hot Jupiters

GPTKB entity

Statements (57)
Predicate Object
gptkbp:instanceOf exoplanets
gptkbp:are gas giants
gptkbp:can_be high atmospheric pressure
thick atmospheres
strong magnetic fields
high wind speeds
variable brightness
extreme weather patterns
atmospheric escape rates that vary
atmospheric layers with different temperatures
atmospheric phenomena similar to storms
atmospheric temperature inversions
clouds of silicate and iron
clouds that affect their thermal structure
complex chemical compositions
high levels of carbon monoxide
high levels of irradiation
high levels of sodium and potassium
high levels of water vapor
high temperatures in their upper atmospheres
metal-rich atmospheres
significant tidal forces
strong thermal inversions
atmospheric conditions that lead to rain of molten glass.
gptkbp:characterizedBy high surface temperatures
gptkbp:designatedAs puffy planets
gptkbp:exhibits atmospheric escape
gptkbp:has short orbital periods
gptkbp:hasExperienceIn strong stellar radiation
https://www.w3.org/2000/01/rdf-schema#label hot Jupiters
gptkbp:is_available_in various star systems
gptkbp:is_essential_for exoplanet research
gptkbp:is_featured_in binary star systems
multi-planet systems
rapid rotation
high albedo
close-in orbits
eccentric orbits
high-density star clusters
less dense than terrestrial planets
strong thermal emissions
hot_star_systems
larger_than_Jupiter
gptkbp:is_monitored_by transit method
gptkbp:is_popular_among gravitational microlensing
gptkbp:is_studied_in space telescopes
planetary formation
atmospheric composition
the diversity of exoplanets
their interaction with stellar winds
their potential habitability
gptkbp:is_used_in gptkb:Jupiter
radial velocity method
Neptune-like planets
theories of planetary migration
gptkbp:mayHave clouds of vaporized metals
gptkbp:mission close to their parent stars