Meet Regulus, Little King of the Ecliptic

Regulus Vitals

Official name (IAU-approved) Regulus
Other Designations Regulus A, Alpha Leonis
Nicknames Cor Leonis, Little King, Heart of the Lion, Prince, Rex
Apparent Magnitude 1.36
Distance from Earth 79 light-years
Type* Main sequence (B8IVn)
Color* Bluish-white
Mass* 3.5 M
Radius* 3.1 R
Constellation Leo
Right Ascension 10h 8m 22.31s
Declination +11° 58' 02''
Multiple system? Yes, three companions
Variable star? No
Exoplanet status None known
Probable fate Uncertain

Physical Characteristics

You probably have a personal list of favorite night-sky objects that you regularly observe. Here's one you might consider adding to your list of go-tos: Regulus, the brightest star in the constellation Leo and one of the 25 brightest stars in the sky.

Regulus-Venus conjunction

Regulus and Venus shine close together in the evening sky.
Daniel Johnson

This “little king” of Leo has a distorted, oblate shape due to its rotation. Many amateur astronomers are familiar with Jupiter’s “equational bulge,” which is visible in a small telescope: Rather than appearing as a true sphere, Jupiter displays a slight “flattening” near the poles that is caused by the centrifugal force created by the planet’s 10-hour spin. The surface at the equator travels around 28,000 mph.

Regulus also spins very fast — rotating every 16 hours — but because of its larger size, the actual speed of the star’s surface at the equator jumps to an incredible 700,000 mph. The stresses created by this speed distort Regulus’s shape. In fact, if Regulus were spinning only 15% faster, it would tear itself apart.

Regulus and Sun diagram

The shape and size of Regulus compared to the Sun (smaller yellow circle).
Sky & Telescope diagram

The cause of Regulus’s rapid rotation is under debate. It’s possible that the star’s gravitaty interacts with its small fleet of minor companion stars to speed up its spin — Regulus has one close white dwarf companion and two more distant stellar companions that are themselves gravitationally bound.

The presence of a white dwarf in a tight, 40-day orbit around Regulus makes the future of the system uncertain: If the white dwarf siphons enough mass from its massive companion, it might obliterate itself in a Type Ia supernova. If it doesn’t, then the two objects may orbit each other as white dwarfs or even merge into a single object.

Origin / Mythology

Like much of our astronomical tradition, the most well-known appearance of Leo in mythology comes from the Greeks, who named the constellation after the lion that Hercules defeated during his 12 labors. But the lion theme is not unique to the Greeks alone. Other cultures also found this image, including the Babylonians and Persians. In Arabic, Regulus is named Qalb al-Asad, meaning “the heart of the lion.”

Regulus itself means “little king” in Latin, and in general, various cultures have referred to Regulus using terms like “king,” “royal,” “strong,” “mighty,” “great,” etc. Interestingly, all of these terms are also appropriate for a lion.

How to See Regulus

On July 25, 2017, Shahrin Ahmad in Kuala Lumpur, Malaysia, took a telescopic video of Regulus emerging from behind the Moon's bright limb.

Leo can be observed throughout the year except around September, when the constellation moves into the glare of the Sun. However, spring is a better time for viewing, as the star moves into a good position early in the evening. Leo is notable for its “sickle” — a group of stars on the right side of the constellation that form a kind of rough hook shape, sometimes compared to a “reversed question mark.” Regulus is the bright star that makes the point of the question mark.

Similar to the way the Big Dipper can serve as a pointer to Polaris, two stars on the left-hand side of the Dipper’s bowl can serve as pointers to Regulus in the opposite direction of the sky. The trick doesn’t work quite as well as it does for Polaris, because the distance is greater and the line is a little off-center, but it’s easy to remember.

Regulus happens to be one of the brightest stars near the ecliptic, and that’s where things get fun. Its proximity to the plane of the solar system means that the star frequently participates in lunar and planetary conjunctions and occultations.

All comments must follow the Sky & Telescope Terms of Use and will be moderated prior to posting. Please be civil in your comments. Sky & Telescope reserves the right to use the comments we receive, in whole or in part, and to use the commenter’s username, in any medium. See also the Terms of Use and Privacy Policy.

COMMENT

This site uses Akismet to reduce spam. Learn how your comment data is processed.