HR1037 is a main-sequence star in the constellation of Perseus.
HR1037 visual magnitude is 5.58. Because of its reltive faintness, HR1037 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 HR1037:
Celestial coordinates and finder chart of HR1037
HR1037 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 HR1037 are provided in the following table:
The simplified sky map below shows the position of HR1037 in the sky:
Visibility of HR1037 from your location
HR1037 is circumpolar and transits at 22:54 UTC (altitude: 88.4°)
Digitized Sky Survey image of HR1037
The image below is a photograph of HR1037 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 HR1037 is 0.028 arcsec per year in Right Ascension and -0.026 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1037 from the Sun and relative movement
HR1037 is distant 553.48 light years from the Sun and it is moving towards the Sun at the speed of 2 kilometers per second.
Spectral properties of HR1037
HR1037 belongs to spectral class B6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1037 is situated in the Hertzsprung–Russell diagram.