Jump to content

11 Persei

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Tom.Reding (talk | contribs) at 15:58, 31 October 2017 (WL 1 first-publisher; WP:GenFixes on; using AWB). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

11 Persei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Perseus
Right ascension 02h 43m 02.83828s [1]
Declination +55° 06′ 21.6643″ [1]
Spectral typeB7IIIp...
Other designations
BD+54° 598, FK5 2188, HD 16727, HIP 12692, HR 785, SAO 23555

11 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.75. Located around 132 parsecs (430 ly) distant, it is a blue giant of spectral type B7III,[1] a star that has used up its core hydrogen and is likely expanding to become a supergiant.

References

  1. ^ a b c "11 Persei". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 2 January 2013.