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Sabik — Double Star in Ophiuchus

HIP 84012; Eta Ophiuchi; 35 Ophiuchi

Magnitude 2.4m DoubleStar Ophiuchus (Oph) Visible
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About Sabik

Description

Sabik is a white star of spectral type A2V at magnitude 2.43 in Ophiuchus. Located about 84 light-years from Earth, it is actually a close binary system with two A-type stars orbiting each other every 88 years. The combined luminosity is about 39 times solar.

Observing Tips

Sabik lies in the southern part of Ophiuchus, roughly between Antares and Rasalhague. It is a white star of moderate brightness. The binary companion can be resolved in a moderate telescope when the stars are near maximum separation. Best observed June through September.

History

The name Sabik comes from the Arabic, possibly meaning 'the preceding one.' Sabik has been an important navigational star due to its brightness and position near the ecliptic. It was one of the 57 navigational stars used in traditional celestial navigation.

Fun Facts

Sabik is one of the 57 traditional navigational stars selected for celestial navigation tables. Its position near the ecliptic means planets regularly pass near it, and it is occasionally occulted by the Moon.

Observe

1Physical Properties

Magnitude 2.43
Spectral Type A2IV-V subgiant
Star Color White (B-V 0.06)
Distance 88 ly

2Position & Identifiers

RA 17h 10m 22.7s
Dec -15° 43' 29.0"
Constellation Ophiuchus (Oph)
HR 6378
HIP 84012
HD 155125
SAO 160332
Bayer Eta
Flamsteed 35 Oph
Double Cat 10374

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
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 May – Jul (peak: Jun)

5Multiple Star System Quadruple D: optical

Components 4 (quadruple)
Component IDs AB
Separation 0.3″
Companion Mag 3.3
Companion Sp A1IV
Position Angle 222°
Star Colors A: White B: White
Discoverer BU 1118
AB 3.0 A2V, 3.5 A3V, 88y, a = 0.86". Combined mag., colors.

Separation over time

Period: 87.8 y Eccentricity: 0.942 Now: 0.30", PA 32° + 0.06" in 5 years
0.00" 0.12" 0.24" 0.37" 0.49" 2025 2030 2035 2040 2045 0.30"

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

Explore

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Size Comparison

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Compare Stars

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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

Discover

15Stellar Notes

0.022".
Sabik.
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Light Travel Time Machine

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Relativistic Travel

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