Abstract
The surfaces of airless bodies, such as the Moon and asteroids, are subject to space weathering, which alters the mineralogy of the upper tens of nanometers of grain surfaces. Atom probe tomography (APT) has the appropriate 3-D spatial resolution and analytical sensitivity to investigate such features at the nanometer scale. Here, we demonstrate that APT can be successfully used to characterize the composition and texture of space weathering products in ilmenite from Apollo 17 sample 71501 at near-atomic resolution. Two of the studied nanotips sampled the top surface of the space-weathered grain, while another nanotip sampled the ilmenite at about 50 nm below the surface. These nanotips contain small nanophase Fe particles (~3 to 10 nm diameter), with these particles becoming less frequent with depth. One of the nanotips contains a sequence of space weathering products, compositional zoning, and a void space (~15 nm in diameter) which we interpret as a vesicle generated by solar wind irradiation. No noble gases were detected in this vesicle, although there is evidence for 4He elsewhere in the nanotip. This lunar soil grain exhibits the same space weathering features that have been well documented in transmission electron microscope studies of lunar and Itokawa asteroidal regolith grains.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 426-440 |
| Number of pages | 15 |
| Journal | Meteoritics and Planetary Science |
| Volume | 55 |
| Issue number | 2 |
| DOIs | |
| State | Published - Feb 1 2020 |
Funding
The authors thank Ryan A. Zeigler (Johnson Space Center) for providing the lunar sample and Jean‐Paul Benkert for preparing the ilmenite grain separate. We also thank Levke Kööp for maintaining the FIB/SEM. J.G. acknowledges support from the National Science Foundation Graduate Research Fellowship (DGE‐1144082 and DGE‐1746045). P.R.H. acknowledges the TAWANI Foundation who funded the Robert A. Pritzker Center through a major grant. Atom probe tomography was performed at the Northwestern University Center for Atom Probe Tomography (NUCAPT). The LEAP tomograph at NUCAPT was purchased and upgraded with grants from the NSF‐MRI (DMR‐0420532) and ONR‐DURIP (N00014‐0400798, N00014‐0610539, N00014‐0910781, N00014‐1712870) programs. NUCAPT received support from the MRSEC program (NSF DMR‐1720139) at the Materials Research Center, the SHyNE Resource (NSF ECCS‐1542205), and the Initiative for Sustainability and Energy (ISEN) at Northwestern University. We appreciate the constructive reviews by Katharine Burgess and Michelle Thompson, and thank associate editor Carlé M. Pieters. The authors thank Ryan A. Zeigler (Johnson Space Center) for providing the lunar sample and Jean-Paul Benkert for preparing the ilmenite grain separate. We also thank Levke K??p for maintaining the FIB/SEM. J.G. acknowledges support from the National Science Foundation Graduate Research Fellowship (DGE-1144082 and DGE-1746045). P.R.H. acknowledges the TAWANI Foundation who funded the Robert A. Pritzker Center through a major grant. Atom probe tomography was performed at the Northwestern University Center for Atom Probe Tomography (NUCAPT). The LEAP tomograph at NUCAPT was purchased and upgraded with grants from the NSF-MRI (DMR-0420532) and ONR-DURIP (N00014-0400798, N00014-0610539, N00014-0910781, N00014-1712870) programs. NUCAPT received support from the MRSEC program (NSF DMR-1720139) at the Materials Research Center, the SHyNE Resource (NSF ECCS-1542205), and the Initiative for Sustainability and Energy (ISEN) at Northwestern University. We appreciate the constructive reviews by Katharine Burgess and Michelle Thompson, and thank associate editor Carl? M. Pieters.
ASJC Scopus subject areas
- Geophysics
- Space and Planetary Science