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Grus (Crane)

COSMOS / CONSTELLATIONS / GRU

Grus (Crane)

The Crane. IAU abbreviation Gru. 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

AlnairTiakiAldhanabε Gruι Gruδ¹ Gru↑ N ← E
Coloured dots are the stars of Grus 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
Gru
Latin name / genitive
Grus / Gruis
Position
Right ascension ≈ 22 h 39 m; declination −54° to −36°
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 28 October.
Number of stars
58 stars brighter than magnitude 6.5 in the catalogue; 13 brighter than 5 and 6 brighter than 4.

INTERACTIVE LAB

Where is Grus 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 28 October).

MYTH, HISTORY AND OBSERVING

A crane that entered star maps through the observations of Keyser and de Houtman. It lies south of Piscis Austrinus; from Türkiye only its northern part peeks above the southern horizon on autumn evenings.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Alnair1.73101B7IV
Tiaki2.07177M5III
Aldhanab3.00211B8III
ε Gru3.49129A3V
ι Gru3.88183K0III
δ¹ Gru3.97309G6/G8III
ζ Gru4.11109G8III
δ² Gru4.12330M4.5IIIa

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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