Discovered in July 1995 by astronomers Alan Hale and Thomas Bopp, Comet Hale-Bopp gained significant attention as it traveled through the solar system. Notably, it became visible to the naked eye in the evening sky in early 1996. By early 1997, it had reached perihelion—the point in its orbit closest to the Sun—and subsequently approached its closest distance from Earth in March of the same year, measured at approximately 1.315 astronomical units (AU), which is about 123 million miles. The comet's distinct appearance featured two tails: a dust tail and an ion tail. The dust tail’s yellowish hue contrasted with the blue glow of the ion tail, creating a stunning visual effect that caught the eye of many around the globe.

The 1997 appearance of Hale-Bopp was extraordinary due to its brightness, lasting visibility, and high altitude in the night sky, making it an object of fascination for both amateur and professional astronomers. As the comet approached Earth, it provided ample opportunities for observation and study, leading to numerous scientific investigations regarding its composition, structure, and dynamics. Public interest surged, resulting in widespread media coverage and engagement in astronomy-related activities, such as comet watch parties and educational programs designed to enhance understanding of celestial phenomena.