HR2349
HR2349 is a double main-sequence star in the constellation of Canis Major.
HR2349 visual magnitude is 6.07. Because of its reltive faintness, HR2349 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 HR2349:
Celestial coordinates and finder chart of HR2349
HR2349 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 HR2349 are provided in the following table:
The simplified sky map below shows the position of HR2349 in the sky:

Visibility of HR2349 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR2349 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR2349
The image below is a photograph of HR2349 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 HR2349 is -0.186 arcsec per year in Right Ascension and -0.218 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Distance of HR2349 from the Sun and relative movement
HR2349 is distant 97.37 light years from the Sun and it is moving far from the Sun at the speed of 36 kilometers per second.
Spectral properties of HR2349
HR2349 belongs to spectral class F9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2349 is situated in the Hertzsprung–Russell diagram.

HR2349 star system properties
HR2349 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 HR2349 double sysyem: