The previous chapter may be found here.
Relief map of the Jemez with El Alto (north), Servilleta Basalt (northeast), Cerros del Rio (southeast), and Santa Ana Mesa (south) outcroppings highlighted in red
We've had some encounters with basalt already. It is the main rock type of the early Lobato Mesa Formation, and it is also found in the Paliza Canyon Formation. However, some of the best exposures of basalt are more recent and are located around the periphery of the Jemez volcanic field. The most voluminous of these is the Cerros del Rio field, but there are similar basalt flows at Santa Ana Mesa and at El Alto.
Basaltic lava is low in viscosity and can easily flow for miles from its source vent. As a result, it tends to form flat plateaus rather than high peaks. These are often quite distinctive in aerial photographs, as the previous Google Map links showed. The basalt flows we will be examining in this section all erupted as the higher-silica Tschicoma eruptions of the Sierra de los Valles were beginning to wind down. The Cerros del Rio dates from about 4.6 to 1.6 million years ago, peaking at around 3.2-2.4 million years ago; Santa Ana Mesa is about 2.5 million years old; and the El Alto flows are around 2.8 million years old.
The pattern of basaltic volcanism around the periphery of an existing felsic volcanic field is seen in other parts of the world, such as the Yellowstone caldera. One explanation for this pattern is that fresh basaltic lava rising from depth is blocked by the great mass of viscous magma in the magma chamber at the heart of the volcanic field. Because this high-silica magma has a relatively low density, the higher-density basaltic lava stagnates underneath it. However, the basaltic magma can reach the surface further out, where the magma chamber has not yet developed, the rock is colder and denser, and the magma can find clear paths to the surface through faults.
The Servilleta Basalt erupted in the Taos area from 4.8 to 3.7 million years ago, about the same time as the oldest Cerros del Rio basalts. Though it is not part of the Jemez volcanic field, this voluminous formation includes the massive flows underlying Black Mesa, north of Espanola.
Black Mesa north of Espanola
A major system of faults runs along the visible south face of
this mesa, which offsets the Rio Grande Rift to the east north of
Espanola. Southeast of these faults is the Velarde Graben, the
deepest portion of the Rio Grande Rift in the Espanola Basin.
The most voluminous of the basaltic formations erupted during this time period is the Cerros del Rio Formation. This is exposed as a large plateau east of the Rio Grande and south of White Rock, but there are numerous exposures west of the Rio Grande that suggest that the Cerros del Rio Formation extends for some distance northwest beneath the younger Bandelier Formation. Drilling on the Pajarito Plateau has brought up basalt resembling Cerros del Rio basalt as far northwest as a well more than halfway from White Rock to the Sierra de los Valles, and it is thought the formation may extend almost to the Pajarito Fault east of the San Miguel Mountains. However, the Bandelier Formation rests directly on Paliza Canyon andesite in upper Los Alamos Canyon, showing that the formation does not reach this far.
Because the Cerros del Rio is the largest of the peripheral basalt fields, and because it is the only one that is located mostly on public lands, I will describe it in some detail.
The earliest eruptions in the Cerros del Rio field likely took the form of maars. Maars are formed when magma rising from below comes into contact with an aquifer saturated with water. The water flashes into steam, blowing the country rock and magma into small fragments that settle around the vent to form a distinctive very shallow crater. Unfortunately, none of the maars in the Jemez area are young enough to be well-preserved as surface features, but the early maars of the Cerros del Rio probably looked something like Menan Buttes in southeastern Idaho.
North Menan Butte, an example of a young maar. 43 47.100N 111 58.607W
Beds of shattered rock and volcanic cinder produced by the interaction of groundwater with magma are described as phreatomagmatic, from the Greek phrear, "spring" or "well". Here are some of the phreatomagmatic beds around North Menan Butte.
Cinder beds at North Menan Butte, an example of a young maar. Near 43 47.100N 111 58.607W
Here's a sample of the phreatomagmatic beds.
The presence of several maars in the Cerros del Rio suggests that
this area was close to the ancestral Rio Grande three to four
million years ago, so that the country rock was well saturated
with groundwater. The associated phreatomagmatic beds usually lie
directly on Santa Fe Group sedimentary beds and are usually buried
under later Cerros del Rio lava flows.
The most accessible of these beds for the casual explorer are on the west slopes of Buckman Mesa, which is prominent as seen from State Road 502 at the northern entrance to White Rock Canyon.
Buckman Mesa at the northern end of
White Rock Canyon. Looking south from 35.876N
The mesa is capped with thick beds of andesite and basaltic andesite. Peeking out under these are beds mapped as phreatomagmatic deposits. Presumably the vent was Otowi Peak, which sits on top of the mesa to the right, and where the phreatomagmatic beds reach their greatest thickness.
If one wishes to view a maar deposit close up, there is no better
place than lower Frijoles Canyon in Bandelier National Monument.
The Upper Falls Trail provides a fairly easy hike from the
visitors' center to some impressive maar beds.
A closer look:
The maar deposits are overlain by thick flows of benmoreite,
which is sodium-rich trachyandesite. Trachyandesite, like
trachybasalt, is unusually rich in sodium and potassium, and like
andesite, it is slightly richer in silica than basalt.
Potassium-rich trachyandesite is known as latite, and we saw
examples from the Espinaso Formation earlier in the book.The
benmoreite at Upper Falls has a radiometric age of about 2.75
Of course, we can't leave Upper Falls without looking at the falls!
So if there is an Upper Falls, is there a Lower Falls? Yes, here. Alas, recent forest fires in the Jemez have resulted in violent flash floods in Frijoles Canyon, and these have completely erased the trail below Upper Falls.
You may have noticed the rusty color of much of the maar deposit and the overlying basalt. This is particularly pronounced at one point on the trail just above the falls.
The red color comes from hydrothermal alteration of the benmoreite. The hot rock in the vent near here continued producing steam from the aquifer for some time after the initial eruption, which reacted with the iron minerals in the benmoreite to produce red hematite.
Another maar deposit is found at Cochiti Dam, right next to the
main outlet channel.
Tuff ring deposit at Cochiti Dam. 35.617N 106.322W
The grayish beds to the right in the photograph are a remnant of a tuff ring, which is the deposit immediately around a maar crater. The tuff contains numerous quartzite clasts probably derived from river gravels deposited here by the ancestral Rio Grande.
A particularly large maar is located at the foot of Montoso Peak
on the east rim of White Rock Canyon.
View from north rim of Montoso Maar. 35.765N
Montoso Maar is likely one of the oldest parts of the Cerros del Rio. The thick maar beds here were subsequently buried by more sediments and by thick basalt flows from Montoso Peak. When the Rio Grande cut the canyon to the west, the maar was exposed, and the relatively soft maar beds have since mostly eroded out.
