133 Tauri is a blue subgiant star that can be located in the constellation of Taurus. HIP27364 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD38622. 133 Tauri has alternative name(s), 133 Tauri , 133 Tau.
The location of the star in the galaxy is determined by the Right Ascension (R.A.) and Declination (Dec.), these are equivalent to the Longitude and Latitude on the Earth. The Right Ascension is how far expressed in time (hh:mm:ss) the star is from celestial equator. The Declination is how up or down compared to the celestial equator and is expressed in degrees. For 133 Tauri, the location is 05h 47m 42.90 and +13 d 53 ` 58.7 .
All stars like planets orbit round a central spot, in the case of planets, its the central star such as the Sun. In the case of a star, its the galactic centre. The constellations that we see today will be different than they were 50,000 years ago or 50,000 years from now. Proper Motion details the movements of these stars and are measured in milliarcseconds. The star is moving -013.00 ± 000.00 towards the north and 005.00 ± 000.00 east if we saw them in the horizon.
133 Tauri has a spectral type of B2IV-V. This means the star is a blue coloured subgiant star. The star has a B-V Colour Index of -0.15 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 13,674 Kelvin.
133 Tauri has been calculated as 3.66 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,544,564.52.km.
133 Tauri has an apparent magnitude of 5.28 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. If you used the 1997 Parallax value, you would get an absolute magnitude of -1.71 If you used the 2007 Parallax value, you would get an absolute magnitude of -1.23. Magnitude, whether it be apparent/visual or absolute magnitude is measured by a number, the smaller the number, the brighter the Star is. Our own Sun is the brightest star and therefore has the lowest of all magnitudes, -26.74. A faint star will have a high number.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 4.00 which gave the calculated distance to 133 Tauri as 815.41 light years away from us or 250 parsecs. In 2007, Hipparcos data was revised with a new parallax of 5.00 which put 133 Tauri at a distance of 652.33 light years or 200 parsecs.
The source of the information if it has a Hip I.D. is from Simbad, the Hipparcos data library based at the University at Strasbourg, France. Hipparcos was a E.S.A. satellite operation launched in 1989 for four years. The items in red are values that I've calculated so they could well be wrong. Information regarding Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional Name||133 Tauri|
|Short Name||133 Tau|
|Alternative Name(s)||133 Tauri|
|Hipparcos Library I.D.||27364|
|Henry Draper Designation||38622|
|Absolute Magnitude||-1.71 / -1.23|
|Right Ascension (R.A.)||05h 47m 42.90|
|Declination (Dec.)||+13 d 53 ` 58.7|
|1997 Distance||4.00 Parallax (milliarcseconds)|
|815.41 Light Years|
|2007 Distance||5.00 Parallax (milliarcseconds)|
|652.33 Light Years|
|Proper Motion Dec.||-13.00 ± 0.00 milliarcseconds/year|
|Proper Motion RA.||5.00 ± 0.00 milliarcseconds/year|
|Star Type||subgiant star|
|Radius (x the Sun)||3.66|
|Calculated Effective Temperature||13,674 Kelvin|