http://dbpedia.org/ontology/abstract
|
WASP-15는 바다뱀자리 방향으로 지구로부터 약 1000 광년 떨어져 있는 … WASP-15는 바다뱀자리 방향으로 지구로부터 약 1000 광년 떨어져 있는 항성이다. 겉보기 등급은 약 11로 맨눈으로는 볼 수 없다. 이 별은 태양보다 더 무겁고, 크고, 뜨거우며 밝다. 그러나 대기중 중원소 함량은 태양보다 적다. WASP-15 주위를 도는 외계 행성 WASP-15b가 발견된바 있으며 이 행성은 비정상적으로 반지름이 큰 뜨거운 목성이다. 이처럼 덩치가 큰 이유로 내부 열원 때문에 가열되어 부풀어 올랐을 것으로 보고 있다. 이 별은 슈퍼WASP 프로그램의 일환으로 2006년 관측되었으며 이후 2007년과 2008년에 추가 연구 및 분석이 이루어졌다. 그 결과 통과법 및 도플러 분광법을 이용하여 외계 행성 WASP-15b를 발견하게 되었다. 및 도플러 분광법을 이용하여 외계 행성 WASP-15b를 발견하게 되었다.
, WASP-15, également nommée Nyamien, est une … WASP-15, également nommée Nyamien, est une étoile située à environ 284 pc (∼926 a.l.) de la Terre dans la constellation du Centaure. D'un âge estimé à environ 3,9 milliards d'années, l'étoile est plus massive, plus grande, plus chaude et plus lumineuse que le Soleil. À la fin des années 2000, on y découvre WASP-15b, une exoplanète de taille semblable à celle de Jupiter.te de taille semblable à celle de Jupiter.
, WASP-15 — звезда, которая находится в созвездии Центавра на расстоянии приблизительно 1004 световых года от нас. Вокруг звезды обращается, как минимум, одна планета.
, WASP-15は、うみへび座の方角に約1000光年の距離にある恒星である。見かけの等級は約11等級と暗く、肉眼では見ることができない。
, WASP-15 — зоря на Головній Послідовності спектрального класу F5 з видимою зоряною величиною в смузі V 11m, що розташована приблизно на відстані 1000 світлових років від Землі у напрямку сузір'я Гідра.
, WASP-15 (Nyamien) – gwiazda w gwiazdozbiorze Centaura, odległa o 927 lat świetlnych od Słońca. Wokół WASP-15 orbituje planeta WASP-15 b (Asye). WASP-15 to żółto-biały karzeł, gwiazda ciągu głównego należąca do typu widmowego F.
, WASP-15 is a magnitude 11 star located abo … WASP-15 is a magnitude 11 star located about 1000 light-years away in the constellation Centaurus. The star, which is more massive, larger, hotter, and more luminous than the Sun, is also less metal-rich than the Sun. WASP-15 has one known planet in its orbit, WASP-15b; the planet is a Hot Jupiter with an anomalously high radius, a phenomenon which may be explained by the presence of an internal heat source. The star was first observed by the SuperWASP program in 2006; future measurements in 2007 and 2008, as well as follow-up observations and analysis, eventually led to the discovery of WASP-15b using the transit method and Doppler spectroscopy.e transit method and Doppler spectroscopy.
