62 Sagittarii is a variable giant star in the constellation of Sagittarius.
62 Sagittarii visual magnitude is 4.58. Because of its moderate brightness, 62 Sagittarii should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 62 Sagittarii:
Celestial coordinates and finder chart of 62 Sagittarii
62 Sagittarii is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of 62 Sagittarii are provided in the following table:
The simplified sky map below shows the position of 62 Sagittarii in the sky:
Visibility of 62 Sagittarii from your location
Digitized Sky Survey image of 62 Sagittarii
The image below is a photograph of 62 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 62 Sagittarii is 0.036 arcsec per year in Right Ascension and 0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 62 Sagittarii from the Sun and relative movement
62 Sagittarii is distant 447.80 light years from the Sun and it is moving far from the Sun at the speed of 10 kilometers per second.
Spectral properties of 62 Sagittarii
62 Sagittarii belongs to spectral class M4 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where 62 Sagittarii is situated in the Hertzsprung–Russell diagram.