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45
The Geological Society of AmericaSpecial Paper 497
2013
Eruption chronology of the Columbia River Basalt Group
T.L. BarryDepartment of Geology, University of Leicester, University Road, Leicester, LE1 7RH, UK
S.P. KelleyDepartment of Physical Sciences, Centre for Earth, Planetary, Space and Astronomy Research,
Open University, Milton Keynes, MK7 6AA, UK
S.P. ReidelSchool of the Environment, Washington State University–Tri-Cities, 2710 Crimson Way, Richland, Washington 99354, USA
V.E. CampDepartment of Geological Sciences, San Diego State University, 5500 Campanile Drive, San Diego, California 92182, USA
S. SelfDepartment of Physical Sciences, Centre for Earth, Planetary, Space and Astronomy Research,
Open University, Milton Keynes, MK7 6AA, UK
N.A. JarboeDepartment of Earth & Planetary Science, University of California, 1156 High Street, Santa Cruz, California 95064, USA
R.A. DuncanCollege of Earth, Ocean, and Atmospheric Sciences, Oregon State University, Corvallis, Oregon 97331, USA
P.R. RenneBerkeley Geochronology Center, 2455 Ridge Road, Berkeley, California 94709, USA, and
Department of Earth & Planetary Science, University of California, Berkeley, California 94720, USA
ABSTRACT
The Columbia River fl ood basalt province, United States, is likely the most well-studied, radiometrically well-dated large igneous province on Earth. Compared with older, more-altered basalt in fl ood basalt provinces elsewhere, the Columbia River Basalt Group presents an opportunity for precise, accurate ages, and the opportunity to study relationships of volcanism with climatic excursions. We critically assess the available 40Ar/39Ar data for the Columbia River Basalt Group, along with K-Ar data, to establish an up-to-date picture of the timing of emplacement of the major forma-tions that compose the lava stratigraphy. Combining robust Ar-Ar data with fi eld
Barry, T.L., Kelley, S.P., Reidel, S.P., Camp, V.E., Self, S., Jarboe, N.A, Duncan, R.A., and Renne, P.R., 2013, Eruption chronology of the Columbia River Basalt Group, in Reidel, S.P., Camp, V.E., Ross, M.E., Wolff, J.A., Martin, B.S., Tolan, T.L., and Wells, R.E., eds., The Columbia River Flood Basalt Province: Geologi-cal Society of America Special Paper 497, p. 45–66, doi:10.1130/2013.2497(02). For permission to copy, contact [email protected]. © 2013 The Geological Society of America. All rights reserved.
46 Barry et al.
INTRODUCTION
The Columbia River continental fl ood basalt province (Fig. 1), with lavas stratigraphically defi ned as the Columbia River Basalt Group (Swanson et al., 1979, and references therein; Tolan et al., 1989), constitutes the mafi c part of Earth’s youngest large igneous province. Basalt volcanism is generally considered to have begun around 17 Ma in the latter part of the early Mio-cene, close in time to the earliest rhyolitic eruptions associated
with the Snake River Plain hotspot track at ca. 16.5 Ma (e.g., Rytuba and McKee, 1984; Swisher, 1992). Some workers have proposed a plate-tectonic origin for the province involving the passive rise of shallow mantle (e.g., Carlson and Hart, 1987; Smith, 1992; Hales et al., 2005; Tikoff et al., 2008), but others have embraced a deep-mantle origin associated with active rise of the Yellowstone mantle plume (e.g., Duncan, 1982; Brandon and Goles, 1988, 1995; Draper, 1991; Hooper and Hawkesworth, 1993; Geist and Richards, 1993; Camp, 1995; Dodson et al.,
constraints and paleomagnetic information leads to the following recommendations for the age of emplacement of the constituent formations: Steens Basalt, ca. 16.9 to ca. 16.6 Ma; Imnaha Basalt, ca. 16.7 to ca. 16 Ma; Grande Ronde Basalt, ca. 16 Ma to ca. 15.6 Ma; Wanapum Basalt, ca. 15.6 to ca. 15 Ma; and Saddle Mountains Basalt from ca. 15 Ma to ca. 6 Ma. The results underline the previously held observation that Columbia River Basalt activity was dominated by a brief, voluminous pulse of lava production during Grande Ronde Basalt emplacement. Under scrutiny, the data highlight areas of complexity and uncertainty in the timing of eruption phases, and demonstrate that even here in the youngest large igneous province, argon dating can-not resolve intervals and durations of eruptions.
Oregon
Nevada
Idaho
MontanaWashington
California
0 50
Kilometers
Miles
0 80Margin of CRBG
Columbia River
Snake River
Cas
cade
Ran
ge
Salmon River
Snake River
Pac
ific
Oce
an
Grande Ronde River
Imnaha River
River
Salem
Prineville
YakimaaPullman
Spokane
Wenatcheee
Columbia Gorge
Extent of GRBRB
Columbia Basin
OregonPlateau
Lowland
Blue Mountains
Wallowa
ClearwaterEmbayment
WeiserEmbayment
PascoPascoBasinn
John Day
Pasco
DeschutesRiver
KlickitatRiver
WillametteValley
Vantage
Lewiston Basin
Stee
ns M
ount
ain
Roc
kyR
ocky
Mou
ntai
ns M
ount
ains
Roc
ky M
ount
ains
Malheur Gorge
48°
47°
46°
45°
44°
43°
42°
123° 121° 119° 117°
Figure 1. Map of the Columbia River Basalt Group within the northwestern states of Washington, Oregon, Idaho and Nevada, USA, shows the main regions of basalt exposure, including Steens Mountain in the south, Malheur Gorge, and the Columbia and Snake Rivers to the north.
Eruption chronology of the Columbia River Basalt Group 47
1997; Hooper et al., 2002, 2007; Camp et al., 2003; Camp and Ross, 2004; Camp and Hanan, 2008; Wolff et al., 2008; Camp et al., this volume).
Large igneous provinces and their extrusive components, fl ood basalt lavas, represent exceptional volcanic events (Eldholm and Coffi n, 2000). It has been recognized for over 20 years that highly voluminous fl ood basalt provinces worldwide had peak periods of lava output (Rampino and Stothers, 1988) emplaced within geologically short periods of time (typically ~<1 m.y.; e.g., Courtillot et al., 1986; Duncan and Pyle, 1988; Chenet et al., 2008, 2009; Reichow et al., 2009). This signifi es a consid-erable potential for atmospheric loading by volcanic gases and for inundating landscapes with vast volumes of basalt lava. Such events have been linked to mass extinctions (e.g., Wignall, 2001; Courtillot and Renne, 2003; Saunders and Reichow, 2009) and near-surface arrival/emplacement of mantle plumes (e.g., Cour-tillot et al., 2003, and references therein).
The Columbia River Basalt Group is estimated to have a total volume of 210,000 km3 and an areal extent of 208,000 km2 (Reidel et al., this volume). Columbia River Basalt Group lavas are the product of the most voluminous outpouring of basalt lava within the Columbia River–Snake River–Yellowstone province. However, the basalt-dominated part of the province is an order of magnitude smaller in volume than many other large igneous provinces, such as the Deccan basalts (~1.3 × 106 km3; Jay and Widdowson, 2008). Conversely, it appears that volumes of lava emplaced during individual Columbia River Basalt Group erup-tions are as large as those reported from other provinces (Reidel et al., 1989; Reidel, 2005; Self et al., 2006; Reidel and Tolan, this volume). The environmental impact of Columbia River Basalt Group eruptions, or groups of eruptions, is uncertain. One motivation for detailed age constraints is to enable comparison between the timing of the eruptions, including periods of high time-averaged magma output, and any mid-Miocene climatic or biotic perturbations (e.g., Kender et al., 2009). In addition, it may be possible to obtain a better understanding of the absolute age of the Columbia River Basalt Group lavas and the relationship to rhyolitic “pre-Yellowstone” volcanism in the Oregon-Nevada-Idaho region.
This paper presents a compilation of K-Ar and Ar-Ar age determinations for the Columbia River Basalt Group and some related units. It discusses some of the past and present issues with defi ning the longevity and pulse-like nature of the basaltic vol-canism. It examines what is known about correlation with the paleomagnetic time scale for lava units with determined paleopo-larity, and proposes directions for future work in improving the understanding of Columbia River Basalt Group geochronology.
NOMENCLATURE AND PREVIOUS GEOCHRONOLOGICAL WORK ON THE COLUMBIA RIVER BASALT GROUP
In the previous Geological Society of America Special Paper 239 on Volcanism and Tectonism in the Columbia River
Basalt Province (Reidel and Hooper, 1989), the Columbia River Basalt Group was considered to consist of lavas from the Imnaha Basalt and the Grande Ronde Basalt, Wanapum Basalt, and Saddle Mountains Basalt of the Yakima Basalt Subgroup. A few outlying lava sequences that erupted synchronously with the Grande Ronde Basalt, e.g., Picture Gorge Basalt, were also included in the Columbia River Basalt Group. Since that time, developments in mapping and new geochronological studies have led to suggestions that the Steens (Mountain) Basalt and the Basalt of Malheur Gorge, lying to the south of the main Columbia River Basalt Group outcrop area, should be included in the Columbia River Basalt Group (Hooper et al., 2002, 2007; Camp et al., 2003; Camp and Ross, 2004). A new defi nition and the status for the Steens Basalt within the Columbia River Basalt Group are explained in Camp et al. (this volume). The basis for inclusion of the Steens Basalt within the Group are that there is a continuity of erupted magma types with shared isotopic end members (Camp and Hanan, 2008), conformable contacts between the major formations, an apparent northward-shifting locus of eruption sites over time, and contemporaneity within the majority of these lavas (see Camp et al., this volume). Reidel et al. (this volume) describe these updates and the current stratigraphic nomenclature of the Columbia River Basalt Group; Figure 2 provides a summary of the units for which we provide age dates.
The major subdivisions defi ned by previous workers have not changed with these latest revisions, except with the addi-tion of the Steens Basalt as the earliest Columbia River Basalt Group eruptions (Camp et al., this volume) and the Prineville Basalt, which, like the Picture Gorge Basalt, is interbedded with the Grande Ronde Basalt (Reidel et al., this volume). The princi-pal changes to the nomenclature are those to the subdivisions of the formations. Reidel et al. (this volume) present these changes and the current stratigraphic nomenclature and the best current estimates of the spatial extent and volume of these fl ows. More detailed descriptions of some of the units are provided in other chapters in this volume: e.g., Camp et al. (this volume) describe the Steens Basalt; Reidel and Tolan (this volume) describe revi-sions to the nomenclature of the Grande Ronde Basalt since 1989 (Reidel et al., 1989); and Martin et al. (this volume) and Vye (2009) describe the Frenchman Springs Member and Wanapum Basalt nomenclature since 1989. Proposed changes to the Saddle Mountains Basalt stratigraphy are provided in Reidel et al. (this volume).
Initial age determinations of Columbia River Basalt Group lavas, since the earliest radioisotopic dating by the 40K-40Ar tech-nique (e.g., Evernden and James, 1964; Holmgren, 1970, and ref-erences therein; McKee et al., 1977), placed the eruption of the whole province between ca. 17 and 6 Ma (for earlier compilations of age determinations, see also Swanson et al., 1979; Baksi, 1989; Tolan et al., 1989). The overall picture has not changed radically since then. These studies recognized early on that a major erup-tive pulse produced the Grande Ronde Basalt lavas, estimated to have been emplaced between ca. 16.0 and ca. 15.0 Ma (see also
48 Barry et al.
Long and Duncan, 1983; Baksi, 1989; Hooper et al., 2002). Tolan et al. (1989) plotted volume of erupted lava versus time, show-ing how the Grande Ronde Basalt lavas dominate volumetrically. These studies also proposed that the bulk of the Columbia River Basalt Group lavas could have been erupted in a short period of time (<1–2 m.y.; Holmgren, 1970; McKee et al., 1977), with the Grande Ronde Basalt pulse only occupying a brief span, conjec-tured to be ~400,000 yr (Barry et al., 2010), and unresolvable with standard geochronological approaches. Recent updates to volume estimates for the Columbia River Basalt Group do not alter this view, but they do clarify a single large peak (acme) of lava production, with slightly earlier peaks, or synchronous high-output periods in different geographic areas.
