Atmospheric circulation of hot Jupiters: Coupled radiative-dynamical general circulation model simulations of HD 189733b and HD 209458b
arXiv:0809.2089 · doi:10.1088/0004-637X/699/1/564
Abstract
We present global, three-dimensional numerical simulations of HD 189733b and HD 209458b that couple the atmospheric dynamics to a realistic representation of non-gray cloud-free radiative transfer. The model, which we call the Substellar and Planetary Atmospheric Radiation and Circulation (SPARC) model, adopts the MITgcm for the dynamics and uses the radiative model of McKay, Marley, Fortney, and collaborators for the radiation. Like earlier work with simplified forcing, our simulations develop a broad eastward equatorial jet, mean westward flow at higher latitudes, and substantial flow over the poles at low pressure. For HD 189733b, our simulations without TiO and VO opacity can explain the broad features of the observed 8 and 24-micron light curves, including the modest day-night flux variation and the fact that the planet/star flux ratio peaks before the secondary eclipse. Our simulations also provide reasonable matches to the Spitzer secondary-eclipse depths at 4.5, 5.8, 8, 16, and 24 microns and the groundbased upper limit at 2.2 microns. However, we substantially underpredict the 3.6-micron secondary-eclipse depth, suggesting that our simulations are too cold in the 0.1-1 bar region. Predicted temporal variability in secondary-eclipse depths is ~1% at Spitzer bandpasses, consistent with recent observational upper limits at 8 microns. We also show that nonsynchronous rotation can significantly alter the jet structure. For HD 209458b, we include TiO and VO opacity; these simulations develop a hot (>2000 K) dayside stratosphere. Despite this stratosphere, we do not reproduce current Spitzer photometry of this planet. Light curves in Spitzer bandpasses show modest phase variation and satisfy the observational upper limit on day-night phase variation at 8 microns. (abridged)
20 pages (emulate-apj format), 21 figures, final version now published in ApJ. Includes expanded discussion of radiative-transfer methods and two new figures
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- Wavelength Does Not Equal Pressure: Vertical Contribution Functions and their Implications for Mapping Hot Jupiters
- Photochemical hazes dramatically alter temperature structure and atmospheric circulation in 3D simulations of hot Jupiters
- ULTRACAM z'-band Detection of the Secondary Eclipse of WASP-12b
- Small hydrocarbon molecules in cloud-forming Brown Dwarf and giant gas planet atmospheres
- An exploration of model degeneracies with a unified phase curve retrieval analysis: The light and dark sides of WASP-43 b
- Hot Jupiter Diversity and the Onset of TiO/VO Revealed by a Large Grid of Non-Grey Global Circulation Models
- Secondary Eclipse Photometry of the Exoplanet WASP-5b with Warm Spitzer
- Community targets for JWST's early release science program: evaluation of WASP-63b
- A Mini-Chemical Scheme with Net Reactions for 3D GCMs II. 3D thermochemical modelling of WASP-39b and HD 189733b
- Atmospheres on Nonsynchronized Eccentric-tilted Exoplanets I: Dynamical Regimes
- Coupled evolutions of the stellar obliquity, orbital distance, and planet's radius due to the Ohmic dissipation induced in a diamagnetic hot Jupiter around a magnetic T Tauri star
- Atmospheric circulation of tidally locked gas giants with increasing rotation and implications for white-dwarf-brown-dwarf systems
- Numerical Convergence of Hot-Jupiter Atmospheric Flow Solutions
- The Influence of Galactic Cosmic Rays on Ion-Neutral Hydrocarbon Chemistry in the Upper Atmospheres of Free-Floating Exoplanets
- Retrieval of the dayside atmosphere of WASP-43b with CRIRES+
- How Does Thermal Scattering Shape the Infrared Spectra of Cloudy Exoplanets? A Theoretical Framework and Consequences for Atmospheric Retrievals in the JWST era
- Spatially Resolved Modeling of Optical Albedos for a Sample of Six Hot Jupiters
- The Mantis Network II: Examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling
- Detectability of Exoplanet Periastron Passage in the Infra-Red
- Diagnosing limb asymmetries in hot and ultra-hot Jupiters with high-resolution transmission spectroscopy
- Ionization in Atmospheres of Brown Dwarfs and Extrasolar Planets V: Alfvén Ionization
- Impact of stellar flares on the chemical composition and transmission spectra of gaseous exoplanets orbiting M dwarfs
- The stable climate of KELT-9b
- The Role of Drag in the Energetics of Strongly Forced Exoplanet Atmospheres
