Re: Risky asteroid 2009 WM1
Since the solutions have become worse since its discovery I ran a impact senerio. Don't be within 50 miles of this one for sure. YIKES!
Impact Effects at around 50 miles from center.
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: 80.50 km = 49.99 miles
Projectile Diameter: 280.00 m = 918.40 ft = 0.17 miles
Projectile Density: 8000 kg/m3
Impact Velocity: 18.10 km/s = 11.24 miles/s
Impact Angle: 45 degrees
Target Density: 2750 kg/m3
Target Type: Crystalline Rock
Energy:
Energy before atmospheric entry: 1.51 x 1019 Joules = 3.60 x 103 MegaTons TNT
The average interval between impacts of this size somewhere on Earth during the last 4 billion years is 6.0 x 104years
Atmospheric Entry:
The projectile begins to breakup at an altitude of 15200 meters = 49800 ft
The projectile reaches the ground in a broken condition. The mass of projectile strikes the surface at velocity 17.9 km/s = 11.1 miles/s
The impact energy is 1.48 x 1019 Joules = 3.53 x 103MegaTons.
The broken projectile fragments strike the ground in an ellipse of dimension 0.503 km by 0.356 km
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 Earth's rotation period or the tilt of its axis.
The impact does not shift the Earth's orbit noticeably.
Crater Dimensions:
What does this mean?
Crater shape is normal in spite of atmospheric crushing; fragments are not significantly dispersed.
Transient Crater Diameter: 5.39 km = 3.35 miles
Transient Crater Depth: 1.91 km = 1.18 miles
Final Crater Diameter: 6.75 km = 4.19 miles
Final Crater Depth: 0.526 km = 0.327 miles
The crater formed is a complex crater.
The volume of the target melted or vaporized is 0.0931 km3 = 0.0223 miles3
Roughly half the melt remains in the crater , where its average thickness is 4.08 meters = 13.4 feet
Thermal Radiation:
What does this mean?
Time for maximum radiation: 0.274 seconds after impact
Visible fireball radius: 4.4 km = 2.73 miles
The fireball appears 12.4 times larger than the sun
Thermal Exposure: 9.46 x 105 Joules/m2
Duration of Irradiation: 63.8 seconds
Radiant flux (relative to the sun): 14.8
Effects of Thermal Radiation:
Much of the body suffers first degree burns
Seismic Effects:
What does this mean?
The major seismic shaking will arrive at approximately 16.1 seconds.
Richter Scale Magnitude: 7.0
Mercalli Scale Intensity at a distance of 80.5 km:
VI. Felt by all, many frightened. Some heavy furniture moved; a few instances of fallen plaster. Damage slight.
VII. Damage negligible in buildings of good design and construction; slight to moderate in well-built ordinary structures; considerable damage in poorly built or badly designed structures; some chimneys broken.
Ejecta:
What does this mean?
The ejecta will arrive approximately 129 seconds after the impact.
Average Ejecta Thickness: 1.45 cm = 0.569 inches
Mean Fragment Diameter: 7.48 cm = 2.95 inches
Air Blast:
What does this mean?
The air blast will arrive at approximately 244 seconds.
Peak Overpressure: 24400 Pa = 0.244 bars = 3.47 psi
Max wind velocity: 52.4 m/s = 117 mph
Sound Intensity: 88 dB (Loud as heavy traffic)
Damage Description:
Interior partitions of wood frame buildings will be blown down. Roof will be severely damaged.
Glass windows will shatter.
About 30 percent of trees blown down; remainder have some branches and leaves blown off.
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.