Perturbations in close binary systems produced by the tides lagging in latitude (Q1097056)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Perturbations in close binary systems produced by the tides lagging in latitude |
scientific article; zbMATH DE number 4033169
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Perturbations in close binary systems produced by the tides lagging in latitude |
scientific article; zbMATH DE number 4033169 |
Statements
Perturbations in close binary systems produced by the tides lagging in latitude (English)
0 references
1987
0 references
The aim of this investigation is to present the periodic and secular perturbations of the orbital elements of close binary systems due to tidal lag in latitude. The variational equations of the problem of plane motion will be set up in terms of the rectangular components R, S, and W of the disturbing accelerations. These equations are highly nonlinear with respect to the orbital elements and we present analytic approximations to the effects produced by the perturbing acceleration due to dynamical tides lagging in latitude. The perturbed elements of the orbit have been expressed by means of Hansen coefficients in the compact form of summations.
0 references
secular perturbations
0 references
orbital elements of close binary systems
0 references
tidal lag
0 references
variational equations
0 references
analytic approximations
0 references
Hansen coefficients
0 references
0 references
0.9539118
0 references
0.8768084
0 references
0.8677318
0 references
0 references
0.86468667
0 references
0.86236954
0 references
0.85852504
0 references
0.85665315
0 references
0.8497329
0 references