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NASA researcher discovers unprecedented meteor shower originating from fragmented asteroid

Chuva de meteoros
Photo: Chuva de meteoros - Photo: Haris McHorror/ Shutterstock.com

An Nasa researcher identified a new meteor shower by analyzing millions of records captured by networks of automated cameras spread across the planet. The cluster made up of 282 meteors indicates the existence of an asteroid not yet directly observed that fragments as it approaches Sol. The study was published in the journal Astrophysical Journal in March 2026.

The data used in the research comes from observatories located at Canadá, Japão, Califórnia and Europa. Esses equipment records shooting stars continuously during the night. Enquanto Most of the fragments that generate meteors originate from comets, asteroids can also release dust and pieces when subjected to thermal stress or other physical processes.

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Nasa – JHVEPhoto/ Shutterstock.com

Formação of meteors in the Earth’s atmosphere

Quando a grain of cosmic sand penetrates the atmosphere of Terra, rapidly heating up at speeds exceeding 24 kilometers per second. The surface instantly vaporizes, forming an electrically charged gas that produces the characteristic glow for a fraction of a second. Larger Fragmentos generate brighter and more visible bolides.

Camera networks accurately capture these events in real time. Cientistas processes the collected data to determine the original orbit of the fragments prior to atmospheric entry. Esse method allows identifying debris streams that Terra periodically passes through along its orbital trajectory. Cada known meteor shower originates from a parent body, usually an active comet or asteroid.

Distinção between active comets and asteroids

Cometas are icy bodies originating from regions distant from Sistema Solar. As they approach Sol, the ice sublimates and releases dust, creating the characteristic visible tails. Asteroides, formed closer to Sol, has a rocky and dry composition in most cases.

Alguns asteroids exhibit activity when solar heat causes surface cracks or releases gases trapped inside. Asteroid 3200 Phaethon represents the best-known example, functioning as the progenitor of December’s Geminídeas. Ele releases material during passes close to Sol. The new identified current follows a low perihelion orbit, compatible with this type of intense thermal process. The meteors from the newly discovered cluster are moderately fragile, more resistant than those originating from comets, but still show signs of recent fragmentation, suggesting that the intense heat continually disintegrates the surface of the progenitor body.

Metodologia used in cluster detection

  • Análise orbital similarity statistics for more than 235 thousand recorded meteors.
  • Aplicação of specific criteria to identify compact and significant clusters.
  • Comparação with null distributions generated by advanced statistical methods to validate the significance of the results.
  • Isolamento of 282 members through computational clustering algorithm.
  • Cruzamento data between four independent camera networks for confirmation.

Essa methodological approach allowed the cluster to be highlighted even amidst the sporadic background of unassociated meteors. The study confirms that the current is recent and diffuse, concentrated in a region of the sky associated with southern Virginídeas.

Relevância for monitoring objects close to Terra

Meteor shower detection works as a sensitive probe to locate active asteroids invisible to traditional telescopes. Debris spreads throughout the orbit over time due to gravitational perturbations exerted by the planets of Sistema Solar.

Identificar these chains help map hidden populations of objects close to Terra. Essa information directly contributes to planetary defense by revealing bodies that may pass close to our planet in future approaches. The parent asteroid of the new rain has not yet been directly observed by telescopes or space probes.

Perspectivas future astronomical research

Nasa’s NEO mission Surveyor, scheduled to launch in 2027, is expected to significantly improve the detection of dark and approaching Sol asteroids. The space telescope was designed especially for planetary defense tasks and monitoring objects close to Terra. Redes cameras keep recording weather events continuously. Cientistas plans to monitor possible reinforcements of the new rain in future years to refine the progenitor’s orbit with greater precision. The discovery reinforces the value of meteor observations as an essential complement to conventional telescopes in space exploration.