105 Tauri is a multiple main-sequence star in the constellation of Taurus.
105 Tauri visual magnitude is 5.89. Because of its reltive faintness, 105 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 105 Tauri:
Celestial coordinates and finder chart of 105 Tauri
105 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 105 Tauri are provided in the following table:
The simplified sky map below shows the position of 105 Tauri in the sky:
Visibility of 105 Tauri from your location
Digitized Sky Survey image of 105 Tauri
The image below is a photograph of 105 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 105 Tauri is 0.005 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 105 Tauri from the Sun and relative movement
105 Tauri is distant 1,031.65 light years from the Sun and it is moving far from the Sun at the speed of 17 kilometers per second.
Spectral properties of 105 Tauri
105 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 105 Tauri is situated in the Hertzsprung–Russell diagram.