  We re-analyze the pristine eclipsing binary data from the $\textit{Kepler}$
and TESS missions, focusing on eccentricity measurements at short orbital
periods to emperically constrain tidal circularization. We find an average
circularization period of $~$6 days, as well as a short circularization period
of $\sim$3 days for the $\textit{Kepler}$/TESS field binaries. We argue
previous spectroscopic binary surveys reported longer circularization periods
due to small sample sizes, which were contaminated by an abundance of binaries
with circular orbits out to $\sim$10 days, but we re-affirm their data shows a
difference between the eccentricity distributions of young ($<$1 Gyr) and old
($>$3 Gyr) binaries. Our work calls into question the long circularization
periods quoted often in the literature.
