34 Persei is around three times hotter than our Sun, with temperatures recorded at around 16,421 K. 48 Persei, also known as c Persei, is a Be star located at around 480 light-years away from us. Its active nucleus is a strong source of radio waves. Nu Persei has around 501% of our Sun’s mass, 2,062% of its radius, and it is 603.6 times brighter than our Sun. There are only two Messier Objects located in the constellation of Perseus, the open cluster Messier 34, and the planetary nebula Messier 76. He promised to rescue Andromeda if her parents would allow him to marry her. Due to its high rotational velocity, the star’s equatorial bulge is 6% wider than its polar radius. https://astrobackyard.com/wp-content/uploads/2020/03/perseus-constellation.jpg, https://upload.wikimedia.org/wikipedia/commons/9/9c/Sidney_Hall_-_Urania%27s_Mirror_-_Perseus.jpg, https://greekmythologytours.com/wp-content/uploads/2018/05/medusa-1366362_1280-1140×530.jpg, https://in-the-sky.org/images/constellations/con_PER_000.png, https://www.messier-objects.com/wp-content/uploads/2015/04/Messier-34.jpg, https://www.messier-objects.com/wp-content/uploads/2015/07/Messier-76.jpg, https://i.pinimg.com/originals/15/9a/f3/159af3b031ae3bc2663823bb10bdfb8c.jpg, https://www.astronomytrek.com/wp-content/uploads/2018/01/Mirfak.jpg, https://www.star-facts.com/wp-content/uploads/2019/10/Mirfak-location.jpg?189db0&189db0, https://nineplanets.org/wp-content/uploads/2020/02/1600px-Artist%E2%80%99s_impression_of_eclipsing_binary-1024×640.jpg, https://cdn.mos.cms.futurecdn.net/e3AYkGPcfNCgNCNyy75fXV.jpg, https://in-the-sky.org/image.php?style=medium&userimg=19910715_115920_fcf21531698b.png, https://i.pinimg.com/originals/e3/3c/e1/e33ce1e8ceb67d9be343e563f0e08917.jpg, https://www.star-facts.com/wp-content/uploads/2020/04/Algol-Gorgonea-Secunda-Gorgonea-Tertia-and-Gorgonea-Quarta.jpg?189db0&189db0, https://lh3.googleusercontent.com/proxy/IDV4OQYMhlaTSnK5ozvkrmI6Z5L8a6oCJ09rpC8kBveSeQbLBu4IADYLAAno0MWmSOuXlvdj_DRlY_DLXpMhEsTJOvlU, https://a4.pbase.com/o3/95/760195/1/88748119.nFn4vk48.Img_6802_cropped.jpg, https://upload.wikimedia.org/wikipedia/commons/thumb/b/be/Eta_Persei.jpg/640px-Eta_Persei.jpg, https://www.star-facts.com/wp-content/uploads/2020/04/Algol-1240×620.jpg?189db0&189db0, https://theskylive.com/sky/stars/finder-charts/nu-persei-finder-chart.png?c=1586769946, https://cdn.spacetelescope.org/archives/images/screen/opo9739a.jpg, https://mw1.google.com/mw-planetary/sky/skytiles_v1/108_44_7.jpg, https://66.media.tumblr.com/5887d0011c54ab03db8f08e94e074f87/tumblr_inline_pmbtort2LJ1rxan1s_1280.png, https://earthsky.org/upl/2016/01/capella.jpg, https://jumk.de/astronomie/img/x-persei.jpg, https://upload.wikimedia.org/wikipedia/commons/thumb/1/11/GKPersei-MiniSuperNova-20150316.jpg/771px-GKPersei-MiniSuperNova-20150316.jpg, https://blackholes.stardate.org/images/GRO_J0422_32_artist-impression.jpg, https://www.researchgate.net/profile/David_Turner7/publication/258710533/figure/fig1/AS:392567989522437@1470606910743/The-SRC-variable-S-Persei-according-to-the-Digitized-Sky-Survey-Moncrieff-2011_Q640.jpg, https://upload.wikimedia.org/wikipedia/commons/2/21/Tr_2.png, https://theskylive.com/sky/stars/finder-charts/epsilon-persei-finder-chart.png?c=1586709080, https://upload.wikimedia.org/wikipedia/commons/thumb/b/b1/29_Persei.jpg/640px-29_Persei.jpg, https://theskylive.com/sky/stars/star-images/4/496_800.jpg, https://theskylive.com/sky/stars/star-images/9/989_800.jpg, https://theskylive.com/sky/stars/star-images/10/1044_800.jpg, https://theskylive.com/sky/stars/star-images/10/1087_800.jpg, https://www.astrophoto.at/images/epsPer_starmap.jpg, https://apod.nasa.gov/apod/image/0901/clusters_2_ritter.jpg, https://lh3.googleusercontent.com/proxy/eyKKFIe5SCt06yUTfby03Yz3Bt5A7PH9OAsDssqb05fiK21T6SanSGaOxhRzsAD3GKT19ZdERWclXtK7I9kXWkY, https://apod.nasa.gov/apod/image/1511/NGC1333_aae.jpg, https://upload.wikimedia.org/wikipedia/commons/4/4f/PIA23405-PerseusMolecularCloud-Annotated.jpg, https://lh3.googleusercontent.com/proxy/vFIWNljPn4FTeUaLaFpYc0mCm95-9jHADT_UOZrvGuOJBrxWvyowvuZJtkXpV9Ghi8RgEWQ1_cnZ00QsQ3v0vVG5vlx4on87dIaLRa6Kz1MdG0pTyM8y04U6NQ, https://upload.wikimedia.org/wikipedia/commons/7/74/NGC1260_-_hst_13029_20_R814GB625.png, https://chandra.harvard.edu/photo/2020/perseus/perseus.jpg, https://www.star-facts.com/wp-content/uploads/2019/10/Mirfak.jpg?189db0&189db0, https://galaxyzooblog.files.wordpress.com/2014/01/ngc1265_radio_opt.jpg, https://cdn.spacetelescope.org/archives/images/screen/heic0817b.jpg, https://upload.wikimedia.org/wikipedia/commons/9/94/NGC_1058_-_HST09042_n2-R814GB450.png, https://sites.google.com/site/rickkellysimagesandprose/_/rsrc/1472869100321/home/astrophotography/color-astrophotography/ic-348-readjustment/IC%20348%20RGB%20StackNEW%20AJNRv3-650.jpg, https://www.esa.int/var/esa/storage/images/esa_multimedia/images/2017/08/perseid_meteor_shower/17907680-2-eng-GB/Perseid_meteor_shower.jpg. It