Universe GuideSearchTwitterComments

TX Canum Venaticorum (Symbiotic/Vampire Star) Facts

TX Canum Venaticorum Facts

TX Canum Venaticorum's Alternative Names

TX Canum Venaticorum has alternative name(s) :- TX CVn.

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+37 2318.

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

Location of TX Canum Venaticorum

The location of the main sequence 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 TX Canum Venaticorum, the location is 12 44 42.0645704232 and +36 45 50.622366015 .

Proper Motion of TX 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 -5.35 milliarcseconds/year towards the north and -13.73 milliarcseconds/year east if we saw them in the horizon. . 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.

Physical Properties (Colour) of TX Canum Venaticorum

TX Canum Venaticorum Colour and Temperature

TX Canum Venaticorum has a spectral type of B1-B9Veq+K0III-M4 C. This means the star is a blue main sequence star.

Distance to TX Canum Venaticorum

The Parallax of the star is given as 0.35 which gives a calculated distance to TX Canum Venaticorum of 9244.99 light years from the Earth or 2834.47 parsecs. It would take a spaceship travelling at the speed of light, 9244.99 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

The star is roughly 584,647,331.48 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.

Hide Explanations
Show GridLines

Additional TX Canum Venaticorum Facts and Figures

Visual Facts

Primary / Proper / Traditional NameTX Canum Venaticorum
Alternative NamesTX CVn, BD+37 2318
Spectral TypeB1-B9Veq+K0III-M4 C
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star Type Main Sequence Dwarf Star
GalaxyMilky Way
ConstellationCanes Venatici
Right Ascension (R.A.)12 44 42.0645704232
Declination (Dec.)+36 45 50.622366015
Distance from Earth0.35 Parallax (milliarcseconds)
 9244.99 Light Years
 2834.47 Parsecs
 584,647,331.48 Astronomical Units
Proper Motion Dec.-5.35 milliarcseconds/year
Proper Motion RA.-13.73 milliarcseconds/year

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Sources and Links


Related Stars

Comments and Questions

There's no register feature and no need to give an email address if you don't need to. All messages will be reviewed before being displayed. Comments may be merged or altered slightly such as if an email address is given in the main body of the comment.

This website is using cookies. More info. That's Fine