Universe Guide

Beta Pavonis

Beta Pavonis Facts

  • Beta Pavonis is a subgiant star that can be located in the constellation of Pavo. The description is based on the spectral class.
  • Beta Pavonis is a main star of the constellation outline.
  • Based on the spectral type (A5IV) of the star, the star's colour is blue - white .
  • The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 135.11 light years away from us. Distance

Beta Pavonis's Alternative Names

Beta Pavonis (Bet Pav) is the Bayer Classification for the star. The Bayer Classification was created by Johann Bayer in 1603. The brightest star in the constellation is normally given the Alpha designation, there are exceptions such as Pollux which is Beta Geminorum.

The Id of the star in the Yale Bright Star Catalogue is HR7913. HIP102395 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD197051.

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

Location of Beta Pavonis

The location of the subgiant 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 Beta Pavonis, the location is 20h 44m 57.56 and -66° 12` 11.7 .

Radial Velocity and Proper Motion of Beta Pavonis

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 9.94 ± 0.09 milliarcseconds/year towards the north and -42.67 ± 0.16 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 3.70000 km/s with an error of about 0.50 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 of Beta Pavonis

Beta Pavonis Colour and Temperature

Based on the star's spectral type of A5IV , Beta Pavonis's colour and type is blue - white subgiant star. The star has a B-V Colour Index of 0.16 which means the star's temperature is about 8,017 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

Beta Pavonis 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 61.39 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Beta Pavonis Radius

Beta Pavonis estimated radius has been calculated as being 4.24 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,946,871.62.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 4.1579225825473746781841925530. 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.

Beta Pavonis Iron Abundance

Beta Pavonis Iron Abundance is -0.36 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.

Beta Pavonis Apparent and Absolute Magnitudes

Beta Pavonis has an apparent magnitude of 3.42 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 0.29 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.33. 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 Beta Pavonis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 23.71000 which gave the calculated distance to Beta Pavonis as 137.56 light years away from Earth or 42.18 parsecs. If you want that in miles, it is about 808,663,706,335,137.39, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 24.14000 which put Beta Pavonis at a distance of 135.11 light years or 41.43 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 8,545,491.38 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. The star's Galacto-Centric Distance is 7,371.00 Parsecs or 24,041.50 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Travel Time to Beta Pavonis

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 A380736123,107,354.27
Speed of Sound (Mach 1)767.269118,090,282.21
Concorde (Mach 2)1,534.5459,045,064.15
New Horizons Probe33,0002,745,667.05
Speed of Light670,616,629.00135.11

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 Beta Pavonis Facts and Figures

Visual Facts

Primary / Proper / Traditional NameBeta Pavonis
Alternative NamesBet Pav, HD 197051, HIP 102395, HR 7913
Spectral TypeA5IV
Constellation's Main StarYes
Multiple Star SystemNo / Unknown
Star TypeSubgiant Star
GalaxyMilky Way
Absolute Magnitude 0.29 / 0.33
Visual / Apparent Magnitude3.42
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)20h 44m 57.56
Declination (Dec.)-66° 12` 11.7
Galactic Latitude-36.00865987 degrees
Galactic Longitude328.96247201 degrees
1997 Distance from Earth23.71000 Parallax (milliarcseconds)
 137.56 Light Years
 42.18 Parsecs
2007 Distance from Earth24.14000 Parallax (milliarcseconds)
 135.11 Light Years
 41.43 Parsecs
 8,545,491.38 Astronomical Units
Galacto-Centric Distance24,041.50 Light Years / 7,371.00 Parsecs
Proper Motion Dec.9.94000 ± 0.09000 milliarcseconds/year
Proper Motion RA.-42.67000 ± 0.16000 milliarcseconds/year
B-V Index0.16
Radial Velocity3.70000 ± 0.50 km/s
Iron Abundance-0.3600 ± 9.99 Fe/H
Semi-Major Axis8521.0000000
Stellar Luminosity (Lsun)61.3900000

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Estimated Calculated Facts

Radius (x the Sun)4.16
Effective Temperature8,017 Kelvin

Sources and Links

SIMBAD SourceLink

Pavo Main Stars

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