Universe Guide


107 Aquarii - HD223024 - HIP117218

107 Aquarii is a blue to white main sequence dwarf star that can be located in the constellation of Aquarius. HIP117218 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD223024. The Id of the star in the Gould Star Catalogue is 262. 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. 107 Aquarii has alternative name(s), 107 Aquarii , 107 Aqr.

Location of 107 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 107 Aquarii, the location is 23h 46m 00.84 and -18d40`42.1 .

Proper Motion of 107 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 010.84 ± 001.14 towards the north and 130.33 ± 001.05 east if we saw them in the horizon.

107 Aquarii 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 4.0000000 that I have given is based on the Spectral Types page that I have found on the Internet. You might find a different figure, one that may have been calculated rather than generalised that I have done. The figure is always the amount times the luminosity of the Sun. It is an imprecise figure because of a number of factors including but not limited to whether the star is a variable star and distance.

Physical Properties (Colour, Temperature, Radius) of 107 Aquarii

107 Aquarii has a spectral type of F2:V+.... This means the star is a blue to white coloured main sequence dwarf star. The star has a B-V Colour Index of 0.29 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 7,270 Kelvin.

107 Aquarii has been calculated as 3.37 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,345,887.22.km.

107 Aquarii Apparent and Absolute Magnitudes

107 Aquarii has an apparent magnitude of 5.28 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 1.21 If you used the 2007 Parallax value, you would get an absolute magnitude of 0.96. 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 107 Aquarii

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 15.37 which gave the calculated distance to 107 Aquarii as 212.21 light years away from Earth or 65.06 parsecs. In 2007, Hipparcos data was revised with a new parallax of 13.66 which put 107 Aquarii at a distance of 238.77 light years or 73.21 parsecs.

It would take a spaceship travelling at the speed of light, 212.21 years using the 1997 distance to get there. We don't have the technology or spaceship that can carry people over that distance yet. 107 Aquarii brightness ranges from a magnitude of 5.000 to a magnitude of 5.000 over its variable period. The smaller the magnitude, the brighter the star.

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 Stellar Age, Metallicity or Mass is from the E.U. Exoplanets. The information was obtained as of 12th Feb 2017.

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107 Aquarii Facts

Alternative Names

Traditional Name107 Aquarii
Short Name107 Aqr
Alternative Name(s)107 Aquarii
Hipparcos Library I.D.117218
Bonner DurchmusterungBD-19 6506
Gould I.D.262
Henry Draper Designation223024

Visual Facts

Star Typemain sequence dwarf star
Absolute Magnitude1.21 / 0.96
Apparent Magnitude5.28
Right Ascension (R.A.)23h 46m 00.84
Declination (Dec.)-18d40`42.1
1997 Distance from Earth15.37 Parallax (milliarcseconds)
 212.21 Light Years
 65.06 Parsecs
2007 Distance from Earth13.66 Parallax (milliarcseconds)
 238.77 Light Years
 73.21 Parsecs
Proper Motion Dec.10.84 ± 1.14 milliarcseconds/year
Proper Motion RA.130.33 ± 1.05 milliarcseconds/year
B-V Index0.29
Spectral TypeF2:V+...
Colour(F) blue to white

Variable Star Details

Estimated Facts

Radius (x the Sun)3.37
Luminosity (x the Sun)4.0000000
Calculated Effective Temperature7,270 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
223024-19 6506.0A5.80000144.0000043.00000A5White

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