53 Aquarii is a multiple main-sequence star in the constellation of Aquarius.
53 Aquarii visual magnitude is 6.35. Because of its reltive faintness, 53 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 53 Aquarii:
Celestial coordinates and finder chart of 53 Aquarii
53 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 53 Aquarii are provided in the following table:
The simplified sky map below shows the position of 53 Aquarii in the sky:
Visibility of 53 Aquarii from your location
Digitized Sky Survey image of 53 Aquarii
The image below is a photograph of 53 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 53 Aquarii is 0.223 arcsec per year in Right Ascension and -0.003 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 53 Aquarii from the Sun and relative movement
53 Aquarii is distant 65.46 light years from the Sun and it is moving towards the Sun at the speed of 6 kilometers per second.
Spectral properties of 53 Aquarii
53 Aquarii belongs to spectral class G1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 53 Aquarii is situated in the Hertzsprung–Russell diagram.
53 Aquarii star system properties
53 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 53 Aquarii double sysyem: