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Resultaten voor 'oscar'
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(170025) 2002 VO
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. (170025) 2002 VO is a main-belt minor planet. A minor planet is an astronomical object in direct orbit around the Sun that is neither a dominant planet nor a comet, and thus includes the dwarf planets. The orbital categories of minor planets are the asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. The first minor planet discovered was Ceres in 1801. The orbits of more than 540,000 objects have been archived at the Minor Planet Center. The term "minor planet" has been used since the 19th century to describe these objects.
€ 156,00 -
Rodney Hill
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Rodney Hill FRS (11 June 1921 - 2 February 2011) was an applied mathematician and a former Professor of Mechanics of Solids at Gonville and Caius College, Cambridge. In 1953 he was appointed Professor of Applied Mathematics at Nottingham University. His 1950 The Mathematical Theory of Plasticity forms the foundation of Plasticity Theory. Hill is widely regarded as among the foremost contributors to the foundations of solid mechanics over the second half of the 20th century. His early work was central to founding the mathematical theory of plasticity. This deep interest led eventually to general studies of uniqueness and stability in nonlinear continuum mechanics, work which has had a profound influence on the field of solid mechanics - theoretical, computational and experimental alike - over the past decades.
€ 156,00 -
11280 Sakurai
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 11280 Sakurai is a main-belt asteroid. The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt is also termed the main asteroid belt or main belt because there are other asteroids in the Solar System such as near-Earth asteroids and trojan asteroids. Maybe half the mass of the belt is contained in the four largest asteroids: 1 Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea. These have mean diameters of more than 400 km, while Ceres, the asteroid belt's only identified dwarf planet, is about 950 km in diameter.
€ 156,00 -
2285 Ron Helin
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 2285 Ron Helin is a main-belt asteroid. The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt is also termed the main asteroid belt or main belt because there are other asteroids in the Solar System such as near-Earth asteroids and trojan asteroids. Maybe half the mass of the belt is contained in the four largest asteroids: 1 Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea. These have mean diameters of more than 400 km, while Ceres, the asteroid belt's only identified dwarf planet, is about 950 km in diameter.
€ 156,00 -
3372 Bratijchuk
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3372 Bratijchuk is a main-belt minor planet. A minor planet is an astronomical object in direct orbit around the Sun that is neither a dominant planet nor a comet, and thus includes the dwarf planets. The orbital categories of minor planets are the asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. The first minor planet discovered was Ceres in 1801. The orbits of more than 540,000 objects have been archived at the Minor Planet Center. The term "minor planet" has been used since the 19th century to describe these objects.
€ 156,00 -
15379 Alefranz
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 15379 Alefranz is a main-belt minor planet. A minor planet is an astronomical object in direct orbit around the Sun that is neither a dominant planet nor a comet, and thus includes the dwarf planets. The orbital categories of minor planets are the asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. The first minor planet discovered was Ceres in 1801. The orbits of more than 540,000 objects have been archived at the Minor Planet Center. The term "minor planet" has been used since the 19th century to describe these objects.
€ 156,00 -
(14844) 1988 VT3
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. (14844) 1988 VT3 is a main-belt minor planet. A minor planet is an astronomical object in direct orbit around the Sun that is neither a dominant planet nor a comet, and thus includes the dwarf planets. The orbital categories of minor planets are the asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. The first minor planet discovered was Ceres in 1801. The orbits of more than 540,000 objects have been archived at the Minor Planet Center. The term "minor planet" has been used since the 19th century to describe these objects.
€ 136,00 -
Splendrillia Coccinata
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Splendrillia coccinata is a species of sea snail, a marine gastropod mollusk in the family Drilliidae. The Gastropoda or gastropods, more commonly known as snails and slugs, are a large taxonomic class within the Mollusca. The class Gastropoda includes snails and slugs of all kinds and all sizes from microscopic to quite large. There are huge numbers of sea snails and sea slugs, as well as freshwater snails and freshwater limpets, and land snails and land slugs.
€ 116,00 -
25176 Thomasaunins
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 25184 Taylorgaines (provisional designation: 1998 SL115) is a main-belt minor planet. It was discovered by the Lincoln Near-Earth Asteroid Research project in Socorro, New Mexico, on September 26, 1998. It is named after Taylor Diahann Gaines, an American student and finalist in the 2008 Society for Science & the Public middle school science competition. Asteroids (from Greek ¿¿¿¿¿ 'star' and ¿¿¿¿¿ 'like, in form') are a class of Small Solar System Bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closely resemble comets, and so were often distinguished from traditional asteroids.
€ 156,00 -
4246 Telemann
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 4246 Telemann (1982 SY2) is a main-belt asteroid discovered on September 24, 1982 by Freimut Börngen at Tautenburg. Asteroids (from Greek ¿¿¿¿¿ 'star' and ¿¿¿¿¿ 'like, in form') are a class of Small Solar System Bodies in orbit around the Sun. They have also been called planetoids, especially the larger ones. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disk of a planet and was not observed to have the characteristics of an active comet, but as small objects in the outer Solar System were discovered, their volatile-based surfaces were found to more closely resemble comets, and so were often distinguished from traditional asteroids.
€ 156,00 -
3454 Lieske
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3454 Lieske is a main-belt asteroid. The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets. The asteroid belt is also termed the main asteroid belt or main belt because there are other asteroids in the Solar System such as near-Earth asteroids and trojan asteroids. Maybe half the mass of the belt is contained in the four largest asteroids: 1 Ceres, 4 Vesta, 2 Pallas, and 10 Hygiea. These have mean diameters of more than 400 km, while Ceres, the asteroid belt's only identified dwarf planet, is about 950 km in diameter.
€ 136,00 -
3749 Balam
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. 3749 Balam is a main-belt minor planet. A minor planet is an astronomical object in direct orbit around the Sun that is neither a dominant planet nor a comet, and thus includes the dwarf planets. The orbital categories of minor planets are the asteroids, trojans, centaurs, Kuiper belt objects, and other trans-Neptunian objects. The first minor planet discovered was Ceres in 1801. The orbits of more than 540,000 objects have been archived at the Minor Planet Center. The term "minor planet" has been used since the 19th century to describe these objects.
€ 156,00