Odyssey image
Vital Statistics
Location:
11.7N, 90.4E
Released:
2003-12-24
Image Size:
18.4 x 65.7 km, 1024 x 3648 px
Resolution: 18m Instrument: VIS
Medium-size image for 20031224a
Image Credit: NASA/JPL/ASU
 
Image Context:
Context image for 20031224a
Wide Context:
Wide context image for 20031224a
Context image credit: NASA/JPL/MOLA
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Detailed information on this image is available at the THEMIS Data Releases website.
 
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
 
This THEMIS image covers a portion of the Isidis Basin at the center of an elliptical region predicted to be the location that Beagle 2 will bounce to the surface. The surface is pockmarked by strange pits and unusual cones whose origin remains enigmatic. The cones may be the result of lava flowing over ice or water-rich ground resulting in explosions of steam that build small “rootless” volcanoes. The pits look like secondary craters that result from the impact of ejecta from larger craters. But they appear too numerous and densely clustered for that explanation. Instead, they also may be the result of some process involving water or ice. With luck, Beagle 2 will survive its violent landing and provide clues to the origin of this unusual landscape and answer questions about the role of water in Mars history. UPDATE: Contact with Beagle 2 was never established after landing. It is likely that Beagle 2 crashed into the surface of Mars.
 
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THEMIS Image of the Day: A Martian Christmas Present (Released 24 December 2003)