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Fawaris — Double Star in Cygnus

HIP 97165; Delta Cygni; 18 Cygni

Observable Double Star Good (56/100)

Sep: 2.8", Companion: mag 6.3

Magnitude 2.9m DoubleStar Cygnus (Cyg) Visible
Star Map
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About Fawaris

Description

Delta Cygni is a binary star system at magnitude 2.87 in Cygnus, consisting of a blue-white subgiant (B9.5IV) and a yellow-white companion (F1V). Located about 165 light-years from Earth, the pair orbits every 780 years. It marks the western wing of the Swan.

Observing Tips

Delta Cyg lies at the western wing-tip of Cygnus, part of the Northern Cross. A moderate telescope can resolve the pair when seeing is steady. The constellation Cygnus is one of the best for exploring the summer Milky Way. Best observed June through November.

History

Delta Cygni has no traditional proper name. Cygnus the Swan is one of the most prominent summer constellations, identified with the mythological swan into which Zeus transformed himself. The Milky Way runs directly through the constellation.

Fun Facts

Delta Cyg will become the north pole star around AD 11,250 as Earth's axis precesses. It will be one of the brighter pole stars in the precession cycle, comparable in brightness to Polaris.

Observe

1Physical Properties

Magnitude 2.87
Spectral Type A0IV subgiant
Star Color Blue-white (B-V -0.03)
Distance 171 ly

2Position & Identifiers

RA 19h 44m 58.5s
Dec +45° 07' 51.0"
Constellation Cygnus (Cyg)
HR 7528
HIP 97165
HD 186882
SAO 48796
Bayer Delta
Flamsteed 18 Cyg
Double Cat 12880

3How easy to split?

Primary 2.9 mag Companion 6.3 mag Separation 2.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard Hard Hard
150mm Newt. Medium Medium Medium
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 Jun – Aug (peak: Jul)

5Multiple Star System Triple F: optical

Components 3 (triple)
Component IDs AB
Separation 2.8″
Companion Mag 6.3
Position Angle 214°
Star Colors A: Blue-white B: Yellow
Discoverer STF2579
AB 2.91 B9.5III, 6.33 F1V, 827.6y, a = 3.20".

Separation over time

Period: 657.2 y Eccentricity: 0.440 Now: 2.8", PA 212° + 0.05" in 5 years
0.00" 0.86" 1.7" 2.6" 3.5" 2025 2030 2035 2040 2045 2.8"

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 214°

A: 2.9 · B: 6.3 · Sep: 2.8″ · PA: 214° · 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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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 12880A is NSV 12381, 2.85 - 2.89V. Component B is NSV 12380, 6.5 ->8.5v.
Color excess E(B-V) = +0.05.
0.021".
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Light Travel Time Machine

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Relativistic Travel

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