Nanophase iron production through laser irradiation and magnetic detection of space weathering analogs
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985831%3A_____%2F16%3A00458598" target="_blank" >RIV/67985831:_____/16:00458598 - isvavai.cz</a>
Výsledek na webu
<a href="http://dx.doi.org/10.1016/j.icarus.2015.12.022" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2015.12.022</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.icarus.2015.12.022" target="_blank" >10.1016/j.icarus.2015.12.022</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Nanophase iron production through laser irradiation and magnetic detection of space weathering analogs
Popis výsledku v původním jazyce
Airless bodies are constantly exposed to space weathering. The Moon and other similar S-type asteroids physically change through comminution, melting, and agglutinate formation, while spectrally they are darkening, steepening (or reddening) the spectral slope toward longer wavelengths, and reducing silicate mineral absorption bands. In these S-type bodies the production of submicroscopic metallic iron, or nanophase iron (SMFe, npFe0) is a major contributor in these spectral changes. We made a qualitative estimate of both quantity and size distribution of produced metallic iron by space weathered analog, olivine irradiated by laser. Through SEM observation we confirmed that nanoparticles of metallic iron formed in the nm range. Spectroscopic and magnetic susceptibility (MS) through temperature analyses reveal an increasing trend of npFe0 formation, darkening, reddening, and shallowing of the 1 μm olivine absorption band. Olivine that produced the larger end of the size range of npFe0 produced similar effects, except for increased reddening. The magnetic data suggests that with laser irradiation there is both a linear increase of nanoparticles and a logarithmic increase in spectral change with SW time.
Název v anglickém jazyce
Nanophase iron production through laser irradiation and magnetic detection of space weathering analogs
Popis výsledku anglicky
Airless bodies are constantly exposed to space weathering. The Moon and other similar S-type asteroids physically change through comminution, melting, and agglutinate formation, while spectrally they are darkening, steepening (or reddening) the spectral slope toward longer wavelengths, and reducing silicate mineral absorption bands. In these S-type bodies the production of submicroscopic metallic iron, or nanophase iron (SMFe, npFe0) is a major contributor in these spectral changes. We made a qualitative estimate of both quantity and size distribution of produced metallic iron by space weathered analog, olivine irradiated by laser. Through SEM observation we confirmed that nanoparticles of metallic iron formed in the nm range. Spectroscopic and magnetic susceptibility (MS) through temperature analyses reveal an increasing trend of npFe0 formation, darkening, reddening, and shallowing of the 1 μm olivine absorption band. Olivine that produced the larger end of the size range of npFe0 produced similar effects, except for increased reddening. The magnetic data suggests that with laser irradiation there is both a linear increase of nanoparticles and a logarithmic increase in spectral change with SW time.
Klasifikace
Druh
J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)
CEP obor
BN - Astronomie a nebeská mechanika, astrofyzika
OECD FORD obor
—
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2016
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Icarus
ISSN
0019-1035
e-ISSN
—
Svazek periodika
268
Číslo periodika v rámci svazku
April
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
11
Strana od-do
204-214
Kód UT WoS článku
000370218100015
EID výsledku v databázi Scopus
2-s2.0-84955059614