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IAU abbreviation · Sge

Sagitta constellation

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

IAU 88Ptolemaic heritage
Official nameSagitta
AbbreviationSge
Genitive formSagittae
Sky regionCelestial equator
Best evening seasonSummer evenings
Reference centreRA -4.6h · Dec +18°

the arrow · pronounced suh-JIT-uh. Sagitta is an official IAU constellation representing the arrow. It occupies the summer Milky Way between Aquila and Vulpecula, where its outline is best understood as a guide to a formally bounded region rather than a physical group of nearby stars. Gamma Sagittae and Delta Sagittae provide practical anchors, while M71 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.

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

About Sagitta

Sagitta is one of the 88 constellations recognized by the International Astronomical Union. Its standard three-letter abbreviation is Sge, and astronomers use the genitive form Sagittae when naming stars associated with it. The constellation's reference position lies around right ascension -4.6 hours and declination +18 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 summer evenings. Exact visibility depends on latitude, local horizon, date and time.

History and mythology of Sagitta

Origin and naming

Sagitta entered the Western constellation record through Ptolemy,2nd century. Its name means the arrow; 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 the summer Milky Way between Aquila and Vulpecula into smaller asterisms, lunar stations or navigational patterns, so apparent overlap is cross-referenced rather than treated as an identical constellation.

How to find Sagitta

  1. Choose an evening when the summer Milky Way between Aquila and Vulpecula is well placed and use a planisphere or sky app set to your location and time.
  2. Begin with the brightest anchor, Gamma Sagittae, then verify the surrounding angles rather than relying on the artwork alone.
  3. Trace toward Delta Sagittae; binoculars help separate the genuine stars from background Milky Way fields or light pollution.
  4. After confirming the pattern, centre M71. Start at low magnification and increase power only after the target is securely located.

Bright stars in Sagitta

Gamma Sagittae

Notable star
Magnitude
3.5
Distance
274 ly

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

Delta Sagittae

Notable star
Magnitude
3.8
Distance
448 ly

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

Alpha Sagittae

Notable star
Magnitude
4.4
Distance
382 ly

Alpha Sagittae 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 Sagitta

globular cluster

M71

M71 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

Sh2-84

Sh2-84 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.

cataclysmic variable

WZ Sagittae

WZ Sagittae 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 Sagitta

  • Sagitta's name means the arrow. Sagitta entered the Western constellation record through Ptolemy,2nd century.
  • Gamma Sagittae is listed at magnitude 3.5. Gamma Sagittae is a characteristic stellar landmark used when tracing this constellation; its brightness, colour or multiplicity rewards comparison in binoculars or a telescope.
  • M71 is a globular cluster. M71 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 Sagitta

Create a symbolic star registration with a certificate and sky coordinates, then use this guide to explore the surrounding sky. Select Sagitta 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 Sagitta

Sources and further reading

Continue across the sky

Constellations near Sagitta

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