Chapter 24
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The document provides an overview of the solar system, including its origin and components. It discusses: 1) The modern view that the solar system formed from a rotating cloud of gas and dust that condensed to form the Sun and planets as it contracted. 2) The inner planets Mercury, Venus, Earth, and Mars, including characteristics such as temperatures, atmospheres, and evidence of past water on Mars. 3) The outer planets Jupiter, Saturn, Uranus, and Neptune, noting their large sizes and gaseous compositions. Moons and rings are also mentioned.
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Saturn has an orbit of 1,429,000 km from the sun and is composed mostly of hydrogen and helium. Uranus has an orbit of 2,870,990,000 km from the sun and its atmosphere consists mostly of hydrogen, helium and methane. Neptune has an orbit of 4,504,000,000 km from the sun and has seven moons including Triton.
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Saturn has an orbit of 1,429,000 km from the sun and is composed mostly of hydrogen and helium. Uranus has an orbit of 2,870,990,000 km from the sun and its atmosphere consists mostly of hydrogen, helium and methane. Neptune has an orbit of 4,504,000,000 km from the sun and has seven moons including Triton.
Earth
Earth began forming over 4.6 billion years ago from a cloud of gas and dust that also formed the Sun and other planets. As the solar system developed, small objects called planetesimals collided and stuck together, eventually forming Earth. When Earth first formed, it was a hot molten planet bombarded by asteroids and comets. As it cooled over millions of years, the first life forms of bacteria emerged and the oceans and atmosphere developed. Today, Earth is a complex system made up of interacting spheres including the atmosphere, biosphere, geosphere, hydrosphere, and cryosphere that sustain life.
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The formation of the solar system began from a large cloud of gas and dust called the solar nebula. As the nebula collapsed due to gravity, it formed a disc with the sun at the center. Planetesimals within the disc collided and accreted to form the planets. The nebular theory explained many characteristics of the solar system but did not account for all observations. The modern condensation theory expanded on this model and better explained features such as the asteroid belt and comets through processes like condensation and fractionation within the early solar system.
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The Solar System formed from a large rotating cloud of gas and dust called a solar nebula. As the nebula condensed due to gravity, a central mass became the Sun and the remaining material formed rings that eventually became the planets. The Sun consists of an inner core where nuclear fusion occurs and surrounding layers including the photosphere, chromosphere, and corona. The eight major planets can be divided into terrestrial and Jovian planets. Smaller bodies like asteroids and comets also orbit the Sun.
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The solar system consists of the sun and everything that orbits it, including eight planets. The planets can be divided into inner terrestrial planets like Earth and outer gas giants like Jupiter. All the planets, along with smaller bodies like Pluto, formed from a rotating cloud of gas and dust called the solar nebula. The inner planets are rocky and dense while the outer planets are larger and gaseous due to forming farther from the sun.
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The inner planets Mercury, Venus, Earth, and Mars are similar to each other. They are the closest planets to the sun and are called terrestrial planets because they are rocky or earth-like. Mercury is the smallest planet and closest to the sun, with extreme temperature variations between its day and night sides. Venus is about the same size as Earth but has a dense carbon dioxide atmosphere that causes a runaway greenhouse effect and surface temperatures over 800 degrees Fahrenheit. Mars is about half the size of Earth, has a reddish appearance, seasonal polar ice caps, evidence of past water, and the lowest average temperature of the four inner planets.
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The document summarizes key facts about the four inner planets of our solar system: Mercury, Venus, Earth, and Mars. It provides details on each planet's diameter, mass, density, atmosphere, distance from the sun, orbital path, moons, surface features, and core composition. Notably, it describes Mercury as the closest planet to the sun with no moons and a heavily cratered surface. Venus is similar in size to Earth but has a dense carbon dioxide atmosphere and retrograde rotation. Earth is unique in its liquid water and life. Mars has the largest volcano in the solar system called Olympus Mons and two small moons.
