The universe is composed of approximately 5% baryonic matter, 25% non-baryonic matter, and 70% dark energy. Current theories attempt to explain dark energy and non-baryonic matter, but none have been conclusively verified through observation. Dark energy is often associated with a small cosmological constant in Einstein's general relativity, although there are significant discrepancies regarding its expected size. Resources like hep-ph/0312013 from arXiv can provide further insights into these topics. Understanding these components is crucial for grasping the universe's fundamental structure.