HIP51112 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD90548.
AU Antliae has alternative name(s) :- , AU Ant.
More details on objects' alternative names can be found at Star Names .
The location of the giant star in the night sky 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 object is compared to the celestial equator and is expressed in degrees. For AU Antliae, the location is 10h 26m 34.67 and -34° 42` 03.0 .
AU Antliae has a spectral type of M3III. This means the star is a red giant star. The star has a B-V Colour Index of 1.57 which means the star's temperature is about 3,850 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu at being .
AU Antliae has an apparent magnitude of 8.40 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied 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 -0.28 which gave the calculated distance to AU Antliae as -11648.69 light years away from Earth or -3571.43 parsecs. If you want that in miles, it is -7,811,805,220,066.
The star is a pulsating Semi-Regular Star w 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. AU Antliae brightness ranges from a magnitude of 8.505 to a magnitude of 8.276 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.2 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.
|Primary / Proper / Traditional Name||AU Antliae|
|Alternative Names||HD 90548, HIP 51112, AU Ant|
|Constellation's Main Star||No|
|Multiple Star System||No / Unknown|
|Star Type||Giant Star|
|Visual / Apparent Magnitude||8.40|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||10h 26m 34.67|
|Declination (Dec.)||-34° 42` 03.0|
|Galactic Latitude||19.31 degrees|
|Galactic Longitude||271.95 degrees|
|Distance from Earth||-0.28 Parallax (milliarcseconds)|
|-11648.69 Light Years|
|-736,655,183.89 Astronomical Units|
|Variable Star Class||Pulsating|
|Variable Star Type||Semi-Regular Star w|
|Mean Variability Period in Days||0.172|
|Variable Magnitude Range (Brighter - Dimmer)||8.276 - 8.505|
|Effective Temperature||3,850 Kelvin|
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