33 Sagittarii is a supergiant star in the constellation of Sagittarius.
33 Sagittarii visual magnitude is 5.69. Because of its reltive faintness, 33 Sagittarii 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 33 Sagittarii:
Celestial coordinates and finder chart of 33 Sagittarii
33 Sagittarii 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 33 Sagittarii are provided in the following table:
The simplified sky map below shows the position of 33 Sagittarii in the sky:
Visibility of 33 Sagittarii from your location
Digitized Sky Survey image of 33 Sagittarii
The image below is a photograph of 33 Sagittarii 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 33 Sagittarii is 0.008 arcsec per year in Right Ascension and -0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 33 Sagittarii from the Sun and relative movement
33 Sagittarii is distant 1,734.04 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Spectral properties of 33 Sagittarii
33 Sagittarii belongs to spectral class K1 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where 33 Sagittarii is situated in the Hertzsprung–Russell diagram.