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- HD_60532_c abstract "HD 60532 c is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more than Jupiter which orbits at 1.58 AU and takes 607 days to revolve in an eccentric orbit. This planet was discovered on September 22, 2008 in La Silla Observatory using the HARPS spectrograph. On this same day, the second planet in this system, HD 60532 b, was discovered in a 3:1 orbital resonance.".
- HD_60532_c wikiPageExternalLink planete.php?etoile=HD+60532&planete=c.
- HD_60532_c wikiPageID "19732644".
- HD_60532_c wikiPageRevisionID "640682757".
- HD_60532_c apastron "1.64".
- HD_60532_c apastronGm "245".
- HD_60532_c appMag "4.458".
- HD_60532_c argPeri "119.49".
- HD_60532_c class "F6V".
- HD_60532_c constell Puppis.
- HD_60532_c discoverers "Desort et al.".
- HD_60532_c discoveryDate "2008-09-22".
- HD_60532_c discoveryMethod Doppler_spectroscopy.
- HD_60532_c discoverySite La_Silla_Observatory.
- HD_60532_c discoveryStatus "Published".
- HD_60532_c distLy "83.8".
- HD_60532_c distPc "25.7".
- HD_60532_c eccentricity "0.038".
- HD_60532_c hasPhotoCollection HD_60532_c.
- HD_60532_c inclination "~20".
- HD_60532_c periastron "1.52".
- HD_60532_c periastronGm "227".
- HD_60532_c period "607.06".
- HD_60532_c periodYear "1.662".
- HD_60532_c planet "c".
- HD_60532_c semimajor "1.58".
- HD_60532_c semimajorGm "236".
- HD_60532_c star HD_60532.
- HD_60532_c star "HD+60532".
- HD_60532_c tPeri "2454000".
- HD_60532_c subject Category:Exoplanets.
- HD_60532_c subject Category:Exoplanets_detected_by_radial_velocity.
- HD_60532_c subject Category:Exoplanets_discovered_in_2008.
- HD_60532_c subject Category:Giant_planets.
- HD_60532_c subject Category:Puppis_(constellation).
- HD_60532_c type CelestialBody.
- HD_60532_c type Planet.
- HD_60532_c type Thing.
- HD_60532_c type Q634.
- HD_60532_c comment "HD 60532 c is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more than Jupiter which orbits at 1.58 AU and takes 607 days to revolve in an eccentric orbit. This planet was discovered on September 22, 2008 in La Silla Observatory using the HARPS spectrograph. On this same day, the second planet in this system, HD 60532 b, was discovered in a 3:1 orbital resonance.".
- HD_60532_c label "HD 60532 c".
- HD_60532_c label "HD 60532 c".
- HD_60532_c sameAs HD_60532_c.
- HD_60532_c sameAs m.04mwyx4.
- HD_60532_c sameAs Q5369351.
- HD_60532_c sameAs Q5369351.
- HD_60532_c wasDerivedFrom HD_60532_c?oldid=640682757.
- HD_60532_c isPrimaryTopicOf HD_60532_c.