Astronomers track interstellar comet at Keck Observatory AI illustrationhow this picture was madeMAUNAKEA, Hawaii, Oct. 16, 2026 - Astronomers have released extended optical observations tracking the interstellar comet 3I/ATLAS through its closest approach to the Sun, showing sustained active morphology across the perihelion period. [1]
The work combines survey data captured in June and July 2026 by the Vera C. Rubin Observatory's Legacy Survey of Space and Time, with targeted high resolution imaging taken 7 October at the W. M. Keck Observatory. [2]
The observing team first obtained calibrated spectra of the comet using Keck's Low Resolution Imaging Spectrometer on 15 May 2026, building a continuous observation window spanning more than five months for the interstellar visitor. [3]Impact Insight. Interstellar comets are objects that formed outside our Solar System before being deflected inward on a single unbound pass. Extended tracking across perihelion allows researchers to measure how these visitors respond to solar heating, and to compare their physical composition to native Solar System bodies. For planetary defense, interstellar visitors arrive with little warning, so tracking and characterising them quickly is the same skill needed for any unexpected object.MAUNAKEA, Hawái, 16 de octubre de 2026, Astrónomos han publicado observaciones ópticas extendidas que registran el paso del cometa interestelar 3I/ATLAS por su punto de máxima aproximación al Sol, demostrando una morfología activa sostenida durante todo el periodo del perihelio. [1]
Este trabajo combina datos de muestreo capturados en junio y julio de 2026 por el Estudio Legado del Espacio y el Tiempo del Observatorio Vera C. Rubin, con imágenes de alta resolución específicas obtenidas el 7 de octubre en el Observatorio W. M. Keck. [2]
El equipo de observación obtuvo primero los espectros calibrados del cometa utilizando el espectrógrafo de imágenes de baja resolución de Keck el 15 de mayo de 2026, construyendo una ventana de observación continua de más de cinco meses para este visitante interestelar. [3]Perspectiva de impacto. Los cometas interestelares son objetos que se formaron fuera de nuestro Sistema Solar antes de ser desviados hacia su interior en un único paso no ligado. El seguimiento extendido durante el perihelio permite a los investigadores medir cómo responden estos visitantes al calentamiento solar, y comparar su composición física con los cuerpos propios del Sistema Solar. Para la defensa planetaria, los visitantes interestelares llegan sin aviso previo, por lo que la capacidad de seguirlos y caracterizarlos rápidamente es la misma habilidad necesaria para cualquier objeto no esperado.
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Optical observations from the Legacy Survey of Space and Time (LSST) at the NSF-DOE Vera C. Rubin Observatory conducted in June and July 2026, combined with Keck/LRIS imaging on October 7, showed active morphology across perihelion over 102 days. · arXiv.org
The observations were conducted at the W. M. Keck Observatory on Maunakea, a site operated by the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. · The Astronomer's Telegram
Astronomers Bryce Bolin, Ian Wong, Leo Alcorn, Matthew Belyakov, Percy Gomez, and Heather Hershley observed the interstellar comet 3I/ATLAS using the Low Resolution Imaging Spectrometer on the 10-meter Keck I telescope on May 15, 2026. · The Astronomer's Telegram
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