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Physics - Mechanics

July 11, 2026
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Physics - Chapter 1: Mechanics

⚙️ Physics — Mechanics

Mechanics Physics
Figure 1: Mechanics — the branch of physics dealing with motion, forces, and energy.

1. Physical Quantity

Mechanics is the branch of science concerned with the behaviour of physical bodies when subjected to forces or displacements, and the subsequent effects on their environment.

A physical quantity is a property of a body, substance, or phenomenon that can be quantified by measurement.

MEASUREMENT & ERRORS

  • Absolute Error: Difference between true value and measured value.
  • Relative Error: Ratio of absolute error to mean value.
  • Percentage Error: Fractional error × 100.

2. Systems of Units

  • CGS: Centimetre, Gram, Second
  • FPS: Foot, Pound, Second
  • MKS: Metre, Kilogram, Second
  • SI: International System (adopted 1971)
FUNDAMENTAL QUANTITIES (SI)

# Quantity Unit Symbol
1 Length Metre m
2 Mass Kilogram kg
3 Time Second s
4 Electric current Ampere A
5 Temperature Kelvin K
6 Luminous intensity Candela cd
7 Amount of substance Mole mol

Supplementary: Radian (plane angle) · Steradian (solid angle)

IMPORTANT DERIVED UNITS

Quantity SI Unit Symbol
Force newton N
Energy / Work joule J
Speed metre/second ms⁻¹
Frequency hertz Hz
Pressure pascal Pa
Power watt W
Surface tension newton/metre Nm⁻¹
Viscosity newton second/metre² Nsm⁻²
Electric charge coulomb C
Electrical resistance ohm Ω
Impulse newton second Ns
LENGTH · MASS · TIME

  • 1 metre = distance travelled by light in vacuum in 1/299,792,458 of a second.
  • 1 light year = 9.46 × 10¹⁵ m
  • 1 parsec = 3.085 × 10¹⁵ m
  • 1 angstrom (Å) = 10⁻¹⁰ m
  • 1 nanometre (nm) = 10⁻⁹ m
  • 1 Fermi = 10⁻¹⁵ m
  • 1 kg = mass of 5.0188 × 10²⁵ atoms of carbon-12
  • 1 amu = 1.66 × 10⁻²⁷ kg
  • 1 second = 1/86400 of a mean solar day
SI PREFIXES

Prefix Symbol Factor
exaE10¹⁸
petaP10¹⁵
teraT10¹²
gigaG10⁹
megaM10⁶
kilok10³
centic10⁻²
millim10⁻³
microμ10⁻⁶
nanon10⁻⁹
picop10⁻¹²
femtof10⁻¹⁵

3. Scalar & Vector Quantities

  • Scalar: Magnitude only (e.g., length, mass, time)
  • Vector: Magnitude and direction (e.g., force, displacement, impulse)
DIMENSIONS

  • Dimensions are the powers to which fundamental units are raised.
  • Velocity: [L T⁻¹]
  • Density: [M L⁻³]

4. Kinematics

Study of motion without considering its cause.

REST & MOTION

  • Rest: No change in position with time
  • Motion: Change in position with time
  • Types: Rectilinear · Angular · Rotational
DISTANCE vs DISPLACEMENT

  • Distance: Scalar, length of actual path (always ≥ 0)
  • Displacement: Vector, change in position (can be +, −, or 0)
SPEED

  • Formula: Speed = Distance / Time
  • Average speed: Total distance / Total time
  • For equal distances with speeds v₁, v₂: average = 2v₁v₂/(v₁ + v₂)
  • For equal times with speeds v₁, v₂: average = (v₁ + v₂)/2
VELOCITY

  • Formula: Velocity = Displacement / Time
  • Relative velocity: |vAB| = √(vA² + vB² − 2vAvB·cos θ)
  • Same direction (θ = 0°): vAB = vA − vB
  • Opposite direction (θ = 180°): vAB = vA + vB
ACCELERATION

  • Formula: Acceleration = Change in velocity / Time
  • Positive: Velocity increases
  • Negative (retardation): Velocity decreases
  • SI unit: ms⁻²
EQUATIONS OF UNIFORMLY ACCELERATED MOTION

  • v = u + at
  • s = ut + ½at²
  • v² = u² + 2as
  • Free fall: replace 'a' with 'g'
  • Vertical upward: replace 'a' with '−g'
  • Distance in nth second: sn = u + (a/2)(2n − 1)
PROJECTILE MOTION

  • Horizontal component (u cos θ) — constant
  • Vertical component (u sin θ) — variable
  • Time of flight: T = 2u sin θ / g
  • Max height: H = u² sin²θ / (2g)
  • Range: R = u² sin 2θ / g
  • Rmax at θ = 45°
CIRCULAR MOTION

  • Angular displacement (θ): arc / radius
  • Angular velocity (ω): θ / t
  • Linear velocity: v = ω · r
  • Centripetal acceleration: v²/r = rω²
  • Centripetal force: Fc = mv²/r = mrω²

5. Force & Newton's Laws

Force: Push/pull that can change the state of rest or motion. SI unit: Newton (N) · 1 N = 10⁵ dyne

FOUR FUNDAMENTAL FORCES

  1. Gravitational force
  2. Electromagnetic force
  3. Weak nuclear force
  4. Strong nuclear force (strongest)
NEWTON'S LAWS

