Comprehensive Study Guide on Gravitational Potential Energy, Kinetic Energy, and Conservation of Mechanical Energy

Gravitational Potential Energy

  • Definition: The energy an object possesses due to its position above a reference point (typically the ground).

  • Fundamental Equation:

    • Ep=m×g×hE_p = m \times g \times h

    • Ep=mghE_p = mgh

  • Variables, Standard Units, and Values:

    • EpE_p: Potential energy, measured in Joules (J\text{J}).

    • mm: Mass of the object, which must strictly be in kilograms (kg\text{kg}).

    • gg: Gravitational acceleration (gravity). On Earth, g=9,8 m/s2g = 9,8\,\text{m/s}^2.

    • hh: Height of the object above the reference point, which must strictly be in metres (m\text{m}).

  • Boundary Condition for Height:

    • If h=0 mh = 0\,\text{m}, then Ep=0 JE_p = 0\,\text{J}.

  • Proportionality and Relationships:

    • As the mass (mm) of an object increases, its potential energy (EpE_p) increases proportionally.

    • As the height (hh) of an object increases, its potential energy (EpE_p) increases proportionally.

  • Formula Triangle Representation:

    • Top vertex: EpE_p

    • Bottom divisions: mm, gg, hh

    • Rearrangements derived from the triangle:

    • m=Epg×hm = \frac{E_p}{g \times h}

    • h=Epm×gh = \frac{E_p}{m \times g}

    • g=Epm×hg = \frac{E_p}{m \times h}

  • Unit Conversion Rules for Potential Energy Calculations:

    • Mass conversions:

    • Convert grams (g\text{g}) to kilograms (kg\text{kg}) by dividing by 10001000 (÷1000\div 1000).

    • Height conversions:

    • Convert centimetres (cm\text{cm}) to metres (m\text{m}) by dividing by 100100 (÷100\div 100).

    • Convert millimetres (mm\text{mm}) to metres (m\text{m}) by dividing by 10001000 (÷1000\div 1000).

    • Convert kilometres (km\text{km}) to metres (m\text{m}) by multiplying by 10001000 (×1000\times 1000).

    • Energy conversions:

    • Convert kilojoules (kJ\text{kJ}) to Joules (J\text{J}) by multiplying by 10001000 (×1000\times 1000).

  • Worked Examples for Gravitational Potential Energy:

    • Example 1: Calculating Potential Energy from Mass and Height

    • Given values:

      • m=300 gm = 300\,\text{g}

      • h=40 mh = 40\,\text{m}

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Unit conversion:

      • m=300 g1000=0,3 kgm = \frac{300\,\text{g}}{1000} = 0,3\,\text{kg}

    • Calculation:

      • Ep=m×g×hE_p = m \times g \times h

      • Ep=0,3×9,8×40E_p = 0,3 \times 9,8 \times 40

      • Ep=117,6 JE_p = 117,6\,\text{J}

    • Example 2: Calculating Mass from Potential Energy and Height

    • Given values:

      • Ep=160 JE_p = 160\,\text{J}

      • h=30 mh = 30\,\text{m}

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Calculation:

      • Ep=m×g×hE_p = m \times g \times h

      • 160=m×9,8×30160 = m \times 9,8 \times 30

      • 160=294×m160 = 294 \times m

      • 160294=294 m294\frac{160}{294} = \frac{294\,m}{294}

      • m=0,544 kgm = 0,544\,\text{kg}

    • Example 3: Calculating Height from Potential Energy and Mass

    • Given values:

      • m=60 kgm = 60\,\text{kg}

      • Ep=0,85 kJE_p = 0,85\,\text{kJ}

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Unit conversion:

      • Ep=0,85 kJ×1000=850 JE_p = 0,85\,\text{kJ} \times 1000 = 850\,\text{J}

    • Calculation:

      • Ep=m×g×hE_p = m \times g \times h

      • 850=60×9,8×h850 = 60 \times 9,8 \times h

      • 850=588×h850 = 588 \times h

      • 850588=588 h588\frac{850}{588} = \frac{588\,h}{588}

      • h=1,446 mh = 1,446\,\text{m}

Kinetic Energy

  • Definition: The energy that an object possesses due to its motion.

  • Fundamental Equation:

    • Ek=12 m v2E_k = \frac{1}{2}\,m\,v^2

  • Variables and Standard Units:

    • EkE_k: Kinetic energy, measured in Joules (J\text{J}).

    • mm: Mass of the object in kilograms (kg\text{kg}).

    • vv: Speed or velocity of the object, measured in metres per second (m/s\text{m/s} or m⋅s−1\text{m}\cdot\text{s}^{-1}).

  • Boundary Condition for Motion:

    • If an object is stationary (v=0 m/sv = 0\,\text{m/s}, not moving), then Ek=0 JE_k = 0\,\text{J}.

  • Unit Conversions for Kinetic Energy Calculations:

    • Velocity conversion:

    • If given speed in kilometres per hour (km/h\text{km/h}), convert it into metres per second (m/s\text{m/s}) by dividing by 3,63,6 (÷3,6\div 3,6).

    • Mass conversion:

    • Convert grams (g\text{g}) to kilograms (kg\text{kg}) by dividing by 10001000 (÷1000\div 1000).

    • Energy conversion:

    • Convert kilojoules (kJ\text{kJ}) to Joules (J\text{J}) by multiplying by 10001000 (×1000\times 1000).

  • Proportionality and Velocity Scaling:

    • Kinetic energy is directly proportional to the square of the velocity (Ek∝v2E_k \propto v^2).

    • When velocity is doubled (v→2vv \rightarrow 2v), kinetic energy increases by a factor of four (4×4\times).


Formula triangle and worked physics problems for potential and kinetic energy
  • Worked Examples for Kinetic Energy:

    • Example 4: Velocity Doubling Derivation and Verification

    • Problem formulation:

      • An object has a kinetic energy of EE when the velocity is vv. Determine the kinetic energy if the velocity doubles.

      • Options: A. EE, B. 2E2E, C. 4E4E, D. 12E\frac{1}{2}E

      • Correct selection: C (4E4E)

    • Algebraic proof:

      • Ek=12 m (2v)2E_k = \frac{1}{2}\,m\,(2v)^2

      • Ek=12 m (4v2)E_k = \frac{1}{2}\,m\,(4v^2)

      • Ek=4×(12 m v2)=4EE_k = 4 \times \left(\frac{1}{2}\,m\,v^2\right) = 4E

    • Numerical demonstration:

      • Let m=50 kgm = 50\,\text{kg} and v=10 m/sv = 10\,\text{m/s}:

      • Ek=12 m v2=0,5×50×(10)2=2500 JE_k = \frac{1}{2}\,m\,v^2 = 0,5 \times 50 \times (10)^2 = 2500\,\text{J}

      • Doubling velocity to v=20 m/sv = 20\,\text{m/s}:

      • Ek=0,5×50×(20)2=0,5×50×400=10000 JE_k = 0,5 \times 50 \times (20)^2 = 0,5 \times 50 \times 400 = 10000\,\text{J}

      • Ratio: 10000 J2500 J=4\frac{10000\,\text{J}}{2500\,\text{J}} = 4

    • Example 5: Calculating Kinetic Energy with Unit Conversions

    • Given values:

      • m=800 gm = 800\,\text{g}

      • v=9 km/hv = 9\,\text{km/h}

    • Unit conversions:

      • m=800 g1000=0,8 kgm = \frac{800\,\text{g}}{1000} = 0,8\,\text{kg}

      • v=9 km/h3,6=2,5 m/sv = \frac{9\,\text{km/h}}{3,6} = 2,5\,\text{m/s}

    • Calculation:

      • Ek=12 m v2E_k = \frac{1}{2}\,m\,v^2

      • Ek=(0,5)(0,8)(2,5)2E_k = (0,5)(0,8)(2,5)^2

      • Ek=0,4×6,25E_k = 0,4 \times 6,25

      • Ek=2,5 JE_k = 2,5\,\text{J}

    • Example 6: Calculating Mass from Kinetic Energy and Velocity

    • Given values:

      • Ek=9,6 kJE_k = 9,6\,\text{kJ}

      • v=20 m/sv = 20\,\text{m/s}

    • Unit conversion:

      • Ek=9,6 kJ×1000=9600 JE_k = 9,6\,\text{kJ} \times 1000 = 9600\,\text{J}

    • Calculation:

      • Ek=12 m v2E_k = \frac{1}{2}\,m\,v^2

      • 9600=12 m (20)29600 = \frac{1}{2}\,m\,(20)^2

      • 9600=12 (400) m9600 = \frac{1}{2}\,(400)\,m

      • 9600=200 m9600 = 200\,m

      • 9600200=200 m200\frac{9600}{200} = \frac{200\,m}{200}

      • m=48 kgm = 48\,\text{kg}

Mechanical Energy and the Conservation Principle

  • Definition: Mechanical energy (also referred to as Total energy) is the sum of the gravitational potential energy and kinetic energy of an object.

  • Fundamental Equations:

    • Emech=Ep+EkE_{\text{mech}} = E_p + E_k

    • Emech=mgh+12 m v2E_{\text{mech}} = mgh + \frac{1}{2}\,m\,v^2

  • Principle of Conservation of Mechanical Energy:

    • Mechanical energy remains constant in an isolated system in the absence of friction or external non-conservative forces.

  • Strategic Rules for Energy Problem Solving:

    • Work out EmechE_{\text{mech}} once per problem scenario, as it remains constant throughout the motion.

    • Use the comprehensive long equation (Emech=mgh+12 m v2E_{\text{mech}} = mgh + \frac{1}{2}\,m\,v^2) whenever more than two unknown variables are present across separated energy states.

    • Physical terminology convention: The word "dropped" explicitly indicates that the initial release speed of an object is zero (v=0 m/sv = 0\,\text{m/s}), making initial kinetic energy Ek=0 JE_k = 0\,\text{J}.


Worked mechanical energy problems for falling bodies and projected objects
  • Worked Examples for Mechanical Energy:

    • Example 7: Dropped Object from a Building

    • System configuration:

      • A ball of mass 400 g400\,\text{g} is dropped from the top of a 90 m90\,\text{m} building.

      • "Dropped" implies initial velocity v=0 m/sv = 0\,\text{m/s}.

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Unit conversion:

      • m=400 g1000=0,4 kgm = \frac{400\,\text{g}}{1000} = 0,4\,\text{kg}

    • Step 7.1: Gravitational potential energy at start position:

      • Ep=mghE_p = mgh

      • Ep=0,4×9,8×90E_p = 0,4 \times 9,8 \times 90

      • Ep=352,8 JE_p = 352,8\,\text{J}

    • Step 7.2: Kinetic energy at start position:

      • Ek=0 JE_k = 0\,\text{J}

      • Explanation: The ball is not moving at the release point.

    • Step 7.3: Total mechanical energy at start position:

      • Emech=Ep+EkE_{\text{mech}} = E_p + E_k

      • Emech=352,8+0E_{\text{mech}} = 352,8 + 0

      • Emech=352,8 JE_{\text{mech}} = 352,8\,\text{J}

    • Example 8: Object Possessing Both Potential and Kinetic Energy

    • System configuration:

      • A ball of mass 600 g600\,\text{g} is at a height of 30 m30\,\text{m} above the ground.

      • Speed of the ball: v=3 m/sv = 3\,\text{m/s}.

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Unit conversion:

      • m=600 g1000=0,6 kgm = \frac{600\,\text{g}}{1000} = 0,6\,\text{kg}

    • Step 8.1: Potential energy at this height:

      • Ep=mghE_p = mgh

      • Ep=0,6×9,8×30E_p = 0,6 \times 9,8 \times 30

      • Ep=176,4 JE_p = 176,4\,\text{J}

    • Step 8.2: Kinetic energy at this height:

      • Ek=12 m v2E_k = \frac{1}{2}\,m\,v^2

      • Ek=0,5×0,6×(3)2E_k = 0,5 \times 0,6 \times (3)^2

      • Ek=0,3×9E_k = 0,3 \times 9

      • Ek=2,7 JE_k = 2,7\,\text{J}

    • Step 8.3: Mechanical energy at this height:

      • Emech=Ep+EkE_{\text{mech}} = E_p + E_k

      • Emech=176,4+2,7E_{\text{mech}} = 176,4 + 2,7

      • Emech=179,1 JE_{\text{mech}} = 179,1\,\text{J}

    • Example 9: Dropped Cellphone and Conservation of Energy

    • System configuration:

      • A man drops a cellphone of mass 200 g200\,\text{g} from a window 40 m40\,\text{m} above the ground.

      • g=9,8 m/s2g = 9,8\,\text{m/s}^2

    • Unit conversion:

      • m=200 g1000=0,2 kgm = \frac{200\,\text{g}}{1000} = 0,2\,\text{kg}

    • Step 9.1: Kinetic energy of the phone at the window:

      • Ek=12 m v2=0,5×0,2×(0)2=0 JE_k = \frac{1}{2}\,m\,v^2 = 0,5 \times 0,2 \times (0)^2 = 0\,\text{J}

      • Explanation: The phone is not moving at the instant of release.

