| dbo:abstract |
HD 52265 b (بالإنجليزية: HD 52265 b) الذي يرمز له بالرمز HD 52265b، هو كوكب خارج المجموعة الشمسية، في كوكبة وحيد القرن، يتبع . (ar) HD 52265 b is a gas giant exoplanet located approximately 98 light-years away in the constellation of Monoceros, orbiting the star HD 52265. The planet has a minimum mass slightly more than that of Jupiter. Mean distance between the planet and the star is half that of Earth from the Sun. It was discovered by both the California and Carnegie Planet Search team and the Geneva Extrasolar Planet Search team independently of each other. By studying the fluctuations of the brightness of a host star, the inclination of the stars equator was determined. This allowed to calculate its true mass, assuming that the planet orbits in the plane of the star's equator. The planet HD 52265 b is named Cayahuanca. The name was selected in the NameExoWorlds campaign by El Salvador, during the 100th anniversary of the IAU. Cayahuanca means "The rock looking at the stars" in the native Nahuat language. (en) HD 52265 b adalah sebuah planet luar surya yang terletak sekitar 97,88 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2000 dengan menggunakan metode kecepatan radial. HD 52265 b memiliki massa sebesar 1,21 massa Jupiter. (in) HD 52265 b는 지구로부터 외뿔소자리 방향으로 약 92광년 떨어진 곳에 있는 외계 행성이다. 어머니 항성은 태양과 비슷한 G형 주계열성 이다. 이 행성의 최소 질량은 목성보다 약간 더 크다. 항성과 떨어져 있는 평균 거리는 태양과 지구 간격의 절반 정도이다. 그러나 궤도는 찌그러져 있으며, 근일점에서는 수성보다 가까이 접근하고 멀어질 때는 근일점의 두 배 가까운 거리만큼 물러난다. (ko) HD 52265 b (Cayahuanca) – planeta pozasłoneczna typu gazowy olbrzym, o masie podobnej do masy Jowisza. Okrąża gwiazdę HD 52265 (Citalá) po ekscentrycznej orbicie. (pl) HD 52265 b é um planeta extrassolar do tipo gigante gasoso localizado a aproximadamente 92 anos-luz na constelação de Monoceros, orbitando a estrela . Este planeta possui uma massa mínima ligeiramente superior à de Júpiter. A distância média entre o planeta e sua estrela-mãe é metade da distância entre a Terra e o Sol. Sua órbita é excêntrica, durante o periastro o planeta se encontra um pouco mais próximo de HD 52265 do que Mercúrio em relação ao Sol, e durante o apoastro essa distância mais que dobra. (pt) HD 52265 b是一顆距離地球約92光年的太陽系外行星，屬於類木行星，位於麒麟座，母恆星是 HD 52265。該行星的質量下限稍高於木星，和母恆星的平均距離是日地距離的一半。該行星由和各自獨立發現。 (zh) |
| dbo:detectionMethod |
Doppler spectroscopy |
| dbo:wikiPageExternalLink |
http://media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+52265 https://web.archive.org/web/20080514235741/http:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+52265 http://exoplanet.eu/planet.php%3Fp1=HD+52265&p2=b |
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16781367 (xsd:integer) |
| dbo:wikiPageLength |
5211 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID |
1036021122 (xsd:integer) |
| dbo:wikiPageWikiLink |
dbr:Doppler_spectroscopy dbc:Exoplanets_detected_by_radial_velocity dbc:Exoplanets_with_proper_names dbc:Giant_planets dbc:Monoceros_(constellation) dbr:Constellation dbr:Gas_giant dbr:Geneva_Extrasolar_Planet_Search dbr:El_Salvador dbr:Monoceros_(constellation) dbr:La_Silla_Observatory dbr:Light-year dbc:Exoplanets_discovered_in_2000 dbr:Minimum_mass dbr:Earth dbr:Exoplanet dbr:HD_52265 dbr:International_Astronomical_Union dbr:Jupiter dbr:Sun dbr:Nawat_language dbr:NameExoWorlds dbr:Keck_Observatory dbr:California_and_Carnegie_Planet_Search |
| dbp:discovered |
2000 (xsd:integer) |
| dbp:discoverer |
Butler et al. and Naef et al. (en) |
| dbp:discoveryMethod |
dbr:Doppler_spectroscopy |
| dbp:discoverySite |
Keck Observatory and La Silla Observatory (en) |
| dbp:name |
HD 52265 b (en) |
| dbp:star |
dbr:HD_52265 |
| dbp:wikiPageUsesTemplate |
dbt:Cite_encyclopedia dbt:Cite_web dbt:Extrasolar-planet-stub dbt:Infobox_planet dbt:Reflist dbt:Short_description dbt:Sky dbt:Val |
| dcterms:subject |
dbc:Exoplanets_detected_by_radial_velocity dbc:Exoplanets_with_proper_names dbc:Giant_planets dbc:Monoceros_(constellation) dbc:Exoplanets_discovered_in_2000 |
| gold:hypernym |
dbr:Exoplanet |
| rdf:type |
owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody wikidata:Q634 yago:CelestialBody109239740 yago:GasGiant109322087 yago:NaturalObject100019128 yago:Object100002684 yago:PhysicalEntity100001930 yago:Planet109394007 yago:WikicatGasGiants dbo:Planet yago:Whole100003553 |
| rdfs:comment |
HD 52265 b (بالإنجليزية: HD 52265 b) الذي يرمز له بالرمز HD 52265b، هو كوكب خارج المجموعة الشمسية، في كوكبة وحيد القرن، يتبع . (ar) HD 52265 b adalah sebuah planet luar surya yang terletak sekitar 97,88 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2000 dengan menggunakan metode kecepatan radial. HD 52265 b memiliki massa sebesar 1,21 massa Jupiter. (in) HD 52265 b는 지구로부터 외뿔소자리 방향으로 약 92광년 떨어진 곳에 있는 외계 행성이다. 어머니 항성은 태양과 비슷한 G형 주계열성 이다. 이 행성의 최소 질량은 목성보다 약간 더 크다. 항성과 떨어져 있는 평균 거리는 태양과 지구 간격의 절반 정도이다. 그러나 궤도는 찌그러져 있으며, 근일점에서는 수성보다 가까이 접근하고 멀어질 때는 근일점의 두 배 가까운 거리만큼 물러난다. (ko) HD 52265 b (Cayahuanca) – planeta pozasłoneczna typu gazowy olbrzym, o masie podobnej do masy Jowisza. Okrąża gwiazdę HD 52265 (Citalá) po ekscentrycznej orbicie. (pl) HD 52265 b é um planeta extrassolar do tipo gigante gasoso localizado a aproximadamente 92 anos-luz na constelação de Monoceros, orbitando a estrela . Este planeta possui uma massa mínima ligeiramente superior à de Júpiter. A distância média entre o planeta e sua estrela-mãe é metade da distância entre a Terra e o Sol. Sua órbita é excêntrica, durante o periastro o planeta se encontra um pouco mais próximo de HD 52265 do que Mercúrio em relação ao Sol, e durante o apoastro essa distância mais que dobra. (pt) HD 52265 b是一顆距離地球約92光年的太陽系外行星，屬於類木行星，位於麒麟座，母恆星是 HD 52265。該行星的質量下限稍高於木星，和母恆星的平均距離是日地距離的一半。該行星由和各自獨立發現。 (zh) HD 52265 b is a gas giant exoplanet located approximately 98 light-years away in the constellation of Monoceros, orbiting the star HD 52265. The planet has a minimum mass slightly more than that of Jupiter. Mean distance between the planet and the star is half that of Earth from the Sun. It was discovered by both the California and Carnegie Planet Search team and the Geneva Extrasolar Planet Search team independently of each other. By studying the fluctuations of the brightness of a host star, the inclination of the stars equator was determined. This allowed to calculate its true mass, assuming that the planet orbits in the plane of the star's equator. (en) |
| rdfs:label |
HD 52265 b (ar) HD 52265 b (de) HD 52265 b (en) HD 52265 b (in) HD 52265 b (ko) HD 52265 b (pl) HD 52265 b (pt) HD 52265 b (zh) |
| owl:sameAs |
freebase:HD 52265 b yago-res:HD 52265 b wikidata:HD 52265 b dbpedia-ar:HD 52265 b dbpedia-de:HD 52265 b dbpedia-id:HD 52265 b dbpedia-ko:HD 52265 b dbpedia-pl:HD 52265 b dbpedia-pt:HD 52265 b dbpedia-zh:HD 52265 b https://global.dbpedia.org/id/4ym8S |
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wikipedia-en:HD_52265_b?oldid=1036021122&ns=0 |
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wikipedia-en:HD_52265_b |
| foaf:name |
HD 52265 b (en) |
| is dbo:wikiPageRedirects of |
dbr:HD_52265b dbr:Cayahuanca |
| is dbo:wikiPageWikiLink of |
dbr:List_of_exoplanets_detected_by_radial_velocity dbr:List_of_exoplanets_discovered_between_2000–2009 dbr:List_of_proper_names_of_exoplanets dbr:HD_52265 dbr:HD_52265b dbr:List_of_stars_in_Monoceros dbr:Cayahuanca |
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dbr:HD_52265 |
| is foaf:primaryTopic of |
wikipedia-en:HD_52265_b |