Objectives (5 minutes)

1. Understand the concept of the movement of celestial bodies: The teacher must present in a clear and didactic way the concept of the movement of celestial bodies, explaining that the Earth and other planets revolve around the Sun, and that the Moon, in turn, revolves around the Earth.

2. Identify the main celestial bodies of the Solar System: The teacher must teach the students which are the main celestial bodies of the Solar System, with a special focus on the Sun, Earth, and Moon, highlighting their characteristics and importance for life on Earth.

3. Recognize the importance of the movement of celestial bodies for life on Earth: The teacher must show the students how the movement of celestial bodies, especially the Sun and the Moon, influences life on Earth, explaining, for example, the occurrence of day and night and the phases of the Moon.

Secondary Objectives:

• Stimulate students' curiosity and interest in the study of space, encouraging sky observation and research on the topic at home.
• Develop students' communication and oral expression skills through questions and answers and the presentation of their observations and discoveries.

Introduction (10 - 15 minutes)

1. Recalling previous content: The teacher starts the lesson by reminding the students about the concept of day and night. He should ask the students if they remember why there is day and night. This serves to contextualize the new content, introducing the idea that the movement of celestial bodies causes these phenomena.

2. Problem situations: The teacher can propose two problem situations that will instigate the curiosity of the students and introduce the subject of the lesson. The first situation could be: "Why does the Sun appear on one side of the sky and then disappear on the other? And why do we have the Moon at night, but not during the day?". The second situation could be: "Have you noticed that the Moon changes shape? How would you explain that?".

3. Contextualization: The teacher must explain to the students that understanding the movement of celestial bodies is very important. He can mention that it is because of this movement that we have day and night, the seasons of the year, and the phases of the Moon. In addition, he can say that ancient people used the movement of celestial bodies to orient themselves and that nowadays scientists use this knowledge to study space.

4. Capturing students' attention: To capture students' attention, the teacher can present some curiosities about space. For example, he can say that the Sun is a star and that if we could place the Earth next to other stars, it would be very small. Another curiosity is that the Moon does not have its own light, it reflects the light of the Sun. Additionally, the teacher can show images of space and celestial bodies to arouse the students' interest.

Development (20 - 25 minutes)

1. Theory of the movement of Celestial Bodies (10 - 12 minutes)

   1.1. Earth's Rotation Movement: The teacher must explain that the Earth rotates around itself, like a spinning ball. This is called the rotation movement, which takes about 24 hours to complete. At this point, the teacher can use a globe or a styrofoam model of the Earth to demonstrate the movement.

   1.2. Earth's Translation Movement: Next, the teacher must explain that the Earth also moves around the Sun, in a movement called translation, which takes about 365 days to complete.

   1.3. Moon's Movement: Finally, the teacher must explain that the Moon, our natural satellite, also moves. It revolves around the Earth, just as the Earth revolves around the Sun. The Moon's movement around the Earth is called revolution, which takes about 29 days to complete.

2. Importance of the Movement of Celestial Bodies for Life on Earth (5 - 6 minutes)

   2.1. Day and Night: The teacher must explain that the Earth's rotation movement is what causes day and night. When a part of the Earth is facing the Sun, it is day there. When that part is facing away from the Sun, it is night.

   2.2. Seasons of the Year: The teacher can mention that the Earth's translation movement is also important. It causes the seasons of the year. For example, when the northern hemisphere is tilted towards the Sun, we have summer there. When the northern hemisphere is tilted away from the Sun, we have winter there.

   2.3. Moon Phases: Finally, the teacher must explain that the Moon's movement around the Earth is what causes the phases of the Moon. When the Moon is between the Earth and the Sun, we do not see the Moon in the sky, it is called New Moon. When the Moon is on the opposite side of the Earth in relation to the Sun, we see the Full Moon.

3. Practical and Playful Activities (5 - 7 minutes)

   3.1. Rotation and Translation Game: The teacher can propose a game where students, standing up, simulate the rotation and translation movements of the Earth. This helps visualize and better understand the concepts.

   3.2. Observation of Moon Phases: The teacher can suggest that students observe the Moon during the week and draw the Moon's phases on paper. This helps reinforce the knowledge about the Moon's revolution around the Earth.

4. Correction of Activities (3 - 5 minutes)

   4.1. Group Discussion: The teacher must gather the students and promote a conversation about the Moon phases they observed. He should ask which phases they drew and why they think the Moon changes shape.

