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Kepler-86, PH2〔 or KIC 12735740 (2MASS 19190326+5157453), is a G-type star〔〔 distant〔 within the constellation Cygnus.〔 Roughly the size and temperature〔 of the Sun, PH2 gained prominence when it was known to be the host of one of 42 planet candidates detected by the Planet Hunters citizen science project in its second data release. The candidate orbiting around PH2, known as PH2 b, had been determined to have a spurious detection probability of only 0.08%, thus effectively confirming its existence as a planet. Located in its parent star's habitable zone, PH2 b (or Kepler-86b〔) is a "Jupiter-size" gas giant which may have a natural satellite suitable for hosting life.〔 The report of the confirmed detection of PH2 b was submitted on January 3, 2013.〔 It was discovered by amateur Pole Rafał Herszkowicz using his laptop and access to the Internet project with data from the ''Kepler'' space observatory. == History of detection == PH2 b was detected, along with 42 other planet candidates, in archival data from ''Kepler'' by the Planet Hunters project, in which human volunteers analyze the light curves of ''Kepler'' target stars, searching for planetary transit signals which may be missed by computer programs.〔 Previous work by Planet Hunters helped to confirm the existence of PH1 b, a Neptune-mass planet within a four-star system. All of the candidates in the second, including PH2 b, were identified by citizen scientists Abe J. Hoekstra, Thomas Lee Jacobs, Daryll LaCourse, Hans Martin Schwengler, Rafał Herszkowicz and Mike Chopin among others, with the help of Yale University astronomers.〔 In addition to PH2 b itself, twenty other planet candidates were found which are located in the habitable zones of their host stars; however, these have a relatively high probability of spurious detection and may well come from non-planetary sources.〔 Although the planet's initial detection was made using ''Kepler'' data, PH2's stellar spectra, required to rule out background stars or faint companions with planets as sources for the observed transits, were collected using the HIRES instrument at the W. M. Keck Observatory.〔 Results of observations confirmed the existence of PH2 b with "99.9 percent confidence."〔〔 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Kepler-86」の詳細全文を読む スポンサード リンク
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