HR1047 is a multiple main-sequence star in the constellation of Perseus.
HR1047 visual magnitude is 6.24. Because of its reltive faintness, HR1047 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 HR1047:
HR1047 is above the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of HR1047
HR1047 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 HR1047 are provided in the following table:
The simplified sky map below shows the position of HR1047 in the sky:
Visibility of HR1047 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR1047 is circumpolar and transits at 10:31 UTC (altitude: 85.5°)
Digitized Sky Survey image of HR1047
The image below is a photograph of HR1047 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 HR1047 is 0.018 arcsec per year in Right Ascension and -0.035 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1047 from the Sun and relative movement
HR1047 is distant 575.97 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR1047
HR1047 belongs to spectral class B7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1047 is situated in the Hertzsprung–Russell diagram.
HR1047 star system properties
HR1047 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR1047 double sysyem: