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132 G. Aquilae

132 G. Aquilae Facts

  • 132 G. Aquilae is a subgiant star that can be located in the constellation of Aquila. The description is based on the spectral class.
  • 132 G. Aquilae is not part of the constellation outline but is within the borders of the constellation.
  • Based on the spectral type (G8III-IV) of the star, the star's colour is yellow .
  • The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • The star is calculated at being about 246.53 light years away from us. Distance

132 G. Aquilae's Alternative Names

HIP100541 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD194013.

The Gould star designation is one that was designed by American astronomer, Benjamin Apthorp Gould. Gould stars are predominantly in the Southern and Equatorial constellations but do appear in northern constellations such as Bootes and Orion. The star has the designation 132 G. Aquilae. There are no stars with a Gould designation in Ursa Major for example.

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+04 4434.

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

Location of 132 G. Aquilae

The location of the subgiant 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 132 G. Aquilae, the location is 20h 23m 10.71 and +05° 20` 35.1 .

Radial Velocity and Proper Motion of 132 G. Aquilae

Proper Motion

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 -38.91 ± 0.28 milliarcseconds/year towards the north and -27.55 ± 0.36 milliarcseconds/year east if we saw them in the horizon.

Radial Velocity

The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -11.40000 km/s with an error of about 0.30 km/s . 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 of 132 G. Aquilae

132 G. Aquilae Temperature and Colour

Based on the star's spectral type of G8III-IV , 132 G. Aquilae's colour and type is yellow subgiant star. The star has a B-V Colour Index of 0.98 which means the star's temperature is about 4,888 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

132 G. Aquilae 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 51.58 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

132 G. Aquilae Radius

132 G. Aquilae estimated radius has been calculated as being 8.56 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 5,958,219.54.km. If you need the diameter of the star, you just need to multiple the radius by 2. The figure is derived at by using the formula from SDSS rather than peer reviewed papers. It has been known to produce widely incorrect figures.

132 G. Aquilae Iron Abundance

132 G. Aquilae Iron Abundance is -0.02 with an error value of 0.04 Fe/H with the Sun has a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.

132 G. Aquilae Apparent and Absolute Magnitudes

132 G. Aquilae has an apparent magnitude of 5.30 which is how bright we see the star from Earth. Apparent Magnitude is also known as Visual Magnitude. Using the supplied Parallax value, you would get an absolute magnitude of 0.91 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 132 G. Aquilae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 13.23000 which gave the calculated distance to 132 G. Aquilae as 246.53 light years away from Earth or 75.59 parsecs. If you want that in miles, it is about 1,449,257,513,250,955.37, based on 1 Ly = 5,878,625,373,183.61 miles.

The star's Galacto-Centric Distance is 7,353.00 Parsecs or 23,982.79 Light Years. The Galacto-Centric Distance is the distance from the star to the Centre of the Galaxy which is Sagittarius A*.

Travel Time to 132 G. Aquilae

The time it will take to travel to this star is dependent on how fast you are going. U.G. has done some calculations as to how long it will take going at differing speeds. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days).

The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. Its primary mission was to visit Pluto which at the time of launch (2006), Pluto was still a planet.

DescriptionSpeed (m.p.h.)Time (years)
Walking441,331,779,386.84
Car1201,377,725,979.56
Airbus A380736224,629,235.80
Speed of Sound (Mach 1)767.269215,474,778.14
Concorde (Mach 2)1,534.54107,737,248.65
New Horizons Probe33,0005,009,912.65
Speed of Light670,616,629.00246.53

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 132 G. Aquilae Facts and Figures

Visual Facts


Primary / Proper / Traditional Name132 G. Aquilae
Alternative NamesHD 194013, HIP 100541, BD+04 4434
Spectral TypeG8III-IV
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeSubgiant Star
ColourYellow
GalaxyMilky Way
ConstellationAquila
Absolute Magnitude 0.91
Visual / Apparent Magnitude5.30
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)20h 23m 10.71
Declination (Dec.)+05° 20` 35.1
Galactic Latitude-17.62890317 degrees
Galactic Longitude48.75074468 degrees
Distance from Earth13.23000 Parallax (milliarcseconds)
 246.53 Light Years
 75.59 Parsecs
 15,591,448.06 Astronomical Units
Galacto-Centric Distance23,982.79 Light Years / 7,353.00 Parsecs
Proper Motion Dec.-38.91000 ± 0.28000 milliarcseconds/year
Proper Motion RA.-27.55000 ± 0.36000 milliarcseconds/year
B-V Index0.98
Radial Velocity-11.40000 ± 0.30 km/s
Iron Abundance-0.0200 ± 0.04 Fe/H
Eccentricity0.09510
Semi-Major Axis7066.0000000
Stellar Luminosity (Lsun)51.5800000

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Estimated Calculated Facts


Radius (x the Sun)8.56
Effective Temperature4,888 Kelvin

Sources and Links


SIMBAD SourceLink

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