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Ainalrami, Nu1 Sagittarii, 32 Sagittarii, HD174974, HIP92761, HR7116

Ainalrami (Nu1 Sagittarii) is a orange to red star that can be located in the constellation of Sagittarius. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.

Nu1 Sagittarii is the Bayer Classification for the star. The Id of the star in the Yale Bright Star Catalogue is HR7116. HIP92761 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD174974. The Id of the star in the Gould Star Catalogue is 111. 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.

Location of Ainalrami

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 Ainalrami, the location is 18h 54m 10.18 and -22d 44` 41.4 .

Proper Motion of Ainalrami

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 -8.41 ± 0.18 miliarcseconds/year towards the north and 2.59 ± 0.30 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 -11.60000 km/s with an error of about 0.80 km/s .

Physical Properties (Colour, Temperature, Radius) of Ainalrami

Ainalrami has a spectral type of K1II. This means the star is a orange to red star. The star is 7074.00000000 Parsecs from the Galactic Centre or terms of Light Years is 23072.7949545600000000s. The star has a B-V Colour Index of 1.41 which means the star's temperature has been calculated using information from Morgans @ Uni.edu at being 4,190 Kelvin.

Ainalrami Radius has been calculated as being 107.28 times bigger than the Sun.The Sun's radius is 695,800km, therefore the star's radius is an estimated 74,644,561.45.km. However with the 2007 release of updated Hipparcos files, the radius is now calculated at being round 65.24. The figure is derived at by using the formula from SDSS and has been known to produce widely incorrect figures.

Ainalrami Apparent and Absolute Magnitudes

Ainalrami has an apparent magnitude of 4.86 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 -3.91 If you used the 2007 Parallax value, you would get an absolute magnitude of -2.83. 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 Ainalrami

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 1.76 which gave the calculated distance to Ainalrami as 1853.20 light years away from Earth or 568.18 parsecs. It would take a spaceship travelling at the speed of light, 1853.20 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 2.90 which put Ainalrami at a distance of 1124.70 light years or 344.83 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 7,074.00 Parsecs or 23,072.79 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.

Ainalrami Facts

Alternative Names

Traditional/Proper NameAinalrami
Flamsteed Name32 Sagittarii
Flamsteed Short Name32 Sgr
Bayer DesignationNu1 Sagittarii
Hipparcos Library I.D.92761
Yale Bright Star Catalogue (HR) Id7116
Bonner DurchmusterungBD-22 4907
Gould I.D.111
Henry Draper Designation174974

Visual Facts

Star Type star
ConstellationSagittarius
Absolute Magnitude-3.91 / -2.83
Visual / Apparent Magnitude4.86
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)18h 54m 10.18
Declination (Dec.)-22d 44` 41.4
Galactic Latitude-10.72 degrees
Galactic Longitude12.74 degrees
1997 Distance from Earth1.76 Parallax (milliarcseconds)
 1853.20 Light Years
 568.18 Parsecs
2007 Revised Distance from Earth2.90 Parallax (milliarcseconds)
 1124.70 Light Years
 344.83 Parsecs
Galacto-Centric Distance23,072.79 Light Years / 7,074.00 Parsecs
Proper Motion Dec.-8.41 ± 0.18 milliarcseconds/year
Proper Motion RA.2.59 ± 0.30 milliarcseconds/year
B-V Index1.41
Radial Velocity-11.60 ± 0.80 km/s
Spectral TypeK1II
Colour(K) Orange to Red

Estimated Facts

Calculated Effective Temperature4,190 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
174974-22 4907.0A5.0000010.00000-9.00000K2Orange
B10.800001888
C10.800001878

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