Earth Impact Effects Program

Damage Map Version

Gareth Collins, H. Jay Melosh and Robert Marcus

Welcome to the Earth Impact Effects Program: an easy-to-use, interactive web site for estimating the regional environmental consequences of an impact on Earth. This program will estimate the ejecta distribution, ground shaking, atmospheric blast wave, and thermal effects of an impact as well as the size of the crater produced.

Please enter a location on Earth to impact, then enter values in the boxes below to describe your impact of choice. Select the impact effect you are interested in and rhen click "Display Impact Effects" to see the damage zone!

Location of Impact

(choose one)

Latitude: and Longitude: or or

Impact Parameters

Impact Examples

Projectile Parameters

Projectile Diameter or

Projectile Density (in kg/m3) or

Impact Parameters

Impact Velocity or

This is the velocity of the projectile before it enters the atmosphere. The minimum impact velocity on Earth is 11 km/s. Typical impact velocities are 17 km/s for asteroids and 51 km/s for comets. The maximum Earth impact velocity for objects orbiting the sun is 72 km/s.

Impact Angle (in degrees) or

The impact angle is measured from a plane tangent to the impact surface. This angle is 90 degrees for a vertical impact. The most probable angle of impact is 45 degrees.

Target Parameters

Target Type (if targeting the sea choose an approximate depth)
Water of depth:
Sedimentary Rock
Crystalline Rock

Tell me more...

Click here for a pdf document that details the observations, assumptions, and equations upon which this program is based. It describes our approach to quantifying the important impact processes that might affect the people, buildings, and landscape in the vicinity of an impact event and discusses the uncertainty in our predictions. The processes included are: atmospheric entry, impact crater formation, fireball expansion and thermal radiation, ejecta deposition, seismic shaking, and the propagation of the atmospheric blast wave.

Copyright © 2010 Imperial College London