More recent attempts at determining ages of Columbia River Basalt Group lavas using the 40Ar/39Ar scheme have been aimed at reducing the errors on the absolute ages (usually ±1.5–0.5 m.y. with K/Ar), so that the temporal inter-relationships between the contributing lava piles (e.g., Steens, Grande Ronde Basalt) can be better understood, and the main pulses of lava effusion can be more precisely defi ned (e.g., Brueseke et al., 2007; Baksi, 2010; Jarboe et al., 2008, 2010; Barry et al., 2010). However, efforts at error reduction in ages of some of the Columbia River Basalt
Figure 2. Summary of the revised stra-tigraphy of the Columbia River Basalt Group, presented in Reidel et al. (this volume), showing the relationship of all the units presented here with radioiso-tope data.
1GSA Data Repository Item 2013234, Appendix DR 1—New 40Ar/39Ar data and Appendix DR2—Compilation of all available related K-Ar and 40Ar/39Ar data, is available at www.geosociety.org/pubs/ft2013.htm, or on request from [email protected] or Documents Secretary, GSA, P.O. Box 9140, Boul-der, CO 80301-9140, USA.
Group lavas have met with limited success (Barry et al., 2010), even though the results of that study underline the rapidity of emplacement of the Grande Ronde Basalt.
A REVIEW OF RADIOMETRIC AGE DATA FOR THE COLUMBIA RIVER BASALT
To present a comprehensive data set of all known radiomet-ric age dates for the Columbia River Basalt units, we have com-piled new (Appendix DR11; see also Camp et al., this volume) and published 40Ar/39Ar data, and older K-Ar data (Appendix DR2 [see footnote 1]). All 40Ar/39Ar dates have been standardized to the normalization value for Fish Canyon sanidine (Jourdan and Renne, 2007) in order to enable accurate comparisons. Both 40Ar/39Ar data and older K-Ar data have been recalculated to the K decay constant of Renne et al. (2010).
Eruption chronology of the Columbia River Basalt Group 49
Criteria for Selection of “Acceptable” Ages for Columbia River Basalt Units
Ages determined by either K-Ar or 40Ar/39Ar total fusion and incremental heating methods are susceptible to errors and large analytical uncertainties due to several factors, such as post-crystallization exchange of K and Ar with the local environment through low-temperature alteration; unsupported (“excess” or “inherited”) 40Ar that is trapped at the time of crystallization or through subsequent hydrothermal alteration; and reactor-induced 37Ar and 39Ar recoil from neutron irradiation. In order to evaluate all published and new age determinations for accuracy, and for the proposal of best estimates for the age and duration of each of the units within the Columbia River Basalt Group, we used the following selection criteria.
1. First, we assessed analytical reproducibility. There are a few instances where multiple ages have been determined for the same sample (e.g., PF7 from the Basalt of Sand Hollow, French-man Springs Member of the Wanapum Formation; see below), and the age has statistically good reproducibility. We view such reproducibility as strong evidence of a reliable age. Furthermore, we looked at individual sample analytical uncertainty (quoted as 1σ error in Tables 1–11), placing less signifi cance on analyses that have high analytical uncertainty.
2. Second, but of equal importance, we examined ages rela-tive to the stratigraphic position of the samples based on observed superposed sequences of lavas in exposed or cored sections.
3. Finally, we examined 40Ar/39Ar incremental heating experiments for evidence of excess 40Ar, and 37Ar and 39Ar recoil, sample alteration, and atmospheric argon (e.g., Koppers et al., 2000, and references therein). We avoided arbitrary “cutoff” val-ues as a means of discrimination for reasons partly discussed in Barry et al. (2012). All these factors may have variably caused a loss of precision (as demonstrated in the 1σ error data), but this procedure allows us to investigate potentially erroneous ages.
K-Ar ages can be evaluated using the fi rst two criteria only. In general, samples analyzed by 40Ar/39Ar incremental heating experiments produced high proportions of radiogenic 40Ar and analytical uncertainties (2σ) of <1%–5%. There is a weak inverse correlation between % K (as indicated by 37Ar/39Ar) and preci-sion, which refl ects variations in radiogenic 40Ar production. In addition to the previous criteria, we also considered fi eld rela-tions and paleomagnetic data when making our fi nal recommen-dations of currently preferred ages for individual units.
RECOMMENDATIONS FOR AGE RANGES OF COLUMBIA RIVER BASALT FORMATIONS
Steens Basalt
The Steens Basalt is the oldest lithostratigraphic unit of the Columbia River Basalt Group and the second largest unit, with an estimated volume of 31,800 km3 (Camp et al., this volume). Although partly covered by younger Tertiary volcanic rocks, it
is well exposed throughout southeastern Oregon, particularly along northerly trending fault scarps associated with Basin and Range extension that began in this region after ca. 12 Ma (Col-gan et al., 2004). The most complete section of Steens Basalt lies along the Steens Mountain escarpment, where an ~950 m section of the unit is exposed (Johnson et al., 1998) (Fig. 1). This thick sequence of lavas was originally defi ned as the “Steens Moun-tain Basalt” by Fuller (1930, 1931), but then redefi ned as “Steens Basalt” by Mankinen et al. (1985).
Paleomagnetic studies in the 1960s and 1970s described the lavas at Steens Mountain as a conformable lithostratigraphic unit with a paleomagnetic transition indicating a very short period of eruption, ranging from ~2000 to 50,000 yr (e.g., Baksi et al., 1967; Watkins, 1969; Gunn and Watkins, 1970). Other work-ers have redefi ned these lavas as a petrochemical type, where chemically similar Steens and “Steens-type” lavas appear to have erupted sporadically over several million years (Hart and Carl-son, 1985; Carlson and Hart, 1987; Brueseke et al., 2007). Camp et al. (this volume) discuss the rationale for defi ning “Steens Basalt” more succinctly, in part by restoring the stratigraphic designation to its original usage. Here, we follow the intent of Article 22 of the Stratigraphic Code of North America, which discourages the establishment of formal stratigraphic units that straddle known, identifi able regional disconformities (Anony-mous, 2005). We therefore retain the term “Steens Basalt” of Mankinen et al. (1985) but restrict its lithostratigraphic usage to the conformable sequence of lavas typifi ed in the Steens Moun-tain stratigraphic section. This criterion eliminates Ar-Ar ages for lavas lying above unconformities that are described as Steens Basalt elsewhere, including sample MB97-2 (15.17 ± 0.36 Ma) in Brueseke et al. (2007), and samples 00HS-6 and MB01-6A (15.97 ± 0.2 Ma and 14.35 ± 0.38 Ma, respectively) in Brueseke and Hart (2008).
Using chemical criteria, Camp et al. (this volume) subdi-vided the Steens Basalt into two informal members, the lower and upper Steens Basalt, with the former extending across the breadth of the Steens outcrop region and the latter being less extensive but thickest in the area of Steens Mountain. A detailed record of paleomagnetic data has also allowed workers to subdivide the Steens Basalt into three magnetostratigraphic units that are best exposed at Steens Mountain, where an ~160-m-thick middle sec-tion of transitional polarity (T) separates lower lavas of reverse polarity (R
0) from upper lavas of normal polarity (N
0) (Baksi et
al., 1967; Watkins, 1969; Gunn and Watkins, 1970; Mankinen et al., 1985; Jarboe et al., 2008, 2010).
The number of Ar-Ar ages for Steens Basalt (Tables 1 and 2; Appendix DR2) exceeds that of any other Columbia River Basalt Group unit. Despite this sizable analytical database, amassed from analyses made at different laboratories, the over-all range of acceptable ages is reasonably constrained between ca. 16.9 and ca. 16.4 Ma. (The older date of 17.29 ± 0.81 Ma for sample KL049 [Hooper et al., 2002] is imprecise, and its inclu-sion does not signifi cantly affect the mean or duration of Steens Basalt activity.) While several of the Steens Basalt lavas with
50 Barry et al.
TA
BLE
1. A
r-A
r D
AT
A F
OR
ST
EE
NS
BA
SA
LTS
For
mat
ion
Pal
eom
ag.
Sam
ple
ID
Typ
e of
m
ater
ial
%40
Ar*
37
Ar/
39A
r 40
Ar/
39A
r ag
e (p
ublis
hed)
(M
a)
Err
or
(1σ)
R
ef
Rec
alc.
ag
e (M
a)
Err
or
(1σ)
Ste
ens
Bas
alt
? F
ig. 1
.e
Grd
mas
s N
o in
fo
No
info
16
.06
0.01
1
16.3
9 0.
11
Ste
ens
Bas
alt
? F
ig. 1
.f G
rdm
ass
No
info
N
o in
fo
16.0
8 0.
02
1 16
.41
0.13
Ste
ens
Bas
alt
N
04C
P02
P
lag
sep
90.5
5 6.
16
16.7
2 0.
08
6 16
.78
0.08
Ste
ens
Bas
alt
N
03S
S02
P
lag
sep
62.0
1 20
.40
16.8
4 0.
20
5 16
.91
0.20
Ste
ens
Bas
alt
N
03S
S09
G-1
P
lag
sep
57.2
8 23
.50
17.1
4 0.
18
5 17
.20
0.18
Ste
ens
Bas
alt
N
03S
S09
G-2
P
lag
sep
56.5
5 23
.32
16.7
1 0.
19
5 16
.77
0.19
Ste
ens
Bas
alt
T
04C
P16
G
Pla
g se
p 49
.60
37.4
4 16
.74
0.36
6
16.8
1 0.
36
Ste
ens
Bas
alt
T
04P
J23
Pla
g se
p 72
.50
16.3
9 16
.53
0.12
6
16.5
9 0.
12
Ste
ens
Bas
alt
T
G-4
0 P
lag
sep
78.1
6 15
.54
16.6
7 0.
25
6 16
.74
0.25
Ste
ens
Bas
alt
T
G-4
1 P
lag
sep
62.6
1 19
.80
16.6
1 0.
28
6 16
.66
0.28
Ste
ens
Bas
alt
R
05C
P63
A
Pla
g se
p 43
.66
28.5
7 16
.46
0.47
6
16.5
3 0.
47
Ste
ens
Bas
alt
R
03P
M10
C
Pla
g se
p 16
.86
3.28
16
.80
0.24
5
16.8
6 0.
24
Ste
ens
Bas
alt
R
04P
J03A
S
anid
ine
54.3
3 30
.56
16.6
5 0.
17
6 16
.71
0.17
Ste
ens
Bas
alt
R
05S
B01
A
Pla
g se
p 39
.16
39.9
0 16
.17
0.24
6
16.2
3 0.
24
Ste
ens
Bas
alt
? M
B97
-32
Pla
g se
p 81
.91
19.1
4 16
.03
0.15
2
16.2
0 0.
16
Ste
ens
Bas
alt
? M
B97
-24
Grd
mas
s 53
.07
3.00
16
.06
0.18
2
16.2
3 0.
18
Ste
ens
Bas
alt
? M
B97
-25
Grd
mas
s 50
.40
12.5
7 16
.24
0.25
2
16.4
1 0.
25
Ste
ens
Bas
alt
? 86
-29
Grd
mas
s 56
.70
3.55
16
.31
0.10
2
16.4
8 0.
10
Ste
ens
Bas
alt
? M
B97
-87
Grd
mas
s 55
.04
4.47
16
.33
0.10
2
16.5
0 0.
10
Ste
ens
Bas
alt
? C
H82
-22B
G
rdm
ass
77.5
5 6.
64
16.5
5 0.
05
2 16
.72
0.05
Ste
ens
Bas
alt
? C
H82
-22G
G
rdm
ass
63.8
3 8.
27
16.5
9 0.
05
2 16
.76
0.05
Ste
ens
Bas
alt
? M
B97
-65
Grd
mas
s 61
.87
4.53
16
.40
0.09
2
16.5
7 0.
09
Ste
ens
Bas
alt
? M
B97
-47
Grd
mas
s 59
.57
5.32
16
.48
0.15
2
16.6
5 0.
15
Ste
ens
Bas
alt
? M
B97
-55
Grd
mas
s 61
.38
5.11
16
.58
0.09
2
16.7
5 0.
09
Ste
ens
Bas
alt
? M
B01
-12
Grd
mas
s 10
.53
13.1
0 16
.07
0.46
3
16.2
3 0.
46
Ste
ens
Bas
alt
? M
B01
-13
Pla
g se
p 72
.85
12.5
4 16
.45
0.17
3
16.6
1 0.
17
Ste
ens
Bas
alt
? M
B01
-24
Grd
mas
s 11
.36
12.0
7 16
.95
0.65
3
17.1
4 0.
66
Ste
ens
Bas
alt
? O
OH
S-X
N
o in
fo
No
info
No
info
16
.73
0.02
3
16.9
0 0.
02
Ste
ens
Bas
alt
? JC
02-P
F25
G
rdm
ass
48.7
6 8.
70
16.3
3 0.
48
4 16
.73
0.49
Ste
ens
Bas
alt
? JC
02-P
F23
G
rdm
ass
59.8
5 3.
44
16.0
7 0.
15
4 16
.47
0.15
Ste
ens
Bas
alt
? JC
02-P
F24
G
rdm
ass
46.3
5 6.
59
17.0
1 0.
90
4 17
.41
0.93
Ste
ens
Bas
alt
R
JS7-
5 P
lag
sep
44.9
1 36
.03
16.8
4 0.
22
7 16
.91
0.21
Ste
ens
Bas
alt
R
JS7-
1 P
lag
sep
43.9
0 27
.04
16.8
2 0.
11
7 16
.88
0.11
Ste
ens
Bas
alt
R
MF
94-6
3 P
lag
sep
40.1
2 26
.91
16.5
4 0.
14
7 16
.60
0.14
Ste
ens
Bas
alt
? M
D06
-142
P
lag
sep
55.6
2 25
.96
16.7
4 0.
11
7 16
.80
0.10
Ste
ens
Bas
alt
? C
R97
-1
Pla
g se
p 71
.04
13.7
3 16
.41
0.10
7
16.4
7 0.
10
(Con
tinue
d)
Eruption chronology of the Columbia River Basalt Group 51T
AB
LE 1
. Ar-
Ar
DA
TA
FO
R S
TE
EN
S B
AS
ALT
S (
Con
tinue
d)
For
mat
ion
Pal
eom
ag.
Sam
ple
ID
Typ
e of
m
ater
ial
%40
Ar*
37
Ar/
39A
r 40
Ar/
39A
r ag
e (p
ublis
hed)
(M
a)
Err
or
(1σ)
R
ef
Rec
alc.
ag
e (M
a)
Err
or
(1σ)
Ste
ens
Bas
alt
? C
R-3
58
Grd
mas
s 53
.22
6.78
16
.40
0.26
7
16.4
6 0.
25
Ste
ens
Bas
alt
? C
R-4
62
Grd
mas
s 8.
66
8.00
16
.51
0.41
7
16.5
7 0.
41
Ste
ens
Bas
alt
? K
CS
-05-
20
Pla
g se
p N
o in
fo
No
info
16
.22
0.15
8
16.4
0 0.
15
Ste
ens
Bas
alt
? C
H82
-22B
P
lag
sep
? ?
16.5
8 0.
05
9 16
.86
0.05
Ste
ens
Bas
alt
? C
H82
-22G
P
lag
sep
? ?
16.5
9 0.
02
9 16
.87
0.03
Ste
ens
Bas
alt
? H
85-1
0A
No
info
N
o in
fo
No
info
16
.30
0.17
10
16
.44
0.17
Ste
ens
Bas
alt
N
NL1
1-6
WR
Who
le-r
ock
No
info
N
o in
fo
16.5
0 0.
30
11
16.6
7 0.
30
Ste
ens
Bas
alt
N
SM
200
WR
Who
le-r
ock
No
info
N
o in
fo
16.2
0 0.
30
11
16.3
7 0.
30
Ste
ens
Bas
alt
N
SM
200
WR
Who
le-r
ock
No
info
N
o in
fo
16.9
0 0.
70
11
17.0
8 0.
71
Ste
ens
Bas
alt
R
SM
263
WR
Who
le-r
ock
No
info
N
o in
fo
16.3
0 0.
50
11
16.4
7 0.
51
Ste
ens
Bas
alt
R
SM
263
WR
Who
le-r
ock
No
info
N
o in
fo
15.8
0 0.
20
11
15.9
6 0.
20
Ste
ens
Bas
alt
R
SM
263
Pla
gP
lag
sep
No
info
N
o in
fo
16.6
0 0.
40
11
16.7
7 0.
40
Ste
ens
Bas
alt
tr
SM
421
WR
Who
le-r
ock
No
info
N
o in
fo
16.5
0 0.
60
11
16.6
7 0.
61
Ste
ens
Bas
alt
tr
SM
421
WR
Who
le-r
ock
No
info
N
o in
fo
17.1
0 0.
70
11
17.2
8 0.
71
Ste
ens
Bas
alt
tr
SM
441
WR
Who
le-r
ock
No
info
N
o in
fo
16.2
0 1.
70
11
16.3
7 1.
72
Ste
ens
Bas
alt
tr
SM
441
Pla
gP
lag
sep
No
info
N
o in
fo
16.4
0 1.
50
11
16.5
7 1.
52
Ste
ens
Bas
alt
tr
NL5
0 W
RW
hole
-roc
k N
o in
fo
No
info
16
.50
0.40
11
16
.67
0.40
Ste
ens
Bas
alt
tr
SM
129
WR
Who
le-r
ock
No
info
N
o in
fo
15.8
0 0.
40
11
15.9
6 0.
40
Ste
ens
Bas
alt
tr
SM
129
WR
Who
le-r
ock
No
info
N
o in
fo
15.7
0 0.
70
11
15.8
6 0.
71
Ste
ens
Bas
alt
tr
NL5
3-5
WR
Who
le-r
ock
No
info
N
o in
fo
16.1
0 0.
30
11
16.2
7 0.
30
Ste
ens
Bas
alt
tr
NL5
3-5
WR
Who
le-r
ock
No
info
N
o in
fo
16.4
0 0.
70
11
16.5
7 0.
71
Ste
ens
Bas
alt
tr
NL5
3 P
lag
Pla
g se
p N
o in
fo
No
info
16
.90
0.40
11
17
.08
0.40
Ste
ens
Bas
alt
tr
SM
166
WR
Who
le-r
ock
No
info
N
o in
fo
16.1
0 0.
30
11
16.2
7 0.
30
Ste
ens
Bas
alt
tr
SM
166
WR
Who
le-r
ock
No
info
N
o in
fo
16.1
0 0.
40
11
16.2
7 0.
40
Ste
ens
Bas
alt
tr
SM
224
WR
Who
le-r
ock
No
info
N
o in
fo
16.4
0 0.
30
11
16.5
7 0.
30
Ste
ens
Bas
alt
tr
SM
224
WR
Who
le-r
ock
No
info
N
o in
fo
16.3
0 0.
70
11
16.4
7 0.
71
Ste
ens
Bas
alt
tr
SM
224
Pla
gP
lag
sep
No
info
N
o in
fo
15.2
0 0.
70
11
15.3
6 0.
71
Ste
ens
Bas
alt
tr
NL6
9 W
RW
hole
-roc
k N
o in
fo
No
info
16
.90
0.90
11
17
.08
0.91
Bas
. of M
alhe
ur G
orge
?
KL0
49
Grd
mas
s N
o in
fo
No
info
17
.00
0.80
12
17
.29
0.81
Bas
. of M
alhe
ur G
orge
?
KL0
33
No
info
N
o in
fo
No
info
15
.80
2.80
12
16
.13
2.81
N
ote:
%40
Ar*
= 1
00 ×
[40A
r Tot
al –
(36
Ar T
otal ×
295
.5)]
/40A
r Tot
al. P
aleo
mag
netic
info
rmat
ion
(tak
en o
r in
ferr
ed fr
om s
ourc
e pa
pers
): N
—no
rmal
pol
arity
; R—
reve
rse
pola
rity;
tr—
tran
sitio
nal p
olar
ity. D
escr
iptio
n of
type
of m
ate
rial:
Grd
mas
s—gr
ound
mas
s (a
lso
impl
ies
that
it is
the
grou
ndm
ass
mat
eria
l dev
oid
of a
ny la
rge
phen
ocry
sts)
; Pla
g se
p—pl
agio
clas
e se
para
te;
San
idin
e—sa
nidi
ne s
epar
ate;
Who
le-r
ock
(tak
en fr
om th
e te
rmin
olog
y pr
esen
ted
in th
e so
urce
pap
ers)
impl
ies
that
ther
e ha
s be
en n
o se
para
tion
of p
heno
crys
t mat
eria
l. R
ecal
c. a
ge—
all d
ata
has
been
rec
alcu
late
d w
ith a
dec
ay c
onst
ant o
f Ren
ne e
t al.
(201
0) a
nd
stan
dard
ized
to th
e no
rmal
izat
ion
valu
e fo
r F
ish
Can
yon
sani
dine
(Jo
urda
n an
d R
enne
, 200
7). D
ata
sour
ces:
1—
Bak
si a
nd F
arra
r (1
990)
; 2—
Bru
esek
e et
al.
(200
7); 3
—B
rues
eke
and
Har
t (20
08);
4—
Col
gan
et a
l. (2
006)
; 5—
Jarb
oe e
t al.
(200
8); 6
—Ja
rboe
et a
l. (2
010)
; 7—
Cam
p et
al.
(thi
s vo
lum
e); 8
—S
carb
erry
et
al. (
2009
); 9
—S
wis
her
et a
l. (1
990)
; 10—
Sho
emak
er a
nd H
art (
2002
); 1
1—B
aksi
et a
l. (1
991)
; 12—
Hoo
per
et a
l. (2
002)
. Num
bers
in g
ray
italic
are
thos
e ag
es,
plus
err
or, t
hat f
all o
utsi
de c
riter
ia o
f dat
a ac
cept
abili
ty.
52 Barry et al.
ages younger than 16.5 Ma are analytically acceptable, others underlie either well-dated sanidine-bearing tuffs or other Steens Basalt lavas with ages ≥16.5 Ma (Henry et al., 2006; Jarboe et al., 2008, 2010).
A precise estimate of the age and duration of Steens vol-canism comes from integrating the large number of acceptable ages with paleomagnetic data. Jarboe et al. (2008, 2010) used such combined data to correlate the age of the Steens reversal to the 16.72 Ma transition separating the C5Cr and C5C.3n chrons on the geomagnetic polarity time scale of Gradstein et al. (2004) (see below). The acceptable ages for Steens Basalt can be fur-ther constrained by the consistency of the Steens paleomagnetic and chemical stratigraphy across the Steens outcrop area (Camp et al., this volume), which leads us to suggest that the most accurate age range for the entire Steens succession is between ca. 16.9 and 16.6 Ma.
Imnaha Basalt
The stratigraphic relationship between the Imnaha and Steens Basalts is best revealed in the Malheur Gorge area of east-central Oregon (Fig. 1). Here, the Basalt of Malheur Gorge was subdivided by Hooper et al. (2002) into three stratigraphic
and compositionally distinct tholeiitic units, with the follow-ing weighted mean 40Ar/39Ar ages: the lower Pole Creek basalt (16.9 ± 0.8 Ma), upper Pole Creek basalt (16.5 ± 0.3 Ma), and Birch Creek basalt (15.7 ± 0.1 Ma). Lying above this succes-sion, there are the ca. 15.3 Ma Hunter Creek basalt and Din-ner Creek tuff. Hooper et al. (2002) described the lower Pole Creek basalt as being chemically equivalent to lower Steens Basalt, the upper Pole Creek basalt as chemically equivalent to Imnaha Basalt, and the Birch Creek and Hunter Creek basalts as chemically equivalent to Grande Ronde Basalt, in correct strati-graphic order (Fig. 3).
The upper Pole Creek basalt (Imnaha) appears to lie con-formably above lower Pole Creek basalt (lower Steens Basalt) in the Malheur Gorge region. Thus, Imnaha Basalt is inferred to lie at the same stratigraphic level as upper Steens Basalt. Although lava fl ows from these units may well be interbedded south of the Malheur Gorge, the outcrops are too poor to verify this relationship.
The timing of Imnaha volcanism is diffi cult to constrain pre-cisely. Many of the available age determinations have insuffi cient data reported to make a full assessment of reliability (Tables 3 and 4). The 40Ar/39Ar ages for Imnaha Basalt range from 17.82 to 15.35 Ma; we exclude sample ages for Columbia River Basalt
TABLE 2. K-Ar DATA FOR STEENS BASALTS
Formation Sample ID K (wt%)
40*Ar/total 40Ar
K-Ar age (published)
(Ma)
Error (1σ)
Ref Recalc. age (Ma)
Error (1σ)
Steens Basalt 11-3 1.53 Av. 21.50 Av. 15.2 Av. 0.3 1 15.7 0.3
Steens Basalt 11-4 1.51 Av. 35.85 Av. 15.1 Av. 0.3 1 15.6 0.3
Steens Basalt 11-7 1.50 15.60 15.1 0.4 1 15.6 0.4
Steens Basalt 17-4(i) 0.84 Av. 45.65 Av. 15.1 Av. 0.4 1 15.6 0.4
Steens Basalt 17-4(ii) 0.83 41.50 14.9 0.3 1 15.4 0.3
Steens Basalt 17-6 0.84 47.10 14.8 0.4 1 15.3 0.4
Steens Basalt 51-1 1.31 60.60 14.8 0.5 1 15.3 0.5
Steens Basalt 51-2 1.34 63.70 15.4 0.4 1 15.9 0.4
Steens Basalt 51-5 1.27 Av. 46.00 Av. 15.3 Av. 0.4 1 15.8 0.4
Steens Basalt 51-6 1.27 Av. 55.30 Av. 14.9 Av. 1.2 1 15.4 1.2
Steens Basalt 61-1 0.99 Av. 94.70 Av. 15.0 Av. 1.7 1 15.5 1.7
Steens Basalt 61-6 0.87 Av. 61.15 Av. 15.2 Av. 0.4 1 15.7 0.4
Steens Basalt 61-7 0.89 Av. 57.90 Av. 15.0 Av. 0.4 1 15.5 0.4
Steens Basalt 68-1 0.89 Av. 84.45 Av. 15.0 Av. 0.8 1 15.5 0.8
Steens Basalt 68-4 1.00 90.70 15.2 0.9 1 15.7 0.9
Steens Basalt 68-5 0.92 93.60 15.3 1.4 1 15.8 1.4
Steens Basalt 68-6 1.00 70.60 15.5 0.4 1 16.0 0.4
Steens Basalt 70-3 0.95 74.50 14.7 0.5 1 15.2 0.5
Steens Basalt 70-5 0.83 65.50 15.0 0.4 1 15.5 0.4
Steens Basalt RCG-185-67 0.26 No info 15.3 1.0 2 15.8 1.0
Steens Basalt KA1251 0.37 No info 14.7 – 3 15.2 –
Steens Basalt KA1165 1.64 No info 14.5 – 3 15.0 –
Note: Recalculated ages make the assumption that publications up to and including 1977 used the decay constant of Dalrymple and Lanphere (1969), and that publications after that time used the decay constant of Steiger and Jäger (1977). Data from pre-1969 publications were similarly recalculated using Dalrymple and Lanphere (1969) values, as they based their calculations on decay constant information presented in Aldrich and Wetherill (1958). All data have been recalculated with a decay constant of Renne et al. (2010). Data sources: 1—Baksi et al. (1967); 2—Fiebelkorn et al. (1982), quoting Greene et al. (1972); 3—Fiebelkorn et al. (1982), quoting Evernden and James (1964).
Eruption chronology of the Columbia River Basalt Group 53
DB-25 (17.82 Ma; Duncan, 1983), sample identifi ed as top of N
0 unit, Imnaha Basalt of Fig. 1a (17.61 Ma; Baksi and Far-
rar, 1990), MLC-2 (15.35 Ma; Barry et al., 2010), and KL164 (17.07 Ma; Hooper et al., 2002) based on our understanding of Imnaha Basalt and its inferred stratigraphic positions (Fig. 4).
The inferred conformable stratigraphic relationship between the lower Steens and Imnaha successions suggests that lower-most Imnaha Basalt is ca. 16.7 Ma in age. Discarding the ages that appear to be out of stratigraphic order, and the imprecise ages for KL319 and KL248 (Hooper et al., 2002), we fi nd that the remaining data appear to be divided into an older group in the south and a younger group in the north. For example, an age of 16.92 ± 0.21 (Jarboe et al., 2010) was obtained from a lava at Squaw Butte in one of the southernmost outcrops of Imnaha Basalt in Idaho, and an age of 15.95 ± 0.31 Ma (Barry et al., 2010) was obtained from a sample collected at the confl uence of the Grande Ronde and Snake Rivers, Washington, directly below the oldest Grande Ronde Basalt lavas (Table 3). Such a geographic progression is consistent with an overall northward migration of Imnaha dike intrusion and volcanism with time (see also Camp and Ross, 2004).
The available 40Ar/39Ar ages in the Malheur Gorge and the apparent stratigraphic equivalency of the Imnaha and upper Steens lavas in that region (Fig. 3) suggest that the oldest Imnaha lavas erupted at ca. 16.7 Ma. The combined data lead us to conclude that the duration of Imnaha Basalt volcanism was ~700,000 yr, from ca. 16.7 Ma to 16 Ma. A ca. 16 Ma age for the last Imnaha fl ows would place the lavas in the C5Cn.1n (normal polarity) paleomagnetic chron (Fig. 4). Although the Imnaha lavas in northeastern Oregon and southeastern Washington appear to have erupted during a single geomagnetic chron of normal polarity, the older ages for the more southern outcrops suggest that the entire 700,000 yr duration may correspond with as many as fi ve geomagnetic chrons on the geomagnetic time scale of Gradstein
Figure 3. A north-south cross section from Steens Mountain in the south to the Columbia River Plateau in the north, summarizing the stratigraphic relationship of the Steens and Imnaha Basalts with con-straints from the Malheur Gorge area. The diagram shows how Im-naha Basalt is thought to correlate with upper Steens Basalt, and that lower Steens Basalt would be older than Imnaha Basalt, and Grande Ronde Basalt would be younger than upper Steens Basalt.
et al. (2004) (see Fig. 4). In this case, two short reverse polarity chrons (C5Cn.2r and C5Cn.1r) have yet to be discovered in the Imnaha Basalt lavas.
Grande Ronde Basalt and Picture Gorge Basalt
Grande Ronde Basalt lavas are the products of the greatest volume of lava production in the Columbia River Basalt Group (Tolan et al., 1989; Reidel et al., 1989, this volume). The Imnaha and Grande Ronde Basalt lavas are not known to be interbedded, but in the absence of any evidence for a signifi cant hiatus between the Imnaha Basalt and the Grande Ronde Basalt, it seems likely that Grande Ronde Basalt volcanism followed soon after the last Imnaha lavas.
The Grande Ronde Basalt is recognized to span at least four paleomagnetic zones and, on this basis, has been strati-graphically subdivided into R
1, N
1, R
2, and N
2 units (where
R indicates reversed and N indicates normal; Swanson et al., 1979; Reidel et al., 1989, this volume). The earliest lavas have a transitional paleomagnetic signature (Hooper et al., 1979), indicating that the fi rst Grande Ronde Basalt lavas were erupted during a polarity transition.
Published radiometric ages for Grande Ronde Basalt lavas are presented in Tables 5 and 6. These data indicate that Grande Ronde Basalt volcanism began ca. 16 Ma. Although many samples have been analyzed from the R
1 succession, several
analyses produce ages that appear to be stratigraphically out of order, either too old (KL-92-231 and KL-91-93; Lees, 1994) or too young (KL034; Hooper et al., 2002), and they are therefore omitted from our estimates of unit ages and durations. Sample CRB05-030 (Barry et al., 2010), which produced an age of 15.59 ± 0.10 Ma, is from a dike of the Teepee Butte Member, Basalt of Joseph Creek. Field exposures indicate that the dike intrudes older R
1 lavas of Buckhorn Springs (Reidel and Tolan,
1992). From this evidence, correlation with the Gradstein et al. (2004) polarity time scale, and the lack of evidence for clear stratigraphic relation between Grande Ronde Basalt and Imnaha units, we conclude that the onset of Grande Ronde Basalt activity occurred before 15.6 Ma at ca. 16 Ma. On the basis of the Ar dat-ing evidence from Grande Ronde Basalts alone, we cannot rule out that volcanism may have started as early as 16.3 Ma. This appears to be at odds, however, with the known fi eld relations and dating evidence for the Imnaha Basalts. Assuming the younger date, the R
1 section of Grande Ronde Basalt would correlate with
the long C5Br chron. The older onset would match the R1 sec-
tion with either of the short C5Cn.2r or C5Cn.1r chrons, and this would strongly support the likelihood that the base of the Grande Ronde Basalt could be diachronous, resulting in slightly different ages for Grande Ronde Basalt lavas sitting on Imnaha Basalt.
The cessation of Grande Ronde Basalt volcanism is equally diffi cult to date precisely. Ages for the N
2 Sentinel Bluffs Mem-
ber, Basalt of Museum, range from 15.27 Ma to 15.89 ± 0.1 Ma (Duncan, 1982; Long and Duncan, 1983, respectively). Although these are both from lavas at the top of the pile, there may still be
54 Barry et al.T
AB
LE 3
. Ar-
Ar
DA
TA
FO
R IM
NA
HA
BA
SA
LTS
For
mat
ion
Mem
ber
Pal
eom
ag.
sign
al
Sam
ple
ID
Typ
e of
m
ater
ial
%40
Ar*
37
Ar/
39A
r 40
Ar/
39A
r ag
e (p
ublis
hed)
(M
a)
Err
or
(1σ)
R
ef
Rec
alc.
ag
e (M
a)
Err
or
(1σ)
Imna
ha B
asal
t
? C
RB
DB
-25
Grd
mas
s 84
.12
0.61
17
.50
0.30
1
17.8
2 0.
31
Imna
ha B
asal
t
? F
ig.1
.a
Grd
mas
s N
o in
fo
No
info
17
.26
0.16
2
17.6
1 0.
17
Imna
ha B
asal
t
? N
o in
fo
Grd
mas
s N
o in
fo
No
info
15
.40
0.20
3
15.6
5 0.
20
Imna
ha B
asal
t
? N
o in
fo
Grd
mas
s N
o in
fo
No
info
15
.50
0.30
3
15.7
5 0.
31
Imna
ha B
asal
t
? C
JC-1
G
rdm
ass
79.5
0 0.
99
16.0
8 0.
34
4 16
.15
0.35
Imna
ha B
asal
t
? C
JC-1
(rpt
) G
rdm
ass
65.7
1 5.
68
16.0
6 0.
15
4 16
.12
0.15
Imna
ha B
asal
t
? C
JC-3
(1)
Grd
mas
s 52
.19
0.23
15
.89
0.30
4
15.9
5 0.
31
Imna
ha B
asal
t
? C
JC-5
G
rdm
ass
66.1
7 6.
08
16.1
1 0.
27
4 16
.17
0.27
Imna
ha B
asal
t
? M
LC-2
G
rdm
ass
71.0
9 1.
69
15.2
9 0.
11
4 15
.35
0.11
Imna
ha B
asal
t
? M
LC-2
(rpt
) G
rdm
ass
73.8
8 3.
74
15.7
0 0.
25
4 15
.76
0.25
Imna
ha B
asal
t
? 04
WB
01A
P
lag
sep
52.0
2 37
.53
16.8
5 0.
21
5 16
.92
0.21
B. o
f Mal
heur
Gor
ge
U. P
ole
Cre
ek
? K
L319
G
rdm
ass
No
info
N
o in
fo
15.2
0 2.
80
3 15
.40
2.85
B. o
f Mal
heur
Gor
ge
U. P
ole
Cre
ek
? K
L001
G
rdm
ass
No
info
N
o in
fo
15.5
0 0.
60
3 15
.76
0.61
B. o
f Mal
heur
Gor
ge
U. P
ole
Cre
ek
? K
L248
G
rdm
ass
No
info
N
o in
fo
16.6
0 0.
80
3 16
.90
0.82
B. o
f Mal
heur
Gor
ge
U. P
ole
Cre
ek
? K
L164
G
rdm
ass
No
info
N
o in
fo
16.8
0 0.
30
3 17
.07
0.31
B. o
f Mal
heur
Gor
ge
Pol
e C
reek
N
04
PC
03
Pla
g se
p 68
.03
20.1
3 16
.45
0.11
5
16.5
2 0.
11
N
ote :
%40
Ar*
= 1
00 ×
[40A
r Tot
al –
(36
Ar T
otal ×
295
.5)]
/40A
r Tot
al. D
escr
iptio
n of
type
of m
ater
ial:
Grd
mas
s—gr
ound
mas
s (a
lso
impl
ies
that
it is
the
grou
ndm
ass
mat
eria
l dev
oid
of
any
larg
e ph
enoc
ryst
s); P
lag
sep—
plag
iocl
ase
sepa
rate
. Rec
alc.
age
—al
l dat
a ha
ve b
een
reca
lcul
ated
with
a d
ecay
con
stan
t of R
enne
et a
l. (2
010)
and
sta
ndar
dize
d to
the
norm
aliz
atio
n va
lue
for
Fis
h C
anyo
n sa
nidi
ne (
Jour
dan
and
Ren
ne, 2
007)
. Dat
a so
urce
s: 1
—D
unca
n (1
983)
; 2—
Bak
si a
nd F
arra
r (1
990
), in
clud
ed in
Lon
g an
d D
unca
n (1
983)
; 3—
Hoo
per
et a
l. (2
002)
; 4—
Bar
ry e
t al.
(201
0); 5
—Ja
rboe
et a
l. (2
010)
. Num
bers
in g
ray
italic
s ar
e th
ose
ages
, plu
s er
ror,
that
fall
outs
ide
crite
ria o
f dat
a ac
cept
abili
ty.
TA
BLE
4. K
-Ar
DA
TA
FO
R IM
NA
HA
BA
SA
LTS
For
mat
ion
Sam
ple
ID
K (
wt%
) 40
*Ar/
tota
l 40
Ar
K-A
r ag
e (p
ublis
hed)
(M
a)
Err
or
(1σ)
R
ef
Rec
alc.
age
(M
a)
Err
or
(1σ)
Imna
ha B
asal
t D
B-1
2 0.
70
0.29
16
.8
0.9
1 16
.9
0.9
Imna
ha B
asal
t D
B-1
5 0.
81
0.23
16
.5
1.1
1 16
.6
1.1
Imna
ha B
asal
t D
B-1
9 0.
83
0.56
17
.4
0.3
1 17
.5
0.3
Imna
ha B
asal
t D
B-2
3 0.
75
0.37
17
.0
0.2
1 17
.1
0.2
Imna
ha B
asal
t I-
74
1.74
N
o in
fo
17.3
0.
5 2
17.4
0.
5
Imna
ha B
asal
t D
B-6
0.
74
No
info
16
.0
1.0
2 16
.1
1.0
Imna
ha B
asal
t D
B-7
0.
69
No
info
13
.9
2.5
2 14
.0
2.5
Imna
ha B
asal
t D
B-2
0 0.
97
No
info
12
.6
1.5
2 12
.7
1.5
Imna
ha B
asal
t D
B-2
0.
47
No
info
5.
3 4.
5 2
5.4
4.5
N
ote:
Rec
alcu
late
d ag
es m
ake
the
assu
mpt
ion
that
pub
licat
ions
afte
r 19
77 u
sed
the
deca
y co
nsta
nt o
f Ste
iger
and
Jäg
er (
1977
). A
ll d
ata
have
bee
n re
calc
ulat
ed w
ith a
dec
ay c
onst
ant o
f Ren
ne e
t al.
(201
0). D
ata
sour
ces:
1—
McK
ee e
t al.
(198
1); 2
—F
iebe
lkor
n et
al.
(198
2),
quot
ing
D.A
. Sw
anso
n an
d E
.H. M
cKee
(19
82, p
erso
nal c
omm
un.)
.
Eruption chronology of the Columbia River Basalt Group 55
Figu
re 4
. A p
lot o
f av
aila
ble
40A
r/39
Ar
data
for
the
Col
umbi
a R
iver
Bas
alt G
roup
(ex
clud
ing
Sadd
le M
ount
ains
Bas
alt)
vs.
geo
mag
netic
pol
arity
tim
e sc
ale.
All
40A
r/39
Ar
erro
rs a
re 1
σ. S
ymbo
ls in
bla
ck c
orre
spon
d to
dat
a in
the
tabl
es th
at fu
lfi ll
our a
ccep
tabi
lity
crite
ria,
whe
reas
thos
e th
at fa
ll sh
ort o
f our
cri
teri
a ar
e sh
own
with
whi
te s
ym-
bols
. Dat
a so
urce
s: A
—B
aksi
and
Far
rar (
1990
); B
—B
rues
eke
et a
l. (2
007)
; C—
Bru
esek
e an
d H
art (
2008
); D
—C
olga
n et
al.
(200
6); E
—Ja
rboe
et a
l. (2
008)
; F—
Jarb
oe
et a
l. (2
010)
; G—
Cam
p et
al.
(thi
s vo
lum
e); H
—Sc
arbe
rry
et a
l. (2
009)
; I—
Swis
her e
t al.
(199
0); J
—Sh
oem
aker
and
Har
t (20
02);
K—
Hoo
per e
t al.
(200
2); L
—D
unca
n (1
983)
; M—
Bar
ry e
t al.
(201
0); N
—L
ees
(199
4); O
—D
unca
n (1
982)
; P—
Lon
g an
d D
unca
n (1
983)
; Q—
Bak
si e
t al.
(199
1); Z
—ne
w d
ata,
this
con
trib
utio
n. G
eom
ag-
netic
tim
e sc
ale
is f
rom
Gra
dste
in e
t al.
(200
4). T
he d
iagr
am d
emon
stra
tes
how
dif
fi cul
t it i
s to
inte
rpre
t arg
on a
ges
for
a la
rge
igne
ous
prov
ince
, eve
n w
hen
ther
e is
as
muc
h da
ta a
s av
aila
ble
for
the
Col
umbi
a R
iver
Bas
alt G
roup
. Sha
ded
area
s sh
ow o
ur r
ecom
men
ded
age
rang
es f
or th
e m
ajor
for
mat
ions
of
the
Col
umbi
a R
iver
Bas
alt
Gro
up; s
ome
confi
den
ce c
an b
e gi
ven
to a
ge o
f th
e ba
se o
f un
its, b
ut th
e ag
es o
f th
e to
ps o
f un
its a
re le
ss c
erta
in.
56 Barry et al.TA
BLE
5. A
r-A
r D
ATA
FO
R G
RA
ND
E R
ON
DE
BA
SA
LTS
Mem
ber
Uni
tP
aleo
mag
. si
gnal
Sam
ple
IDTy
pe o
f m
ater
ial
%40
Ar*
37A
r/39
Ar
40A
r/39
Ar
age
(pub
lishe
d(M
a)E
rror
(1σ)
Ref
Rec
alc.
ag
e (M
a)E
rror
(1σ)
(Uni
ts s
ittin
g on
R
hyol
ite o
f Cot
tonw
ood
Mtn
?K
L046
Grd
mas
sN
o in
foN
o in
fo15
.50
0.70
115
.76
0.72
Gra
nd R
onde
Bas
alt)
Rhy
olite
of C
otto
nwoo
d M
tn?
Kl0
46G
rdm
ass
No
info
No
info
15.7
00.
201
15.9
60.
21
Rhy
olite
of C
otto
nwoo
d M
tn?
KL2
30G
rdm
ass
42.5
8†0.
90†
14.6
01.
001
14.8
41.
02
Din
ner
Crk
tuff
?K
L246
Grd
mas
s89
.33†
0.73
†15
.10
2.00
115
.28
2.09
Din
ner
Crk
tuff
?K
L206
Grd
mas
s95
.64†
0.04
†15
.40
0.60
115
.66
0.61
Din
ner
Crk
tuff
?D
C27
0G
rdm
ass
No
info
No
info
15.3
00.
401
15.5
50.
10
Sen
tinel
Blu
ffsM
cCoy
Can
yon
N2
DC
-12-
3202
Grd
mas
s49
.90
0.87
15.1
00.
302
15.2
80.
30
Sen
tinel
Blu
ffsN
o in
foN
2D
C-1
2-22
68G
rdm
ass
36.7
71.
0215
.60
0.20
215
.86
0.20
Sen
tinel
Blu
ffsM
useu
mN
2W
H1a
-1G
rdm
ass
80.8
52.
5915
.48
0.11
415
.54
0.11
Sen
tinel
Blu
ffsM
useu
mN
2W
H1b
-1G
rdm
asssv
86.8
10.
5115
.71
0.13
415
.77
0.13
Sen
tinel
Blu
ffsM
useu
mN
2W
H1b
-2G
rdm
assa-
sv94
.61
3.40
15.5
50.
164
15.6
10.
16
Sen
tinel
Blu
ffsM
useu
mN
2C
RB
05-1
06G
rdm
assa
43.7
43.
0515
.94
0.10
416
.00
0.10
Ort
ley
Flo
w 2
abo
ve N
2-R
2N
2D
C-1
2-39
26G
rdm
ass
65.1
30.
4915
.20
0.30
215
.38
0.31
Win
ter W
ater
Um
tanu
mN
2D
C-1
2-34
34G
rdm
ass
46.9
61.
0316
.00
0.20
316
.20
0.21
Win
ter W
ater
Um
tanu
mN
2D
C-1
2-33
62G
rdm
ass
28.9
40.
1916
.00
0.20
216
.20
0.21
Gro
use
Cre
ekU
pper
mos
t R2
R2
DC
-12-
2990
Grd
mas
s51
.29
0.70
15.6
00.
302
15.8
00.
30
Wap
shill
a R
idge
Wap
shill
a R
idge
R2
CR
B05
-033
Grd
mas
s92
.60
1.08
15.4
60.
114
15.5
20.
12
Wap
shill
a R
idge
Wap
shill
a R
idge
R2
Fig
.1.d
Grd
mas
sN
o in
foN
o in
fo15
.70
0.14
516
.02
0.15
From
Mal
heur
Gor
ge
B. o
f Hun
ter
Crk
R2
No
info
No
info
No
info
No
info
15.3
00.
101
15.5
50.
10
From
Mal
heur
Gor
ge
B. o
f Hun
ter
Crk
R2
HO
R09
Grd
mas
s50
.24†
1.67
†15
.80
0.60
§1
16.0
50.
61
From
Mal
heur
Gor
ge
B. o
f Hun
ter
Crk
R2
KL-
91-1
02P
lag
sep
64.2
5†1.
47†
16.5
01.
206
16.8
11.
22
From
Mal
heur
Gor
ge
B. o
f Hun
ter
Crk
R2
KL-
92-2
69G
rdm
ass
62.7
3†1.
17†
15.0
00.
736
15.2
80.
74
From
Mal
heur
Gor
ge
B. o
f Hun
ter
Crk
R2
KL-
92-2
78G
rdm
ass
75.8
7†2.
53†
15.9
00.
266
16.2
00.
26
Dow
ny G
ulch
Dow
ny G
ulch
N1
Fig
.1.c
Grd
mas
sN
o in
foN
o in
fo15
.94
0.10
516
.26
0.11
Teep
ee B
utte
B. o
f Jos
eph
Crk
R1
CR
B05
-030
Grd
mas
s93
.33
1.61
15.5
30.
104
15.5
90.
10
Buc
khor
n S
prin
gsN
o in
foR
1C
JC-7
Grd
mas
s45
.34
4.20
16.2
50.
144
16.3
10.
14
Buc
khor
n S
prin
gsN
o in
foR
1F
ig. 1
bG
rdm
ass
No
info
No
info
16.0
30.
115
16.3
60.
