Jupiter is the largest planet in the solar system, over 10 times the diameter of Earth. It is made up primarily of hydrogen and helium and has a turbulent, colorful atmosphere with the Great Red Spot, a giant storm that has raged for over 300 years. Jupiter has over 60 moons, four of which - Io, Europa, Ganymede, and Callisto - were discovered by Galileo and are some of the largest in the solar system.
Jupiter is the largest planet in the solar system, over 10 times the diameter of Earth. It is made up primarily of hydrogen and helium and has a turbulent, colorful atmosphere with the Great Red Spot, a giant storm that has raged for over 300 years. Jupiter has over 60 moons, four of which - Io, Europa, Ganymede, and Callisto - were discovered by Galileo and are some of the largest in the solar system.
Uranus was the first planet discovered with a telescope by William Herschel in 1781, though he initially thought it was a comet. It orbits the sun every 84 Earth years at a distance of about 3 billion km. Uranus rotates on its side with an axial tilt of 98 degrees, and has 27 known moons as well as 13 known rings composed of small, dark particles. Uranus is composed of ice and rock, and has a blue-green color due to the scattering of light by methane ice crystals in its atmosphere.
Jupiter is the largest planet in our solar system, with a diameter 11 times larger than Earth. It rotates very quickly, completing a rotation in just 10 hours, and has over 63 known moons. Jupiter is made primarily of hydrogen and helium, and has colorful bands and zones created by strong winds, as well as the famous Great Red Spot storm that has raged for over 300 years.
Saturn is the 6th planet from the Sun and 2nd largest in the solar system. It is made up primarily of hydrogen and helium and has a dense atmosphere. Saturn is most notable for its extensive ring system composed of ice particles. The rings were first observed by Galileo in 1610 but their nature was not understood until the late 1600s. Modern space probes like Voyager and Cassini have revealed Saturn's atmospheric composition and weather patterns as well as details of its interior structure and ring system.
Powerpoint presentation discussing six of the planets in our solar system: Earth, Saturn, Mars, Jupiter, Venus and Pluto.
The presentation includes credible information on the above planets which include - descriptions, moons, rings, sizes and interesting facts.
Images and references are provided.
Collaborated by Ash Bell, Catherine Bond, Charlie Miles, Olivia McMillan, Paige Harrington and Phil Rodis of Swinburne University of Technology, 2014.
El documento presenta información sobre los planetas del Sistema Solar. Comienza describiendo brevemente al Sol y sus capas, luego resume los datos básicos y características de los planetas terrestres como Mercurio, Venus y la Tierra. También habla sobre los planetas gaseosos Júpiter y Saturno, destacando la Gran Mancha Roja en Júpiter y los anillos de Saturno.
The Solar System consists of the Sun and everything that orbits it, including 8 planets, Pluto, moons, asteroids, comets and other objects. The 4 inner planets are small and rocky, while the 4 outer planets are large gas giants. The document describes each planet's characteristics such as composition, size, orbital period, moons, temperature and other features. It explains that the Sun is at the center and provides energy through nuclear fusion, while planets reflect sunlight.
Venus is the second planet from the Sun and has the densest atmosphere of the terrestrial planets. It rotates backwards compared to most planets and has no natural satellites. Venus is similar in size and mass to Earth but has extreme surface temperatures due to a runaway greenhouse effect. The surface is covered in volcanic plains and has few impact craters, indicating its surface is geologically young. The thick carbon dioxide atmosphere creates an intense greenhouse effect, trapping heat and causing surface temperatures over 460°C. Despite being closer to the Sun, Venus is the hottest planet due to its atmospheric composition. Venus has played an important role in many human cultures throughout history.
The solar system consists of the Sun and everything bound to it by gravity, including 8 planets that orbit the Sun. The planets are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Other objects in the solar system include asteroids, comets, and meteors. Each planet has unique characteristics such as size, composition, temperature, and number of moons. Earth stands out as the only known planet capable of supporting life.
The document summarizes the formation of the solar system based on the nebular hypothesis. It explains that the solar system formed from the gravitational collapse of a giant gas and dust cloud about 4.6 billion years ago. As the cloud collapsed and spun faster, the heavier elements collected in the center to form the inner terrestrial planets, while the outer parts formed the outer gaseous jovian planets. Over time, small particles collided and merged to form larger bodies called planetesimals, which eventually formed the planets.
The document provides information about the planets and dwarf planets in our solar system. It describes the 8 major planets and 5 dwarf planets, and discusses their key characteristics such as composition, atmosphere, rotation, and moons. Examples include Mercury having no atmosphere and many impact craters, Venus rotating backwards and having extreme temperatures, and Pluto being the first and largest dwarf planet discovered.
