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HIP 92394 — Double Star in Pavo

Magnitude 6.1m DoubleStar Pavo (Pav) Visible
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1Physical Properties

Magnitude 6.06
Spectral Type B9.5IV-V subgiant
Star Color White (B-V 0.00)

2Position & Identifiers

RA 18h 49m 43.5s
Dec -72° 59' 41.0"
Constellation Pavo (Pav)
HR 7027
HIP 92394
HD 172881
SAO 257630

3How easy to split?

Primary 6.1 mag Companion 8.1 mag Separation 2.0″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard Hard Hard
150mm Newt. Medium+ Medium+ Medium+
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season May – Jul (peak: Jun)

5Multiple Star System

Separation 2.0″
Companion Mag 8.1
Position Angle 273°
Star Colors A: White B: Yellow-white
Discoverer R 314

Separation over time

Measured 1880 → 2015 (135 y)
Separation drift 1.0" → 2.0" (+1.00")
Rate +0.0074" / y
PA drift 260° → 273° (+13°, +0.096°/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 273°

A: 6.1 · B: 8.1 · Sep: 2.0″ · PA: 273° · N up, E right

At limit · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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6

Size Comparison

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8

Spectral Classification

9

Hertzsprung-Russell Diagram

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Stellar Lifecycle

11

Blackbody Spectrum

12

Stellar Absorption Spectrum

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

13

Stellar Fusion

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14Stellar Notes

Brighter component of visual double. Secondary of SB much fainter.
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