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Created page with 'Antares, also known as Alpha Scorpii is a binary system that consists of a red supergiant and it’s hot, blue companion star located in the constellation Scorpius. Antares ...'
Antares, also known as Alpha Scorpii is a binary system that consists of a red supergiant and it’s hot, blue companion star located in the constellation [[Scorpius]]. Antares is easily seen in the night sky as the fifteenth brightest star in the sky, known since ancient times.
==Antares in history==
The name Antares is a derivative of the [[Ancient Greek]] Αντάρης, meaning "(holds) against [[Ares]] ([[Mars]])" because like [[Mars]], the star appears with a reddish hue in the sky, it is this distinct color that made Antares well known to ancient cultures.
In [[Ancient Egypt]], many temples are aligned in such a way that the light from Antares plays a role in the temple ceremonies. The [[Persians]] referred to Antares as ''Satevis'' and it was referenced in their culture to as far back as 3000 B.C. as one of the four royal stars. In ancient [[India]] the star was called ''Jyeshtha'', the [[Arabs]] called it Ķalb al Άķrab, or the "Scorpion's heart"<ref>Richard Hinckley Allen, Star-names and their meanings (1936), p. 365.</ref>.
== The star ==
The Antares system is actually a binary star system even though the unaided eye sees only the primary star. The system itself is estimated to be some 600 light years from [[Earth]]; despite this distance Antares still has an apparent luminosity of +0.9 to +1.8, as it is a variable star.
The primary, Antares, is a class M1.5Iab-b [[supergiant]]<ref>http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=antares&submit=SIMBAD+search</ref> with a radius of 34 AUs, or some 700 times the radius of our own sun, if the star was at the center of our [[solar system]], it would extend to between the orbits of [[Mars]] and [[Jupiter]]. Despite Antares’ size, it contains only 15 to 18 times the mass of the sun; giving Antares a very low average density. Its visual luminosity is some 10,000 time of the sun, with an absolute luminosity of 60,000 times, much of which is in the infrared. Like all M class stars, its surface is relativity cool in comparison to other stars at 3600K<ref name="Illinois">http://www.astro.illinois.edu/~jkaler/sow/antares.html</ref>.
Antares b, the companion star is a blue star of spectral type B2.5V. Although much dimmer then it’s giant companion, Antares b is still 170 times as luminous as our [[sun]]. By itself the star could be since by the unaided eye but because of the glare of its neighbor, a small [[telescope]] is required to see the star at all. It is estimated that the two stars are some 550AUs from each other, but their orbit is still poorly understood.
Antares is coming towards the end of its [[stellar evolution]] and will soon develop an [[iron]] core, the last stage for a star of its mass before exploding into a [[supernova]]<ref name="Illinois">http://www.astro.illinois.edu/~jkaler/sow/antares.html</ref>.
[[Category:Astronomy]]
==References==
{{reflist}}
==Links==
*[http://www.co-intelligence.org/newsletter/comparisons.html Antares in comparison to other stellar bodies]
==Antares in history==
The name Antares is a derivative of the [[Ancient Greek]] Αντάρης, meaning "(holds) against [[Ares]] ([[Mars]])" because like [[Mars]], the star appears with a reddish hue in the sky, it is this distinct color that made Antares well known to ancient cultures.
In [[Ancient Egypt]], many temples are aligned in such a way that the light from Antares plays a role in the temple ceremonies. The [[Persians]] referred to Antares as ''Satevis'' and it was referenced in their culture to as far back as 3000 B.C. as one of the four royal stars. In ancient [[India]] the star was called ''Jyeshtha'', the [[Arabs]] called it Ķalb al Άķrab, or the "Scorpion's heart"<ref>Richard Hinckley Allen, Star-names and their meanings (1936), p. 365.</ref>.
== The star ==
The Antares system is actually a binary star system even though the unaided eye sees only the primary star. The system itself is estimated to be some 600 light years from [[Earth]]; despite this distance Antares still has an apparent luminosity of +0.9 to +1.8, as it is a variable star.
The primary, Antares, is a class M1.5Iab-b [[supergiant]]<ref>http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=antares&submit=SIMBAD+search</ref> with a radius of 34 AUs, or some 700 times the radius of our own sun, if the star was at the center of our [[solar system]], it would extend to between the orbits of [[Mars]] and [[Jupiter]]. Despite Antares’ size, it contains only 15 to 18 times the mass of the sun; giving Antares a very low average density. Its visual luminosity is some 10,000 time of the sun, with an absolute luminosity of 60,000 times, much of which is in the infrared. Like all M class stars, its surface is relativity cool in comparison to other stars at 3600K<ref name="Illinois">http://www.astro.illinois.edu/~jkaler/sow/antares.html</ref>.
Antares b, the companion star is a blue star of spectral type B2.5V. Although much dimmer then it’s giant companion, Antares b is still 170 times as luminous as our [[sun]]. By itself the star could be since by the unaided eye but because of the glare of its neighbor, a small [[telescope]] is required to see the star at all. It is estimated that the two stars are some 550AUs from each other, but their orbit is still poorly understood.
Antares is coming towards the end of its [[stellar evolution]] and will soon develop an [[iron]] core, the last stage for a star of its mass before exploding into a [[supernova]]<ref name="Illinois">http://www.astro.illinois.edu/~jkaler/sow/antares.html</ref>.
[[Category:Astronomy]]
==References==
{{reflist}}
==Links==
*[http://www.co-intelligence.org/newsletter/comparisons.html Antares in comparison to other stellar bodies]