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189 G. Cet - HD11803 - HIP8998

189 G. Cet is a blue to white main sequence dwarf star that can be located in the constellation of Cetus. HIP8998 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD11803. The Id of the star in the Gould Star Catalogue is 189. 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 189 G. Cet

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 189 G. Cet, the location is 01h 55m 53.74 and +01d50`58.3 .

Proper Motion of 189 G. Cet

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 186.27 ± 000.62 towards the north and 154.24 ± 001.06 east if we saw them in the horizon.

189 G. Cet Luminosity

Luminosity is the amount of energy that a star pumps out and its relative to the amount that our star, the Sun gives out. The figure of 2.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.

Physical Properties (Colour, Temperature, Radius) of 189 G. Cet

189 G. Cet has a spectral type of F7V+.... This means the star is a blue to white main sequence dwarf star. The star has a B-V Colour Index of 0.54 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,122 Kelvin.

189 G. Cet has been calculated as 2.03 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,411,143.36.km.

189 G. Cet Apparent and Absolute Magnitudes

189 G. Cet has an apparent magnitude of 6.01 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 3.06 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.01. 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 189 G. Cet

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 25.71 which gave the calculated distance to 189 G. Cet as 126.86 light years away from Earth or 38.90 parsecs. It would take a spaceship travelling at the speed of light, 126.86 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 25.07 which put 189 G. Cet at a distance of 130.10 light years or 39.89 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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

189 G. Cet Facts

Alternative Names

Traditional Name189 G. Cet
Hipparcos Library I.D.8998
Bonner DurchmusterungBD+01 347
Gould I.D.189
Henry Draper Designation11803

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude3.06 / 3.01
Apparent Magnitude6.01
Right Ascension (R.A.)01h 55m 53.74
Declination (Dec.)+01d50`58.3
1997 Distance from Earth25.71 Parallax (milliarcseconds)
 126.86 Light Years
 38.90 Parsecs
2007 Revised Distance from Earth25.07 Parallax (milliarcseconds)
 130.10 Light Years
 39.89 Parsecs
Proper Motion Dec.186.27 ± 0.62 milliarcseconds/year
Proper Motion RA.154.24 ± 1.06 milliarcseconds/year
B-V Index0.54
Spectral TypeF7V+...
Colour(F) blue to white

Estimated Facts

Radius (x the Sun)2.03
Luminosity (x the Sun)2.0000000
Calculated Effective Temperature6,122 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
11803+01 347.0A7.00000144.00000185.00000G0Yellow
B7.000001831

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