Skip Navigation

This Article
Right arrow Full Text Freely available
Right arrow FREE Full Text (PDF) Freely available
Right arrow Alert me when this article is cited
Right arrow Alert me if a correction is posted
Services
Right arrow Email this article to a friend
Right arrow Similar articles in this journal
Right arrow Similar articles in ISI Web of Science
Right arrow Alert me to new issues of the journal
Right arrow Add to My Personal Archive
Right arrow Download to citation manager
Right arrow Search for citing articles in:
ISI Web of Science (12)
Right arrowRequest Permissions
Google Scholar
Right arrow Articles by LIU, T.-C.
Right arrow Articles by PRESNALL, D. C.
Right arrow Search for Related Content
GeoRef
Right arrow GeoRef Citation
Social Bookmarking
 Add to CiteULike   Add to Connotea   Add to Del.icio.us  
What's this?

Journal of Petrology Volume 41 Number 1 Pages 3-20 2000
© Oxford University Press 2000

Liquidus Phase Relations in the System CaO–MgO–Al2O3–SiO2 at 2·0 GPa: Applications to Basalt Fractionation, Eclogites, and Igneous Sapphirine

T.-C. LIU1 and D. C. PRESNALL2,*

1DEPARTMENT OF EARTH SCIENCES, NATIONAL TAIWAN NORMAL UNIVERSITY, TAIPEI 117, TAIWAN
2MAGMALOGY LABORATORY, DEPARTMENT OF GEOSCIENCES, UNIVERSITY OF TEXAS AT DALLAS, RICHARDSON, TX 75083-0688, USA

To model magmatic crystallization processes for mafic to intermediate compositions at high pressure, liquidus phase relations in the forsterite–anorthite–diopside–silica (FADS) tetrahedron within the CaO–MgO–Al2O3–SiO2 system have been determined at 2·0 GPa. Compositions of five liquidus invariant points have been determined and the approximate compositions of five others have been inferred. These involve primary phase volumes for forsterite (fo), enstatite (en), diopside (di), high quartz (qz), spinel (sp), sapphirine (sa), garnet (gt), anorthite (an), and corundum (cor). The determined (with wt % coefficients) and inferred reactions (without coefficients) that define each isobaric invariant point are as follows:

23 en + 68 di + 9 sp = 84 liq + 16 fo

37 di + 63 sa = 47 liq + 40 sp + 13 en

100 gt = 21 liq + 27 sa + 55 en + 18 di

1 di + 59 en + 41 an = 43 liq + 57 gt

18 di + 21 qz + 15 en + 47 an = 100 liq

di + an + gt = liq + sa

an + gt = liq + sa + en

sa + an + di = liq + sp

sa + an = liq + cor + sp

di + cor = liq + an + sp.

These phase relations provide a diverse range of constraints on igneous processes at pressures near 2 GPa. They show that fractional crystallization of a model basalt gives a residual liquid strongly enriched in SiO2, strongly depleted in MgO, and mildly enriched in Al2O3. Such a trend is consistent with the calc-alkaline fractionation trend observed at subduction zones, but is in disagreement with suggestions that fractionation of tholeiitic basalt in this pressure range yields an alkalic basalt. Both trends may occur for natural basalts depending on the Na2O content of the parental magma. Also, the data show that the minimum pressure for the formation of cumulate eclogites and garnet pyroxenites is about 1·8–1·9 GPa. The lower limit of pressure at which sapphirine can crystallize from a liquid in the FADS tetrahedron is estimated to be 1·1–1·5 GPa and the upper limit is >3 GPa. Sapphirine crystallizes from magmas intermediate in composition between basalt and andesite. Probable igneous sapphirine in mafic associations is rare, but it occurs as part of a pyroxenite xenolith from Delegate, Australia, that we suggest is a cumulate assemblage and in a sapphirine norite at Wilson Lake, Labrador, Canada.

KEY WORDS: basalt; eclogite; sapphirine; fractional crystallization


Add to CiteULike CiteULike   Add to Connotea Connotea   Add to Del.icio.us Del.icio.us    What's this?


This article has been cited by other articles:


Home page
J PetrologyHome page
D. C. Presnall and G. H. Gudfinnsson
Origin of the Oceanic Lithosphere
J. Petrology, April 1, 2008; 49(4): 615 - 632.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
S. Keshav, G. Sen, and D. C. Presnall
Garnet-bearing Xenoliths from Salt Lake Crater, Oahu, Hawaii: High-Pressure Fractional Crystallization in the Oceanic Mantle
J. Petrology, September 1, 2007; 48(9): 1681 - 1724.
[Abstract] [Full Text] [PDF]


Home page
Can MineralHome page
X. Liu and H. St.C. O'Neill
EFFECTS OF P2O5 AND TiO2 ON THE PARTIAL MELTING OF SPINEL LHERZOLITE IN THE SYSTEM CaO-MgO-Al2O3-SiO2 AT 1.1 GPa
Can Mineral, June 1, 2007; 45(3): 649 - 655.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
A. ULIANOV and A. KALT
Mg-Al Sapphirine- and Ca-Al Hibonite-bearing Granulite Xenoliths from the Chyulu Hills Volcanic Field, Kenya
J. Petrology, May 1, 2006; 47(5): 901 - 927.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
T. KOGISO, M. M. HIRSCHMANN, and M. PERTERMANN
High-pressure Partial Melting of Mafic Lithologies in the Mantle
J. Petrology, December 1, 2004; 45(12): 2407 - 2422.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
X. LIU and H. ST. C. O'NEILL
Partial Melting of Spinel Lherzolite in the System CaO-MgO-Al2O3-SiO2 {+/-} K2O at 1{middle dot}1 GPa
J. Petrology, July 1, 2004; 45(7): 1339 - 1368.
[Abstract] [Full Text] [PDF]


Home page
American MineralogistHome page
A.G. Christy, Y. Tabira, A. Holscher, E.S. Grew, and W. Schreyer
Synthesis of beryllian sapphirine in the system MgO-BeO-Al2O3-SiO2-H2O and comparison with naturally occurring beryllian sapphirine and khmaralite. Part 1: Experiments, TEM, and XRD
American Mineralogist, August 1, 2002; 87(8-9): 1104 - 1112.
[Abstract] [Full Text] [PDF]


Home page
Can MineralHome page
Y.-H. Weng and D. C. Presnall
THE SYSTEM DIOPSIDE FORSTERITE ENSTATITE AT 5.1 GPa: A TERNARY MODEL FOR MELTING OF THE MANTLE
Can Mineral, April 1, 2001; 39(2): 299 - 308.
[Abstract] [Full Text] [PDF]


Home page
J PetrologyHome page
G. H. GUDFINNSSON and D. C. PRESNALL
Melting Behaviour of Model Lherzolite in the System CaO-MgO-Al2O3-SiO2-FeO at 0{middle dot}7-2{middle dot}8 GPa
J. Petrology, August 1, 2000; 41(8): 1241 - 1269.
[Abstract] [Full Text] [PDF]



Disclaimer:
Please note that abstracts for content published before 1996 were created through digital scanning and may therefore not exactly replicate the text of the original print issues. All efforts have been made to ensure accuracy, but the Publisher will not be held responsible for any remaining inaccuracies. If you require any further clarification, please contact our Customer Services Department.