| |
| | Planetary Formation: Contents of Simulating the Capture Theory |
 | | If a body is to remain in equilibrium throughout its collapse, it must be capable of contracting at such a rate that it is able to generate the energy lost from radiation, and also enough additional energy to raise the temperature sufficiently to maintain the pressure balance. |
 | | It was concluded that if these were kept constant during the course of a simulation, the rate of collapse of the protoplanet, once it had reached a dynamic equilibrium configuration, was approximately constant, and was proportional to the square of the mass of the protoplanet, as predicted by Equation 5.5. |
 | | However, once dynamic quasi-static equilibrium has set in, the profiles of the protoplanets throughout the rest of the experiment, are similar to those at the end of the experiment. |
| www.droxley.freeserve.co.uk /node12_ct.html (7339 words) |
|