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Orion (Hunter)

COSMOS / CONSTELLATIONS / ORI

Orion (Hunter)

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

STAR CHART

RigelBetelgeuseBellatrixAlnilamAlnitakSaiph↑ N ← E
Coloured dots are the stars of Orion 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
Ori
Latin name / genitive
Orion / Orionis
Position
Right ascension ≈ 5 h 35 m; declination −11° to +20°
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 10 February.
Number of stars
204 stars brighter than magnitude 6.5 in the catalogue; 50 brighter than 5 and 15 brighter than 4.

INTERACTIVE LAB

Where is Orion 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 10 February). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

Orion, the giant hunter of myth and one of the best-known constellations. The red supergiant Betelgeuse dimmed noticeably in 2019–2020; the blue supergiant Rigel and the three stars of the Belt stand out at a glance. In the sword below the Belt, the Orion Nebula (M42), about 1,350 light-years away, is visible to the naked eye.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Rigel0.18863B8Ia
Betelgeuse0.45498M2Ib
Bellatrix1.64252B2III
Alnilam1.691,977B0Ia
Alnitak1.74736O9.5Ib
Saiph2.07647B0.5Iavar
Mintaka2.25692O9.5II
Hatysa2.752,330O9III

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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