    • Step 9.2: Potential energy of the phone at the window:

      • Ep=mghE_p = mgh

      • Ep=0,2×9,8×40E_p = 0,2 \times 9,8 \times 40

      • Ep=78,4 JE_p = 78,4\,\text{J}

    • Step 9.3: Mechanical energy of the phone at the window:

      • Emech=Ep+EkE_{\text{mech}} = E_p + E_k

      • Emech=78,4+0E_{\text{mech}} = 78,4 + 0

      • Emech=78,4 JE_{\text{mech}} = 78,4\,\text{J}

    • Step 9.4: Mechanical energy after falling 15 m15\,\text{m} downwards:

      • Emech=78,4 JE_{\text{mech}} = 78,4\,\text{J}

      • Explanation: Mechanical energy remains constant throughout free fall in the absence of friction.

Practice Problems and Energy Worksheet

  • Problem 1:

    • The speed of a 3 kg3\,\text{kg} object is 18 km/h18\,\text{km/h}.

    • Objective: Calculate its kinetic energy.

    • Necessary conversion: Convert 18 km/h18\,\text{km/h} into m/s\text{m/s} by dividing by 3,63,6: 183,6=5 m/s\frac{18}{3,6} = 5\,\text{m/s}.

  • Problem 2:

    • The speed of a 1400 g1400\,\text{g} ball is 4 m/s4\,\text{m/s}.

    • Objective: Calculate its kinetic energy.

    • Necessary conversion: Convert 1400 g1400\,\text{g} to kilograms: 14001000=1,4 kg\frac{1400}{1000} = 1,4\,\text{kg}.

  • Problem 3:

    • A 2 kg2\,\text{kg} object is thrown downwards in the air at 3 m/s3\,\text{m/s} from a 60 m60\,\text{m} ledge.

    • Sub-problems:

    • 3.1 Calculate the potential energy of the object at this position.

    • 3.2 Calculate the kinetic energy of the object at this position.

    • 3.3 Calculate the mechanical energy of the object at this position.

    • 3.4 Explain why the speed of the object increases as it travels downwards.

    • 3.5 The object descends to reach a new height of 24 m24\,\text{m}:

      • 3.5.1 Will its potential energy increase, decrease, or stay the same?

      • 3.5.2 Will its kinetic energy increase, decrease, or stay the same?

      • 3.5.3 Will its mechanical energy increase, decrease, or stay the same?

  • Problem 4:

    • A stone has a mass of 80 g80\,\text{g} at a height of 260 cm260\,\text{cm} above the roof of a car.

    • Objective: Calculate its potential energy at this position.

    • Necessary conversions:

    • Mass: 80 g1000=0,08 kg\frac{80\,\text{g}}{1000} = 0,08\,\text{kg}

    • Height: 260 cm100=2,6 m\frac{260\,\text{cm}}{100} = 2,6\,\text{m}

  • Problem 5:

    • The potential energy of a stationary 4 kg4\,\text{kg} object is 0,8 kJ0,8\,\text{kJ} at a height hh.

    • Sub-problems:

    • 5.1 Calculate the height hh.

    • 5.2 Determine the weight (W=m×gW = m \times g) of this object.

    • 5.3 Calculate the mechanical energy of this object.

  • Problem 6:

    • A metal ball has a weight of 588 N588\,\text{N} at a height of 400 cm400\,\text{cm} above the ground and is moving at a velocity of 2 m/s2\,\text{m/s}.

    • Sub-problems:

    • 6.1 Calculate the mass of the ball (using W=mgW = mg, where g=9,8 m/s2g = 9,8\,\text{m/s}^2).

    • 6.2 Calculate the potential energy of the ball at this height.

    • 6.3 Calculate the mechanical energy of the ball at this height.

Gravitational Potential Energy
  • Definition: Energy an object possesses due to its position above a reference point (usually the ground).

  • Formula:

    • Ep=mghE_p = mgh

  • Variables and Standard Units:

    • EpE_p: Potential energy in Joules (J\text{J}

    • mm: Mass in kilograms (kg\text{kg}

    • gg: Gravitational acceleration (9.8 m/s29.8\,\text{m/s}^2 on Earth)

    • hh: Height above the reference point in metres (m\text{m}

  • Key Rules and Proportionalities:

    • If h=0 mh = 0\,\text{m}, then Ep=0 JE_p = 0\,\text{J}.

