AE Phoenicis is a white to yellow eclipsing subgiant star that can be located in the constellation of Phoenix. The star can not be seen by the naked eye, you need a telescope to see it.
HIP7183 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD9528.
AE Phoenicis has alternative name(s), AE Phe.
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 AE Phoenicis, the location is 01h 32m 32.80 and -49d31`40.8 .
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 -55.79 ± 0.72 miliarcseconds/year towards the north and 150.64 ± 0.90 miliarcseconds/year east if we saw them in the horizon.
AE Phoenicis has a spectral type of G1/G2IV/V. This means the star is a white to yellow subgiant star. The star is 7394.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24116.5176553600000000s. The star has a B-V Colour Index of 0.64 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,755 Kelvin.
AE Phoenicis Radius has been calculated as being 1.27 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 885,634.58.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.32. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is -0.20 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.
AE Phoenicis has an apparent magnitude of 7.78 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 4.34 If you used the 2007 Parallax value, you would get an absolute magnitude of 4.26. 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 20.49 which gave the calculated distance to AE Phoenicis as 159.18 light years away from Earth or 48.80 parsecs. It would take a spaceship travelling at the speed of light, 159.18 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 19.74 which put AE Phoenicis at a distance of 165.23 light years or 50.66 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 star's Galacto-Centric Distance is 7,394.00 Parsecs or 24,116.52 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.
The star is a eclipsing W Ursae Majoris/Contact systems of the W UMa type, with ellipsoidal components of F0-K spectral type 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. AE Phoenicis brightness ranges from a magnitude of 8.356 to a magnitude of 7.673 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.4 days (variability).
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 Metallicity and/or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.
|Traditional/Proper Name||AE Phoenicis|
|Short Name||AE Phe|
|Hipparcos Library I.D.||7183|
|Henry Draper Designation||9528|
|Star Type||subgiant star|
|Absolute Magnitude||4.34 / 4.26|
|Visual / Apparent Magnitude||7.78|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||01h 32m 32.80|
|Galactic Latitude||-66.25 degrees|
|Galactic Longitude||286.22 degrees|
|1997 Distance from Earth||20.49 Parallax (milliarcseconds)|
|159.18 Light Years|
|2007 Revised Distance from Earth||19.74 Parallax (milliarcseconds)|
|165.23 Light Years|
|Galacto-Centric Distance||24,116.52 Light Years / 7,394.00 Parsecs|
|Proper Motion Dec.||-55.79 ± 0.72 milliarcseconds/year|
|Proper Motion RA.||150.64 ± 0.90 milliarcseconds/year|
|Radial Velocity||-9.50 ± 2.50 km/s|
|Iron Abundance||-0.20 ± 9.99 Fe/H|
|Colour||(G) White to Yellow|
|Variable Star Class||Eclipsing|
|Variable Star Type||W Ursae Majoris/Contact systems of the W UMa type, with ellipsoidal components of F0-K spectral type|
|Mean Variability Period in Days||0.362|
|Variable Magnitude Range (Brighter - Dimmer)||7.673 - 8.356|
|Calculated Effective Temperature||5,755 Kelvin|