Asteroid Impact Energy Calculator
Model asteroid impacts from small meteors to extinction-level events. Enter size, composition, speed, and angle to calculate impact energy, crater dimensions, and potential global effects. Covers Chelyabinsk-scale through Chicxulub-scale events.
Diameter of the asteroid (10 m = Chelyabinsk, 300 m = Apophis, 10 km = Chicxulub)
Enter a custom density value
Typical Earth impact velocity: 11-72 km/s (average ~20 km/s)
Angle relative to horizontal (45° is most probable)
Mass Estimate: m = ⁴⁄₃πr³ρ (assuming spherical body)
Energy in Megatons: EMT = Ek / 4.184×10¹⁵
Crater Diameter: Dc ≈ 60 × (da)0.65 (for large impacts)
Earthquake Magnitude: M = 4 + 0.67 × log₁₀(EMT)
• Mass: ~10,000 tonnes
• Energy: ~500 kT TNT
• Crater: ~135 m
• Airburst at ~30 km
Chicxulub-scale (10 km, 3000 kg/m³, 25 km/s):
• Mass: ~1.6 × 10¹⁵ kg
• Energy: ~100 million MT TNT
• Crater: ~180 km
• Extinction event confirmed
How is asteroid impact energy calculated?
Asteroid impact energy is calculated using the kinetic energy formula E = ½mv², where m is the mass of the asteroid and v is its velocity. The mass is determined from the asteroid diameter and density (assuming a spherical shape: m = ⁴⁄₃πr³ρ). This yields energy in Joules, which is typically converted to megatons of TNT (1 megaton = 4.184 × 10¹⁵ J). Additional factors like impact angle affect energy partitioning, crater formation, and atmospheric blast wave generation.
What would happen if a 100-meter asteroid hit Earth?
A 100-meter rocky asteroid (typical density 3000 kg/m³) impacting at 20 km/s would release about 84 megatons of energy — roughly 5,000 times the Hiroshima bomb. It would create a crater ~1.5 km wide, cause severe local devastation within a 50 km radius, and potentially trigger a regional tsunami if it struck the ocean. Events of this size occur about once every 5,000-10,000 years. The 1908 Tunguska event (estimated 50-60 m object) flattened 2,000 km² of forest.
What is the difference between an airburst and a ground impact?
An airburst occurs when a smaller or less dense asteroid explodes in the atmosphere before reaching the ground, typically for objects under 50 m in diameter. The 2013 Chelyabinsk meteor (~18 m) airburst at about 30 km altitude, releasing ~500 kT of energy. Larger and denser objects penetrate the atmosphere more effectively, reaching the ground to form impact craters. The threshold for ground impact versus airburst depends on size, density, velocity, and entry angle. Objects over 100 m typically reach the surface largely intact.
How does impact angle affect the outcome?
Impact angle significantly influences the energy transfer and resulting effects. A 45° angle (the most statistically probable) transfers maximum energy to the target surface. Steeper angles (near 90°) direct more energy downward, creating deeper craters but distributing the ejecta more symmetrically. Shallow angles (<15°) can cause the asteroid to skip through the atmosphere, potentially reducing the impact energy but spreading debris over a wider area. The angle also affects the shape of the crater and the direction of ejecta distribution.
🔗 Related Calculators
📐 Formula
Mass Estimate: m = ⁴⁄₃πr³ρ (assuming spherical body)
Energy in Megatons: EMT = Ek / 4.184×10¹⁵
Crater Diameter: Dc ≈ 60 × (da)0.65 (for large impacts)
Earthquake Magnitude: M = 4 + 0.67 × log₁₀(EMT)
📝 Example Calculation
• Mass: ~10,000 tonnes
• Energy: ~500 kT TNT
• Crater: ~135 m
• Airburst at ~30 km
Chicxulub-scale (10 km, 3000 kg/m³, 25 km/s):
• Mass: ~1.6 × 10¹⁵ kg
• Energy: ~100 million MT TNT
• Crater: ~180 km
• Extinction event confirmed