Physics — General Awareness
Overview
Physics questions in UPSC Prelims test your conceptual understanding of everyday phenomena rather than numerical problem-solving. These questions reward candidates who understand the "why" behind physical principles rather than memorising formulas.
This topic connects strongly with Science & Technology current affairs, especially space missions, defence technology, and energy. A solid grasp of basic physics also helps in Geography (atmospheric phenomena, ocean currents) and Environment (solar radiation, greenhouse effect). Focus on understanding principles qualitatively and linking them to real-world applications that UPSC favours.
Key Concepts
- Newton's Laws of Motion: First law (inertia)—objects resist change in motion; Second law—Force = mass × acceleration; Third law—every action has an equal and opposite reaction. These explain rocket propulsion, seatbelt necessity, and recoil of guns.
- Gravitation and Orbits: Objects in orbit are in continuous free fall around Earth. Geostationary satellites (36,000 km altitude) match Earth's rotation, appearing stationary—used for communication and weather monitoring.
- Pressure and Fluids: Pressure increases with depth (explains dam design, ear pain while diving). Atmospheric pressure decreases with altitude (why water boils at lower temperatures at high altitudes).
- Heat Transfer Mechanisms: Conduction (through solids, metal spoons getting hot), convection (fluids, sea breezes), radiation (no medium needed, solar energy reaching Earth). Vacuum flasks minimise all three.
- Wave Nature of Light and Sound: Light is electromagnetic (travels through vacuum), sound is mechanical (needs medium). Reflection, refraction, diffraction explain mirrors, lenses, rainbows, and why we hear sounds around corners.
- Electromagnetic Spectrum: Radio waves → Microwaves → Infrared → Visible light → Ultraviolet → X-rays → Gamma rays. Wavelength decreases and energy increases left to right. Each has specific applications.
- Electric Current and Circuits: Current = charge flow per second. Conductors allow easy flow, insulators resist it. Series circuits share current; parallel circuits share voltage. Household wiring uses parallel connections.
- Nuclear Reactions: Fission (heavy nucleus splits, used in reactors and atomic bombs) vs Fusion (light nuclei combine, powers the Sun, basis of hydrogen bombs). Fusion releases more energy but is harder to control.
Formulas / Key Facts
| Principle | Formula/Fact | Application |
|---|---|---|
| Speed of light | 3 × 10⁸ m/s in vacuum | Basis for light-year measurement |
| Speed of sound | ~330 m/s in air at 20°C | Thunder heard after lightning |
| Ohm's Law | V = I × R (Voltage = Current × Resistance) | Electrical circuit design |
| Power | P = V × I (Watts = Volts × Amperes) | Appliance ratings |
| Acceleration due to gravity | 9.8 m/s² on Earth's surface | Projectile motion, free fall |
| Escape velocity (Earth) | 11.2 km/s | Minimum speed to leave Earth's gravity |
| Absolute zero | −273.15°C (0 Kelvin) | Lowest theoretically possible temperature |
| Critical angle | Light undergoes total internal reflection beyond this | Optical fibres, mirages |
Worked Examples
Example 1: Pressure Cooker Principle Why does food cook faster in a pressure cooker?
Step 1: Sealed container traps steam, increasing pressure inside. Step 2: Higher pressure raises the boiling point of water above 100°C (typically to 120°C). Step 3: Higher temperature cooks food faster. Key insight: At high altitudes (lower atmospheric pressure), pressure cookers become even more essential as normal boiling point drops significantly.
Example 2: Why is the Sky Blue?
Step 1: Sunlight contains all colours (white light). Step 2: Earth's atmosphere scatters shorter wavelengths (blue, violet) more than longer wavelengths (red, orange)—Rayleigh scattering. Step 3: Blue light is scattered in all directions across the sky; we see blue when looking up. Step 4: At sunset, light travels through more atmosphere, scattering away blue light, leaving red/orange.
Example 3: How do Satellites Stay in Orbit?
Step 1: A satellite moves forward at high speed while Earth's gravity pulls it downward. Step 2: The curved Earth "falls away" at the same rate the satellite falls toward it. Step 3: Result: The satellite continuously falls around Earth without hitting it. Step 4: No fuel needed to maintain orbit—only to correct trajectory or change orbit.
Common Mistakes
- Confusing mass and weight: Mass is constant everywhere (measured in kg); weight is gravitational force on mass (measured in Newtons) and varies with location. You weigh less on the Moon but your mass stays the same.
- Thinking sound travels in vacuum: Sound requires a medium. There is no sound in space—explosions in space movies are scientifically inaccurate.
- Believing satellites need constant fuel: Satellites in stable orbits need fuel only for course corrections and manoeuvres, not to stay aloft. Drag from thin upper atmosphere gradually slows low-orbit satellites.
- Mixing up conduction, convection, radiation: Remember—conduction needs contact, convection needs fluid movement, radiation needs neither. A microwave oven heats via radiation (electromagnetic waves), not heat conduction.
- Assuming higher voltage always means more danger: Current (amperes) kills, not voltage alone. A static shock can be thousands of volts but tiny current. Household 230V is dangerous because it can drive lethal current through the body.
Quick Reference
- Inertia: Resistance to change in motion; why passengers lurch forward when a bus brakes.
- Electromagnetic waves: Travel at light speed, need no medium; includes radio, microwave, visible light, X-rays.
- Total Internal Reflection: Light trapped inside denser medium; principle behind optical fibres.
- Doppler Effect: Frequency change when source/observer moves; ambulance siren pitch change, redshift of galaxies.
- Greenhouse Effect: Certain gases trap infrared radiation; natural effect keeps Earth warm, excess causes global warming.
- Nuclear fission: Uranium/Plutonium splits → chain reaction → nuclear reactors; fusion: hydrogen → helium → stars and H-bombs.