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- HD_16760 abstract "HD 16760 is a binary star system approximately 150 light-years away in the constellation Perseus. The primary star HD 16760 (HIP 12638) is a G-type main sequence star similar to our Sun. The secondary, HIP 12635 is 1.521 magnitudes fainter and located at a separation of 14.6 arcseconds from the primary, corresponding to a physical separation of at least 660 AU. Announced in July 2009, HD 16760 has been confirmed to have a substellar object orbiting it. Whether or not this object is a brown dwarf or an extrasolar planet is currently not understood.".
- HD_16760 wikiPageID "23811497".
- HD_16760 wikiPageRevisionID "562438378".
- HD_16760 absmagV "5.41".
- HD_16760 appmagV "8.74".
- HD_16760 bV "0.715".
- HD_16760 class "G5V".
- HD_16760 constell Perseus_(constellation).
- HD_16760 eccentricity "0.084".
- HD_16760 epe "HD+16760".
- HD_16760 epoch Epoch_(astronomy).
- HD_16760 exoplanet "b".
- HD_16760 gravity "4.47".
- HD_16760 group ""note"".
- HD_16760 hasPhotoCollection HD_16760.
- HD_16760 luminosityBolometric "0.72".
- HD_16760 mass "0.78".
- HD_16760 mass "≥13.13 ± 0.56".
- HD_16760 metal "[Fe/H] = +0.067 ± 0.05".
- HD_16760 nsted "HD+16760".
- HD_16760 pError "2.35".
- HD_16760 parallax "22".
- HD_16760 period "466.47".
- HD_16760 propMoDec "-110.65".
- HD_16760 propMoRa "82.84".
- HD_16760 radius "0.81".
- HD_16760 rotationalVelocity "0.5".
- HD_16760 semimajor "1.084".
- HD_16760 simbad "HD+16760".
- HD_16760 temperature "5629".
- HD_16760 subject Category:Brown_dwarfs.
- HD_16760 subject Category:Durchmusterung_objects.
- HD_16760 subject Category:G-type_main-sequence_stars.
- HD_16760 subject Category:Henry_Draper_Catalogue_objects.
- HD_16760 subject Category:Hipparcos_objects.
- HD_16760 subject Category:Perseus_(constellation).
- HD_16760 subject Category:Planetary_systems.
- HD_16760 type CelestialBody.
- HD_16760 type Star.
- HD_16760 type PhysicalBody.
- HD_16760 comment "HD 16760 is a binary star system approximately 150 light-years away in the constellation Perseus. The primary star HD 16760 (HIP 12638) is a G-type main sequence star similar to our Sun. The secondary, HIP 12635 is 1.521 magnitudes fainter and located at a separation of 14.6 arcseconds from the primary, corresponding to a physical separation of at least 660 AU. Announced in July 2009, HD 16760 has been confirmed to have a substellar object orbiting it.".
- HD_16760 label "HD 16760".
- HD_16760 label "HD 16760".
- HD_16760 label "HD 16760".
- HD_16760 sameAs HD_16760.
- HD_16760 sameAs m.06_x391.
- HD_16760 sameAs Q2067421.
- HD_16760 sameAs Q2067421.
- HD_16760 wasDerivedFrom HD_16760?oldid=562438378.
- HD_16760 isPrimaryTopicOf HD_16760.
- HD_16760 name "HD 16760".