Celestial objects exhibiting a yellowish hue are commonly observed in the night sky. These luminous spheres, primarily composed of hydrogen and helium, generate energy through nuclear fusion in their cores. Our Sun serves as a prime example of such an object, radiating light across the visible spectrum, with a significant portion perceived as yellow by the human eye.
Observation and study of these radiant bodies have been fundamental to the development of astronomy and astrophysics. Their characteristics, including luminosity, temperature, and spectral class, provide invaluable data for understanding stellar evolution, galactic structure, and the overall composition of the universe. Throughout history, these celestial beacons have served as navigational aids, timekeeping markers, and objects of cultural significance across various civilizations.