Montoso Peak itself is on the skyline to the left, and its flows extend across the center of the panorama. To the right, we see the far rim of White Rock Canyon, with Bandelier Tuff sitting on top of Cerros del Rio Basalt sitting on top of Santa Fe Group sediments. The mouths of several tributary canyons to White Rock Canyon are visible. Beyond are the San Miguel Mountains and the Sierra de los Valles west of Los Alamos. You can see one of the technical areas of Los Alamos National Laboratory on top of the mesa, with a large VLA dish radio telescope. The tributary canyon to the right of the mesa is Ancho Canyon.
Note the junked appliance in the foreground at right. Geologists sometimes refer to such deposits as “locally-derived anthrogenic colluvium”, or, when it consists of automobile parts, simply as “Detroitus.”
Here’s a closer look at the maar beds.
View from north rim of Montoso Maar. 35.765N
Notice the great thickness of the beds, over a hundred meters in this area. This must have been a truly enormous maar, though not as large as the enormous Seward Peninsula maars in Alaska, which are over three hundred meters thick.
Eventually the maar eruptions transitioned to cinder code
eruptions, as the supply of ground water was depleted (either
through the aquifer being sealed off or the ancestral Rio Grande
shifting away from the maars.) Otowi Peak, which we saw earlier,
seems to have started as a maar and transitioned to a cinder cone.
Another cinder cone remnant is visible in the east wall of White
Rock Canyon directly across from the village of White Rock, where
it has been cut in half by erosion.
Eroded cinder cone viewed from 35.810N 106.201W
You can see that some of the beds here are a bit lighter than the usual dark basalt beds of White Rock Canyon. The cinder cone appears as a low area in the canyon rim, probably because later flows ponded around the cinder cone, which was subsequently mostly eroded away to leave a depression. This is unmistakable in the overhead satellite view.
The cinder cone most accessible for close examination is located
along Forest Road 56, where it ascends onto the Cerros del Rio
Plateau from the east. Here the road cuts through this small
Cinder cone in road cut. 35.617N
The dip on the beds strongly suggests that the area just left of the car is a breach in the cinder cone wall. The breach is now filled with sediments and blocks of the overlying lava, which forms a thin bed over the cider cone.
Here are the beds close up.
Cinder cone in road cut. Car keys at
lower left for scale. 35.617N
These are very typical cinder beds, thrown up around a vent where blobs of basaltic lava were blasted into the air as gas escaped from the lava, with the blobs cooling in the air before landing around the vent. Such vents often also have a flow of degassed lava emerging from the base of the cinder cone, but here the flow likely would have been to the northwest, and is now buried under later flows.
The cinder has some commercial value. Apparently the breach here was actually excavated for cinder and is not a natural feature. Further up the road, there are two large cinder quarries, one active. The inactive quarry has a locked gate, but can be viewed from a nearby hill.
Inactive cinder quarry. 35.620N
The cinder is here oxidized to a deep red. The color makes coarse cinder valuable as decorative stone, and finer cinder is used on highways to improve traction.
Following the maar phase of the Cerros del Rio field, basalt magma continued to rise from the depths. The magma would have shot out of the vent with considerable velocity, driven by the formation of gas bubbles in the magma as it approached the surface. Some of the bits of lava cooled while still in the air, falling to the surface as solid cinder that built up a cinder cone around the vent. However, most of the magma, still liquid but now free of gas, pooled around the vent and began flowing away from the cinder cone, often for miles. Repeated eruptions of this nature from multiple vents built up the plateau of the Cerros del Rio.
The flows show a fairly consistent chemical stratification,
particularly around White Rock Canyon and to the west. The
lowermost flows tend to be composed of alkali-enriched rocks such
as benmoreite, hawaiite, and mugearite, which correspond in silica
content to basalt, basaltic andesite, and andesite, but are
enriched in sodium. The upper flows tend to be tholeiitic basalt,
rich in aluminum and poorer in alkali metals. This pattern is seen
in at least two separate pulses of activity, at 2.8 Ma and at 2.3
to 2.6 Ma.
The layers of basalt flows making up most of the Cerros del Rio
Formation are best examined around the perimeter of the plateau.
Because the basalt is far more durable than the underlying soft
sediments of the Santa Fe Group, erosion has created an escarpment
around nearly the entire perimeter of the Cerros del Rio. Only
along a short stretch of the eastern perimeter is the escarpment
low enough for easy access by vehicle.
We'll begin our tour of the perimeter of the Cerros del Rio at
Overlook Park on the west rim of White Rock Canyon.
White Rock Canyon is part of the valley of the Rio Grande River, which has cut through the Cerros del Rio Formation into the softer sediments of the Tesuque and Chamita Formations underneath. This produces spectacular cliffs and large landslides where parts of the basalt plateau have broken loose and slid down into the canyon.
At far left are mesas of light-colored Bandelier Tuff sitting on
a plateau of much darker basaltic andesite of the Cerros del Rio.
Black Mesa is visible to the right, in the far distance. It is
likely a far northern outlier of the Cerros del Rio field. To its
right in the middle distance is Otowi Peak sitting atop the
basaltic andesite of Buckman Mesa, which we saw from a different
angle earlier in this chapter.
Next comes the mouth of Canada Ancha, with exposures of Chamita and Tesuque Formation beds of the Santa Fe Group. This area is the location of the ghost town of Buckman, and now contains several wells supplying water to the city of Santa Fe.
The rest of the panorama show upper White Rock Canyon, with its
rim of basalt and basaltic andesite overlying Santa Fe Group
sediments. This includes the cinder code we saw earlier. The
skyline above the cinder cone is underlain by thick flows of
andesite erupted from the Ortiz Mountain center, whose peak is
hidden to the south. This is one of the younger flows of the
Cerros del Rio, with a radiometric age of 2.32 million years.
At far right is Montoso Peak, which is underlain by basalt with a radiometric age of about 2.59 million years.
While the eastern rim of White Rock Canyon forms the western escarpment of the Cerros del Rio Plateau, lava flows of the Cerros del Rio Formation are also present along the entire western rim of White Rock Canyon. The western boundary of the Cerros del Rio Formation is buried under younger tuffs of the Bandelier Formation west of White Rock, as we noted earlier. After we've completed our tour around the Cerros del Rio Plateau, we'll comer back and look at some of the outcroppings of Cerros del Rio Formation west of the Rio Grande.
There are two trails into White Rock Canyon from the village of
White Rock, the Blue Dot Trail and the Red Dot Trail. They are so
named because the trails are marked with paint spots of their
respective colors. The Blue Dot Trail is a fairly steep trail from
canyon rim just south of Overlook Park down to the level of
the Rio Grande. It is also well maintained, with such features as
Achh, ssss, it's the only way yes Precious ... 35
49.430N 106 11.008W
After the initial descent down the basalt cliffs, the trail comes out on a slump block. The landslides in the area unfortunately conceal the contact between the Cerros del Rio Basalt and the underlying Santa Fe Group, but the presence of large amounts of tan sediments in the landslides shows that this slump block is already below the level of the contact.
