Physical and orbital properties of Beta Pictoris b
arXiv:1407.4001 · doi:10.1051/0004-6361/201424041
Abstract
The intermediate-mass star Beta Pictoris is known to be surrounded by a structured edge-on debris disk within which a gas giant planet was discovered orbiting at 8-10 AU. The physical properties of Beta Pic b were previously inferred from broad and narrow-band 0.9-4.8 microns photometry. We used commissioning data of the Gemini Planet Imager (GPI) to obtain new astrometry and a low-resolution (R=35-39) J-band (1.12-1.35 microns) spectrum of the planet. We find that the planet has passed the quadrature. We constrain its semi-major axis to 10 AU (90 % prob.) with a peak at 8.9+0.4-0.6 AU. The joint fit of the planet astrometry and the most recent radial velocity measurements of the star yields a planet's dynamical mass 20 MJup (greater than 96 % prob.). The extracted spectrum of Beta Pic b is similar to those of young L1-1.5+1 dwarfs. We use the spectral type estimate to revise the planet luminosity to log(L/Lsun)=-3.90+-0.07. The 0.9-4.8 microns photometry and spectrum are reproduced for Teff=1650+-150 K and a log g lower than 4.7 dex by 12 grids of PHOENIX-based and LESIA atmospheric models. If we adopt the most recent system age estimate (21+-4 Myr), the bolometric luminosity and the constraints on the dynamical mass of Beta Pic b are only reproduced by warm- and hot-start tracks with initial entropies Si greater than 10.5 kB/baryon. Such initial conditions may result from an inefficient accretion shock and/or a planetesimal density at formation higher than in the classical core accretion model. Considering a younger age for the system or a conservative formation time for Beta Pic b does not change these conclusions.
arXiv comment4 pages, 4 figures, 2 tables. 4 online appendices. Accepted for publication in A&A letters
References in corpus (36)
- Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945
- Evolutionary models for very-low-mass stars and brown dwarfs with dusty atmospheres
- Angular Differential Imaging: a Powerful High-Contrast Imaging Technique
- A giant planet imaged in the disk of the young star Beta Pictoris
- A probable giant planet imaged in the Beta Pictoris disk
- On the Luminosity of Young Jupiters
- Spectral and Photometric Diagnostics of Giant Planet Formation Scenarios
- A Near-Infrared Spectroscopic Study of Young Field Ultracool Dwarfs
- Solar System Abundances of the Elements
- A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group
- The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets
- Orbital characterization of the βPictoris b giant planet
- Subtle Signatures of Multiplicity in Late-type Dwarf Spectra: The Unresolved M8.5 + T5 Binary 2MASS J03202839-0446358
- A library of near-infrared integral field spectra of young M-L dwarfs
- Constraining the initial entropy of directly-detected exoplanets
- The Directly Imaged Planet around the Young Solar Analog 1RXS J160929.1-210524: Confirmation of Common Proper Motion, Temperature and Mass
- Near-infrared cross-dispersed spectroscopy of brown dwarf candidates in the Upper Sco association
- The Gemini NICI Planet-Finding Campaign : Discovery of a Substellar L Dwarf Companion to the Nearby Young M Dwarf CD-35 2722
- A Combined VLT and Gemini Study of the Atmosphere of the Directly-Imaged Planet, beta Pictoris b
- The near-infrared spectral energy distribution of β Pictoris b
- Discovery of a Planetary-mass Companion to a Brown Dwarf in Taurus
- Deuterium Burning in Massive Giant Planets and Low-Mass Brown Dwarfs formed by Core-Nucleated Accretion
- Luminosity of young Jupiters revisited. Massive cores make hot planets
- Discovery of the Young L Dwarf WISE J1741102.78-464225.5
- First Results From VLT NACO Apodizing Phase Plate: 4-micron Images of the Exoplanet beta Pictoris b
- Physical Properties of Young Brown Dwarfs and Very Low-Mass Stars Inferred from High-Resolution Model Spectra
- Searching for companions down to 2 AU from beta Pictoris using the L'-band AGPM coronagraph on VLT/NACO
- Accurate Astrometry and Photometry of Saturated and Coronagraphic Point Spread Functions
- Magellan Adaptive Optics first-light observations of the exoplanet Pic b. I. Direct imaging in the far-red optical with MagAO+VisAO and in the near-IR with NICI
- Constrains on planets around beta Pic with Harps radial velocity data
- Near-infrared integral-field spectra of the planet/brown dwarf companion AB Pic b
- Near-Infrared Detection and Characterization of the Exoplanet HD 95086 b with the Gemini Planet Imager
- The Coolest Isolated Brown Dwarf Candidate Member of TWA
- New constraints on the formation and settling of dust in the atmospheres of young M and L dwarfs
- Planets around stars in young nearby associations *** radial Velocity searches: a feasibility study, and first results
- Independent confirmation of β Pictoris b imaging with NICI
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- Population Properties of Brown Dwarf Analogs to Exoplanets
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- The SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE
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- Peering into the formation history of beta Pictoris b with VLTI/GRAVITY long baseline interferometry
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- Interpreting the photometry and spectroscopy of directly imaged planets: a new atmospheric model applied to beta Pictoris b and SPHERE observations
- 1 to 2.4 micron Near-IR spectrum of the Giant Planet Pictoris b obtained with the Gemini Planet Imager
- Atmospheric Regimes and Trends on Exoplanets and Brown Dwarfs
- Magellan Adaptive Optics first-light observations of the exoplanet beta Pic b. II. 3-5 micron direct imaging with MagAO+Clio, and the empirical bolometric luminosity of a self-luminous giant planet
- Spectroscopic characterization of HD 95086 b with the Gemini Planet Imager
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- High-Cadence, High-Contrast Imaging for Exoplanet Mapping: Observations of the HR 8799 Planets with VLT/SPHERE Satellite Spot-Corrected Relative Photometry
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- Astrometric Confirmation and Preliminary Orbital Parameters of the Young Exoplanet 51 Eridani b with the Gemini Planet Imager
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- The Inner Disk Structure, Disk-Planet Interactions, and Temporal Evolution in the Beta Pictoris System: A Two-Epoch HST/STIS Coronagraphic Study
- The LEECH Exoplanet Imaging Survey. Further constraints on the planet architecture of the HR 8799 system
- Post conjunction detection of Pictoris b with VLT/SPHERE
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- MASSIVE: A Bayesian analysis of giant planet populations around low-mass stars
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- A High-Contrast Search for Variability in HR 8799bc with VLT-SPHERE
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- Dynamical masses of M-dwarf binaries in young moving groups: I - The case of TWA 22 and GJ 2060
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- The beta Pictoris system: Setting constraints on the planet and the disk structures at mid-IR wavelengths with NEAR
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- Machine learning for exoplanet detection in high-contrast spectroscopy Combining cross correlation maps and deep learning on medium-resolution integral-field spectra