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Carina (Keel)

COSMOS / CONSTELLATIONS / CAR

Carina (Keel)

The Keel. IAU abbreviation Car. One of the three parts into which Lacaille divided Ptolemy’s huge constellation Argo Navis in 1756.

STAR CHART

CanopusMiaplacidusAviorAspidiskeθ Carυ Car↑ N ← E
Coloured dots are the stars of Carina 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
Car
Latin name / genitive
Carina / Carinae
Position
Right ascension ≈ 9 h 24 m; declination −75° to −51°
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 9 April.
Number of stars
227 stars brighter than magnitude 6.5 in the catalogue; 45 brighter than 5 and 18 brighter than 4.

INTERACTIVE LAB

Where is Carina 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 9 April).

MYTH, HISTORY AND OBSERVING

The keel of the Argonauts’ ship Argo; in 1756 Lacaille split Ptolemy’s huge constellation Argo Navis into three. Canopus, the second-brightest star in the sky, can be glimpsed from Türkiye only from the southernmost coasts, just above the horizon and only briefly. The vast Carina Nebula and the unstable supergiant Eta Carinae are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Canopus-0.62309F0Ib
Miaplacidus1.67113A2IV
Avior1.86605K3III+B2V
Aspidiske2.21766A8Ib
θ Car2.74456B0Vp
υ Car2.921,437A9
ω Car3.29342B8III
HIP 515763.30483B4Vne

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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