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Guniibuu — Double Star in Ophiuchus

HIP 84405; 36 Ophiuchi

Observable Double Star Excellent (74/100)

Sep: 5.2", Companion: mag 5.1

Magnitude 5.1m DoubleStar Ophiuchus (Oph) Visible
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About Guniibuu

Description

36 Ophiuchi is a triple K-dwarf system about 19.5 light-years away. The two main components A and B are K1 V and K1 V stars almost identical in mass and luminosity (magnitudes 5.07 and 5.10), separated by 5–7″ in a 471-year orbit. A faint third component C lies 12 arc-minutes away and is a K5 V dwarf physically bound to the inner pair.

Observing Tips

Very pretty pair in any small telescope — two equal-magnitude orange K-stars, an unusual sight. Use 80×–150× to comfortably split AB. Component C is a wide field-of-view target, easy to identify because it shares the system's high proper motion (1.13″/yr).

History

Discovered as a binary by Sir John Herschel in 1837 during his Cape of Good Hope southern survey. Long studied as a benchmark for K-dwarf physics because the near-twin components allow direct comparison without the complications of unequal masses.

Fun Facts

All three components are slow rotators with active chromospheres — they appear chemically depleted in lithium, a hallmark of mature K-dwarfs that have churned their outer layers down to fusion temperatures over billions of years.

Observe

1Physical Properties

Magnitude 5.07
Spectral Type K0V
Star Color Orange (B-V 0.85)
Distance 17 ly

2Position & Identifiers

RA 17h 15m 20.8s
Dec -26° 36' 05.0"
Constellation Ophiuchus (Oph)
HR 6402
HIP 84405
HD 155886
SAO 185198
Flamsteed 36 Oph
Double Cat 10417

3How easy to split?

Primary 5.1 mag Companion 5.1 mag Separation 5.2″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
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 Quintuple D,E: optical

Components 5 (quintuple)
Component IDs AB
Separation 5.2″
Companion Mag 5.1
Companion Sp K1V
Position Angle 138°
Star Colors A: Orange B: Orange
Discoverer SHJ 243
AB 5.05 K0V, 5.08 K1V, 548.7y, a = 13.91". Mag. and colors for combined light, 4.34V, +0.855(B-V), +0.53(U-B), | +0.44(R-I).

Separation over time

Period: 470.9 y Eccentricity: 0.916 Now: 5.2", PA 137° + 0.06" in 5 years
0.00" 1.6" 3.1" 4.7" 6.2" 2025 2030 2035 2040 2045 5.2"

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

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 138°

A: 5.1 · B: 5.1 · Sep: 5.2″ · PA: 138° · 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

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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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14Stellar Notes

0.177".
15

Light Travel Time Machine

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Relativistic Travel

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