JOURNAL OF PETROLOGY VOLUME 37 NUMBER • PAGES ffll-636 1996 ANTHONY R. PHILPOTTS*, MAUREEN CARROLL and JAMES M. HILL DEPARTMENT OF GEOLOGY AND GEOPHYSICS, UNIVERSITY OF CONNECTICUT, STORRS, CT 06269, USA Crystal-Mush Compaction and the Origin of Pegmatitic Segregation Sheets in a Thick Flood-Basalt Flow in the Mesozoic Hartford Basin, Connecticut Where the Holyokeflood-basaltflowin the Mesozoic Hartford & Horter, 1993; Wheelock & Marsh, 1994). Similar Basin in Connecticut is thick and contains coarse-grained, hori-sheets are found in the Hawaiian lava lakes (Richter zontal segregation sheets in its central part, the lower part of the & Moore, 1966; Moore & Evans, 1967; Wright & flow is strongly depleted in incompatible elements; where the Okamura, 1977; Helz, 1980) and in many basaltic sills and shallow intrusions (Carman, 1994; Larsen & flow is thin and contains no segregation sheets it is homogeneous throughout. This chemical variation can be explained only Brooks, 1994; Marsh & Wheelock, 1994). through compaction of the partly crystallized basalt. The com- Two distinct types of segregation sheet are recogposition of the segregation sheets shows that they separatedfrom nized, a more abundant coarse-grained basaltic type, the basalt following only 33% crystallization. The segregation and a fine-grained granophyric (granitic) variety. sheets, however, are clearly intrusive into the basalt, which must The composition of the basaltic type corresponds to therefore have alreadyformed a crystal mush withfinitestrengthliquids that would form after as little as ~25% at this low degree of crystallinity. The incompatible element crystallization of the host basalt, and the granoconcentrations indicate that the partly crystallized basalt phyric type, following ~75% crystallization. The underwent as much as 28% compaction in the lowest 60 m of segregation of the liquids is thought normally to the flow. Between 60 and 130 m above the base of theflow,the have resulted from some type of filter pressing. crystal mush became dilated, and eventually ruptured with for- Although this might be expected in the case of latemation of the segregation sheets. No segregation sheet has a forming granophyric liquid, separation of the composition indicating separation after more than 33% crys- basaltic fraction from a still largely molten parent is tallization of the basalt. This is interpreted to indicate that more difficult to envision. Clearly the rheological compaction ceased at this stage because of the increasing properties of partly crystallized basalt must play an strength of the mush and the increasing density of the fraction- important role in the formation of these sheets. ating interstitial liquid Detailed sampling through a thick flood basalt, which contains many segregation sheets, in the Basin of Connecticut has allowed where in the flow the segregation liquid was derived and the degree of solidification of the host basalt at the time of formation of the segregation sheets. The data indicate that the basalt, when only one-third crystallized, already formed a rigid, but elastic, framework, which was capable of being fractured but through which residual liquid was able to move by porous flow. The generation of these fractionated rocks in the relatively simple KEY WORDS ciystal-mush compaction; segrtgation shtets; flood Mesozoic Hartford basalt; tholeiitie; Connecticut us to identify from INTRODUCTION The central parts of thick tholeiitieflood-basaltflows commonly contain thin sheets of rock that apparently have formed from fractionated residual liquids (Cornwall, 1951; Lindsley et al., 1971; Dostal & Greenough, 1992; Greenough & Dostal, 1992; Puffer *Corre»ponding author. e-mail; [email protected] I Oxford Univerrity Preu 1996 JOURNAL OF PETROLOGY VOLUME S7 environment of a crystallizing flood basalt provides insight into mechanisms that also must operate in magma chambers at depth, where interpretation is complicated by other factors, such as magma replenishment and mixing, and wallrock assimilation. FIELD RELATIONS The Hartford Basin in Connecticut (Fig. 1) contains three flood-basalt units, which are of early Jurassic age (Puffer et al., 1981). All three contain segregation sheets, but the Holyoke Basalt, which was the second to erupt, contains the thickest and most abundant sheets. This basalt is also the thickest of the three flood-basalt units, typically being ~100 m thick. Its original lateral extent is uncertain but, in addition to occurring in the Hartford Basin, it is found to the west in the Southbury Basin, and the Deerfield Basalt in the Deerfield Basin to the north (Fig. 1) is stratigraphically correlative (Luttrell, 1989). The flow must therefore have extended for > 150 km in a north-south direction and at least 50 km east—west. Deerfield Basin Holyoke Basalt Southbury Basin 0 tO 20 30 40 Fig. 1. Outline map of the Mesozoic Hartford Basin and the smaller Deerfield and Southbury buini. The eutward-dipping sedimentary rocks of the hatinj are interrupted near the Triassic— Jurauic boundary by three flood basalts, the middle and thickest of which is the Holyoke Basalt. Sills (diagonal rule) related to the first flood basalt occur near the base of the Mesozoic succession. Feeder dikes to the flood basalts are shown by heavy lines. NUMBER 4 AUGUST 1996 The Holyoke Basalt, like all of the rocks in the Hartford Basin, dips gently eastward as a result of the greater down-drop of the basin rocks on the eastern border fault than on the western one. The basalt consequently forms a north-south-trending ridge through the basin. At Tariffville, the Farmington River cuts through the ridge to form a prominent gorge, which provides a complete section through the flow. The continuous exposures of basalt in the gorge and in road cuts on both sides of the river were mapped using an electronic total station, which measures horizontal and vertical angles relative to a given reference frame (e.g. north and horizontal), and it measures distances by determining the travel time of a laser beam bounced off a prism held at the point to be surveyed. From these measurements, the instrument calculates internally the x (east), y (north), and z (vertical) coordinates of the surveyed point to millimeter accuracy. These values can be down-loaded directly into a portable computer in the field, thus providing a rapid and accurate way of collecting three-dimensional field data. Thus, despite the length of the exposure through the gently dipping (23°) flow, we were able to calculate the original stratigraphic positions of all contacts and sample locations in the flow with considerable accuracy. The section of Holyoke Basalt exposed in the Tariffville gorge is 174 m thick. The flow is underlain and overlain by lacustrine sediments, many of which contain salt casts, indicative of a playa lake environment. The great thickness of the basalt at this locality cannot, therefore, be attributed to the filling of an erosional channel. Instead, the locality may have been near the center of the Hartford basin, and thus it experienced the deepest ponding of the basalt. The flow can be divided into upper and lower parts based on the nature of fractures. The upper part is characterized by irregularly oriented fractures, which give the outcrop a blocky appearance, whereas the lower part is characterized by vertical fractures which commonly break the rock into meter-long slender prisms. In places, colonnade-type joints with horizontal striations are present in the lower part of the flow, but most of these columns appear to have broken into the vertical splinter-like joints. The boundary between the upper and lower parts of the flow in the Tariffville section occurs 97 m above the base, that is, 55% of the way up through the flow. In contrast, the boundary between colonnade and entablature style jointing in most thick flows is ~ 20-40% of the height of the flow (Long & Wood, 1986; Marsh, 1988). The upward 812 PHILPOTTS et d. CRYSTAL-MUSH COMPACTION displacement of this boundary in the Tariffville section probably results from a redistribution of heat within the flow during the formation of the segregation sheets (see, e.g. Moore & Evans, 1967), as described below. The surface of the flow was weathered in the Mesozoic before being buried beneath sediments. No erosion took place, however, as indicated by the preservation of flow-top features, such as scoria, rafted crustal slabs, and even ropy structures. The section therefore still preserves the original flow thickness. During weathering, the primary minerals in the upper part of the flow were completely altered (to clay and carbonate minerals), which makes it impossible to obtain reliable whole-rock chemical analyses from the upper third of the flow. From textures, however, the types and abundances of the phenocrysts and the nature of the groundmass can still be determined. Although the flow top and lower chilled margin contain abundant vesicles which are now filled with chlorite, carbonate, quartz, and zeolites, the rest of the flow is completely devoid of them, except near the tops of segregation sheets. The main part of the flow appears to have purged itself of gas bubbles early in the cooling history, but gas that was exsolved during the final stages of crystallization did produce a dictytaxitic texture, which occurs throughout the basalt and the segregation sheets. These late-forming gas cavities are typically filled with chlorophaeite. The basaltic segregation sheets are distinguished from the host basalt by their coarser grain size and dark brown color on the weathered surface; the basalt weathers a rusty orange. In addition, the sheets are not as closely jointed as the basalt, and their fracture surfaces are much rougher. The strike and dip of the sheets is precisely the same as that of the flow itself, and therefore they must originally have been horizontal. The sheets occur in a central zone extending from 70 to 85 m above the base of the flow (Fig. 2). The zone contains 15 sheets which are spaced ~ 1 m apart. Most sheets are a few decimeters thick, but the lowest one is 2 m thick. Their cumulative thickness is 3-9 m, which is 26% of this central zone. They are laterally extensive, with the thicker sheets being traceable from one side of the gorge to the other, a distance of at least 400 m. Some are seen to thin and pinch out, but in such cases their stratigraphic position in the flow is marked by a horizontal fracture. Others are seen to bifurcate (Fig. 3) or to connect with underlying or overlying sheets via short dikes (Fig. 4). The matching of irregularities in the contacts on opposing sides of such dike—sheet 813 intersections indicates that room for the segregation liquid was created by dilation of fractures in the host basalt. However, no angular corners are found on the contacts; instead, they are all rounded. Similar plastic, intrusive relations have been described from the prehistoric Makaopuhi lava lake in Hawaii (Moore & Evans, 1967). The contacts on all but the lowest of the segregation sheets at Tariflville are sharp. The upper contact on the lowest sheet is also sharp, but the lower contact is gradational over a few decimeters. The fine-gTained granophyric segregation sheets, which are typically ~ 1 cm thick, occur toward the tops of basaltic segregation sheets, in the fine-grained basalt immediately overlying these sheets, and as extensions from the tapering ends of these sheets. For comparison, we have also studied the Holyoke Basalt in a section from the Southbury Basin (Fig. 1), where the flow is thinner and contains no segregation sheets. A series of cuestas in this highly faulted basin provide exposures through the eastwarddipping flow. The 57-m-thick flow has a welldeveloped colonnade in the lower 15 m, which is overlain by an entablature and a scoriaceous flow top. Thus the boundary between the colonnade and entablature in this exposure of the Holyoke Basalt is more typical in being at 37% of the flow's height. The basalt at this locality has well-preserved immiscible glasses in its mesostasis (Philpotts, 1979; Philpotts & Doyle, 1983). PETROGRAPHY At Tariffville, the upper part of the flow that is characterized by irregular fractures, and the lower chilled margin contain a small percentage of millimeter-size phenocrysts of plagioclase and microphenocrysts of totally altered olivine in a groundmass of plagioclase, augite, and pigeonite crystals, with a mesostatis characterized by dendritic magnetite crystals and micron-size droplets of ironrich immiscible liquid (now opaque spheres). Throughout the rest of the flow, plagioclase (An73_63) is the only phenocrystic mineral ( < 5 % ) , olivine having been reacted out to form pigeonite. The groundmass consists of a fine-grained subophitic intergrowth of plagioclase (An<63), augite (\Vo34En52-36Fsi6_3o), and pigeonite (WoiiEn 5 ,_4 3 Fs38^t6) (Fig. 5), with equant, subhedral grains of magnetite in a felsic mesostasis. The grain size of the basalt remains fine throughout, despite the great thickness of the flow. The basaltic segregation sheets, however, are coarse grained, with centimeter-long bladed crystals of plagioclase (An €0 _ w ) and pyroxene forming a JOURNAL OF PETROLOGY VOLUME 37 NUMBER • AUGUST 1996 E T -•-65 Fig. 2. Vertical section through the central part of the Holyoke Basalt exposed in the road-cut (outlined) on the north side of the Farmington River gorge at Tariflville, Connecticut. The section has been rotated 23° to restore the lava to its original horizontal position. The zone between 70 and 85 m above the base of the flow contains coane-grained basaltic segregation sheets (black) which transgress the fine-grained host basalt. Boxes indicate areas shown in more detail in Figs 3 and 4. Fig. 3. Bifurcation in a segregation sheet (see center of Fig. 2). (Note the bullet-nosed termination on the finger of basalt, which suggests plastic behavior at the time of intrusion of the segregation sheet.) subophitic texture with a mesostasis of a feathery to granophyric intergrowth of alkali feldspar and tridymitc, and skeletal crystals of titanifcrous magnetite. Most pyroxene laths consist of a core of pigeonite (altered) rimmed by augite (\V033_37En52_21 FS15-42) (Fig. 5), both of which contain exsolution lamellae of the other. These lamellae typically form a herring-bone pattern because of the presence of a 814 PHILPOTTS ttd. CRYSTAL-MUSH COMPACTION Fig. 4. Intrusive relationj of the tegregation theett in the bauJt (fourth theet up in Fig. 2). DtoptW* htadwitwrgit* Augit* w O,lv1n, ;"°n»' , „ +./W o io Bilt (lit* Fig. 5. Pyroxene composition! in the batalt ( • ) , the coarsegrained tegregation iheeU ( • ) , and the granophyre theeti ( + ) in the Holyoke Basalt at TariflVille, plotted following the method of Iindiley (1983). Pigeonite occun in the tegregation theets but u too altered for analysu. Olivinc it alto totally altered in the rockt. central twin in the pyroxene lath. Some reddish brown interstitial patches of alteration material were initially fayalitic olivine crystals, but most of them are dictytaxitic cavity fillings, as evidenced by their concentric banding. Plagioclase and pyroxene laths are locally up to 10 cm long (Emerson, 1905). Many of them are curved, commonly through angles of >90° (Fig. 6a). This apparently resulted from deformation during growth, and in extreme cases the crystals were actually broken (Fig. 6b). In parts of the thicker sheets, the febic mesostasis is segregated into centimeter-size blobs, which commonly have a quartz and carbonate amygdale at their center. The amygdales are more abundant toward the tops of thick sheets, or where the sheets are thin. The granophyre sheets are fine grained and consist of a cloudy alkali feldspar, tridymite needles, brownish green ferrohedenbergite (Wosg.jEnj.jFsss), altered fayalitic olivine, magnetite, and minute needles of apatite. Amygdales filled with quartz, bladed albite crystals, and carbonate are common. In thin section, the lower sides of granophyre sheets are seen to have small, irregular veinlets cutting the underlying basalt (Fig. 7). These could have been the conduits through which the granophyre liquid entered the horizontal sheets. The Holyoke Basalt in the Southbury exposure is much fresher than that in the Hartford Basin, and even has unaltered glass preserved in its mesostasis. The basalt is remarkably constant in appearance throughout most of the flow and consists of scattered phenocrysts of plagioclase set in a fine-grained, subophitic groundmass of plagioclase and pyroxene crystals, with a dark mesostasis consisting of immiscible iron- and silica-rich glasses. Many of the Ferich globules have crystallized to form spheres of pyroxene and magnetite. The mesostasis constitutes 32% of this rock (Philpotts, 1982). The rock's texture changes significantly across the lowest 9 m even though its composition remains essentially the same (Philpotts & Doyle, 1983). The abundance of Fe-rich globules decreases toward the base of the 815 JOURNAL OF PETROLOGY VOLUME 37 NUMBER • AUGUST 1996 Fig. 6. (a) Bent crystal of pyroxene in segregation sheet (width of Geld is 8 mm), (b) Bent and broken cryital of plagiodase in segregation iheet (width of field is 2 mm). flow and none are present below 5-6 m. Instead, the and under controlled oxygen fugacities. The results mesostasis consists of a clear Si-rich glass that con- of these studies have been compiled in Fig. 8. tains equant-shaped magnetite crystals. Analyses Philpotts & Reichenbach (1985) studied the nearshow that the flow becomes more oxidized toward liquidus phase relations in representative samples of the base, and this caused magnetite to crystallize each of the three basalt units in the Hartford Basin earlier there and prevent the iron enrichment to determine their possible eruption temperatures. necessary to fractionate the residual liquid into the ' The sample of Holyoke Basalt was from the base of immiscibility field (Philpotts & Doyle, 1983). This the flow in the Tariffville gorge. The experiments oxidation probably resulted from interaction of the show that this basalt is saturated with both olivine ponded lava with the underlying red beds. and plagiodase on its liquidus and that augite and pigeonite appear only 20°G below this. With falling temperature, olivine decreases and pigeonite increases in abundance, as would be expected from a PREVIOUS EXPERIMENTAL reaction relation, but at the lowest temperature investigated (1125°C), olivine was still not comSTUDIES Three different experimental studies have been pletely eliminated. Based on previous lower-temcarried out on the Holyoke Basalt at low pressure perature experiments (Philpotts & Doyle, 1983) 816 PHILPOTTS tt at CRYSTAL-MUSH COMPACTION Fig. 7. Base of a fine-grained 1-cm-thick granophyre sheet near the top of a coarse-grained basaltic segregation sheet. Small granophyre veinlets connect with the lower side of the granophyre sheet (see to the right of the photograph). The base of the granophyre sheet is mounded up around the veinlet in a manner similar to the chimneys produced in laboratory experiments by channelized buoyant liquid rising from a crystallizing mush (Tait * Jaupart, 1992). Width of photomicrograph is 8 mm. olivinc is known to be absent at 1100°C, so a postulated olivine-out line has been inserted as a dashed line in Fig. 8 at ~1120°C. In the earlier study, phase relations just above the solidus of the Holyoke Basalt were investigated to determine whether the immiscible liquid droplets found in the mesostasis of this rock were the products of stable or metastable immiscibility (Philpotts & Doyle, 1983). The results show that the residual liquid in the basalt enters a stable two-liquid field on cooling below 1020°C at oxygen fugacities near the quartz-fayalite-magnetite (QFM) buffer. However, at the higher oxygen fugacities of the nickel—nickel oxide (NNO) buffer, no two-liquid field is encountered, because of the earlier crystallization of magnetite at these higher oxygen fugacities (Fig. 8). On the low-temperature side of the two-liquid field, crystallization of magnetite consumes the iron-rich immiscible liquid and only the silica-rich liquid remains, which eventually crystallizes at ~980°C. The experiments demonstrate that oxygen fugacity plays a crucial role in determining whether immiscible liquids form. Although the sample of basalt 1180 1160 1140 1120 ° 1100 3 1080 e L + PI + 2P> + Mt 8.1060 ' L/+ PI + 2Py 4 Mt + Tr £ 1040 1020 1000 13 12 11 10 980 Fig. 8. Experimentally determined phase relations in the Holyoke Basalt from Philpotu (1979), Fhilpotts & Doyle (1983), and Philpotts & Reichenbach (1985). The heavy dashed line marks the experimentally measured intrinsic oxygen