maximus
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exactly how gravity in a star can generate temperatures high enough for thermonuclear reactions? i need a straight answer this time.
This discussion centers on the mechanisms by which gravity generates the extreme temperatures necessary for thermonuclear reactions in stars. Key points include that gravitational forces compress hydrogen atoms, overcoming electronic repulsion and allowing nuclear fusion to occur. The process begins with gravitational collapse, which increases kinetic energy and temperature, ultimately leading to fusion at temperatures around 10 million Kelvin. The conversation highlights that pressure is a result of gravitational forces, not the initiator of nuclear reactions, and emphasizes the role of gravitational potential energy in heating.
PREREQUISITESAstronomers, astrophysicists, students of physics, and anyone interested in the processes governing star formation and thermonuclear reactions.
Originally posted by Integral
If the mass is great enough the force of gravity is sufficient to over come the electronic forces which sperate atoms. When this happens the nucleons are crushed close enough together to allow nuclear reactions to occur.
Originally posted by maximus
exactly how gravity in a star can generate temperatures high enough for thermonuclear reactions? i need a straight answer this time.
Originally posted by chroot
The gravitational potential energy is transferred into translational kinetic energy of the falling particles. Another name for 'translational kinetic energy' of microscopic particles is 'heat.'
If you drop a bowling ball, it gains kinetic energy as it falls. As the hydrogen atoms fall in towards a protostar, they also gain kinetic energy.
- Warren
Originally posted by Alexander
Exactly. It is not pressure, but change of position (protons come closer) in mutual attraction force (gravity) which makes protons move faster. Make Earth and ball come closer, and both will move faster (=gain "temperature").
Originally posted by Alexander
Well, what we call pressure is just a change of momentum of moving particles in collisions with each other, with walls of a container (if any) and with the device measuring pressure (pressure gauge, barometer, etc). What we call temperature is average kinetic energy per particle. So, still these are different (though closely related as momentum and energy are closely related) concepts.
That is how you can use 1/r-1/2 as the calculator for the Earths increasing internal gravitational ability, with respect to it's pressurization, and it thermal energy output(s).
Originally posted by FZ+
Actually, Mr. Parsons, there is an error in your maths.
1/r-0.5 == (r-0.5)-1
== r0.5, which is the square root of r.
Originally stated at the Cal Tech site
The possibility that electromagnetic zero-point energy may be involved in the production of inertial and gravitational forces opens the possibility that both inertia and gravitation might someday be controlled and manipulated. This could have a profound impact on propulsion and space travel.