Every morning during the Martian spring and summer, a thin, extremely long cloud emerges near the volcano Arsia Mons. Known as the Arsia Mons Elongated Cloud (AMEC), it gradually elongates until it reaches over 1,000 miles, about the distance from New York to Kansas City, before dissipating. The cycle repeats for several months. Since its first detection by a probe in 2018, scientists have been unable to explain the cloud’s existence.
Now, researchers have successfully modeled the cloud’s formation for the first time. Their results suggest it may be driven by exotic physics that has been treated as theoretical and is usually thought not to occur in nature. “We found that we needed to include some exotic physics… physics that, while included in textbooks, is treated as theoretical and usually thought not to happen in nature. It certainly hasn’t been seen in action before,” said Jorge Hernández-Bernal, a planetary scientist at Paris’ Sorbonne Université and lead author of the study, in a press release. “Once we included this physics in our simulations, the AMEC emerged just as we hoped.”
