In 2007, Hipparcos data was revised with a new parallax of 39.21000 which put Phecda at a distance of 83.18 light years or 25.50 parsecs. Phecda - γ Ursae Majoris (gamma Ursae Majoris) Phecda, also designated as γ Ursae Majoris (gamma Ursae Majoris), is a variable hypergiant star in the constellation of Ursa Major . [14] Dựa trên các đo đạc thị sai với … Gamma Ursae Majoris ( Gamma UMa, γ Ursae Majoris, γ UMa) is a star in the constellation Ursa Major. Phecda is easy to find because it is part of a bright and recognizable northern asterism, the Big Dipper. Jest oddalona o około 111 lat świetlnych od Słońca Nazwa. which to calculate using this website is too large. Phecda (Gamma Ursae Majoris), the 6th brightest star in Ursa Major and 85th brightest star in the night sky, marks out the lower left corner of the Big Dipper’s bowl. Using statistical and phylogenetic tools, Julien d'Huy reconstructs the following Palaeolithic state of the story: "There is an animal that is a horned herbivore, especially an elk. Using the 2007 distance, the star is roughly 5,259,715.91 Astronomical Units from the Earth/Sun give or take a few. Gamma Ursae Majoris on saatavilla 30 muulla kielellä. Gamma Ursae Majoris (Phad, Phecda, Phegda, Phekha, Phacd, 64 Ursae Majoris) é uma estrela na direção da constelação de Ursa Major. Nimi Phecda tulee arabian kielen فخذ الدب الأكبر "fakhð al … 61 Ursae Majoris is a star system (also known as the Archer system) centered around yellow dwarf star (spectral class G8V) of the same name located about 9.5 parsecs (31 light-years) from Earth, where it is visible in the constellation of Ursa Major. Gamma Ursae Majoris eli Phecda, Phekda, Phad on Otavan tähtikuvion eräs tähti. It lies at a distance of 83.2 light years from Earth. Gamma Ursae Majoris, formally named Phecda, is a star in the constellation of Ursa Major.Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Phecda is located in the northern constellation Ursa Major, the Great Bear. The traditional name Phecda comes from the Arabic phrase فخذ الدب (fakhð ad-dubb) which means thigh of the bear. Ursa Major is one of the 48 Greek constellations, listed by the Greco-Roman astronomer Ptolemy in the 2nd century CE, but it has likely been known since prehistoric times. Phecda is a member of the Ursa Major Moving Group (Collinder 285), a loose stellar association of stars with an estimated age of 300 million years that share a common origin and motion through space. The items in red are values that I've calculated so they could well be wrong. It operates the La Silla Paranal Observatory in Chile and has its … They are particularly injurious as regards to the affairs of natio… Gamma Ursae Majoris (γ UMa / γ Ursae Majoris) — звезда в созвездии Большой Медведицы. is the number of times that the star is from the Earth compared to the Sun. Phecda on Otavan suorakaidemaisen "kattilaosan" alavasemmalla. Palaa sivulle Gamma Ursae Majoris. Query : Gamma Ursae Majoris : C.D.S. Exoplanets. Gamma Ursae Majoris ni jina la Bayer; Gamma ni herufi ya tatu katika alfabeti ya Kigiriki lakini Fahidhi ni nyota angavu ya sita na hii ni mfano ya kwamba Bayer hakufuata mwangaza kamili wakati wa kuorodhesha nyota. The Radial Velocity, that is the speed at which the star is moving away/towards the Sun is -11.90000 km/s with an error of about 0.70 km/s . 