13 Orionis is a multiple sub-giant star in the constellation of Orion.
13 Orionis visual magnitude is 6.17. Because of its reltive faintness, 13 Orionis 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 13 Orionis:
Celestial coordinates and finder chart of 13 Orionis
13 Orionis 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 13 Orionis are provided in the following table:
The simplified sky map below shows the position of 13 Orionis in the sky:
Visibility of 13 Orionis from your location
Digitized Sky Survey image of 13 Orionis
The image below is a photograph of 13 Orionis 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 13 Orionis is -0.003 arcsec per year in Right Ascension and -0.378 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 13 Orionis from the Sun and relative movement
13 Orionis is distant 92.25 light years from the Sun and it is moving towards the Sun at the speed of 24 kilometers per second.
Spectral properties of 13 Orionis
13 Orionis belongs to spectral class G1 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 13 Orionis is situated in the Hertzsprung–Russell diagram.
13 Orionis star system properties
13 Orionis is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the 13 Orionis double sysyem: