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Psi Centauri, HD125473, HIP70090, HR5367

Psi Centauri 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.

Psi Centauri is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR5367. HIP70090 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD125473. The Id of the star in the Gould Star Catalogue is 338. 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 Psi Centauri

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 Psi Centauri, the location is 14h 20m 33.48 and -37d 53` 07.0 .

Proper Motion of Psi Centauri

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 -10.65 ± 0.11 miliarcseconds/year towards the north and -63.69 ± 0.20 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 1.80000 km/s with an error of about 0.90 km/s .

Physical Properties (Colour, Temperature, Radius) of Psi Centauri

Psi Centauri has a spectral type of A0IV. This means the star is a blue star. The star is 7342.00000000 Parsecs from the Galactic Centre or terms of Light Years is 23946.9127164800000000s. The star has a B-V Colour Index of -0.03 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 10,010 Kelvin.

Psi Centauri Radius has been calculated as being 3.65 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,538,184.05.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 3.82. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Psi Centauri Apparent and Absolute Magnitudes

Psi Centauri has an apparent magnitude of 4.05 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 -0.35 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.45. 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 Psi Centauri

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 13.19 which gave the calculated distance to Psi Centauri as 247.28 light years away from Earth or 75.82 parsecs. It would take a spaceship travelling at the speed of light, 247.28 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 12.60 which put Psi Centauri at a distance of 258.86 light years or 79.37 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 7,342.00 Parsecs or 23,946.91 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.

Psi Centauri Facts

Alternative Names

Bayer DesignationPsi Centauri
Hipparcos Library I.D.70090
Yale Bright Star Catalogue (HR) Id5367
Gould I.D.338
Henry Draper Designation125473

Visual Facts

Star Type star
Absolute Magnitude-0.35 / -0.45
Visual / Apparent Magnitude4.05
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)14h 20m 33.48
Declination (Dec.)-37d 53` 07.0
Galactic Latitude21.71 degrees
Galactic Longitude321.72 degrees
1997 Distance from Earth13.19 Parallax (milliarcseconds)
 247.28 Light Years
 75.82 Parsecs
2007 Revised Distance from Earth12.60 Parallax (milliarcseconds)
 258.86 Light Years
 79.37 Parsecs
Galacto-Centric Distance23,946.91 Light Years / 7,342.00 Parsecs
Proper Motion Dec.-10.65 ± 0.11 milliarcseconds/year
Proper Motion RA.-63.69 ± 0.20 milliarcseconds/year
B-V Index-0.03
Radial Velocity1.80 ± 0.90 km/s
Spectral TypeA0IV
Colour(A) blue

Estimated Facts

Calculated Effective Temperature10,010 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

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
125473-37 9336.2A4.20000-68.00000-16.00000A0White

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