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Venus Clouds Driven by Solar System’s Largest Waves

“Up until now, we used a global circulation model (GCM) for Venus that is similar to Earth’s, but this model doesn’t include the hydraulic jump which we have now identified,” said Dr. Takeshi Imamura. [ https://www.labroots.com/trending/space/30535/venus-clouds-d…gest-waves](https://www.labroots.com/trending/space/30535/venus-clouds-d…gest-waves)


What explains the unique behavior of Venus’ clouds? This is what a recent study published in the Journal of Geophysical Research: Planets hopes to address as an international team of scientists led by Japan and included the United States and Spain investigated a longstanding conundrum regarding Venus’ meteorology, specifically cloud weather patterns. This study has the potential to help scientists better understand planetary cloud patterns and what this can teach us about planetary formation and evolution.

For the study, the researchers used a series of computer models to simulate Venus’ cloud weather patterns, specifically focusing on a 6,000-kilometer-wide (3,728-mile-wide) cloud front whose behavior has puzzled scientists for years. The primary puzzlement is the origin of the massive cloud wave, which current global climate models can’t explain. Along with the puzzlement, the motivation behind the study also comes from a knowledge gap in the formation of the lower cloud regions within Venus’ atmosphere.

In the end, the researchers found that a phenomenon known as a “hydraulic jump” was responsible for producing the massive cloud wave front. This jump is caused by changes in airflow in the lower cloud regions combined with a strong updraft, resulting in sulfuric acid vapor (which comprises Venus’ clouds) to condense, forming the massive cloud wave front. This study helps explain the connection between the Venusian atmosphere motion and clouds.

Dual spacecraft capture both hemispheres of interstellar comet 3I/ATLAS at once

The Southwest Research Institute-led Ultraviolet Spectrograph (UVS) instruments aboard ESA’s Jupiter Icy Moons Explorer (Juice) spacecraft and NASA’s Europa Clipper made unique observations of interstellar comet 3I/ATLAS in late 2025. SwRI leads the UVS instruments on both spacecraft, simultaneously imaging both hemispheres of the comet and detecting the comet’s ultraviolet emissions.

Only the third recognized interstellar object, 3I/ATLAS, entered our solar system in July of 2025.

“As the comet passed between Juice and Europa Clipper, we were able to informally coordinate observations between the two spacecraft,” said Dr. Kurt Retherford, the principal investigator of Juice-UVS and Europa-UVS. “Crucially, we observed hydrogen, oxygen and carbon emissions. These elements are produced when gases escaping the comet’s nucleus break apart into atoms when exposed to sunlight.”

Resilient quantum sensor monitors Earth’s magnetic field from space for 10 months

From navigation to solar weather forecasting, many different areas of research require space-based sensors to measure Earth’s magnetic field as accurately as possible at any given moment. So far, however, existing sensors have consistently struggled with effects including drift, interference from the spacecraft itself, and the harsh conditions of orbit.

Through new research published in Physical Review Applied, Yarne Beerden and colleagues at Hasselt University in Belgium have developed a diamond-based quantum sensor which could offer a promising solution to these problems.

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