HR2348 is a double main-sequence star in the constellation of Puppis.
HR2348 visual magnitude is 5.76. Because of its reltive faintness, HR2348 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 HR2348:
Celestial coordinates and finder chart of HR2348
HR2348 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 HR2348 are provided in the following table:
The simplified sky map below shows the position of HR2348 in the sky:
Visibility of HR2348 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
HR2348 is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of HR2348
The image below is a photograph of HR2348 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 HR2348 is -0.005 arcsec per year in Right Ascension and -0.032 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2348 from the Sun and relative movement
HR2348 is distant 674.95 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR2348
HR2348 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2348 is situated in the Hertzsprung–Russell diagram.
HR2348 star system properties
HR2348 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR2348 double sysyem: