  We prove that charged gravitini cannot have parametrically small or vanishing
Lagrangian mass in de Sitter vacua of extended supergravity while respecting
the magnetic weak gravity conjecture. This places large classes of de Sitter
solutions of gauged supergravity in the swampland, including all known stable
solutions of the N=2 theory. We illustrate this result by analyzing a variety
of de Sitter critical points of N=2 matter-coupled supergravity that also
include new stable de Sitter solutions. Our results provide concrete evidence
that (quasi) de Sitter with charged light gravitini should belong to the
swampland, which also strongly resonates with the festina lente bound.
