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- HD_113766 abstract "HD 113766 is a binary star system located 424 ly from Earth in the direction of the constellation Centaurus. The star system is approximately 10 million years old and both stars are slightly more massive than our sun. The two are separated by an angle of 1.3 arcseconds, which, at the distance of this system, corresponds to a projected separation of at least 170 AU.What makes HD 113766 special is the presence of a large belt of warm (~440 K) dust surrounding the star HD 113766 A. The dense dust belt, more than 100 times more massive than our own asteroid belt, is thought to be collapsing to form a rocky planet, which when it has formed will lie within the star's terrestrial habitable zone where liquid water can exist on its surface. HD 113766 represents the most well understood system in a growing class of objects that should provide more clues to how rocky planets like the Earth formed.".
- HD_113766 thumbnail HD_113766_circumstellar_disk.jpg?width=300.
- HD_113766 wikiPageExternalLink 0610102.
- HD_113766 wikiPageExternalLink Chambers_Accretion.pdf.
- HD_113766 wikiPageID "13578381".
- HD_113766 wikiPageRevisionID "591601377".
- HD_113766 absmagV "2.99".
- HD_113766 appmagV "7.56".
- HD_113766 constell Centaurus.
- HD_113766 epoch Epoch_(astronomy).
- HD_113766 hasPhotoCollection HD_113766.
- HD_113766 luminosity "4.4".
- HD_113766 metalFe "+0.01".
- HD_113766 pError "1.01".
- HD_113766 parallax "8.16".
- HD_113766 propMoDec "-17.9".
- HD_113766 propMoRa "-34.09".
- HD_113766 radialV "–0.6".
- HD_113766 subject Category:Binary_stars.
- HD_113766 subject Category:Centaurus_(constellation).
- HD_113766 subject Category:Circumstellar_disks.
- HD_113766 subject Category:F-type_main-sequence_stars.
- HD_113766 subject Category:Henry_Draper_Catalogue_objects.
- HD_113766 type CelestialBody.
- HD_113766 type Star.
- HD_113766 type PhysicalBody.
- HD_113766 comment "HD 113766 is a binary star system located 424 ly from Earth in the direction of the constellation Centaurus. The star system is approximately 10 million years old and both stars are slightly more massive than our sun. The two are separated by an angle of 1.3 arcseconds, which, at the distance of this system, corresponds to a projected separation of at least 170 AU.What makes HD 113766 special is the presence of a large belt of warm (~440 K) dust surrounding the star HD 113766 A.".
- HD_113766 label "HD 113766".
- HD_113766 label "HD 113766".
- HD_113766 label "HD 113766".
- HD_113766 sameAs HD_113766.
- HD_113766 sameAs HD_113766.
- HD_113766 sameAs m.03c9yt3.
- HD_113766 sameAs Q682637.
- HD_113766 sameAs Q682637.
- HD_113766 wasDerivedFrom HD_113766?oldid=591601377.
- HD_113766 depiction HD_113766_circumstellar_disk.jpg.
- HD_113766 isPrimaryTopicOf HD_113766.
- HD_113766 name "HD 113766 A / B".
