Gravitation — Study Plan
NEST · Physics
Step-by-step Gravitation study plan for NEST Physics 2026 — structured month-wise approach to mastering this chapter.
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A structured approach to studying Gravitation for NEST Physics.
Study Plan for Gravitation
Day 1–2: Learn the Theory
Study the chapter thoroughly. Note down definitions, formulas, and key concepts.
Day 3: Practice Problems
Solve practice questions and previous year NEST problems. There are 234 questions available for this chapter.
Day 4: Revise & Test
Revise key formulas and concepts without looking at notes. Take a practice quiz to test your understanding.
What to Focus On
- Copernicus proposed the heliocentric model (Sun at center)
- Tycho Brahe provided accurate observational data
- Kepler formulated three laws of planetary motion
- Orbits are elliptical, not circular
- Planets move faster when closer to the Sun
- Angular momentum is conserved in planetary motion
- Force is proportional to product of masses
- Force is inversely proportional to square of distance
- G is universal constant = 6.67 × 10⁻¹¹ N⋅m²/kg²
Common Mistakes to Avoid
The value of acceleration due to gravity (g) is always 9.8 m/s² everywhere and for all problems
Gravitational force becomes zero at the center of Earth
Orbital velocity increases with height above Earth's surface
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