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The view from HD 131399Ab would be spectacular if not for the ferocious winds, the lack of solid ground, and a steady rain of liquid iron.
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Imagine a world where the average daytime temperature is -179°C, and torrential rains of liquid methane fall from the skies, forming vast but shallow pools that cover an area larger than the Great Lakes.
The Cassini–Huygens mission to Titan discovered clouds formed from methane or ethane which deposit rain composed of liquid methane and other organic compounds.
It has a thick atmosphere and weather similar to ours, although instead of water, its sea, lakes and rain are composed of liquid methane.
Titan's surface, like Earth's, is sculpted by wind and probably also rain (in the form of liquid methane).
Precipitation in the form of liquid (rain) or solid (snow) varies in composition depending on atmospheric temperature, pressure, composition, and altitude.
Later, it is thought, much of the water vapour in the atmosphere condensed to form clouds and rain that left large deposits of liquid water on Earth's surface.
The Huygens probe that visited Titan in 2005 found evidence of liquid methane raining down on its surface, as well as a mix of water and ammonia seeping up from its interior.
Wind-driven rain has the potential to deposit large amounts of liquid water on the exterior surface, as well inside walls through rain penetration, providing a significant source for moisture transport.
Outside the tent-flap, the rain has turned the ground into a churn of liquid mud.
Celestial bodies classified as brown dwarfs exhibit planetlike weather with clouds of liquid metals and thunderstorms of liquid iron rain, researchers have discovered.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com