Abstract. Unique bell-shaped underwater speleothems were recently reported from the
deep (∼ 55 m) meromictic El Zapote sinkhole (cenote) on the
Yucatán Peninsula, Mexico. The local diving community has termed these
speleothems as Hells Bells because of their shape and appearance in a dark
environment in ∼ 28–38 m water depth above a sulfidic halocline. It
was also suggested that Hells Bells form under water, yet the mystery of
their formation remained unresolved. Therefore, we conducted detailed
hydrogeochemical and geochemical analyses of the water column and Hells Bells
speleothems including stable carbon isotopes. Based on the comprehensive
results presented in this study we deduce that both biogeochemical processes
in the pelagic redoxcline and a dynamic halocline elevation of El Zapote
cenote are essential for Hells Bells formation. Hells Bells most likely form
in the redoxcline, a narrow 1–2 m thick water layer immediately above the
halocline where a pelagic chemolithoautotrophic microbial community thrives
from the upward diffusion of reduced carbon, nitrogen and sulfur species
released from organic matter degradation in organic-rich debris. We
hypothesize that chemolithoautotrophy, in particular proton-consuming
nitrate-driven anaerobic sulfide oxidation, favors calcite precipitation in
the redoxcline and hence Hells Bells formation. A dynamic elevation of the
halocline as a hydraulic response to droughts, annual tidal variability and
recharge events is further discussed, which might explain the shape of Hells
Bells as well as their occurrence over a range of 10 m water depth. Finally,
we infer that highly stagnant conditions, i.e., a thick halocline, a
low-light environment and sufficient input of organic material into a deep
meromictic cenote are apparent prerequisites for Hells Bells formation. This
might explain their exclusivity to only a few cenotes in a restricted area of
the northeastern Yucatán Peninsula.