# Magnetostratigraphy and Tectonic Rotation of the Eocene-Oligocene Makah and Hoko River Formations, Northwest Washington, USA

Authors: Donald R. Prothero; Elizabeth Draus; Casey Burns
Journal: International Journal of Geophysics
 (2009)

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## Abstract

The Eocene-Oligocene Makah Formation and subjacent middle Eocene Hoko River Formation of the northwestern Olympic Peninsula, Washington, yield mollusks, crustaceans, foraminifera, and early neocete whales; their age has never been precisely established. We sampled several sections; most samples showed a stable single-component remanence held largely in magnetite and passed a Class I reversal test. The upper Refugian (late Eocene) and lower Zemorrian (early Oligocene) rocks at Baada Point correlate with Chron C13r (33.7–34.7 Ma) and Chron C12r (30–33 Ma). The Ozette Highway section of the Makah Formation spanned the early Refugian to late Refugian, with a sequence that correlates with Chrons C15r-C13r (33.7–35.3 Ma), and a long reversed early Zemorrian section that correlates with Chron C12r (30–33 Ma). The type section of the Hoko River Formation correlates with Chron C18r (40.0–41.2 Ma). The area sampled shows about45∘ of post-Oligocene counterclockwise tectonic rotation, consistent with results obtained from the Eocene-Oligocene rocks in the region.


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## Body

## 1. Introduction

During the Eocene-Oligocene transition (from about 40 to 30 Ma), the Earth went through a dramatic transformation, with the “greenhouse” conditions of the early Eocene being replaced by the “icehouse” conditions of the Oligocene [1–5]. Antarctic glaciers appeared for the first time since the Permian, and cold Antarctic bottom waters were formed, beginning the modern pattern of oceanic circulation [1, 6]. Several episodes of mass extinction occurred through this interval, especially at the end of the middle Eocene (37 Ma), and in the earliest Oligocene (33 Ma), primarily in response to pulses of global cooling. Several extraterrestrial objects struck the Earth as well, but these impacts all occurred during the middle of the late Eocene (most of them are dated at 35.5–36.0 Ma) and are associated with no extinctions of consequence [7].In recent years, our understanding of the Eocene-Oligocene transition has greatly improved. Several deep marine sections and ocean cores have been recovered from around the world, and these have allowed a detailed examination of the paleoceanographic, stable isotopic, and micropaleontologic changes at high resolution  [1, 2, 5]. Much of the information for the global marine record was summarized in Berggren  and Prothero  [2] and Prothero, Ivany, and Nesbitt [5]. In addition, some shallow marine sequences, such as those in the Gulf Coast, have been analyzed in detail, allowing studies of the biotic changes in the benthic foraminifera  [9], mollusks [10, 11], echinoids [12], and pollen [13].  The terrestrial record in North America has also been calibrated by magnetic stratigraphy, and the systematics and biostratigraphy of the terrestrial organisms have recently been   summarized [2–4, 14].Compared with all these recent researchs, our understanding of the rich fossil record of the marine Eocene-Oligocene in the Pacific Coast has lagged behind. Since the beginning of this century, the biostratigraphy of these strata has been based primarily on the abundant benthic organisms because planktonic microfossils are scarce in these mostly shallow-water deposits. Mollusks have long been used, but their biostratigraphic zones are very long and thus low in resolution. For example, the middle-late Eocene-early Oligocene “Tejon” molluscan stage spans almost the entire Eocene-Oligocene transition, or about 10 million years in duration (from about 34–44 Ma), and the other molluscan stages of the Eocene and Oligocene are almost as long [15].Benthic foraminifera are the most abundant and widespread fossils in these strata, so they have been used for most biostratigraphic studies in the Pacific Coast. However, many of the benthic foraminiferal zones are also very long and low in resolution. For example, the middle Eocene Narizian stage spans about 8 million years (39–48 Ma), the late Eocene Refugian stage  spans  about 7 million years (39–32 Ma), and the Zemorrian stage spans most of the Oligocene [15]. In addition, benthic foraminifera also track paleobathymetric changes, and so some of the zonations based on benthic foraminifera have proven to be time-transgressive, especially between California and Washington [15, 16].Where planktonic microfossils are available, they have greatly improved the correlation with the global time scale (see papers summarized in [15]). However, the majority of these Pacific Coast sections yield few or no planktonic microfossils, usually, because they were deposited in shallow marine conditions, or have undergone too much dissolution and diagenesis.When the available biostratigraphic data are combined with magnetic stratigraphy, much higher resolution is possible as well as precise (to the nearest 100 000 years) correlation with the global time scale. For example, Prothero and Armentrout [17] used calcareous nannoplankton to calibrate their magnetic stratigraphy and were able to date the upper Eocene-Oligocene Lincoln Creek Formation in the southern Olympic Peninsula of Washington. This study showed that the Refugian stage as recognized in Washington by Rau [18, 19] is both late Eocene and early Oligocene in age (magnetic Chrons C15r-C12r, about 33–35 Ma). The type area of the Refugian stage in the western Santa Ynez Range, Santa Barbara County, California, is mostly late Eocene but also earliest Oligocene (magnetic Chrons C13n-C12r, about 34.5–33.5 Ma) [20].Finally, the Eocene-Oligocene transition is an important period of earth history because it marks the origination of both major living groups of whales, the baleen-bearing mysticetes, and the toothed odontocetes [21]. Although it is possible that the earliest mysticete comes from the late Eocene of New Zealand and Seymour Island, Antarctica, the oldest odontocete so far reported comes from the lower Oligocene part of the Makah Formation in Washington [21–23]. The lower Makah also yields specimens of some of the most primitive mysticetes, which bear both teeth and the insertion areas for baleen as well. Thus, precise dating of these marine beds of the northwest Olympic Peninsula is critical to our understanding of whale evolution.


## 2. Geologic Setting

The Makah and Hoko River Formations are an important deep-marine record of the Eocene and Oligocene exposed to low-tide beaches, sea cliffs, creeks, and roadcuts on the northwestern corner of the Olympic Peninsula (Figures1 and 2). They crop out in a northward-dipping homoclinal sequence along the northwestern coast of the Olympic Peninsula, part of almost 6000 m of Eocene to Miocene marine sediments. The entire sedimentary sequence unconformably overlies pillow basalts and breccias of the Crescent volcanics, which were exotic oceanic ridge and seamount terranes that accreted to North America in the early Eocene [24–26]. The Makah Formation is conformably overlain by the Oligocene Pysht Formation, which is better exposed in the north-central coast of the Olympic Peninsula between Clallam Bay and Lyre River [27] to the east of our study area.(A) Index map showing location of study in the northwest Olympic Peninsula. Modified from Snavely et al. [8, Figure 1]. (b) Geologic map of the northwest Olympic Peninsula, showing the location of the sections mentioned in this paper. Stippled outcrop pattern (Tm) indicates the Makah Formation, and its various named members (Tmb = Baada Point Member; Tmd = Dtokoah Point Member; Tmc = Carpenters Creek Member; Tmk = Klachopis Creek Member; Tmj = Jansen Creek Member). Unshaded outcrop = Hoko River Formation (Th symbols). Other formations: Tc = Clallam Formation (open circle pattern); Tp = Pysht Formation (vertical line pattern); Tl = Lyre River Formation (diagonal line pattern); Ta = Aldwell Formation (fine stipple pattern); Tme = mélange (wide vertical line pattern); Ts = lower sandstone and siltstone (horizontal line pattern); Tcr = Crescent Formation (basal volcanic unit). Modified from Snavely et al. [8, Figure 2].
(a)(b)Figure 2
Index map showing location of sampling sites (bold numbers) along Ozette Road and the Hoko River. Formation abbreviations as in Figure1(a). Modified from Snavely et al. [8, Figure  3].Not only is the Makah Formation fossiliferous with mollusks [8, 28], crustaceans [8, 29–35], and benthic foraminifera  [8], but it also yields it also yields birds [36], terrestrial plants [37–39], and some of the earliest known fossils of baleen and toothed whales [23]. Some of these fossils come from apparent chemosymbiotic communities [40–42], including communities that are apparently associated with decaying whale carcasses and sunken wood [22, 43–45].The rocks in the area were originally mapped as part of the Twin River Formation [46–49]. Snavely et al. [24] raised the Twin River Formation to group rank and subdivided it into three new formations: Hoko River, Makah, and Pysht. Snavely et al. [28] further subdivided the Makah Formation into members named (from lowest to highest): the Baada Point, Dtokoah Point, Klachopis Point, Third Beach, and Jansen Creek Members, with marker beds such as the Carpenter Creek Tuff member serving as dividing points. Snavely et al. [24] designated the type section of the Makah Formation as the wave-cut beaches along the Straits of Juan de Fuca from Waadah Island and Baada Point to Kydaka Point. Rocks along the Sekiu and Hoko rivers were selected as reference sections.Most of the Makah Formation consists of deep-water siltstones and thick turbidite sandstones, with occasional conglomerates. The uppermost unit, the Jansen Creek Member, is bathyal as well, Snavely et al. [28] interpreted some of the Jansen Creek Member as shallow-marine deposits. Snavely et al.  [28] pointed out that there are many olistostromes in the Jansen Creek Member, and there are also sandstones containing bathyal turrids and other mollusks (C. Hickman, written comm.) as well as numerous cold seeps (J. Goedert, pers. comm.). The Jansen Creek Member is the most fossiliferous unit in the Makah Formation.In some places the cumulative thickness of the Makah Formation is estimated to be about 2800 m, but most surface sections are much less thick and complete than this. The Makah Formation yields Refugian (late Eocene) benthic foraminifera in the lower part  and Zemorrian (Oligocene) foraminifera in the upper half.The Hoko River Formation was named by Snavely et al.[24] for a deep marine sequence of siltstones and lesser sandstones exposed beneath and to the south of the main belt of Makah exposures (Figure 1). In some places, there are channels and lenses of conglomerate and lithic sandstone in the formation, filled with clasts of basalt, phyllite, and metaigneous rocks; these clasts occasionally reach 3–5.6 m in diameter. Calcareous concretions in the formation yield fossil crabs [30, 46–50], gastropods, cephalopods [51], and carbonized wood. The type section is about 1600 m thick, although exposures are poor in most places, even in the best outcrops along the Ozette Highway and Hoko River (Figure 2). However, Snavely et al. [24, page A115] report up to 2300 m of section in the reference section at Deep Creek. A major unconformity separates the Hoko River Formation from the overlying Makah Formation. The Lyre Formation conformably underlies the Hoko River Formation in some places, but intertongues with the Hoko River Formation in others.


