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Gamma Trianguli Australis — Star in Triangulum Australe

Magnitude 2.9m Star Triangulum Australe (TrA) Visible
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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

Magnitude 2.89
Spectral Type A2Vn
Star Color White (B-V 0.00)
Distance 184 ly

2Position & Identifiers

RA 15h 18m 54.6s
Dec -68° 40' 46.0"
HR 5671
HIP 74946
HD 135382
SAO 253097
Bayer Gamma

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 Apr – Jun (peak: May)

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

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

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Stellar Fusion

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Light Travel Time Machine

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Relativistic Travel

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