HR1215 is a variable main-sequence star in the constellation of Perseus.
HR1215 visual magnitude is 5.49. Because of its reltive faintness, HR1215 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR1215:
Celestial coordinates and finder chart of HR1215
HR1215 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1215 are provided in the following table:
The simplified sky map below shows the position of HR1215 in the sky:
Visibility of HR1215 from your location
Digitized Sky Survey image of HR1215
The image below is a photograph of HR1215 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of HR1215 is 0.005 arcsec per year in Right Ascension and -0.001 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR1215 from the Sun and relative movement
HR1215 is distant 970.24 light years from the Sun and it is moving far from the Sun at the speed of 17 kilometers per second.
Spectral properties of HR1215
HR1215 belongs to spectral class B1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1215 is situated in the Hertzsprung–Russell diagram.