|
http://dbpedia.org/ontology/wikiPageExternalLink
|
http://media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=WASP-15 +
, http://wasp-planets.net/ +
, https://web.archive.org/web/20120401192714/http:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=WASP-15 +
|
http://dbpedia.org/ontology/wikiPageID
|
17720233
|
http://dbpedia.org/ontology/wikiPageLength
|
10229
|
http://dbpedia.org/ontology/wikiPageRevisionID
|
1093291277
|
http://dbpedia.org/ontology/wikiPageWikiLink
|
http://dbpedia.org/resource/Category:Planetary_systems_with_one_confirmed_planet +
, http://dbpedia.org/resource/List_of_extrasolar_planets +
, http://dbpedia.org/resource/La_Silla_Observatory +
, http://dbpedia.org/resource/Parsec +
, http://dbpedia.org/resource/2MASS +
, http://dbpedia.org/resource/Light_year +
, http://dbpedia.org/resource/Effective_temperature +
, http://dbpedia.org/resource/Light-year +
, http://dbpedia.org/resource/Ivory_Coast +
, http://dbpedia.org/resource/Category:2MASS_objects +
, http://dbpedia.org/resource/Tidal_heating +
, http://dbpedia.org/resource/Kelvin_scale +
, http://dbpedia.org/resource/Star +
, http://dbpedia.org/resource/Solar_radius +
, http://dbpedia.org/resource/EulerCam +
, http://dbpedia.org/resource/Star_catalogue +
, http://dbpedia.org/resource/Constellation +
, http://dbpedia.org/resource/Centaurus_%28constellation%29 +
, http://dbpedia.org/resource/South_African_Astronomical_Observatory +
, http://dbpedia.org/resource/NameExoWorlds +
, http://dbpedia.org/resource/Transit_method +
, http://dbpedia.org/resource/Hot_Jupiter +
, http://dbpedia.org/resource/Leonhard_Euler_Telescope +
, http://dbpedia.org/resource/WASP-15b +
, http://dbpedia.org/resource/Category:Planetary_transit_variables +
, http://dbpedia.org/resource/CORALIE_spectrograph +
, http://dbpedia.org/resource/Doppler_spectroscopy +
, http://dbpedia.org/resource/Apparent_magnitude +
, http://dbpedia.org/resource/Akan_people +
, http://dbpedia.org/resource/Metallicity +
, http://dbpedia.org/resource/International_Astronomical_Union +
, http://dbpedia.org/resource/Category:F-type_main-sequence_stars +
, http://dbpedia.org/resource/SuperWASP +
, http://dbpedia.org/resource/Astronomical_unit +
, http://dbpedia.org/resource/Solar_luminosity +
, http://dbpedia.org/resource/Stellar_classification +
, http://dbpedia.org/resource/Solar_mass +
, http://dbpedia.org/resource/Sun +
, http://dbpedia.org/resource/Category:Centaurus_%28constellation%29 +
, http://dbpedia.org/resource/Category:Wide_Angle_Search_for_Planets +
, http://dbpedia.org/resource/Tycho-2_Catalogue +
|
http://dbpedia.org/property/ageGyr
|
3.9
|
http://dbpedia.org/property/appmag
|
~11.0
, 9.693
, ~11.3
, 9.713
, 9.956
|
http://dbpedia.org/property/appmag1Passband
|
B
|
http://dbpedia.org/property/appmag2Passband
|
R
|
http://dbpedia.org/property/appmag3Passband
|
J
|
http://dbpedia.org/property/appmag4Passband
|
H
|
http://dbpedia.org/property/appmag5Passband
|
K
|
http://dbpedia.org/property/appmagV
|
10.9
|
http://dbpedia.org/property/class
|
F5
|
http://dbpedia.org/property/constell
|
http://dbpedia.org/resource/Centaurus_%28constellation%29 +
|
http://dbpedia.org/property/eccentricity
|
0
|
http://dbpedia.org/property/epe
|
WASP-15
|
http://dbpedia.org/property/epoch
|
J2000
|
http://dbpedia.org/property/exoplanet
|
http://dbpedia.org/resource/WASP-15b +
|
http://dbpedia.org/property/mass
|
0.542
, 1.18
|
http://dbpedia.org/property/metalFe
|
−0.17 ± 0.11
|
http://dbpedia.org/property/pError
|
0.0416
|
http://dbpedia.org/property/parallax
|
3.5168
|
http://dbpedia.org/property/period
|
3.7520656
|
http://dbpedia.org/property/radialV
|
-1.6
|
http://dbpedia.org/property/radius
|
1.477
, 1.428
|
http://dbpedia.org/property/semimajor
|
0.0499
|
http://dbpedia.org/property/simbad
|
WASP-15
|
http://dbpedia.org/property/temperature
