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4.3: Jointing and Faulting

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    21490
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    Brittle Deformation

    A body of rock that is brittle—either because it is cold or because of its composition, or both— is likely to break rather than fold when subjected to stress, and the result is jointing or faulting.

    Jointing

    A joint is a fracture in a rock in which no displacement or side-to-side movement has occurred. Most joints form where a body of rock is expanding because of reduced pressure, which is the case of Half Dome in Yosemite National Park (Figure \(\PageIndex{1}\)). Joints can also form where the rock itself is contracting but the body of rock remains the same size (the cooling volcanic rock in (Figure \(\PageIndex{2}\)). In all of these cases, the pressure regime is one of tension as opposed to compression.

    Jointing within the rock of a mountain, which appears to have a rough, flaky surface. People climb up a trail to the top.
    Figure \(\PageIndex{1}\): Exfoliation joints, sometimes called “sheeting”, on Half Dome in Yosemite National Park. “Half_dome_yosemite_nationalpark-2.JPG” by Saibo via Wikimedia Commons is licensed under CC BY-SA 3.0.
    Fractures exposed on the eroded upper surface of a hill within a forest.
    Figure \(\PageIndex{2}\): Polygonal fractures at Devil’s Postpile in the eastern Sierra Nevada. This jointing pattern formed during the cooling and shrinking of the lava. "IMG_0908" by Jared Sneed via Flickr is licensed under CC BY-NC.

    Joints can also develop when rock is under compression as shown on Figure \(\PageIndex{3}\), where there is differential stress on the rock, and joint sets develop at angles to the compression directions.

    Cross-section of a rectangular rock, with diagonal indicated in X pattern. Arrows point into each face of the rectangle, showing the forces exerted.
    Figure \(\PageIndex{3}\): Joints developed in a rock under compressive stresses. "Joints developed in a rock" by Steven Earle is licensed under CC BY 4.0.

    Faulting

    A fault is a boundary between two bodies of rock along which there has been relative motion. An earthquake occurs when one body of rock slides past another. Earthquakes don’t always happen on existing faults, but once an earthquake occurs, a fault will form at that location. Some large faults, like the San Andreas Fault in California, show evidence of hundreds of kilometers of movement, while others show less than a millimeter. In order to estimate the amount of motion on a fault, we need to find some geological feature that shows up on both sides and has been offset (Figure \(\PageIndex{4}\)).

    Creeks offset by the San Andreas Fault in the Carrizo Plain
    Figure \(\PageIndex{4}\): The San Andreas Fault exposed in the Carrizo Plain. Streams which once flowed uninterrupted straight across the fault are now displaced by the fault, taking a step to the right, illustrating the right-lateral movement the fault has experienced. "2018_01_23_sba-188-sba_107" by Doc Searls via Flickr is licensed under CC BY 2.0.

    There are several kinds of faults and they develop under different stress conditions. The terms hanging wall and footwall apply to situations where the fault is not vertical. The body of rock above the fault is called the hanging wall, and the body of rock below it is called the footwall (Figure \(\PageIndex{5}\)). When a fault is vertical, there is no obvious hanging wall or footwall. Hanging wall and footwall are mining terminology. Many mines are in fault zones. When a miner is walking within an adit, or horizontal tunnel within the Earth, their feet are on one side of the fault, the footwall, and their head could bump on the other side of the fault, the hanging wall.

    A fault with a stick figure, showing their feet on the footwall and their head bumping the hanging wall
    Figure \(\PageIndex{5}\): A cross section of a dip slip fault. The hanging wall is the upper block and the footwall is the lower block. "Dip-Slip Faults" by Chloe Branciforte, a derivative of "Footwall/Hanging Wall", is licensed under CC BY-SA 3.0.

    Dip-Slip Faults

    A dip-slip fault is a fault which moves in the dip direction of the fault plane. In other words, the hanging wall is moving up or down relative to the footwall.

    Normal faults are dip slip faults in which the hanging wall moves down relative to the footwall. Normal faults are created by extension of the crust and commonly occur at divergent plate boundaries, where the crust is being stretched.

    A normal fault, described in the caption.
    Figure \(\PageIndex{6}\): A normal fault forms where the hanging wall has dropped down relative to the footwall. The lateral tension caused by a normal fault results in extension and overall thinning of the crust. "Normal Fault" by Allison Jones, a derivative of "What Causes Dip-slip Faults?", is licensed under CC BY-SA 4.0.
    3D Model of a Normal Fault

    The following 3D model is of a normal fault. As shown in this model, the hanging wall moves downward as the footwall moves upward. The area of the hanging wall that is left exposed is called the "scarp."

    "Normal fault" by paulinkenbrandt via Sketchfab is licensed under CC BY 4.0.

    Video \(\PageIndex{1}\): Normal fault

    The following video illustrates the formation of a normal fault. There is no audio, but the the animation shows the process that has been described in the text. In a normal fault, the block above the fault (the hanging wall) moves down relative to the block below the fault (the foot wall), exposing the fault plane. This fault motion (earthquake) is caused by extensional forces and results in lengthening.

     

    Normal faults are very common in both the Basin and Range and Mojave Desert provinces of California where the crust is undergoing extension. In these locations, the crust is being pulled apart, which can result in down dropped blocks known as grabens and raised blocks called horsts.

