HIP 14810 b: Difference between revisions
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Revision as of 05:02, 18 October 2008
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HIP 14810 b is a massive hot Jupiter approximately 172 light-years away in the constellation of Aries. It has mass 3.84 times that of Jupiter and orbits at 0.0692 AU. HIP 14810 is a metal-rich ([Fe/H] = 0.23) G5 V, V=8.5 star which we have observed at Keck Observatory as part of the N2K program (Fischer et al. 2005) since Nov 2005.
References
- Wright J. T. (2006). "Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars". The Astrophysical Journal. 3. Retrieved 2008-08-16.
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- "Four New Exoplanets, and Hints of Additional Substellar Companions to Exoplanet Host Stars" (PDF). http://arxiv.org/.
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External links
- "Notes for planet HIP 14810 b". The Extrasolar Planets Encyclopaedia. Retrieved 2008-08-16.
- "HIP 14810". Exoplanets. Retrieved 2008-08-16.
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