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Thuban, Alpha Draconis (α Dra), is a spectroscopic binary star system located in the constellation Draco. Even though it has the designation Alpha, it is only the eighth brightest star in Draco. It has an apparent magnitude of 3.6452 and lies at an approximate distance of 303 light years from Earth. From 3942 BCE to 1793 BCE, Thuban was the north pole star, the nearest visible star to the north celestial pole.

Star system

Alpha Draconis is a single-lined spectroscopic binary star system, which means that only the spectral lines of the primary component are visible. The binary pair orbit each other with a period of 51.5 days and an eccentricity of 0.43. The stars are separated by about 0.46 astronomical units.

The primary component, formally named Thuban and designated Alpha Draconis A, has the stellar classification A0III, indicating a white giant star. The star has been used as a spectral standard for its class. It has a mass 2.8 times that of the Sun and is 479 times more luminous. It has stopped fusing hydrogen in its core and has expanded to a size of 3.4 solar radii. It has an effective temperature of 10,100 K.

thuban star,alpha draconis

Thuban (Alpha Draconis), image: Wikisky

The companion, Alpha Draconis B, has 2.6 solar masses and shines with 40 solar luminosities. It is 1.83 magnitudes fainter than the primary component. It is believed to be a main sequence star slightly cooler than the giant, possibly of the spectral type A2.

In 2019, a survey with the Transiting Exoplanet Survey Satellite (TESS) revealed that the system was an eclipsing binary star. It exhibits primary and secondary eclipses with depths of 9% and 2%, indicating that the eclipses are partial, with an inclination of slightly less than 90°. They last only six hours.

Pole star

Thuban is one of the stars that take their turn as the North Star during the Earth’s precession cycle. It last held the title from 3942 BCE to 1793 BCE, when some of ancient Egypt’s largest pyramids were built. It was closest to the pole in 2830 BCE.

Of all the pole stars, Thuban comes closest to the north celestial pole – within 0.2° – but it is also fainter than most other pole stars. In comparison, Polaris, the current North Star, comes within 0.5° of the north celestial pole and has an apparent magnitude of 1.98. Polaris is very useful in navigation because it is both relatively bright and located very close to the pole. The same cannot be said for the current south pole star, Sigma Octantis (Polaris Australis), which is barely visible with a magnitude of 5.47 and cannot be used in navigation. The brightest stars that serve as indicators of true north – Vega (mag. 0.026) and Deneb (mag. 1.25) – only come within 5° and 7° of the pole.

axial precession,north stars

Animation of the cycle of precession of Earth’s axis, depicting the orientation of the axis in relation to the North Ecliptic Pole. Image: Wikimedia Commons/Tfr000 (CC BY-SA 3.0)

As the North Star, Thuban was preceded by Edasich (Iota Draconis, mag. 3.29) and succeeded by the brighter Kochab (Beta Ursae Minoris, mag. 2.08), one of the stars of the Little Dipper, and the fainter Kappa Draconis (mag. 3.82). Kochab and Kappa Draconis share timing as near-north stars, coming within 6° and 7° of the north celestial pole.

north pole stars

North Stars (marked red), image: Roberto Mura

Thuban has slowly drifted away from true north over the last 4,800 years but will gradually move back and be the North Star again in 20346 CE.

Other than Polaris, Thuban, Edasich, Vega, Deneb, Kochab and Kappa Draconis, the stars that serve as the North Star over the course of Earth’s 26,000-year precession cycle are Errai (Gamma Cephei), Iota Cephei and Alfirk (Beta Cephei), Alderamin (Alpha Cephei), Fawaris (Delta Cygni), Iota Herculis, and Tau Herculis.

Thuban, Big Dipper and Little Dipper, image: Wikisky


The name Thuban (pronunciation: /ˈθjuːbæn/) comes from the Arabic word thuʿbān, denoting a large snake. Thuban has also been known as Adib, derived from the Arabic Al Dhi’bah, meaning “the hyenas,” and as the Dragon’s Tail, the latter indicating its position in the constellation.

The name Thuban was approved by the International Astronomical Union’s (IAU) Working Group on Star Names (WGSN) on June 30, 2016. It formally applies only to the component Alpha Draconis A.

