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Athebyne — Double Star in Draco

HIP 80331; Eta Draconis; 14 Draconis

Magnitude 2.7m DoubleStar Draco (Dra) Visible
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About Athebyne

Description

Eta Draconis is a yellow giant of spectral type G8IIIab at magnitude 2.74 in Draco. Located about 92 light-years from Earth, it has a luminosity of roughly 60 times solar. It lies in the body of the Dragon, between the head (marked by Eltanin) and the long, winding tail.

Observing Tips

Eta Dra lies in the body of Draco, which winds between the Big and Little Dippers. It is circumpolar from mid-northern latitudes. Its warm yellow color is apparent in binoculars. The constellation Draco requires dark skies to trace its full serpentine form. Best placed high in summer evenings.

History

Eta Draconis has no widely used traditional name. Draco is one of the oldest constellations, recognized since Babylonian and Egyptian times. Around 2800 BC, the star Thuban (Alpha Dra) was the pole star, making the entire constellation more prominent.

Fun Facts

Eta Dra is one of the brightest stars in Draco's long, winding body, which extends nearly 180 degrees across the northern sky — from the head near Vega all the way around the Little Dipper to the tail between the Big and Little Bears.

Observe

1Physical Properties

Magnitude 2.74
Spectral Type G8III-IV giant
Star Color Orange (B-V 0.91)
Distance 92 ly

2Position & Identifiers

RA 16h 23m 59.5s
Dec +61° 30' 51.0"
Constellation Draco (Dra)
HR 6132
HIP 80331
HD 148387
SAO 17074
Bayer Eta
Flamsteed 14 Dra
Double Cat 10058

3How easy to split?

Primary 2.7 mag Companion 8.2 mag Separation 4.7″
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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 Triple D,F: optical

Components 3 (triple)
Component IDs ABxC
Separation 4.7″
Companion Mag 8.2
Companion Sp K1V
Position Angle 142°
Star Colors A: Orange C: Orange
Discoverer STT 312

Separation over time

Measured 1843 → 2016 (173 y)
Separation drift 4.4" → 4.7" (+0.30")
Rate +0.0017" / y
PA drift 150° → 142° (-8°, -0.046°/y)

Essentially fixed on human timescales — the same view your grandchildren will see.

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 142°

A: 2.7 · B: 8.2 · Sep: 4.7″ · PA: 142° · N up, E right

Resolved · 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

Discover

15Stellar Notes

ADS 10058A, var. suspect NSV 7713; ADS 10058B, var. suspect NSV 7712, 8.8v, dK2, amp. about 2v.
0.014".
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Light Travel Time Machine

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Relativistic Travel

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