Simulation of Asteroid/Comet Impacts with Earth
Simulation 1047: One hundred thousand years, looking at worst event each decade.
By Michael Paine 18 Feb 2000This page provide further information about the simulation described in Benny Peiser's AAAS paper.MSNBC: Adding up the risks of cosmic impact: Researchers turn attention to smaller, more frequent blasts (interview with Benny Peiser and David Morrison). See also my Explorezone/Space.com article "SIMULATING ARMAGEDDON ON YOUR PC: ASTEROID IMPACTS WITH EARTH".
If you have a copy of the software check out, and contribute to, the Users Page.
The computer program is available on diskette distributed with the book "Comet and Asteroid Impact Hazards on a Populated Earth" by John S. Lewis, Academic Press. It was released late in 1999. See review.
Due to its random nature, each time the program is run it generates a completely different set of results. As described below, the overwhelming influence of a few horrendous events means that the total number of fatalities can vary considerably between successive runs.
As John Lewis points out in his book, the hazard from small Near Earth Objects (NEOs) has been underestimated in the past because 'average' properties were used in the estimates. His program simulates a mix of asteroid/comet types, speeds and entry angles. The strong iron asteroids are more likely to do damage than the 'average' stony asteroid. Also an object with a shallow entry angle is more likely to slow down without breaking up, and therefore reach a lower altitude where it is more destructive.
Set out below are the results of a total of one hundred thousand years of simulation, looking at the worst event in each of 10,000 decades. I want to stress that these are NOT predictions and that no known NEOs are on a collision course with Earth. There is also a page with the results of a one million year simulation.
The original program uses a tsunami runup factor of 30 (the height of the wave at the shoreline was assumed to be 30 times the height of the wave in deep water). A more conservative runup factor of 5 was used in the simulation.
The program is mainly intended for runs covering a several thousand years. In these time periods impacts massive enough to cause global climatic trauma are extremely rare and the program did not fully account for these effects. Lewis and others suggest an explosion equivalent to one million megatons of TNT would be sufficient to cause over a billion human fatalities, mainly due to global starvation. A typical asteroid about 1 mile across would do the trick. Global climatic effects probably become insignificant for asteroids smaller than 500 yards across, with a typical explosion of 10,000 megatons of TNT (some 200 times larger than an H-bomb). The potential fatalities from these climatic effects have been included in the following fatality estimates.
Asteroid/comet diameter is estimated from mass (randomly generated by the program) and density (derived from the type of object - also randomly generated).
A constant world population of 5 billion people is assumed. It is also assumed that impacts occur without warning (the current situation) and that there is no time for evacuation or preparation, such as stockpiling of food supplies.
The big one!
The largest impact recorded over the 100,000 year run was a stony asteroid 5 kilometres in diameter travelling at 29 kilometres per second. The 23 million megaton explosion produced a crater 60 kilometres across and the resulting climate catastrophe was sufficient to wipe out the human population. Fortunately there is only an estimated 1 in 500 chance of such an event occurring during 100,000 years of simulation. This event was ignored for the current analysis, which was intended to
give an idea of "typical" impacts over a 10,000 year period.Size of asteroid/comet
* Ignoring the 23 million Mt event
Asteroid/ comet diameter
(m)No. of events No. of fatal events % Fatal Average yield of fatal
event
(Mt TNT)Average fatalities per fatal event Annual risk of fatal event 13-99 9792 949 10% 18 43 000 1 in 100 100-199 173 124 72% 300 280 000 1 in 800 200-499 31 29 94% 2000 700 000 1 in 3500 500-999 3 3 100% 35 000 13 million 1 in 30 000 All 9999* 1105 11% 170 120 000 1 in 90
Type of impactor
15% of the fatal events were due to long period comets, 6% were due to short period comets and the remainder were due to asteroids. The proportion of comets was much lower than that with the one million year simulation, over which several catastrophic comet impacts can be expected.Type of impact
Excludes events where the object skipped out of the Earth's atmosphere.
Type of impact No. of events No. of fatal events (%) Average fatalities
per fatal eventAirburst over land 2850 834 (28%) 80 000 Land impact with crater 40 38 (95%) 400 000 Airburst over ocean 6760 120 (2%) 32 (shipping) Ocean impact with tsunami 119 114 (96%) 470 000 Craters
Over the 100,000 year simulation only 40 land craters were produced. 38 of these resulted in fatalities. In other words out of a total of 1105 fatal events only 3% resulted in a land crater. Furthermore, many of these craters would be eroded or buried over a few thousand years. .Land craters are therefore a very poor indicator of the hazard due to comets and asteroids.Note that small craters resulting from the impact of fragments are not counted.
Crater Diameter (km) No. of craters Less than 1 km 9 1 to 1.9km 14 2 to 4.9km 15 5km or more 2 What can be expected in a typical 10,000 years?
