HIP78053 is the reference name for the star in the Hipparcos Star Catalogue.
IM Lupi has alternative name(s) :- , IM Lup.
More details on objects' alternative names can be found at Star Names .
The location of the variable 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 IM Lupi, the location is 15h 56m 09.21 and -37° 56` 05.9 .
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||IM Lupi|
|Alternative Names||HIP 78053, IM Lup|
|Constellation's Main Star||No|
|Multiple Star System||Yes|
|Star Type||Variable Star|
|Visual / Apparent Magnitude||11.57|
|Naked Eye Visible||Requires a 4.5 - 6 Inch Telescope - Magnitudes|
|Right Ascension (R.A.)||15h 56m 09.21|
|Declination (Dec.)||-37° 56` 05.9|
|Galactic Latitude||11.87 degrees|
|Galactic Longitude||338.49 degrees|
|Distance from Earth||-4.77 Parallax (milliarcseconds)|
|-683.78 Light Years|
|-43,241,052.67 Astronomical Units|
|Radial Velocity||-1.00 ± 999.00 km/s|
|Mean Variability Period in Days||0.475|
|Variable Magnitude Range (Brighter - Dimmer)||11.390 - 12.080|
The star has been identified as being a multi-star system, one in which there is at least one star in close orbit to another star or two or more stars orbiting a central point. The stars may be of equal mass, unequal mass where one star is stronger than the other or be in groups orbiting a central point which doesn't necessarily have to be a star. More information can be found on my dedicated multiple star systems page. The source of the info is Simbad. The file is dated 2000 so any differences between this and any other source will be down to the actual source from where the information came from.
|Proper Motion mas/yr|
|H.D. Id||B.D. Id||Star Code||Magnitude||R.A.||Dec.||Spectrum||Colour||Year|
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