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Using optical long baseline interferometry, we resolved for the first time the two wide components of HD 167971, a candidate hierarchical triple system known to efficiently accelerate particles. Our multi‐epoch Very Large Telescope Interferometer observations provide direct evidence for a gravitational link between the O8 supergiant and the close eclipsing O + O binary. The separation varies from 8 to 15 mas over the 3‐year baseline of our observations, suggesting that the components evolve on a wide and very eccentric orbit (most probably  e  &gt; 0.5). These results provide evidence that the wide orbit revealed by our study is not coplanar with the orbit of the inner eclipsing binary. From our measurements of the near‐infrared luminosity ratio, we constrain the spectral classification of the components in the close binary to be O6–O7, and confirm that these stars are likely main‐sequence objects. Our results are discussed in the context of the bright non‐thermal radio emission already reported for this system, and we provide arguments in favour of a maximum radio emission coincident with periastron passage. HD 167971 turns out to be an efficient O‐type particle accelerator that constitutes a valuable target for future high angular resolution radio imaging using Very Long Baseline Interferometry facilities.

The long‐period eccentric orbit of the particle accelerator HD 167971 revealed by long baseline interferometry ★