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Epsilon Persei — Double Star in Perseus

Magnitude 2.9–3.0m DoubleStar Perseus (Per) Visible
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About Epsilon Per

Description

Epsilon Persei is a hot blue binary star of spectral type B0.5V at magnitude 2.89 in Perseus. Located about 540 light-years from Earth, it consists of a massive B-type primary and a fainter A-type companion. Combined luminosity is about 26,000 times solar.

Observing Tips

Epsilon Per lies in the body of Perseus, south of the Alpha Persei Cluster. It is a blue-white star in a rich Milky Way field. Best observed October through February when Perseus is well-placed in the evening sky.

History

Epsilon Persei has no widely used traditional name. It is a member of the Perseus OB1 association, a group of young massive stars in the Perseus arm of the Milky Way.

Fun Facts

Epsilon Per is one of the hottest bright stars in Perseus, with a surface temperature of about 28,000 K. Despite appearing as a single point of light, it is actually a close binary whose orbit has been studied through speckle interferometry.

Observe

1Physical Properties

Magnitude 2.89
Range 2.89 - 2.91
Period 4.6 hours
Variable Type Beta Cephei (Pulsating)
Spectral Type B0III/IV giant
Star Color Blue (B-V -0.18)
Distance 637 ly

2Position & Identifiers

RA 03h 57m 51.2s
Dec +40° 00' 37.0"
Constellation Perseus (Per)
HR 1220
HIP 18532
HD 24760
SAO 56840
Bayer Epsilon
Flamsteed 45 Per
Variable ID Eps Per
Double Cat 2888

3How easy to split?

Primary 2.9 mag Companion 8.9 mag Separation 8.8″
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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 Oct – Dec (peak: Nov)

5Light Curve

6Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 8.8″
Companion Mag 8.9
Companion Sp A2V
Position Angle 12°
Star Colors A: Blue B: White
Discoverer STF 471
AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s.

Separation over time

Measured 1821 → 2020 (199 y)
Separation drift 8.6" → 8.8" (+0.20")
Rate +0.0010" / y
PA drift 10° → 12° (+2°, +0.010°/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 12°

A: 2.9 · B: 8.9 · Sep: 8.8″ · PA: 12° · N up, E right

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

Explore

8

Size Comparison

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Spectral Classification

11

Hertzsprung-Russell Diagram

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Stellar Lifecycle

13

Blackbody Spectrum

14

Stellar Absorption Spectrum

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

15

Stellar Fusion

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16Stellar Notes

Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods | found are submultiples of 26.9 hrs or 1.12d.
Color excess E(B-V) = +0.10.
Cas-Tau OB1; member of Pleiades group.
17

Light Travel Time Machine

18

Relativistic Travel

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