Chrbolková, K. und Brunetto, Rosario und Durech, J. und Kohout, Tomas und Mizohata, K. und Malý, P. und Dědič, V. und Lantz, C. und Penttilä, A. und Trojánek, F. und Maturilli, Alessandro (2021) Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene. Astronomy & Astrophysics, 654, A143. EDP Sciences. doi: 10.1051/0004-6361/202140372. ISSN 0004-6361.
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Offizielle URL: https://www.aanda.org/articles/aa/abs/2021/10/aa40372-21/aa40372-21.html
Kurzfassung
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 1018 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.
elib-URL des Eintrags: | https://elib.dlr.de/147446/ | ||||||||||||||||||||||||||||||||||||||||||||||||
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Dokumentart: | Zeitschriftenbeitrag | ||||||||||||||||||||||||||||||||||||||||||||||||
Titel: | Comparison of space weathering spectral changes induced by solar wind and micrometeoroid impacts using ion- and femtosecond-laser-irradiated olivine and pyroxene | ||||||||||||||||||||||||||||||||||||||||||||||||
Autoren: |
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Datum: | 22 Oktober 2021 | ||||||||||||||||||||||||||||||||||||||||||||||||
Erschienen in: | Astronomy & Astrophysics | ||||||||||||||||||||||||||||||||||||||||||||||||
Referierte Publikation: | Ja | ||||||||||||||||||||||||||||||||||||||||||||||||
Open Access: | Ja | ||||||||||||||||||||||||||||||||||||||||||||||||
Gold Open Access: | Nein | ||||||||||||||||||||||||||||||||||||||||||||||||
In SCOPUS: | Ja | ||||||||||||||||||||||||||||||||||||||||||||||||
In ISI Web of Science: | Ja | ||||||||||||||||||||||||||||||||||||||||||||||||
Band: | 654 | ||||||||||||||||||||||||||||||||||||||||||||||||
DOI: | 10.1051/0004-6361/202140372 | ||||||||||||||||||||||||||||||||||||||||||||||||
Seitenbereich: | A143 | ||||||||||||||||||||||||||||||||||||||||||||||||
Verlag: | EDP Sciences | ||||||||||||||||||||||||||||||||||||||||||||||||
ISSN: | 0004-6361 | ||||||||||||||||||||||||||||||||||||||||||||||||
Status: | veröffentlicht | ||||||||||||||||||||||||||||||||||||||||||||||||
Stichwörter: | planets and satellites: surfaces, solar wind, meteorites, meteors, meteoroids, methods: data analysis, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Space Physics | ||||||||||||||||||||||||||||||||||||||||||||||||
HGF - Forschungsbereich: | Luftfahrt, Raumfahrt und Verkehr | ||||||||||||||||||||||||||||||||||||||||||||||||
HGF - Programm: | Raumfahrt | ||||||||||||||||||||||||||||||||||||||||||||||||
HGF - Programmthema: | Erforschung des Weltraums | ||||||||||||||||||||||||||||||||||||||||||||||||
DLR - Schwerpunkt: | Raumfahrt | ||||||||||||||||||||||||||||||||||||||||||||||||
DLR - Forschungsgebiet: | R EW - Erforschung des Weltraums | ||||||||||||||||||||||||||||||||||||||||||||||||
DLR - Teilgebiet (Projekt, Vorhaben): | R - Projekt BepiColombo - MERTIS und BELA | ||||||||||||||||||||||||||||||||||||||||||||||||
Standort: | Berlin-Adlershof | ||||||||||||||||||||||||||||||||||||||||||||||||
Institute & Einrichtungen: | Institut für Planetenforschung > Planetare Labore | ||||||||||||||||||||||||||||||||||||||||||||||||
Hinterlegt von: | Maturilli, Dr. Alessandro | ||||||||||||||||||||||||||||||||||||||||||||||||
Hinterlegt am: | 15 Dez 2021 10:59 | ||||||||||||||||||||||||||||||||||||||||||||||||
Letzte Änderung: | 05 Dez 2023 07:20 |
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