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33 Leonis Minoris — Double Star in Leo Minor

Magnitude 5.9m DoubleStar Leo Minor (LMi) Visible
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1Physical Properties

Magnitude 5.90
Spectral Type A0IV subgiant
Star Color White (B-V 0.11)

2Position & Identifiers

RA 10h 31m 51.4s
Dec +32° 22' 46.0"
Constellation Leo Minor (LMi)
HR 4124
HIP 51556
HD 91130
SAO 62101
Flamsteed 33 LMi
Double Cat 7813

3How easy to split?

Primary 5.9 mag Companion 11.8 mag Separation 58.9″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard V. hard+ V. hard
150mm Newt. Medium Hard+ Hard
C8 203mm Medium+ Medium Hard+
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Jan – Mar (peak: Feb)

5Multiple Star System

Separation 58.9″
Companion Mag 11.8
Position Angle 249°
Star Colors A: White
Discoverer HJ 482
Optical.

Separation over time

Measured 1827 → 2023 (196 y)
Separation drift 25.0" → 58.9" (+33.90")
Rate +0.1730" / y
PA drift 225° → 249° (+24°, +0.122°/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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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 249°

A: 5.9 · B: 11.8 · Sep: 58.9″ · PA: 249° · 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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