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词条 Eccentric Jupiter
释义

  1. See also

  2. References

An eccentric Jupiter is a Jovian planet that orbits its star in an eccentric orbit.[1] Eccentric Jupiters may probably disqualify a planetary system from having Earth-like planets (not habitable exomoons) in it because a massive gas giant with an eccentric orbit 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|date=April 2008}}

Out of the more than 200 extrasolar planet discoveries (as of 2006), 15 planets have high eccentricities (e > 0.6).[2]

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

Possible habitable zone planets near eccentric Jupiters:[3]

Planet SMA ecc MJ Notes
HD 3651 b0.290.610.22Might allow for planets at or beyond 0.6 AU
HD 37605 b0.260.732.84Might allow for planets at or beyond 0.8 AU
HD 45350 b1.920.771.79Restricted stable orbits to the innermost 0.2 AU
HD 80606 b0.450.934.0Only beyond 1.75 AU did test particles remain
HD 20782 b1.3810.972.620
HD 89744 b0.930.678.58No terrestrial planets in the habitable zone
16 Cygni Bb1.680.681.68No terrestrial planets in the habitable zone

See also

  • Exoplanet

References

1. ^{{cite journal |author1=Raymond, Sean N. |author2=Quinn, Thomas |author3=Lunine, Jonathan I. | title=Making other earths: dynamical simulations of terrestrial planet formation and water delivery | journal=Icarus | volume=168 | issue=1 | pages=1–17 |date=March 2004 | doi=10.1016/j.icarus.2003.11.019 | bibcode=2004Icar..168....1R |arxiv = astro-ph/0308159 }} Note: this study treats eccentric Jupiters as giant planets having an orbital eccentricity of 0.1 or greater.
2. ^{{cite journal | author=Kathryn; Fischer; Marcy | title=Old, Rich, and Eccentric: Two Jovian Planets Orbiting Evolved Metal-Rich Stars | journal=Publications of the Astronomical Society of the Pacific | year=2009 | volume=121 | issue=880 | pages=613–620 | id= | arxiv=0904.2786|bibcode = 2009PASP..121..613P |doi = 10.1086/599862 |display-authors=etal}}
3. ^{{cite journal | url=http://www.iop.org/EJ/article/1538-3881/134/3/1276/205882.html | author=Wittenmyer | year=2007 | title=Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems | journal=The Astronomical Journal | volume=134 | issue=3 | pages=1276–1284 | doi=10.1086/520880 | last2=Endl | first2=Michael | last3=Cochran | first3=William D. | last4=Levison | first4=Harold F. | bibcode=2007AJ....134.1276W|arxiv = 0706.1962 }}
{{exoplanet}}

2 : Types of planet|Giant planets

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