31 Tauri is a double main-sequence star in the constellation of Taurus.
31 Tauri visual magnitude is 5.67. Because of its reltive faintness, 31 Tauri 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 31 Tauri:
Celestial coordinates and finder chart of 31 Tauri
31 Tauri 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 31 Tauri are provided in the following table:
The simplified sky map below shows the position of 31 Tauri in the sky:
Visibility of 31 Tauri from your location
Digitized Sky Survey image of 31 Tauri
The image below is a photograph of 31 Tauri 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 31 Tauri is 0.009 arcsec per year in Right Ascension and -0.008 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of 31 Tauri from the Sun and relative movement
31 Tauri is distant 704.10 light years from the Sun and it is moving far from the Sun at the speed of 16 kilometers per second.
Spectral properties of 31 Tauri
31 Tauri belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 31 Tauri is situated in the Hertzsprung–Russell diagram.
31 Tauri star system properties
31 Tauri is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the 31 Tauri double sysyem: