V. sign of zodiac
Particulars:
General:
The fifth constellation of the zodiac. Its asterism, the Sickle, has the appeareance of an arched mane.
Stars and other objects
The brightest star of this constellation, alpha Leo, called
Regulus (meaning: the little king), is a blue-white star
(spectral type B7 V) of 1.35 mag. When viewed with binoculars or small
telescopes a wide companion of 8th mag is revealed.
At the tip of the lion's tail the beautiful blue-white main sequence star
beta Leo, Denebola is located. Viewed through a
telescope beta Leo seems to have an orange companion. But actually the
two stars are far away from each other.
Another optical double is tau Leo; the 7th mag campanion of this orange
5th mag star can be seen in binoculars.
The binary gamma Leo, called Algieba (the lion's mane),
is a magnificent pair, which compenents consists of a orange-red giant of 2.6
mag brightness and a yellow giant with 3.8 mag. A small telescope is sufficient
to split gamma Leo into the single stars. Using binoculars a unrelated
5th mag star, 40 Leo, can be seen next to them.
The binary omega Leo (a 7390) is a very difficult object to resolve.
You will at least need a scope with 250mm aperture. The two stars revolve each
other with a period of 117 years.
With very low power 54 Leo can easily be resolved into a pair of 4.5 mag
and 6.3 mag.
Between eta Leo and gamma Leo the double a 7704 can be
found; but to resolve its components into single stars (both are about 7.5 mag)
telescopes of at least 100mm aperture are required.
Zeta Leo is an optical triple star of 3.44 mag. Using binoculars this
stars seems to have two companions of 6th mag, but they are not physically
related together.
The red giant R Leo is a long period variabale star. Its brightness
variies from mag 4.4 to mag 11.6 (the Bright Stars Catalog gives an average
of 6th mag) with a period of about 313 days. It is located in the Lion's
foreleg.
For Leo is located far away enough from the dust and the starclouds of the
Milky Way the farther away galaxies became visible. There are some interesting
galaxies in this region, but they are not easy objects for small telescopes.
The three galaxies M65,
M66 and
NGC 3628 form a
conspicuous triple.
The other two Messier objects, M95
and M96 are two fainter spiral
galaxies. For more information and observing hints please follow the links to the Messier
database.
There is a large number of meteor showers assiciated with this constellation.
The most famous are the Leonids.
This shower radiates from the region of gamma Leo and can be seen form
November 14-20; the maximum can be observed on November 17th. Although the
hourly rate from 10 to 15 meteor seems to be small there is a cyclus of about
33 years with an enhanced activity. The next spectacular storm is predicted to
take place in 1999.
The shower of the Alpha Leonids
was first confirmed by Radio Meteor Project. The duration of this shower cover
the period from January 13th to February 13th.
From February 14th to April 25th the
Beta Leonids are active.
The maximum takes place around March 20th.
Nearly at the same time - from February 2nd to March 19th - the
Delta Leonids can be
observed. The maximum of the activity peaks at February 22nd.
A rather weak shower are the
Gamma Leonids, which are
active from August 14th to September 12th with a maximum occuring on August
25th.
The meteor shower of the Rho
Leonids seems to be non-existent; yet it has been discovered by radio
studies in the 1960's. It seems to be "active" around March 14-15th.
The Sigma Leonids are another
storm of doubt. Only one observation has been made.
Detailed information for all meteor showers can be found in Gary Kronk's
database about meteor showers.
Mythological Background:
One of the twelve tasks of Hercules was to kill the lion, which this constellation is thought to represent.