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Gravity/Universe
Space Distance and Objects
| Term | Definition |
|---|---|
| astronomical unit (AU) | the average distance between the Sun and the Earth, 150,000 million km, 93 million miles |
| light year | the distance light travels in one year, 9.46 trillion km, 5.88 trillion miles |
| rotate | movement of an object on its axis, one day |
| revolve | movement of an object in its orbit around the Sun, one year |
| gravity | a force that every object exerts on another object because of mass, determined by mass and distance between objects |
| planet | an object that orbits the Sun, is spherical in shape, and has cleared its orbit |
| dwarf planet | do not have clear orbits and are made of rock and ice, at least 5 in our solar system |
| asteroid | small, rocky, oddly shaped objects that orbit the Sun in the asteroid belt which separates the inner and outer planets |
| comets | made of gas, dust, and ice and have an oval shaped orbit around the sun |
| meteors | shooting stars, made of metal and rock |
| star | a giant ball of super hot plasma, hydrogen fuses into helium during nuclear fusion creating heat and energy |
| solar system | part of a galaxy, containing at least one star, orbiting planets, and smaller objects |
| galaxy | a massive collection of billions of stars, gas, dust, and dark matter, all bound together by gravity |
| universe | all matter (planets, stars, galaxies, you), all energy, space, and time, originating from a hot, dense point about 13.8 billion years ago in the Big Bang and constantly expanding |
| geocentric model | the model of the universe showing all objects orbiting in a circular orbit around a central, stationary Earth |
| heliocentric model | the model of the solar system showing planets orbiting in an elliptical orbit around the Sun |