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R Leonis — Variable Star in Leo

Observable Variable Star Showpiece (82/100)

Range: 4.40 - 11.00, Period: 312.2d, Type: M

Magnitude 4.4–11.3m VariableStar Leo Visible
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1Physical Properties

Magnitude 6.02
Range 4.40 - 11.00
Period 312 days
Variable Type Mira (Long-period Pulsating)
Spectral Type M8IIIe bright giant
Star Color Red (B-V 1.30)
Distance 163 ly

2Position & Identifiers

RA 09h 47m 33.5s
Dec +11° 25' 44.0"
Constellation Leo
HR 3882
HIP 48036
HD 84748
SAO 98769
Variable ID R Leo

3How easy to follow?

Magnitude 4.4 – 11.3 mag Amplitude 6.9 mag Period 312.2 d Type M
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Imp. Imp. Imp.
50mm finder V. hard+ V. hard Imp.
150mm scope 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)

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

M 4.4 - 11.3v, 309.95d. Period varies from 307.4 to 317.8d. Discovered by Koch in 1782.
R-I corresponds to 7.52V, +1.41(B-V), +0.28(U-B).
Wolf 630 group.
SiO maser. H2O bands. Silicate emission. Also classified M6e-M9.5IIIe.
Speckle interferometer observations show abrupt variations in diameter as a function of wavelength, interpreted as due | to large opacity of TiO. 0.032" at 5400A to 0.054" at 7300A to 0.030" at 7400A. Occultation diam. = 0.067", the | largest measured angular diameter of any star other than the Sun.
17

Light Travel Time Machine

18

Relativistic Travel

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Visibility scores assume a 150 mm Newton at Bortle 4.

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