Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Interaction of an Fe–Ni Melt with Anthracene (C14H10) in the Presence of Olivine at 3 GPa: Fluid Phase Composition. / Chepurov, A. I.; Tomilenko, A. A.; Sonin, V. M. и др.
в: Doklady Earth Sciences, Том 492, № 1, 01.05.2020, стр. 333-337.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Interaction of an Fe–Ni Melt with Anthracene (C14H10) in the Presence of Olivine at 3 GPa: Fluid Phase Composition
AU - Chepurov, A. I.
AU - Tomilenko, A. A.
AU - Sonin, V. M.
AU - Zhimulev, E. I.
AU - Bul’bak, T. A.
AU - Chepurov, A. A.
AU - Sobolev, N. V.
PY - 2020/5/1
Y1 - 2020/5/1
N2 - The first results on the interaction between an Fe–Ni melt and anthracene (С14Н10) in the presence of olivine at 3 GPa and 1500°С and on the study of the component composition of the fluid generated in this process are presented. The stability of aliphatic hydrocarbons in the implemented conditions is confirmed experimentally. It is established that, under these conditions, crystallization of high-magnesian olivines occurs (Fo = 97–98 mol %). The composition of the fluid is similar to the composition of the fluid from inclusions in synthetic diamonds. The conditions implemented in the experiment might have occurred at the early stages of the Earth’s evolution.
AB - The first results on the interaction between an Fe–Ni melt and anthracene (С14Н10) in the presence of olivine at 3 GPa and 1500°С and on the study of the component composition of the fluid generated in this process are presented. The stability of aliphatic hydrocarbons in the implemented conditions is confirmed experimentally. It is established that, under these conditions, crystallization of high-magnesian olivines occurs (Fo = 97–98 mol %). The composition of the fluid is similar to the composition of the fluid from inclusions in synthetic diamonds. The conditions implemented in the experiment might have occurred at the early stages of the Earth’s evolution.
KW - diamond
KW - Fe–Ni melt
KW - fluid
KW - high pressures and high temperatures
KW - hydrocarbons
KW - olivine
KW - Fe-Ni melt
KW - POLYCYCLIC AROMATIC-HYDROCARBONS
KW - IRON
KW - DIAMONDS
KW - PLACERS
UR - http://www.scopus.com/inward/record.url?scp=85087522854&partnerID=8YFLogxK
U2 - 10.1134/S1028334X20050050
DO - 10.1134/S1028334X20050050
M3 - Article
AN - SCOPUS:85087522854
VL - 492
SP - 333
EP - 337
JO - Doklady Earth Sciences
JF - Doklady Earth Sciences
SN - 1028-334X
IS - 1
ER -
ID: 24720300