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75 Pegasi, HD222133, HIP116611, HR8963

75 Pegasi is a blue eclipsing binary system main sequence dwarf star that can be located in the constellation of Pegasus. The description is based on the spectral class. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

75 Pegasi's Alternative Names

The Id of the star in the Yale Bright Star Catalogue is HR8963. HIP116611 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD222133.

75 Pegasi has alternative name(s) :- , KS Peg.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John numbered the stars in the constellation with a number and the latin name, this star's Flamsteed designation is 75 Pegasi with it shortened to 75 Peg.

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+17 4952.

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

Location of 75 Pegasi

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 75 Pegasi, the location is 23h 37m 56.77 and +18° 24` 02.2 .

Proper Motion of 75 Pegasi

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 17.37 ± 0.15 miliarcseconds/year towards the north and 48.85 ± 0.27 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 -3.27000 km/s with an error of about 0.62 km/s .

75 Pegasi 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 31.21 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Physical Properties (Colour, Temperature) of 75 Pegasi

75 Pegasi has a spectral type of A1Vn. This means the star is a blue main sequence dwarf star. The star is 7,409.00 Parsecs from the Galactic Centre or terms of Light Years is 24,165.44 s. The star has a B-V Colour Index of 0.01 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 9,392 Kelvin.

75 Pegasi Radius has been calculated as being 2.06 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,431,726.87.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 2.01. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

75 Pegasi Apparent and Absolute Magnitudes

75 Pegasi has an apparent magnitude of 5.49 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 1.17 If you used the 2007 Parallax value, you would get an absolute magnitude of 1.22. 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 75 Pegasi

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 13.65 which gave the calculated distance to 75 Pegasi as 238.95 light years away from Earth or 73.26 parsecs. It would take a spaceship travelling at the speed of light, 238.95 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 14.01 which put 75 Pegasi at a distance of 232.81 light years or 71.38 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's Galacto-Centric Distance is 7,409.00 Parsecs or 24,165.44 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Variable Type of 75 Pegasi

The star is a eclipsing binary system Beta Lyrae (Sheliak) 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. 75 Pegasi brightness ranges from a magnitude of 5.567 to a magnitude of 5.469 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.5 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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75 Pegasi Facts

Visual Facts


Primary / Proper / Traditional Name75 Pegasi
Alternative NamesHD 222133, HIP 116611, HR 8963, 75 Peg, BD+17 4952, KS Peg
Spectral TypeA1Vn
Multiple Star SystemYes
Star Type main sequence Dwarf Star
Colour blue
GalaxyMilky Way
ConstellationPegasus
Absolute Magnitude1.17 / 1.22
Visual / Apparent Magnitude5.49
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)23h 37m 56.77
Declination (Dec.)+18° 24` 02.2
Galactic Latitude-41.11 degrees
Galactic Longitude99.54 degrees
1997 Distance from Earth13.65 Parallax (milliarcseconds)
 238.95 Light Years
 73.26 Parsecs
2007 Distance from Earth14.01 Parallax (milliarcseconds)
 232.81 Light Years
 71.38 Parsecs
Galacto-Centric Distance24,165.44 Light Years / 7,409.00 Parsecs
Proper Motion Dec.17.37 ± 0.15 milliarcseconds/year
Proper Motion RA.48.85 ± 0.27 milliarcseconds/year
B-V Index0.01
Radial Velocity-3.27 ± 0.62 km/s
Eccentricity0.10
Semi-Major Axis8133.00
Stellar Luminosity (Lsun)31.21

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassEclipsing binary system
Variable Star TypeBeta Lyrae (Sheliak)
Mean Variability Period in Days0.502
Variable Magnitude Range (Brighter - Dimmer)5.469 - 5.567

Estimated Facts


Calculated Effective Temperature9,392 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
222133+17 4952.0A5.4000052.0000017.00000A0White
B11.600001958

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