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Interstellar comet reveals unprecedented chemical composition after passing by the Sun

Comet 3i atlas
Comet 3i atlas - Divulgação

Comet 3I/ATLAS showed a significant chemical transformation in its gas cloud during its approach to Sistema Solar. The interstellar object recorded a drastic reduction in the ratio of carbon dioxide to water shortly after reaching perihelion on October 29, 2025. Pesquisadores used Telescópio Subaru, located on Havaí, to capture the light signatures of the extrasolar visitor in January 2026. The discovery marks a fundamental advance in understanding materials formed outside the cosmic neighborhood.

Observações accurate on the summit of the volcano Mauna Kea

The scientific team responsible for monitoring used Telescópio Subaru to collect spectroscopic data essential to the research. The cutting-edge instrument has an 8.2 meter diameter main mirror and operates at the summit of the Mauna Kea volcano, at Havaí. The measurements took place specifically on January 7, 2026, when astronomers focused on the colors emitted by the object’s coma during the night of observation. The coma consists of the diffuse cloud of dust and gas that surrounds the icy core and glows when reflecting sunlight.

EJA released an impressive photograph of the interstellar comet 3I/ATLAS - ESA/JUICE/JANUS
EJA released an impressive photograph of the interstellar comet 3I/ATLAS – ESA/JUICE/JANUS

The group of experts was led by researcher Yoshiharu Shinnaka, from Instituto of Ciências Espaciais Koyama, linked to Universidade Kyoto Sangyo. Practitioners have applied traditionally used analytical methods to study local comets with great success. The strategy made it possible to measure the so-called forbidden oxygen lines in the visitor’s gaseous structure. Essa indirect technique made it possible to accurately calculate the ratio between the gases released in the space vacuum.

Dinâmica warm-up and core exposure

The chemical variation points to a highly heterogeneous internal structure in the newly discovered interstellar body. Objetos nomads travel for billions of years in the absolute darkness of the interstellar medium, exposed to a constant bombardment of cosmic rays and energetic particles. Essa prolonged interaction chemically alters the outer crust long before any encounter with an intense heat source. The hardened crust acts as a temporary shield for gases trapped in the deep core.

The approach to Sol triggered a violent process of thermal peeling in the comet’s structure. The extreme heat melted and ejected the highly volatile material that had accumulated on the surface over millennia. Gases trapped in deeper layers began to leak into space in visible jets. The new measured ratio more faithfully reflects the true chemical nature of the interior of the original nucleus. January records showed a significant drop in the proportion of volatile compounds compared to data from August 2025.

Visitor Singularidade relative to local bodies

Cometas originating from Nuvem of Oort often exhibit predictable evaporation patterns as distance decreases. 3I/ATLAS surprised the scientific community by demonstrating extremely high levels of carbon dioxide in the first readings captured by the telescopes. The subsequent drastic decrease reinforces the uniqueness of the visitor in relation to the already cataloged local bodies. The behavior differs substantially from patterns observed in native Sistema Solar comets.

  • 3I/ATLAS represents the third confirmed body with an origin external to our system.
  • The pioneer in the category was the rocky object 1I/’Oumuamua detected years ago.
  • The second cataloged visitor was named comet 2I/Borisov after discovery.
  • The complete study is scheduled for publication on April 22, 2026 in the journal The Astronomical Journal.

Instrumentos next-generation spacefarers also actively participated in the global comet tracking effort. The James Webb telescope provided infrared images during the critical closest approach phase. The JUICE interplanetary probe recorded the signature of several complex organic compounds in the object’s tail. The joint work of space agencies has created a detailed profile of cometary activity at different wavelengths.

Implicações for planetary formation models

The analysis of interstellar fragments works as a privileged window into the remote past of the cosmos. Astrônomos treat these bodies as intact time capsules that roam the universe, carrying the exact raw materials that orbited other stars during the genesis of distant worlds. Documented chemical evolution now helps refine mathematical models of gas sublimation and condensation. The diversity of elements found challenges classical theories of star formation.

The direct study of these materials allows unprecedented comparisons with the building blocks of Terra and neighboring planets. Understanding the formation of planetesimals gains new contours with recent data extracted from the comet’s gas cloud. Pesquisadores project that the next generation of scanning telescopes will identify dozens of similar targets over the next decade. Expanding the visitor catalog will provide a robust statistical basis for future space interception missions. Comet 3I/ATLAS continues its accelerated trajectory towards the icy limits of the heliosphere, while new observation campaigns will try to capture the last gasps of activity before the object definitively plunges into the darkness of deep space.

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