3.14), and Theta Ursae Majoris (mag. Tagged under Gamma Ursae Majoris, Mizar, Manufacturing, Mizar And Alcor, Machine. To give idea of size, the Sun is 99.86% the mass of the solar system. The constellation symbolized a funeral and its slow circular motion around the north celestial pole was associated with the slow movement of a funeral procession. Phecda [12] eller Gamma Ursae Majoris (γ Ursae Majoris, γ UMa) som är stjärnans Bayer-beteckning, är en dubbelstjärna i den mellersta delen av stjärnbilden Stora Björnen och ingår i Karlavagnen.Den har en skenbar magnitud på +2,44 [2] och är synlig för blotta ögat. The M109 Group is a member of the Ursa Major Cluster, a galaxy cluster particularly rich in spiral galaxies. Tabia. Phecda’s spectrum has been used as one of the anchor points for the Morgan-Keenan (MK) spectral classification system since 1943. An older star would have a high metallicity whereas a new star would have a lower one. A note about the calculations, when I'm talking about years, I'm talking non-leap years only (365 days). It has a mass of 2.94 solar masses and a radius 3.04 times that of the Sun. In the case of a star, its the galactic centre. U.G. Keenan and E. Kellman. Learn definitions, uses, and phrases with ursae. The star can be seen with the naked eye, that is, you don't need a telescope/binoculars to see it. The source of the information if it has a Hip I.D. Unitățile SI și condiții de temperatură și presiune normale dacă nu s-a specificat altfel. The Phecda's solar mass is 1.23 times that of our star, the Sun. Phekda on Aurinkoa kirkkaampi, kuumempi ja suurempi valkoinen pääsarjan tähti. However, a number of recent studies have failed to detect the companion, so the effect is possibly deceiving. The star is moving 11.01 ± 0.25 milliarcseconds/year towards the north and 107.68 ± 0.40 milliarcseconds/year east if we saw them in the horizon. Tagged under Alpha Ursae Majoris, Mizar, Beta Ursae Majoris, Gamma Ursae Majoris, Eta Ursae Majoris. It is only 8.55 light years from Mizar and Alcor, while its distance to Merak is 11 light years. In addition to the famous seven stars of the Plough or Dipper there are three pairs of stars that mark the feet of the bear. The brighter members include Menkalinan (Beta Aurigae), Skat (Delta Aquarii), Gamma Leporis, Alphecca (Alpha Coronae Borealis) and Beta Serpentis. Phecda (Gamma Ursae Majoris) is a blue main sequence star that can be located in the constellation of Ursa Major. The spiral galaxy Messier 106 can be found by extending an imaginary line from Dubhe through Phecda. Gabriela Torrini. The name Phecda (pronunciation: /ˈfɛkdə/) or Phad, as the star has also been commonly known, refers to the star’s position in the Great Bear constellation. Using the most recent figures given by the 2007 Hipparcos data, the star is 83.18 light years away from us. Phecda ( γ Ursae Majoris, abreviado Gamma UMa, γ UMa), llamada formalmente Phecda / f ɛ k d ə /, es una estrella en la constelación de la Osa Mayor.Desde 1943, el espectro de esta estrella ha servido como uno de los puntos de anclaje estables por los que se clasifican otras estrellas. An Astronomical Unit is the distance between Earth and the Sun. Nimi Phecda tulee arabian kielen فخذ الدب الأكبر "fakhð al … Ursae is contained in 9 matches in Merriam-Webster Dictionary. The figure of 64.25 that I have given is based on the value in the Simbad Hipparcos Extended Catalogue at the University of Strasbourg from 2012. With an apparent magnitude of 2.438, it is the sixth brightest star in the constellation Ursa Major. Phecda is a main star in the constellation Ursa Major and makes up the constellation outline. mv : 2.44; Mv : 0.5; spectral type: A0 Van; distance: 24.5 pc Explanation of Gamma Ursae Majoris 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. If the R.A. is positive then its eastwards. Dubhe is distinctly yellow, especially when viewed with binoculars or a telescope. Proctor was the first to notice that most of the stars of the Big Dipper have proper motions that are taking them toward a common point located in the constellation Sagittarius. The star's Galacto-Centric Distance is 7,410.00 Parsecs or 24,168.70 Light Years. 