
Southgate Road - Danville
Entrance
Northgate Road - Walnut Creek Entrance
Summit Road - Junction
Ranger Station to Summit
Southgate
Road - Danville Entrance
0.00 (Odometer Reading)
Set odometer to zero as you turn north onto Mt. Diablo Scenic Blvd (South Gate
Road) from Diablo Road or Blackhawk Rd. (see map) For the first half mile you will be
crossing non-marine strata of Pliocene and Upper-Miocene age. The beds are almost vertical and
you will be traveling 90 degrees to the strike of the beds, progressing over increasingly
older strata as you proceed north past the Athenian School.
These beds are the same age as those containing the Blackhawk Ranch
Quarry mammal fossils. Up ahead you can see the light tan stratified rocks of the Eocene Domengine at the top of the
ridge.
0.5
The rounded hills to the right with scattered oaks and newly built homes represent the
transition from non-marine to marine in this area. You will continue for about four-tenths
of a mile, past the first sharp turn to the left until you reach the second sharp turn to the left.
0.9
Here you take the second sharp turn to the left. Almost all of the maps show this as the
upper boundary of the Neroly Formation. The
Neroly sandstone and shale is brownish in color along the roadcuts and contains rich
fossil clam beds, well exposed farther east in Sycamore Canyon. The material making up the
rock is volcanic debris in origin, material eroded from an ancient Sierran highlands.
1.1
Boundary Gate to park. You will traverse eastward (and occasionally northward) and begin
your climb up the south flank of Mt. Diablo. You will continue to travel over increasingly
older Neroly for the next one-third mile, expressed as rounded grass-covered hills with
oak trees prominent.
2.1
Final turn north in the Neroly brings into view the steepalmost
verticalchaparral-covered slope of the Miocene Briones Formation just ahead.
2.3
As you make a sharp turn to the right, you will begin the serious climb up the south side
of Mt. Diablo, driving on the Briones Formation.
The shallow marine sandstone beds are not only almost vertical here, they are in fact
slightly overturned, which means the underside of the beds (facing south) is
younger than the topsides (facing north). The beds frequently contain marine
fossil shells.
As you climb up the Briones wall, the difference in the
character of the topography and plant communities between the Neroly and Briones
formations is very apparent. The Neroly is represented by the adjacent grass- and
oak-covered rounded hills to the south, which stand in sharp contrast to the steep
chaparral-covered slope of the Briones to the north.
3.5

This is a rather spectacular overlook across Sycamore Canyon to the hogback ridges plunging down the
western edge of Blackhawk Ridge into the
canyon. Immediately to the left beside the road are corresponding beds forming Fossil Ridge. There are several beds with fossils
exposed here, but the park does not allow pull-outs except in an emergency.
You may want to proceed to the South Gate
Entrance Station just ahead and get permission to park there briefly and walk back
down to the overlook.
These hogbacks represent the basal (oldest) beds of the
Briones Formation. As you walk (drive) back to the entrance station you will be in an
underlying siltstone unit, with pebbly siltstones and conglomerates. Less resistant to
erosion, this interval of Miocene beds forms a characteristic grassy saddle
between the overlying Briones, and the underlying Mid-Eocene
Domengine.
3.65
South Entrance Station. After passing the
entrance station, you will be entering the mid-Eocene
Domengine Formation. The rocks exhibit a wide variety of erosion features.
As we now travel northwest away from the entrance station, the deep valley to the north
(right) is formed by the West Fork of Sycamore Creek. The rocky slope across the valley is
Domengine as well.
It is interesting to note that after passing the
chaparral-covered Briones, we now find that the gray pine has become a prominent tree.
They seem to thrive in the sandy soils of the Domengine and their presence has been used
to help map the Domengine outcrops on the north side of the mountain in Black Diamond
Mines Regional Park.
4.1
The rocks you soon see on the right are the upper most part of the "Boy Scout
Rocks", a group of rocks popular with climbers. A short distant ahead on the left is
the massive monolith called "Gibraltar Rock".
4.5
Rock City. There are many short trails for exploring this area that include the Wind
Caves, Sentinel Rock and other fascinating erosion features. The Wind Caves at Rock City
are not formed by wind, but in fact are formed by water percolating through the sand and
dissolving the cement holding the sand grains together. Note the iron stained bands in the
sandstone near the Wind Caves. They are known as Liesegang structures. These formed as a
source of iron hydroxide diffused through the sandstone creating a beautiful banded
appearance in the rock.
The sandstone rocks here are part of the Domengine formation of
Middle Eocene age, deposited down slope of the shelf edge in deep
water. The sandstones form prominent ridges
which rise well above the surrounding landscape and trend for several miles along the
flank of the mountain.
This area also offers parking access to the Trail Through Time. An Overview Panel
is located near the restroom building.
4.6
After passing the rangers house on the right, you will be driving over rocks that
are less sand and more shale, a significant change from the massive sandstones of Rock
City. During the next half mile, you will notice the trees give way to more open
grassland.
5.2
Curry Point. There is a pull-out here at Curry Point that provides a view of the
distant Sierra on a clear day and the summit of Mt. Diablo to the north. Rocks of the
Franciscan Complex cap the mountain.
Looking north, the nearby valley is formed in shale of upper
Cretaceous age. The Cretaceous beds are separated from the Franciscan Complex by a major
thrust fault. The fault trace on the surface is mostly covered by landslide deposits.
Above the thrust fault is Franciscan mélange material and farther up is the hard
resistant greenstone and chert forming the rocky crest of Mt. Diablos main peak and
North Peak. The protruding rock to the east of Mt. Diablo summit is Devils Pulpit, a
resistant chert outcrop.
After leaving Curry
Point, you will be driving west, parallel and just above the contact between Upper
Cretaceous shale to the right and the younger early
Eocene beds to the left.
5.8
Near this point, you will be crossing over the Cretaceous/Eocene
contact. This contact is a major unconformity with a hiatus (an interval of time
represented by the missing rocks) of about 25 million years where 15 million years of
Upper Cretaceous rocks and the entire record of Paleocene history is missing. This
unconformity marks the boundary between the Age of Dinosaurs and the Age
of Mammals
6.0
Here you turn to cross the open valley to the north.
6.1
Thrust Fault. After passing a sign that says
2000 Feet, you will notice on your right a slight dip in the surface of the
road bank with a sign that says Authorized Vehicles Only and a trail
Interpretive Panel. Take the opportunity to park along side the road here.
If you examine the road bank (facing east), to the left you will find blocks of Franciscan
chert and greenstone. To the right down the road about 20 to 30 feet, these rock types are
missing; instead you will see an exposure of brown shale in the road cut. These two rock
types, Franciscan to the left and Upper Cretaceous to the right, are separated by a major
thrust fault. Franciscan rocks have been thrust up to the southwest and over the younger
Cretaceous shale. There is an interpretive panel here that describes the geology at this
point.
From this point to the Junction Office, you will be driving in
Franciscan mélange, where large blocks of typical Franciscan rocks are exposed along the
side of the road. The red-brown soils are characteristic of the iron-rich greenstone that
makes up much of the Franciscan on the mountain. Red radiolarian chert, along with lesser
amounts of shale and graywacke are also exposed.
6.8
Junction OfficeEnd .
Northgate
Road - Walnut Creek Entrance
0.00
Set odometer to zero at the North Gate
entrance kiosk. For the next 1.6 miles you will be traveling over Upper Cretaceous sedimentary rocks made up mostly
of shale with some sandstone beds. The topography consists of low rounded hills cut by the
Little Pine Creek running parallel to the road. Beds dip steeply to the southwest.
1.6
Park Boundary. Continue traveling on
Upper Cretaceous rocks. The rocks at the top of the hills to the right are Eocene in age. The eastern branch of the Concord
Fault follows the road in this valley.
1.9
As you turn left and then right, crossing a stream gully, you will notice gray-green rocks
along the left side of the road cut just before you cross over the gully. The gray-green
rock outcrop itself is a badly weathered exposure of serpentinite, forming the westernmost edge of the long
serpentinite band that runs easterly across the mountain. The fault that separates
the serpentinite from the Franciscan is probably expressed topographically by the
east-trending gully at this point. The fault plane dips down to the north. The serpentinite is separated from
the Upper Cretaceous beds (on which you have been traveling) by a major fault.
As you cross the gully and round the next bend (again driving briefly
on the Upper Cretaceous shale), you will notice a large rock outcrop ahead on the left
side of the road. It is at this point you once again cross a major fault. Continue in the
Franciscan Complex from this point on. The large imposing rock outcrop is greenstone, not
serpentinite. 
As you continue to drive south, keep an eye out for the typical
assemblage of rocks you find in the Franciscan Complexgreenstone (basalt), red radiolarian chert,
graywacke, and shale along with a few blocks of dark blueschist. In this area, these
varied rock types are enclosed in a mélange.
Red
Radiolarian Chert
3.1
Camel Rock. As you approach 3 miles, watch on
the left for Camel Rocka rock outcrop that (with the help of a little imagination)
resembles the outline of a single hump camel. After you pass the rock for about 100 feet,
you will get the best view if you look back toward the area you have just traveled. To
walk to the outcrop, best access is from Burma Road near where it crosses Northgate
Road.
3.4
Just past Camel Rock, you go over a rise of a hill and you will notice ranch
buildings ahead. The prominent ridge across the valley to the west is made up of
lower-Eocene-age sandstone and shale while the valley below on the west side of the Mt.
