11 Canis Minoris
11 Canis Minoris is a variable main-sequence star in the constellation of Canis Minor.
11 Canis Minoris visual magnitude is 5.3. Because of its reltive faintness, 11 Canis Minoris 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 11 Canis Minoris:
Celestial coordinates and finder chart of 11 Canis Minoris
11 Canis Minoris 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 11 Canis Minoris are provided in the following table:
The simplified sky map below shows the position of 11 Canis Minoris in the sky:
Visibility of 11 Canis Minoris from your location
Digitized Sky Survey image of 11 Canis Minoris
The image below is a photograph of 11 Canis Minoris 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 11 Canis Minoris is -0.029 arcsec per year in Right Ascension and -0.024 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 11 Canis Minoris from the Sun and relative movement
11 Canis Minoris is distant 312.26 light years from the Sun and it is moving far from the Sun at the speed of 28 kilometers per second.
Spectral properties of 11 Canis Minoris
11 Canis Minoris belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 11 Canis Minoris is situated in the Hertzsprung–Russell diagram.