The construction of a third order J-S theory is presented. The Hori theory of planetary perturbations is employed. No Critical J-S terms due to the 2:5 commensurabilities and its multiples exist, when we take into account the periodic terms of order 0, 1, 2 with respect to the eccentricityinclinatio
โฆ LIBER โฆ
A third-order intermediate orbit for planetary theory
โ Scribed by David L. Richardson
- Publisher
- Springer Netherlands
- Year
- 1982
- Tongue
- English
- Weight
- 336 KB
- Volume
- 26
- Category
- Article
- ISSN
- 1572-9478
No coin nor oath required. For personal study only.
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