HR2017 is a giant star in the constellation of Columba.
HR2017 visual magnitude is 6.61. Because of its reltive faintness, HR2017 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 HR2017:
Celestial coordinates and finder chart of HR2017
HR2017 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2017 are provided in the following table:
The simplified sky map below shows the position of HR2017 in the sky:
Visibility of HR2017 from your location
Digitized Sky Survey image of HR2017
The image below is a photograph of HR2017 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 HR2017 is 0.007 arcsec per year in Right Ascension and 0.032 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2017 from the Sun and relative movement
HR2017 is distant 958.82 light years from the Sun and it is moving far from the Sun at the speed of 13 kilometers per second.
Spectral properties of HR2017
HR2017 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 HR2017 is situated in the Hertzsprung–Russell diagram.