16 Draconis is a multiple main-sequence star in the constellation of Draco.
16 Draconis visual magnitude is 5.53. Because of its reltive faintness, 16 Draconis 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 16 Draconis:
Celestial coordinates and finder chart of 16 Draconis
16 Draconis is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 16 Draconis are provided in the following table:
The simplified sky map below shows the position of 16 Draconis in the sky:
Visibility of 16 Draconis from your location
16 Draconis is circumpolar and transits at 11:16 UTC (altitude: 88.6°)
Digitized Sky Survey image of 16 Draconis
The image below is a photograph of 16 Draconis 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 16 Draconis is -0.009 arcsec per year in Right Ascension and 0.033 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 16 Draconis from the Sun and relative movement
16 Draconis is distant 399.51 light years from the Sun and it is moving towards the Sun at the speed of 9 kilometers per second.
Spectral properties of 16 Draconis
16 Draconis belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 16 Draconis is situated in the Hertzsprung–Russell diagram.