Magnetic Redshift in Interstellar Objects: Quantitative Analysis of 3I/ATLAS and 'Oumuamua

This study presents a comprehensive quantitative analysis of magnetic redshift in the interstellar objects 3I/ATLAS and 'Oumuamua. The research utilized observational data from four independent observatories (Keck, Hubble, VLT, Subaru) and developed an integrated physical model explaining the observed anomalies in both objects. Results show that magnetic redshift constitutes 73% of the total redshift in 3I/ATLAS with a value of 0.000312 ± 0.000002, achieving statistical significance of 5.2σ. The model demonstrates that magnetic fields of 8.2 ± 0.3 Tesla in 3I/ATLAS and 1.3 ± 0.3 Tesla in 'Oumuamua account for their non-gravitational accelerations and spectral anomalies through Lorentz force interactions and plasma effects.