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V Puppis — Variable Star in Puppis

Observable Variable Star Excellent (70/100)

Range: 4.35 - 4.92, Period: 1.5d, Type: EB/SD

Magnitude 4.3–4.9m VariableStar Puppis (Pup) Visible
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1Physical Properties

Magnitude 4.41
Range 4.35 - 4.92
Period 34.9 hours
Variable Type Eclipsing Binary (Beta Lyrae-type)
Spectral Type B1Vp+B3IV:
Star Color Blue (B-V -0.17)

2Position & Identifiers

RA 07h 58m 14.4s
Dec -49° 14' 42.0"
Constellation Puppis (Pup)
HR 3129
HIP 38957
HD 65818
SAO 219226
Variable ID V Pup

3How easy to follow?

Magnitude 4.4 – 4.9 mag Amplitude 0.6 mag Period 1.45 d Type EB/SD
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Hard Hard V. hard+
50mm finder Medium Medium Medium
150mm scope Medium Medium Medium
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Dec – Feb (peak: Jan)

5Survey Image

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6Light Curve

7Comparison Stars

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9

Size Comparison

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10

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11

Spectral Classification

12

Hertzsprung-Russell Diagram

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13

Stellar Lifecycle

14

Blackbody Spectrum

15

Stellar Absorption Spectrum

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

16

Stellar Fusion

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17Stellar Notes

Comp. A of visual double, EB 4.74 - 5.25p, 1.4544877d, contact binary, equal components.
Component A of visual system, 1.4545d. Relative vel. 610k. Probably consists of two ellipsoids in nearly circular orbit | inclined 75d. Matter appears to stream from secondary to primary.
Member of Pleiades group.
Also classified B2II-III(n). Possible X-ray source 3U0750-49.
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