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Marfik — Double Star in Ophiuchus

Lambda Oph

Observable Double Star Fair (30/100)

Sep: 1.3", Companion: mag 5.2

Magnitude 3.8m DoubleStar Ophiuchus (Oph) Visible
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About Marfik

Description

Marfik, Lambda Ophiuchi, is a binary star system about 173 light-years away in the constellation Ophiuchus. The primary is a B9/A0 III subgiant and the companion is an A-type dwarf at 1.5 arcseconds separation. Combined magnitude is 3.82. The orbital period is about 130 years, making Marfik a fine binary for long-term observation.

Observing Tips

Marfik sits in the eastern part of Ophiuchus, near the boundary with Serpens Cauda. The 1.5-arcsecond double challenges small scopes — needs a 4-inch or larger at 200x on steady seeing nights. The two components are similar in brightness, providing a pleasing matched pair. Best observed May through September.

History

The name Marfik comes from the Arabic "al-mirfaq," meaning "the elbow" — referring to Ophiuchus's elbow in the traditional figure. The IAU adopted the name in 2017.

Fun Facts

The Marfik binary has been observed since the 19th century, and its orbit is now well-determined through accumulated position measurements. Its 130-year period means that a single human lifetime can witness roughly two-thirds of a full revolution — a modest but real demonstration of gravitational orbital motion.

Observe

1Physical Properties

Magnitude 3.82
Spectral Type B9/A0 III
Star Color Blue-white (B-V 0.01)
Distance 173 ly

2Position & Identifiers

RA 16h 30m 54.8s
Dec +01° 59' 02.0"
Constellation Ophiuchus (Oph)
HR 6149
HIP 80883
HD 148857
SAO 121658
Bayer Lambda
Flamsteed 10 Oph
Double Cat 10087

3How easy to split?

Primary 3.8 mag Companion 5.2 mag Separation 1.3″
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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)

5Multiple Star System Quadruple D: optical

Components 4 (quadruple)
Component IDs AB
Separation 1.3″
Companion Mag 5.2
Companion Sp A0V
Position Angle 46°
Star Colors A: Blue-white B: Blue-white
Discoverer STF2055
AB 4.16 A1V, 5.22 A4V. 129.87y, a = 0.970" or 126.78y, a = 0.95", combined mag., colors. Component C, 11.0v, 120" CPM.

Separation over time

Period: 129.0 y Eccentricity: 0.615 Now: 1.3", PA 51° -0.06" in 5 years
0.00" 0.39" 0.78" 1.2" 1.6" 2025 2030 2035 2040 2045 1.3"

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 46°

A: 3.8 · B: 5.2 · Sep: 1.3″ · PA: 46° · N up, E right

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

Explore

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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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15Stellar Notes

0.019".
Marfic; Marfik; Marsic.
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Light Travel Time Machine

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Relativistic Travel

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