Celestial illumination, observed from Earth, primarily originates from distant suns. These luminous orbs, powered by nuclear fusion, emit vast amounts of energy, a portion of which reaches our planet as visible light. Observation of the night sky reveals numerous points of light, the vast majority of which represent these remote stellar bodies.
Understanding the nature of these pinpoints of light is fundamental to astronomical science and has profound implications for comprehending the scale and structure of the universe. Throughout history, cultures have developed cosmologies and navigational systems based on the perceived positions and movements of these celestial beacons. Accurate identification and measurement of their properties allows for the determination of distances, compositions, and evolution of galaxies.