12
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L034
Grd
mas
s64
.88†
0.76
†14
.40
0.40
114
.64
0.41
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L-91
-93
Grd
mas
s73
.04†
1.24
†17
.00
0.53
617
.32
0.54
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L220
Grd
mas
s45
.65†
1.69
†15
.10
0.30
115
.35
0.30
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L-92
-225
Grd
mas
s79
.47†
0.87
†16
.00
0.39
616
.30
0.40
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L-92
-231
Grd
mas
s58
.64†
1.33
†16
.90
0.67
617
.21
0.68
B. o
f Mal
heur
Gor
geB
irch
Cre
ekR
1K
L278
Grd
mas
s75
.87†
2.53
†15
.90
0.10
116
.20
0.10
Not
e: %
40A
r* =
100
× [40
Ar To
tal –
(36
Ar To
tal ×
295
.5)]
/40A
r Tota
l. D
escr
iptio
n of
type
of m
ater
ial:
Grd
mas
s—gr
ound
mas
s (a
lso
impl
ies
that
it is
the
grou
ndm
ass
mat
eria
l dev
oid
of a
ny la
rge
phen
ocry
sts)
; Pla
g se
p—pl
agio
clas
e se
para
te; G
rdm
asssv
—gr
ound
mas
s m
ater
ial (
fres
h) th
at h
as b
een
sele
cted
from
a s
egre
gatio
n ve
sicl
e cy
linde
r; G
rdm
assa-
sv—
alte
red
grou
ndm
ass
mat
eria
l fro
m a
seg
rega
tion
vesi
cle
cylin
der;
Grd
mas
sa —al
tere
d gr
ound
mas
s. R
ecal
c. a
ge—
all d
ata
have
bee
n re
calc
ulat
ed w
ith a
dec
ay c
onst
ant o
f Ren
ne e
t al.
(201
0) a
nd s
tand
ardi
zed
to th
e no
rmal
izat
ion
valu
e fo
r F
ish
Can
yon
sani
dine
(Jo
urda
n an
d R
enne
, 200
7). D
ata
sour
ces:
1—
Hoo
per
et a
l. (2
002)
; 2—
Dun
can
(198
2), i
nclu
ded
in L
ong
and
Dun
can
(198
3); 3
—Lo
ng a
nd D
unca
n (1
983)
; 4—
Bar
ry e
t al.
(201
0); 5
—B
aksi
and
Far
rar
(199
0); 6
—Le
es (
1994
). † A
vera
ged
valu
es c
alcu
late
d fr
om d
ata
pres
ente
d in
Lee
s (1
994)
, ass
umin
g th
at d
ata
are
quot
ed a
s cc
ST
P ×
10–1
0 (c
ubic
cen
tilite
rs a
t sta
ndar
d te
mpe
ratu
re p
ress
ure
x 10
–10 )
.§ E
rror
val
ue a
men
ded
from
pub
lishe
d va
lue
to v
alue
orig
inal
ly q
uote
d in
Lee
s (1
994)
, whi
ch s
tate
d th
at e
rror
s ar
e gi
ven
as 1
σ.
Eruption chronology of the Columbia River Basalt Group 57
questions about diachronism along this boundary. The younger of these ages is in good agreement with the youngest date of 15.28 ± 0.74 Ma (Lees, 1994) from the Basalt of Hunter Creek, Wapshilla Ridge Member, at the top of the Grande Ronde Basalt succession in the Malheur Gorge area. However, the Basalt of Hunter Creek is R
2, rather than N
2, and both dates are at odds
with data for the overlying Wanapum Basalt (see following). Wanapum Basalt data suggest that Grande Ronde Basalt volca-nism must have fi nished by ca. 15.6 Ma, if not before.
If we assume Grande Ronde Basalt volcanism started at ca. 16.0 Ma and ended at ca. 15.6 Ma, then the total duration for Grande Ronde Basalt volcanism would be ~0.4 m.y., con-sistent with the ~420,000 yr duration estimated by Barry et al. (2010). Such an age range for the Grande Ronde Basalt presents an inconsistency with the current geomagnetic time scale. The available data suggest that Grande Ronde Basalt lavas most likely erupted within the geomagnetic chron C5Br (15.974–15.160 Ma; Gradstein et al., 2004). However, this poses a problem for the signifi cance of the geomagnetic reversals recorded within the Grande Ronde Basalt; there appears to be a lack of short mag-netic reversals during C5Br (e.g., Gradstein et al., 2004). We have no solution to this dilemma at present, though we note that there has been a history of moving geomagnetic transitions if neces-sary to fi t with chronologic constraints (e.g., Steens reversal once thought to be 15.5 Ma when dated by K-Ar technique [Baksi et al., 1967] has since moved to 16.7 Ma following modern studies, with further calls to shift the geomagnetic reversals constraining the Grande Ronde Basalt succession [Baksi et al., this volume]). Potential solutions to this mismatch may be (1) that the reversals measured in the Grande Ronde Basalt are merely short excur-sions within the long interval of reverse polarity; or (2) that rapid reversals C5Cn.2r to C5Cn.1n (currently dated from 16.453 Ma
to 15.974 Ma; Gradstein et al., 2004) should all be younger than 16 Ma; or (3) that the groundmass ages determined for the Grande Ronde Basalt and Imnaha are too young by ~0.5 m.y.
The Picture Gorge Basalt of northern Oregon (Fig. 2) is a coeval unit with the middle of the Grande Ronde Basalt vol-canism. Originally dated by K-Ar (Watkins and Baksi, 1974), these lavas have received no modern treatment by 40Ar/39Ar dat-ing methods (Table 7). Ages regarded as generally acceptable by Baksi (1989) range from 16.4 Ma to 15.2 ± 0.4 Ma, thus overlap-ping and agreeing with Grande Ronde Basalt 40Ar/39Ar data.
Wanapum Basalt
The Wanapum Basalt is distinctive within the Columbia River Basalt Group stratigraphy in that it follows an appar-ently signifi cant time break, expressed in the fi eld in the western part of the province by the Vantage interbeds (Smith, 1988). Although the Vantage sediments are not found every-where between the underlying Grande Ronde Basalt and the Wanapum Basalt, they are extensive and locally up to 20 m in thickness. Also, several of the Wanapum lavas are coarsely feldspar-phyric, which helps with their recognition and correla-tion in the fi eld (Beeson et al., 1985).
The basal Wanapum Basalt lavas are represented by the fairly locally distributed Eckler Mountain Member, confi ned to the central part of the province (Tolan et al., 1989; Reidel and Tolan, this volume). Eckler Mountain Member lavas outcrop around the Blue Mountains of southeastern Washington, for which we have but one 40Ar/39Ar plateau age (15.76 ± 0.17 Ma; Barry et al., 2010; Table 8). Additional information about the beginning of Wanapum Basalt volcanism comes from data for the Frenchman Springs Member. The lowest unit dated within
TABLE 6. K-Ar DATA FOR THE GRANDE RONDE BASALTS (GRB)
Formation Sample ID K (wt%)
40*Ar/total 40Ar
K-Ar age (published)
(Ma)
Error (1σ)
Ref Recalc. age (Ma)
Error (1σ)
6.0 4.51 1 6.0 3.51 .vA 13.0 .vA 54.1 .vA 4777 BRG
4.0 9.41 1 4.0 8.41 24.0 51.1 5677 BRG
4.0 3.51 1 4.0 2.51 45.0 15.1 94PS87 BRG
5.0 2.51 1 5.0 1.51 14.0 93.1 WA7977 BRG
4.0 1.51 1 4.0 0.51 84.0 60.1 5977 BRG
4.0 0.51 1 4.0 9.41 16.0 41.1 4977 BRG
8.0 7.51 1 8.0 6.51 34.0 80.1 2277 BRG
2.0 6.51 1 2.0 5.51 25.0 03.1 7277 BRG
4.0 1.51 1 4.0 0.51 25.0 61.1 9077 BRG
4.0 6.41 1 4.0 5.41 84.0 30.1 9277 BRG
4.0 8.51 1 4.0 7.51 94.0 05.1 7577 BRG
2.0 3.51 1 2.0 2.51 36.0 54.1 5577 BRG
GRB–Buckhorn Springs No info No info No info 16.5 – 2 16.6 –
Note: Recalculated ages make the assumption that publications up to and including 1977 used the decay constant of Dalrymple and Lanphere (1969), and that publications after that time used the decay constant of Steiger and Jäger (1977). All data have been recalculated with a decay constant of Renne et al. (2010). Data sources: 1—Fiebelkorn et al. (1982), and references therein; 2—Reidel et al. (1989).
58 Barry et al.
TABLE 7. K-Ar DATA FOR THE PICTURE GORGE BASALTS
Formation Sample ID K (wt%)
Atm Ar K-Ar age (published)
(Ma)
Error (1σ)
Ref Recalc. age (Ma)
Error (1σ)
Picture Gorge Basalt 14 0.63 38.6 14.9 0.3 1 15.4 0.3
Picture Gorge Basalt 13 0.48 58.5 15.9 0.3 1 16.4 0.3
Picture Gorge Basalt 8 0.50 43.9 15.9 0.2 1 16.4 0.2
Picture Gorge Basalt 5 0.66 49.5 14.7 0.3 1 15.2 0.3
Picture Gorge Basalt 4 0.45 43.6 14.7 0.2 1 15.2 0.2
Picture Gorge Basalt 3 0.39 64.8 15.6 0.4 1 16.1 0.4
Picture Gorge Basalt 1 0.44 62.0 15.7 0.3 1 16.2 0.3
Note: Recalculated ages make the assumption that publications up to and including 1977 used the decay constant of Dalrymple and Lanphere (1969). All data have been recalculated with the decay constant of Renne et al. (2010). Data source: 1—Watkins and Baksi (1974). Atm Ar (atmospheric argon) is presented instead of 40Ar*/total Ar for the Picture Gorge data because only atmospheric argon data are available.
TABLE 8. Ar-Ar DATA FOR THE WANAPUM FORMATION
Member Unit Sample ID Type of material
%40Ar* 37Ar/39Ar 40Ar/39Ar age (published)
(Ma)
Error (1σ)
Ref Recalc. age (Ma)
Error (1σ)
Priest Rapids B. of Rosalia Ds1-(1) Grdmass 90.87 1.21 This study – 0 15.07 0.07
yduts sihT 55.0 01.68 ssamdrG pud )2(-1sD – 0 15.25 0.08 yduts sihT 42.4 23.77 ssamdrG )3(-1sD – 0 14.80 0.17
Roza DF1-(1)* Grdmass 86.11 2.79 16.34 0.24 1 16.41 0.25
ssamdrG )1(-3LC 35.32 0.31 This study – 0 12.87 0.37 351-60BRC
dup Grdmass 79.37 0.67 This study – 0 14.98 0.06
Frenchman Springs
B. of Sand Hollow
No information No info No info No info 15.30 – 3 15.59 –
yduts sihT 51.0 72.87 ssamdrG pud 7FP – 0 15.27 0.18 91.0 81.51 1 91.0 21.51 85.0 29.07 ssamdrG )tpr( 7FP 11.0 67.41 1 11.0 07.41 51.0 72.87 ssamdrG 7FP
ssamdrG 4LC –7.08 0.47 This study – 0 16.42 0.38 ssamdrG 800-50BRC 17.43 1.25 This study – 0 13.54 0.16
yduts sihT 10.3 81.57 ssamdrG 940-50BRC – 0 14.71 0.08
Frenchman Springs
B. of Palouse Falls
DC-12-2236 Grdmass 45.93 1.57 22.80 0.30 2 23.21 0.31
Frenchman Springs
B. of Ginkgo DC-12-2212 Grdmass 69.17 1.38 15.50 0.20 2 15.78 0.20
yduts sihT 10.1 43.66 ssamdrG 110-50BRC – 0 12.48 0.14 yduts sihT 39.1 28.19 ssamdrG )1(-8CsF – 0 16.20 0.10 yduts sihT 05.1 98.35 ssamdrG pud )2(-8CsF – 0 15.97 0.28
Eckler Mountain B. of Dodge CRB05-081 Grdmass 67.67 7.96 15.70 0.17 1 15.76 0.17
Note: Sample DF1-(1) is marked with *. It appeared in the online electronic appendix of Barry et al. (2010) as part of a preliminary test of suitable material for dating the Grande Ronde Basalts. As such, it is here presented as a recalculated age, but it has never been discussed in any previous manuscript. Description of type of material: Grdmass—groundmass (also implies that it is the groundmass material devoid of any large phenocrysts). Recalc. age—all data have been recalculated with a decay constant of Renne et al. (2010) and standardized to the normalization value for Fish Canyon sanidine (Jourdan and Renne, 2007). Data sources: 0—this study; 1—Barry et al. (2010); 2—Duncan (1982); 3—Reidel et al. (1989).
