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Triangulum Australe (Southern Triangle)

COSMOS / CONSTELLATIONS / TRA

Triangulum Australe (Southern Triangle)

The Southern Triangle. IAU abbreviation TrA. One of the 12 southern constellations based on the observations of the Dutch navigators Pieter Dirkszoon Keyser and Frederick de Houtman on their 1595–1597 voyage and spread by the globes of Petrus Plancius.

STAR CHART

Atriaβ TrAγ TrAδ TrAε TrAζ TrA↑ N ← E
Coloured dots are the stars of Triangulum Australe brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
TrA
Latin name / genitive
Triangulum Australe / Trianguli Australis
Position
Right ascension ≈ 16 h 08 m; declination −70° to −60°
Visibility from Türkiye
Not visible from Türkiye; it is observed from the southern hemisphere.
Best time to observe
From the southern hemisphere it is best placed around 21:00 in early July.
Number of stars
35 stars brighter than magnitude 6.5 in the catalogue; 6 brighter than 5 and 4 brighter than 4.

INTERACTIVE LAB

Where is Triangulum Australe tonight?

This constellation cannot be seen from Türkiye, so the lab opens for Sydney. Drag the time slider through the southern night, use the “Best night” button to jump to the best date, and switch the city to Ankara to see why it never rises there.

MYTH, HISTORY AND OBSERVING

A distinctive southern constellation of three bright stars, mapped from the observations of Keyser and de Houtman. Its brightest star, Atria, is an orange giant. It is not visible from Türkiye.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Atria1.91391K2IIb-IIIa
β TrA2.8340F2III
γ TrA2.87184A1V
δ TrA3.86607G5II
ε TrA4.11202K0III
ζ TrA4.9040F9V
HIP 821295.10697Ap
κ TrA5.111,208G6VII

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

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