Lambda Cassiopeiae

Lambda Cassiopeiae (λ Cas, λ Cassiopeiae) is a binary star in the constellation Cassiopeia. The system has a combined apparent magnitude of +4.74 and is approximately 355 light years from Earth.

Both components are blue-white B-type main sequence dwarfs. The brighter, λ Cassiopeiae A, has an apparent magnitude of +5.5, while its companion, λ Cassiopeiae B, has an apparent magnitude of +5.8. The two stars are separated by 0.6 arcseconds and complete one orbit around their common centre of mass once every 640 years.

Stars of Cassiopeia
Bayer
  • α (Schedar)
  • β (Caph)
  • γ (Tsih)
  • δ (Ruchbah)
  • ε (Segin)
  • ζ
  • η (Achird)
  • θ
  • ι
  • κ
  • λ
  • μ
  • ν
  • ξ
  • ο
  • π
  • ρ
  • σ
  • τ
  • υ1
  • υ2
  • φ
  • χ
  • ψ
  • ω
  • A
Flamsteed
  • 1
  • 2
  • 4
  • 5 (τ)
  • 6
  • 7 (ρ)
  • 8 (σ)
  • 9
  • 10
  • 11 (β, Caph)
  • 12
  • 13
  • 14 (λ)
  • 15 (κ)
  • 16
  • 17 (ζ)
  • 18 (α, Schedar)
  • 19 (ξ)
  • 20 (π)
  • 21
  • 22 (ο)
  • 23
  • 24 (η, Achird)
  • 25 (ν)
  • 26 (υ1)
  • 27 (γ, Tsih)
  • 28 (υ2)
  • 30 (μ)
  • 31
  • 32
  • 33 (θ)
  • 34 (φ)
  • 35
  • 36 (ψ)
  • 37 (δ, Ruchbah)
  • 38
  • 39 (χ)
  • 40
  • 42
  • 43
  • 44
  • 45 (ε, Segin)
  • 46 (ω)
  • 47
  • 48 (A)
  • 49
  • 50
  • 51
  • 52
  • 53
  • 54
  • 55
  • List