KnowraHot JupiterLinked fromLinked fromThe 23 pages that link to Hot Jupiter, each with the reason it gives.All 23Broader topic 13Related 2Narrower topic 5Compared with 3ExoplanetBroader topic: Its unexpectedly close orbit challenged assumptions about where giant planets form.Radial velocity methodBroader topic: Large, rapid stellar wobbles made these planets especially accessible to early surveys.Planetary migrationBroader topic: Close-in gas giants are a prominent clue that planets can move far from their birthplaces.Transit methodBroader topic: Its frequent, deep transits made this class especially accessible to early surveys.Tidal heatingRelated: Tidal dissipation can affect the interiors and orbital evolution of close-in giant planets.Exoplanet atmosphereBroader topic: These intensely irradiated planets provide strong atmospheric signals and were early targets for characterization.Kepler Space TelescopeCompared with: Kepler’s findings showed that hot Jupiters are only one striking kind among many planetary architectures.Planet formationBroader topic: Its close orbit requires formation and migration histories unlike simple in-place growth.Super-EarthCompared with: Hot Jupiters show that close-in exoplanets can occupy a radically larger mass regime.Core accretionBroader topic: Its close orbit challenges models that form giant planets beyond the disk's ice line.Gas giantBroader topic: These unusually warm, close-in giants challenge simple accounts of where planets form.51 Pegasi bNarrower topic: 51 Pegasi b became the prototype for this unexpectedly close-in class of planets.Disk instabilityRelated: Explaining how a rapidly formed distant fragment might become a close-in giant requires later migration.HD 209458 bNarrower topic: HD 209458 b is a well-studied example of this planetary class.Orbital migrationBroader topic: Their close orbits are often explained by migration from farther out.PhotoevaporationBroader topic: Some hot Jupiters show extended atmospheres losing gas under stellar irradiation.Michel MayorBroader topic: 51 Pegasi b revealed this unexpected class of close-orbiting giant planets.Didier QuelozNarrower topic: 51 Pegasi b was the first recognized example of this unexpected planet class.Jupiter massBroader topic: These planets are often compared by mass in Jupiter units despite their varied compositions.Carbon planetCompared with: A planet's orbital category does not establish carbon-rich composition; the terms describe different properties.Giant planetBroader topic: Hot Jupiters expose giant planets to intense irradiation and tidal effects absent from the Solar System's giants.Chthonian planetNarrower topic: This is the proposed progenitor class for chthonian planets.HD 189733 bNarrower topic: HD 189733 b belongs to this close-in class, whose intense stellar heating shapes its atmosphere.
KnowraHot JupiterLinked fromLinked fromThe 23 pages that link to Hot Jupiter, each with the reason it gives.All 23Broader topic 13Related 2Narrower topic 5Compared with 3ExoplanetBroader topic: Its unexpectedly close orbit challenged assumptions about where giant planets form.Radial velocity methodBroader topic: Large, rapid stellar wobbles made these planets especially accessible to early surveys.Planetary migrationBroader topic: Close-in gas giants are a prominent clue that planets can move far from their birthplaces.Transit methodBroader topic: Its frequent, deep transits made this class especially accessible to early surveys.Tidal heatingRelated: Tidal dissipation can affect the interiors and orbital evolution of close-in giant planets.Exoplanet atmosphereBroader topic: These intensely irradiated planets provide strong atmospheric signals and were early targets for characterization.Kepler Space TelescopeCompared with: Kepler’s findings showed that hot Jupiters are only one striking kind among many planetary architectures.Planet formationBroader topic: Its close orbit requires formation and migration histories unlike simple in-place growth.Super-EarthCompared with: Hot Jupiters show that close-in exoplanets can occupy a radically larger mass regime.Core accretionBroader topic: Its close orbit challenges models that form giant planets beyond the disk's ice line.Gas giantBroader topic: These unusually warm, close-in giants challenge simple accounts of where planets form.51 Pegasi bNarrower topic: 51 Pegasi b became the prototype for this unexpectedly close-in class of planets.Disk instabilityRelated: Explaining how a rapidly formed distant fragment might become a close-in giant requires later migration.HD 209458 bNarrower topic: HD 209458 b is a well-studied example of this planetary class.Orbital migrationBroader topic: Their close orbits are often explained by migration from farther out.PhotoevaporationBroader topic: Some hot Jupiters show extended atmospheres losing gas under stellar irradiation.Michel MayorBroader topic: 51 Pegasi b revealed this unexpected class of close-orbiting giant planets.Didier QuelozNarrower topic: 51 Pegasi b was the first recognized example of this unexpected planet class.Jupiter massBroader topic: These planets are often compared by mass in Jupiter units despite their varied compositions.Carbon planetCompared with: A planet's orbital category does not establish carbon-rich composition; the terms describe different properties.Giant planetBroader topic: Hot Jupiters expose giant planets to intense irradiation and tidal effects absent from the Solar System's giants.Chthonian planetNarrower topic: This is the proposed progenitor class for chthonian planets.HD 189733 bNarrower topic: HD 189733 b belongs to this close-in class, whose intense stellar heating shapes its atmosphere.