A standard form of a first order differential equation is:
(1) $$\tau \frac{dy}{dt} + y = k * x(t)$$
The laplace transform of this:
(2) $$G(s) = \frac{Y(s)}{X(s)} = \frac{k}{\tau s+1}$$
but sometimes it is given as
(3) $$H(s) = \frac{1}{\tau s +1} = \frac{a}{s+a}$$
A standard form of a second order differential equation is:
(4) $$\tau ^{2} \frac{d^{2}y}{dt^{2}}+2 \tau \zeta \frac{dy}{dt} + y = k * x(t)$$
The laplace transform of this:
(5) $$G(s) = \frac{Y(s)}{X(s)} = \frac{k}{\tau^2s^2 + 2\tau\zeta s+1}$$
but sometimes this is given as
(6) $$H(s) = \frac{\omega_n^2}{s^2+2\zeta \omega_n s + \omega_n^2}$$
Here are my questions:
What is the physical meaning of "first" and "second order"? (apart from the fact that the highest power of the differential in the first is 1 and in the second is 2). How do I know if a system is first or second order?
Where do equations (1) and (4) come from? Why were these decided to be the "standard form"? What is so special about this form and how were these equations derived?
When given a first order system, why is sometimes equation (2) given, and sometimes equation (3) as the transfer function for this system? Likewise, when given a second order system why is equation (6) usually given, when the laplace transform is actually equation (5)?