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Creation of Lunar-like Rims in Ilmenite Using Synthetic Solar Wind

  • Authors: Roshan S. Trivedi, Advik D. Vira, Brant M. Jones, Katherine D. Burgess, Ziyu Huang, Honglin Liu, Pranav Rane, Mengkun Tian, Masatoshi Hirabayashi, Thomas M. Orlando, Zhigang Jiang, Phillip N. First

Roshan S. Trivedi et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A5.

EELS characterization of Ti-rich regions in SSW rims. (a) HAADF image of the 2 hr sample. (b) Fe/Ti ratio map (see Section 2) of the 2 hr sample in the same region as (a). (c) EELS low-loss spectra of the Ti-rich regions (blue) in (b) along with spectra from unexposed ilmenite (black). Dashed line marks the 10.5 eV peak, which arises from the formation of a TiO2 phase. (d) Ti L-edge spectra of the Ti-rich regions (blue) alongside an unexposed ilmenite spectrum (black). (e)–(h) Same as (a)–(d), but for the 12 hr sample. (i)–(l) Same as (a)–(d), but for the 14 hr sample.

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