Pi Ceti is a blue subgiant star that can be located in the constellation of Cetus. Pi Ceti is the Bayer Classification for the star. HIP12770 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD17081. The Id of the star in the Gould Star Catalogue is 296. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major. Pi Ceti has alternative name(s), 89 Ceti , 89 Cet.
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 along the celestial equator. If the R.A. is positive then its eastwards. The Declination is how far north or south the star is compared to the celestial equator and is expressed in degrees. For Pi Ceti, the location is 02h 44m 07.35 and -13d51`31.2 .
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 -009.07 ± 000.15 towards the north and -008.62 ± 000.21 east if we saw them in the horizon.
Pi Ceti has a spectral type of B7IV. This means the star is a blue subgiant star. The star has a B-V Colour Index of -0.12 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 12,367 Kelvin.
Pi Ceti has been calculated as 3.89 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,709,398.91.km.
Pi Ceti has an apparent magnitude of 4.24 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 -1.41 If you used the 2007 Parallax value, you would get an absolute magnitude of -1.16. 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 7.40 which gave the calculated distance to Pi Ceti as 440.76 light years away from Earth or 135.14 parsecs. It would take a spaceship travelling at the speed of light, 440.76 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
In 2007, Hipparcos data was revised with a new parallax of 8.30 which put Pi Ceti at a distance of 392.97 light years or 120.48 parsecs. It should not be taken as though the star is moving closer or further away from us. It is purely that the distance was recalculated.
The Pi Cetids Meteor Shower radiants from a point near this star. The meteor shower runs typically between 16 Jun- 4 Jul with a peak date of 26-Jun. The speed of a meteor in the shower is 67 Km/s. The amount of meteors predicted to be seen per hour (Zenith Hourly Rate) is 67. p>
|Short Name||89 Cet|
|Bayer Designation||Pi Ceti|
|Alternative Name(s)||89 Ceti|
|Hipparcos Library I.D.||12770|
|Bonner Durchmusterung||BD-14 519|
|Henry Draper Designation||17081|
|Star Type||subgiant star|
|Absolute Magnitude||-1.41 / -1.16|
|Right Ascension (R.A.)||02h 44m 07.35|
|1997 Distance from Earth||7.40 Parallax (milliarcseconds)|
|440.76 Light Years|
|2007 Revised Distance from Earth||8.30 Parallax (milliarcseconds)|
|392.97 Light Years|
|Proper Motion Dec.||-9.07 ± 0.15 milliarcseconds/year|
|Proper Motion RA.||-8.62 ± 0.21 milliarcseconds/year|
|Radius (x the Sun)||3.89|
|Calculated Effective Temperature||12,367 Kelvin|