Eruption chronology of the Columbia River Basalt Group 59
the Frenchman Springs Member (Basalt of Ginkgo) provided ages between 16.20 Ma and 15.78 ± 0.05 Ma (Appendix DR1 and Duncan [1982], respectively; excluding the single date of 12.48 ± 0.14 Ma [Appendix DR1], on grounds of it being strati-graphically out of place). Interestingly, though, this places the timing of Wanapum Basalt volcanism in confl ict with the end of Grande Ronde Basalt volcanism, unless both Grande Ronde Basalt and Wanapum volcanism were active at the same time, within potentially different parts of the large igneous province. This is not easy to reconcile with the presence of the interven-ing Vantage sediments and would require detailed mapping and dating along the contact to resolve. It is evident, though, that the hiatus between the end of Grande Ronde Basalt activity and the onset of Wanapum Basalt volcanism may have been brief, despite the presence of the Vantage sediments. We propose that the age of the base of the Wanapum Basalt is ca. 15.6 Ma, allow-ing time for the Grande Ronde Basalt to erupt after a start date of ca. 16 Ma, but within error of the youngest acceptable age for the lowest part of the Frenchman Springs Member, Basalt of Ginkgo (Tables 8 and 9).
The best estimate for the top of the Frenchman Springs Mem-ber comes from the dates of the Basalt of Sand Hollow below (14.76–15.27 ± 0.04 Ma; Barry et al. [2010] and Appendix DR1, respectively), and the Roza Member above (14.98 ± 0.06 Ma; Appendix DR1). These ages are unresolvable from each other and thus are coincidental with the best estimate for the age of the top of the Wanapum Basalt, at ca. 15 Ma. This is consistent with the age of the overlying Basalt of Rosalia, Priest Rapids Member, dated at 14.80–15.25 ± 0.01 Ma (Table 8).
In summary, the age range for the Wanapum Basalt is from ca. 15.6 Ma to ca. <15 Ma, suggesting that the ~10 eruptions of the Wanapum Basalt occurred spasmodically for a little more than half a million years. The lava fl ow fi elds often have thin sediments between them (Beeson et al., 1985; Jolley et al., 2008) and weathering of fl ow tops beneath a contact, indicative of rea-sonably long average hiatuses between eruptions. Clearly, the
TABLE 9. K-Ar DATA FOR THE WANAPUM FORMATION
Member Unit Sample ID K (wt%) 40*Ar/total 40Ar
K-Ar age (published)
(Ma)
Error (1σ)
Ref Recalc. age (Ma)
Error (1σ)
Priest Rapids B. of Lolo No info No info No info 13.1–16.2 (probable 14.9)
No info 1 13.5–16.7 (15.4)
–
Priest Rapids B. of Rosalia No info No info No info 11.9–15.5 No info 1 12.3–16.0 –
Priest Rapids B. of Rosalia KA1236 1.16 0.51 14.5 No info 2 15.0 –
ofni oN ofni oN ofni oN azoR 12.5–16.3 No info 1 12.9–16.9 –
Frenchman Springs B. of Ginkgo No info No info No info 13.4 No info 1 13.9 –
Eckler Mountain Icicle Flat Basalt
VC79-282 Av. 0.73
Av. 0.38 16.4 1.2 3 16.5 1.2
Note: Recalculated ages make the assumption that publications up to and including 1977 used the decay constant of Dalrymple and Lanphere (1969), and that publications after that time used the decay constant of Steiger and Jäger (1977). Data from pre-1969 publications are similarly recalculated using Dalrymple and Lanphere (1969) values, as they based their calculations on decay constant information presented in Aldrich and Wetherill (1958). All data have been recalculated with a decay constant of Renne et al. (2010). Data sources: 1—dates given as reported, including the notation of “probable” age, as in U.S. Energy Research and Development Administration (1976); 2—Evernden and James (1964); 3—Krueger Enterprises Inc., Geochron Laboratory Division (1984, personal commun.).
overlap with the Grande Ronde Basalt is problematic, and under-standing may be advanced by more targeted dating programs in the future.
Saddle Mountains Basalt
Lavas of the Saddle Mountains Basalt are characteristi-cally constrained by topography and form thick, channelized or dammed lavas with well-developed columnar jointing. Unlike other parts of the Columbia River Basalt Group stratigraphy, there is a bias in the age dating data set for the Saddle Mountains Basalt (Appendix DR2); there was an abundance of early K-Ar analyses on this late stage of the Columbia River Basalt Group stratigraphy (e.g., McKee et al., 1977), but there has since been a paucity of modern 40Ar/39Ar studies (Tables 10 and 11; Appendix DR2). We have thus constrained the stratigraphy, where possible, on the basis of the available 40Ar/39Ar data, but many of the units have recommended ages given by corrected K-Ar dates.2
The Saddle Mountains Basalt volcanism began shortly after the cessation of the underlying Wanapum Basalt. The Mabton sedimentary interbed occurs between the Wanapum and Sad-dle Mountain Basalts, but there is no evidence for an erosional unconformity. Given that Wanapum Basalt activity appears to have ended close to 15 Ma, we can be fairly confi dent that the Saddle Mountains lavas are younger than 15 Ma. The oldest date, a K-Ar age of 14.57 Ma (U.S. Energy Research and Develop-ment Administration, 1976), comes from the Umatilla Member, supporting a short hiatus between the end of the Wanapum and the beginning of the Saddle Mountains volcanism. Basaltic activ-ity seems to have persisted through to ca. 6 Ma (on the basis of
2K-Ar values have been corrected for changes to the K decay constant. Publica-tions prior to, and including, 1977 are assumed to have used the decay constant of Dalrymple and Lanphere (1969). Publications with a date after 1977 are assumed to have used the decay constant of Steiger and Jäger (1977). All K-Ar values have been calculated to a newer value proposed by Renne et al. (2010).
60 Barry et al.T
AB
LE 1
0. A
r-A
r D
AT
A F
OR
SA
DD
LE M
OU
NT
AIN
S B
AS
ALT
Mem
ber
Uni
t S
ampl
e ID
T
ype
of
mat
eria
l %
40A
r 37
Ar/
39A
r 40
Ar/
39A
r ag
e (p
ublis
hed)
(M
a)
Err
or
(1σ)
R
ef
Rec
alc.
ag
e (M
a)
Err
or
(1σ)
Ele
phan
t Mtn
DH
5 28
2.2
Grd
mas
s 14
.79
2.28
10
.00
0.50
2
10.1
8 0.
51
Pom
ona
D
H5
368.
0 G
rdm
ass
80.3
0 0.
49
11.0
0 0.
20
2 11
.21
0.21
P
omon
a
DC
y5
Grd
mas
s 54
.21
9.25
–
– 0
10.3
4 0.
21
Aso
tin
B. o
f Hun
tzin
ger
No
info
rmat
ion
No
info
N
o in
fo
No
info
13
.00
– 1
13.2
4 –
N
ote:
Des
crip
tion
of ty
pe o
f mat
eria
l: G
rdm
ass—
grou
ndm
ass
(als
o im
plie
s th
at it
is th
e gr
ound
mas
s m
ater
ial d
evoi
d of
any
larg
e ph
enoc
ryst
s). R
ecal
c. a
ge—
all d
ata
have
bee
n re
calc
ulat
ed w
ith a
dec
ay c
onst
ant o
f Ren
ne e
t al.
(201
0) a
nd s
tand
ardi
zed
to th
e no
rmal
izat
ion
valu
e fo
r F
ish
Can
yon
sani
dine
(Jo
urda
n an
d R
enne
, 200
7). D
ata
sour
ces:
0—
this
stu
dy; 1
—R
eide
l et a
l. (1
989)
; 2—
Dun
can
(198
3).
TA
BLE
11.
K-A
r D
AT
A F
OR
TH
E S
AD
DLE
MO
UN
TA
INS
BA
SA
LT
Mem
ber
Uni
t S
ampl
e ID
K
(w
t%)
40*A
r/to
tal
40A
r K
-Ar
age
(pub
lishe
d)
(Ma)
Err
or
(1σ)
R
ef
Rec
alc.
age
(M
a)
Err
or (
1σ)
Low
er M
onum
enta
l
No
info
N
o in
fo
No
info
6.
0 N
o in
fo
1 6.
2 –
ofni oN
ofni oN
ofni oN
robra
H ecI7.
9–11
.3
(pro
babl
e 8.
5)
No
info
2
8.1–
11.6
(8
.8)
–
7.8 1
ofni oN
5.8 ofni o
N ofni o
N ofn i o
N
rob raH e cI
–
Ele
phan
t Mtn
No
info
N
o in
fo
No
info
8.
1–12
.0
(pro
babl
e 9.
5)
No
info
2
8.4–
12.4
(9
.8)
–
Ele
phan
t Mtn
No
info
N
o in
fo
No
info
10
.5
No
info
1
10.8
–
Cra
igm
ont B
asal
t
VC
79-2
14
Av.
1.6
0 A
v. 0
.56
11.9
0.
7 3
12.0
0.
7
Sw
amp
Cre
ek B
asal
t
VC
79-3
17
Av.
1.1
3 A
v. 0
.56
11.4
0.
8 3
11.5
0.
8
B. o
f Fea
ry C
reek
VC
79-3
49
Av.
1.6
0 A
v.0.
48
11.9
0.
7 3
12.0
0.
7
B. o
f Fea
ry C
reek
VC
79-7
04
Av.
1.5
5 A
v.0.
40
11.2
0.
7 3
11.3
0.
7
ofni oN
ofn i oN
ofni oN
ano
moP
7.7–
13.3
(p
roba
ble
10.5
) N
o in
fo
2 8.
0–13
.8
(10.
9)
–
4.21 1
ofni oN
0.21 ofni o
N ofni o
N of ni o
N
anomo
P–
Esq
uatz
el
Gab
le B
utte
N
o in
fo
No
info
N
o in
fo
10.3
–12.
9 N
o in
fo
2 10
.7–1
3.3
–
Gra
ngev
ille
Bas
alt
K
A12
92
0.13
0.
78
12.1
N
o in
fo
4 12
.5
–
Gra
ngev
ille
Bas
alt
V
C79
-190
A
v. 0
.62
Av.
0.29
14
.3
1.3
3 14
.4
1.3
Gra
ngev
ille
Bas
alt
V
C79
-193
A
v. 0
.64
Av.
0.30
13
.0
1.2
3 13
.1
1.2
Aso
tin
B. o
f Hun
tzin
ger
No
info
N
o in
fo
No
info
10
.8–1
2.9
No
info
2
11.2
–13.
3 –
Wilb
ur C
reek
B
. of W
ahlu
ke
No
info
N
o in
fo
No
info
12
.7
No
info
2
13.1
–
Um
atill
a B
. of U
mat
illa
No
info
N
o in
fo
No
info
12
.0–1
5.0
(pro
babl
e 14
.1)
No
info
2
12.4
–15.
5 (1
4.6)
–
N
ote :
Rec
alcu
late
d ag
es m
ake
the
assu
mpt
ion
that
pub
licat
ions
up
to a
nd in
clud
ing
1977
use
d th
e de
cay
cons
tant
of D
alry
mpl
e an
d La
nph
ere
(196
9), a
nd th
at
publ
icat
ions
afte
r th
at ti
me
used
the
deca
y co
nsta
nt o
f Ste
iger
and
Jäg
er (
1977
). D
ata
from
pre
-196
9 pu
blic
atio
ns a
re s
imila
rly r
ecal
cula
ted
usin
g D
alry
mpl
e an
d La
nphe
re (
1969
) va
lues
, as
they
bas
ed th
eir
calc
ulat
ions
on
deca
y co
nsta
nt in
form
atio
n pr
esen
ted
in A
ldric
h an
d W
ethe
rill (
1958
). A
ll da
ta h
ave
been
rec
alcu
late
d w
ith a
de
cay
cons
tant
of R
enne
et a
l. (2
010)
. Av—
aver
age,
not
atio
n fo
r av
erag
e of
mor
e th
an o
ne v
alue
. Dat
a so
urce
s: 1
—M
cKee
et a
l. (1
977)
; 2—
date
s gi
ven
as r
epor
ted,
in
clud
ing
the
nota
tion
of “
prob
able
” ag
e, in
U.S
. Ene
rgy
Res
earc
h an
d D
evel
opm
ent A
dmin
istr
atio
n (1
976)
; 3—
Kru
eger
Ent
erpr
ises
Inc
, Geo
chro
n La
b. D
ivis
ion
(198
4,
pers
onal
com
mun
.); 4
—E
vern
den
and
Jam
es (
1964
).
