Asteroid Crater Diameter Calculator
Calculate the transient and final crater diameter from an asteroid impact using the Pi-scaling law.
How Asteroid Impact Craters Form
When an asteroid strikes a planetary surface at cosmic velocities (typically 15-25 km/s for Earth), the kinetic energy is so immense that both the impactor and target material are vaporized, melted, or shattered. The impact creates a transient cavity that then collapses and modifies into the final crater we observe.
The Pi-Scaling Law
The Pi-scaling law uses dimensional analysis to relate impactor properties to crater size. The transient crater diameter is:
Dtc = 1.16 × (ρi/ρt)1/3 × D0.78 × v0.43 × g-0.22 × sin(θ)1/3
Where D is impactor diameter (m), v is velocity (m/s), g is surface gravity (m/s²), and θ is the impact angle. The final crater is approximately 1.3 times the transient diameter due to rim collapse and ejecta settling.
Impact Angle Effects
The most probable impact angle on a sphere is 45 degrees (not 90 degrees, due to the sine-weighted probability distribution of approach trajectories). At 45 degrees, the effective energy transfer is about 79% of a vertical impact. Very oblique impacts (under 15 degrees) create elongated, butterfly-shaped ejecta patterns and shallower craters.
Famous Impact Craters
The Chicxulub crater (Mexico, 180 km diameter) was formed by a ~12 km asteroid 66 million years ago, triggering the mass extinction that ended the dinosaurs. Meteor Crater (Arizona, 1.2 km) was formed by a ~50 m iron meteorite only 50,000 years ago. The Vredefort crater (South Africa, 300 km) is the largest known impact structure on Earth, formed 2 billion years ago.
Energy Scale
A 1 km asteroid at 20 km/s carries energy equivalent to roughly 50,000 megatons of TNT (about 1 million times the Hiroshima bomb). Even a 50-meter object like the Chelyabinsk meteor (2013) released energy equivalent to 500 kilotons, thirty times the Hiroshima bomb, though most was absorbed by the atmosphere.