The terrain here is level enough to set up camp, and I have actually camped overnight with my son's Boy Scout troop here, at roughly the spot shown in the center of the photograph. Note the considerable amount of well-rounded clasts along the trail; these match a similar gravel bank on top of the rim adjacent to this point, deposited as a gravel bar from one of the lakes formed when eruptions in the Cerros del Rio dammed the ancestral Rio Grande River.
If one detours well off the trail, continuing south along the slump block, one sees what looks very much like an eruptive center, underlying the gravel mesa described in the previous section. This cannot be spotted from above, but is only visible from the slump block well off the trail.
Why do I think this is an eruptive center? Well, for one thing, the rock here is much lighter than the surrounding rock, and close examination suggests that this is because it is more coarsely grained than the surrounding basalt -- almost like a diabase.
For another, the rock is foliated in a way that looks like a subsurface dome. I'm not sure these photographs do it justice.
It's a bit of a subtle thing, but the texture of the rock is
different here from anything I've seen anywhere else in the
canyon. However, it resembles the benmoreite outcroppings around
Upper Falls in lower Frijoles Canyon. The relatively high
viscosity of this magma could explain why the rock here formed a
plug rather than flowing easily from the vent.
The sheer cliffs forming the rim of White Rock Canyon are
ideal for rappelling, and one finds rope anchors at scattered
points along the rim, which are readily accessible from the Rim
The rock into which this anchor has been sunk is described in the most recent paper on the Cerros del Rio as hawaiite. This is a sodic trachybasalt found throughout the Cerros del Rio. A trachybasalt is a basalt that is high in sodium and potassium, and a sodic trachybasalt has significantly more sodium than potassium.
Most of the rocks of the Cerros del Rio are somewhat alkaline, so that some of the basalt is actually trachybasalt and some of the andesite is actually trachyandesite. This is typical of mafic rocks produced by continental rifting like that along the Rio Grande Rift. It reflects a low degree of partial melting of undepleted mantle.
It is very common for a thick basalt flow, as cools and
contracts, to fracture into roughly hexagonal columns. You
can see the tops of such columns in this photograph, which looks
down on a portion of the basalt flow that has slumped into the
Further south along the Rim Trail a branch of the rim trail affords a view into the confluence of Pajarito Canyon and White Rock Canyon. Here an intermittent stream has carved a very deep canyon into the thick basalt flows.
The basalt is several hundred feet thick at this location, much thicker than in most of the canyon. Here's a view from below, from along the Red Dot Trail.
Confluence of Pajarito Canyon and White Rock Canyon. Looking north from near 35.808N 106.198W
Most likely, the basalt here fills a paleocanyon coincident with the present-day Pajarito Canyon. This closer view shows that there are at least four distinct flow units in the basalt.
Thick basalt flows at confluence. Looking north from near 35 48.550N 106 11.919W
At the base of this thick section of basalt is a bed of cinder.
Cinder bed at confluence of Pajarito Canyon and White Rock Canyon. Looking northeast from near 35.810N 106.199W
The reddish color represents oxidation, either at the time the
cinders were deposited or when the overlying basalt was deposited.
The darker color near the top of the bed suggests baking by the
overlying basalt flow, but such baked zones are usually quite
thin. Perhaps both processes were at work here.
There is a very distinct ledge in this area, formed by the boundary between two successive basalt flows. The boundary is visible in this photograph as a horizontal joint near the top of the cliff to the right of center.
The ledge is formed when the top flow is eroded away to expose the flow underneath, which is apparently slightly more resistant. One can see ropy patterns on the top of the lower flow, typical of pahoehoe flows.
This kind of preservation of an original flow surface is rare in White Rock Canyon, occurring only where relatively recent erosion has exposed a lower flow that was previously protected from the elements by an overlying flow. Here is a close up of the boundary between the upper and lower flows.
This area also has a number of petroglyphs, which we'll discuss later in the book.
Here's a view from further south in White Rock Canyon, at the trailhead of the Red Dot Trail.
White Rock Canyon viewed from 35.810N 106.201W
The cinder cone in the canyon wall now appears at left in the
panorama. Towards the right is a cliff of light-colored Bandelier
Tuff laid down in a paleocanyon in the Cerros del Rio. This may be
the cliff from which the canyon gets its name. At far right is
Montoso Peak in the distance.
Here's a closer look at Montoso Peak and the canyon to its north.
White Rock Canyon looking south from 35.810N 106.201W
In the middle distance, a large shoulder of basalt is visible on th east side of the canyon. The peak behind and to the left of Montoso Peak is Cerro Micho, which is underlain by andesite 2.76 million years in age. The cone at the extreme left in the photograph is an outlier of Cerro Micho underlain by basaltic andesite that is slightly younger, at 2.73 million years in age.
The Red Dot Trail is another well maintained from the canyon rim in the Pajarito Acres subdivision to the river. The basalt cliffs are particularly impressive here.
Cliffs above Red Dot Trail. Near 35 48.508N 106 12.097N
Cliffs crossed by Red Dot Trail. Looking west from near 35 48.548N 106 12.019W
The furthest point south in White Rock Canyon that is easily
accessible from White Rock is near the mouth of Potrillo Canyon.
White Rock Canyon panorama showing tongue of Bandelier Tuff perched in paleocanyon. Looking east from 35.789N 106.210W
The light pink outcrops on the left side of the panorama are the
cliffs of Bandelier Tuff seen in the last panorama. The
pyroclastic flows that produced these cliffs likely flowed down
the ancestral Water Canyon and filled an eastward meander of the
ancestral White Rock Canyon form the beds here. These beds mark
the limit of the Bandelier Tuff to the southeast.
There is a kind of natural amphitheater right of center, formed by landslides. This exposes a great thickness of Cerros del Rio lava flows lying atop beds of phreatomagmatic cinder. The basalt shoulder from the previous photograph is now visible to the left of this natural amphitheater. It is identified on the geologic map as a hypabyssal plug, which cooled at some depth below ground. I am inclined to interpret this as a paleocanyon that was filled to a great depth with lava.
To the right, some distance down the canyon, is a conical hill of basaltic andesite at the mouth of Ancho Canyon. This is likely an erosional remnant of a natural dam that once blocked the canyon at this point, where it is particularly narrow. This dam produced a large lake, which geologists have named Lake Culebra, filling the entire Espanola Valley to the north. Lake bed deposits are scattered across the mesas to the west of the Rio Grande, north of Pueblo Canyon and the main highway to Los Alamos. We'll have more to say about Lake Culebra later in this chapter.
The eroded valley at the foot of Montoso Peak is Montoso Maar, which we saw earlier.
South of its confluence with Potrillo Canyon, White Rock Canyon is largely inaccessible except by boat along the Rio Grande. It was once possible to reach the canyon via a fairly easy hike down Frijoles Canyon from the Bandelier National Monument headquarters, but the trail is now washed out. However, the road into Frijoles Canyon gives one a glimpse of a large cinder cone that was nearly buried under the Tsherige Member.
