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Equuleus

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Equuleus is a faint constellation located just north of the celestial equator. Its name is Latin for "little horse," which refers to a foal. This grouping is one of the 88 modern constellations used by astronomers today. It is quite small in the vast sky. In fact, it is the second smallest constellation known. Only Crux is smaller, covering a tiny area of 72 square degrees.

EquuleusCC
EquuleusCC

Because it is so small and distant from the plane of the Milky Way, it lacks many large objects. It is somewhat devoid of deep-sky objects like bright star clusters or large nebulae. However, it does contain several very faint galaxies. These are found in the New General Catalogue, such as NGC 7015, NGC 7040, and NGC 7046. Another interesting object is NGC 7045. This is a triple star system that the discoverer John Herschel once mistook for a nebula.

Equuleus 20191202
Equuleus 20191202

Many stars within Equuleus exhibit interesting behaviors, such as being variable stars. A variable star is one that changes in brightness over time. There are about 25 known variable stars in this constellation, though most are very faint. For example, gamma Equulei is an alpha2 CVn type variable star. It is a white star located 115 light-years from Earth. Its brightness changes between magnitudes 4.58 and 4.77 every 12.5 minutes. Another example is R Equulei, which is a Mira variable star. Its brightness ranges from magnitude 8.0 to 15.7 over a period of nearly 261 days.

Equuleus 20191202
Equuleus 20191202

Astronomers also study the complex star systems in this region. The brightest star is alpha Equulei, also known as Kitalpha. This yellow star is 186 light-years away and has a magnitude of 3.9. Its name means "the section of the horse." Another system, epsilon Equulei, is a triple star system also called 1 Equulei. It is located 197 light-years away. It consists of a primary binary star and a secondary star. The primary components have a period of 101 years. These two stars are moving closer together. Because of this, they will not be divisible in amateur telescopes starting in 2015.

EquuleusCC
EquuleusCC

Binary stars are another major feature of Equuleus. A binary star system consists of two stars that orbit one another. The star delta Equulei is a binary system with an orbital period of 5.7 years. At one time, this was the shortest known orbital period for an optical binary. The two components of this system stay very close, never more than 0.35 arcseconds apart. Additionally, gamma Equulei has an optical companion called 6 Equulei. This companion has a magnitude of 6.1. The system 6 Equulei is itself an astrometric binary with a magnitude of 6.07.

Equuleus 20191202
Equuleus 20191202

Humans have been mapping these stars for many centuries. The astronomer Ptolemy included Equuleus in his list of 48 constellations during the 2nd century. The constellation was originally created by Hipparchus. Later, the astronomer Bayer assigned designations to four stars, from Alpha through Delta. In 1801, the astronomer Bode added more designations up to Lambda. Today, most people only use the designation Epsilon from that list.

Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014)
Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014)

Mythology provides different ways to view this constellation. In Greek myths, Equuleus may represent the foal Celeris. Celeris was the offspring or brother of the winged horse Pegasus. Some stories say the horse was struck by Poseidon's trident during a contest with Athena. Because this constellation rises before Pegasus, it is sometimes called Equus Primus, or the First Horse. Other myths link the stars to Philyra and Saturn. In Chinese astronomy, these stars belong to a different system. They are located within the Black Tortoise of the North.

Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014)
Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014)
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EquuleusCC.jpg
File:Equuleus 20191202.jpg
Equuleus 20191202.jpg
File:Sidney Hall - Urania's Mirror - Pegasus and Equuleus (best currently available version - 2014).jpg
Sidney Hall - Urania's Mirror - Pegasus...
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