Physical simulations prove that gas jet drives interstellar comet and rule out exotic theories

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NASA Foto: NASA - Foto: LaserLens/Shutterstock.com

Researchers have identified the exact cause for the atypical orbital behavior of comet 3I/ATLAS, an interstellar object that intrigued the scientific community by presenting an acceleration greater than that explained solely by the gravity of Sol. A new study published on the preprint server arXiv demonstrates that the release of internal volatile gases is enough to justify the extra impulse observed in the celestial body’s trajectory.

The investigation focused on determining whether motion detected more than 200 million kilometers from the central star would require new physical theories or whether known natural processes were the answer. The analyzes confirmed that the outgassing phenomenon, where jets of sublimated material function as natural propellants, fully explains the object’s dynamics.

Imagem através do Telescópio Espacial Hubble do cometa interestelar 3IATLAS, mostrando sua cabeleira e uma cauda crescente
Telescópio Espacial Hubble image of the interstellar comet 3IATLAS, showing its mane and growing tail – Foto: NASA/ESA/David Jewitt (UCLA)

The celestial body, officially identified in July 2025, had classic features such as an icy core and a dust tail, but its speed raised questions about its composition and structure. Validation of the current physical model ends speculation about exotic forces acting on the cosmic visitor.

Computational modeling details propulsion mechanism

To unravel the inner workings of 3I/ATLAS, physicist and computer engineer Florian Neukart, linked to Instituto of Ciência of Computação Avançada of Através of Monte Carlo simulations, it was possible to test different combinations of temperatures and gas mixtures to replicate deep space conditions.

Computational tests revealed that great activity across the entire length of the object is not necessary to generate the observed acceleration. The model indicates that a minimal fraction of the surface exposed to solar heat is capable of producing the thrust necessary to change the orbital speed.

  • Only less than 1% of the comet’s total area needs to be active to generate the effect.
  • The sublimation of carbon monoxide and dioxide acts as the prime mover.
  • Ice mixtures containing methane and ammonia supplement the propulsion force.

Neukart concluded that the conventional mechanism, driven by the physics of volatiles, accurately reproduces both the magnitude and direction of acceleration measured by ground- and space-based telescopes.

Monitoring confirms presence of water and intense activity

The validation of computational simulations was reinforced with observational data collected by large astronomical observatories. The MeerKAT radio telescope, located at África of Sul, detected chemical signatures that prove the intense activity of the comet during its passage through the inner solar system.

The instruments identified the presence of hydroxyl (OH) molecules in the object’s coma, a direct indicator of the dissociation of water molecules. The detection occurred as the comet approached perihelion, a moment when solar heat intensifies the sublimation of the ices preserved in its nucleus.

Experts from Universidade of The late detection of water is attributed to the object’s large initial distance from Sol, which kept the vapor production rate below the sensitivity limits of previous instruments.

Implications for the study of distant planetary systems

Confirmation of the physical nature of 3I/ATLAS and the absence of technological anomalies or unknown forces increase the scientific value of the object. Como a visitor from another star system, he transports materials that have remained untouched for billions of years, functioning as a time capsule for the galaxy.

Analysis of its chemical composition offers a rare opportunity for scientists to compare the matter that forms other planetary systems with that of our own Sistema Solar. The data collected helps to understand the distribution of organic and volatile elements throughout the Via Láctea.

Observations continue to be essential as the object begins its return trajectory to interstellar space. Continuous monitoring will allow us to refine cometary evolution models and better understand the diversity of protoplanetary disks spread throughout the universe.

Discarding unconventional hypotheses

Before the consolidation of the degassing model, the non-gravitational acceleration of 3I/ATLAS opened the door to several speculative theories in the scientific community.

Some hypotheses suggested that the pressure of solar radiation could be pushing an extremely light and thin object, or even considered the remote possibility of artificial artifacts.

The current study demonstrates that such conjectures are unnecessary given the robustness of explanations based on classical comet physics.

Science reaffirms that simple natural processes, when well understood and modeled, are sufficient to explain apparently mysterious phenomena in the cosmos.

Luís Henrique Costa é jornalista formado pela FMU, editor-chefe e fundador do Mix Vale, portal de notícias em atividade desde 2013. Responde pela direção editorial do veículo, que cobre Brasil e mundo em economia, benefícios sociais, esportes, tecnologia, ciência e entretenimento. Atua na área há mais de 15 anos e lidera uma equipe de cerca de 15 colaboradores.

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