‘LA.UR -83-2229 LA-UR--83-2229 DE93 015217 TITLE:GEOCHEMICAL SIMILARITIES BETWEEN VOLCANIC UN!TS AT YUCCA MOUNTAIN AND PAHUTE MESA: EVIDENCE FOR A COMMON MAGMATIC ORIGIN FOR VOLCANIC SEQUENCES THAT FLANK THE TIMBER MOUNTAIN CALDERA WTHOIW: R. G. Warren, ES. . SUBMITTEDTO: 2nd Containment Symposium 2-4 August 1983 Kirtland AFB Albuquerque, NM DISCLAIMER This report WMS prcpnrcd us ●r uccount of work qmrwwrod by an ngency of drc Unital S{ma (krvcrhmen!. Ncilhor Ihc iJnllcd SInlU Govcrnmont nor wry ● gency thereof, nor wry of their cmploycm, mukos WY wnrrwrly, cxprem or implied, or nmumob nny Iegd Iinhillty or rOSlXVVMl- billiy for the mxxrncy, complctonec:, or um[ulncm of wry informslhn, ~pparmrm, produoI, or proccu dinclrwcd, or reprcaents thnt ho UM would rml Infringe privnmly ownod rishtm. Refer. encctracin mmy npocific~~rciml PWIUCL p~,~r -i=hy trndc n-lr~em~rkl mmwfrncturcr, or olherwitc drva nul nwcamrily wn-tihrtc or imply itn cndorwnoni, rcamr- n!cnduliwn, III I’mwring lIy i he 1 Jnikd SLulca (hwcrruwcm or wry qcncy lhcrcof, The wiowm wvd opinionn uf mulhm~ CP prcwxl herein rlu rrwl ncwwrily stulr or rclkl thooo of Ik (Jnitcrl SIUICK I hwcrrrmcnl or mry u~cncy Ihcrcof. BY w.captmwa of lFdI nrldo, 11’m publmh.r I-ognlzas Ihal UVa U.S. aovornmalt rolwrt a rvorvwcluwo, roydly.lrca hcwwo 10 pubhgn or rooroduca Ilw publmhad term of Ihlm corvw!bulion, or 10 allow olhwm w do SO, Iwr U S, Oovarnmonl Durposcm, Th. LOI AlarnO~ Nwond Lsboralory foquosls 11’w ma publlohcr ldsnll~ lhlg mtlclo ●s work pqrfofmgd unda 150 waDIcag 01 Uva U s D~parlmanl Of enwQ~ W’wui m!TR1l’llTlflli ofUll\ Ofl(,llMl HIl,, LOSAllaIIIITIOS l...l,...,.ew.~~~..~~~.~ LosAlamos National Laboratory wlull[fl
32
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‘LA.UR -83-2229
LA-UR--83-2229
DE93 015217
TITLE:GEOCHEMICAL SIMILARITIES BETWEEN VOLCANIC UN!TS AT YUCCAMOUNTAIN AND PAHUTE MESA: EVIDENCE FOR A COMMON MAGMATICORIGIN FOR VOLCANIC SEQUENCES THAT FLANK THE TIMBER MOUNTAINCALDERA
WTHOIW: R. G. Warren, ES..
SUBMITTEDTO: 2nd Containment Symposium2-4 August 1983Kirtland AFBAlbuquerque, NM
DISCLAIMER
This report WMS prcpnrcd us ●r uccount of work qmrwwrod by an ngency of drc Unital S{ma(krvcrhmen!. Ncilhor Ihc iJnllcd SInlU Govcrnmont nor wry ●gency thereof, nor wry of theircmploycm, mukos WY wnrrwrly, cxprem or implied, or nmumob nny Iegd Iinhillty or rOSlXVVMl-billiy for the mxxrncy, complctonec:, or um[ulncm of wry informslhn, ~pparmrm, produoI, orproccu dinclrwcd, or reprcaents thnt ho UM would rml Infringe privnmly ownod rishtm. Refer.encctracin mmy npocific~~rciml PWIUCL p~,~r -i=hy trndc n-lr~em~rklmmwfrncturcr, or olherwitc drva nul nwcamrily wn-tihrtc or imply itn cndorwnoni, rcamr-
n!cnduliwn, III I’mwring lIy i he 1 Jnikd SLulca (hwcrruwcm or wry qcncy lhcrcof, The wiowmwvd opinionn uf mulhm~ CP prcwxl herein rlu rrwl ncwwrily stulr or rclkl thooo of Ik
(Jnitcrl SIUICK I hwcrrrmcnl or mry u~cncy Ihcrcof.
BY w.captmwa of lFdI nrldo, 11’m publmh.r I-ognlzas Ihal UVa U.S. aovornmalt rolwrt a rvorvwcluwo, roydly.lrca hcwwo 10 pubhgn or rooroduca
Ilw publmhad term of Ihlmcorvw!bulion, or 10 allow olhwm w do SO, Iwr U S, Oovarnmonl Durposcm,
Th. LOI AlarnO~ Nwond Lsboralory foquosls 11’w ma publlohcr ldsnll~ lhlg mtlclo ●s work pqrfofmgd unda 150 waDIcag 01 Uva U s D~parlmanl Of enwQ~
This official electronic version was created by scanning the best available paper or microfiche copy of the original report at a 300 dpi resolution. Original color illustrations appear as black and white images. For additional information or comments, contact: Library Without Walls Project Los Alamos National Laboratory Research Library Los Alamos, NM 87544 Phone: (505)667-4448 E-mail: [email protected]
GEOCHEMICAL SIMILARITIES BETWEEN VOLCAdIC UNITS
AT YUCCA MOUNTAIN AND PAHUTE MESA:
EVIDENCE FOR A Cf)M?4014MAGMATICORIGINFOR VOLCANIC SEQUENCES
THAT FLANK THE TIMBER MOUNTAIN CALDERA
R. G. Warren
Los Alamos National LaboratoryLos Alamos, NM 87545
ABSTRACT
Chemical compositions have been determined for sanidlne, plagioclase,
hiotite, and hornblende phenocrysts by electron microprobe for a comprehensive
set of samples of Crater Flat Tuff and tuffs of Calico Hills. Most of these
samples were obtained from drill holes at Yucca Mountain. Samples of tuffs
and lavas of Area 20, obtained from locations at Pahute Mesa, have similarly
been subjected to microprobe analysis. Complete modal petrography has been
determined for all samples.
Biotite and hornblende in the samples from both Yucca Mountain and Pahute
Mesa have Fe-rich compositions that contrast strikingly with Fe-poor COMpOSi-
t~ons In the overlying paintbrush Tuff and the underlying Lithic Ridge Tuff at
Yucca Mountain. Each unit from Yucca Mountain has distinctive compositicms
for both sanfdine and plagioclase that very closely match compositions for a
corresponding unit identified within the lower, middle and upPer portions of
the Area 20 tuffs and lavas from Pahute Mesa. Each of these paired units
probably originated fran a conmron parental magma and was erupted contempor-
aneously or nearly so.
Each pair of units with matching phenocryst chemistries has a similar,
but not identical set of petrographic characteristics. The petrographic
differences, as well as small differences in phenocryst chemistry, result from
a zonal distribution of phenucrysts within the parent magma chamber and
eruption through earlier un!ts that differ markedly between Yucca Mountain and
Pahute Mesa.
INTRODUCTION
During the past two years, intensive research into the geochemistry of
the volcanic rocks of Pahute Mesa has been pursued at Los Alamos. The purpose
of thts research has been to establish the usefulness of m~jor, minor, ~nd
trace element geochemistry (fletermlned mostly by neutron actlvotlo~ andlysis,
or NAA) and mineral chemistry !deterinlnedby electron microprobe) in establish-
ing stratlgraphlc correlatioris among units In Pahute Mesa drill holes. This
geochefn!cal approach has been highly successful and allows the definition of
units based on chemistry and petrography rather than lithology; units so
defined are termed “Petrologic Units.” A single Petrologic Unit may Includ<
s?vcral llthologlc units, as seen in Table 1. For example, the Pyroxb,,~
bearing RhyolIte of the Scrugham Peak Quadrangle (Petrologic Unit symbol TRW)
1
Table 1.
Pahutemesaandvicinity
YuccaMountain&ndvicinity
Nomenclature and symbols for Petrologic Units discussed in this report. (Units withfn eact arealisted in stratlgraphic successfcm, youngest unit at the top. Complete stratfgraphic secuencenot given.)
Fig. 1Location of sample sites . Outcrop Iocatlons are open symbo; s, drf11 holelocatlons are closed symbols. Volcanlc units of NTS are present throughoutregion except In stippled areas. Exact locations are given for samples southof Timber Mountain In Warren et al. (In prep.), and for samples of the TRA(u1)unit In Table 2. Locations for samples of other units north of TimberMountain arc Tpb: RW19f; TRA(u2) : Ue20f, RH19f; TRA(P): Ue19pp Ue19x;TRA(p)?: Ue20f; TRA(m): Ue19p, U19ab, Ue19fS; TRA(l r): RW19r, Ue19p, U19ab,Ue191; TRA(sw): RW19r, RU18a; TCT: RW18a. Mineral chemical data me avail-able for all samples frfnn each of these locatlons (USW-G2 and lJe25b-lh fromBroxton et al., 1982), and mudal petrographic data are available for alllocations (except USW-G2 and Ue25b-lh. )
4
—
of tuffs and lavas that comprise
section Is devoted to these topics.
.
a single Petrologic Unit. The following
DESCRIPTION OF PETROLOGIC UNITS OF THE TUFF5 AND LAVAS OF AREA 20
The tuffs and lavas of Area 20 (Byers et al., 1976a) are here divided
into four major Petrologic Units, tenned the upper, plagioclase--icll, middle,
and lower members (Table I). The upper member is further subdivided into an
upper, mafic-poor portion [symbol TRA(u1)] and a lower, mafic-rich portion
[symbol TRA(IJ2)I. The lower member includes highly lichic-rich tuff [symbol
TRA(lr)] av4 the Stockade Wash Tuff [TR4(sw)]. An additional Petrologic Unit
related to the tuffs and lavas of Area 20 iS present beneath the Stockade Wash
Tuff at Rattlesnake Ridge (see Fig. 1 for location), southeast of Pahute Mesa.
On the basis of a single sample, this unit (symbol TCT) is correlated with the
Tr~m Member of the Crater Flat Tuff (Tct).
Each Petrologic Uilit is defined on the basis of well-defirled range in
certain petrographic and mineral chemical parameters; the most useful and
reliable of these is the sanidine composition. Other silicic- to inte~ediate-
composition lavas also occur within the TRA sequence; preliminary study
Indicates that they are associated with the uppermost portions of the TRA!P)
and/or TRA(lr) units. These lavas include the olivine latite of Itawich Vdlley
(Sargent et al., 1966), and~sites of U19e and U19g, and a iava misidentified
as the pre-Pah lnva in U19aj. These lavas are not treated in this report.
6elow, sutnnary tables of petrographic and mfneral compositional data are
given for individual samples of the TRA(u1) unit to illustrate their ranges
within a Petro’iogic Unit (Tables 2-5), but only combined data for all samples
of other Petrologic Units are presented. Tables 6-11 include data for each
Petrologic Unit of the tuffs and lavas of Area 20, as well as its correlative
unit from Yucca Mountain. In each of these tables, data for Petrologic Units
appear in groups; the Petrologic Unit at the bottom of
Yucca Mountain and all those above it are correlat~ve
Mesa and vicinity. Petrologic Units increase in age
each table. For comparison, Table 11 also contains
younger and older than the tuffs and Iavas of Area 20.
each group is found at
units found at Pahute
towards the bottom of
data for units both
5
TRA(u1) Petrologic Unit
The upper, maflc-poor member of the tuffs and lavas of Area 20 consists
of ash-flow tuff, bedded tuff, and lava. The TRA(u1) unit is present in mosr
drill holes in Pahute Mesa (where penetrated), and attains a thickness
exceeding 1000 m in Ue20h. Petrographic results are given for twelve samples
of this unit in Table 2, including
samples of bedded tuff, and a sing’
results for a single sample of the
presented at the bottom of Table 2,
(in sequence) three samples of lava, eight
e sample of ash-flow tuff. For comparison,
tuff of Blacktop Buttes (Tpb unit) is also
This unit is positioned stratigraphically
within the Paintbrush Tuff by Byers et al. (1976a), but has petrographic and
chemical characteristics identical to those of the TRA(u1) unit, and
strikingly different from those of other Paintbrush Tuffs. Field work is in
proqess by Byers and Warren to investigate the possibility that the presently
accepted stratigraphlc position of the Tpb unit is incorrect.
All samples of the TRA(ul) unit show a consistently low phenocryst
content, ranging from 1.4 to 4.5%, and con~istently high proportion of quartz
phenocrysts. They also have a strikingly low content, of mafic m!nerals, iron-
titanium oxides, and accessory minerals. Bi6tite is the nnly mafic mineral
present irI most samples. Ilmenite, sphene, and perrierite (all abundant in
most units of the Paintbrush Tuff and many other ~olcanic units of the NTS)
were not found in any of these samples, but allanite is present in many
samples. Except for the presence of appreciable hornblende, pyroxene, and
apatite in sample RW19r-7, there are no significant differences among the
primary mineral contents of the samples of TRA(I!l) unit (Table 2).
Sanidine compositions, represented by their orthoclase (Or, KAlSi308) +
celsian (Cn, BaA12Si208) molecular percents (mol%) and BaO contents (Table 3)
are also very similar for all samples of the TRA(u1) unit. Compared to other
units of tho NTS, sanidine of the TRA(u1) unit is potassium-rich and barium-
poor. There fs a slight, but consistent, decrease in the Or+Cn content of
sanidine stratigraph!cally upward at each drill core location, from Or+Cn ■ 69
in the stratigraphically lowest sample at each location to a value as
potassium-poor as Or+Cn r 65 in Ue20e-1. The sanidine compositions near the
base of the TRA(u1) unit match those of the underlying TRA(u2) unit, and those
near the top match those at the base of the overlying Topopah Spring Member of
the Paintbrush Tuff (M~rren et al., in prep.; Caporuscio et al., 1982).
