HR2545 is a multiple main-sequence star in the constellation of Canis Major.
HR2545 visual magnitude is 5.7. Because of its reltive faintness, HR2545 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 HR2545:
Celestial coordinates and finder chart of HR2545
HR2545 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2545 are provided in the following table:
The simplified sky map below shows the position of HR2545 in the sky:
Visibility of HR2545 from your location
Digitized Sky Survey image of HR2545
The image below is a photograph of HR2545 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 HR2545 is -0.002 arcsec per year in Right Ascension and 0.012 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2545 from the Sun and relative movement
HR2545 is distant 718.06 light years from the Sun and it is moving far from the Sun at the speed of 20 kilometers per second.
Spectral properties of HR2545
HR2545 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 HR2545 is situated in the Hertzsprung–Russell diagram.
HR2545 star system properties
HR2545 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR2545 double sysyem: