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Betelgeuse — Variable Star in Orion

HIP 27989; Alpha Orionis; 58 Orionis

Observable Variable Star Excellent (66/100)

Range: 0.0 - 1.6, Period: 420.0d, Type: SRC

Magnitude 0.4–1.3m VariableStar Orion (Ori) Visible
Star Map
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About Betelgeuse

Description

Betelgeuse is a red supergiant of spectral type M1-2Ia-Iab at magnitude 0.5 (variable between about 0.0 and 1.6) in Orion. Located roughly 650 light-years from Earth, it is one of the largest stars known — with a diameter of roughly 1,000 times the Sun's, if placed at the center of our solar system its surface would extend beyond the orbit of Mars. It is a semi-regular variable star with multiple overlapping pulsation periods.

Observing Tips

Betelgeuse is the unmistakable orange-red star at Orion's upper-left shoulder. Its deep color contrasts dramatically with blue-white Rigel diagonally opposite. The color is obvious to the naked eye and striking in binoculars. Watch its brightness over months — it varies noticeably. Best observed December through March.

History

The name Betelgeuse is a corruption of the Arabic 'yad al-jawza,' meaning 'the hand of the central one.' Its enormous size was first measured interferometrically by Albert Michelson and Francis Pease in 1920, making it the first star (beyond the Sun) to have its diameter directly measured. The 'Great Dimming' of late 2019 to early 2020 made worldwide headlines.

Fun Facts

Betelgeuse is expected to explode as a Type II supernova sometime within the next 100,000 years. When it does, it will briefly outshine the full Moon and be visible in daylight. The Great Dimming of 2019-2020 was caused by a mass ejection that cooled into a dust cloud, temporarily blocking about two-thirds of the star's light.

Observe

1Physical Properties

Magnitude 0.50
Range 0.0 - 1.6
Period 420 days
Variable Type Semi-Regular Variable (Supergiant)
Spectral Type M4Ib supergiant
Star Color Deep ruby red (B-V 1.85)
Temperature 3479 K
Radius 887.0 R☉
Distance 489 ly

2Position & Identifiers

RA 05h 55m 10.3s
Dec +07° 24' 25.0"
Constellation Orion (Ori)
HR 2061
HIP 27989
HD 39801
SAO 113271
Bayer Alpha
Flamsteed 58 Ori
Variable ID Alp Ori
Double Cat 4506

3How easy to follow?

Magnitude 0.4 – 1.3 mag Amplitude 0.9 mag Period 420 d Type SRC
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Medium+ Medium+ Medium+
50mm finder Medium+ Medium+ Medium+
150mm scope Medium+ Medium+ Medium+
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Nov – Jan (peak: Dec)

5Survey Image

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6Light Curve

7Comparison Stars

Nearby stable stars for estimating brightness (AAVSO)

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Explore

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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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17Stellar Notes

ADS 4506A, SRc 0.40 - 1.3V, 2335d. Also superimposed waves 200-400d.
Components B-E all 11 to 14.5v at sep. 40" to 174" from A. D 13.5 at 77", optical. Speckle interferometric observations | in 1983 November (Karovska et al. 1986, ApJ, 308, 360) show A to be a triple system with closer companion at 0.06" | (mag. diff. 3.4 at H alpha) and more distant companion at 0.51" (mag. diff. 4.6 at H alpha).
ADS 4506A, 5.781y, K 3.08k/s, V0 +20.33k/s, asini 81.773.
Ultraviolet FeII emission. 5-micron observations indicate carbon monoxide. STRATOSCOPE II observations indicate infrared | H2O bands. UV observations from OAO-2 indicate C and O underabundant. MgII emissions indicate a cooler shell | surrounding the supergiant.
Expanding circumstellar shell, extending at least 29" or about 600 stellar radii. If rate constant, initial potassium | ejection about 2700 years ago. 2.85-cm radio emission indicates mass loss.
BETELGEUSE; Betelguex; Betelgeuze; Beteiguex; Al Mankib.
The first star whose diameter was measured with the interferometer, .047", by Michelson and Pease at Mt. Wilson in 1920.
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Light Travel Time Machine

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Relativistic Travel

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