THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE ORBIT OF THE YOUNG EXOPLANET beta PICTORIS b: THE ORBIT OF THE YOUNG EXOPLANET beta PICTORIS b

Eric L. Nielsen*, Michael C. Liu, Zahed Wahhaj, Beth A. Biller, Thomas L. Hayward, Jared R. Males, Laird M. Close, Katie M. Morzinski, Andrew J. Skemer, Marc J. Kuchner, Timothy J. Rodigas, Philip M. Hinz, Mark Chun, Christ Ftaclas, Douglas W. Toomey

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

We present new astrometry for the young (12-21 Myr) exoplanet beta Pictoris b taken with the Gemini/NICI and Magellan/MagAO instruments between 2009 and 2012. The high dynamic range of our observations allows us to measure the relative position of beta Pic b with respect to its primary star with greater accuracy than previous observations. Based on a Markov Chain Monte Carlo analysis, we find the planet has an orbital semi-major axis of 9.1(-0.5)(+5.3) AU and orbital eccentricity

Original languageEnglish
Article number158
Number of pages9
JournalAstrophysical Journal
Volume794
Issue number2
DOIs
Publication statusPublished - 20 Oct 2014

Keywords / Materials (for Non-textual outputs)

  • planetary systems
  • planet-disk interactions
  • planets and satellites: detection
  • stars: individual (beta Pic)
  • DEBRIS DISK
  • EXTRASOLAR PLANETS
  • GIANT PLANET
  • MOVING GROUP
  • ECCENTRICITY DISTRIBUTION
  • NEAR-IR
  • STARS
  • DISCOVERY
  • FREQUENCY
  • COMPANION

Fingerprint

Dive into the research topics of 'THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE ORBIT OF THE YOUNG EXOPLANET beta PICTORIS b: THE ORBIT OF THE YOUNG EXOPLANET beta PICTORIS b'. Together they form a unique fingerprint.

Cite this