Highlight
Free Access

Fig. 5

image

Mass loss flux as a function of temperature (Eq. (12)) for different materials, whose properties are listed in Table 3. Typical uncertainties (in temperature) are indicated by the error bars next to the legend. The horizontal lines mark the sublimation rates required to explain the observed tail lengths (Eq. (22)), with light grey bands indicating their uncertainties. The black-body temperatures (Eq. (16)) at the distance of the planets and their uncertainties are indicated by vertical line segments and dark grey patches.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.