The UK Met Office GCM with a sophisticated radiation scheme applied to the hot Jupiter HD 209458b
arXiv:1608.08593 · doi:10.1051/0004-6361/201629183
Abstract
To study the complexity of hot Jupiter atmospheres revealed by observations of increasing quality, we have adapted the UK Met Office global circulation model (GCM), the Unified Model (UM), to these exoplanets. The UM solves the full 3D Navier-Stokes equations with a height-varying gravity, avoiding the simplifications used in most GCMs currently applied to exoplanets. In this work we present the coupling of the UM dynamical core to an accurate radiation scheme based on the two-stream approximation and correlated-k method with state-of-the-art opacities from ExoMol. Our first application of this model is devoted to the extensively studied hot Jupiter HD 209458b. We have derived synthetic emission spectra and phase curves, and compare them to both previous models also based on state-of-the-art radiative transfer, and to observations. We find a reasonable a agreement between observations and both our day side emission and hot spot offset, however, our night side emission is too large. Overall our results are qualitatively similar to those found by Showman et al. (2009) with the SPARC/MITgcm, however, we note several quantitative differences: Our simulations show significant variation in the position of the hottest part of the atmosphere with pressure, as expected from simple timescale arguments, and in contrast to the "vertical coherency" found by Showman et al. (2009). We also see significant quantitative differences in calculated synthetic observations. Our comparisons strengthen the need for detailed intercomparisons of dynamical cores, radiation schemes and post-processing tools to understand these differences. This effort is necessary in order to make robust conclusions about these atmospheres based on GCM results.
Accepted for publication in Astronomy & Astrophysics. 11 pages, 11 figures, 1 table
References in corpus (22)
- Sodium Absorption From the Exoplanetary Atmosphere of HD189733b Detected in the Optical Transmission Spectrum
- Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy
- Water Vapor in the Spectrum of the Extrasolar Planet HD 189733b: 1. the Transit
- Can TiO Explain Thermal Inversions in the Upper Atmospheres of Irradiated Giant Planets?
- Ground-based detection of sodium in the transmission spectrum of exoplanet HD209458b
- Fingering convection and cloudless models for cool brown dwarf atmospheres
- Multi-Wavelength Constraints on the Day-Night Circulation Patterns of HD 189733b
- Dynamics and Disequilibrium Carbon Chemistry in Hot Jupiter Atmospheres, With Application to HD 209458b
- Atmospheric Circulation of Hot Jupiters: Three-dimensional circulation models of HD 209458b and HD 189733b with Simplified Forcing
- HST hot-Jupiter transmission spectral survey: detection of potassium in WASP-31b along with a cloud deck and Rayleigh scattering
- Atmospheric Circulation of Hot Jupiters: A Shallow Three-Dimensional Model
- The Effects of Consistent Chemical Kinetics Calculations on the Pressure-Temperature Profiles and Emission Spectra of Hot Jupiters
- The Atmospheric Circulation of the Hot Jupiter WASP-43b: Comparing Three-Dimensional Models to Spectrophotometric Data
- The 4.5 m full-orbit phase curve of the hot Jupiter HD 209458b
- Atmospheric Circulation of Eccentric Hot Neptune GJ436b
- Pseudo 2D chemical model of hot Jupiter atmospheres: application to HD 209458b and HD 189733b
- New Analysis Indicates No Thermal Inversion in the Atmosphere of HD 209458b
- Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models
- A search for TiO in the optical high-resolution transmission spectrum of HD 209458b: Hindrance due to inaccuracies in the line database
- Evidence against a strong thermal inversion in HD 209458 b from high-dispersion spectroscopy
- The atmospheric circulation of the super Earth GJ 1214b: Dependence on composition and metallicity
- The mid-infrared spectrum of the transiting exoplanet HD 209458b
Cited by in corpus (58)
- A hybrid line list for CH and hot methane continuum
- Treatment of overlapping gaseous absorption with the correlated-k method in hot Jupiter and brown dwarf atmosphere models
- The cloudy shape of hot Jupiter thermal phase curves
- Atmospheric Dynamics of Hot Giant Planets and Brown Dwarfs
- Implications of three-dimensional chemical transport in hot Jupiter atmospheres: results from a consistently coupled chemistry-radiation-hydrodynamics model
- Vertically resolved magma ocean-protoatmosphere evolution: H, HO, CO, CH, CO, O, and N as primary absorbers
- A unique hot Jupiter spectral sequence with evidence for compositional diversity
- Awesome SOSS: Transmission Spectroscopy of WASP-96b with NIRISS/SOSS
- Tracing the Hercules stream with Gaia and LAMOST: new evidence for a fast bar in the Milky Way
- A Review of Exoplanetary Biosignatures
- Water vapor detection in the transmission spectra of HD 209458 b with the CARMENES NIR channel
- Idealised simulations of the deep atmosphere of hot jupiters: Deep, hot, adiabats as a robust solution to the radius inflation problem
- 3D simulations of photochemical hazes in the atmosphere of hot Jupiter HD 189733b
- EXOPLINES: Molecular Absorption Cross-Section Database for Brown Dwarf and Giant Exoplanet Atmospheres
- The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI). Part III: Simulated Observables -- The return of the spectrum
- Simulating gas giant exoplanet atmospheres with Exo-FMS: Comparing semi-grey, picket fence and correlated-k radiative-transfer schemes
- Laboratory spectra of hot molecules: data needs for hot super-Earth exoplanets
- Grid of Pseudo-2D Chemistry Models for Tidally-Locked Exoplanets. I. The Role of Vertical and Horizontal Mixing
- Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
- Overcast on Osiris: 3D radiative-hydrodynamical simulations of a cloudy hot Jupiter using the parameterised, phase-equilibrium cloud formation code EddySed
- Outstanding Challenges of Exoplanet Atmospheric Retrievals
- 3D modelling of the impact of stellar activity on tidally locked terrestrial exoplanets: atmospheric composition and habitability
- The Climates of Other Worlds: A Review of the Emerging Field of Exoplanet Climatology
- THOR 2.0: Major Improvements to the Open-Source General Circulation Model
- Mineral cloud and hydrocarbon haze particles in the atmosphere of the hot Jupiter JWST target WASP-43b
- The Impact of Mixing Treatments on Cloud Modelling in 3D Simulations of Hot Jupiters
- A chemical kinetics code for modelling exoplanetary atmospheres
- The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres
- Aura-3D: A Three-dimensional Atmospheric Retrieval Framework for Exoplanet Transmission Spectra
- Pseudo-2D Modelling of Heat Redistribution Through H Thermal Dissociation/Recombination: Consequences for Ultra-Hot Jupiters
- A Mini-Chemical Scheme with Net Reactions for 3D GCMs II. 3D thermochemical modelling of WASP-39b and HD 189733b
- Rotational spectral modulation of cloudless atmospheres for L/T Brown Dwarfs and Extrasolar Giant Planets
- Implications of different stellar spectra for the climate of tidally-locked Earth-like exoplanets
- Impact of stellar flares on the chemical composition and transmission spectra of gaseous exoplanets orbiting M dwarfs
- BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
- The Acceleration of Superrotation in Simulated Hot Jupiter Atmospheres
- Discriminating between hazy and clear hot-Jupiter atmospheres with CARMENES
- The THOR+HELIOS general circulation model: multi-wavelength radiative transfer with accurate scattering by clouds/hazes
- 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
- Clouds and Hazes in GJ 1214b's Metal-Rich Atmosphere
- Hot exoplanetary atmospheres in 3D
- A Gaian Habitable Zone
- Atmospheric Characterization via Broadband Color Filters on the PLAnetary Transits and Oscillations of stars (PLATO) Mission
- Cloudy mornings and clear evenings on a gas giant exoplanet
- ARES VI: Viability of one-dimensional retrieval models for transmission spectroscopy characterization of exo-atmospheres in the era of JWST and Ariel
- Constraints on Planets in Nearby Young Moving Groups Detectable by High-Contrast Imaging and Gaia Astrometry
- A Biotic Habitable Zone: Impacts of Adaptation in Biotic Temperature Regulation
- Examining NHD vs QHD in the GCM THOR with non-grey radiative transfer for the hot Jupiter regime
- Reflected-light Phase Curves with PICASO: A Kepler-7b Case Study
- Global flow regimes of hot Jupiters
- Three-dimensional Transport-induced Chemistry on Temperate sub-Neptune K2-18b, Part I: the Effects of Atmospheric Dynamics
- Evidence of a sub-solar star in a microlensing event toward the LMC
- The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation
- Examining the detectability of ringing on highly eccentric exoplanets
- Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures
- Cloudy and Cloud-free Thermal Phase Curves with PICASO: Applications to WASP-43b
- Three-dimensional transport-induced chemistry on temperate sub-Neptune K2-18b, Part II: the combined effects of atmospheric dynamics and chemical reactions