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

Ophiuchus (Serpent Bearer)

COSMOS / CONSTELLATIONS / OPH

Ophiuchus (Serpent Bearer)

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

STAR CHART

RasalhagueSabikζ OphYed PriorCebalraiκ Oph↑ N ← E
Coloured dots are the stars of Ophiuchus 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
Oph
Latin name / genitive
Ophiuchus / Ophiuchi
Position
Right ascension ≈ 17 h 20 m; declination −30° to +14°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 42° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 8 August.
Number of stars
183 stars brighter than magnitude 6.5 in the catalogue; 40 brighter than 5 and 14 brighter than 4.

INTERACTIVE LAB

Where is Ophiuchus 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 8 August). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

The healer Asclepius holding a serpent. The ecliptic passes through it, so the Sun crosses Ophiuchus every year in early December, yet it is not one of the traditional signs of the zodiac. Kepler’s supernova of 1604, Barnard’s Star, one of the Sun’s nearest neighbours, and many globular clusters such as M10 and M12 are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Rasalhague2.0849A5III
Sabik2.4388A2.5Va
ζ Oph2.54366O9.5V
Yed Prior2.73171M1III
Cebalrai2.7682K2III
κ Oph3.1991K2IIIvar
Yed Posterior3.23106G8III
θ Oph3.27436B2IV

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.