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V918 Scorpii — Double Star in Scorpius

Magnitude 5.5m DoubleStar Scorpius (Sco) Visible
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1Physical Properties

Magnitude 5.47
Range 5.42 - 5.50
Period 9.8 days
Variable Type Ellipsoidal Variable
Spectral Type O9Ia supergiant
Star Color Yellow-white (B-V 0.40)

2Position & Identifiers

RA 16h 36m 22.5s
Dec -42° 51' 32.0"
Constellation Scorpius (Sco)
HR 6164
HIP 81305
HD 149404
SAO 226953
Variable ID V918 Sco

3How easy to split?

Primary 5.5 mag Companion 11.4 mag Separation 6.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard+
150mm Newt. Hard+ Hard+ Hard+
C8 203mm Medium Medium Medium
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Apr – Jun (peak: May)

5Light Curve

6Multiple Star System

Separation 6.8″
Companion Mag 11.4
Position Angle 120°
Star Colors A: Yellow-white
Discoverer SNA 42

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 120°

A: 5.5 · B: 11.4 · Sep: 6.8″ · PA: 120° · N up, E right

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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Size Comparison

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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

9.813d, k1 101k/s, K2 60k/s, V1 -37k/s, V2 -28k/s, m1sin3i 1.6, m2sin3i 2.7, | a1sini 13.7, a2sini 8.1.
Ara OB1a. Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out | that it is a nonmember background star.
H alpha emission.
Two available determinations of vsini, 140 and 45k/s.
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