About: OGLE-2016-BLG-1190Lb

An Entity of Type: planet, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

OGLE-2016-BLG-1190Lb is an extremely massive exoplanet, with a mass about 13.4 times that of Jupiter (MJ), or is, possibly, a low mass brown dwarf, orbiting the G-dwarf star OGLE-2016-BLG-1190L, located about 22,000 light years from Earth, in the constellation of Sagittarius, in the galactic bulge of the Milky Way.

Property Value
dbo:Planet/orbitalPeriod
  • 1223.6
dbo:abstract
  • OGLE-2016-BLG-1190Lb masa ikaragarria duen exoplaneta bat da, Jupiterren masa 13,4 aldiz biderkatuta lor dezakegu objektu honen masa. Astronomoek oraindik ez dakite seguru nolako objektua den OGLE-2016-BLG-1190Lb, planeta bat izateko masiboegia baita eta nano marroi bat izateko txikiegia, azken objektu hauen ezaugarririk ere ez zaizkio atzeman. Nano hori motako izar baten inguruan biraka dabil, Lur planetatik 22 arg- urtera, Sagittarius konstelazioan, Esne Bidearen barnealdean. Bestalde, gorputz arraro honek beste berezitasun bat gehiago gorde digu, astronomoek egin dituzten ikerketek erakutsi baitute, biraka dabilen izarretik, OGLE-2016-BLG-1190L, hurbilegi dagoela. Izar nagusitik daukan hurbiltasun handiak ezinezko bilakatzen du planeta bat izatea, edozein planeta gune honetan ezingo litzakeelako mantendu, grabitatearen ondorioz izar nagusiak irentsiko lukeelako. (eu)
  • OGLE-2016-BLG-1190Lb is an extremely massive exoplanet, with a mass about 13.4 times that of Jupiter (MJ), or is, possibly, a low mass brown dwarf, orbiting the G-dwarf star OGLE-2016-BLG-1190L, located about 22,000 light years from Earth, in the constellation of Sagittarius, in the galactic bulge of the Milky Way. “Since the existence of the brown dwarf desert is the signature of different formation mechanisms for stars and planets, the extremely close proximity of OGLE-2016-BLG-1190Lb to this desert raises the question of whether it is truly a ‘planet’ (by formation mechanism) and therefore reacts back upon its role tracing the galactic distribution of planets," according to astronomers reporting the findings. (en)
  • OGLE-2016-BLG-1190Lb est une exoplanète extrêmement massive ayant une masse équivalente à 13,4 fois celle de Jupiter. Cet objet céleste est en orbite autour de la naine jaune OGLE-2016-BLG-1190L, situé à environ 22 000 années-lumière de la Terre, dans la constellation du Sagittaire, dans le renflement galactique de la Voie lactée. (fr)
  • OGLE-2016-BLG-1190Lb는 궁수자리에 위치해 있으며, 22,000광년 떨어진 OGLE-2016-BLG-1190L를 도는 외계 행성이다. 목성질량의 약 13.4 배인 질량을 가진 거대한 외계 행성이거나, G형 왜성을 돌고 있는 OGLE-2016-BLG-1190L을 도는 작은 갈색 왜성이다. (ko)
  • OGLE-2016-BLG-1190Lb是一顆質量極高的太陽系外行星，質量約為木星的13.4倍，因此該天體也可能是低質量的棕矮星。它的母恆星是黃矮星 OGLE-2016-BLG-1190L，距離地球約2.2萬光年，在天球上位於人馬座，在銀河系內位於中心核球。 發現OGLE-2016-BLG-1190Lb 的天文學家在報告這項發現時宣稱「由於棕矮星沙漠的存在是行星和恆星不同形成機制的標誌，並且OGLE-2016-BLG-1190Lb 的軌道範圍相當接近棕矮星沙漠範圍。這引發了該天體是否真的是行星的疑問（依照形成機制），並因此反映它在追蹤銀河系內行星分布的角色。」 (zh)
