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Tau2 Capricorni, 14 Capricorni, HD196662, HIP101923, HR7889

Tau2 Capricorni is a blue giant star that can be located in the constellation of Capricornus. 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.

Tau2 Capricorni's Alternative Names

Tau2 Capricorni (Tau Cap) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR7889. HIP101923 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD196662.

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 14 Capricorni with it shortened to 14 Cap.

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-15 5743.

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

Location of Tau2 Capricorni

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 Tau2 Capricorni, the location is 20h 39m 16.32 and -14° 57` 17.0 .

Proper Motion of Tau2 Capricorni

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 -19.46 ± 0.29 miliarcseconds/year towards the north and 2.62 ± 0.65 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 -4.10000 km/s with an error of about 2.10 km/s .

Physical Properties (Colour, Temperature) of Tau2 Capricorni

Tau2 Capricorni has a spectral type of B7III. This means the star is a blue giant star. The star has a B-V Colour Index of -0.12 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 12,367 Kelvin.

Tau2 Capricorni Radius has been calculated as being 9.78 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 6,806,010.06.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 6.34. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Tau2 Capricorni Apparent and Absolute Magnitudes

Tau2 Capricorni has an apparent magnitude of 5.24 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 -3.41 If you used the 2007 Parallax value, you would get an absolute magnitude of -2.47. 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 Tau2 Capricorni

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 1.86 which gave the calculated distance to Tau2 Capricorni as 1753.57 light years away from Earth or 537.63 parsecs. It would take a spaceship travelling at the speed of light, 1753.57 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 2.87 which put Tau2 Capricorni at a distance of 1136.46 light years or 348.43 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.

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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Tau2 Capricorni Facts

Visual Facts


Primary / Proper / Traditional NameTau2 Capricorni
Alternative NamesTau Cap, HD 196662, HIP 101923, HR 7889, 14 Capricorni, 14 Cap, BD-15 5743
Spectral TypeB7III
Multiple Star SystemYes
Star TypeGiant Star
Colour blue
GalaxyMilky Way
ConstellationCapricornus
Absolute Magnitude-3.41 / -2.47
Visual / Apparent Magnitude5.24
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)20h 39m 16.32
Declination (Dec.)-14° 57` 17.0
Galactic Latitude-30.50 degrees
Galactic Longitude30.94 degrees
1997 Distance from Earth1.86 Parallax (milliarcseconds)
 1753.57 Light Years
 537.63 Parsecs
2007 Distance from Earth2.87 Parallax (milliarcseconds)
 1136.46 Light Years
 348.43 Parsecs
Proper Motion Dec.-19.46 ± 0.29 milliarcseconds/year
Proper Motion RA.2.62 ± 0.65 milliarcseconds/year
B-V Index-0.12
Radial Velocity-4.10 ± 2.10 km/s
Associated / Clustered StarsTau1 Capricorni

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Facts


Calculated Effective Temperature12,367 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
196662-15 5743.0A5.600005.00000-21.00000B5Blue/White
B6.900001900
C12.100001912

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