    Reverse and thrust faults are created by compressional forces within the crust. In both reverse and thrust faults the hanging wall moves up relative to the footwall. Thrust faults are a particular type of reverse fault that is dipping at a very low angle (<30º). Often, thrust faults underlie other structural features like anticlines (Figure \(\PageIndex{7}\)).

    A reverse fault, described in the caption.
    Figure \(\PageIndex{7}\): Reverse faults form when the hanging wall has moved up relative to the footwall, due to compression forces. They result in shortening and thickening of the crust. "Reverse Fault" by Allison Jones, a derivative of "What Causes Dip-slip Faults?", is licensed under CC BY-SA 4.0.
    The formation of low-angle thrust faults, described in the caption.
    Figure \(\PageIndex{8}\): A thrust fault. Top: Before faulting, strata are continuous. Bottom: After faulting and significant offset, strata are thrust up and over each other, creating a repeating sequence. "Thrust Fault Deformation" by Steven Earle is licensed under CC BY 4.0.

    Reverse faults, thrust faults, and compressional forces commonly occur at convergent plate boundaries, where the crust is either overlapping at subduction zones or colliding at continent-continent collisions. Reverse and thrust faults are common in the Transverse Ranges and parts of the Coast Range provinces of California where the crust is actively experiencing compression.

    3D Model of a Reverse Fault

    The following 3D model is of a reverse fault that shows how the hanging wall has moved up relative to the footwall. The exposed area of the hanging wall is called the "scarp."

    "Reverse Fault" by paulinkenbrandt via Sketchfab is licensed under CC BY.

    3D Model of a Thrust Fault

    The following 3D model is of a thrust fault. Like a reverse fault, the hanging wall has moved up relative to the footwall, however the fault is dipping at a much shallower angle.

    "Thrust Fault" by paulinkenbrandt via Sketchfab is licensed under CC BY.

    Video \(\PageIndex{2}\): Reverse fault

    The following video illustrates the formation of a reverse fault. There is no audio, but the the animation shows the process that has been described in the text. In a reverse fault, the block above the fault (the hanging wall) moves up relative to the block below the fault (the foot wall). This fault motion (earthquake) is caused by compressional forces and results in shortening. A reverse fault is called a thrust fault if the dip of the fault plane is small.

     

    Strike-Slip Faults

    Strike-slip faults (Figure \(\PageIndex{9}\)) are created by shear stresses within the crust. They commonly occur at transform plate boundaries: the San Andreas fault zone of California is a transform plate boundary between the Pacific and the North American plates that consists of a system of strike-slip faults.

    Strike-slip faulting is common in the Peninsular Ranges province of southern California and the Coast Ranges province of central California, where many faults are parallel to the orientation of the San Andreas fault zone. Strike-slip faults move with mostly horizontal motion and typically are vertical or near vertical and thus do not have hanging walls or footwalls. These faults are named strike-slip because the direction of motion or slip is along the line of their strike.

    Strike-slip faults described in the caption.
    Figure \(\PageIndex{9}\): Strike-slip faults. Rocks on either side of the fault move parallel to the fault. In dextral (right-lateral) strike-slip faults the far side moves to the right of the observer. In sinistral (left-lateral) strike-slip faults the far side moves to the left of the observer. "Types of Strike-slip Faults" by Karla Panchuk is licensed under CC BY 4.0.
    3D Model of a Strike Slip Fault

    The following 3D model is of a strike-slip fault where the two fault blocks are moving past one another. In this example, the far side has moved to the right of the observer, indicating that it is a right-lateral strike-slip fault.

    "Strike Slip" by paulinkenbrandt via Sketchfab is licensed under CC BY.

    Video \(\PageIndex{3}\): Strike-slip fault

    The following video illustrates the formation of a strike-slip fault. There is no audio, but the the animation shows the process that has been described in the text. In a strike-slip fault, the movement of blocks along a fault is horizontal. If the block on the far side of the fault moves to the left, as shown in this animation, the fault is called left-lateral. If the block on the far side moves to the right, the fault is called right-lateral. The fault motion (earthquake) of a strike-slip fault is caused by shearing forces.

    Oblique Slip Faults

    It is not uncommon for faults to have components of both strike-slip and dip slip. If that is the case, the fault is said to have oblique slip. The Corona Heights fault in San Francisco has experienced both strike-slip and dip-slip motion. We can tell because the fault is covered in slickenside surfaces, surfaces that indicate the direction of slip on the fault either with slickenlines, grooves in the surface of the fault, or slickenfibers, mineral fibers that have grown in the direction of fault slip. The slickenlines here indicate that the block to the left has moved relatively up and away from where the photographer is standing in Figure \(\PageIndex{10}\).

    Rock wall with a grooved surface. The photographer appears to be standing on a surface high up on the wall, with their left shoulder close to the wall face.
    Figure \(\PageIndex{10}\): Slickenside covered Corona Heights fault in San Francisco. The hanging wall is the block to the left and the footwall is the ground on which the photographer is standing. "Corona Heights Fault" by Allison Jones is licensed under CC BY 4.0.

    References

    1. Earle, S. (2019). Physical Geology – 2nd Edition. Victoria, B.C.: BCcampus. Retrieved from https://opentextbc.ca/physicalgeology2ed March 2024

    4.3: Jointing and Faulting is shared under a CC BY-NC 4.0 license and was authored, remixed, and/or curated by Allison Jones.