Bright & Nearby Stars · Constellation Leo

Regulus (Alpha Leonis)

Coordinates, Hipparcos distance (79.3 ly), magnitude 1.36, 15.9-hour rapid oblate rotation, wide companions, and observing guide for Regulus.

Right Ascension (J2000.0)10h 08m 22.31s
Declination (J2000.0)+11° 58′ 02.0″
Primary ClassificationRapidly rotating B/A subgiant in a hierarchical quadruple system
Best Observing SeasonSpring (February–June)

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 Regulus (Alpha Leonis)
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Apparent visual magnitude (V)1.36 mag± 0.01 magJohnson UBV photoelectric photometrydefinitiveHipparcos New Reduction Catalog
Trigonometric parallax41.13 mas± 0.35 masHipparcos New Reduction astrometric solution (24.31 ± 0.21 pc) (J2000.0)definitiveHipparcos New Reduction Catalog
Distance in light-years79.3 ly± 0.7 lyDerived from Hipparcos parallax 41.13 ± 0.35 masdefinitiveHipparcos New Reduction Catalog
Equatorial radius (oblate rotator)4.16 R☉± 0.08 R☉CHARA optical interferometry (polar radius = 3.14 ± 0.06 R☉)definitiveSIMBAD Astronomical Database (CDS)
Primary stellar mass (Regulus A)3.8 M☉± 0.2 M☉CHARA gravity-darkened model + 40.11-day pre-white-dwarf binary orbithigh-confidenceSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: Viewed nearly equator-on (inclination ~86°) while spinning at 317 km/s, Regulus A exhibits severe gravity darkening between its 15,400 K poles and 10,200 K equator, making its orientation-averaged luminosity (288 L☉) model-dependent.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots Regulus (Alpha Leonis Quadruple System) at RA 10h 08m 22.31s, Dec +11° 58′ 02.0″ within Leo, 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 (Leo) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 62° 40°N Lat 48° 30°S Lat RA: 10h 08m 22.31s Dec: +11° 58′ 02.0″ Epoch: J2000.0 · V = 1.36 mag First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

Regulus (Alpha Leonis, Latin for 'Little King' and traditionally called Cor Leonis, the Heart of the Lion) is the brightest star in Leo at apparent visual magnitude 1.36, lying 24.31 ± 0.21 parsecs (79.3 light-years) from Earth. Sitting just 0.46° (27.6 arcminutes) north of the ecliptic—closer to the Sun's apparent path than any other first-magnitude star—Regulus is regularly occulted by the Moon, Venus, and Mercury, and was revered by ancient Babylonian and Persian astronomers as one of the four 'Royal Stars' guarding the heavens.

Optical interferometry with the CHARA Array revealed that Regulus A (spectral type B8 IVn, 3.8 solar masses) spins on its axis once every 15.9 hours at an equatorial velocity of 317 ± 3 km/s—96.5% of the speed at which centrifugal force would tear the star apart! That extreme spin flattens its equatorial radius to 4.16 solar radii compared to 3.14 solar radii at its poles, while gravity darkening makes its poles five times brighter per unit area than its equator.

In 2008 spectroscopic radial-velocity measurements explained why Regulus spins so fast: Regulus A is orbited every 40.11 days at a separation of 0.35 AU by a faint ~0.30-solar-mass pre-white-dwarf companion that transferred mass and angular momentum onto Regulus A hundreds of millions of years ago. At an angular separation of 176.9 arcseconds (~4,200 AU) northwest orbits the co-moving binary Regulus BC, a pair of K2 V and M4 V dwarfs.

Practical Visual Observing Guide

Minimum InstrumentNaked eye (50 mm telescope / binoculars for wide companion Regulus B)
Recommended Magnification40×–80× for Regulus B; 200×+ in 150 mm+ scope for Regulus BC split
Best Evening SeasonSpring (February–June)
  • Anchors the base of the famous 'Sickle of Leo' (a backward question-mark asterism), with Regulus serving as the dot at the bottom of the question mark.
  • Any 50–60 mm telescope or 10×50 binocular easily shows 8.13-magnitude orange companion Regulus B located 176.9 arcseconds (nearly 3 arcminutes) northwest of dazzling blue-white Regulus A.
  • In a 150–200 mm telescope at 180×–250×, Regulus B itself splits into a tight 2.5-arcsecond binary with its 13.5-magnitude red dwarf partner Regulus C.

Catalog Cross-Identifications & Aliases

Common Aliases: α Leonis · Cor Leonis · HD 87901 · HIP 49669 · 32 Leonis

Cross-Catalog Identifiers for Regulus (Alpha Leonis)
Catalog AuthorityIdentifier
HIPHIP 49669
HDHD 87901
SIMBAD* alf Leo
WIKIDATAQ13022
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Arcturus (Alpha Bootis Red Giant)

Coordinates, Hipparcos distance (36.7 ly), magnitude −0.05, halo-stream kinematics, and observing guide for Arcturus in Boötes.

Related Object · Aquila

Altair (Alpha Aquilae Rapid Rotator)

Coordinates, Hipparcos distance (16.73 ly), magnitude 0.76, 8.9-hour oblate spin imaged by CHARA, and observing guide for Altair in Aquila.

Reference Guide

Angular Size, Separation & Field of View

How angular diameter (degrees, arcminutes, arcseconds), spherical angular separation, and small-angle physical diameter relate to telescope field of view.

Reference Guide

Celestial Coordinates (RA & Dec) Explained

Practical reference to J2000 equatorial coordinates: Right Ascension (RA in hours, minutes, seconds), Declination (Dec in degrees), and sexagesimal conversion.

Scientific Sources & Dataset Provenance