Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene
Context. Space weathering is a process that changes the surface of airless planetary bodies. Prime space weathering agents are solar wind irradiation and micrometeoroid bombardment. These processes alter planetary reflectance spectra and often modify their compositional diagnostic features. Aims. In...
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creator | Chrbolková, Kateřina Brunetto, Rosario Ďurech, Josef Kohout, Tomáš Mizohata, Kenichiro Malý, Petr Dědič, Václav Lantz, Cateline Penttilä, Antti Trojánek, František Maturilli, Alessandro |
description | Context.
Space weathering is a process that changes the surface of airless planetary bodies. Prime space weathering agents are solar wind irradiation and micrometeoroid bombardment. These processes alter planetary reflectance spectra and often modify their compositional diagnostic features.
Aims.
In this work we focused on simulating and comparing the spectral changes caused by solar wind irradiation and by micrometeoroid bombardment to gain a better understanding of these individual space weathering processes.
Methods.
We used olivine and pyroxene pellets as proxies for planetary materials. To simulate solar wind irradiation we used hydrogen, helium, and argon ions with energies from 5 to 40 keV and fluences of up to 10
18
particles cm
−2
. To simulate micrometeoroid bombardment we used individual femtosecond laser pulses. We analysed the corresponding evolution of different spectral parameters, which we determined by applying the Modified Gaussian Model, and we also conducted principal component analysis.
Results.
The original mineralogy of the surface influences the spectral evolution more than the weathering agent, as seen from the diverse evolution of the spectral slope of olivine and pyroxene upon irradiation. The spectral slope changes seen in olivine are consistent with observations of A-type asteroids, while the moderate to no slope changes observed in pyroxene are consistent with asteroid (4) Vesta. We also observed some differences in the spectral effects induced by the two weathering agents. Ions simulating solar wind have a smaller influence on longer wavelengths of the spectra than laser irradiation simulating micrometeoroid impacts. This is most likely due to the different penetration depths of ions and laser pulses. Our results suggest that in some instances it might be possible to distinguish between the contributions of the two agents on a weathered surface. |
doi_str_mv | 10.1051/0004-6361/202140372 |
format | Article |
fullrecord | <record><control><sourceid>proquest_hal_p</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_hal_03855483v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2590107618</sourcerecordid><originalsourceid>FETCH-LOGICAL-c356t-1d18b0bd55d2972873ef564365153540ca55af96ecf04b2447badf14fea758653</originalsourceid><addsrcrecordid>eNo9kc2KFDEURoMo2LY-gZuAKxfl5Leqejk0OiM0uNF1uJXcTGeoSsqkesZ-HN_U1LT0IlzycThc7kfIR86-cKb5DWNMNa1s-Y1ggismO_GKbLiSomGdal-TzZV4S96V8li_gvdyQ_7u0zRDDiVFmjwtM1ikzwjLEXOIDzVAu2QYqT1CfMBCQ3Qni44OZ1rSCJk-14RCfVOwOU24YMopOBqq1y6FnsrqCSk2L5THaUkFbYquGaFgbkLO4AIsVZrG8BQivoDzOac_GPE9eeNhLPjh_9ySX9--_tzfN4cfd9_3t4fGSt0uDXe8H9jgtHZi14m-k-h1q2SruZZaMQtag9-1aD1Tg1CqG8B5rjxCp_tWyy35fPEeYTRzDhPks0kQzP3twawZk73WqpdPvLKfLuyc0-8TlsU8plOOdT0j9I5x1rX1ulsiL1S9SykZ_VXLmVl7M2srZm3FXHuT_wCIJY0V</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2590107618</pqid></control><display><type>article</type><title>Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene</title><source>Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>EDP Sciences</source><creator>Chrbolková, Kateřina ; Brunetto, Rosario ; Ďurech, Josef ; Kohout, Tomáš ; Mizohata, Kenichiro ; Malý, Petr ; Dědič, Václav ; Lantz, Cateline ; Penttilä, Antti ; Trojánek, František ; Maturilli, Alessandro</creator><creatorcontrib>Chrbolková, Kateřina ; Brunetto, Rosario ; Ďurech, Josef ; Kohout, Tomáš ; Mizohata, Kenichiro ; Malý, Petr ; Dědič, Václav ; Lantz, Cateline ; Penttilä, Antti ; Trojánek, František ; Maturilli, Alessandro</creatorcontrib><description>Context.
Space weathering is a process that changes the surface of airless planetary bodies. Prime space weathering agents are solar wind irradiation and micrometeoroid bombardment. These processes alter planetary reflectance spectra and often modify their compositional diagnostic features.
Aims.
In this work we focused on simulating and comparing the spectral changes caused by solar wind irradiation and by micrometeoroid bombardment to gain a better understanding of these individual space weathering processes.
Methods.
We used olivine and pyroxene pellets as proxies for planetary materials. To simulate solar wind irradiation we used hydrogen, helium, and argon ions with energies from 5 to 40 keV and fluences of up to 10
18
particles cm
−2
. To simulate micrometeoroid bombardment we used individual femtosecond laser pulses. We analysed the corresponding evolution of different spectral parameters, which we determined by applying the Modified Gaussian Model, and we also conducted principal component analysis.
Results.
The original mineralogy of the surface influences the spectral evolution more than the weathering agent, as seen from the diverse evolution of the spectral slope of olivine and pyroxene upon irradiation. The spectral slope changes seen in olivine are consistent with observations of A-type asteroids, while the moderate to no slope changes observed in pyroxene are consistent with asteroid (4) Vesta. We also observed some differences in the spectral effects induced by the two weathering agents. Ions simulating solar wind have a smaller influence on longer wavelengths of the spectra than laser irradiation simulating micrometeoroid impacts. This is most likely due to the different penetration depths of ions and laser pulses. Our results suggest that in some instances it might be possible to distinguish between the contributions of the two agents on a weathered surface.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>EISSN: 1432-0756</identifier><identifier>DOI: 10.1051/0004-6361/202140372</identifier><language>eng</language><publisher>Heidelberg: EDP Sciences</publisher><subject>Argon ions ; Astrophysics ; Earth and Planetary Astrophysics ; Evolution ; Femtosecond pulses ; Irradiation ; Lasers ; Micrometeoroids ; Mineralogy ; Olivine ; Parameter modification ; Physics ; Principal components analysis ; Pyroxenes ; Sciences of the Universe ; Simulation ; Solar wind ; Space weathering ; Spectra ; Vesta asteroid</subject><ispartof>Astronomy and astrophysics (Berlin), 2021-10, Vol.654, p.A143</ispartof><rights>2021. This work is licensed under https://creativecommons.org/licenses/by/4.0 (the “License”). Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the terms of the License.</rights><rights>Attribution</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c356t-1d18b0bd55d2972873ef564365153540ca55af96ecf04b2447badf14fea758653</citedby><cites>FETCH-LOGICAL-c356t-1d18b0bd55d2972873ef564365153540ca55af96ecf04b2447badf14fea758653</cites><orcidid>0000-0003-3001-9362 ; 0000-0001-7403-1721 ; 0000-0003-4458-3650 ; 0000-0003-4914-3646 ; 0000-0001-9101-9548 ; 0000-0001-7159-5521 ; 0000-0003-2174-6402 ; 0000-0003-0974-4770 ; 0000-0003-2742-7939 ; 0000-0003-4613-9799</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,315,781,785,886,3728,27925,27926</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03855483$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Chrbolková, Kateřina</creatorcontrib><creatorcontrib>Brunetto, Rosario</creatorcontrib><creatorcontrib>Ďurech, Josef</creatorcontrib><creatorcontrib>Kohout, Tomáš</creatorcontrib><creatorcontrib>Mizohata, Kenichiro</creatorcontrib><creatorcontrib>Malý, Petr</creatorcontrib><creatorcontrib>Dědič, Václav</creatorcontrib><creatorcontrib>Lantz, Cateline</creatorcontrib><creatorcontrib>Penttilä, Antti</creatorcontrib><creatorcontrib>Trojánek, František</creatorcontrib><creatorcontrib>Maturilli, Alessandro</creatorcontrib><title>Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene</title><title>Astronomy and astrophysics (Berlin)</title><description>Context.
Space weathering is a process that changes the surface of airless planetary bodies. Prime space weathering agents are solar wind irradiation and micrometeoroid bombardment. These processes alter planetary reflectance spectra and often modify their compositional diagnostic features.
Aims.
In this work we focused on simulating and comparing the spectral changes caused by solar wind irradiation and by micrometeoroid bombardment to gain a better understanding of these individual space weathering processes.
Methods.
We used olivine and pyroxene pellets as proxies for planetary materials. To simulate solar wind irradiation we used hydrogen, helium, and argon ions with energies from 5 to 40 keV and fluences of up to 10
18
particles cm
−2
. To simulate micrometeoroid bombardment we used individual femtosecond laser pulses. We analysed the corresponding evolution of different spectral parameters, which we determined by applying the Modified Gaussian Model, and we also conducted principal component analysis.
