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Serpens (Serpent)

COSMOS / CONSTELLATIONS / SER

Serpens (Serpent)

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

STAR CHART

Unukalhaiη Serξ Serμ Serβ Serε Ser↑ N ← E
Coloured dots are the stars of Serpens 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
Ser
Latin name / genitive
Serpens / Serpentis
Position
Right ascension ≈ 16 h 39 m; declination −16° to +25°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 55° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 29 July.
Number of stars
115 stars brighter than magnitude 6.5 in the catalogue; 19 brighter than 5 and 8 brighter than 4.

INTERACTIVE LAB

Where is Serpens 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 29 July). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

The snake held by Ophiuchus; it is the only constellation split into two separate parts, the Head (Serpens Caput) and the Tail (Serpens Cauda). The Eagle Nebula (M16), famous for Hubble’s “Pillars of Creation” image, and the bright globular cluster M5 are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Unukalhai2.6374K2III
η Ser3.2360K0III-IV
μ Ser3.54170A0V
ξ Ser3.54105F0IIIp
β Ser3.65155A3V
ε Ser3.7170A2m
δ Ser3.80228F0IV
γ Ser3.8537F6V

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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