- Atmospheric Circulation and Thermal Phase-Curve Offset of Tidally and Non-Tidally Locked Terrestrial Exoplanets
- ACCESS: Ground-based Optical Transmission Spectroscopy of the Hot Jupiter WASP-4b
- More Evidence for Variable Helium Absorption from HD 189733b
- Modeling the high-resolution emission spectra of clear and cloudy non-transiting hot Jupiters
- TAU: A 1D radiative transfer code for transmission spectroscopy of extrasolar planet atmospheres
- Assessing telluric correction methods for Na detections with high-resolution exoplanet transmission spectroscopy
- Exoplanetary Monte Carlo Radiative Transfer with Correlated-k I. Benchmarking Transit and Emission Observables
- Signatures of Clouds in Hot Jupiter Atmospheres: Modeled High Resolution Emission Spectra from 3D General Circulation Models
- Atmospheres on Nonsynchronized Eccentric-tilted Exoplanets II: Thermal Light Curves
- A new approach to spectroscopic phase curves: The emission spectrum of WASP-12b observed in quadrature with HST/WFC3
- No evidence for radius inflation in hot Jupiters from vertical advection of heat
- Transmission strings: a technique for spatially mapping exoplanet atmospheres around their terminators
- The effect of interior heat flux on the atmospheric circulation of hot and ultra-hot Jupiters
- Evaluating Climate Variability Of The Canonical Hot Jupiters Hd 189733b & Hd 209458b Through Multi-epoch Eclipse Observations
- Distinguishing Between Stellar and Planetary Companions With Phase Monitoring
- A Lack of Variability Between Repeated Spitzer Phase Curves of WASP-43b
- Smaller than expected bright-spot offsets in Spitzer phase curves of the hot Jupiter Qatar-1b
- Global Chemical Transport on Hot Jupiters: Insights from 2D VULCAN photochemical model
- Chemical modeling of exoplanet atmospheres
- An investigation of a super-Earth exoplanet with a greenhouse-gas atmosphere using a general circulation model
- The THOR+HELIOS general circulation model: multi-wavelength radiative transfer with accurate scattering by clouds/hazes
- A Comparison of Simulated JWST Observations Derived from Equilibrium and Non-Equilibrium Chemistry Models of Giant Exoplanets
- Ground-based Spectroscopy of the Exoplanet XO-2b using a Systematic Wavelength Calibration
- Nonequilibrium thermodynamics of circulation regimes in optically-thin, dry atmospheres
- Molecular tracers of planet formation in the atmospheres of hot Jupiters
- Spitzer thermal phase curve of WASP-121 b
- Electrostatic activation of prebiotic chemistry in substellar atmospheres
- Time Resolved Absorption of Six Chemical Species With MAROON-X Points to Strong Drag in the Ultra Hot Jupiter TOI-1518 b
- A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE and HARPS-N
- Angular momentum transport, layering, and zonal jet formation by the GSF instability: nonlinear simulations at a general latitude
- A New Line-By-Line General Circulation Model for Simulations of Diverse Planetary Atmospheres: Initial Validation and Application to the Exoplanet GJ 1132b
- Supervised Learning Detection of Sixty Non-Transiting Hot Jupiter Candidates
- Analytical Models of Exoplanetary Atmospheres. IV. Improved Two-stream Radiative Transfer for the Treatment of Aerosols
- A Direct Comparison between the use of Double Gray and Multiwavelength Radiative Transfer in a General Circulation Model with and without Radiatively Active Clouds
- Exploring deep and hot adiabats as a potential solution to the radius inflation problem in brown dwarfs: Long-timescale models of the deep atmospheres of KELT-1b, Kepler-13Ab, and SDSS1411B
- Non-Local Thermodynamic Equilibrium Transmission Spectrum Modelling of HD209458b
- Coupled Day-Night Models of Exoplanetary Atmospheres
- The Influence of Differential Irradiation and Circulation on the Thermal Evolution of Gas Giant Planets. I. Upper Limits from Radiative Equilibrium
- Exoplanetary Geophysics -- An Emerging Discipline
- Thermal Phase Curves of XO-3b: an Eccentric Hot Jupiter at the Deuterium Burning Limit
- Hot exoplanetary atmospheres in 3D
- Semidiurnal thermal tides in asynchronously rotating hot Jupiters
- Clouds and Hazes in GJ 1214b's Metal-Rich Atmosphere
- A Panchromatic Characterization of the Evening and Morning Atmosphere of WASP-107 b: Composition and Cloud Variations, and Insight into the Effect of Stellar Contamination
- Toward a multidimensional analysis of transmission spectroscopy. Part III: Modelling 2D effects in retrievals with TauREx
- Atmospheric Characterization via Broadband Color Filters on the PLAnetary Transits and Oscillations of stars (PLATO) Mission
- Evidence of Radius Inflation in Radiative GCM Models of WASP-76b due to the Advection of Potential Temperature
