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Sigma Orionis — Double Star in Orion

Magnitude 3.8m DoubleStar Orion (Ori) Visible
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1Physical Properties

Magnitude 3.81
Spectral Type O9.5V
Star Color Blue (B-V -0.24)
Distance 950 ly

2Position & Identifiers

RA 05h 38m 44.8s
Dec -02° 36' 00.0"
Constellation Orion (Ori)
HR 1931
HIP 26549
HD 37468
SAO 132406
Bayer Sigma
Flamsteed 48 Ori
Double Cat 4241

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Medium+ Medium+
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Nov – Jan (peak: Dec)

5Multiple Star System Quintuple

Components 5 (quintuple)
Component IDs AB
Separation 0.3″
Companion Mag 5.3
Companion Sp B?
Position Angle 239°
Star Colors A: Blue B: Blue
Discoverer BU 1032
AB 4.1 O9.5V, 5.1 B0.5V, 170y, a = 0.247". Combined mag. and colors. C, 8.79V, A2V at 11" may be physical; D, 6.62V, | -0.20(B-V), B2V, at 13" and E = HR 1932, at 42" CPM with A. A multiple system similar to trapezium. ADS 4241 possibly | the most massive visual binary known, 35 solar masses.

Separation over time

Period: 23.0 y Eccentricity: 0.024 Now: 0.26", PA 46° + 0.01" in 5 years
0.00" 0.08" 0.15" 0.23" 0.31" 2015 2020 2025 2030 2035 0.26"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

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7

Size Comparison

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8

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9

Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

14

Stellar Fusion

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15Stellar Notes

Ori OB1b1; Orion belt; HII reg.; IC 434; a trapezium system.
Hydrogen deficient. Interstellar Lyman alpha absorption observed by AEROBEE rocket.
0.003".
16

Light Travel Time Machine

17

Relativistic Travel

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