Bright & Nearby Stars · Constellation Carina

Canopus (Alpha Carinae)

Coordinates, Hipparcos distance (310 ly), magnitude −0.74, 71 R☉ yellow-white supergiant radius, and observing guide for Canopus in Carina.

Right Ascension (J2000.0)06h 23m 57.11s
Declination (J2000.0)-52° 41′ 44.4″
Primary ClassificationYellow-white F-type bright giant / supergiant star
Best Observing SeasonWinter / Southern Summer (December–March)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for Canopus (Alpha Carinae)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Apparent visual magnitude (V)-0.74 mag± 0.01 magJohnson UBV photoelectric photometrydefinitiveHipparcos New Reduction Catalog
Trigonometric parallax10.55 mas± 0.56 masHipparcos New Reduction astrometric solution (94.8 ± 5.0 pc) (J2000.0)definitiveHipparcos New Reduction Catalog
Distance in light-years309.2 ly± 16.4 lyDerived from Hipparcos parallax 10.55 ± 0.56 mashigh-confidenceHipparcos New Reduction Catalog
Photospheric linear radius71.4 R☉± 4 R☉VLTI/AMBER limb-darkened angular diameter (6.93 ± 0.15 mas) at 94.8 pchigh-confidenceSIMBAD Astronomical Database (CDS)
Bolometric luminosity10700 L☉± 1100 L☉Integrated bolometric flux and Hipparcos distance modulushigh-confidenceSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Canopus heavily saturates Gaia's detectors at V = −0.74, so its distance (94.8 ± 5.0 pc) and derived luminosity (10,700 ± 1,100 L☉) carry a ~5.3% fractional uncertainty from the Hipparcos New Reduction parallax.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Canopus (Alpha Carinae Bright Supergiant) at RA 06h 23m 57.11s, Dec -52° 41′ 44.4″ within Carina, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Carina) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 0° 40°N Lat 67° 30°S Lat RA: 06h 23m 57.11s Dec: -52° 41′ 44.4″ Epoch: J2000.0 · V = -0.74 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Canopus (Alpha Carinae) is the second-brightest star in Earth's night sky at apparent visual magnitude −0.74, outshone only by Sirius. Situated 94.8 ± 5.0 parsecs (309 light-years) away in the southern keel of Argo Navis (Carina), Canopus owes its brilliance to tremendous intrinsic power: within 700 light-years of the Solar System, it has the highest absolute visual magnitude (M_V = −5.71) of any star, radiating 10,700 times the bolometric output of the Sun.

Long-baseline optical interferometry with the Very Large Telescope Interferometer (VLTI) resolved Canopus's limb-darkened disk at 6.93 milliarcseconds, corresponding to a physical radius of 71.4 solar radii—if placed at the center of our Solar System, its photosphere would extend 90% of the way to the orbit of Mercury. Having exhausted its core hydrogen, this 8-to-9 solar-mass intermediate-mass star is currently executing a 'blue loop' across the Hertzsprung-Russell diagram while fusing helium in its core at an effective surface temperature of 7,400 K.

Because Canopus sits far from the ecliptic plane (ecliptic latitude −75.8°) where sunlight and zodiacal dust never interfere, and shines as an unmistakable zero-magnitude beacon, spacecraft since Mariner 4 in 1964 have used dedicated 'Canopus Star Trackers' to lock their roll attitude during interplanetary voyages across the Solar System.

Practical Visual Observing Guide

Minimum InstrumentNaked eye (south of +37°N latitude)
Recommended MagnificationNaked eye / wide-field binoculars
Best Evening SeasonWinter / Southern Summer (December–March)
  • Located 36° south of Sirius at declination −52°42′, Canopus is invisible north of +37°N latitude, but skims the southern winter horizon from the southern United States (Florida, Texas, Arizona, southern California) and the Mediterranean.
  • From the Southern Hemisphere, Canopus rides high overhead on January and February nights, shining with a pure creamy-white luster free of the fierce atmospheric scintillation that affects low-altitude northern views.

Catalog Cross-Identifications & Aliases

Common Aliases: α Carinae · Suhel · HD 45348 · HIP 30438

Cross-Catalog Identifiers for Canopus (Alpha Carinae)
Catalog AuthorityIdentifier
HIPHIP 30438
HDHD 45348
SIMBAD* alf Car
WIKIDATAQ12189
Related Object · Canis Major

Sirius (Alpha Canis Majoris Binary)

Coordinates, Hipparcos parallax (379.21 mas, 8.60 ly), magnitude −1.46, Sirius B white dwarf orbit, and observing guide for Sirius.

Related Object · Eridanus

Achernar (Alpha Eridani Oblate Be Star)

Coordinates, Hipparcos distance (139 ly), magnitude 0.46, extreme 1.35:1 equatorial flattening, and observing guide for Achernar in Eridanus.

Reference Guide

Apparent vs Absolute Magnitude Explained

Understand the logarithmic Pogson astronomical magnitude scale, apparent visual magnitude (m), absolute magnitude (M at 10 parsecs), and bolometric corrections.

Reference Guide

Trigonometric Parallax, Parsecs & Gaia DR3

How trigonometric parallax (d_pc = 1 / p_arcsec), the distance modulus equation, Hipparcos, and Gaia DR3 microarcsecond astrometry measure cosmic distances.

Scientific Sources & Dataset Provenance