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Muliphein (Gamma Canis Majoris, 23 Canis Majoris) Star Facts

Muliphein Facts

  • Muliphein is a luminous giant star that can be located in the constellation of Canis Major. The description is based on the spectral class.
  • Muliphein is a main star of the constellation outline.
  • Based on the spectral type (B8II) of the star, the star's colour is blue .
  • 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 441.96 light years away from us. Distance

Muliphein's Alternative Names

Gamma Canis Majoris (Gam Cma) 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 HR2657. HIP34045 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD53244.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John named the stars in the constellation with a number and its latin name, this star's Flamsteed designation is 23 Canis Majoris. The Flamsteed name can be shortened to 23 Cma.

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-15 1625.

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

Location of Muliphein

The location of the luminous 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 Muliphein, the location is 07h 03m 45.49 and -15° 37` 59.7 .

Radial Velocity and Proper Motion of Muliphein

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 -11.36 ± 0.16 milliarcseconds/year towards the north and -0.14 ± 0.21 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 32.00000 km/s with an error of about 7.40 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 Muliphein

Muliphein Colour and Temperature

Based on the star's spectral type of B8II , Muliphein's colour and type is blue luminous giant star. The star has a B-V Colour Index of -0.11 which means the star's temperature is about 14,384 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

Muliphein 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 715.56 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Muliphein Radius

Muliphein estimated radius has been calculated as being 2.79 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,939,284.99.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 3.0701477353318885949623650008. 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.

Muliphein Apparent and Absolute Magnitudes

Muliphein has an apparent magnitude of 4.11 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 -1.34 If you used the 2007 Parallax value, you would get an absolute magnitude of -1.55. 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 Muliphein

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 8.11000 which gave the calculated distance to Muliphein as 402.17 light years away from Earth or 123.30 parsecs. If you want that in miles, it is about 2,364,206,766,333,252.43, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 7.38000 which put Muliphein at a distance of 441.96 light years or 135.50 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 27,948,686.50 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 7,490.00 Parsecs or 24,429.63 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 Muliphein

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)
Walking474,096,431,338.21
Car1202,469,881,044.61
Airbus A380736402,697,996.40
Speed of Sound (Mach 1)767.269386,286,589.65
Concorde (Mach 2)1,534.54193,143,043.10
New Horizons Probe33,0008,981,385.62
Speed of Light670,616,629.00441.96

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 Muliphein Facts and Figures

Visual Facts


Primary / Proper / Traditional NameMuliphein
Alternative NamesGamma Canis Majoris, Gam Cma, HD 53244, HIP 34045, HR 2657, 23 Canis Majoris, 23 Cma, BD-15 1625
Spectral TypeB8II
Constellation's Main StarYes
Multiple Star SystemNo / Unknown
Star TypeLuminous Giant Star
ColourBlue
GalaxyMilky Way
ConstellationCanis Major
Absolute Magnitude -1.34 / -1.55
Visual / Apparent Magnitude4.11
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)07h 03m 45.49
Declination (Dec.)-15° 37` 59.7
Galactic Latitude-4.40618159 degrees
Galactic Longitude228.25182917 degrees
1997 Distance from Earth8.11000 Parallax (milliarcseconds)
 402.17 Light Years
 123.30 Parsecs
2007 Distance from Earth7.38000 Parallax (milliarcseconds)
 441.96 Light Years
 135.50 Parsecs
 27,948,686.50 Astronomical Units
Galacto-Centric Distance24,429.63 Light Years / 7,490.00 Parsecs
Proper Motion Dec.-11.36000 ± 0.16000 milliarcseconds/year
Proper Motion RA.-0.14000 ± 0.21000 milliarcseconds/year
B-V Index-0.11
Radial Velocity32.00000 ± 7.40 km/s
Eccentricity0.11100
Semi-Major Axis6700.0000000
Stellar Luminosity (Lsun)715.5600000

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Calculated Facts


Radius (x the Sun)3.07
Effective Temperature14,384 Kelvin

Sources and Links


SIMBAD SourceLink

Location of Muliphein in Canis Major


Muliphein Location in Canis Major

The map was generated using Night Vision, an awesome free application by Brian Simpson.

Canis Major Main Stars


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