Cinder cone in TA-33 nearly buried under Bandelier Tuff. Looking northeast from 35 46.617N 106 15.892W
The dark patch of ground is part of the southern summit of the
cinder cone. Note how the lowermost beds of the Tshirege Member
conform to the slope of the cinder cone. This area on restricted
DoE land and is not accessible to casual visitors, but LANL
geologists have dated a dike running through the cone as about
2.55 million years old.
The next point that is still accessible is the area of Cochiti. Here the escarpment bounding the Cerros del Rio becomes particularly spectacular, in part because it coincides with a major fault. Both escarpment and fault bear the name, La Bajada.
The pan begins towards the northeast, looking up the valley of
the Rio Grande. At extreme left are the San
Miguel Mountains, with mesas of Tsherige Member, Bandelier
Tuff, at their feet. La Bajada stretches across the left side of
the panorama with Tetilla
Peak just poking over the skyline near center. Sandia Crest
is on the distant skyline to the right, and Cochiti
Dam crosses the right end of the panorama.
The portion of La Bajada directly to the east is a bit unusual. Close study of the lava flows here shows that one of the flows was erupted recently enough (around 1.14 million years ago by radiometric dating) that La Bajada already existed, and the flow cascaded down the face of the escarpment and pooled on the low ground below.
La Bajada continues south to the canyon of the Santa Fe River, which bounds the southern end of the plateau. This area can be seen from atop Cerro Seguro near La Cienega. )We visited this area in Chapter Five.) This is southeast of the Cerros del Rio and provides a nice panorama of much of the plateau.
Panorama from atop Cerro Seco. 35 34.228N 106 08.263W
The panorama begins with a view to the southwest, towards Sandia
Crest (washed out but just visible in the distance.) The hills in
front are not named on my map, but lie just north of a bend in
Interstate 25 and mark the southern limit of the Cerros del Rio.
The canyon crossing much of the panorama and disappearing into the
horizon at left is the canyon of the Santa Fe River. The hills to
its right are underlain by Ortiz monzonite, which rises like
islands (kipukas) out of the much younger Cerros del Rio Basalt on
the other side of the Santa Fe River. The peak to the right of the
hills is Tetilla
Peak, which dominates the western escarpment of the Cerros
del Rio along the La Bajada Fault. The La Bajada Fault is a
southern extension of the Pajarito Fault.
The flat mesa extending north (right) from the Santa Fe River canyon is Tsinat Mesa, underlain by Cerros del Rio basalt flows.
South of the Santa Fe River canyon is Mesa de Juanita. Though geographically detached from the Cerros del Rio, it is underlain by Cerros del Rio basalt. It is bounded by escarpments to the west and south, but to the east the basalt is buried under alluvial fans of the Cerillos Hills.
The escarpment on the east side of the Cerros del Rio is less dramatic than that on the west side, since the small rivers and intermittent streams here are not as effective as agents of erosion as the Rio Grande. The escarpment is easily scaled and there are numerous petroglyphs in the area.
East escarpment of Cerros del Rio near
La Cieneguilla. 35
36.526N 106 07.398W
This escarpment forms the northeastern boundary of Tsinat Mesa. The rock here is a trachybasalt dated at 2.68 million years old. My geologic map is not so specific, but this is probably hawaiite. The sediments beneath the lava cap are rich in red granite fragments, and are shown on my map as Ancha Formation. The granite came from the Sangre de Cristo Mountains to the east and was probably transported to this area by the ancestral Santa Fe River.
The escarpment is buried under sheetwash further to the north, where the two gravel road access points are located.
Here is a panorama of the northern Cerros del Rio from the northeast.
Cerros del Rio from the northeast. Looking southwest from 35 44.253N 106 04.461W
We’re looking across low hills of the Tesuque Formation at the Cerros del Rio on the skyline. The little knob on the skyline at left is one of the Twin Peaks; the other is lost against background hills to its right. The knob just right of center is Ortiz Mountain, an andesite vent whose flows cover the northern part of the Cerros del Rio.
The escarpment becomes substantial again further north, where Alamo Creek, an ephemeral stream, parallels the eastern escarpment of the Cerros del Rio.
The mesa is capped with Cerros del Rio olivine basalt about 2.5 million years in age. Underneath are thin beds of volcanic cinders and other sediments. These rest on the Ancha and Tesuque Formations of the Santa Fe Group.
Further north, andesite flows from Ortiz Peak reached the edge of
The lower slopes are the Cuarteles Member of the Tesuque
Formation, with possibly a thin layer of Ancha Formation at top;
closer examination would be required to be sure. Then come
alternating beds of sediments and very dark volcanic debris. On
top are very thick flows of andesite, with a a layer of shattered
andesite (breccia) at the bottom of the flow.
Notice how very flat the beds are, including the base of the andesite flow. The Rio Grande Valley was higher in elevation and very flat when the Cerros del Rio began erupting 2.5 million years ago. Since then, changes in the flow of the Rio Grande downstream have caused the river to cut downwards, and sediments not protected by lava flows have eroded away to the new lower level of the river. This process is still taking place, producing the spectacular badlands of this area.
A favorite destination for the adventurous in this area is Diablo Canyon, at the north end of the Cerros del Rio. This area is accessible via Buckman Road from Santa Fe.
Notice the very thick section of basalt to the right, with pronounced columns. This area is described on the latest geological map as a former lava lake. The road in is suitable for passenger vehicles in good weather, and there is an excellent parking area with descriptive signage and a trail, but be warned that the canyon itself is notorious for a large population of rattlesnakes. Keep a sharp eye if you choose to hike the area.
There is some particularly striking columnar basalt just right of center. A closer look:
Columns like this form as the basalt cools, and the joints (formed as the cooling basalt cracks under the thermal stress) are usually perpendicular to the surface of the basalt. This shows that the basalt here was pooled against a fairly steep hill, now partially eroded away.
Buckman Mesa is separated from the Cerros del Rio by Canada Ancha, a wide valley leading to the Rio Grande.
The mesa is named after an Oregon lumberman who loaded his lumber, cut from the Jemez, onto the Chili Line railroad at this location. The area is now a well field for the city of Santa Fe.
Geologically, the mesa is part of the Cerros del Rio, being
capped with basalt and basaltic andesite similar in age to the
other Cerros del Rio flows. There is a large cone, Otowi Peak,
atop the mesa, which is not visible from this perspective. Both
can be reached via a hiking trail from the parking area near the
Rio Grande, though this is poorly marked and very difficult to
find without detailed instructions. The trail affords an excellent
close up view of the beds immediately under the lava cap.
The light tan Chamita Formation beds appear to be full of coarse boulders, but that may be the angle of the sun. There is a very distinct sequence of light gray beds, probably of mixed volcanic debris and sediment, then another distinct sequence of very dark beds that must be mostly volcanic debris, then the brecciated base of the basalt lava flow.
The trail then comes onto the top of the mesa, with Otowi Peak ahead.
With the high escarpments on all sides and the flat mesa top, Buckman Mesa has some of the feel of an island in the sky. The proximity of the Cerros del Rio and the Pajarito Plateau keep it from being a true island in the sky, however.
The mesa top is covered with geologically young deposits of sheetwash and eolium. Sheetwash is what you get when water laden with sediments floods across a flat surface. Eolium is what the wind deposits. This is deeply gullied in some locations.
This particular gully exposes a bed of tuff.
This is a fairly well cemented tuff composed mostly of bits of dark igneous rock in a light tan matrix. It’s what I imagine the stuff just under the basalt flows looks like close up, but this is on top of the flows. The basalt fragments rule out either member of the Bandelier Tuff, and they’re unlikely to be found this far east anyway. I’m guessing that this tuff is the result of Otowi Peak erupting through the basalt capping Buckman Mesa and producing small volumes of phreatomagmatic deposits.
Closer to Otowi Peak, the ground is covered with reddish volcanic cinder.
Otowi Peak itself is mostly cinder, with some blocky lava.
The flank of tte peak is also cut in places by partially eroded
dikes or squeeze-ups.
North of White Rock Canyon, there is an isolated mesa known variously as Black Mesa or Round Mountain by Anglos, as Tunyo Piñ by the San Ildefonso people, and as Mesa Huerfana by the Spanish. This is not to be confused with the much larger Black Mesa north of Espanola.
The other Black Mesa. Looking southeast from near 35.932N 106.120W
Black Mesa is located on tribal lands and has religious
significance to the San Ildefonso Tribe, and so it is off limits
to casual visitors. This is a volcanic neck formed in an eruptive
vent, probably about 2.73 million years ago. The southwest
side of the mesa has visible beds of cinders. These are visible in
the panorama below.
Black Mesa (Round Mesa) seen from the
Black Mesa is the core of a volcanic vent that erupted not quite 3 million years ago. You can see the curved beds of cinders on the right side of the mesa. There are also columns of cooled lava at the base of the cliffs just left of center (click to enlarge).
West of the Rio Grande, the Cerros del Rio Formation is mostly overlain by younger tuffs of the Bandelier Formation, but there are occasional exposures. Some of these are fairly extensive, as at White Rock and in Pueblo Canyon along the main road into Los Alamos from the east.
Bandelier Formation sitting on top of Cerros del Rio Formation on State Road 502 west of Totavi. 35 52.099N 106 11.913W
This particular road cut is iconic. You will see it in almost
every decent book on Jemez geology. At the bottom is a layer of
dark basalt of the Cerros del Rio Formation, which apparently
erupted from a center somewhere to the west (left in this
photograph). On top of the basalt is a very thin layer of lake
silt from Culebra Lake, which formed about 2.46 million years ago
when Cerros del Rio flows dammed the Rio Grande in White
Rock Canyon. There have been a number of lakes north of the
canyon as a result of such damming, which we'll discuss in greater
depth later in the book.
Opposite this road cut is a deep canyon in the Cerros del Rio. At this point, the flows are very thick.
It's rare to see this great a thickness of Cerros del Rio Basalt, and in fact we see a sloping contact further down the canyon with Santa Fe Formation sediments that bring the Cerros del Rio to a more typical thickness.
It's likely that we are seeing where the lava pooled in a deep
Further west, the road takes a short turn north, and from that point the Cerros del Rio is present only on the south side of the canyon. Here it is the topmost unit.
Cerros del Rio Formation in lower Pueblo Canyon. 35 52.090N 106 10.986W
Cerros del Rio Formation in lower Pueblo Canyon
Cerros del Rio Formation in lower Pueblo Canyon
The Cerros del Rio rests here on lacustrine beds (lake bottom deposits) of the upper Puye Formation. In some places, the lava shows signs of having cooled rapidly on contact with water. Note that, in this exposure, the beds seem to dip slightly to the southwest. This assumes I held the camera straight! But if we can trust my inner ear, this suggests that the Diamond Drive Graben extends this far east, and continued subsidence to the west has tilted the beds.
The last photograph shows prominent columnar fractures from the bottom of the flow up, and a more irregular pattern of fractures from the top down. This is a very common pattern in thick basalt flows, and arises from the way the flow cools rapidly from the top and much more slowly from the bottom. The lower columnar part of the flow is called the colonnade, and the irregular top part is called the entablature, by analogy with Greek temple architecture.
The Cerros del Rio continues down the west side of White Rock
Canyon for its entire length. Here's the northern section, seen
from Buckman Mesa across the canyon.
White Rock is visible atop the mesa to the left. The dark Cerros del Rio beds contrast with the light pinkish mesas of Bandelier Tuff resting on the Cerros del Rio.
Across the canyon are some impressive cooling columns.
The great thickness of lava here indicates that it filled a paleocanyon in the Santa Fe Group.
In the next panorama, we look almost directly down the canyon as
it passes White Rock.
The village of White Rock is built on a plateau of Cerros del Rio basalt with a thin covering of sheetwash and eolium deposits. The basalt is best exposed in the La Vista subdivision, which forms a topographic high on the Cerros del Rio surface and may have been an eruptive center. This is close to my neighborhood; my house is built on Cerros del Rio basalt on the west side of Pajarito Canyon.
Cerros del Rio Formation in La Vista area. 35 49.359N 106 13.359W
Cerros del Rio Formation underlying Chez Budge.
Cerros del Rio basalts are also exposed in the confluence of
Water Canyon and Potrillo Canyon and the lower portions of other
canyons of the Pajarito Plateau south of White Rock.
Cerros del Rio basalts in the confluence
of Water Canyon and Potrillo Canyon. 35
47.445N 106 12.712W
At far left and far right are the basalt cliffs that mark the sudden drop from the relatively shallow Potrillo Canyon into the much deeper Water Canyon. Water Canyon descends from the Pajarito Plateau at center right, and continues to its confluence with White Rock Canyon at keft. Here oart of the east rim of White Rock Canyon is visible, with Montoso Peak on the skyline.
The feature of greatest geological interest is probably the large outcropping of light pink Bandelier Tuff in the south wall of Water Canyon. It appears that this outcropping has not slumped down the canyon wall; it was this thick when deposited 1.21 million years ago. Since older Cerros del Rio basalt and underlying Santa Fe Group sediments form the rest of the canyon wall, this shows that the Bandelier Tuff filled a deep ancestral Water Canyon, or perhaps a meander of White Rock Canyon, when it was erupted, and erosion has since re-cut the canyon, leaving this remnant on the canyon walls.
The Cerros del Rio is exposed in lower Frijoles Canyon, where some interesting features of the formation can be examined. The basalt first appears in the canyon bottom about halfway from the visitors' center to Upper Falls.
The Frijoles River is soon cutting deep into the basalt, exposing basal breccia at the bottom of the top flow unit. That is, the cliff here is a thick lava flow with broken basalt fragments buried beneath. These typically form at the front of a slow-moving lava flow, crumble off the face of the flow as it advances, and are buried beneath it.
Further down, on the west side of the canyon, there is a spectacular contact between the benmoreite of the Cerros del Rio and the overlying Bandelier Formation.
Seen from the canyon rim above:
Contact between Cerros del Rio and Bandelier Formations in lower Frijoles Canyon. 35 45.888N 106 15.661W
This illustrates how the Bandelier Tuff filled low-lying areas in the surface over which it was erupted. The Cerros del Rio was evidently already heavily eroded in this area 1.2 million years ago, and this particular paleocanyon has been interpreted as the previous course of the Rio Grande, prior to the Bandelier Tuff eruption.
Cerros del Rio basalts are common on the west side of the Rio Grande in the area north of Cochiti. These are relatively young flows. The area is on tribal lands and mostly inaccessible to casual visitors.
The basalt and basaltic andesite flows that define the Cerros del
Rio Plateau, and which we have now seen in cross section in
numerous locations, range in age from about 3 million to about 2.6
million years. About 2.6 million years ago, there was a
particularly voluminous pulse of more silica-rich magma, mostly
basaltic andesite and andesite (or their alkaline equivalents),
which formed most of the high terrain on the Cerros del Rio.
Additional high terrain was produced by a second pulse at around
2.4 million years. We'll now look at the plateau itself and its
many hills and small mountains.
We'll begin at the southern end of the Cerros del Rio, atop Tsinat
Mesa.This is mostly underlain by level flows of olivine
basalt, forming a very flat surface, but the northern end of the
mesa is bounded by hills and mountains of more silicic rock.
Panorama from Tsinat Mesa. Looking west
to north from 35
35.052N 106 10.859W
Tetilla Peak is the shapely mountain to the left, which is a distinctive landmark visible for great distances. At 7206′, it is not actually the highest point in the Cerro del Rio, but it is the most prominent. It may also be one of the older features of the Cerros del Rio, erupted 3.04 million years ago, according to radioisotope dating. What makes this more surprising is that it has a cap of dacite that is the most evolved lava in the entire Cerros del Rio. But the radioisotope age may be off; magnetic data and field relations suggest the age is more like 2.7 million years.
Tetilla Peak is surrounded to the east by andesite flows. Because andesite lava is considerably more viscous than basalt lava, these andesite flows have steeper faces.
Face of andesite flow at foot of Tetilla
Compare the basalt flows surrounding the peak with the andesite
Arroyo at foot of Tetilla Peak. 35.607N
The basalt is probably younger, but has been eroded away where it made contact with the andesite flow to produce the cliffs. The andesite flow to the right is much thicker. Here is a sample taken from the right side of the arroyo.
Andesite of Tetilla Peak
The presence of plagioclase and hornblende phenocrysts (white
patches and dark needles) is typical of andesite, but the rock
also has green patches of what appers to be olivine. Olivine
andesite is not unknown, but it’s uncommon and noteworthy, and the
geologic map of the area mentions no olivine in the andesite of
Tetilla Peak, only in the basalt around it. Or perhaps the green
patches are an unusual pyroxene mineral, which would be more
consistent with an andesite.
Most of the plateau is basalt or basaltic andesite flows, on which is superimposed several tall hills composed mostly of andesite flows and cinder. Basalt lava is relatively low in silica, relatively fluid, and flowed out freely to form the flat surface of the Cerros del Rio. Later, more silica-rich, and therefore more viscous, andesite lava was erupted to form the hills and peaks. Typical is Colorado Peak.
Colorado Peak. Looking northwest from 35.626N
Colorado Peak is underlain by andesite about 2.6 million years old. The flat top is surrounded by a ring of dikes intruding the cinder making up most of the upper part of the mountain.
Further north we come to Cerro Ruiz.
Cerro Ruiz. 35
41.311N 106 11.215W
Cerro Ruiz is underlain by 2.61-million-year-old andesite.
Next is Cerro Rito.
Cerro Rito. 35
42.001N 106 11.010W
This is underlain by basaltic andesite a bit younger than the other features we’ve seen so far, at 2.53 million years old.
Incidentally, the rock under most of these peaks takes the form of cinders, while the lower slopes are solid flows. This is quite typical of cinder cones.
This is also a good spot for viewing Cerro Micho.
Cerro Micho. 35
42.552N 106 12.176W
This one is a little older, being underlain by andesite that is about 2.76 million years old.
Another turn and Montoso Peak comes into view. This is very prominent on the skyline directly south of my house.
Montoso Peak. 35
44.425N 106 13.143W
Montoso Peak is underlain by basalt 2.59 million years old. The
low-viscosity basalt has produced a mountain with relatively
gentle slopes: A shield volcano.
The northernmost part of the Cerros del Rio Plateau is Sagebrush
Flats, which resembles Tsinat Mesa at the other end of the
plateau. South of Sagebrush Flats is a
wild maze of steep-sided andesite flows, quite striking on
the topographic map.
Ortiz andesite flows
The andesite here all erupted from around Ortiz Peak.
Ortiz Peak. 35 44.918N 106 08.911W
Ortiz Peak seen from the east,
highlighted by distant rain shafts.
The Ortiz Andesite is one of the younger flows in the Cerros del Rio at 2.32 million years old. This seems to rule out the possibility that its rugged topography is the result of more extensive erosion that other parts of the Cerros del Rio. Looking at the topo map for the area, I get the sense that most of the andesite flows had a tendency towards this deeply lobed structure, but none were nearly as voluminous as the Ortiz flows and so did not fully develop it.
South of Ortiz Peak are the Twin Hills.
Twin Hills. 35
42.534N 106 10.243W
These are also relatively young, being underlain by basaltic andesite with an age of about 2.53 million years.
A final pulse of magmatism came around 1.3 million years ago,
almost simultaneously with the Valles event. This produced Cochiti
Volcano and its associated flows. One of these flows
actually overlies a bed of Otowi Member, Bandelier Tuff. Another
flow is the one I mentioned earlier, which cascaded down La Bajada
and pooled at the base of the escarpment. This area is all tribal
lands and inaccessible to the general public.
This is the second most voluminous of the basalt eruptions around
the periphery of the Jemez from this time period. It is dominated
by San Felipe Volcano, a classical small shield volcano, whose
flows have a radiometric age of 2.5 million years.
San Felipe Volcano, a typical small shield volcano, viewed from the south from 35 15.168N 106 33.942W
Santa Ana Mesa is cut by several north-south faults that are
clear to see on the topographic map and even in the satellite
photo. San Felipe Volcano erupted along one of these vents. The
displacements on these faults are as much as 110 meters (350'). As
with the Cerros del Rio, the oldest beds include cinder beds
likely from a maar eruption early in the field's history. There is
also evidence of cinder cones that were subsequently buried by a
fluid lava flow, like the cinder cone exposed in the east wall of
White Rock Canyon.
