Oxygen is in many ways a unique element: It is the only known diatomic molecular magnet, and it exhibits an unusual O 8 cluster in its high-pressure solid phase. Pressure-induced molecular dissociation as one of the fundamental problems in physical sciences has been reported from theoretical or experimental studies of diatomic solids H 2 , N 2 , F 2 , Cl 2 , Br 2 , and I 2 but remains elusive for molecular oxygen. We report here the prediction of the dissociation of molecular oxygen into a polymeric spiral chain O 4 structure (space group I4 1 ∕acd, θ-O 4 ) above 1.92-TPa pressure using the particleswarm search method. The θ-O 4 phase has a similar structure as the high-pressure phase III of sulfur. The molecular bonding in the insulating ε-O 8 phase or the isostructural superconducting ζ-O 8 phase remains remarkably stable over a large pressure range of 0.008-1.92 TPa. The pressure-induced softening of a transverse acoustic phonon mode at the zone boundary V point of O 8 phase might be the ultimate driving force for the formation of θ-O 4 . Stabilization of θ-O 4 turns oxygen from a superconductor into an insulator by opening a wide band gap (approximately 5.9 eV) that originates from the sp 3 -like hybridized orbitals of oxygen and the localization of valence electrons.solid oxygen | spiral chain structure A s a long-standing problem in physics and chemistry, as well as earth and planetary sciences, high-pressure dissociation of diatomic molecules, such as H 2 , N 2 , O 2 , F 2 , Cl 2 , Br 2 , and I 2 , has attracted a lot of attention. Among these molecular systems, solid oxygen is a system of particular interest and exhibits many unusual physical properties by virtue of its molecular spin and the resultant spin-spin interactions, which make the system a critical test case for condensed-matter theory (1, 2). Oxygen is also the third most abundant element in the Solar System, and its behavior under extreme pressures provides important insight into the oxygen-related systems for a better understanding of the physics and chemistry of planetary interiors.Oxygen exhibits a rich polymorphism with seven unambiguously established crystalline phases. Upon cooling at ambient pressure, oxygen is in turn solidified to the paramagnetic γ-phase, the magnetically disordered (short-range ordered) β-phase (3, 4), and ultimately the antiferromagnetic α-phase (5). Upon compressing to approximately 6 GPa, the α-phase transforms into the antiferromagnetic δ-phase (6-8). Under a higher pressure of approximately 8 GPa, the magnetic order of oxygen is destroyed, which leads to the ε-O 8 phase consisting of O 8 clusters (9, 10). The ε-O 8 phase displays the bonding characteristics of a closedshell system, in which the intermolecular interactions primarily involve the half-filled 1π g à orbital of O 2 (11). Above 96 GPa, ε-O 8 has been observed to transform into a metallic ζ-phase (12, 13) and intriguingly exhibits superconductivity with a transition temperature of 0.6 K (14). This superconducting ζ-phase has been predicted by theory ...