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Overview of the generated maps used for the erosion–accumulation simulation. The visualized area is the same as in Figure 2 and Figure 3 (18.48°N; 77.37°E). Note that the crater rim runs from top right toward lower left as a curved feature, while the delta structure is located at the middle of the four images. Inset (a): sediment size map (m); inset (b): flow width map (m); inset (c): flow velocity map (m/s); inset (d): calculated flow depth map (m). Please note that the calculated depth is only a model-based approach that should be further improved in the future. The coarse sand fraction grains are primarily located in the riverbed that flows into the Jezero Crater.

Overview of the generated maps used for the erosion–accumulation simulation. The visualized area is the same as in Figure 2 and Figure 3 (18.48°N; 77.37°E). Note that the crater rim runs from top right toward lower left as a curved feature, while the delta structure is located at the middle of the four images. Inset (a): sediment size map (m); inset (b): flow width map (m); inset (c): flow velocity map (m/s); inset (d): calculated flow depth map (m). Please note that the calculated depth is only a model-based approach that should be further improved in the future. The coarse sand fraction grains are primarily located in the riverbed that flows into the Jezero Crater.

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Identifying surface sites with significant astrobiological potential on Mars requires a comprehensive understanding of past geological processes and conditions there, including the shallow subsurface region. Numerical modelling could distinguish between regions dominated by erosion and those characterized by sediment accumulation in ancient wet env...

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... To achieve the goal of this study, we recognized the need to select regions on Earth that exhibit geomorphological characteristics similar to those observed on interesting sites on Mars, such as Jezero crater (e.g., [9,10]). This Martian crater, with a diameter of approximately 49 km, and located to the northwest of the Isidis impact basin on Mars, displays unique features suggesting a history rich in fluvial activity [11]. ...
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