Matches in DBpedia 2014 for { <http://dbpedia.org/resource/HD_142022_Ab> ?p ?o. }
Showing items 1 to 57 of
57
with 100 items per page.
- HD_142022_Ab abstract "HD 142022 Ab is an exoplanet discovered by the radial velocity method by Eggenberger et al. in 2005 after finding that HD 142022 A is wobbling which indicated the presence of a massive planet, designating as HD 142022 Ab, with mass of 4.5 times Jupiter. It has a relatively wide separation between a planet and a star with nearly 3 AU, which takes 1928 days or 5.28 years to revolve. As it is typical for long-period planets, it has a relatively high eccentricity of 53±20%.".
- HD_142022_Ab wikiPageExternalLink etoile.php?nom=HD+142022+A.
- HD_142022_Ab wikiPageExternalLink aa3720-05.html.
- HD_142022_Ab wikiPageExternalLink planettour.asp?StarCatId=normal&PlanetId=288.
- HD_142022_Ab wikiPageID "16782383".
- HD_142022_Ab wikiPageRevisionID "582062165".
- HD_142022_Ab angDist "81.6".
- HD_142022_Ab apastron "4.48".
- HD_142022_Ab apastronGigameter "670".
- HD_142022_Ab appmagV "7.69".
- HD_142022_Ab argPeri "170".
- HD_142022_Ab class "G9V".
- HD_142022_Ab constell Octans.
- HD_142022_Ab discoverers "Eggenberger et al.".
- HD_142022_Ab discoveryDate "2005-02-14".
- HD_142022_Ab discoveryMethod Doppler_spectroscopy.
- HD_142022_Ab discoverySite La_Silla_Observatory.
- HD_142022_Ab discoveryStatus "Published".
- HD_142022_Ab distLy "117".
- HD_142022_Ab distPc "35.9".
- HD_142022_Ab eccentricity "0.53".
- HD_142022_Ab hasPhotoCollection HD_142022_Ab.
- HD_142022_Ab minimumMass "4.47".
- HD_142022_Ab minimumMassEarth "1420".
- HD_142022_Ab periastron "1.38".
- HD_142022_Ab periastronGigameter "206".
- HD_142022_Ab period "1928".
- HD_142022_Ab periodYear "5.278".
- HD_142022_Ab planet "b".
- HD_142022_Ab semiAmp "92".
- HD_142022_Ab semimajor "2.93".
- HD_142022_Ab semimajorGigameter "438".
- HD_142022_Ab speed "16.6".
- HD_142022_Ab star HD_142022.
- HD_142022_Ab star "HD+142022+A".
- HD_142022_Ab tPeri "2450971".
- HD_142022_Ab subject Category:Exoplanets.
- HD_142022_Ab subject Category:Exoplanets_detected_by_radial_velocity.
- HD_142022_Ab subject Category:Exoplanets_discovered_in_2005.
- HD_142022_Ab subject Category:Gas_giants.
- HD_142022_Ab subject Category:Octans_(constellation).
- HD_142022_Ab type CelestialBody.
- HD_142022_Ab type Planet.
- HD_142022_Ab type PhysicalBody.
- HD_142022_Ab comment "HD 142022 Ab is an exoplanet discovered by the radial velocity method by Eggenberger et al. in 2005 after finding that HD 142022 A is wobbling which indicated the presence of a massive planet, designating as HD 142022 Ab, with mass of 4.5 times Jupiter. It has a relatively wide separation between a planet and a star with nearly 3 AU, which takes 1928 days or 5.28 years to revolve. As it is typical for long-period planets, it has a relatively high eccentricity of 53±20%.".
- HD_142022_Ab label "HD 142022 Ab".
- HD_142022_Ab label "HD 142022 Ab".
- HD_142022_Ab label "HD 142022 Ab".
- HD_142022_Ab label "HD 142022 Ab".
- HD_142022_Ab sameAs HD_142022_Ab.
- HD_142022_Ab sameAs HD_142022_Ab.
- HD_142022_Ab sameAs HD_142022_Ab.
- HD_142022_Ab sameAs m.04y5kk_.
- HD_142022_Ab sameAs Q1075500.
- HD_142022_Ab sameAs Q1075500.
- HD_142022_Ab wasDerivedFrom HD_142022_Ab?oldid=582062165.
- HD_142022_Ab isPrimaryTopicOf HD_142022_Ab.