HR2353 is a double main-sequence star in the constellation of Columba.
HR2353 visual magnitude is 6.48. Because of its reltive faintness, HR2353 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 HR2353:
Celestial coordinates and finder chart of HR2353
HR2353 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 HR2353 are provided in the following table:
The simplified sky map below shows the position of HR2353 in the sky:
Visibility of HR2353 from your location
Digitized Sky Survey image of HR2353
The image below is a photograph of HR2353 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 HR2353 is -0.011 arcsec per year in Right Ascension and 0.042 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2353 from the Sun and relative movement
HR2353 is distant 162.27 light years from the Sun and it is moving far from the Sun at the speed of 30 kilometers per second.
Spectral properties of HR2353
HR2353 belongs to spectral class F3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2353 is situated in the Hertzsprung–Russell diagram.
HR2353 star system properties
HR2353 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR2353 double sysyem: