When Comet 3I/ATLAS entered the solar system in the summer of this year, it sparked a flurry of scientific activity to study what astronomers quickly identified as only the third interstellar object to pass through our cosmic neighborhood. This rare detection prompted astronomers to turn their attention beyond our solar system, with NASA and the European Space Agency (ESA) spacecraft at Mars shifting their focus to observe the interloper. In the coming weeks, missions bound for Jupiter will also join in this interplanetary quest.
The excitement surrounding the discovery of Comet 3I/ATLAS is palpable among scientists, who see each interstellar object as a unique opportunity for exploration. Karen Meech, a planetary astronomer at the University of Hawaii, describes these discoveries as “special and precious,” with researchers dropping everything to study them. In the absence of specialized missions to intercept these unusual visitors, scientists are leveraging existing spacecraft exploring the solar system to gather data on these interstellar objects, providing a valuable opportunity for scientific study.
Comet 3I/ATLAS, named after the Asteroid Terrestrial-Impact Last Alert System (ATLAS) survey telescope in Chile that first detected it on July 1, is the third confirmed interstellar object to pass through our solar system. Traveling at a staggering speed of 137,000 miles per hour, its hyperbolic trajectory signaled its extraterrestrial origin. Joining the ranks of ‘Oumuamua and Comet 2I/Borisov, Comet 3I/ATLAS offers scientists a new window into the diversity of objects traversing our cosmic neighborhood.
As astronomers work to unravel the mysteries of interstellar comets, comparisons with conventional solar system comets offer valuable insights. The detection of frozen carbon dioxide in Comet 3I/ATLAS’s coma suggests a unique formation process in a distant, frigid region far from its parent star. This discovery hints at the potential differences in comet formation between solar systems, shedding light on the universal processes of planet formation.
Observing Comet 3I/ATLAS as it nears perihelion, the point closest to the sun in its trajectory, provides a rare opportunity to study the object’s behavior as temperature changes trigger outbursts of gas and brightness. Monitoring these fluctuations offers clues to the comet’s composition and history, revealing hidden layers of dry ice buried beneath its surface.
Despite the challenges of observing an interstellar comet from Earth, spacecraft throughout the solar system are poised to capture valuable data on Comet 3I/ATLAS. Coordinating an interplanetary observation campaign, NASA and ESA missions are leveraging their instruments to study the comet as it approaches different planets. Recent images shared by ESA’s ExoMars orbiter showcase Comet 3I/ATLAS from a distance of 19 million miles, offering a glimpse into its characteristics.
While the U.S. federal shutdown has temporarily halted NASA’s operations, early data from spacecraft like the Earth-observing weather satellite GOES-19 hint at the comet’s brightening and evolving behavior. As ESA’s Jupiter Icy Moons Explorer (JUICE) mission prepares to observe Comet 3I/ATLAS, scientists eagerly anticipate new insights into this interstellar visitor as it cools after its solar encounter.
A particularly tantalizing opportunity awaits NASA’s Europa Clipper spacecraft, which may pass through Comet 3I/ATLAS’s ion tail between October 30 and November 6. This unprecedented event could offer groundbreaking observations of charged particles interacting with the comet’s gas, revealing a dynamic region shaped by the convergence of interstellar and solar influences.
As scientists eagerly await the results of these observations, the study of interstellar comets presents a unique opportunity to explore objects from distant star systems up close. With each new discovery, researchers gain valuable insights into the universal processes of planetary formation and the rich diversity of objects traversing our galactic neighborhood.
 
					
 
			 
                                 
                             