Although Mars is a frigid and hostile world today, the Red Planet may have once been capable of hosting some form of life. Unlike Earth, Mars lacks a strong magnetic field to protect it against incoming solar wind. As a result, the Sun\u2019s stream of charged particles may have gradually stripped Mars of its atmosphere similar to how wind blows across the surface of water, according to a new study.<\/p>\n
In a new paper<\/a> published in Science Advances, researchers describe how solar wind on Mars can stir the edges of the planet\u2019s atmosphere, creating giant, rippling waves that carry its atmospheric particles into space. The new findings provide new clues as to how Mars lost its atmosphere, and how the same process could cause other planets to evolve over time.<\/p>\n Riding the wave <\/p>\n The Sun releases a constant outflow of charged particles<\/a> in the form of solar wind, which directly interact with Mars\u2019 atmosphere. Previous research has shown that large clouds of plasma in Mars\u2019 upper atmosphere are the main culprit behind the bulk escape of atmospheric ions to space, but scientists have not been able to track down their origin.<\/p>\n \u201cMars is thought to have once been potentially habitable, with a thicker atmosphere and surface liquid water. Understanding how it became the cold, dry planet we see today is important for understanding how planetary environments evolve over time,\u201d Chi Zhang<\/a>, a research scientist at Boston University\u2019s Center for Space Physics and lead author of the new study, said in a statement<\/a>.<\/p>\n The main obstacle behind studying how these clouds of plasma form is that no single spacecraft can observe the undisturbed solar wind upstream on Mars while also measuring the atmospheric ions escaping into space. To help overcome this challenge, the researchers behind the new study relied on observations by two spacecraft: NASA\u2019s MAVEN and China\u2019s Tianwen-1.<\/p>\n Tianwen-1 monitored solar wind while MAVEN observed atmospheric ions escaping near Mars. Using simultaneous measurements from MAVEN and Tianwen-1, the researchers could connect changes in the incoming solar wind with conditions around Mars. They found that the plasma clouds are generated by Kelvin\u2013Helmholtz waves: fluid, wave-like structures that form in the atmosphere due to wind shear.<\/p>\n On Earth, a similar process occurs when wind generates rolling waves and vortices as it sweeps across the surface of water. In the case of Mars\u2019 atmosphere, solar wind stirs the edge of the planet\u2019s atmosphere and generates large boundary waves.<\/p>\n Uneven loss <\/p>\n The new study not only revealed Kelvin-Helmholtz waves as the key mechanism behind bulk atmospheric escape on Mars, it also showed that the process does not occur evenly around the planet.<\/p>\n \u201cInstead, it is mainly observed on one side of the planet, depending on the direction of the solar wind electric field,\u201d Zhang said. \u201cFuture research will focus on identifying the conditions that favor the formation and growth of Kelvin-Helmholtz waves and determining how much they contribute to atmospheric escape from Mars.\u201d<\/p>\n