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2 Puppis — Double Star in Puppis

Magnitude 6.1m DoubleStar Puppis (Pup) Visible
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1Physical Properties

Magnitude 6.07
Spectral Type A2V
Star Color White (B-V 0.11)

2Position & Identifiers

RA 07h 45m 29.1s
Dec -14° 41' 27.0"
Constellation Puppis (Pup)
HR 3010
HIP 37843
HD 62864
SAO 153363
Flamsteed 2 Pup
Double Cat 6348

3How easy to split?

Primary 6.1 mag Companion 6.7 mag Separation 16.7″
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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 Triple C: optical

Components 3 (triple)
Component IDs AB
Separation 16.7″
Companion Mag 6.7
Companion Sp A1V
Position Angle 340°
Star Colors A: White B: White
Discoverer STF1138
Binary with HR 3009.

Separation over time

Measured 1782 → 2019 (237 y)
Separation drift 17.4" → 16.7" (-0.70")
Rate -0.0030" / y
PA drift 339° → 340° (+1°, +0.004°/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 340°

A: 6.1 · B: 6.7 · Sep: 16.7″ · PA: 340° · N up, E right

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

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Size Comparison

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

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

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Stellar Fusion

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