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80 Tauri — Double Star in Taurus

Observable Double Star Fair (21/100)

Sep: 1.4", Companion: mag 8.1

Magnitude 5.6m DoubleStar Taurus (Tau) Visible
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Observe

1Physical Properties

Magnitude 5.58
Spectral Type F0V
Star Color Yellow-white (B-V 0.32)
Distance 105 ly

2Position & Identifiers

RA 04h 30m 08.6s
Dec +15° 38' 17.0"
Constellation Taurus (Tau)
HR 1422
HIP 20995
HD 28485
SAO 93970
Flamsteed 80 Tau
Double Cat 3264

3How easy to split?

Primary 5.6 mag Companion 8.1 mag Separation 1.4″
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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 210 mm reflector.

4Visibility

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Best season Oct – Dec (peak: Nov)

5Multiple Star System

Separation 1.4″
Companion Mag 8.1
Companion Sp G0V
Position Angle 17°
Star Colors A: Yellow-white B: Yellow
Discoverer STF 554
5.7 F0V, 7.98 G2V, 189.5y, a = 1.01" (alternates 180.0y, a = 1.00"; 170y, a = 1.029"). Combined mass 2.82 solar. | Speckle interferometric sep. 1.300" (1980.94).

Separation over time

Period: 172.5 y Eccentricity: 0.915 Now: 1.4", PA 14° -0.09" in 5 years
0.00" 0.41" 0.82" 1.2" 1.6" 2025 2030 2035 2040 2045 1.4"

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 17°

A: 5.6 · B: 8.1 · Sep: 1.4″ · PA: 17° · N up, E right

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

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6

Size Comparison

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7

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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

ADS 3264A, 30.5d.
In Hyades cluster; Mel 25 #80.
0.022".
15

Light Travel Time Machine

16

Relativistic Travel

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