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Beta Reticuli - HD23817 - HIP17440

Beta Reticuli is a orange to red subgiant star that can be located in the constellation of Reticulum. Beta Reticuli is the Bayer Classification for the star. HIP17440 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD23817.

Location of Beta Reticuli

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 Beta Reticuli, the location is 03h 44m 11.55 and -64d48`25.5 .

Proper Motion of Beta Reticuli

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 077.50 ± 000.50 towards the north and 307.13 ± 000.53 east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Radius) of Beta Reticuli

Beta Reticuli has a spectral type of K0IV SB. This means the star is a orange to red subgiant star. The star has a B-V Colour Index of 1.13 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,611 Kelvin.

Beta Reticuli has been calculated as 7.64 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 5,318,433.62.km.

Beta Reticuli Apparent and Absolute Magnitudes

Beta Reticuli has an apparent magnitude of 3.84 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 1.41 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.46. 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 Beta Reticuli

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 32.71 which gave the calculated distance to Beta Reticuli as 99.71 light years away from Earth or 30.57 parsecs. It would take a spaceship travelling at the speed of light, 99.71 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 33.49 which put Beta Reticuli at a distance of 97.39 light years or 29.86 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.

Beta Reticuli Facts

Alternative Names

Bayer DesignationBeta Reticuli
Hipparcos Library I.D.17440
Henry Draper Designation23817

Visual Facts

Star Typesubgiant star
Absolute Magnitude1.41 / 1.46
Apparent Magnitude3.84
Right Ascension (R.A.)03h 44m 11.55
Declination (Dec.)-64d48`25.5
1997 Distance from Earth32.71 Parallax (milliarcseconds)
 99.71 Light Years
 30.57 Parsecs
2007 Revised Distance from Earth33.49 Parallax (milliarcseconds)
 97.39 Light Years
 29.86 Parsecs
Proper Motion Dec.77.50 ± 0.50 milliarcseconds/year
Proper Motion RA.307.13 ± 0.53 milliarcseconds/year
B-V Index1.13
Eccentricity0.21
Inclination82.85
Semi-Major Axis27.10
Orbital Period (Days)1911.50
Argument Of Periastron13.80
Spectral TypeK0IV SB
Colour(K) Orange to Red

Estimated Facts

Radius (x the Sun)7.64
Calculated Effective Temperature4,611 Kelvin

Sources and Links

SIMBAD SourceLink

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