Iota Andromedae
Encyclopedia
Iota Andromedae is a star
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...

 in the constellation
Constellation
In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....

 Andromeda
Andromeda (constellation)
Andromeda is a constellation in the northern sky. It is named after Andromeda, the princess in the Greek legend of Perseus who was chained to a rock to be eaten by the sea monster Cetus...

.

Iota Andromedae is a blue-white B-type
Stellar classification
In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure...

 main sequence dwarf
Main sequence
The main sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. These color-magnitude plots are known as Hertzsprung–Russell diagrams after their co-developers, Ejnar Hertzsprung and Henry Norris Russell...

 with an apparent magnitude
Apparent magnitude
The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...

 of +4.29. It is approximately 503 light years
Light Years
Light Years is the seventh studio album by Australian recording artist Kylie Minogue. It was released on 25 September 2000 by Parlophone and Mushroom Records. The album's style was indicative of her return to "mainstream pop dance tunes"....

 from Earth.

Name

In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Keff al-Salsalat (كف المسلسلة - kaf al-musalsala), which was translated into Latin
Latin
Latin is an Italic language originally spoken in Latium and Ancient Rome. It, along with most European languages, is a descendant of the ancient Proto-Indo-European language. Although it is considered a dead language, a number of scholars and members of the Christian clergy speak it fluently, and...

 as Manus Catenata, meaning palm of chained woman.

In Chinese
Chinese language
The Chinese language is a language or language family consisting of varieties which are mutually intelligible to varying degrees. Originally the indigenous languages spoken by the Han Chinese in China, it forms one of the branches of Sino-Tibetan family of languages...

, , meaning Flying Serpent
Flying serpent (asterism)
Flying Serpent is an asterism in the Chinese constellation Encampment .The Jin Shu describes this asterism as: "Flying/Ascending Serpent, 22 stars north of the Ying "Camp" constellation, [a.k.a.] Heavenly Snake, chief of the water reptiles."...

, refers to an asterism consisting of ι Andromedae, α Lacertae
Alpha Lacertae
Alpha Lacertae is an A-type main sequence star in the constellation of Lacerta...

, 4 Lacertae, π2 Cygni
Pi2 Cygni
Pi² Cygni is a fourth-magnitude star in the constellation Cygnus. It has the traditional name Pennae Caudalis, which is Latin for "Tail Feathers"...

, π1 Cygni
Pi1 Cygni
Pi1 Cygni is a star in the constellation Cygnus. It has the traditional name Azelfafage.In Chinese, , meaning Flying Serpent, refers to an asterism consisting of π1 Cygni, α Lacertae, 4 Lacertae, π2 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR...

, HD 206267
HD 206267
HD 206267 is a star....

, ε Cephei
Epsilon Cephei
Epsilon Cephei is a Class F0, fourth-magnitude star in the constellation Cepheus. Epsilon Cephei is a yellow-white, Delta Scuti variable star, located about 85 light-years from Earth....

, β Lacertae, σ Cassiopeiae
Sigma Cassiopeiae
Sigma Cassiopeiae is a binary star in the constellation Cassiopeia. It is approximately 1520 light years from Earth and is a combined apparent magnitude of +4.88....

, ρ Cassiopeiae
Rho Cassiopeiae
Rho Cassiopeiae is a yellow hypergiant star in the constellation Cassiopeia. It is about away from Earth, yet can still be seen by the naked eye , as it is 550,000 times as luminous as the Sun. On average, it has an absolute magnitude of −7.5, making it one of the most luminous stars known...

, τ Cassiopeiae
Tau Cassiopeiae
Tau Cassiopeiae is a star in the constellation Cassiopeia.τ Cassiopeiae is an orange K-type giant with an apparent magnitude of +4.88. It is approximately 172.8 light years from Earth....

, AR Cassiopeiae
AR Cassiopeiae
AR Cassiopeiae is a multiple star system in the constellation of Cassiopeia. It is thought to be a septuple star system. It is only one of two star systems with a multiplicity of 7, the other being Nu Scorpii, with no physical multiple stars of greater multiplicity yet found.The star was...

, 9 Lacertae, 3 Andromedae
3 Andromedae
3 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.64....

, 7 Andromedae
7 Andromedae
7 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.53....

, 8 Andromedae
8 Andromedae
8 Andromedae is a red giant star in the constellation Andromeda. Its apparent magnitude is 4.85.-Component:-References:#...

, λ Andromedae
Lambda Andromedae
Lambda Andromedae is a binary star in the constellation Andromeda. It is approximately 84.2 light years from Earth....

, κ Andromedae
Kappa Andromedae
Kappa Andromedae is a star in the constellation Andromeda.Kappa Andromedae is a blue-white B-type subgiant with an apparent magnitude of +4.15. It is approximately 170 light years from Earth.-References:*...

 and ψ Andromedae
Psi Andromedae
Psi Andromedae is a double star system in the constellation Andromeda. It is approximately 1310 light years from Earth. The system consists of a spectroscopic binary with a yellow G-type supergiant and a white A-type main sequence dwarf. It has a combined apparent magnitude of +4.97.-References:*...

. Consequently, ι Andromedae itself is known as
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