Ground-based observatories confirm radio silence on interstellar comet 3I/ATLAS with 1 km nucleus

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Comet Foto: Comet - Photo: Nazarii Neshcherenskyi/istock

The international astronomical community recently consolidated a new set of fundamental data about the celestial body 3I/ATLAS, classified as the third interstellar visitor confirmed to cross the boundaries of our Sistema Solar. Análises exhaustive and prolonged radio frequency emissions categorically ruled out the presence of any active or targeted artificial technology on the celestial body, ending speculation about its origin. Continuous monitoring, carried out by a global network of observatories, also allowed scientists to calculate the exact physical dimensions of the object, establishing an approximate diameter of one kilometer for its rocky, frozen core. The information comes from intensive observation campaigns carried out by large radio telescope complexes over the past few months, which have turned their antennas into deep space in search of answers about the formation of distant star systems. Tracking anomalous signals represents a standard and rigorous step in investigating bodies from outside our cosmic neighborhood, ensuring that all scientific possibilities are exhausted during the object’s passage.

The absolute absence of radio emissions reinforces the purely geological and natural nature of the comet, bringing it in line with the theoretical expectations of modern astrophysics. The researchers applied rigorous digital filters to separate the background noise generated by Terra from possible alien transmissions, resulting in total silence in the frequency range analyzed by ground-based observatories.

In addition to the thorough search for technological signatures, the celestial body’s orbital mechanics provided crucial clues about its internal composition and its behavior under the extreme thermal influence of Sol. The constant release of gases and dust creates a natural propulsion effect that alters the trajectory expected by pure gravity, allowing astrophysicists to unravel the structure of the distant visitor.

Frequency scanning in deep space

The Allen Telescope Array complex dedicated more than seven hours of continuous and uninterrupted observation to 3I/ATLAS shortly after the official confirmation of its interstellar trajectory. During this period of active listening, the ultrasensitive instruments recorded approximately 74 million initial detections in a narrowband range, operating specifically between the frequencies of 1 to 9 GHz.

This massive volume of raw data required the immediate application of complex radio frequency interference mitigation algorithms. Our planet’s own telecommunications infrastructure generates constant and chaotic noise that can easily mask true signals or simulate false positives coming from deep space, requiring very high-level computational processing.

After the first round of intensive digital cleaning, the number of signal candidates dropped sharply to around two million records. The next step involved filtering by spatial location, crossing the exact coordinates of the moving object with the origin of the captured waves, which eliminated almost all of the records and left only 211 anomalies which, after visual inspection, proved to be just background noise without artificial characteristics.

Transmit power limits

The absence of valid signals allowed scientists to establish extremely stringent upper limits for any hypothetical radio transmission originating from the celestial body. Considerando the effect Doppler generated by the high radial velocity of the object in relation to

This energy level is considered extremely low by astronomical standards, being comparable to the consumption of a common incandescent lamp or small amateur radio transmitters. The technical inability to detect even this tiny amount of energy in the 1 to 9 GHz band definitively consolidates the thesis that the object is inert from a technological point of view.

Restrictions imposed by ground-based observatories

Additional data collected by Green Bank Telescope during the object’s closest approach to Terra imposed even more severe restrictions on the mathematical models. The temporary proximity offered a unique observation window that was taken full advantage of by radio astronomy teams.

Detailed analyzes reduced the possible power to just 0.1 watt at frequencies from 1 to 12 GHz. The result virtually eliminated any theoretical margin for the existence of active communications devices housed in the comet’s nucleus.

Orbital dynamics and cometary thermodynamics

Accurately determining the size of 3I/ATLAS required combining high-resolution astrometric data with advanced physical models of cometary thermodynamics. The researchers focused intensely on the object’s non-gravitational acceleration, a phenomenon widely documented in comets approaching Sol.

Intense solar heating causes the rapid sublimation of volatile elements present both on the surface and inside the rocky core. Esse thermal process is fundamental to understanding the loss of mass that the celestial body suffers during its journey through our system.

This direct transition from the solid to the gaseous state generates directed jets of material that work exactly like small natural propellants. The force exerted by this ejection subtly changes the directional velocity and rate of rotation of the celestial body in the vacuum of space.

By crossing the estimated rates of mass loss with the intensity of this anomalous acceleration, mathematical calculations based on conservation of momentum pointed to a clear result. The modeling confirmed a nucleus with a diameter of the order of one kilometer, validating the initial theoretical predictions.

Variables in astrophysical modeling

Despite the remarkable consistency of the diameter calculations, the 3I/ATLAS physical modeling still faces significant uncertainties that demand continued study. The measurement of non-gravitational acceleration has undergone multiple rigorous revisions due to small margins of error in the exact location of the object and the direct dependence on its distance from Sol during the phase of greatest thermal activity. Monitoring a body traveling at interstellar speeds requires perfect calibration of terrestrial instruments to avoid distortions in the data collected.

Another extremely complex factor involves the exact composition of the material ejected into space. The transfer of momentum to the core may be dominated by the violent expulsion of macroscopic ice fragments rather than just fine gaseous particles and microscopic dust. The exact direction and speed of these jets diverge from the standard values ​​assumed in previous astronomical models, requiring fine adjustments to thermodynamic equations to reflect the true physical nature of this distant visitor.

Advances in the exploration of external celestial bodies

The evolution of scientific understanding of 3I/ATLAS intrinsically depends on the ability of next-generation observatories to perform direct spectroscopic measurements of jet velocities and the exact chemical composition of sublimated material. Telescópios Advanced spacecraft, equipped with state-of-the-art sensors, have the sensitivity necessary to map the thermal distribution on the surface of the nucleus with millimeter precision and identify specific molecules being released into the space vacuum. The lack of full consideration of the change in direction of the jets over the months of observation represents a technical gap that these new technological tools could fill in future passes of similar objects. The systematic accumulation of data on this specific visitor calibrates terrestrial and space-based instruments for much faster and more accurate detection of future celestial bodies ejected from other planetary systems, raising the standard of international astronomical research to a new level of operational excellence.

Scientific validation protocols

Systematic monitoring campaigns have established a strict and permanent protocol for validating any anomaly detected in deep space. The seamless integration of radio telescope data with very high-resolution optical observations ensured complete coverage of the astronomical event, successfully isolating radio frequency pollution of terrestrial origin and confirming the absolute silence of the celestial body.

Carolina Costa é colaboradora da redação do Mix Vale, portal de notícias com cobertura de Brasil e mundo. Produz conteúdo nas editorias de economia e benefícios, com foco em informação de serviço para o leitor brasileiro. Escreve para o portal desde 2019. Formação: Administração

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