Mars Pavonis Mons Volcano

Martian Volcanic Vent East of Pavonis Mons this image shows an equatorial plane of the volcano active on the planet mars, here are images of the Vent East of Pavonis Mons . 

As a volcano vent is still open into the crust of a planet that emits lava (molten rock) and volcanic gases. The rough texture of the plains surrounding the vent is indicative of lava. There’s a large number of snake-like features emanating from the vent. The parallel lines that outline the features are levees, which mark the edges of channels that carried molten lava. As the lava flows, it moves slowest at its edges and bottom because the lava sticks to the non-flowing rocks, and as the lava slows, it cools off and hardens. Levees form when the sides harden but the center of the flow keeps moving. As the eruption episode ends, and the lava drains, the center is left lower than the sides producing these high-standing structures. follow the glaciation from path from surface Martian telemetry.

Mars is fundamentally a volcanic planet. Geologic mapping of Mars shows that about half the surface seems to be covered with volcanic materials. 
These have been modified to some extent by other processes (such as meteorite impacts, blowing wind, and floods of water). Mars has the largest volcanoes in the entire Solar System. The great volumes of erupted lava have had a profound impact on the entire planet, extracting heat and selected chemicals from within, adding large amounts of acidic gas to the atmosphere, and providing heat to melt frozen water in the crust. Mars cannot be understood without studying its volcanoes.

HiRISE provides the ideal tool to study some of the most puzzling aspects of Mars volcanism. 
One example is: what were the eruptions that formed the giant lava flows like? Did the lava ooze quietly out of the ground or did it come blasting up in massive explosions? Detailed pictures of the vents are essential for answering these questions. We know that lava flows on Earth are usually fed by fountains or lakes of lava. HiRISE has already found examples of ancient lava lakes on Mars, but the evidence for fountains is more difficult to find. But we are finding exciting hints of cinder cones on Mars. The pictures from other cameras have been too fuzzy to show these kinds of details. Another high priority is to image places where both lava and water have come gushing from the ground. These are places where microbes that might live in the deep, warm, wet parts of the crust could have been brought to the surface. Finding scientifically interesting spots that are safe to land future rovers is one of the primary goals for the MRO mission.