Eruption chronology of the Columbia River Basalt Group 61
an unverifi able K-Ar age of 6.2 Ma for the lower Monumental Member at the top of the Saddle Mountains Basalt), although frequency of eruptions tailed off at ca. 12 Ma.
Final Recommendations
The recommendations are based on a nonbiased approach to examining, where possible, the raw isotope data, coupled with detailed knowledge of fi eld constraints and paleomagnetic data. This does not always lead to the most obvious suggestions, and in particular there are clear shortfalls in our recommenda-tions, for example, the apparent overlap in timing between the end of the Grande Ronde Basalt volcanism and the start of the Wanapum Basalt, without supporting evidence for synchronicity of these two formations. Furthermore, individual dates are not always within stratigraphic order. For example, Basalt of Rosalia, Priest Rapids Member (15.07–15.25 ± 0.11 Ma) clearly strati-graphically overlies the Roza Member (14.98 ± 0.06 Ma). At fi rst glance, the age data might appear at odds with that relation-ship, but the age data are within the margins of analytical error and therefore valid (Table 8). However, this has been a rigorous exercise to examine all the available radioisotope age data for the Columbia River Basalt Group, and our fi nal recommendations are presented in Figure 4.
DISCUSSION
Volume versus Timing of Eruptions and Effusion Rates for the Columbia River Basalt Group
The thick succession of Steens Basalt (31,800 km3 estimated total volume) erupted between ca. 16.9 Ma and ca. 16.6 Ma, with activity concentrated around 16.7 Ma (Table 1). Using an alterna-tive method to examining effusion rates, Camp et al. (this volume) were able to constrain the eruption of the bulk of the Steens Basalt to <50,000 yr, giving an average effusion rate of 0.67 km3/yr. They acknowledge the possibility that lingering eruptions of much smaller volume could extend the overall duration beyond this interval, but that it is unlikely to exceed ~300,000 yr.
The Imnaha Basalt appears to have erupted between 16.7 Ma and 16.0 Ma (Tables 3 and 4). Current estimates for the volume of the Imnaha Basalt are 11,000 km3 (Reidel et al., this volume). Over a time span of 700,000 yr, this would suggest a time-averaged magma eruption rate of 0.016 km3/yr, although clearly mean output rates for individual eruptions or eruptive epi-sodes are likely to have been higher than this for specifi c peri-ods of time, on account of volcanism being more sporadic, with variable-length hiatuses between eruptions.
With an estimated eruptive volume of 150,000 km3, the Grande Ronde Basalt phase of effusion represents an enormous outpouring of lava (Fig. 5). The effusion rates for the Grande Ronde Basalt give a time-averaged magma eruption rate of 0.375 km3/yr, i.e., somewhat lower than estimates for the Steens lava sequences. Individual Grande Ronde Basalt eruptions varied
considerably in volume, but many were considerably greater than 1000 km3 in size. As with all other parts of the stratigraphy, erup-tive events would not have been equally spaced in time; some eruptions may have followed short periods of volcanic repose (possibly as low as months to several years), whereas others could have been considerably longer (many thousands to >104 yr).
The volumes of the Wanapum and Saddle Mountains Basalts lava dramatically decline with time (Fig. 5, inset). After the main pulse of the Grande Ronde Basalt, volcanism rapidly waned. Furthermore, volcanism shifted geographically toward the Snake River Plain and centralized silicic systems (e.g., Pierce et al., 2002, and references therein).
The amount of lava erupted over the life span of the large igneous province has long been investigated using the best avail-able age data versus volume estimates (Baksi, 1989; Hooper et al., 2002; Tolan et al., 1989). A revised version of Figure 5 of Tolan et al. (1989) is shown as Figure 5 here, with the latest revi-sions adding detail to earlier attempts (shown with a log scale for volume). Little has changed from earlier attempts at estimating volume-time relationships, but additional details of mean magma eruption rates show how the initial start-up of the Steens Basalt and the highly voluminous Grande Ronde Basalt dominate the formation of the Columbia River Basalt Group.
Suggestions for Future Work
In compiling the available radiometric age data for the Columbia River Basalt Group, there were surprisingly few 40Ar/39Ar dates on the Saddle Mountains Basalt. It appears that much of the early interest (1970s and 1980s), when the most appropriate dating technique was K-Ar, concentrated on the episodic eruptions of the Saddle Mountain Basalt. Despite the continuing interest in the periodicity of large-scale eruptions, there has been little work on the youngest part of the Columbia River Basalt Group. As such, this waning phase of volcanism is poorly constrained, and much of the available data cannot be critically assessed for its quality (Table 8). It would be inter-esting, for example, to examine the younger Saddle Mountain Basalt eruptions that occurred at a time of change from a domi-nantly basaltic system (the Columbia River Basalt Group) to a bimodal one (which presently manifests itself as the Yellow-stone system).
Although modern 40Ar/39Ar analyses can date to within 1% precision, there are few high-precision dates from the Columbia River Basalt Group units. A handful of analyses (e.g., Henry et al., 2006) have produced highly precise results, but on sanidines from intercalated tuffaceous units. One study examined different types of material from the Wanapum and Grande Ronde Basalts in an attempt to fi nd the type of material that gave the best ana-lytical results for these crystal-poor basalts (Barry et al., 2010). Surprisingly, the study found that large basalt-hosted feldspar crystals yielded meaningless results. Yet, in the Ar dating of the Steens Basalt, good results have been obtained from analyzing feldspar crystals (e.g., Jarboe et al., 2008). We speculate that
62 Barry et al.
complex feldspar antecrysts are more abundant in later lavas, and bring with them multiple phases of fl uid inclusions. These inclu-sions carry a budget of volatile concentrations, which appears from the data to complicate analyses of not just the host crys-tals but also nearby groundmass. To avoid such issues, it seems that material from intercalated silicic ash deposits, which may contain sanidine, would be a profi table target for future dating. Additionally, it seems worthwhile to undertake further detailed studies of the large antecrysts (e.g., Ramos et al., 2005, 2009) to better understand the origin and nature of these crystals. They
clearly have much to tell us about the plumbing, accumulation, and storage of material prior to a fl ood basalt eruption.
There are a number of K-Ar ages for Picture Gorge Basalt (Baksi et al., 1991), but there is an absence of Ar-Ar ages. Pic-ture Gorge Basalt appears to be derived from the same magma source as Steens Basalt, both having identical mixing arrays with the same isotopic end members (Camp and Hanan, 2008). Many of the Picture Gorge lavas are strongly plagioclase-phyric with large phenocrysts similar in appearance to those found in Steens Basalt. The implication of these relationships suggests that the
Lower Monumental
Ice Harbor
Pomona
Asotin-Wilbur Cr
Imnaha
Roza
Swamp CrFeary CrCraigmont
Frenchman Springs
Steens
Eckler Mt.
Grande Ronde
Esquatzel
Priest Rapids
Umatilla
WeisenfelsRidge
Elephant Mt.
Buford
Picture Gorge
0
18 17 16 15 14 13 12 11 10 9 8 7 6 5
Million Years Before Present
Vol
ume
(km
3 )
1,000
10,000
100,000
1,000,000
100V
olum
e (k
m3 )
Age (Ma)
Age (Ma)
Figure 5. Volume (km3) (logarithmic scale) against time (Ma) (linear scale) for the dated units of the Columbia River Basalt Group. The plot shows how volcanism waned signifi cantly after the Basalt of Priest Rapids, Wanapum Basalt, around 15 Ma. Inset: The same plot but with both scales linear, to illustrate the huge volumetric outpouring of the Grande Ronde Basalt in comparison with other Columbia River Basalt units. Revised from Tolan et al. (1989). Inset fi gure: S—Steens Basalt; IB—Imnaha Basalt; GRB—Grande Ronde Basalt; FS— Frenchman Springs; R—Roza; PR—Priest Rapids; U—Umatilla; A-WC—Asotin-Wilbur Creek; ESQ—Esquatzel; P-W—Pomona; EM—Elephant Mountain; IH—Ice Harbor; LM—Lower Monumental.
Eruption chronology of the Columbia River Basalt Group 63
very good Ar-dating results obtained from the Steens feldspars (e.g., Jarboe et al., 2008) could be replicated with Picture Gorge feldspars. Since the Picture Gorge lavas are interbedded with Grande Ronde Basalt, a focused Ar-dating study on Picture Gorge Basalt could provide better age constraints on the Grande Ronde lavas.
Well-constrained geochronologic data coupled with the geomagnetic time scale should place constraints on the timing of reversals. There is clearly scope for improved studies of the Imnaha and Grande Ronde Basalt relating to the ways in which these units correlate with the geomagnetic time scale. Age con-straints for Imnaha Basalt currently place it within a period of rapid reversals, where no reversals are currently recognized in the fi eld (Fig. 4). In contrast, the dates for the Grande Ronde Basalt currently fall within a long reversed period, when the rock record shows four reversals (Fig. 4). As has been done in the Steens succession (Jarboe et al., 2008), the Imnaha and Grande Ronde Basalt need a focused, combined paleomagnetic and argon dating study to examine (1) whether reversals occur within the Imnaha and (2) whether the reversals noted in the Grande Ronde Basalt are merely excursions.
Given the complex geometry of eruption units, with abut-ting internal lobes and sheets, and scope for variable activity across a lava fi eld (e.g., Vye, 2009; Vye-Brown et al., 2013), it seems highly likely that different units could be emplaced at the same time. The chances of diachroneity of units also seem highly plausible and could help explain some of the Ar dates; e.g., the uppermost part of the Imnaha could be much older in one place than another, and could have continued while Grande Ronde Basalt volcanism started elsewhere. To verify this, detailed fi eld and chronological studies would be needed, but they may help to elucidate some of the complexities in the relationships among the Steens Basalt, Imnaha Basalt, and Grande Ronde Basalt.
SUMMARY
From a detailed assessment of the available radioisotope data for the Columbia River Basalt Group, we compiled the most accurate and precise ages and propose the most valid dates for each of the formations, and some key units. Our recommenda-tions are based on a critical analysis of all the available raw data. Using our stated criteria, we recommend that the overall age range for Steens Basalt is ca. 16.9–16.6 Ma, but that the greatest bulk of Steens Basalt may have erupted in <50,000 yr, concen-trated at ca. 16.7 Ma, as demonstrated by paleomagnetic evidence on the estimated eruption rate of the Steens reversal (Camp et al., this volume). Steens activity was possibly synchronous with the onset of Imnaha Basalt volcanism, which began at ca. 16.7 Ma and ended ca. 16.0 Ma. Shortly after Imnaha volcanism fi nished, Grande Ronde Basalt volcanism started at ca. 16.0 Ma, but ended by ca. 15.6 Ma, and possibly considerably earlier. Dates for the Grande Ronde Basalt are currently at odds with data for the over-lying Wanapum Basalt activity, which appears to have started by 15.6 Ma and continued until ca. 15.0 Ma. The data support
evidence that suggests the Vantage sediments were only a short-lived feature (Reidel and Tolan, this volume) and do not repre-sent a long hiatus between the voluminous Grande Ronde Basalt and the sporadic volcanism of the Wanapum Basalt. During the period of time in which the Wanapum Basalt erupted, the locus of activity shifted to the SE with the onset of Snake River Plain bimodal volcanism. Following the Wanapum Basalt volcanism, activity declined during the emplacement of the Saddle Moun-tains Basalt. Activity associated with the Columbia River Basalt Group ceased by 6 Ma.
ACKNOWLEDGMENTS
New 40Ar/39Ar data presented in Appendix DR1 were funded by Natural Environment Research Council grant NER/A/S/2003/00444 to S. Self, S.P. Kelley, and T.L. Barry. Thanks are extended to C.L. Vye-Brown for use of samples she had col-lected. M. Widdowson and M.-N. Guilbaud are also thanked for assistance with collection of samples used to provide new age dates in this study. We are also very grateful to reviewers Robert Fleck and Ingrid Ukstins-Peate for their thoughtful and useful comments, which helped to improve this paper.
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