Low-temperature plasma treatments were applied to barley seeds using a dielectric barrier-stabilized corona discharge operated in ambient air enriched with oxygen or nitrogen to quantify surface chemical modifications and seed wettability. X-ray photoelectron spectroscopy showed that oxygen-enriched plasma produced the strongest oxidation, increasing surface oxygen from 9 ± 5 at% (control) to 24 ± 5 at%, while reducing carbon from 88 ± 5 at% to 76 ± 5 at%. Nitrogen-enriched plasma induced more moderate changes (O: 13 ± 5 at%, C: 85 ± 5 at%) but resulted in clear nitrogen incorporation, with an enhanced N 1s amine/amide component at ~400.8 eV. The hydroxyl O 1s contribution increased from 70% (control) to 82% (oxygen) and 90% (nitrogen), indicating substantial surface hydroxylation. SEM-EDX showed only minor micrometer-scale composition changes and no detectable morphological damage. Raman and ATR-FTIR spectra confirmed that polysaccharide, protein, and lipid structures remained intact, with intensity variations reflecting increased hydrophilicity. Water imbibition kinetics fitted with the Peleg model demonstrated faster initial hydration after plasma exposure, with 1/k₁ increasing from 20.25 ± 1.90 h⁻¹ (control) to 36.70 ± 6.56 h⁻¹ (oxygen) and 38.87 ± 7.57 h⁻¹ (nitrogen), while 1/k₂ remained nearly unchanged.

Low-temperature plasma treatments are increasingly explored to stimulate seed germination and early plant development. In this study, barley seeds were exposed to dielectric barrier discharge (DBD) plasma generated in air with controlled oxygen or nitrogen admixtures to elucidate surface chemical and structural modifications. X-ray photoelectron spectroscopy (XPS) showed a pronounced increase in oxygen-containing functional groups (C–O, C=O, O–C=O) and the emergence of nitrogen functionalities after plasma exposure, indicating oxidative activation and partial surface amination. SEM-EDX analysis revealed slight oxygen enrichment and nitrogen incorporation at the near-surface region, while backscattered electron images confirmed that the plasma treatments did not induce measurable morphological damage. Raman and ATR-FTIR spectra demonstrated that the molecular backbone of polysaccharides and proteins remained intact, although bands associated with –OH and –NH vibrations intensified, confirming increased surface hydrophilicity. Water absorption kinetics, modeled using the Peleg equation, showed that plasma-treated seeds absorbed water more rapidly than untreated controls, evidencing improved wettability and hydration efficiency. Overall, the combined results indicate that plasma exposure primarily induces surface oxidation and mild nitrogen incorporation without compromising seed integrity, thereby enhancing water uptake.

The Esquel pallasite provides a valuable record of metal–silicate interaction in differentiated planetesimals, yet many aspects of its formation and thermal evolution remain uncertain. Here, we present a comprehensive multi-technique characterization of a single Esquel specimen, integrating SC-XRD, Raman spectroscopy, SEM–EDS, XPS, magnetic force microscopy, and X-ray computed tomography. Olivine grains are shown to be structurally pristine, with the first full crystallographic refinement for Esquel confirming a single-domain silicate lattice. XPS demonstrates a stoichiometric silicate surface containing only lattice O²⁻, Si⁴⁺, Mg²⁺, and Fe²⁺, indicating that olivine remained chemically unaltered. The Fe–Ni metal preserves diffusion-controlled taenite–kamacite exsolution, compositionally distinct plessite, accessory schreibersite and troilite as resolved by SEM. Quantitative Ni zoning, evaluated through interface-to-center gradients and a width–center-Ni correlation method, yields a self-consistent cooling rate of ~10–20 °C/Myr. MFM reveals microscale magnetic structures that correlate directly with Fe–Ni chemical zoning, providing magnetic confirmation of slow cooling. CT analysis further identifies interconnected metal networks, inclusions, and micro-porosity reflecting melt migration and late-stage modification. These results establish Esquel as an exceptionally well-preserved pallasite and demonstrate the value of integrated, multi-scale analytical workflows for reconstructing early Solar System processes.