υ Sagittarii (upsilon Sagittarii)
υ Sagittarii is a variable and double main-sequence star in the constellation of Sagittarius.
υ Sagittarii visual magnitude is 4.61. Because of its moderate brightness, υ 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 υ Sagittarii:
Celestial coordinates and finder chart of υ Sagittarii
υ 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 υ Sagittarii are provided in the following table:
The simplified sky map below shows the position of υ Sagittarii in the sky:
Visibility of υ Sagittarii from your location
Digitized Sky Survey image of υ Sagittarii
The image below is a photograph of υ 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 υ Sagittarii is 0.002 arcsec per year in Right Ascension and -0.006 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of υ Sagittarii from the Sun and relative movement
υ Sagittarii is distant 1,671.79 light years from the Sun and it is moving far from the Sun at the speed of 9 kilometers per second.
Spectral properties of υ Sagittarii
υ Sagittarii belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where υ Sagittarii is situated in the Hertzsprung–Russell diagram.
υ Sagittarii star system properties
υ Sagittarii is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the υ Sagittarii double sysyem: