Direct answer: No source in the supplied evidence reports survival fractions of Earth-analogue planets in binaries from an N-body grid, so the number cannot be stated from data β it must be produced by a new simulation. The literature provided only establishes the ingredients: (1) binaries are dynamically hostile zones whose stability depends on separation and mass ratio (the 1974 premise, now known to be an over-generalization since planets do form and survive in binaries); (2) post-formation N-body evolution over 100 Myr preserves most planets in isolated systems but reshapes eccentricities β the same machinery needed for the binary grid; (3) modern N-body/TTV pipelines (jnkepler, SPOCK, exoplanet in JAX) are the validated toolchain for such experiments
Curve is a BGPT parametrized expectation around the empirical critical periastron boundary; it must be replaced by the actual N-body histogram output of the grid.
Confidence note: high confidence that the empirical answer is absent from supplied sources and that the toolchain above is the validated route; the plotted fractions are assumptions to be falsified by the run.
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