Arcturus: Difference between revisions
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''This article is about the star. For a musical ensemble, see [[Arcturus (band)]].'' |
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'''Arcturus''', [[alpha (letter)|α]] [[Boötes|Boötis]], is the fourth brightest star in the sky at magnitude -0.05. |
'''Arcturus''', [[alpha (letter)|α]] [[Boötes|Boötis]], is the fourth brightest star in the sky at magnitude -0.05. |
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[[Category:Stars]] |
[[Category:Stars]] |
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[[ca:Arcturus]] [[de:Arcturus]] [[es:Arturo (estrella)]] [[it:Arturo]] |
[[ca:Arcturus]] [[de:Arcturus]] [[es:Arturo (estrella)]] [[it:Arturo]] |
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=Also= |
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[[Arcturus (band)]] |
Revision as of 10:27, 19 July 2004
This article is about the star. For a musical ensemble, see Arcturus (band).
Arcturus, α Boötis, is the fourth brightest star in the sky at magnitude -0.05.
Declination: 19°10'57" Right Ascension: 14h15m39.7s
It is a K1.5 IIIpe red giant star -- the letters "p" and "e" stand for "peculiar" and "emission", which indicates that the spectrum of light given off by the star is unusual and full of emission lines. This is not too unusual for red giants, but Arcturus has a particularly bad case of the phenomenon. It is 110 times more luminous than the Sun, but this underestimates its strength as much of the "light" it gives off is in the infrared; total power output is about 180 times than of the Sun.
According to the Hipparcos satellite, Arcturus is 36.7 light years (11.3 parsecs) from Earth, relatively close by in astronomical terms. From this satellite's observations, Arcturus is now known to be slightly variable, by about 0.04 magnitudes over 8.3 days. It is believed that the surface of the star oscillates slightly, a common feature of red giant stars. In the case of Arcturus, this was an interesting discovery as it is known that the redder (more towards or within the M spectral class) a giant gets, the more variable it will be. Extreme cases like Mira undergo large swings over hundreds of days; Arcturus is not very red and is a borderline case between variability and stability with its short period and tiny range.
Hipparcos also suggested that Arcturus is a binary star, with the companion about twenty times dimmer than the primary and orbiting close enough to be at the very limits of our current ability to make it out. The most recent studies of the issue are generally coming down on the side of it being a single star, however.
The name of the star derives from ancient Greek Arktouros and means "Bear Guard". This is a reference to it being the brightest star in the constellation Boötes, the Hunter, which is next to the Big and Little Bears, Ursa Major and Ursa Minor.
Pre-historic Polynesian navigators knew Arcturus as Hokule'a, the "Star of Joy". Arcturus is the zenith star of the Hawaiian Islands. Using Hokule'a and other stars, the Polynesians launched their double-hulled canoes from from Tahiti and the Marquesas Islands. Traveling east and north they eventually crossed the equator and reached the latitude where Arcturus would appear directly overhead in the summer night sky. Knowing they had arrived at the exact latitude of the island chain, they sailed due west on the trade winds until making landfall. If Hokule'a could be kept directly overhead, they landed on the southeastern shores of the Big Island of Hawaii. For a return trip to Tahiti the navigators could use Sirius, the zenith star of that island.
Arcturus is mentioned by name in the Bible, in Job 38:32.
An easy way to find Arcturus is to follow the arc of the handle of the Big Dipper. By continuing in this path, one can find Spica (α Virginis) as well.