  We present the discovery of a rare system detected in the TESS data showing
three different eclipsing-like signals. TIC 452991707 and TIC 452991693 seem to
be the second such system on the sky, whose two components separated about 16"
are gravitationally bounded, or comprise a co-moving pair. The three periods
detected from the TESS data are: PA=1.46155 d, PB=1.77418 d, and PC=1.03989 d,
respectively. The A and B periods belong to TIC 452991707, while the C comes
from the component TIC 452991693. The pair A shows the deepest eclipses, and
its orbit is very slightly eccentric. The third period C has lowest amplitude
(eclipsing or ellipsoidal nature), but originates from TIC 452991693, which is
connected to A+B because both visual components share similar proper motion and
distance. Long-term collection of data from older photometry from various
surveys also shows that the two inner pairs A and B orbit around their
barycenter. Its period is probably of a few years, but for a final derivation
of its orbital parameters one needs more up-to-date data. Hence, we call for
new observations of this amazing system.
