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8 G. Hya - HD70110 - HIP40858

8 G. Hya is a blue to white main sequence dwarf star that can be located in the constellation of Hydra. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. The star has an estimated age of 3.00 Billion of Years but could be as young as 2.90 to 4.20 according to Hipparcos.

HIP40858 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD70110. The Id of the star in the Gould Star Catalogue is 8. 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. The Gliese ID of the star is Gliese GJ2067. The star was added to the Gliese catalogue in 1970 by Richard van der Riet Woolley hence the GJ rather than GL prefix. Ref : Star Names.

Location of 8 G. Hya

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 8 G. Hya, the location is 08h 20m 12.98 and -00d54`32.8 .

Proper Motion of 8 G. Hya

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 -86.94 ± 0.25 miliarcseconds/year towards the north and 40.95 ± 0.41 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Age, Radius) of 8 G. Hya

8 G. Hya has a spectral type of F9V. This means the star is a blue to white main sequence dwarf star. The star is 7427.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24224.1515588800000000s. The star has a B-V Colour Index of 0.6 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,895 Kelvin.

8 G. Hya Radius has been calculated as being 2.12 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,473,633.49.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 2.05. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is 0.11 with an error value of 0.02 Fe/H with the Sun has a value of 1 to put it into context.

The stars age according to Hipparcos data files put the star at an age of about 3.00 Billion years old but could be between 2.90 and 4.20 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

8 G. Hya Apparent and Absolute Magnitudes

8 G. Hya has an apparent magnitude of 6.18 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 3.13 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.20. 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 8 G. Hya

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 24.50 which gave the calculated distance to 8 G. Hya as 133.13 light years away from Earth or 40.82 parsecs. It would take a spaceship travelling at the speed of light, 133.13 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 25.32 which put 8 G. Hya at a distance of 128.82 light years or 39.49 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 7,427.00 Parsecs or 24,224.15 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.

8 G. Hya Facts

Alternative Names

Traditional/Proper Name8 G. Hya
Hipparcos Library I.D.40858
Bonner DurchmusterungBDD-00 1966
Gould I.D.8
Gliese ID2067
Henry Draper Designation70110

Visual Facts

Star Typemain sequence dwarf star
Age3.00 Billion Years Old
Age Range2.90 - 4.20 Billion Years Old
Absolute Magnitude3.13 / 3.20
Visual / Apparent Magnitude6.18
Naked Eye VisibleYes - Ref: Wiki
Right Ascension (R.A.)08h 20m 12.98
Declination (Dec.)-00d54`32.8
Galactic Latitude19.20 degrees
Galactic Longitude224.31 degrees
1997 Distance from Earth24.50 Parallax (milliarcseconds)
 133.13 Light Years
 40.82 Parsecs
2007 Revised Distance from Earth25.32 Parallax (milliarcseconds)
 128.82 Light Years
 39.49 Parsecs
Galacto-Centric Distance24,224.15 Light Years / 7,427.00 Parsecs
Proper Motion Dec.-86.94 ± 0.25 milliarcseconds/year
Proper Motion RA.40.95 ± 0.41 milliarcseconds/year
B-V Index0.60
Radial Velocity9.30 ± 1.89 km/s
Iron Abundance0.11 ± 0.02 Fe/H
Spectral TypeF9V
Colour(F) blue to white

Estimated Facts

Calculated Effective Temperature5,895 Kelvin

Sources and Links

SIMBAD SourceLink

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