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: 500.00 km ( = 311.00 miles )
- Projectile diameter: 20.00 meters ( = 65.60 feet )
- Projectile Density: 3000 kg/m3
- Impact Velocity: 12000.00 km per second ( = 7450.00 miles per second )
(Your chosen velocity is higher than the maximum for an object orbiting the sun)
- Impact Angle: 60 degrees
- Target Density: 2500 kg/m3
- Target Type: Sedimentary Rock
- Energy before atmospheric entry: 9.05 x 1020 Joules = 2.16 x 105 MegaTons TNT
- The average interval between impacts of this size somewhere on Earth during the last 4 billion years is 1.4 x 106years
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 159000 meters = 522000 ft
- The projectile bursts into a cloud of fragments at an altitude of 19800 meters = 64900 ft
- The residual velocity of the projectile fragments after the burst is 7370 km/s = 4580 miles/s
- The energy of the airburst is 5.63 x 1020 Joules = 1.35 x 105 MegaTons.
- No crater is formed, although large fragments may strike the surface.
- What does this mean?
The air blast will arrive approximately 25.3 minutes after impact.
- Peak Overpressure: 10200 Pa = 0.102 bars = 1.45 psi
- Max wind velocity: 23.1 m/s = 51.7 mph
- Sound Intensity: 80 dB (Loud as heavy traffic)
- Damage Description:
Glass windows may shatter.
Glass windows will shatter.
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