HR8614 is a giant star in the constellation of Piscis Austrinus.
HR8614 visual magnitude is 6.47. Because of its reltive faintness, HR8614 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 HR8614:
Celestial coordinates and finder chart of HR8614
HR8614 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR8614 are provided in the following table:
The simplified sky map below shows the position of HR8614 in the sky:
Visibility of HR8614 from your location
Digitized Sky Survey image of HR8614
The image below is a photograph of HR8614 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 HR8614 is -0.035 arcsec per year in Right Ascension and 0.001 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8614 from the Sun and relative movement
HR8614 is distant 402.97 light years from the Sun and it is moving far from the Sun at the speed of 3 kilometers per second.
Spectral properties of HR8614
HR8614 belongs to spectral class K1 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR8614 is situated in the Hertzsprung–Russell diagram.