Universe Guide

13 Cassiopeiae - HD2729 - HIP2474

13 Cassiopeiae is a blue main sequence dwarf star that can be located in the constellation of Cassiopeia. HIP2474 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD2729. 13 Cassiopeiae has alternative name(s), 13 Cassiopeiae , 13 Cas.

Location of 13 Cassiopeiae

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 from celestial equator. The Declination is how up or down compared to the celestial equator and is expressed in degrees. For 13 Cassiopeiae, the location is 00h 31m 25.20 and +66 d 31 ` 10.7 .

Proper Motion of 13 Cassiopeiae

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 -004.00 ± 000.00 towards the north and 019.00 ± 000.00 east if we saw them in the horizon.

13 Cassiopeiae 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 240.0000000 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 13 Cassiopeiae

13 Cassiopeiae has a spectral type of B6V. This means the star is a blue coloured main sequence dwarf star. The star has a B-V Colour Index of -0.1 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 11,677 Kelvin.

13 Cassiopeiae has been calculated as 2.66 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,848,112.95.km.

13 Cassiopeiae Apparent and Absolute Magnitudes

13 Cassiopeiae 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 -0.33 If you used the 2007 Parallax value, you would get an absolute magnitude of -0.81. 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 13 Cassiopeiae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 5.00 which gave the calculated distance to 13 Cassiopeiae as 652.33 light years away from us or 200 parsecs. In 2007, Hipparcos data was revised with a new parallax of 4.00 which put 13 Cassiopeiae at a distance of 815.41 light years or 250 parsecs.

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.

13 Cassiopeiae Facts


Traditional Name13 Cassiopeiae
Short Name13 Cas
Alternative Name(s)13 Cassiopeiae
Hipparcos Library I.D.2474
Henry Draper Designation2729
Celestial TypeStar
Absolute Magnitude-0.33 / -0.81
Apparent Magnitude6.18
Right Ascension (R.A.)00h 31m 25.20
Declination (Dec.)+66 d 31 ` 10.7
1997 Distance5.00 Parallax (milliarcseconds)
 652.33 Light Years
 200 Parsecs
2007 Distance4.00 Parallax (milliarcseconds)
 815.41 Light Years
 250 Parsecs
Proper Motion Dec.-4.00 ± 0.00 milliarcseconds/year
Proper Motion RA.19.00 ± 0.00 milliarcseconds/year
B-V Index-0.10
Spectral TypeB6V
Colour(B) blue
Star Typemain sequence dwarf star
Radius (x the Sun)2.66
Luminosity (x the Sun)240.0000000
Calculated Effective Temperature11,677 Kelvin


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