Understanding the atmospheric properties and chemical composition of the ultra-hot Jupiter HAT-P-7b: III. Changing ionisation and the emergence of an ionosphere
arXiv:2101.05767 · doi:10.1051/0004-6361/202039699
Abstract
Ultra-hot Jupiters are the hottest close-in exoplanets discovered so far, and present a unique possibility to explore hot and cold chemistry on one object. The tidally locked ultra-hot Jupiter HAT-P-7b has a day/night temperature difference of ~ 2500K, confining cloud formation to the nightside and efficient ionisation to the dayside. Both have distinct observational signatures. We analyse plasma and magnetic processes in the atmosphere of the ultra-hot Jupiter HAT-P-7b to investigate the formation of a thermal ionosphere and the possibility of magnetically coupling the atmospheric gas as the base for an extended exosphere. We show which ions and atoms may be used as spectral tracers, and if and where conditions for lightning may occur within the clouds of HAT-P-7b, evaluate characteristic plasma and magnetic coupling parameters, and a LTE radiative transfer is solved for the ionised gas phase. The ionisation throughout HAT-P-7b's atmosphere varies drastically between day- and nightside. The dayside has high levels of thermal ionisation and long-range electromagnetic interactions dominate over kinetic electron-neutral interactions, suggesting a day-night difference in magnetic coupling. K+, Na+, Li+, Ca+, and Al+ are more abundant than their atomic counterparts on the dayside. The minimum magnetic flux density for electrons for magnetic coupling is B<0.5G for all regions of HAT-P-7b's atmosphere. HAT-P-7b's dayside has an asymmetric ionosphere that extends deep into the atmosphere, the nightside has no thermally driven ionosphere. A corresponding asymmetry is imprinted in the ion/neutral composition at the terminators. The ionosphere on HAT-P-7b may be directly traced by the Ca+ H&K lines if the local temperature is > 5000K. The whole atmosphere may couple to a global, large-scale magnetic field, and lightning may occur on the nightside.
11 pages, accepted for publication in A&A
References in corpus (19)
- petitRADTRANS: a Python radiative transfer package for exoplanet characterization and retrieval
- A spectral survey of an ultra-hot Jupiter: Detection of metals in the transmission spectrum of KELT-9 b
- Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e
- HAT-P-7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field
- Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) IV. A spectral inventory of atoms and molecules in the high-resolution transmission spectrum of WASP-121 b
- Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX
- Ionized calcium in the atmospheres of two ultra-hot exoplanets WASP-33b and KELT-9b
- Detection of sodium in the atmosphere of WASP-69b
- Detection of ionized calcium in the atmosphere of the ultra-hot Jupiter KELT-9b
- A temperature inversion with atomic iron in the ultra-hot dayside atmosphere of WASP-189b
- The Influence of Host Star Spectral Type on Ultra-Hot Jupiter Atmospheres
- Sparkling nights and very hot days on WASP-18b: the formation of clouds and the emergence of an ionosphere
- Exoplanetary atmospheric sodium revealed by the orbital motion. Narrow-band transmission spectroscopy of HD 189733b with UVES
- Electrodynamics on extrasolar giant planets
- Emission lines in the atmosphere of the irradiated brown dwarf WD0137-349B
- MOVES IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b
- Lightning climatology of exoplanets and brown dwarfs guided by Solar System data
- Large-scale changes of the cloud coverage in the Indi Ba,Bb system
- Lightning in other planets
Cited by in corpus (12)
- Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants
- Exoplanet weather and climate regimes with clouds and thermal ionospheres: A model grid study in support of large-scale observational campaigns
- The Mantis Network II: Examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling
- MOVES V. Modelling star-planet magnetic interactions of HD 189733
- No evidence for radius inflation in hot Jupiters from vertical advection of heat
- The atmospheric composition of the ultra-hot Jupiter WASP-178 b observed with ESPRESSO
- Photodissociation and induced chemical asymmetries on ultra-hot gas giants. A case study of HCN on WASP-76 b
- Evidence of Radius Inflation in Radiative GCM Models of WASP-76b due to the Advection of Potential Temperature
- The CHEOPS view on the climate of WASP-3 b
- Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows
- : Accelerating Bayesian atmospheric retrievals with transformer neural networks
- CARMENES detection of the CaII infrared triplet and possible evidence of HeI in the atmosphere of WASP-76b