Rotational Kinetic Energy of Planet

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SUMMARY

The discussion focuses on calculating the rotational kinetic energy of a planet modeled as a uniform sphere with a radius of 6420 km and a mass of 5.59x10^24 kg. The first part confirms the rotational energy as 2.44x10^29 J, while the second part addresses the decrease in kinetic energy due to tidal friction, resulting in a change of -2.32x10^17 J/day. The key equations utilized include KE = 1/2Iω^2, I = 2/5MR^2, and ω = 2π/T. The solution emphasizes the importance of consistent unit conversion for accurate results.

PREREQUISITES
  • Understanding of rotational kinetic energy calculations
  • Familiarity with the moment of inertia for a uniform sphere
  • Knowledge of angular velocity and its relationship to rotational period
  • Proficiency in unit conversion and dimensional analysis
NEXT STEPS
  • Study the effects of tidal friction on planetary rotation
  • Learn about the conservation of angular momentum in celestial mechanics
  • Explore advanced rotational dynamics and energy loss mechanisms
  • Investigate the implications of changing rotational periods on planetary climates
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Students in physics, particularly those studying mechanics and celestial dynamics, as well as educators looking for practical examples of rotational energy calculations.

rrfergus
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Homework Statement


This question has two parts; the first part I understand but the second part I do not.
Part 1: What is the rotational energy of a planet about its spin axis? Model the planet as a uniform sphere of radius 6420 km, and mass 5.59x10^24 kg. Assume it has a rotational period of 24.0 h. The answer to this is 2.44x10^29J. I understand this part.
Part 2: Suppose the rotational kinetic energy of the planet is decreasing steadily because of tidal friction. Assuming the rotational period increases 15.0 μs each year, find the change in one day. (Let 1 yr = 365 d.). The answer to this is -2.32x10^17 J/day, but I do not understand how to get it. Thank you! :)

Homework Equations


KE = 1/2Iω^2
I = 2/5MR^2
ω = 2π/T (T is period)

The Attempt at a Solution


If T increases by 15μs each year, then at the end of 1 year the period will be 24h(3600s/h) + 15x10^-6s. So, I use that to find the rotational kinetic energy of the planet at the end of the year and I get 2.4369x10^29J. Then, I subtract the original rotational kinetic energy (the answer from part 1) and divide the result by 365 (since there are 365 days/year). The result is about -8.39x10^23J/day, which is way off from the correct answer.
 
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Make sure your units are consistent between problems. I recommend converting everything into units of days when determining the kinetic energy. Simply diving by 365 in the very end may not give you what you're looking for, try calculating \Delta E = \frac{1}{2}I(\omega_2^2-\omega_1^2) after your units of \omega are consistent. It's likely the error was made with unit conversion.

Once all your units are for a single day, you won't need to divide by anything in the end. Your answer will be the change in energy from one day to the next, so it would be equivalent to Joules/Day
 
Great! I got the right answer! Thank you so much!
 

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