Earth Impact Effects Program

Robert Marcus, H. Jay Melosh, and Gareth Collins

Please note: the results below are estimates based on current (limited) understanding of the impact process and come with large uncertainties; they should be used with caution, particularly in the case of peculiar input parameters. All values are given to three significant figures but this does not reflect the precision of the estimate. For more information about the uncertainty associated with our calculations and a full discussion of this program, please refer to this article

Your Inputs:

Distance from Impact: 12900.00 km ( = 8000.00 miles )
Projectile diameter: 10.00 meters ( = 32.80 feet )
Projectile Density: 3000 kg/m3
Impact Velocity: 72.00 km per second ( = 44.70 miles per second ) (Your chosen velocity is higher than the maximum for an object orbiting the sun)
Impact Angle: 90 degrees
Target Density: 2500 kg/m3
Target Type: Sedimentary Rock


Energy before atmospheric entry: 4.07 x 1015 Joules = 972.65 KiloTons TNT
The average interval between impacts of this size somewhere on Earth is 107.7 years

Major Global Changes:

The Earth is not strongly disturbed by the impact and loses negligible mass.
The impact does not make a noticeable change in the tilt of Earth's axis (< 5 hundreths of a degree).
The impact does not shift the Earth's orbit noticeably.

Atmospheric Entry:

The projectile begins to breakup at an altitude of 77100 meters = 253000 ft
The projectile bursts into a cloud of fragments at an altitude of 27800 meters = 91200 ft
The residual velocity of the projectile fragments after the burst is 53.4 km/s = 33.1 miles/s
The energy of the airburst is 1.84 x 1015 Joules = 0.44 x 100 MegaTons.
No crater is formed, although large fragments may strike the surface.

Air Blast:

What does this mean?

The air blast will arrive approximately 10.8 hours after impact.
Peak Overpressure: 1.65 Pa = 0 bars = 0.000234 psi
Max wind velocity: 0.00388 m/s = 0.00867 mph
Sound Intensity: 4 dB (Barely Audible)

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.

Recent improvements in the airblast calculation are described here.

Earth Impact Effects Program Copyright 2004, Robert Marcus, H.J. Melosh, and G.S. Collins
These results come with ABSOLUTELY NO WARRANTY