|
6300
|
http://dbpedia.org/property/wikiPageUsesTemplate
|
http://dbpedia.org/resource/Template:Short_description +
, http://dbpedia.org/resource/Template:Stars_of_Centaurus +
, http://dbpedia.org/resource/Template:Starbox_end +
, http://dbpedia.org/resource/Template:Starbox_character +
, http://dbpedia.org/resource/Template:Starbox_reference +
, http://dbpedia.org/resource/Template:Val +
, http://dbpedia.org/resource/Template:RA +
, http://dbpedia.org/resource/Template:DEC +
, http://dbpedia.org/resource/Template:Reflist +
, http://dbpedia.org/resource/Template:Starbox_begin +
, http://dbpedia.org/resource/Template:Starbox_catalog +
, http://dbpedia.org/resource/Template:Starbox_astrometry +
, http://dbpedia.org/resource/Template:Starbox_detail +
, http://dbpedia.org/resource/Template:Starbox_observe +
, http://dbpedia.org/resource/Template:Orbitbox_end +
, http://dbpedia.org/resource/Template:OrbitboxPlanet_begin +
, http://dbpedia.org/resource/Template:Sky +
, http://dbpedia.org/resource/Template:Cite_web +
, http://dbpedia.org/resource/Template:OrbitboxPlanet +
, http://dbpedia.org/resource/Template:Good_article +
, http://dbpedia.org/resource/Template:%C2%B1 +
|
http://purl.org/dc/terms/subject
|
http://dbpedia.org/resource/Category:Wide_Angle_Search_for_Planets +
, http://dbpedia.org/resource/Category:Planetary_systems_with_one_confirmed_planet +
, http://dbpedia.org/resource/Category:Centaurus_%28constellation%29 +
, http://dbpedia.org/resource/Category:2MASS_objects +
, http://dbpedia.org/resource/Category:F-type_main-sequence_stars +
, http://dbpedia.org/resource/Category:Planetary_transit_variables +
|
http://purl.org/linguistics/gold/hypernym
|
http://dbpedia.org/resource/Star +
|
http://www.w3.org/ns/prov#wasDerivedFrom
|
http://en.wikipedia.org/wiki/WASP-15?oldid=1093291277&ns=0 +
|
http://xmlns.com/foaf/0.1/isPrimaryTopicOf
|
http://en.wikipedia.org/wiki/WASP-15 +
|
http://xmlns.com/foaf/0.1/name
|
WASP-15
|
owl:sameAs |
http://vi.dbpedia.org/resource/WASP-15 +
, http://ru.dbpedia.org/resource/WASP-15 +
, http://www.wikidata.org/entity/Q2656182 +
, http://fr.dbpedia.org/resource/WASP-15 +
, http://pl.dbpedia.org/resource/WASP-15 +
, http://ko.dbpedia.org/resource/WASP-15 +
, http://uk.dbpedia.org/resource/WASP-15 +
, http://ja.dbpedia.org/resource/WASP-15 +
, http://yago-knowledge.org/resource/WASP-15 +
, http://fa.dbpedia.org/resource/%D8%AF%D8%A8%D9%84%DB%8C%D9%88%D8%A7%DB%8C%E2%80%8C%D8%A7%D8%B3%E2%80%8C%D9%BE%DB%8C-%DB%B1%DB%B5 +
, http://rdf.freebase.com/ns/m.05_5p0r +
, http://dbpedia.org/resource/WASP-15 +
, https://global.dbpedia.org/id/2VmwA +
, http://bn.dbpedia.org/resource/%E0%A6%A1%E0%A6%AC%E0%A7%8D%E0%A6%B2%E0%A6%BF%E0%A6%89%E0%A6%8F%E0%A6%8F%E0%A6%B8%E0%A6%AA%E0%A6%BF_%E0%A7%A7%E0%A7%AB +
|
rdf:type |
http://dbpedia.org/ontology/Star +
, http://dbpedia.org/ontology/Location +
, http://dbpedia.org/class/yago/NaturalObject100019128 +
, http://dbpedia.org/ontology/Place +
, http://dbpedia.org/class/yago/CelestialBody109239740 +
, http://schema.org/Place +
, http://dbpedia.org/class/yago/Star109444100 +
, http://dbpedia.org/class/yago/PhysicalEntity100001930 +
, http://dbpedia.org/ontology/CelestialBody +
, http://dbpedia.org/class/yago/WikicatF-typeStars +
, http://dbpedia.org/class/yago/Variable109468959 +
, http://dbpedia.org/class/yago/WikicatF-typeMain-sequenceStars +
, http://dbpedia.org/class/yago/Thing100002452 +
, http://dbpedia.org/class/yago/Object100002684 +
, http://dbpedia.org/class/yago/WikicatPlanetaryTransitVariables +
, http://dbpedia.org/class/yago/Whole100003553 +
|
rdfs:comment |
WASP-15は、うみへび座の方角に約1000光年の距離にある恒星である。見かけの等級は約11等級と暗く、肉眼では見ることができない。
, WASP-15 — звезда, которая находится в созвездии Центавра на расстоянии приблизительно 1004 световых года от нас. Вокруг звезды обращается, как минимум, одна планета.
