Now the rover is checking out a layer enriched with sulfates– salty minerals that often form as water evaporates.Pan around inside this 360-degree video to see Gediz Vallis channel from the point of view of NASAs Curiosity Mars rover. Only after these lengthy procedures– as well as intensely dry durations during which the surface of Mount Sharp was a sandy desert– could the Gediz Vallis channel have been carved.Scientists believe the boulders and other particles that subsequently filled the channel came from high up on the mountain, where Curiosity will never go, offering the team a peek of what kinds of product may be up there.The steep course NASAs Curiosity Mars rover took to reach Gediz Vallis channel is indicated in yellow in this visualization made with orbital information. These cycles can be seen in evidence of mud cracks; shallow, salty lakes; and, straight listed below the channel, cataclysmic particles streams that stacked up to produce the sprawling Gediz Vallis ridge.Last year, Curiosity made a challenging climb to study the ridge, which drapes throughout the slopes of Mount Sharp and appears to grow out of the end of the channel, suggesting both are part of one geologic system.Viewing the Channel Up CloseCuriosity recorded the channel with a 360-degree black-and-white panorama from the rovers left navigation electronic camera.
Curiositys expedition of the Gediz Vallis channel on Mars uses new insights into the worlds past, exposing a potential history of water flows and climatic changes that challenge previous beliefs about Mars aridity. Now the rover is checking out a layer enriched with sulfates– salted minerals that frequently form as water evaporates.Pan around inside this 360-degree video to see Gediz Vallis channel from the point of view of NASAs Curiosity Mars rover. Just after these lengthy procedures– as well as intensely dry durations throughout which the surface of Mount Sharp was a sandy desert– could the Gediz Vallis channel have actually been carved.Scientists believe the boulders and other debris that subsequently filled the channel came from high up on the mountain, where Curiosity will never ever go, giving the group a glance of what kinds of material may be up there.The steep path NASAs Curiosity Mars rover took to reach Gediz Vallis channel is indicated in yellow in this visualization made with orbital data. These cycles can be seen in evidence of mud cracks; shallow, salty lakes; and, straight listed below the channel, cataclysmic particles flows that piled up to develop the sprawling Gediz Vallis ridge.Last year, Curiosity made a challenging climb to study the ridge, which drapes across the slopes of Mount Sharp and seems to grow out of the end of the channel, recommending both are part of one geologic system.Viewing the Channel Up CloseCuriosity documented the channel with a 360-degree black-and-white panorama from the rovers left navigation video camera.
