Molecular-dynamics simulations of the Z3< 110X211) twin boundary in Ag predict a thin (1 nm) boundary phase of the 9R (a-Sm) structure. High-resolution electron microscopy shows the presence of the predicted structure. We also calculate the energy ab initio for several hypothetical structures of Cu and Ag. Low energies of the 9R structure and other polytypes, low experimental stacking-fault energies, and the hcp-fcc energy difference are correlated and explained in terms of an effective nearest-neighbor Ising interaction. PACS numbers: 61.16.Di, 61.70.Ng, 68.35.Bs It has been recognized for some time that the 9R polytype or a-Sm structure occurs as a martensitic product in a number of alloys [1-7] and compounds [8][9][10]. In pure metals, besides in Sm itself, the structure has been seen in quenched, ultrafine Co particles [11], in Cu precipitates in a-Fe [12], and in our own work on Cu and Ag twin boundaries to be reported. Furthermore, the 9R structure has received increasing attention recently from the physics community since it was identified by Overhauser [13] from neutron scattering data [14] as a stable structure of Li below 75 K. Subsequent work by Smith and others confirmed that there is a 9R phase, albeit heavily faulted, in Li below 75 K [15] and also in Na below 35 K [16]. The evidence that it exists at all in K appears to be weaker [16,17]. From a theoretical point of view firstprinciples calculations for metallic hydrogen have shown [18] that, among several candidate structures, the 9R is the most stable.We report here the first observation of the 9R structure in pure Ag. It occurs in a rather special situation, namely, at a S3 (211) twin boundary, where a thin (1 nm) layer of the phase appears as a means to ease the reversal of the stacking sequence ABC...to CBA . . . from grain to grain. Its structure is appropriate for this purpose since it can be thought of as fee with a stacking fault on every third close-packed plane. However, to occur at the boundary it is necessary that 9R be only slightly higher in energy than fee, and as we shall show this is enabled by the low stacking-fault energy of Ag. The boundary structure was predicted by computer simulation, as described below. It has also been predicted and found in Cu [19]. Evidence has been published that it appears in Au [20], although it was not recognized at the time as such. Our direct experimental evidence for the structure was obtained by high-resolution transmission electron microscopy (HRTEM). We have also made first-principles total-energy calculations for polytypes and obtained stacking-fault energies which support our interpretation.To understand the geometry of the 97? and other polytype structures it is helpful to note that the possible stacking sequences of close-packed planes are isomorphic to the Ising model. This is a useful way to think about polytypes [21-23]. The familiar notation ABCABC. . . for the stacking sequence in fee, for example, obscures the fact that each close-packed plane has the same translation with respect ...