✦ LIBER ✦

A second-order Uranus-Neptune theory by Hori's method

✍ Scribed by Osman M. Kamel

Publisher: Springer Netherlands
Year: 1988
Tongue: English
Weight: 834 KB
Volume: 40
Category: Article
ISSN: 1573-0794
DOI: 10.1007/bf00056021

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Third-order Uranus-Neptune theory by Hor

Third-order Uranus-Neptune theory by Hori's method

✍ Osman M. Kamel 📂 Article 📅 1989 🏛 Springer Netherlands 🌐 English ⚖ 427 KB

We construct a U-N secular canonical planetary theory of the third order with respect to planetary masses. The Hori-Lie procedure is adopted to solve the problem. ## Expansions have been carried out by hand, neglecting powers higher than the second with respect to the eccentricityinclination. We

The elimination of the critical terms of

The elimination of the critical terms of a first order Uranus-Neptune theory by Hori's method

✍ Osman M. Kamel 📂 Article 📅 1983 🏛 Springer Netherlands 🌐 English ⚖ 1012 KB

The elimination of the critical terms of

The elimination of the critical terms of a first order Uranus-Neptune theory through Hori's method

✍ Osman M. Kamel 📂 Article 📅 1982 🏛 Springer Netherlands 🌐 English ⚖ 362 KB

On the elimination of the critical term

On the elimination of the critical term in a general first-order Uranus-Neptune theory

✍ Osman M. Kamel; Abdel A. Bakry 📂 Article 📅 1981 🏛 Springer Netherlands 🌐 English ⚖ 669 KB

The construction of a third order secula

The construction of a third order secular analytical J-S-U-N theory by Hori-Lie technique

✍ Abdel Aziz Bakry; Osman M. Kamel; Salwa M. Waziry 📂 Article 📅 1994 🏛 Springer Netherlands 🌐 English ⚖ 870 KB

The construction of a third order secula

The construction of a third order secular analytical J-S-U-N theory by Hori-Lie technique

✍ Osman M. Kamel 📂 Article 📅 1990 🏛 Springer Netherlands 🌐 English ⚖ 356 KB

We construct the outline of a third order secular theory for the four major planets. We apply the Hori-Lie technique to solve the problem. We take into consideration both parts of the perturbing function. Our canonical variables are those of H. Poincare. Our periodic terms arc the only 2 : 5 and 1: