Cassiopeia (Constellation)
Contents
Image: Constellation Cassiopeia
Overview
Cassiopeia, the seated queen, is a circumpolar constellation of the northern hemisphere.
Mythology
Cassiopeia was wife to King Cepheus of Aethiopia and mother to Andromeda. Queen Cassiopeia was vain an arrogant and proclaimed that her daughter Andromeda was more beautiful than the sea nymphs. The sea-god was angered by this and sent a sea monster, Cetus, to terrorize the King and Queen's subjects. The only way to stop Cetus was if Andromeda was sacificed to him. Andromeda was chained to the rocks in the sea to await her fate but was saved by the hero Perseus when he turned Cetus to stone with the severed head of Medusa.
Named stars
Shedir (or Shedar or Schedar or Schedir) (Alpha Cassiopeiae / α Cas)
A K0 orange giant star 230ly from our solar system
Caph (Beta Cassiopeia / β Cas)
An F2 class star with an apparent brightness of magnitude 2.27
Navi (or Cih or Tsih) (Gamma Cassiopeiae / γ Cas)
The middle star of the 'W' of Cassiopeia. An optical double and Be-type star, Gamma Cassiopeiae is also a spectroscopic binary with a companion star about the same size as the Sun.
Ruchbah (or Rucha or Rukbah) (Delta Cassiopeiae / δ Cas)
An A5 class star about 100ly from Earth
Segin (Epsilon Cassiopeiae / ε Cas)
A blue-white B3 class giant star 440ly from Earth
Achird (Eta Cassiopeiae / η Cas)
A G type dwarf star similar to the sun
Open Clusters
M52 (NGC 7654)
Discovered in 1774 by Charles Messier this cluster has an apparent magnitude of +7.3
M103 (NGC 581)
Discovered in 1781 by Pierre Mechain, M103 is a type-d open cluster with an apparent magnitude of +7.4 and lies at a distance of 8500ly from Earth
NGC 103
Open cluster with an apparent magnitude of +9.8
NGC 129
An open cluster located between beta and gamma Cassiopeiae
NGC 133
A type IV1p cluster with an apparent magnitude of +9.4
NGC 146
A very loose open cluster
NGC 189
Discovered in 1783 by Caroline Herschel this cluster has an apparent magnitude of +8.8
NGC 225 (Sailboat Cluster)
An open cluster discovered by Caroline Herschel in 1787 with an apparent magnitude of +7
NGC 381
Discovered in 1787 by William Herschel this open cluster has an apparent magnitude of +9.4
NGC 457 (Owl Cluster or ET Cluster / Caldwell 13)
An open cluster about 7900ly away, discovered by Friedrich Wilhelm Herschel in 1787
NGC 559 (Caldwell 8)
Open cluster with an apparent magnitude of +9.5
NGC 609
Open cluster with an apparent magnitude of +11
NGC 637
Open cluster with an apparent magnitude of +8.2
NGC 654
An open cluster discovered by Friedrich Wilhelm Herschel in 1787
NGC 659
Discovered in 1783 by Caroline Herschel this cluster has an apparent magnitude of +7.9
NGC 7788
A faint cluster with an apparent magnitude of +9
NGC 7789
An open cluster discovered in 1783 by Caroline Herschel
NGC 7790
An open cluster with an apparent magnitude of +8.5
Nebulae
IC 59 and IC 63 (Sharpless 2-185)
This pair of arc-shaped emission/reflection nebulae are collectively known as Sharpless 2-185 and are associated with the star γ Cas
IC 289
A planetary nebula discovered by Lewis Swift in 1888
Heart Nebula (IC 1805)
An emission nebula (sometimes classed as a cluster associated with nebulosity) 7500ly away
Soul Nebula (IC 1848)
An emission nebula (sometimes classed as a cluster associated with nebulosity) 7500ly away. The Soul Nebula is the eastern neighbour of IC 1805
Galaxies
NGC 147
A dwarf elliptical galaxy which is a satellite of the Andromeda Galaxy. NGC 147 was discovered by John Herschel in 1829
NGC 185
A dwarf spheroidal galaxy which is a satellite of the Andromeda Galaxy and is 2.3 million light years from Earth
NGC 278
A spiral galaxy 38.5 million light years away
NGC 1343
A galaxy with an apparent magnitude of +12.3
Andromeda VII (Cassiopeia Dwarf Spheroidal Galaxy)
A dwarf spheroidal galaxy associated with M31 galaxy in Andromeda. It is about 2.6 million light years away.
Bordering Constellations
Cassiopeia shares its borders with the following constellations: Cepheus, Lacerta, Andromeda, Perseus and Camelopardalis