HR2475 is a double main-sequence star in the constellation of Puppis.
HR2475 visual magnitude is 6.12. Because of its reltive faintness, HR2475 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 HR2475:
Celestial coordinates and finder chart of HR2475
HR2475 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2475 are provided in the following table:
The simplified sky map below shows the position of HR2475 in the sky:
Visibility of HR2475 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR2475 is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of HR2475
The image below is a photograph of HR2475 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 HR2475 is -0.014 arcsec per year in Right Ascension and 0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2475 from the Sun and relative movement
HR2475 is distant 1,058.44 light years from the Sun and it is moving far from the Sun at the speed of 17 kilometers per second.
Spectral properties of HR2475
HR2475 belongs to spectral class B4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2475 is situated in the Hertzsprung–Russell diagram.
HR2475 star system properties
HR2475 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 HR2475 double sysyem: