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Ursa Major is the largest northern constellation and third largest constellation in the sky. Its brightest stars form the Big Dipper asterism, one of the most recognizable shapes in the sky, also known as the Plough. Ursa Major is well-known in most world cultures and associated with a number of myths.


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Ursa Major ( / ˈɜːrsə ˈmeɪdʒər /; also known as the Great Bear) is a constellation in the northern sky, whose associated mythology likely dates back into prehistory. Its Latin name means "greater (or larger) bear", referring to and contrasting it with nearby Ursa Minor, the lesser bear. [1]


Ursa Major The

Ursa Major, also known as the Great Bear, is the third-largest constellation in the sky and the largest constellation in the Northern Hemisphere. It includes the Big Dipper asterism and is one.


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January 4, 2021 Ursa Major is a constellation in the northern sky. It is known as the Great Bear, and it is among the oldest constellations, with associated mythologies dating back into prehistory. Key Facts & Summary Ursa Major was in antiquity, among the 48 Greek constellations listed by Ptolemy in the 2 nd century AD.


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Ursa Major Moving Group is the debut project of multi-instrumentalist, composer and writer Ursula Russell. Her self-titled debut album is an intense and dynamic musical journal of a process of individuation, wherein songs are offered as myths for a new world.


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Inside the Ursa Major moving group Astronomers have found nearly 60 stars that appear to be members of the nearest moving group to Earth. By Richard Talcott | Published: January 24, 2005.


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They are known as the Ursa Major Moving Group, or Collinder 285. The other two stars, Dubhe and Alkaid, move independently of the group of five and of each other. The Big Dipper contains one of the most famous double stars in the sky.


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The Ursa Major Groups are a very distinctive band of galaxies in the northern hemisphere. Unlike the dense enviroment of the Virgo cluster, most of the major galaxies here are spiral galaxies.


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Ursa Major Moving Group By Stephen James O'Meara | Published: January 1, 2024 Credit: A. Fujii/Hubble The seven brightest stars in the constellation Ursa Major comprise one of the.


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The stars' shared distance and motion implied that they were once bound more tightly but have since dispersed into a loose confederation we know today as the Ursa Major Moving Cluster (also referred to as the Ursa Major Moving Group), or Collinder 285.


Ursa Major (Constellation)

The Ursa Major Moving Group, also known as Collinder 285 and the Ursa Major association, is the closest stellar moving group - a set of stars with common velocities in space and thought to have a common origin in space and time. In the case of the Ursa Major group, all the stars formed about 300 million years ago. Its core is located roughly 80 light years away and part of the Local Bubble.


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Ursa Major, (Latin: "Greater Bear") in astronomy, a constellation of the northern sky, at about 10 hours 40 minutes right ascension and 56° north declination. It was referred to in the Old Testament ( Job 9:9; 38:32) and mentioned by Homer in the Iliad (xviii, 487).


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HD 63433d is the third planet detected in this multiplanet system. The kinematic, rotational, and abundance properties of the host star indicate that it belongs to the young (414 $\pm$ 23 Myr) Ursa Major moving group, whose membership we update using new data from Gaia DR3 and TESS.


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Ursa Major Moving Group, the solo alias of singer and composer Ursula Russell, announces her self-titled debut album, due out June 9th via Faith & Industry R.


(PDF) Stellar Kinematic Groups. II. A Reexamination of the Membership, Activity, and Age of the

For example, Vereshchagin, Reva & Chupina studied a sample of 128 Ursa Major Group (UMaG) members from Chupina, Reva & Vereshchagin , and concluded through a statistical analysis that two apparent density fluctuations on the phase-space vectors distribution are, in fact, two groups representing true kinematic subsystems at the 95 |${{\ \rm per.


Ursa Major Moving Group

The Ursa Major Moving Group was discovered in 1869 by Richard A. Proctor, and may once have been a part of a much larger open star cluster.

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