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Unit 3
The Solar System
| Term | Definition |
|---|---|
| Solar system | The solar system is the sun and all of the bodies that orbit the sun. |
| heliocentric | In the heliocentric model, Earth and the other planets orbit the sun. |
| geocentric | These models, which used Earth as the center, are called Earth-centered |
| Gravity | Gravity is a force of attraction between objects that is due to their masses and the distances between them. |
| orbit | An orbit is the path that a body follows as it travels around another body in space. |
| aphelion | When an object follows an elliptical orbit around the sun, there is one point |
| perihelion | where the object is closest to the sun. |
| Centripetal force | The inward Force required to keep particle or an object moving in a circular path. |
| Solar nebula | A rotating cloud of gas and dust from which the sun and planets formed. |
| Planetesimal | A small body from which a planet originated in the early stages of development of the solar system |
| Nuclear fusion | The process by which nuclei of small atoms combine to form a new, more massive nucleus; the process releases energy. |
| Sunspots | A dark area of the photosphere of the sun that is cooler than the surrounding areas and that has a strong magnetic field |
| Solar flare | An explosive release of energy that comes from the sun and that is associated with magnetic disturbances on the sun's surface. |
| Prominence | A loop of relatively cool, incandescent gas that extends above the photosphere and above the sun's edge as seen from Earth. |
| Terrestrial planet | One of the highly dense planets nearest to the sun Mercury, Venus, Mars, and Earth. |
| Astronomical Unit | The average distance between Earth and the sun; approximately 150 million kilometers symbol, AU. |