The human intervertebral disc is commonly described as a 'shock absorber', resisting compressive loads through the interaction between its hydrated nucleus pulposus and the surrounding annulus fibrosus. While this is certainly true, the disc also plays an essential role in stabilising the spinal motion segment when subjected to shear and torsional forces. To achieve this, it relies upon a remarkable combination of structural features, including the annular lamellae, their anchorage to adjacent vertebral bodies through Sharpey's fibres, the vertebral endplates and the supporting ligamentous structures. The orientation of the facet joints provides additional constraints upon movement.
However, the disc's ability to perform these functions depends upon more than the integrity of its external attachments. It also relies upon the mechanical properties of its internal nucleus pulposus, particularly its capacity to attract and retain water and generate pressure.
In this respect, the intervertebral disc has some interesting similarities to a car tyre.
A tyre is designed to operate within a particular range of inflation pressures. When appropriately inflated, its internal air pressure supports the tyre's structure, helps maintain its shape and allows the sidewalls and tread to respond predictably to the forces generated during driving. But when inflation pressure falls, the mechanical behaviour of the tyre begins to change. The sidewalls deform more readily, particularly during cornering, and the resulting distortion can produce unwanted movement, uneven loading and accelerated wear. In extreme circumstances, the tyre may even move relative to the wheel rim.
The intervertebral disc operates according to a surprisingly similar principle, although its internal pressure is generated by a very different mechanism.
The nucleus pulposus contains a high concentration of proteoglycans, particularly aggrecan, whose negatively charged glycosaminoglycan chains attract water and generate an osmotic swelling pressure. This pressure is resisted by the surrounding annulus fibrosus and vertebral endplates, creating a mechanically integrated structure capable of distributing substantial compressive loads. When the spine is loaded, pressure within the nucleus increases, generating outward forces that place the annular fibres under tension (2).
This internal pressurisation is important because it helps maintain disc height, distributes loads across the vertebral endplates and contributes to the mechanical behaviour of the surrounding annulus.
But just as a tyre becomes mechanically compromised when its inflation pressure falls, the intervertebral disc can experience significant changes when its capacity to generate and maintain internal pressure deteriorates.
Ageing, genetic influences and injury can contribute to the progressive depletion or alteration of proteoglycans within the nucleus pulposus. As its capacity to attract and retain water diminishes, the nucleus loses some of its swelling pressure and its ability to distribute compressive forces effectively. The resulting changes in load sharing can reduce the tension developed within the annular fibres and increase deformation of the disc under load (2).
This is not merely a theoretical proposition. In 1999, Sato and colleagues measured intradiscal pressure in healthy volunteers and patients with low back pain or sciatica, demonstrating that pressure was significantly reduced with increasing MRI-assessed disc degeneration (3).
More recently, a 2025 investigation by Liebsch and Wilke examined intradiscal pressure in 107 human lumbar motion segments obtained from 68 donors. They found that discs exhibiting mild or moderate degeneration demonstrated significantly reduced intradiscal pressure compared with non-degenerative specimens. Pressure also declined significantly with increasing age, with the researchers observing these differences across multiple loading directions, including flexion, extension, lateral bending and axial rotation (4).
These findings lend considerable support to the concept that degeneration compromises the internal pressurisation of the disc, potentially altering the distribution of mechanical loads between the nucleus and annulus.
And this is where the tyre analogy becomes particularly interesting.
An underinflated tyre may still be securely attached to its wheel, but its ability to resist deformation during cornering is compromised. Similarly, a degenerative disc may remain firmly anchored between adjacent vertebrae while becoming less effective at resisting the forces that attempt to deform or translate the spinal segment.
The consequences may include greater annular bulging, altered load distribution, increased shear stresses between annular lamellae and progressive disruption of their structural organisation. Over time, these changes may contribute to further mechanical deterioration, creating a potentially self-perpetuating cycle in which degeneration alters mechanical loading, and abnormal loading contributes to further degeneration (2).
Of course, unlike a car tyre, the disc is a living, viscoelastic structure whose internal pressure varies continuously with posture, activity and loading. Furthermore, degeneration does not invariably produce excessive spinal movement; advanced degenerative changes may ultimately make a motion segment less mobile rather than more unstable.
Nevertheless, the underlying principle remains remarkably similar: when a pressurised structure loses its capacity to maintain internal support, the mechanical demands placed upon its surrounding walls change, potentially compromising their ability to resist deformation.
And this brings us to an interesting question. If degeneration reduces the disc's internal pressurisation and alters the mechanical behaviour of its annular wall, just how much of its ability to resist shear might be lost?
A recent investigation provides some fascinating answers.