Results.
The original mineralogy of the surface influences the spectral evolution more than the weathering agent, as seen from the diverse evolution of the spectral slope of olivine and pyroxene upon irradiation. The spectral slope changes seen in olivine are consistent with observations of A-type asteroids, while the moderate to no slope changes observed in pyroxene are consistent with asteroid (4) Vesta. We also observed some differences in the spectral effects induced by the two weathering agents. Ions simulating solar wind have a smaller influence on longer wavelengths of the spectra than laser irradiation simulating micrometeoroid impacts. This is most likely due to the different penetration depths of ions and laser pulses. Our results suggest that in some instances it might be possible to distinguish between the contributions of the two agents on a weathered surface.</description><subject>Argon ions</subject><subject>Astrophysics</subject><subject>Earth and Planetary Astrophysics</subject><subject>Evolution</subject><subject>Femtosecond pulses</subject><subject>Irradiation</subject><subject>Lasers</subject><subject>Micrometeoroids</subject><subject>Mineralogy</subject><subject>Olivine</subject><subject>Parameter modification</subject><subject>Physics</subject><subject>Principal components analysis</subject><subject>Pyroxenes</subject><subject>Sciences of the Universe</subject><subject>Simulation</subject><subject>Solar wind</subject><subject>Space weathering</subject><subject>Spectra</subject><subject>Vesta asteroid</subject><issn>0004-6361</issn><issn>1432-0746</issn><issn>1432-0756</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNo9kc2KFDEURoMo2LY-gZuAKxfl5Leqejk0OiM0uNF1uJXcTGeoSsqkesZ-HN_U1LT0IlzycThc7kfIR86-cKb5DWNMNa1s-Y1ggismO_GKbLiSomGdal-TzZV4S96V8li_gvdyQ_7u0zRDDiVFmjwtM1ikzwjLEXOIDzVAu2QYqT1CfMBCQ3Qni44OZ1rSCJk-14RCfVOwOU24YMopOBqq1y6FnsrqCSk2L5THaUkFbYquGaFgbkLO4AIsVZrG8BQivoDzOac_GPE9eeNhLPjh_9ySX9--_tzfN4cfd9_3t4fGSt0uDXe8H9jgtHZi14m-k-h1q2SruZZaMQtag9-1aD1Tg1CqG8B5rjxCp_tWyy35fPEeYTRzDhPks0kQzP3twawZk73WqpdPvLKfLuyc0-8TlsU8plOOdT0j9I5x1rX1ulsiL1S9SykZ_VXLmVl7M2srZm3FXHuT_wCIJY0V</recordid><startdate>20211001</startdate><enddate>20211001</enddate><creator>Chrbolková, Kateřina</creator><creator>Brunetto, Rosario</creator><creator>Ďurech, Josef</creator><creator>Kohout, Tomáš</creator><creator>Mizohata, Kenichiro</creator><creator>Malý, Petr</creator><creator>Dědič, Václav</creator><creator>Lantz, Cateline</creator><creator>Penttilä, Antti</creator><creator>Trojánek, František</creator><creator>Maturilli, Alessandro</creator><general>EDP Sciences</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><scope>VOOES</scope><orcidid>https://orcid.org/0000-0003-3001-9362</orcidid><orcidid>https://orcid.org/0000-0001-7403-1721</orcidid><orcidid>https://orcid.org/0000-0003-4458-3650</orcidid><orcidid>https://orcid.org/0000-0003-4914-3646</orcidid><orcidid>https://orcid.org/0000-0001-9101-9548</orcidid><orcidid>https://orcid.org/0000-0001-7159-5521</orcidid><orcidid>https://orcid.org/0000-0003-2174-6402</orcidid><orcidid>https://orcid.org/0000-0003-0974-4770</orcidid><orcidid>https://orcid.org/0000-0003-2742-7939</orcidid><orcidid>https://orcid.org/0000-0003-4613-9799</orcidid></search><sort><creationdate>20211001</creationdate><title>Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene</title><author>Chrbolková, Kateřina ; Brunetto, Rosario ; Ďurech, Josef ; Kohout, Tomáš ; Mizohata, Kenichiro ; Malý, Petr ; Dědič, Václav ; Lantz, Cateline ; Penttilä, Antti ; Trojánek, František ; Maturilli, Alessandro</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c356t-1d18b0bd55d2972873ef564365153540ca55af96ecf04b2447badf14fea758653</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Argon ions</topic><topic>Astrophysics</topic><topic>Earth and Planetary Astrophysics</topic><topic>Evolution</topic><topic>Femtosecond pulses</topic><topic>Irradiation</topic><topic>Lasers</topic><topic>Micrometeoroids</topic><topic>Mineralogy</topic><topic>Olivine</topic><topic>Parameter modification</topic><topic>Physics</topic><topic>Principal components analysis</topic><topic>Pyroxenes</topic><topic>Sciences of the Universe</topic><topic>Simulation</topic><topic>Solar wind</topic><topic>Space