Program 12: How Planets form around the Sun
Introduction and Purpose
The purpose of this program is to simulate how planets are formed around the Sun.
Planets are created from grains with mass 1.
For simple operation:
A shape of 0 will generate highly elliptical objects.
After some time: Select 2 and C
- After Start # of objects, Enter 100
- After End # of objects, Enter 100
- After Shape, Enter 100
- After Mass Correction, Enter 100
The display shows:
When ever two objects collide the one with mass 2 will be shown.
- The Sun in the center.
- At the bottom of the screen all the objects with the masses >= 2
- At the top: Display limit value, Revolution counter and three values i, j and distance.
Distance is the minimum value between the objects i and j. There is a collision when this value becomes less than 2.
In order to see all the objects: Select 1
In order to see the objects with mass => 2 : Select 2
In order to see the objects with mass => 9 : Select 9
In order to clear the screen : Select C
In order to terminate the simulation : Select E
Program: SOLAR.BAS source
In order to retrieve the source select:SOLAR.BAS
To see the program listing select:SOLAR.HTM
The whole simulation is based on Newton's Law.
The mass of the Sun is 1000. The mass of each object is 1 divided by the mass correction factor.
If an object is ejected a new one will be created.
If two objects collide a new one will be created.
For further reading
Last modified: 12 March 1998
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