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Glossy Silicate Clouds on the Scorched Dayside of LTT9779b

Authors: Suman Saha, James S. Jenkins, Jonathan Brande, Reza Ashtari, Ian J. M. Crossfield, Sarah Stamer, Diana Dragomir, Kevin B. Stevenson, Vivien Parmentier, Thomas M. Evans-Soma, Tansu Daylan, Hayley Beltz, Emma Esparza-Borges

Suman Saha et al 2026 The Astrophysical Journal Letters 1005 .

Provider: AAS Journals

Caption: Figure 1.

Equilibrium temperature versus planetary radius for known transiting exoplanets. The UHN LTT9779b is highlighted as the red star. The purple shaded region indicates the Neptunian radius regime, whereas the green shaded region demarcates the “Neptunian desert.”

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