HR930 is a main-sequence star in the constellation of Perseus.
HR930 visual magnitude is 6.31. Because of its reltive faintness, HR930 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 HR930:
HR930 is above the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of HR930
HR930 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 HR930 are provided in the following table:
The simplified sky map below shows the position of HR930 in the sky:
Visibility of HR930 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR930 is circumpolar and transits at 10:09 UTC (altitude: 89.3°)
Digitized Sky Survey image of HR930
The image below is a photograph of HR930 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 HR930 is 0.032 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 HR930 from the Sun and relative movement
HR930 is distant 693.62 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR930
HR930 belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR930 is situated in the Hertzsprung–Russell diagram.