Sadalbari — Star in Pegasus
HIP 112748; Mu Pegasi; 48 Pegasi
About Sadalbari
Description
Sadalbari, Mu Pegasi, is a K-type giant of spectral class K1 III about 106 light-years away. It shines at magnitude 3.48 and is a mature red-clump star in the core helium-fusing phase. Sadalbari has a mass of about 1.7 Suns and a radius of 13 Suns.
Observing Tips
Sadalbari lies in the central area of Pegasus, slightly east of Matar and south of Scheat. In binoculars it is an unmistakable warm yellow-orange point. Best observed August through December.
History
The name comes from the Arabic "al-sa'd al-bārī'," meaning "the luck of the excelling one" — a pre-Islamic astronomical label marking a "lucky" weather star. Several Arabic names of Pegasus and Aquarius begin with "Sadal-" (luck of the ...), reflecting this cultural theme.
Fun Facts
Sadalbari is part of a long line of pre-Islamic "luck" stars, including Sadalsuud (Beta Aquarii), Sadalmelik (Alpha Aquarii), and Sadachbia (Gamma Aquarii) — all stars whose heliacal rising marked specific seasonal-weather phenomena in ancient Arabian folklore.
Observe
1Physical Properties
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Easy | Medium+ |
| 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
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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
Discover
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Light Travel Time Machine
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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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