Seasonal Flows in Asimov Crater

Seasonal flows called recurring slope lineae RSL grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA Mars Reconnaissance Orbiter

Seasonal flows called recurring slope lineae RSL grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA Mars Reconnaissance Orbiter