  Context - Around the year 2000, Triton's south pole experienced an extreme
summer solstice that occurs every about 650 years, when the subsolar latitude
reached about 50{\deg}. Bracketing this epoch, a few occultations probed
Triton's atmosphere in 1989, 1995, 1997, 2008 and 2017. A recent ground-based
stellar occultation observed on 6 October 2022 provides a new measurement of
Triton's atmospheric pressure which is presented here.
  Aims- The goal is to constrain the Volatile Transport Models (VTMs) of
Triton's atmosphere that is basically in vapor pressure equilibrium with the
nitrogen ice at its surface.
  Methods - Fits to the occultation light curves yield Triton's atmospheric
pressure at the reference radius 1400 km, from which the surface pressure is
induced.
  Results - The fits provide a pressure p_1400= 1.211 +/- 0.039 microbar at
radius 1400 km (47 km altitude), from which a surface pressure of p_surf= 14.54
+/- 0.47 microbar is induced (1-sigma error bars). To within error bars, this
is identical to the pressure derived from the previous occultation of 5 October
2017, p_1400 = 1.18 +/- 0.03 microbar and p_surf= 14.1 +/- 0.4 microbar,
respectively. Based on recent models of Triton's volatile cycles, the overall
evolution over the last 30 years of the surface pressure is consistent with N2
condensation taking place in the northern hemisphere. However, models typically
predict a steady decrease in surface pressure for the period 2005-2060, which
is not confirmed by this observation. Complex surface-atmosphere interactions,
such as ice albedo runaway and formation of local N2 frosts in the equatorial
regions of Triton could explain the relatively constant pressure between 2017
and 2022.