&rlm FelstcIrm Polmts Ptbtno- Relttlwt t fclsici(Dzl cMCtU Voids Pmtce Lltbics trysts u I P
—— .— —— .———— —— ——— .— —
0
02
0
0
0
0
0
0
0
0
0
0
—— ——— —— —
o 10
000 23
00
02
05
07
00
00
00
08
0 27
0 92
6K@-1 Trm
1.k&-l-1715 Trw
-352S Tr~
Ut9r-7 Trab
M20g-5 Treb
ue19p-16a Trab
-1652 Treb
lJe191-ml Tr&
w-2474 Trab
ll19~16M Trab
-1 740-5d Trab
uE&-1-3155 Tr*
9M9f-L2 Tpb
:f6Mult.c2Pc#P~*lLs
o
c
c
o
0
c
c
c
04
4s
c
0
11
1
B
b
b
b
b
b
b
b
C1.*
61
S+,zc
c1 .D2C
c1c1c1ZcZc
61
Zc .61
Zc
61
3.4
22
4.0
17
12
5.2
11
2.5
2.3
2.6
z-i
2.0
8.1
C.o
0.0
0.0
1.4
3.9
11
1.1
0.4
14
13
6.4
1.2
3.0
1.9
1.5
4.5
18* M“ 48*
44* 3P 17*
46 42 12
0
00
0
0
0
0
0
0
0
0
0
0
9 14
6 16
026
33 3
0.6 0.3
23
25
03
05
00
25
0 0.2
97
M
100
41m
o
0
0
0 0.6 0n4 595
617 457
523 528
14S 435
724 595
153 559
123 535
640 475
626 515
153 310
234 w
534 - ~m
617 504
0
0
0
3300
.30 0
440 0
00
00
210 29
0
0
0
0
0
0
0
13
0
0
0
0
4.1
1.4
2.3
2.1
2.5
2.2
2.1
3.1
42* 42* 16*
63* 23” 14*
52” 31* 11”46* u’ 1P
51* 43” 6“
33* 479 ZtV
39* 33* 20*
39* 26* 35*
37
0
0
0
00
0
0
0
0
0
0
0
0
0
0
600 0
100 0
120 0
120 0
93 0
140 12b
32 0
lm o
440
280
82
170
77
350
62
110
0
0
0
0
0
0
0
0
0
0
0
0
00
0
0
0
7
12
2a
44
22
23
25
Mo2.6 28* 29” 43* 140 o
2@3 o2.1 35* ’28” 37* 410 71 0rNt
Explzmatim of S-IS:
L1*IosIcrniC: Trm = mmer tiollcs It-a of brea 20: Ireb ● ~ w asts-flow Mffs of AR4 20: Tob ■ luff ofCl=k~ Battes ““ -
. .
~le ~: c - &fll core; de = cuttlfbps -t am repmsent4tiwe of lftilog; e = outcrop lnewsdJ Ststecnordl MM, In inters: MOg-; 28519W. 1157=; 3M09-5 2ZM161M, 17601~; W19r-7 2WM?M. lWW.2E;Msf-lz -1-. 17%4X). wrs foi- core ssd cuttl~s ftiicata ~le &pth, tm f-t.
Table 3. Frequency distribution of Or+Cn and BaO contents for sanidlne phenocrysts Inlndlvldual samples of TRA(u1) and single sample of Tpb unit (RM19f-12). (Each valuerepresents the number of analyses that have orthoclase+celslan (Or+Cn) end-membercontents, and barium oxide wefght contents, wfth~n the interval Indicated. Symbol Sfor rock type defined In Table 2.)
Units of the tuffs and lavas of Area 20, and ?i~ striki~gly magnesium-poor
(Mg*@.4) compared to most NTS units.
Petrographic results for the TRA(u1) unit are summarized as median values
in Table 6. Mineral compositional data discussed above are combined for all
samples of the TRA(u1) unit in Table 7 for sanidine, in Table 8 ior plaglo-
clase, in Table 9 for biotite, and in Table 10 for hornblende. Dominant
values for the compositional parameters represented in Tables 7-10 are given
in Table 11; the dominant value is equivalent to the statistical mode.
TRA(u2) Petrologic Unit
The upper, mafic-rich member of the tuf;s and lavas of Area 20 consists
of ash-flow tuff, bedded tuff, and lava. The TRA(u2) unit is about 230 m
thick In iJe20f but is absent in Ue19p. Samples of the TRA(u2) unft contain
the same primary minerals as those of the TRA(u1) unit, except that the
9
Table 5.
Sample no.
——.
Frequency distribution of molecu:ar Mg/(Mg+Fe) contents for biotite phenocrysts in individualsamples of TRA(u1) and single samDle of TDb unit (RW19f-12). (Each value represents the number ofanalyses that have molecul~r t4g/(Mg+Fe) end-member contents within the Interval indicated. Symbolsfor rock type defined In Table 2.)
concentrations of these minerals are much higher (Table 6). The complete
I
1
I
absence of all other mafic minerals despite a high concentration of biotite
(up to 3.6% in one sample) is particularly distinctive.
Sanidine (Table 7) and plagioclase (Table f3) compositions of the TRA(u2)
unit are very similar to those at the base of the TRA(u1) unit, as previously
noted. Biotite of the TRA(u2) unit has a slightly, but significantly higher
Mg content than biotite of the TRA(u1) unit. Compared t’ other NTS units
(Table 11), sanidine is highly potassium-rich and moderately barium-rich, and
plagioclase is calcium-rich.
-m petrologic Unit
The plagioclase-rich member of the tuffs and lavas of Area 20 consists of
ash-flow tuff, bedded tuff, and lava. The stratigraphic positicn of the
TRA(p) unit is well established in Ue19p between the TRA(u1) and TRA(m) units,
10
5.2
3.0
2.52
0.7
3.0
3.7
9.0
2.0
c.?
z;
S.n
0.5
1.4
6.3
2.3
2.7
2.4
12
25
9.s
13
4.3
9.6
6.9
5.0
12
12
11
lts.jor ccqawnts. %
Uder Fel SIC Relative \ felsics Raflc phenocryscs (ppmv)Petrologic of ~Fnw-
untt Lmatfon -Ies Ltthlcs trysts G K P—. . .
T2A(lsll m 12
Tpe m i
Tti E m 5
m(p) m 3
TM(p)-l m 3
m(m) m 5
TIP m 22
d
4T’AA(’:! m 10
T-M(S9) m zTC6 m 35
TCT m 1
TC1 m 21
—44
35
52
35
32
16
1!
5
13
29
22
Is
m
33
ii-m22
29
14
20
25
67
44
47
50
36
39
33
—17
37
27
26
51
64
60
a
43
25
n
45
32
M
Eliot Hbld Cpx OpI 01 M Arf—— —.—. ——
155 0 0
410 71 0
770 0 0
6WO0
woo
MMOOO
61m 48M O
lm 170 0
25000
56000
la w 15
mmao
4um9 o
35M 0 0
000070C0
o 000
0000
0000
0000
0 000
Ooco
t 000
0060
0 0 9 0.5
0000
0000
0000
Fe-Tt oxides(pm]
H* 11=—.
130 02200
:25
1300 0
1lm
8200
1500 0
4a02
m
370 0
410 0
Hal
770 0
Im
o0
00
0c
o00
00
4
92
0
0
510
00
5
40
0
99
0
000
00
00
00
00
0
4
0
Sph All Per Ap 2r
T
o0
1
9
0.2
130
17
20
170
0e
2
16
26
77
52
4
7
4
33
53
49
lW
12
25
19
11
34
28
?5
~Petrolqlc of Or+cn. Ml& ho, Wti
Umi t Lmtf- ~les 7C 64 w 40 M 0 0.6 :.2 1.8 2.4
II 1 I II 1 w I I I 1- 1-1 II I .-r I I l-l
1 11
12
1
11
lli13
I
1
i T-T lT 1~1362742
n 1
67 11
61711621
3642964
20-..
51
269;
70 8 11
10 10 1
mid) Fn 12~
11?148205
1P m 1 ,3 3
m 10 ( 82s
22
2
99
2 11
1 1
1 535
13
259:
24
15
1TtA[mz)
Tn2
1
m(p)
m(p)?
mFH
3
3
3732
1032
3143i
1 ! 21 74
1355
3793:
m(m)
TcP
7
33il
13”;
111
s20
962< 71111
15 13 2
451299626 3 1
W(lr)
TM(9)
m
10
2
26
mnm
mm
1
2s ,111 m 157 43 aI
but its position with respect to the TRA(uZ) unit is uncertain. A 500-m-thick
unit in Ue20f has been identified as the TRA(p)? unit (see Tables 7-11); this
unit directly underlies the TRA(u2) unit. Samples of the TRA(p) unit
characteristically have consistently high plagioclase contents, and most
contain abundant hornblende in addition to biotite (see Table 6).
Sanidine (Table 7) and plagioclase (Table 8) compositions of the TRA(P)
unit are slgnfffcantly more sodium-rfch than those of the TRA(u2) unit, and
sanfdine fs considerably more potassium-rfch than sanidfne of the underlying
TRA(m) unft. However, a sample of the TRA(p) unft cannot be confidently
distinguished from one of the TRA(lr) unft on the basis of mineral chemistry
(compare unfts In Tables 7-10). Furthermore, some individual samples of the
TRA(lr) unit thdt have relatively hfgh plagfoclase contents and relatively low
contents of lfthic fragments are petrographically simflar to samples of the
TRA(p) unft, and so a distinction between thc~e units based on petrography is
also uncertain. The TRA(lr) and TRA(p) units can be confidently distinguished
only if th~’ strat~grdphic relatfon to the distinctive TRA(m) unit Is known.
TRA(m) Petrologic Unit
The middle member of the tuffs and lavas of Area 20 consists of ash-flow
tuff and bedded tuff. Lavas have not presently been recognized for the TRA(m)
unit, which consists mostly of very fine (a$h fall) tuff where characterized.
The unit fs 65 m thick in Ue19p. The TRA(m) unit fs distfnct due to a con-
sistently and distinctly low content of quartz and high content of sanfdine
(Table 6). In additfon, samples of the TRA(m) unft exhfbit extremely low
biotite contents, but contain hornblende contents that approximately equal
that of biotite.
Sanidlne (Table 7) and plagioclase (Table 8) compositions of the TRA(m)
unit are relatively sodium-rich. Sanldine compositions are particularly
rllstlnct from those of any other TRA unit (Table 7). In addition, one sample
of the TRA(m) unit contains an appreciable content of Fe-rich orthopyroxene
(Mg* w.3). Such orthopyroxcne is rarely found in NTS rocks and has been
presently ~dentified only In single samples of the TRA(P), Tpb, and TCP units.
TRA(lr) Petrologic Unit
The lithic”.richmember of the tuffs and lavas of Area 2(Iconsfsts of non-
to partially welded ash-flow tuff. The TRA(lr) unit fs widely distributed
13
T#bl@ 8. Froqumcy al ttribution of An contonts for pl~gloclasc phenocrysts In sawlesYucca tiufi~tln, and RittlesnJke Rtdge. (Each value represents themanber of●nd~r contents within the intww~l indtcated. Results c~ined for tllYucca Muntttn fr~ Uarren et *I., in prep.).
Ntierof An, Dolt
Unit 5e~les Lecttfon 10 20 30 40
of Petrologic Untt! of Pahute !lega.anti ses that have anortht te (An)
zscmp ●s of ●ach untt. Data for
so 60 70
I I 1 I
i 2 21 63
115
1 6 11 25
5 11
61577
3 13 1P
923144
91711
I I 1 1
\71851
33 1
!9311
381s52
713964
712
21 1
121
14231
1 I I I
211
322
112S3
12121
131
1 21
13242
—— —.I I I 1 I I I I
1
k
/211
1 I 1 I
1
1
1
1
1
12
TRA(U1)
Tpb
nil
12 m
1 m
8 YM
1
1
1
1
19
1
Ill
3213
112
11
11
1113
TRA(u2)
7n2
3 Pm
3 m
TAA(P)m(p)?
3 Pm
3 Pm
TR4(m)
KP5 M
16 w
22645130
141i61
3 35 127 79 16
2
~3322
153466
44 1
TRA(lr)
IRA(W)Tce
10 Pm
2 RR
29 m
21543
11
‘66646
L
2
10 14 14 13 13Lla31
1 1
6155
1:1
944i l!-111
1 1
1
531311
TCTTCT
1 RR
26 w! L 12532
L
Table 9. Frequency distribution of molecular 74g/(Mg+Fe) contents for blotfte phenocrystsIn samples o? Petrologic un~ts of Pahuta 14es#, Yucca Hountafn, and RattlesnakeRld9e. (Each value reDrasents the number of #nalYses that havcmolecultr14g/iM +FQ) end-met
?v contents wfthtn the fntervai fndfcated. Refults Cdfnd
for a 1 stmples of each unft. Data for YUCCR Wuntaln from blarren et al., Inprtpo).
Numberof
S4mp 1es.—
12
1
7
6
6
3
3
4
6
10
2
20
1
le
I ~ molacultr Mg/(Mg+Fe)
Location .30 .40 . 5U .60 .70Unit
TRA(u1)
Tpb
TH 1
TRA(u2)
TH2
TilA(p)
TRA[p)?
TRA(m)
Tcp
TRA(lr)
TRA( SW ]
TCB
TCT
TC T
I I 1 I I I I t3 2 13 24 6 10 2
I I I I
121
22
135
11
11
2
PM
PM
YM
PM
YM
PM
PM
PM
YM
PM
RR
YM
RR
YM
1
1
1
211
151
6 lJ 13 21
701?4
1 11 4799
232 3178
3 1171
?133 1
1 2 635
1 72712 4 4 1 3
14 5J
35”’I 3441
211
14 S022271341.-L
14
throughout Pahute Mesa. It Is >400 m thick In Ue19p and about 500 m thick in
Ue20f. Except ne~r the uppermost portion of the unit, samples of the TRA(lr)
unit consistently contain e~ceptionally high contents of lithic fragments
(Table 6) derived almost exclusively from the underlying peralkal ine units of
the Silent Canyon area. These lithic fragnents are unusually poorly sorted;
their sizes range down to microscopic, as ~llustrated In Figure 2, and up to
meters. Their presence provides a highly distinct petrographic characteristic
of the TRA(lr) unit. Samples of the TRA(lr) unit characteristically contain a
low to moderate content of felsic phenocrysts with plagioclase subordinate to
sanidine and quartz (Table 6). The biotite content is low, and hornblende is
absent. However, near both the top and bottom of the unit, samples have pheno-
cryst contents as high as 26%, plagioclase is dominant, and both biotite and
hornblende are abundant. “
Two very distinct compositions occur for sanldine In samples of the
TRA(lr) unit; one with a dominant Or+Cn value of 62 mol% and the other with an
Or+Cn value of 40 mol% (see Table 7). The former composition is similar to
danlnant compositions for other TRA units (see Tables 7,11), and represents
the true phenocryst chemistry. The latter composition matches those for
santdine In samples of the underlying peralkallne rocks and for sanidlne
phenocrysts within the lithic fragments of the TRA(lr) unit; sanldine grains
with th~se compositions are clearly xenocrysts. No other unit of the NTS is
known to contain sanidlne xenocrysts In such abundance. Plagioclase
compositions (Table 8) are not unusual compared to other NTS urlits (Table 11),
and both biotite (Table 9) and hornblende (Table 10) compositions are
magnesium-poor (Table 11), typical of the tuffc and rhyolltes of Area 20.
TRA(sw) Petrologic Unit
The TRA(SW) Petrologic llnlt is equivalent to the Stockade Hash Tuff(7) of
Byers et al. (1976d) and mly additionally include bedded tuff stratigraph-
Ically bounding the ash-flow coollng unit. TWC samples of the Stockade Wash
Tuff were examined; these were collected from locations (RW19r and RU18a, Fig.
1) that Byers et al. (1976a) consider probably not strati graphically
equivalent. The Strdtigraphic position of the TRA(sw) unit in the Quartet
Dome quadrangle (Sargent et al., 1966) has been confidently established at
lccation RW19r, where it directly underlies the TRA(lr) Petrologic Unit
(“conglomerate” of Sargent et al., 1966). The petrogr~phy and mineral
15
a.
b.
Fig. 2Photomlcrographs of sample Ue19p-2204, TRA(lr) unit. Note the abundantfragnents (mottled appearance), particularly those with very small}“ieldof view 1.9 x 2.8 m. (a) reflected Ilght, (b) transmitted l{ght.
16
llthlcsizes.
.
Table 10.
Unit
TRA(u1)
Tpb
TRA(p)
TRA(p)?
TRA(m)
TCP
TRA(lr)
TRA( SW)
TCB
TCT
within the IntervalYucca Pbuntain frm.,
Numberof
Samples Location
Frequency distribution of molecular Mg/(Mg+Fe) contents for Ilornblelide phenocrysts In
samples of Petrologic units of Pahute mesa, Yucca Mountiln, and Rattlesnake Ridge. (Eachvalue represents the nmber of analyses that have u?oleculer Mg/(Mg+Fe) ●nd-~er contents
Indfcated. Results canblned for tll smoles of each unit. Dat# forWarren et al., in prep.].
—r
molecular Mg/(Mg+Fe).30 .40 .50 .60 .70
I PM
1 PM
3 PM
2 PM
4 PM
2 YM
4 PM
2 RR
4 Ym
1 RR
chemistry of
(Hlnrichs et
Quartet Dome
these areas
TRA(p) unit.
r~
1
I I I I
1 2
34
2
11384
11
212
11
1
I 1 Ill I i
I I 1 I
11
2
355
10712
11
11
1422 1
351
75
I I I I1
1 I
I I I I
1
11
1
-J-LJ-l-
the sample at locatlon Rli18a from the Ammonia Tanks quadrangle
al,, 1967) Identically matches the sample of this unit from the
quadrangle. Nonetheless, the correlation of the unit between
Is considered uncertain due to a possible confusion wtth the
TCT Petrologic Unit (Rattlesnake Ridge Location)-—A single sample of bedded tuff from Rottleznake Ridge (locatlon In Figure
1) is tentatively correlated with the TCT unit of Yucca 140untaln. This thin
(18 m thick) bedded tuff Is bounded stratlgraphlcally below by the Grouse
Canyon Member of the Belted Range Tuff and abuve by the TRA(sw) unit. It iS
conceivable that the TRA(sw) unit at this locatlon correlates with the TRA(p)
rather than the TRA(lr) unit [see discussion of TRA(sw) unit]; In tt?ls case
the sample of bedded tuff might represent the base of the TRA(p) unit. Such
lb considered unllkcly because the petrography and mineral chemistry of this
sample of TCT unit differs distinctly from all known or tentatively assigned
samples of TRA(p) unit (see Tables 6-11).
.
17
Table 11. Dominant values for compositional parameters of phenocrysts for Petrologic Units ofPahute Mesa Yucca Mountain, and Rattlesnake Rid ●. (The dominant value isequlvalent to
!rthe statlst{cisl mode for the frequency dlstribut on of anal ses represented in Tables7-10. S~bols for all Petrologic Units defined in Table 1.
Maflc MineralsSanidine Plagioclase
MoltAn
Numberof
Samples
Molecular Hg/(14wF@)Ml%
OrtCnw tzBaO
PetrologicUnit
.Location Blot
——Hbld
0.00, 1.13b 19, 24b
1313
l~c6
13
202020
2524
1713
1211
15
;:
H
Ii
:!
TMRu a
PMb
;:
PM
PMPMYM
PMYM
PmPM
PMYM
PhiRRYM
RRYM
Yn)?!YMYM
6
;
:
9
12
1;
37
33
2:
102
35
131
16826
60 0.62 0.64
TMR 1 upper1ower
O.OO0.00 0.60 0.72
0.650.70
TPCU upperlower
TRPP
4936
0.050.05
0.680.66
0.6549 0.75
TRA(u1)TbTh
0.120.090.10
0.37
0.350.38
0.460.39
TRA(U2)TH2
6971
0.500,71
0.440.43
6361
0.360.25
0.430.42
0.470.44
TRA(m)TCP
5353
0.050.14
0.370.42
0.37
62, 40b6261
0.13, O.oob0.290.56
0.370.400.40
0.430.440.44
TRA( 1 r)TRA( SW)TCB
TCTTCT
6967
0.270.55
0.420.42
TLRTTATTBTTc
0.67l!: 0.5566 0.9672 3.4
0.590.550.590.6?
~ !-ocatlons throughoutc Bimodal population
K-rfch anorthoclase.
NTS
Ca-rich plagfoclase (mantl@d by K-rich feldspar) also present.
18
other Petrologic Units.—Most other Petrologic Units discussed in this report (Table 1) consist of
well-described ash-flow coolfng units, mostly from Yucca Mountain (location
shown in Figure 1). Each such Petrologic Unit also includes strat+graphfcally
bounding bedded tuff that can be petrogruphically and chemically related to
the ash flow, but this added tuff is so volumetrically insignificant that the
distinction between Petrologic and Lith~logic Units is unimportant.
Descriptions of units younger than the TRA units are found in Byers et al.
(1976a), and descriptions for Petrologic Units of Yucca Mountain ar. ontained
in Warren et al. (in prep.).
COMPARISON OF TRA PETROLOGIC U!.ITSOF PAHUTE MESA WITH UNITS OF YUC,TAMOUNTAIN
The occurrence of substantial petrographic variations within single
‘Iithologic units of the NTS are well documented. Many NTS ash-flow cooling
units have mafic-r!ch caprocks (e.g., Lipman et al. 1966; Byers et al.,
1976a) . Substantial petrographic variations are now well documented for ash-
flow cooling units that do not h~ve mafic-rich caprocks; for example, the
upper porticn of the TCB ur,ltof USW-G1 is quartz-rich, but the lower pcrtion
IS quartz-poor (Carr et al., in press; Warren et al., in prep.). The TPCU
unit is a single cooling unit only 22 m thick in Ue19p, but the phenocryst
content differs by a factor of 3.5 between top afld bottom of the unit and
mafic mineral and trace mineral contents differ by an order of magnitude or
more (Warren, in prep.). It is clear that primary minerals (phenocrysts) are
not homogeneously distributed within most mag!nas. Furthermore, It might be
etl’~rted that the upper portion of a magma miqht concentrate volatiles.
Explosive release of these volatlles would result in eruption of the upper
portion of the magma as tuff, whereas the lower, more volatile-depleted
portion of the magma would tend to erupt more quietly, as a lava flow. Such
an eruption would result In both tuff and lava from the same magma.
Historical eruptions In such a manner are known (tiildreth and Drake, 1983).
Additionally, lary-vol~rne eruptions of tuff will occur ne~r-source as massive
and poorly scrted ash tlows, but os well sorted (bedded) tuffs farther from
the source (see, for example, Figure 8 in Sheridan, 1979). Overprinted on
these primary features
features of compaction
tilthough eruption of a
due to emplacement mechanics are the Tonal cooling
and crystallization described by Smith (1960). Thus ,
gfvcn magma might provide a time-stratigraphic marke”,
19
the recognition of this “pulse” might be very difficult due to verticai and
lateral variations both in the lithology and iil the primary mineral content in
the erupted matsrial.
Fortunately, the mineral chemistry of most eruptive sequences of the NTS
has bsen found to be unaffected by petrographic and lithologic variations.
For example, suost.antial petrographic variations occur both vertically and hori-
zontally wtthin the TCB unit (W~rren et al., +n prep.). Although samples from
this unit were obtained from numerous locations, separated by as much as 55
km, coinnosicions for sanidine are identical at all locations within the small
analytical uncert~lnty of about 1 mol% Or+Cn. Similar results have been
obtained for other minerals, particularly biotite and plagioclase. In
gener~al, each ucit II?S a unique set of mineral compositions that differs from
those of all other NTS units cnd serves as an invaluable aid in its recogni-
tim. The similarity in mineral chemistries between the TRA(p) and TRA(sw)
units noted in their descriptions is an unusual, and highly significant
exception. It should be noted, however, that not all units show as remarkable
a vertical and ?~teral consistency in mineral compositions as does the TCB
unit. There are sigllific~nt systematic vtiriat!ons in sanidine composition
within the Topopah Spring (Broxton et al., 1982) iind Rainier Mesa rhyolites
that could be employed to define stratigraphi; levels within these units.
Comparison of Mineral Chemistry
Although there are small (but significant) differences among individual
units, all TRA units have distl~ictively ilg-poor mafic minerals. In ccntrast,
mafic minerals in urltts of the overlying Paintbrush Tuff and all~ed lavas of
Pahute Mesa havq characteristically Mg-rich compositions (see Table 11). The
peralkallne rocks that underlie the TRA sequence are extremely biotite-poor
(most samples lack biotite) and Instead contain 01ivine and clinopyroxene
phcnocrysts that irlmany cases are nearly pure Fe end members.
At Yucca Mountain, mafi( miner?ls In the Crater Flat Tuff and overlying
tuffs and lavas of Calico Hills have Mg-poor compositions that are identical
to those of the TRA units of Pahute Mesa (see Tables 9-11). The overly+ng
Paintbrush Tuffs, except for the Topopah Spring rhyolite, have characteris-
tically Mg-rich maflc minerals identical to those in the Paintbrush Tuffs and
allied lavus of Pahute Mesa. The Crater Flat Tuff of Yucca Mountain, however,
overlies the Lithic Ridge Tuff And associated lavas rather than the
20
peralkaline rocks that underlie the TRA units of Pahute Mesa. The Lithic
Ridge and older units are generally plagioclase-rich units (Warren et al., in
prep. ! that bear Mg-rich mafic minerals (Table 11). It Is clear that the TRA
units of Pahute Mesa and the Crater Flat and Calico Hills tuffs of Yucca
Mountain have compositions for mafic minerals that are indistinguishable from
each other hut are highly different from those of bounding volcanic groups.
In contrast to mafic mineral compositions, sanidine and plagioclase
compositions dfffer distinctly among units, an~ can be compared unit-by--unit
thrcugbout the stratigraphic columns of Pahute Mesa and Yucca Mountafn (Figure
). Sanidine compositions (Table 7) a)~ Identical within the small analytical
uncertainties for each pair of units in the stratigraphic sequence at both
locfltions. All compositions of fndividu~l phenocrysts that differ substan-
tially from those of the daninant composition (Table 11) are due to xenocrysts
PAHUTE MESA
I- ///YUCCA MOUNTAIN ,/
M
/’Palntbruah ,/luffs
/TH 1 _ _ —.— — - -
TH2
u’K,
- — —.. _ _
TCP \\
<TCB \\’\
\~\
\\ -.=
TCT \\
\VM ---— — — _
TLR
PdntlwmhTuffab AHbd IAVn
TRA (uI)
TRA (u21”,----------
TRA (P)*
TRA (It)
[ TCT
TSCP
* R, IMIvomratlgr@k rmhm uncmmln
Fig. 3Correlation diagram between Petrologic Units of Yucca Mountain and PahuteMesa. (symbols for units defined in Table 1. TSCP ■ peralkaline rock of theSilent Canyon area. Greatest known or inferred thickness for each unitIllustrated. )
21
or to the occurrence of narrow sodium-rich rims (see Figure 4) produced from
late-stage deuteric alteration (Warren et al., in prep.). Matching units,
stratigraphically downward ,unit present at Fahute Mesa listed first), are
TRA(u1) and TH1; TRA(u2) and TH2; TRA(m) and TCP; TRA(lr) and TCB; and TCT and
TCT . A unit equivalent to the TRA(p) unit of Pahute Mesa is not known for
Yucca Mountain. Plagioclase compositions (Table 8) match in similar fashion.
