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NASA reveals detection of organic molecules in interstellar comet 3I/ATLAS during solar trajectory

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An Nasa space observatory has captured evidence of organic molecules being released by an interstellar comet during its passage through Sistema Solar. The object, identified as 3I/ATLAS, revealed compounds that form the basis for chemical processes that can lead to the formation of biological structures, although it does not indicate the presence of living organisms.

The data was collected in December 2025, when the comet was moving away from Sol after its closest approach. Cientistas analyzed the expelled material, confirming the presence of elements such as methanol, hydrogen cyanide and methane, which are common in environments where organic chemistry develops.

This detection reinforces the understanding of the distribution of primordial matter in the universe. Objetos like this comet offer clues about how basic ingredients for life can travel between distant star systems.

Details of the initial discovery

Comet 3I/ATLAS was identified on July 1, 2025 by the ATLAS monitoring system, located at Chile. Esse automated equipment tracks objects near Terra and detected the visitor from outside Sistema Solar, marking it as the third known interstellar object after 1I/’Oumuamua and 2I/Borisov.

The hyperbolic trajectory confirmed its external origin, with a speed that prevents it from being captured by solar gravity. Astrônomos calculated that it approached about 170 million kilometers from Terra, without posing any risk.

Chemical composition revealed

Observations carried out by the SPHEREx telescope, launched in March 2025, captured infrared signatures of the comet between December 8 and 15. The instruments detected an active coma, formed by gas and dust released by the heating of the core.

Among the compounds identified, methanol and methane stand out for their role in chemical reactions that predate biology. Esses elements were found in significant quantities, suggesting that the comet carries material formed billions of years ago in another star system.

Hydrogen cyanide, another detected component, is known to contribute to the synthesis of amino acids in cosmic environments. Essa mixture reinforces theories about panspermia, where blocks of life spread throughout space.

Increased post-perihelion activity

After passing through the closest point to Sol, the comet exhibited a significant increase in brightness. Esse phenomenon occurred about two months later, when internal layers of ice sublimated, releasing large volumes of material.

Researchers observed the ejection of carbon dioxide and carbon monoxide, as well as water in smaller quantities. Essa late eruption indicates that solar heat penetrated deep into the core, activating underground reservoirs.

The intensified brightness allowed for more precise measurements of the coma, revealing an organic-rich composition. Astrônomos compare this to solar comets, but note differences in the abundance of certain gases, which highlights interstellar chemical diversity.

Physical characteristics of the object

The 3I/ATLAS nucleus was estimated to be between 440 meters and 5.6 kilometers in diameter, based on images from Telescópio Espacial Hubble in August 2025. The Essa variation reflects the difficulty in measuring distant objects, but confirms a modest size by cometary standards.

The icy surface, composed mainly of frozen water mixed with dust and organics, began to sublimate as it approached Sol. Isso generated a visible tail, typical of active comets, distinguishing it from inert asteroids.

Implications for future studies

Space missions like SPHEREx continue to monitor the comet as it moves away. Dados collected help map the distribution of organic molecules in the universe, contributing to models on the formation of habitable planets.

Proposals to intercept similar objects include complex maneuvers, such as Solar Oberth, which would use the gravity of Júpiter to propel probes. A 2035 launch window could allow for a rendezvous in later decades.

These initiatives require advances in propulsion, but promise direct samples of interstellar material. Enquanto this, terrestrial and space observations refine knowledge about these cosmic travelers.

Searches for technological signals

Teams dedicated to detecting technosignatures scanned 3I/ATLAS for artificial emissions. Utilizando radio telescopes like MeerKAT, scientists scanned radio frequencies in October 2025.

No signs of technological origin were found, confirming the natural nature of the object. Instead, they detected hydroxyl, indicative of evaporating water ice, aligning with the expected behavior of a comet.

Trajectory and passage through planets

The comet passed within 30 million kilometers of Marte in October 2025, allowing observations from the Perseverance probe. Imagens screenshots show the coma expanding, with dust reflecting sunlight.

In March 2026, it will approach Júpiter at 53 million kilometers, offering another opportunity for study. The gas giant’s gravity may slightly alter its exit trajectory.

These close passages facilitate data from multiple perspectives, enriching the set of information about its composition and dynamics.

Comparisons with previous visitors

Unlike ‘Oumuamua, which did not exhibit an active coma, 3I/ATLAS behaves like a classic comet. Isso contrasts with Borisov, which also released gases, but in different patterns.

Analysis shows that 3I/ATLAS has a higher abundance of cyanide compared to solar comets. Essa variation suggests differences in original star formation, possibly in systems older than our own.

Comparative studies help to understand interstellar chemical evolution. Objetos like these act as time capsules, preserving primordial conditions from distant regions.

Contributions from multiple missions

Several Nasa spacecraft collaborated on the observations, including James Webb and Hubble. Webb captured spectra in August 2025, identifying early traces of organics.

The Lucy mission, en route to asteroids, adjusted instruments to record the comet. Já PUNCH, focused on Sol, monitored interactions with the solar wind.

This coordination demonstrates the ability to respond quickly to rare astronomical events. Integrated data provides a comprehensive view of the 3I/ATLAS journey.

Expanded scientific perspectives

The detection of organic molecules on the comet reinforces the idea that the ingredients for life are common in the cosmos. Isso impacts fields such as astrobiology, which seeks to understand the origins of life on other worlds.

Future missions, such as ESA’s Comet Interceptor, aim to await interstellar visitors for on-site studies. Tais efforts could reveal more about the universal chemistry and potential habitability of exoplanets.

3I/ATLAS serves as a reminder that Sistema Solar is not isolated, receiving material from distant stars periodically.

Continuous monitoring

As the comet recedes, ground-based telescopes continue to track its position. Regular Atualizações refine trajectory predictions, ensuring there are no unlikely future collisions.

Archived data remains available for further analysis, fueling global research. Essa open approach accelerates advances in understanding interstellar objects.

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