NASA released spacecraft images of interstellar comet 3I/ATLAS—only the third confirmed object from beyond the solar system after 2017’s ‘Oumuamua and 2019’s 2I/Borisov—which appear as a bright nucleus with a faint, elongated tail; the photos were taken by missions including PUNCH, SOHO, MAVEN and Perseverance from late September through mid‑October but were not released until after a government shutdown delayed work. Officials say all observations to date are consistent with a natural comet (no techno‑signatures), and the object, which reached perihelion at the end of October, will reemerge from behind the Sun in early December and fly by Earth on Dec. 19 at a safe distance of roughly 170 million miles; JWST and major ground telescopes such as Keck are scheduled to observe it in December. Additional data are still being downlinked and processed, offering a rare opportunity to characterize the composition, trajectory and possible origin of extrasolar material and to refine models of small‑body populations from other star systems.
NASA released new spacecraft images of interstellar comet 3I/ATLAS — the third confirmed interstellar visitor after 2017’s 'Oumuamua and 2019’s 2I/Borisov — showing a bright nucleus with a faint, elongated tail; the photos were captured by PUNCH, SOHO, MAVEN and Perseverance from late September through mid‑October but were embargoed until the government shutdown ended. Officials, including Nicky Fox, stated observations so far are consistent with a natural comet and show no techno‑signatures, which frames the event as a scientific opportunity rather than evidence of non‑natural activity. The object reached perihelion at the end of October, will reemerge from behind the Sun in early December and will pass Earth on Dec. 19 at a safe distance of roughly 170 million miles; the James Webb Space Telescope and ground observatories such as Keck are scheduled to observe it in December. ESA’s ExoMars Trace Gas Orbiter also imaged the comet at about 18.6 million miles, and NASA notes additional data are still being downlinked, so forthcoming measurements of speed, composition and origin could incrementally refine models of extrasolar small bodies but are unlikely to produce immediate commercial knock‑on effects.
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