Updated
Updated · New Scientist · Jun 24
Scientists Detect Carbon Monoxide on Uranus, Pointing to Ice-Rich Interior
Updated
Updated · New Scientist · Jun 24

Scientists Detect Carbon Monoxide on Uranus, Pointing to Ice-Rich Interior

2 articles · Updated · New Scientist · Jun 24

Summary

  • Carbon monoxide has been detected in Uranus’s lower atmosphere for the first time, giving fresh evidence that the planet’s interior contains far more water ice than previously thought.
  • Three ALMA observations from 2022 to 2024 found significant lower-atmosphere carbon monoxide, and researchers said only ice-rich interior models could reproduce the measured amounts.
  • The finding could narrow a long-running debate over whether Uranus formed differently from Neptune, whose abundant carbon monoxide had already pointed to an ice-rich center.
  • Carbon monoxide was also seen in Uranus’s upper atmosphere, but researchers said that signal likely came from an external source—possibly a comet impact centuries ago.
  • Some scientists cautioned the result does not fully settle Uranus’s makeup because atmospheric chemistry, mixing and interior-structure models still allow multiple rock-to-ice ratios.

Insights

What will a future probe find deep inside Uranus: a frozen core, a magma ocean, or something stranger?
Why is ice-rich Uranus a quiet, cold twin to Neptune’s stormy, hot interior?