
The planet Mars shares many landforms and weather patterns with the Earth, including changing seasons, volcanoes, canyons, dust storms and dust devils, and water ice. But one feature that Earth and Mars share among the eight planets in our solar system are polar ice caps. Both are one of each planet’s striking features, but the major difference is while Earth’s polar ice caps are both comprised of water, Mars’ north polar ice cap is only comprised of water while its southern polar ice cap is carbon dioxide. The reasons for this are determined by altitude, but Mars’ northern polar ice cap is one of the most studied regions primarily due to its water ice composition. But how does the north polar ice cap water ice change with the seasons compared to Earth, and what can this teach scientists about Mars’ climate history?













![A view of the Taurus Molecular Cloud from the Herschel Space Observatory. The bright region at the lower left is the pre-stellar core Lynds 1544. Astronomers looked at it using radio astronomy techniques to understand what's happening in a prestellar core. [ESA/Herschel/SPIRE]](https://www.universetoday.com/article_images/Taurus_molecular_cloud_20261028_002429.jpg)
































