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arearank = 27th |
arearank = 27th |
numbermainstars = 7 |
numbermainstars = 7 |
numberstars = 35 |
numberbfstars = 35 |
numberbrightstars = 1 |
numberbrightstars = 1 |
numbernearbystars = 7 |
numbernearbystars = 5 |
numberstarsplanets = '''1''', 0 |
numberstarsplanets = 1 |
brighteststarname = [[Alpha Cephei|α Cep]] (Alderamin) |
brighteststarname = [[Alpha Cephei|α Cep]] (Alderamin) |
starmagnitude = 2.44 |
starmagnitude = 2.44 |
neareststarname = [[Eta Cephei|η Cep]] |
neareststarname = [[Kruger 60]] |
stardistance = 45.8 |
stardistance = 13.15 |
numbermessierobjects = 0 |
numbermessierobjects = 0 |
meteorshowers = None |
meteorshowers = None |

Revision as of 22:44, 5 March 2007

Cepheus
Constellation
Cepheus
AbbreviationCep
GenitiveCephei
Right ascension22
Declination+70
Area588 sq. deg. (27th)
Main stars7
Bayer/Flamsteed
stars
35
Stars with planets1
Stars brighter than 3.00m1
Stars within 10.00 pc (32.62 ly)5
Brightest starα Cep (Alderamin) (2.44m)
Messier objects0
Meteor showersNone
Bordering
constellations
Ursa Minor
Draco
Cygnus
Lacerta
Cassiopeia
Camelopardalis
Visible at latitudes between +90° and −10°.
Best visible at 21:00 (9 p.m.) during the month of November.

Cepheus (IPA: /ˈsiːfiəs, ˈsiːˌfjuːs/) is a northern constellation named after King Cepheus in Greek mythology, and is considered to represent a king. It is one of the 88 modern constellations, and was also one of the 48 listed by Ptolemy.

Notable features

γ Cephei is a binary star approximately 50 light years away from Earth. The system consists of an orange subgiant and a red dwarf. Due to the precession of the equinoxes, γ Cephei will be the pole star between 3000 and 5200 AD, with the closest approach to the north celestial pole around 4000 AD. The primary component is orbited by a planet.

δ Cephei is the prototype Cepheid variable. It was discovered to be variable by John Goodricke in 1784. It varies between 3.5m and 4.3m over a period around 5.4 days.

There are three red supergiants in the constellation that are visible to the naked eye. μ Cephei is known as Herschel's Garnet Star due to its deep red colour. It is a semiregular variable star that varies between 3.4m and 5.1m over a period of 730 days. The star is around 11.8 AU in radius. If it were placed at the centre of our Solar System, it would extend to the orbit of Saturn. Like μ Cep, VV Cephei is also variable, ranging from 4.8m and 5.4m over a period around 20 years. The third red supergiant is HR 8164, whose apparent magnitude is 5.66m. Each of the stars are among the largest known.

Kruger 60 is a 10th magnitude binary star consisting of two red dwarfs. The star system is one of the nearest being only 13 light years away from Earth.

Notable deep sky objects

NGC 188 is an open cluster that has the distinction of being the closest open cluster to the north celestial pole, as well as one of the oldest known open clusters. The Fireworks Galaxy (NGC 6946) is a spiral galaxy in which eight supernovae have been observed, more than in any other galaxy.

Mythology

When including fainter stars, visible to the naked eye, Cepheus appears as a man with a crown (upside down with respect to the ecliptic). Together with other constellations nearby (Andromeda, Perseus, Cassiopeia, and possibly Pegasus), and the constellation Cetus below Cepheus, this may be the source of the myth of the Boast of Cassiopeia, with which it is usually identified.

See also