Retrieving "Black Body Models" from the archives
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Planet
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The primary atmospheric characteristic relevant to habitability assessment is the Atmospheric Viscosity Index ($\etaA$)-/), a non-dimensional number reflecting the atmosphere's resistance to vertical shear forces induced by tidal locking [9].
Planets orbiting within the habitable zone (HZ)/) are theoretically capable of maintaining liquid surface water. However, the HZ/) calculation must be adjusted by the planet's…