Gamma Doradus is a blue to white giant star that can be located in the constellation of Dorado. Gamma Doradus is the Bayer Classification for the star. HIP19893 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD27290. Gamma Doradus has alternative name(s), gam_Dor.
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 Gamma Doradus, the location is 04h 16m 01.49 and -51d29`13.5 .
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 183.32 ± 000.34 towards the north and 100.79 ± 000.36 east if we saw them in the horizon.
Gamma Doradus has a spectral type of F4III. This means the star is a blue to white giant star. The star has a B-V Colour Index of 0.31 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 7,167 Kelvin.
Gamma Doradus has been calculated as 1.73 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,204,165.88.km.
Gamma Doradus has an apparent magnitude of 4.26 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 2.72 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.71. 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 49.26 which gave the calculated distance to Gamma Doradus as 66.21 light years away from Earth or 20.30 parsecs. It would take a spaceship travelling at the speed of light, 66.21 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 48.87 which put Gamma Doradus at a distance of 66.74 light years or 20.46 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. Gamma Doradus brightness ranges from a magnitude of 4.000 to a magnitude of 4.000 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.0 days (variability).
The Gamma Doradids Meteor Shower radiants from a point near this star. The meteor shower runs typically between 27 Aug- 3 Sep with a peak date of 28-Aug. The speed of a meteor in the shower is 40 Km/s. The amount of meteors predicted to be seen per hour (Zenith Hourly Rate) is 40. p>
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.
|Short Name||gam Dor|
|Bayer Designation||Gamma Doradus|
|Hipparcos Library I.D.||19893|
|Henry Draper Designation||27290|
|Star Type||giant star|
|Absolute Magnitude||2.72 / 2.71|
|Right Ascension (R.A.)||04h 16m 01.49|
|1997 Distance from Earth||49.26 Parallax (milliarcseconds)|
|66.21 Light Years|
|2007 Revised Distance from Earth||48.87 Parallax (milliarcseconds)|
|66.74 Light Years|
|Proper Motion Dec.||183.32 ± 0.34 milliarcseconds/year|
|Proper Motion RA.||100.79 ± 0.36 milliarcseconds/year|
|Colour||(F) blue to white|
|Mean Variability Period in Days||1.000|
|Radius (x the Sun)||1.73|
|Calculated Effective Temperature||7,167 Kelvin|