HR2351 is a sub-giant star in the constellation of Monoceros.
HR2351 visual magnitude is 6.59. Because of its reltive faintness, HR2351 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 HR2351:
Celestial coordinates and finder chart of HR2351
HR2351 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 HR2351 are provided in the following table:
The simplified sky map below shows the position of HR2351 in the sky:
Visibility of HR2351 from your location
Digitized Sky Survey image of HR2351
The image below is a photograph of HR2351 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 HR2351 is -0.027 arcsec per year in Right Ascension and -0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2351 from the Sun and relative movement
HR2351 is distant 198.18 light years from the Sun and it is moving far from the Sun at the speed of 41 kilometers per second.
Spectral properties of HR2351
HR2351 belongs to spectral class A9 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR2351 is situated in the Hertzsprung–Russell diagram.