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Vulpecula (Little Fox)

COSMOS / CONSTELLATIONS / VUL

Vulpecula (Little Fox)

The Little Fox. IAU abbreviation Vul. One of the seven constellations introduced by Johannes Hevelius and published in his star atlas of 1690.

STAR CHART

Anser23 Vul31 Vul13 Vul15 Vul1 Vul↑ N ← E
Coloured dots are the stars of Vulpecula 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
Vul
Latin name / genitive
Vulpecula / Vulpeculae
Position
Right ascension ≈ 20 h 06 m; declination +20° to +29°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 74° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 19 September.
Number of stars
71 stars brighter than magnitude 6.5 in the catalogue; 11 brighter than 5 and 0 brighter than 4.

INTERACTIVE LAB

Where is Vulpecula tonight?

The lab opens for Ankara on today’s date. Drag the time slider through the night; the “Best night” button jumps to the date when the constellation is highest at 21:00 (around 19 September). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

Hevelius introduced this faint constellation in 1687 as the “little fox with a goose” (Vulpecula cum Anser); its brightest star is named Anser, the goose. The Dumbbell Nebula (M27) and the first pulsar ever discovered, PSR B1919+21 (1967), are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Anser4.44297M0
23 Vul4.50339K3III
31 Vul4.56189G8III
13 Vul4.57335B9.5III
15 Vul4.66236A4III
1 Vul4.76811B4IV
HIP 998244.79991B3V
29 Vul4.81233A0V

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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