88 Tauri is a variable and double star in the constellation of Taurus.
88 Tauri visual magnitude is 4.25. Because of its moderate brightness, 88 Tauri should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 88 Tauri:
Celestial coordinates and finder chart of 88 Tauri
88 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 88 Tauri are provided in the following table:
The simplified sky map below shows the position of 88 Tauri in the sky:
Visibility of 88 Tauri from your location
Digitized Sky Survey image of 88 Tauri
The image below is a photograph of 88 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 88 Tauri is 0.055 arcsec per year in Right Ascension and -0.046 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of 88 Tauri from the Sun and relative movement
88 Tauri is distant 150.37 light years from the Sun and it is moving far from the Sun at the speed of 29 kilometers per second.
Spectral properties of 88 Tauri
88 Tauri belongs to spectral class A5
The red dot in the diagram below shows where 88 Tauri is situated in the Hertzsprung–Russell diagram.
88 Tauri star system properties
88 Tauri is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the 88 Tauri double sysyem: