Properties (60)
Predicate | Object |
---|---|
gptkbp:instanceOf |
Exoplanet
|
gptkbp:canBe |
Tidal locking
|
gptkbp:canEstablish |
Cloud formation
Variable brightness Temperature inversions Thermal inversions Atmospheric_escape |
gptkbp:hasFacilities |
Similar_to_or_greater_than_Jupiter
|
gptkbp:hasGoals |
3 to 5 days
Similar_to_or_larger_than_Jupiter |
https://www.w3.org/2000/01/rdf-schema#label |
Hot Jupiter
|
gptkbp:isAssociatedWith |
Hot Jupiters category
|
gptkbp:isCharacterizedBy |
High surface temperatures
|
gptkbp:isConsidered |
A challenge for planet formation theories
A key to understanding planetary migration A type of exoplanet A unique class of exoplanets |
gptkbp:isFoundIn |
Various star systems
Close proximity to their stars |
gptkbp:isInfluencedBy |
Host star's gravity
|
gptkbp:isKnownFor |
Have diverse atmospheric compositions
Have high atmospheric pressure Have high heat retention Have varying densities High temperatures due to proximity to host star |
gptkbp:isLocatedIn |
Galaxy
|
gptkbp:isMaintainedBy |
Various telescopes
|
gptkbp:isOftenAccompaniedBy |
Space telescopes
|
gptkbp:isOftenMadeWith |
Other exoplanet types
Earth-like_planets Gas_giants_in_our_Solar_System |
gptkbp:isOftenUsedIn |
Binary star systems
Hot star systems Transit surveys |
gptkbp:isPartOf |
Astrobiology research
Exoplanet research Planetary science research Exoplanet classification system Exoplanet databases Exoplanet population studies Hot_Jupiter_category |
gptkbp:isProtectedBy |
Radial velocity method
Transit method |
gptkbp:isStudiedIn |
Astrophysicists
Understanding planetary evolution Understanding planetary atmospheres Potential for hosting moons Potential habitability of moons Understanding atmospheric dynamics Understanding star-planet interactions |
gptkbp:isSubjectTo |
Extreme radiation from host star
Intense stellar winds |
gptkbp:mayHave |
Magnetic fields
Clouds and storms in atmosphere Different chemical compositions Different orbital eccentricities High levels of irradiation Metal-rich atmospheres Rapid rotation rates Strong atmospheric winds |