Antares

Location of Antares in Scorpius.

Antares (α Scorpii, Alpha Scorpii) is a red supergiant star in the Milky Way galaxy and the sixteenth brightest star in the nighttime sky. It is listed as 15th or 16th brightest, depending on how the two brighter components of the Capella quadruple star system are counted.

Antares is the brightest and most massive star in the Scorpius-Centaurus Association. The Scorpius-Centaurus Association contains thousands of stars with a mean age of 11 million years.^[1]

Antares has a secondary, or companion star, Antares B. The orbit of the companion star and its properties are not properly known, with an estimated period of 1,200 to 2,562 years.

Antares has a radius of about 600 to 800 times that of the Sun. This gives Antares a diameter between 835 million to 1.114 billion kilometers in size. If Antares was placed in the center of our solar system, its outer surface would lie between the orbits of Mars and Jupiter, in the asteroid belt. Antares is about 550 light-years (or 170 parsecs) from the Earth. Its visual luminosity is about 10,000 times that of the Sun. Because the star radiates much of its energy in the infrared part of the spectrum, the bolometric luminosity is about 65,000 times that of the Sun.^[2] The mass of the star is in the range of 15 to 18 solar masses.

Antares is one of the first red supergiants to be directly imaged.

Antares is the star in the yellow nebula.
Constructed picture of Antares up-close.
Antares compared to Arcturus and the Sun.
Video of flying into Antares

Antares Media

Antares between τ (lower left) and σ Scorpii; Antares appears white in this WISE false-colour infrared image.
Lunar Occultation of Antares (reappearance) was observed on 2006 May 14 from The Blue Mountains, Australia. Antares B reappears first, followed by Antares A 7.53 seconds later.
VLTI reconstructed view of the surface of Antares A
Antares seen from the ground. The very bright star towards the upper left corner of the frame is Antares.

Related pages

References

↑ Pecaut, Mark J. et al 2012. A revised age for Upper Scorpius and the star formation history among the F-type members of the Scorpius-Centaurus OB Association. Astrophysical Journal 746 (2): 154 [1].
↑ Schaaf, Fred 2008. The brightest stars: discovering the Universe through the sky's most brilliant stars. Wiley. p. 218. ISBN 978-0-471-70410-2

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[1] Pecaut, Mark J. et al 2012. A revised age for Upper Scorpius and the star formation history among the F-type members of the Scorpius-Centaurus OB Association. Astrophysical Journal 746 (2): 154 [1].

[2] Schaaf, Fred 2008. The brightest stars: discovering the Universe through the sky's most brilliant stars. Wiley. p. 218. ISBN 978-0-471-70410-2

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