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Lacerta

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Lacerta is one of the 88 modern constellations recognized by the International Astronomical Union. Its name is the Latin word for lizard.

LacertaCC
LacertaCC

This constellation is relatively small and faint. It is located on the northern celestial sphere. You can find it positioned between the constellations Cygnus, Cassiopeia, and Andromeda. The northern section of Lacerta lies along the path of the Milky Way. Because its brightest stars form a "W" shape, some people call it "Little Cassiopeia."

Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser
Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser

Lacerta is a typical Milky Way constellation. It does not contain bright galaxies or globular clusters. Instead, it features open clusters and several interesting deep-sky objects. One example is NGC 7243, which is an open cluster located 2,500 light-years from Earth. This cluster contains a few dozen scattered stars. The brightest stars in this group have a magnitude of 8. The constellation also contains the faint planetary nebula IC 5217.

LacertaCC
LacertaCC

Many unique stars reside within this constellation. Alpha Lacertae is a blue-white main-sequence star. It has a magnitude of 3.8 and sits 102 light-years away from Earth. This star is an optical double star with a spectral type of A1 V. Beta Lacertae is much dimmer with a magnitude of 4.4. It is a yellow giant star located 170 light-years away. There is also a multiple star system called Roe 47. It consists of five different components with magnitudes ranging from 5.8 to 10.1.

Some objects in Lacerta are quite unusual. The binary star system ADS 16402 is orbited by a planet named HAT P-1. This planet is about the size of Jupiter. However, it has an unexpectedly low density. Its density is roughly the same as cork. Another interesting star is EV Lacertae. It is a magnitude 10 red dwarf that spins very rapidly. It is a flare star with a strong magnetic field. It can emit powerful flares that are thousands of times more energetic than those from our sun.

LacertaCC
LacertaCC

One of the most significant objects is BL Lacertae. This object is the prototype for a whole class of celestial bodies called BL Lacertae objects. These are a subtype of blazars. While they may appear to be dim variable stars, they are actually the variable nuclei of elliptical galaxies. They are similar to quasars. The object varies irregularly between magnitudes 14 and 17 over a period of a few days. This discovery helped scientists name an entire category of cosmic objects.

Lacerta was not recognized by ancient Western astronomers. The constellation was defined in 1687 by the astronomer Johannes Hevelius. He originally named it "Stellio," which refers to a lizard with star-like spots. Other people tried to give the constellation different names later. In 1670, Augustin Royer created "Sceptrum et Manus Iustitiae" to honor Louis XIV. In 1787, Johann Elert Bode named it "Frederici Honores" to honor Frederick the Great. Both of these names are now obsolete, while Lacerta remains the official name.

Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser
Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser

Different cultures have viewed these stars in their own ways. Early Chinese astronomers combined these stars with parts of Cygnus to create a "Flying serpent." The Chumash people of California also refer to this area as "Lizard." They include the lizard in many of their traditional stories. Even the United States Navy used the name for a ship. They named an attack cargo ship the USS Lacerta (AKA-29) after this constellation.

Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser
Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser
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File:Sidney Hall - Urania's Mirror - Lacerta, Cygnus, Lyra, Vulpecula and Anser.jpg
Sidney Hall - Urania's Mirror - Lacerta,...
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