Theta Muscae is a eclipsing binary system Wolf-Rayet star that can be located in the constellation of Musca. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
Theta Muscae is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR4952. HIP64094 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD113904.
Theta Muscae has alternative name(s) :- , the Mus.
More details on star alternative names can be found at Star Names .
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 Theta Muscae, the location is 13h 08m 07.16 and -65° 18` 21.7 .
The star is a Wolf-Rayet, a rare type of star of which not many are known. These stars are extremely luminous and large compared to our Sun. They live fast and die hard in a matter of millions not billions of years like our Sun. They exhaust their hydrogen supplies, turning to other gasses and expand outwards with massive solar winds, moving a step closer in the stellar evolution towards their death in a super or hypernova explosion.
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 -2.18 ± 0.34 miliarcseconds/year towards the north and -4.26 ± 0.48 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 -28.40000 km/s with an error of about 2.80 km/s .
Theta Muscae has a spectral type of WC6 + O9.5I. The star has a B-V Colour Index of -0.03 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 11,122 Kelvin.
Theta Muscae Radius has been calculated as being 683.37 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 475,490,153.67.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 79.18. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.
Theta Muscae has an apparent magnitude of 5.44 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 -12.17 If you used the 2007 Parallax value, you would get an absolute magnitude of -7.49. 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.
Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 0.03 which gave the calculated distance to Theta Muscae as 108721.11 light years away from Earth or 33333.33 parsecs. It would take a spaceship travelling at the speed of light, 108721.11 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 0.26 which put Theta Muscae at a distance of 12544.74 light years or 3846.15 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 is a eclipsing binary system Eclipsing variable type which means that its size changes over time. The Variable Type is usually named after the first star of that type to be spotted. Theta Muscae brightness ranges from a magnitude of 5.500 to a magnitude of 5.460 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.0 days (variability).
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.
|Alternative Names||HD 113904, HIP 64094, HR 4952, the Mus, WR 48|
|Spectral Type||WC6 + O9.5I|
|Multiple Star System||Yes|
|Star Type||very luminous Supergiant StarWolf-Rayet star|
|Absolute Magnitude||-12.17 / -7.49|
|Visual / Apparent Magnitude||5.44|
|Naked Eye Visible||Yes - Magnitudes|
|Right Ascension (R.A.)||13h 08m 07.16|
|Declination (Dec.)||-65° 18` 21.7|
|Galactic Latitude||-2.49 degrees|
|Galactic Longitude||304.67 degrees|
|1997 Distance from Earth||0.03 Parallax (milliarcseconds)|
|108721.11 Light Years|
|2007 Distance from Earth||0.26 Parallax (milliarcseconds)|
|12544.74 Light Years|
|Proper Motion Dec.||-2.18 ± 0.34 milliarcseconds/year|
|Proper Motion RA.||-4.26 ± 0.48 milliarcseconds/year|
|Radial Velocity||-28.40 ± 2.80 km/s|
|Variable Star Class||Eclipsing binary system|
|Variable Star Type||Eclipsing|
|Mean Variability Period in Days||0.028|
|Variable Magnitude Range (Brighter - Dimmer)||5.460 - 5.500|
|Calculated Effective Temperature||11,122 Kelvin|
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. Id||B.D. Id||Star Code||Magnitude||R.A.||Dec.||Spectrum||Colour||Year|