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Title: Characterizing 51 Eri b from 1 to 5 μm: A Partly Cloudy Exoplanet

Journal Article · · The Astronomical Journal (Online)
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Herein, we present spectrophotometry spanning 1–5 μm of 51 Eridani b, a 2–10 $${M}_{\mathrm{Jup}}$$ planet discovered by the Gemini Planet Imager Exoplanet Survey. In this study, we present new K1 (1.90–2.19 μm) and K2 (2.10–2.40 μm) spectra taken with the Gemini Planet Imager as well as an updated LP (3.76 μm) and new MS (4.67 μm) photometry from the NIRC2 Narrow camera. The new data were combined with J (1.13–1.35 μm) and H (1.50–1.80 μm) spectra from the discovery epoch with the goal of better characterizing the planet properties. The 51 Eri b photometry is redder than field brown dwarfs as well as known young T-dwarfs with similar spectral type (between T4 and T8), and we propose that 51 Eri b might be in the process of undergoing the transition from L-type to T-type. We used two complementary atmosphere model grids including either deep iron/silicate clouds or sulfide/salt clouds in the photosphere, spanning a range of cloud properties, including fully cloudy, cloud-free, and patchy/intermediate-opacity clouds. The model fits suggest that 51 Eri b has an effective temperature ranging between 605 and 737 K, a solar metallicity, and a surface gravity of log(g) = 3.5–4.0 dex, and the atmosphere requires a patchy cloud atmosphere to model the spectral energy distribution (SED). From the model atmospheres, we infer a luminosity for the planet of –5.83 to –5.93 ($$\mathrm{log}L/{L}_{\odot }$$), leaving 51 Eri b in the unique position of being one of the only directly imaged planets consistent with having formed via a cold-start scenario. Comparisons of the planet SED against warm-start models indicate that the planet luminosity is best reproduced by a planet formed via core accretion with a core mass between 15 and 127 $${M}_{\oplus }$$.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); National Science Foundation (NSF); National Research Council Canada (NRC); CONICYT; Australian Research Council (ARC); Ministério da Ciéncia, Tecnologia e Inovaçao; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration (NASA); Fonds de Recherche du Québec
Contributing Organization:
GPIES Team
Grant/Contract Number:
AC52-07NA27344; AST- 411868; AST-1518332; DGE-1311230; NNX14AJ80G; NNX15AD95G; AC52-06NA25396
OSTI ID:
1608096
Alternate ID(s):
OSTI ID: 1375176
Report Number(s):
LLNL-JRNL-804132; LA-UR-17-20913; 1007267; TRN: US2105010
Journal Information:
The Astronomical Journal (Online), Vol. 154, Issue 1; ISSN 1538-3881
Publisher:
IOP Publishing - AAASCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 80 works
Citation information provided by
Web of Science

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