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Beta Trianguli Australis — Star in Triangulum Australe

Magnitude 2.9m Star Triangulum Australe (TrA) Visible
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About Beta TrA

Description

Beta Trianguli Australis is a yellow-white giant of spectral type F2III at magnitude 2.85 in Triangulum Australe. Located about 40 light-years from Earth, it has a luminosity of roughly 9 times solar. It is one of the nearest F-type giant stars to the Sun.

Observing Tips

Beta TrA is the second brightest vertex of the compact southern triangle. It appears as a warm white star. Triangulum Australe is easy to identify near Alpha and Beta Centauri. Only visible from the southern hemisphere. Best observed April through August.

History

Beta TrA has no traditional proper name. Triangulum Australe is one of the most easily recognized small southern constellations, forming a nearly equilateral triangle south of Norma.

Fun Facts

At only 40 light-years, Beta TrA is remarkably close for a giant star — most giants visible to the naked eye are hundreds of light-years away. Its proximity makes it an excellent target for detailed studies of evolved stellar atmospheres.

Observe

1Physical Properties

Magnitude 2.85
Spectral Type F1V
Star Color Yellow-white (B-V 0.29)
Distance 39 ly

2Position & Identifiers

RA 15h 55m 08.5s
Dec -63° 25' 50.0"
HR 5897
HIP 77952
HD 141891
SAO 253346
Bayer Beta

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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