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V486 Carinae, HD84416, HIP47591

V486 Carinae is a blue eclipsing binary system main sequence dwarf star that can be located in the constellation of Carina. The description is based on the spectral class. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

V486 Carinae's Alternative Names

HIP47591 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD84416.

V486 Carinae has alternative name(s) :- , V486 Car.

More details on star alternative names can be found at Star Names .

Location of V486 Carinae

The location of the 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 star is compared to the celestial equator and is expressed in degrees. For V486 Carinae, the location is 09h 42m 12.99 and -66° 54` 53.4 .

Proper Motion of V486 Carinae

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 -0.11 ± 0.28 miliarcseconds/year towards the north and -14.84 ± 0.32 miliarcseconds/year east if we saw them in the horizon.

V486 Carinae Luminosity

Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 65.33 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Physical Properties (Colour, Temperature) of V486 Carinae

V486 Carinae has a spectral type of A0V. This means the star is a blue main sequence dwarf star. The star is 7,359.00 Parsecs from the Galactic Centre or terms of Light Years is 24,002.36 s. The star has a B-V Colour Index of 0.07 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,718 Kelvin.

V486 Carinae Radius has been calculated as being 4.02 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,796,106.49.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 3.55. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

V486 Carinae Apparent and Absolute Magnitudes

V486 Carinae has an apparent magnitude of 6.33 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 0.04 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.31. 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.

Distance to V486 Carinae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 5.51 which gave the calculated distance to V486 Carinae as 591.95 light years away from Earth or 181.49 parsecs. It would take a spaceship travelling at the speed of light, 591.95 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 6.25 which put V486 Carinae at a distance of 521.86 light years or 160 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 7,359.00 Parsecs or 24,002.36 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Variable Type of V486 Carinae

The star is a eclipsing binary system Beta Lyrae (Sheliak) 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. V486 Carinae brightness ranges from a magnitude of 6.451 to a magnitude of 6.288 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 1.1 days (variability).

Source of Information

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.

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V486 Carinae Facts

Visual Facts


Primary / Proper / Traditional NameV486 Carinae
Alternative NamesHD 84416, HIP 47591, V486 Car
Spectral TypeA0V
Multiple Star SystemYes
Star Type main sequence Dwarf Star
Colour blue
GalaxyMilky Way
ConstellationCarina
Absolute Magnitude0.04 / 0.31
Visual / Apparent Magnitude6.33
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)09h 42m 12.99
Declination (Dec.)-66° 54` 53.4
Galactic Latitude-10.54 degrees
Galactic Longitude285.89 degrees
1997 Distance from Earth5.51 Parallax (milliarcseconds)
 591.95 Light Years
 181.49 Parsecs
2007 Distance from Earth6.25 Parallax (milliarcseconds)
 521.86 Light Years
 160 Parsecs
Galacto-Centric Distance24,002.36 Light Years / 7,359.00 Parsecs
Proper Motion Dec.-0.11 ± 0.28 milliarcseconds/year
Proper Motion RA.-14.84 ± 0.32 milliarcseconds/year
B-V Index0.07
Stellar Luminosity (Lsun)65.33

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassEclipsing binary system
Variable Star TypeBeta Lyrae (Sheliak)
Mean Variability Period in Days1.094
Variable Magnitude Range (Brighter - Dimmer)6.288 - 6.451

Estimated Facts


Calculated Effective Temperature8,718 Kelvin

Sources and Links


SIMBAD SourceLink

Multi-Star System

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. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
84416-66 1042.4A6.60000-5.00000-2.00000A0White
-66 1039.4B10.60000-6.0000013.000001918

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