The document describes the inner and outer planets of the solar system, as well as their natural and artificial satellites. It provides details about the moons of each planet, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also discusses different types of artificial satellites such as communication, resource, navigation, military, scientific, and weather satellites and how they are used.
Neptune is the 8th and farthest planet from the Sun. It is smaller than Uranus but more massive. Neptune was discovered in 1846 based on calculations by Urbain Le Verrier and independent predictions by John Couch Adams. Voyager 2 is the only spacecraft to have visited Neptune, discovering its rings and 6 of its 14 known moons during a flyby in 1989. Neptune has a rocky core and is composed primarily of ice giants with winds reaching over 1,500 mph.
The document summarizes tides, including their causes due to the gravitational interaction between the Earth, Moon and Sun. It describes the stages of a tidal cycle from flood tide to low tide. It distinguishes between spring tides, which occur during full and new moons when gravitational forces align to produce stronger tides, and neap tides during quarter moons when forces are perpendicular and tides are weaker. Rare proxigean spring tides result from a close and aligned positioning of the Moon.
The document discusses the 8 planets in our solar system - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It describes their key characteristics such as composition, size, distance from the sun, temperature, and number of moons. The inner planets are smaller and rockier, while the outer planets are giant gas planets. Features such as rings are unique to Saturn. The document also provides details about specific planets like the extreme temperatures on Mercury and Venus.
The ancient Greeks observed that objects in the sky seemed to move in circles around the Earth, leading to the geocentric model where the Earth is at the center of the universe. Ptolemy refined earlier Greek astronomical models, proposing that planets moved in smaller circles within larger circles, called the Ptolemaic model. This view persisted for over 1500 years until Copernicus and Galileo proposed the heliocentric model, which placed the Sun at the center. Today we recognize our Solar System formed from a collapsing cloud of gas and dust around the Sun, resulting in terrestrial, rocky planets near the Sun and larger gaseous Jovian planets farther out.
Urano es el séptimo planeta del Sistema Solar. Fue descubierto en 1781 y se formó por la condensación de gases. Tiene un núcleo de hielo y rocas, una atmósfera que representa el 15% de su masa planetaria y temperaturas extremadamente frías. La misión Voyager 2 en 1986 proporcionó mayor comprensión de la atmósfera de Urano, el descubrimiento de satélites pequeños y las primeras observaciones de sus anillos.
Uranus was the first planet discovered with a telescope by William Herschel in 1781, though he initially thought it was a comet. It orbits the sun every 84 Earth years at a distance of about 3 billion km. Uranus rotates on its side with an axial tilt of 98 degrees, and has 27 known moons as well as 13 known rings composed of small, dark particles. Uranus is composed of ice and rock, and has a blue-green color due to the scattering of light by methane ice crystals in its atmosphere.
Jupiter is the largest planet in our solar system, with a diameter 11 times larger than Earth. It rotates very quickly, completing a rotation in just 10 hours, and has over 63 known moons. Jupiter is made primarily of hydrogen and helium, and has colorful bands and zones created by strong winds, as well as the famous Great Red Spot storm that has raged for over 300 years.
Saturn is the 6th planet from the Sun and 2nd largest in the solar system. It is made up primarily of hydrogen and helium and has a dense atmosphere. Saturn is most notable for its extensive ring system composed of ice particles. The rings were first observed by Galileo in 1610 but their nature was not understood until the late 1600s. Modern space probes like Voyager and Cassini have revealed Saturn's atmospheric composition and weather patterns as well as details of its interior structure and ring system.
Powerpoint presentation discussing six of the planets in our solar system: Earth, Saturn, Mars, Jupiter, Venus and Pluto.
The presentation includes credible information on the above planets which include - descriptions, moons, rings, sizes and interesting facts.
Images and references are provided.
Collaborated by Ash Bell, Catherine Bond, Charlie Miles, Olivia McMillan, Paige Harrington and Phil Rodis of Swinburne University of Technology, 2014.
El documento presenta información sobre los planetas del Sistema Solar. Comienza describiendo brevemente al Sol y sus capas, luego resume los datos básicos y características de los planetas terrestres como Mercurio, Venus y la Tierra. También habla sobre los planetas gaseosos Júpiter y Saturno, destacando la Gran Mancha Roja en Júpiter y los anillos de Saturno.
The Solar System consists of the Sun and everything that orbits it, including 8 planets, Pluto, moons, asteroids, comets and other objects. The 4 inner planets are small and rocky, while the 4 outer planets are large gas giants. The document describes each planet's characteristics such as composition, size, orbital period, moons, temperature and other features. It explains that the Sun is at the center and provides energy through nuclear fusion, while planets reflect sunlight.
