  This study presents photometric solutions for a carefully selected sample of
181 detached eclipsing binary systems recently observed by the Transiting
Exoplanet Survey Satellite (TESS) mission. Our findings contribute to
discussions about OBA-type systems and the orbital circularization influenced
by tidal interactions. The results encompass crucial parameters, including the
sum of radii fraction ($r_{\rm a}\,+\,r_{\rm b}$), radii ratio ($k$), orbital
inclination ($i$), surface brightness ratio ($J$), and combinations of the
longitude of the periastron and orbital eccentricity ($e\,\sin\,\omega$ and
$e\,\cos\,\omega$). Geometric light curve fitting is performed using version 43
of the {\sc jktebop} code, serving as the primary tool for determining orbital
elements and physical ratios. Careful uncertainty estimates for these findings
are derived through bootstrap simulations. This work introduces unprecedented
photometric solutions for 172 well-detached eclipsing systems, while the
results for the remaining nine systems exhibit excellent agreement with those
previously reported in the literature. Additionally, a critical primary radius
fraction ($R_{\rm a}/a$) of 0.266 is identified for our sample of radiative
envelope stars, consistent with observational and theoretical findings in the
literature. Finally, we determine a circularization period of 5.762 days based
on a function from the literature, revealing a discrepancy with Zahn's theory
for hot stars.