The southernmost part of the Santa Ana field, and thus the
southernmost flow we can plausibly assign to the Jemez volcano
field, is Canjilon Hill. The most prominent feature here is
Octopus Plug, near southern end of Santa Ana basalt field. 35 21.676N 106 32.245W
Canjjilon Hill is a diatreme, a wide vent filled with
volcanic rubble that likely lay under a maar that has since been
Most of the mesa can be viewed from favored locations around the village of Placitas, in the northern foothills of Sandia Crest to the south.
Santa Ana Mesa viewed from near
18.883N 106 27.135W
This photograph shows that the mesa dips slightly to the east.
The beds were almost certainly level when first laid down, so this
indicates continuing tilting towards the east side of Santo
Domingo Basin in the last three million years.
Finally, here is a view of Santa Ana Mesa from the southwest.
View of Santa Ana basalt field. Looking northeast from near 35.392N 106.639W
Santa Ana Mesa dominates the center of the panorama. At left is
the Sierra Nacimiento, with Chamisa Mesa and Borrego Mesa to the
right. Redondo Peak is the high point of the skyline.
I'm not likely to add many photos in the future. The entire mesa
is on tribal lands and thus is not open to the general public.
This was the least voluminous of the basalt eruptions from this
time period, consisting of just a few flows in the northeastern
Jemez. However, one of the flows is quite prominent from Abiquiu,
since it caps Abiquiu
Abiquiu Mesa. Looking southwest from 36 12.528N 106 17.662W
A flow of El Alto basalt forms an imposing wall south of Forest
Road 31 just where it turns to make the ascent to El Alto Mesa.
El Alto Basalt. Looking south from 36 09.988N 106 21.330W
Note that this is on tribal land and visitors are restricted to the roadway.
The source of at least some of these flows is Cerro Pelon. This is remarkable in that the bulk of Cerro Pelon is Tschicoma dacite. The El Alto flow appears to come from a vent on the north side of the dome, possibly opened by a landslide (now buried by El Alto basalt.
Panorama from northwest flank of Cerro
07.441N 106 24.207W
At left, smoke from a small fire, and, on the skyline, the La Grulla Plateau. Bandelier Tuff extends across the left side of the panorama, with the unmistakable profile of Cerro Pedernal on the skyline. Mesozoic beds of the Colorado Plateau extend across the rest of the skyline, with Abiquiu Reservoir visible.
The foreground ridge to left is Tshicoma dacite forming the west flank of Cerro Pelon. The upper part of the ridge to right is also underlain by Tshicoma Dacite, but the lower part of the ridge and the ridge in the middle distance at center is underlain by El Alto Basalt erupted from Cerro Pelon. The grassy valley may also be underlain by El Alto Basalt under its surface layer of alluvium.
Here's a sample of the basalt from this area.
El Alto Basalt from Cerro Pelon. 36
07.458N 106 23.802W
This is a somewhat unusual basalt, with numerous coarse
From a vantage point well to the west, the level surface of the Abiquiu Mesa flow is striking.
El Alto surface looking southeast from 36
14.662N 106 22.095W
Note how the flat surface of Abiquiu Mesa (left of center on the skyline) lies below the level of El Alto (to the right on the skyline) and how it appears to emerge out of a canyon in the higher country. The ground at the foot of El Alto must have been fairly level at the time of eruption.
About 2.35 million years ago, an eruption in the Cerros del Rio
created a lava dam across the Rio Grande south
of the present location of White Rock, near Water Canyon.
This created Culebra Lake, which at its maximum was over 80 meters
(240') deep and covered an area greater than 1000 km2
(400 square miles) in what is now the Espanola Valley and Abiquiu
Culebra Lake deposited lacustrine sediments throughout its lake bed, but most of these have already eroded away. A few beds are preserved beneath Bandelier Tuff in the area east of Los Alamos. There was also for many years an outcropping of Cerros del Rio basalt next to the main highway to Los Alamos that showed ripple marks imprinted in the basalt when it flowed into the lake and made a cast of the lake floor. Regrettably, this was destroyed when the road cut was expanded some years ago. (However, the same road expansion produced the iconic road cut shown earlier in this chapter.)
Lacustrine sediment beds are still visible north of where this outcropping once existed.
Lacustrine sediment beds. 35.877N 106.194W
The lacustrined sediment beds are located at the center of the
phograph, below a hill of badly fractured Bandelier Tuff. The beds
are rich in clay and form a superb slip surface for the overlying
rocks to slump.
Relief map of the Jemez with exposures of the Tuerto Gravel in red, the Gravel of Lookout Park in yellow, and other pediments in green.
You may have noticed in many of the photographs of the Cerros del Rio that the basalt flows capping the plateau appear to have erupted across a fairly level surface. This is one of the older surviving examples in the Jemez area of a physiographic surface. Physiographic surfaces are typically formed on valley bottoms where the base level is set by some resistant feature downstream in the river system (a knickpoint), such as a resistant bed of rock over which the river flows to produce rapids or a waterfall. Such surfaces can be constructive, formed by accumulation of flat beds of sediment, or destructive, where erosion bevels the region flat. Some physiographic surfaces are formed by both processes.
The surface on which the Cerros del Rio formed is thought to be
part of the Divide surface, which was first recognized by
geologists in the area just north of Santa Fe. There are at least
three such surfaces in the Santa Fe area, each corresponding to a
different base level from a different time in the past. The older
surfaces are deeply gullied by erosion that is now leveling the
area to form a new physiographic surface corresponding to the
modern base level. However, the preservation of the older surfaces
is striking, and may be a result of extensive calichification of
the surfaces in the arid Southwest climate.
One of the oldest and most spectacular of the physiographic surfaces is the Ortiz surface, first recognized by geologist I.H.Ogilvie in 1905. The Ortiz surface was one of the first recognized examples of a pediment. A pediment is a nearly level surface cut in the bedrock at the foot of an eroding highlands. Pediments seems to be characteristic of arid regions with poor drainage, suggesting that northern New Mexico was already an arid climate two to three million years ago.
Remnants of this surface extend for great distances around the Ortiz Mountains. The surface is well preserved south of Los Cerillos.
Ortiz Surface south of Los Cerillos. 35 23.764N 106 07.360W
Pediment surfaces are often covered with sheet wash,
which is a layer of gravel and boulders washed across the surface
by infrequent but heavy runoff. The Ortiz surface is covered by
such a sheet wash, which has been named the Tuerto Gravel. This is
composed of very coarse gravel that is unusually resistant to
erosion due to pervasive calicification. Unfortunately, it has
proven very difficult to pin down the precise age of the Tuerto
Gravel, but the best guess is that it is Pliocene, betwen 5.3 and
2.6 million years in age.
The Ortiz Surface is plainly visible from a vantage point in the Cerillos Hills.
