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Eta3 Fornacis, HD17829, HIP13265, HR851

Eta3 Fornacis is a orange to red giant star that can be located in the constellation of Fornax. 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.

Eta3 Fornacis's Alternative Names

Eta3 Fornacis (Eta03 For) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR851. HIP13265 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD17829.

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

Location of Eta3 Fornacis

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 Eta3 Fornacis, the location is 02h 50m 40.40 and -35° 40` 32.6 .

Proper Motion of Eta3 Fornacis

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 -54.79 ± 0.20 miliarcseconds/year towards the north and 4.52 ± 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 11.70000 km/s with an error of about 0.80 km/s .

Eta3 Fornacis 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 202.98 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Physical Properties (Colour, Temperature) of Eta3 Fornacis

Eta3 Fornacis has a spectral type of K2III. This means the star is a orange to red giant star. The star is 7,434.00 Parsecs from the Galactic Centre or terms of Light Years is 24,246.98 s. The star has a B-V Colour Index of 1.25 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,405 Kelvin.

Eta3 Fornacis Radius has been calculated as being 20.94 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 14,571,414.05.km. If you need the diameter of the star, you just need to multiple the radius by 2. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 18.07. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Eta3 Fornacis Apparent and Absolute Magnitudes

Eta3 Fornacis has an apparent magnitude of 5.48 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 -0.58 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.26. 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 Eta3 Fornacis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 6.14 which gave the calculated distance to Eta3 Fornacis as 531.21 light years away from Earth or 162.87 parsecs. It would take a spaceship travelling at the speed of light, 531.21 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 7.10 which put Eta3 Fornacis at a distance of 459.38 light years or 140.85 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.

The star's Galacto-Centric Distance is 7,434.00 Parsecs or 24,246.98 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.

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Eta3 Fornacis Facts

Visual Facts


Primary / Proper / Traditional NameEta3 Fornacis
Alternative NamesEta03 For, HD 17829, HIP 13265, HR 851
Spectral TypeK2III
Multiple Star SystemYes
Star TypeGiant Star
Colour orange to red
GalaxyMilky Way
ConstellationFornax
Absolute Magnitude-0.58 / -0.26
Visual / Apparent Magnitude5.48
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)02h 50m 40.40
Declination (Dec.)-35° 40` 32.6
Galactic Latitude-63.28 degrees
Galactic Longitude239.01 degrees
1997 Distance from Earth6.14 Parallax (milliarcseconds)
 531.21 Light Years
 162.87 Parsecs
2007 Distance from Earth7.10 Parallax (milliarcseconds)
 459.38 Light Years
 140.85 Parsecs
Galacto-Centric Distance24,246.98 Light Years / 7,434.00 Parsecs
Proper Motion Dec.-54.79 ± 0.20 milliarcseconds/year
Proper Motion RA.4.52 ± 0.28 milliarcseconds/year
B-V Index1.25
Radial Velocity11.70 ± 0.80 km/s
Eccentricity0.22
Semi-Major Axis6561.00
Stellar Luminosity (Lsun)202.98

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Facts


Calculated Effective Temperature4,405 Kelvin

Sources and Links


SIMBAD SourceLink

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