Repository logo
 

Prebiotic magnetite enables chirality-magnetic surface feedback

Accepted version
Peer-reviewed

Change log

Abstract

The emergence of biomolecular homochirality requires both an initial symmetry-breaking event and a mechanism to amplify and preserve a chiral imbalance. Magnetic minerals have been shown to function as chiral agents through the chiral-induced spin selectivity (CISS) effect and may have enabled homochirality on early Earth, yet the magnetic properties of magnetite formed under realistic prebiotic conditions remain unexplored. Here we show that magnetite synthesized through two geochemically plausible pathways—UV-driven photo-oxidation and nitrite-mediated oxidation of Fe(II)—produces particles dominated by single-vortex and multi-vortex magnetic domain states. Magnetic measurements and electron microscopy confirm that these populations differ markedly from the nano-fabricated thin-film substrates conventionally used in previous CISS experiments. Using 3D micromagnetic simulations, we demonstrate that single-domain and vortex-state grains undergo irreversible, exchange-driven re-magnetization when interacting with spin-polarized homochiral compounds. This magnetic irreversibility provides a robust mechanism for storing and reinforcing weak chiral bias, suggesting that prebiotic magnetite could have contributed to the emergence and stabilization of persistent chiral bias on the early Earth.

Description

Keywords

Journal Title

Science Advances

Conference Name

Journal ISSN

2375-2548
2375-2548

Volume Title

Publisher

American Association for the Advancement of Science (AAAS)

Publisher DOI

Publisher URL

Rights and licensing

Except where otherwised noted, this item's license is described as Attribution 4.0 International
Sponsorship
S.F.O. and D.D.S. acknowledge the Harvard Origins of Life Initiative; S.F.O. further acknowledges support from the Kavli Laukien fellowship program, Caltech startup funds, the William H. Hurt Scholarship Program, and the Fellows of King’s College Cambridge for their hospitality. R.J.H., N.J.T. and J.A.P.M.D. acknowledge the Leverhulme Centre for Life in the Universe (LCLU) funding (LBAG/329), with additional LCLU support for N.J.T. and Z.L. (RC-2021-032). Part of this work was performed by J.A.P.M.D. as a visiting researcher at the Institute for Rock Magnetism (IRM) at the University of Minnesota, which is supported by the National Science Foundation (NSF EAR 2153786) and the University of Minnesota. T.G. acknowledges the Wolfson Electron Microscopy suite for the use of the TF Spectra 300.

Relationships

Is supplemented by: