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VV Cephei — Star in Cepheus

Magnitude 4.8–5.4m Star Cepheus (Cep) Visible
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1Physical Properties

Magnitude 4.91
Range 4.73 - 5.55
Period 7430 days
Variable Type Eclipsing Binary (Algol-type)
Spectral Type M2Iaep+B8Ve
Star Color Red (B-V 1.77)
Distance 815 ly

2Position & Identifiers

RA 21h 56m 39.1s
Dec +63° 37' 32.0"
Constellation Cepheus (Cep)
HR 8383
HIP 108317
HD 208816
SAO 19753
Variable ID VV Cep

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Medium+ Medium Hard+
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Jul – Sep (peak: Aug)

5Survey Image

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6

Size Comparison

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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

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14Stellar Notes

EA 4.80 - 5.36V, 6.65 - 7.46p, 7430d. Also slow oscillations, amp. 0.15, per. 13.7y and amp. 0.03, per. 349d. Red | observations indicate Sr amp. 0.4m, 58d. H alpha varies in 118.37d, period stable over 20y interval. This is probably | the pulsation period of the red component. Amplitude varies in period 825d or more. The blue companion may be | intrinsically variable. VV Cep also magnetic variable.
A* var. M2Iab, B6IIe. Combined mag., colors. Absolute magnitudes based on astrometric and spectroscopic data are | -4.0V for red component, -2.3 for the blue.
7430.5d, K 19.4k/s, V0 -20.2k/s, msin3i 18.0, asini 1860. The SB secondary is probably also the visual | companion. Mass transfer from red star to the hot companion. SB unresolved by speckle interferometry at 4-meter Mayall | telescope in 1975-6.
Cep OB2.
Companion variously classified B9, B8Ve, and B6II.
15

Light Travel Time Machine

16

Relativistic Travel

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