Rahul Sharma (Editor)

Iota Andromedae

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Magnitude
  
4.29

Apparent magnitude (V)
  
4.29

Constellation
  
Andromeda

Iota Andromedae

Similar
  
Epsilon Andromedae, Mu Andromedae, Eta Andromedae, 51 Andromedae, Nu Andromedae

Iota Andromedae (ι And, ι Andromedae) is a star in the constellation Andromeda. It has an apparent magnitude of +4.29 and is approximately 500 light years from Earth.

Iota Andromedae is a B-type main sequence star with a stellar classification of B8 V. It is among the least variable stars observed during the Hipparcos mission.

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 as Manus Catenata, meaning palm of chained woman.
  • In Chinese, 螣蛇 (Téng Shé), meaning Flying Serpent, refers to an asterism consisting of ι Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, λ Andromedae, κ Andromedae and ψ Andromedae. Consequently, ι Andromedae itself is known as 螣蛇二十二 (Téng Shé èrshíèr, English: the Twenty Second Star of Flying Serpent)

    • References

    Iota Andromedae Wikipedia
    (Text) CC BY-SA


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