  We present the first analysis of results from the SuperWASP Variable Stars
Zooniverse project, which is aiming to classify 1.6 million phase-folded light
curves of candidate stellar variables observed by the SuperWASP all sky survey
with periods detected in the SuperWASP periodicity catalogue. The resultant
data set currently contains $>$1 million classifications corresponding to
$>$500,000 object-period combinations, provided by citizen scientist
volunteers. Volunteer-classified light curves have $\sim$89 per cent accuracy
for detached and semi-detached eclipsing binaries, but only $\sim$9 per cent
accuracy for rotationally modulated variables, based on known objects. We
demonstrate that this Zooniverse project will be valuable for both population
studies of individual variable types and the identification of stellar
variables for follow up. We present preliminary findings on various unique and
extreme variables in this analysis, including long period contact binaries and
binaries near the short-period cutoff, and we identify 301 previously unknown
binaries and pulsators. We are now in the process of developing a web portal to
enable other researchers to access the outputs of the SuperWASP Variable Stars
project.
