  Aims: Using the unprecedented combination of high resolution and sensitivity
offered by ALMA, we aim to investigate whether and how hot corinos,
circumstellar disks, and ejected gas are related in young solar-mass
protostars. Methods: We observed CH$_3$CHO and deuterated water (HDO)
high-excitation ($E_{\rm u}$ up to 335 K) lines towards the Sun-like protostar
HH212--MM1. Results: For the first time, we have obtained images of CH$_3$CHO
and HDO emission in the inner $\simeq$ 100 AU of HH212. The multifrequency line
analysis allows us to contrain the density ($\geq$ 10$^{7}$ cm$^{-3}$),
temperature ($\simeq$ 100 K), and CH$_3$CHO abundance ($\simeq$ 0.2--2 $\times$
10$^{-9}$) of the emitting region. The HDO profile is asymmetric at low
velocities ($\leq$ 2 km s$^{-1}$ from $V_{\rm sys}$). If the HDO line is
optically thick, this points to an extremely small ($\sim$ 20--40 AU) and dense
($\ge$ 10$^{9}$ cm$^{-3}$) emitting region. Conclusions: We report the first
detection of a hot corino in Orion. The HDO asymmetric profile indicates a
contribution of outflowing gas from the compact central region, possibly
associated with a dense disk wind.
