Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q5178080> ?p ?o }
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- Q5178080 subject Q10657.
- Q5178080 subject Q8789073.
- Q5178080 abstract "HD 136118 b is a brown dwarf located approximately 171 light-years away in the constellation of Serpens Cauda. This object had a minimum mass of 11.9 times that of Jupiter. Due to its high mass the planet is likely to be very hot and possibly glowing faintly. The lower limit on its mass is only slightly less than the deuterium burning threshold that some astronomers use to distinguish between planets and brown dwarfs. Depending on the inclination of its orbit, the true mass could be above this limit. The orbit of the object is located at the average distance of 1.45 astronomical units from the parent star, taking 40 months to complete one eccentric orbit.On November 25, 2009, its inclination was calculated to be 163.1° and its true mass 42 times that of Jupiter, classifying this as a brown dwarf.".
- Q5178080 wikiPageExternalLink planet.php?p1=HD+136118&p2=b.
- Q5178080 wikiPageExternalLink etoile.php?nom=HD+136118.
- Q5178080 wikiPageWikiLink Q101600.
- Q5178080 wikiPageWikiLink Q10657.
- Q5178080 wikiPageWikiLink Q15704567.
- Q5178080 wikiPageWikiLink Q171594.
- Q5178080 wikiPageWikiLink Q1811.
- Q5178080 wikiPageWikiLink Q2273386.
- Q5178080 wikiPageWikiLink Q2306635.
- Q5178080 wikiPageWikiLink Q319.
- Q5178080 wikiPageWikiLink Q4112212.
- Q5178080 wikiPageWikiLink Q448946.
- Q5178080 wikiPageWikiLink Q456119.
- Q5178080 wikiPageWikiLink Q531.
- Q5178080 wikiPageWikiLink Q8789073.
- Q5178080 wikiPageWikiLink Q8910.
- Q5178080 wikiPageWikiLink Q8928.
- Q5178080 wikiPageWikiLink Q964623.
- Q5178080 wikiPageWikiLink Q99.
- Q5178080 type Place.
- Q5178080 type CelestialBody.
- Q5178080 type Location.
- Q5178080 type Place.
- Q5178080 type Planet.
- Q5178080 type Thing.
- Q5178080 type Q634.
- Q5178080 comment "HD 136118 b is a brown dwarf located approximately 171 light-years away in the constellation of Serpens Cauda. This object had a minimum mass of 11.9 times that of Jupiter. Due to its high mass the planet is likely to be very hot and possibly glowing faintly. The lower limit on its mass is only slightly less than the deuterium burning threshold that some astronomers use to distinguish between planets and brown dwarfs.".
- Q5178080 label "HD 136118 b".