The haze veiling LP 791-18 c is likely created through photochemistry, where ultraviolet radiation from the planet’s active red-dwarf star breaks apart methane molecules high in the planet’s atmosphere. The fragments recombine into…
The haze veiling LP 791-18 c is likely created through photochemistry, where ultraviolet radiation from the planet’s active red-dwarf star breaks apart methane molecules high in the planet’s atmosphere. The fragments recombine into…