I describe the evidence for the Big Bang, including the various cosmologica
l parameters. There is general concordance on their values, although the un
certainties remain large enough to justify the ensuing debate. Structure fo
rmation is reviewed, and here there is consensus on the hierarchical nature
of the sequence of formation. The cosmic microwave background anisotropies
provide a glimpse of the initial conditions that seeded structure, and the
evolution of clouds of dar matter is an inevitable consequence. There are
two outstanding mysteries: the very beginning, where a theory of quantum gr
avity is eagerly awaited, and the detailed nature of galaxy formation, wher
e observations are well ahead of theory. (C) Academie des sciences/Elsevier
, Paris.