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Webb spots first hints of atmosphere on a potentially habitable world

Hints of an atmosphere on TRAPPIST-1e raise hopes it could be a watery, potentially habitable world. Astronomers using the James Webb Space Telescope are unraveling the mysteries of TRAPPIST-1e, an Earth-sized exoplanet 40 light years away that could harbor liquid water. Early data suggests hints of an atmosphere, but much remains uncertain. Researchers have already ruled out a hydrogen-rich primordial atmosphere, pointing instead to the possibility of a secondary atmosphere that could sustain oceans or ice.

University of Bristol astrophysicists are helping shed new light on an Earth-sized exoplanet 40 light years away where liquid water in the form of a global ocean or icy expanse might exist on its surface.

That would only be possible if an atmosphere is present – a big mystery the scientists are attempting to unravel and now even closer to solving using the largest telescope in Space.

Hera’s first year in space

What a difference a year makes! Today Hera’s asteroid mission for planetary defence is cruising through deep space on the far side of the Sun, headed to its final destination: the Didymos binary asteroid system. But a year ago, on 7 October 2024, it was unsure if the mission was ever going to take off at all.

Cassini proves complex chemistry in Enceladus ocean

Scientists digging through data collected by the Cassini spacecraft have found new complex organic molecules spewing from Saturn’s moon Enceladus. This is a clear sign that complex chemical reactions are taking place within its underground ocean. Some of these reactions could be part of chains that lead to even more complex, potentially biologically relevant molecules.

Published in Nature Astronomy, this discovery further strengthens the case for a dedicated European Space Agency (ESA) mission to orbit and land on Enceladus.

In 2005, Cassini found the first evidence that Enceladus has a hidden ocean beneath its icy surface. Jets of water burst from cracks close to the moon’s south pole, shooting ice grains into space. Smaller than grains of sand, some of the tiny pieces of ice fall back onto the moon’s surface, while others escape and form a ring around Saturn that traces Enceladus’s orbit.

Physicists detect water’s ultraviolet fingerprint in interstellar comet 3I/ATLAS

For millions of years, a fragment of ice and dust drifted between the stars—like a sealed bottle cast into the cosmic ocean. This summer, that bottle finally washed ashore in our solar system and was designated 3I/ATLAS, only the third known interstellar comet. When Auburn University scientists pointed NASA’s Neil Gehrels Swift Observatory toward it, they made a remarkable find: the first detection of hydroxyl (OH) gas from this object, a chemical fingerprint of water.

Swift’s space-based telescope could spot the faint ultraviolet glow that ground observatories can’t see—because, high above Earth’s atmosphere, it captures light that never reaches Earth’s surface.

Detecting water—through its ultraviolet by-product, hydroxyl—is a major breakthrough for understanding how interstellar comets evolve. In solar-system comets, water is the yardstick by which scientists measure their overall activity and track how sunlight drives the release of other gases. It’s the chemical benchmark that anchors every comparison of volatile ices in a ’s nucleus.

New study rules out binary hardening as cause of Dimorphos’s orbital period drop

A new study has challenged a popular explanation for the unexpected 30-second shortening of Dimorphos’s orbital period. The researchers found that the proposed mechanism would actually produce the opposite effect, given the gravitational dynamics of the small moon. The paper has been accepted for publication in Astronomy & Astrophysics and is currently available on the arXiv preprint server.

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