Universe Guide
HomeAliensConstellationsTelevision and Films ListFact ListGames ListWarcraftSearchTwitterFacebook

180 G. Centauri, HD114461, HIP64395

180 G. Centauri is a blue to white luminous giant star that can be located in the constellation of Centaurus. 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.

180 G. Centauri's Alternative Names

HIP64395 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD114461.

The Gould star designation is one that was designed by American astronomer, Benjamin Apthorp Gould. Gould stars are predominantly in the Southern and Equatorial constellations but do appear in northern constellations such as Bootes and Orion. The star has the designation 180 G. Centauri. There are no stars with a Gould designation in Ursa Major for example.

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

Location of 180 G. Centauri

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 180 G. Centauri, the location is 13h 11m 53.07 and -63° 18` 10.7 .

Proper Motion of 180 G. 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 -2.56 ± 0.33 miliarcseconds/year towards the north and -4.56 ± 0.45 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 -3.30000 km/s with an error of about 2.10 km/s .

Physical Properties (Colour, Temperature) of 180 G. Centauri

180 G. Centauri has a spectral type of F0II. This means the star is a blue to white luminous giant star. The star has a B-V Colour Index of 0.42 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,335 Kelvin.

180 G. Centauri Apparent and Absolute Magnitudes

180 G. Centauri has an apparent magnitude of 6.32 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 If you used the 2007 Parallax value, you would get an absolute magnitude of -5.02. 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 180 G. Centauri

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as -0.29 which gave the calculated distance to 180 G. Centauri as -11247.01 light years away from Earth or -3448.28 parsecs. It would take a spaceship travelling at the speed of light, -11247.01 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 0.54 which put 180 G. Centauri at a distance of 6040.06 light years or 1851.85 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.

Hide Explanations
Show GridLines

180 G. Centauri Facts

Visual Facts


Primary / Proper / Traditional Name180 G. Centauri
Alternative NamesHD 114461, HIP 64395
Spectral TypeF0II
Multiple Star SystemNo / Unknown
Star TypeLuminous Giant Star
Colour blue to white
GalaxyMilky Way
ConstellationCentaurus
Visual / Apparent Magnitude6.32
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)13h 11m 53.07
Declination (Dec.)-63° 18` 10.7
Galactic Latitude-0.52 degrees
Galactic Longitude305.23 degrees
1997 Distance from Earth-0.29 Parallax (milliarcseconds)
 -11247.01 Light Years
 -3448.28 Parsecs
2007 Distance from Earth0.54 Parallax (milliarcseconds)
 6040.06 Light Years
 1851.85 Parsecs
Proper Motion Dec.-2.56 ± 0.33 milliarcseconds/year
Proper Motion RA.-4.56 ± 0.45 milliarcseconds/year
B-V Index0.42
Radial Velocity-3.30 ± 2.10 km/s

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Facts


Calculated Effective Temperature6,335 Kelvin

Sources and Links


SIMBAD SourceLink

Related Stars


Add a Comment


Name:
Email: (Optional)
Comment: