Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q132124> ?p ?o }
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- Q132124 subject Q6392646.
- Q132124 subject Q7009248.
- Q132124 subject Q7033876.
- Q132124 subject Q7217167.
- Q132124 subject Q7217174.
- Q132124 subject Q9142574.
- Q132124 abstract "OGLE-TR-132b is an extrasolar planet orbiting the star OGLE-TR-132.In 2003 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements were necessary to calculate the mass of the body. In 2004 the object was proved to be a new transiting extrasolar planet.The planet has a mass 1.14 times that of Jupiter. Since the planet's inclination is known, this represents the best measured true mass of the planet, rather than simply the minimum mass as is the case when the inclination is unknown. It orbits the star (OGLE-TR-132) in an extremely close orbit, even closer than the famous planets 51 Pegasi b and HD 209458 b. The planet races around the star every 1 day 16.6 hours. The radius of the planet is only 18% larger than Jupiter's, despite the heating effect by the star. Planets of its kind are sometimes called "super-hot Jupiters".".
- Q132124 thumbnail Exoplanet_Comparison_OGLE-TR-132_b.png?width=300.
- Q132124 wikiPageExternalLink planete.php?etoile=OGLE-TR-132&planete=b.
- Q132124 wikiPageWikiLink Q101600.
- Q132124 wikiPageWikiLink Q1032158.
- Q132124 wikiPageWikiLink Q10470.
- Q132124 wikiPageWikiLink Q1069393.
- Q132124 wikiPageWikiLink Q240105.
- Q132124 wikiPageWikiLink Q242309.
- Q132124 wikiPageWikiLink Q272085.
- Q132124 wikiPageWikiLink Q319.
- Q132124 wikiPageWikiLink Q382979.
- Q132124 wikiPageWikiLink Q4112212.
- Q132124 wikiPageWikiLink Q44559.
- Q132124 wikiPageWikiLink Q523.
- Q132124 wikiPageWikiLink Q5893.
- Q132124 wikiPageWikiLink Q591022.
- Q132124 wikiPageWikiLink Q634.
- Q132124 wikiPageWikiLink Q6392646.
- Q132124 wikiPageWikiLink Q675076.
- Q132124 wikiPageWikiLink Q6888.
- Q132124 wikiPageWikiLink Q7009248.
- Q132124 wikiPageWikiLink Q7033876.
- Q132124 wikiPageWikiLink Q7217167.
- Q132124 wikiPageWikiLink Q7217174.
- Q132124 wikiPageWikiLink Q9142574.
- Q132124 wikiPageWikiLink Q954788.
- Q132124 type Place.
- Q132124 type CelestialBody.
- Q132124 type Location.
- Q132124 type Place.
- Q132124 type Planet.
- Q132124 type Thing.
- Q132124 type Q634.
- Q132124 comment "OGLE-TR-132b is an extrasolar planet orbiting the star OGLE-TR-132.In 2003 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements were necessary to calculate the mass of the body. In 2004 the object was proved to be a new transiting extrasolar planet.The planet has a mass 1.14 times that of Jupiter.".
- Q132124 label "OGLE-TR-132b".
- Q132124 depiction Exoplanet_Comparison_OGLE-TR-132_b.png.