Feel like going for a spin around Mars? A new video shows a 3D view of where the European-Russian ExoMars (opens in new tab) rover may land, in a region that was likely filled with water billions of years ago.
The video shows the terrain that the rover, named Rosalind Franklin (opens in new tab), will likely drive upon after its scheduled landing in 2021. In the middle of the view is an eroded crater, luckily with flat terrain toward the center, which would give Rosalind Franklin a safe area in which to touch down and wander. The crater is located in Oxia Planum, a plain located in Mars' northern hemisphere, just southwest of Mawrth Vallis, one of the biggest valleys on Mars.
The European Space Agency explained that this region could be rich with signs of past life. Rosalind Franklin is optimized to look for signs of biosignatures, including detecting organic molecules (opens in new tab) that could have arisen from life processes.
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Video: See the ExoMars Rover's Proposed Landing Site in 3D (opens in new tab)
"Oxia Planum lies at the boundary where many channels emptied into the vast lowland plains," ESA said in a statement (opens in new tab). "Observations from orbit show that the region exhibits layers of clay-rich minerals that were formed in wet conditions some four billion years ago, likely in a large body of standing water."
The video is based on high-resolution images from NASA's Mars Reconnaissance Orbiter (opens in new tab), using the close-up views available from the HiRISE (High Resolution Imaging Science Experiment) camera on board. Technicians took a few steps to translate the single-dimensional pictures into a 3D-rich video.
First, they took the raw images and combined them to form "stereo" images, which are a combination of two images that were taken of the same region but from slightly different angles. This produces an interim, 3D image. In flat regions such as Oxia Planum, however, the result is not very three dimensional.
So scientists at TU Dortmund University in Germany used a technique called "shape from shading," which involves translating the intensity of light reflected off the Martian surface into information about the surface slopes, ESA explained. The resulting 3D image provides a better estimate of the landing zone, even showing off small terrain differences in dune ripples.
These models were presented at the European Planetary Science Congress-Division for Planetary Sciences joint meeting in Geneva on Monday (Sept. 16).
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