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06 Febbraio 2021

zeta ursae majoris

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It was discovered by the German astronomer Johann Georg Liebknecht on December 2, 1722. The two members of the double, visible separately with keen eyesight, are called Mizar and Alcor. The predicted doubling of the lines of Zeta Ursae Majoris on December 8th was confirmed on that day by each of three photographs. In Indian astronomy, Mizar is known as Vashishtha, one of the Saptarishi (Seven Sages), credited as the main author of Mandala 7 (book 7) of Rigveda. The seven stars are Alpha Ursae Majoris, Beta Ursae Majoris, Gamma Ursae Majoris, Delta Ursae Majoris, Epsilon Ursae Majoris, Zeta Ursae Majoris and Eta Ursae Majoris. Zeta Ursae Majoris (Mizar): A multiple star. The name was approved by the International Astronomical Union’s (IAU) Working Group on Star Names (WGSN) on June 30, 2016. It … The Zeta Ursae Majoris star system consists of two pairs of spectroscopic binary stars appearing as a visual double star. The Northern Dipper is a Chinese asterism that corresponds to the Big Dipper. The hunters are represented by the stars of the Big Dipper’s handle and four stars in the constellation Boötes, while the stars of the Dipper’s bowl represent the bear, and the semi-circular pattern of the constellation Corona Borealis outlines the bear’s cave. Ursae is contained in 9 matches in Merriam-Webster Dictionary. Mizar, also called Zeta Ursae Majoris, first star found (by the Italian astronomer Giovanni Battista Riccioli in 1650) to be a visual binary—i.e., to consist of two optically distinguishable components revolving around each other. Mizar is located in the same area of the sky as two famous bright galaxies, the Pinwheel Galaxy (Messier 101) and the Whirlpool Galaxy (Messier 51). Related to Zeta Ursae Maioris: 80 Ursae Majoris. The two symbolize marriage and the closeness it brings to a couple. 3.14), and Theta Ursae Majoris (mag. The stars orbit each other with a period of 20.586 days (20 days, 12 hours and 55 minutes). eta Ursae Majoris Starfield, that name really sounds nice! 82.9 ± 0.6 light years (25.4 ± 0.2 parsecs), Mizar, Zeta Ursae Majoris, ζ UMa, 79 Ursae Majoris, HIP 65378, CCDM J13240+5456, WDS J13239+5456, BD+55 1598, IRAS 13219+5511. It is the upper left star of the bowl. They were nicknamed “horse and rider” in the Arabic-speaking world. We also use third-party cookies that help us analyze and understand how you use this website. 1.86), Mizar (Zeta UMa, mag. Mizar, Alkaid, Alioth, M51 and M101, image: Wikisky. The two components of the Mizar B star system revolve around each other about every six months (175.55 days). In the myth, Mizar represents Chickadee, one of the hunters, and Alcor his cooking pot, in which he cooks the bear. Mizar is located in Ursa Major constellation, representing the Great Bear. Mizar, Zeta Ursae Majoris (ζ UMa), is a quadruple star system in Ursa Major. Necessary cookies are absolutely essential for the website to function properly. Mizar A and Mizar B take 5,000 or more years to complete an orbit and come within 380 astronomical units of each other. Based on photometric data, some light variability was suspected by R. A. Baker in 1926, and it may be a Delta Scuti variable. Liebknecht thought the star was a planet and he named it after his patron, Louis V, Landgrave of Hesse-Darmstadt. Ludwig’s Star is an 8th magnitude star of the spectral type A8/F0 III, about five times more distant than Mizar and Alcor. Zeta Ursae Majoris → Mizar (star system) – "Mizar" is the common name for this system, and also the official name recognised by the International Astronomical Union for its Aa component . In Chinese Taoism, Mizar is known as the star of Lu (禄) and associated with prosperity and influence. : COMMENTS: This is the famous double star in the middle of the handle of the Big Dipper. One of the warzones that the main character, John Perry, is deployed to is Colony 622, a fictional terrestrial planet in the 47 Ursae Majoris … The two components of Mizar A both show overabundances of strontium and silicon. It was most likely discovered by the Italian mathematician Benedetto Castelli, who