107 Aquarii is a double giant star in the constellation of Aquarius.
107 Aquarii visual magnitude is 5.29. Because of its reltive faintness, 107 Aquarii 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 107 Aquarii:
Celestial coordinates and finder chart of 107 Aquarii
107 Aquarii 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 107 Aquarii are provided in the following table:
The simplified sky map below shows the position of 107 Aquarii in the sky:
Visibility of 107 Aquarii from your location
Digitized Sky Survey image of 107 Aquarii
The image below is a photograph of 107 Aquarii 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 107 Aquarii is 0.134 arcsec per year in Right Ascension and 0.03 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 107 Aquarii from the Sun and relative movement
107 Aquarii is distant 212.10 light years from the Sun and it is moving towards the Sun at the speed of 2 kilometers per second.
Spectral properties of 107 Aquarii
107 Aquarii belongs to spectral class F2 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where 107 Aquarii is situated in the Hertzsprung–Russell diagram.
107 Aquarii star system properties
107 Aquarii is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the 107 Aquarii double sysyem: