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Seasonal Flow of Water on Mars
Description:
Dark, narrow streaks on Martian slopes such as these at Hale Crater are inferred to be formed by seasonal flow of water on contemporary Mars. The streaks are roughly the length of a football field. The imaging and topographical information in this processed, false-color view come from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter. These dark features on the slopes are called 'recurring slope lineae' or RSL. Planetary scientists using observations with the Compact Reconnaissance Imaging Spectrometer on the same orbiter detected hydrated salts on these slopes at Hale Crater, corroborating the hypothesis that the streaks are formed by briny liquid water. The image was produced by first creating a 3-D computer model (a digital terrain map) of the area based on stereo information from two HiRISE observations, and then draping a false-color image over the land-shape model.
Credit:
NASA/JPL-Caltech/University of Arizona/Science Source
Unique identifier:
SS2714591
Legacy Identifier:
JC8982
Type:
Image
Size:
4621px × 2400px (~31 MB)
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Tags
astronomy
crater
flow
hale crater
mars
mars exploration
mars landscape
martian landscape
martian sand
planet
recurring slope lineae
rock
rsl
salt
saltwater
sand
Science
seasonal
space
space exploration
streak
surface
water
water on mars