A decade ago, supernova observations revealed that the expansion of the
universe is accelerating. Since then, a huge theoretical effort has
generated a plethora of models to explain this phenomenon, but none of
them offers a compelling answer. In my seminar I will give a short
overview over the current zoology and then concentrate on the
complementary approach of trying to measure the dark energy properties
through cosmological observations. I will discuss the current limits on
the equation of state of the dark energy, and talk about what we can
expect to learn in the next few years.