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Zeta Herculis — Double Star in Hercules

Observable Double Star Fair (30/100)

Sep: 1.6", Companion: mag 5.4

Magnitude 2.8m DoubleStar Hercules (Her) Visible
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About Zeta Her

Description

Zeta Herculis is a yellow subgiant of spectral type G0IV at magnitude 2.81 in Hercules. Located only about 35 light-years from Earth, it is one of the nearest bright stars and is a well-studied binary system with a G-type primary and a faint K-type companion orbiting every 34.5 years.

Observing Tips

Zeta Her lies at the southeastern corner of the Keystone asterism in Hercules. The binary companion can be resolved in a moderate telescope when near maximum separation. Best observed May through September when Hercules is high overhead.

History

Zeta Herculis has no widely used traditional proper name. Its proximity (35 light-years) and binary nature have made it a frequent target for high-resolution studies. It is also a prime example of a star that is evolving off the main sequence into a subgiant.

Fun Facts

At only 35 light-years, Zeta Her is one of the nearest binary star systems that can be visually resolved in a small telescope. Its primary is slightly more evolved than the Sun, giving astronomers a preview of the Sun's future evolution.

Observe

1Physical Properties

Magnitude 2.81
Spectral Type G2IV subgiant
Star Color Yellow (B-V 0.65)
Distance 35 ly

2Position & Identifiers

RA 16h 41m 17.2s
Dec +31° 36' 11.0"
Constellation Hercules (Her)
HR 6212
HIP 81693
HD 150680
SAO 65485
Bayer Zeta
Flamsteed 40 Her
Double Cat 10157

3How easy to split?

Primary 2.8 mag Companion 5.4 mag Separation 1.6″
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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

Separation 1.6″
Companion Mag 5.4
Position Angle 110°
Star Colors A: Yellow B: Orange
Discoverer STF2084
ADS 10157AB, 2.90 F9IV, 5.53 G7V, 34.49y, a = 1.355". ADS 10157A*, 10.5y, a = 0.08".

Separation over time

Period: 34.5 y Eccentricity: 0.463 Now: 1.6", PA 75° -0.32" in 5 years
0.00" 0.45" 0.90" 1.3" 1.8" 2025 2030 2035 2040 2045 1.6"

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 110°

A: 2.8 · B: 5.4 · Sep: 1.6″ · PA: 110° · N up, E right

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

Explore

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Size Comparison

Querying VizieR for stellar data…
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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

12

Blackbody Spectrum

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Stellar Absorption Spectrum

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

14

Stellar Fusion

Discover

15Stellar Notes

ADS 10157A is var. suspect NSV 7915.
ADS 10157A, 34.417y D, K 3.8k/s, V0 -69.9k/s, asini 590. Resolved by speckle interferometry.
Zeta Her group.
0.096".
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Light Travel Time Machine

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Relativistic Travel

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