## 3. Methods

In the summers of 2001 and 2002, we sampled the major sections of the Makah Formation and Hoko River Formation highlighted by Snavely et al. [8]. These include the following.(1)
The type section of the Makah Formation along the tidal exposures from Baada Point to Third Beach on the Makah Reservation (Figure1(b)). This section described by Snavely et al. [8, Figure  4] is one of the most complete exposures of the lower Makah Formation and spans all the named members of the formation through about 1600 m of section. A total of 57 sites (each consisting of multiple samples) were taken to sample the available exposures as densely as possible.(2)
The referred section of the Makah Formation along the Hoko River and Ozette highway (Figures1(b), 2). This section was illustrated by Snavely et al. [8, Figure   5], and appears to span about 2000 m, although exposures are poor in many parts of the section. Eighteen sites were taken along the Hoko River, along with additional sites around Sekiu Point to cover the upper part of the section.(3)
The type section of the Hoko River Formation, also along Ozette Highway and the Hoko River, just to the south of the previous section (Figure2). This section was illustrated by Snavely et al. [24, Figure   10]. Due to poor exposures, only 5 sites could be taken spanning 1600 m of section.(4)
A third section of Makah Formation was taken along the low-tide exposures between the mouth of the Sekiu River and Shipwreck Point, which samples mostly the Jansen Creek Member and is the source of most of the recent discoveries of marine mammals from the Makah Formation (Figure1(b)).A minimum of three oriented block samples, and usually more, were taken at each site. Most of the rocks are well indurated and did not crumble, but dilute sodium silicate was used to harden samples that required it. In the laboratory, each block was then subsampled into standard cores using a drill press. Samples that were too poorly indurated were molded into disks of Zircar aluminum ceramic for analysis. The samples were then measured on a 2G Enterprises cryogenic magnetometer using an automatic sample changer at the California Institute of Technology.Samples were measured at natural remanent magnetization (NRM) and then demagnetized at alternating fields (AF) 2.5, 5.0, 7.5, and 10 millitesla (mT) to assess the response by low-coercivity magnetic phases. Each sample was then thermally demagnetized at multiple steps (200–630°C  in 50°C increments) to determine how much remanence persisted above the maximum laboratory unblocking temperature of magnetite and also to remove any overprints held in iron hydroxides, such as goethite.About 0.1 g of powdered samples of selected lithologies was placed in epindorph tubes and subjected to increased isothermal remanent magnetization (IRM) to determine their IRM acquisition and saturation response. These same samples were also AF demagnetized twice, once after having acquired an IRM produced in a 100 mT peak field, and once after having acquired an  anhysteretic remanent magnetization (ARM) in a 100 mT alternating field. These data are used for a modified Lowrie-Fuller test [52].Demagnetization data were inspected on orthogonal demagnetization (“Zijderveld’’) plots and average directions of each sample were determined by the least-squares method of Kirschvink [53]. Mean directions for each site were then analyzed using Fisher [54] statistics, and classified according to the scheme of Opdyke et al. [55].


## 4. Results

Representative orthogonal demagnetization (“Zijderveld”) plots (Figure3) demonstrate that the vast majority of the samples (Figures 3(a)–3(c)) show a single, southeast, and up (reverse polarity, rotated almost 45° counterclockwise) component that was apparent at NRM and demagnetized steadily to the origin. This component typically has a high coercivity, suggesting that chemical remanence  is held in goethite or hematite, which was apparently unblocked during thermal demagnetization. However, these samples were completely unblocked by the maximum unblocking temperature of magnetite (580°C), suggesting that most of the remanence is held in magnetite, not hematite. Some samples have a slight overprint to the southwest (Figure 3(d)), which were removed  by the 200°C thermal step  and revealed a southeast component that decayed to the origin by 580°C. Figure 3(e) shows a single component of remanence pointed northwest and down and held in magnetite with high-coercivity overprints that were removed in the first thermal step; it is antipodal to the reversed samples, and it is interpreted as a normal magnetization with a counterclockwise rotation. Some samples (Figure 3(f)) show a slightly different behavior. The sample originally had an overprint directed north and down that was removed by 200°C, revealing a southeast and negative magnetization. Unlike the behavior of the previous samples, the sample shown in Figure 3(f)   has very little high-coercivity component, suggesting that most of the remanence resides in magnetite. As is apparent from these results, all these samples (after dip correction) yield a magnetization that trends southeast and up or northwest and down.Orthogonal demagnetization (“Zijderveld”) plots of representative samples after dip correction (stratigraphic coordinates). Solid squares indicate declination (horizontal projection); open squares indicate inclination (vertical projection). First step is NRM, followed by AF steps of 2.5, 5, and 10 mT, then thermal steps from200° to 630°C in 50°C increments. Each division equals 10−3 A/m. See text for discussion of individual sample behavior.
(a)(b)(c)(d)(e)(f)Petrographic analysis by Snavely et al. [8, page 10-11] confirmed that magnetite was present in the matrix, along with traces of goethite or hematite cement rimming some of the framework grains. This is consistent with the magnetic behavior we have observed.IRM acquisition experiments (Figure4) show that the samples are dominated by magnetite as the principal magnetic phase  because the samples are saturated by 300 mT. The Lowrie-Fuller tests indicate that the grains in the sample are single-domain or pseudo-single-domain, as the ARM is more resistant to AF demagnetization than IRM.Figure 4
IRM acquisition (ascending curve on right) and Lowrie-Fuller test (two descending AF demagnetization curves on left) of a representative powdered sample. Open circles = IRM; solid circles = ARM. In all samples, the IRM saturates by 300 mT, indicating that magnetite is a primary carrier of the remanence. The ARM is more resistant to AF demagnetization than the IRM, showing that the remanence is held largely in single-domain or  pseudo-single-domain grains.Based on relatively consistent demagnetization behavior, the direction of remanence isolated between 300 to500°C in most samples was determined using the least squared method of Kirschvink [53], and each site was averaged using Fisher [54] statistics. Results are shown in Table 1. The normal and reverse directions are antipodal within error estimates, so the samples pass a reversal test. The positive reversal test suggests that the magnetizations are primary, and that most overprints have been removed (Figure 5). The dips of the beds are  homoclinal (30–45° to the northeast), so a fold test is not possible. However, it is clear that this is a primary remanence because the samples pass a reversal test, and the reverse polarity directions before tilt correction are east and up (clearly not a modern normal overprint). Inverting the reverse directions and averaging all vectors, the entire section yields a mean direction of  D=320.5, I=45.2, k=10.0 and α95=3.7 (n=162). This suggests about 35° of counterclockwise rotation when compared to the Eocene cratonic poles [57, 58].Table 1
