Solar-type stars emit a nearly constant EUV flux for their first ~70 million years, then decay as a power law, so the young Sun flooded its planets with about 100 times today's EUV.
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A Semi-Empirical Estimate of Solar EUV Evolution from 10 Myr to 10 Gyr
Solar-type stars emit a nearly constant EUV flux for their first ~70 million years, then decay as a power law, so the young Sun flooded its planets with about 100 times today's EUV.