| dbo:Planet/apoapsis |
5.01152866845E7 |
| dbo:Planet/averageSpeed |
46.8 |
| dbo:Planet/orbitalPeriod |
0.17999999999999997 70.45672499999999 |
| dbo:Planet/periapsis |
1.15190360439E7 |
| dbo:abstract |
HD 101930 b (بالإنجليزية: HD 101930 b) الذي يرمز له بالرمز HD 101930b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع . (ar) HD 101930 b is an extrasolar planet orbiting the star HD 101930. It has a minimum mass a third of Jupiter's, nearly the same as Saturn's so it is thought to be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric. (en) HD 101930 b adalah sebuah planet luar surya yang terletak sekitar 98,01 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 101930 b memiliki massa sebesar 0,25 massa Jupiter. (in) HD 101930 b는 항성 을 돌고 있는 외계 행성이다. 최소 질량은 목성의 3분의 1이 되지 않는데 이는 토성과 거의 비슷한 값이다. 질량으로 볼 때 가스 행성으로 분류할 수 있다. 항성으로부터의 거리는 태양~수성 정도이며, 공전 궤도는 약간 찌그러져 있다. (ko) HD 101930 b— планета-гигант, обращающаяся вокруг оранжевого карлика, в созвездии Живописца, находящегося на расстоянии 99 световых лет от Земли. Открытие было совершено методом доплеровской спектроскопии с помощью телескопа HARPS 14 февраля 2005 года. (ru) HD 101930b是一颗位于半人马座、距离地球99.42光年的系外行星，其母星为HD 101930。该行星的质量下限为1/3倍木星质量，接近土星的质量，因此被认为属于类木行星。其轨道与其母星的距离比水星轨道与太阳的距离还小，并带有轻微的离心率。 (zh) |
| dbo:apoapsis |
50115286684.500000 (xsd:double) |
| dbo:averageSpeed |
168480.000000 (xsd:double) |
| dbo:detectionMethod |
Doppler spectroscopy (HARPS) |
| dbo:discovered |
2005-02-14 (xsd:date) |
| dbo:discoverer |
dbr:Michel_Mayor dbr:C._Lovis dbr:F._Pepe |
| dbo:orbitalPeriod |
15552.000000 (xsd:double) 6087461.040000 (xsd:double) |
| dbo:periapsis |
11519036043.900000 (xsd:double) |
| dbo:wikiPageExternalLink |
http://media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+101930 https://web.archive.org/web/20160303171249/https:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+101930 |
| dbo:wikiPageID |
16796941 (xsd:integer) |
| dbo:wikiPageInterLanguageLink |
dbpedia-de:HD_101930_b |
| dbo:wikiPageLength |
3004 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID |
1011306214 (xsd:integer) |
| dbo:wikiPageWikiLink |
dbr:Saturn dbr:Day dbr:Doppler_spectroscopy dbc:Exoplanets_detected_by_radial_velocity dbc:Exoplanets_discovered_in_2005 dbc:Giant_planets dbr:Gas_giant dbr:La_Silla_Observatory dbr:Star dbr:Minimum_mass dbr:Extrasolar_planet dbc:Centaurus_(constellation) dbr:HD_101930 dbr:Jupiter dbr:Year dbr:HARPS dbr:Mercury_(planet) dbr:Michel_Mayor dbr:C._Lovis dbr:F._Pepe dbr:Eccentricity_(orbit) |
| dbp:apsis |
astron (en) |
| dbp:argPeri |
251 (xsd:integer) |
| dbp:avgSpeed |
46.800000 (xsd:double) |
| dbp:discovered |
2005-02-14 (xsd:date) |
| dbp:discoverer |
dbr:Michel_Mayor dbr:C._Lovis Pepe et al. (en) |
| dbp:discoveryMethod |
dbr:Doppler_spectroscopy (en) |
| dbp:discoverySite |
dbr:La_Silla_Observatory |
| dbp:eccentricity |
0.110000 (xsd:double) |
| dbp:mass |
(en) >0.30 (en) |
| dbp:name |
HD 101930 b (en) |
| dbp:period |
15551.999999999996 6087461.039999999 |
| dbp:semiAmplitude |
18.100000 (xsd:double) |
| dbp:star |
dbr:HD_101930 |
| dbp:timePeriastron |
2453145 (xsd:integer) |
| dbp:wikiPageUsesTemplate |
dbt:Cite_web dbt:Convert dbt:Extrasolar-planet-stub dbt:Infobox_planet dbt:Jupiter_mass dbt:Reflist dbt:Short_description dbt:Sky dbt:Earth_mass dbt:Centaurus |
| dcterms:subject |
dbc:Exoplanets_detected_by_radial_velocity dbc:Exoplanets_discovered_in_2005 dbc:Giant_planets dbc:Centaurus_(constellation) |
| 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 101930 b (بالإنجليزية: HD 101930 b) الذي يرمز له بالرمز HD 101930b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع . (ar) HD 101930 b is an extrasolar planet orbiting the star HD 101930. It has a minimum mass a third of Jupiter's, nearly the same as Saturn's so it is thought to be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric. (en) HD 101930 b adalah sebuah planet luar surya yang terletak sekitar 98,01 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 101930 b memiliki massa sebesar 0,25 massa Jupiter. (in) HD 101930 b는 항성 을 돌고 있는 외계 행성이다. 최소 질량은 목성의 3분의 1이 되지 않는데 이는 토성과 거의 비슷한 값이다. 질량으로 볼 때 가스 행성으로 분류할 수 있다. 항성으로부터의 거리는 태양~수성 정도이며, 공전 궤도는 약간 찌그러져 있다. (ko) HD 101930 b— планета-гигант, обращающаяся вокруг оранжевого карлика, в созвездии Живописца, находящегося на расстоянии 99 световых лет от Земли. Открытие было совершено методом доплеровской спектроскопии с помощью телескопа HARPS 14 февраля 2005 года. (ru) HD 101930b是一颗位于半人马座、距离地球99.42光年的系外行星，其母星为HD 101930。该行星的质量下限为1/3倍木星质量，接近土星的质量，因此被认为属于类木行星。其轨道与其母星的距离比水星轨道与太阳的距离还小，并带有轻微的离心率。 (zh) |
| rdfs:label |
HD 101930 b (ar) HD 101930 b (en) HD 101930 b (in) HD 101930 Ab (fr) HD 101930 b (ko) HD 101930 b (ru) HD 101930b (zh) |
| owl:sameAs |
freebase:HD 101930 b yago-res:HD 101930 b wikidata:HD 101930 b dbpedia-ar:HD 101930 b dbpedia-fr:HD 101930 b dbpedia-id:HD 101930 b dbpedia-ko:HD 101930 b dbpedia-ru:HD 101930 b dbpedia-zh:HD 101930 b https://global.dbpedia.org/id/7cZo |
| prov:wasDerivedFrom |
wikipedia-en:HD_101930_b?oldid=1011306214&ns=0 |
| foaf:isPrimaryTopicOf |
wikipedia-en:HD_101930_b |
| foaf:name |
HD 101930 b (en) |
| is dbo:wikiPageRedirects of |
dbr:HD_101930b |
| is dbo:wikiPageWikiLink of |
dbr:List_of_exoplanets_detected_by_radial_velocity dbr:List_of_exoplanets_discovered_between_2000–2009 dbr:HD_101930 dbr:High_Accuracy_Radial_Velocity_Planet_Searcher dbr:HD_101930b dbr:List_of_stars_in_Centaurus |
| is dbp:exoplanet of |
dbr:HD_101930 |
| is foaf:primaryTopic of |
wikipedia-en:HD_101930_b |