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Kappa Aurigae, 44 Aurigae, HD43039, HIP29696, HR2219

Kappa Aurigae is a white to yellow star that can be located in the constellation of Auriga. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

Kappa Aurigae is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR2219. HIP29696 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD43039.

Location of Kappa Aurigae

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 Kappa Aurigae, the location is 06h 15m 22.74 and +29d 29` 55.4 .

Proper Motion of Kappa Aurigae

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 -261.42 ± 0.14 miliarcseconds/year towards the north and -70.88 ± 0.23 miliarcseconds/year east if we saw them in the horizon. The Radial Velocity, that is the speed at which the star is moving away/towards us is 20.69000 km/s with an error of about 0.23 km/s .

Physical Properties (Colour, Temperature, Radius) of Kappa Aurigae

Kappa Aurigae has a spectral type of G8IIIvar. This means the star is a white to yellow star. The star is 7454.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24312.2156617600000000s. The star has a B-V Colour Index of 1.02 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,811 Kelvin.

Kappa Aurigae Radius has been calculated as being 9.52 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 6,620,789.09.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 9.96. 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 -0.33 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

Kappa Aurigae Apparent and Absolute Magnitudes

Kappa Aurigae has an apparent magnitude of 4.32 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 0.75 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.65. 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 Kappa Aurigae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 19.31 which gave the calculated distance to Kappa Aurigae as 168.91 light years away from Earth or 51.79 parsecs. It would take a spaceship travelling at the speed of light, 168.91 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 18.43 which put Kappa Aurigae at a distance of 176.97 light years or 54.26 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 7,454.00 Parsecs or 24,312.22 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

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.

Kappa Aurigae Facts

Alternative Names

Flamsteed Name44 Aurigae
Flamsteed Short Name44 Aur
Bayer DesignationKappa Aurigae
Hipparcos Library I.D.29696
Yale Bright Star Catalogue (HR) Id2219
Bonner DurchmusterungBD+29 1154
Henry Draper Designation43039

Visual Facts

Star Type star
Absolute Magnitude0.75 / 0.65
Visual / Apparent Magnitude4.32
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)06h 15m 22.74
Declination (Dec.)+29d 29` 55.4
Galactic Latitude5.92 degrees
Galactic Longitude182.73 degrees
1997 Distance from Earth19.31 Parallax (milliarcseconds)
 168.91 Light Years
 51.79 Parsecs
2007 Revised Distance from Earth18.43 Parallax (milliarcseconds)
 176.97 Light Years
 54.26 Parsecs
Galacto-Centric Distance24,312.22 Light Years / 7,454.00 Parsecs
Proper Motion Dec.-261.42 ± 0.14 milliarcseconds/year
Proper Motion RA.-70.88 ± 0.23 milliarcseconds/year
B-V Index1.02
Radial Velocity20.69 ± 0.23 km/s
Iron Abundance-0.33 ± 9.99 Fe/H
Spectral TypeG8IIIvar
Colour(G) White to Yellow

Estimated Facts

Calculated Effective Temperature4,811 Kelvin

Sources and Links

SIMBAD SourceLink

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