|Symbolism||the Winged Horse / Pegasus|
|Right ascension||21h 12.6m to 00h 14.6m|
|Declination||+2.33° to +36.61°|
|Area||1121 sq. deg. (7th)|
|Main stars||9, 17|
|Stars with planets||12|
|Stars brighter than 3.00m||5|
|Stars within 10.00 pc (32.62 ly)||3|
|Brightest star||ε Peg (Enif) (2.38m)|
|Nearest star||EQ Peg
(20.38 ly, 6.25 pc)
|Meteor showers||July Pegasids|
|Visible at latitudes between +90° and −60°.
Best visible at 21:00 (9 p.m.) during the month of October.
Pegasus is a constellation in the northern sky, named after the winged horse Pegasus in Greek mythology. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations.
With an apparent magnitude varying between 2.37 and 2.45, the brightest star in Pegasus is the orange supergiant Epsilon Pegasi, also known as Enif, which marks the horse's muzzle. Alpha (Markab), Beta (Scheat), and Gamma (Algenib), together with Alpha Andromedae (Alpheratz or Sirrah) form the large asterism known as the Square of Pegasus. Twelve star systems have been found to have exoplanets.
The Babylonian constellation IKU (field) had four stars of which three were later part of the Greek constellation Hippos (Pegasus). Pegasus, in Greek mythology, was a winged horse with magical powers. One myth regarding his powers says that his hooves dug out a spring, Hippocrene, which blessed those who drank its water with the ability to write poetry. Pegasus was the one who delivered Medusa's head to Polydectes, after which he travelled to Mount Olympus in order to be the bearer of thunder and lightning for Zeus. Eventually, he became the horse to Bellerophon, who was asked to kill the Chimera and succeeded with the help of Athena and Pegasus. Despite this success, after the death of his children, Bellerophon asked Pegasus to take him to Mount Olympus. Though Pegasus agreed, he plummeted back to Earth after Zeus either threw a thunderbolt at him or made Pegasus buck him off. In ancient Persia, Pegasus was depicted by al-Sufi as a complete horse facing east, unlike most other uranographers, who had depicted Pegasus as half of a horse, rising out of the ocean. In al-Sufi's depiction, Pegasus's head is made up of the stars of Lacerta the lizard. Its right foreleg is represented by β Peg and its left foreleg is represented by η Peg, μ Peg, and λ Peg; its hind legs are marked by 9 Peg. The back is represented by π Peg and μ Cyg, and the belly is represented by ι Peg and κ Peg.
In Chinese astronomy, the modern constellation of Pegasus lies in The Black Tortoise of the north (北方玄武), where the stars were classified in several separate asterisms of stars. Epsilon and Theta Pegasi are joined with Alpha Aquarii to form Wei 危 "rooftop", with Theta forming the roof apex.
Covering 1121 square degrees, Pegasus ranks 7th of the 88 constellations in size. Pegasus is bordered by Andromeda to the north and east, Lacerta to the north, Cygnus to the northwest, Vulpecula, Delphinus and Equuleus to the west, Aquarius to the south and Pisces to the south and east. The three-letter abbreviation for the constellation, as adopted by the IAU in 1922, is 'Peg'. The official constellation boundaries, as set by Eugène Delporte in 1930, are defined as a polygon of 35 segments. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 21h 12.6m and 00h 14.6m, while the declination coordinates are between 2.33° and 36.61°. Its position in the Northern Celestial Hemisphere means that the whole constellation is visible to observers north of 53°S.[a]
Pegasus is dominated by an asterism in the shape of a rough square, although one of the stars, Delta Pegasi or Sirrah, is now officially considered to be part of Andromeda, (α Andromedae) and is more usually called "Alpheratz". Traditionally, the body of the horse consists of a quadrilateral formed by the stars α Peg, β Peg, γ Peg, and α And. The front legs of the winged horse are formed by two crooked lines of stars, one leading from η Peg to κ Peg and the other from μ Peg to 1 Pegasi. Another crooked line of stars from α Peg via θ Peg to ε Peg forms the neck and head; ε is the snout.
Bayer catalogued what he counted as 23 stars in the constellation, giving them the Bayer designations Alpha to Psi. He saw Pi Pegasi as one star, and was uncertain of its brightness, wavering between magnitude 4 and 5. Flamsteed labelled this star 29 Pegasi, but Bode concluded that the stars 27 and 29 Pegasi should be Pi1 and Pi2 and that Bayer had seen them as a single star. Flamsteed added lower case letters e through to y, omitting A to D as they had been used on Bayer's chart to designate neighbouring constellations and the equator. He number 89 stars with Flamsteed designations, though 6 and 11 turned out to be stars in Aquarius. Within the constellation's borders, there are 177 stars brighter than or equal to apparent magnitude 6.5.[b]
Epsilon Pegasi, also known as Enif, marks the horse's muzzle. The brightest star in Pegasus, is an orange supergiant of spectral type K21b that is around 12 times as massive as the Sun and lies around 690 light-years distant from Earth. It is an irregular variable, its apparent magnitude varying between 2.37 and 2.45. Lying near Enif is AG Pegasi, an unusual star that brightened to magnitude 6.0 around 1885 before dimming to magnitude 9. It is composed of a red giant and white dwarf, estimated to be around 2.5 and 0.6 times the mass of the Sun respectively. With its outburst taking over 150 years, it has been described as the slowest nova ever recorded.
