Interstellar comet 3I/ATLAS has garnered significant attention from astronomers due to its remarkable age, estimated to

be between 8 and 14 billion years. This timeframe places it well before the formation of our solar system, which is

approximately 4.6 billion years old. Associate Professor Michele Bannister from the University of Canterbury has led

efforts to study this comet since its discovery in July 2025, emphasizing its potential to provide insights into the

early building blocks of planet formation across the galaxy.

The age of 3I/ATLAS suggests that it may originate from a star that has long since died. This notion raises intriguing

questions about the lifecycle of stars and the materials they leave behind. Stars undergo processes of nuclear fusion

during their lifetimes, eventually leading to their demise in spectacular events such as supernovae. The remnants of

these stellar explosions can contribute to the formation of new celestial bodies, including comets like 3I/ATLAS.

Therefore, studying this comet could allow scientists to piece together the history of stellar evolution and the

conditions that prevailed billions of years ago.

Bannister describes 3I/ATLAS as a 'calling card from the past,' indicating that it carries chemical signatures from its

origins that can inform researchers about the physical and chemical processes that occurred in its parent star system.

The study of interstellar objects like 3I/ATLAS is particularly valuable because they allow astronomers to gather

evidence about planetary formation processes that may differ from those in our solar system. This is largely due to the

unique composition of such objects, which can include elements and compounds that are scarce or absent in our own

celestial neighborhood.

The research team at the University of Canterbury has developed a theoretical framework known as the Ōtautahi-Oxford

model. This model assists in understanding the dynamics of interstellar objects, including their formation, movement

through space, and chemical properties. With this model, the team analyzed the comet's trajectory and velocity shortly

after its discovery, which provided critical information about its age and origin.

Moreover, the composition of 3I/ATLAS is being closely examined. The comet features a visible coma and two distinct

tails: one trailing behind it and an anti-tail pointing toward the Sun. Bannister characterizes 3I/ATLAS as 'a dusty wee

snowball,' highlighting that its tails are formed from ice and dust particles that reflect sunlight, creating the

observable features we see from Earth.

However, while the study of 3I/ATLAS is groundbreaking, it is essential to recognize the limitations of our

understanding. The exact conditions that led to the formation of this comet and its parent star remain uncertain. The

current findings do not imply that all interstellar comets will share a similar history or composition, nor do they

provide a complete picture of cosmic evolution.

As research continues, there are still many unanswered questions regarding the implications of 3I/ATLAS's findings for

our understanding of the Milky Way's history and the nature of other interstellar objects. The transient nature of these

comets means that astronomers have a limited timeframe to gather data, underscoring the urgency of this research. The

study of 3I/ATLAS exemplifies the broader scientific effort to unravel the mysteries of our universe's past and the

processes that shape it.

In conclusion, the investigation of interstellar comet 3I/ATLAS not only sheds light on the characteristics of ancient

stellar systems but also enriches our understanding of the diverse conditions that govern planet formation across the

galaxy. It serves as a reminder of the complexity of the cosmos and the ongoing quest to understand our place within it.