SpaceTRCSpaceTRC/Research platform
TürkçeLet’s collaborate
SpaceTRC / Cosmos / Constellations

Aquarius (Water Bearer)

COSMOS / CONSTELLATIONS / AQR

Aquarius (Water Bearer)

The Water Bearer. IAU abbreviation Aqr. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

SadalsuudSadalmelikSkatζ¹ Aqr88 Aqrλ Aqr↑ N ← E
Coloured dots are the stars of Aquarius 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
Aqr
Latin name / genitive
Aquarius / Aquarii
Position
Right ascension ≈ 22 h 27 m; declination −25° to +2°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 39° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 25 October.
Number of stars
179 stars brighter than magnitude 6.5 in the catalogue; 33 brighter than 5 and 9 brighter than 4.

INTERACTIVE LAB

Where is Aquarius 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 25 October). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

Depicted as a figure pouring water from a jar, this zodiac constellation goes back to Babylonian star lore. It contains the Helix Nebula (NGC 7293), one of the nearest planetary nebulae, and the bright globular cluster M2. The radiant of the early-May Eta Aquariid meteor shower also lies here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Sadalsuud2.90537G0Ib
Sadalmelik2.95524G2Ib
Skat3.27161A3V
ζ¹ Aqr3.6592F3III-IV
88 Aqr3.68271K1III
λ Aqr3.73385M2IIIvar
Albali3.78208A1V
Sadachbia3.86164A0V

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.

SPACETRC / KNOWLEDGE

Follow your curiosity.

SPACETRC / GET STARTED

What would you like to do?

This short guide is available in six languages. Full scientific articles are in Turkish and English.

Open a workspace

Search publicationsExamine dataSpace eventsPlan a team projectPrepare a publication

Take selected reading with you

Open Turkish and English dossiers and introductory lessons in the reading area. Offline preparation and installation options are available there.

Open the offline library ↗

The language preference stays in this browser; no account or location permission is required.