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Explore Mars with JMARS
"The THEMIS infrared camera imaged the same impact craters in both daytime and nighttime. Infrared images depict the heat materials emit.
Warmer areas appear brighter
and cooler areas darker.
Fine-grained materials like dust
cool quickly after sundown, so
they appear dark in the nighttime
image, while rocky areas cool
slowly and appear lighter. The
extent of rocky material ejected
from the craters can be clearly
mapped. The daytime image
resembles one taken in visible
light, because Sun-facing slopes
are warmer and shaded areas
cooler."
Mars Odyssey, THEMIS
NASA/JPL/Arizona State University image
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