Gravitation Notes

Gravitation

Introduction

  • Objects in motion and the concept of force.
  • Force is required to change the speed or direction of an object's motion.
  • Objects dropped from a height fall towards the Earth.
  • Planets revolve around the Sun, and the Moon revolves around the Earth.
  • A force is responsible for these phenomena: gravitational force.
  • This chapter covers gravitation, the universal law of gravitation, motion of objects under gravitational force, weight variation, and conditions for objects to float in liquids.

Gravitation

  • The Moon revolves around the Earth.
  • Objects thrown upwards fall downwards after reaching a certain height.
  • Newton's observation: an apple falling from a tree.
  • Question: If Earth can attract an apple, can it also attract the Moon?
  • Conjecture: The same force is responsible for both.
  • Argument: The Moon falls towards the Earth at each point of its orbit instead of going in a straight line; hence, it is attracted by the Earth.
  • Activity 9.1: Stone tied to a thread whirled around.
    • Observation: The stone moves in a circular path with a certain speed and changes direction at every point.
    • Change in direction implies change in velocity or acceleration.
    • The force causing this acceleration and keeping the body moving along the circular path is directed towards the center: centripetal force.
Universal Law of Gravitation
  • Every object in the universe attracts every other object.

  • The force is proportional to the product of their masses.

  • The force is inversely proportional to the square of the distance between them.

  • The force acts along the line joining the centers of the two objects.

  • Tangent to a circle: A straight line that meets the circle at one and only one point.

  • The motion of the Moon around the Earth is due to the centripetal force provided by the Earth's attraction.

  • If there were no such force, the Moon would move in a uniform straight line.

  • A falling apple is attracted towards the Earth; the apple also attracts the Earth.

  • According to the third law of motion, the apple does attract the earth. But according to the second law of motion, for a given force, acceleration is inversely proportional to the mass of an object (Eq.8.4)(Eq. 8.4).

  • The mass of the apple is negligibly small compared to the Earth, so we don't see the Earth moving towards the apple.

  • The same argument applies to why the Earth does not move towards the Moon.

  • In the solar system, planets revolve around the Sun, indicating a force between them.

  • Newton concluded that all objects in the universe attract each other: gravitational force.

  • Mathematical representation:

    • Let two objects A and B have masses MM and mm, respectively, and be separated by a distance dd. Let FF be the force of attraction between them.
    • FM×mF \propto M \times m (9.1)(9.1)
    • F1d2F \propto \frac{1}{d^2} (9.2)(9.2)
    • Combining equations (9.1) and (9.2):
      • FM×md2F \propto \frac{M \times m}{d^2} (9.3)(9.3)
      • F=GM×md2F = G \frac{M \times m}{d^2} (9.4)(9.4)
      • Where GG is the universal gravitation constant.
    • F×d2=GM×mF \times d^2 = G M \times m (9.5)(9.5)
  • The SI unit of GG is Nm2kg2N m^2 kg^{-2}.

  • Henry Cavendish found the value of GG using a sensitive balance.

  • The accepted value of GG is 6.673×1011Nm2kg26.673 \times 10^{-11} N m^2 kg^{-2}.

  • The law is universal, applicable to all bodies, big or small, celestial or terrestrial.

Inverse-square
  • If dd is bigger by a factor of 6, FF becomes 136\frac{1}{36} times smaller.
  • Example 9.1: Calculating the force exerted by the Earth on the Moon.
    • Mass of the Earth, M=6×1024kgM = 6 \times 10^{24} kg
    • Mass of the Moon, m=7.4×1022kgm = 7.4 \times 10^{22} kg
    • Distance between the Earth and the Moon, d=3.84×105km=3.84×108md = 3.84 \times 10^5 km = 3.84 \times 10^8 m
    • G=6.7×1011Nm2kg2G = 6.7 \times 10^{-11} N m^2 kg^{-2}
    • F=G×M×md2=6.7×1011Nm2kg2×6×1024kg×7.4×1022kg(3.84×108m)2=2.02×1020NF = \frac{G \times M \times m}{d^2} = \frac{6.7 \times 10^{-11} N m^2 kg^{-2} \times 6 \times 10^{24} kg \times 7.4 \times 10^{22} kg}{(3.84 \times 10^8 m)^2} = 2.02 \times 10^{20} N
    • The force exerted by the Earth on the Moon is 2.02×1020N2.02 \times 10^{20} N.
Importance of the Universal Law of Gravitation
  • Explains several phenomena:
    • The force that binds us to the Earth.
    • The motion of the Moon around the Earth.
    • The motion of planets around the Sun.
    • Tides due to the Moon and the Sun.

