• by

Enif, Epsilon Pegasi (ε Peg) is an orange supergiant star located in the constellation Pegasus. It marks the muzzle of the mythical winged horse. With an average apparent magnitude of 2.399, Enif is the brightest star in Pegasus. It lies at an approximate distance of 690 light years from Earth.

Star type

Enif has the stellar classification K2 Ib, indicating a supergiant star appearing orange in colour. The star has a mass about 11.7 times that of the Sun and a radius 185 times solar. If placed at the centre of the solar system, it would extend between the orbits of Venus (154 – 157 R) and Earth (211 – 219 R).

With a surface temperature of 4,379 K, Enif is 3,895 times more luminous than the Sun. It has an absolute magnitude of -4.142 and a bolometric luminosity 12,250 times that of the Sun.

Enif has a projected rotational velocity of 8 km/s. Its estimated age is about 20 million years. Even though it is a young star, it will reach the end of its life cycle in the next few million years. It may be massive enough to be a supernova candidate, but it may also end its life as a neon-oxygen white dwarf.

epsilon pegasi, enif star

Enif (Epsilon Pegasi), image: Wikisky

The star is classified as a slow irregular variable (type LC). Its brightness varies from magnitude 0.7 to 3.5.

Enif has also shown dramatic changes in brightness on several occasions. In 1972, it briefly appeared as bright as Altair only to fade again 10 minutes later. Such superflares are extremely rare and their mechanism is not yet understood.

A 2010 study of young runaway stars revealed that Enif has a relatively high peculiar velocity (velocity relative to the surrounding interstellar medium) of 21.6 km/s-1.


Enif is believed to have formed in the same molecular cloud as the nearby yellow supergiants Sadalsuud (Beta Aquarii) and Sadalmelik (Alpha Aquarii), the brightest stars in the constellation Aquarius. The three stars lie at similar distances and share a space velocity that is taking them perpendicular to the Galactic plane. Sadalsuud is a supergiant of the spectral type G0 Ib located about 540 light years away, and Sadalmelik has the stellar classification G2 Ib and lies at a distance of 520 light years.

Enif is one of the 58 stars selected for navigation. Navigational stars have a special role in the field of celestial navigation because they are some of the brightest and most recognizable stars in the sky. The only other navigational star in Pegasus is Markab, Alpha Pegasi, one of the stars that form the Great Square of Pegasus.

Pegasus stars, image: Wikisky

Enif has two visual companions. One has an apparent magnitude of 12.80 and is separated by 83.2 arcseconds from the supergiant and the other is brighter, at magnitude 8.74, and located 144.6 arcseconds away. The stars do not share a common proper motion with Enif and are not physically related to the supergiant.

Enif is unofficially known as the Pendulum Star. The supergiant and the companion at a separation of 144.6 arcseconds are an example of the Pulfrich effect, a phenomenon that occurs when lateral movement of an object in a field of view is “seen” as having a depth component – appearing to approach and recede – when it is viewed with both eyes. The optical illusion is the result of the difference in signal timings between the eyes. If Enif and the companion star are observed in a telescope at a magnification of 60 to 100 and the telescope is lightly tapped so that the stars appear to move at right angles to the imaginary line connecting them, Enif appears to move up and down, as expected, while the companion appears to wildly bounce around to and fro. The pendulum-like oscillations are due to the fact that the companion is much fainter and it takes longer for its light to stimulate the retina. English astronomer John Herschel (1792 – 1871), who noted the phenomenon, suggested that the companion appears to traverse a larger arc when the telescope is tapped because it takes more time for its light to affect the eye and “the reversal of motion is first perceived in the larger object.”


The name Enif (pronunciation: /ˈiːnɪf/) comes from the Arabic word for “nose.” It refers to the star’s position in the constellation, marking the muzzle of Pegasus. The star was also known as Fum al Faras, meaning “the horse’s mouth,” and as Al Jahfalah, “the lip.” The former was translated into Latin as Os Equi.

The name Enif was approved by the International Astronomical Union’s (IAU) Working Group on Star Names (WGSN) July 20, 2016.

