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Geology Rocks – 2019 Classic

Ian Madin has worked as a geologist with the Oregon Department of Geology and Mineral Industries for nearly 30 years. In his spare time he enjoys riding with Cycle Oregon and sharing stories about the incredibly cool geology of Oregon.

Day 1: Greens and Glaciers

Figure 1. View to the west of deep, “U”-shaped glacial valleys where the North Fork of the Middle Fork of the Willamette (left) and South Fork of the McKenzie (right) meet. The ice was flowing from the bottom of the image towards the top.

On Day 1, we will be riding through the poorly exposed volcanic rocks of the Western Cascades as we ascend the North Fork of the Middle Fork of the Willamette.  We will start out riding in a deep, steep green canyon, like Brice Creek or Canton Creek on later days, but about the time we get to our snack stop at Kiahane Campground, the terrain will change dramatically, as we enter a wide valley with a flat bottom.  This valley, and the upper reaches of the South Fork of the McKenzie, have both been carved out by glaciers descending from the High Cascades (figure 1).  In Figure 1, you can clearly see the broad “U” shape that is characteristic of glacial valleys.

Day 2: Fire and Ice

Figure 1. Overview of Day 2 route. We will start in the broad valley of the McKenzie River, then turn up Lost Creek and the White Branch of Lost Creek, then climb to McKenzie Pass through  miles of barren lava before descending to Sisters and Tumalo State Park.

On our second day we will travel through some of the most dramatic and dynamic geology in Oregon, and the scenery isn’t half bad either. The good news is that you will be riding slowly and steadily uphill through most of the best geology and scenery, so you will have plenty of time to take it in.

Before we leave Rainbow, you should walk down to the McKenzie River at least once. You will be amazed by the clarity of the water, and we will see similar crystal waters in the upper reaches of the North Umpqua.  Many of the Rivers flowing out of the High Cascades have this beautifully clear water. Most of the rocks in the High Cascades are lava flows of various types, but almost all are very porous and very permeable. Porous means that there is a lot of space for water in fractures and openings in the rock, permeable means that those spaces are connected, and water can easily flow through. As a result, much of the heavy snow and rain that falls here every year simply percolates into the ground and fills a giant volcanic sponge instead of running off across the surface.  The water travels through the rocks to emerge in large springs which feed rivers like the North Santiam, McKenzie, North Umpqua, Deschutes and Metolius. Lost Creek and the White Branch both disappear into the porous lava for many miles. If you have time on your way home, take a hike along the McKenzie near the Blue Pool, or stop at Clear Lake at the head of the McKenzie and hike over to the Big Springs that feed the lake.

Figure 2. Lidar perspective view to the east, showing our route up McKenzie Pass. As we ride up the glacier-carved White Branch valley, we will cross numerous active faults, ride along one of the youngest lava flows in Oregon, and switchback up to cross the pass through a raw landscape of barren lava.

On our way up McKenzie Pass, (Figure 2) we ride past glacial valleys and moraines, dozens of active faults, cinder cones and lava flows only a few thousand years old, all under the shadow of some of the most spectacular High Cascade Volcanoes. The landscape is shaped by the powerful forces of volcanism and glaciation interacting in the very recent past.

20,000 years ago, most of the highlands along the route were completely covered by an ice cap, and the White Branch and nearby valleys filled with thick glaciers.  What remains are glacial moraines, glacier scoured lava flows, and deep “U” shaped glacial valleys. In Figure 3, you can see the classic “U”-shaped profile of the glacial valley; steep straight valley walls and broad flat valley floor.  Most of the high plateau above the valley consists of pre-glacial (but still very young) lava flows that were scraped and scoured by the flow of ice across them. This leaves a surface that is not as rough and chaotic as the fresh lava flows, but still retains a very irregular surface, typically dotted with small meadows, ponds and lakes.  Although we will not be able to see them from the road, we will be passing an incredible set of glacial moraines as we ride up the White Branch. Rock debris gets incorporated into flowing ice, and where the ices melts away along the glacier front and edges, the debris accumulates into piles called moraines. On the south wall of the White Branch valley, and in the highlands on either side, there are beautifully preserved sets of nested moraines, which appear as sets of parallel linear ridges.  These record a progressive decline in the extent of ice, with each moraine formed during a period of relative stability, followed by a new and lower moraine after the ice has receded a bit and temporarily stabilized. These types of nested moraines only form when the ice is retreating, if the ice advances, it obliterates all earlier moraines.

Figure 3. 3D perspective lidar view of the White Branch valley showing the “U”-shaped valley profile, glacier scoured lava flows, nested glacial moraines, and active faults.

The highlands on either side of the White Branch glacial valley are sliced by dozens of active faults. These features were completely unsuspected until they were revealed by lidar collected in 2016.  The faults run north south, and must have moved recently, because they cut across moraines that formed during the last glaciation, which ended 20,000 years ago. The most spectacular of these faults creates a 45-foot high wall across the landscape.  Geologists have just begun to study these faults to learn their history, but they are some of the most impressive in Oregon.

Figure 4. 3D lidar perspective view of the switchback section of McKenzie Pass.  The Collier Cone lava flow fills the valley here, impounding Linton Lake. The flow shows excellent example of flow levees.

Shortly after our morning snack stop, we will encounter the snout of the Collier Cone lava flow. Collier Cone is a cinder cone on the north flank of the North Sister that produced several fluid lava flows 1500 years ago.  One flow found its way into the head of the White Branch and cascaded down into the valley, partly filling the upper reaches. From the road it will appear as a huge wall of lava rubble on your right, and there is a very short hike that will take you on to the surface of the flow, but to really see the cool features, we need to look at the lidar image in Figure 4.  The flow has many short lobes, that look rather like molten wax flowing off a candle. It also has pronounced levees along the edges. These are formed when the rate of flow decreases, and the fluid lava drains away from the frozen edges. Sets of nested levees show that there were numerous pulses of lava. Linton Lake, across the flow from the highway, was formed when the flow blocked a side valley.

At the top of the switchbacks we will pass Sims Butte, a post-glacial cinder cone, and after a few miles we will enter a stretch of lava barrens that extend all the way to the top of the pass at the Dee Wright Observatory.  These young lava flows came from Belknap Crater to the left, and from Four in One, Yapoah and Collier cones to the right. Most of these flows erupted about 1,500 years ago and their rough, rubbly surfaces have changed little since then.   This is a very hostile environment for vegetation because there is no soil so that snowmelt and rainfall disappear into the porous lava, leaving little to support trees or shrubs.

Figure 5. Lidar (above) and Google Earth (below) views of the McKenzie Pass area, showing the young lava flows and vents.  Most of this bare lava is only 1500 years old.

The highway through the lava fields provides excellent views of the North and Middle Sisters to the south.  The North Sister (10,085 ft) was built by eruptions between 45,000 and 140,000 years ago, while the Middle Sister(10,047 ft) is only 20,000 to 25,000 years old.  Both are heavily eroded by glaciers, but the glaciers are rapidly retreating, and may soon disappear altogether as our climate warms. The Collier Glacier, which occupies the north side of the North Sister, extended nearly to Collier Cone in the early 1900’s. It has retreated about a mile since then.  To the north you will see Mt. Washington (7,790 ft), the eroded stump of an older volcano, and Mt. Jefferson (10,496 ft) which was largely built over the last 100,000 years, with the most recent eruptions 15,000 years ago.


Day 3: The Young and the Restless

Figure 1. View to the north of the route of Day 3.

Our ride today starts in the sagebrush and Juniper forests of the central Oregon high desert. For the first dozen miles we will skirt the western edge of Bend, across a broad plateau that slopes gently to the east and is interrupted by small canyons coming down from the High Cascades to our west. This plateau is made of a mix of river sediment,  glacial deposits and lava flowing off the Cascades. Under these young rocks are older layers of volcanic ash and pumice. The terrain is subdued, so we won’t see much in the way of rocks. We also won’t see a series of faults underneath our tires (Figure 2). Although they won’t be obvious when we cross them, these faults show up as straight steps in the land surface that run for miles across the plateau. Part of the Tumalo fault zone, they have probably been active in the last 10,000 to 20,000 years, and may pose a significant seismic threat to Bend and nearby communities.

Figure 2. Faults of the Tumalo fault zone break up the plateau we cross in the morning. The black arrows point to three of the more prominent faults visible on this lidar image.

Pumice was mined at several sites along this part of the route, but the mines have been closed and in many cases reclaimed for suburban development. Most pumice is used for making lightweight concrete, like the familiar cinder block.

Figure 3. Lidar imagery looking to the NE along the chain of craters that form the Mt. Bachelor rift. In addition to the numerous small cinder cones, you can see the highly irregular surface of the lava flows that came from the rift.

We will turn west and begin the climb up the Cascade lakes Highway towards the High Cascades and Mt. Bachelor. The forest will start to change to huge, red-barked Ponderosa pines as we climb, which eventually give way to scrawny lodgepole pines as we near Mt. Bachelor. We will get great view of Mt. Bachelor as we ride, though at this time of year it may be a dull brown cone with only a few hints of the snow cover that makes it such a great winter sport destination. Mt. Bachelor is a 9,068 ft high stratovolcano, composed of layers of volcanic cinder and lava. The mountains original cone shape is well preserved, because it was formed about 9,500 years ago, after the last major glaciation, and has seen little glacial erosion. The eruptions that formed Mt. Bachelor were part of a larger rift eruption; a series of volcanic vents that formed along a 15 mile-long fault. If we strip away the forest with lidar imagery (Figure 3) you can easily see the dozens of small cinder cones that make up this chain of craters. These eruptions build cinder cones by spraying fluid lava in the air, which freezes into small bits and falls back to pile up in a cone. More fluid lava wells up out of the rift and flows across the landscape, leaving intricate multi-lobed flows.

Figure 4. Active and abandoned meanders of the Little Deschutes River. Image from DOGAMI 2013 Lidar Calendar
Figure 5. Lava Butte cone and flow. The far end of the flow blocked the Deschutes River. Image from DOGAMI 2011 Lidar Calendar

After we turn onto Forest Road 45 we will descend along the edge of the young flows from the Bachelor rift, but the forest will obscure most of the geology. We will see a nice cinder cone on our right shortly after we make the turn. As we arrive in the Sunriver area, we will cross the Deschutes River and then turn right to ride up the Little Deschutes River. The climb will be very gentle, because the valley here is very flat, as a result, the rivers form contorted looping meanders (Figure 4). The reason that the valley floor here is so flat is that 6,000 years ago, an eruption at Lava Butte (Figure 5) blocked the Deschutes river, forming a series of falls and cascades, and causing the valley upstream to fill in with sediment, which in turn made the rivers meander. The cinder cone at the vent for the Lava Butte flow has a great visitor center and opportunities for hikes around the cone and flow.

Figure 6. Perspective view to the West across Newberry caldera. Several young lava flows are obvious, like the Big Obsidian Flow, and all were the result of eruption of thick pasty lava, resulting in a “cow pie” appearance. The cinder cone just visible at the lower left is one of dozens that dot the flanks of this huge volcano. The curved ring fracture at the bottom of the image is part of the fracture system that formed when the caldera collapsed during a major eruption 75,000 years ago. You can see a where a small lava flow erupted from the fracture right above the word “Ring”, and flowed down into the caldera floor.

As we ride up the Little Deschutes River to La Pine, the low forested mountain on our left is Newberry Volcano. Newberry is the largest active volcano in the Cascades, but has a very different character than the more familiar snow capped cones like Mt. Bachelor or Mt. Hood. Mt. Hood rises 7000 feet above the surrounding terrain, and has a footprint of about 75 square miles; Newberry stands only 3,400 feet above the surrounding terrain, but covers an area of over 500 square miles. Newberry is a shield volcano, which is formed by eruptions of very fluid basalt lava. The lava flows so easily that it spreads our rapidly and doesn’t build a steep cone like most of the Cascade volcanoes. One lava flow from Newberry traveled over 40 miles to reach the Crooked River north of Bend.

