Gamma Trianguli Australis — Star in Triangulum Australe
About Gamma TrA
Description
Gamma Trianguli Australis is a white main-sequence star of spectral type A1V at magnitude 2.89 in Triangulum Australe. Located about 183 light-years from Earth, it has a luminosity of roughly 55 times solar. It is the faintest of the three main stars forming the small equilateral triangle.
Observing Tips
Gamma TrA completes the compact triangle of Triangulum Australe, with Atria (Alpha) and Beta TrA. It is a white star easy to spot near Alpha and Beta Centauri. Only visible from the southern hemisphere. Best observed April through August.
History
Gamma TrA has no traditional proper name. Triangulum Australe is one of the most easily recognized small southern constellations due to its compact, regular shape.
Fun Facts
The three stars of Triangulum Australe span a wide range of types — a cool orange giant (Alpha), a warm F-type giant (Beta), and a hot A-type star (Gamma) — making the triangle a showcase of different stellar evolutionary stages in one compact group.
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
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5Survey Image
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Explore
7
Size Comparison
8
Compare Stars
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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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