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See HR 6084 — Star in Scorpius

HIP 81266; Tau Scorpii; 23 Scorpii

Magnitude 2.8m Star Scorpius (Sco) Visible
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About See HR 6084

Description

Tau Scorpii is a blue main-sequence star of spectral type B0.2V at magnitude 2.82 in Scorpius, located about 470 light-years from Earth. It has a surface temperature of roughly 31,000 K and a luminosity of about 18,000 times solar. Tau Sco is remarkable for possessing an unusually strong and complex magnetic field for a B-type star — far stronger than expected for its spectral type.

Observing Tips

Tau Sco is located near the head of Scorpius, close to the brighter Antares. It appears as a blue-white star in a region rich with other luminous Scorpius members. Best observed from June through August when Scorpius is prominent in the southern evening sky. Compare its blue color with the red of Antares just a few degrees away.

History

Tau Scorpii has no widely used proper name. Its unusual magnetic properties were discovered in the early 2000s through spectropolarimetric observations. The star is a member of the Upper Scorpius subgroup of the Scorpius-Centaurus OB association, one of the nearest OB associations to the Sun.

Fun Facts

Tau Sco's magnetic field is a mystery — it is far too complex and strong for a normal B-type star. One theory suggests it may be the product of a stellar merger, where two less massive stars collided and combined, generating the unusual magnetic topology in the process.

Observe

1Physical Properties

Magnitude 2.82
Spectral Type B0IV subgiant
Star Color Blue (B-V -0.25)
Distance 447 ly

2Position & Identifiers

RA 16h 35m 53.0s
Dec -28° 12' 58.0"
Constellation Scorpius (Sco)
HR 6165
HIP 81266
HD 149438
SAO 184481
Bayer Tau
Flamsteed 23 Sco

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Apr – Jun (peak: May)

5Survey Image

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Explore

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Size Comparison

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Compare Stars

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

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

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Stellar Fusion

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15Stellar Notes

Color excess E(B-V) = +0.06.
Sco OB2; Sco-Cen cluster; Sco-Cen assoc.; upper Sco region. Faint HII region surrounds star. Member of Pleiades group.
Spectra indicate high velocity stellar wind. Lyman beta observed from COPERNICUS. High resolution UV spectrum | obtained from COPERNICUS. Large amount of atomic hydrogen, but only small amount of molecular hydrogen in line of sight.
See HR 6084.
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Light Travel Time Machine

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Relativistic Travel

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