MadSci Network: Astronomy |
emilio, If the Earth had no atmosphere, the answer would be pretty simple. Simply consider that the Earth has a potential well of the form U=-GMm/r where G is Newton's gravitational constant, M is the mass of Earth, m is the mass of your object, and r is the distance from the Earth's center. Assume that the object starts with no net energy. By conservation of energy, the object's kinetic energy (1/2*m*v^2) plus its gravitational potential energy must always be zero. 1/2mv^2-GMm/r=0 which through a little bit of algebra yields a velocity of v=sqrt(2*G*M/r) (independent of the mass of the object) Now, plug in the radius fo the Earth for r, and we get a value of 11,173 m/s as the impact velocity. However, as you rightly noted, there is air resistance to consider. Let's first assume that as the object enters the atmosphere, it is moving close to 11,000 m/s. Let's use the formula for the air friction force for fast moving objects: F=(1/2)*C*rho*A*v^2 Here, rho is the density of air, A is the cross-sectional area of the meteorite, v is the velocity, and C is a factor dependent on the geometry of the object. Spherical objects have a value of C of .5, so I will use .7 due to the irregular shape of a typical meteorite. Terminal velocity occurs when the friction force balances the gravitational force downward. 1/2*c*rho*A*v^2 = m*g Here, we neglect the ablation of the meteorite, that is, the blasting off of particles from the surface due to collision with air molecules. For objects of this size range, that is a significant effect. Let's just assume that, to first order, we can do this calculation anyway. I ran a few calculations for a baseball-sized meteorite (r=3.6 cm). I simply used Newton's second law: m(dv/dt)=1/2*C*rho*A*v^2-m*g (This was done numerically, though it would not be difficult to solve the equation exactly if you so desired.) If you have a baseball-sized meteorite of density 3.2 g/cc, using a value of 1.2 kg/m^3 for the density of air, you will find that the meteorite will slow from its approach velocity of roughly 11000 meters per second to its terminal velocity of 60 m/s in a mere 28 seconds, having traveled only 3 km. (By comparison, the speed of sound is roughly 315 m/s.) It then spends another 100 mins or so falling before it hits the ground, giving it ample time to cool down below its original temperature it gained during entry into the atmosphere. (At 60 m/s, it's moving like a fastball, but not much more. It'll still cause a lot of damage if your car or house is in the way, but it wouldn't start a fire or create any appreciable crater. It would probably be a bit warm to the touch. ---Bob Macke MIT S.B. '96, Physics in St. Louis Ph.D. candidate, Physics References: Serway, "Physics for Scientists and Engineers," Saunders College Pub., Philadelphia, 1990, p. 139. (Explanation of air resistance)
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