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Gamma Orionis (γ Ori)

Bellatrix star

Bellatrix is Orion's blue-white western shoulder, positioned opposite the visibly warmer Betelgeuse. It is an evolved massive star with a relatively uncluttered naked-eye identity, making its strongest story the contrast between stellar temperature, colour and short high-mass lifetimes.

Astronomical data and identity checked against cited catalogue and agency sources. Updated September 2026.

Apparent magnitude1.64
Distanceabout 250 light-years
Spectral typeB2 III
ConstellationOrion
Right ascension05h 25m 07.86s
Declination+06° 20′ 58.9″
Real survey imagery

Bellatrix at three sky scales

Each view is centred on the same catalogue coordinates. Moving from wide context to close field helps distinguish the star from its surrounding Milky Way neighbourhood.

What kind of star is Bellatrix?

Bellatrix, catalogued as Gamma Orionis (γ Ori), appears in the official constellation Orion. Its apparent visual magnitude is 1.64, while its estimated distance is about 250 light-years. Astronomers classify the object as B2 III. These labels describe temperature, luminosity class or system components; they should not be read as a claim that every naked-eye point is a single isolated star.

Gamma Orionis is a hot B-type giant whose surface temperature is several times the Sun's and whose luminosity is thousands of times greater. It has left or is leaving the main sequence after consuming core hydrogen far faster than a solar-mass star. Broad-band measurements once treated Bellatrix as exceptionally stable, but precise photometry has reported low-level variability; the amplitude and classification should not be exaggerated into an obvious naked-eye change. Published masses, ages and distances differ with stellar models and astrometric inputs, so rounded values are more honest than false precision. Unlike nearby-looking Betelgeuse, Bellatrix has not expanded into a cool red supergiant, and their sharp colour contrast reflects genuinely different surface temperatures and evolutionary states.

The coordinate pair RA 05h 25m 07.86s, Dec +06° 20′ 58.9″ fixes the object's direction on the celestial sphere for the J2000 reference epoch. Right ascension works like celestial longitude measured in hours, while declination works like latitude north or south of the celestial equator. Proper motion and improved measurements can refine catalogue positions, but these coordinates are sufficiently precise for a finder chart or planetarium search.

Bellatrix data at a glance

Key catalogue and observing data for Bellatrix
Proper nameBellatrixCatalogue designationGamma Orionis (γ Ori)
ConstellationOrionApparent magnitude1.64
Spectral or system typeB2 IIIEstimated distanceabout 250 light-years
Right ascension (J2000)05h 25m 07.86sDeclination (J2000)+06° 20′ 58.9″

Values are rounded for an observer-friendly overview. Consult the linked SIMBAD record for component-level identifiers, bibliography, measurement provenance and newer catalogue values.

The name Bellatrix

Latin for “female warrior.” The historical name is now standardized by the IAU.

The Latin name Bellatrix means a female warrior and appeared in medieval astronomical tradition, while an older Arabic anatomical name linked the star with Orion's shoulder. Bayer labelled it Gamma Orionis in 1603. Its title later inspired the widespread “Amazon Star” interpretation and entered literature beyond astronomy. Bellatrix also served in systems of photometric standards, but improving detectors showed that even apparently steady bright stars deserve repeated measurement rather than permanent assumptions of constancy.

Modern professional catalogues retain identifiers such as the Bayer designation alongside a proper name. The International Astronomical Union standardizes which name belongs to which component—an important distinction for systems whose combined light looks like one star from Earth.

How to find Bellatrix

Bellatrix is Orion’s western shoulder, opposite red Betelgeuse. Compare the two directly; slightly defocused binoculars make their strong colour difference easier to see.

Visible worldwide outside extreme polar regions; best during northern winter and southern summer. Visibility on a particular night still depends on latitude, season, time, horizon obstructions, weather and local light pollution. Use the interactive atlas below to check the surrounding field before observing.

Observation checklist

  • Find Bellatrix at the shoulder opposite Betelgeuse above Orion's Belt.
  • Compare the two shoulders directly to see blue-white versus orange-red starlight.
  • Observe Orion near culmination on winter evenings for the steadiest image.
  • Do not expect Bellatrix's reported low-amplitude variability to be obvious by eye.

Interesting facts about Bellatrix

  • Bellatrix is a hot blue-white giant and strongly contrasts with red Betelgeuse.
  • It frames the top of Orion’s familiar hourglass figure.
  • The star was once used as a photometric standard before subtle variability was recognized.
  • Its traditional title inspired the popular description “Amazon Star.”
  • Orion’s equatorial position makes Bellatrix accessible from both hemispheres.
Create your own connection to the night sky

Name your own star

Bellatrix already has an established astronomical name and cannot be renamed. You can create a separate symbolic star registration, receive its unique sky coordinates and certificate, then use our guides to explore the real night sky around it.

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

Continue from Bellatrix into the night sky

Use the Orion constellation guide to place this star within its larger pattern. When you are ready to observe, compare dark-sky places, find a nearby observatory, or follow our practical guide to finding a star in the night sky. Symbolically registered names are kept separately in the searchable Star-Register catalogue.

Sources and further reading

Measurements are rounded for readability. Multiple systems, variable stars and distant supergiants can have component-specific or model-dependent values. Survey panels show photographic sky fields, not the physical surface of the star.

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