1st quarter es review
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Created by:
FAITHSBOYZ on November 5, 2010
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41 terms
Terms | Definitions |
|---|---|
Inference | An interpretationg of an observation. |
Measurement | Means of expressing an observation with greater accuracy or precision. |
Mass | The amount of matter in an object. |
Volume | The amount of space that an object occupies. |
Density | The concentration of matter in an object. |
Change | Occurs when the properties or characteristics of a part of the environment have been altered. |
Event | The ovvurrence of a change in the properties of an object or a system. |
Field | How much a meazsurable aspect of the environment. |
Prediction | A type of inference about the conditions and behavior of the environment in the future. |
Natural Hazard | A non-human-related object, process, or situation that has the possibiolity of causing loss of life, personal injury, or loss of property. |
Interface | The boundary between regions with different properties. |
Dynamic Equilibrium | Evironmental equilibrium resulting from opposing forces or actions balancing out. |
Natural Resources | The materials and energy sources found in the environment that humans use in their daily lives. |
Pollution | The environment occurs when the concentration of any substance or form of energy reaches a proportion that adversely affects people or their property, or other life forms. |
Model | A way of representing the properties of an object or system. |
Atmosphere | The layer of gases that surrounds Earth above the surface of liquid water and rocky material. |
Pauses | The interfaces, or boundaries, of the layers of Earth's atmosphere. |
Hydrosphere | The layer of liquid water that lies between the atmosphere and much of the upper layer of Earth's interior. |
Lithosphere | The layer of rock that forms the solid outer shell at the top of Earth's interior. |
Crust | Upper portion of the lithosphere. |
Soil | Material contains abundant organic matter. |
Earth's Interior | The region extending from the rocky part of Earth's surface to Earth's center. |
Gradient | The rate of change from place to place within the field. |
Galaxy | A huge group of stars held together by gravity. |
Milky Way Galaxy | The group of billions of stars that includes the sun and our solar system, it is visible as a faint band of light acrss the night sky |
Light-Year | The distance electromagnetic energy can travel in one year, approximately 6 trillion miles (10 trillion km) |
Red Shift | A displacementr of the spectral lines of very distant stars and galaxies, an invrease in the wavelength of starlight caused by rapid relative motion of star waway from the observer. |
Doppler Effect | The apparent change in frequency and wavelenth of energy radiated by a source as a result of the motion of the source or the ovserver |
Cosmic Backround Radiation | Weak electromagnetic radiation (radio waves) left over from the formation of the universe (big bang) |
Big Bang Theory | The theory that the universe formed as a concentration of matter expanded explosively |
Liminosity | The acrual brightness of a star or rate of total energy emitted compared to the Sun. |
Nuclear Fusion | The combining of the nuclei of smaller elements with some of the mas being converted into energy. |
Star | Usually a large ball of gas held together by gravity that produces trmendous amounts of energy and shines. |
Terrestial Planets | Close to the sun and mostly solid. Mercury, Venus, Earth, and Mars. |
Jovian Planits | Far from the sun and are largely gaseous. Jupiter, Saturn, Uranus, and Neptune. |
Rotation | Planets spin on an imaginary axis in a motion. |
Revolution | Its movement around the sun in a path. |
Ellipse | Earth's orbit is an obal shape. |
Eccentricity | The out-of-roundness of an ellipse. |
Inertia | THe concept that an object at rest will rtend to remain at rest. |
Gravitation | The attractive force that exists between any two objects in the universe. |
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