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: 30.00 km ( = 18.60 miles )
 Projectile diameter: 450.00 meters ( = 1480.00 feet )
 Projectile Density: 2650 kg/m^{3}
 Impact Velocity: 15.00 km per second ( = 9.32 miles per second )
 Impact Angle: 90 degrees
 Target Density: 2500 kg/m^{3}
 Target Type: Sedimentary Rock

Energy:
 Energy before atmospheric entry: 1.42 x 10^{19} Joules = 3.40 x 10^{3} MegaTons TNT
 The average interval between impacts of this size somewhere on Earth during the last 4 billion years is 1.2 x 10^{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.

Atmospheric Entry:
 The projectile begins to breakup at an altitude of 55800 meters = 183000 ft
 The projectile reaches the ground in a broken condition. The mass of projectile strikes the surface at velocity 14.8 km/s = 9.18 miles/s
 The impact energy is 1.38 x 10^{19} Joules = 3.30 x 10^{3}MegaTons.
 The broken projectile fragments strike the ground in an ellipse of dimension 0.62 km by 0.62 km

Crater Dimensions:
 What does this mean?
 Crater shape is normal in spite of atmospheric crushing; fragments are not significantly dispersed.
 Transient Crater Diameter:
5.75 km ( = 3.57 miles )
 Transient Crater Depth: 2.03 km ( = 1.26 miles )
 Final Crater Diameter:
7.26 km ( = 4.51 miles )
 Final Crater Depth: 537 meters ( = 1760 feet )
 The crater formed is a complex crater.
 The volume of the target melted or vaporized is 0.123 km^{3} = 0.0295 miles^{3}
 Roughly half the melt remains in the crater, where its average thickness is 4.74 meters ( = 15.5 feet ).

Thermal Radiation:
 What does this mean?
 At this impact velocity ( < 15 km/s), little vaporization occurs; no fireball is created, therefore, there is no thermal radiation damage.

Seismic Effects:
 What does this mean?
The major seismic shaking will arrive approximately 6 seconds after impact.  Richter Scale Magnitude: 7.0
 Mercalli Scale Intensity at a distance of 30 km:
VII. Damage negligible in buildings of good design and construction; slight to moderate in wellbuilt ordinary structures; considerable damage in poorly built or badly designed structures; some chimneys broken.
VIII. Damage slight in specially designed structures; considerable damage in ordinary substantial buildings with partial collapse. Damage great in poorly built structures. Fall of chimneys, factory stacks, columns, monuments, walls. Heavy furniture overturned.

Ejecta:
 What does this mean?
The ejecta will arrive approximately 1.31 minutes after the impact.  At your position there is a fine dusting of ejecta with occasional larger fragments
 Average Ejecta Thickness: 36.1 cm ( = 14.2 inches )
 Mean Fragment Diameter: 1.1 meters ( = 3.62 feet )

Air Blast:
 What does this mean?
The air blast will arrive approximately 1.52 minutes after impact.  Peak Overpressure: 157000 Pa = 1.57 bars = 22.3 psi
 Max wind velocity: 242 m/s = 540 mph
 Sound Intensity: 104 dB (May cause ear pain)
 Damage Description:
Multistory wallbearing buildings will collapse.
Wood frame buildings will almost completely collapse.
Highway truss bridges will collapse.
Glass windows will shatter.
Up to 90 percent of trees blown down; remainder stripped of branches and leaves.
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