Question about energy (explosions)

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SUMMARY

The discussion focuses on calculating the energy required to destroy an object at a specific distance from an explosion, using the example of a supernova and Earth located 10 AU away. The key concept is the inverse-square law, which states that energy spreads uniformly over the surface of a sphere, affecting the intensity of energy per square meter at varying distances. The calculation involves determining the energy density at the distance of interest and confirming that the inverse-square law applies to the scenario. The participants clarify that the energy needed to destroy the planet is 2×10^32 joules.

PREREQUISITES
  • Understanding of basic physics concepts, particularly energy and explosions
  • Familiarity with the inverse-square law in physics
  • Knowledge of energy units, specifically joules
  • Basic grasp of spherical geometry and surface area calculations
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  • Study the inverse-square law in detail and its applications in physics
  • Learn about energy dispersion in explosions and related calculations
  • Explore the concept of supernovae and their energy outputs
  • Investigate the effects of distance on energy intensity and damage potential
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Physics students, educators, and anyone interested in understanding the principles of energy distribution in explosive events, particularly in astrophysics contexts.

nicholas0211510
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I'm new to physics I tried doing some research but I can't seem to fully grasp the concept.
My question is, how would one find how much energy is needed to destroy a object a select distence away from the blast

For example if a star when super nova and had a x amount of joules, and let's say a planet was 10 AU away, and that planet was Earth and the energy needed to destroy it was 2×10^32 joules

How would you calculate the intensity of the intial explosion to be able to still destroy the planet at that distance?

I believe it was square inversed law but I'm not sure could someone help me out?
 
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Hi nicholas0211510. :welcome:

If the energy spreads out uniformly in all directions, then imagine a sphere totally enclosing the exploding body. At whatever distance out from the centre of the exploding body you choose to draw the enclosing sphere, all that liberated energy will be spread over the surface of the sphere and you can calculate a Joules/m2 figure for that radius out. Do this calculation for whatever distance away the planet is located, and see whether you can figure out the remaining step.
 
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Thank you, I didn't imagin it would be as simple as that
 
I figured you would need to find a lot of variables like I was reading about the square inversed law, but i guess that formula does not associate with the topic at all?
 
nicholas0211510 said:
I figured you would need to find a lot of variables like I was reading about the square inversed law, but i guess that formula does not associate with the topic at all?
The inverse-square law certainly does apply: if you double the radius of the enclosing sphere, the Joules/m2 changes by a factor of 1/4.
 
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I see, I appreciate the help
 

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