Free Fall

  • Activity 9.2: Throwing a stone upwards.
  • The Earth attracts objects towards it due to gravitational force.
  • Objects falling towards the Earth under this force alone are in free fall.
  • During free fall, there is no change in the direction of motion.
  • The magnitude of velocity changes due to Earth's attraction.
  • Any change in velocity involves acceleration.
  • Acceleration due to the Earth's gravitational force: acceleration due to gravity (gg).
  • The unit of gg is ms2m s^{-2}.
  • From the second law of motion, force is the product of mass and acceleration.
    • F=mgF = m g (9.6)(9.6)
    • From equations (9.4) and (9.6):
      • mg=GMmd2mg = G \frac{M m}{d^2}
      • g=GMd2g = G \frac{M}{d^2} (9.7)(9.7)
    • Where MM is the mass of the Earth, and dd is the distance between the object and the Earth.
  • For objects on or near the surface of the Earth, d=Rd = R (radius of the Earth).
    • g=GMR2g = G \frac{M}{R^2} (9.9)(9.9)
To Calculate the Value of g
  • G=6.7×1011Nm2kg2G = 6.7 \times 10^{-11} N m^2 kg^{-2}
  • M=6×1024kgM = 6 \times 10^{24} kg
  • R=6.4×106mR = 6.4 \times 10^6 m
    • g=GMR2=6.7×1011Nm2kg2×6×1024kg(6.4×106m)2=9.8ms2g = \frac{G M}{R^2} = \frac{6.7 \times 10^{-11} N m^2 kg^{-2} \times 6 \times 10^{24} kg}{(6.4 \times 10^6 m)^2} = 9.8 m s^{-2}
  • The value of acceleration due to gravity of the Earth, g=9.8ms2g = 9.8 m s^{-2}.
Motion of Objects Under the Influence of Gravitational Force of the Earth
  • Activity 9.3: Dropping a sheet of paper and a stone from a height.
  • Paper reaches the ground later than the stone due to air resistance.
  • Air resistance affects the paper more than the stone.
  • In a glass jar from which air has been sucked out, the paper and the stone would fall at the same rate.
  • Acceleration experienced by an object during free fall is independent of its mass.
  • Galileo's experiment at the Leaning Tower of Pisa.
  • All equations for uniformly accelerated motion are valid with aa replaced by gg.
    • v=u+atv = u + at (9.10)(9.10)
    • s=ut+12at2s = ut + \frac{1}{2} at^2 (9.11)(9.11)
    • v2=u2+2asv^2 = u^2 + 2as (9.12)(9.12)
  • Take aa as positive when it is in the direction of motion and negative when it opposes the motion.
  • Example 9.2: A car falls off a ledge and drops to the ground in 0.5 s. Let g=10ms2g = 10 m s^{-2}.
    • (i) What is its speed on striking the ground?
    • (ii) What is its average speed during the 0.5 s?
    • (iii) How high is the ledge from the ground?
    • Solution:
      • Time, t=0.5st = 0.5 s
      • Initial velocity, u=0ms1u = 0 m s^{-1}
      • Acceleration due to gravity, g=10ms2g = 10 m s^{-2}
      • Acceleration of the car, a=+10ms2a = + 10 m s^{-2} (downward)
      • (i) Speed v=at=10ms2×0.5s=5ms1v = a t = 10 m s^{-2} \times 0.5 s = 5 m s^{-1}
      • (ii) Average speed =u+v2=0ms1+5ms12=2.5ms1= \frac{u + v}{2} = \frac{0 m s^{-1} + 5 m s^{-1}}{2} = 2.5 m s^{-1}
      • (iii) Distance travelled, s=12at2=12×10ms2×(0.5s)2=1.25ms = \frac{1}{2} a t^2 = \frac{1}{2} \times 10 m s^{-2} \times (0.5 s)^2 = 1.25 m
  • Example 9.3: An object is thrown vertically upwards and rises to a height of 10 m. Calculate (i) the velocity with which the object was thrown upwards and (ii) the time taken by the object to reach the highest point.
    • Solution:
      • Distance travelled, s=10ms = 10 m
      • Final velocity, v=0ms1v = 0 m s^{-1}
      • Acceleration due to gravity, g=9.8ms2g = 9.8 m s^{-2}
      • Acceleration of the object, a=9.8ms2a = -9.8 m s^{-2} (upward motion)
      • (i) v2=u2+2asv^2 = u^2 + 2 a s
        • 0=u2+2×(9.8ms2)×10m0 = u^2 + 2 \times (-9.8 m s^{-2}) \times 10 m
        • u2=2×9.8×10m2s2-u^2 = -2 \times 9.8 \times 10 m^2 s^{-2}
        • u=196ms1=14ms1u = \sqrt{196} m s^{-1} = 14 m s^{-1}
      • (ii) v=u+atv = u + a t
        • 0=14ms19.8ms2×t0 = 14 m s^{-1} - 9.8 m s^{-2} \times t
        • t=149.8s=1.43st = \frac{14}{9.8} s = 1.43 s

Mass

  • Mass is the measure of inertia.
  • Greater the mass, the greater is the inertia.
  • Mass remains the same whether the object is on the Earth, the Moon, or in outer space.
  • The mass of an object is constant and does not change from place to place.

Weight

  • The Earth attracts every object with a certain force.
  • This force depends on the mass (mm) of the object and the acceleration due to gravity (gg).
  • The weight of an object is the force with which it is attracted towards the Earth.
    • F=m×aF = m \times a (9.13)(9.13)
    • F=m×gF = m \times g (9.14)(9.14)
  • The force of attraction of the Earth on an object is known as the weight of the object (WW).
    • W=m×gW = m \times g (9.15)(9.15)
  • The SI unit of weight is the same as that of force: Newton (N).
  • Weight is a force acting vertically downwards; it has both magnitude and direction.
  • The value of gg is constant at a given place; therefore, at a given place, the weight of an object is directly proportional to its mass.
    • WmW \propto m
  • The mass of an object remains the same everywhere, whereas its weight depends on location because gg depends on location.
Weight of an Object on the Moon
  • The weight of an object on the Moon is the force with which the Moon attracts that object.
  • The mass of the Moon is less than that of the Earth; hence, the Moon exerts lesser force of attraction on objects.
  • Let the mass of an object be mm. Let its weight on the Moon be W<em>mW<em>m. Let the mass of the Moon be M</em>mM</em>m and its radius be RmR_m.
    • W<em>m=GM</em>m×mRm2W<em>m = G \frac{M</em>m \times m}{R_m^2} (9.16)(9.16)
  • Let the weight of the same object on the Earth be WeW_e. The mass of the Earth is MM and its radius is RR.
    • We=GM×mR2W_e = G \frac{M \times m}{R^2} (9.17)(9.17)
  • Substituting values from Table 9.1:
    • Wm=G7.36×1022kg×m(1.74×106m)2=2.431×1010GmW_m = G \frac{7.36 \times 10^{22} kg \times m}{(1.74 \times 10^6 m)^2} = 2.431 \times 10^{10} G m (9.18a)(9.18a)
    • We=G5.98×1024kg×m(6.37×106m)2=1.474×1011GmW_e = G \frac{5.98 \times 10^{24} kg \times m}{(6.37 \times 10^6 m)^2} = 1.474 \times 10^{11} G m (9.18b)(9.18b)
    • W<em>mW</em>e=2.431×10101.474×1011=0.165\frac{W<em>m}{W</em>e} = \frac{2.431 \times 10^{10}}{1.474 \times 10^{11}} = 0.165
      • W<em>mW</em>e=16\frac{W<em>m}{W</em>e} = \frac{1}{6} (9.19)(9.19)
  • Weight of the object on the Moon = 16\frac{1}{6} × its weight on the Earth.
  • Example 9.4: Mass of an object is 10 kg. What is its weight on the Earth?
    • m=10kgm = 10 kg
    • g=9.8ms2g = 9.8 m s^{-2}
    • W=m×g=10kg×9.8ms2=98NW = m \times g = 10 kg \times 9.8 m s^{-2} = 98 N
  • Example 9.5: An object weighs 10 N when measured on the surface of the Earth. What would be its weight when measured on the surface of the Moon?
    • W<em>m=16×W</em>e=16×10N=1.67NW<em>m = \frac{1}{6} \times W</em>e = \frac{1}{6} \times 10 N = 1.67 N