Dividing the results of this simulation by 10 will give us an idea of a "typical" 10,000 years. With a constant human population of 5 billion cosmic impacts over 10,000 years can be expected to produce:If there were no reliable human records of the 110 fatal events then the only strong physical evidence for the cause of 13 million fatalities would be 4 impact craters, if they had not been eroded or buried.
- 110 fatal events resulting in a total of 13 million fatalities (an average of 120,000 fatalities per event).
- 300 "Tunguska" style airbursts over land, with 80 of these producing fatalities (roughly 1 fatal event per century).
- 12 ocean impacts that produce tsunami, with an average of 500,000 fatalities per event.
- Just 4 land impacts, with an average of 500,000 fatalities per event.
More stats
Here are some further stats for the 100,000 years in decade steps. There may be some slight disagreements with the values shown in the tables above due to the filters applied.
Key:
RANGE OF NEO DIAMETER
EVENT Count of decades where the worst incident was in the range
DIA_M Mean diameter of impactors
DIA_M Std. Dev. of diameter of impactor
ENGY_MT Mean kinetic energy at entry to atmosphere Mt TNT
CRATER_KM Max crater diameter in km
YIELD_MT Mean explosive yield Mt TNT
BLASTFAT Sum of blast fatalities
FIREFAT Sum of firestorm fatalities
TSUFAT Sum of tsunami fatalities
GLASFAT Sum of glass fatalities (if they survive blast and firestorm)
DUSTFAT# Sum of climate-change fatalities (my addition to program)
TOTFAT# Sum of all fatalitiesNEOS 13 to 49m in DIAMETER (smallest for fatality 14m, most were irons)
EVENT Count 8955 (666 Fatal)
DIA_M Mean 26.44
DIA_M Std. Dev. 7.55
ENGY_MT Mean 2.89
CRATER_KM Max 0
YIELD_MT Mean 2.82
BLASTFAT Sum 220567
FIREFAT Sum 7050187
TSUFAT Sum 43
GLASFAT Sum 2153
DUSTFAT# Sum 0.00
TOTFAT# Sum 7272945
NEOS 50 to 99m in DIAMETER
EVENT Count 837 (317 Fatal)
DIA_M Mean 65.16
DIA_M Std. Dev. 13.05
ENGY_MT Mean 37.48 Mt
CRATER_KM Max 1 (iron)
YIELD_MT Mean 36.42 Mt
BLASTFAT Sum 2619067
FIREFAT Sum 31816799
TSUFAT Sum 186597
GLASFAT Sum 0
DUSTFAT# Sum 0.00
TOTFAT# Sum 34622464
NEOS 100 to 199m DIA
EVENT Count 173 (125 fatal)
DIA_M Mean 132.96
DIA_M Std. Dev. 26.87
ENGY_MT Mean 351.46
CRATER_KM Max 3
YIELD_MT Mean 350.33
BLASTFAT Sum 6648347
FIREFAT Sum 20743470
TSUFAT Sum 7244506
GLASFAT Sum 0
DUSTFAT# Sum 0.00
TOTFAT# Sum 34636322
NEOs 200 to 499m DIA
EVENT Count 31 (29 fatal)
DIA_M Mean 261.35
DIA_M Std. Dev. 45.18
ENGY_MT Mean 2392.14
CRATER_KM Max 7
YIELD_MT Mean 2391.29
BLASTFAT Sum 12081152
FIREFAT Sum 0
TSUFAT Sum 3883049
GLASFAT Sum 0
DUSTFAT# Sum 3298108.00
TOTFAT# Sum 19262310
NEOS 500 to 999m DIA
EVENT Count 3 (all fatal!)
DIA_M Mean 707.67
DIA_M Std. Dev. 206.65
ENGY_MT Mean 22779.13
CRATER_KM Max 9
YIELD_MT Mean 22788.50
BLASTFAT Sum 0
FIREFAT Sum 0
TSUFAT Sum 28884
GLASFAT Sum 0
DUSTFAT# Sum 39072387
TOTFAT# Sum 39101271
ALL AIRBURSTS (FRAGMENTATION OVER LAND)
EVENT Count 2850 (834 fatal)
DIA_M Mean 30.67 (44.6 for fatals, Max 184)
DIA_M Std. Dev. 16.28
ENGY_MT Mean 9.81
CRATER_KM Max 0
YIELD_MT Mean 9.79 (28.3 for fatals)
BLASTFAT Sum 6686741
FIREFAT Sum 59606680
TSUFAT Sum 0
GLASFAT Sum 2140
DUSTFAT# Sum 0.00
TOTFAT# Sum 66295562
References
Lewis J.S. (1999). Comet and Asteroid Impact Hazards on a Populated
Earth. Academic Press, San Diego.Paine M. (1999) 'Asteroid Impacts: the Extra Hazard Due to Tsunami', The
Science of Tsunami Hazards 17-3, 155-166. The Tsunami Society, Hawaii.