Last edited 9may02 by Darin Pike
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# illiSolarSystem

## Abstract

In this project, illiSkel is extended into several objects. These objects are arranged like a solar system. In the center is the "sun," and the other objects "orbit" around it like planets. The objects are spinning. The user of the program is allowed to "fly" around the arrangement and alter the position and movement of the objects. Also, the user can view the arrangement through the objects and see the coordinate axes of each object.

### Narrative

There are four objects in this project. The torus is the "sun." The cube and tetrahedron orbit the sun as "planets." The teapot orbits the cube as a "moon."

The arrangement is not quite that of a real solar system. The orbits are circular, not elliptical. Also, the objects are allowed to pass through one another. The numbers displayed for orbit speed are values of angular velocity. The actual velocity of an object is the angular velocity multiplied by the radius. The orbiting of the objects was first tried using Euler's Method. However, with this method, the radius of the objects continuously increased. The Gauss-Seidel method was then used, which resulted in a constant radius for each object.

The drawing of the cube and tetrahedron was hard-coded, while a built-in function was used to draw the teapot. These three objects spin about the y-axis. So that the spinning of the cube does not affect the orbit and spin of the teapot, the teapot has additional calls to the orbit and spin functions to compensate for the spinning of the cube.

The user of the program is allowed to view the arrangement of objects through the affine matrix and also through each of the objects. To view through the torus, cube, or tet, the matrix corresponding to the object is inverted. To view through the teapot, the teapot matrix and cube matrix are multiplied, and then the inverse of the product is taken.

Viewing the arrangement through the torus.

Viewing the arrangement through the cube.

When viewing through an object, the object is drawn in line segments so that the user can see through the object.

The user interface allows one to instantaneously alter the position or radius of an object. See the instructions section for details.

A final feature of this project is being able to see the coordinate axes of each object. With the correct input, all the objects are drawn with line segments and the coordinate axes of each object are displayed. The x-axis is red, the y-axis, green, and the z-axis, blue. There are tic marks on each axis in the positive direction. One of the six directed axes for each object is longer. This allows the coordinate axes to point in the direction that the user will look when viewing through the object.

### Instructions

How to operate illiSolarSystem is shown on the screen. The input used for illiSkel still applies to this project. Additional inputs are also added. The orbit and spin speeds of the cube, tetrahedron, and teapot can be changed by pressing the correct letter. The capital letter increases the value, and a lowercase letter decrease the value. Pressing 'U' changes the value of vumat. 1 corresponds to viewing through the affine matrix, 2 to viewing through the cube, 3 the tet, 4 the teapot, and 0 the torus. The user can type a numerical value and then press 'K' to store it as an x/radius value, or 'J' to store it as a z value. Pressing the letter corresponding to an object moves the object to a new position. The lowercase letter moves the object to the (x,z) value relative to the object it's orbiting. The capital letter changes the radius. 'D' can be pressed to switch between viewing wire figures and coordinate axes and just the solid objects.

### Problems and Possible Future Improvements

One problem is that the world misbehaves when very large values for orbit speed and/or spin are used. As the orbit speed becomes large, the object will seemingly appear at random positions along its orbit, and then suddenly disappear. When the cube has a large value for spin, the teapot will not orbit it like it's supposed to. The best way to fix these problems would be to limit how big the values for spin and orbit speed can get.

Several additional improvements can be made. First, an improvement could be made so that when viewing through an object, the stars move in the appropriate manner. Also, more objects could be added, and all the objects could be put in elliptical orbits. Perhaps a comet could be added that travels in a hyperbola. This is a creative project, so there are many possibilities for improvements and additions.