PH2 (original) (raw)
ケプラー86(英語:Kepler-86)とは地球から見てはくちょう座の方向、1206光年離れたところにある太陽に非常によく似たG型主系列星である。
| Property | Value |
|---|---|
| dbo:abstract | El Kepler-86, PH-2 o KIC 12735740 és una estrella tipus G situada a aproximadament 1.205,9 anys llum de distància. S'ubica a la Constel·lació del Cigne. Es calcula que compta amb gairebé la mateixa mida i temperatura que el Sol. Ph-2 guanyà prominència quan es va conéixer per ésser l'amfitrió d'un dels 42 exoplanetes candidats per contrindre vida pel projecte de ciència ciutadana Planet Hunters en la seva segona publicació de l'informe. El candidat que orbita el Kepler-86 s'anomena Kepler-86b (O PH-2b) ha sigut confirmat oficialment com un planeta. El Kepler-86b es localitza a la zona habitable respecte a la seva estrella mare. És un gegant gasós de la mida aproximada de Júpiter. S'especula que pot tenir un exosatèl·lit natural també adequat per a la vida. El report de confirmació del descobriment fou presentat el 3 de gener del 2013. Fou descobert per l'astrònom amateur polonès Rafał Herszkowicz amb el seu ordinador portàtil i accés al projecte d'internet amb dades de l'observatori espacial Kepler. (ca) PH2, also known as Kepler-86, or KIC 12735740 (2MASS 19190326+5157453), is a G-type star 1,130 ly (350 pc) 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 using his laptop and access to the Internet project with data from the Kepler space observatory. (en) Kepler-86, nota anche come PH2, è una stella di tipo G situata nella costellazione del Cigno. Di dimensioni e temperatura simili a quelle del Sole, ha conosciuto un'elevata attenzione da parte dei media a seguito dell'annuncio il 3 gennaio 2013 dell'esistenza di un pianeta extrasolare in orbita attorno ad essa, insieme ad altre 41 stelle individuate da Planet Hunters. Il pianeta candidato, Kepler-86 b, è stato rivelato con un margine di errore dello 0,08%, rendendolo quindi un pianeta confermato a tutti gli effetti. Situato all'interno della zona di abitabilità della propria stella, Kepler-86 b è un gigante gassoso delle dimensioni di Giove, e un suo eventuale satellite potrebbe essere in grado di ospitare la vita. (it) ケプラー86(英語:Kepler-86)とは地球から見てはくちょう座の方向、1206光年離れたところにある太陽に非常によく似たG型主系列星である。 (ja) PH2 b (Kepler-86b) – planeta pozasłoneczna typu gazowy olbrzym orbitująca wokół gwiazdy , odkryta w 2012 w ramach programu analizującego dane odebrane z teleskopu kosmicznego Keplera. Istnienie planety zostało potwierdzone z pewnością wynoszącą 99,92%. (pl) PH2, também conhecida como KIC 12735740 ou Kepler-86, é uma estrela da classe G, localizada na constelação de Cygnus. Tem aproximadamente o mesmo tamanho e a mesma temperatura que o Sol. (pt) PH2，即克卜勒86（Kepler-86），或稱為KIC 12735740，是一顆天鵝座的光譜類型 G 型恆星，距離地球1205.9光年（369.7秒差距）。該恆星的體積與表面溫度和太陽相當。PH2 因為是公民科學計畫行星獵人第二批釋出資料中的42個擁有行星的候選恆星之一而受到注意。環繞 PH2 的候選天體即 PH2 b，它的假訊號機率只有0.08%，因此被確認是真實存在的行星。 PH2 b 是一顆位於 PH2 適居帶的木星尺寸類木行星，該行星周圍可能存在適合生命生存的系外衛星。PH2 b 的觀測確認報告於2013年1月3日送出，它是被波蘭業餘天文學家 在他的電腦上透過網際網路處理來自克卜勒太空望遠鏡的資料時發現的。 (zh) |
| dbo:thumbnail | wiki-commons:Special:FilePath/PH2_b_and_PH2_from_an_exomoon.jpg?width=300 |
| dbo:wikiPageExternalLink | https://web.archive.org/web/20131105082102/http:/www.nasa.gov/mission_pages/kepler/main/index.html https://archive.today/20130215193638/http:/www.cthreepo.com/stars/viewK.php%3FKIC=12735740 https://www.youtube.com/watch%3Fv=qHvb9mewXJo |
| dbo:wikiPageID | 38218985 (xsd:integer) |
| dbo:wikiPageLength | 11656 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1105983206 (xsd:integer) |
| dbo:wikiPageWikiLink | dbc:Kepler_objects_of_interest dbr:Extrasolar_moon dbr:Methods_of_detecting_exoplanets dbr:Light_curve dbc:Cygnus_(constellation) dbc:G-type_main-sequence_stars dbc:Planetary_systems_with_one_confirmed_planet dbr:Gas_giant dbr:G-type_star dbr:NASA dbr:File:PH2_b_and_PH2_from_an_exomoon.jpg dbr:Transit_method dbr:Main_sequence dbr:Kepler-1625b_I dbr:Kepler_Input_Catalog dbc:Planetary_transit_variables dbr:W._M._Keck_Observatory dbr:Habitability_of_natural_satellites dbr:2MASS dbc:2MASS_objects dbr:Cygnus_(constellation) dbr:Exomoon dbr:File:LombergA1024.jpg dbr:HIP_41378_f dbr:Habitable_zone dbr:Kepler-1708b_I dbr:Kepler_(spacecraft) dbr:Planet_Hunters dbr:Poles dbr:Citizen_science dbr:HIRES dbr:Neptune dbr:Yale_University dbr:PH1 dbr:Rafał_Herszkowicz |
| dbp:appmag | 12.340000 (xsd:double) 12.620000 (xsd:double) |
| dbp:appmag1Passband | J (en) |
| dbp:appmag2Passband | H (en) |
| dbp:appmag3Passband | K (en) |
| dbp:appmag4Passband | B1 (en) |
| dbp:appmag5Passband | R1 (en) |
| dbp:bV | 0.072000 (xsd:double) |
| dbp:caption | Artist's conception of PH2 and its planet, PH2b, viewed from a hypothetical moon of the planet. (en) |
| dbp:class | G5V (en) |
| dbp:constell | dbr:Cygnus_(constellation) |
| dbp:credit | Haven Giguere, Matthew Giguere/Yale (en) |
| dbp:epoch | J2000 (en) |
| dbp:exoplanet | b (en) |
| dbp:kic | 12735740 (xsd:integer) |
| dbp:names | 2 (xsd:integer) |
| dbp:pError | 0.030200 (xsd:double) |
| dbp:parallax | 2.879600 (xsd:double) |
| dbp:simbad | KIC+12735740 (en) |
| dbp:type | dbr:Main_sequence |
| dbp:wikiPageUsesTemplate | dbt:! dbt:About dbt:Clear_left dbt:Convert dbt:OrbitboxPlanet dbt:OrbitboxPlanet_begin dbt:Orbitbox_end dbt:Portal_bar dbt:Reflist dbt:Short_description dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_reference dbt:Val dbt:Dec dbt:RA dbt:Stars_of_Cygnus dbt:Exoplanets dbt:Extraterrestrial_life |
| dcterms:subject | dbc:Kepler_objects_of_interest dbc:Cygnus_(constellation) dbc:G-type_main-sequence_stars dbc:Planetary_systems_with_one_confirmed_planet dbc:Planetary_transit_variables dbc:2MASS_objects |
| rdf:type | owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody dbo:Star |
| rdfs:comment | ケプラー86(英語:Kepler-86)とは地球から見てはくちょう座の方向、1206光年離れたところにある太陽に非常によく似たG型主系列星である。 (ja) PH2 b (Kepler-86b) – planeta pozasłoneczna typu gazowy olbrzym orbitująca wokół gwiazdy , odkryta w 2012 w ramach programu analizującego dane odebrane z teleskopu kosmicznego Keplera. Istnienie planety zostało potwierdzone z pewnością wynoszącą 99,92%. (pl) PH2, também conhecida como KIC 12735740 ou Kepler-86, é uma estrela da classe G, localizada na constelação de Cygnus. Tem aproximadamente o mesmo tamanho e a mesma temperatura que o Sol. (pt) PH2，即克卜勒86（Kepler-86），或稱為KIC 12735740，是一顆天鵝座的光譜類型 G 型恆星，距離地球1205.9光年（369.7秒差距）。該恆星的體積與表面溫度和太陽相當。PH2 因為是公民科學計畫行星獵人第二批釋出資料中的42個擁有行星的候選恆星之一而受到注意。環繞 PH2 的候選天體即 PH2 b，它的假訊號機率只有0.08%，因此被確認是真實存在的行星。 PH2 b 是一顆位於 PH2 適居帶的木星尺寸類木行星，該行星周圍可能存在適合生命生存的系外衛星。PH2 b 的觀測確認報告於2013年1月3日送出，它是被波蘭業餘天文學家 在他的電腦上透過網際網路處理來自克卜勒太空望遠鏡的資料時發現的。 (zh) El Kepler-86, PH-2 o KIC 12735740 és una estrella tipus G situada a aproximadament 1.205,9 anys llum de distància. S'ubica a la Constel·lació del Cigne. Es calcula que compta amb gairebé la mateixa mida i temperatura que el Sol. Ph-2 guanyà prominència quan es va conéixer per ésser l'amfitrió d'un dels 42 exoplanetes candidats per contrindre vida pel projecte de ciència ciutadana Planet Hunters en la seva segona publicació de l'informe. El candidat que orbita el Kepler-86 s'anomena Kepler-86b (O PH-2b) ha sigut confirmat oficialment com un planeta. (ca) PH2, also known as Kepler-86, or KIC 12735740 (2MASS 19190326+5157453), is a G-type star 1,130 ly (350 pc) 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. (en) Kepler-86, nota anche come PH2, è una stella di tipo G situata nella costellazione del Cigno. Di dimensioni e temperatura simili a quelle del Sole, ha conosciuto un'elevata attenzione da parte dei media a seguito dell'annuncio il 3 gennaio 2013 dell'esistenza di un pianeta extrasolare in orbita attorno ad essa, insieme ad altre 41 stelle individuate da Planet Hunters. Il pianeta candidato, Kepler-86 b, è stato rivelato con un margine di errore dello 0,08%, rendendolo quindi un pianeta confermato a tutti gli effetti. (it) |
| rdfs:label | PH2 (en) Kepler-86 (ca) Kepler-86 (it) ケプラー86 (ja) PH2 b (pl) PH2 (pt) PH2 (zh) |
| owl:sameAs | wikidata:PH2 dbpedia-ca:PH2 dbpedia-it:PH2 dbpedia-ja:PH2 dbpedia-mk:PH2 dbpedia-pl:PH2 dbpedia-pt:PH2 dbpedia-zh:PH2 https://global.dbpedia.org/id/384sk |
| prov:wasDerivedFrom | wikipedia-en:PH2?oldid=1105983206&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/PH2_b_and_PH2_from_an_exomoon.jpg wiki-commons:Special:FilePath/LombergA1024.jpg |
| foaf:isPrimaryTopicOf | wikipedia-en:PH2 |
| foaf:name | PH2 / Kepler-86 (en) |
| is dbo:wikiPageRedirects of | dbr:Kepler-86b dbr:PH2b dbr:Kepler-86 dbr:PH2_b dbr:Kepler_86 dbr:Kepler_86b |
| is dbo:wikiPageWikiLink of | dbr:Kepler-86b dbr:PH2b dbr:Kepler-86 dbr:Ph2 dbr:PH2_b dbr:Kepler_86 dbr:Kepler_86b |
| is foaf:primaryTopic of | wikipedia-en:PH2 |
