W Volantis is a eclipsing/rotating star that can be located in the constellation of Volans. The description is based on the spectral class. The star can not be seen by the naked eye, you need a telescope to see it.
HIP37120 is the reference name for the star in the Hipparcos Star Catalogue.
W Volantis has alternative name(s) :- , W Vol.
More details on star alternative names can be found at Star Names .
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 W Volantis, the location is 07h 37m 40.07 and -69° 32` 32.5 .
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 11.24 ± 1.51 miliarcseconds/year towards the north and -11.44 ± 1.56 miliarcseconds/year east if we saw them in the horizon.
W Volantis has a spectral type of k-m. The star has a B-V Colour Index of 0.34 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,614 Kelvin.
W Volantis Radius has been calculated as being 2.41 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,676,626.70.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 2.24. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.
W Volantis has an apparent magnitude of 10.66 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 2.35 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.51. 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 2.18 which gave the calculated distance to W Volantis as 1496.16 light years away from Earth or 458.72 parsecs. It would take a spaceship travelling at the speed of light, 1496.16 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 2.34 which put W Volantis at a distance of 1393.86 light years or 427.35 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/rotating Beta Persei (Algol)/Detached Systems of the AR Lacertae (subtype) 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. This is a some uncertainty as to the type but the type mentioned is the current variable star classification for this star. W Volantis brightness ranges from a magnitude of 11.500 to a magnitude of 10.600 over its variable period. The smaller the magnitude, the brighter the star.
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.
|Primary / Proper / Traditional Name||W Volantis|
|Alternative Names||HIP 37120, W Vol|
|Multiple Star System||No / Unknown|
|Absolute Magnitude||2.35 / 2.51|
|Visual / Apparent Magnitude||10.66|
|Naked Eye Visible||Requires a 4.5 - 6 Inch Telescope - Magnitudes|
|Right Ascension (R.A.)||07h 37m 40.07|
|Declination (Dec.)||-69° 32` 32.5|
|Galactic Latitude||-21.40 degrees|
|Galactic Longitude||281.35 degrees|
|1997 Distance from Earth||2.18 Parallax (milliarcseconds)|
|1496.16 Light Years|
|2007 Distance from Earth||2.34 Parallax (milliarcseconds)|
|1393.86 Light Years|
|Proper Motion Dec.||11.24 ± 1.51 milliarcseconds/year|
|Proper Motion RA.||-11.44 ± 1.56 milliarcseconds/year|
|Variable Star Class||Eclipsing/Rotating|
|Variable Star Type||Beta Persei (Algol)/Detached Systems of the AR Lacertae (subtype) probably|
|Variable Magnitude Range (Brighter - Dimmer)||10.600 - 11.500|
|Calculated Effective Temperature||6,614 Kelvin|