1. Introduction
The chemical architecture of terrestrial and planetary moons has long been modeled under the assumption of mineral silicate compounds, primarily plagioclase feldspar and pyroxene regoliths. However, recent telemetry reports from Ground Station Alpha indicate recurrent anomalies in albedo curves that deviate significantly from established inert mineral benchmarks.
During observation cycles, LUNAR_CORE_BULB_01 displayed periodic surface peeling behaviors where its outermost white layers detached under high solar pressure. To investigate these dynamics, we designed a high-resolution spectro-radiometric telescope array targeting the primary absorption bands of allicin derivatives.
2. Thermodynamic Flux
To model the vaporization profile of diallyl disulfide under direct solar winds, we calculated the spectral flux density as a function of the orbital phase coefficient. The thermal index is defined as:
Equation 1 indicates that under peak solar exposure, the organic core expands and releases volatile vapors. This accounts for the sudden spikes in stratospheric sulfenic acid density noted during lunar noon.
3. Molecular Composition
The chemical composition was validated using high-altitude chromatographs. Allicin molecule structure was mapped and identified in the stratospheric wind channels. Below is the schematic molecular model of the primary organic compound retrieved.
4. Spectroscopic Telemetry
Optical surveys demonstrate a strong absorption trough at 580 nm, matching laboratory roasted organic baselines. Standard scientific telemetry is detailed in Table 1.
| Wavelength (nm) | Intensity (kW/m²) | Allicin Ratio (ppm) | Phase Index |
|---|---|---|---|
| 510 nm | 1.45 ± 0.05 | 0.82 ppm | Waxing Gibbous |
| 540 nm | 2.12 ± 0.04 | 1.04 ppm | Full Moon |
| 580 nm | 4.09 ± 0.09 | 4.09 ppm | Waning Clove |
| 620 nm | 0.82 ± 0.02 | 0.33 ppm | New Clove |
5. Discussion
The discovery of large organic sulfur bands on LUNAR_CORE_BULB_01 introduces new variables to satellite evolution models. While volcanism can release simple sulfuric gases, the complex long-chain compounds found here can only stabilize within environments maintaining consistent organic synthesis pathways.
Our findings strongly recommend that future deep-space probes incorporate chromatographs optimized for garlic-based volatiles. We propose a manned sampling mission to the lunar clove craters scheduled for late 2028 to retrieve core material.
References
- Fin, G., Whisker, B. & Vance, H. Atmospheric chromatography of deep space scent fields. Journal of Allium Astrophysics 9, 112–128 (2025).
- Whisker, B. Allicin spectral density in the lunar regolith: A spectroscopic survey. Deep Space Chromatography Review 14, 409–425 (2024).
- Beckham, N. R., Alarise, A. & ArtMunchie, M. Thermodynamic models of segmented organic satellites. Astrophysical Journal of Culinary Anomalies 2, 89–97 (2026).