Nature of e=mc^2 and other miscelaneous questions

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The energy equivalent of 1 kg of matter is approximately 9 x 10^16 joules, based on Einstein's mass-energy equivalence principle. In fusion reactions, a small fraction of the mass, such as heavy hydrogen, is converted to energy, with deuterium-tritium fusion yielding about 17.6 MeV. The discussion also speculates on the potential for a crash of the Galileo orbiter into Jupiter to create enough pressure to trigger fusion in the planet's atmosphere, although this remains theoretical. Additionally, questions arise about the energy required to heat hydrogen isotopes to the necessary temperatures for fusion and the density variations of objects under gravitational compression. Overall, the conversation blends theoretical physics with speculative scenarios regarding fusion and energy dynamics in celestial bodies.
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If you have 1 kg of matter, what is the energy equivalent of it in say joules?

How much of the matter (heavy hidrogen?) that goes into a fusion reaction is transformed to energy?


And to the point...

Last year there was this discussion about what would happened if the Galileo orbiter would crash into Jupiter. More precisely, there were some (I don't know if actual physicists) that hinted that the uranium present on board of the craft (from the reactor powering it) would explode with enough power to trigger a fusion reaction within the Jupiter lower atmosphere.

Now, theoretically speaking, is it possible for an explosion within Jupiter (or what should Jupiter be like) to create a powerful enough pressure shock front, to trigger the fusion of the hydrogen atoms in it's path, and if it's possible to create a chain reaction this way...
 
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For the last question,well i don't know,it may be pure speculation,though...For the first,approximately 9\cdot 10^{16}J,as for the second,well,look for the reaction in a book,then for the rest masses of proton (H nucleus) and the alpha particle and compute the mass defect.

Daniel.
 
What is the energy required to heat up one H2 and one H3 from a given temperature n (Kelvin), up to 10^9 K (required for fission)?

How does the density of an object bound solely by it's gravitational compression and electron repulsion vary? My guess is that it should be cubic or quadratic-like as we start moving inwards from the surface but aproaching a finite limit as we approach the center of mass. How do you put this into a relation?


So the energy output of a fusion reaction (deuterium-tritium) is 17.6 MeV
The mean density of Jupiter is 1.326 g/cm^3.
 
I think it's easist first to watch a short vidio clip I find these videos very relaxing to watch .. I got to thinking is this being done in the most efficient way? The sand has to be suspended in the water to move it to the outlet ... The faster the water , the more turbulance and the sand stays suspended, so it seems to me the rule of thumb is the hose be aimed towards the outlet at all times .. Many times the workers hit the sand directly which will greatly reduce the water...
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