R Bootis is a red pulsating star that can be located in the constellation of Bootes. HIP71490 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD128609. R Bootis has alternative name(s), R_Boo.
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 R Bootis, the location is 14h 37m 11.59 and +26 d 44`11.6 .
R Bootis has a spectral type of M3e-M8e. This means the star is a red star. The star has a B-V Colour Index of 1.5 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,014 Kelvin.
R Bootis has an apparent magnitude of 9.98 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 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 -2.00 which gave the calculated distance to R Bootis as -1630.82 light years away from Earth or -500 parsecs. It would take a spaceship travelling at the speed of light, -1630.82 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.
The star is a pulsating Omicron Ceti variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. R Bootis brightness ranges from a magnitude of 11.000 to a magnitude of 7.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 225.0 days (variability).
|Traditional Name||R Bootis|
|Short Name||R Boo|
|Hipparcos Library I.D.||71490|
|Bonner Durchmusterung||BD+27 2400|
|Henry Draper Designation||128609|
|Right Ascension (R.A.)||14h 37m 11.59|
|Declination (Dec.)||+26 d 44`11.6|
|1997 Distance from Earth||-2.00 Parallax (milliarcseconds)|
|-1630.82 Light Years|
|Variable Star Class||Pulsating|
|Variable Star Type||Omicron Ceti|
|Mean Variability Period in Days||225.000|
|Variable Magnitude Range (Brighter - Dimmer)||7.000 - 11.000|
|Calculated Effective Temperature||4,014 Kelvin|