Mars’ glaciers are over 80% pure ice, formed by similar processes worldwide. This discovery sheds light on past climate and future exploration resources. On the slopes of Martian mountains and within its craters lie formations that look like streams of honey, blanketed in dust and frozen in place. These structures are, in fact, glaciers that […]



Summary

Mars harbors surprisingly pure glaciers, composed of over 80% water ice. These formations, resembling frozen honey streams covered in dust, are located on mountain slopes and crater floors. The dust layer protects the underlying ice from sublimation, allowing it to persist over long periods. This discovery highlights the presence of substantial water resources on Mars and offers valuable insights into the planet’s past climate. Understanding the distribution and composition of these glaciers is crucial for future Mars exploration and potential resource utilization.

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