HIP73152 is the reference name for the star in the Hipparcos Star Catalogue.
EN Trianguli Australis has alternative name(s) :- EN TrA, EN TrA.
More details on objects' alternative names can be found at Star Names .
The location of the supergiant 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 EN Trianguli Australis, the location is 14h 57m 00.69 and -68° 50` 22.9 .
EN Trianguli Australis has a spectral type of F2Ib. This means the star is a yellow to white supergiant star. The star has a B-V Colour Index of 0.74 which means the star's temperature is about 5,558 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu at being .
EN Trianguli Australis has an apparent magnitude of 8.69 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 -1.29 which gave the calculated distance to EN Trianguli Australis as -2528.40 light years away from Earth or -775.19 parsecs. If you want that in miles, it is -1,695,587,084,764.
The star is a pulsating Cepheids 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. EN Trianguli Australis brightness ranges from a magnitude of 9.120 to a magnitude of 8.750 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 37.1 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||EN Trianguli Australis|
|Alternative Names||EN TrA, HIP 73152, EN TrA|
|Constellation's Main Star||No|
|Multiple Star System||No / Unknown|
|Star Type||very luminous Supergiant Star less luminour Supergiant Star|
|Colour||Yellow - White|
|Visual / Apparent Magnitude||8.69|
|Naked Eye Visible||Requires a 7x50 Binoculars - Magnitudes|
|Right Ascension (R.A.)||14h 57m 00.69|
|Declination (Dec.)||-68° 50` 22.9|
|Galactic Latitude||-8.68 degrees|
|Galactic Longitude||313.90 degrees|
|Distance from Earth||-1.29 Parallax (milliarcseconds)|
|-2528.40 Light Years|
|-159,893,301.00 Astronomical Units|
|Radial Velocity||-3.00 ± 999.00 km/s|
|Variable Star Class||Pulsating|
|Variable Star Type||Cepheids|
|Mean Variability Period in Days||37.100|
|Variable Magnitude Range (Brighter - Dimmer)||8.750 - 9.120|
|Effective Temperature||5,558 Kelvin|
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