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
- Distance from Impact: 161.00 km ( = 100.00 miles )
- Projectile diameter: 2.00 meters ( = 6.56 feet )
- Projectile Density: 8000 kg/m3
- Impact Velocity: 14.70 km per second ( = 9.10 miles per second )
- Impact Angle: 90 degrees
- Target Density: 2750 kg/m3
- Target Type: Crystalline Rock
- Energy before atmospheric entry: 3.60 x 1012 Joules = 0.86 x 10-3 MegaTons TNT
- The average interval between impacts of this size somewhere on Earth is 0.5 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.
- The projectile begins to breakup at an altitude of 10200 meters = 33500 ft
- The projectile bursts into a cloud of fragments at an altitude of 8620 meters = 28300 ft
- The residual velocity of the projectile fragments after the burst is 5.37 km/s = 3.34 miles/s
- The energy of the airburst is 3.12 x 1012 Joules = 0.74 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 size-frequency distribution of meteoroid fragments and predict the number and size of craters formed.
- What does this mean?
The air blast will arrive approximately 8.14 minutes after impact.
- Peak Overpressure: 21 Pa = 0.00021 bars = 0.00299 psi
- Max wind velocity: 0.0496 m/s = 0.111 mph
- Sound Intensity: 26 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
Earth Impact Effects Program Copyright 2004, Robert Marcus, H.J. Melosh, and G.S. Collins
These results come with ABSOLUTELY NO WARRANTY