    • EpE_p is directly proportional to both mass (mm) and height (hh).

  • Rearranged Formulas:

    • m=Epghm = \frac{E_p}{gh}

    • h=Epmgh = \frac{E_p}{mg}

    • g=Epmhg = \frac{E_p}{mh}

  • Unit Conversions:

    • Mass: Grams (g\text{g}) to kilograms (kg\text{kg}) →÷1000\rightarrow \div 1000

    • Height:

    • Centimetres (cm\text{cm}) to metres (m\text{m}) →÷100\rightarrow \div 100

    • Millimetres (mm\text{mm}) to metres (m\text{m}) →÷1000\rightarrow \div 1000

    • Kilometres (km\text{km}) to metres (m\text{m}) →×1000\rightarrow \times 1000

    • Energy: Kilojoules (kJ\text{kJ}) to Joules (J\text{J}) →×1000\rightarrow \times 1000

Kinetic Energy
  • Definition: Energy an object possesses due to its motion.

  • Formula:

    • Ek=12 m v2E_k = \frac{1}{2}\,m\,v^2

  • Variables and Standard Units:

    • EkE_k: Kinetic energy in Joules (J\text{J}

    • mm: Mass in kilograms (kg\text{kg}

    • vv: Speed or velocity in metres per second (m/s\text{m/s}

  • Key Rules and Proportionalities:

    • If stationary (v=0 m/sv = 0\,\text{m/s}), then Ek=0 JE_k = 0\,\text{J}.

    • E<em>k∝v2E<em>k \propto v^2: Doubling velocity (2v2v) quadruples kinetic energy (4×E</em>k4 \times E</em>k).

  • Unit Conversions:

    • Speed: km/h\text{km/h} to m/s\text{m/s} →÷3.6\rightarrow \div 3.6

    • Mass: g\text{g} to kg\text{kg} →÷1000\rightarrow \div 1000

    • Energy: kJ\text{kJ} to J\text{J} →×1000\rightarrow \times 1000

Mechanical Energy and Conservation
  • Definition: The total energy of an object, equal to the sum of its potential and kinetic energy.

  • Formula:

    • E<em>mech=E</em>p+EkE<em>{\text{mech}} = E</em>p + E_k

    • Emech=mgh+12 m v2E_{\text{mech}} = mgh + \frac{1}{2}\,m\,v^2

  • Conservation Principle: In an isolated system (no friction or external forces), total mechanical energy remains constant throughout the motion.

  • Problem-Solving Guidelines:

    • Calculate EmechE_{\text{mech}} once per scenario, as it does not change.

    • The word "dropped" means initial speed is zero (v=0 m/sv = 0\,\text{m/s}), so initial Ek=0 JE_k = 0\,\text{J}.

    • As an object falls, E<em>pE<em>p decreases and converts into E</em>kE</em>k, causing speed to increase while EmechE_{\text{mech}} stays constant.

Practice Problem Prompts
  1. Calculate EkE_k for a 3 kg3\,\text{kg} object moving at 18 km/h18\,\text{km/h} (convert: 18÷3.6=5 m/s\text{convert: } 18 \div 3.6 = 5\,\text{m/s}.

  2. Calculate EkE_k for a 1400 g1400\,\text{g} ball moving at 4 m/s4\,\text{m/s} (convert: 1400÷1000=1.4 kg\text{convert: } 1400 \div 1000 = 1.4\,\text{kg}.

  3. A 2 kg2\,\text{kg} object is thrown downwards at 3 m/s3\,\text{m/s} from a height of 60 m60\,\text{m}:

    • Find E<em>pE<em>p, E</em>kE</em>k, and EmechE_{\text{mech}}.

    • Explain changes in E<em>pE<em>p, E</em>kE</em>k, and EmechE_{\text{mech}} as it falls to 24 m24\,\text{m}.

  4. Calculate EpE_p of an 80 g80\,\text{g} stone at a height of 260 cm260\,\text{cm}.

  5. A stationary 4 kg4\,\text{kg} object has Ep=0.8 kJE_p = 0.8\,\text{kJ}:

    • Calculate height hh, weight (W=mgW = mg), and EmechE_{\text{mech}}.

  6. A ball with a weight of 588 N588\,\text{N} is 400 cm400\,\text{cm} high and moving at 2 m/s2\,\text{m/s}:

    • Calculate mass, E<em>pE<em>p, and E</em>mechE</em>{\text{mech}}.