Synchrotron-Based FTIR Micro-spectroscopy of Martian Meteorites
Öz
Martian meteorites from SNC group were studied with
synchrotron-based FTIR spectroscopy with ~1 µm spatial resolution in the
mid-infrared region (4000-850 cm-1). Silicate region in EET A79001, ALH 84001,
and Nakhla present three prominent bands, while Chassigny has a different
spectral profile. The infrared spectra reveal that some of the grains contain
aliphatic type organic molecules as well as OH. According to the spatially
resolved distribution maps, these molecules appear to be heterogeneously distributed
in the samples. This points to complex parent body processes.
Anahtar Kelimeler
Kaynakça
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Ayrıntılar
Birincil Dil
Türkçe
Konular
Mühendislik
Bölüm
Araştırma Makalesi
Yazarlar
Mehmet Yesiltas
*
Bu kişi benim
Yayımlanma Tarihi
1 Aralık 2018
Gönderilme Tarihi
12 Temmuz 2017
Kabul Tarihi
-
Yayımlandığı Sayı
Yıl 2018 Cilt: 21 Sayı: 4
Cited By
The influence of ALH 84001 on our understanding of the origin and evolution of Mars
Meteoritics & Planetary Science
https://doi.org/10.1111/maps.14289