110 Tauri
110 Tauri is a sub-giant star in the constellation of Taurus.
110 Tauri visual magnitude is 6.08. Because of its reltive faintness, 110 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 110 Tauri:
110 Tauri is below the horizon from Greenwich, United Kingdom .
Altitude: -19.5°
Azimuth: 339.3°
Direction: North-North-West
Celestial coordinates and finder chart of 110 Tauri
110 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 110 Tauri are provided in the following table:
The simplified sky map below shows the position of 110 Tauri in the sky:

Visibility of 110 Tauri from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's 110 Tauri rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of 110 Tauri
The image below is a photograph of 110 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 110 Tauri is -0.029 arcsec per year in Right Ascension and -0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of 110 Tauri from the Sun and relative movement
110 Tauri is distant 445.36 light years from the Sun and it is moving far from the Sun at the speed of 21 kilometers per second.
Spectral properties of 110 Tauri
110 Tauri belongs to spectral class A2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 110 Tauri is situated in the Hertzsprung–Russell diagram.
