HR1371 is a double star in the constellation of Perseus.
HR1371 visual magnitude is 6.23. Because of its reltive faintness, HR1371 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 HR1371:
HR1371 is above the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of HR1371
HR1371 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 HR1371 are provided in the following table:
The simplified sky map below shows the position of HR1371 in the sky:
Visibility of HR1371 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR1371 is circumpolar and transits at 11:21 UTC (altitude: 80.9°)
Digitized Sky Survey image of HR1371
The image below is a photograph of HR1371 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 HR1371 is 0.024 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 HR1371 from the Sun and relative movement
HR1371 is distant 552.54 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR1371
HR1371 belongs to spectral class A1 HR1371 is also a Si chemically peculiar star.
The red dot in the diagram below shows where HR1371 is situated in the Hertzsprung–Russell diagram.
HR1371 star system properties
HR1371 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR1371 double sysyem: