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Indus (Indian)

COSMOS / CONSTELLATIONS / IND

Indus (Indian)

The Indian. IAU abbreviation Ind. 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

α Indβ Indθ Indδ Indη Indε Ind↑ N ← E
Coloured dots are the stars of Indus 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
Ind
Latin name / genitive
Indus / Indi
Position
Right ascension ≈ 21 h 48 m; declination −74° to −45°
Visibility from Türkiye
From Türkiye only its northern part is seen, low on the southern horizon; the southern provinces are better placed.
Best time to observe
Best placed at 21:00 Türkiye time around 15 October.
Number of stars
45 stars brighter than magnitude 6.5 in the catalogue; 7 brighter than 5 and 2 brighter than 4.

INTERACTIVE LAB

Where is Indus tonight?

Only the northern part of this constellation is seen from Türkiye, low on the southern horizon. The lab opens for Ankara on today’s date; switch the city to Antalya and then to Sydney and watch how the “Visible part” row and the chart change. The “Best night” button jumps to the best date (around 15 October).

MYTH, HISTORY AND OBSERVING

A constellation representing an indigenous person, from the observations of Keyser and de Houtman. Epsilon Indi, 11.9 light-years away, has a pair of brown dwarfs and a giant planet. From Türkiye only its northern edge rises just above the horizon.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
α Ind3.1198K0III
β Ind3.67612K0III
θ Ind4.3999A5V
δ Ind4.40188F0IV
η Ind4.5179A6:var
ε Ind4.6912K5V
ζ Ind4.90413K5III
ι Ind5.06467K1II/III

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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