| Display title | Eccentricity vector |
| Default sort key | Eccentricity Vector |
| Page length (in bytes) | 2,243 |
| Namespace ID | 0 |
| Page ID | 180779 |
| Page content language | en - English |
| Page content model | wikitext |
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| Counted as a content page | Yes |
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| Page creator | imported>Sherlock |
| Date of page creation | 16:21, 6 February 2024 |
| Latest editor | imported>Sherlock |
| Date of latest edit | 16:21, 6 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In celestial mechanics, the eccentricity vector of a Kepler orbit is the dimensionless vector with direction pointing from apoapsis to periapsis and with magnitude equal to the orbit's scalar eccentricity. For Kepler orbits the eccentricity vector is a constant of motion. Its main use is in the analysis... |
