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Polaris, Pole Star Facts

Polaris Facts

  • Polaris is a pulsating supergiant star that can be located in the constellation of Ursa Minor. The description is based on the spectral class.
  • Polaris is a main star of the constellation outline.
  • Based on the spectral type (F7:Ib-IIv SB) of the star, the star's colour is yellow to white .
  • Polaris is the 48th brightest star in the night sky and is the brightest star in Ursa Minor based on the Hipparcos 2007 apparent magnitude. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it.
  • Polaris has a radius that is 37.50 times bigger than the Suns. Radius
  • Using the most recent figures given by the 2007 Hipparcos data, the star is 432.58 light years away from us. Distance

Information on Polaris

Polaris is the most important star used for navigation, if you can locate the star, then you have a good idea of which direction is north. Polaris is the star nearly directly up from the North Pole in the Arctic hence why it is also known as the "North Star" in addition to being the "Pole Star". If you was to take a picture of the night sky so that you had star trails, If you then looked at all the photos, you would see that Polar stays still. Although it is the brightest star in the constellation, it is nowhere near being the brightest star in the night star, it is still bright but its only at position 45.

Polaris hasn't always been the Pole Star, in 3,000 B.C., the Pole Star title was Thuban, a star in Draco. 3,000 B.C. was roughly about the time when the Great Pyramids were being built.

Over time, Polaris will loose its title and Vega will gain the title in 13,000 years. Its a long way off so no need to worry about it. Then another 13,000 years after that, Polaris will regain its title as the Pole Star.Ref: N.A.S.A.

It is multiple star system with two stars close by, one nearby Polaris Ab and the other just a little further out Polaris B. There are also two distant stars in this system, C and D but are not as well documented at the closest.

Polaris is also the name given to the nuclear missiles that were used by the Royal Navy submarines of the United Kingdom of the sixties to the nineties. The missiles were then replaced by the Trident nuclear system.

It is relatively easy to locate if you know what you are looking for. If you first look for the distinctive Ursa Major first and then use the two stars on the right of the plough part, Merak and Dubhe and then fellow up from those stars in a line, you will come across Polaris.

At the other end of the night sky is Polaris Australis in the constellation of Octans is the closest you will get to a star being "under" the South Pole.

Polaris's Alternative Names

Alpha Ursae Minoris (Alf Umi) is the Bayer Classification for the star. The Bayer Classification was created by Johann Bayer in 1603. The brightest star in the constellation is normally given the Alpha designation, there are exceptions such as Pollux which is Beta Geminorum.

The Id of the star in the Yale Bright Star Catalogue is HR424. HIP11767 is the reference name for the star in the Hipparcos Star Catalogue. The Id of the star in the Henry Draper catalogue is HD8890.

Polaris has alternative name(s) :- Pole Star, alf UMi.

Flamsteed designations are named after the creator, Sir John Flamsteed. Sir John named the stars in the constellation with a number and its latin name, this star's Flamsteed designation is 1 Ursae Minoris. The Flamsteed name can be shortened to 1 Umi.

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+88 8.

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

Location of Polaris

The location of the supergiant 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 Polaris, the location is 02h 31m 47.08 and +89° 15` 50.9 .

Radial Velocity and Proper Motion of Polaris

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 -11.85 ± 0.10 milliarcseconds/year towards the north and 44.48 ± 0.11 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 -16.42000 km/s with an error of about 0.03 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 Polaris

Polaris Temperature and Colour

Based on the star's spectral type of F7:Ib-IIv SB , Polaris's colour and type is yellow to white supergiant star. The star's effective temperature is 6,015 Kelvin which is hotter than our own Sun's effective Temperature which is 5,777 Kelvin.

Polaris 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 2,634.12 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012.

Polaris Radius

Polaris Radius has been calculated as being 37.50 times bigger than the Sun. The Sun's radius is 695,800km, therefore the star's radius is an estimated 26,092,500.00.km. If you need the diameter of the star, you just need to multiple the radius by 2.

Polaris Mass

The Polaris's solar mass is 5.40 times that of our star, the Sun. The Sun's Mass is 1,989,100,000,000,000,000,000 billion kg. which to calculate using this website is too large. To give idea of size, the Sun is 99.86% the mass of the solar system.