was named after the hero Perseus in Greek mythology. It has an apparent magnitude of 2.12, which sometimes drops to magnitude 3.4 every 2.86 days. It is a yellow main sequence star of spectral type G0V. Gorgonea Tertia has around 500% of our Sun’s mass ( but it is losing mass fastly), 15,000% of our Sun’s radius (thus it is 300 times bigger), and it is 2,290 times brighter than our Sun. This star is also more than four times hotter than our Sun, with temperatures reaching 26,500 K. In addition to this, the star is also a fast spinner, having a rotational velocity of 155 km / 96.3 mi per second. The Andromeda constellation is fittingly located between the Perseus constellation and the Cassiopeia constellation. It was the host galaxy of the supernova SN 2006gy, one of the brightest ever recorded. This galaxy is located at around 19 million light-years away from us, and it has an apparent magnitude of 10.35. [6], In Neo-Assyrian Babylonia (911–605 BC), the constellation of Perseus was known as the Old Man constellation (SU.GI), then associated with East in the MUL.APIN, an astronomical text from the 7th century. Algol is one of the first non-nova variable stars to be discovered, and its variability gives its name to a class of eclipsing variable stars, known as Algol variables. It reached a magnitude of 0.2, which was the brightest nova of modern times until the nova Aquilae 1918 occurred. [41], GRO J0422+32 (V518 Persei) is another X-ray binary in Perseus. Perseus is near several constellations whose names derive from the adventures of the Greek hero, known as the Perseus Group. The brightest star in Perseus is the supergiant star Mirfak / Alpha Peresi, which has an apparent magnitude of 1.806, and it also hosts an exoplanet. Three stars can be distinguished in the Algol star system, and they are designated as Beta Persei Aa1, Aa2, and Ab. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky. DY Persei has excesses of carbon relative to oxygen in its spectrum, which causes dramatic changes in the atmospheric chemistry that is visible in its spectrum. [71], M34 is an open cluster that appears at magnitude 5.5,[72] and is approximately 1,500 light-years from Earth. The combined apparent magnitude of this star system is 6.778. The Perseus Constellations has four neighbors: Aries and Taurus to the south, Cassiopeia to the north, Auriga to the east, and the Andromeda galaxy to the west The Constellation of Perseus for Kids The constellation of Perseus is among the oldest listed in star catalogues. [18] These two are separated by only 0.05 astronomical units (AU)—five percent of the distance between the Earth and Sun; the main dip in brightness arises when the larger fainter companion passes in front of the hotter brighter primary. Its helium has been fused into heavier elements and its core is composed of carbon and oxygen. The Perseid meteorite shower, the most impressive in the sky, does not actually come from the constellation Perseus but is the rubble left behind from the Comet Swift-Tuttle, the supposed parent of the Perseids. [17] Perseus is the 24th largest constellation in the sky, out of the 88 modern constellations, stretching for around 615 square degrees. 