🌍 GRAVITATION · Universal Law · Fields · Satellites
Newton's law • Gravitational potential • Escape velocity • Orbital motion • Kepler's laws • NEET problems
🍎 NEWTON'S UNIVERSAL LAW
Every particle attracts every other particle with a force: F = G m₁ m₂ / r²
G = 6.67 × 10⁻¹¹ N m²/kg² (universal constant)
Vector form: F₁₂ = –G m₁ m₂ / r² · r̂
✏️ Two masses attracting
🌀 GRAVITATIONAL FIELD & POTENTIAL
Field intensity (g): Force per unit mass: g = F/m = GM/r² (direction towards M)
Gravitational potential (V): V = –GM/r (zero at infinity)
U = m V = –GMm/r
Relation: g = –dV/dr
For spherical shell: Inside (r < R) → g = 0, V = –GM/R (constant).
For solid sphere: Inside → g ∝ r, V = –GM(3R² – r²)/(2R³).
📜 KEPLER'S LAWS OF PLANETARY MOTION
1st Law (Law of Orbits)
Planets move in elliptical orbits with Sun at one focus.
2nd Law (Law of Areas)
Areal velocity constant → dA/dt = L/(2m) = constant. Planets move faster near perihelion.
3rd Law (Law of Periods)
T² ∝ r³ (for circular orbits). More precisely: T² = (4π²/GM) r³.
🪐 Kepler's 2nd law – equal areas in equal time
🚀 ESCAPE VELOCITY & SATELLITE MOTION
Escape velocity: vesc = √(2GM/R) = √(2gR) ≈ 11.2 km/s (Earth)
Orbital velocity (circular): vo = √(GM/r) = √(gR²/r)
For near-Earth orbit (r ≈ R): vo ≈ 7.9 km/s
Time period: T = 2πr / vo = 2π √(r³/GM)
Total energy of satellite: E = –GMm/(2r) = –K (KE = –E, PE = 2E)
🛰️ Satellite in circular orbit
📉 VARIATION OF g & POTENTIAL ENERGY
g with height: gh = g(1 – 2h/R) for h << R
g with depth: gd = g(1 – d/R)
g with rotation: geff = g – ω²R cos²λ (λ = latitude)
Potential energy (near Earth): U = mgh (valid only for small h)
True U = –GMm/r; gravitational binding energy of a sphere = –(3/5) GM²/R.
💡 NEET TIPS & SHORTCUTS
- For circular orbits, v ∝ 1/√r, T ∝ r³/², KE ∝ 1/r, PE ∝ –1/r.
- If orbital radius increases, speed decreases but time period increases.
- Escape velocity is √2 times orbital velocity.
- At the center of Earth, g = 0 but gravitational potential is minimum (most negative).
⚠️ COMMON MISTAKES
- Using g = GM/r² for points inside Earth – only valid outside.
- Confusing gravitational potential energy with potential (V = U/m).
- Forgetting that satellites in lower orbits have higher speeds.
- Applying Kepler's 3rd law for non-circular orbits without using semi-major axis.
📌 QUICK REVISION CARD
Newton's law: F = GMm/r²
Gravitational field: g = GM/r²
Potential: V = –GM/r
Orbital velocity: vo = √(GM/r)
Escape velocity: vesc = √(2GM/r)
Time period: T = 2π√(r³/GM)
🌍 GRAVITATION • NEET REVISION NOTES
📸 NOTES PREVIEW
Preview of Gravitation Notes
📥 DOWNLOAD GRAVITATION NOTES PDF
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📊 WEIGHTAGE ANALYSIS
2–3 Questions
Orbital + escape velocity
High Weightage
Theory + numericals