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It is smaller and less luminous than our Sun , with a spectral class of K3V, which makes it an orange-red hued star. HR is relatively close to our system, with an estimated distance of This star is close to the limit of apparent magnitude that can still be seen by the unaided eye. The limit is considered to be magnitude 6 for most observers.
This star has a magnitude 9. As of March , the star is known to have at least 5 planets, two of them HD b and c known to be transiting, rocky Super-Earths. Coordinates : 23 h 13 m From Wikipedia, the free encyclopedia.
November , "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 2 : β, arXiv : August , "UBV photometry of stars whose positions are accurately known. Rotation periods and starspot parameters", Astronomy and Astrophysics , 3 : β, arXiv : Catalogue of suspected variable stars ", Nachrichtenblatt der Vereinigung der Sternfreunde e. Part I. July , "The Geneva-Copenhagen survey of the solar neighbourhood.
Improved distances, ages, and kinematics", Astronomy and Astrophysics , 3 : β, arXiv : Retrieved September , "Chromospheric activity and rotation of FGK stars in the solar vicinity. September , "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 2 : β, arXiv : Retrieved 30 July Retrieved 31 July The Astrophysical Journal. Bibcode : ApJ Nature Astronomy.
Bibcode : NatAs The HR system. Cassiopeia constellation. Category in space β Category in space β Category in space. Namespaces Article Talk. Views Read Edit View history. By using this site, you agree to the Terms of Use and Privacy Policy.