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CN Gruis

CN Gruis Facts

CN Gruis's Alternative Names

HIP107745 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD207399.

CN Gruis has alternative name(s) :- , CN Gru.

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

Location of CN Gruis

The location of the 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 CN Gruis, the location is 21h 49m 35.70 and -36° 41` 48.6 .

Proper Motion of CN Gruis

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 -16.00 ± 0.44 miliarcseconds/year towards the north and 8.53 ± 0.64 miliarcseconds/year east if we saw them in the horizon. . 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 CN Gruis

CN Gruis has a spectral type of M5III. This means the star is a red giant star. The star has a B-V Colour Index of 1.43 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,110 Kelvin.

CN Gruis Radius has been calculated as being 40.67 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 28,295,741.07.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 16.72. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

CN Gruis Apparent and Absolute Magnitudes

CN Gruis has an apparent magnitude of 8.15 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 -1.72 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.21. 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 CN Gruis

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 1.06 which gave the calculated distance to CN Gruis as 3077.01 light years away from Earth or 943.40 parsecs. It would take a spaceship travelling at the speed of light, 3077.01 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 2.58 which put CN Gruis at a distance of 1264.20 light years or 387.60 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 79,947,681.82 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.

Variable Type of CN Gruis

The star is a eruptive Irregular 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. CN Gruis brightness ranges from a magnitude of 8.164 to a magnitude of 8.003 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.2 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 CN Gruis Facts and Figures

Visual Facts


Primary / Proper / Traditional NameCN Gruis
Alternative NamesHD 207399, HIP 107745, CN Gru
Spectral TypeM5III
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeGiant Star
ColourRed
GalaxyMilky Way
ConstellationGrus
Absolute Magnitude -1.72 / 0.21
Visual / Apparent Magnitude8.15
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)21h 49m 35.70
Declination (Dec.)-36° 41` 48.6
Galactic Latitude-50.62 degrees
Galactic Longitude7.20 degrees
1997 Distance from Earth1.06 Parallax (milliarcseconds)
 3077.01 Light Years
 943.40 Parsecs
2007 Distance from Earth2.58 Parallax (milliarcseconds)
 1264.20 Light Years
 387.60 Parsecs
 79,947,681.82 Astronomical Units
Proper Motion Dec.-16.00 ± 0.44 milliarcseconds/year
Proper Motion RA.8.53 ± 0.64 milliarcseconds/year
B-V Index1.43

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassEruptive
Variable Star TypeIrregular
Mean Variability Period in Days0.158
Variable Magnitude Range (Brighter - Dimmer)8.003 - 8.164

Estimated Calculated Facts


Radius (x the Sun)16.72
Effective Temperature4,110 Kelvin

Sources and Links


SIMBAD SourceLink

Related Stars


Comments and Questions

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