Dark energy is a theoretical form of energy that is thought to make up about 68% of the universe. It is distinct from both ordinary matter and dark matter, and its existence was inferred from observations of the expansion rate of the universe. Unlike gravity, which tends to pull things together, dark energy seems to be causing the universe to expand at an accelerating rate.
The existence of dark energy was first inferred from observations of distant supernovae in the late 1990s. These observations suggested that the expansion of the universe was not slowing down as expected, but rather was speeding up. This led to the idea that a mysterious force, now known as dark energy, was counteracting the effects of gravity and driving the accelerated expansion.
Dark energy is thought to be the dominant component of the universe's energy density, but its nature is not well understood. Its presence has significant implications for the ultimate fate of the universe. If dark energy continues to drive the acceleration of the universe's expansion, it is believed that galaxies will eventually move so far apart that they will no longer be visible from one another, leading to a "Big Freeze" scenario.
Scientists are actively studying dark energy through a variety of techniques, including observations of supernovae, measurements of the cosmic microwave background radiation, and large-scale galaxy surveys. These efforts aim to better understand the nature of dark energy and its role in the evolution of the universe.