Class 9th Physics Chapter 5 – Gravitation

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Chapter 5 of Class 9 Physics focuses on Gravitation, which is the force of attraction between two masses. This chapter introduces students to the fundamental concepts of gravitational force, its effects, and the laws governing it.

Key Concepts:

  • Gravitational Force: The chapter begins with the definition of gravitational force as the attractive force that exists between any two objects with mass. This force is proportional to the product of their masses and inversely proportional to the square of the distance between their centers, as described by Newton’s Law of Universal Gravitation:F=Gm1m2r2F = G \frac{m_1 m_2}{r^2}F=Gr2m1​m2​​where FFF is the gravitational force, GGG is the universal gravitational constant, m1m_1m1​ and m2m_2m2​ are the masses, and rrr is the distance between the centers of the two masses.
  • Weight and Mass: The chapter distinguishes between mass (the amount of matter in an object) and weight (the gravitational force acting on an object). Weight can be calculated using the formula:W=m×gW = m \times gW=m×gwhere WWW is weight, mmm is mass, and ggg is the acceleration due to gravity (approximately 9.81 m/s29.81 \, \text{m/s}^29.81m/s2 on Earth).
  • Acceleration Due to Gravity: Students learn about the value of acceleration due to gravity and how it varies with altitude and depth. The chapter discusses how gravity influences the motion of objects on Earth.
  • Free Fall and Projectile Motion: The concepts of free fall (when an object falls under the influence of gravity alone) and projectile motion (the curved path of an object thrown into the air) are introduced, highlighting the effects of gravity on their trajectories.
  • Kepler’s Laws of Planetary Motion: The chapter briefly covers Kepler’s laws, which describe the motion of planets around the Sun, emphasizing the elliptical orbits and the relationship between the distance from the Sun and the orbital period.

This chapter lays the groundwork for understanding gravitational phenomena, which are essential for further studies in physics, astronomy, and related fields.

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