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Iota Scorpii — Star in Scorpius

HIP 87073; Iota1 Scorpii

Magnitude 3.0m Star Scorpius (Sco) Visible
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About Iota Sco

Description

Iota Scorpii is an F-type yellow supergiant of spectral class F2 Ia about 1,900 light-years away, one of the intrinsically brightest stars in the tail region of Scorpius. It shines at magnitude 3.03 and has a luminosity of roughly 25,000 Suns. The primary is paired with a faint companion at about 37 arcseconds — likely an optical double rather than a physical system.

Observing Tips

Iota Sco sits in the stinger region of Scorpius, close to Shaula (Lambda Sco) and Mu Sco. Binoculars show a rich star field packed with the young members of the Upper Sco OB association. Best observed from the southern hemisphere or mid-southern latitudes, May through September.

History

Iota Sco has no widely-used traditional name. The star retains its Bayer designation in current catalogs.

Fun Facts

Iota Sco is an F-type supergiant — the rarer "warm" cousin of the more familiar red supergiants. The star is in a brief evolutionary phase as it transitions from being a blue-giant to a red-giant; its total lifetime in this state is just a few hundred thousand years.

Observe

1Physical Properties

Magnitude 3.03
Spectral Type F2Ia supergiant
Star Color Yellow (B-V 0.51)
Distance 1,912 ly

2Position & Identifiers

RA 17h 47m 35.1s
Dec -40° 07' 37.0"
Constellation Scorpius (Sco)
HR 6615
HIP 87073
HD 161471
SAO 228420
Bayer Iota1

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 May – Jul (peak: Jun)

5Survey Image

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Size Comparison

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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

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Stellar Fusion

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Relativistic Travel

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