Over the last two decades, scientists have found ice in many locations on Mars. Most Martian ice has been observed from orbital satellites like NASA's Mars Reconnaissance Orbiter. But determining the grain size and dust content of the ice from that far above the surface is challenging. And those aspects of the ice are crucial in helping scientists determine how old the ice is and how it was deposited.

So planetary scientists Aditya Khuller and Philip Christensen of Arizona State University, with Stephen Warren, an Earth ice and snow expert from the University of Washington, developed a new approach to determine how dusty Mars ice really is.

By combining data from NASA's Phoenix Mars Lander and Mars Reconnaissance Orbiter with computer simulations used to predict snow and glacier ice brightness on Earth, they were able to successfully match the brightness of Martian ice and determine its dust content. Their results have been recently published in AGU's Journal of Geophysical Research: Planets.

Mars is a dusty planet, so much of its ice is also dusty and much darker than fresh snow we might see on Earth. The dustier the ice is, the darker and thus warmer the ice gets, which can affect both its stability and evolution through time. Under certain conditions, this might also mean that the ice could melt on Mars.

"There is a chance that this dusty and dark ice might melt a few centimeters down," Khuller said. "And any subsurface liquid water produced from melting will be protected from evaporating in Mars' wispy atmosphere by the overlying blanket of ice."

Based on their simulations, they predict that the ice dug up by the Phoenix Mars Lander formed by dusty snowfall, sometime over the last million years, similar to other ice deposits found previously across the mid-latitudes of Mars.

"It is widely believed that Mars has experienced multiple ice ages throughout its history, and it looks like the ice being exposed throughout the mid-latitudes of Mars is a remnant of this ancient dusty snowfall," Khuller said.

For next steps, the team hopes to further analyze ice exposures on Mars, assess if the ice could actually melt, and learn more about Mars' climate history.

"We are working on developing improved computer simulations of Martian ice to study how it evolves over time, and whether it might melt to form liquid water," Khuller said. "The results from this study will be integral to our work because knowing how dark the ice is directly influences how warm it gets."

Related Links
Arizona State University
Mars News and Information at MarsDaily.com
Lunar Dreams and more

Thanks for being here; We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain. With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords. Our news coverage takes time and effort to publish 365 days a year. If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceDaily Contributor $5 Billed Once credit card or paypal		SpaceDaily Monthly Supporter $5 Billed Monthly paypal only

Trio of orbiters shows small dust storms help dry out Mars
Greenbelt MD (SPX) Aug 17, 2021
By combining observations from three international spacecraft at Mars, scientists were able to show that regional dust storms play a huge role in drying out the Red Planet. Dust storms heat up higher altitudes of the cold Martian atmosphere, preventing water vapor from freezing as usual and allowing it to reach farther up. In the higher reaches of Mars, where the atmosphere is sparse, water molecules are left vulnerable to ultraviolet radiation, which breaks them up into their lighter components o ... read more

Read more from original source...