Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q1077290> ?p ?o }
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- Q1077290 subject Q6392646.
- Q1077290 subject Q6421057.
- Q1077290 subject Q7009278.
- Q1077290 subject Q7217174.
- Q1077290 subject Q7233310.
- Q1077290 abstract "HD 210277 b is an extrasolar planet orbiting the star HD 210277. It was discovered in September 1998 by the California and Carnegie Planet Search team using the highly successful radial velocity method. The planet is at least 24% more massive than Jupiter. The mean distance of the planet from the star is slightly more than Earth's distance from the Sun. However, the orbit is very eccentric, so at periastron this distance is almost halved, and at apastron it is as distant as Mars is from the Sun.In 2000, a group of scientists proposed, based on preliminary data from the Hipparcos astrometrical satellite, that the planet would have an inclination of 175.8° and a true mass of 18 times Jupiter making it a brown dwarf instead of a planet. However these measurements were later proved useful only for upper limits of inclination. If the planet orbits in the same plane as the claimed circumstellar disk, which seems a plausible assumption, it would have an inclination of 40° and an absolute mass of 2.2 times Jupiter, however later observations failed to confirm the disk's existence.".
- Q1077290 wikiPageExternalLink etoile.php?nom=HD+210277.
- Q1077290 wikiPageExternalLink hd210277.shtml.
- Q1077290 wikiPageExternalLink planete.php?etoile=HD+210277&planete=b.
- Q1077290 wikiPageExternalLink atlas_skymap.cfm?Planet=125.
- Q1077290 wikiPageWikiLink Q101600.
- Q1077290 wikiPageWikiLink Q10576.
- Q1077290 wikiPageWikiLink Q111.
- Q1077290 wikiPageWikiLink Q1563271.
- Q1077290 wikiPageWikiLink Q181505.
- Q1077290 wikiPageWikiLink Q2.
- Q1077290 wikiPageWikiLink Q208474.
- Q1077290 wikiPageWikiLink Q2273386.
- Q1077290 wikiPageWikiLink Q240105.
- Q1077290 wikiPageWikiLink Q26540.
- Q1077290 wikiPageWikiLink Q319.
- Q1077290 wikiPageWikiLink Q4112212.
- Q1077290 wikiPageWikiLink Q44559.
- Q1077290 wikiPageWikiLink Q555846.
- Q1077290 wikiPageWikiLink Q6392646.
- Q1077290 wikiPageWikiLink Q6421057.
- Q1077290 wikiPageWikiLink Q6543515.
- Q1077290 wikiPageWikiLink Q7009278.
- Q1077290 wikiPageWikiLink Q7217174.
- Q1077290 wikiPageWikiLink Q7233310.
- Q1077290 wikiPageWikiLink Q736811.
- Q1077290 wikiPageWikiLink Q83481.
- Q1077290 wikiPageWikiLink Q964623.
- Q1077290 type Place.
- Q1077290 type CelestialBody.
- Q1077290 type Location.
- Q1077290 type Place.
- Q1077290 type Planet.
- Q1077290 type Thing.
- Q1077290 type Q634.
- Q1077290 comment "HD 210277 b is an extrasolar planet orbiting the star HD 210277. It was discovered in September 1998 by the California and Carnegie Planet Search team using the highly successful radial velocity method. The planet is at least 24% more massive than Jupiter. The mean distance of the planet from the star is slightly more than Earth's distance from the Sun.".
- Q1077290 label "HD 210277 b".