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24 Aquarii - HD206058 - HIP106942

24 Aquarii is a blue to white giant star that can be located in the constellation of Aquarius. The star can not be seen by the naked eye, you need a telescope to see it. The star has an estimated age of 3.10 Billion of Years but could be as young as 2.80 to 3.40 according to Hipparcos.

HIP106942 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD206058. The Id of the star in the Gould Star Catalogue is 83. Stars in the southern hemisphere are more likely to have a Gould Id than the northern hemisphere. For example, there are no Gould classified stars in Ursa Major.

24 Aquarii has alternative name(s), 24 Aquarii , 24 Aqr. 24 Aquarii is a multiple star system with 2 stars orbiting in its solar system.

Location of 24 Aquarii

The location of the star in the galaxy 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 24 Aquarii, the location is 21h 39m 31.39 and -00d03`04.1 .

Proper Motion of 24 Aquarii

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 8.81 ± 0.48 miliarcseconds/year towards the north and 232.76 ± 0.81 miliarcseconds/year east if we saw them in the horizon.

Physical Properties (Colour, Temperature, Age, Radius) of 24 Aquarii

24 Aquarii has a spectral type of F7III. This means the star is a blue to white giant star. The star is 7380.00000000 Parsecs from the Galactic Centre or terms of Light Years is 24070.8547872000000000s. The star has a B-V Colour Index of 0.51 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 6,243 Kelvin.

24 Aquarii Radius has been calculated as being 1.61 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 1,118,322.33.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 1.64. 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 -0.11 with an error value of 0.08 Fe/H with the Sun has a value of 1 to put it into context.

The stars age according to Hipparcos data files put the star at an age of about 3.10 Billion years old but could be between 2.80 and 3.40 Billion years old. In comparison, the Sun's age is about 4.6 Billion Years Old.

24 Aquarii Apparent and Absolute Magnitudes

24 Aquarii has an apparent magnitude of 6.66 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 3.48 If you used the 2007 Parallax value, you would get an absolute magnitude of 3.44. 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 24 Aquarii

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 23.13 which gave the calculated distance to 24 Aquarii as 141.01 light years away from Earth or 43.23 parsecs. It would take a spaceship travelling at the speed of light, 141.01 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 22.74 which put 24 Aquarii at a distance of 143.43 light years or 43.98 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 7,380.00 Parsecs or 24,070.85 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

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.

24 Aquarii Facts

Alternative Names

Traditional/Proper Name24 Aquarii
Short Name24 Aqr
Alternative Name(s)24 Aquarii
Hipparcos Library I.D.106942
Bonner DurchmusterungBDD-00 4245
Gould I.D.83
Henry Draper Designation206058

Visual Facts

Star Typegiant star
Age3.10 Billion Years Old
Age Range2.80 - 3.40 Billion Years Old
Absolute Magnitude3.48 / 3.44
Visual / Apparent Magnitude6.66
Naked Eye VisibleRequires a 7x50 Binoculars - Ref: Wiki
Right Ascension (R.A.)21h 39m 31.39
Declination (Dec.)-00d03`04.1
Galactic Latitude-36.60 degrees
Galactic Longitude55.22 degrees
1997 Distance from Earth23.13 Parallax (milliarcseconds)
 141.01 Light Years
 43.23 Parsecs
2007 Revised Distance from Earth22.74 Parallax (milliarcseconds)
 143.43 Light Years
 43.98 Parsecs
Galacto-Centric Distance24,070.85 Light Years / 7,380.00 Parsecs
Proper Motion Dec.8.81 ± 0.48 milliarcseconds/year
Proper Motion RA.232.76 ± 0.81 milliarcseconds/year
B-V Index0.51
Radial Velocity-15.86 ± 0.06 km/s
Iron Abundance-0.11 ± 0.08 Fe/H
Spectral TypeF7III
Colour(F) blue to white
Stars in Solar System2

Estimated Facts

Calculated Effective Temperature6,243 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

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
206058-00 4245.0A7.30000218.0000027.00000F8Yellow/White
B7.800001890
C10.900001959

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