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IAU abbreviation · Ser

Serpens constellation

A visual guide to Serpens: its position in the celestial sphere, best observing season, historical classifications and nearby regions of sky.

IAU 88Ptolemaic heritage
Official nameSerpens
AbbreviationSer
Genitive formSerpentis
Sky regionCelestial equator
Best evening seasonSpring evenings
Reference centreRA -8.5h · Dec +5°

the serpent · pronounced SUR-penz. Serpens is an official IAU constellation representing the serpent. It occupies two separated regions held by Ophiuchus, where its outline is best understood as a guide to a formally bounded region rather than a physical group of nearby stars. Unukalhai and Eta Serpentis provide practical anchors, while M5 gives observers a destination beyond the line figure. The stars only appear together from Earth: they lie at very different distances and move independently through the Galaxy. Its classical identity has survived repeated reinterpretation, but the modern boundary is an astronomical convention, not the outline used by every historical culture. Naked-eye recognition depends on latitude, season, darkness and moonlight. This guide therefore separates the official sky area, the traditional picture and the objects that can actually be observed.

Serpens official constellation chart
Serpens chart by International Astronomical Union and Sky & Telescope. CC BY 3.0. Source and licence ↗

About Serpens

Serpens is one of the 88 constellations recognized by the International Astronomical Union. Its standard three-letter abbreviation is Ser, and astronomers use the genitive form Serpentis when naming stars associated with it. The constellation's reference position lies around right ascension -8.5 hours and declination +5 degrees.

Its location places it in the celestial equator. For a typical mid-latitude observer, this part of the celestial sphere is especially well placed during spring evenings. Exact visibility depends on latitude, local horizon, date and time.

History and mythology of Serpens

Origin and naming

Serpens entered the Western constellation record through Ptolemy,2nd century. Its name means the serpent; historical artwork varies and should not be confused with the IAU boundary adopted for positional astronomy.

From figure to official sky region

The IAU standardised constellation names in 1922, and Eugène Delporte published the modern boundaries in 1930. Every coordinate inside that polygon belongs to this constellation, including stars and galaxies unrelated to its traditional stick figure.

Cultural context

The familiar Western figure is one layer of sky history. Star traditions from other cultures may divide two separated regions held by Ophiuchus into smaller asterisms, lunar stations or navigational patterns, so apparent overlap is cross-referenced rather than treated as an identical constellation.

How to find Serpens

  1. Choose an evening when two separated regions held by Ophiuchus is well placed and use a planisphere or sky app set to your location and time.
  2. Begin with the brightest anchor, Unukalhai, then verify the surrounding angles rather than relying on the artwork alone.
  3. Trace toward Eta Serpentis; binoculars help separate the genuine stars from background Milky Way fields or light pollution.
  4. After confirming the pattern, centre M5. Start at low magnification and increase power only after the target is securely located.

Bright stars in Serpens

Unukalhai

Notable star
Magnitude
2.6
Distance
74 ly

Unukalhai is a characteristic stellar landmark used when tracing this constellation; its brightness, colour or multiplicity rewards comparison in binoculars or a telescope.

Eta Serpentis

Notable star
Magnitude
3.3
Distance
61 ly

Eta Serpentis is a characteristic stellar landmark used when tracing this constellation; its brightness, colour or multiplicity rewards comparison in binoculars or a telescope.

Mu Serpentis

Notable star
Magnitude
3.5
Distance
156 ly

Mu Serpentis is a characteristic stellar landmark used when tracing this constellation; its brightness, colour or multiplicity rewards comparison in binoculars or a telescope.

Deep-sky objects in Serpens

globular cluster

M5

M5 is one of the most useful observing or imaging targets in this field. Its apparent size and surface brightness make dark skies and an appropriate field of view important.

emission nebula

M16 Eagle Nebula

M16 Eagle Nebula is one of the most useful observing or imaging targets in this field. Its apparent size and surface brightness make dark skies and an appropriate field of view important.

galaxy group

Seyfert’s Sextet

Seyfert’s Sextet is one of the most useful observing or imaging targets in this field. Its apparent size and surface brightness make dark skies and an appropriate field of view important.

Interesting facts about Serpens

  • Serpens's name means the serpent. Serpens entered the Western constellation record through Ptolemy,2nd century.
  • Unukalhai is listed at magnitude 2.6. Unukalhai is a characteristic stellar landmark used when tracing this constellation; its brightness, colour or multiplicity rewards comparison in binoculars or a telescope.
  • M5 is a globular cluster. M5 is one of the most useful observing or imaging targets in this field.
  • The IAU standardised constellation names in 1922, and Eugène Delporte published the modern boundaries in 1930.
A personal connection to the night sky

Name a star in Serpens

Create a symbolic star registration with a certificate and sky coordinates, then use this guide to explore the surrounding sky. Select Serpens when that constellation is available during checkout.

Star naming is a symbolic gift service. It does not change scientific names or designations maintained by the IAU.

Astronomy databases for Serpens

Sources and further reading

Continue across the sky

Constellations near Serpens

These are the closest directory reference centres, useful for exploration. They are not a formal boundary-adjacency list.