- A Global Non-Hydrostatic Atmospheric Model with a Mass and Energy Conserving Vertically-Implicit-Correction (VIC) Scheme
- Turbulence-driven thermal and kinetic energy fluxes in the atmospheres of hot Jupiters
- ACCESS: An optical transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b
- Repeated Cyclogenesis on Hot-Exoplanet Atmospheres with Deep Heating
- Radiative Transfer for Exoplanet Atmospheres
- Non-Axisymmetric Flows on Hot Jupiters with Oblique Magnetic Fields
- The Hubble/STIS Near-ultraviolet Transmission Spectrum of HD 189733b
- A physically derived eddy parameterization for giant planet atmospheres with application on hot-Jupiter atmospheres
- Unstructured Grid Dynamical Modeling of Planetary Atmospheres using planetMPAS: The Influence of the Rigid Lid, Computational Efficiency, and Examples of Martian and Jovian Application
- Detecting the Wind-Driven Shapes of Extrasolar Giant Planets from Transit Photometry
- Magnetic winding and turbulence in ultra-hot Jupiters
- Linear and nonlinear properties of the Goldreich-Schubert-Fricke instability in stellar interiors with arbitrary local radial and latitudinal differential rotation
- Reassessing Exoplanet Light Curves with a Thermal Model
- Variability from thermo-resistive instability in the atmospheres of hot jupiters
- Unveiling the atmospheres of giant exoplanets with an EChO-class mission
- Hotter Than Expected: HST/WFC3 Phase-resolved Spectroscopy of a Rare Irradiated Brown Dwarf with Strong Internal Heat Flux
- Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
- ARES VI: Viability of one-dimensional retrieval models for transmission spectroscopy characterization of exo-atmospheres in the era of JWST and Ariel
- Is the hot, dense sub-Neptune TOI-824b an exposed Neptune mantle? Spitzer detection of the hot day side and reanalysis of the interior composition
- The Hubble PanCET program: Transit and Eclipse Spectroscopy of the Hot Jupiter WASP-74b
- Semi-Transparent Shear Turbulence in Hot Jupiter Atmospheres
- Signature of the atmospheric asymmetries of hot and ultra-hot Jupiters in lightcurves
- Under the magnifying glass: A combined 3D model applied to cloudy warm Saturn type exoplanets around M-dwarfs
- Horizontal and vertical exoplanet thermal structure from a JWST spectroscopic eclipse map
- Influences of internal forcing on atmospheric circulations of irradiated giant planets
- Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution
- Examining NHD vs QHD in the GCM THOR with non-grey radiative transfer for the hot Jupiter regime
- PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). III. Composition and winds in the atmosphere of TOI-1518 b
- Global flow regimes of hot Jupiters
- The GAPS Programme at TNG. LXIX.The Dayside of WASP-76b revealed by GIANO-B, HARPS-N and ESPRESSO: Evidence for Three-Dimensional Atmospheric Effects
- Large-amplitude Variability Driven by Giant Dust Storms on a Planetary-mass Companion
- Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows
- Magnetic field strengths of hot giant exoplanets consistent with Solar System values
- Flows, Circulations, and Energy Transport in the Outer and Deep Atmospheres of Synchronous and Non-synchronous Hot Jupiters
- Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions for JWST
- A Two-limb Explanation for the Optical-to-infrared Transmission Spectrum of the Hot Jupiter HAT-P-32Ab
- Quantifying thermal water dissociation in the dayside photosphere of WASP-121 b using NIRPS
- Cloudy solutions for the clear skies of WASP-80b: 3D cloud feedback on the atmosphere and spectra of a warm Jupiter
- Effects of the internal temperature on vertical mixing and on cloud structures in Ultra Hot Jupiters
- Examining the detectability of ringing on highly eccentric exoplanets
- Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission
- HyDRo: Atmospheric Retrieval of Rocky Exoplanets in Thermal Emission
- First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b
- Patchy nightside clouds on ultra-hot Jupiters: General Circulation Model simulations with radiatively active cloud tracers
- Effective drag in rotating, poorly conducting plasma turbulence
- Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST
- GCM-Motivated Multidimensional Temperature Parametrization Scheme for Phasecurve Retrieval
- Mechanisms of Superrotation in Slowly-Rotating and Tidally-Locked Planets
- A Possible Mechanism to Explain the Prograde Equatorial Jet of a Jupiter-like Gaseous Giant
- Angular Momentum and Heat Transport on Tidally Locked Hot Jupiter Planets
- Cloudy and Cloud-free Thermal Phase Curves with PICASO: Applications to WASP-43b