asked his friend and teacher Galileo Galilei to observe the star in 1617. Every star has a unique orbit and evolution. The multiple star system zeta UMa (called Mizar - from the arabian word for girdle) belongs to the most famous multiple stars in the sky. Both stars are members of the Ursa Major Moving Group and share a common proper motion through space. Mizar or Zeta Ursae Majoris (Zet UMa) is the 4th brightest naked eye star in the constellation Ursa Major.With an apparent magnitude of 2.23, Mizar is the 70th brightest star in the entire sky (see: 50 Brightest Stars ).Its absolute magnitude is 0.33 and its distance is 78 light years.The Equinox J2000 equatorial coordinates are RA = 13h 23m 55.5s, Dec = +54° 55' 31". Tähti on Otavan kattilan varren keskimmäinen tähti. ζ Ursae Majoris (zeta Ursae Majoris) ζ Ursae Majoris is a variable and multiple star in the constellation of Ursa Major . The star has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.28. They are referred to either as Zeta Ursae Majoris A and Zeta Ursae Majoris B or as Zeta1 Ursae Majoris and Zeta2 Ursae Majoris. Merak is located in relatively close physical proximity to Phecda (11 light years or 3.4 parsecs) and it is even closer to the star 37 Ursae Majoris … This brilliant white and pale emerald star also appears in the handle of the Big Dipper asterism. Both stars have the stellar classification A2Vp, which means that they are hydrogen-fusing dwarfs, appearing white or blue-white in colour. The 10 brightest stars in Ursa Major are Alioth (Epsilon UMa, mag. 1.79), Alkaid (Eta UMa, mag. Zeta Ursae Majoris synonyms, Zeta Ursae Majoris pronunciation, Zeta Ursae Majoris translation, English dictionary definition of Zeta Ursae Majoris. 1.77), Dubhe (Alpha UMa, mag. They are also commonly called Mizar A and Mizar B. Zeta Ursae Minoris, which is Latinized from ζ Ursae Minoris, is a single[12] star in the northern circumpolar constellation of Ursa Minor, forming the northernmost part of the bowl in this "little dipper" asterism. Mizar (Zeta Ursae Majoris), image: Wikisky. It is mandatory to procure user consent prior to running these cookies on your website. Mizar (Zeta Ursae Majoris) and Alcor (80 Ursae Majoris) form a true binary that can be seen without optical aid as a stellar pair in the handle of the Big Dipper asterism of Ursa Major. Trong tiếng Trung nó được gọi là 開陽 (sao Khai Dương). Mizar hay Zeta Ursae Majoris (ζ UMa / ζ Ursae Majoris), là một hệ 4 sao nằm ở vị trí thứ hai tính từ cuối cánh tay đòn của chòm sao Đại Hùng.Tên gọi Mizar có nguồn gốc từ tiếng Ả Rập ميزر mi'zar, nghĩa là cạp [quần, váy] hay đai. Mizar, Zeta Ursae Majoris (ζ UMa), is a quadruple star system in Ursa Major. This would make the visual double a sextuple system, but it has not yet been proven beyond question that the stars really are gravitationally bound, mainly because the stars’ exact distances from Earth are still uncertain. It forms an optical double with the 4th-magnitude Alcor with a separation of 12′. Alcor is known as Arundhati, his wife. Zeta2 Ursae Majoris was discovered to be a spectroscopic binary in 1908. Mizar on ensimmäinen tunnettu … 47 Ursae Majoris c is known as Wolf,and there are two fictional terrestrial planets, Fox and Raven, which orbit inward from Bear and Wolf. Mizar (Zeta Ursae Majoris) is the fourth brightest star in the constellation Ursa Major and the middle star in the handle of the Big Dipper.It forms a well known naked-eye double with fourth magnitude Alcor (80 Ursae Majoris), 0.2° to the northeast (see Figure 1). Mizar - ζ Ursae Majoris (zeta Ursae Majoris) Mizar, also designated as ζ Ursae Majoris (zeta Ursae Majoris), is a variable and multiple main-sequence star in the constellation of Ursa Major . It is radiating 227[2] times the luminosity of the Sun from its photosphere at an effective temperature of 8,720 K.