  Over the past three decades, we have witnessed one of the great revolutions
in our understanding of the cosmos - the dawn of the Exoplanet Era. Where once
we knew of just one planetary system (the Solar system), we now know of
thousands, with new systems being announced on a weekly basis. Of the thousands
of planetary systems we have found to date, however, there is only one that we
can study up-close and personal - the Solar system.
  In this review, we describe our current understanding of the Solar system for
the exoplanetary science community - with a focus on the processes thought to
have shaped the system we see today. In section one, we introduce the Solar
system as a single well studied example of the many planetary systems now
observed. In section two, we describe the Solar system's small body populations
as we know them today - from the two hundred and five known planetary
satellites to the various populations of small bodies that serve as a reminder
of the system's formation and early evolution. In section three, we consider
our current knowledge of the Solar system's planets, as physical bodies. In
section four, we discuss the research that has been carried out into the Solar
system's formation and evolution, with a focus on the information gleaned as a
result of detailed studies of the system's small body populations. In section
five, we discuss our current knowledge of planetary systems beyond our own -
both in terms of the planets they host, and in terms of the debris that we
observe orbiting their host stars.
  As we learn ever more about the diversity and ubiquity of other planetary
systems, our Solar system will remain the key touchstone that facilitates our
understanding and modelling of those newly found systems, and we finish section
five with a discussion of the future surveys that will further expand that
knowledge.
