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Vela (Sails)

COSMOS / CONSTELLATIONS / VEL

Vela (Sails)

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

STAR CHART

γ² VelAlsephinaSuhailMarkebμ VelHIP 46701↑ N ← E
Coloured dots are the stars of Vela 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
Vel
Latin name / genitive
Vela / Velorum
Position
Right ascension ≈ 9 h 21 m; declination −57° to −37°
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
220 stars brighter than magnitude 6.5 in the catalogue; 36 brighter than 5 and 14 brighter than 4.

INTERACTIVE LAB

Where is Vela 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 sails of the ship Argo, created when Lacaille divided Argo Navis. Gamma Velorum is a system containing the brightest Wolf–Rayet star; the Vela supernova remnant and pulsar are here too. From Türkiye only its northern part rises just above the southern horizon.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
γ² Vel1.751,117WC8
Alsephina1.9381A1V
Suhail2.23545K4Ib-II
Markeb2.47572B2IV
μ Vel2.69117G5III
HIP 467013.16239K5III
φ Vel3.521,591B5Ib
HIP 425363.60493B3IV

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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