| http://dbpedia.org/ontology/Planet/apoapsis
|
2.6927616726E8
|
| http://dbpedia.org/ontology/Planet/orbitalPeriod
|
409.08
, 1.0
|
| http://dbpedia.org/ontology/Planet/periapsis
|
9.5742637248E7
|
| http://dbpedia.org/ontology/abstract
|
HD 154857 b adalah sebuah planet luar surya yang terletak sekitar 207,31 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 154857 b memiliki massa sebesar 2,45 massa Jupiter.
, HD 154857 b ist ein Exoplanet, der den gel … HD 154857 b ist ein Exoplanet, der den gelben Zwerg HD 154857 umrundet. Er wurde mit Hilfe der Radialgeschwindigkeitsmethode entdeckt (Publikation von McCarthy et al. im Jahr 2004). Der Exoplanet umkreist den Zentralstern mit einer Periode von 398,5 Tagen in einer Entfernung von ca. 1,1 Astronomischen Einheiten und hat eine Mindestmasse von ca. 1,9 Jupitermassen.ne Mindestmasse von ca. 1,9 Jupitermassen.
, HD 154857 b is an extrasolar planet approximately 224 light years away in the constellation of Ara. This is a gas giant mass that orbits the star in an eccentric orbit. This planet was detected by using Anglo-Australian Telescope (AAT) UCLE spectrometer.
, HD 154857 b는 지구로부터 제단자리 방향으로 약 224광년 떨어진 곳에 있는 외계 행성이다. 질량이 크기 때문에 가스 행성으로 볼 수 있으며, 항성을 이심률 큰 궤도를 그리면서 돌고 있다. 2004년 오스트레일리아 소재 앵글로-오스트레일리안 망원경을 이용, 매커시 연구진이 도플러 효과를 응용하여 발견했다.
, إتش دي 154857 بي (بالإنجليزية: HD 154857 b) الذي يرمز له بالرمز HD 154857b، هو كوكب خارج المجموعة الشمسية، في كوكبة المجمرة، يتبع .
, HD 154857 b é um planeta extrassolar que o … HD 154857 b é um planeta extrassolar que orbita a estrela subgigante de classe G HD 154857, localizada a aproximadamente 210 anos-luz (64 parsecs) da Terra na constelação de Ara. É um gigante gasoso com uma massa mínima de 2,24 ± 0,05 vezes a massa de Júpiter. Orbita a estrela a uma distância média de 1,29 UA em 409 dias, com uma excentricidade moderada de 0,46. Foi detectado em 2004 pelo espectrômetro do Telescópio Anglo-Australiano.ctrômetro do Telescópio Anglo-Australiano.
, HD 154857 b是一顆距離地球約209光年的太陽系外行星，位於天壇座。該行星是在高離心率軌道上的氣體巨行星。天文學家使用澳洲英澳天文台的英澳望遠鏡 UCLE 光譜儀進行觀測而發現了它。
|
| http://dbpedia.org/ontology/apoapsis
|
269276167260
|
| http://dbpedia.org/ontology/detectionMethod
|
Radial velocity
|
| http://dbpedia.org/ontology/discoverer
|
http://dbpedia.org/resource/Australia +
, http://dbpedia.org/resource/Anglo-Australian_Telescope +
|
| http://dbpedia.org/ontology/orbitalPeriod
|
35344512
, 86400
|
| http://dbpedia.org/ontology/periapsis
|
95742637248
|
| http://dbpedia.org/ontology/wikiPageExternalLink
|
http://news.bbc.co.uk/1/hi/sci/tech/1065910.stm +
, https://web.archive.org/web/20071203100742/http:/media4.obspm.fr/exoplanets/base/planete.php%3Fetoile=HD%2B154857&planete=b +
, http://exoplanet.eu/star.php%3Fst=HD%2B154857 +
, http://www.phys.unsw.edu.au/~cgt/planet/AAPS_Home.html +
|
| http://dbpedia.org/ontology/wikiPageID
|
16782350
|
| http://dbpedia.org/ontology/wikiPageLength
|
3333
|
| http://dbpedia.org/ontology/wikiPageRevisionID
|
1021302120
|
| http://dbpedia.org/ontology/wikiPageWikiLink
|
http://dbpedia.org/resource/Category:Giant_planets +
, http://dbpedia.org/resource/Extrasolar_planet +
, http://dbpedia.org/resource/Category:Exoplanets_detected_by_radial_velocity +
, http://dbpedia.org/resource/Year +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_in_2004 +
, http://dbpedia.org/resource/Day +
, http://dbpedia.org/resource/Category:Ara_%28constellation%29 +
, http://dbpedia.org/resource/Light_year +
, http://dbpedia.org/resource/Spectrometer +
, http://dbpedia.org/resource/Ara_%28constellation%29 +
, http://dbpedia.org/resource/HD_154857 +
, http://dbpedia.org/resource/Constellation +
, http://dbpedia.org/resource/Radial_velocity +
, http://dbpedia.org/resource/Gas_giant +
, http://dbpedia.org/resource/Anglo-Australian_Telescope +
|
| http://dbpedia.org/property/apsis
|
astron
|
| http://dbpedia.org/property/argPeri
|
59
|
| http://dbpedia.org/property/discovered
|
2004
|
| http://dbpedia.org/property/discoverer
|
http://dbpedia.org/resource/Anglo-Australian_Telescope +
, McCarthy et al.
|
| http://dbpedia.org/property/discoveryMethod
|
http://dbpedia.org/resource/Radial_velocity +
|
| http://dbpedia.org/property/discoverySite
|
http://www.phys.unsw.edu.au/~cgt/planet/AAPS_Home.html +
|
| http://dbpedia.org/property/eccentricity
|
0.47
|
| http://dbpedia.org/property/mass
|
>1.8±0.4
|
| http://dbpedia.org/property/name
|
HD 154857 b
|
| http://dbpedia.org/property/period
|
3.5344512E7
, 86400.0
|
| http://dbpedia.org/property/semiAmplitude
|
50.4
|
| http://dbpedia.org/property/star
|
http://dbpedia.org/resource/HD_154857 +
|
| http://dbpedia.org/property/timePeriastron
|
2450346
|
| http://dbpedia.org/property/wikiPageUsesTemplate
|
http://dbpedia.org/resource/Template:Jupiter_mass +
, http://dbpedia.org/resource/Template:Infobox_planet +
, http://dbpedia.org/resource/Template:Convert +
, http://dbpedia.org/resource/Template:Flag +
, http://dbpedia.org/resource/Template:Stars_of_Ara +
, http://dbpedia.org/resource/Template:Short_description +
, http://dbpedia.org/resource/Template:Earth_mass +
, http://dbpedia.org/resource/Template:Sky +
, http://dbpedia.org/resource/Template:Reflist +
, http://dbpedia.org/resource/Template:Extrasolar-planet-stub +
, http://dbpedia.org/resource/Template:Cite_encyclopedia +
|
| http://purl.org/dc/terms/subject
|
http://dbpedia.org/resource/Category:Exoplanets_detected_by_radial_velocity +
, http://dbpedia.org/resource/Category:Ara_%28constellation%29 +
, http://dbpedia.org/resource/Category:Exoplanets_discovered_in_2004 +
, http://dbpedia.org/resource/Category:Giant_planets +
|
| http://purl.org/linguistics/gold/hypernym
|
http://dbpedia.org/resource/Planet +
|
| http://www.w3.org/ns/prov#wasDerivedFrom
|
http://en.wikipedia.org/wiki/HD_154857_b?oldid=1021302120&ns=0 +
|
| http://xmlns.com/foaf/0.1/homepage
|
http://www.phys.unsw.edu.au/~cgt/planet/AAPS_Home.html +
|
| http://xmlns.com/foaf/0.1/isPrimaryTopicOf
|
http://en.wikipedia.org/wiki/HD_154857_b +
|
| http://xmlns.com/foaf/0.1/name
|
HD 154857 b
|
| owl:sameAs |
http://zh.dbpedia.org/resource/HD_154857_b +
, http://www.wikidata.org/entity/Q841901 +
, http://ar.dbpedia.org/resource/HD_154857_b +
, http://rdf.freebase.com/ns/m.04f7khb +
, http://de.dbpedia.org/resource/HD_154857_b +
, http://fi.dbpedia.org/resource/HD_154857_b +
, http://dbpedia.org/resource/HD_154857_b +
, http://pt.dbpedia.org/resource/HD_154857_b +
, http://yago-knowledge.org/resource/HD_154857_b +
, http://id.dbpedia.org/resource/HD_154857_b +
, https://global.dbpedia.org/id/4ziaD +
, http://ko.dbpedia.org/resource/HD_154857_b +
, http://lt.dbpedia.org/resource/HD_154857_b +
|
| rdf:type |
http://dbpedia.org/class/yago/NaturalObject100019128 +
, http://dbpedia.org/ontology/Planet +
, http://dbpedia.org/class/yago/GasGiant109322087 +
, http://dbpedia.org/class/yago/WikicatGasGiants +
, http://www.wikidata.org/entity/Q634 +
, http://dbpedia.org/class/yago/Planet109394007 +
, http://schema.org/Place +
, http://dbpedia.org/ontology/Place +
, http://dbpedia.org/ontology/Location +
, http://dbpedia.org/class/yago/CelestialBody109239740 +
, http://dbpedia.org/ontology/CelestialBody +
, http://dbpedia.org/class/yago/PhysicalEntity100001930 +
, http://dbpedia.org/class/yago/Whole100003553 +
, http://dbpedia.org/class/yago/Object100002684 +
|
| rdfs:comment |
HD 154857 b is an extrasolar planet approximately 224 light years away in the constellation of Ara. This is a gas giant mass that orbits the star in an eccentric orbit. This planet was detected by using Anglo-Australian Telescope (AAT) UCLE spectrometer.
, HD 154857 b é um planeta extrassolar que o … HD 154857 b é um planeta extrassolar que orbita a estrela subgigante de classe G HD 154857, localizada a aproximadamente 210 anos-luz (64 parsecs) da Terra na constelação de Ara. É um gigante gasoso com uma massa mínima de 2,24 ± 0,05 vezes a massa de Júpiter. Orbita a estrela a uma distância média de 1,29 UA em 409 dias, com uma excentricidade moderada de 0,46. Foi detectado em 2004 pelo espectrômetro do Telescópio Anglo-Australiano.ctrômetro do Telescópio Anglo-Australiano.
, HD 154857 b是一顆距離地球約209光年的太陽系外行星，位於天壇座。該行星是在高離心率軌道上的氣體巨行星。天文學家使用澳洲英澳天文台的英澳望遠鏡 UCLE 光譜儀進行觀測而發現了它。
, HD 154857 b adalah sebuah planet luar surya yang terletak sekitar 207,31 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 154857 b memiliki massa sebesar 2,45 massa Jupiter.
, HD 154857 b ist ein Exoplanet, der den gel … HD 154857 b ist ein Exoplanet, der den gelben Zwerg HD 154857 umrundet. Er wurde mit Hilfe der Radialgeschwindigkeitsmethode entdeckt (Publikation von McCarthy et al. im Jahr 2004). Der Exoplanet umkreist den Zentralstern mit einer Periode von 398,5 Tagen in einer Entfernung von ca. 1,1 Astronomischen Einheiten und hat eine Mindestmasse von ca. 1,9 Jupitermassen.ne Mindestmasse von ca. 1,9 Jupitermassen.
, HD 154857 b는 지구로부터 제단자리 방향으로 약 224광년 떨어진 곳에 있는 외계 행성이다. 질량이 크기 때문에 가스 행성으로 볼 수 있으며, 항성을 이심률 큰 궤도를 그리면서 돌고 있다. 2004년 오스트레일리아 소재 앵글로-오스트레일리안 망원경을 이용, 매커시 연구진이 도플러 효과를 응용하여 발견했다.
, إتش دي 154857 بي (بالإنجليزية: HD 154857 b) الذي يرمز له بالرمز HD 154857b، هو كوكب خارج المجموعة الشمسية، في كوكبة المجمرة، يتبع .
|
| rdfs:label |
HD 154857 b
|
