Difference between revisions of "Precession of the equinoxes"
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| − | The '''precession of the equinoxes''' describes an astronomical phenomenon whereby the earth appears to wobble on its axis relative to the stars. This wobble is very slow | + | The '''precession of the equinoxes''' describes an astronomical phenomenon whereby the earth appears to wobble on its axis relative to the stars. This wobble is very slow.<ref>[http://findarticles.com/p/articles/mi_m1134/is_10_115/ai_n16883025 "Turn, turn, turn: in addition to its daily spin and its annual trip around the Sun, the Earth wobblesaffecting the seasons, the "north star," and human history," ''Natural History'', 2006]</ref> The result of this is that the position of stars and [[constellation]]s overhead at any particular time gradually changes over the years. For example, the constellation that rises above the horizon at the spring [[equinox]] gradually cycles through the signs of the [[zodiac]] backwards. The star around which all the other stars seem to revolve (to an observer on Earth) also changes over time, meaning that Polaris, or the present North Star, has not always been the star closest to north, and will be replaced by other stars in the future. The Earth's axis pointed to the star Thuban in the year 3000 B.C.<ref>[http://www.essortment.com/all/northstarastro_rmdz.htm "What is the north star?" ''Essortment.com'']</ref> |
| − | [[ | + | |
| + | ==List of selected North Stars<ref>http://www.glyphweb.com/esky/concepts/northerncelestialpole.html</ref>== | ||
| + | {| class="wikitable" | ||
| + | |- | ||
| + | !Approximate year | ||
| + | !Common name | ||
| + | !Astronomical name | ||
| + | |- | ||
| + | |3000 BC | ||
| + | |[[Thuban]] | ||
| + | |Alpha [[Draco (constellation)|Draco]]nis | ||
| + | |- | ||
| + | |1000 BC | ||
| + | |[[Kochab]] | ||
| + | |Beta [[Ursa Minor]]is | ||
| + | |- | ||
| + | |2000 AD | ||
| + | |[[Polaris]] | ||
| + | |Alpha [[Ursa Minor]]is | ||
| + | |- | ||
| + | |} | ||
| + | |||
| + | ==List of selected South Stars== | ||
| + | {| class="wikitable" | ||
| + | |- | ||
| + | !Approximate year | ||
| + | !Common name | ||
| + | !Astronomical name | ||
| + | |- | ||
| + | |4000 BC | ||
| + | |Achernar | ||
| + | |Alpha [[Eridanus|Eridani]] | ||
| + | |- | ||
| + | |2000 AD | ||
| + | |n/a | ||
| + | |Sigma [[Octent|Octans]] | ||
| + | |- | ||
| + | |} | ||
| + | |||
| + | == References == | ||
| + | {{reflist}} | ||
| + | |||
| + | [[Category:Astronomy]] | ||
Latest revision as of 20:22, May 14, 2017
The precession of the equinoxes describes an astronomical phenomenon whereby the earth appears to wobble on its axis relative to the stars. This wobble is very slow.[1] The result of this is that the position of stars and constellations overhead at any particular time gradually changes over the years. For example, the constellation that rises above the horizon at the spring equinox gradually cycles through the signs of the zodiac backwards. The star around which all the other stars seem to revolve (to an observer on Earth) also changes over time, meaning that Polaris, or the present North Star, has not always been the star closest to north, and will be replaced by other stars in the future. The Earth's axis pointed to the star Thuban in the year 3000 B.C.[2]
List of selected North Stars[3]
| Approximate year | Common name | Astronomical name |
|---|---|---|
| 3000 BC | Thuban | Alpha Draconis |
| 1000 BC | Kochab | Beta Ursa Minoris |
| 2000 AD | Polaris | Alpha Ursa Minoris |
List of selected South Stars
| Approximate year | Common name | Astronomical name |
|---|---|---|
| 4000 BC | Achernar | Alpha Eridani |
| 2000 AD | n/a | Sigma Octans |