Polaris Iron Abundance

Polaris Iron Abundance is 0.13 with an error value of 9.99 Fe/H with the Sun has a value of 1 to put it into context. The value comes from the Hipparcos Extended Catalog.

Polaris Apparent and Absolute Magnitudes

Polaris has an apparent magnitude of 1.97 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 -3.64 If you used the 2007 Parallax value, you would get an absolute magnitude of -3.64. 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 Polaris

Using the original Hipparcos data that was released in 1997, the parallax to the star was given as 7.56000 which gave the calculated distance to Polaris as 431.43 light years away from Earth or 132.28 parsecs. If you want that in miles, it is about 2,536,215,344,752,604.86, based on 1 Ly = 5,878,625,373,183.61 miles.

In 2007, Hipparcos data was revised with a new parallax of 7.54000 which put Polaris at a distance of 432.58 light years or 132.63 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 27,356,710.63 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. The star's Galacto-Centric Distance is 7,466.00 Parsecs or 24,351.36 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 Polaris

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)
Walking472,523,835,343.21
Car1202,417,461,178.11
Airbus A380736394,151,279.04
Speed of Sound (Mach 1)767.269378,088,182.08
Concorde (Mach 2)1,534.54189,043,844.65
New Horizons Probe33,0008,790,767.92
Speed of Light670,616,629.00432.58

Variable Type of Polaris

The star is a pulsating Delta Cepheid 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. Polaris brightness ranges from a magnitude of 2.124 to a magnitude of 2.093 over its variable period. The smaller the magnitude, the brighter the star. Its variable/pulsating period lasts for 4.0 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 Polaris Facts and Figures

Visual Facts


Primary / Proper / Traditional NamePolaris
Alternative NamesAlpha Ursae Minoris, Alf Umi, Pole Star, HD 8890, HIP 11767, HR 424, 1 Ursae Minoris, 1 Umi, BD+88 8, alf UMi
Spectral TypeF7:Ib-IIv SB
Constellation's Main StarYes
Multiple Star SystemYes
Star TypeLuminous Giant Star less luminour Supergiant Star
ColourYellow - White
GalaxyMilky Way
ConstellationUrsa Minor
Absolute Magnitude -3.64 / -3.64
Visual / Apparent Magnitude1.97
Naked Eye VisibleYes - Magnitudes
Right Ascension (R.A.)02h 31m 47.08
Declination (Dec.)+89° 15` 50.9
Galactic Latitude26.46137410 degrees
Galactic Longitude123.28042130 degrees
1997 Distance from Earth7.56000 Parallax (milliarcseconds)
 431.43 Light Years
 132.28 Parsecs
2007 Distance from Earth7.54000 Parallax (milliarcseconds)
 432.58 Light Years
 132.63 Parsecs
 27,356,710.63 Astronomical Units
Galacto-Centric Distance24,351.36 Light Years / 7,466.00 Parsecs
Proper Motion Dec.-11.85000 ± 0.10000 milliarcseconds/year
Proper Motion RA.44.48000 ± 0.11000 milliarcseconds/year
B-V Index0.63
Radial Velocity-16.42000 ± 0.03 km/s
Iron Abundance0.1300 ± 9.99 Fe/H
Eccentricity0.13220
Semi-Major Axis6543.0000000
Stellar Luminosity (Lsun)2634.1200000
Brightest in Night Sky48th
Associated / Clustered StarsPolaris Ab
Polaris B

Companions (Multi-Star and Exoplanets) Facts


Exoplanet CountNone/Unaware

Variable Star Details


Variable Star ClassPulsating
Variable Star TypeDelta Cepheid
Mean Variability Period in Days3.971
Variable Magnitude Range (Brighter - Dimmer)2.093 - 2.124

Estimated Calculated Facts


Radius (x the Sun)37.50
Effective Temperature5,807 Kelvin
Mass Compared to the Sun5.40

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
8890+88 8.0A2.1000058.00000-4.00000F8Yellow/White
B9.100001955
C13.100001890
D12.100001884

Location of Polaris in Ursa Minor


Polaris Location in Ursa Minor

The map was generated using Night Vision, an awesome free application by Brian Simpson.

Ursa Minor Main Stars


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