Key Points

Gravitation

14 Sections
  • Universal Law of Gravitation

    Every object in the universe attracts every other object with a force FF that is directly proportional to the product of their masses (MM and mm) and inversely proportional to the square of the distance (dd) between their centers. The formula is F=GM×md2F = G \frac{M \times m}{d^2}.

  • Universal Gravitational Constant G

    The constant GG is called the universal gravitational constant. Its value is the same for all pairs of objects in the universe. The accepted value of G is 6.673×1011 N m2 kg26.673 \times 10^{-11} \text{ N m}^2 \text{ kg}^{-2}.

  • Importance of Gravitational Law

    The universal law of gravitation explains several key phenomena, including the force that binds us to the earth, the motion of the moon around the earth, the motion of planets around the sun, and the formation of tides.

  • Free Fall and Acceleration Due to Gravity g

    When an object falls towards the earth under gravitational force alone, it is in free fall. This motion involves a constant acceleration called acceleration due to gravity, denoted by gg. On Earth, its average value is g9.8 m s2g \approx 9.8 \text{ m s}^{-2}.

  • Calculating Acceleration Due to Gravity

    The value of gg on the surface of a celestial body can be calculated using the formula g=GMR2g = G \frac{M}{R^2}, where MM is the mass and RR is the radius of the body. This shows that gg is independent of the mass of the falling object.

  • Variation in the Value of g

    The value of gg is not constant on the surface of the Earth. It is greatest at the poles and decreases towards the equator because the Earth's radius is smaller at the poles.

  • Equations of Motion for Free Fall

    For an object in free fall, the standard equations of motion apply with acceleration aa replaced by gg. The equations are v=u+gtv = u + gt, s=ut+12gt2s = ut + \frac{1}{2}gt^2, and v2=u2+2gsv^2 = u^2 + 2gs. We take gg as positive for downward motion and negative for upward motion.

  • Mass versus Weight

    Mass is the amount of matter in an object and is constant everywhere, measured in kilograms (kg). Weight is the gravitational force on an object, calculated as W=m×gW = m \times g, and it varies with location, measured in Newtons (N).

  • Weight of an Object on the Moon

    Due to the moon's smaller mass and radius, its gravitational force is weaker than Earth's. The weight of an object on the moon is approximately one-sixth of its weight on Earth, or Wmoon16WearthW_{\text{moon}} \approx \frac{1}{6} W_{\text{earth}}.

  • Thrust and Pressure

    Thrust is the force acting perpendicular to a surface. Pressure is the thrust per unit area, given by the formula P=ThrustAreaP = \frac{\text{Thrust}}{\text{Area}}. The SI unit of pressure is the Pascal (Pa), where 1 Pa=1 N/m21 \text{ Pa} = 1 \text{ N/m}^2.

  • Buoyancy

    When an object is immersed in a fluid (a liquid or a gas), it experiences an upward force called the buoyant force or upthrust. This force opposes the object's weight and makes it feel lighter.

  • Archimedes Principle

    Archimedes' principle states that the buoyant force on an object immersed in a fluid is equal to the weight of the fluid displaced by the object. This principle is used in designing ships and submarines.

  • Principle of Flotation

    An object floats or sinks in a liquid based on its density relative to the liquid. An object floats if its density is less than the liquid's density, and it sinks if its density is greater than the liquid's density.

  • Density Formula

    Density is defined as mass per unit volume. The formula is ρ=mV\rho = \frac{m}{V}, where ρ\rho is density, mm is mass, and VV is volume. The SI unit for density is kg/m3\text{kg/m}^3.

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