Although the TRA(lr) unit of Pahute Mesa contains sanidine whose
composition (dominant Or+Cn value = 62, Tables 7 and 11) matches the TCB unit
of Yucca Mountain, it also contains a population of sodium-rich sanidine
xenocrysts that do not occur in the TCB unit. Additlcnally, there are
significant differences in the barium contents of Sanidine for many paired
units, moS*. notably between the TRA{lr) and TCB units (see Table 11).
Discussion o’ these differences is deferred to a following section.
Comparison of Lithology and Petrography
The primary mineral contents of the TRA units of Pahute Mesa are quite
similar to their paired unit of Yucca Mountain (Table 6). At both locations,
Fig. 4Transmitted light photomicrograph (crossed nicols), of sodium-enriched rim ofsanidlne in sample CFLSM-5, TCB unit. Field of view 0.24 x 0.35 nun.
22
these units contain abundant quartz, and variable amounts of biotite, horn-
blende, and allanite. Pyroxene, sphene, and perrierite rarely occur in
samples of these units. These petrographic characteristics contrast
strikingly with those of stratigraphically bounding units of both areas (Byers
et al., 1976a; Warren et al., in prep.; Warren, in prep.). The match in
primary mineral contents is excellent for several of the paired units of
Figure 3, particularly for the TRA(u1) and TH1 units.
The most substantial Iithologic and petrographic differences between
paired units occur between the TRA(lr) and TCB units. Samples of these units
are grossly- dissimilar in hand sample; the TRA(lr) unit is exceptionally
lithic-rich and generally non-welded whereas the TCB unit is quite lithic-poor
and always occurs as a well-defined c~oling unit. Portions of the TCB cooling
unit may be densely welded or even vitrophyric. Differences in the primary
mineral contents of these units ar’” not as great, but nonetheless they are
appreciable. Most conspicuous is the much higher .,mdian biotite content of
the TCB unit (0.20%) compared to that of the TRA(lr) ~n’lt (0.06%). However,
highly phenocryst- and mafic-rich zones occur within the TRA(lr) but not
within the TCB unit. Thus, the average phenocryst and mafic contents of the
TRA(lr) unit are considerably higher than median values, and averages probably
match much better for the two units than the medians. The TRA(m) unit of
Pahcte Mesa also differs appreciably in lithology and primary mineral content
from the TCP unit of Yucca Mountain. The TRA(m) unit generally has a low tu
moderate content of phenocrysts, mostly saniriine (Table 6), and occurs as a
well-sorted (bedded) tuff where presently characterized. It is distinctly
quartz-poor. The TCP unit contains a considerable) higher phenocryst content,
and occurs as a well-defined ash-flow cooling u~lit. Both units, however,
contain a highly distinctive, magnesium-poor orttopyroxene
striking correlation of primary mineral contents.
DISCUSSION OF RESULTS: EVIDENCE FOR A COMMON MAGMATIC
that provides a
ORIGIN OF
VOLCANIC SEQUENCES THAT FLANK ‘HE TIMBER MOUNTAIN CALDERA
Each TRA unit of Pahute Mesa and correlative unit of Yucca Mountain
(Figure 3) contains Mg-puor mafic minerals, consisting primarily of biotite
and/or hornblende. The chemistry of these minerals differs distinctly from
those of bounding volcanic groups, and suggests
location were derived from closely similar magmas
that the sequences at each
or from the same magma. By
23
contrast, the chemistry of sanidine and plagioclase differs markedly between
successive Petrologic Units. These large chemical differences within each
stratigraphic succession are parallel at each location. It is considered
htghly unlikely that separate magmas could evolve in such a manner to produce
the observed correspondence in feldspar chemistry. The mineral chemical data
thus strongly indicates that each of the paired units of Yucca Mountain and
Pahute Mesa was derived from the same magma.
It is unlikely that Petrologic Units that include lavas have been
emplaced very far from their source; such units include the TRA(u1), TRA(u2),
and TRA(p) units of Pahute Mesa and the TH1 and TH2 units of Yucca Mountain.
Thick exposures of the TH ~nits occur north of Yucca Mountain and at Calico
Hills (Byers et al., 1976b). If these lavas ascended directly upward from a
magma chamber, a very large magma chamber must have been present during
eruption of the TH and TRA(u) units if indeed these units represent magma from
the same chamber. The distribution of TRA and TH lavas (shown in Figure 5)
may then represent the approximate limits of this magma chamber. The Timber
Mountain Caldera, a much younger feature, is loca~ed near its center. Lavas
intermediate in age between the tuffs and lavas of Area 20 and the Timber
Mountain Tuff have also been correlated iicross the Timber Mountain Caldera
(see Figure 19 in Byers et al. , 1976a). This suggests that the Timber
Mountain area has been the center of a sequence of chemically different magma
systems throughout an extensive period of time. It is probable that these
magma systems, which ~roduced a thick sequence of NTS volcanic rocks including
the tuffs and lavas of Calico Hills, tuffs and lavas of Area 20, Paintbrush
Tuff and Timber Mountain Tuff are related as a single, large evolving magma
system centered beneath Timber Mour~tain. A model that might describe such a
magma system is described by Hlldreth (1981). Each pair of unfts fcund on
opposite sides of Timber Mountain might have been erupted from a central
source, the present location of Timber Mountain, or from separate sources. If
the former is true, Pahute Mesa and Yucca Mountain are marginal to a major
structure (e.g., caldera) associated with eruption of these units. The latter
possibility, eruption from separate sources, IS consistent with presently
accepted views. In this case, the Crater Flat Tuffs and tuffs and lavas of
Area 20 were erupted from structures that flank Timber Mountain (Carr, 1982;
Orkild et al., 19LP). It is likely that the magma chamber was not fully
emptied during the tinal stages of erupt~on and the remaining llq[ld h~s
24
11
TI
-...*w
,,, *,
\
%,3PN [ .’
i ..- 1
i #-la;
L m 00W0ARY———— —0,,*I,,, :,
‘o,,,,,/10,,,
,,, ,. .,,,,,, :%,/,,,,,,,,1’
,1
‘. :-’ %,,rt...b1 ,.. .,,
“\... :.,, ! ,.