fiigacity of the rock. 817 JOURNAL OF PETROLOGY VOLUME 37 used in this study is from the Southbury Basin, its composition is almost identical to that used in the higher-temperature study from the base of the flow at Tariffville (see Tables 1 and 2). In a still earlier study of the basalt from the Southbury Basin, Philpotts (1979) measured the intrinsic oxygen fugacity of this rock with an yttrium-doped zirconia cell. The measurements indicate that, at 1150°C, the oxygen fugacity was near that of the magnetite—wiistite (MW) buffer but, by 1000°C, it had risen to almost the QFM buffer (Fig. 8). These experimental results provide a framework with which to interpret the crystallization history of the Holyoke Basalt and the fractionation that led to the development of the segregation sheets. Because the chilled margins of the flow contain only a few percent phenocrysts of plagioclase and olivine, the basalt must have been erupted near its liquidus temperature at ~1160cC and under oxygen fugacities between those of the MW and QFM buffers. Despite a brief period during which only plagioclase and olivine crystallized, the Holyoke Basalt must have been multiply saturated with plagioclase, augite, and pigeonite throughout most of its crystallization history, with the early crystallizing olivine reacting out to form pigeonite. When a tholeiitic basalt is multiply saturated, its rate of solidification changes almost linearly with temperature (Ryerson et al., 1988). Thus, if olivine reacted out by 1120°C, the basalt would have been ~25% crystallized at this stage. At lower temperatures, better estimates of the fraction crystallized can be made using the nonlinear relation of McKenzie & Bickle (1988) which is based on many careful experimental studies, but the differences from the linear extrapolation are only a few percent. According to this relation, plagioclase, augite, and pigeonite would have been joined by magnetite after ~ 6 3 % crystallization of the basalt, and after 71% crystallization, the residual liquid would have entered the two-liquid field, with the generation of silica-rich and iron-rich immiscible liquids. CHEMISTRY OF THE FLOW To obtain an accurate picture of the compositional variation through the flow at Tariffville, samples were collected at ~5-m intervals, except in the zone of the segregation sheets where the interval was decreased so that any migration of residual liquids towards the sheets might be detected. The location of each sample in the flow was determined with the electronic total station. Obtaining representative analyses of the coarse-grained segregation sheets was NUMBER 4 AUGUST 1996 difficult because of their coarse grain size and blotchy distribution of felsic mesostasis. Samples for analysis of a sheet were prepared by crushing sawn slabs that passed through the entire sheet. Care was taken to avoid amygdales, but dictytaxitic cavity fillings could not be eliminated. Despite these precautions, analyses of the sheets appear slightly variable. Whole-rock X-ray fluorescence (XRF) analyses for the major elements were done on glass disks prepared by fusing two parts lithium tetraborate with one part rock, whereas the trace elements were done on pressed-powder pellets. The analyses were performed on a Kevex Delta analyzer, equipped with a thin-windowed energy-dispersive detector and a multiple X-ray target head, which allows the excitation radiation to be selected so as to maximize the peak to background counts for any given group of elements. Five different targets were used for each major-element analysis and for each trace-element analysis. Analyses were calibrated against US Geological Survey standards BCR-1 and W-l, which were run with each batch of samples. Estimated relative errors, based on replicate analyses of W-l, are < 1 % for the major elements except for Na (5%), Mg (1-7%), K (1-5%), and P (10%). Estimated relative errors for the trace elements are 5% for V, Cr, Ni, Cu, Zn, Sr, and Zr, and 10% for Rb, Y, Nb, and Ba. Quantification was through the Toolbox software. Ferrous iron was determined in each sample by the vanadate method (Wilson, 1955). Mineral analyses were obtained using an M.A.C. 5 electron microprobe equipped with a Kevex Quantum energy-dispersive detector. The electron beam was operated at 15 kV and 800 pA. Spectra were processed and quantified with the Quantex software, which is based on the MAGIC V ZAF correction procedure. The analytical results, CIPW norms, and stratigraphic heights of the Tariffville samples are given in Table 1 and those of the Southbury samples in Table 2. Analyses of samples from the highly altered upper part of the Tariffville section are not included in Table 1, but analyses 26, 27, and 28 already show signs of this alteration. Their lack of normative quartz and elevated Sr are probably a result of alteration. These analyses have been included, however, because elements such as Ti, Zr, Nb, P, and Y have been shown to be relatively immobile during the low-grade zeolite type of metamorphism to which these rocks were exposed (Wood et al., 1976). With these elements we can compare the upper part of the flow with the lower part, which is essentially unaltered. Despite the homogeneous appearance of the basalt in the Tariffville section, the analyses reveal a 818 CRYSTAL-MUSH COMPACTION ; 2 3 S 2 en o 9 CM eh CM ch T 2 -2 IO O O iCN ch CN c< a cp en ch CN to CD CO CN 6 tb o CM O) f;cn O CM o CM Q cp en eh CM 6 cn 6 en cp CM ch o u> cn 81-29 9 6 o CO co LQ ch CM 2-44 3 66 9-83 0-14 0-19 9-20 2-44 5-79 5-65 0-19 0-18 8-98 2-45 ^h 6 o r- 82 0-18 0-19 0-19 1-59 9-84 9 28 6 9-99 14-48 •51 2 OD 200 A <T> CN CM 19-95 ch cn 5-21 CO s ch CD a s 8 P CO s 3 - S in o in o CM 8 8 CD cn cn cn "~ CN CO S en i~ o o o og 6 6§ JQ ^» ^^ fxy co co c3 oo ^^ fi& ff^ ^p ^^ «~ cn »— cn r*» oo *~ cn CM r*> CM co cn to r«- SN 8 g 6 CM 2 cn ri 6 66 6 ^» c n c M c p c n c n o o o c n r * r * p « . 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V CM ch 80-72 cn en s -2 a 8 § C» 3-14 ID CM 9-65 CO Jo? 33 78-65 r* 74-24 CO 69-35 en 67-68 s 84-37 PHILPOTTS tt aL f? ? 8 6 6 8 f? ? f o o g If s 819 ^S en t c n c n o o c n c o c n ^^t tLLoo cc o o r ^ e M c o rt • - • - JOURNAL OF PETROLOGY * CM «- ** cn I D VOLUME 37 NUMBER 4 AUGUST 1996 CM CM m o i r t u i i l » i 5 m v iococM«cbobco^-6 N r» o CM «- w- w- en co at co n h o i o n n IN r O CO S LO 69-36 CO 74-24 OOvfCNCpLOCOCncNr* r - n o i y i y c p i n n p _ 67-68 CO 66- cn 63- LO CM - s CM IM • - r- O) «O ss coiocMcooococncnrCM . Tf^-cocM^-ci^-r-cMeb cn CM co ^ LD CM CM cn c N p L p o p c p c p c n c n p I D r N N r 6 ^ < b n 6 "~ LO CM rp~ r* co at L p i a c M c p m L p r - e > < r p* co o LO cn co Th r— o N M r i- co^cn ( b n c b o b h 6 n r - 6 r- IN CM » - CM CM ^* ^- tn cn CM o f o i o i LO r* CN o) CM cn 00 IM CM "~ § io CO LO CO Oi LO CO LO o i c o c M O r - L o r - o co o cn co at co ^ o CM CM CO CN CM T- o <n o o cn _ _-,cMr**r^r**(o in c M ^ - T f c M c n 6 i n c n c o 6 cn r- r« s CO CM 9 CM r» r- ^ CM i- O N ^ s m CM cn s 4-31 29-62 24-73 17-18 16-14 2-45 1-58 007 23-44 2501 18-37 22-72 2-31 1-65 0-07 25-18 17-59 IN 25-47 2-15 s 4-14 CO CM CM CM •21 •32 $ -94 LO LO 3 s S LO c M c b ^ r c M c n o c b o b c o o coo>cp!NcMcn*-cnr~LO c M O i o c M c h o L b c h c o o 23-16 20-49 3-6 1-79 4-22 1-29 3-42 1-88 0-14 r- n . 0-14 17-72 16-41 7-33 1-71 25-27 26-88 0-22 2-12 23-52 19-46 4-55 4-37 1-49 4-73 6-56 4-56 6-85 9 | a 99-1 0-54 LO at CM Vl-0 0-09 C M O ^ - C N O O « C f O C N O 3 X S CN •- ib E 1 -5 820 Pjo, 002 0-05 0-07 0-02 0-05 005 0-08 002 0-06 0-10 0-13 0-10 006 10000 100-00 100-00 100-00 100-00 10000 100-00 10000 10000 100-00 10000 10000 100-00 275 259 165 264 206 246 176 337 273 311 186 257 412 13 16 19 18 23 17 21 21 35 37 16 29 4 Tl 5773 5808 5827 5939 5830 5937 6055 5771 8656 8512 8462 8543 2553 V 334 330 357 362 355 356 361 335 368 352 351 357 33 4 11 23 14 11 9 6 13 0 0 0 0 0 1522 1454 1563 1665 1605 1894 1662 1709 1933 1672 1826 1810 550 pjun. S Sc Cr Mn Ni 31 35 42 40 36 34 30 35 32 18 14 21 18 Cu 59 64 59 68 68 64 66 66 104 141 138 128 36 Zn 87 88 90 98 96 101 95 78 113 94 101 102 90 Rb 18 17 19 24 22 26 17 9 39 21 41 33 72 77 Sr s 135 143 148 149 134 207 306 201 229 136 219 195 Y 29 28 30 28 28 26 28 27 39 47 42 42 60 Zr 86 80 89 82 87 75 85 77 122 118 118 119 366 Nb 6 6 5 3 6 4 6 4 8 9 6 7 14 Bo 143 119 143 97 144 105 139 154 314 151 191 219 552 La 29 18 17 23 16 15 17 25 33 34 15 27 28 Ce 47 22 23 21 30 21 26 34 74 50 35 53 46 CIPWnorm Q 3-85 2-4 7-36 Or 3-84 4-37 408 Ab 23-27 24-71 An 24-15 Cpx 20-29 Opx 18-3 4-58 11-21 705 7-61 43-72 a o 5-55 408 6-85 3-9 508 5-28 10-64 34-1 35-29 31-31 26-32 19-04 2903 24-80 15-65 22-81 1808 17-03 21-16 19-48 23-42 16-99 19-96 11-12 17-69 16-49 19-25 22-19 15-14 18-46 1202 15-21 4-79 4-79 18-7 28-26 28-26 24-35 27-52 22-81 21-93 18-27 17-69 609 1688 1706 20-36 20-36 16-65 9-22 12-11 17-85 12-74 22-67 17-76 Mt 4-31 3-25 4-87 3-07 3-07 3-51 3-58 2-97 6-74 7-41 406 607 2-54 II 1-81 1-84 1-84 1-84 1-84 1-88 1-96 1-92 2-73 2-72 2-64 2-70 0-82 Ap 005 0-12 0-17 0-12 0-12 0-12 0-19 005 0-14 0-24 0-31 0-23 0-14 0-93 0-93 396 7-79 408 01 13-43 1-79 corundum An% 49 48 58 43 43 33 31 39 41 54 36 44 40 mg-no. 60 50 58 58 58 60 55 57 50 55 48 61 43 a JOURNAL OF PETROLOGY VOLUME 37 NUMBER 4 AUGUST 1996 O)CDLD*?lDCOtpO)CDCO0 U5 "~ i - O Q CO n N 4 i - i D o i n m S 1 7 9 1 0 9 ( 0 1 0 9 ^ M ^^ 8 8 00i-mcocoio<-iDcnr-<D CMcn<pcMCM(OCM«« "S o c N t o g r j o i o r - i - Q O t o O Cl S 5 I D « C D CM CM r- t o c ^C cM j il n o ni r -- i o c N O DC CM CM 1 - r- p-r~CMCOQIDCMt~CD fflo^r-rtin^ort O *- IQ CO iS co * 4 - C M C M ^ i l c b l i ) C M O CM CM CM T- N 0 ) CO i - to e n c o r r •- S CN (D CnQ^COlDtDCniOIDtD p3r-(DCMlOC0<pCprc M ^ c o ID *- CM iD.-»- CM • - 1- «ID 3 c M m m m c M c o c n p f ^ c o c p r - P C M c n ^ < b c M c b < o c b o b i o ^ - p T - CM • - • - S O T - ( O 2a 8 SR S SS8SSSSS83J d 6 i 6 6 6 ^ 00 P^ CO CO 00 00 CO ip3r--5pr-55co •- 8 CM ^ f- cpcDr^^oapT-oo 5Br.(i3^9rt O N 6 l i ) d ) h . l D N 6 CM " NQOOtor-toco cnooomr* t O N O C J ^ C O C J O ID »— »— I r l o A o «— ID <- CO S r»<N CM CM ID i— csi *- CMCOQtpcopcMCO 4 - i D p S c o S c n c M b b b A COCOCMCOcbcMC) 8 r r o r r m » i D CN n- o> rID M co ^ - O Q I D C O C M ^ - P CM CM • - CM «S 8 r c n u j r ^ c o r ^ f r m m N N l O O l M N f N O l ID i c b c b r CM CM * • 1 - «^tiDcn pr-cpai CMr-Atb CO iA 1 n P T - ^ - p c n t p c o r - c o ^ o o cptpcpcp^-cpcnoocp (bcNichr^cbob^cr^-p <- CM * - • - ab ID CM ^ S ^ 822 CM «- in en PHILPOTTS it aL CRYSIAL-MUSH COMPACTION systematic variation in composition with height. Figure 9 shows profiles through the flow for several major and minor elements. The concentration of Ti, for example, steadily decreases with height until reaching a minimum at 47 m. It then steadily increases, and at 60 m passes the concentration it had at the base of the flow. It then reaches a maximum at 63 m and decreases to the initial concentration again by 130 m. Zirconium and ferric iron show similar profiles, but ferrous iron remains relatively constant throughout the flow. The MgO profile, on the other hand, is a mirror image of the Ti profile, with MgO being elevated where Ti is low, and vice versa. The analyses of the coarse-grained segregation sheets (Nos. 30-33) are somewhat variable, probably as a result of the inhomogeneity of this pegmatitic rock. These three analyses, consequently, have been averaged (Table 3) to obtain a more representative composition for this rock type. These segregation sheets are similar to the basalt but are slightly depleted in MgO and GaO and enriched in ferric iron, Ti, and Zr. The segregation sheets have a lower ferrous to ferric iron ratio than the basalt. The granophyre sheet (Analysis 34) has rather low alkalis and relatively calcic normative plagioclase (Aoto) compared with normal granites. It consequently resembles more the plagiogranites associated with ophiolites and mid-ocean ridge basalts (e.g. Dixon & Rutherford, 1979; Gerlach ct aL, 1981). The nor- mative corundum in this rock probably results from the cloudy alteration products in the feldspar. In contrast to the variable composition of the Holyoke Basalt at Tariffville, the flow at Southbury (Table 2) is remarkably constant throughout most of the section (Fig. 10). Only in the bottom few meters does the composition vary significantly, and here it is probably contaminated with the underlying sediments (Philpotts & Doyle, 1983). The Southbury analyses are almost identical to those of the basalt from the bottom of the flow at Tariffville, except that the Southbury samples contain ~0-5% less alumina. A small but significant increase in incompatible elements (Ti and Zr in Fig. 10) and decrease in MgO is evident with increasing height in the flow at Southbury. The profiles do not, however, have sigmoid shapes and therefore probably reflect primary variations in the composition of the erupted lava rather than post-emplacement differentiation. The compositional variation in the Tariffville section is clearly the result of crystal—liquid fractionation. Rocks in the lower zone, extending from 10 to 60 m above the base, are depleted in the incompatible elements that would be expected to enter the liquid (e.g. Ti, Zr) and enriched in the compatible elements (Mg, Cr). Between 60 and 130 m, however, the basalt is slightly enriched in incompatible elements and depleted in compatible ones. This zone contains the segregation sheets, which are significantly enriched in incompatible elements. The Flow Top 1801 O) 4000 6000 8000 60 80 100 120 4 Ti (ppm) Zr (ppm) 5 6 MgO(wt%) 7 9 10 11 1 2 FeO(wt%) 3 4 5 Fe2O3(wt%) Fig. 9. Chemical profiles through the flow at Tariffville. • , basalt; • , segregation sheeU. Dashed lines indicate the calculated initial magma composition. Cross-hatches indicate upper zone of irregular cooling fractures. 823 JOURNAL OF PETROLOGY VOLUME 37 NUMBER 4 AUGUST 1996 Table 3: Analyses ofminerals from sample 2 and the calculated bulk composition of the early crystallizing solids, and the average of the segregation sheets and the calculated initial magma composition (see text for explanation) 1 2 3 4 5 Plagiodasa Auglte Plgeonite Bulk Average Initial 55% 21% 24% solids segregation magma 53-38 6 SIO2 50-09 62-77 52-33 51-19 54-08 TiO2 0-00 0-20 0-13 007 1-43 0-97 30-97 1-17 0-55 17-41 13-18 14-60 AljOj Fe,O3 1-33 O-OO 000 0-72 2 93 2-13 FeO 000 9-36 20-96 6-99 11-62 9-76 MnO 0-00 0-35 0-63 0-22 0-24 0-20 MgO 0-00 1908 20-46 8-92 4-61 6-94 13-85 16-61 4-39 12-16 788 9-35 3-42 0-16 008 1-93 2-94 2-60 CaO NajO K20 0-36 002 002 0-21 0-94 0-73 P2O, 0-00 000 000 000 0-10 0-05 Total 100-00 99-71 99-56 99-83 99-84 99-71 Flow Top E 60 , ~ 4000 6000 800060 80 100 120 4 Ti (ppm) Zr (ppm) MgO(wt%) Fe2O3 (wt Fig. 10. Chemical profiles through the flow at Southbury. Cross-hatches indicate upper zone of irregular cooling fractures. question then is: what were the minerals involved in this fractionation and when did the fractionation occur? The effect of crystal fractionation on the composition of the liquid should be evident in a plot of Zr vs Ti (Fig. 11), because these elements are essentially incompatible and should therefore be enriched in the liquid while maintaining the same relative proportions during crystallization. Figure 11 shows that, indeed, all of the analyses, except for that of the granophyre (which is not plotted), cluster along a straight line having a Ti:Zr ratio of 66 (regression line, R = 0-95). The granophyre does not plot on this line because titaniferous magnetite had begun to crystallize (estimated to begin after 63% crystallization) by the time this late-stage liquid formed, and therefore Ti was no longer incompatible. However, the coarse-grained basaltic segregations do lie on this line, and therefore they can be interpreted as fractionated liquids that formed before crystallization of magnetite from an initial magma that probably had a composition similar to that of the basalt near the base of the flow (Table 1, No. 1), which is shown by a A in Fig. 11. The analyses of samples from the 10-60-m zone (x in Fig. 11) also lie on the same linear trend but at lower concentrations of Ti and Zr. Thus their compositions probably resulted from either the addition of early crystallizing minerals or the subtraction of a liquid fraction having a Ti:Zr ratio of 66. The samples of basalt from above the depleted zone (O in Fig. 11) are slightly enriched in Ti and Zr and therefore must be enriched in the liquid fraction. The linear trend in Fig. 11 is to be expected if Zr and Ti are incompatible. No zircon crystals are found in any of the rocks, and the amount of zir- 824 PHILPOTTS etd. CRYSTCAL-MUSH COMPACTION the segregation samples, and for AI2O3, total iron (FeO1), MgO, CaO, and K2O the regression lines agree well with the lines joining the two extreme 100 compositions. The variation in these elements is «£• 80 therefore satisfactorily explained by the model. Unlike the total iron trend, the FeO and Fe2O3 & 60 trends (not shown in Fig. 12) deviate slightly from Bulk Solids the line joining the extreme compositions; the segreM 40 gation liquid is too poor in FeO and too rich in 20 Fc2C>3. The most probable explanation for this discrepancy is that before crystallization of the coarse0 2000 4000 6000 grained segregation sheets, the residual magma was 8000 slightly oxidized, perhaps by water expelled from the Ti (ppm) underlying playa lake sediments (compare the Fig. 11. Plot of Zr v» Ti for Tariflville rocki. Symbols arc ai ferrous/ferric ratios in the segregation sheets and in followi: coarse-grained segregations (O); basalt from above 60 m the basalts). (O); basalt from below 60 m ( x ) , except for lowest sample (A); calculated initial magma ( + ); daihed regression line through The SiC>2 in the samples of basalt and coarsedata; and Rayleigh fractionation of initial magma is shown as grained segregations arc similar, which is consistent continuous line with numbers indicating the per cent crystallized (see text for explanation). with fractionation of plagioclase, augite, and pigeonite because these minerals all have approxiconium that entered the early crystallizing minerals mately the same concentrations of SiC>2 as the basalt. was so small that this clement can be considered Had early crystallizing olivine been involved, the totally incompatible. Small amounts of Ti, however, SiC>2 in the residual liquid would have increased. did enter the early crystallizing pyroxenes. The There is a slight, but significant increase in SiC>2 amount of Ti removed from the liquid by the early toward the base of the flow, with the lowest sample crystallizing minerals can be estimated from electron having the highest SiC>2 content of all the basalt microprobe and modal analyses of the minerals. For samples. This increased silica is largely responsible example, the modal weight percentages of these for the difference between the regression line and the minerals in the sample at 19-9 m above the base, line joining the bulk solids and the average of the where the first depletion in incompatible elements is coarse-grained segregations. The higher silica evident, is 55% plagioclasc, 21% augite, and 24% probably resulted from a small degree of conpigeonite (no olivine is present). Based on typical tamination by the underlying sediments, which are analyses of these minerals from this rock (Table 3), now composed largely of albite, quartz, and minor the bulk composition of the early crystallizing sphene. The slightly elevated TiO 2 of the lowest minerals would have had zero Zr and 444 p.p.m. Ti. sample may also be due to contamination. The Precisely the same composition is indicated by the lowest sample from the flow at Southbury also has a intercept on the Ti axis of the regression line slightly elevated TiO2 content (Table 2), and as (R = 0-95) through the data in Fig. 11. Thus, at least stated above, this rock was probably contaminated in terms of Ti and Zr, the compositional variation in by the underlying sediments (Philpotts & Doyle, all of the rocks, except the granophyre, can be 1983). attributed to fractional crystallization of plagioclase, The most puzzling variation is that of sodium. augite, and pigeonite from the initial magma. Whereas the basalt samples in general have Na2O If valid, this interpretation must account for the contents between those of the coarse-grained segrevariation in the other elements through the flow. In gations and the calculated bulk composition of the Fig. 12, the major-element abundances in the early crystallizing minerals, the Na2O values themsamples from the lowest 60 m (i.e. the lower chilled selves are negatively correlated with the Ti values. margin and the zone of depletion) have been plotted This is surprising