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HR 297 is a solitary star in the northern circumpolar constellation of Cassiopeia. It has an apparent visual magnitude of 5.8, making it faintly visible to the naked eye from dark suburban skies. Parallax measurements put this system at a distance of roughly 256 light years. It is drifting closer with a heliocentric radial velocity of −20.4 km/s. This star has been examined for the presence of an infrared excess, but no statistically significant amount was detected. The detection of such an excess can indicate the presence of a dusty circumstellar disk.

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rdf:type
rdfs:label
  • HR 297 (en)
  • HD 6210 (sv)
  • HD 6210 (zh)
rdfs:comment
  • HD 6210 är en gulvit stjärna i huvudserien i Cassiopejas stjärnbild.Den har visuell magnitud +5,83 och är synlig för blotta ögat vid god seeing. (sv)
  • HD 6210，又名BD+60 158，SAO 11557、HR 297，是一颗恒星，视星等为5.84，位于銀經124.47，銀緯-1.25，其B1900.0坐标为赤經0h 58m 8.7s，赤緯+61° -1.25′ 38″。 (zh)
  • HR 297 is a solitary star in the northern circumpolar constellation of Cassiopeia. It has an apparent visual magnitude of 5.8, making it faintly visible to the naked eye from dark suburban skies. Parallax measurements put this system at a distance of roughly 256 light years. It is drifting closer with a heliocentric radial velocity of −20.4 km/s. This star has been examined for the presence of an infrared excess, but no statistically significant amount was detected. The detection of such an excess can indicate the presence of a dusty circumstellar disk. (en)
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absmag v
age gyr
appmag v
b-v
  • +0.56 (en)
class
  • F6V (en)
constell
epoch
  • J2000 (en)
gravity
luminosity
mass
metal fe
  • −0.01 (en)
p error
parallax
radial v
  • −20.40 (en)
radius
rotational velocity
temperature
type
  • Main sequence (en)
u-b
  • +0.11 (en)
has abstract
  • HR 297 is a solitary star in the northern circumpolar constellation of Cassiopeia. It has an apparent visual magnitude of 5.8, making it faintly visible to the naked eye from dark suburban skies. Parallax measurements put this system at a distance of roughly 256 light years. It is drifting closer with a heliocentric radial velocity of −20.4 km/s. This is an F-type main sequence star with a stellar classification of F7V. Because of the stability of this star, it is used as a standard in the photometric WBVR system. The angular diameter of this star has been measured directly using the CHARA Array, yielding an estimate of 4.5 times the diameter of the Sun. Stellar models suggest a mass equal to about twice that of the Sun, with 25 times the Sun's luminosity. This is a young star with an estimated age of 1.3 billion years. It is rotating rapidly, with a projected rotational velocity of 42 km/s. The abundance of elements other than hydrogen and helium is about the same as that in the Sun. The effective temperature of the stellar atmosphere is 6,089 K, giving it the yellow-white hued glow of an F-type star. This star has been examined for the presence of an infrared excess, but no statistically significant amount was detected. The detection of such an excess can indicate the presence of a dusty circumstellar disk. (en)
  • HD 6210 är en gulvit stjärna i huvudserien i Cassiopejas stjärnbild.Den har visuell magnitud +5,83 och är synlig för blotta ögat vid god seeing. (sv)
  • HD 6210，又名BD+60 158，SAO 11557、HR 297，是一颗恒星，视星等为5.84，位于銀經124.47，銀緯-1.25，其B1900.0坐标为赤經0h 58m 8.7s，赤緯+61° -1.25′ 38″。 (zh)
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