Giausar — Star in Draco
HIP 56211; Lambda Draconis; 1 Draconis
About Giausar
Description
Giausar, Lambda Draconis, is an M-type red giant of spectral class M0 III-IIIa Ca1 about 333 light-years away. It shines at magnitude 3.84 and is a semiregular variable with small-amplitude pulsations. Giausar marks the tip of the Dragon's tail, near the Ursa Major border. Its cool surface temperature gives it a strikingly warm amber color.
Observing Tips
Giausar marks the westernmost star of Draco's winding body, near the end of the dragon's tail. In binoculars its deep orange color stands out against the paler stars nearby. Circumpolar from mid-northern latitudes. Best observed March through July.
History
The name Giausar comes from the Arabic "al-jawzahr" or possibly from an older astronomical term for the lunar nodes. The IAU adopted the name in 2017.
Fun Facts
Giausar is one of the cooler M-type giants in the sky — its surface temperature of about 3,950 K is nearly 2,000 K cooler than the Sun's. Semiregular variables like Giausar are ideal for long-term amateur monitoring projects.
Observe
1Physical Properties
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Medium+ | 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
7
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
15Stellar Notes
16
Light Travel Time Machine
17
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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