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Antares

HIP 80763; Alpha Scorpii; 21 Scorpii

Observable Double Star Good (58/100)

Sep: 2.7", Companion: mag 5.4

HIP 80763; Alpha Sco; 21 Sco DoubleStar Scorpius (Sco) Visible
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About Antares

Description

Antares is a red supergiant of spectral type M1.5Iab-Ib at magnitude 0.96 (slightly variable), the brightest star in Scorpius. Located about 550 light-years from Earth, it has a diameter roughly 680 times the Sun's — if placed at the Sun's position, its surface would extend beyond the orbit of Mars. Antares has a blue-white companion (Antares B, magnitude 5.5) orbiting at a projected separation of about 2.5 arcseconds.

Observing Tips

Antares is the fiery red heart of Scorpius, unmistakable during summer evenings. Its deep red-orange color is obvious to the naked eye and is often compared to Mars — hence the name 'rival of Mars.' The companion Antares B is a challenging but rewarding target in a 6-inch or larger telescope at high magnification; it appears greenish by contrast. Best observed June through August.

History

The name Antares means 'rival of Ares' (Mars) in Greek, because its red color and brightness often mimic the planet. It was one of the four Royal Stars of ancient Persia, marking the autumnal equinox around 3000 BC. In many cultures it represents a heart — the heart of the Scorpion in Western astronomy, and the Fire Star in Chinese astronomy.

Fun Facts

Antares is so large that it has been directly imaged by interferometers and radio telescopes, revealing details of its extended atmosphere and convection cells. It is expected to end its life as a supernova within the next million years. Its companion Antares B appears green through a telescope — one of the few stars that genuinely appears green, though this is partly a contrast effect.

Observe

1Physical Properties

Magnitude 0.96
Range 0.75 - 1.21
Period 2180 days
Variable Type Semi-Regular Variable (Supergiant)
Spectral Type M1.5Iab-Ib
Star Color Deep ruby red (B-V 1.83)
Temperature 3497 K
Radius 680.1 R☉
Distance 550 ly

Position & Identifiers

RA 16h 29m 24.4s
Dec -26° 25' 55.0"
Constellation Scorpius (Sco)
HR 6134
HIP 80763
HD 148479
Bayer Alpha
Flamsteed 21 Sco
Variable ID Alp Sco
Double Cat 10074

2How easy to split?

Primary 1.0 mag Companion 5.4 mag Separation 2.7″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard+
150mm Newt. Hard Hard Hard
C8 203mm Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

3Visibility

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Best season Apr – Jun (peak: May)

4Light Curve

5Multiple Star System

Separation 2.7″
Companion Mag 5.4
Position Angle 277°
Star Colors A: Red
Discoverer GNT 1

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 277°

A: 1.0 · B: 5.4 · Sep: 2.7″ · PA: 277° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

Explore

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Size Comparison

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Compare Stars

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Stellar Lifecycle

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Spectral Classification

11

Hertzsprung-Russell Diagram

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Blackbody Spectrum

13

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

14

Stellar Fusion

Discover

15Stellar Notes

ADS 10074A, SRc 0.88 - 1.8V, 1733d. Possibly considerably fainter before 150 A.D.: see HR 5685.
Var. M1Ib, 5.5 B2.5V, 878y, a = 2.90", masses 15.5 and 7.0 solar. Companion is radio source. SKYLAB confirms cool star, | hot companion.
Sco OB2; Sco-Cen stream; in reflection nebula; assoc. Sco R1; dust shell beyond 12 R.
Ultraviolet FeII emission. 5-micrometer observations indicate carbon monoxide.
0.011".
7.5 yrs.
ANTARES; Cor Scorpii; Kalb al Akrab; Vespertilio.
Occultation diam. = 0.041".
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Light Travel Time Machine

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Relativistic Travel

Survey Image

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