Universe Guide

AQ Andromedae

AQ Andromedae Facts

  • AQ Andromedae is a pulsating variable star that can be located in the constellation of Andromeda. The description is based on the spectral class.
  • AQ Andromedae is not part of the constellation outline but is within the borders of the constellation.
  • The star can not be seen by the naked eye, you need a telescope to see it.
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 8583.25 light years away from us. Distance

AQ Andromedae's Alternative Names

HIP2180 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD2342.

AQ Andromedae has alternative name(s) :- , AQ And.

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+34 56.

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

Location of AQ Andromedae

The location of the variable 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 AQ Andromedae, the location is 00h 27m 31.69 and +35° 35` 14.6 .

Radial Velocity and Proper Motion of AQ Andromedae

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 -12.49 ± 0.56 milliarcseconds/year towards the north and -4.09 ± 0.92 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 -14.00000 km/s with an error of about 3.10 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 AQ Andromedae

AQ Andromedae Temperature and Colour

Based on the star's spectral type of N0v The star has a B-V Colour Index of 2.1 which means the star's temperature is about 1,181 Kelvin. The temperature was calculated using information from Morgans @ Uni.edu.

AQ Andromedae Radius

AQ Andromedae estimated radius has been calculated as being 8,137.30 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 5,661,932,792.05.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 1715.7227196736844311726590365. 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.

AQ Andromedae Apparent and Absolute Magnitudes

AQ Andromedae has an apparent magnitude of 7.67 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 -7.81 If you used the 2007 Parallax value, you would get an absolute magnitude of -4.43. 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 AQ Andromedae

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 0.08000 which gave the calculated distance to AQ Andromedae as 40770.42 light years away from Earth or 12500 parsecs. If you want that in miles, it is about 239,674,025,487,352,516.82, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 0.38000 which put AQ Andromedae at a distance of 8583.25 light years or 2631.58 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 542,798,556.55 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.

Travel Time to AQ Andromedae

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)
Airbus A3807367,820,747,528.35
Speed of Sound (Mach 1)767.2697,502,023,646.03
Concorde (Mach 2)1,534.543,751,006,934.24
New Horizons Probe33,000174,426,369.12
Speed of Light670,616,629.008,583.25

Variable Type of AQ Andromedae

The star is a pulsating Semi-Regular Star w 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. AQ Andromedae brightness ranges from a magnitude of 7.982 to a magnitude of 7.569 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 0.4 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 AQ Andromedae Facts and Figures

Visual Facts

Primary / Proper / Traditional NameAQ Andromedae
Alternative NamesHD 2342, HIP 2180, BD+34 56, AQ And
Spectral TypeN0v
Constellation's Main StarNo
Multiple Star SystemNo / Unknown
Star TypeVariable Star
GalaxyMilky Way
Absolute Magnitude -7.81 / -4.43
Visual / Apparent Magnitude7.67
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Right Ascension (R.A.)00h 27m 31.69
Declination (Dec.)+35° 35` 14.6
Galactic Latitude-27.03095383 degrees
Galactic Longitude117.47640233 degrees
1997 Distance from Earth0.08000 Parallax (milliarcseconds)
 40770.42 Light Years
 12500 Parsecs
2007 Distance from Earth0.38000 Parallax (milliarcseconds)
 8583.25 Light Years
 2631.58 Parsecs
 542,798,556.55 Astronomical Units
Proper Motion Dec.-12.49000 ± 0.56000 milliarcseconds/year
Proper Motion RA.-4.09000 ± 0.92000 milliarcseconds/year
B-V Index2.1
Radial Velocity-14.00000 ± 3.10 km/s

Companions (Multi-Star and Exoplanets) Facts

Exoplanet CountNone/Unaware

Variable Star Details

Variable Star ClassPulsating
Variable Star TypeSemi-Regular Star w
Mean Variability Period in Days0.356
Variable Magnitude Range (Brighter - Dimmer)7.569 - 7.982

Estimated Calculated Facts

Radius (x the Sun)1,715.72
Effective Temperature1,181 Kelvin

Sources and Links

SIMBAD SourceLink

Related Stars

Comments and Questions

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