Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies

Samples from the Genesis Solar Wind Sample Return (NASA Discovery 5) are a unique opportunity to study the initial stages of space weathering, i.e., the physical and chemical effects of solar-wind irradiation. Arrays of collectors containing multiple materials were each exposed to a different solar-...

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Main Authors: Amy J. G. Jurewicz, Karen D. Rieck, Chad Olinger, Judy Allton, Mukul Sharma, Lindsay P. Keller, Roy Christoffersen
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Planetary Science Journal
Subjects:
Online Access:https://doi.org/10.3847/PSJ/acd33c
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author Amy J. G. Jurewicz
Karen D. Rieck
Chad Olinger
Judy Allton
Mukul Sharma
Lindsay P. Keller
Roy Christoffersen
author_facet Amy J. G. Jurewicz
Karen D. Rieck
Chad Olinger
Judy Allton
Mukul Sharma
Lindsay P. Keller
Roy Christoffersen
author_sort Amy J. G. Jurewicz
collection DOAJ
description Samples from the Genesis Solar Wind Sample Return (NASA Discovery 5) are a unique opportunity to study the initial stages of space weathering, i.e., the physical and chemical effects of solar-wind irradiation. Arrays of collectors containing multiple materials were each exposed to a different solar-wind regime (fast, slow, bulk, or coronal mass ejection) at the L1 point for long durations (years). Materials exposed to the solar wind included metals, semiconductors, and insulators. Although the time of exposure was obviously short relative to samples having extraterrestrial origins, optical properties, surface chemical properties, and matrix structure have changed in many collectors due to exposure to solar wind. The thickness of amorphous zones, where present, appears to correspond with the depth of the peak of the solar-wind H distribution in each regime. Damage from high-energy particles was negligible because the collectors were 700 μ m or less in thickness and shielded from the back by the spacecraft. Micrometeorite impacts and sputtering were also negligible because of the short exposure times. Our current results are preliminary: We hope future workers will extend this study both to support Genesis characterization efforts and to further understand space-weathering processes on a geologic timescale.
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spelling doaj.art-fb28d36c0ba841a6b24d11d6e62191362024-02-03T07:56:45ZengIOP PublishingThe Planetary Science Journal2632-33382023-01-01459810.3847/PSJ/acd33cSpace Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless BodiesAmy J. G. Jurewicz0https://orcid.org/0000-0002-3282-5782Karen D. Rieck1https://orcid.org/0000-0002-7427-9134Chad Olinger2https://orcid.org/0000-0002-9509-6345Judy Allton3Mukul Sharma4https://orcid.org/0000-0003-4328-3090Lindsay P. Keller5https://orcid.org/0000-0003-1560-2939Roy Christoffersen6BCMS/SESE Arizona State University , Tempe AZ 85287-6004, USA ; Amy.Jurewicz@asu.edu; Department of Earth Sciences, Dartmouth College , Hanover, NH 03755, USANew Mexico Consortium , 4200 W. Jemez Road, Suite 200, Los Alamos, NM 87544, USADepartment of Energy , AU-62, 19901 Germantown Road, Germantown, MD 20875, USAAstromaterials Curation , NASA JSC, Mail Code XI2, Houston TX 77058, USADepartment of Earth Sciences, Dartmouth College , Hanover, NH 03755, USAMail Code XI, ARES, NASA Johnson Space Center , Houston, TX 77058, USAJacobs Engineering, Mail Code XI, ARES, NASA Johnson Space Center , Houston, TX 77058, USASamples from the Genesis Solar Wind Sample Return (NASA Discovery 5) are a unique opportunity to study the initial stages of space weathering, i.e., the physical and chemical effects of solar-wind irradiation. Arrays of collectors containing multiple materials were each exposed to a different solar-wind regime (fast, slow, bulk, or coronal mass ejection) at the L1 point for long durations (years). Materials exposed to the solar wind included metals, semiconductors, and insulators. Although the time of exposure was obviously short relative to samples having extraterrestrial origins, optical properties, surface chemical properties, and matrix structure have changed in many collectors due to exposure to solar wind. The thickness of amorphous zones, where present, appears to correspond with the depth of the peak of the solar-wind H distribution in each regime. Damage from high-energy particles was negligible because the collectors were 700 μ m or less in thickness and shielded from the back by the spacecraft. Micrometeorite impacts and sputtering were also negligible because of the short exposure times. Our current results are preliminary: We hope future workers will extend this study both to support Genesis characterization efforts and to further understand space-weathering processes on a geologic timescale.https://doi.org/10.3847/PSJ/acd33cSpace researchSolar windPlanetary science
spellingShingle Amy J. G. Jurewicz
Karen D. Rieck
Chad Olinger
Judy Allton
Mukul Sharma
Lindsay P. Keller
Roy Christoffersen
Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
The Planetary Science Journal
Space research
Solar wind
Planetary science
title Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
title_full Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
title_fullStr Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
title_full_unstemmed Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
title_short Space Weathering of Genesis Mission Solar-wind Collectors with Inferences for Weathering on Airless Bodies
title_sort space weathering of genesis mission solar wind collectors with inferences for weathering on airless bodies
topic Space research
Solar wind
Planetary science
url https://doi.org/10.3847/PSJ/acd33c
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