On the floor of Mars, there are quite a few options that inform of a previous age when the planet was hotter and wetter, with rivers, lakes, and even an ocean that lined a lot of its northern hemisphere. These embody river channels, delta followers, sedimentary deposits, and low-lying areas wealthy in clay minerals. The invention and examine of those options over the previous fifty years have raised some urgent questions for scientists. These embody the query of how a lot water as soon as flowed on Mars and what led to the gradual transition that left the planet a frigid, desiccated world, the place the one water on the floor comes within the type of ice and permafrost.
In response to new research by a workforce of Japanese researchers, the reply might lie deep inside Martian craters that comprise deposits of water ice. Much like how glaciers on Earth report cycles within the Earth’s local weather stretching again eons, these craters comprise layers of ice which are primarily a report of the planet’s previous. In response to their paper, which appeared within the journal Geology, these craters reveal that Mars skilled a number of ice ages over a whole lot of hundreds of thousands of years. Nonetheless, the quantity of ice decreased steadily, indicating that Mars misplaced its water over the course of eons.
The analysis was led by Trishit Ruj, an affiliate professor from the Institute for Planetary Materials at Okayama College and the chief of its Planetary Geology and Surface Simulation Laboratory (PGSSL). He was joined by researchers from the Kochi Institute for Core Sample Research, the International Research School of Planetary Sciences, Kochi College, Brown College, the College of Tokyo, and the JAXA Institute of Space and Astronautical Science (ISAS).
Modifications in Mars’ axial tilt (obliquity) drive shifts between polar ice caps at low obliquity and widespread mid-latitude glaciation at excessive obliquity. Credit score: Ruj, T. et al. (2025).
The workforce targeted their examine on the glacial landforms preserved in craters between 20°N and 45°N latitude utilizing high-resolution photographs taken by the Context Digital camera (CTX) and the Excessive-Decision Imaging Science Experiment (HiRISE) aboard NASA’s Mars Reconnaissance Orbiter (MRO). They additional targeted on craters that had all of the indications of glaciation, like ridges, particles left behind by ice sheets, and maze-like pit formations and in contrast their shapes and orientations to local weather fashions.
This revealed that the ice in these craters constantly clustered within the shadowed southerwestern partitions. What’s extra, this was constant over the course of a number of glacial intervals all through the Amazonian interval (from ca. 640 to 98 million years in the past). Stated Dr. Ruj in an Okayama College press release:
Mars went by repeated ice ages, however the quantity of ice deposited in craters steadily shrank over time. These icy ‘time capsules’ not solely reveal how Mars misplaced its water but in addition mark locations the place future explorers may faucet into hidden ice sources.
Like Earth, these shifts in Mars’ local weather had been attributable to adjustments within the planet’s axial tilt (obliquity), which is equally inclined as Earth’s (about 25 levels in comparison with Earth’s 23.4 degree-tilt). In contrast to Mars, Mars obliquity can change dramatically over the course of eons, triggering intervals of glaciation and thaws that step by step left much less ice with every cycle. These outcomes exhibit that Mars dried step by step all through the Amazonian Period, the most recent (and longest) geological interval in Martian historical past.
The workforce’s analysis may additionally act as a information for future crewed missions that might want to depend on locally-sourced water ice to develop meals, produce oxygen gasoline and ingesting water, and vogue propellant. Given the space between Earth and Mars and the truth that it takes spacecraft six to 9 months to make a one-way transit (utilizing standard propulsion), in-situ useful resource utilization (ISRU) can be an absolute necessity. What’s extra, this examine may even have functions right here on Earth, the place local weather change is inflicting the ice caps and glaciers to shrink with each passing 12 months.
*Artist’s impression of NASA’s Mars Reconnaissance Orbiter (MRO) within the skies above Mars. Credit score: NASA*
Globally, rising temperatures are resulting in elevated charges of drought, forest fires, soil erosion, and flooding, which is putting elevated stress on diminishing provides of contemporary water. On this sense, the identical imaging and modeling instruments used to review how the Martian local weather has advanced may assist scientists monitor glaciers, permafrost, and hidden caches of water right here on Earth. Along with serving to future generations of explorers reside and thrive on one other planet, these strategies may additionally help folks reside in an more and more altering surroundings right here at dwelling.
“Mars serves as a pure laboratory for understanding how ice behaves over huge timescales,” mentioned co-author Dr. Hasegawa from Kochi College, The insights we achieve right here can sharpen our understanding of local weather processes on Earth as nicely.”
Additional Studying: Okayama University, Geology
.webp){kind=small}
