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 language | English |
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Article number | 158 |
Number of pages | 9 |
Journal | Astrophysical Journal |
Volume | 794 |
Issue number | 2 |
DOIs | |
Publication status | Published - 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