Antares (α Scorpii, α Sco, Alpha Scorpii) is a red supergiant star in the Milky Way galaxy and the sixteenth brightest star in the nighttime sky (sometimes listed as 15th brightest, if the two brighter components of the Capella quadruple star system are counted as one star). Along with Aldebaran, Spica, and Regulus it is one of the four brightest stars near the ecliptic. Antares is a slow variable star with an average magnitude of +1.09.
1.1 Companion star
1.2 Position on the ecliptic
2 Antares in ancient cultures
3 See also
5 External links
Comparison between the red supergiant Antares and the Sun, shown as the tiny dot toward the upper right. The black circle is the size of the orbit of Mars. Arcturus is also included in the picture for size comparison.
Antares is a class M supergiant star, with a radius of approximately 800 times that of the sun; if it were placed in the center of our solar system, its outer surface would lie between the orbits of Mars and Jupiter. Antares is approximately 600 light-years (180 pc) from our solar system. Its visual luminosity is about 10,000 times that of the Sun, but because the star radiates a considerable part of its energy in the infrared part of the spectrum, the bolometric luminosity equals roughly 65,000 times that of the Sun. The mass of the star is calculated to be 15 to 18 solar masses. Its large size and relatively small mass give Antares a very low average density.
The size of Antares may be calculated using its parallax and angular diameter. The parallax angle is given in the box to the right, and the angular diameter is known from lunar occultation measurements (41.3 ± 0.1 mas). This leads to a radius of 822 ± 80 solar radii.[clarification needed]
Antares is a type LC slow irregular variable star, whose apparent magnitude slowly varies from +0.88 to +1.16.
The best time to view Antares is on or around May 31 of each year, when the star is at opposition to the Sun. At this time, Antares rises at dusk and sets at dawn, and is thus in view all night. For approximately two to three weeks on either side of November 30, Antares is not visible at all, being lost in the Sun’s glare; this period of invisibility is longer in the Northern Hemisphere than in the Southern Hemisphere, since the star’s declination is significantly south of the celestial equator.
 Companion star
Antares has a hot blue companion star, Antares B, of spectral type B2.5 at a separation of about 2.9 arcseconds, or 550 AUs at Antares’ estimated distance. At magnitude 5.5, it is only 1/370th as bright visually as Antares A, although it shines with 170 times the Sun’s luminosity. It is normally difficult to see in small telescopes due to Antares’ glare, but can sometimes be seen in apertures over 150 mm (5.9 in). The companion is often described as green, but this is probably a contrast effect. Antares B can be observed with a small telescope for a few seconds during lunar occultations while Antares itself is hidden by the Moon; it was discovered by Johann Tobias Bürg during one such occultation on April 13, 1819.
The orbit is poorly known, with an estimated period of 878 years.
 Position on the ecliptic
Antares is one of the 4 first magnitude stars that lies within 5° of the ecliptic and therefore can be occulted by the Moon and rarely by the planets. On 31 July 2009, Antares was occulted by the moon. The event was visible in much of southern Asia and the Middle East. Every year around December 2 the Sun passes 5° north of Antares.
 Antares in ancient cultures
Antares, the proper name of this star, derives from the Ancient Greek Άντάρης, meaning “(holds) against Ares (Mars)”, due to the similarity of its reddish hue to the appearance of the planet Mars. It is the brightest star in the constellation Scorpius. However, it is also thought that Antares may have been named after the ancient Arab warrior-poet Antar. Its distinctive color has made the star an object of interest to many societies throughout history.
Many of the old Egyptian temples are oriented so that the light of Antares plays a role in the ceremonies performed there.
In ancient Persia (around 3000 BC), Antares was known as Satevis, one of the four “royal stars”.
In ancient India, it with σ and τ Sco were one of nakshatra (Hindu lunar mansion), as Jyeshthā “Oldest”, and Rohinī “Ruddy”.
In ancient China, it was named 心宿二 (Mandarin: xī xìu èr), because it was the second star of the asterism 心宿 (“Heart”).
In the religion of Stregheria, Antares is a fallen angel and quarter guardian of the western gate.
In astrology, Antares is one of the Behenian fixed stars and has the symbol Agrippa1531 corScorpii.png.
The Wotjobaluk Koori people of Victoria knew Antares as Djuit, son of Marpean-kurrk (Arcturus); the stars on each side represented his wives. The Kulin Kooris saw Antares (Balayang) as the brother of Bunjil (Altair).
Alternative name of this star, meaning “the Heart of Scorpion”:
Calbalakrab from the Arabic Qalb al-Άqrab. This had been directly translated from the Ancient Greek Καρδία Σκορπίου Kardia Skorpiū.
Cor Scorpii translated above Greek name into Latin.