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Regulus

HIP 49669; Alpha Leonis; 32 Leonis

HIP 49669; Alpha Leo; 32 Leo DoubleStar Leo Visible
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About Regulus

Description

Regulus is the brightest star in Leo at magnitude 1.35, a blue-white main-sequence star of spectral type B7V located about 79 light-years from Earth. It is actually a quadruple star system. Regulus spins extremely rapidly — at about 96% of its breakup velocity — completing a rotation in just 15.9 hours and making it severely oblate. Its luminosity is about 288 times solar.

Observing Tips

Regulus sits at the base of the Sickle of Leo — the reversed question-mark asterism forming the Lion's head and mane. It is the brightest star on the ecliptic, so it is frequently occulted by the Moon and occasionally by planets. The wide companion Regulus B/C (magnitude 8.1) is visible in a small telescope about 177 arcseconds away. Best observed February through June.

History

The name Regulus means 'little king' in Latin, given by Copernicus. It was one of the four Royal Stars of ancient Persia (along with Aldebaran, Antares, and Fomalhaut), marking the summer solstice around 3000 BC. The Babylonians called it 'the star that stands in the breast of the Lion.' Its position on the ecliptic has made it astronomically important since antiquity.

Fun Facts

Regulus rotates so fast that it is about 32% wider at the equator than at the poles. Its equatorial surface temperature is about 10,000 K while the poles reach 15,400 K due to gravity darkening. If it spun just 16% faster, it would tear itself apart.

Observe

1Physical Properties

Magnitude 1.35
Spectral Type B8IVn
Star Color Blue-white (B-V -0.11)
Temperature 12433 K
Radius 3.1 R☉
Distance 79 ly

Position & Identifiers

RA 10h 08m 22.3s
Dec +11° 58' 02.0"
Constellation Leo
HR 3982
HIP 49669
HD 87901
Bayer Alpha
Flamsteed 32 Leo
Double Cat 7654

2How easy to split?

Primary 1.4 mag Companion 8.2 mag Separation 175.9″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

3Visibility

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Best season Jan – Mar (peak: Feb)

4Multiple Star System D: optical

Components 4
Component IDs AB
Separation 175.9″
Companion Mag 8.2
Position Angle 308°
Star Colors A: Blue-white
Discoverer STFB 6

Eyepiece View

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32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 308°

A: 1.4 · B: 8.2 · Sep: 175.9″ · PA: 308° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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Size Comparison

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Stellar Lifecycle

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Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Blackbody Spectrum

12

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

13

Stellar Fusion

Discover

14Stellar Notes

AB binary, B, 8.13V, +0.86(B-V), +0.51(U-B), K1V. BC, 7.6, 13.1v, 2000y, a = 4.163".
Color excess E(B-V) = +0.01.
C1 neutral carbon continuum shows discontinuities in UV. Excess IR emission.
REGULUS; Cor Leonis; Rex; Al Kalb al Asad; Kabeleced.
Diam. = 0.00132 - 0.00137".
15

Light Travel Time Machine

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Relativistic Travel

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