PH1b (standing for "Planet Hunters 1"), or by its NASA designation Kepler-64b,[4] is an extrasolar planet found in a circumbinary orbit in the quadruple star system Kepler-64. The planet was discovered by two amateur astronomers from the Planet Hunters project of amateur astronomers using data from the Kepler space telescope with assistance of a Yale University team of international astronomers. The discovery was announced on 15 October 2012.[5][6] It is the first known transiting planet in a quadruple star system,[7] first known circumbinary planet in a quadruple star system,[8] and the first planet in a quadruple star system found. It was the first confirmed planet discovered by PlanetHunters.org.[2] An independent and nearly simultaneous detection was also reported from a revision of Kepler space telescope data using a transit detection algorithm.[9]
The giant planetisNeptune-sized, about 20-55 Earth-masses (ME). It has a radius 6.2 times that of Earth. The star system is 7200 light years[10] from Earth.[3][11][6][12] The planet orbits a close binary, with a more distant binary orbiting at a distance, forming the quadruple star system. The star system has the Kepler Input Catalogue name KIC 4862625 as well as the designation Kepler-64. The close binary (Aa+Ab) that the planet circles has an orbital period of 20 days. They form an eclipsing binary pair.[1] The two stars are (Aa) 1.384 solar mass (M☉) F-type main-sequence star and (Ab) 0.336 M☉red dwarf.[13][3][11][7] The planet orbits this binary pair in a 138.3-day orbit. The binary pairs have a separation of 1000 AUs.[1] A photometric-dynamical model was used to model the planetary system of the close binary pair. The distant binary (Ba+Bb) have a pair separation of 60 AU. The two stars are (Ba) 0.99 M☉G-type main-sequence star and (Bb) 0.51 M☉ red dwarf. The quadruple star system has an estimated age of two billion years (2 gigayears).[3] The system is located at right ascension19h52m 51.624sdeclination +39° 57′ 18.36″, so also has a 2MASS catalogue entry of 2MASS 19525162+3957183[14]
Light curve signaling the discovery of PH1, showing the first three transits of Kepler-64 (KIC 4862625)
Kian Jin Jek (Chinese: 易建仁, son of Jek Yeun Thong), from San Francisco, and Robert Gagliano, from Cottonwood, Arizona, spotted the signature of the planet in the Kepler data, and it was reported through the PlanetHunters.org program run by Dr. Chris Lintott, from Oxford University.[6] Kian Jek first spotted a light dip indicative of a transit in May 2011. JKD reported a second. Robert Gagliano performed a systematic search, and confirmed the second dip, and found a third, in February 2012. Using this, Kian predicted another transit, and found it. The planet was subsequently detected by eclipsing binary timing variation method.[1] At the time of discovery, it was the sixth known circumbinary planet.
The planet PH1b and were used as a benchmark system for automated detection algorithms. As a benchmark system PH1 is used to improve the algorithm and to demonstrate improvement in the detection of circumbinary planets.[15]
^Kostov, V. B.; McCullough, P. R.; Hinse, T. C.; Tsvetanov, Z. I.; Hébrard, G.; Díaz, R. F.; Deleuil, M.; Valenti, J. A. (2013-01-01). "A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the Two Transiting Planets in the Kepler-47 System". The Astrophysical Journal. 770 (1): 52. arXiv:1210.3850. Bibcode:2013ApJ...770...52K. doi:10.1088/0004-637X/770/1/52. ISSN0004-637X. S2CID119279690.
Discovery Paper: arXiv. "Planet Hunters: A Transiting Circumbinary Planet in a Quadruple Star System", Megan E. Schwamb, Jerome A. Orosz, Joshua A. Carter, William F. Welsh, Debra A. Fischer, Guillermo Torres, Andrew W. Howard, Justin R. Crepp, William C. Keel, Chris J. Lintott, Nathan A. Kaib, Dirk Terrell, Robert Gagliano, Kian J. Jek, Michael Parrish, Arfon M. Smith, Stuart Lynn, Robert J. Simpson, Matthew J. Giguere, Kevin Schawinski, 2012 October, arXiv:1210.3612 ; Bibcode:2012arXiv1210.3612S ;
