In a discovery that feels straight out of science fiction, astronomers using the James Webb Space Telescope (JWST) have captured the most detailed images yet of two young exoplanets—YSES-1b and YSES-1c—revealing swirling silicate clouds and a rare moon-forming disk in a planetary system 300 light-years away.
The YSES-1 system, orbiting a sun-like star, is just 16.7 million years old—an infant in cosmic terms. Yet it’s already rewriting what we thought we knew about planetary formation. The outer planet, YSES-1c, stunned scientists with its atmosphere filled with silicate clouds—essentially, space-born sandstorms. These clouds are made of minerals like pyroxene and forsterite, and they behave much like water vapor on Earth, cycling through sublimation and condensation. The result? A planet where it literally rains sand.
Meanwhile, the inner planet, YSES-1b, is still forming and is surrounded by a circumplanetary disk—a flattened ring of dust and gas that may be actively building moons. This is only the third such disk ever observed, and the first around a planet this old, raising new questions about how long these moon nurseries can survive.
What makes this discovery even more remarkable is that both planets were directly imaged by JWST, a feat possible only because of their wide orbits—five to ten times the distance between the Sun and Neptune. This allowed astronomers to bypass the blinding glare of the host star and capture high-resolution spectra of the planets’ atmospheres.
The implications are profound. These observations offer a rare glimpse into the early stages of gas giant evolution and provide a living laboratory for understanding how planets like Jupiter and Saturn may have formed. They also challenge existing models of planetary system development, especially regarding how long circumplanetary disks can persist.
As JWST continues to peer deeper into the cosmos, discoveries like this remind us that the universe is not only stranger than we imagine—it’s stranger than we can imagine.
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