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WW Puppis

WW Puppis Facts

WW Puppis's Alternative Names

HIP37511 is the reference name for the star in the Hipparcos Star Catalogue.

WW Puppis has alternative name(s) :- WW Pup, WW Pup.

BD number is the number that the star was filed under in the Durchmusterung or Bonner Durchmusterung, a star catalogue that was put together by the Bonn Observatory between 1859 to 1903. The star's BD Number is BD-20 2125.

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

Location of WW Puppis

The location of the variable 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 WW Puppis, the location is 07h 41m 54.89 and -21° 07` 59.1 .

Radial Velocity and Proper Motion of WW Puppis

Proper Motion

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 1.78 ± 1.10 milliarcseconds/year towards the north and -2.11 ± 1.80 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is 87.00 km/s with an error of about 4.80 km/s . 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 (Colour, Temperature) of WW Puppis

WW Puppis Colour and Temperature

WW Puppis has a spectral type of F6.7. This means the star is a yellow to white variable star. The star has a B-V Colour Index of 0.74 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 5,558 Kelvin.

WW Puppis Radius

Radius has been calculated as being 3.66 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,544,070.53.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 4.08. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

WW Puppis Apparent and Absolute Magnitudes

WW Puppis has an apparent magnitude of 10.62 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 2.20 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.96. 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 WW Puppis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 2.07 which gave the calculated distance to WW Puppis as 1575.67 light years away from Earth or 483.09 parsecs. If you want that in miles, it is 10,364,310,464,191,345.98.

In 2007, Hipparcos data was revised with a new parallax of 1.85 which put WW Puppis at a distance of 1763.05 light years or 540.54 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 111,493,601.47 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.

Time to Travel to WW Puppis

A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

If you were to drive there at about 120 m.p.h. in a car with an infinity engine so you didn't have to pull over for petrol, it would take you 77,189,780,348,035.03 hours or 8,811,618,761.19 years.

At the time of writing, the fastest probe so far created is the New Horizon probe which is travelling at a speed of 33,000 m.p.h. If the probe was travelling to WW Puppis then it would take 280,690,110,356.49 hours / 32,042,250.04 years to get there. Speed Ref: N.A.S.A.

It would to take a spaceship journey travelling at the speed of light, 1575.67 years to get there. We don't have the technology or spaceship that can carry people over that distance yet.

Variable Type of WW Puppis

The star is a pulsating Delta Cepheid 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. WW Puppis brightness ranges from a magnitude of 11.188 to a magnitude of 10.220 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 5.5 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 WW Puppis Facts and Figures

Visual Facts


Primary / Proper / Traditional NameWW Puppis
Alternative NamesWW Pup, HIP 37511, BD-20 2125, WW Pup
Spectral TypeF6.7
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeVariable Star
ColourYellow - White
GalaxyMilky Way
ConstellationPuppis
Absolute Magnitude 2.20 / 1.96
Visual / Apparent Magnitude10.62
Naked Eye VisibleRequires a 4.5 - 6 Inch Telescope - Magnitudes
Right Ascension (R.A.)07h 41m 54.89
Declination (Dec.) -21° 07` 59.1
Galactic Latitude0.97 degrees
Galactic Longitude237.38 degrees
1997 Distance from Earth2.07 Parallax (milliarcseconds)
 1575.67 Light Years
 483.09 Parsecs
2007 Distance from Earth1.85 Parallax (milliarcseconds)
 1763.05 Light Years
 540.54 Parsecs
 111,493,601.47 Astronomical Units
Proper Motion Dec.1.78 ± 1.10 milliarcseconds/year
Proper Motion RA.-2.11 ± 1.80 milliarcseconds/year
B-V Index0.74
Radial Velocity87.00 ± 4.80 km/s

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassPulsating
Variable Star TypeDelta Cepheid
Mean Variability Period in Days5.517
Variable Magnitude Range (Brighter - Dimmer)10.220 - 11.188

Estimated Calculated Facts


Radius (x the Sun)4.08
Effective Temperature5,558 Kelvin

Sources and Links


SIMBAD SourceLink

Related Stars


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