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10 Draconis — Double Star in Draco

DoubleStar Draco (Dra) Visible
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Observe

1Physical Properties

Magnitude 4.65
Range 4.52 - 4.67
Variable Type LB:
Spectral Type M3.5III
Star Color Red (B-V 1.58)
Distance 233 ly

2Position & Identifiers

RA 13h 51m 25.9s
Dec +64° 43' 24.0"
Constellation Draco (Dra)
HR 5226
HIP 67627
HD 121130
Flamsteed 10 Dra
Variable ID CU Dra
Double Cat 9039

3How easy to split?

Primary 4.7 mag Companion 11.7 mag Separation 88.9″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard V. hard+ V. hard
150mm Newt. Medium 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 Mar – May (peak: Apr)

5Multiple Star System Triple

Components 3 (triple)
Component IDs AC
Separation 88.9″
Companion Mag 11.7
Position Angle 61°
Star Colors A: Red
Discoverer HJ 3342

Separation over time

Measured 1879 → 2015 (136 y)
Separation drift 86.2" → 88.9" (+2.70")
Rate +0.0199" / y
PA drift 65° → 61° (-4°, -0.029°/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 61°

A: 4.7 · B: 11.7 · Sep: 88.9″ · PA: 61° · N up, E left

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

Explore

6

Size Comparison

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7

Compare Stars

8

Spectral Classification

9

Hertzsprung-Russell Diagram

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10

Stellar Lifecycle

11

Blackbody Spectrum

12

Stellar Absorption Spectrum

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

13

Stellar Fusion

Discover

14Stellar Notes

Lb? 4.52 - 4.67V.
15

Light Travel Time Machine

16

Relativistic Travel

Survey Image

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Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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