Venus is the second planet from the Sun and has the densest atmosphere of the terrestrial planets. It rotates backwards compared to most planets and has no natural satellites. Venus is similar in size and mass to Earth but has extreme surface temperatures due to a runaway greenhouse effect. The surface is covered in volcanic plains and has few impact craters, indicating its surface is geologically young. The thick carbon dioxide atmosphere creates an intense greenhouse effect, trapping heat and causing surface temperatures over 460°C. Despite being closer to the Sun, Venus is the hottest planet due to its atmospheric composition. Venus has played an important role in many human cultures throughout history.
The solar system consists of the Sun and everything bound to it by gravity, including 8 planets that orbit the Sun. The planets are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Other objects in the solar system include asteroids, comets, and meteors. Each planet has unique characteristics such as size, composition, temperature, and number of moons. Earth stands out as the only known planet capable of supporting life.
The document summarizes the formation of the solar system based on the nebular hypothesis. It explains that the solar system formed from the gravitational collapse of a giant gas and dust cloud about 4.6 billion years ago. As the cloud collapsed and spun faster, the heavier elements collected in the center to form the inner terrestrial planets, while the outer parts formed the outer gaseous jovian planets. Over time, small particles collided and merged to form larger bodies called planetesimals, which eventually formed the planets.
The document provides information about the planets and dwarf planets in our solar system. It describes the 8 major planets and 5 dwarf planets, and discusses their key characteristics such as composition, atmosphere, rotation, and moons. Examples include Mercury having no atmosphere and many impact craters, Venus rotating backwards and having extreme temperatures, and Pluto being the first and largest dwarf planet discovered.
The document describes the inner and outer planets of the solar system, as well as their natural and artificial satellites. It provides details about the moons of each planet, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It also discusses different types of artificial satellites such as communication, resource, navigation, military, scientific, and weather satellites and how they are used.
Neptune is the 8th and farthest planet from the Sun. It is smaller than Uranus but more massive. Neptune was discovered in 1846 based on calculations by Urbain Le Verrier and independent predictions by John Couch Adams. Voyager 2 is the only spacecraft to have visited Neptune, discovering its rings and 6 of its 14 known moons during a flyby in 1989. Neptune has a rocky core and is composed primarily of ice giants with winds reaching over 1,500 mph.
The document summarizes tides, including their causes due to the gravitational interaction between the Earth, Moon and Sun. It describes the stages of a tidal cycle from flood tide to low tide. It distinguishes between spring tides, which occur during full and new moons when gravitational forces align to produce stronger tides, and neap tides during quarter moons when forces are perpendicular and tides are weaker. Rare proxigean spring tides result from a close and aligned positioning of the Moon.
The document discusses the 8 planets in our solar system - Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. It describes their key characteristics such as composition, size, distance from the sun, temperature, and number of moons. The inner planets are smaller and rockier, while the outer planets are giant gas planets. Features such as rings are unique to Saturn. The document also provides details about specific planets like the extreme temperatures on Mercury and Venus.
The ancient Greeks observed that objects in the sky seemed to move in circles around the Earth, leading to the geocentric model where the Earth is at the center of the universe. Ptolemy refined earlier Greek astronomical models, proposing that planets moved in smaller circles within larger circles, called the Ptolemaic model. This view persisted for over 1500 years until Copernicus and Galileo proposed the heliocentric model, which placed the Sun at the center. Today we recognize our Solar System formed from a collapsing cloud of gas and dust around the Sun, resulting in terrestrial, rocky planets near the Sun and larger gaseous Jovian planets farther out.
Urano es el séptimo planeta del Sistema Solar. Fue descubierto en 1781 y se formó por la condensación de gases. Tiene un núcleo de hielo y rocas, una atmósfera que representa el 15% de su masa planetaria y temperaturas extremadamente frías. La misión Voyager 2 en 1986 proporcionó mayor comprensión de la atmósfera de Urano, el descubrimiento de satélites pequeños y las primeras observaciones de sus anillos.
Raport Media2.pl - Badania Internetu z artykułem Mariusza Karbowskiego (Wyszukali.pl) pod tytułem "Aktywni konsumenci, trendsetterzy
i grupy wyznawców"
Projekt Edukacja ekonomiczna z wykorzystaniem gry symulacyjnej „Chłopska Szkoła Biznesu”- sprawozdanie merytoryczne z raportem ewaluacyjnym
Projekt został zrealizowany przez Małopolski Instytut Kultury w Krakowie we współpracy z Gminą Andrychów od czerwca 2012 roku do kwietnia 2013 roku.
