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
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Easy | Easy |
| 50 mm finder 50mm finder | Easy | Easy | Easy |
| 150 mm telescope 150mm scope | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
Set a location in User Settings to see visibility data.
5Survey Image
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Explore
7
Size Comparison
8
Compare Stars
9
Spectral Classification
10
Hertzsprung-Russell Diagram
11
Stellar Lifecycle
12
Blackbody Spectrum
13
Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
14
Stellar Fusion
Discover
15
Light Travel Time Machine
16
Relativistic Travel
Nearby in the Sky
Other targets within a few degrees — pan your scope a little and keep exploring.
Visibility scores assume a 150 mm Newton at Bortle 4.
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