Nome_ Nome Date CONCEPT CONGEPTUAL Physical SciencE eChapter 24: The Oceans, Atmosphere, and Climatic Effects PRACTICE SLET Chap T Earth The Earth's Seasons Here w apple. part of part of tha...
Nome_ Nome Date CONCEPT CONGEPTUAL Physical SciencE eChapter 24: The Oceans, Atmosphere, and Climatic Effects PRACTICE SLET Chap T Earth The Earth's Seasons Here w apple. part of part of that cc L. The warmth of equatorial regions and coldness of polar regions on the Earth can be understood by considering light from a flashlight striking a surface. If it strikes perpendicularly, light energy is more concentrated as it covers a smaller area; if it strikes at an angle, the energy preads over a larger area. So the energy per unit area is less. Draw Moor d, exx The arrows represent rays of light from the distant Sun incident upon the Earth. Two areas of equal size are shown, Area A near the north pole and Area B near the equator. Count the rays that reach each area, and explain why region B is warmer than region A 2. The Earth's seasons result from the 23.5-degree tit of the Earth's daily spin axis as it orbits the Sun. When the Earth is at the position shown on the right in the sketch below (not shown to scale), the Northern Hemihere tilts toward the Sun, and sunlight striking it is strong (more rays per area). Sunlight striking the Southern Hemisphere is weak (fewer rays per area). Days in the north are warmer, and daylightlasts longer. You can see this by imagining the Earth making its complete daily 24-hour spin. Do two things on the sketch: (1) Shade the Earth in nighttime darkness for all positions, as is already done in the left position.(2) Label each position with the proper month- March, June, or December. Be sure to do the shading before you answer questions on the backside of this sheetl 165