 English ⚖ 478 KB

The periodic solutions of the restricted three-body problem representing analytic continuations of Keplerian rectilinear periodic motions are well known (Kurcheeva, 1973). Here the stability of these solutions are examined by applying Poincar6's characteristic equation for periodic solutions. It is

Numerical explorations of the rectilinea

Numerical explorations of the rectilinear problem of three bodies

✍ R. Broucke; D. E. Walker 📂 Article 📅 1980 🏛 Springer Netherlands 🌐 English ⚖ 326 KB

The invariance of the restricted problem

The invariance of the restricted problem of three bodies

✍ D. J. Jezewski 📂 Article 📅 1985 🏛 Springer Netherlands 🌐 English ⚖ 441 KB

The photogravitational restricted three-

The photogravitational restricted three-body problem

✍ Ioan Todoran 📂 Article 📅 1994 🏛 Springer Netherlands 🌐 English ⚖ 306 KB

Set-theoretical aspects of the restricte

Set-theoretical aspects of the restricted problem of three bodies

✍ Rudolf Kurth 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 516 KB

Integration theory for the restricted pr

Integration theory for the restricted problem of three axisymmetric bodies

✍ S. M. El-Shaboury 📂 Article 📅 1990 🏛 Springer Netherlands 🌐 English ⚖ 332 KB

In this paper the circular planar restricted problem of three axisymmetric ellipsoids S,(i = 1,2,3), such that their equatorial planes coincide with the orbital plane of the three centres of masses. be considered. The equations of motion of infinitesimal body Sa be obtained in the polar coordmates.