NASA's Europa Clipper captures rare view of interstellar comet

NASA's Europa Clipper spacecraft has obtained ultraviolet observations of the interstellar comet 3I/ATLAS, filling a viewing gap when Earth and Mars telescopes were obstructed. The data reveals hydrogen, oxygen, and signs of intense gas release from the comet. These findings could provide insights into cometary formation around other stars.

In November 2025, NASA's Europa Clipper spacecraft, en route to Jupiter, unexpectedly observed the interstellar comet 3I/ATLAS using its Ultraviolet Spectrograph (UVS) instrument, led by the Southwest Research Institute. This comet, confirmed as the third interstellar object to enter our solar system in July 2025, was difficult to view from Earth due to its proximity to the Sun and suboptimal conditions from Mars.

The spacecraft's position offered a unique perspective, positioned between the comet and the Sun, allowing a view of the dust and plasma tails from behind, toward the nucleus and coma. This complemented earlier Mars observations from late September and anticipated Earth views. "We're excited that this opportunity to view another target on the way to Jupiter was completely unexpected," said Dr. Kurt Retherford, principal investigator for Europa-UVS at SwRI. "Our observations have allowed for a unique and nuanced view of the comet."

The UVS detected oxygen, hydrogen, and dust signatures, indicating high outgassing activity shortly after the comet's closest solar approach. "Europa-UVS is particularly adept at measuring fundamental transitions from atoms and molecules," Retherford explained. "We can see gases come off the comet, and water molecules break apart into hydrogen and oxygen atoms."

Simultaneously, the UVS on ESA's Jupiter Icy Moons Explorer (JUICE) provided an opposing view, aiding a fuller understanding of the tails' structure. "We're hopeful that this new view, along with observations from Earth-based assets and other spacecraft, will help us to piece together a more complete understanding of the tails' geometries," noted Dr. Thomas Greathouse, co-deputy principal investigator.

Such data on the comet's composition and gas emissions may illuminate its origins beyond our solar system. "Understanding the composition of the comet and how readily these gases are emitted can give us a clearer view of the comet's origin and how it may have evolved during transit from elsewhere in the galaxy to our solar system," said Dr. Tracy Becker, another co-deputy principal investigator. The Europa Clipper, launched in 2024, will arrive at Jupiter in 2030 for 49 flybys of Europa, studying its atmosphere and surface. The mission is managed by NASA's Jet Propulsion Laboratory in partnership with the Johns Hopkins University Applied Physics Laboratory.

Makala yanayohusiana

Astronomers using the James Webb Space Telescope have observed the ultra-hot gas giant WASP-121b losing its atmosphere over a full orbit, revealing two enormous helium tails extending across more than half its path around its star. This marks the first continuous tracking of such atmospheric escape, providing unprecedented details on the process. The findings, published in Nature Communications, highlight the complexity of exoplanetary environments.

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New measurements from NASA's Juno spacecraft suggest that the ice covering Jupiter's moon Europa is thicker than previously thought, potentially isolating its subsurface ocean from the surface. This thick barrier may complicate efforts to detect life, though alternative nutrient transport mechanisms could still exist. The findings highlight challenges for upcoming missions like the Europa Clipper.

New research indicates that salty, nutrient-rich ice on Europa could sink through the moon's icy shell to feed its hidden ocean, potentially supporting life. Geophysicists at Washington State University used computer simulations to show this process, inspired by Earth's crustal delamination. The findings address a key habitability challenge for the Jupiter moon.

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A Sun-like star 3,000 light-years away abruptly dimmed for nine months, revealing a colossal cloud of gas and dust likely from a planetary collision. Astronomers used advanced telescopes to measure metallic winds within the cloud for the first time. The event highlights ongoing chaos in ancient star systems.

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