HR894 is a main-sequence star in the constellation of Perseus.
HR894 visual magnitude is 6.11. Because of its reltive faintness, HR894 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 HR894:
Celestial coordinates and finder chart of HR894
HR894 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 HR894 are provided in the following table:
The simplified sky map below shows the position of HR894 in the sky:
Visibility of HR894 from your location
Digitized Sky Survey image of HR894
The image below is a photograph of HR894 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 HR894 is 0.006 arcsec per year in Right Ascension and -0.028 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR894 from the Sun and relative movement
HR894 is distant 1,112.63 light years from the Sun and it is moving towards the Sun at the speed of 16 kilometers per second.
Spectral properties of HR894
HR894 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR894 is situated in the Hertzsprung–Russell diagram.