A third giant planet orbiting HIP 14810

J. T. Wright, D. A. Fischer, Eric B. Ford, D. Veras, J. Wang, G. W. Henry, G. W. Marcy, A. W. Howard, John Asher Johnson

Research output: Contribution to journalArticlepeer-review

21 Scopus citations


We present new precision radial velocities and a three-planet Keplerian orbit fit for the V = 8.5, G5 V star HIP 14810. We began observing this star at Keck Observatory as part of the N2K Planet Search Project. Wright etal. announced the inner two planets to this system, and subsequent observations have revealed the outer planet and the proper orbital solution for the middle planet. The planets have minimum masses of 3.9, 1.3, and 0.6 M Jup and orbital periods of 6.67, 147.7, and 952 day, respectively. We have numerically integrated the family of orbital solutions consistent with the data and find that they are stable for at least 106 yr. Our photometric search shows that the inner planet does not transit.

Original languageEnglish (US)
Pages (from-to)L97-L101
JournalAstrophysical Journal
Issue number2 PART 2
StatePublished - 2009

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'A third giant planet orbiting HIP 14810'. Together they form a unique fingerprint.

Cite this