Zeta, Xi, Rho and Sigma Pegasi mark the horse's neck. The brightest of these with a magnitude of 3.4 is Zeta, also traditionally known as Homam. Lying seven degrees southwest of Markab, it is a blue-white main sequence star of spectral type B8V located around 209 light-years distant. Xi lies 2 degrees northeast, and is a yellow-white main sequence star of spectral type F7V with a red dwarf companion. Theta Pegasi marks the horse's eye. Also known as Biham, it is a 3.43-magnitude white main sequence star of spectral type A2V, around 25 times as luminous as the Sun and 2.3 times its diameter.
Alpha (Markab), Beta (Scheat), and Gamma (Algenib), together with Alpha Andromedae (Alpheratz or Sirrah) form the large asterism known as the Square of Pegasus. The brightest of these, Alpheratz was also known as both Delta Pegasi and Alpha Andromedae before being placed in Andromeda in 1922 with the setting of constellation boundaries. The second brightest star is Scheat, a red giant of spectral type M2.5II-IIIe located around 196 light-years away from Earth. It has expanded until it is some 95 times as large, and has a total luminosity of 1500 times that of the Sun. Beta Pegasi is a semi-regular variable that varies from magnitude 2.31 to 2.74 over a period of 43.3 days. Markab and Algenib are blue-white stars of spectral types B9III and B2IV located 133 and 391 light-years distant respectively. Appearing to have moved off the main sequence as their core hydrogen supply is being or has been exhausted, they are enlarging and cooling to eventually become red giant stars. Markab has an apparent magnitude of 2.48, while Algenib is a Beta Cephei variable that varies between magnitudes 2.82 and 2.86 every 3 hours 38 minutes, and also exhibits some slow pulsations every 1.47 days.
Eta and Omicron Pegasi mark the left knee and Pi Pegasi the left hoof, while Iota and Kappa Pegasi mark the right knee and hoof. Also known as Matar, Eta Pegasi is the fifth-brightest star in the constellation. Shining with an apparent magnitude of 2.94, it is a multiple star system composed of a yellow giant of spectral type G2 and a yellow-white main sequence star of spectral type A5V that are 3.2 and 2.0 times as massive as our Sun. The two revolve around each other every 2.24 years. Farther afield is a binary system of two G-type main sequence stars, that would take 170,000 years to orbit the main pair if they are in fact related.
IK Pegasi is a close binary comprising an A-type main-sequence star and white dwarf in very close orbit; the latter a candidate for a future type Ia supernova as its main star runs out of core hydrogen fuel and expands into a giant and transfers material to the smaller star.
Twelve star systems have been found to have exoplanets. 51 Pegasi was the first Sun-like star discovered to have an exoplanet companion; 51 Pegasi b (unofficially named Bellerophon) is a hot Jupiter close to its sun, completing an orbit every four days. Spectroscopic analysis of HD 209458 b, an extrasolar planet in this constellation has provided the first evidence of atmospheric water vapor beyond the solar system, while extrasolar planets orbiting the star HR 8799 also in Pegasus are the first to be directly imaged. V391 Pegasi is a hot subdwarf star that has been found to have a planetary companion.
|Markab||α||Arabic||the saddle of the horse|
|Homam||ζ||Arabic||man of high spirit|
|Matar||η||Arabic||lucky rain of shooting stars|
|Sadalbari||μ||Arabic||luck star of the splendid one|
M15 (NGC 7078) is a globular cluster of magnitude 6.4, 34,000 light-years from Earth. It is a Shapley class IV cluster, which means that it is fairly rich and concentrated towards its center. M15 was discovered in 1746 by Jean-Dominique Maraldi.
NGC 7331 is a spiral galaxy located in Pegasus, 38 million light-years distant with a redshift of 0.0027. It was discovered by musician-astronomer William Herschel in 1784 and was later one of the first nebulous objects to be described as "spiral" by William Parsons. Another of Pegasus's galaxies is NGC 7742, a Type 2 Seyfert galaxy. Located at a distance of 77 million light-years with a redshift of 0.00555, it is an active galaxy with a supermassive black hole at its core. Its characteristic emission lines are produced by gas moving at high speeds around the central black hole.
