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Centaurus (Centaur)

COSMOS / CONSTELLATIONS / CEN

Centaurus (Centaur)

The Centaur. IAU abbreviation Cen. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

Rigil KentaurusHadarTolimanMenkentγ Cenε Cen↑ N ← E
Coloured dots are the stars of Centaurus 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
Cen
Latin name / genitive
Centaurus / Centauri
Position
Right ascension ≈ 13 h 06 m; declination −65° to −31°
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 5 June.
Number of stars
287 stars brighter than magnitude 6.5 in the catalogue; 61 brighter than 5 and 21 brighter than 4.

INTERACTIVE LAB

Where is Centaurus 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 5 June).

MYTH, HISTORY AND OBSERVING

The wise centaur Chiron. It contains Alpha Centauri, the nearest star system to the Sun (about 4.4 light-years), and Omega Centauri, the largest globular cluster. The northern part of the constellation is visible low in the south from Türkiye; Omega Centauri can be picked out very close to the horizon from the southern provinces, but Alpha Centauri never rises.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Rigil Kentaurus-0.014G2V
Hadar0.61392B1III
Toliman1.354K1V
Menkent2.0659K0IIIb
γ Cen2.20130A1IV
ε Cen2.29427B1III
η Cen2.33306B1Vn
ζ Cen2.55382B2.5IV

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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