133 Tauri is a multiple sub-giant star in the constellation of Taurus.
133 Tauri visual magnitude is 5.29. Because of its reltive faintness, 133 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 133 Tauri:
Celestial coordinates and finder chart of 133 Tauri
133 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 133 Tauri are provided in the following table:
The simplified sky map below shows the position of 133 Tauri in the sky:
Visibility of 133 Tauri from your location
Digitized Sky Survey image of 133 Tauri
The image below is a photograph of 133 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 133 Tauri is 0.002 arcsec per year in Right Ascension and -0.012 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 133 Tauri from the Sun and relative movement
133 Tauri is distant 799.02 light years from the Sun and it is moving far from the Sun at the speed of 29 kilometers per second.
Spectral properties of 133 Tauri
133 Tauri belongs to spectral class B2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 133 Tauri is situated in the Hertzsprung–Russell diagram.
133 Tauri star system properties
133 Tauri 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 133 Tauri double sysyem: