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Alpha Canis Minoris (α CMi)

Procyon star

A researched guide to Procyon: where to find it, what kind of star it is, why it matters and how it fits into Canis Minor.

Apparent magnitude0.34
Distance11.46 light-years
Spectral typeF5 IV–V + DQZ white dwarf
ConstellationCanis Minor
Right ascension07h 39m 18.12s
Declination+05° 13′ 30.0″
Digitized Sky Survey field centred on Procyon
Real sky field centred on Procyon at RA 07h 39m 18.12s, Dec +05° 13′ 30.0″. Digitized Sky Survey imagery served through CDS.

What kind of star is Procyon?

Procyon, catalogued as Alpha Canis Minoris (α CMi), appears in the official constellation Canis Minor. Its apparent visual magnitude is 0.34, while its estimated distance is 11.46 light-years. Astronomers classify the object as F5 IV–V + DQZ white dwarf. 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.

The coordinate pair RA 07h 39m 18.12s, Dec +05° 13′ 30.0″ 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.

The name Procyon

Greek Prokyōn means “before the dog,” because it rises before Sirius, the Dog Star, from many northern latitudes.

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 Procyon

Use Betelgeuse and Sirius to complete the nearly equilateral Winter Triangle; Procyon is its northeastern vertex for northern observers. It remains visible through moderate urban light pollution.

Visible from nearly the entire inhabited world; best on northern winter and southern summer evenings. 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.

Interesting facts about Procyon

  • Procyon is a nearby binary with a bright late-main-sequence/subgiant star and a faint white dwarf.
  • Astrometric irregularities predicted Procyon B before it was visually observed.
  • The pair orbit one another in roughly 41 years.
  • Procyon forms the Winter Triangle with Sirius and Betelgeuse.
  • Procyon and Gomeisa dominate the exceptionally simple familiar outline of Canis Minor.
Observation recording Procyon A and its faint white-dwarf companion.
Observation recording Procyon A and its faint white-dwarf companion. Credit: Giuseppe Donatiello. CC0 1.0. Image source and licence ↗
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Name a star in Canis Minor

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

Sources and further reading

Measurements are rounded for readability. Multiple systems, variable stars and distant supergiants can have component-specific or model-dependent values.

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