Mu Ursae Majoris (μ UMa / μ Ursae Majoris) is a star in the constellation Ursa Major. It also has the proper names Tania Australis (former Tania australis) meaning "the Southern (star) of Tania." The word Tania comes from the Arabic phrase (al-Qafza) al-Thāniya meaning "the Second (Leap)" (the distinctions "southern" (australis) is added in Latin), Alkafzah Borealis, and El Phekrah comes from the Arabic phrase al-Fiqra (al-Thāniya) meaning "(the ...
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Mu Ursae Majoris
Astronomy
Constellation
Ursa Major
Ursa Major is a constellation visible throughout the year in most of the northern hemisphere. Its name means the Great Bear in Latin. It is dominated by the widely recognized asterism known as the Big Dipper or Plough, which is a useful pointer toward north, and which has mythological significance...
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Mizar
Mizar (ζ UMa / ζ Ursae Majoris) is a star in the constellation Ursa Major and is the second star from the end of the Big Dipper's handle. Its apparent magnitude is 2.23 and its spectral class is A1V. Mizar's name comes from the Arabic ميزر mīzar, meaning a waistband or girdle. In Chinese it is 开阳... -
Gamma Ursae Majoris
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 الفخذ الدب al-faxð ad-dubb (the thigh of the bear). It is more familiar to most observers in the northern hemisphere as the lower-left star... -
Beta Ursae Majoris
Beta Ursae Majoris (β UMa / β Ursae Majoris) is a star in the constellation of Ursa Major. It has the traditional name Merak. It is more familiar to northern hemisphere observers as one of the "pointer stars" in the Big Dipper, and a line connecting it with nearby Alpha Ursae Majoris (Dubhe)... -
Winnecke 4
Winnecke 4 (also known as Messier 40 or WNC 4) is a double star in the constellation Ursa Major. It was discovered by Charles Messier in 1764 while he was searching for a nebula that had been reported in the area by Johann Hevelius. Not seeing any nebulae, Messier catalogued this double star... -
Tau Ursae Majoris
Tau Ursae Majoris (τ UMa / τ Ursae Majoris) is a binary star in the constellation Ursa Major. It is approximately 122 light years from Earth. Tau Ursae Majoris is a spectroscopic binary which is classified as a yellow-white F-type giant with an apparent magnitude of +4.67. The binary system... -
47 Ursae Majoris
47 Ursae Majoris, often abbreviated as 47 UMa, is a solar twin, yellow dwarf star approximately 46 light-years away from Earth in the constellation of Ursa Major. As of 2008, it has been confirmed that two extrasolar planets orbit the star. Because of this, 47 Ursae Majoris was listed as one of top... -
W Ursae Majoris
W Ursae Majoris (W UMa) is a variable star in the constellation Ursa Major. It is an eclipsing contact binary whose two component stars share a common outer layer, and is the prototype of a class of contact binary variables known as W Ursae Majoris variables. Unlike with normal eclipsing binaries,... -
HD 118203
HD 118203 is a K-type subgiant star located in the Ursa Major constellation 289 light years away from Earth. It has higher metallicity by 25% and very similar stellar age of 4.6 billion years. It has mass 23% greater than the Sun. It is invisible to the naked eye but it can be visible using... -
Lambda Ursae Majoris
Lambda Ursae Majoris (λ UMa / λ Ursae Majoris) is a star in the constellation Ursa Major. It also has the proper names Tania Borealis (former Tania borealis) meaning "the Northern (star) of Tania." The word Tania comes from the Arabic phrase (al-Qafza) al-Thāniya meaning "the Second (Leap)" (the... -
Rho Ursae Majoris
Rho Ursae Majoris (ρ UMa / ρ Ursae Majoris) is a star in the constellation Ursa Major. Rho Ursae Majoris is a M-type red giant with an apparent magnitude of +4.74. It is approximately 287 light years from Earth.
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