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Rotation of the Earth
Quiz by Emelou A Tanudtanud
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Quarter 4 Science 6 Rotation of the EarthPS1.1h Revolution and rotation of the EarthROTATION AND REVOLUTION OF THE EARTH-ELICIT Based on the provided sources, here is a comprehensive extraction of the information regarding the water cycle, energy transfer, and Earth's wind systems, organized into key points: The Water Cycle and Its Reservoirs • Definition: The water cycle is the continuous movement of water among various reservoirs on Earth. • Water Reservoirs: These are storage locations for water and include: ◦ Oceans, seas, and lakes. ◦ Rivers, glaciers, soil, and rocks. ◦ The atmosphere and living organisms. • Total Volume: The total amount of water on Earth does not change, even when it changes state, because it is constantly being replaced or recycled through the cycle. Main Processes and Energy Transfer The movement of water through the cycle is driven by energy (thermal energy from the Sun) and force (gravity and wind). • Energy Gain (Absorption): ◦ Melting: Water changes from a solid state (ice) to a liquid state and gains energy. ◦ Evaporation: Liquid water changes into a gas state (water vapor) by gaining thermal energy. ◦ Transpiration: A specialized type of evaporation occurring in plants where water vapor is released through tiny holes in leaves called stomata. Approximately 10% of water vapor in the air comes from transpiration. • Energy Loss (Release): ◦ Condensation: Water vapor (gas) cools down and changes back into liquid water, releasing energy. ◦ Freezing: Liquid water changes into a solid state (ice) and loses energy. • Other Key Steps: ◦ Precipitation: Water falls back to Earth as rain, snow, sleet, or hail (snow pellets). ◦ Runoff: Water flows over Earth's surface into streams, rivers, and eventually larger bodies of water like oceans. ◦ Collection: Rainwater is collected in different water bodies to start the cycle again. Forces Driving Water Movement • Gravity: The main force that pulls water downward. It is responsible for: ◦ Bringing precipitation (rain and snow) from clouds to the surface. ◦ Moving ice in glaciers from higher to lower elevations. ◦ Causing liquid water to flow downhill into rivers and seas. ◦ Leakage: Pulling liquid water down into the ground to reach groundwater reservoirs. • Wind: Another force that affects water movement and transports water to different locations on Earth. Atmospheric Processes • Cloud Formation: Water vapor attaches to particles such as dust or smoke in the air and condenses into tiny droplets. When millions of these droplets join, they become heavy and fall as rain. • Convection: The transfer of heat in liquids and gases. ◦ Warm air/liquid: Becomes less dense, lighter, and rises upward. ◦ Cold air/liquid: Is more dense, heavier, and moves downward to replace the warm fluid. ◦ This process leads to convection currents, which help determine regional climates and drive wind and ocean currents. Solar Radiation and Climate The amount of solar energy reaching Earth differs from place to place, which affects the weather: • Hottest Regions (Equator): Sun rays fall perpendicular (vertical). Heat is concentrated on a small area, making the weather hot. • Moderate Regions: Sun rays fall semi-inclined. Heat is distributed over a larger area, making the weather warm. • Coolest Regions (Poles): Sun rays fall very slanted (inclined). Heat is spread over a very large area, making the weather very cold. Earth's Wind System • Wind Formation: Wind is generated when warm air (heated by the Sun) rises and is replaced by cooler air flowing from nearby areas. • Factors Affecting Wind: The amount of solar radiation and the rotation of Earth determine global wind directions. • Global Wind Cycle: Unequal heating between the equator and the poles generates a constant wind system. Warm air rises at the equator and moves toward the poles, while cold air from the poles moves toward the equator. • Importance: If there were no wind, the equator would become extremely hot, the poles would freeze solid, and many ecosystems would disappear. Practical Examples • Turkey’s Salt Lake: High evaporation in the summer can turn this large lake into a small puddle or dry it up completely. It is a critical site for flamingos, which migrate there to breed and feed on algae in the shallow, warm water.6.2 The student will investigate and understand that the solar system is organized and the various bodies in the solar system interact. Key ideas include matter is distributed throughout the solar system; planets have different sizes and orbit at different distances from the sun; gravity contributes to orbital motion; and the understanding of the solar system has developed over time. 6.3 The student will investigate and understand that there is a relationship between the sun, Earth, and the moon. Key ideas include Earth has unique properties; the rotation of Earth in relationship to the sun causes day and night; the movement of Earth and the moon in relationship to the sun causes phases of the moon; Earth’s tilt as it revolves around the sun causes the seasons; and the relationship between Earth and the moon is the primary cause of tides.Motions of The Earth: Rotation and Revolution QuizDuring daytime, the sky is bright and clear because the sun shines bright. We can see clouds, the sun and sometimes there is a rainbow. The sun is the nearest and brightest star on earth, the reason why we don’t see stars during daytime because the sun overpowers the weak lights of the stars. Do you know that the sun changes its position at different time of the day? Yes, early in the morning we can see the sun rising at the East. At this time of the day our surroundings is bright but not very hot, this is the reason why many children especially new born are placed under the sun because the light coming from the sun is good for them. At noontime the sun is overhead. It is very hot at this time of the day. This is the reason why it is not advisable for us to go outside. In the afternoon, we can see the sun setting at the West part of the sky. It is said that this the best time for the children to play outside because the sky s less bright and the temperature is cooler. SCIENCE 2 – MODULE 10 SEIBO COLLEGE 5 It is during daytime we do our chores, like cleaning the house, washing clothes, going to school or office and play. What do you think the reason why we do all these things during daytime? Now, close your eyes then imagine it is nighttime already. What can you see in the sky? Open your eyes then observe the picture below. Can you see these? Very good! You can see the moon and the stars. Sometimes you can see shooting stars or falling stars. At nighttime, we can not see the sun because it is already dark, we can only see the moon and the stars twinkling in the sky. Since there is no sun at night, the temperature is cooler. This is also the best time for us to rest and sleep. Do you know that the moon doesn’t have its own light? Yes, the moon only reflects the light from the sun. Do you now understand the difference of daytime from nighttime? Very good! But the question is how and why do we experience day and night? We experience day and night because the earth is moving around its axis. This movement is called rotation. SCIENCE 2 – MODULE 10 SEIBO COLLEGE 6 When the earth continuously rotates on its axis, part of it faces the sun and the other part is dark. The part of the earth that faces the sun experience daytime and the other part that is dark experience nighttime. meteor meteorite meteoroid Milky Way moon Neptune orbit physical characteristics Pluto revolve / revolution rotate / rotation Saturn solar system Sun Uranus Venus Essential Understandings (Content Elaboration): ● Planets in the solar system orbit the sun. Some of the planets have one or more orbiting moons. Earth is a planet that has a moon. The moon orbits Earth. Gravitational forces between the sun and its planets cause the planets to orbit the sun. Gravitational forces between a planet and its moon(s) cause the moon(s) to orbit the planet. If no forces were present, planets and moons would continue their motion toward outer space without changes in speed or direction. However, gravitational forces between the sun and each planet continuously change the planet’s direction so it remains in orbit. In the same way, gravitational forces between each moon and its planet continuously change the moon’s direction so it remains in orbit.