The Solar System[1][1]
Saturn has an orbit of 1,429,000 km from the sun and is composed mostly of hydrogen and helium. Uranus has an orbit of 2,870,990,000 km from the sun and its atmosphere consists mostly of hydrogen, helium and methane. Neptune has an orbit of 4,504,000,000 km from the sun and has seven moons including Triton.
The Solar System[1][1] 1
Saturn has an orbit of 1,429,000 km from the sun and is composed mostly of hydrogen and helium. Uranus has an orbit of 2,870,990,000 km from the sun and its atmosphere consists mostly of hydrogen, helium and methane. Neptune has an orbit of 4,504,000,000 km from the sun and has seven moons including Triton.
Earth
Earth began forming over 4.6 billion years ago from a cloud of gas and dust that also formed the Sun and other planets. As the solar system developed, small objects called planetesimals collided and stuck together, eventually forming Earth. When Earth first formed, it was a hot molten planet bombarded by asteroids and comets. As it cooled over millions of years, the first life forms of bacteria emerged and the oceans and atmosphere developed. Today, Earth is a complex system made up of interacting spheres including the atmosphere, biosphere, geosphere, hydrosphere, and cryosphere that sustain life.
Our solar system
The solar system consists of the Sun and everything that orbits it, including 8 planets, their moons, asteroids, comets, and other small celestial objects. The inner planets closest to the Sun are Mercury, Venus, Earth, and Mars. The outer planets farther from the Sun are gas giants Jupiter, Saturn, Uranus, and Neptune. Smaller objects like asteroids and comets also orbit the Sun.
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This document provides an overview of the resources included in the Glencoe Science textbook for the chapter on plate tectonics. It includes reproducible student pages for hands-on activities, assessments, and materials for meeting individual student needs. It also provides transparency activities and teacher support materials such as lesson planning guides, answer keys, and Spanish translations.
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Atmosphere 15
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The document summarizes major periods in geologic time from the Precambrian era to present day. It describes how trilobites and other early life evolved and adapted to changing environments over millions of years. Major events included the formation of Pangaea during the Paleozoic era and mass extinctions at the boundaries of the Paleozoic and Mesozoic eras. During the Mesozoic, dinosaurs and early mammals appeared while flowering plants evolved in the Cretaceous period. The Cenozoic era saw continued evolution of mammals, mountain building, and the emergence of humans.
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Chapter 24
- 1. The Solar System Section I The Solar System
- 7. A cloud of material in the nebula slowly rotated in space
- 9. The cloud became more dense, rotated faster, heated up, and flattened to form a disk.
- 10. As the cloud contracted, it grew warmer, triggering a nuclear fusion reaction that created the Sun
- 29. Two small moons, Phobos and Deimos
- 35. The Great Red Spot is the most spectacular of Jupiter’s many constant high-pressure gas storms
- 37. Has rings
- 38. Has at least 61 moons – four are large and have atmospheres
- 51. Has at least 31 moons
- 56. Axis of rotation nearly parallel to plane of orbit
- 60. A. Comet: dust and rock particles combined with frozen water, methane, and ammonia.
- 61. 1. Halley’s comet: orbits Sun every 76 years.
- 62. 2. Oort Cloud: large group of comets surrounding solar system beyond Pluto.
- 63. 3. Amateur astronomers discovered Hale-Bopp in 1995.
- 64. 4. Comet structure: large dirty snowball of frozen rock and ice.
- 66. Comets vaporize and break up after passing close to the Sun several times. When the nucleus breaks up, pieces spread out. The dust and rock fragments are called Meteoroids .
- 67. B. (1.) Meteoroid : name given to small pieces of comet when they move through space.
- 68. B. (2.) Meteor : small meteoroid that burns up in Earth’s atmosphere.
- 69. B. (3.) Meteor Showers : occur when Earth’s orbit passes through a group of meteoroids that enter the atmosphere.
- 70. B. (4.) Meteorite : meteoroid that strikes Earth.
- 71. C. Asteroid : rock similar to that which formed planets.
- 72. C. (1.) Most asteroids lie in an asteroid belt located between Mars and Jupiter.
- 75. Near: The Near Earth Asteroid Rendezvous probe indicates asteroid 433 Eros has been in many collisions over time.