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Volans (Flying Fish)

COSMOS / CONSTELLATIONS / VOL

Volans (Flying Fish)

The Flying Fish. IAU abbreviation Vol. 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

β Volγ² Volζ Volδ Volα Volε Vol↑ N ← E
Coloured dots are the stars of Volans 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
Vol
Latin name / genitive
Volans / Volantis
Position
Right ascension ≈ 7 h 56 m; declination −74° to −65°
Visibility from Türkiye
Not visible from Türkiye; it is observed from the southern hemisphere.
Best time to observe
From the southern hemisphere it is best placed around 21:00 in early March.
Number of stars
34 stars brighter than magnitude 6.5 in the catalogue; 6 brighter than 5 and 5 brighter than 4.

INTERACTIVE LAB

Where is Volans tonight?

This constellation cannot be seen from Türkiye, so the lab opens for Sydney. Drag the time slider through the southern night, use the “Best night” button to jump to the best date, and switch the city to Ankara to see why it never rises there.

MYTH, HISTORY AND OBSERVING

The flying fish from the observations of Keyser and de Houtman, a small constellation south of Carina. Gamma Volantis is a colourful double star for a small telescope. It is not visible from Türkiye.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
β Vol3.77108K2IIIvar
γ² Vol3.78140G8IIIvar
ζ Vol3.93141K0III
δ Vol3.97738F6II
α Vol4.00125Am
ε Vol4.35562B6IV
HIP 406805.06297K1III
HIP 336825.18292K3III

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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