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Solar System Study Guide Solar System The sun, the eight planets and all the celestial bodies (moons, asteroids, comets meteoroids) that orbit the sun in its gravitational pull. The solar system is 4.6 billion years old. Geocentric The belief that the Earth was the center of the solar system. Heliocentric The belief that the sun is in the center of the solar system. Planet Celestial object that revolves around a star. Asteroid A solid body that orbits the sun. (Minor planets or planetoids.) Asteroid Belt 90% of the asteroids are found orbiting in between Mars and Jupiter. Comet An icy body that releases gases or dust AKA dirty snowballs. Comets travel around the sun in long, highly elliptical orbits. Meteoroid A sand to boulder size particle of rocky, metallic (iron-nickel) debris in our solar system. Meteor In Earth’s atmosphere AKA “shooting star” Meteorite Right on Earth’s surface. Gravity The attractive force that exists between every object in the Universe. Gravity is stronger than natures other fundamental forces, because it acts over great distances and between all bodies of possessing mass. Gravity has played a major part in shaping the Universe. It is also crucial in determining orbits and creating phenomena such as planetary rings and black holes. As mass increases, gravitational pull increases. As distance increases, gravitational pull decreases. Gravity is responsible for rings and the gas planets. Terrestrial Planets Mercury, Venus, Earth and Mars. Solid and rocky (iron/nickel core and silicate surface.) Low Mass Small Volume High Density State of Matter: Solid Atmosphere: Carbon dioxide, nitrogen, and oxygen. Little or no atmosphere. Small and less moons. Few or no moons. No rings Jovian Planets Jupiter, Saturn, Uranus and Neptune. Gaseous (Hydrogen, Helium, Methane, Gas and rock core) High Mass Large Volume Low Mass State of Matter: Gas Atmosphere: Hydrogen, helium and methane. (Thick atmosphere) Bigger and greater moons. Greater than 20 moons. Many rings The solar system formed from a gigantic cloud of gas and dust called the solar nebula. This cloud was seven times bigger than the sun. It collapsed into a flat, spinning disk, which had a hot, dense central region. This central part of the disk became the Sun, while the planets and everything else formed from the remaining material.