HR3397 is a sub-giant star in the constellation of Pyxis.
HR3397 visual magnitude is 6.43. Because of its reltive faintness, HR3397 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 HR3397:
Celestial coordinates and finder chart of HR3397
HR3397 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 HR3397 are provided in the following table:
The simplified sky map below shows the position of HR3397 in the sky:
Visibility of HR3397 from your location
Digitized Sky Survey image of HR3397
The image below is a photograph of HR3397 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 HR3397 is -0.044 arcsec per year in Right Ascension and -0.133 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR3397 from the Sun and relative movement
HR3397 is distant 204.65 light years from the Sun and it is moving far from the Sun at the speed of 8 kilometers per second.
Spectral properties of HR3397
HR3397 belongs to spectral class G5 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR3397 is situated in the Hertzsprung–Russell diagram.