Paleomagnetic data and Fisher statistics.N = number of samples per site; D = declination; I = inclination; K = precision parameter; α95 = radius of circle of 95% confidence around the estimated mean direction.
SITENDIKα95Type Makah Formation, Baada Point13157.3-67.14.764.622308.636.413.574.433333.444.536.920.644309.539.311.138.953132.6-54.04.665.863134.0-50.75.956.375145.3-25.616.031.983148.0-43.04.863.693118.7-27.6182.69.2103118.9-29.0109.711.8113137.1-29.912.935.8123131.6-36.49.442.8132140.0-17.9419.63.9144161.1-72.912.336.8155116.6-24.430.222.8163124.8-27.929.323.2174147.9-20.318.829.3183128.3-26.060.416.0195157.5-40.729.823.0Baada Point type Makah FormationNormal mean(n=8)317.841.217.013.8Reversed mean(n=47)135.1-37.49.37.2Overall mean(n=55)316.937.59.86.5(Rotation=37.7°)Ozette Road-Hoko River Makah sites13139.5-67.2820.94.324129.2-65.835.920.933134.5-63.18.046.943150.6-54.021.827.154152.9-63.017.530.463140.6-71.9102.512.275143.4-64.3542.75.383135.4-61.7146.310.293165.6-57.211.438.4102169.1-73.4111.023.9113160.9-51.626.924.3124178.8-49.114.433.7133308.425.313.135.6143343.843.715.732.2Ozette Road Makah FormationNormal mean(n=8)329.334.011.617.0Reversed mean(n=51)149.1-55.513.95.5Overall mean(n=59)329.352.612.65.5(Rotation=21.2°)Ozette Road-Hoko River Formation sites153132.6-49.69.343.0162342.227.8134.721.7174131.6-23.142.219.2183145.1-35.619.029.1193180.6-41.876.414.2203147.0-36.111.937.4Hoko River formational mean(n=17)150.0-37.013.110.2(Rotation=33.9°)Upper Makah Formation, coastline east of Shipwreck Point and west of Sekiu13124.5-34.936.520.723148.2-59.413.534.933139.0-48.34.467.942122.3-20.426.350.954135.5-50.76.154.763137.9-36.531.322.473127.8-32.155.216.883120.8-34.9195.68.895154.1-26.49.542.5103137.9-35.620.727.8113136.3-49.314.833.3124153.6-65.38.545.2134129.2-35.416.931.0143142.1-29.08.645.1153164.7-57.44.666.0163136.4-64.354.016.9173115.2-61.46.155.1Shipwreck Point-Sekiu Makah mean(n=51)135.9-44.410.26.6(Rotation=40.5°)Combined mean from all Makah-Hoko River sites(n=180)320.545.210.03.7(Rotation=31.1°)Figure 5
Equal area projections of estimated means directions of sites in the Makah Formation. Solid dots, rectangles, and solid circles indicate mean for normal polarity sites (lower hemisphere projection). Open dots and dashed lines indicate mean of reverse polarity samples (upper hemisphere projection). As can be seen from the plot, the directions are antipodal, suggesting that the primary remanence has been obtained and most overprinting has been  removed. “Baada N mean” and “Baada R mean” refer to the means of normal and reversed sites from the Baada Point section; “Ozette N mean” and “Ozette R mean” are from the Ozette Road-Hoko River section; and  “Sekiu N mean;”  “Sekiu R mean” are from the coastal section between Shipwreck Point and the mouth of the Sekiu River.


## 5. Magnetostratigraphic Correlations

Previously, the Makah Formation has been roughly interpreted to be late Eocene and early Oligocene in age, based on its benthic foraminiferans, but little precision was possible [8]. With better age information on the benthic foraminiferal  zonation  [15, 16] and also magnetic polarity correlations calibrated by planktonic organisms such as nannofossils [17], much more precise correlations of the Makah and Hoko River Formations with the global time scale are now possible.


### 5.1. Makah Formation Type Section, Baada Point

The magnetic polarity stratigraphy of the type section Snavely et al. [8] (Figure 6) shows that the lowest 300 m of section (except for the poorly exposed base) below the Baada Point Member marker bed is a normal polarity magnetozone. The remaining sequence (from the 400 m level through the Baada Point, Dtokoah Point, Klachopis Point,  Third Beach members, and all the intervening shale intervals, up to 1400 m on the section) is entirely reverse in polarity. The section ended at the Third Beach member because the remaining part is much more poorly exposed, with long intervals that could not be sampled, so it was too patchy and incomplete to provide a intepretable record of the upper part of the Makah Formation.Figure 6
Magnetic stratigraphy of the type section of the Makah Formation at Baada Point. Solid circles are Class I sites of Opdyke et al. [55], which have three or more sample directions that are statistically removed from a random distribution at the 95% confidence level. Hachured circles are Class II sites of  Opdyke et al. [55], which had only 2 samples that survived sampling and transport, so no statistics could be calculated. Open circles are Class III sites of Opdyke et al. [55], where two directions show a clear polarity preference, but the third sample direction is divergent. Stratigraphy modified from Snavely et al. [8, Figure    4].


### 5.2. Makah Formation Reference Section, Hoko River-Ozette Road

The magnetic pattern for the reference section of Snavely et al. [8] is shown in Figure 7. As in the previous section the lowermost sites are of normal polarity (sites 14 and 15, covering the lower 100 m). All of the remaining exposed parts of the formation are of  reverse polarity, extending above the Klachopis Point Member marker bed and into the Jansen Creek Member.Figure 7
Magnetic stratigraphy of the Ozette Road-Hoko River section. Conventions as in Figure6. Modified from Snavely et al. [8, Figure   5].


### 5.3. Makah Formation Reference Section, Coast East of Shipwreck Point

The polarity pattern for this section of the upper part of the Makah Formation (including the Jansen Creek Member) is shown in Figure8. This section is mostly deep-water siltstones and occasional thin turbidite sandstones as well as the spectacular soft-sediment folds and olistostromes described by Snavely et al. [8]. Samples were taken only from beds with uniform dip and not from deformed or slumped layers. Although the slumped layers were inspected for a possible fold test, it turned out that the folds were too poorly exposed or defined to get reliable dips, so this effort was abandoned. The Shipwreck Point section is particularly important because it yields nearly all the fossils of marine mammals found in the Makah Formation, particularly some of the earliest known fossils of baleen and toothed whales.Figure 8
Magnetic stratigraphy of the coastal section between Shipwreck Point and the mouth of the Sekiu River. Conventions as in Figure6.The entire section is a reverse polarity magnetozone. Based on the early Zemorrian foraminifera from this unit as well as mollusks from theLiracassis rex  Zone (Figure 10), the best correlation of this reverse polarity section is with Chron C12r (30.0–33.0 Ma), based on similar magnetobiostratigraphic patterns observed in the Ozette Highway section (Figure 7) as well as the pattern shown in the Lincoln Creek Formation of the southeastern Olympic Peninsula [17]. The oldest known baleen and toothed whales from this region are found near the base of the Jansen Creek Member exposures along the beaches east of Shipwreck Point [22], so these fossils are early Chron C12r in age, or earliest Oligocene (about 33 Ma).


### 5.4. Hoko River Formation Type Section, Hoko River-Ozette Highway

The best exposures of the Hoko River Formation are found along Ozette Highway and the Hoko River, just south and down-section from the Ozette Highway Makah sections described above. The section closely follows that of Snavely et al. [24, Figure 10] (Figure 9). Although this is the type section, the exposures are now extremely poor, and only five discrete sites could be taken spanning the 1600 m of section reported by Snavely et al. [8]. The lower four sites (spanning almost 1200 m of section) are reverse polarity; the uppermost site (site 15) is the only normal polarity site.Figure 9
Magnetic stratigraphy of type section of the Hoko River Formation along Ozette Highway. Stratigraphy after Snavely et al. [24, Figure   10]. Conventions as in Figure 6.Figure 10
Correlation of the three Makah sections, based on the dates and age constraints discussed in the text. Lincoln Creek Formation magnetostratigraphy after Prothero and Armentrout [17]. Time scale after [15, 56].Correlation of the type section of the Hoko River Formation is less straightforward than the correlation of the Makah Formation (Figure10). Based on the late Narizian benthic foraminiferal fauna, the long reverse magnetozone could be correlated with the relatively short Chron C17r (38.0–38.2 Ma) or the much longer Chron C18r (40.0–41.2 Ma). Because there is 1200 or more meters of reverse section in this sequence, we prefer the latter correlation. However, if the Hoko River Formation interfingers with the underlying Lyre Formation, then it is more likely that the correlation with Chron C17r is correct because the Lyre River Formation is correlated with the same interval (Prothero et al., [59]). Without planktonic microfossils or some sort of isotopic age determination, it is not possible to provide a more robust correlation on the Hoko River Formation.


## 5.1. Makah Formation Type Section, Baada Point

The magnetic polarity stratigraphy of the type section Snavely et al. [8] (Figure 6) shows that the lowest 300 m of section (except for the poorly exposed base) below the Baada Point Member marker bed is a normal polarity magnetozone. The remaining sequence (from the 400 m level through the Baada Point, Dtokoah Point, Klachopis Point,  Third Beach members, and all the intervening shale intervals, up to 1400 m on the section) is entirely reverse in polarity. The section ended at the Third Beach member because the remaining part is much more poorly exposed, with long intervals that could not be sampled, so it was too patchy and incomplete to provide a intepretable record of the upper part of the Makah Formation.Figure 6
Magnetic stratigraphy of the type section of the Makah Formation at Baada Point. Solid circles are Class I sites of Opdyke et al. [55], which have three or more sample directions that are statistically removed from a random distribution at the 95% confidence level. Hachured circles are Class II sites of  Opdyke et al. [55], which had only 2 samples that survived sampling and transport, so no statistics could be calculated. Open circles are Class III sites of Opdyke et al. [55], where two directions show a clear polarity preference, but the third sample direction is divergent. Stratigraphy modified from Snavely et al. [8, Figure    4].


## 5.2. Makah Formation Reference Section, Hoko River-Ozette Road

The magnetic pattern for the reference section of Snavely et al. [8] is shown in Figure 7. As in the previous section the lowermost sites are of normal polarity (sites 14 and 15, covering the lower 100 m). All of the remaining exposed parts of the formation are of  reverse polarity, extending above the Klachopis Point Member marker bed and into the Jansen Creek Member.Figure 7
Magnetic stratigraphy of the Ozette Road-Hoko River section. Conventions as in Figure6. Modified from Snavely et al. [8, Figure   5].


## 5.3. Makah Formation Reference Section, Coast East of Shipwreck Point

The polarity pattern for this section of the upper part of the Makah Formation (including the Jansen Creek Member) is shown in Figure8. This section is mostly deep-water siltstones and occasional thin turbidite sandstones as well as the spectacular soft-sediment folds and olistostromes described by Snavely et al. [8]. Samples were taken only from beds with uniform dip and not from deformed or slumped layers. Although the slumped layers were inspected for a possible fold test, it turned out that the folds were too poorly exposed or defined to get reliable dips, so this effort was abandoned. The Shipwreck Point section is particularly important because it yields nearly all the fossils of marine mammals found in the Makah Formation, particularly some of the earliest known fossils of baleen and toothed whales.Figure 8
Magnetic stratigraphy of the coastal section between Shipwreck Point and the mouth of the Sekiu River. Conventions as in Figure6.The entire section is a reverse polarity magnetozone. Based on the early Zemorrian foraminifera from this unit as well as mollusks from theLiracassis rex  Zone (Figure 10), the best correlation of this reverse polarity section is with Chron C12r (30.0–33.0 Ma), based on similar magnetobiostratigraphic patterns observed in the Ozette Highway section (Figure 7) as well as the pattern shown in the Lincoln Creek Formation of the southeastern Olympic Peninsula [17]. The oldest known baleen and toothed whales from this region are found near the base of the Jansen Creek Member exposures along the beaches east of Shipwreck Point [22], so these fossils are early Chron C12r in age, or earliest Oligocene (about 33 Ma).


