Universe Guide

Cor Caroli (Alpha2 Canum Venaticorum, 12 Canum Venaticorum A) Star Facts

Cor Caroli Facts

Cor Caroli's Alternative Names

Alpha2 Canum Venaticorum (Alf02 Cvn) is the Bayer Classification for the star. The Bayer Classification was created by Johann Bayer in the early nineteenth century. The brightest star in the constellation is normally given the Alpha designation although there are exceptions such as Pollux which is Beta Geminorum.

The Id of the star in the Yale Bright Star Catalogue is HR4915. HIP63125 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD112413.

Cor Caroli has alternative name(s) :- , alf02 CVn.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 12 Canum Venaticorum A with it shortened to 12 Cvn A.

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD+39 2580.

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

Location of Cor Caroli

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 Cor Caroli, the location is 12h 56m 01.84 and +38° 19` 05.7 .

Radial Velocity and Proper Motion of Cor Caroli

Proper Motion

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 53.54 ± 0.55 milliarcseconds/year towards the north and -235.08 ± 0.90 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -4.10 km/s with an error of about 0.20 km/s . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

Cor Caroli 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 148.46 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 Cor Caroli

Cor Caroli Colour and Temperature

Cor Caroli has a spectral type of A0spe.... This means the star is a blue - white variable star. The star has a B-V Colour Index of -0.11 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 14,384 Kelvin.

Cor Caroli Radius

Radius has been calculated as being 1.34 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 932,451.02.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 1.40. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Cor Caroli Apparent and Absolute Magnitudes

Cor Caroli has an apparent magnitude of 2.89 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 0.25 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.16. 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 Cor Caroli

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 29.60 which gave the calculated distance to Cor Caroli as 110.19 light years away from Earth or 33.78 parsecs. If you want that in miles, it is 674,924,979,095,209.12.

In 2007, Hipparcos data was revised with a new parallax of 28.41 which put Cor Caroli at a distance of 114.81 light years or 35.20 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.

Using the 2007 distance, the star is roughly 7,260,470.59 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun.

The star's Galacto-Centric Distance is 7,403.00 Parsecs or 24,145.87 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Time to Travel to Cor Caroli

A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

If you were to drive there at about 120 m.p.h. in a car with an infinity engine so you didn't have to pull over for petrol, it would take you 5,398,047,748,925.84 hours or 616,215,496.45 years.

At the time of writing, the fastest probe so far created is the New Horizon probe which is travelling at a speed of 33,000 m.p.h. If the probe was travelling to Cor Caroli then it would take 19,629,264,541.55 hours / 2,240,783.62 years to get there. Speed Ref: N.A.S.A.

It would to take a spaceship journey travelling at the speed of light, 110.19 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

Variable Type of Cor Caroli

The star is a rotating Alpha2 Canum Venatic 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. Cor Caroli brightness ranges from a magnitude of 2.893 to a magnitude of 2.828 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 5.5 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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Additional Cor Caroli Facts and Figures

Visual Facts

Primary / Proper / Traditional NameCor Caroli
Alternative NamesAlpha2 Canum Venaticorum, Alf02 Cvn, HD 112413, HIP 63125, HR 4915, 12 Canum Venaticorum A, 12 Cvn A, BD+39 2580, alf02 CVn
Spectral TypeA0spe...
Constellation's Main StarNo
Multiple Star SystemYes
Star TypeVariable Star
GalaxyMilky Way
ConstellationCanes Venatici
Absolute Magnitude 0.25 / 0.16
Visual / Apparent Magnitude2.89
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)12h 56m 01.84
Declination (Dec.)+38° 19` 05.7
Galactic Latitude78.77 degrees
Galactic Longitude118.30 degrees
1997 Distance from Earth29.60 Parallax (milliarcseconds)
 110.19 Light Years
 33.78 Parsecs
2007 Distance from Earth28.41 Parallax (milliarcseconds)
 114.81 Light Years
 35.20 Parsecs
 7,260,470.59 Astronomical Units
Galacto-Centric Distance24,145.87 Light Years / 7,403.00 Parsecs
Proper Motion Dec.53.54 ± 0.55 milliarcseconds/year
Proper Motion RA.-235.08 ± 0.90 milliarcseconds/year
B-V Index-0.11
Radial Velocity-4.10 ± 0.20 km/s
Semi-Major Axis7421.00
Stellar Luminosity (Lsun)148.46
Associated / Clustered StarsAlpha1 Canum Venaticorum

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassRotating
Variable Star TypeAlpha2 Canum Venatic
Mean Variability Period in Days5.470
Variable Magnitude Range (Brighter - Dimmer)2.828 - 2.893

Estimated Calculated Facts

Radius (x the Sun)1.40
Effective Temperature14,384 Kelvin

Sources and Links

SIMBAD SourceLink

Location of Cor Caroli in Canes Venatici

Cor Caroli Location in Canes Venatici

The map was generated using Night Vision, an awesome free application by Brian Simpson.

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