Ortiz Surface south of Los Cerillos. Looking south from 35 27.434N 106 07.798W
The surface forms the skyline at center, and remnants of the surface can be seen extending back towards the camera.
Some geologists believe the Totavi Lentil of the Puye Formation was deposited on the Ortiz Surface and correlates with the Tuerto Gravel.
At about the same time the peripheral basalt eruptions peaked,
erosion of the Keres Group volcanoes in the southern Jemez began
to produce another pediment surface. Like the Ortiz surface, this
is covered with a sheetwash layer, the Gravel of Lookout Park.
This is well exposed where the road climbs up to the Veterans'
Memorial Overlook at Kashe-Katuwe National Monument. (This area
was formerly known as Lookout Park and gives the formation its
Gravel of Overlook Park near Veterans'
Memorial Overlook. Near 35
39.994N 106 26.790W
The clasts are mostly Paliza Canyon Formation and Bearhead Rhyolite that was eroded off the mountains to the north.
The contact between the Gravel of Lookout Park and the Cochiti
Formation is exposed further down the road.
Contact between Cochiti Formation and
Gravel of Lookout Park. 35
40.040N 106 26.906W
The Cochiti Formation is the sandy beds at the bottom of the photographs. The beds of gravel and cobbles above are the Gravel of Lookout Park. In the second photograph, it looks like a microfault has thrown down the beds of the Gravel of Lookout Park to the right (east).
The transition is not terribly dramatic, though it is more so
when seen from a distance. It is unsurprising that some recent
geologic papers describe the Gravel of Lookout Park as the Lookout
Park Member of the Cochiti Formation. However, since the Gravel of
Lookout Park is reworked Cochiti Formation sediments mixed with
additional clasts freshly eroded off the mountains to the north,
and deposited on an erosional surface, I am not sure it is quite
correct to make it a member of the Cochiti Formation.
The pediment surface forms the plateau on which the Veterans Memorial Overlook is located. This area has actually been thrown down a short distance by a fault just to the west of the Overlook. From a vantage point west of this fault, one can see the pediment surface beautifully displayed on the mesa to the south.
Notice how remarkably flat the top of the mesa is. The flat areas further away at the left end of the panorama are also part of this pediment surface, but have been thrown down by the fault I mentioned earlier. The pediment surface extends for miles to the west and south (albeit with numerous cross-cutting arroyos) and is everywhere surfaced with Gravel of Lookout Park. The Gravel of Lookout Park was deposited across this surface in a geologically short period of time, around 2.5 million years ago. Later, river drainage patterns shifted and erosion cut numerous arroyos into this pediment surface, but the surface is still discernible.
One wonders if the Gravel of Lookout Park correlates with the
Tuerto Gravel to the south. However, the ages seem to be wrong.
The Gravel of Lookout Park can be quite accurately dated from
underlying and overlying volcanic rock, and it appears to be
younger than the Tuerto Gravel. However, the latter is
sufficiently difficult to precisely date that the possibility
cannot be entirely ruled out. In any case, the source rock for the
Lookout Park gravel is from the Jemez, while that from the Tuerto
Gravel is primarily from the Ortiz porphry belt.
In many places, the Gravel of Lookout Park is overlain by a thin eolium, wind-deposited sediments.
These are very young deposits, so we are getting a bit ahead of
our story, but I mention them here to complete the story of the
Gravel of Lookout Park.
Once, while visiting the Veterans' Overlook Memorial, I hiked along the trail east of the overlook, more out of idle curiosity than anything else. (I had not brought my own map of the area.) The trail goes some distance east, then south across the entrance road, then gradually loops around to the southwest. Where I met one of the natives:
Crotalus atrox near the Veteran's Memorial Scenic Overlook. 35 40.138N 106 26.984W
Click for the full resolution image, and you'll clearly see the rattle and the diamond pattern. Yep, this is a fine fat specimen of Crotalux atrox, the western diamondback rattlesnake. It was leisurely making its way across the trail when I happened along, and we both reared back and regarded each other with alarm. Oddly, I did not hear the snake rattle, nor did it coil in the usual rattlesnake manner. I might wonder if this actually a bull snake (the two species look a lot alike) but the rattle is very obvious in the full-resolution photograph and the coloration is precisely correct. It was a cool day; the snake may have been torpid enough to behave oddly. Regardless, it made no move to leave the trail, and I was disinclined to try to go around. (Who knows what else was lurking off the trail?) I turned around.
The youngest surface in the Santa Fe Area is the Airport Surface, which is quite striking from certain vantage points.
Airport Surface. Looking northwest from 35 35.419N 106 04.805W
You can see the very level surface at the foot of the Cerros del Rio lining up perfectly with the inter-arroyo divides in the middle distance.
Relief map of the Jemez with Ancha Formation outcroppings highlighted in red.
The youngest rift fill formation in the Jemez area is the Ancha
Formation, which is exposed mostly in the area west and south of
Santa Fe. It is usually but not universally regarded as part of
the upper Santa Fe Group. Radioisotope dates from zircon grains in
pumice of the Ancha Formation give it an age of around 1-3 million
years, roughly contemporaneous with the peripheral basalts, with
which it appears to interfinger on the east side of the Cerros del
Rio. The Ancha Formation also appears to overlie parts of the
Tuerto Gravel, supporting the estimate that the Tuerto Gravel is
at least 2.6 million years old.
Ancha Formation rests directly on much older Galisteo Formation
beds near the village of La Cienega.
Contact of Ancha and Galisteo
The Galisteo Formation is the red beds at the bottom, while the
light tan beds on top are Ancha Formation. The contact here is a
discontinuity of at least 25 million years in the geologic record.
The Ancha Formation thins out and disappears to the north.
Northwest of Santa Fe, the Ancha forms the top of the higher hills
and ridges, whose lower slopes are Tesuque Formation. Here's the
contact visible in a road cut.
Contact between Ancha Formation and
35 42.239N 106 04.807W
The Tesuque Formation is the reddish beds at bottom, full of bits of red granitic rock. This has to be Lithosome A, though I can’t guess which member; the geological map for this area is not specific.The tan beds on top are Ancha Formation.
Further south, in the Los Cerillos-Gallisteo area, the Ancha Formation becomes quite prominent.
Ancha Formation in road cut near Los Cerillos. 35 27.327N 106 04.322W
Here the Ancha Formation tends to lie directly on rocks of Eocene age or earlier. A particularly spectacular contact is found at Garden of the Gods.
Ancha Formation resting on Galisteo Formation. 35 26.505N 106 04.927W
Nearly horizontal beds of the Ancha Formation on the top of the hill overlie beds of the Galisteo Formation that have been tilted nearly vertical by the nearby Cerillos Hills intrusion.
The pulse of basaltic magmatism peaking 3 million years ago had largely wound down by 2 million years ago. However, big things were now cooking in the heart of the Jemez Volcanic Field.
Next page: Things gets tuff in the Jemez
Copyright © 2015 Kent G. Budge. All rights reserved.