67 Leonis is a double sub-giant star in the constellation of Leo.
67 Leonis visual magnitude is 5.68. Because of its reltive faintness, 67 Leonis 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 67 Leonis:
Celestial coordinates and finder chart of 67 Leonis
67 Leonis 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 67 Leonis are provided in the following table:
The simplified sky map below shows the position of 67 Leonis in the sky:
Visibility of 67 Leonis from your location
Digitized Sky Survey image of 67 Leonis
The image below is a photograph of 67 Leonis 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 67 Leonis is 0.003 arcsec per year in Right Ascension and 0.004 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of 67 Leonis from the Sun and relative movement
67 Leonis is distant 408.01 light years from the Sun and it is moving towards the Sun at the speed of 6 kilometers per second.
Spectral properties of 67 Leonis
67 Leonis belongs to spectral class A3 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 67 Leonis is situated in the Hertzsprung–Russell diagram.
67 Leonis star system properties
67 Leonis 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 67 Leonis double sysyem: