HR357 is a main-sequence star in the constellation of Cepheus.
HR357 visual magnitude is 6.26. Because of its reltive faintness, HR357 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 HR357:
Celestial coordinates and finder chart of HR357
HR357 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 HR357 are provided in the following table:
The simplified sky map below shows the position of HR357 in the sky:
Visibility of HR357 from your location
HR357 is circumpolar and transits at 20:31 UTC (altitude: 61.6°)
Digitized Sky Survey image of HR357
The image below is a photograph of HR357 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 HR357 is -0.055 arcsec per year in Right Ascension and 0.059 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR357 from the Sun and relative movement
HR357 is distant 235.55 light years from the Sun and it is moving towards the Sun at the speed of 43 kilometers per second.
Spectral properties of HR357
HR357 belongs to spectral class F5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR357 is situated in the Hertzsprung–Russell diagram.