Omicron Serpentis (ο Ser, ο Serpentis) is a star in the constellation Serpens.
Omicron Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +4.24. It is approximately 168 light years from Earth. It is classified as a Delta Scuti type variable star and its apparent magnitude varies by 0.01 with a period of 76 minutes.
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Stars of Serpens
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| Bayer |
- α (Unukalhai)
- β (Chow)
- γ
- δ (Tsin)
- ε
- ζ
- η (Tang)
- θ (Alya)
- ι
- κ
- λ
- μ
- ν
- ξ
- ο
- π
- ρ
- σ
- τ1
- τ2
- τ3
- τ4
- τ5
- τ6
- τ7
- τ8
- υ
- φ
- χ
- ψ
- ω
- b
- c
- d
- e
- A1
- A2
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| Flamsteed |
- 3
- 4
- 5
- 6
- 7
- 8
- 9 (τ1)
- 10
- 11 (A1)
- 12 (τ2)
- 13 (δ, Tsin)
- 14
- 15 (τ3)
- 16
- 17 (τ4)
- 18 (τ5)
- 19 (τ6)
- 20 (χ)
- 21 (ι)
- 22 (τ7)
- 23 (ψ)
- 24 (α, Unukalhai)
- 25 (A2)
- 26 (τ8)
- 27 (λ)
- 28 (β, Chow)
- 29
- 31 (υ)
- 32 (μ)
- 34 (ω)
- 35 (κ)
- 36 (b)
- 37 (ε)
- 38 (ρ)
- 39
- 40
- 41 (γ)
- 43
- 44 (π)
- 45
- 46
- 47
- 50 (σ)
- 53 (ν)
- 55 (ξ)
- 56 (ο)
- 57 (ζ)
- 58 (η, Tang)
- 59 (d)
- 60 (c)
- 61
- 63 (θ, Alya)
- 64
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| Nearby |
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