## 5.4. Hoko River Formation Type Section, Hoko River-Ozette Highway

The best exposures of the Hoko River Formation are found along Ozette Highway and the Hoko River, just south and down-section from the Ozette Highway Makah sections described above. The section closely follows that of Snavely et al. [24, Figure 10] (Figure 9). Although this is the type section, the exposures are now extremely poor, and only five discrete sites could be taken spanning the 1600 m of section reported by Snavely et al. [8]. The lower four sites (spanning almost 1200 m of section) are reverse polarity; the uppermost site (site 15) is the only normal polarity site.Figure 9
Magnetic stratigraphy of type section of the Hoko River Formation along Ozette Highway. Stratigraphy after Snavely et al. [24, Figure   10]. Conventions as in Figure 6.Figure 10
Correlation of the three Makah sections, based on the dates and age constraints discussed in the text. Lincoln Creek Formation magnetostratigraphy after Prothero and Armentrout [17]. Time scale after [15, 56].Correlation of the type section of the Hoko River Formation is less straightforward than the correlation of the Makah Formation (Figure10). Based on the late Narizian benthic foraminiferal fauna, the long reverse magnetozone could be correlated with the relatively short Chron C17r (38.0–38.2 Ma) or the much longer Chron C18r (40.0–41.2 Ma). Because there is 1200 or more meters of reverse section in this sequence, we prefer the latter correlation. However, if the Hoko River Formation interfingers with the underlying Lyre Formation, then it is more likely that the correlation with Chron C17r is correct because the Lyre River Formation is correlated with the same interval (Prothero et al., [59]). Without planktonic microfossils or some sort of isotopic age determination, it is not possible to provide a more robust correlation on the Hoko River Formation.


## 6. Tectonic Rotation

The interpreted counterclockwise tectonic rotation described was unexpected because most inferred crustal rotations reported on the basis of paleomagnetic data from western Washington are clockwise in sense (Figure11). These results include the middle Eocene Humptulips Formation in the southwestern Olympics [57, 58], the Oligocene Blakeley Formation on Bainbridge Island due east of the Olympics [60],  the Oligocene-Miocene Pysht Formation [27] and Clallam Formation [61]. The underlying lower Eocene Crescent Formation, to the south of the Pysht and Clallam Formations, also shows a slight clockwise rotation [62]. However, it is consistent with several other results. Irving and Massey [63] reported a slight counterclockwise rotation for the Eocene Metchosin volcanic rocks of southern Vancouver Island, British Columbia, confirming an earlier result by Symons [64] on the Sooke Gabbro. Our 2002 sampling and analysis of the overlying Oligocene Sooke Formation [65] also showed that the region has been rotated in a counterclockwise sense. All of the 21 Sooke Formation sites are of reverse polarity, so the characteristic remanence  of this formation is clearly not an overprint. Sites from the Sooke Formation showed about 30° of counterclockwise rotation with respect to Oligocene cratonic poles. Beck and Engebretson [66] reported a slight counterclockwise rotation for the Eocene volcanic rocks of the Port Townsend area in the northeastern Olympic Peninsula. Our sampling and analysis of the Eocene-Oligocene Lyre River, Quimper, and Marrowstone Formations of the Quimper Peninsula in the northeast Olympics (Prothero et al., [59]) also yielded a counterclockwise rotation. These rocks yielded both normal and reverse polarity magnetizations, which passed a reversal test  and resulted in a formation mean direction of  D=308.4, I=51.0, k=6.7 and  α95=9.5.Figure 11
Sketch summary of the paleomagnetic data from lower Cenozoic units in the Olympic Peninsula. M = Makah Formation; S = Sooke Formation; SG = Sooke Gabbro; Q = Quimper Peninsula units; PT = Port Townsend basalts; BR = Bremerton basalts; BH = Black Hills; WH = Willapa Hills; GV = Goble volcanics (modified from [62]).The pattern of tectonic rotations (Figure11) within the Olympic Peninsula is now much more complicated than previously thought. Except for the Pysht and Clallam results, and the data from the Crescent Formation to the south, all other rocks on the north flank of the Olympic Peninsula show a counterclockwise rotation. Beck and Engebretson [66] reported no net rotation of the Eocene Bremerton volcanic rocks, east of the Olympic Mountains. All paleomagnetic data south and southeast of the Olympic Mountains, including the Blakely Formation, the Humptulips Formation, and many earlier results on Eocene rocks south of the Olympics [67–73] show a consistent clockwise rotation. A tectonic model that might explain these results is in progress. Dr. Mark Brandon (pers. commun., 2009) currently thinks that a model in which the Olympic block pushes eastward, rotating its north flank counterclockwise and its south flank clockwise, might be able to explain most of the available data.



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*Source: 930612-2009-06-04.xml*