HR2667 is a multiple main-sequence star in the constellation of Puppis.
HR2667 visual magnitude is 5.54. Because of its reltive faintness, HR2667 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 HR2667:
Celestial coordinates and finder chart of HR2667
HR2667 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 HR2667 are provided in the following table:
The simplified sky map below shows the position of HR2667 in the sky:
Visibility of HR2667 from your location
Digitized Sky Survey image of HR2667
The image below is a photograph of HR2667 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 HR2667 is -0.105 arcsec per year in Right Ascension and 0.386 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR2667 from the Sun and relative movement
HR2667 is distant 52.97 light years from the Sun and it is moving far from the Sun at the speed of 86 kilometers per second.
Spectral properties of HR2667
HR2667 belongs to spectral class G3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2667 is situated in the Hertzsprung–Russell diagram.
HR2667 star system properties
HR2667 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR2667 double sysyem: