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HIP 42455 — Double Star in Pyxis

Magnitude 6.1m DoubleStar Pyxis (Pyx) Visible
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1Physical Properties

Magnitude 6.13
Spectral Type F1IV subgiant
Star Color Yellow-white (B-V 0.42)
Distance 136 ly

2Position & Identifiers

RA 08h 39m 22.1s
Dec -36° 36' 25.0"
Constellation Pyxis (Pyx)
HR 3434
HIP 42455
HD 73900
SAO 199473

3How easy to split?

Primary 6.1 mag Companion 7.9 mag Separation 1.0″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard+
150mm Newt. Hard Hard Hard
C8 203mm Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 230 mm reflector.

4Visibility

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Best season Dec – Feb (peak: Jan)

5Multiple Star System

Separation 1.0″
Companion Mag 7.9
Position Angle 241°
Star Colors A: Yellow-white B: Yellow
Discoverer I 314
6.5 F3IV, 7.6 F6V, 66.5y, a = 0.527". Combined mag., color.

Separation over time

Period: 65.8 y Eccentricity: 0.824 Now: 0.98", PA 240° -0.01" in 5 years
0.00" 0.28" 0.56" 0.84" 1.1" 2025 2030 2035 2040 2045 0.98"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 241°

A: 6.1 · B: 7.9 · Sep: 1.0″ · PA: 241° · N up, E right

Unresolved · 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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Relativistic Travel

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