HR1714 is a main-sequence star in the constellation of Cepheus.
HR1714 visual magnitude is 6.6. Because of its reltive faintness, HR1714 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 HR1714:
Celestial coordinates and finder chart of HR1714
HR1714 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1714 are provided in the following table:
The simplified sky map below shows the position of HR1714 in the sky:
Visibility of HR1714 from your location
HR1714 is circumpolar and transits at 05:00 UTC (altitude: 55.8°)
Digitized Sky Survey image of HR1714
The image below is a photograph of HR1714 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 HR1714 is -0.016 arcsec per year in Right Ascension and 0.002 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1714 from the Sun and relative movement
HR1714 is distant 472.46 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR1714
HR1714 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1714 is situated in the Hertzsprung–Russell diagram.