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Earth Science
Regents Basic Review NY
| Term | Definition |
|---|---|
| Density | material’s mass divided by its volume; (how much “stuff” is in a certain space) |
| Relative Humidity | how much water vapor is in the air compared to how much water vapor could be present in the air |
| Dew Point | the temperature to which the air must be cooled to reach water vapor saturation (no more water vapor can be added); where relative humidity is 100%: even though this value is a temperature, it can only be changed by adding or subtracting water vapor |
| Transpiration | release of water vapor into the air by plants |
| Evapotranspiration | evaporation and transpiration combined |
| Insolation | incoming solar radiation (sunlight) |
| “Duration of Insolation” | length of daylight (how long the sun shines); greatest on June 21 and shortest on December 21 |
| Angle of Insolation | height of sun measured in degrees; highest in summer and at noon; lowest in winter and at sunrise/sunset |
| Gradient | slope or steepness of change (think steepness of a hill). change in some value over distance. |
| Rate | how fast something happens/moves (think “speed”); change in some value over time. |
| Condensation | change from water vapor into liquid water (how clouds, dew and fog form) |
| Revolution | orbiting around another celestial body (Earth revolves around the sun) |
| Rotation | spinning on its axis (Earth rotates one time around in about 24 hours) |
| Spring tides | (higher high and lower low tides than normal) occur at full and new moon phases. |
| Solar eclipses | occur at new moon phase |
| Lunar eclipses | occur at full moon phase |
| Jovian (Jupiter-like) | planets are large and made mostly of low density gas |
| Terrestrial planets (Earth-like) | Terrestrial planets (Earth-like) are smaller, high-density rocky/metallic spheres. |
| Nuclear fusion of hydrogen atoms into helium | is the source for the sun’s energy. |
| the “Big Bang”. | The universe is expanding and has been since |
| Red Shift: | indicates stars/galaxies moving away from the observer. |
| Contour lines | point upstream/uphill (lines form a v-shape). |
| Latitude lines | are drawn east-west, but measure distances north and south of the equator. (Remember: latitude=flatitude) |
| Longitude lines | are drawn north-south, but measure distances east or west of the Prime Meridian. |
| Summer solstice | June 21st; longest daylight (duration of insolation) of the year; our highest noontime sun. |
| Winter solstice | December 21st; shortest daylight of the year, lowest noontime sun. |
| Equinoxes are | March 21st and September 23rd; 12 hours of daylight everywhere on Earth. |
| Foucault’s pendulum and the Coriolis Effect | are proof that Earth rotates. |
| Divergent boundary | plates spreading; mid-ocean ridge or rift valley; volcanoes and shallow earthquakes. |
| Convergent boundary | plates coming together; subduction zones and trenches, volcanoes and deep earthquakes |
| Transform boundary: | plates sliding by each other; (San Andreas Fault), earthquakes only |
| P waves move faster than | S waves. |
| Porosity | does not depend on particle size (small particles have same porosity as large). |
| Know this Process: | Air is warmed, becomes less dense due to expansion; is forced upwards; expands and cools as it rises; temperature falls to the dew point; condensation of clouds occurs. |
| Index fossils | are good time markers because they lived for a short time, but over a large area. |
| Sedimentary rocks | (compaction and cementation) are most likely to have fossils. |
| Igneous rocks | (cooling and solidification) have large crystals from slow cooling (intrusive) and small crystals from fast cooling (extrusive). |
| Metamorphic rocks | (heat and pressure) can show foliation (banding) and distortion. |