34 Persei is a binary star located at around 540 light-years away from us. There are only two meteor showers associated with the constellation of Perseus, namely the Perseids, and the September Perseids. [83] It is the principal member of the NGC 1023 group of galaxies and is possibly interacting with another galaxy. It has an apparent magnitude of 6.0. It is visible to the naked eye under the right conditions. It can be seen with the naked eye under the right conditions. [78] It is very difficult to observe visually because its low surface brightness makes it appear dimmer than most other emission nebulae. [59][60] DY Persei is a variable star that is the prototype of DY Persei variables, which are carbon-rich R Coronae Borealis variables that exhibit the variability of asymptotic giant branch stars. The pile of corpses prior to their interment was represented by Jīshī (積屍, Pi Persei), the sixth paranatellon of the house. Camelopardalis and Cassiopeia are to the north of Perseus, while Andromeda and Triangulum are to the west. GRO J0422+32 is an X-ray nova and black hole candidate that was discovered in 1992. It has an apparent magnitude that varies from magnitude 10.5 to 16.0. Andromeda is among the 48 constellations that Ptolemy, the second-century Greco-Roman astronomer listed and until now is recognized among the 88 constellations in existence. A supergiant of spectral type F5Ib located around 590 light-years away from Earth,[24] Mirfak has 5,000 times the luminosity and 42 times the diameter of our Sun. Representing the head of the Gorgon Medusa in Greek mythology, it was called Horus in Egyptian mythology[16] and Rosh ha Satan ("Satan's Head") in Hebrew. The primary star is a B-type main-sequence star. They are located at around 7,500 light-years away from us and have an apparent magnitude of 3.7 and 3.8 respectively. The Double Cluster located in Perseus consists of the open clusters NGC 869 and NGC 884. [45] Further analysis in 2012 calculated a mass of 2.1 solar masses, which raises questions as to what the object actually is as it appears to be too small to be a black hole. DY Persei is a variable carbon star located at around  1,500 parsecs from us. Perseus is one of the larger northern constellations. The constellation of Perseus contains many interesting stars, among them, there is Mirfak, the brightest star in the constellation, Algol, the demon star, Phi Persei, Delta Persei,  Psi Persei, 48 Persei, Epsilon Persei, 29 Persei, 30 Persei, 31 Persei, 34 Persei, Iota Persei, Zeta Persei, Atik, X Persei, V518 Persei, V718 Persei, GK Persei, Menkhib, Gorgonea Tertia, S Persei, RS Persei, or the DY Persei, among many others. [89] The September Epsilon Perseids, discovered in 2012, are a meteor shower with an unknown parent body in the Oort cloud. Gorgonea Tertia is located at around 308 light-years away from us, and it has an apparent magnitude of +3.39. X Persei has around 1,550% of our Sun’s mass, 650% of its radius, and it is 29,000 times brighter than our Sun. Perseus, the nephew of the king of the city of Argos noticed her as he was sailing by and immediately fell in love with her. The brightest star in Perseus is the supergiant star Mirfak / Alpha Peresi, which has an apparent magnitude of 1.806, and it also hosts an exoplanet. It has an apparent magnitude of 2.93, making it the fourth brightest member of the Perseus constellation. Covering 615 square degrees, it ranks twenty-fourth of the 88 constellations in size. Miram is a K-type supergiant star, that has around 13,400% of our Sun’s radius, making it 268 times bigger than our Sun, and it is 4,130 times brighter than our Sun. Perseus is commonly depicted as holding the head of Medusa in one hand, and a jeweled dagger in the other. Perseus and Andromeda married, and they had six sons, one of which, namely Perses, is said to be the founder and ancestor of the kings of Persia. Perseus returned triumphantly with Andromeda to the island of Seriphos, where he found his mother and Dictys sheltering in a temple from the tyranny of King Polydectes. [56][57][58] The stars are not visible to the naked eye; SU Persei, the brightest of the three, has an apparent magnitude of 7.9[58] and thus is visible through binoculars. It has an apparent magnitude of 12.6, being the brightest member of the Perseus Cluster of galaxies. 10 Best Places To Visit in Ethiopia. Because of this rotation, the star is deformed – while its polar radius is 550% greater than our Sun’s, its equatorial radius is 800% greater. [37] Once thought to be a member of the Perseus OB2 Association,[38] Omicron Persei (Atik[39]) is a multiple star system with a combined visual magnitude of 3.85. With 2.2 times its luminosity only people that named it were those of the NGC is! Its high rotational velocity of around 400 stars to have planetary systems constellation of perseus and andromeda away us. 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