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Eccentric Jupiter

 
Wikipedia: Eccentric Jupiter
Eccentric Jupiter HD 96167 b has a comet like orbit.

An Eccentric Jupiter is a Jovian planet that orbits its star in a highly eccentric orbit,[citation needed] much like a comet. Eccentric Jupiters may disqualify a planetary system from having earth-like planets in it because a massive and highly eccentric gas giant may remove all earth mass planets from the habitable zone.

To date, it appears that approximately 7% of all stars (half of the known planetary systems) have an Eccentric Jupiter (e > 0.1), making these planets more common than Hot Jupiters.[citation needed]

One surprising result that has come out of the more than 200 extrasolar planet discoveries as of 2006 is that 15 planets have high eccentricities (e > 0.6).[1]

The typical exoplanet with an orbital period greater than 5 days has a median eccentricity of 0.23.[2]

Habitable zone planets near Eccentric Jupiters:[1]

Planet SMA ecc MJ Notes
HD 3651 b 0.29 0.61 0.22 Might allow for planets at or beyond 0.6 AU
HD 37605 b 0.26 0.73 2.84 Might allow for planets at or beyond 0.8 AU
HD 45350 b 1.92 0.77 1.79 restricted stable orbits to the innermost 0.2 AU
HD 80606 b 0.45 0.93 4.0 only beyond 1.75 AU did test particles remain
HD 89744 b 0.93 0.67 8.58 No planets in the habitable zone
16 Cygni Bb 1.68 0.68 1.68 No planets in the habitable zone

See also

References

  1. ^ a b Wittenmyer et al. (2007). "Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems". The Astronomical Journal 134 (3): 1276–1284. doi:10.1086/520880. http://www.iop.org/EJ/article/1538-3881/134/3/1276/205882.html. 
  2. ^ Kathryn; Fischer; Marcy; et al. (2009). Old, Rich, and Eccentric: Two Jovian Planets Orbiting Evolved Metal-Rich Stars. . Publications of the Astronomical Society of the Pacific 121 (880): 613–620. arΧiv:0904.2786. 

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