It has a surface temperature of about 4,030 Kelvin. It is one of the four bright stars that form the bowl of the Big Dipper.

Kochab is … Alkaid (Benetnash) – η Ursae Majoris (Eta Ursae Majoris) Alkaid is … Query : Beta Ursae Minoris C.D.S. Polaris took over as the North Star from Kochab, Beta Ursae Minoris, around the year 500 CE. Megrez (Delta Ursae Majoris) is the least luminous of all the seven Dipper stars, with an apparent visual magnitude of +3.3. From around the year 2.500 B.C., the celestial pole was near Thuban, located in the constellation Draco.

Today, Kochab and Pherkad, Gamma Ursae Minoris, are known as the Guardians of the Pole. - SIMBAD4 rel 1.7 - 2020.05.09CEST01:26:44 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations

Little Dipper Series – Kochab Kochab (Beta Ursae Minoris, β UMi, β Ursae Minoris) is the brightest star in the bowl of the "Little Dipper" (which is part of the constellation Ursa Minor), and only slightly fainter than Polaris, the northern pole star and brightest star in Ursa Minor. It belongs to the Ursa Major Moving Group and is a suspected variable star. Detailed information on planet beta Umi b orbiting around star beta Umi. Gamma Ursae Minoris (γ Ursae Minoris, Gamma UMi, γ UMi) is a main sequence star in the constellation of Ursa Minor, the little bear. Practically Thuban was the North Star when the Egyptians built the pyramids. Merak, Beta Ursae Majoris (β UMa) is a blue-white subgiant star in the constellation Ursa Major.

Together with the star Beta Ursae Minoris (Kochab), it is one of the Guardians of the Pole.

Beta Ursae Minoris (Kochab) is the brightest star in the bowl of the "Little Dipper" - part of the constellation Ursa Minor. With an apparent magnitude of 2.37, it is the fifth brightest star in Ursa Major. Its only real, and not all that unusual, physical distinction is a high rotation speed of 174 kilometers per second that makes its spectrum lines fuzzy. Beta Ursae Minoris (Kochab) is the brightest star in the bowl of the "Little Dipper" - part of the constellation Ursa Minor. Gamma Ursae Minoris (γ Ursae Minoris, abbreviated Gamma UMi, γ UMi), also named Pherkad / ˈ f ɜːr k æ d /, is a star in the northern circumpolar constellation of Ursa Minor.Together with Beta Ursae Minoris (Kochab), it forms the end of the dipper pan of the "Little Dipper", which is an asterism forming the tail of the bear. It has a surface temperature of about 4,030 Kelvin. The star is sometimes also called "Pherkad", "Phecda" or "Phad" (from the Arabic fakhð ad-dubb, “the thigh of the bear”). Beta Ursae Majoris is 2.7 times more massive than the Sun, has 2.84 times the radius, and is about 68 times more luminous. World's most comprehensive interactive database of extrasolar planets updated daily since 1995. This blue-white main sequence dwarf star is located around 58.4 light years from Earth, and is also an outlying member of the Ursa Major Moving Group, a collection of stars that share the same proper motion across the sky, and therefore likely have a common origin. Later, in the year 400 B.C., the pole was closer to Kochab, Beta Ursae Minoris, than it was to Alpha UMi.

Physically, Yildun is a quite-ordinary white class A star (A1) 183 light years away with a temperature of 9000 Kelvin, a luminosity 47 times that of the Sun, and a diameter of 2.8 solar. Kochab, the second brightest star in Ursa Minor and the brightest star in the bowl of the Little Dipper, held the title from 1500 BCE to 100 CE.



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