Antares

From WikiMD's Wellness Encyclopedia

Infrared Rho Ophiuchi Complex.jpg
Antares near the Sun every year around 2 December.jpg

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VLTI reconstructed view of the surface of Antares.jpg
Star-sizes.jpg

Antares is a red supergiant star located in the constellation of Scorpius. It is one of the largest and most luminous stars known, and it is often referred to as the "heart of the scorpion" due to its prominent position in the constellation. Antares is classified as a type M1.5Iab star, indicating its status as a red supergiant.

Characteristics[edit | edit source]

Antares is approximately 550 light-years away from Earth. It has a radius about 680 times that of the Sun, making it one of the largest known stars. The star's surface temperature is around 3,500 K, which gives it a distinct reddish appearance. Antares is also a variable star, meaning its brightness changes over time.

Companion Star[edit | edit source]

Antares has a faint companion star, Antares B, which is a main-sequence star of spectral type B2.5V. This companion is much hotter and smaller than Antares itself. The two stars form a binary star system, with Antares B orbiting the primary star at a distance of about 529 AU.

Mythology and Cultural Significance[edit | edit source]

In ancient Greek mythology, Antares was associated with the god Ares, the god of war, due to its reddish color, which resembles the planet Mars. The name "Antares" means "rival of Ares" or "like Ares" (Mars). In various cultures, Antares has been an important star for navigation and timekeeping.

Observational History[edit | edit source]

Antares has been observed since antiquity and has been an important star in various astronomical catalogues. It was first catalogued by the Greek astronomer Hipparchus in the 2nd century BCE. Modern observations have provided detailed information about its size, temperature, and variability.

Future Evolution[edit | edit source]

As a red supergiant, Antares is in the late stages of its stellar evolution. It is expected to end its life in a supernova explosion, which will leave behind a neutron star or black hole. This event is predicted to occur within the next few million years.

See Also[edit | edit source]

References[edit | edit source]

External Links[edit | edit source]

Contributors: Prab R. Tumpati, MD