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62 G. Cen, HD101995, HIP57211

62 G. Cen is a blue star that can be located in the constellation of Centaurus. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

HIP57211 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD101995. The Id of the star in the Gould Star Catalogue is 62. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major.

Location of 62 G. Cen

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 62 G. Cen, the location is 11h 43m 52.82 and -62d 52` 41.7 .

Proper Motion of 62 G. Cen

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 -14.80 ± 0.21 miliarcseconds/year towards the north and 13.64 ± 0.28 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 2.30000 km/s with an error of about 3.00 km/s .

Physical Properties (Colour, Temperature, Radius) of 62 G. Cen

62 G. Cen has a spectral type of A2III/IV. This means the star is a blue star. The star is 7341.00000000 Parsecs from the Galactic Centre or terms of Light Years is 23943.6510830400000000s. The star has a B-V Colour Index of 0.06 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 8,815 Kelvin.

62 G. Cen Radius has been calculated as being 2.93 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,036,744.35.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 3.41. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

62 G. Cen Apparent and Absolute Magnitudes

62 G. Cen has an apparent magnitude of 6.10 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 0.68 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.35. 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 62 G. Cen

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 8.23 which gave the calculated distance to 62 G. Cen as 396.31 light years away from Earth or 121.51 parsecs. It would take a spaceship travelling at the speed of light, 396.31 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 7.09 which put 62 G. Cen at a distance of 460.03 light years or 141.04 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 7,341.00 Parsecs or 23,943.65 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.

62 G. Cen Facts

Alternative Names

Traditional/Proper Name62 G. Cen
Hipparcos Library I.D.57211
Gould I.D.62
Henry Draper Designation101995

Visual Facts

Star Type star
Absolute Magnitude0.68 / 0.35
Visual / Apparent Magnitude6.10
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)11h 43m 52.82
Declination (Dec.)-62d 52` 41.7
Galactic Latitude-1.01 degrees
Galactic Longitude295.32 degrees
1997 Distance from Earth8.23 Parallax (milliarcseconds)
 396.31 Light Years
 121.51 Parsecs
2007 Revised Distance from Earth7.09 Parallax (milliarcseconds)
 460.03 Light Years
 141.04 Parsecs
Galacto-Centric Distance23,943.65 Light Years / 7,341.00 Parsecs
Proper Motion Dec.-14.80 ± 0.21 milliarcseconds/year
Proper Motion RA.13.64 ± 0.28 milliarcseconds/year
B-V Index0.06
Radial Velocity2.30 ± 3.00 km/s
Spectral TypeA2III/IV
Colour(A) blue

Estimated Facts

Calculated Effective Temperature8,815 Kelvin

Sources and Links

SIMBAD SourceLink

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