MECHANICSDynamicsPhysics Calculator
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Newton's Law of Universal Gravitation

Newton's law states that every mass attracts every other mass with a force proportional to the product of masses and inversely proportional to the square of distance.

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Force follows inverse-square law: double distance = 1/4 force G = 6.67430×10⁻¹¹ N⋅m²/kg² (CODATA 2018) Surface gravity g depends only on planet mass and radius Escape velocity from Earth is ~11.2 km/s

Key quantities
Gm₁m₂/r²
F
Key relation
GM/R²
g
Key relation
√(2GM/r)
v_esc
Key relation
√(GM/r)
v_orb
Key relation

Ready to run the numbers?

Why: Gravity governs planetary motion, satellite orbits, and everyday weight.

How: Enter masses and distance. The calculator computes force, surface gravity, escape velocity, and orbital parameters.

Force follows inverse-square law: double distance = 1/4 forceG = 6.67430×10⁻¹¹ N⋅m²/kg² (CODATA 2018)

Run the calculator when you are ready.

Calculate Gravitational ForceF = Gm₁m₂/r²

🔧 Calculation Type

⚙️ Input Parameters

📊 Results

🌌
Universal Gravitational Force
Newton's Law of Universal Gravitation
Gravitational Force
9.820e+3
Newtons (N)
Gravity (g)
9.820
m/s²

📈 Visualizations

Surface Gravity Comparison

Force vs Distance

📝 Step-by-Step Solution

📊 Input Parameters

Gravitational constant: G = 6.674e-11 N⋅m²/kg²

Mass 1: m₁ = 1.000e+3 kg

Mass 2: m₂ = 5.972e+24 kg

Distance: r = 6.371e+6 m

🧮 Calculation

Newton's Law of Universal Gravitation: F = Gm₁m₂/r²

F = (6.674e-11 × 1.000e+3 × 5.972e+24) / 6.371e+6²

→ F = 9.820e+3 N

Gravitational acceleration on m₁: a = Gm₂/r²

→ a = 9.820e+0 m/s²

Gravitational potential energy: U = -Gm₁m₂/r

→ U = -6.256e+10 J

For educational and informational purposes only. Verify with a qualified professional.

🔬 Physics Facts

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Newton published the law in Principia (1687); G was first measured by Cavendish in 1798.

— Newton

📐

G is the least precisely known fundamental constant (~1 part in 10⁵).

— NIST CODATA

🚀

Escape velocity is √2 times orbital velocity at the same radius.

— Orbital mechanics

🛰️

ISS orbits at ~400 km; orbital period ~90 min.

— NASA

📋 Key Takeaways

  • • Newton's Law of Universal Gravitation: F = Gm₁m₂/r²
  • • Gravitational constant G = 6.67430×10⁻¹¹ N⋅m²/kg² (CODATA 2018)
  • • Force follows an inverse-square law with distance
  • • Surface gravity: g = GM/R² depends only on planet mass and radius

📖 What is Gravitational Force?

Gravitational force is the attractive force between any two objects with mass. It's one of the four fundamental forces of nature and is described by Newton's Law of Universal Gravitation (1687).

Always Attractive

Unlike electric/magnetic forces, gravity always attracts. There's no "negative mass" to create repulsion.

Inverse Square Law

Force decreases with distance squared. Double the distance = 1/4 the force. Triple = 1/9, etc.

Extremely Weak

Gravity is 10³⁶ times weaker than electromagnetism. We notice it only because Earth is so massive.

📐 Gravitational Formulas

Universal Gravitation

F = Gm₁m₂/r²

G = 6.674×10⁻¹¹ N⋅m²/kg²

F = gravitational force (N)

r = distance between centers (m)

Surface Gravity

g = GM/R²

M = mass of planet (kg)

R = radius of planet (m)

g = acceleration due to gravity (m/s²)

Escape Velocity

v_esc = √(2GM/r)

Minimum speed to escape gravity

Earth: ~11.2 km/s

Orbital Velocity

v_orbit = √(GM/r)

T = 2π√(r³/GM) (Kepler's 3rd)

For circular orbit

🌍 Solar System Data

BodyMass (kg)Radius (km)g (m/s²)Escape (km/s)
Sun1.989×10³⁰696,340274617.5
Earth5.972×10²⁴6,3719.8111.2
Moon7.348×10²²1,7371.622.38
Mars6.417×10²³3,3903.725.03
Jupiter1.898×10²⁷69,91124.7959.5
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