2.1 Predicting the dice roll
If you’re going to predict how a rolled die will land, you need data. There are numerous factors here related to the die itself, and to the environment in which it is rolled.
Question 3
Can you think of some factors which will need to be considered?
Answer
Factors involving the die:
material properties of the die
size
launch velocity
angle of launch
speed and direction of spin
vertical distance to landing surface
Factors involving the environment:
material properties of the landing surface(e.g., its friction and bounciness)
air resistance.
Here’s Marcus to discuss a few of the key considerations.
Transcript: Video 3 Predicting a dice roll
Even with the data and the mathematical machinery in hand, there is still something missing – the scientific or physical theory that ties it together.
This comes in the form of Newton’s three famous laws of motion which relate an object’s motion to the forces acting upon it. Newton explained these laws in his Principia Mathematica, first published in 1687. (This is one of the most important scientific books ever to be published, and it nearly didn’t make it to the press. Newton was always extremely reluctant to publish his work, and it was published only through the intervention of Edmund Halley, who personally financed its publication after the Royal Society had spent its book budget on a History of Fishes!)
Applying Newton’s laws to physical systems (like the rolling of a die or the motion of a planet) can be written as mathematical equations. The differential calculus mentioned earlier is the key to solving these equations, and giving us the position of the object in motion at any desired time. However, as you shall see, solving these equations can turn out to be an extremely difficult problem. Sometimes it can even be impossible, or at least impossible to the necessary degree of accuracy.
Newton’s laws can nevertheless be used to make some remarkable deductions. Newton himself applied his mathematics to the solar system, calculating the relative masses of the large planets, the motion of the moon, and much more. He was even able to deduce the shape of the earth as a ‘squashed’ sphere (somewhat like a grapefruit) rather than perfectly spherical, as had been previously believed. Experiments carried out around the globe after Newton’s death proved his deduction to be correct.