dbo:detectionMethod
  • Gravitational microlensing
dbo:orbitalPeriod
  • 105719040.000000 (xsd:double)
dbo:wikiPageExternalLink
dbo:wikiPageID
  • 55762602 (xsd:integer)
dbo:wikiPageLength
  • 5160 (xsd:nonNegativeInteger)
dbo:wikiPageRevisionID
  • 1092996799 (xsd:integer)
dbo:wikiPageWikiLink
dbp:apsis
  • astron (en)
dbp:discovered
  • 2017 (xsd:integer)
dbp:discoverer
  • Ryu, Y.-H. et al (en)
dbp:discoveryMethod
dbp:discoverySite
dbp:eccentricity
  • 0.420000 (xsd:double)
dbp:inclination
  • 41.200000 (xsd:double)
dbp:mass
  • 13.380000 (xsd:double)
dbp:name
  • OGLE-2016-BLG-1190Lb (en)
dbp:period
  • 1.0571904E8
dbp:star
dbp:wikiPageUsesTemplate
dcterms:subject
rdf:type
rdfs:comment
  • OGLE-2016-BLG-1190Lb est une exoplanète extrêmement massive ayant une masse équivalente à 13,4 fois celle de Jupiter. Cet objet céleste est en orbite autour de la naine jaune OGLE-2016-BLG-1190L, situé à environ 22 000 années-lumière de la Terre, dans la constellation du Sagittaire, dans le renflement galactique de la Voie lactée. (fr)
  • OGLE-2016-BLG-1190Lb는 궁수자리에 위치해 있으며, 22,000광년 떨어진 OGLE-2016-BLG-1190L를 도는 외계 행성이다. 목성질량의 약 13.4 배인 질량을 가진 거대한 외계 행성이거나, G형 왜성을 돌고 있는 OGLE-2016-BLG-1190L을 도는 작은 갈색 왜성이다. (ko)
  • OGLE-2016-BLG-1190Lb是一顆質量極高的太陽系外行星，質量約為木星的13.4倍，因此該天體也可能是低質量的棕矮星。它的母恆星是黃矮星 OGLE-2016-BLG-1190L，距離地球約2.2萬光年，在天球上位於人馬座，在銀河系內位於中心核球。 發現OGLE-2016-BLG-1190Lb 的天文學家在報告這項發現時宣稱「由於棕矮星沙漠的存在是行星和恆星不同形成機制的標誌，並且OGLE-2016-BLG-1190Lb 的軌道範圍相當接近棕矮星沙漠範圍。這引發了該天體是否真的是行星的疑問（依照形成機制），並因此反映它在追蹤銀河系內行星分布的角色。」 (zh)
  • OGLE-2016-BLG-1190Lb masa ikaragarria duen exoplaneta bat da, Jupiterren masa 13,4 aldiz biderkatuta lor dezakegu objektu honen masa. Astronomoek oraindik ez dakite seguru nolako objektua den OGLE-2016-BLG-1190Lb, planeta bat izateko masiboegia baita eta nano marroi bat izateko txikiegia, azken objektu hauen ezaugarririk ere ez zaizkio atzeman. Nano hori motako izar baten inguruan biraka dabil, Lur planetatik 22 arg- urtera, Sagittarius konstelazioan, Esne Bidearen barnealdean. (eu)
  • OGLE-2016-BLG-1190Lb is an extremely massive exoplanet, with a mass about 13.4 times that of Jupiter (MJ), or is, possibly, a low mass brown dwarf, orbiting the G-dwarf star OGLE-2016-BLG-1190L, located about 22,000 light years from Earth, in the constellation of Sagittarius, in the galactic bulge of the Milky Way. (en)
rdfs:label
  • OGLE-2016-BLG-1190Lb (eu)
  • OGLE-2016-BLG-1190L b (fr)
  • OGLE-2016-BLG-1190Lb (ko)
  • OGLE-2016-BLG-1190Lb (en)
  • OGLE-2016-BLG-1190Lb (zh)
owl:sameAs
prov:wasDerivedFrom
foaf:isPrimaryTopicOf
foaf:name
  • OGLE-2016-BLG-1190Lb (en)
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