HR3381 is a multiple sub-giant star in the constellation of Pyxis.
HR3381 visual magnitude is 6.19. Because of its reltive faintness, HR3381 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 HR3381:
Celestial coordinates and finder chart of HR3381
HR3381 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 HR3381 are provided in the following table:
The simplified sky map below shows the position of HR3381 in the sky:
Visibility of HR3381 from your location
Digitized Sky Survey image of HR3381
The image below is a photograph of HR3381 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 HR3381 is -0.007 arcsec per year in Right Ascension and -0.016 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3381 from the Sun and relative movement
HR3381 is distant 255.09 light years from the Sun and it is moving towards the Sun at the speed of 8 kilometers per second.
Spectral properties of HR3381
HR3381 belongs to spectral class A8 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR3381 is situated in the Hertzsprung–Russell diagram.
HR3381 star system properties
HR3381 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 HR3381 double sysyem: