Titanate Clouds Above a Scorching Giant ✛

Original: "Evidence of Titanate Clouds in the Day-side Atmosphere of the Ultra-Hot Jupiter WASP-121b"
· Suman Saha, James S. Jenkins
arXiv:2508.20022 · 2025-08-27 · CC BY 4.0 · 2 min
For the first time, clouds of calcium titanate have been detected in the daytime atmosphere of the ultra-hot Jupiter WASP-121b.

The dayside of WASP-121b is scorching at 2358 kelvins, hotter than the surface of many stars. Here, in perpetual light, the atmosphere does not just boil: it melts rock and turns it into gas. But not all gas stays gaseous. Some condenses into clouds, and those clouds hide titanium the way a trap hides its prey.

Calcium titanate (CaTiO3) is the mineral perovskite, which gave its name to an entire class of materials used in solar cells.

The dayside spectrum, captured by the James Webb Space Telescope from 0.6 to 5.1 micrometers, showed something unexpected: titanium oxide (TiO) in the gas phase was far less abundant than models predicted. Instead, the data revealed signs of condensate, solid particles that scatter light. A free-chemistry retrieval (fitting an atmospheric model to the observations) yielded confident detections of water (13.4σ), carbon monoxide (14.7σ), silicon monoxide (4.9σ), titanium oxides (5.4σ), and vanadium oxides (6.6σ). The clouds were detected at 10.2σ significance, with the titanate component at 6.7σ. This is the first direct proof that titanate clouds exist in the atmosphere of any exoplanet.

The trap snapped shut: titanium, which should have remained a gas at these temperatures, has bonded into CaTiO3 crystals. That is why it is missing from the gas phase; it is hidden in the clouds. The carbon-to-oxygen ratio (C/O) turned out to be supersolar: 0.963 ± 0.024. This means the planet formed far from its star, beyond the snow line (the distance where water freezes), and then migrated inward. The metallicity, the fraction of elements heavier than helium, came out to 4.7 times solar, also pointing to a birth in the cold outskirts of the system.

An analysis of a sample of planets showed a sharp rise in C/O at an equilibrium temperature of about 1890 K, possibly a universal threshold beyond which atmospheric chemistry changes dramatically.

Previously, models of ultra-hot Jupiter atmospheres did not account for the condensation of refractory compounds into clouds, so estimates of elemental abundances could be skewed. Now it is clear that some titanium and other metals are "hidden" in particles, and this must be considered when interpreting spectra. In the future, titanate clouds will be sought on other scorching giants, and three-dimensional models will help understand how these traps are transported between the day and night sides. Thus, clouds over a distant planet become a key to the story of its birth and wanderings.

Calcium titanate (CaTiO3) is the mineral perovskite, which lent its name to an entire class of materials used in solar cells.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
titanium oxide hot jupiter atmospheres jwst exoplanet atmospheres titan water vapor exoplanet atmosphere sulfur dioxide europa jupiter wolf rayet star gas giant OISST v2.1 james webb space telescope JWST solar corona hot jupiter carbon monoxide trappist 1