Where Did I Go Wrong in Calculating the Kinetic Energy of an Asteroid Impact?

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Discussion Overview

The discussion revolves around calculating the kinetic energy of an asteroid impact and comparing it to the kinetic energy of a hypothetical impact by the space shuttle. Participants explore relativistic effects and the mathematical challenges involved in the calculations.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant attempts to calculate the speed at which the space shuttle would need to impact Earth to match the kinetic energy of the asteroid that killed the dinosaurs, initially using relativistic kinetic energy equations.
  • Some participants point out potential errors in the mathematical steps, particularly regarding the manipulation of equations and the treatment of constants like the speed of light.
  • There is a discussion about the implications of atmospheric re-entry for the shuttle, with some noting that it would likely disintegrate at high speeds.
  • Another participant suggests that the calculations lead to an imaginary result, indicating a possible sign error in the equations used.
  • Further contributions explore the theoretical nature of the scenario, emphasizing that it assumes perfect conditions without atmospheric interference.
  • Participants also discuss the implications of the energy involved, comparing it to significant explosive yields and the potential effects on the biosphere.

Areas of Agreement / Disagreement

Participants express differing views on the mathematical approach and the implications of the calculations. There is no consensus on the correct method or the implications of the results, with ongoing debate about the errors and assumptions made.

Contextual Notes

Some participants highlight limitations in the calculations, such as the treatment of constants and the assumptions made about the conditions of the impact scenario. The discussion remains focused on theoretical considerations without resolving the mathematical uncertainties.

Who May Find This Useful

This discussion may be of interest to those studying relativistic physics, mathematical modeling of impacts, or the effects of high-energy events on planetary environments.

newjerseyrunner
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I want to know how fast the space shuttle would have to hit the Earth to unleash the same kinetic energy as the asteroid that killed the dinosaurs. I've already determined that it's relativistic, by showing that Newtonian physics gives a v greater than c
4.2e25J = (2e6 * v ^ 2 ) / 2.
8.4e25J = 2e6 * v ^ 2
v = sqrt(8.4e25J / 2e6)
v = 6,480,740,698 m/s
But once I plug in the equations, I get a wrong result.

KE = (m * c ^ 2) / sqrt(1 - (v ^ 2 / c ^ 2))
KE / (m * c ^ 2) = sqrt(1 - (v ^ 2 / c ^ 2))
((KE / (m * c ^ 2)) ^ 2) - 1 = -(v ^ 2 / c ^ 2)
v = -sqrt((((KE / (m * c ^ 2)) ^ 2) - 1) * c ^ 2)

KE = 4.2e25J
c = 1
m = 2e6kg

v = -sqrt((((4.2e25 / (2e6)) ^ 2) - 1) * 1)
v = -2.1e+19

I'm expecting an answer between 0 and 1, where did I go wrong?
 
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In the first step.
 
newjerseyrunner said:
I want to know how fast the space shuttle would have to hit the Earth to unleash the same kinetic energy as the asteroid that killed the dinosaurs. I've already determined that it's relativistic, by showing that Newtonian physics gives a v greater than c
4.2e25J = (2e6 * v ^ 2 ) / 2.
8.4e25J = 2e6 * v ^ 2
v = sqrt(8.4e25J / 2e6)
v = 6,480,740,698 m/s
But once I plug in the equations, I get a wrong result.

KE = (m * c ^ 2) / sqrt(1 - (v ^ 2 / c ^ 2))
KE / (m * c ^ 2) = sqrt(1 - (v ^ 2 / c ^ 2))
((KE / (m * c ^ 2)) ^ 2) - 1 = -(v ^ 2 / c ^ 2)
v = -sqrt((((KE / (m * c ^ 2)) ^ 2) - 1) * c ^ 2)

KE = 4.2e25J
c = 1
m = 2e6kg

v = -sqrt((((4.2e25 / (2e6)) ^ 2) - 1) * 1)
v = -2.1e+19

I'm expecting an answer between 0 and 1, where did I go wrong?
You mixed nominator and denominator of the quotient on the RHS of your second line.
 
and with setting c = 1
 
fresh_42 said:
You mixed nominator and denominator of the quotient on the RHS of your second line.
Where? I divided both sides of the equation by the term m * c ^ 2? It was in the numerator of the RHS in the 1st line and in the denominator of the LHS on the second line. I'm sure this is going to be one of those things that's stupidly obvious once I see it, but I'm still missing it.
BvU said:
and with setting c = 1
I did? Isn't that the value I'm supposed to use? If I want v as a percentage of c, shouldn't c be 1 exactly?
 
You have ##a = b/c## and proceed with ##a/b = c##
newjerseyrunner said:
Isn't that the value I'm supposed to use?
No: c is 3 x 108 in your system of units.

v/c is usually called ##\beta##. Your numerical value for KE/m has a factor c2 that you can't simply set to 1.
 
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... instead of ##a/b = 1/c##
 
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BvU said:
You have ##a = b/c## and proceed with ##a/b = c##

No: c is 3 x 108 in your system of units.

v/c is usually called ##\beta##. Your numerical value for KE/m has a factor c2 that you can't simply set to 1.
Oh, see, there's the stupid mistake. I need caffeine. I still would have gotten the wrong answer though so thanks pointing out my unit mistake too. :)
 
There's a few other problems to deal with in this scenario: they had big problems with re-entry even at very low velocities. Like most meteorites, your speeding shuttle would evaporate in the first few km of atmosphere -- fortunately.
 
  • #10
I get ##\beta = {465\over 466}## and worry about fuel prices (but only for a short time).

[edit] Missed ! see #14 below
 
Last edited:
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  • #11
I'm still getting something very wrong.

Relativistic Kinetic Energy
KE = (m * c ^ 2) / sqrt(1 - (v ^ 2 / c ^ 2))

Divide both sides by m * c ^ 2
(m * c ^ 2) / KE = sqrt(1 - (v ^ 2 / c ^ 2))

Square both sides
((m * c ^ 2) / KE)^2 = 1 - (v ^ 2 / c ^ 2)

Replace the subtraction by addition of a negative
((m * c ^ 2) / KE)^2 = 1 + -(v ^ 2 / c ^ 2)

Subtract 1 from both sides
((m * c ^ 2) / KE)^2 - 1 = -(v ^ 2 / c ^ 2)

Simplify the negative
((m * c ^ 2) / KE)^2 - 1 = -v ^ 2 / c ^ 2

Multiply both sides by c ^ 2
(((m * c ^ 2) / KE)^2 - 1) * c ^ 2 = -v ^ 2

Take the square root of both sides
sqrt((((m * c ^ 2) / KE)^2 - 1) * c ^ 2) = -v

Multiple both sides by -1
v = -sqrt((((m * c ^ 2) / KE)^2 - 1) * c ^ 2)

Input known values
v = -sqrt((((2e6 * 3e5 ^ 2) / 4.2e25)^2 - 1) * 3e5 ^ 2)

Solve
v = -300000 i
 
  • #12
BvU said:
There's a few other problems to deal with in this scenario: they had big problems with re-entry even at very low velocities. Like most meteorites, your speeding shuttle would evaporate in the first few km of atmosphere -- fortunately.
Agreed, this is purely theoretical assuming perfect conditions. No atmosphere.
 
  • #13
I think you still have a sign error which gives you the imaginary solution. ##\sqrt{-v^2} = vi \neq -v##.
 
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  • #14
Yes, and this is a not-so-smart way to find something close to 300000.

You have ##\displaystyle {\rm{E} \over \ mc^2} = 233 = \gamma = {1\over \sqrt{1-\beta^2}} \ ##, so clearly ##\beta\approx 1## and you can write

##1-\beta^2 = (1+\beta) (1-\beta) = 2(1-\beta)##

and now I have to correct meself (post #10):$$
1-\beta ={\textstyle {1\over 2} } {1\over 233^2} \ \Rightarrow \ \beta = 1 - {1\over 108889} = {108888\over 108889} \ \Rightarrow v = 0.999991\ {\rm c} $$
 
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  • #15
BvU said:
There's a few other problems to deal with in this scenario: they had big problems with re-entry even at very low velocities. Like most meteorites, your speeding shuttle would evaporate in the first few km of atmosphere -- fortunately.
newjerseyrunner said:
Agreed, this is purely theoretical assuming perfect conditions. No atmosphere.
##v \approx c##, and ##c \approx 3 \times 10^8 m/s##, so if the atmosphere is 100km thick, the shuttle will take approximately 0.3 milliseconds to traverse it. Will the spaceship evaporate in that period? Does it matter? You're still depositing a mole of joules into the system.

Edit: Of some relevance.
 
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  • #16
BvU said:
Yes, and this is a not-so-smart way to find something close to 300000.

You have ##\displaystyle {\rm{E} \over \ mc^2} = 233 = \gamma = {1\over \sqrt{1-\beta^2}} \ ##, so clearly ##\beta\approx 1## and you can write

##1-\beta^2 = (1+\beta) (1-\beta) = 2(1-\beta)##

and now I have to correct meself (post #10):$$
1-\beta ={\textstyle {1\over 2} } {1\over 233^2} \ \Rightarrow \ \beta = 1 - {1\over 108889} = {108888\over 108889} \ \Rightarrow v = 0.999991\ {\rm c} $$
Awesome, that's the exact same answer I got when I put in 299792458 instead of 3e5, just with an i in it. I'm sure I'd find the mistake if I looked, but I don't really care if my mistake only changes the imaginary factor. Thanks for the simplification too.
 
  • #17
TeethWhitener said:
##v \approx c##, and ##c \approx 3 \times 10^8 m/s##, so if the atmosphere is 100km thick, the shuttle will take approximately 0.3 milliseconds to traverse it. Will the spaceship evaporate in that period? Does it matter? You're still depositing a mole of joules into the system.

Edit: Of some relevance.
I was thinking that too. I doesn't really make a difference, you're still adding the amount of energy that killed the dinosaurs into the system. It'd go off like a bomb and obliterate the biosphere no matter where something with that much power exploded.
 
  • #18
TeethWhitener said:
##v \approx c##, and ##c \approx 3 \times 10^8 m/s##, so if the atmosphere is 100km thick, the shuttle will take approximately 0.3 milliseconds to traverse it. Will the spaceship evaporate in that period? Does it matter? You're still depositing a mole of joules into the system.
Granted. I got stuck in the immediate vicinity of the actual speeds of descent and forget to 'think' relativistically.
Does it matter ? No. There's no way you can get this kind of energy in a 2000 metric ton vehicle. Think of it: the energy equivalent of 470 kilotonne of matter ...

But it sure is fun as a thought experiment... and to bicker about :smile:
 

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