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Lesson plan of Earth: Movements

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Lara from Teachy


Geography

Original Teachy

Earth: Movements

Lesson Plan | Traditional Methodology | Earth: Movements

KeywordsEarth Movements, Rotation, Revolution, Tilt of the Earth's Axis, Day and Night, Seasons, Daily Phenomena, Annual Phenomena, Calendar, Physical Time, Geography
Required MaterialsGlobe, Maps, Diagrams of Earth's Orbit, Board and Markers, Notebook and Pen for Notes, Computer and Projector (optional for displaying videos and images), Visual Support Material (images, charts)

Objectives

Duration: (10 - 15 minutes)

The purpose of this stage of the lesson plan is to introduce students to the fundamental concepts of the Earth's movements, highlighting the importance of understanding these movements for the comprehension of physical time and the seasons. This prepares students for detailed analysis and application of knowledge in everyday and scientific situations.

Main Objectives

1. Understand the main movements of the Earth: rotation and revolution.

2. Identify the consequences of the Earth's movements for the perception of time and the seasons.

3. Analyze the relationship between the Earth's movements and daily and annual phenomena, such as day and night, and the seasons.

Introduction

Duration: (10 - 15 minutes)

The purpose of this stage of the lesson plan is to introduce students to the fundamental concepts of the Earth's movements, highlighting the importance of understanding these movements for the comprehension of physical time and the seasons. This prepares students for detailed analysis and application of knowledge in everyday and scientific situations.

Context

To begin the lesson on the movements of the Earth, it is important to situate students in the context in which these movements occur and how they affect our daily lives. Explain that the Earth is not still; it is constantly moving in space. These movements are responsible for phenomena we observe every day, such as sunrise and sunset, and also for the seasonal changes we experience throughout the year. Using maps or globes can help illustrate these movements in a visual and tangible way.

Curiosities

Did you know that the Earth rotates around its own axis at a speed of approximately 1,670 kilometers per hour at the equator? And that it takes about 365.25 days to complete one orbit around the Sun, resulting in our calendar year? These movements are so precise that scientists can predict eclipses and calculate the exact duration of days and nights at any point on the planet.

Development

Duration: (50 - 60 minutes)

The purpose of this stage of the lesson plan is to deepen students' understanding of the Earth's movements and their consequences. By addressing the topics of rotation, revolution, and tilt of the Earth's axis in detail, students can visualize and comprehend how these movements influence daily and annual phenomena, such as day and night and the seasons. Resolving questions in the classroom reinforces learning and helps consolidate the concepts presented.

Covered Topics

1. Earth's Rotation: Explain that the Earth rotates around its own axis, a movement called rotation. This movement takes approximately 24 hours to complete, resulting in the alternation between day and night. Use a globe to visually demonstrate this movement. 2. Earth's Revolution: Detail that, in addition to rotation, the Earth also moves around the Sun in an elliptical orbit. This movement is known as revolution and takes about 365.25 days to complete, defining our year. Use diagrams to illustrate the Earth's orbit around the Sun. 3. Tilt of the Earth's Axis: Explain that the Earth's axis is tilted at approximately 23.5 degrees relative to the orbital plane around the Sun. This tilt is responsible for the variation in the amount of sunlight that different parts of the planet receive throughout the year, resulting in the seasons. 4. Consequences of Rotation: Describe how the Earth's rotation is responsible for the alternation between day and night. Explain that while one part of the Earth is facing the Sun and experiencing day, the other part is in shadow and experiencing night. 5. Consequences of Revolution and Axis Tilt: Detail how the Earth's revolution around the Sun, combined with the tilt of the axis, results in the seasons. Explain that when the northern hemisphere is tilted toward the Sun, it is summer in that hemisphere and winter in the southern hemisphere, and vice versa.

Classroom Questions

1. Explain the difference between Earth's rotation and revolution. 2. How does the tilt of the Earth's axis affect the seasons? 3. Why do we have days and nights?

Questions Discussion

Duration: (20 - 25 minutes)

The purpose of this stage of the lesson plan is to consolidate the knowledge acquired by students throughout the lesson. Discussing the questions allows students to review and clarify their doubts, while the questions and reflections stimulate critical thinking and the application of learned concepts to hypothetical and everyday situations. This feedback moment is essential to ensure that all students have understood the topics covered and are prepared to apply them in future contexts.

Discussion

  • Explain the difference between Earth's rotation and revolution: Rotation is the movement that the Earth makes as it spins around its own axis. This movement takes approximately 24 hours to complete and results in the alternation between day and night. Revolution is the movement that the Earth makes as it orbits around the Sun. This movement takes about 365.25 days to complete and defines our year.

  • How does the tilt of the Earth's axis affect the seasons: The tilt of the Earth's axis, which is approximately 23.5 degrees, causes different parts of the planet to receive different amounts of sunlight throughout the year. When the northern hemisphere is tilted toward the Sun, it receives more sunlight and is summer in that hemisphere, while the southern hemisphere, receiving less sunlight, is in winter, and vice versa.

  • Why do we have days and nights: We have days and nights due to the Earth's rotation. As the Earth spins around its axis, different parts of the planet are exposed to the Sun or are in shadow. The part of the Earth that is facing the Sun experiences day, while the opposite part, in shadow, experiences night.

Student Engagement

1. Ask students: How do you think life would be if the Earth did not rotate around its axis? 2. Ask students to reflect: What would happen if the Earth did not have a tilt in its axis? 3. Question: What would be the consequences for the climate and the seasons if the Earth were more tilted or less tilted? 4. Suggest to students to think: How do the rotation and revolution of the Earth influence our perception of time and the calendar that we use?

Conclusion

Duration: (10 - 15 minutes)

The purpose of this stage of the lesson plan is to review and consolidate the main points covered, ensuring that students have a clear and cohesive understanding of the Earth's movements. The conclusion allows for recapping the theory, connecting concepts to practice, and emphasizing the importance of the topic for daily life, promoting a deeper and more lasting understanding.

Summary

  • The Earth performs two main movements: rotation and revolution.
  • The rotation of the Earth around its axis takes approximately 24 hours and results in the alternation between day and night.
  • The revolution of the Earth around the Sun takes about 365.25 days and defines the year.
  • The tilt of the Earth's axis at approximately 23.5 degrees causes variations in the amount of sunlight received throughout the year, resulting in the seasons.
  • Rotation is responsible for days and nights, while revolution and axis tilt cause the seasons.

The lesson connected the theory of the Earth's movements with practice by using globes and diagrams to illustrate the concepts of rotation and revolution. This helped students visualize and understand how these movements affect daily and annual phenomena, such as day and night, and the seasons, making learning more concrete and applicable to everyday life.

Understanding the movements of the Earth is essential for grasping the succession of days, nights, and seasons. This knowledge is fundamental not only for geography but also for organizing the calendar, agricultural planning, and even for navigation and orientation. Curiosities such as the speed of rotation at the equator and the prediction of eclipses make the subject even more fascinating and relevant.


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