Leges Keplerianae? sive leges Kepleranae ab Ioanne Keplero astronomo et philosopho naturae nomen trahunt, qui has leges fundamentales, quibus orbitae planetarum circa solem reguntur, statuit.
Illae formam viae, motum viae, et relationem inter periodum orbitalem ac magnitudinem viae tractant.
Prima lex Keplerana:
Ubi semi-latus rectum, ε eccentricitas ellipsis et r distantia ex solo ad planetam in systemate polari coordinatarum sunt.
Secunda lex Keplerana:
Tertia lex Keplerana:
Sunt autem multa sidera quorum motus variis causis ab his legibus aberrant, ut puta cometes, quorum multi orbitas parabolicas habent.
Vicimedia Communia plura habent quae ad motus Kepleranos spectant. |
This article uses material from the Wikipedia Latina article Leges Keplerianae, which is released under the Creative Commons Attribution-ShareAlike 3.0 license ("CC BY-SA 3.0"); additional terms may apply (view authors). Textus sub CC BY-SA 4.0 praebetur nisi aliter indicatus. Images, videos and audio are available under their respective licenses.
®Wikipedia is a registered trademark of the Wiki Foundation, Inc. Wiki Latina (DUHOCTRUNGQUOC.VN) is an independent company and has no affiliation with Wiki Foundation.