Mineralogical, Spectral, and Compositional Changes During Heating of Hydrous Carbonaceous Chondrites

التفاصيل البيبلوغرافية
العنوان: Mineralogical, Spectral, and Compositional Changes During Heating of Hydrous Carbonaceous Chondrites
المؤلفون: Nakamura, T, Matsuoka, M, Yamashita, S, Sato, Y, Mogi, K, Enokido, Y, Nakata, A, Okumura, S, Furukawa, Y, Zolensky, M
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 2017.
سنة النشر: 2017
مصطلحات موضوعية: Lunar And Planetary Science And Exploration, Geosciences (General)
الوصف: Hydrous carbonaceous chondrites experienced hydration and subsequent dehydration by heating, which resulted in a variety of mineralogical and spectral features [e. g., 1-6]. The degree of heating is classified according to heating stage (HS) II to IV based on mineralogy of phyllosilicates [2], because they change, with elevating temperature, to poorly crystal-line phases and subsequently to aggregates of small secondary anhydrous silicates of mainly olivine. Heating of hydrous carbonaceous chondrites also causes spectral changes and volatile loss [3-6]. Experimental heating of Murchison CM chondrite showed flattening of whole visible-near infrared spectra, especially weakening of the 3μm band strength [1, 4, 7]. In order to understand mineralogical, spectral, and compositional changes during heating of hydrous carbonaceous chondrites, we have carried out systematic investigation of mineralogy, reflectance spectra, and volatile composition of hydrated and dehydrated carbonaceous chondrites as well as experimentally-heated hydrous carbonaceous chondrites. In addition, we investigated reflectance spectra of tochilinite that is a major phase of CM chondrites and has a low dehydration temperature (~250degC).
نوع الوثيقة: Report
اللغة: English
الوصول الحر: https://ntrs.nasa.gov/citations/20170001380Test
رقم الانضمام: edsnas.20170001380
قاعدة البيانات: NASA Technical Reports