Polar Regions - page 3
Mars' Polar Regions
When the Martian polar caps were first viewed through telescopes, most scientists believed that they were made of water ice, like the polar caps on Earth. Like Earth, Mars has a North and South Pole. But while Earth's polar ice caps consist solely of water ice, Mars' polar caps are a combination of water ice and carbon dioxide ice. As the Martian seasons change, the carbon dioxide ice sublimates (vaporizes) in summer, revealing the surface, and freezes again in winter. As fall approaches, in each respective hemisphere, clouds begin to form over the polar region and the ice cap begins to grow. In spring, the polar caps recede.
The Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) acquired this image of the Martian north polar cap in early northern summer. The north polar cap is about 1100 km (680 miles) across. (Image Credit: NASA/JPL/Malin Space Science Systems)
Aside from ice, Mars' polar regions have some interesting geologic features. The north polar dune field is a vast concentration of sand dunes that stretches around the entire north polar cap. In some areas, the sand measures up to 500 km (300 miles) across. When the dunes begin to thaw in spring, dark spots form on their surfaces. The north polar dunes were first seen during the 1972 mapping of Mars by Mariner 9, and they are identical to dunes in Earth's desert regions.
Satellite imagery also shows the presence of polygon-patterned ground in Martian high latitudes. On Earth, polygons typically form in polar regions as a result of repeated freeze and thawing of ground ice. Some scientists believe that polygons on Mars could be an indicator of subsurface water ice.
This Mars Orbiter Camera image shows frozen carbon dioxide in Mars' south polar residual cap. (Image Credit: NASA/JPL/Malin Space Science Systems)
Just a few decades ago, nobody knew for certain what the Martian surface looked like. But in the 1970s, Mars orbiter and lander missions began producing striking images of Martian geomorphology. Now, satellite imagery and photos enable scientists to see landforms and the shape of the terrain at the Martian poles.
This image of sand dunes in the north polar region of Mars covers an area about 3 km (1.9 miles) across. As the sand dunes begin to defrost in mid-spring, dark spots form on their surfaces. (Image Credit: NASA/JPL/Malin Space Science Systems)
Poles in the Solar System
Say the words South Pole and North Pole and you'll most likely conjure up images of a barren, frozen territory. This is an accurate description of the polar regions on Mars and Earth, but are polar regions on all planets in the solar system alike? Because Mercury is so close to the Sun, could its polar regions be boiling oceans?
Although we know a lot about the poles on Earth and Mars, much less is known about the poles on the other seven planets in our Solar System. But thanks to advanced telescopes and data from spacecraft orbiter missions, scientists are now learning some interesting facts about polar regions on other planets.
This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows polygon-patterned ground in Mars' south polar region. Polygons are fairly common at high latitudes in both Martian hemispheres. (Image Credit: NASA/JPL/Malin Space Science Systems)
Phoenix Landing Site
The Phoenix Mars Lander will touch down in the northern arctic plains of Mars at a site between 65° and 72° North, a region where the Mars Odyssey observed a reservoir of near-surface ground ice.
Given the extreme, cold conditions of polar regions, you might wonder why the Phoenix Mission would choose the arctic plains as a landing site. Actually, many factors make this an ideal location to conduct the Phoenix experiments. First, Phoenix will land during the retreat of the Martian northern polar cap, when soil is first exposed to sunlight after a long winter. The interaction between the ground surface and the Martian atmosphere that occurs at this time is critical to understanding Mars' climate history.
This NASA Hubble Space Telescope image shows a close-up view of an electric-blue aurora eerily glowing in Jupiter's north polar region. (Image Credit: NASA/Hubble Heritage Team; Acknowledgment: NASA/ESA, John Clarke - University of Michigan)
Second, since the sun never sets during the Martian polar summer, Phoenix can take advantage of maximum sunlight, which is essential to the two solar panels that Phoenix will deploy as an energy source for the robotic arm and other instruments. Sunlight is also important for keeping batteries warm, which will store electrical power.
Lastly, the ice-rich soil in the Martian polar regions may be the only place on Mars where microbial life can survive, and sampling in this region could provide researchers with insight into the planet's habitability.
Although the polar regions probably wouldn't be an ideal location for a long-term base during human missions to Mars, due to the long Martian winter (about one Earth year long), they might be the best place to set up a seasonal base during the summer. Scientists now know that there is water at the Martian poles, which would be an important consideration for human missions.
Three potential landing regions (boxes) for the Phoenix Mars Lander are shown. Currently, the Phoenix team is actively working on selecting a landing site. (Image Credit: NASA/UA/Wash. U)