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Big Bear, Little Bear

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Kaler, James B. (20 December 2013). "Pherkad". Stars. University of Illinois . Retrieved 18 May 2014. If you are a fan of the more realistic cold war spy story, then you are in for a treat. In fact, Big Bear Little Bear may have crept into my top five best spy novels ever written. Eta Ursae Minoris". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg . Retrieved 30 July 2014. Little London Bear Candy Cane Lane Shirt, Cute Christmas Bear Shirt, Paddington Bear Christmas Shirt, Paddington Bear in London Shirt

Big Bear, Little Bear by Marine Schneider, Board Book Big Bear, Little Bear by Marine Schneider, Board Book

Zeta Ursae Minoris – Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg . Retrieved 21 June 2014. Organic crawling shoes with name (personalized leather punches) with Indian bear - baby, child, toddler - Handmade gift a b c Ridpath, Ian. "Constellations: Lacerta–Vulpecula". Star Tales. Self-published . Retrieved 21 June 2014. Little London Bear Candy Cane Lane Sweatshirt, Paddington Bear Christmas Sweatshirt, Cute Bear Sweatshirt, Paddington Bear in London Hoodie O'Meara, Stephen James (2007). Steve O'Meara's Herschel 400 Observing Guide. Cambridge, UK: Cambridge University Press. p.227. ISBN 978-0-521-85893-9.Because Ursa Minor consists of seven stars, the Latin word for "north" ( i.e., where Polaris points) is septentrio, from septem (seven) and triones ( oxen), from seven oxen driving a plough, which the seven stars also resemble. This name has also been attached to the main stars of Ursa Major. [16]

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Brown (1899) suggested a non-Greek origin of the name (a loan from an Assyrian An‑nas-sur‑ra "high-rising"). [14] 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] Big Bear, Little Bear is a simple board book with a sweet take on contrasts, featuring a parent and child from Marine Schneider. Big Bear ski print - California, Big Bear ski poster, Wedding gift, Birthday present, Custom Text, Personalised Gift

Traditionally known as Pherkad, Gamma Ursae Minoris has an apparent magnitude that varies between 3.04 and 3.09 roughly every 3.4hours. [32] It and Kochab have been termed the "guardians of the pole star". [3] A white bright giant of spectral type A3II-III, [32] with around 4.8times the Sun's mass, 1,050times its luminosity and 15times its radius, [33] it is 487±8 light-years distant from Earth. [28] Pherkad belongs to a class of stars known as Delta Scuti variables [32]—short period (six hours at most) pulsating stars that have been used as standard candles and as subjects to study asteroseismology. [34] Also possibly a member of this class is Zeta Ursae Minoris, [35] a white star of spectral type A3V, [36] which has begun cooling, expanding and brightening. It is likely to have been a B3 main-sequence star and is now slightly variable. [35] At magnitude 4.95 the dimmest of the seven stars of the Little Dipper is Eta Ursae Minoris. [37] A yellow-white main-sequence star of spectral type F5V, it is 97 light-years distant. [38] It is double the Sun's diameter, 1.4times as massive, and shines with 7.4times its luminosity. [37] Nearby Zeta lies 5.00-magnitude Theta Ursae Minoris. Located 860 ± 80light-years distant, [39] it is an orange giant of spectral type K5III that has expanded and cooled off the main sequence, and has an estimated diameter around 4.8times that of the Sun. [40] Perley, R. A.; Bridle, A. H.; Willis, A. G. (1984). "High-resolution VLA Observations of the Radio Jet in NGC 6251". Astrophysical Journal Supplement Series. 54: 291–334. Bibcode: 1984ApJS...54..291P. doi: 10.1086/190931. O'Meara, Stephen James (1998). The Messier Objects. Deep-sky Companions. Cambridge, UK: Cambridge University Press. p. 10. ISBN 978-0-521-55332-2.

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NGC 6251 – Seyfert 2 Galaxy". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg . Retrieved 21 July 2015. a b c d e f "Ursa Minor, Constellation Boundary". The Constellations. International Astronomical Union . Retrieved 12 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]Rogers, John H. (1998). "Origins of the Ancient Constellations: II. The Mediterranean traditions". Journal of the British Astronomical Association. 108: 79–89. Bibcode: 1998JBAA..108...79R.

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Mama Bear Shirt - Papa Bear - Baby Bear - Little Bear - "Custom" Bear - Family Set - Family Shirt Set - Mama Bear SetLee, B.-C.; Han, I.; Park, M.-G.; Mkrtichian, D.E.; Hatzes, A.P.; Kim, K.-M. (2014). "Planetary Companions in K giants β Cancri, μ Leonis, and β Ursae Minoris". Astronomy and Astrophysics. 566: 7. arXiv: 1405.2127. Bibcode: 2014A&A...566A..67L. doi: 10.1051/0004-6361/201322608. S2CID 118631934. A67. Bianchini, A.; Tappert, C.; Canterna, R.; Tamburini, F.; Osborne, H.; Cantrell, K. (2003). "RW Ursae Minoris (1956): An Evolving Postnova System". Publications of the Astronomical Society of the Pacific. 115 (#809): 811–18. Bibcode: 2003PASP..115..811B. doi: 10.1086/376434. 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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