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HomeFactsConstellationsCanes Venatici

TU Canum Venaticorum, HD112264, HIP63024, HR4909

TU Canum Venaticorum is a red pulsating giant star that can be located in the constellation of CanesVenatici. TU Canum Venaticorum is the brightest star in Canes Venatici based on the Hipparcos 2007 apparent magnitude. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

The Id of the star in the Yale Bright Star Catalogue is HR4909. HIP63024 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD112264.

TU Canum Venaticorum has alternative name(s), TU CVn.

Location of TU Canum Venaticorum

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 TU Canum Venaticorum, the location is 12h 54m 56.54 and +47d 11` 48.3 .

Proper Motion of TU Canum Venaticorum

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 -6.11 ± 0.20 miliarcseconds/year towards the north and -17.24 ± 0.32 miliarcseconds/year east if we saw them in the horizon.

TU Canum Venaticorum 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 5.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.

Physical Properties (Colour, Temperature, Radius) of TU Canum Venaticorum

TU Canum Venaticorum has a spectral type of M5III. This means the star is a red giant star. The star is 7441.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24269.8144270400000000s. The star has a B-V Colour Index of 1.45 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,076 Kelvin.

TU Canum Venaticorum Radius has been calculated as being 28.61 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 19,903,456.85.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 28.21. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

TU Canum Venaticorum Apparent and Absolute Magnitudes

TU Canum Venaticorum has an apparent magnitude of 5.75 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 -0.92 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.89. 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 TU Canum Venaticorum

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 4.63 which gave the calculated distance to TU Canum Venaticorum as 704.46 light years away from Earth or 215.98 parsecs. It would take a spaceship travelling at the speed of light, 704.46 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 4.69 which put TU Canum Venaticorum at a distance of 695.44 light years or 213.22 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 7,441.00 Parsecs or 24,269.81 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 TU Canum Venaticorum

The star is a pulsating Semiregular late- (M, C, S or Me, Ce, Se) giants with poorly defined periodicity 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. TU Canum Venaticorum brightness ranges from a magnitude of 5.801 to a magnitude of 5.552 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.2 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.

TU Canum Venaticorum Facts

Alternative Names

Traditional/Proper NameTU Canum Venaticorum
Short NameTU CVn
Hipparcos Library I.D.63024
Yale Bright Star Catalogue (HR) Id4909
Bonner DurchmusterungBD+47 2003
Henry Draper Designation112264

Visual Facts

Star Typegiant star
ConstellationCanes Venatici
Absolute Magnitude-0.92 / -0.89
Visual / Apparent Magnitude5.75
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)12h 54m 56.54
Declination (Dec.)+47d 11` 48.3
Galactic Latitude69.92 degrees
Galactic Longitude121.20 degrees
1997 Distance from Earth4.63 Parallax (milliarcseconds)
 704.46 Light Years
 215.98 Parsecs
2007 Revised Distance from Earth4.69 Parallax (milliarcseconds)
 695.44 Light Years
 213.22 Parsecs
Galacto-Centric Distance24,269.81 Light Years / 7,441.00 Parsecs
Proper Motion Dec.-6.11 ± 0.20 milliarcseconds/year
Proper Motion RA.-17.24 ± 0.32 milliarcseconds/year
B-V Index1.45
Radial Velocity-17.94 ± 0.42 km/s
Spectral TypeM5III
Colour(M) Red

Variable Star Details

Variable Star ClassPulsating
Variable Star TypeSemiregular late- (M, C, S or Me, Ce, Se) giants with poorly defined periodicity
Mean Variability Period in Days0.203
Variable Magnitude Range (Brighter - Dimmer)5.552 - 5.801

Estimated Facts

Luminosity (x the Sun)5.0000000
Calculated Effective Temperature4,076 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

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