text:   Temperatures I: Thermal Structures and Broadband Phase Curve Predictions",6,"['🗣 New paper alert! <LINK> In this work, led by Michael Roman, we present a grid of 3D models of hot Jupiters with clouds (temperature dependent and with radiative feedback) across a wide range of irradiation temperature, for different assumed cloud properties. <LINK>', 'In order of decreasing irradiation temperate, clouds form successively on: the night, the cool western terminator, the eastern terminator, and even across the dayside!', 'For planets cooler than irradiation temperatures of about 3000 K (Teq ~ 2100 K) clouds influence observable properties, like phase curves (both thermal and reflected)!', 'Sometimes clouds even produce temperature inversions!', 'Also see a lovely complementary paper by @V_Parmentier that is also on arXiv today!', '(Sorry this thread isn’t snazzier... my kindergartener needs help with his class work and is crying in my lap right now)']",20,10,862