Stishovite is an important phase in subducting oceanic crust. The post-garnet assemblage from a precursor eclogite lithology contains up to 25 % stishovite at pressures above 25 GPa. This stishovite may contain up to 5 wt. % Al
2O
3. We measured the hydrogen contents of stishovite samples synthesized at 20–25 GPa and 1200–1800 °C from several starting materials containing up to 10 wt. % Al
2O
3. FTIR spectra of stishovite show major bands at 3111–3134 cm
− 1, with the frequencies increasing as H
2O and Al
2O
3 contents increase, and several minor bands at 2659–2667, 3240, 3261, 3312–3334, and 3351 cm
− 1. The H
2O content of Al-free stishovite is in the range of 16–30 wt. ppm. The maximum H
2O content of Al-bearing stishovite (4.4 wt. % Al
2O
3) synthesized at 20 GPa and 1400 °C is 3010 ± 300 wt. ppm. Most hydrogen in stishovite is associated with Al
3+ substitutional defects on the octahedral (Si
4+) site. The hydrogen can occupy 40 % of vacancies created by incorporation of Al
3+ at 20 GPa. This observation along with some anomalies in the FTIR spectra may indicate an alternative mechanism of Al
3+ incorporation into stishovite via the formation of oxygen vacancies or interstitial Al
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defects. We report the highest H
2O concentrations in Al-stishovite to date, and argue that it is the most important carrier of water into the lower mantle post-garnet eclogitic assemblages.