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Sarin — Double Star in Hercules

HIP 84379; Delta Herculis; 65 Herculis

Magnitude 3.1m DoubleStar Hercules (Her) Visible
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About Sarin

Description

Sarin is a white subgiant of spectral type A3IV at magnitude 3.14 in Hercules. Located about 75 light-years from Earth, it has a luminosity of roughly 26 times solar. It is a spectroscopic binary with a period of about 10 years. Sarin forms the southwestern corner of the Keystone asterism.

Observing Tips

Sarin marks one of the four corners of the Keystone in Hercules — the trapezoidal asterism used to find the great globular cluster M13. M13 lies along the western side of the Keystone, between Sarin and Eta Her. Best observed May through September.

History

The name Sarin is of uncertain origin. The Keystone asterism is the most important feature of Hercules for amateur astronomers, as it serves as the guide to finding both M13 and M92, two magnificent globular clusters.

Fun Facts

M13, the Great Hercules Cluster, lies about one-third of the way from Eta Her to Sarin along the Keystone's western edge. This makes Sarin one of the most useful guide stars in all of amateur astronomy.

Observe

1Physical Properties

Magnitude 3.14
Range 3.12 - 3.14
Period 2.0 hours
Variable Type Delta Scuti (Pulsating)
Spectral Type A1IVn supergiant
Star Color White (B-V 0.08)
Distance 74 ly

2Position & Identifiers

RA 17h 15m 01.9s
Dec +24° 50' 21.0"
Constellation Hercules (Her)
HR 6410
HIP 84379
HD 156164
SAO 84951
Bayer Delta
Flamsteed 65 Her
Double Cat 10424

3How easy to split?

Primary 3.1 mag Companion 8.3 mag Separation 14.0″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium+ Medium+ Medium+
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)

5Light Curve

6Multiple Star System Quadruple optical

Components 4 (quadruple)
Component IDs AB
Separation 14.0″
Companion Mag 8.3
Position Angle 293°
Star Colors A: White B: Yellow-white
Discoverer STF3127
ADS 10424B, dG4, optical.

Separation over time

Measured 1779 → 2023 (244 y)
Separation drift 33.8" → 14.0" (-19.80")
Rate -0.0811" / y
PA drift 163° → 293° (+130°, +0.533°/y)

Apparent motion is significant on a human timescale — worth revisiting in a decade.

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 293°

A: 3.1 · B: 8.3 · Sep: 14.0″ · PA: 293° · 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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16Stellar Notes

Sarin.
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Light Travel Time Machine

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Relativistic Travel

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