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
|