Comets are celestial objects composed of rock, ice, and other materials, typically ranging in size from a few hundred meters to several kilometers. They are remnants from the early Solar System and often originate from the distant regions beyond Neptune’s orbit. Some comets, like Oumuamua and 3I/Atlas, are believed to have come from other star systems, making them interstellar objects. These comets have sparked interest among scientists, as they offer clues about the formation of planetary systems and the distribution of materials across the galaxy. The study of exocomets—comets that orbit stars other than the Sun—has been ongoing for decades. The first confirmed exocomets were discovered in 1987 around the star Beta Pictoris, which is located about 63 light-years away from Earth. These discoveries have helped astronomers understand how comets might behave in different star systems and what role they might play in the development of life-supporting environments. A widely accepted theory in astronomy is that comets may have delivered the basic ingredients for life to Earth through impacts. This idea is known as the panspermia hypothesis, which suggests that organic molecules and water could have been brought to Earth by comets and other celestial bodies. Recent research has expanded this theory to other star systems, exploring whether similar processes might occur elsewhere in the galaxy. A groundbreaking study published in Nature Communications has identified the first potential exocomets in the youngest planetary system ever discovered, known as PDS 70. This system is only about 5 million years old, making it a unique opportunity to observe the early stages of planet formation. The discovery supports the idea that comets might play a similar role in other planetary systems, potentially delivering essential materials for the development of life. This finding adds new insights into the processes that may have shaped the early Solar System and could influence the search for life beyond Earth.