[8] This anomalously high temperature and an absolute magnitude of −0.98[2] may indicate it is on the verge of evolving into a giant star. 3.06), Talitha (Iota UMa, mag. They are both Ap stars, which exhibit overabundances of certain metals in the photosphere and tend to spin more slowly than other class A stars. [6], The stellar classification of Zeta UMi is A3Vn,[3] a notation that indicates this is an A-type main-sequence star with broad "nebulous" absorption lines in its spectrum due to rapid rotation. ζ Ursae Majoris: Zeta Ursae Majoris is called Mizar girdle or waistband. These cookies do not store any personal information. It is the fourth brightest star in Ursa Major. [9], Zeta Ursae Minoris is about 180[10] million years old with 6.15[8] times the radius of the Sun. Learn definitions, uses, and phrases with ursae. Both are blue main sequence dwarf stars that are loosely bound to one another, despite being separated by a hefty one light year distance. Zeta Ursae Minoris, which is Latinized from ζ Ursae Minoris, is a single star in the northern circumpolar constellation of Ursa Minor, forming the northernmost part of the bowl in this "little dipper" asterism. The components of the system were imaged in 1996 using the Navy Prototype Optical Interferometer, an astronomical interferometer capable of exceptionally high resolution. The stars are associated with the Mi’kmaq First Nations myth that explains why leaves turn red in the autumn and why the Big Dipper changes its position from one season to the next. The bear’s skeleton lies on its back all winter (when the Bear constellation appears upside down) until its spirit enters another bear that lies in the cave until the spring, when it leaves the cave and is hunted again. The composite image of Mizar A shows the stars’ orbital motion. The Big Dipper, Arcturus and Spica, image: Wikisky. Zeta is the second star on the handle and is one of the most famous binary systems in the heavens: binoculars. 2.37), Phecda (Gamma UMa, 2.438), Psi Ursae Majoris (mag. Zeta Ursae Majoris (ζ UMa /ζ Ursae Majoris, Zêta Ursae Majoris) este o stea din constelația Ursa Mare și este cea de a doua stea pornind de la capătul oiștii Carului Mare.Numele său tradițional, Mizar sau Mirza, provin din arabă ميزر mi'zar, care semnifică „curea”. Mizar B is a single-lined spectroscopic binary (SB1), which means that the spectrum of only one star in the system can be observed, but the star shows periodic variations in radial velocity that indicate the presence of a companion. In the myth, seven hunters (birds) are hunting the bear. [7] An infrared excess has been detected from an orbiting circumstellar disk. They are nearly as well-known as the Dipper itself. n. The binary star in the middle of the handle of the Big Dipper, in the constellation Ursa Major, approximately 78 light years from Earth. Just remember eta Ursae Majoris because eta Ursae Majoris is in the vicinity to a starfield with a completely developed military base which is what we call the Po Military Starfield, the other starfields are not inhabited by humans.” “Oh! At the bend of the Big Dipper's handle is the striking pair of Zeta and 80 Ursae Majoris, or Mizar and Alcor. Ea are o magnitudine aparentă de +2,27 și este de tipul spectral A1 V. They can easily be seen on a clear night or, if the viewing conditions are less than perfect, in binoculars. Zeta1 Ursae Majoris was another first: the first spectroscopic binary star ever discovered. The “p” indicates that the stars are chemically peculiar. The Big Dipper never sets for most northern observers and can be seen year-round. The grand design spiral galaxy M51 and its smaller companion NGC 5195, also visible in small telescopes, lie about 3.5 degrees southwest of Alkaid. Megrez forms the Big Dipper’s bowl with the stars Phecda (Gamma Ursae Majoris), Dubhe (Alpha Ursae Majoris) and Merak (Beta Ursae Majoris). But Mizar itself is also a double, a fact discovered by Riccioli in 1650. Second in line along the tail is the wide double star Zeta Ursae Majoris. Galileo subsequently gave Castelli a detailed report on the binary star system. Mizar is the middle star of the Big Dipper‘s handle and it forms a naked-eye double with Alcor, a fainter binary star located at a separation of about 12 arcminutes. Mizar is easy to find because it is part of one of the best known asterisms in the sky. Mizar (mÿ -zar) (ζ UMa) A white main-sequence dwarf that is one of the brighter stars of the Plough. Mizar and Alcor are 78 and 81 light-years away, so they are not a true binary pair. Zeta Ursae Majoris was the first