  This essay is a nontechnical primer for a broader audience, in which I paint
a broad-brush picture of modern cosmology. I begin by reviewing the evidence
for the big bang, including the expansion of our Universe, the cosmic microwave
background, and the primordial abundances of the light elements. Next, I
discuss how these and other cosmological observations can be well explained by
means of the concordance model of cosmology, putting a particular emphasis on
the composition of the cosmic energy budget in terms of visible matter, dark
matter, and dark energy. This sets the stage for a short overview of the
history of the Universe from the earliest moments of its existence all the way
to the accelerated expansion at late times and beyond. Finally, I summarize the
current status of the field, including the challenges it is currently facing
such as the Hubble tension, and conclude with an outlook onto the bright future
that awaits us in the coming years and decades. The text is complemented by an
extensive bibliography serving as a guide for readers who wish to delve deeper.
