Assessment of the likelihood of Being in a Dome that is Struck by a Meteorite.

Introduction

As the planers of a community we must evaluate possible sources of danger so we can prepare against them. A community on mars is closer to the asteroid belt and has less atmosphere. Consequently the risk of an asteroid puncturing a surface structure is greater.

The most common meteorites come from the dust in the tail of a comment. These meteorites are typically the size of a grain of sand. Since mars has a limited atmosphere it should provide adequate protection against these shower meteorites.

The other type of meteorites are called sporadic meteorites. These are the meteorites that arrive randomly. On average these meteorites hit the earths atmosphere at a rate of 8-10 per hour. One source of these meteorites is collisions between asteroids. The goal of this paper is to gain incite into the constraints (if any) that the frequency these meteorites hits the Martian surface imposes on the design of a Martian community..

Assumptions

To begin our analysis we assume: With the above assumptions the probability of n meteorite hits is given by a Poisson distribution.
(1)

n The number of occurrences
lambda The average number of occurrences.
P(x; lambda) The potability of n occurrences for a given lambda.

And Lambda is given by:
 
(2)

r The average rate meteorites hit the atmosphere of mars.
f The fraction of the meteorites that hit the atmosphere of mars that make it to the surface
Am The surface area of mars
At The area of the place on the surface we wish to know the probability of a given number of meteorite hits.
t The time interval of interest

Evaluating The Risk

For some incite we may choose the following values.
t 80 years (The average age of a human) 
24*365.2422= 701265 hours
At 31416 m2 (The area of a dome with a radius of 100 m. People will not likely be in domes much bigger)
r 10 per hour (This is the average rate at which meteorites hit the atmosphere of earth).
f 0.01 A wild guess but I wouldn't expect more then 1% of the meteorites to make it through the Martian atmosphere.
Am 1.447*1014 m2 pi*d^2=pi*(6787000) m2

For these numbers we obtain lambda=1.218*10-5

With this lambda the probability of a meteorite hitting a dome with a 100 meter radius in an 80 year period is 0.001%. Table 1 gives the probability of n occurrences for a given value of lambda. The reader is free to choose his own numbers to calculate what he/she feels is a more reasonable number.

Table. 1 The probability (%) of n Occurrences for a given value of Lambda.
Number of Occurrences Lambda
10-03 10-04 10-05 10-06 10-07
0  99.9  99.99  99.999  99.9999  99.99999 
1  9.99*10-02  9.999*10-03  1*10-03  1*10-04  1*10-05 
2  4.995*10-05  5*10-07  5*10-19  5*10-13  5*10-15 
3  1.665*10-8  1.667*10-11  1.667*10-14  1.667*10-17  1.667*10-20 

Conclusion

Assuming:- the rate meteorites hit the Martian Surface is comparable to that of earth, a person spends 80 years in a 100m dome and 1% of the Meteorites that hit the Martian atmosphere make it to the surface: the likelihood that person will be in a dome that is struck by a meteorite is0.001%.Most people will not:- live for 80 years. They will also not spend most of their time in large unprotected structures. As a consequence they are unlikely to be in a structure that is breached by a meteorite. Even if we were to assume that all of the meteorites made it through to the Martian surface a 100 m in radius dome still only have likely hood of 0.1% of being struck in an 80 year period. The likelihood of multiple strikes in an 80 year period approaches zero. We should expect that domes will be practical to build and on average should last some time without rupture from a meteorite. The safety of people can be addressed by ensuring if a rupture occurs that suitable time will be given for people to evacuate.
 
 
 
 
 
 
 
 
 
 
 
 
 
 
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