telescopic binary star discovered. Mizar is a member of the Ursa Major Moving Group, a stellar association that also includes Big Dipper stars Alioth, Megrez, Phecda and Merak, as well as a number of bright stars in other constellations, among them Alphecca (Alpha Coronae Borealis), Skat (Delta Aquarii), Adhafera (Zeta Leonis), Menkalinan (Beta Aurigae),  Beta Serpentis, Zeta Boötis A and Gamma Leporis A. 2.04), Merak (Beta UMa, mag. Zeta Ursae Majoris sextuple star system in the constellation Ursa Major. It is the middle star of the Big Dipper’s handle, which it forms with the brighter Alioth and Alkaid. Ap stars also tend to have stronger magnetic fields than regular class A stars. Acamar Achernar Acrux Adhara Albireo Alchiba Alcor Alcyone Aldebaran Alderamin Algenib Algol Algorab Alhena Alioth Alkaid Alkes Almach Alnair Alnilam Alnitak Alpha Centauri Alphard Alphecca Alpheratz Altair Aludra Ankaa Anser Antares Arcturus Ascella Asterope Atlas Atria Avior Baten Kaitos Bellatrix Betelgeuse Bharani Canopus Capella Caph Castor Celaeno Deneb Denebola Diphda Dubhe Electra Elnath Eltanin Enif Epsilon Lyrae Fomalhaut Gacrux Gamma Cassiopeiae Gienah Ginan Hadar Hamal Imai Izar Kaus Australis Kaus Borealis Kaus Media Kepler-22 Kochab Kraz Maia Marfik Markab Megrez Meissa Menkalinan Menkar Menkent Merak Merope Mesarthim Methuselah Star Miaplacidus Mimosa Minkar Mintaka Mira Mirach Mirfak Mirzam Mizar Mu Cephei Naos Nunki Peacock Phecda Pherkad Pleione Polaris Pollux Procyon Proxima Centauri Rasalhague Regor Regulus Rho Ophiuchi Rigel Rigil Kentaurus Ruchbah Sabik Sadr Saiph Sargas Scheat Schedar Segin Seginus Shaula Sheratan Sirius Spica Stephenson 2-18 Suhail Taygeta Thuban Toliman Unukalhai UY Scuti Vega Vindemiatrix VV Cephei VX Sagittarii Wasat Wezen WOH G64 Zeta Reticuli Zubenelgenubi Zubeneschamali. The system is an excellent target for small telescopes. Primary / Proper / Traditional Name: Mizar: Alternative Names: Zeta Ursae Majoris, Zet Uma, HD 116656, HIP 65378, HR 5054, TYC 3850-1386-1, 79 Ursae Majoris A, 79 Uma A, BD+55 1598 It forms a triangle with Mizar and Alkaid above the Big Dipper‘s handle, about 5.5 degrees from each star. Observers with good eyesight or suing binoculars will see that this star of magnitude 2.2 has a partner of magnitude 4.0, known as Alcor or 80 Ursae Majoris. The names may originally refer to a pair of Ibexes, and are more properly applied to γ UMi and β UMi respectively, the brighter two stars in the rectangle of Ursa Minor. These include the Pinwheel Galaxy (M101), the galaxy pair M81 and M82 (Bode’s Galaxy and the Cigar Galaxy), the barred spiral galaxies M108 and M109, and the planetary nebula M97, also known as the Owl Nebula. The name Mizar (pronunciation: /ˈmaɪzɑːr/) comes from the Arabic miʼzar, meaning “cover,” “wrapper” or “apron.” It is the traditional name for the whole star system, but now only formally applies to the star Zeta Ursae Majoris Aa. Mizar is an Arabic word meaning waistband or girdle. Their estimated masses are about 1.6 solar masses. Mizar ili Zeta Ursae Majoris (drugi nazivi: Zeta UMa, ζ Ursae Majoris, ζ UMa) je zvezda u sazvežđu Veliki medved, a takođe pripada i asterizmu Velika kola.Mizar je višestruka zvezda i ima još 5 pratilaca. Arcturus, the brightest star in the northern celestial hemisphere and the fourth brightest star in the sky, is the first bright star that appears along the imaginary line that follows the arc of the Dipper’s handle. Ursa Major’s brightest star, Alioth, was given the designation Epsilon Ursae Majoris because it lies in the eastern part of the constellation, in the Bear’s tail. Disregarding for a moment the famous duo Mizar and Alcor, there is another reason for Mizar's fame. The two stars have been known since ancient times. This system was visited for the first time on EDSM by Fenris Wolf.. 4045 ships passed through Mizar space, including 33 ships in the last 7 days. It has a combined apparent magnitude of 2.04 and lies at a distance of 82.9 light years from Earth. This category only includes cookies that ensures basic functionalities and security features of the website. Mizar Aa and Mizar Ab – the two components of Mizar A – have roughly the same mass (2.2 times that of the