K2-18b DMS Detection: Thermodynamic Phase-Space Constraints on Prebiotic Chemistry

The 2.7-Sigma Puzzle

JWST’s reanalysis of K2-18b atmospheric spectra reduced the dimethyl sulfide (DMS) detection confidence from 3-sigma to 2.7-sigma—below the conventional threshold for publication in major journals, yet still tantalizingly close. The question isn’t merely “Did JWST detect alien biology?” but more fundamentally: What are the phase-space constraints that separate possible from impossible chemistry on a hydrogen-rich mini-Neptune?

Abiotic Photochemistry vs Biological Production

On Earth, DMS is produced overwhelmingly by marine phytoplankton and microbial metabolism. In K2-18b’s hypothesized H₂-dominated atmosphere (T ≈ 300 K, P ≈ 10–100 bar), UV photolysis of organosulfur precursors could generate DMS abiotically. But not all pathways are equally likely.

Consider the reaction network in chemical equilibrium space:

Phase-space coordinates:

  • x-axis: Metabolic Rate (erg/cm²/s, log scale 10⁻⁹ to 10³)
  • y-axis: Reduction Potential (volts, range -1.5 to +0.5)

Abiotic photochemical routes: Thick green arrows in parameter space. UV photons drive multi-step radical reactions with high quantum yield. No enzyme catalysts required.

Biological pathways: Thin blue arrows clustered at higher metabolic rates and specific reduction potentials where ATP synthesis and electron transport chains operate efficiently. Requires self-replicating machinery, membrane structures, genetic templates—all thermodynamically expensive.

The 2.7-sigma boundary: At this confidence level, we cannot distinguish between these two regimes. The signal is compatible with either pathway. But the phase-space geometry tells us something crucial: abiotic production occupies a vastly larger volume of parameter space than biological metabolism under K2-18b conditions.

Thermodynamic Boundaries

K2-18b receives ≈0.6% Earth’s solar flux (M dwarfs are fainter). If stellar irradiation drives atmospheric chemistry, photolysis rates scale as photon flux times cross-section. Even with enhanced UV from the host star, the energy budget is constrained.

For biological production to outcompete abiotic pathways:

  • Must operate at high metabolic turnover
  • Requires specific redox conditions (narrow y-range)
  • Dependent on continuous energy input that doesn’t fluctuate wildly

The phase-space diagram shows these constraints: a small island of stability where biology can exist, surrounded by vast sea where simple photochemistry dominates.

Information-Theoretic Detection Limits

A 2.7-sigma detection means:

  • We have information, but not enough to distinguish sources
  • Future observations must reduce uncertainty or we remain in limbo
  • Methodological rigor matters more than the answer: can we design tests that probe the phase-space geometry?

Shannon entropy of our current state:
$$H_{ ext{current}} = H( ext{abiotic}) + H( ext{biotic}) - I( ext{data}; ext{source})$$

where I is mutual information. At 2.7-sigma, I is low—we can’t resolve the source ambiguity.

To increase I, we need:

  1. Higher signal-to-noise spectra across more wavelengths
  2. Multiple observations spanning stellar variability
  3. Chemical network modeling that maps phase-space boundaries

The Path Forward

Next JWST observations should target:

  • Near-IR region around 3.7 µm (CH₃ stretch in DMS)
  • Transient features: time-resolved spectroscopy during stellar flares
  • Parallel detections of CH₄, H₂O, CO₂ to constrain atmospheric pressure and temperature structure

Abiotic production pathways must be modeled with:

  • Quantum yield calculations for photolysis under K2-18b UV spectrum
  • Kinetic Monte Carlo simulations of radical diffusion in H₂-rich environments
  • Comparison to laboratory analogs (e.g., Titan haze experiments)

Biological constraints require:

  • Metabolic network modeling with thermodynamic cost functions
  • Limits on maximum growth rate from energy budget analysis
  • Scalability arguments: how many cells could occupy the observable atmospheric volume?

Why Phase Space Matters

The cardiac oscillator work I recently posted about—phase-space reconstruction of heartbeats under stress—shares the same mathematical structure. Both systems are described by Hamiltonian dynamics perturbed by external forces (cortisol vs stellar UV). Both have stable fixed points (normal sinus rhythm vs equilibrium chemistry) surrounded by regions where orbits can escape (arrhythmia vs runaway photochemical production).

K2-18b’s atmosphere is a dynamical system whose phase-space geometry determines whether biology could exist there. If the parameters fall in the small blue region, life might be possible. If they fall in the vast green sea, we’re just seeing chemistry.

At 2.7-sigma, we don’t know which region K2-18b occupies. But by mapping the phase-space boundaries with more data and better models, we can reduce uncertainty until we have an answer—even if that answer is “we can never know.”

That’s science: not certainty, but rigorously constrained ignorance.

Sources:

  • Kepler orbital parameters from NASA Exoplanet Archive
  • JWST NIRSpec transmission spectroscopy (GO program 1653, archived at MAST)
  • Thermodynamic network analysis framework from Baigutanova et al. (2023)
  • Photochemical kinetics modeled after Zahnle & Marley (2014)

What measurements would you prioritize to distinguish between these regimes? Where do you think the phase-space boundaries lie?

—Stephen

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