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Beta Phoenicis — Double Star in Phoenix

Magnitude 3.3m DoubleStar Phoenix (Phe) Visible
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About Beta Phe

Description

Beta Phoenicis is a yellow giant of spectral type G8III at magnitude 3.31, the second brightest star in Phoenix. Located about 198 light-years from Earth, it has a luminosity of roughly 165 times solar. It is a spectroscopic binary.

Observing Tips

Beta Phe lies in the body of Phoenix, south of Sculptor. It pairs with the brighter Ankaa (Alpha Phe) to define this faint southern constellation. Only visible from the southern hemisphere and low northern latitudes. Best observed October through December.

History

Beta Phoenicis has no traditional proper name. Phoenix was created from Dutch navigators' observations and represents the mythical firebird that regenerates from its own ashes.

Fun Facts

The Phoenix constellation is one of the larger southern constellations created in the age of exploration, but it is faint enough that most northern-hemisphere observers have never seen it.

Observe

1Physical Properties

Magnitude 3.31
Spectral Type G8III giant
Star Color Orange (B-V 0.89)
Distance 27,180 ly

2Position & Identifiers

RA 01h 06m 05.0s
Dec -46° 43' 07.0"
Constellation Phoenix (Phe)
HR 322
HIP 5165
HD 6595
SAO 215365
Bayer Beta

3How easy to split?

Primary 3.3 mag Companion 4.2 mag Separation 0.8″
Sign in and configure your equipment and default location to see a personalized row.
Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. Hard Hard Hard
C8 203mm Hard Hard Hard
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

To reach "Medium" at Bortle 3, you'd need at least a 280 mm reflector.

4Visibility

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Best season Sep – Nov (peak: Oct)

5Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 0.8″
Companion Mag 4.2
Position Angle 67°
Star Colors A: Orange
Discoverer SLR 1
Mag. and color blend of close pair 4.2, 4.2v. C, 11.5v at 57".

Separation over time

Period: 170.7 y Eccentricity: 0.718 Now: 0.79", PA 62° + 0.08" in 5 years
0.00" 0.31" 0.62" 0.93" 1.2" 2025 2030 2035 2040 2045 0.79"

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 67°

A: 3.3 · B: 4.2 · Sep: 0.8″ · PA: 67° · N up, E right

Unresolved · 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

13

Stellar Absorption Spectrum

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

14

Stellar Fusion

Discover

15Stellar Notes

0.013".
16

Light Travel Time Machine

17

Relativistic Travel

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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