Energy Conservation: Solving the 670kg Meteorite Problem

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Homework Help Overview

The discussion centers around a problem involving energy conservation related to a meteorite composed of aluminum that crashes into Earth. The meteorite has a mass of 670 kg, an initial temperature of -15°C, and a speed of 14 km/s. Participants are tasked with determining the final temperature of the meteorite after the impact, considering the sharing of internal energy between the meteor and the planet.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants discuss the need to apply kinetic and potential energy concepts, questioning how to set up the initial and final energy equations. Some seek clarification on the sharing of energy between the meteor and Earth, while others express confusion about the conversion of gravitational potential energy to heat.

Discussion Status

The discussion is ongoing, with participants exploring various interpretations of the energy conservation principles involved. Some guidance has been offered regarding the application of energy equations, but there is no explicit consensus on the setup of the problem or the assumptions being made.

Contextual Notes

Participants note the importance of considering gravitational potential energy in the context of the meteor's fall and its conversion to thermal energy upon impact. There is a mention of homework constraints and the challenge of understanding the energy sharing aspect of the problem.

thenewbosco
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Energy Conservation Question

here is a problem i need help getting started on:

A 670kg meteorite composed of aluminum far from the Earth has a temperature of -15C and moves with a speed of 14km/s relative to earth.
As it crashes, assume that the resulting additional internal energy is shared equally between the meteor and the planet and that all of the material of the meteor rises to the same final temperature. Find this temperature.

assume that the specific heat of liquid and gaseous aluminum is 1170 J/kg*C.

No idea how to begin this although i am reminded not to forget about gravitational potential energy,
thanks for some help on this one
 
Last edited:
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no help on this...
 
E = KE + PE
 
right i know this is to be used but i don't know how to set up the initial and final energies. and also the wording about the energy being equally shared.

can i get some more clarification on how to set these equations up.
thanks
 
i really need some help with this one...
 
no one can help ??
 
thenewbosco said:
As it crashes, assume that the resulting additional internal energy is shared equally between the meteor and the planet and that all of the material of the meteor rises to the same final temperature.
What's the KE of the meteor when it hits earth? (It falls from "infinitely" far away to the surface of the earth. What's the change in gravitational PE?)

Assume half of that energy remains in the meteor. You have the specific heat and the mass of the meteor; calculate the temperature change.
 
Remember that initial energy is equal to final energy by the law of conservation of energy and that change in K+ change in U+change in Q = 0 as well, where U is potential energy, Q is thermal energy and K is kinetic energy.

Hope that helps some :P
 
Could someone please explain why the meteor's gravitational potential energy is converted to heat after the collision? I understand why the meteor's kinetic energy is converted to heat; after all, it's moving very quickly and then stops. That kinetic energy must go somewhere! But why is there any change in the meteor's gravitational potential energy from right before to right after the meteor strikes the Earth?
 
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