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13 Vulpeculae — Double Star in Vulpecula

Observable Double Star Fair (27/100)

Sep: 1.5", Companion: mag 7.4

Magnitude 4.6m DoubleStar Vulpecula (Vul) Visible
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Observe

1Physical Properties

Magnitude 4.58
Spectral Type B9.5III giant
Star Color Blue-white (B-V -0.06)
Distance 362 ly

2Position & Identifiers

RA 19h 53m 27.7s
Dec +24° 04' 47.0"
Constellation Vulpecula (Vul)
HR 7592
HIP 97886
HD 188260
SAO 87883
Flamsteed 13 Vul

3How easy to split?

Primary 4.6 mag Companion 7.4 mag Separation 1.5″
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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 Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 210 mm reflector.

4Visibility

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Best season Jun – Aug (peak: Jul)

5Multiple Star System

Separation 1.5″
Companion Mag 7.4
Position Angle 245°
Star Colors A: Blue-white B: Yellow-white
Discoverer DJU 4

Separation over time

Measured 1953 → 2021 (68 y)
Separation drift 0.80" → 1.5" (+0.70")
Rate +0.0103" / y
PA drift 242° → 245° (+3°, +0.044°/y)

Slow change over generations — observable in lifetime comparisons.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 245°

A: 4.6 · B: 7.4 · Sep: 1.5″ · PA: 245° · N up, E right

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

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Size Comparison

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

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

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Stellar Fusion

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Light Travel Time Machine

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Relativistic Travel

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