Universe Guide

UZ Volantis

UZ Volantis Facts

  • UZ Volantis is a eclipsing giant star that can be located in the constellation of Volans. The description is based on the spectral class.
  • UZ Volantis is not part of the constellation outline but is within the borders of the constellation.
  • Based on the spectral type (G8III) of the star, the star's colour is yellow .
  • The star can not be seen by the naked eye, you need a telescope to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 867.46 light years away from us. Distance

UZ Volantis's Alternative Names

HIP31539 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD48406.

UZ Volantis has alternative name(s) :- , UZ Vol.

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

Location of UZ Volantis

The location of the giant 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 object is compared to the celestial equator and is expressed in degrees. For UZ Volantis, the location is 06h 36m 08.04 and -72° 47` 06.9 .

Proper Motion of UZ Volantis

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 18.01 ± 1.13 milliarcseconds/year towards the north and -8.88 ± 1.23 milliarcseconds/year east if we saw them in the horizon. . When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Its nothing to fear as the stars are so far apart, they won't collide in our life-time, if ever.

Physical Properties of UZ Volantis

UZ Volantis Colour and Temperature

Based on the star's spectral type of G8III , UZ Volantis's colour and type is yellow giant star. The star has a B-V Colour Index of 0.97 which means the star's temperature is about 4,907 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

UZ Volantis Radius

UZ Volantis estimated radius has been calculated as being 5.59 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 3,888,103.76.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 4.6908299705610769066048414059. The figure is derived at by using the formula from SDSS rather than peer reviewed papers. It has been known to produce widely incorrect figures.

UZ Volantis Apparent and Absolute Magnitudes

UZ Volantis has an apparent magnitude of 9.32 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 1.82 If you used the 2007 Parallax value, you would get an absolute magnitude of 2.20. 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 UZ Volantis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 3.16000 which gave the calculated distance to UZ Volantis as 1032.16 light years away from Earth or 316.46 parsecs. If you want that in miles, it is about 6,067,681,965,185,194.90, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 3.76000 which put UZ Volantis at a distance of 867.46 light years or 265.96 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.

Using the 2007 distance, the star is roughly 54,857,805.61 Astronomical Units from the Earth/Sun give or take a few. An Astronomical Unit is the distance between Earth and the Sun. The number of A.U. is the number of times that the star is from the Earth compared to the Sun.

Travel Time to UZ Volantis

The time it will take to travel to this star is dependent on how fast you are going. U.G. has done some calculations as to how long it will take going at differing speeds. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. Its primary mission was to visit Pluto which at the time of launch (2006), Pluto was still a planet.

DescriptionSpeed (m.p.h.)Time (years)
Airbus A380736790,398,235.04
Speed of Sound (Mach 1)767.269758,186,634.66
Concorde (Mach 2)1,534.54379,092,823.25
New Horizons Probe33,00017,628,275.79
Speed of Light670,616,629.00867.46

Variable Type of UZ Volantis

The star is a eclipsing Beta Persei (Algol) 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. UZ Volantis brightness ranges from a magnitude of 9.902 to a magnitude of 9.410 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.8 days (variability).

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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Additional UZ Volantis Facts and Figures

Visual Facts

Primary / Proper / Traditional NameUZ Volantis
Alternative NamesHD 48406, HIP 31539, UZ Vol
Spectral TypeG8III
Constellation's Main StarNo
Multiple Star SystemYes
Star TypeGiant Star
GalaxyMilky Way
Absolute Magnitude 1.82 / 2.20
Visual / Apparent Magnitude9.32
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)06h 36m 08.04
Declination (Dec.)-72° 47` 06.9
Galactic Latitude-26.94481178 degrees
Galactic Longitude283.58700719 degrees
1997 Distance from Earth3.16000 Parallax (milliarcseconds)
 1032.16 Light Years
 316.46 Parsecs
2007 Distance from Earth3.76000 Parallax (milliarcseconds)
 867.46 Light Years
 265.96 Parsecs
 54,857,805.61 Astronomical Units
Proper Motion Dec.18.01000 ± 1.13000 milliarcseconds/year
Proper Motion RA.-8.88000 ± 1.23000 milliarcseconds/year
B-V Index0.97

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassEclipsing
Variable Star TypeBeta Persei (Algol)
Mean Variability Period in Days0.793
Variable Magnitude Range (Brighter - Dimmer)9.410 - 9.902

Estimated Calculated Facts

Radius (x the Sun)4.69
Effective Temperature4,907 Kelvin

Sources and Links

SIMBAD SourceLink

Multi-Star System

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. IdB.D. IdStar CodeMagnitudeR.A.Dec.SpectrumColourYear
48406-72 513.4A9.2000021.00000-61.00000G5Yellow

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