113 Tauri is a main-sequence star in the constellation of Taurus.
113 Tauri visual magnitude is 6.25. Because of its reltive faintness, 113 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 113 Tauri:
Celestial coordinates and finder chart of 113 Tauri
113 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 113 Tauri are provided in the following table:
The simplified sky map below shows the position of 113 Tauri in the sky:
Visibility of 113 Tauri from your location
Digitized Sky Survey image of 113 Tauri
The image below is a photograph of 113 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 113 Tauri is -0.009 arcsec per year in Right Ascension and -0.003 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of 113 Tauri from the Sun and relative movement
113 Tauri is distant 654.62 light years from the Sun and it is moving far from the Sun at the speed of 31 kilometers per second.
Spectral properties of 113 Tauri
113 Tauri 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 113 Tauri is situated in the Hertzsprung–Russell diagram.