| dbo:Planet/apoapsis |
1.37630041044E7 |
| dbo:Planet/averageSpeed |
120.0 |
| dbo:Planet/periapsis |
7180697.7936 |
| dbo:Planet/temperature |
1496.0 |
| dbo:abstract |
HD 118203 b (بالإنجليزية: HD 118203 b) الذي يرمز له بالرمز HD 118203b، هو كوكب خارج المجموعة الشمسية، في كوكبة الدب الأكبر، يتبع . (ar) HD 118203 b ist ein Exoplanet, der den Hauptreihenstern HD 118203 mit einer Umlaufperiode von 6,13 Tagen umrundet. Das Objekt wurde im Jahr 2005 von da Silva et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die große Halbachse seiner Umlaufbahn misst rund 0,07 Astronomischen Einheiten und es weist eine Mindestmasse von etwas mehr als 2 Jupitermassen auf. (de) HD 118203 b is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star HD 118203 at a distance of 0.07 astronomical units. The exact mass was not known since inclination was not known until TESS detected the planet. This hot Jupiter is unusual since it has relatively high eccentricity of 0.31. The planet HD 118203 b is named Staburags. The name was selected in the NameExoWorlds campaign by Latvia, during the 100th anniversary of the IAU. Staburags is the name of a character from the Latvian poem , and denotes a rock with symbolic meaning in literature and history. HD 118203 b was discovered in August 2005 in Haute-Provence Observatory in France by Da Silva who used the doppler spectroscopy to look for shifts in the star's spectrum caused by the planet's gravity as the planet orbits the star. In 2019 the transits of the planet were detected with the Transiting Exoplanet Survey Satellite. The host star is one of the brightest stars for transiting planets and HD 118203 b is therefore a good target for follow-up observations. (en) HD 118203 b adalah sebuah planet luar surya yang terletak sekitar 301,74 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 118203 b memiliki massa sebesar 2,79 massa Jupiter. (in) HD 118203 b는 어머니 항성 주위를 0.07 천문단위 거리를 두고 6.13일(147시간)에 1회 공전하는, 목성형 행성이다. 최소 질량은 목성의 2.14배이지만 발견 방법의 한계 때문에 궤도경사각을 모르는 한 실제 질량은 더 클 가능성이 높다. 항성으로부터 가까움에도 이 행성의 공전궤도 이심률은 0.31로 큰데, 이는 뜨거운 목성 중에서는 흔치 않은 사례이다. 2005년 8월 프랑스 소재 Haute-Provence 천문대에서 다 실바가 이끄는 연구진이 이 행성을 발견했다. 발견에는 도플러 분광법이 사용되었다. (ko) |
| dbo:apoapsis |
13763004104.400000 (xsd:double) |
| dbo:averageSpeed |
432000.000000 (xsd:double) |
| dbo:detectionMethod |
Doppler spectroscopy (ELODIE) |
| dbo:discovered |
2005-08-22 (xsd:date) |
| dbo:periapsis |
7180697793.600000 (xsd:double) |
| dbo:temperature |
1496.000000 (xsd:double) |
| dbo:wikiPageExternalLink |
http://media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+118203 https://web.archive.org/web/20091125001831/http:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+118203 |
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dbpedia-ru:HD_118203 |
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| dbo:wikiPageRevisionID |
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| dbo:wikiPageWikiLink |
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| dbp:apsis |
astron (en) |
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120 (xsd:integer) |
| dbp:density |
1.850000 (xsd:double) |
| dbp:discovered |
2005-08-22 (xsd:date) |
| dbp:discoverer |
Da Silva et al. (en) |
| dbp:discoveryMethod |
dbr:Doppler_spectroscopy (en) |
| dbp:discoverySite |
dbr:France dbr:Haute-Provence_Observatory |
| dbp:eccentricity |
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| dbp:name |
HD 118203 b (en) |
| dbp:period |
d (en) |
| dbp:star |
dbr:HD_118203 |
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| dcterms:subject |
dbc:Exoplanets_detected_by_radial_velocity dbc:Exoplanets_discovered_in_2005 dbc:Exoplanets_with_proper_names dbc:Giant_planets dbc:Ursa_Major_(constellation) dbc:Transiting_exoplanets |
| gold:hypernym |
dbr:Planet |
| 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 118203 b (بالإنجليزية: HD 118203 b) الذي يرمز له بالرمز HD 118203b، هو كوكب خارج المجموعة الشمسية، في كوكبة الدب الأكبر، يتبع . (ar) HD 118203 b ist ein Exoplanet, der den Hauptreihenstern HD 118203 mit einer Umlaufperiode von 6,13 Tagen umrundet. Das Objekt wurde im Jahr 2005 von da Silva et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die große Halbachse seiner Umlaufbahn misst rund 0,07 Astronomischen Einheiten und es weist eine Mindestmasse von etwas mehr als 2 Jupitermassen auf. (de) HD 118203 b adalah sebuah planet luar surya yang terletak sekitar 301,74 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 118203 b memiliki massa sebesar 2,79 massa Jupiter. (in) HD 118203 b는 어머니 항성 주위를 0.07 천문단위 거리를 두고 6.13일(147시간)에 1회 공전하는, 목성형 행성이다. 최소 질량은 목성의 2.14배이지만 발견 방법의 한계 때문에 궤도경사각을 모르는 한 실제 질량은 더 클 가능성이 높다. 항성으로부터 가까움에도 이 행성의 공전궤도 이심률은 0.31로 큰데, 이는 뜨거운 목성 중에서는 흔치 않은 사례이다. 2005년 8월 프랑스 소재 Haute-Provence 천문대에서 다 실바가 이끄는 연구진이 이 행성을 발견했다. 발견에는 도플러 분광법이 사용되었다. (ko) HD 118203 b is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star HD 118203 at a distance of 0.07 astronomical units. The exact mass was not known since inclination was not known until TESS detected the planet. This hot Jupiter is unusual since it has relatively high eccentricity of 0.31. The planet HD 118203 b is named Staburags. The name was selected in the NameExoWorlds campaign by Latvia, during the 100th anniversary of the IAU. Staburags is the name of a character from the Latvian poem , and denotes a rock with symbolic meaning in literature and history. (en) |
| rdfs:label |
HD 118203 b (ar) HD 118203 b (de) HD 118203 b (en) HD 118203 b (in) HD 118203 b (ko) |
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freebase:HD 118203 b yago-res:HD 118203 b wikidata:HD 118203 b dbpedia-ar:HD 118203 b dbpedia-de:HD 118203 b dbpedia-id:HD 118203 b dbpedia-ko:HD 118203 b https://global.dbpedia.org/id/51RQr |
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wikipedia-en:HD_118203_b?oldid=1122552333&ns=0 |
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HD 118203 b (en) |
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