because both elements would be against the Ti content of the rocks. The calculated expected to concentrate in the liquid, so that as the bulk composition of the early crystallizing minerals Ti content increased so would the Na2O content. and the average composition of the coarse-grained The negative correlation is evident only in the segregation sheets are also plotted and joined by samples between 20 and 60 m (Fig. 13a); samples dashed lines. Linear regression lines through the from above this show a random spread. Not only is analyzed rocks are shown as continuous lines. In all the negative correlation pronounced (the R value of cases, the basalt samples have compositions inter- the regression line in Fig. 12 is 0-91), but the change mediate between the early crystallizing minerals and is systematic with height. This is shown by the line 120 825 JOURNAL OF PETROLOGY VOLUME 37 2000 NUMBER 4 4000 Ti (ppm) 6000 AUGUST 1996 8000 Fig. 12. Plot of major oxides vs Ti in lamples from the lowest 60 m of the flow. Dashed lines join the compositions of the average of the coarse-grained segregations and the calculated bulk composition of the early crystallizing minerals (Table 3). Continuous lines are regression lines drawn through the analyzed rocks. T. JU 70 " 8 4.00- o o 3.50(M Zro 2.502.004500 o V 5500 ft O O ° o 60. x x I fe 50 • • E a. co v> 2 40 .. o o o 3.00 • T o ^ o o 30' 20 i6500 45 Ti (ppm) o o •+• -+• 50 55 60 % Total normative feldspar Fig. 13. (a) Variation in NajO vs Ti in basalt samples from Tariffville. The systematic change in the composition with height of samples from below 60 m ( x ) is shown by the arrowed line connecting successively higher samples starting with the lower chilled margin (A)The long arrow shows the trend that these rocks would have followed if compaction had involved simply expulsion of interstitial liquid. (b) The same samples are plotted in terms of their total normative feldspar content vs their normative anorthite content. joining the samples starting with the lower chilled margin (A in Fig. 13a). With increasing height, the Ti decreases and the Na2O increases until the sample at 47 m, after which the trend is reversed. This leaves little doubt that the Na2O content of these rocks is related to the process that caused the depletion in titanium. As argued above, this zone has the greatest concentration of early crystallizing minerals and would therefore be expected to have a greater concentration of more calcic plagioclase and a lower Ti content. Whereas the zone as a whole has 826 slightly higher anorthite contents than the basalt from above 60 m, the rocks that contain the largest amount of feldspar contain the least anorthite-rich plagioclase. Indeed, as shown in Fig. 13b, the higher the plagioclase content of the rock the lower is the anorthite content of its normative plagioclase. Also of interest is the magnitude of the change in the concentration of Na2O relative to that of Ti across this zone, the NajO changing by 33% and the Ti by only 20%. The cause of this large change in is uncertain. In the upper part of the flow, PHILPOTTS«a£ CRYSTAL-MUSH COMPACTION where the basalt is altered, high NajO can be attributed to albitization of the primary plagioclase, but in this lower zone the plagioclase is unaltered. The sodium could have been derived from the underlying playa-lake sediments by some process of vapor transport into the bottom of the still molten lava, but this would not explain the negative correlation with Ti. As the lava cooled and a solidification front moved upward from the base, exsolved volatiles also could have transported sodium upward, but why this should then have been concentrated in rocks with low Ti contents is not obvious. The simplest explanation is that the sodium content of the plagioclase was increased during recrystallization that accompanied compaction of the crystal mush. We will return to this problem after further discussion of the mechanism of fractionation in the flow. Except for the sodium data, the compositional variation in the basalt and the coarse-grained segregation sheets is satisfactorily accounted for by the fractional crystallization of plagioclase, augite, and pigeonite from a magma that initially would have had a composition similar to that of the basalt near the base of the flow. However, as argued above, the lowest analyzed sample (Table 1, No. 1) appears to be slightly contaminated with SiOj and Ti from the underlying sediment. However, because of the linear arrays produced by most of the elements in Fig. 11, the regression lines can be used to extrapolate through the samples from the lowest 60 m of the flow to the composition that the basalt probably had before contamination. This method of determining the composition of the initial magma has the added advantage of making use of multiple analyses of different rocks rather than basing the determination on one analysis of one rock. To make the calculation, a reasonable value for the initial Ti content of the magma must be selected. A value of 5800 p.p.m. was chosen from the basalt analyses from just above the zone of segregation sheets. This value is only slightly lower than that of the possibly contaminated sample from the bottom of the flow, and it allows a reasonable mass balance calculation to be made of the various rocks in the flow (see below). Because of the disparate sodium trend, the initial NajO was calculated from the linear extrapolation between the average of the segregations and the early crystallizing bulk solids. Analysis 6 in Table 3 gives the results of this calculation. Using this calculated original magma composition and the analyses of the early crystallizing minerals (Table 3), we can calculate the composition of successive liquids, produced by any given fractionation scheme (Rayleigh or equilibrium, in the extreme cases). If this is done for Zr and Ti, the specific 827 fractionation scheme makes little difference to the results, because both of these elements are essentially incompatible. Figure 11 shows the composition of liquids formed by fractionation of the assumed initial magma. The calculated trend is seen to pass through the plotted positions of the basaltic segregation sheets after ~ 3 3 % crystallization of the initial magma. This value is similar to the degree of crystallization that has been estimated for segregation sheets in other basalt flows—26% in the Lolo flow of the Columbia River Group and 28% in the Watchung flows of New Jersey (Puffer & Horter, 1993), and, based on TiO 2 analyses, 26-33% in the Keweenawan basalts of Michigan (Cornwall, 1951). Thus, ignoring for the moment the question of how the fractionated liquids were able to segregate, their composition corresponds to that of a residual liquid that would form after no more than one-third crystallization of the basalt. Similarly, based on the enrichment in zirconium, the granophyric sheets in the Holyoke Basalt would have formed after 75% fractional crystallization of the original magma. The elements that are concentrated in the coarsegrained segregation sheets almost certainly came from the zone between 20 and 60 m above the base of the flow where the incompatible elements are most strongly depleted. They were not, for example, derived from the basalt surrounding the segregation sheets, for this rock is actually slighdy enriched in these components. The zone of depletion has two possible origins. Early crystallizing minerals could have accumulated there by settling through the magma. The fractionated liquid remaining above then would have formed the segregation sheets. On the other hand, the depletion could have resulted by compaction of the partly crystallized basalt, with the expelled liquid rising to form the segregation sheets. Plagioclase is the only mineral that forms phenocrysts throughout the flow, and their abundance remains relatively constant ( < 5 % ) , even at 47 m, where the basalt has the lowest concentration of incompatible elements. Furthermore, plagioclase is most unlikely to have settled, because its density would have been almost identical to that of the magma (p m = 2-64 Mg/m 3 ). The chemical variation through the lower zone would have required accumulation, not only of plagioclase, but also of pyroxenes. However, pyroxenes never form phenocrysts in this basalt, nor is there any macroscopic field evidence for their accumulation, such as mineral layering. The steadily decreasing Ti content through this zone also is difficult to explain by crystal settling, because it would have required the rate of accumulation of early crystallizing minerals to have steadily increased while the relative proportions of JOURNAL OF PETROLOGY VOLUME 37 these minerals remained the same. The only simple way of concentrating all of the early crystallizing minerals (primocrysts) in a fixed proportion is through compaction of the partly crystallized basalt. The flow could have maintained a homogeneous composition until it was one-third crystallized, and then compaction of the crystal mush, which would have contained plagioclase, augite, and pigeonite by this stage of crystallization, would have expelled the residual liquid to higher levels in the pile, where some of it would have formed the segregation sheets. The steady variation through the 10—60-m zone would then simply reflect different degrees of compaction. Two important conclusions can therefore be drawn from the analyses. First, the coarse-grained segregations have compositions that are consistent with their having been derived from the original basalt following ~ 33 wt % crystallization of the three-phase assemblage plagioclase + augite + pigeonite in the proportions that these minerals coprecipitated from the basaltic magma. Second, the chemical variation through the flow indicates that this segregation liquid, which forms the sheets between 70 and 85 m above the base of the flow, was derived from the zone between 10 and 60 m, probably as a result of compaction of the crystal mush. PREVIOUS MODELS FOR THE GENERATION OF SEGREGATION SHEETS Several mechanisms have been proposed for the formation of the coarse-grained basaltic- and the finegrained granophyric-segregation sheets in flood basalts, but none satisfactorily explains all of the features seen in the Tariflville occurrence. Puffer & Horter (1993) concluded that the basaltic segregation liquid is generated on the lower solidification front of the flow, from where it rises, buoyed up by bubbles, to accumulate beneath the downwardgTOwing upper crust. Helz (1980) suggested a similar origin for the segregation sheets in the Kilauea Iki lava lake. Segregation liquids formed in this way would have to rise through the less fractionated central part of the flow without mixing with it. This mechanism also does not account for the clear intrusive and branching nature of many of the sheets, not only in the Holyoke Basalt, but in the Columbia River basalts (Lindsley et al., 1971), in the Kcweenawan basalts (Cornwall, 1951), and in the Hawaiian lava lakes (Moore & Evans, 1967). Cornwall (1951) believed the segregation sheets in the Keweenawan basalts formed from cool, dense, NUMBER 4 AUGUST 1996 volatile-rich crystal mush that periodically fell from the roof and accumulated on the floor of the flow, where it was covered and trapped beneath accumulations of plagioclase, olivine, and pyroxene which settled as individual crystals to form the host basalt between the sheets. Such an origin would not account for the compositional variation seen in the Holyoke Basalt. Wright & Okamura (1977) suggested that residual liquids in the Makaopuhi lava lake, Hawaii, were injected into horizontal fractures that formed when the upper crust became supported by the walls of the lava lake and thus was not free to subside with the cooling and shrinking lens of liquid in the lake. Although this is feasible in a lava lake, it is not likely to have happened in the Holyoke flow, where the 'shoreline' of the lava lake (or sea) may have been many tens of kilometers away from the Tariffville locality. PROPOSED MODEL FOR THE GENERATION OF SEGREGATION SHEETS A successful model for the origin of the coarsegrained segregation sheets must account for the following features: (1) Segregation sheets form only in thickflowsor lava lakes. The minimum thickness probably depends on the type of lava but is of the order of 70 m. (2) The sheets, which are commonly regularly spaced (~1 m), form in a central zone of the flow, where they constitute from 10 to 26% of that zone. (3) Their grain size is at least an order of magnitude greater than that of the host basalt and in places is pegmatitic. They commonly contain amygdales or are dictytaxitic. Many of their long bladed crystals of plagioclase and pyroxene are bent. (4) Contacts with the basalt are normally sharp but some are gradational, as in the case of the bottom contact on the lowest sheet at Tarifrville. (5) The sheets are essentially horizontal, but they can bifurcate or have small dikes connecting them with sheets above or below them, which clearly demonstrates their intrusive nature. (6) The host basalt was capable of being fractured, but the rounding of contacts suggests that it was also plastic at the time the sheets were intruded. (7) The composition of the segregations corresponds to liquids that can form by as little as 25% crystallization of the initial basalt. (8) This fractionated liquid is extracted from the basalt in the lower part of the flow beneath the zone of segregation sheets. 828 PHILPOTTS et aL CRYSTAL-MUSH COMPACTION (9) Whereas thin granophyric segregation sheets, which form after > 75% crystallization of the initial basalt, can also be present, segregation sheets with compositions intermediate between the granophyres and the coarse-grained basalt do not occur. (10) Granophyre segregation sheets occur either in the coarse-grained segregation sheets or in the basalt immediately overlying such sheets. The restriction of segregation sheets to thick, slowly cooled flows and lava lakes is probably attributable to kinetic factors and process that are restricted to thick piles of crystal mush. The Holyoke Basalt, and other similarly thick flows, would have taken many tens of years to solidify. Consequently, volatiles that were exsolved during eruption or were derived from underlying sediments had adequate time to rise and accumulate in the early formed upper crust. The lower and central parts of the flow consequently are completely devoid of vesicles. The early convection of magma brought about by these rising bubbles eventually would have been replaced by thermal convection once the magma had purged itself of bubbles (Worster et al., 1993). The result of this convection was to keep the magma thoroughly mixed and, as it cooled, crystal nuclei would have been distributed throughout the main part of the flow. This accounts for the fine grain size of the basalt throughout the flow. Convection eventually would have stopped when the crystallizing magma developed a yield strength that could oppose the convective forces. This must have occurred before the Holyoke Basalt was intruded by the segregation sheets, whose composition indicates that the initial basalt had undergone 33 w t % (31 vol. %) crystallization by that time (Fig. 11). In other flows this fraction can be as low as 25 vol. %. Laboratory measurements on a Kilauea Iki picrite show a marked non-Newtonian behavior when the crystal fraction goes above 25%, and the yield strength increases rapidly with increasing crystal content (Ryerson et al., 1988). Convection therefore probably stopped in the Holyoke Basalt by the time it was one-quarter crystallized. Once convection had stopped, the lower and central parts of the flow would have consisted of a delicate crystal mush that was at least two-thirds liquid. The more abundant plagioclase, with its lathshaped crystals, probably played a dominant role in forming this network. As cooling and crystallization continued, the network would have developed more strength, and by the time the segregation sheets formed, the mush was capable of being fractured, albeit in a plastic manner. Before this, however, there was a redistribution of the melt within the mush, as indicated by variation in the abundance of incompatible elements, with melt migrating upward from the zone between 10 and 60 m above the base of the flow into the zone between 60 and 130 m. The mush must therefore have undergone compaction below and dilation above. The bulk density of the primocrysts is calculated to have been 3 0 Mg/m 3 , whereas the magmatic liquid changed its density from an initial value of 266 Mg/m at 1160°C to 2-68 Mg/m 3 at 1100°C when the liquid had the composition of the segregation sheets [calculated from data of Lange & Carmichael (1987) and Warren (1995)]. Thus the residual liquid would have been buoyant relative to the crystal mush during this entire period of crystallization. The degree of compaction or dilation of the crystal mush can be estimated from the concentration of the incompatible elements. The rock analyses can be -'interpreted in terms of two components, a liquid fraction and a bulk solids fraction that would have existed at the time of compaction. Given that the liquid that formed the segregation sheets was expelled from the crystal mush, its composition should have been the same as that of the liquid that remained in the mush (Table 3, No. 5), and the bulk composition of the solids is known from the electron microprobe and modal analyses of the early crystallizing minerals (Table 3, No. 4). The concentration of Ti in the liquid fraction would have been 8533 p.p.m. and in the solids, 444 p.p.m. If the concentration of Ti in a rock is Ti r , the weight percentage of solids at the time of compaction would have been 100 x (8533- Ti r )/(8533- 444). For example, the calculated initial magma composition, with 5800 p.p.m. Ti, would have consisted of 34 wt % solids at this time. This can be taken to be the fraction of solids in the uncompacted mush. Where the concentration of Ti reaches its lowest value at 47 m and the degree of compaction was presumably greatest, the percentage of solids would have been 47 wt %, and at 68 m, where Ti reaches its highest concentration and the mush would have been most dilated, the percentage of solids decreased to only 27 wt%. From these numbers we can calculate the percentage of compaction, or dilation, as a function of height in the flow (Fig. 14). Interpreted in this light, the analyses point to a zone between 10 and 60 m where the degree of compaction steadily increased to a maximum of 28% at a height of 47 m and then steadily decreased to zero. Just above 60 m the mush was dilated by ~ 2 0 % , but this decreased to zero at 90 m. Between 90 and 130 m, the mush must also have been slightly dilated. Analyses of the altered basalt above 130 m 829 JOURNAL OF PETROLOGY -30 -20 -10 0 10 20 VOLUME 37 30 Percent compaction Fig. 14. Per cent compaction (positive valua) or dilation (negative values) in the crystal mush as a function of height in the flow, based on the Ti content of the rocks (lee text for explanation). indicate essentially constant Ti values, which implies there was no dilation or compaction above 130 m. The smooth variation in degree of compaction in the lower 60 m contrasts dramatically with the erratic variation in the degree of dilation between 60 and 130 m. The smooth variation in the lower part is consistent with the proposed model in that the degree of compaction would be expected to increase steadily downward until prevented from doing so by the rising solidification front. The erratic variation between 60 and 130 m is probably related to the intrusion of the segregation sheets between 70 and 85 m, which probably produced local variations in the amount of dilation. The variation shown in Fig. 14 is interpreted to indicate that the crystal mush that existed beneath the solid crust of the Holyoke flow became compacted in its lower part while becoming dilated in its upper part, with the maximum dilation occurring between 63 and 75 m above the base of the flow. This was probably where the mush was hottest and weakest. The lowest and thickest of the segregation sheets occurs at 70 m. If this sheet originally was composed entirely of liquid, the continuity of the crystal network across this level must have been broken at this time. Therefore, it is concluded that, as gravitational forces redistributed the melt through the mush, the increased pore pressure in the zone of dilation finally exceeded the tensile strength of the mush and caused it to fail. Once ruptured, the mush below the fracture would have been free to continue compacting, with the expelled liquid rising through