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Tau Tauri — Double Star in Taurus

Observable Double Star Good (53/100)

Sep: 62.5", Companion: mag 7.0

Magnitude 4.3m DoubleStar Taurus (Tau) Visible
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1Physical Properties

Magnitude 4.28
Spectral Type B3V
Star Color Blue (B-V -0.13)
Distance 192 ly

2Position & Identifiers

RA 04h 42m 14.7s
Dec +22° 57' 25.0"
Constellation Taurus (Tau)
HR 1497
HIP 21881
HD 29763
SAO 76721
Bayer Tau
Flamsteed 94 Tau

3How easy to split?

Primary 4.3 mag Companion 7.0 mag Separation 62.5″
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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 Oct – Dec (peak: Nov)

5Multiple Star System Quintuple

Components 5 (quintuple)
Separation 62.5″
Companion Mag 7.0
Position Angle 214°
Star Colors A: Blue
Discoverer S 455
AB CPM, 4.3, 8.9v sep. 0.1", 28y? C, 7.3A1V at 63" vsini 100k/s, physical. D. W. Dunham gives 4.9, 5.6v sep. 0.1" and | 4.9, 6.4 sep. 0.0005".

Separation over time

Measured 1777 → 2017 (240 y)
Separation drift 60.0" → 62.5" (+2.50")
Rate +0.0104" / y
PA drift 212° → 214° (+2°, +0.008°/y)

Slow change over generations — observable in lifetime comparisons.

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 214°

A: 4.3 · B: 7.0 · Sep: 62.5″ · PA: 214° · N up, E right

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

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7

Size Comparison

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8

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9

Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

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

14

Stellar Fusion

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15Stellar Notes

2.9565d, K 53.6k/s, V0 +12.3k/s, msin3i 2.96, asini 2.18. Resolved by speckle interferometry 1983.93, | sep. 0.26".
Cas-Tau OB1.
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Light Travel Time Machine

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Relativistic Travel

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