Placing Venus in an orbit similar to that of the Earth. I: Perturbations after alteration in a third-order theory (Q1312117)
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: Placing Venus in an orbit similar to that of the Earth. I: Perturbations after alteration in a third-order theory |
scientific article; zbMATH DE number 488192
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Placing Venus in an orbit similar to that of the Earth. I: Perturbations after alteration in a third-order theory |
scientific article; zbMATH DE number 488192 |
Statements
Placing Venus in an orbit similar to that of the Earth. I: Perturbations after alteration in a third-order theory (English)
0 references
6 April 1994
0 references
We introduce the physical and dynamical considerations for producing a second Earth-like planet on which life sustaining conditions may exist, and hence we acquire multiplication of the cosmic resources of the human race. We investigate the perturbations in our solar system after alteration through a third order Hamiltonian planetary theory for the eight principal planets. The Hori-Lie theorem, the Jacobi-Radau coordinates, and the canonical variables of H. Poincaré are adopted.
0 references
third order Hamiltonian planetary theory
0 references
Hori-Lie theorem
0 references
Jacobi-Radau coordinates
0 references
canonical variables
0 references
0 references
0.7324904203414917
0 references
0.7229806780815125
0 references
0.7129970788955688
0 references
0.7111350893974304
0 references
0.6992129683494568
0 references