- Joined
- Nov 2, 2006
- Messages
- 55
- Reaction score
- 0
I am having a hard time w/this problem.
Info:
-The repulsive forces between two small nuclei is called the Coulomb barrier. The height of the Coulomb barrier is about 400 keV.
-Temperature in thermonuclear studies are reported in terms of the most probable kinetic energy K of the interacting particles via the relation: K = kT. Where k is Boltzmann constant (8.62X10^-5eV/K) and T is the temperature in Kelvins.
-1.3 keV is the temperature at the core of the sun.
-An electron carries a charge of 1.6 X 10^-19C.
Question:
What is the approximate temperature of the sun's core in kelvins?
Answer:
1.5 X 10^7 K
I don't get how to get this answer😕
Info:
-The repulsive forces between two small nuclei is called the Coulomb barrier. The height of the Coulomb barrier is about 400 keV.
-Temperature in thermonuclear studies are reported in terms of the most probable kinetic energy K of the interacting particles via the relation: K = kT. Where k is Boltzmann constant (8.62X10^-5eV/K) and T is the temperature in Kelvins.
-1.3 keV is the temperature at the core of the sun.
-An electron carries a charge of 1.6 X 10^-19C.
Question:
What is the approximate temperature of the sun's core in kelvins?
Answer:
1.5 X 10^7 K
I don't get how to get this answer😕