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'''Antares''' (α Scorpii / [[alpha (letter)|Alpha]] Scorpii) is a [[red supergiant]] [[star]] in the [[Milky Way]] [[galaxy]] and [[list of brightest stars|the |
'''Antares''' (α Scorpii / [[alpha (letter)|Alpha]] Scorpii) is a [[red supergiant]] [[star]] in the [[Milky Way]] [[galaxy]] and [[list of brightest stars|the 15th brightest star]] in the nighttime sky (sometimes listed as 15th brightest, if the two brighter components of the [[Capella (star)|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]]. |
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Antares is a variable star, whose apparent magnitude varies from +0.9 to +1.8. |
Antares is a variable star, whose apparent magnitude varies from +0.9 to +1.8. |
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Revision as of 08:39, 20 March 2009
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Scorpius |
| Right ascension | 16h 29m 24s[1] |
| Declination | −26° 25′ 55″[1] |
| Apparent magnitude (V) | +0.9~1.8, Average: +1.09[1] |
| Characteristics | |
| Spectral type | M1.5Iab-b / B2.5V[1] |
| U−B color index | 1.34 |
| B−V color index | 1.87 |
| Variable type | LC-type |
| Astrometry | |
| Radial velocity (Rv) | −3.4[1] km/s |
| Proper motion (μ) | RA: −10.16[1] mas/yr Dec.: −23.21[1] mas/yr |
| Parallax (π) | 5.40 ± 1.68 mas[1] |
| Distance | approx. 600 ly (approx. 190 pc) |
| Absolute magnitude (MV) | −5.28 |
| Details | |
| Mass | 15.5 M☉ |
| Radius | 700 R☉ |
| Luminosity | 65,000(bolometric) L☉ |
| Temperature | 3,500 K |
| Other designations | |
| Database references | |
| SIMBAD | data |
Antares (α Scorpii / Alpha Scorpii) is a red supergiant star in the Milky Way galaxy and the 15th 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 variable star, whose apparent magnitude varies from +0.9 to +1.8.
Properties
Antares is a class M supergiant star, with a diameter of approximately 700 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 parsecs) 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.[2] Its large size and relatively small mass give Antares a very low average density.
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.[2] 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 becomes easy in apertures over 150 mm (5.9 in).[3] The companion is often described as green, but this is probably a contrast effect.[2] 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 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 which lie within 5° of the ecliptic and therefore can be occulted by the Moon and rarely by the planets. On 17 November 2400 Antares will be occulted by Venus[citation needed]. Every year around December 2 the Sun passes 5° north of Antares.
Of the 21 first-magnitude stars, Antares now lies farthest in angular distance from any other first-magnitude star; i.e. it is possible to draw a larger circle centered around Antares without including any other first-magnitude star inside that circle, than around any other first-magnitude star. The nearest first-magnitude star to Antares is Alpha Centauri, lying approximately 39°6.75′ away. The high proper motion of Alpha Centauri is gradually increasing this angle. Before about March 2000, Achernar and Fomalhaut held this distinction of being the most isolated from other first-magnitude stars.[citation needed]
Antares in ancient cultures
Antares' name derives from the Ancient Greek Αντάρης, 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. Its distinctive coloration has made the star an object of interest to many societies throughout history. According to ancient Arab tradition, Antares is the warrior-poet Antar's star[citation needed]. Many of the old Egyptian temples are oriented so that the light of Antares plays a role in the ceremonies performed there. Antares was also known as Satevis in ancient Persia and was one of the four "royal stars" of the Persians around 3000 BC[citation needed]. It was also known as Jyeshtha in ancient India. 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 
.[4]
An old Arabic name was [Ķalb al Άķrab] Error: {{Lang}}: Non-latn text (pos 9)/Latn script subtag mismatch (help), the 'Scorpion's heart'. This had been directly translated to the Ancient Greek Καρδια Σκορπιου Kardia Scorpiou and Latin Cor Scorpii.[4]
See also
External links
- A comparison of the size of Antares to other celestial objects
- Exploring the Full Stellar Population of the upper Scorpius OB Association
- Antares on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
References
- ^ a b c d e f g h i j k l m n o p q "SIMBAD Astronomical Database". Results for CCDM J16294-2626A/B. Retrieved 2006-10-23.
- ^ a b c Kaler, James. "Antares". Retrieved 13 August.
{{cite web}}: Check date values in:|accessdate=(help); Unknown parameter|accessyear=ignored (|access-date=suggested) (help) - ^ Burnham, Robert, Jr. (1978). Burnham's Celestial Handbook. New York: Dover Publications. p. 1666.
{{cite book}}: Cite has empty unknown parameter:|coauthors=(help)CS1 maint: multiple names: authors list (link) - ^ a b Richard Hinckley Allen, Star-names and their meanings (1936), p. 365.