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TU Canum Venaticorum — Variable Star in Canes Venatici

Observable Variable Star Excellent (67/100)

Range: 5.50 - 6.20, Period: 44.2d, Type: SRB

Magnitude 5.5–6.6m VariableStar Canes Venatici (CVn) Visible
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1Physical Properties

Magnitude 5.84
Range 5.50 - 6.20
Period 44 days
Variable Type Semi-Regular Variable (Late-type Giant)
Spectral Type M5III giant
Star Color Red (B-V 1.55)

2Position & Identifiers

RA 12h 54m 56.5s
Dec +47° 11' 48.0"
HR 4909
HIP 63024
HD 112264
SAO 44383
Variable ID TU CVn

3How easy to follow?

Magnitude 5.6 – 6.6 mag Amplitude 1.1 mag Period 44.2 d Type SRB
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye V. hard+ V. hard V. hard
50mm finder Medium+ Medium+ Medium+
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Feb – Apr (peak: Mar)

5Survey Image

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6Light Curve

7Comparison Stars

Nearby stable stars for estimating brightness (AAVSO)

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8

Size Comparison

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9

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10

Spectral Classification

11

Hertzsprung-Russell Diagram

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12

Stellar Lifecycle

13

Blackbody Spectrum

14

Stellar Absorption Spectrum

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

15

Stellar Fusion

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16Stellar Notes

SRb 5.55 - 6.6V, 7.2 - 7.7p, 50d.
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