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Enif — Star in Pegasus

HIP 107315; Epsilon Pegasi; 8 Pegasi

Magnitude 0.7–3.5m Star Pegasus (Peg) Visible
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About Enif

Description

Enif is an orange supergiant of spectral type K2Ib at magnitude 2.39, the brightest star in Pegasus. Located about 670 light-years from Earth, it has a luminosity of roughly 6,700 times solar. Enif marks the nose or muzzle of the winged horse. It is a slow irregular variable and has been observed to produce rare flare events.

Observing Tips

Enif lies well west of the Great Square of Pegasus, marking the horse's muzzle. Its warm orange color is noticeable to the naked eye. The globular cluster M15 lies just 4 degrees to the northwest, making Enif a useful guide star. Best observed August through December.

History

The name Enif comes from the Arabic 'anf al-faras,' meaning 'the nose of the horse.' In 1972, Enif produced a remarkable flare event, briefly brightening by nearly 3 magnitudes to magnitude 0.7 — making it momentarily the brightest star in Pegasus by a wide margin.

Fun Facts

Enif's 1972 flare remains one of the most dramatic brightness eruptions ever observed in a supergiant star. For a few minutes, this normally modest star became one of the 20 brightest in the sky. The cause remains poorly understood.

Observe

1Physical Properties

Magnitude 2.39
Range 2.37 - 2.45
Variable Type LC
Spectral Type K2Ib-II supergiant
Star Color Red (B-V 1.53)
Distance 688 ly

2Position & Identifiers

RA 21h 44m 11.2s
Dec +09° 52' 30.0"
Constellation Pegasus (Peg)
HR 8308
HIP 107315
HD 206778
SAO 127029
Bayer Epsilon
Flamsteed 8 Peg
Variable ID Eps Peg
Double Cat 15268

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
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 Jul – Sep (peak: Aug)

5Survey Image

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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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15Stellar Notes

0.7 - 3.5V. 1.7m flare 1972 Sept. 26-7; fainter than normal following night.
ADS 15268AB optical.
Large infrared excess.
See HR 8232.
Ultraviolet FeII emission. MgII emissions indicate a cooler shell surrounding the supergiant. Barium marginally | overabundant.
ENIF; Enf; Enir; Al Anf; Os Pegasi; Fom.
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Light Travel Time Machine

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Relativistic Travel

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