weathering</topic><topic>Spectra</topic><topic>Vesta asteroid</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Chrbolková, Kateřina</creatorcontrib><creatorcontrib>Brunetto, Rosario</creatorcontrib><creatorcontrib>Ďurech, Josef</creatorcontrib><creatorcontrib>Kohout, Tomáš</creatorcontrib><creatorcontrib>Mizohata, Kenichiro</creatorcontrib><creatorcontrib>Malý, Petr</creatorcontrib><creatorcontrib>Dědič, Václav</creatorcontrib><creatorcontrib>Lantz, Cateline</creatorcontrib><creatorcontrib>Penttilä, Antti</creatorcontrib><creatorcontrib>Trojánek, František</creatorcontrib><creatorcontrib>Maturilli, Alessandro</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chrbolková, Kateřina</au><au>Brunetto, Rosario</au><au>Ďurech, Josef</au><au>Kohout, Tomáš</au><au>Mizohata, Kenichiro</au><au>Malý, Petr</au><au>Dědič, Václav</au><au>Lantz, Cateline</au><au>Penttilä, Antti</au><au>Trojánek, František</au><au>Maturilli, Alessandro</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2021-10-01</date><risdate>2021</risdate><volume>654</volume><spage>A143</spage><pages>A143-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>Context.
Space weathering is a process that changes the surface of airless planetary bodies. Prime space weathering agents are solar wind irradiation and micrometeoroid bombardment. These processes alter planetary reflectance spectra and often modify their compositional diagnostic features.
Aims.
In this work we focused on simulating and comparing the spectral changes caused by solar wind irradiation and by micrometeoroid bombardment to gain a better understanding of these individual space weathering processes.
Methods.
We used olivine and pyroxene pellets as proxies for planetary materials. To simulate solar wind irradiation we used hydrogen, helium, and argon ions with energies from 5 to 40 keV and fluences of up to 10
18
particles cm
−2
. To simulate micrometeoroid bombardment we used individual femtosecond laser pulses. We analysed the corresponding evolution of different spectral parameters, which we determined by applying the Modified Gaussian Model, and we also conducted principal component analysis.
Results.
The original mineralogy of the surface influences the spectral evolution more than the weathering agent, as seen from the diverse evolution of the spectral slope of olivine and pyroxene upon irradiation. The spectral slope changes seen in olivine are consistent with observations of A-type asteroids, while the moderate to no slope changes observed in pyroxene are consistent with asteroid (4) Vesta. We also observed some differences in the spectral effects induced by the two weathering agents. Ions simulating solar wind have a smaller influence on longer wavelengths of the spectra than laser irradiation simulating micrometeoroid impacts. This is most likely due to the different penetration depths of ions and laser pulses. Our results suggest that in some instances it might be possible to distinguish between the contributions of the two agents on a weathered surface.</abstract><cop>Heidelberg</cop><pub>EDP Sciences</pub><doi>10.1051/0004-6361/202140372</doi><orcidid>https://orcid.org/0000-0003-3001-9362</orcidid><orcidid>https://orcid.org/0000-0001-7403-1721</orcidid><orcidid>https://orcid.org/0000-0003-4458-3650</orcidid><orcidid>https://orcid.org/0000-0003-4914-3646</orcidid><orcidid>https://orcid.org/0000-0001-9101-9548</orcidid><orcidid>https://orcid.org/0000-0001-7159-5521</orcidid><orcidid>https://orcid.org/0000-0003-2174-6402</orcidid><orcidid>https://orcid.org/0000-0003-0974-4770</orcidid><orcidid>https://orcid.org/0000-0003-2742-7939</orcidid><orcidid>https://orcid.org/0000-0003-4613-9799</orcidid><oa>free_for_read</oa></addata></record> |
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source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; EDP Sciences |
subjects | Argon ions Astrophysics Earth and Planetary Astrophysics Evolution Femtosecond pulses Irradiation Lasers Micrometeoroids Mineralogy Olivine Parameter modification Physics Principal components analysis Pyroxenes Sciences of the Universe Simulation Solar wind Space weathering Spectra Vesta asteroid |
title | Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene |
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