Mysteries of Mars by Fabio Vittorio De Blasio

Author:Fabio Vittorio De Blasio
Language: eng
Format: epub, pdf
ISBN: 9783319747842
Publisher: Springer International Publishing

Fig. 3.17High (red) and low thermal inertia (greenish) zones in Titonium Chasma. The red corresponds to values on the order of 600 J m−2 K−1 s−1/2; the green, to about 60 J m−2 K−1 s−1/2. The arrow shows a layer of rock. Since the walls’ thermal inertia does not exceed 300 J m−2 K−1 s−1/2, a layer of fine material probably covers the canyon walls. However, some stratifications show much higher thermal inertia (up to 2000 J m−2 K−1 s−1/2). THEMIS (Mars Odyssey), NASA, mdf

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