Diablo Thrust Fault is Upper Cretaceous. The Mt. Diablo Thrust Fault itself runs along the
slope about halfway between the road and the creek bed. The hills are relatively treeless,
typical of an unstable soil such as a mélange.
4.6
As you round a bend at this point you will notice a pile of rocks ahead. This rock
formation is called Turtle Rock. It is made of
radiolarian chert and from this perspective doesnt look much like a turtle. Better
views later. As you pass the Diablo Ranch gate, you will be traveling on
material formed by a large landslide. This
material also encloses blocks of Franciscan rock types and looks a lot like mélange topography. It is often difficult to
distinguish the two landforms from each other.
5.0
If you look down hill to the left, you will get a good view of Turtle Rock.
5.3
Here you may want to pull off the road to the right along an open grass area and walk the
short distant to the large block of blueschist exposed here. In the past, stone was
quarried from this area. This schist is
common in the Franciscan mélange and is named for the noticeable blue color of the
mineral glaucophane. Blueschist is largely
altered basalt and reflects a history of hi-pressure/low-
temperature metamorphism. On Mt. Diablo it is about 165 million years old.
You will continue traveling on landslide material containing large blocks of Franciscan rocks up several major switchbacks.
Look back as you go and you will see that Turtle Rock is aptly named (shell to the south
and head to the north).
6.25
By the time you reach the rangers house, you will be out of the landslide and back
into Franciscan mélange topography.
6.6
Junction OfficeEnd
Summit Road - Junction
Ranger Station to Summit
0.00
Set your odometer to zero when you
turn up Summit Road at the Junction Ranger Station. The entire drive to the summit will be
in the Franciscan Complex. Watch for the characteristic exposures of Franciscan type rocks
including red charts, greenstone (basalt),
and a few outcrops of graywacke and blueschist. The soils are typically red-brown in
color due to the high iron content of the parent rocks. Between here and near Toyon Picnic
area the drive will be through Franciscan mélange.
0.5
As you round the curve (turning right) after passing the Rocky Point Picnic area, you will notice a dark
blue-black boulder about 5 feet across protruding from the bank on the left side of the
road ahead. This is one of the rather common blueschist
found in the Franciscan. Blueschist is largely altered basalt and reflects a history
of hi-pressure/low-temperature metamorphism. On
Mt. Diablo it is about 165 million years old (younger than the greenstone, but older than
the graywacke).
1.15
To the left you will pass a prominent exposure of red radiolarian chert. If you pull off at the
turnout, you will also be able to look out over the ridges of younger rocks to the south.
As you look south and southwest, the valley below contains Cretaceous rocks bordered on
the north by a thrust fault that separates it from the Franciscan Complex and on the south
by younger Eocene age rocks that include the yellow-tan sandstone exposed around Rock City
and Castle Rocks. The more distant row of ridges (Fossil Ridge, Blackhawk Ridge, and
Oyster Point) are Miocene in age and are quite fossiliferous.
If you look to the north, you will see the rugged chert-greenstone
capped summit of Mt. Diablo.
1.5
At about 1.5 miles, you will leave the mélange and the chert and greenstone outcrops
become more frequent.
1.9
On the right side of the road and continuing for another 0.2 miles, is a major (and
typical) outcrop of sheared and broken greenstone
(basalt).
2.3
Pull out on left at Juniper Camp Ground. Good
views to the west. You will be looking out over the San Ramon Valley and the towns of
Danville, Alamo and Walnut Creek (left to right). The Calaveras Fault runs down a portion
of this valley. The ridge on the far side of the valley is Las Trampas Ridge and is made
up of Miocene age rocks similar to the Miocene age rocks on Mt. Diablo including highly
fossiliferous sandstone beds.
3.2
Another good exposure of greenstone, highly
sheared, with slickensides visible.
3.55
As you make a sharp turn to the left (Devils Elbow), you may want to pull off
here to view a moonscape of more chert and greenstone rocks toward the north, capped by
the prominent chert outcrop known as Devils Pulpit. These rocks are resistant
to erosion and are responsible for the rugged topography. Back on the road, the red rock
immediately on the right is thin-bedded radiolarian chert with interbeds of reddish shale.
Continue to the summit.
4.5
Summit
parking lot.
The summit museum has an excellent geology display.
A short walk along the Mary Bowerman Interpretive Trail is also recommended. This
is a quarter-mile walk along the northside of the mountain to an overlook platform. The
trail is accessed from the Lower Summit Parking Lot. There is an informative Geology
Interpretive Panel at the end of this short walk to the platform that describes the
geological setting of the mountains northside. This short walk will also provide an
opportunity to inspect greenstone, graywacke, red chert, and a small amount of shale up
close. The quarry you see to the north is producing diabase (part of the Mt. Diablo
Ophiolite) for crushed rock used in the construction of roadbeds.
Reproduced from Geology of Mt. Diablo - Roi Peers |