Melt inclusion record of immiscibility between silicate, hydrosaline, and carbonate melts: Applications to skarn genesis at Mount Vesuvius

被引:5
作者
Fulignati, P
Kamenetsky, VS
Marianelli, P
Sbrana, A
Mernagh, TP
机构
[1] Univ Pisa, Dipartimento Sci Terra, I-56126 Pisa, Italy
[2] Univ Tasmania, Sch Earth Sci, Hobart, Tas 7001, Australia
[3] Univ Tasmania, Ctr Ore Deposit Res, Hobart, Tas 7001, Australia
[4] Australian Geol Survey Org, Canberra, ACT 2601, Australia
关键词
Vesuvius; skarn; melt inclusions; immiscibility;
D O I
10.1130/0091-7613(2001)029<1043:MIROIB>2.0.CO;2
中图分类号
P5 [地质学];
学科分类号
0709 [地质学]; 081803 [地质工程];
摘要
Foid-bearing syenites and endoskarn xenoliths of the A.D. 472 Vesuvius eruption represent the magma chamber-carbonate wall-rock interface. Melt inclusions hosted in crystals from these rocks offer a rare opportunity to depict the formation and the composition of metasomatic skarn-forming fluids at the peripheral part of a growing K-alkaline magma chamber disrupted by an explosive eruption. Four principal types of melt inclusions represent highly differentiated phonolite (type 1), hydrosaline melt (type 3), unmixed silicate-salt melts (type 2), and a complex chloride-carbonate melt with minor sulfates (type 4). The high-temperature (700-800 degreesC) magmatic-derived hydrosaline melt is considered to be the main metasomatic agent for the skarn-forming reactions. The interaction between this melt (fluid) and carbonate wall rocks produces a Na-K-Ca carbonate-chloride melt that shows immiscibility between carbonate and chloride constituents at similar to 700 degreesC in 1 atm experiments. This unmixing can be viewed as a possible mechanism for the origin of carbonatites associated with intrusion-related skarn systems.
引用
收藏
页码:1043 / 1046
页数:4
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