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. Megrez forms the Big Dipper’s bowl with the stars Phecda (Gamma Ursae Majoris), Dubhe (Alpha Ursae Majoris) and Merak (Beta Ursae Majoris). Gamma Ursae Majoris (Phad, Phecda, Phegda, Phekha, Phacd, 64 Ursae Majoris) é uma estrela na direção da constelação de Ursa Major.Possui uma ascensão reta de 11h 53m 49.74s e uma declinação de +53° 41′ 41.0″. Mach 1 is the speed of sound, Mach 2 is twice the speed of sound. The galaxy lies in the neighbouring constellation Canes Venatici, the Hunting Dogs. The system was named for Captain Jonathan Archer, who surveyed the system in 2151 aboard the Earth Starfleet starship Enterprise. The Chinese know Phecda as the Third Star of Northern Dipper (北斗三), referring to its position in an asterism that corresponds to the Big Dipper. 3.01), Tania Australis (Mu UMa, mag. The asterism is formed by the seven brightest stars of Ursa Major constellation: Alkaid (η UMa), Mizar (ζ UMa), Alioth (ε UMa), Megrez (δ UMa), Phecda (γ UMa), Dubhe (α UMa) and Merak (β UMa). Phad, Phecda, Phekda, Phegda, Phekha, Phacd, Fekda, γ Ursae Majoris, γ UMa, Gamma UMa, 64 Ursae Majoris, BD +54 1475, FK5 447, GC 16268, HD 103287, HIP 58001, HR 4554, PPM 33292, SAO 28179. 2.37), Phecda (Gamma UMa, 2.438), Psi Ursae Majoris (mag. Cookies / About Us / Contact Us / Twitter / Facebook, Gamma Ursae Majoris, Gam Uma, Phad and Phekda, HD 103287, HIP 58001, HR 4554, TYC 3833-1034-1, 64 Ursae Majoris, 64 Uma, BD+54 1475. The constellation of Ursa Major has been seen as a bear, usually female, by many distinct civilizations. 1.86), Mizar (Zeta UMa, mag. satellite operation launched in 1989 for four years. Merak, Mirak, β Ursae Majoris, β UMa, Beta UMa, 48 Ursae Majoris, BD+57°1302, FK5 416, GC 15145, HD 95418, HIP 53910, HR 4295, PPM 32912, SAO 27876. has done some calculations as to how long it will take going at differing speeds. It … Gamma Ursae Majoris. 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 Alioth is listed as one of the 58 navigational stars, along with its Big Dipper neighbours Dubhe (Alpha Ursae Majoris) and Alkaid (Eta Ursae Majoris). Ursa Major is the third largest constellation in the sky, after Hydra and Virgo, and it contains a great number of interesting deep sky objects. Phecda is one of the major stars in the Ursa Major constellation or the Greater Bear as it is also known. ESO is the European Organisation for Astronomical Research in the Southern Hemisphere. Considerando sua distância de 84 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.36. Translation memories are created by human, but computer aligned, which might cause mistakes. When the value is negative then the star and the Sun are getting closer to one another, likewise, a positive number means that two stars are moving away. Gamma Ursae Majoris eli Phecda, Phekda, Phad on Otavan tähtikuvion eräs tähti. Epsilon Ursae Majoris, Eps Uma, Epsilon UMA, Eps Uma, Al-Jawn, HD 112185, HIP 62956, HR 4905, TYC 3845-1190-1, 77 Ursae Majoris, 77 Uma, BD+56 1627, eps UMa Spectral Type A0p Based on the spectral type (A0V SB) of the star, the star's colour is blue - white . Gamma Ursae Majoris. The Owl Nebula is located about 2.5 degrees from Merak in the direction of Phecda and Messier 108 appears in the same field of view, about 48 arcminutes northwest of the nebula. This website uses cookies to improve your experience while you navigate through the website. The Sun's radius is 695,800km, therefore the star's radius is an estimated 2,251,592.92.km. It is calculated at being 4.604 Billion Years old. