Red Planet, Blue Past: Watermarks of a Young Mars

Mars as you’ve never seen it: not a billion-year-old desert, but a world shaped in just a few centuries. Within a young-Earth creation framework (6–7 ka BP), this paper models a Mars that began with a powerful magnetic field, a dense volatile-rich atmosphere, and abundant water above and below its surface. Using Humphreys’ exponential decay theory, MAVEN ion escape data, SNC meteorite volatiles, and high-resolution geomorphic imagery, I reconstruct a catastrophic early hydrologic episode consistent with a biblical timescale.

Key findings include:

Magnetic collapse: Decay constant τ ≈ 535 yr implies >99% field loss within ~3000 yr.

Atmospheric stripping: Without shielding, ~0.6 bar could vanish in only 200–400 yr.

Transient hydrosphere: Steam atmospheres >0.6 bar persist for weeks–months after outgassing/impacts.

Rapid geomorphology: Jezero’s 6 km³ delta could form in <1 yr at peak modeled runoff.

This integrated scenario reproduces NASA/ESA datasets (MGS, MAVEN, HiRISE/CTX) without invoking billions of years. Crater counts are reinterpreted as post-catastrophe impact fluxes, and crustal magnetic anomalies confirm a strong primordial field. Together, these lines of evidence argue for a short-lived but intense episode of habitability on Mars, fully consistent with the Genesis timescale.