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Mira — Variable Star in Cetus

68 Cet

Observable Variable Star Showpiece (86/100)

Range: 2.0 - 10.1, Period: 332.0d, Type: M

Magnitude 2.0–10.1m VariableStar Cetus (Cet) Visible
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About Mira

Description

Mira (Omicron Ceti) is the prototype long-period variable star, the most famous pulsating red giant in the sky. Its spectral type is M7IIIe and its brightness varies dramatically between about magnitude 2.0 and 10.0 over a period of roughly 332 days. Located about 420 light-years from Earth, Mira swells and shrinks as it pulsates, with a diameter varying between about 400 and 500 times the Sun's.

Observing Tips

When near maximum brightness, Mira is easily visible to the naked eye in Cetus — look for it roughly between Diphda and Menkar. At minimum, it requires a telescope. Check predictions for its brightness cycle (available in astronomy magazines and online) to know when to look. Its deep red color is visible in binoculars. Best observed October through January when Cetus is well-placed.

History

The name Mira means 'wonderful' or 'astonishing' in Latin, given by Johannes Hevelius in 1662. Its variability was first noted by David Fabricius in 1596, making it the first variable star discovered (other than supernovae). Mira defined an entire class of long-period variables — the Mira variables.

Fun Facts

Mira has a comet-like tail of gas stretching 13 light-years behind it, discovered by NASA's GALEX ultraviolet telescope in 2007. The tail is material shed by Mira as it races through space at 130 km/s, leaving a trail of its own atmosphere behind it like a cosmic comet.

Observe

1Physical Properties

Magnitude 3.04
Range 2.0 - 10.1
Period 332 days
Variable Type Mira (Long-period Pulsating)
Spectral Type M5/6 IIIe
Star Color Red (B-V 1.42)
Temperature 2943 K
Radius 370.1 R☉
Distance 418 ly

2Position & Identifiers

RA 02h 19m 20.7s
Dec -02° 58' 39.0"
Constellation Cetus (Cet)
HR 681
HIP 10826
HD 14386
SAO 129825
Flamsteed 68 Cet
Variable ID Omi Cet
Double Cat 1778

3How easy to follow?

Magnitude 2.0 – 10.1 mag Amplitude 8.1 mag Period 332 d Type M
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Imp. Imp. Imp.
50mm finder Hard+ Hard V. hard+
150mm scope Easy Easy Medium+
Easy Medium Hard Very hard Impossible

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

4Visibility

Set a location in User Settings to see visibility data.

Best season Sep – Nov (peak: Oct)

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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Compare Stars

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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

Discover

17Stellar Notes

Two variables: Mira and VZ Cet. Mira, ADS 1778A, M 2.0 - 10.1v, 331.96d; var. CO emission from circumstellar envelope. | Speckle interferometry indicates large abrupt variation of diameter as a function of wavelength. Hydrogen lines vary on | time scale of 1-2 days. Mira was discovered to be variable by Fabricius in 1596, the first such variable discovered. | ADS 1778P, Ne "Novoides" class, VZ Cet, 9.5 - 12.0v, dBe.
AP var. M7IIIe, var. dBe, 400y, a = 0.85". The faint companion was first predicted in 1920 by Joy on the basis of a | slightly displaced blue secondary spectrum. First seen by Aitken in 1923. Visible only when Mira is faint. Light | variations on scale of hours superimposed by variations of 10-15 min. and rare flares of 2 min. duration. Components B, | 13v at 73" and C, optical.
The tabulated magnitude and colors refer to a time near maximum. Another determination at 6.99V gives B-V +1.56, | U-B +0.12, R-I +3.08.
Stratoscope II observations indicate infrared H2O bands. SiO maser source. Technetium found in spectrum. Also | classified M5e-M9e.
0.0058". Masses A 15.7, P 4.0 solar.
MIRA.
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Light Travel Time Machine

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Relativistic Travel

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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