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. The ensemble’s name derives from the star Gamma Ursae Majoris and as well as the term for 'major scale' in Russian musical terms (гамма - … ET Ursae Majoris estimated radius has been calculated as being 2.12 times bigger than the Sun. The Right Ascension is how far expressed in time (hh:mm:ss) the star is along the celestial equator. Apparent Magnitude is also known as Visual Magnitude. Gamma Ursae Majoris is called Phecda, from the Arabic word fakhidh meaning ‘the thigh’. It is derived from the Arabic phrase fakhth al-dubb, meaning “the thigh of the bear.” The name was officially approved for Gamma Ursae Majoris Aa by the International Astronomical Union’s (IAU) Working Group on Star Names (WGSN) on July 20, 2016. Studying angularly extended gamma-ray sources with VERITAS Project Advisor: David Kieda, University of Utah Alpha Ursae Majoris Mizar Beta Ursae Majoris Gamma Ursae Majoris is a 1500x2000 PNG image with a transparent background. Gamma Ursae Majoris (γ Ursae Majoris, abbreviated Gamma UMa, γ UMa), also named Phecda, is a star in the constellation of Ursa Major. Gamma Ursae Majoris (γ UMa, γ Ursae Majoris) is a star in the constellation Ursa Major It has the traditional name Phad, or Phecda, from the Arabic phrase فخذ الدب "fakhð ad-dubb" ("thigh of the bear"). With an apparent magnitude of 2.438, it is the sixth brightest star in the constellation Ursa Major. I almost want to think that Black Mist and Vector tentatively teaming up isn't a coincidence, particularly after the point someone on Tumblr made about the fact that all the Barians (except Vector since he's an irredeemable douchebag) have forged bonds with others through dueling, and while Yuuma does it … We also use third-party cookies that help us analyze and understand how you use this website. Found 0 sentences matching phrase "Gamma Ursae Majoris".Found in 0 ms. Necessary cookies are absolutely essential for the website to function properly. There's no register feature and no need to give an email address if you don't need to. The hunt locates or get to the sky. Gamma Ursae Majoris , tên chính thức là Phecda, [12][13] là một ngôi sao trong chòm sao Đại Hùng. Phecda can be used to find several bright deep sky objects. Showing page 1. Database references; SIMBAD: data: The apparent visual magnitude of this star is +2.37, which means it is readily visible to the naked eye. Gamma Ursae Majoris (γ Ursae Majoris, viết tắt Gamma Uma, γ UMa), tên chính thức là Phecda, là một ngôi sao trong chòm sao Đại Hùng.Kể từ năm 1943, quang phổ của ngôi sao này đã đóng vai trò là một trong những điểm neo ổn định để phân loại các ngôi sao … Gamma Ursae Majoris (γ UMa / γ Ursae Majoris) — звезда в созвездии Большой Медведицы. The New Horizons space probe is the fastest probe that we've sent into space at the time of writing. The star's effective temperature is 9,272 Kelvin which is hotter than our own Sun's effective Temperature which is 5,777 Kelvin. Gamma Ursae Majoris , tên chính thức là Phecda, [12][13] là một ngôi sao trong chòm sao Đại Hùng. It is mandatory to procure user consent prior to running these cookies on your website. The time it will take to travel to this star is dependent on how fast you are going. Tabia. Z UMa's spectrum reveals delta and gamma hydrogen lines in emission and the presence of peculiar molecular absorption bands such as TiO (titanium oxide). Phecda (Schreibweise der IAU), Phekda, Phegda, Phekha, Pachd, Phacd oder Phad, auch Gamma Ursae Majoris, γ Ursae Majoris oder γ UMa (Bayer-Bezeichnung), ist ein etwa 83 Lichtjahre von der Sonne entfernter Doppelstern im Sternbild Großer Bär (Ursa Major) mit einer gemeinsamen scheinbaren Helligkeit von 2,44 mag.. Der Hauptstern der Komponente A des Mehrfachsternsystems γ Ursae Majoris … Along with most of the Dipper’s stars, Phecda is an inner member of the Ursa Major Moving Group, which is a relatively large group of stars (which may include Sirius) that share a common proper motion across the sky.

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