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Discovery of the interstellar star 3I/ATLAS generates mystery with NASA’s official silence

Carolina Costa
Por 5 min de leitura
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Cometa
Foto: Cometa - Foto: Nazarii Neshcherenskyi/istock

The present interstellar star 3I/ATLAS, detected on July 1, 2025 by the ATLAS telescope on Chile, has an atypical chemical composition that defies known models of comet formation. The North American space agency, mainly responsible for monitoring, has imposed restrictions on the release of detailed information since October, due to budget constraints imposed by the government shutdown of Estados Unidos. Astrônomos from several countries questions the lack of transparency, while independent observatories collect data to fill the gaps. The object’s hyperbolic trajectory confirms its origin outside of Sistema Solar, making it the third recorded interstellar visitor.

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Initial observations reveal high levels of carbon dioxide in the star’s coma, outnumbering the presence of water by eight to one. The Essa anomaly suggests formation processes in cold regions of distant protoplanetary disks. Telescópios in Chile and Europa have recorded 3I/ATLAS activity since May 2025, when the object activated 6.4 astronomical units of Sol. The passage close to Marte on October 3 allowed captures by orbital probes, however the results await joint analysis.

Chemical composition reveals distant origins

Spectroscopic analyzes indicate a predominance of volatile compounds such as carbon monoxide, exposed to cosmic radiation during billions of years of interstellar travel. The star’s core measures between 300 meters and 5.6 kilometers in diameter, with an active surface area of ​​more than 8%.

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The absence of heavy metals aligns 3I/ATLAS with ancient stars in Via Láctea’s thick disk, estimating its age at between 7.6 and 14 billion years. July’s Estudos points to chemical exchanges between stellar systems, influenced by gravitational encounters.

These characteristics differentiate the object from local comets, which have a higher water content and reddish dust. Observações from Telescópio James Webb confirmed in August ultraviolet emissions, similar to water jets at cold distances from Sol.

Global surveillance compensates for limitations

Collaboration with Agência Espacial Europeia fills gaps left in NASA’s dataset. Sondas, as well as Mars Express and ExoMars Trace Gas Orbiter captured infrared records during the approach to Marte.

  • Trace gas records indicate symmetrical emission patterns, rare in known comets.
  • Subtle vibrations in the core suggest a complex internal structure, with metallic grains on the surface.
  • Unexpected accelerations near planets point to unforeseen gravitational interactions.

These joint efforts maximize the limited observation window before perihelion on October 30. Os terrestrial Observatórios plan intensive sessions to record possible dust ejections.

Trajectory anomalies challenge models

3I/ATLAS displays speeds of 210 to 221 thousand kilometers per hour, with projected increases in solar approach. As Estimativas masses range from 1,000 to 10,000 times that of typical comets, with no signs of fragmentation to date.

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The unusual negative slant and lack of debate on powder tail fuel classification. Os Alguns astronomers propose using missions like Hera and Europa Clipper to detect ions in the tail, capturing matter from another star system.

Preliminary data from Telescópio Hubble, expected in November, will focus on ultraviolet spectroscopy to measure sulfur and oxygen ratios. The trajectory passes 1.4 astronomical units from Sol, without risk of collision with Terra, which will occur at a minimum distance of 240 million kilometers.

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Nasa – Foto: SNEHIT PHOTO / Shutterstock.com

Initial observations from the ATLAS telescope

The detection occurred on the NASA-funded Río Hurtado, confirming a hyperbolic orbit. The Atividade star began in May, shining continuously until September.

Reactions from the scientific community

Astronomers highlight the potential of 3I/ATLAS to redefine the understanding of interstellar objects. Debates takes place at global forums on implications for planetary formation.

  • Proposals include integrating data from multiple missions to map ice and emissions.
  • Collaborations with observatories on Hemisfério Sul prioritize night sessions.
  • Bayesian analyzes estimate a low probability of natural origin in certain scenarios.
  • Expectations involve the publication of high-resolution post-perihelion records.

The urgency increases when the object moves away, requiring accelerated telemetry processing.

Future study perspectives

The Vera C. Rubin Observatory captured fortuitous records in June, refining the coma diameter measurements. Telescópio Espacial Transiting Exoplanet Survey Satellite recorded pre-discovery activity, expanding the history of observations.

The estimated mass reinforces the hypotheses of formation in dense galactic regions. Novembro Observações to Hubble will monitor the production of Sistema Solar, evaluating the persistence of emissions.

These measures depend on international partnerships to overcome budgetary restrictions, ensuring continuity of monitoring.

Astro 3I/ATLAS offers a unique window to explore chemical diversity beyond Sol, driving advances in interstellar astronomy. The passage of Sua reinforces the need for investment in global detection and analysis, with ground-based telescopes visible by December 2025. Especialistas awaits consolidated data to validate theories about galactic evolution, while the object continues its outward trajectory.

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