Figure 7. The central Pumice Cone in Newberry caldera. After building a cone of pumice fragments during the beginning of the eruption, this vent squeezed out pasty lava which dribbled out of the side of the cone, and left a mysterious eye in the center of the cone. Steam explosion pits are visible in the lower left corner of the image.

The caldera of Newberry volcano is a fascinating place (Figure 6) and is worth a visit on a future trip (the ride up into the caldera is a great climb). The caldera formed in explosive eruptions about 75,000 years ago, and is filled with two beautiful lakes and many cool volcanic features. The Big Obsidian Flow erupted only 1,300 years ago, and the central Pumice Cone (Figure 7) looks like something out of Mordor. The floor of the caldera is littered with steam explosion pits formed by the heat from the magma that lies near the surface, and both lakes have hot springs in their beds. An exploratory geothermal well in the caldera encountered temperatures of 500 degrees at a depth of 3000 feet, and exploration for geothermal energy continues today on the flanks of the volcano.

Day 4: Lava and Lakes

Figure 1. Our rides on Day 3 and 4 goes through one of the highest concentrations of volcanic vents anywhere. The orange icons mark the locations of young volcanoes.

Today’s ride takes us through part of the Cascades Lakes region before settling in for some long straight slogs down Highway 97 and west to Diamond Lake. Like Day 3, the area we are riding through has a huge concentration of young volcanoes, ranging in size from a cinder cone a few hundred feet across to the 9,000-ft high cone of Mt. Bachelor (Figure 1). In fact, on Day 3 we passed within five miles of 124 young volcanoes, and today we will pass another 101. These volcanoes come in a wide variety shapes and sizes and erupt a wide range of materials; lava, cinders, pumice and ash. The way in which a volcano erupts depends on the chemical composition of the molten rock, or magma, that is rising to the surface. Most volcanic rocks contain iron, aluminum, magnesium, sodium, calcium, titanium, and loads of silica, a compound made up of silicon and oxygen. Although silica is always the most abundant material in volcanic rocks, the amount varies quite a bit. At one end of the range is basalt, which is about half silica. Because of the low silica, basalt erupts at nearly 2,200 degrees F and is very fluid. Rhyolite, at the other end of the range is nearly three quarters silica, and is relatively cool (about 1,200 F) and very stiff and sticky when it erupts. This difference in the fluidity of lava makes all the difference in how it erupts.

Figure 2. Young faults are visible in this Lidar image, and our route crosses two of them. The Lidar image has been tweaked to enhance the visibility of the fault; we probably won’t notice them, because they are subtle steps in the land surface a few feet high.

All magma contains dissolved gasses like water vapor, carbon dioxide and sulfur dioxide. As magma rises near the surface, this highly compressed gas begins to bubble out of the magma. If the magma is basalt, the lava is so fluid when it reaches the surface that the gasses easily escape, often casting spectacular lava fountains. The fountain lava freezes in the air into small bits, called cinders, which rain down and build a cone around the vent. When there is less gas, the basalt lava flows freely away from the vent, behaving almost like water as it flows for many miles. If the magma is rhyolite, huge pressure can build up in the lava as it reached the surface with the gas still trapped in the sticky molten rock. That often leads to spectacular explosions, as all of the gas suddenly expands, ripping the lava body to shreds and blowing it miles in the sky. The gas bubbles in the hot lava expand as the fragments fly through the air, and then freeze into pumice. Magma that falls between these two extremes has a range of eruption styles and we will see many along the way.

As we leave La Pine and head west, we will cross another series of active faults (Figure 2) about 10 miles into the day. This group is part of the La Pine graben, which is a geologic structure that is formed when an area of land subsides between sets of parallel faults, and occurs when the landscape is being stretched. We will also pass by the southern end of the Mt. Bachelor rift, which probably extends beneath our route but is buried by young sediments deposited by the Deschutes River.