Sun), radius (2.4 times solar), temperature (9,000 K), and luminosity (33.3 solar luminosities). The visible spectrum indicates an Am star (metallic-line star), a chemically peculiar class A star whose spectrum shows strong metal absorption lines and a deficiency of calcium or scandium. It is only a line-of-sight companion to its two brighter neighbours and perhaps too faint to test eyesight. Ursa Major constellation, image: Roberto Mura. The stellar class also means that calcium K lines indicate spectral type A1, hydrogen lines indicate early A, while other metals indicate type A7. Spica, the 16th brightest star in the sky, is the second star to appear a bit further along the same line. [10] A black body fit to the data yields a mean dust temperature of 160 K and an orbital radius of 42.5 AU. Mizar and Alcor were believed to be physically unrelated until 2009, when two teams of astronomers independently discovered not only that Alcor was a binary star itself with a faint red dwarf companion, but that it was gravitationally bound to Mizar. 3.01), Tania Australis (Mu UMa, mag. Mizar and its fourth magnitude neighbour Alcor are a visual double appearing only 11.8 arcminutes apart. ζ Ursae Majoris visual magnitude is 3.95. Zeta Ursae Majoris In the UK this star grouping is called 'the Plough', in the USA it is known as 'the Big Dipper', German people call it Großer Wagen ('Great Cart'), Native Americans know it as the hunting party (of the bear), and it is known as Saptarshi ('the seven rishes' - … [8], In some Arabic star charts it is listed as أخفى الفرقدين ʼakhfā al-farqadayn, meaning "the dimmer of the two calves", and paired with η Ursae Minoris as ʼanwar al-farqadayn, "the brighter of the two calves". [14], Centre de données astronomiques de Strasbourg, Monthly Notices of the Royal Astronomical Society,, Creative Commons Attribution-ShareAlike License, This page was last edited on 9 January 2021, at 02:28. You also have the option to opt-out of these cookies. It is located at a distance of approximately 369 light years from the Sun based on parallax,[1] but is drifting further closer with a radial velocity of about −13 km/s. 3.99) Alcor was said to be a good test of eyesight, but since even people with imperfect eyesight have no difficulty seeing the two stars, the English amateur astronomer Sir Patrick Moore has suggested that the old saying really refers to a different star that appears between Mizar and Alcor. When the hunters finally kill the bear, its blood spatters over the trees, which is why the leaves turn red. Every star has a unique orbit and evolution. The stars forming the handle of the Big Dipper can be used to find Arcturus and Spica, the brightest stars in the constellations Boötes and Virgo. OBJECT: Zeta Ursae Majoris TELESCOPE: Meade 10" f/10 SCT: DATE: 05.30.1996 TIME: 12:47 am EDT: TRANSPARENCY: Fair SEEING: Good: MAGNIFICATION: 96x: LOCATION: Kalamazoo Twp. The Pinwheel Galaxy can be seen in a small telescope. Only two Big Dipper stars – Dubhe and Alkaid – are not members of the group, but as they are the westernmost and easternmost star in the asterism, and moving in opposite directions, the Big Dipper will eventually fall apart over time. The two main components are separated by only 14.4 arcseconds. Mizar visual magnitude is 2.27, making it the 74th brightest star in the sky. [13] The star has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.28. Zeta Ursae Maioris synonyms, Zeta Ursae Maioris pronunciation, Zeta Ursae Maioris translation, English dictionary definition of Zeta Ursae Maioris. Ursa Major is the third largest constellation in the sky and contains a number of well-known deep sky objects. Out of these, the cookies that are categorized as necessary are stored on your browser as they are essential for the working of basic functionalities of the website. Ovaj šestostruki sistem se zapravo sastoji od četvorostrukog sistema kojem pripada zvezda Mizar, i … Any cookies that may not be particularly necessary for the website to function and is used specifically to collect user personal data via analytics, ads, other embedded contents are termed as non-necessary cookies. Tải lên phương tiện These stars are believed to have formed in the