We show that periodic close encounters between Neptune's arc particles and the nearby satellite Galatea lead to a usually neglected secular perturbation on the osculating longitude at epoch ( \(\varepsilon\) ). This perturbation changes the effective mean motion (i.e., the mean motion averaged over
Where are the rings of Neptune?
โ Scribed by Anthony R. Dobrovolskis
- Publisher
- Elsevier Science
- Year
- 1980
- Tongue
- English
- Weight
- 287 KB
- Volume
- 43
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
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