University of Hertfordshire

From the same journal

From the same journal

By the same authors

A Neptune-mass Planet Orbiting the Nearby G Dwarf HD 16417

Research output: Contribution to journalArticle

  • S. O'Toole
  • C.G. Tinney
  • R.P. Butler
  • H.R.A. Jones
  • J. Bailey
  • B.D. Carter
  • S. Vogt
  • G. Laughlin
  • E. Rivera
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Original languageEnglish
Pages (from-to)1263-1268
JournalThe Astrophysical Journal
Volume697
Issue2
DOIs
Publication statusPublished - 2009

Abstract

Precision Doppler measurements from an intensive 48 night "Rocky Planet Search" observing campaign on the Anglo-Australian Telescope (AAT) have revealed the presence of a low-mass exoplanet orbiting the G1 dwarf HD 16417. Subsequent Doppler observations with the AAT, as well as independent observations obtained by the Keck Planet Search, have confirmed this initial detection and refine the orbital parameters to period 17.24 ± 0.01 d, eccentricity 0.20 ± 0.09, orbital semimajor axis 0.14 ± 0.01 AU, and minimum planet mass 22.1 ± 2.0 M Earth. HD 16417 raises the number of published exoplanets with minimum masses of less than 25 M Earth to 18. Interestingly, the distribution of detected sub-25 M Earth planets over the spectral types G, K, and M is almost uniform. The detection of HD 16417b by an intensive observing campaign clearly demonstrates the need for extended and contiguous observing campaigns when aiming to detect low-amplitude Doppler planets in short-period orbits. Perhaps most critically it demonstrates that the search for low-mass Doppler planets will eventually require these traditional "bright-time" projects to extend throughout dark lunations.

Notes

Original article can be found at: http://www.iop.org/EJ/journal/1538-3881 Copyright IOP Publishing / American Astronomical Society. DOI: 10.1088/0004-637X/697/2/1263 [Full text of this article is not available in the UHRA]

ID: 166409