The Chinese know Alpha Draconis as 紫微右垣一 (Zǐ Wēi Yòu Yuán yī), or the First Star of Right Wall of Purple Forbidden Enclosure. The Chinese asterism called the Right Wall of Purple Forbidden Enclosure is formed by Thuban with Kappa Draconis, Giausar (Lambda Draconis), 24 Ursae Majoris, Alpha Camelopardalis, 43 Camelopardalis, and BK Camelopardalis. The Purple Forbidden Enclosure is located in the area of the sky around the north celestial pole and it represents the imperial palace. Thuban represents the Right Pivot (右樞,Yòu Shū).


Thuban is easy to identify but challenging to see from light-polluted areas. The star lies about halfway between Mizar, the middle star of the Big Dipper’s handle, and Kochab and Pherkad, the stars that form the outer side of the Little Dipper’s bowl.

An imaginary line extended from Phecda through Megrez, the inner stars of the Big Dipper’s bowl, points toward the star.

find thuban, where is thuban

Thuban location, image: Wikisky


Thuban lies in the constellation Draco. Draco is the eighth largest constellation in the sky and the fourth largest northern constellation, occupying an area of 1,083 square degrees. However, it is not particularly conspicuous, as its brightest star, Eltanin (Gamma Draconis), has an apparent magnitude of 2.24.

Draco lies in the far northern sky, winding around the north celestial pole, and is circumpolar, i.e. it never sets and is visible throughout the year, for observers in northern latitudes.

Draco constellation,draco stars,draco star map,dragon constellation

Draco constellation map by IAU and Sky&Telescope magazine

The constellation contains several interesting deep sky objects. These include the lenticular galaxy NGC 5866, nicknamed the Spindle Galaxy and believed to be the object Charles Messier catalogued as M102, the disrupted spiral galaxy known as the Tadpole Galaxy (Arp 188), the Cat’s Eye Nebula (NGC 6543), a bright planetary nebula with a visual magnitude of 9.8, the massive galaxy cluster Abell 2218, and the Draco Dwarf Galaxy, one of the faintest satellites of the Milky Way.

The best time of year to observe the stars and deep sky objects in Draco is during the month of July.

The 10 brightest stars in Draco are Eltanin (Gamma Dra, mag. 2.23), Athebyne (Eta Dra, mag. 2.73), Rastaban (Beta Dra, mag. 2.79), Altais (Delta Dra, mag. 3.07), Aldhibah (Zeta Dra, mag. 3.17), Edasich (Iota Dra, mag. 3.29), Chi Draconis (mag. 3.57), Thuban (Alpha Dra, mag. 3.6452), Grumium (Xi Dra, mag. 3.75), and Giausar (Lambda Dra, mag. 3.85).

Thuban – Alpha Draconis

Spectral classA0III
Variable typeEclipsing binary
U-B colour index-0.08
B-V colour index-0.04
Apparent magnitude3.6452
Absolute magnitude-1.20
Distance303 ± 5 light years (93 ± 1 parsecs)
Parallax10.76 ± 0.17 mas
Radial velocity-13.0 km/s
Proper motionRA: -56.34 mas/yr
Dec.: 17.21 mas/yr
Mass (α Dra A, α Dra B)2.8 M, 2.6 M
Luminosity (α Dra A, α Dra B)479 L, 40 L
Radius (α Dra A)3.4 R
Temperature (α Dra A)10,100 K
Metallicity (α Dra A)-0.20 dex
Rotational velocity (α Dra A)26 km/s
Surface gravity (α Dra A)3.5 cgs
Right ascension14h 04m 23.3498s
Declination64° 22′ 33.062″
Names and designationsThuban, Alpha Draconis, α Dra, 11 Draconis, HD 123299, HR 5291, HIP 68756, GC 19019, GCRV 8269, PPM 18861, SAO 16273, FK5 521, BD+65° 978, AG+64° 666, GSC 04174-01262, IRAS 14030+6436, 2MASS J14042335+6422331, PLX 3209, TYC 4174-1262-1, Gaia DR2 1667976701458550400