A custodial worker at UC Santa Barbara was cleaning a storage closet filled with old military searchlight mirrors when he saw something strange. Dust that seemed to float in the air and couldn't be wiped away. A physicist identified it as a real image, an optical effect where light comes together so precisely that it makes something appear to be there even when it's not. This accidental discovery led to the creation of the mirascope, and the parabolic shape of those surplus mirrors has been the basis for every version made since then.
Over the next few decades, researchers found that parabolas have a special mathematical property: any light ray coming from the focal point bounces off perfectly parallel to the axis, and the other way around. This property is exact and makes the mirascope's image very sharp. However, a small assumption was overlooked. Since the parabola creates a perfect focus, it was considered the best mirror shape for the device. Nobody made a distinction between making the focus as precise as possible and making the experience better for the viewer. These are actually two different problems. Every parabolic mirascope built has a viewing angle of about 55 degrees from horizontal. This angle is a result of the parabolic shape, not a fundamental law of optics.
This project starts with a basic idea: the only physical rules that apply to the mirascope are that light moves in straight lines and bounces back at the same angles. The parabolic shape and the need for rays to travel parallel between the mirrors, as well as the 55-degree viewing limit, are all results of one specific geometric solution, not limits set by physics. A different mirror shape could send light along completely different paths and still bring the rays together at the image point, even if no human designer would think of drawing those paths. Such a shape might be able to trade some of the parabola's perfect focus for a wider viewing area, especially when the object is small and gives off its own light, and a slightly blurry image would be okay if it means being able to see it from more angles.
The tools needed to search for a shape like this, such as evolutionary algorithms that can explore millions of freeform surface geometries, exact ray-tracing engines that can evaluate each one, and multi-objective scoring that balances image quality with viewing angle and brightness, did not exist when the mirascope was first discovered. They were also not available for practical use when it was last studied in 2007. However, these tools are available now. This project plans to use them, starting with the two basic laws of reflection and making no assumptions about the mirror shape, to explore a question that has never been asked before: is the parabola really the best shape for a mirascope, or was it just the shape that was readily available?