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Fig. 5


Evolution over two orbits of the mean surface temperature and the mean ice thickness of a planet orbiting a 1 L star (L00, green), a 10-2L star (L02, blue), and a 10-4L (L04, red) star on an orbit of eccentricity 0.0 (e00), 0.2 (e02), and 0.4 (e04). We note that the orbital periods are different for each case (see Tables 2 and 3).

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