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NV Puppis — Double Star in Puppis

Observable Double Star Good (54/100)

Sep: 241.6", Companion: mag 5.1

Magnitude 4.6–4.8m DoubleStar Puppis (Pup) Visible
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1Physical Properties

Magnitude 4.66
Range 4.58 - 4.78
Variable Type Gamma Cassiopeiae (Eruptive Be Star)
Spectral Type B2V+B3IVne
Star Color Blue (B-V -0.10)

2Position & Identifiers

RA 07h 18m 18.4s
Dec -36° 44' 03.0"
Constellation Puppis (Pup)
HR 2787
HIP 35363
HD 57150
SAO 197824
Variable ID NV Pup

3How easy to split?

Primary 4.7 mag Companion 5.1 mag Separation 241.6″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
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)

5Multiple Star System Quadruple

Components 4 (quadruple)
Component IDs AB
Separation 241.6″
Companion Mag 5.1
Companion Sp B3IV
Position Angle 102°
Star Colors A: Blue B: Blue
Discoverer JC 10

Separation over time

Measured 1846 → 2011 (165 y)
Separation drift 238.7" → 241.6" (+2.90")
Rate +0.0176" / y
PA drift 97° → 102° (+5°, +0.030°/y)

Apparent motion is significant on a human timescale — worth revisiting in a decade.

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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32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 102°

A: 4.7 · B: 5.1 · Sep: 241.6″ · PA: 102° · N up, E right

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

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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

Amp. 0.18V.
Shell star. Strong H alpha and FeII emission.
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