Tidal circularization
Tidal circularization is an effect of the tidal forces between an orbiting body, and the primary object that it orbits whereby the eccentricity of the orbit is reduced over time so that the orbit becomes less elliptical and more circular.
See also
References
- William I. Hartkopf; Edward F. Guinan; Petr Harmanec (2007). Binary Stars as Critical Tools and Tests in Contemporary Astrophysics. Cambridge University Press. ISBN 978-0-521-86348-3.
- Yi-Sui Sun; Sylvio Ferraz-Mello; Ji-Lin Zhou (2008). Exoplanets: Detection, Formation and Dynamics. Cambridge University Press. ISBN 978-0-521-87471-7.
- SJ Peale (1999). Origin and evolution of the natural satellites. Annual Review of Astronomy and Astrophysics.
This article is issued from Wikipedia - version of the Monday, May 25, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.