the pores to accumulate in the sheet at 70 m. The amount of liquid that accumulated at this level therefore would have been dependent on the amount of compaction that went on after the rupture. NUMBER 4 AUGUST 1996 Because the liquid accumulating at this level was expelled from the underlying compacting crystal mush by porous flow, it was relatively free of crystal nuclei, and therefore it formed a coarse-grained rock on crystallizing. Once residual liquid began to accumulate in segregation sheets, the dense mush forming the roof to this sheet would have become unstable and spalled off into the underlying liquid. The density contrast between the solids and the liquid (~320 kg/m3) would have resulted in a stress gradient in the roof of slighdy more than 3000 Pa/m. The minimum thickness of the spalled sheet would have been determined by the tensile strength of the crystal mush. Because most of the sheets are spaced ~ 1 m apart, this tensile strength must have been ~3000 Pa, that is, the sheet had to be at least 1 m thick to generate stresses great enough to exceed the tensile strength of the roof. As melt migrated up and around the spalled roof slab, a second segregation sheet would have formed. As this thickened, its roof would have become unstable, and further spalling would have occurred. In this way, multiple segregation sheets were formed. During the upward passage of the liquid through the sheets, fractionation could have occurred if the liquid had been crystallizing at the time. This does not appear to have been die case in the Holyoke Basalt, but it could explain die vertical variation in the segregation sheets in the Keweenawan basalts described by Cornwall (1951). The concentration of vesicular segregation material toward the distal ends of sheets in the Holyoke Basalt probably indicates that a more volatile-rich fraction was able to migrate into the fractures before die main body of segregation liquid entered. Because the segregation sheets do not have chilled margins, the temperatures throughout the part of the flow involved in the compaction and the intrusion of segregation sheets could not have varied greatly. Moreover, following the transfer of liquid from the crystal mush to the segregation sheets, this variation would have been still less. The interstitial liquid in the zone of compaction, being closer to the bottom of the flow, may have been slightly cooler than die central part of dieflow.This liquid, on rising to form the first segregation sheet at 70 m, therefore may have cooled the central part of the flow slighdy. As the segregation liquid rose to form die higher segregation sheets it would have transferred heat to higher levels in the flow. This probably explains why the boundary between the colonnade and entablature in thick flows containing segregation sheets is higher dian in flows that do not contain segregation sheets. The result of die redistribution of the segre- 830 PHILPOTTS et d. CRYSTIAL-MUSH COMPACTION gation liquid was to produce a region where the temperature was very nearly constant at ~1100°C and the basalt would have been ~ 3 5 % crystallized. If compaction continued during crystallization, the composition of the expelled liquid should have changed progressively with time. The basaltic segregation sheets in the Holyoke, however, do not have compositions indicating segregation after more than 35% crystallization. Basaltic segregation sheets in other flood basalts show similar limits to the degree of fractionation, despite considerable variation in the thickness of the flows, and hence in their cooling times (Puffer & Horter, 1993). In Hawaiian lava lakes, the limit may be closer to 50% (Helz, 1980). Compaction, therefore, appears to occur only during a small fraction of the total crystallization period of a flow, and appears to be mainly independent of the total crystallization time. A number of factors would contribute to stopping compaction. As crystals become more tightly packed, the amount of strain that can result from rotation of plagioclase laths decreases, and the strain rate would approach the diffusion rate. With the increase in percentage of solids, the mush also becomes stronger. And finally, as crystallization continues, the residual liquid becomes more iron rich and denser, which would decrease the driving force for compaction. These factors are believed to have combined to terminate compaction in the Holyoke Basalt. At the time compaction ended, the segregation sheets were still essentially liquid and at a temperature of 1100°C. With cooling, however, plagioclase and pyroxene would have crystallized from this liquid. No compaction of crystals appears to have occurred within the sheets, probably because the thickness of mush was not great enough and the density of the residual liquid was still increasing. However, it was probably during this stage of crystallization of the segregation sheets that the long plagioclase and pyroxene crystals were bent, when roof slabs of the basalt fell into the partly crystallized segregation liquid. At 1055°C, when magnetite began to crystallize (Fig. 8), the segregation sheets would have been ~ 3 7 % crystallized, but the surrounding basalt was already 63% crystallized. When the temperature reached 1020°C, the residual liquid entered the two-liquid field (Fig. 8) and split into iron-rich and silica-rich liquids. With the appearance of the silica-rich fraction, a residual liquid was formed for the first time in the flow that was significantly less dense (2*4 Mg/m 3 ) than all the other phases present. These residual liquids would have constituted 33% of the segregation sheets at this temperature, and where the interstitial patches of liquids were connected, buoyancy was able to 831 cause the silica-rich liquid to rise as blobs toward the top of the sheets. In addition, by this late stage of crystallization, volatiles were again being exsolved from the residual liquids. Gas bubbles in the silicarich liquid would have increased the buoyancy of this fraction still more. Toward the top of some sheets, the silica-rich liquid was able to segregate and form continuous thin sheets of liquid that eventually crystallized to form granophyre. The iron-rich liquid, with a density of 3-24 Mg/m 3 (Philpotts & Doyle, 1983) would have remained with the denser minerals and eventually crystallized as pyroxene, magnetite, and apatite. The sequence of events envisaged for the crystallization of a thick flood basalt, or lava lake, are shown schematically in Fig. 15, where time is represented on the horizontal axis in terms of the degree of crystallization in the center of the flow. Following an early period of degassing, the magma enters a period of thermal convection, during which crystal nuclei become distributed throughout the flow, thus ensuring, eventually, a fine grain size to the basalt. Convection ceases following 25% crystallization, and by 33% crystallization the crystal mush develops an interconnected network which undergoes compaction in its lower part and dilation in its upper part. A horizontal rupture in the dilated mush fills with liquid expelled from the compacting mush below and, because it is free of nuclei, the rock eventually formed from it is coarse grained. Overlying sheets arc formed as slabs spall from the roof of the first sheet. Finally, when the basalt is > 7 1 % crystallized, the residual liquid splits into immiscible fractions, with the low-density silica-rich liquid rising toward the tops of the earlier segregation sheets to form thin granophyre sheets. DISCUSSION AND CONCLUSIONS Perhaps the most controversial aspect of the proposed model is that a tholeiitic basalt, when only one-third crystallized, can form a crystal mush that is capable of being fractured and from which the interstitial liquid can be removed. Is it reasonable to expect a basaltic crystal mush to behave in this way with such a low fraction of solids? Direct evidence of the degree of crystallization needed to produce a rigid framework comes from measurements in drill holes in Hawaiian lava lakes. At the base of the crust, where a drill can be pushed by hand into the underlying liquid, the degree of crystallization was found to be 65% at Kilauea Iki (Helz, 1980) and 55% at Makaopuhi (Wright & Okamura, 1977). These are much higher degrees of crystallization JOURNAL OF PETROLOGY VOLUME 37 NUMBER 4 AUGUST 1996 yyyyyxxxxx "^V'XA .2 .3 xxx .4 .5 .6 .7 .8 .9 1.0 Fraction Crystallized in Central Part Fig. 15. Schematic representation of events in the solidification of the Holyoke Basalt. Time is represented by the fraction of melt crystallized in the central part of the flow (see text for discussion). than are proposed in the model, but the stresses and entiation could begin. The fact that this occurred strain rates produced by a drill are large compared when the magma was only one-third crystallized is with those resulting from compaction. However, important for two reasons. First, the high porosity Bruce Marsh (personal communication, 1995) would have provided abundant channels through reports that 3-D networks form in the Makaopuhi which the liquid could be expelled from the mush. lava lake at crystallinities as low as 10%. Based on Second, only small amounts of recrystallization geochemical arguments, Irvine (1980) concluded would have been necessary to bring about large that the olivine cumulates in the Muskox Intrusion amounts of compaction. initially contained only 42% crystals. Campbell ttal. The rate of compaction is difficult to quantify. (1978) produced olivine cumulates from basaltic The fluxes of the descending solids and rising liquids melt in high-temperature centrifuge experiments must have been equal, and because there was that contained as low as 40% crystals. However, the approximately twice as much liquid as solid, the crystal mush in the Holyoke Basalt would have dif- solids would have had to move twice as fast as the fered from these cumulates in that it was dominated liquid. The rate of compaction must, therefore, have by thin laths of plagioclase, and even the pyroxene been controlled by the rate of deformation of the grains are elongate. It is well known that elongate solids and not by the rate of porous flow of the particles can form highly porous aggregates, as is liquid. The rate law describing such deformation is evident from examining the contents