TERM – 3RD TERM
WEEK SEVEN AND EIGHT
Class: Junior Secondary School 1
Age: 12 years
Duration: 40 minutes of 5 periods each
Date:
Subject: BASIC SCIENCE
Topic: EARTH IN SPACE
SPECIFIC OBJECTIVES: At the end of the lesson, pupils should be able to
INSTRUCTIONAL TECHNIQUES: Identification, explanation, questions and answers, demonstration, videos from source
INSTRUCTIONAL MATERIALS: Videos, loud speaker, textbook, pictures,
INSTRUCTIONAL PROCEDURES
PERIOD 1-2
PRESENTATION |
TEACHER’S ACTIVITY |
STUDENT’S ACTIVITY |
STEP 1 INTRODUCTION |
The teacher introduces the solar system and discusses the components of the solar system. |
Students pay attention |
STEP 2 EXPLANATION |
Teacher explains how the rotation and revoution of the Earth and Moon takes place.
|
Students pay attention and participate |
STEP 3 DEMONSTRATION |
Teacher describes the eclipse and seasons. |
Students pay attention and participate |
STEP 4 NOTE TAKING |
The teacher writes a summarized note on the board |
The students copy the note in their books |
NOTE
EARTH IN SPACE
The Solar System
The solar system refers to the collection of celestial bodies that orbit the Sun, including planets, moons, dwarf planets, asteroids, comets, and other objects. At the center of the solar system is the Sun, a star that accounts for the vast majority of its mass. The gravitational pull of the Sun keeps the planets and other objects in orbit around it.
The solar system consists of various components, including:
- Inner Planets (Terrestrial Planets): Mercury, Venus, Earth, and Mars. These planets are primarily composed of rock and metal and have solid surfaces.
- Outer Planets (Gas Giants): Jupiter, Saturn, Uranus, and Neptune. These planets are primarily composed of gases, such as hydrogen and helium, with relatively small solid cores.
Rotation and Revolution of the Earth
Rotation: The Earth rotates around its axis, an imaginary line passing through its North and South Poles. This rotation gives rise to the cycle of day and night. It takes approximately 24 hours for the Earth to complete one full rotation, resulting in one day-night cycle.
Revolution: The Earth revolves around the Sun in an elliptical orbit. This motion, known as revolution, takes approximately 365.25 days to complete, resulting in one Earth year. The tilt of the Earth's axis relative to its orbital plane causes the changing seasons as different parts of the Earth receive varying amounts of sunlight throughout the year.
Rotation and Revolution of the Moon
Rotation: The Moon rotates on its axis as it orbits the Earth. However, unlike the Earth, the Moon's rotation period is equal to its orbital period, meaning it takes the same amount of time (about 27.3 days) for the Moon to complete one rotation as it does to orbit the Earth once. As a result, the same side of the Moon always faces Earth, a phenomenon known as synchronous rotation.
Revolution: The Moon revolves around the Earth in an elliptical orbit. This motion takes approximately 27.3 days to complete, resulting in one lunar month. As the Moon orbits the Earth, its position relative to the Sun changes, giving rise to the phases of the Moon, such as full moon, new moon, waxing crescent, and waning gibbous.
Description of Eclipses
An eclipse is an astronomical event that occurs when one celestial body passes into the shadow of another celestial body, temporarily blocking or partially obscuring its light. There are two main types of eclipses:
Description of Seasons
Seasons are regular periods of time characterized by distinct weather patterns and changes in temperature, daylight hours, and natural phenomena. The changing seasons are primarily caused by the tilt of the Earth's axis relative to its orbital plane around the Sun. There are four main seasons:
EVALUATION: 1. Describe the solar system, identifying the components.
CLASSWORK: As in evaluation
CONCLUSION: The teacher commends the students positively