Heavy water ice found in planet-forming disk ✎ express

Original: "First detection of HDO ice in a protoplanetary disk"
arXiv:2606.10888 · 2026-06-09 · arXiv non-exclusive · independent analysis · 1 min
For the first time, the Webb telescope has spotted heavy water ice in a disk where planets are born.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

The James Webb Space Telescope peered into a disk of gas and dust around a young star where planets are born, and for the first time spotted ice made of heavy water. This water is not ordinary: in its molecules, regular hydrogen is replaced by deuterium, its heavier sibling. Such water is like a diary page, holding chemical clues from the past.

Measurements revealed an anomalously high amount of heavy water in the disk — more than in comets or meteorites. This means the ice repeatedly melted and refroze, accumulating deuterium. This cycle could explain how water arrived on Earth: some of it may be older than the Sun itself: it came from interstellar space.

Now that diary page has been read, it tells the story of water that crossed the galaxy to become our planet's oceans.

Every liter of seawater hides a few drops of heavy water. It tastes slightly sweet but is harmless.

Scientists
Charles-Augustin de CoulombJohannes RydbergTheodore LymanDaniel BernoulliLeonhard EulerArchimedes
Concepts
protoplanetary disk chemistry protoplanetary disk snow line dust planetary composition formation planetary accretion chemistry water detection water ice gap cold gas young star chemical galactic archaeology organic molecules in space first stars nucleosynthesis stellar chemical abundances sub neptune formation gas first stars titanium oxide carbon to oxygen ratio