Super-Jupiter

A super-Jupiter is a gas giant exoplanet that is more massive than the planet Jupiter.For example, companions at the planet–brown dwarf borderline have been called super-Jupiters, such as around the star Kappa Andromedae.[2] The increased mass compresses the planet due to gravity, thus keeping it from being larger.[3] An example of this may be the exoplanet HAT-P-1b with about half the mass of Jupiter but about 1.38 times larger diameter.Extreme compression of matter inside it causes the high density, because it is likely composed mainly of hydrogen.
Artist's impression of 2M1207b
Roland MKS-802M1207bJupitercompanionsbrown dwarfKappa Andromedaecompresses the planet due to gravitypuffy planetsHAT-P-1bCoRoT-3bosmiumhydrogensurface gravityKappa Andromedae bNeptuneIce giantKepler-1704bList of planet typesRed dwarfSub-brown dwarfSuper-EarthThe New York TimesAigrain, S.Astronomy and AstrophysicsBibcodePlanetDefinitionPlanetary scienceExoplanetExoplanet orbital and physical parametersMethods of detecting exoplanetsPlanetary systemPlanet-hosting starsTerrestrialCarbon planetCoreless planetDesert planetDwarf planetHycean planetIce planetIron planetLava planetOcean worldMega-EarthSub-EarthGaseousEccentric JupiterMini-NeptuneHelium planetHot JupiterHot NeptuneGas giantSuper-NeptuneSuper-puffUltra-hot JupiterUltra-hot NeptuneBlanetChthonian planetCircumbinary planetCircumtriple planetDisrupted planetDouble planetEcumenopolisEyeball planetGiant planetMesoplanetPlanemoPlanetesimalProtoplanetPulsar planetSub-NeptuneToroidal planetUltra-cool dwarfUltra-short period planet (USP)Formation and evolutionAccretionAccretion diskAsteroid beltCircumplanetary diskCircumstellar discCircumstellar envelopeCosmic dustDebris diskDetached objectExozodiacal dustExtraterrestrial materialsExtraterrestrial sample curationGiant-impact hypothesisGravitational collapseHills cloudInternal structureInterplanetary dust cloudInterplanetary mediumInterplanetary spaceInterstellar cloudInterstellar dustInterstellar mediumKuiper beltList of interstellar and circumstellar moleculesMolecular cloudNebular hypothesisOort cloudOuter spacePlanetary migrationProtoplanetary diskRing systemRubble pileSample-return missionScattered discStar formationSystemsExocometInterstellarExomoonTidally detachedRogue planetPulsarDetectionAstrometryMicrolensingPolarimetryRadial velocityTransit-timing variationHabitabilityAstrobiologyAstrooceanographyCircumstellar habitable zoneEarth analogExtraterrestrial liquid waterGalactic habitable zoneHabitability of binary star systemsHabitability of F-type main-sequence star systemsHabitability of K-type main-sequence star systemsHabitability of natural satellitesHabitability of neutron star systemsHabitability of red dwarf systemsHabitability of yellow dwarf systemsHabitable zone for complex lifeList of potentially habitable exoplanetsTholinSuperhabitable planetNearby Habitable SystemsExoplanet Data ExplorerExtrasolar Planets EncyclopaediaNASA Exoplanet ArchiveNASA Star and Exoplanet DatabaseOpen Exoplanet CatalogueHost starsMultiplanetary systemsStars with proto-planetary discsExoplanetsDiscoveriesExtremesFirstsNearestLargestHeaviestTerrestrial candidatesKeplerPotentially habitableProper namesbefore 20002000–2009Carl Sagan InstituteExoplanet naming conventionExoplanetary Circumstellar Environments and Disk ExplorerExtragalactic planetExtrasolar planets in fictionGeodynamics of terrestrial exoplanetsNeptunian desertNexus for Exoplanet System ScienceSmall planet radius gapSudarsky's gas giant classificationDiscoveries of exoplanetsSearch projects