Pegasus is also noted for its more unusual galaxies and exotic objects. Einstein's Cross is a quasar that has been lensed by a foreground galaxy. The elliptical galaxy is 400 million light-years away with a redshift of 0.0394, but the quasar is 8 billion light-years away. The lensed quasar resembles a cross because the gravitational force of the foreground galaxy on its light creates four images of the quasar. Stephan's Quintet is another unique object located in Pegasus. It is a cluster of five galaxies at a distance of 300 million light-years and a redshift of 0.0215. First discovered by Édouard Stephan, a Frenchman, in 1877, the Quintet is unique for its interacting galaxies. Two of the galaxies in the middle of the group have clearly begun to collide, sparking massive bursts of star formation and drawing off long "tails" of stars. Astronomers have predicted that all five galaxies may eventually merge into one large elliptical galaxy.
USS Pegasus (AK-48) and USS Pegasus (PHM-1) are United States navy ships named after the constellation "Pegasus".
- While parts of the constellation technically rise above the horizon to observers between the 53°S and 87°S, stars within a few degrees of the horizon are to all intents and purposes unobservable.
- Objects of magnitude 6.5 are among the faintest visible to the unaided eye in suburban-rural transition night skies.
- "Pegasus, Constellation Boundary". The Constellations (International Astronomical Union). Retrieved 13 February 2014.
- Thuston, Hugh (1996). Early Astronomy. Springer. p. 3. ISBN 978-0-387-94822-5.
- Staal 1998, pp. 27–32
- Ridpath, Ian. "Charting the Chinese sky". Star Tales. self-published. Retrieved 21 May 2014.
- Schlegel 1967, pp. 233-34.
- Russell, Henry Norris (1922). "The New International Symbols for the Constellations". Popular Astronomy 30: 469. Bibcode:1922PA.....30..469R.
- Ian Ridpath. "Constellations: Lacerta–Vulpecula". Star Tales. self-published. Retrieved 29 November 2014.
- Wagman 2003, p. 235.
- Wagman 2003, p. 236.
- Wagman 2003, p. 448.
- Bortle, John E. (February 2001). "The Bortle Dark-Sky Scale". Sky & Telescope. Sky Publishing Corporation. Retrieved 29 November 2014.
- "Epsilon Pegasi -- Pulsating Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 12 February 2014.
- Otero, Sebastian Alberto (7 June 2011). "Epsilon Pegasi". AAVSO Website. American Association of Variable Star Observers. Retrieved 12 February 2014.
- Kenyon, Scott J.; Mikolajewska, Joanna; Mikolajewski, Maciej; Polidan, Ronald S.; Slovak, Mark H. (1993). "Evolution of the symbiotic binary system AG Pegasi - The slowest classical nova eruption ever recorded" (PDF). Astronomical Journal 106 (4): 1573–98. Bibcode:1993AJ....106.1573K. doi:10.1086/116749.
- Wagman 2003, p. 513.
- Kaler, James B. (16 November 2007). "Homam (Zeta Pegasi)". Stars. University of Illinois. Retrieved 13 February 2014.
- Kaler, James B. (15 October 2010). "Biham (Theta Pegasi)". Stars. University of Illinois. Retrieved 14 February 2014.
- "Beta Pegasi -- Pulsating Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 13 February 2014.
- Kaler, James B. (22 May 2009). "Scheat (Beta Pegasi)". Stars. University of Illinois. Retrieved 13 February 2014.
- Watson, Christopher (25 August 2009). "Beta Pegasi". AAVSO Website. American Association of Variable Star Observers. Retrieved 13 February 2014.
- "Alpha Pegasi -- Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 13 February 2014.
- "Gamma Pegasi -- Variable Star of Beta Cephei type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 13 February 2014.
- Kaler, James B. "Markab (Alpha Pegasi)". Stars. University of Illinois. Retrieved 13 February 2014.
- Kaler, James B. "Algenib (Gamma Pegasi)". Stars. University of Illinois. Retrieved 13 February 2014.
- Otero, Sebastian Alberto (26 March 2011). "Gamma Pegasi". AAVSO Website. American Association of Variable Star Observers. Retrieved 13 February 2014.
- Kaler, James B. "Matar (Eta Pegasi)". Stars. University of Illinois. Retrieved 14 February 2014.
- Levy 2005, pp. 157-158.
- Wilkins, Jamie; Dunn, Robert (2006). 300 Astronomical Objects. Firefly Books. ISBN 978-1-55407-175-3.
- Ian Ridpath and Wil Tirion (2007). Stars and Planets Guide, Collins, London ISBN 978-0-00-725120-9. Princeton University Press, Princeton. ISBN 978-0-691-13556-4.
- Schlegel, Gustaaf (1967) . Uranographie Chinoise (in French). Taipei, Republic of China: Ch'eng Wen Publishing Company.
- Wagman, Morton (2003). Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. Blacksburg, Virginia: The McDonald & Woodward Publishing Company. ISBN 978-0-939923-78-6.
|Wikimedia Commons has media related to:|
- The Deep Photographic Guide to the Constellations: Pegasus
- Star Tales – Pegasus
- Pegasus Constellation at Constellation Guide