Thrust and Pressure

  • Thrust: Net force acting in a particular direction.
  • Pressure: Force per unit area acting on the object.
  • Situation 1: Fixing a poster on a bulletin board using drawing pins.
  • Situation 2: Standing on loose sand versus lying down on the sand.
  • The force acting on an object perpendicular to the surface is called thrust.
    • Pressure=ThrustareaPressure = \frac{Thrust}{area} (9.20)(9.20)
  • The SI unit of pressure is N/m2N/m^2 or Nm2N m^{-2}, also called Pascal (Pa).
  • Example 9.6: A block of wood (mass 5 kg, dimensions 40 cm × 20 cm × 10 cm) on a tabletop.
    • (a) 20 cm × 10 cm side:
      • Thrust = F=m×g=5kg×9.8ms2=49NF = m \times g = 5 kg \times 9.8 m s^{-2} = 49 N
      • Area = 20cm×10cm=200cm2=0.02m220 cm \times 10 cm = 200 cm^2 = 0.02 m^2
      • Pressure = 49N0.02m2=2450Nm2\frac{49 N}{0.02 m^2} = 2450 N m^{-2}
    • (b) 40 cm × 20 cm side:
      • Thrust = 49 N
      • Area = 40cm×20cm=800cm2=0.08m240 cm \times 20 cm = 800 cm^2 = 0.08 m^2
      • Pressure = 49N0.08m2=612.5Nm2\frac{49 N}{0.08 m^2} = 612.5 N m^{-2}
  • The same force acting on a smaller area exerts a larger pressure, and a smaller pressure on a larger area.
  • This is why nails have pointed tips, knives have sharp edges, and buildings have wide foundations.
Pressure in Fluids
  • Liquids and gases are fluids.
  • Fluids exert pressure on the base and walls of the container in which they are enclosed.
  • Pressure exerted in any confined mass of fluid is transmitted undiminished in all directions.
Buoyancy
  • Activity 9.4: Empty plastic bottle in a bucket of water.
  • Water exerts a force on the bottle in the upward direction.
  • The upward force exerted by the water goes on increasing as the bottle is pushed deeper until it is completely immersed.
  • The upward force exerted by the water on the bottle is known as upthrust or buoyant force.
  • All objects experience a force of buoyancy when they are immersed in a fluid.
  • The magnitude of this buoyant force depends on the density of the fluid.
Why Objects Float or Sink When Placed on the Surface of Water?
  • Activity 9.5: Iron nail and cork in a beaker filled with water.
  • The nail sinks because the downward force acting on the nail is greater than the upthrust of water on the nail.
  • Activity 9.6: Cork and iron nail of equal mass on the surface of water.
  • The cork floats because the upthrust of water on the cork is greater than the weight of the cork.
  • The density of a substance is defined as the mass per unit volume.
  • Objects of density less than that of a liquid float on the liquid.
  • Objects of density greater than that of a liquid sink in the liquid.

Archimedes’ Principle

  • Activity 9.7: Stone tied to a rubber string or a spring balance, gradually lowered in water.
  • The elongation of the string or the reading of the balance decreases as the stone is gradually lowered in the water.
  • This indicates that some force acts on the stone in an upward direction: force of buoyancy.
  • Archimedes' principle: When a body is immersed fully or partially in a fluid, it experiences an upward force that is equal to the weight of the fluid displaced by it.
  • Archimedes used this principle to determine the purity of gold in the crown made for the king.
  • Archimedes’ principle has many applications. It is used in designing ships and submarines.
  • Lactometers and hydrometers are based on this principle.