Tidal circularization

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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.

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References[edit]

  • 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.