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: 1000.00 meters ( = 3280.00 feet )
 Projectile diameter: 1.00 meters ( = 3.28 feet )
 Projectile Density: 8000 kg/m^{3}
 Impact Velocity: 70.00 km per second ( = 43.50 miles per second )
 Impact Angle: 90 degrees
 Target Density: 2500 kg/m^{3}
 Target Type: Sedimentary Rock

Energy:
 Energy before atmospheric entry: 1.03 x 10^{13} Joules = 0.25 x 10^{2} MegaTons TNT
 The average interval between impacts of this size somewhere on Earth is 1.1 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 36700 meters = 120000 ft
 The projectile bursts into a cloud of fragments at an altitude of 32900 meters = 108000 ft
 The residual velocity of the projectile fragments after the burst is 58.2 km/s = 36.2 miles/s
 The energy of the airburst is 3.16 x 10^{12} Joules = 0.75 x 10^{3} MegaTons.
 Large fragments strike the surface and may create a crater strewn field. A more careful treatment of atmospheric entry is required to accurately estimate the sizefrequency distribution of meteoroid fragments and predict the number and size of craters formed.

Air Blast:
 What does this mean?
The air blast will arrive approximately 1.66 minutes after impact.  Peak Overpressure: 128  256 Pa = 0.00128  0.00256 bars = 0.0181  0.0363 psi
 Max wind velocity: 0.301 m/s = 0.673 mph
 Sound Intensity: 42 dB (Easily Heard)
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.
Earth Impact Effects Program Copyright 2004, Robert Marcus, H.J. Melosh, and G.S. Collins
These results come with ABSOLUTELY NO WARRANTY