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| − | '''Thuban''', also known as '''Alpha Draconis''', is a fourth magnitude binary star, some 310 light years away in the constellation of [[Draco]]. The star is notable, because most stars this faint do not carry a proper name. Thuban, though, is a star that plays a significant historical role because it was once the pole, or north star of the ancient world. The name Thuban itself is derived from the [[Arabic]] ثعبان ''θu‘bān'', meaning "the basilisk", which was also applied to the entire Draco constellation.<ref>http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html</ref> | + | {{Night Sky |
| | + | | image = |
| | + | | designation =HD 123299<br/>HIP 68756 |
| | + | | rightascension =14<sup>h</sup> 04<sup>m</sup> 23.34995<sup>s</sup><ref name=simbad>[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=thuban&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id Alpha Draconis] from the [http://simbad.u-strasbg.fr/simbad SIMBAD Astronomical Database]</ref> |
| | + | | declination =+64° 22′ 33.0619″<ref name=simbad/> |
| | + | | distance =303 ly<ref>Calculated from given [[parallax]] of 10.76 mas.</ref> |
| | + | | constellation =Draco |
| | + | | type =Binary star |
| | + | | dimensions = |
| | + | | magnitude =Apparent Mag: +3.65<ref name=simbad/><br/>Absolute Mag: -1.19<ref>From definition of absolute magnitude, using apparent magnitude (+3.65) and distance (303 ly) given here.</ref> |
| | + | | redshift = |
| | + | | radvelocity =-13.0±0.9 km/s<ref name=simbad/> |
| | + | | propmotion =RA: -56.34 mas/yr<ref name=simbad/><br/>Dec.: 17.21 mas/yr<ref name=simbad/> |
| | + | | parallax =10.76±0.17 mas<ref name=simbad/> |
| | + | }} |
| | + | '''Thuban''', also known as '''Alpha Draconis''', is a fourth magnitude [[binary star]], some 310 light years away in the [[constellation]] of [[Draco]]. The star is notable, because most stars this faint do not carry a proper name. Thuban, though, is a star that plays a significant historical role because it was once the pole, or north star of the ancient world. The name Thuban itself is derived from the [[Arabic]] ثعبان ''θu‘bān'', meaning "the basilisk", which was also applied to the entire Draco constellation.<ref>Allen, Richard Hinkley (1963). Star Names, Their Lore and Meaning. New York: Dover. ISBN 0-486-21079-0. Available online at: [http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html penelope.uchicago.edu]</ref> |
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| − | Thuban has an apparent magnitude of 3.65, also making its alpha [[Bayer designation]] unusual. The designation is usually reserved for the brightest star in a constellation, in this case - [[Gamma Draconis]]. Alpha Draconis is only the fourth brightest. The star itself is easy to spot, despite its faintness, because of its location relative to the [[Big Dipper]]. The two inner stars of the Big Dipper can be used to locate Thuban, which appears very nearby in the night sky. | + | Thuban has an apparent magnitude of 3.65, also making its alpha [[Bayer designation]] unusual. The designation is usually reserved for the brightest star in a constellation, in this case - [[Gamma Draconis]]. Alpha Draconis is only the fourth brightest. The star itself is easy to spot, despite its faintness, because of its location relative to the [[Big Dipper]]. The two inner stars of the Big Dipper can be used to locate Thuban, which appears very nearby in the night sky. |
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| | ==The Star== | | ==The Star== |
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| − | Thuban is a rare white giant [[star]] of spectral class A0 III.<ref>http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Alpha+Draconis</ref> The star is much like [[Vega]]. As a giant star, however, Thuban has already evolved off of the main sequence. The star is 3.5 times the mass of our [[Sun]], and is 265 times the radius. The star is 300 times as visually luminous as the Sun even though much of the energy emitted is in the [[ultraviolet]]. The surface temperature is 9800 K.<ref name="illinos">http://stars.astro.illinois.edu/sow/thuban.html</ref> | + | Thuban is a rare white giant [[star]] of spectral class A0 III.<ref name=simbad/> The star is much like [[Vega]]. As a giant star, however, Thuban has already evolved off of the main sequence. The star is 3.5 times the mass of our [[Sun]], and is 265 times the radius. The star is 300 times as visually luminous as the Sun even though much of the energy emitted is in the [[ultraviolet]]. The surface temperature is 9,800 K.<ref name="illinos">[http://stars.astro.illinois.edu/sow/thuban.html Thuban] from stars.astro.illinois.edu</ref> |
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| − | As a giant, Thuban has already used up its core [[hydrogen]] fuel. Depending on the stage of its life as a giant, the star may be either expanding and cooling to become an orange giant or that the [[helium]] fuel in the core has already been used up. If the latter is true, the star is actually contracting and will start to fuse [[carbon]] in the core, becoming a blue giant.<ref name="illinos"/> | + | As a giant, Thuban has already used up its core [[hydrogen]] fuel. Depending on the stage of its life as a giant, the star may be either expanding and cooling to become an orange giant or that the [[helium]] fuel in the core has already been used up. If the latter is true, the star is actually contracting and will start to fuse [[carbon]] in the core, becoming a blue giant.<ref name="illinos"/> |
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| | It is known that Thuban has a small companion star. The companion, which has not been directly imaged, orbits the primary once every 51 days and may be either a red or [[white dwarf]].<ref name="illinos"/> | | It is known that Thuban has a small companion star. The companion, which has not been directly imaged, orbits the primary once every 51 days and may be either a red or [[white dwarf]].<ref name="illinos"/> |
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| | ==Thuban as a Pole Star== | | ==Thuban as a Pole Star== |
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| − | Thuban was the pole star, meaning the closest star to the celestial north pole that can be seen with the unaided eye. Due to the [[precession of the equinoxes]], Thuban was the pole star from around 3900 BC until 1900 BC, when the much brighter [[Beta Ursae Minoris]] replaced it (Although Thuban was still closer to the celestial pole until 1793 BC).<ref>http://www.daviddarling.info/encyclopedia/T/Thuban.html</ref> At present, Thuban is slowly moving away from the northern celestial pole. | + | Thuban was the pole star, meaning the closest star to the celestial north pole that can be seen with the unaided eye. Due to the [[precession of the equinoxes]], Thuban was the pole star from around 3900 BC until 1900 BC, when the much brighter [[Beta Ursae Minoris]] replaced it (although Thuban was still closer to the celestial pole until 1793 BC).<ref>[http://www.daviddarling.info/encyclopedia/T/Thuban.html Thuban] from daviddarling.info</ref> At present, Thuban is slowly moving away from the northern celestial pole. |
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| − | [[Category:Astronomy]]
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| − | [[Category:Double Stars]]
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| | ==References== | | ==References== |
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| | {{Stars}} | | {{Stars}} |
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| | + | [[Category:Astronomy]] |
| | + | [[Category:Stars]] |
| | + | [[Category:Double Stars]] |