Little Bear longs to be as big and fast as his mother. In the arctic snow, Mother Bear shows the little polar cub what it's like to be grown up Bear Big Little Reveal Shirt, Cute Big Little Bear Reveal Shirt, Bear Shirt For Big Little Reveal, Big Little Bear Cute Shirt For Reveal only later, according to Strabo (I.1.6, C3) due to a suggestion by Thales, who suggested it as a navigation aid to the Greeks, who had been navigating by Ursa Major. In classical antiquity, the celestial pole was somewhat closer to Beta Ursae Minoris than to Alpha Ursae Minoris, and the entire constellation was taken to indicate the northern direction. Since the medieval period, it has become convenient to use Alpha Ursae Minoris (or " Polaris") as the North Star. (Even though, in the medieval period, Polaris was still several degrees away from the celestial pole. [9] [a] ) Now, Polaris is within 1° of the north celestial pole and remains the current Pole star. Its Neo-Latin name of stella polaris was coined only in the early modern period. [10] There are various proposed explanations for the name Cynosura. One suggestion connects it to the myth of Callisto, with her son Arcas replaced by her dog being placed in the sky by Zeus. [11] In Inuit astronomy, the three brightest stars—Polaris, Kochab and Pherkad—were known as Nuutuittut "never moving", though the term is more frequently used in the singular to refer to Polaris alone. The Pole Star is too high in the sky at far northern latitudes to be of use in navigation. [17] In Chinese astronomy, the main stars of Ursa Minor are divided between two asterisms:

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Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging in apparent magnitude from 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and 3rd-magnitude Gamma Ursae Minoris have been called the "guardians of the pole star" or "Guardians of The Pole". [3] Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star— Calvera—and H1504+65, the hottest white dwarf yet discovered, with a surface temperature of 200,000 K.Rogers, John H. (1998). "Origins of the Ancient Constellations: I. The Mesopotamian Traditions". Journal of the British Astronomical Association. 108: 9–28. Bibcode: 1998JBAA..108....9R. The main character George Orris has to survive on his wits rather than cordite. He is out for revenge after his network in Czecho is rolled up.

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NGC 6251 – Seyfert 2 Galaxy". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg . Retrieved 21 July 2015. Disney Country Bear Jamboree Group Movie Poster Retro Shirt, Magic Kingdom Trip Unisex T-shirt Family Birthday Gift Adult Kid Toddler Tee a b "Epsilon Ursae Minoris – Variable of RS CVn type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg . Retrieved 21 June 2014. The tradition of naming the northern constellations "bears" appears to be genuinely Greek, although Homer refers to just a single "bear". [8] Comments have to be in English, and in full sentences. They cannot be abusive or personal. Please abide by our community guidelines for posting your comments.Otero, Sebastian Alberto (16 November 2009). "RR Ursae Minoris". The International Variable Star Index. American Association of Variable Star Observers . Retrieved 18 May 2014. According to Diogenes Laërtius, citing Callimachus, Thales of Miletus "measured the stars of the Wagon by which the Phoenicians sail". Diogenes identifies these as the constellation of Ursa Minor, which for its reported use by the Phoenicians for navigation at sea were also named Phoinikē. [6] [7] a b c d van Leeuwen, F. (2007). "Validation of the New Hipparcos Reduction". Astronomy and Astrophysics. 474 (2): 653–64. arXiv: 0708.1752. Bibcode: 2007A&A...474..653V. doi: 10.1051/0004-6361:20078357. S2CID 18759600. Rare Dead Star Found Near Earth". BBC News: Science/Nature. BBC. 20 August 2007. Archived from the original on 13 July 2014 . Retrieved 21 August 2007.

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Albright, William F. (1972). "Neglected Factors in the Greek Intellectual Revolution". Proceedings of the American Philosophical Society. 116 (3): 225–42. JSTOR 986117. Condos, T., The Katasterismoi (Part 1), 1967. Also mentioned by Servius On Virgilius' Georgics 1. 246, c. AD 400; a mention of doubtful authenticity is Hyginus, De Astronomica 2.2.Benson, Priscilla J.; Clayton, Geoffrey C.; Garnavich, Peter; Szkody, Paula (1994). "Z Ursa Minoris – a New R Coronae Borealis Variable". The Astronomical Journal. 108 (#1): 247–50. Bibcode: 1994AJ....108..247B. doi: 10.1086/117063. a b c Ridpath, Ian. "Constellations: Lacerta–Vulpecula". Star Tales. Self-published . Retrieved 21 June 2014. Located close to Polaris is Lambda Ursae Minoris, a red giant of spectral type M1III. It is a semiregular variable varying between magnitudes 6.35 and 6.45. [46] The northerly nature of the constellation means that the variable stars can be observed all year: The red giant R Ursae Minoris is a semiregular variable varying from magnitude 8.5 to 11.5 over 328days, while S Ursae Minoris is a long-period variable that ranges between magnitudes 8.0 and 11 over 331days. [47] Located south of Kochab and Pherkad towards Draco is RR Ursae Minoris, [3] a red giant of spectral type M5III that is also a semiregular variable ranging from magnitude 4.44 to 4.85 over a period of 43.3days. [48] T Ursae Minoris is another red-giant variable star that has undergone a dramatic change in status—from being a long-period (Mira) variable ranging from magnitude 7.8 to 15 over 310–315 days, to being a semiregular variable. [49] The star is thought to have undergone a shell helium flash—a point where the shell of helium around the star's core reaches a critical mass and ignites—marked by its abrupt change in variability in 1979. [50] Z Ursae Minoris is a faint variable star that suddenly dropped 6magnitudes in 1992 and was identified as one of a rare class of stars— R Coronae Borealis variables. [51] Absolutely stunning. Baby Bear is too little, so he can't do as much as Mummy Bear can. Mummy Bear shows him what it's going to be like to be tall and fast, able to dive into the sea and swim strongly, but she tells him she doesn't want him to grow up just yet because she likes being able to snuggle him. He agrees - although it's going to be fun to be big, he doesn't want to be big right now.