HR2607 is a double dwarf star in the constellation of Canis Major.
HR2607 visual magnitude is 5.46. Because of its reltive faintness, HR2607 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 HR2607:
Celestial coordinates and finder chart of HR2607
HR2607 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR2607 are provided in the following table:
The simplified sky map below shows the position of HR2607 in the sky:
Visibility of HR2607 from your location
Digitized Sky Survey image of HR2607
The image below is a photograph of HR2607 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 HR2607 is -0.058 arcsec per year in Right Ascension and 0.106 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR2607 from the Sun and relative movement
HR2607 is distant 125.67 light years from the Sun and it is moving far from the Sun at the speed of 20 kilometers per second.
Spectral properties of HR2607
HR2607 belongs to spectral class F0
The red dot in the diagram below shows where HR2607 is situated in the Hertzsprung–Russell diagram.
HR2607 star system properties
HR2607 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR2607 double sysyem: