| gptkbp:instanceOf | gptkb:Exoplanet_type 
 | 
                        
                            
                                | gptkbp:albedo | Low 
 | 
                        
                            
                                | gptkbp:alsoKnownAs | gptkb:Pegasid 
 | 
                        
                            
                                | gptkbp:atmosphere | Hydrogen and helium dominated 
 | 
                        
                            
                                | gptkbp:atmosphericEscapeMechanism | Hydrodynamic escape 
 | 
                        
                            
                                | gptkbp:clouds | Silicate and iron clouds possible 
 | 
                        
                            
                                | gptkbp:commonDetectionMethod | Radial velocity method Transit method
 
 | 
                        
                            
                                | gptkbp:compatibleWith | gptkb:Solar_System 
 | 
                        
                            
                                | gptkbp:corePresence | Uncertain 
 | 
                        
                            
                                | gptkbp:dayNightTemperatureDifference | Large 
 | 
                        
                            
                                | gptkbp:diameter | ~1 Jupiter radius 
 | 
                        
                            
                                | gptkbp:discoveredBy | gptkb:51_Pegasi_b 
 | 
                        
                            
                                | gptkbp:discoveredIn | 1995 
 | 
                        
                            
                                | gptkbp:distanceFromStar | <0.1 AU 
 | 
                        
                            
                                | gptkbp:eccentricity | Usually low 
 | 
                        
                            
                                | gptkbp:evaporation | Atmospheric escape observed 
 | 
                        
                            
                                | gptkbp:formationLocation | Beyond snow line (theory) 
 | 
                        
                            
                                | gptkbp:frequency | Sodium, potassium, water vapor 
 | 
                        
                            
                                | gptkbp:frequencyInSolarNeighborhood | ~1% of Sun-like stars 
 | 
                        
                            
                                | gptkbp:hasMoon | None detected 
 | 
                        
                            
                                | gptkbp:hostedBy | gptkb:Main-sequence_star 
 | 
                        
                            
                                | gptkbp:hostStarIrradiation | Very high 
 | 
                        
                            
                                | gptkbp:influenceOnHostStar | Tidal interactions 
 | 
                        
                            
                                | gptkbp:magneticFieldStrength | Possible, not confirmed 
 | 
                        
                            
                                | gptkbp:mass | >0.3 Jupiter masses 
 | 
                        
                            
                                | gptkbp:metallicityCorrelation | More common around metal-rich stars 
 | 
                        
                            
                                | gptkbp:migrationTheory | Disk migration High-eccentricity migration
 
 | 
                        
                            
                                | gptkbp:migrationToCurrentOrbit | Likely 
 | 
                        
                            
                                | gptkbp:notableExample | gptkb:HD_209458_b gptkb:Kepler-7b
 gptkb:WASP-12b
 gptkb:HD_189733_b
 
 | 
                        
                            
                                | gptkbp:oblateness | Slightly oblate due to rapid rotation 
 | 
                        
                            
                                | gptkbp:orbitType | <10 days 
 | 
                        
                            
                                | gptkbp:phaseCurveObservation | Possible 
 | 
                        
                            
                                | gptkbp:polarization | Detectable in some cases 
 | 
                        
                            
                                | gptkbp:publicInterest | High in exoplanet research 
 | 
                        
                            
                                | gptkbp:rings | Unlikely 
 | 
                        
                            
                                | gptkbp:spinOrbitAlignment | Can be misaligned 
 | 
                        
                            
                                | gptkbp:temperature | >1000 K 
 | 
                        
                            
                                | gptkbp:thermalEmission | Detectable in infrared 
 | 
                        
                            
                                | gptkbp:tidalLocking | gptkb:Common 
 | 
                        
                            
                                | gptkbp:transitDepth | Large, easy to detect 
 | 
                        
                            
                                | gptkbp:transitTimingVariations | Can indicate additional planets 
 | 
                        
                            
                                | gptkbp:winds | Very strong, supersonic 
 | 
                        
                            
                                | gptkbp:bfsParent | gptkb:51_Pegasi_b 
 | 
                        
                            
                                | gptkbp:bfsLayer | 6 
 | 
                        
                            
                                | https://www.w3.org/2000/01/rdf-schema#label | Hot Jupiter 
 |