Dark Energy
Overview
Dark energy is the name given to the invisible mechanism that has caused the universe to expand at an accelerated rate for the past five billion years. Rather than conventional kinetic energy—the energy of objects moving through space—dark energy causes space itself to stretch out, pushing otherwise stationary objects farther apart. Calculations of the prevalence of this repulsion reveal that approximately 70% of the universe is made of dark energy.
Astronomers have known the universe was expanding since Edwin Hubble observed galaxies moving away from Earth in 1929, which served as evidence for the Big Bang. However, cosmologists believed the mutual gravitational attraction of everything in the universe would slow this expansion. By 1998, two independent research teams used type Ia supernovae—stellar remnants that reignite and undergo runaway thermonuclear explosions—to map the universe's expansion over time and discovered it was instead speeding up.
While the nature of dark energy remains unknown, Albert Einstein's equations of gravity once included a term that represented a uniform, repulsive energy filling space. This cosmological constant represents the leading candidate for what dark energy is, but that may be changing. Data from 2025 suggests that the density of dark energy is slowly decreasing with time, weakening its accelerating effect.
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