, WASP-15 is a magnitude 11 star located abo … WASP-15 is a magnitude 11 star located about 1000 light-years away in the constellation Centaurus. The star, which is more massive, larger, hotter, and more luminous than the Sun, is also less metal-rich than the Sun. WASP-15 has one known planet in its orbit, WASP-15b; the planet is a Hot Jupiter with an anomalously high radius, a phenomenon which may be explained by the presence of an internal heat source. The star was first observed by the SuperWASP program in 2006; future measurements in 2007 and 2008, as well as follow-up observations and analysis, eventually led to the discovery of WASP-15b using the transit method and Doppler spectroscopy.e transit method and Doppler spectroscopy.
, WASP-15 (Nyamien) – gwiazda w gwiazdozbiorze Centaura, odległa o 927 lat świetlnych od Słońca. Wokół WASP-15 orbituje planeta WASP-15 b (Asye). WASP-15 to żółto-biały karzeł, gwiazda ciągu głównego należąca do typu widmowego F.
, WASP-15, également nommée Nyamien, est une … WASP-15, également nommée Nyamien, est une étoile située à environ 284 pc (∼926 a.l.) de la Terre dans la constellation du Centaure. D'un âge estimé à environ 3,9 milliards d'années, l'étoile est plus massive, plus grande, plus chaude et plus lumineuse que le Soleil. À la fin des années 2000, on y découvre WASP-15b, une exoplanète de taille semblable à celle de Jupiter.te de taille semblable à celle de Jupiter.
, WASP-15 — зоря на Головній Послідовності спектрального класу F5 з видимою зоряною величиною в смузі V 11m, що розташована приблизно на відстані 1000 світлових років від Землі у напрямку сузір'я Гідра.
, WASP-15는 바다뱀자리 방향으로 지구로부터 약 1000 광년 떨어져 있는 … WASP-15는 바다뱀자리 방향으로 지구로부터 약 1000 광년 떨어져 있는 항성이다. 겉보기 등급은 약 11로 맨눈으로는 볼 수 없다. 이 별은 태양보다 더 무겁고, 크고, 뜨거우며 밝다. 그러나 대기중 중원소 함량은 태양보다 적다. WASP-15 주위를 도는 외계 행성 WASP-15b가 발견된바 있으며 이 행성은 비정상적으로 반지름이 큰 뜨거운 목성이다. 이처럼 덩치가 큰 이유로 내부 열원 때문에 가열되어 부풀어 올랐을 것으로 보고 있다. 이 별은 슈퍼WASP 프로그램의 일환으로 2006년 관측되었으며 이후 2007년과 2008년에 추가 연구 및 분석이 이루어졌다. 그 결과 통과법 및 도플러 분광법을 이용하여 외계 행성 WASP-15b를 발견하게 되었다. 및 도플러 분광법을 이용하여 외계 행성 WASP-15b를 발견하게 되었다.
|
rdfs:label |
WASP-15
|