  We present Atacama Large Millimeter/sub-millimeter Array (ALMA) Cycle-5
observations of HBC 494, as well as calculations of the kinematic and dynamic
variables which represent the object's wide-angle bipolar outflows. HBC 494 is
a binary FU Orionis type object located in the Orion A molecular cloud. We take
advantage of combining the ALMA main array, Atacama Compact Array (ACA), and
Total Power (TP) array in order to map HBC 494's outflows and thus, estimate
their kinematic parameters with higher accuracy in comparison to prior
publications. We use $^{12}$CO, $^{13}$CO, C$^{18}$O and SO observations to
describe the object's outflows, envelope, and disc, as well as estimate the
mass, momentum, and kinetic energy of the outflows. After correcting for
optical opacity near systemic velocities, we estimate a mass of
$3.0\times10^{-2}$ M$_{\odot}$ for the southern outflow and $2.8\times10^{-2}$
M$_{\odot}$ for the northern outflow. We report the first detection of a
secondary outflow cavity located approximately $15$" north of the central
binary system, which could be a remnant of a previous large-scale accretion
outburst. Furthermore, we find CO spatial features in HBC 494's outflows
corresponding to position angles of $\sim35^{\circ}$ and $\sim145^{\circ}$.
This suggests that HBC 494's outflows are most likely a composite of
overlapping outflows from two different sources, i.e., HBC 494a and HBC 494b,
the two objects in the binary system.
