China successfully warned of asteroid impact, so far no impact on Earth, what happens next depends on the latest news
Sadly, it is like a terrorist trying to sneak a bomb onto a plane - we have to be observant and be successful 100% of the time, the terrorist, in this case asteroids, only have to be successful once by sneaking by us to be potentially catastrophic.
If we take a 100m nickel-iron asteroid lets look at details and damage.
- Object - 100m
- Density - 8000kg/m3
- Velocity at atemospheric entry - 25km/s
- Impact angle to surface - 45°
- Distance from impact - 10km
Now lets look at the effects
- Energy before atmospheric entry: 1.31x 10E18 Joules (3.13 x10E2 Megatons TNT)
- The average interval between impacts of this size somewhere on Earth during the last 4 billion years is approximately estimate to be 15,000 years, however, on the Moon these appear to occur at a rate of about every 500 years, which does indicate our crater rates for Earth are wrong.
- The projectile begins to break up at an altitude of 20.4 km (12.6 miles).
- The projectile reaches the ground in a broken condition. The mass of projectile strikes the surface at a velocity of 23.2 km/s (14.4 miles/s).
- The energy lost in the atmosphere is 1.86x 10E17 Joules (4.44 Megatons TNT).
- The impact energy is 1.12x 10E18 Joules (268 Megatons TNT).
- The broken projectile fragments strike the ground in an ellipse of dimension 391 m (1282 ft) by 276 m (906.3 ft).
- Crater shape is normal in spite of atmospheric crushing; fragments are not significantly dispersed.
- Transient CraterDiameter: 2.79 km (1.73 miles)
- Transient Crater Depth: 986 m (3236 ft)
- Final CraterDiameter: 3.21 km (1.99 miles)
- Final Crater Depth: 420 m (1379 ft)
- The crater formed is a complex crater.
- The volume of the target melted or vaporized is 0.00707 km3 (0.00170 miles3).
- Roughly half the melt remains in the crater.
- Time for maximum radiation: 89.8 millisecondsafter impact
- Visible fireball radius: 2.07 km (1.29 miles)
- The fireball appears 47.1 times larger than the sun
- Thermal Exposure: 5.34 x 106 Joules/m2
- Duration of Irradiation: 27.0 seconds
- Radiant flux (relative to the sun): 198
- Effects of Thermal Radiation:
- Clothing ignites
- Much of the body suffers third degree burns
- Newspaper ignites
- Plywood flames
- Deciduous trees ignite
- Grass ignites
- The major seismic shaking will arrive approximately 2 secondsafter impact.
- Richter Scale Magnitude: 6.2
- Mercalli Scale Intensity at a distance of 10 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.
- The ejecta will arrive approximately 45.2 seconds after the impact.
- At 10km there is a fine dusting of ejecta with occasional larger fragments.
- Average Ejecta Thickness: 54.1 cm (21.3 inches)
- Mean Fragment Diameter: 8.74 m (28.66 ft)
- The air blast will arrive approximately 30.3 seconds after impact.
- Peak Overpressure: 273000 Pa = 2.73 bars = 38.7 psi
- Max wind velocity: 352 m/s (1154 ft/s)
- Sound Intensity: 109 dB (may cause ear pain)
- Damage Description: (at 10km)
- Multistory wall-bearing 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.
If such an impact landed occured on a major city, the death toll would be multiple millions. Even landing outside a city but within 10km, the death toll would still be around 250,000 plus.