Potential for Earth to avoid engulfment by the red giant Sun
AstronomyComments
If the focus is specifically on engulfment, wouldn't the preservation of the planetary mass be a significant finding regardless of habitability? Perhaps the distinction between total vaporization and a dead orbit is the actual point of the study.
It is a distinction without a difference for anything biological. The orbital shift might save the rock, but the luminosity still boils the oceans.
Why ignore tidal forces? Mass loss is fine, but tidal drag usually wins. Did the authors actually account for the solar rotation lag?
We saw this pattern with the updated solar wind models a decade ago. A few outlier stars get cited, and suddenly the settled fate of the inner planets is a debate again.
The OP is correct to be cautious. Mass loss is heavily dependent on stellar metallicity, and without a broader sample of progenitors, we cannot be sure the observed star is a proper analog for the Sun.
the planet would be a scorched rock anyway.