Ultra-short period planet

[1] At this short distance, tidal interactions lead to relatively rapid orbital and spin evolution.WASP-47e and 55 Cnc e have a lower density and are compatible with pure rock, or a rocky-iron body surrounded by a layer of water (or other volatiles).[1] A difference between hot Jupiters and terrestrial USP planets is the proximity of planetary companions.Hot Jupiters are rarely found with other planets within a factor of 2–3 in orbital period or distance.[1] A study by the TESS-Keck Survey using 17 USP planets found that USP planets predominantly have an Earth-like compositions with iron core mass of about 32% and have masses below runaway accretion.
exoplanetorbital periodmain-sequence starcircular orbittidally lockedG dwarfsM dwarfsF dwarfsK2-229bWASP-47e55 Cnc ehot Jupitersmetallicitygas dwarfsTESS-Keck Surveyrunaway accretionmultiple-planet systemsBibcodePlanetDefinitionPlanetary scienceExoplanet orbital and physical parametersMethods of detecting exoplanetsPlanetary systemPlanet-hosting starsTerrestrialCarbon planetCoreless planetDesert planetDwarf planetHycean planetIce planetIron planetLava planetOcean worldMega-EarthSub-EarthSuper-EarthGaseousEccentric JupiterMini-NeptuneHelium planetHot JupiterHot NeptuneGas giantIce giantSuper-JupiterSuper-NeptuneSuper-puffUltra-hot JupiterUltra-hot NeptuneBlanetBrown dwarfChthonian planetCircumbinary planetCircumtriple planetDisrupted planetDouble planetEcumenopolisEyeball planetGiant planetMesoplanetPlanemoPlanetesimalProtoplanetPulsar planetSub-brown dwarfSub-NeptuneToroidal planetUltra-cool dwarfFormation 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