The Chinese know Epsilon Pegasi as 危宿三 (Wēi Sù sān), the Third Star of Rooftop. The Chinese Rooftop asterism is formed by Enif with Sadalmelik (Alpha Aquarii) and Biham (Theta Pegasi). It is one of the seven mansions of the Black Tortoise.


Enif is easy to find because it lies next to the Great Square of Pegasus, a conspicuous asterism outlining the main body of Pegasus. The star can be found in the area between Markab, the star at the southwest corner of the Great Square, and the constellation Delphinus, recognizable for its prominent kite-shaped pattern. Enif is the brightest star in this region of the sky.

find enif in the sky

Enif location, image: Wikisky

Enif is located just over three degrees southeast of Messier 15, also known as the Great Pegasus Cluster. The globular cluster is one of the brightest (mag. 6.2), densest and oldest clusters of its kind in the Milky Way. It lies 33,600 light years away and is 12 billion years old.

Enif and Messier 15, image: Wikisky


Enif is located in the constellation Pegasus. Pegasus is the third largest northern constellation and the seventh largest of all 88 constellations. It occupies 1,121 square degrees of the northern sky. Representing the winged horse from Greek mythology, it is one of the 48 Greek constellations, first listed by the astronomer Claudius Ptolemy in the 2nd century CE.

pegasus stars

Pegasus constellation, image: Roberto Mura

The constellation is dominated by the Great Square of Pegasus, a prominent asterism formed by three Pegasus stars – Algenib, Scheat and Markab – with Alpheratz, the brightest star in the neighbouring Andromeda.

Pegasus contains several bright deep sky objects: the globular cluster Messier 15 (mag. 6.2), the unbarred spiral galaxies NGC 7331 (mag. 10.4), NGC 7217 (mag. 11.0) and NGC 7742 (mag. 12.35), also known as the Fried Egg Galaxy, the barred spiral galaxy NGC 7479 (mag. 11.6), nicknamed the Propeller Galaxy, and the compact galaxy group HCG 92, also known as Stephan’s Quintet. The constellation also contains the Einstein Cross, a gravitationally lensed quasar located behind the lensing galaxy ZW 2237+030 and appearing in four images around the foreground galaxy.

Pegasus is also home to about a dozen star systems with confirmed exoplanets. These include 51 Pegasi, the first Sun-like star discovered to have a planet orbiting it.

The best time of year to observe the stars and deep sky objects in Pegasus is during the month of October.

The 10 brightest stars in the constellation are Enif (Epsilon Peg, mag. 2.399), Scheat (Beta Peg, mag. 2.42), Markab (Alpha Peg, mag. 2.48), Algenib (Gamma Peg, mag. 2.84), Matar (Eta Peg, mag. 2.95), Homam (Zeta Peg, mag. 3.414), Sadalbari (Mu Peg, mag. 3.514), Biham (Theta Peg, mag. 3.52), Iota Pegasi (mag. 3.77), and Lambda Pegasi (mag. 3.93).

Enif – Epsilon Pegasi

Spectral classK2 Ib
Variable typeSlow irregular variable (LC)
U-B colour index+1.722
B-V colour index+1.527
Apparent magnitude2.399 (0.7 – 3.5)
Absolute magnitude-4.142
Distance690 ± 20 light years (211 ± 8 parsecs)
Parallax4.73 ± 0.17 mas
Radial velocity3.39 ± 0.06 km/s
Proper motionRA: +26.92 mas/yr
Dec.: +0.44 mas/yr
Mass11.7 ± 0.8 M
Luminosity3,895 L
Bolometric luminosity12,250 L☉ 
Radius185 R
Temperature4,379 K
Metallicity-0.04 dex
Age20.0 ± 4.5 million years
Rotational velocity8 km/s
Surface gravity1.01 cgs
Right ascension21h 44m 11.15614s
Declination+09° 52′ 30.0311″
Names and designationsEnif, Epsilon Pegasi, ε Peg, 8 Pegasi, HD 206778, HR 8308, HIP 107315, GC 30431, GCRV 13654, FK5 815, BD+09°4891, SAO 127029, PPM 172188, CCDM J21441+0953A, IDS 21393+0925, IRAS 21417+0938, 2MASS J21441114+0952302, PLX 5242, TYC 1125-2186-1, AAVSO 2139+09, Gaia DR2 1765433632573306496