same molecular cloud at around the same time and share common velocities and proper motion. Similarly, the seven stars making up the little dipper in Ursa Minor were known as the Little Daughters of the Bier. It is particularly prominent in the evening sky during the months of spring. It connects the bowl to the handle, formed by the brighter Alioth (Epsilon Ursae Majoris), Mizar (Zeta Ursae Majoris) and Alkaid (Eta Ursae Majoris).. Star type Old Man's War (2005), by John Scalzi. Theta Ursae Majoris (Theta UMa, θ Ursae Majoris, θ UMa) is a suspected spectroscopic binary star system in the northern circumpolar constellation of Ursa Major.It has an apparent visual magnitude of 3.17, placing it among the brighter members of this constellation. 1100 and 2909). Zeta Ursae Majoris (ζ UMa / ζ Ursae Majoris) eli Mizar lienee tunnetuin Otavan tähdistä. Mizar . Harvard College Observatory, Cambridge, U.S., Nov. 12, 1889. The stars’ masses differ only very slightly – Mizar Aa has 2.2224 solar masses and Mizar Ab has 2.2381 – and reflect the slight variations in the stars’ radial velocities. This website uses cookies to improve your experience while you navigate through the website. The primary star (Mizar A) is the by far the brightest and is blue-white in color. Two more stars have been found showing a similar periodicity: Beta Aurigae and b Ophiuchi (H.P. Seeing the fainter (mag. By clicking “Accept”, you consent to the use of ALL the cookies. companion, called 'Alcor' or 80 UMa (otherwise a small binocular will help). But opting out of some of these cookies may affect your browsing experience. Mizar B has been given the spectral type kA1h(eA)mA7IV-V, indicating a star between a hydrogen-fusing dwarf and subgiant in terms of luminosity. American astronomer Antonia Maury, who published a catalogue of stellar spectra in 1897, had observed periodic doubling in some of the star’s spectral lines and included her discovery – the first spectroscopic binary orbit – in her publication. Other well-known Am stars include Sirius A (Alpha Canis Majoris A), Castor Ba (Alpha Geminorum Ba), Kurhah (Xi Cephei), Tureis (Rho Puppis), Acubens A (Alpha Cancri), Alpha Volantis and Theta1 Crucis. This star is sometimes referred to as Ludwig’s Star (Sidus Ludoviciana). n. The binary star in the middle of the handle of the Big Dipper, in the constellation Ursa Major, approximately 78 light years from Earth. The estimated distance between Mizar and Alcor is no more than 0.5 to 1.5 light years, or 74,000 ± 39,000 astronomical units. [5] The star is spinning with a projected rotational velocity of 210 km/s, which is creating an equatorial bulge that is estimated to be 10% larger than the polar radius. It has a combined apparent magnitude of 2.04 and lies at a distance of 82.9 light years from Earth. Later, each of the visual components was determined to be a spectroscopic binary; Mizar is actually a quadruple star. The Chinese know Mizar as the Sixth Star of Northern Dipper (北斗六) and the Star of The Opener of Heat (開陽). The seven stars are Alpha Ursae Majoris, Beta Ursae Majoris, Gamma Ursae Majoris, Delta Ursae Majoris, Epsilon Ursae Majoris, Zeta Ursae Majoris and Eta Ursae Majoris. The entire star system has the Hipparcos designation HIP 65378, but the components are catalogued separately in the Bright Star Catalogue (BSC) and the Henry Draper Catalogue (HD). The four components of the system are designated as Zeta Ursae Majoris Aa, Ab, Ba and Bb. If both stars are located at the same distance from Earth (which is not very likely), then the estimated distance between them drops to only 0.281 light years, or 17,800 astronomical units. Mizar is located in the Tail of the Big Bear, Ursa Major constellation. 3.166). It's brightness is about 2.4 mag; therefore under very good conditions it is possible for the naked eye to see the 4th mag. Fixed star Mizar, Zeta Ursae Majoris, forms a double star with Alcor (15°52′ Virgo). Their estimated age is 370 million years. These cookies will be stored in your browser only with your consent. We use cookies on our website to give you the most relevant experience by remembering your preferences and repeat visits.

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