of a box of corn uncertain (Ashby & Verrall, 1977). Fluid-phase flakes. Crystals with an aspect ratio of 10:1, for transfer was probably an important factor, because example, can form an interlocking network with the minerals were in contact with liquid from which only 20% solids (Burgers, 1938). We conclude, they had just crystallized, but power-law creep may therefore, that clusters of plagioclase laths and pyr- also have been involved as the mush became more oxene grains were primarily responsible for pro- compacted and began to solidify. The relation ducing the highly porous framework. between the diffusion rate of components through Before the formation of the framework, differ- the melt and the strain rates in the crystal pile is entiation of the magma could have been effected complicated and would have changed with time as only by settling of individual mineral grains, but the geometry of the solids changed (e.g. were the there is no evidence that this occurred in the plagioclase laths able to rotate?). The solids Holyoke Basalt. Once the interconnected crystal probably behaved as a non-Newtonian viscous liquid mush was formed, however, compaction and differ- with a significant yield strength. This yield strength 832 PHILPOTTS tt aL CRYSTAL-MUSH COMPACTION may be what prevents compaction from occurring in thinner flows. Because the crystal mush contained > 50% plagioclase, compaction of the crystal mush probably involved recrystallization or dissolution and redeposition of the plagioclase. Where this occurred, the plagioclase would have re-equilibrated with the residual liquid and become more sodic. This may provide an explanation for the unexpected negative correlation between the NajO and Ti contents of the rocks in the zone of compaction. The long arrow in Fig. 13a shows the trend that these rocks would have followed if compaction had simply involved expulsion of the interstitial liquid, that is, the Na2O and Ti would both have decreased. At the lowest Ti values, however, the Na2O content is 1-5% higher than predicted by this trend. The alumina content of these Ti-poor rocks is elevated (Fig. 12), as would be expected from the compaction of anorthitic plagioclase, but up to 30% of this alumina must have been transferred from the anorthite to the albite component of the plagioclase during the recrystallization that accompanied compaction. The fact that sodium is the only element that shows this unusual trend suggests that plagioclase recrystallization controlled the compaction of the crystal mush, which is not surprising, given its abundance. According to the model, the total thickness of the segregation veins depends on the amount of compaction that occurred after the dilated part of the crystal mush ruptured. In addition, all of the liquid that was displaced from the compacted zone should have entered the dilated crystal mush or the segregation sheets themselves. Using the chemical profiles through the flow as indicators of the distribution of this liquid in the compacted and dilated parts of the crystal mush, we can calculate the amount of segregation material needed to effect a mass balance. As described above, the deviation of a rock's Ti content from that of the assumed initial magma (5800 p.p.m.) is a measure of its liquid content at the time of compaction. Based on a graphical integration of the Ti profile, a total of 4-4 m of segregation sheets, having an average Ti content of 8533 p.p.m., should be present in the flow. This is slightly more than the 3-9 m that was actually recorded in the field, but this measurement is only of the stratigraphic thickness of the sheets and does not take account of any of the segregation material that is in dikes connecting the sheets. The calculated and observed amounts are therefore in reasonable agreement. We are unaware of compaction having been proposed as a mechanism of differentiation in thick lava flows, although upward migration of volatile ele- ments and filter pressing in general have been invoked [see, e.g. Hart et al. (1971) and Helz (1980)]. Compaction of cumulates on the floor of plutonic bodies, however, has been carefully documented (Irvine, 1980; Shirley, 1987) and the mechanics of the process have been investigated by McKenzie (1984), Richter & McKenzie (1984), and Shirley (1986). Some workers question whether piles of cumulates are ever thick enough to generate the pressure necessary to cause compaction (Morse, 1986). Sparks et al. (1985), in evaluating the role of compaction as a postcumulus process in layered mafic intrusions, calculated typical compaction rates for olivine cumulates. Their calculated time and length scales, however, are considerably greater than those of the Holyoke Basalt. Even in a 1-km-thick sill, their calculated freezing rate is faster than that of compaction, so negligible compaction would occur. If the Holyoke mush did undergo compaction, and we believe the evidence strongly suggests that it did, the high porosity and low viscosity of this mush must have greatly reduced the time and length scales, because compaction would have occurred in only tens of years in < 100 m of mush. If this is possible in a thick lava flow, compaction must be a viable mechanism in plutonic bodies, at least where the cumulates are dominated by the same minerals as in the Holyoke Basalt (i.e. plagioclase and pyroxene). Recent geophysical data suggest that magma chambers beneath ocean ridges consist mainly of crystal mush, with lenses of liquid forming only in the upper parts of those beneath fast spreading axes (Sinton & Detrick, 1992; Barth et al., 1994). These lenses of liquid may form in exactly the same way as those in the Holyoke Basalt. Compaction has also been invoked as a segregation mechanism for basaltic magmas in their source regions in the upper mantle (Walker et al., 1978; Stolper et al., 1981; McKenzie, 1984, 1985). Whereas this involves the migration of small fractions of melt through a largely crystalline peridotite, the physical arrangement of segregation sheets relative to the zone of compaction in the Holyoke Basalt may provide a model for the structure in such source regions. In the Holyoke Basalt, the transition from compacting crystal mush to segregation liquid is sharp, and only on the lower side of the lowest sheet (i.e. the top of the compacting crystal mush) is the boundary gradational over a few decimeters. The transition from a mush to a crystal-free liquid is therefore rapid. If crystals from the mush had been carried along in the segregation liquid, the liquid would not have crystallized to such a coarse-grained rock. By analogy, primary basaltic magma in its source region could be relatively free of restite 833 JOURNAL OF PETROLOGY VOLUME 37 AUGUST 1996 ruptures the crystal mush in the zone of dilation to form a horizontal sheet of liquid. (5) As the underlying crystal mush continues to compact, the sheet of liquid thickens. Because the liquid enters the sheet by porous flow, it is essentially free of crystal nuclei, and consequently crystallizes eventually to a coarse-grained basaltic segregation sheet. (6) Because the dilated basalt above the sheet of liquid is denser than the liquid, the roof becomes unstable, and thin slabs sink into the liquid. In this way, multiple thin sills of segregation liquid are produced at ~l-m spacings above the initial segregation sheet. (7) Compaction is arrested by the increasing strength of the crystal mush and the increasing density of the residual liquid. In quartz tholeiites the compaction process is terminated by the time the basalt becomes ~35% crystallized. (8) A second generation of segregation sheets is formed near the top of the earlier sheets when the original basalt is >71% crystallized. These are granophyric in composition, and are probably formed from a late-stage, silica-rich immiscible liquid which, because of its low density, collects near the top of the earlier segregation sheets. crystals and thus have a narrow compositional range, which would depend only on the degree of partial melting. The focus of such segregation depends on where the buildup of melt and pore pressure becomes great enough to break the continuity of the framework of the partly molten crystal mush (Stolper et al., 1981). Once a rupture forms, it is likely to propagate in the plane normal to the minimum stress direction and form a laterally extensive horizontal sheet, as it did in the Holyoke Basalt. By analogy, it is also likely that a series of interconnected sheets would form above the primary segregation sheet, but here magma movement would be by channeled flow rather than by porous flow. Just as the rigid crust on the Holyoke Basalt arrested the upward movement of the segregation liquid, so does the lithosphere provide a cap for the melts from the upper mantle. However, if the lithosphere is fractured, the sheets of primary magma at its base would provide a laterally extensive source of homogeneous magma that could rise in regional dikes to form flood basalts. On the other hand, diapiric structures could also develop from these sheets to give rise to central complexes. Even in the Holyoke Basalt such diapirs may have formed in places on the segregation sheets, for at Totocket Mountain at the southeastern end of the Hartford Basin, the segregation material, rather than forming thin sheets, has thickened into lenses that are many tens of meters thick. ACKNOWLEDGEMENTS We are grateful to Jim Garabedian and Dan Zeidler for their assistance with the surveying and sampling of the flow under very chilly winter conditions. We are also grateful to Richard Tollo and Bruce Marsh for their thoughtful reviews of the manuscript. The following are the main conclusions that can be drawn from this study: (1) Quartz tholeiitic magmas with compositions similar to that of the Holyoke Basalt, when only onethird crystallized, can form an interconnected network of crystals that has a finite strength (it can be fractured and intruded by segregation liquid). We caution against assuming that all basalts would behave similarly at this degree of crystallization. Hawaiian olivine tholeiites, for example, appear to develop a strength at ~50% crystallization. (2) The strength of the mush is not great enough to prevent compaction from taking place in flows that are sufficiently thick. 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