Many people are drawn to physics because they wish to understand why the
world around us is like it is. For instance, why the sky is blue, why raindrops
are spherical, why we do not fall through the floor, et cetera. It turns
out that
thermodynamics is a very powerful tool for
accounting for the observed features of the physical world. For example, in this course, we shall explain
why heat spontaneously flows from hot to cold bodies;
why it is impossible to
measure
a temperature below -273
centigrade; why there is a maximum theoretical
efficiency of a power generation unit that can never be exceeded, no matter
what the design; why the Earth's atmosphere becomes thinner and
colder at higher altitudes; why the Sun appears yellow,
whereas colder
stars appear red, and hotter stars appear bluish-white; and why high mass stars must ultimately collapse
to form black-holes.