Comet Crashes in Earth Conservation of Energy

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SUMMARY

The forum discussion centers on calculating the total energy converted to thermal energy when a comet, with a mass of 4.80E+12 kg and a radius of 385 m, impacts Earth. The comet travels at an initial speed of 19 km/s and slows to 10.1 km/s before impact. Key equations used include gravitational potential energy, translational kinetic energy, and rotational kinetic energy, with constants such as G = 6.673E-11 N m²/kg² and the mass of Earth at 5.976E+24 kg. The user struggles to derive the correct thermal energy value despite using the appropriate equations and constants.

PREREQUISITES
  • Understanding of gravitational potential energy and kinetic energy equations
  • Familiarity with the moment of inertia for a solid sphere
  • Knowledge of angular velocity and its relationship to rotational motion
  • Basic principles of energy conservation in physics
NEXT STEPS
  • Calculate gravitational potential energy using the formula: deltU(g) = -G*mE*mC/r
  • Determine the change in translational kinetic energy: deltK(trans) = 1/2*mC*v(f)² - 1/2*mC*v(i)²
  • Evaluate the change in rotational kinetic energy: deltK(rot) = 1/2*I*omega(f)² - 1/2*I*omega(i)²
  • Explore the implications of energy conversion during atmospheric entry for celestial bodies
USEFUL FOR

Students and educators in physics, particularly those focusing on energy conservation, celestial mechanics, and impact dynamics. This discussion is also beneficial for anyone studying the effects of large-scale impacts on planetary bodies.

kchurchi
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Homework Statement



A comet is traveling towards the earth. The comet has a mass of 4.80E+12 kg and a radius of 385 m. The comet is traveling with a speed of 19 km/s and spinning with a period of 0.12 seconds when its center is a distance 1.88E+7 m away from the center of the earth. The comet is roughly spherical, so its moment of inertia will be that of a uniform, solid sphere. Just before the comet strikes the surface of the earth, its speed is 10.1 km/s, and its rotation is essentially zero. Use the following values for constants
G = 6.673E-11 N m2/kg2
mass of Earth = 5.976E+24 kg
radius of Earth = 6.378E+6 m


A lot of energy is converted to thermal energy as the comet travels through the atmosphere. Using the information above, determine the total amount of energy converted to thermal energy.


Homework Equations


W(tot) = deltE(sys)
deltU(g) = -G*mE*mC/r(f) + G*mE*mC/r(i)
deltK(translational) = 1/2*mC*v(f)^2 - 1/2*mC*v(i)^2
deltK(rot) = 1/2*I*omega(f)^2 - 1/2*I*omega(i)^2
I = I(sphere)

The Attempt at a Solution


I have the right equation, several TA's have already checked it. But for some reason I cannot get the right answer. I solved for the change in thermal energy by taking the system to be everything so work is 0. Then I said the energy of the system is equal to the potential energy of gravity + the kinetic energy of rotation + the kinetic energy of translation + thermal energy. I just brought all terms except thermal energy to the other side and solved. What am I doing wrong?

Equation:
deltE(therm) = -deltU(g) - deltK(rot) - deltK(trans)
deltE(therm) = -(-G*mE*mC/(rE+rC) + G*mE*mC/r(i)) -(1/2*I*omega(f)^2 - 1/2*I*w(i)^2) - (1/2*mC*v(f)^2 - 1/2*mC*v(i)^2)

v(i), v(f), mE, mC, rE, rC, r(i), G, period (T), and I are given
I(sphere)= 2/5*(mC/(rC^2))
omega(f) = 0
omega(i) = 2*pi/T
 
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Do you have individual values for deltU(g), deltK(rot), deltK(trans)? What is your final result, what is the correct result?
The equations look fine.

The comet has twice the density of lead, but well...
 

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