5. Content Reinforcement (2 - 3 minutes)

   5.1. Learning Confirmation: The teacher must ask the students if they have any doubts about the movement of celestial bodies and reaffirm the main points covered in the lesson. He should remind the students that the movement of celestial bodies is a very important subject and that they can continue exploring the topic at home, making more observations and research.

Return (10 - 15 minutes)

1. Group Discussion (5 - 7 minutes)

   1.1. Sharing Discoveries: The teacher must ask the students to share their observations about the Moon phases. Each student can show their drawing and explain what they understood about the Moon's movement around the Earth.

   1.2. Connection with Theory: The teacher must then ask questions to connect the students' observations with the presented theory. For example, he can ask: "When the Moon was like this in the sky, do you think it was closer or farther from the Earth?" or "When the Moon was like this in the sky, which part of it was illuminated by the Sun?".

2. Individual Reflection (3 - 4 minutes)

   2.1. Silent Moment: The teacher must propose a moment of silence for the students to reflect on what they learned in the lesson. He can ask two simple questions to guide the reflection: "What was the most interesting thing you learned today about the movement of celestial bodies?" and "How can you use this knowledge to better understand the world around you?".

   2.2. Note-taking: After the reflection moment, the teacher must ask the students to record their answers in their notebooks. This helps reinforce learning and allows the teacher to assess the students' understanding of the subject.

3. Teacher's Feedback (2 - 3 minutes)

   3.1. Recognition of Effort: The teacher must praise the students' effort in the lesson, highlighting the interesting observations they made and the questions they raised.

   3.2. Reinforcement of Main Points: The teacher must reinforce the main points of the lesson, summarizing what was learned about the movement of celestial bodies and its importance for life on Earth.

4. Lesson Closure (1 minute)

   4.1. Preparation for the Next Lesson: The teacher must tell the students that in the next lesson they will continue learning about space, exploring other celestial bodies and astronomical phenomena.

   4.2. Farewell: The teacher must end the lesson by wishing everyone a good day and encouraging them to continue observing the sky and asking questions about the world around them.

Conclusion (5 - 7 minutes)

1. Lesson Summary (2 - 3 minutes)

   1.1. Review of Main Points: The teacher must recap the main topics covered during the lesson, reminding the students about the Earth's rotation and translation movements, the Moon's revolution movement around the Earth, and the importance of these movements for the occurrence of day and night, the seasons of the year, and the Moon's phases.

   1.2. Connection between Theory and Practice: The teacher must emphasize how the practical and playful activities carried out during the lesson helped consolidate the students' theoretical understanding. He can mention, for example, how the rotation and translation game allowed students to visualize and better understand the Earth's movements, and how the observation of the Moon's phases allowed students to connect theory with practice.

2. Extra Materials (1 - 2 minutes)

   2.1. Book Suggestions: The teacher can suggest some children's books that address the topic of space in a playful and didactic way. Some examples are: "What's Out There?" by Rosalind Mist and "My First Book of Astronomy" by Patricia J. Wynne and Donald M. Silver.

   2.2. Educational Videos: The teacher can recommend some educational videos available on the internet that explain the movement of celestial bodies in a simple and interesting way. Some YouTube channels that produce content aimed at children and address the topic of space are: "Little Explorers", "Mundo Bita", and "Monica's Gang".

3. Importance of the Subject (1 - 2 minutes)

   3.1. Application in Daily Life: The teacher must explain to the students that knowledge about the movement of celestial bodies is not only interesting to know but also has practical applications in our daily lives. For example, he can mention that it is because of the Earth's rotation movement that we have day and night, and that it is because of the Earth's translation movement that we have the seasons of the year. Additionally, he can say that the Moon's movement around the Earth is what causes the Moon's phases, which we can observe in the sky.

   3.2. Importance for Science: Finally, the teacher can mention that the study of the movement of celestial bodies is very important for scientists, as it helps to better understand the Universe and our place in it. He can say, for example, that it was thanks to the study of the movement of celestial bodies that scientists discovered that the Earth revolves around the Sun, and not the other way around, as people believed in ancient times.

4. Lesson Closure (1 minute)

   4.1. Continuous Learning: The teacher must end the lesson by encouraging the students to continue exploring the topic of space, observing the sky, and asking questions. He can say that as the students grow up, they will be able to learn more and more about the Universe, as space is a subject that never ends.

   4.2. Farewell: The teacher must conclude the lesson by wishing everyone a good day and reminding them that the next lesson will be even more fun and full of discoveries.