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Propus, Eta Geminorum, 7 Geminorum, HD42995, HIP29655, HR2216

Propus (Eta Geminorum) Location in Gemini

Propus (Eta Geminorum) is a red pulsating giant star that can be located in the constellation of Gemini. 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.

Propus's Alternative Names

Eta Geminorum (Eta Gem) is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR2216. HIP29655 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD42995.

Propus has alternative name(s) :- Tejat Prior, eta Gem.

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 7 Geminorum with it shortened to 7 Gem.

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+22 1241.

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

Location of Propus

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 Propus, the location is 06h 14m 52.70 and +22° 30` 24.6 .

Proper Motion of Propus

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 -12.12 ± 0.61 miliarcseconds/year towards the north and -62.46 ± 1.23 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 22.39000 km/s with an error of about 0.36 km/s .

Physical Properties (Colour, Temperature) of Propus

Propus has a spectral type of M3III. This means the star is a red giant star. The star is 7,514.00 Parsecs from the Galactic Centre or terms of Light Years is 24,507.91 s. The star has a B-V Colour Index of 1.6 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 3,779 Kelvin.

Propus Radius has been calculated as being 50.84 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 35,371,388.69.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 56.00. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures. The star's Iron Abundance is 0.00 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context.

Propus Apparent and Absolute Magnitudes

Propus has an apparent magnitude of 3.31 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 -1.84 If you used the 2007 Parallax value, you would get an absolute magnitude of -2.05. 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 Propus

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 9.34 which gave the calculated distance to Propus as 349.21 light years away from Earth or 107.07 parsecs. It would take a spaceship travelling at the speed of light, 349.21 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 8.48 which put Propus at a distance of 384.63 light years or 117.92 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 7,514.00 Parsecs or 24,507.91 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 Propus

The star is a pulsating Semi-Regular Star which are giants or supergiants of intermediate and late spectral and Eclipsing 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. Propus brightness ranges from a magnitude of 3.392 to a magnitude of 3.183 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 233.0 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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Propus Facts

Visual Facts


 Propus
Alternative NamesEta Geminorum, Eta Gem, Tejat Prior, HD 42995, HIP 29655, HR 2216, 7 Geminorum, 7 Gem, BD+22 1241, eta Gem
Spectral TypeM3III
Multiple Star SystemYes
Star TypeGiant Star
Colour red
GalaxyMilky Way
ConstellationGemini
Absolute Magnitude-1.84 / -2.05
Visual / Apparent Magnitude3.31
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)06h 14m 52.70
Declination (Dec.)+22° 30` 24.6
Galactic Latitude2.52 degrees
Galactic Longitude188.85 degrees
1997 Distance from Earth9.34 Parallax (milliarcseconds)
 349.21 Light Years
 107.07 Parsecs
2007 Distance from Earth8.48 Parallax (milliarcseconds)
 384.63 Light Years
 117.92 Parsecs
Galacto-Centric Distance24,507.91 Light Years / 7,514.00 Parsecs
Proper Motion Dec.-12.12 ± 0.61 milliarcseconds/year
Proper Motion RA.-62.46 ± 1.23 milliarcseconds/year
B-V Index1.60
Radial Velocity22.39 ± 0.36 km/s
Iron Abundance0.00 ± 9.99 Fe/H
Eccentricity0.25
Semi-Major Axis9665.00

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassPulsating
Variable Star TypeSemi-Regular Star which are giants or supergiants of intermediate and late spectral and Eclipsing
Mean Variability Period in Days233.000
Variable Magnitude Range (Brighter - Dimmer)3.183 - 3.392

Estimated Facts


Calculated Effective Temperature3,779 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
42995+22 1241.0A-66.00000-12.00000M1Red
B8.800001958

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