J,’ ,,
...! ,,!’ ,,,
i . .‘J:,.! .. vWa R81
:. ,,
i \\‘,,
,, lb., . ..,,, ,,”
,,,!,,,,,7:,... “’....,.,,,.,!,,,,,‘, .%‘!.,,,1
J,,
“\
r
1 “.,’
— 1’ ,, ...
Fig. 5Loc~tlon of lavas of the TRA(u) unit (cllagonal pattern north of TimberMountain) and of the TH unit (same pattern south of Timber Mountain). Non-welded tuff shows CI wider dlstrlbutlon for both units. The single magmachamber Inferred to be the source of both lavas Is centered beneath TimberMountafn; the d~strlbutlon of the lavas may approximate the location uf theouter portion of a magma chamber.
w
37%J
solidified to fornr a large pluton beneath Timber Mountain. If the size and
shape of the magma chamber did not change substantially through time, then the
distribution of lavas shown in Figure 5 may also approximate the subsurface
location of such a pluton, which presumably would be a granitlc body.
The nearly identical mineral chemistry for units erupted from opposite
sides of this hypothetical magma chamber indicates that chemical equilibrium
between phenocrysts and liquid is closely maintained throughout an
extraordinarily large volume of magma. This is true even where substantial
variations tif phenocryst concentrations occur within a unit. This indicates
that the magma has an inhomogeneous distribution of phenocrysts, a~d the
concentration obsei~ed withi~ a unit depends upon the precise position that
the sample occupied as a liquld
variations in phenocryst content
and water pressure variations.
chemistry, but the data at hand
in the magma chamber. Probable causes for
throughout a magma chamber are temperature
Such factors might also af’ect the mineral
indicate that for many units they do not.
There is good evidence (Warren, in preparation) that mixing of magmas occurs
at the margi~s of the magma system. This is not an equilibrium process and
non-equilibrium conditions are evident in units affected by magma mixing.
The crystallization sequerce is preserved, however, by variations In the
bariu:llcontents of sanidine. Sanidine has a marked tendency to concentrate
barium {Leeman and Phelps, 1981; Vanson, 1978), which readily substitutes for
potassium because these elements are very large ions of s’nilar size. As
crystallization proceeds, changing physiochemical conditions require the
equilibrium composition of sanidine to change. The primary change usually
requires progwssive replacement of orthoclase component (KAlSi308) by albite
component (N jC8) as temperature decreases. This Is rapidly accomplished
under magnati, dltlons simply by exchang~ of Na with K. Early crystallized
sanidine contains relatively high Da concentrations compared to sanidine
fornred later. However, equilibrium for 13a between early and late sanidines
requires an exchange of celslan component (BaA12SiZ08) with albite. This
equilibrium cannot be attained simply by exchange of Ba with Na, because it
also requires a coupled substitution of Al with Si. The latter elements are
present in a much more tightly bound (tetrahedral) structural site wlt;,ln
sanidine, and require considerably greater energies for exchange.
Consequently, although the Na and K exchange is rapid and complete up to the
time of eruption and reflects equilibrium, Da exchange Is limited or does not
26
occur. This process Is here termed “limited equilibrium.” Thus, Portions of
the magma that began to crystallize sanidine earliest will have the highest Ba
contents, and those that formed sani line latest will have the lowest. Thus ,
the differing Ba contents for sar,id!ne between paired Petrologic Units of
Yucca Mountain and Pahute Me$a simply relate to the crystallization history of
the magma, ind not to inherent canposltional differences between the units.
The distribution ana concentration of volatiles (primarily water) within
the megma chamber Is very important, because they certainly provide the
driving force of the eruption. Tile higher their concentration, the more
violent an eruption might be expected. The element cesl~m concentrates
strongly In the upper portion of the magma that produced the Bishop Tuff
(Hildreth, 1979); this element. shows an extremely strong association with
volatiles. Ceslum concentrations In the TRA(lr) un~t are extraordinarily
high, generally more than an order of magnitude higher than those of other NIS
units, Including the TCB unit (Warren, In prep.). The cesium contents suggest
that volatlles concentrated strol~gly in Lhc portion of the magma chamber that
erupted the TRA(lr) unit, but not In the portion of this same magma chamber
that erupted the TCB unit. These volatiles drove an unusually violent
eruption of the TRA(lr) unit that resulted In the tncorporatlon of remarkably
lhrge and poorly sorted lithlc frhgments within the TRA(lr) unit.
CONCLUSIC’NS AND FUTURE RESEARCH
A very strtklng geochemlcal similarity, ba-nd on chemistry of primary
mineral phases, has been demonstrated between volcanic groups that fl~nk the
Timber Mountain Caldcra. It Is concluded that paired units wlthln the two
locations were derived from the same magma. Llthologlc and petrographic
differences between units flanklng Timber Mountain that have simflar mineral
chcmlstrles are ~ttributable to an Inhomogeneous distribution of phenocrysts
and volatile: within the magma. The dlsti’ibutlon of paired units that contain
thick lavas Indicates that the magma body was very large and centered on
Timber Mountain. The similarities In maflc mineral compositions among an
entire group of units suggest that each successive unit represents the
evolution of a single, large magma system.
It Is the author’s bclluf th~t, thn hypothesized magma system centered at
Timber Mountain was also associated with the eruption of the oldest known NTS
volcanic rocks. The nllncral chcml~try Is presently being Invcstlgated for
such units of Pahute Mesa for comparison wlch well-characterized units of
Yucca Mountain (Warren et al., in prep.). The Petrologic Unit Introduced here
serves as a valuable correlative tool for beddsd tuffs, and is particularly
valuable for drill holes that do not penetrats the ash-flow cooling units used
as marker teds. Volcanic units In other areas of the NTS (e.g., Yucca Flat)
can probably be related to those of Pahute Mesa and Yucca Mountain by utll-
Izing the Petrologic Unit. Such use Is required to correlate older, poorly
exposed units effectively over a large region such as the NTS due to mark~d
llthologic differences that may occur among such units at different locations.
ACKNOWLEDGMENTS
This work has built on 20 years of geologic mapping and study, largely by
geologists of the U.S. Geological Survey but also geologists of several other
organizations. Many of their names are found among the references cited. The
correlations described herein could not have been accomplished without the
basic stratlgraphlc framework developed by previous NIS workers.
David E. Broxton, Frank M. 8yers, Jr., and B. W. Smith provided very
timely and thoughtful reviews. The advice and counsel of Frank M. Byers, Jr.,
has been very helpful. Roland C. Hagan and Lois F. Grltzo have greatly aided
in the microprobe analyses. The ability of Marcia A. Jones to produce complex
tables without error and with remarkable speet Is simply astounding.
Similarly, the ability of David A. Mann and Tlno Lucero to create wonderful
probe sections from r~ks that fall apart In one’s hands Is remarkable. Thfs
research has been vigorously supported by Thomas A. Weaver and Wayne A.
Morris, past and present group leaders of the ESS-2 (Geochemistry) group, and
by Jack H. House, program leader for containment. I am vary gratefbl to all
for their generous contribution.
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—.
28
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