Matches in DBpedia 2014 for { <http://dbpedia.org/resource/81_Ceti_b> ?p ?o. }
Showing items 1 to 49 of
49
with 100 items per page.
- 81_Ceti_b abstract "81 Ceti b (abbreviated 81 Cet b) is an extrasolar planet approximately 300 light years away in the constellation of Cetus. It orbits the G-type giant star 81 Ceti at an average distance of 2.5 AU, taking about 2.6 years to revolve with 20.6% eccentricity. This planet was discovered on July 3, 2008 by Sato et al., who used Doppler Spectroscopy and found the wobbling of the star caused by the planet’s gravity during its revolution.".
- 81_Ceti_b wikiPageExternalLink planet.php?p1=81+Cet&p2=b.
- 81_Ceti_b wikiPageExternalLink etoile.php?nom=81+Cet.
- 81_Ceti_b wikiPageID "18747545".
- 81_Ceti_b wikiPageRevisionID "606687849".
- 81_Ceti_b apastron "3".
- 81_Ceti_b apastronGm "440".
- 81_Ceti_b appMag "5.65".
- 81_Ceti_b argPeri "175".
- 81_Ceti_b class "G5III".
- 81_Ceti_b colwidth "30".
- 81_Ceti_b constell Cetus.
- 81_Ceti_b discoverers "Sato et al.".
- 81_Ceti_b discoveryDate "2008-07-03".
- 81_Ceti_b discoveryMethod Doppler_spectroscopy.
- 81_Ceti_b discoveryStatus "Published".
- 81_Ceti_b distLy "300".
- 81_Ceti_b distPc "93".
- 81_Ceti_b eccentricity "0.206".
- 81_Ceti_b hasPhotoCollection 81_Ceti_b.
- 81_Ceti_b periastron "2".
- 81_Ceti_b periastronGm "300".
- 81_Ceti_b period "952.7".
- 81_Ceti_b periodYear "2.608".
- 81_Ceti_b planet "b".
- 81_Ceti_b semimajor "2.5".
- 81_Ceti_b semimajorGm "370".
- 81_Ceti_b star "81".
- 81_Ceti_b tPeri "2486".
- 81_Ceti_b subject Category:Cetus_(constellation).
- 81_Ceti_b subject Category:Exoplanets.
- 81_Ceti_b subject Category:Exoplanets_detected_by_radial_velocity.
- 81_Ceti_b subject Category:Exoplanets_discovered_in_2008.
- 81_Ceti_b subject Category:Gas_giants.
- 81_Ceti_b type CelestialBody.
- 81_Ceti_b type Planet.
- 81_Ceti_b type PhysicalBody.
- 81_Ceti_b comment "81 Ceti b (abbreviated 81 Cet b) is an extrasolar planet approximately 300 light years away in the constellation of Cetus. It orbits the G-type giant star 81 Ceti at an average distance of 2.5 AU, taking about 2.6 years to revolve with 20.6% eccentricity. This planet was discovered on July 3, 2008 by Sato et al., who used Doppler Spectroscopy and found the wobbling of the star caused by the planet’s gravity during its revolution.".
- 81_Ceti_b label "81 Ceti b".
- 81_Ceti_b label "81 Ceti b".
- 81_Ceti_b label "81 Кита b".
- 81_Ceti_b label "鲸鱼座81b".
- 81_Ceti_b sameAs 81_Ceti_b.
- 81_Ceti_b sameAs 고래자리_81_b.
- 81_Ceti_b sameAs m.04gv2x5.
- 81_Ceti_b sameAs Q1039740.
- 81_Ceti_b sameAs Q1039740.
- 81_Ceti_b wasDerivedFrom 81_Ceti_b?oldid=606687849.
- 81_Ceti_b isPrimaryTopicOf 81_Ceti_b.