Comparative analysis of the influence of Sgr A* and nearby active galactic nuclei on the mass loss of known exoplanets

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Table 8

Total mass loss of the older EPs (>8 Gyr) in their lifetimes.

Name	Age (Gyr)	M_lost (g)	M_lost (%)
Kepler-20 e	8.8	2.86E+18	1.55E-08
Kepler-10 b	10.6	1.29E+19	6.49E-08
CoRoT-24 b	11	1.05E+20	3.06E-07
55 Cnc e	10.2	1.30E+19	2.68E-08
EPIC 210894022 b	10.77	1.03E+19	2.00E-08

Notes. The mass loss is due to the quiescent and active Sgr A*. For this result, ɛ = 0.1, not true in reality, even when Sgr A* became an AGN.

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