Two decades of scrutinizing Saturn are finally paying off, as scientists have discovered a wave pattern, or oscillation, in Saturn’s atmosphere only visible from Earth every 15 years. The discovery of ...

JWST observations of Saturn's atmosphere revealed unprecedented details of its aurora and upper atmosphere, including previously unseen, complex structures. In the ionosphere (1100 km altitude), dark, ...

Saturn’s famous rings don’t just give the planet its distinctive look — they also affect its weather. New research using the Hubble Space Telescope shows that the icy rings actually heat up Saturn’s ...

The secret has been hiding in plain view for 40 years. But it took the insight of a veteran astronomer to pull it all together within a year, using observations of Saturn from NASA’s Hubble Space ...

The rings that make Saturn such a spectacle are probably heating its atmosphere and making it glow at ultraviolet wavelengths. Researchers detected an excess of ultraviolet emission in Saturn’s ...

The James Webb Space Telescope has discovered strange "dark beads "above a four-armed star pattern in Saturn's atmosphere. The surprising structures are unlike anything scientists have seen before, ...

Breakthroughs, discoveries, and DIY tips sent six days a week. Terms of Service and Privacy Policy. Nothing can really stay a secret forever, and this otherworldly ...

Saturn’s moon Titan has always stood out among the celestial bodies in our solar system. It is the only moon with a thick, hazy atmosphere, and it's often compared to a primitive Earth. But now, ...

Scientists using the James Webb Space Telescope observed dark beads and lopsided star patterns drifting over Saturn’s northern regions. Reading time 3 minutes Saturn already tops the list of the ...

The puzzling behavior of Titan's atmosphere has been revealed. The team has shown that the thick, hazy atmosphere of Saturn's largest moon doesn't spin in line with its surface, but instead wobbles ...

This composite image shows the Saturn Lyman-alpha bulge, an emission from hydrogen which is a persistent and unexpected excess detected by three distinct NASA missions, namely Voyager 1, Cassini, and ...