Figure 3. The twin lakes are part of a chain of maars, craters formed by eruptions that mix hot magma and groundwater to make explosions driven by steam and volcanic gasses.

We will make a big turn to the south near the Twin Lakes, which have an unusual origin. Natural lakes almost always point to very young and active geology. Lakes fill up with sediment rapidly, so it typically takes some sort of very powerful or rapid geologic process to create one that we see today. Most natural lakes in Oregon were formed when glaciers dug holes in bedrock, or left dams of glacial rubble. The Twin Lakes (Figure 3) have a much more exciting and unusual origin. They are maars, which are volcanic vents that form when rapidly rising magma encounters groundwater very close to the surface. The intense heat causes the water to flash into steam, producing an explosion and leaving behind a crater that fills with water.

Figure 4. The Davis Lake lava flow forms a natural dam that impounds Odell Creek to form Davis Lake. The creek emerges as a giant spring on the downstream side of the dam.

As we turn south past the Twin Lakes, we will cross the Deschutes River, and then in a few miles we will cross over Odell Creek. If you look to the right as you cross the bridge, you will notice that the creek seems to end abruptly at a wall of dark gray lava. This is the Davis Lake andesite flow which erupted about 5,000 years ago. Andesite is a lava type that is intermediate between basalt and rhyolite. In this case the lava flowed, but was sticky enough that it built up in a series of lobes right around the vent (Figure 4). The lava flows slowly enough that a crust of solid rock several feet thick develops, which is then broken as the molten material beneath continues to move. This type of lava flow is called an aa flow, and leaves the surface of the flow a chaotic jumble of sharp jagged blocks. Much of the surface of the flow is still bare lava, and in the last 5,000 years vegetation has only found a foothold on the smoother surfaces of cinder cones near the center. Walking across the surface of an aa flow is very difficult and hazardous. Don’t try in your bike shoes!

Figure 5. The Black Rock and Black Rock Butte lava flows are very young and have incredible flow shapes. Figure from DOGAMI 2015 lidar calendar, ( ) image credit Dan Coe. Our route crosses the upper left corner of the image.

We will ride along the edge of the flow, and arrive at Davis Lake, which is another example of a volcanic lake. In this case the lava flow blocked Odell creek forming a huge natural dam. An aa flow is typically very porous, so the lake actually drains through the flow, emerging on the north side as a large spring.

About 8 miles past Davis Lake we may see another young lava flow about a mile to our left, and then another mile along we will pass right by a similar flow. Both of these lava flows, the Black Rock and Black Rock Butte flow, are also about 5,000 years old.

We soon reach Highway 97 and turn south, and from here the geology is much harder to see. The landscape is very flat and forested, and affords few views. As we leave Chemult we will pass a roadcut 10-20 ft high in which you will see bright white rock fragments of many sizes. This is pumice that came from an explosive rhyolite-type eruption about 7,700 years ago. You will continue to see this white pumice material, sometimes yellowish, from here all the way to camp.

Figure 6. A view to the west along the long straight stretch of Hwy 138. The road is absolutely straight for the first 10.5 miles. Diamond Lake is in the valley between Mt. Bailey and Mt. Thielsen.

About 1.5 miles after we turn onto Highway 138 and begin the long, slow climb up to the pass, you may see a small red cone off to your right. This is one of many small basalt cinder cones in the area. These cones are a common source of gravel and sand that is used to spread on the highways in icy conditions. The cinders are usually loose and easy to dig, and can be easily crushed or separated into the right size for road sanding. Enjoy the sight, because the next 10 miles are one of the longest and most monotonous straightaways you will ever see.

As we near the pass, you may be able to see Mt. Thielsen on your right through the trees. This is another major Cascade volcano that is 9,184 ft high. Eruptive activity ceased here about 250,000 years ago, and what must once have been a very impressive mountain has been ground to a sharp point by several periods of glaciation.

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1 Comment

  1. Awesome, I can’t wait to see all of this. If you can recommend a book about the geology of this area that I could read before I come visit that would be great, maybe something similar to “Annals of the Former World”. I’m a flatlander from the craton of Michigan.