We've been dabbling a lot in the mysterious world of quantum physics lately, so to get back down to Earth we thought we'd bring you reminder of good old classical physics.

The London Velodrome's track is designed for maximum speed using Newton's laws of motion.
Newton's first law: An object at rest will remain at rest unless acted upon by an external and unbalanced force. An object in motion will remain in motion unless acted upon by an external and unbalanced force.
This is also called the law of inertia and it doesn't need much explanation. No stationary object will start moving of its own accord without a force being applied. And the reason why in our everyday experience moving objects tend to slow down unless they are being powered by something is due to factors such as friction and air resistance.
Newton's second law: The acceleration a of a body is parallel and proportional to the net force F acting on it. The exact relationship is F=ma, where m is the body's mass.
In this equation both F and a are vectors with a direction and a magnitude.
Newton's third law: When two bodies exert a force on each other the forces are equal in magnitude, but opposite in direction. For every action there is an equal and opposite reaction.
Thus, if you kick a ball with your foot, then the ball exerts an equal and opposite force on your foot.
The three laws of motion were first published in 1687 in Newton's famous work Philosophiae Naturalis Principia Mathematica which translates as Mathematical Principles of Natural Philosophy. Newton's law of universal gravitation and mathematical techniques we'd now call calculus were also published in Principia Mathematica and together with the laws of motion they gave the first comprehensive description of the physical processes we observe in everyday life. It later turned out that the laws don't hold when you look at the world at very small scales (that's where quantum mechanics reigns) or at objects that move at very high speed or when there are very strong gravitational fields. However, Newton's laws still give a very good approximation for the physics we observe in our normal lives.
To read more about Newton's laws and its applications, from understanding the melting Arctic to building the Olympic Velodrome, have a look at our teacher package on classical mechanics.
where
and
are ordinary numbers and
stands for the square root of
The number
and
Numbers of this form are called complex numbers. ![\[ (x+iy) + (u+iv) = (x+u) + i(y+v). \]](/MI/9e6f2228064ccab1d0d41ffbdcf1cb8e/images/img-0001.png)
![\[ (x+iy)(u+iv) = xu + i(xv+yu) + i^2yv = xu - yv + i(xv+yu). \]](/MI/9e6f2228064ccab1d0d41ffbdcf1cb8e/images/img-0002.png)
and
components are normal numbers so we can associate to them the point with coordinates
on the plane, which is where you get to if you walk a distance
which is the sum of
and
corresponds to the point you get to by walking a distance
in the horizontal direction and a distance
in the vertical direction. Makes sense.
Multiplying them by
flips them over to the other side of the point
:
goes to
goes to
and so on. In fact, you can think of multiplication by

the square root of
? Multiplying twice by
is the same as multiplying by
So if the latter corresponds to a rotation through 180 degrees, the former should correspond to rotation by 90 degrees. And this works. Try multiplying any complex number, say
by
but by a more difficult complex number
Well, multiplying by an ordinary positive number corresponds to stretching or shrinking the plane: multiplication by 2 takes a point
to
which is further away from
(that’s stretching) and multiplication by 1/2 takes it to
which is closer to 
corresponds to a combination of rotation and shrinking/stretching. For example, multiplication by
is rotation through 120 degrees followed by stretching by a factor of 2. So complex numbers are not just weird figments of the imagination designed to help you solve equations, they’ve got a geometric existence in their own right. 

, for example the one shown in the picture? Here’s how to do it for the limit superior. First look at the whole sequence and find its least upper bound: that’s the smallest number that’s bigger than all the numbers in the sequence. Then chop off the first number in the sequence,
and again find the least upper bound for the new sequence. This might be smaller than the previous least upper bound (if that was equal to
), but not bigger. Then chop off the first two numbers and again find the least upper bound. 

