Subsurface temperature maps of 67P/Churyumov–Gerasimenko, showing the southern hemisphere of the comet. The maps are based on observations obtained with the Microwave Instrument for the Rosetta Obiter (MIRO) at millimeter (left) and sub-millimeter (right) wavelengths between September and October 2014. The MIRO data are projected on a digital shape model of the comet. A temperature bar (in degrees Kelvin), is to the right. Credits: ESA/Rosetta/NASA/JPL-Caltech
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