Leo, the Lion

The zodiacal constellation Leo, the lion, is one of a handful of constellations that really does look like its namesake. It consists of two patterns of stars that the brain puts together to make a lion. A backward question mark represents the head and mane, and a triangle of stars to the lower left forms the lion's hindquarters and tail. Look for Leo high in the south in April and May.

Leo, the Lion

Leo's brightest star is blue-white Regulus, one of the brightest stars in the night sky. It is about 79 light-years away. Regulus rises almost due east, with the body of the lion following it into the sky over the next couple of hours. Once Regulus climbs into the sky, look to its left — toward the north — for the backwards question mark, known as the Sickle, that outlines his head and mane.

About two hours later, look low in the east for Leo's tail — a white star named Denebola, which comes from an Arabic name that, appropriately enough, means "tail of the lion."

At a distance of just 36 light-years, Denebola is a fairly close neighbor. Even so, the fact that we can see it at all means that Denebola is quite bright -- more than 10 times brighter than the Sun. Denebola's brightness is a product of its mass. The star is about twice as heavy as the Sun, so it "fuses" the hydrogen in its core at a much faster rate. That makes the star's surface thousands of degrees hotter than the Sun's. The combination of high temperature and large size makes Denebola outshine the Sun and all but a few percent of all the stars in the Milky Way galaxy.

Denebola is surrounded by a disk of dust grains. It may be supplied with fresh material by collisions between small planet-building bodies. So far, no one has seen any evidence of planets around the star, although they can't be ruled out, either. Astronomers continue to hunt for companions to this bright stellar neighbor.

Leo also contains quite a few bright galaxies. Leading the list are three galaxies that together form the Leo Triplet: M65, M66, and NGC 3628.

NGC 3628 is the most interesting of the three. Like our own Milky Way, it's a spiral -- a pinwheel that spans at least a hundred thousand light-years. We see it edge-on, so it looks like a streak of light with lanes of dark dust running down the middle. Gravitational encounters with the other galaxies have triggered the birth of perhaps millions of new stars near the galaxy's center. They have pulled out a tail of gas that spans a quarter-million light-years. The tail contains enough gas to make half a billion stars as massive as the Sun. In fact, it has given birth to millions of stars in several large clumps.

FacebookTwitterYouTube

©2014 The University of Texas McDonald Observatory