  • First Law (Inertia): Body remains at rest or uniform motion unless acted upon by external force.
  • Second Law: F = Δp/Δt = ma (for constant mass)
  • Third Law: Every action has an equal and opposite reaction.
MOMENTUM & IMPULSE

  • Momentum: p = m·v (vector, kg ms⁻¹)
  • Conservation of linear momentum: Rocket propulsion
  • Impulse: Force × Time = Change in momentum

6. Friction

  • Static friction: Opposes tendency to move (self-adjusting)
  • Limiting friction: μsR = μsmg
  • Kinetic friction: Opposes actual motion
    • Sliding friction
    • Rolling friction (smaller than sliding)
COEFFICIENT OF FRICTION

  • Formula: μ = F / R
  • Applications: Ball bearings, tyre threading, braking, walking

7. Work, Energy & Power

WORK

  • Formula: W = F · s · cos θ
  • Scalar, SI unit: Joule (J) · 1 J = 10⁷ erg
  • Work = 0 when s = 0 or θ = 90°
ENERGY

  • Kinetic Energy: K = ½mv² = p²/2m
  • Potential Energy: U = mgh
  • Forms: Solar · Fossil · Hydroelectric · Nuclear
  • Einstein's Mass-Energy: E = Δmc²
POWER

  • Formula: P = W/t = F·v
  • SI unit: Watt (W)
  • 1 HP = 746 W · 1 kW = 1000 W

8. Collision

  • Elastic: Momentum & kinetic energy conserved
  • Inelastic: Only momentum conserved
  • Perfectly inelastic: Bodies stick together

9. Gravitation

NEWTON'S LAW OF GRAVITATION

  • Formula: F = G·m₁·m₂ / r²
  • G = 6.67 × 10⁻¹¹ Nm²kg⁻²
ACCELERATION DUE TO GRAVITY

  • Formula: g = GM/R² ≈ 9.8 ms⁻²
  • Maximum at poles, minimum at equator
  • Decreases with height & depth
  • Becomes zero at Earth's centre
ESCAPE VELOCITY

  • Formula: ve = √(2GM/R) = √(2gR) ≈ 11.2 km/s
PLANETS (Distance from Sun)

Mercury → Venus → Earth → Mars → Jupiter → Saturn → Uranus → Neptune

KEPLER'S LAWS

  1. Elliptical orbits with Sun at one focus
  2. Areal speed is constant
  3. T² ∝ a³
SATELLITES

  • Geostationary: height ≈ 36,000 km, T = 24 h
  • Polar: height ≈ 800 km, T ≈ 84 min
  • Formula: T = 2π√(R/g) ≈ 84.6 min (near Earth)

📌 Summary: Mechanics at a Glance

Topic Key Formula Key Point
Speed v = s/t Scalar quantity
Velocity v = d/t Vector quantity
Acceleration a = Δv/t SI unit: ms⁻²
Force F = ma SI unit: Newton (N)
Work W = F·s·cosθ SI unit: Joule (J)
Kinetic Energy K = ½mv² Energy of motion
Potential Energy U = mgh Energy of position
Power P = W/t SI unit: Watt (W)
Gravitation F = Gm₁m₂/r² G = 6.67×10⁻¹¹
Escape Velocity ve = √(2gR) ≈ 11.2 km/s
KEY TAKEAWAYS FOR UPSC

  • SI Fundamental Units: 7 — metre, kg, second, ampere, kelvin, candela, mole
  • Scalar vs Vector: Scalar = magnitude only; Vector = magnitude + direction
  • Equations of Motion: v = u + at, s = ut + ½at², v² = u² + 2as
  • Projectile: Range maximum at 45°; Time of flight = 2u sinθ/g
  • Newton's Laws: Inertia, F = ma, Action-Reaction
  • Energy Conservation: Energy cannot be created or destroyed
  • Escape Velocity: 11.2 km/s (Earth)
  • Geostationary Satellite: 36,000 km, 24 hours
🎯 High-Yield Interactive UPSC Quiz (Physics — Mechanics)

Q1. What is the SI unit of force?

Correct Answer: B. The SI unit of force is Newton (N). 1 N = 1 kg·m/s².

Q2. Which of the following is a vector quantity?

Correct Answer: C. Displacement is a vector quantity (has both magnitude and direction). Mass, speed, and time are scalars.

Q3. The equation v = u + at represents:

Correct Answer: B. v = u + at is the first equation of motion (velocity-time relation).

Q4. At what angle is the range of a projectile maximum?

Correct Answer: C. The range of a projectile is maximum at an angle of 45°.

Q5. Which of Newton's laws explains the working of a rocket?

Correct Answer: C. Rocket propulsion works on Newton's third law — action and reaction are equal and opposite.

Q6. The value of acceleration due to gravity (g) is maximum at:

Correct Answer: B. The value of g is maximum at the poles and minimum at the equator.

Q7. What is the escape velocity from Earth's surface?

Correct Answer: B. Escape velocity from Earth's surface is approximately 11.2 km/s.

Q8. A geostationary satellite has a time period of:

Correct Answer: B. A geostationary satellite has a time period of 24 hours, matching Earth's rotation.

Q9. Which of the following is NOT a fundamental quantity in SI system?

Correct Answer: D. Force is a derived quantity, not a fundamental quantity in the SI system.

Q10. The centripetal force required for circular motion is provided by which force for electrons orbiting the nucleus?

Correct Answer: B. The electrostatic force of attraction between the electron and nucleus acts as the centripetal force.
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