Projekt dofinansowano ze środków Narodowego Banku Polskiego
Więcej o grze symulacyjnej „Chłopska Szkoła Biznesu”: www.csb.mik.krakow.pl
Człowiek jest gatunkiem, który w niespotykanym do tej pory zakresie czerpie z zasobów środowiska, przekształca krajobrazy i ekosystemy, próbuje zapanować nad procesami biologicznymi toczącymi się w jego organizmie. Coraz mniej odległe wydaje się opóźnienie starzenia, zachowanie przy życiu niemal każdego noworodka oraz poprawa wydajność produkcji przemysłowej, zwłaszcza produkcji żywności. Koszty tych technologii są jednak wysokie i towarzyszą im budzące obawy skutki uboczne. Ich konsekwencją jest m.in. nieodwracalna zmiana warunków życia i zanik różnorodności biologicznej. Czy te wszystkie koszty są uzasadnione? Ucząc się z biologii z podręcznika do pierwszej klasy ponadgimnazjalnej, będziecie mieli okazję zachwycić się możliwościami nowych technologii oraz poddać ocenie działania człowieka.
El documento proporciona información sobre la historia, epidemiología, definición, fisiopatología y clínica de la diabetes mellitus tipo 1 y 2. Explica que la diabetes ha sido documentada desde hace miles de años y describe las etapas de progresión de la diabetes tipo 2, la cual afecta principalmente a adultos y se debe principalmente a resistencia a la insulina. También destaca que América Latina tiene altas tasas de diabetes debido a factores genéticos y de estilo de vida, y que representa una gran carga económica para los
2. Witaj! Teraz, pokażę Ci jak zbudowany jest wszechświat. Poznasz planety układu słonecznego, dowiesz się co to jest gwiazda i asteroida oraz kim był Mikołaj Kopernik.
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10. Ziemia – dane liczbowe Średnica wokół równika 12 756,270 km Powierzchnia 510 065 284,702 km² Objętość 1,0832×10 12 km³ Masa 5,9736×10 24 kg Średnia temperatura powierzchni 287K Okres obiegu wokół Słońca 365dni Okres obrotu wokół własnej osi 24h Liczna księżyców 1
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12. Mars - dane liczbowe Odkrywca Nieznany Średnica wokół równika 6 804.9 km (0.533 śr. Ziemi) Powierzchnia 1.448×10 8 km 2 (0.284 pow. Ziemi) Objętość 1.638×10 11 km 3 (0.151 obj. Ziemi) Masa 6.4185×10 23 kg (0.105 m. Ziemi) Średnia temp 210 K Okres obiegu wokół Słońca 687 dni Okres obrotu wokół własnej osi 24,62 h Licz b a księżyców 2
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14. Jowisz - dane liczbowe Jowisz posiada 3 pierścienie: Ażurowy, Główny i Halo. Zdjęcie w tle przedstawia porównanie wielkości Jowisza i Ziemi. Odkrywca Nieznany Średnica wokół równika 142 984 km(11.2089 śr.Ziemi) Powierzchnia 621 796×10 5 km 2 (121.9 pow. Ziemi) Objęto ść 14 255×10 11 km 3 (13obj. Ziemi) Masa 18 987×10 23 kg (317.8 m. Ziemi) Średnia temp 152 K Okres obiegu wokół Słońca 11,86 lat Okres obrotu wokół własnej osi 9,84 h Licz b a księżyców 63
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18. Uran- dane liczbowe Odkrywca William Herschel (13 marca 1781) Średnica równikowa 51 118 km (4,007 śr. Ziemi) Powierzchnia 8,084×10 9 km 2 (15,849 pow. Ziemi) Objętość 6,834×10 13 km 3 (63,086 obj. Ziemi) Masa 8,6832×10 25 kg (14,536 m. Ziemi) Średnia temperatura 68 K Okres obiegu wokół Słońca 84,01 lat Okres obiegu wokół własnej osi 17,23 h Liczba księżyców 27
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20. Neptun - dane liczbowe Odkrywca Johann Gale (1846r) Średnica wokół równika 49500 km (3,880 śr. Ziemi) Powierzchnia 7,619×10 9 km 2 (14,937 pow. Ziemi) Objętość 6,2526×10 13 km 3 (57,723 obj. Ziemi) Masa 1,0243×10 26 kg (17,147 masy Ziemi) Okres obiegu wokół Słońca 16,04 h Okres obrotu wokół własnej osi 1644,79 lat Okres obrotu wokół własnej osi 18h Liczba księżyców 8