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Fig. 7

image

Temperature as a function of cometary depth for the orbital position corresponding to early August 2015. A slow rotator model is applied for Model C accounting for surface erosion. The depth is measured from the surface position after ten orbital periods (showing results for orbits 510). The primordial temperature is fixed at 30 K and the thermal inertia is set to 30 J m-2 K-1 s0.5 (upper value from MIRO analysis).

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