DIVISION 02 // AEROSPACE FORENSICS

ISOTOPIC DRIFT
INDEX Diso

A standardized, theory-agnostic forensic metric for identifying isotopic gradients inconsistent with industrial melt-phase mixing. Demonstrated on the Ubatuba fragment. Proposed as a falsifiable prediction for 3I/ATLAS.

Diso
Ni-62: Predicted
May 2026 Window

THE METRIC RESIDUE HYPOTHESIS

Standard forensic protocols applied to recovered UAP materials typically seek functional components — circuitry, fasteners, identifiable mechanical geometry. This orientation may systematically overlook a distinct class of signature: isotopic gradients inconsistent with any known industrial process.

We propose that certain anomalous samples represent precipitates formed under extreme non-equilibrium conditions. The transition from anecdotal description to predictive materials science requires a standardized coefficient. The Isotopic Drift Index provides that foundation.

The Diso Formula

Diso = Σᵢ | (Iobs − Istd) / Istd |

Iobs = Observed isotopic abundance

Istd = Terrestrial / solar standard

< 0.1

Terrestrial Baseline

Consistent with known industrial melt-phase processing.

0.1 – 0.5

Anomalous

Investigate enrichment or contamination sources.

> 0.5

Falsifying Threshold

Falsifies industrial melt-phase mixing as origin.

Diso LIVE CALCULATOR

Pre-loaded with Ubatuba Mg demonstration values. Edit any field to recalculate in real time.

Isotope
Iₛₜᵈ Standard
Iₒᵇₛ Observed
Deviation
0.0885
0.5000
0.1807
Total DisoMethodology protected under USPTO 63/929,089. This tool calculates the Isotopic Drift Index to distinguish between terrestrial industrial processing and metric-field precipitates (Vacuum Condensates).
0.7692
Dᵢₛₒ ≥ 0.5 — Falsifies melt-phase mixing
Ubatuba Mg Fragment — Illustrative

3I/ATLAS — MACRO VALIDATION

The 2026 encounter with Interstellar Object 3I/ATLAS provides an opportunity for macro-scale application. Remote sensing indicates an extreme NiI/FeI abundance ratio consistent with non-equilibrium dissociation, alongside significant methanol enrichment.

We propose as a testable prediction that high-resolution spectrographic analysis of the object's ejecta will confirm Diso > 0.5 for the Nickel-62 system — proposed as a primary observational objective for the May 2026 Jovian periapsis window.

Current Spectroscopic Data
0.02 : 1

Fe / Ni ratio — 3I/ATLAS

Falsifiable Prediction // May 2026

High-resolution spectrographic analysis of 3I/ATLAS ejecta at the Jovian periapsis window will confirm:

Diso > 0.5 for the Nickel-62 system

Supporting Literature

[1]

Pre-perihelion evolution of the NiI/FeI abundance ratio in 3I/ATLAS.

Rahatgaonkar et al. (2025) — arXiv:2509.26053

[2]

CH₃OH and HCN in 3I/ATLAS: High ratios from ALMA.

Roth et al. (2026) — ApJL 999, L32

[3]

JWST detection of CO₂-dominated gas coma surrounding 3I/ATLAS.

Cordiner et al. (2025) — arXiv:2508.18209

RESEARCH RESOURCES

Diso PREPRINT

Isotopic Drift Index methodology — Zenodo 19004156

View Preprint

JBIS PAPER

Kinematic & spectroscopic constraints on 3I/ATLAS — Vol. 79, 2026

Read Paper

ISOTOPIC TOPOLOGY

The foundational hardware assurance paper — C4-TR-26-001

Read Paper

COLLABORATION &
DATA ACCESS

The Diso methodology is proposed as an open forensic standard. Direct application to raw NanoSIMS datasets — beginning with Powell et al. (2022) — is the proposed next step toward formal validation.

Researchers with access to relevant sample archives, spectrographic datasets, or institutional partnerships are invited to reach out.

NanoSIMS / SIMS isotopic datasets
Astronomical spectroscopic archives
Recovered material sample access

SUBMIT INQUIRY