TESS will count with 4 extended angle telescopes, and in order to indentify exoplanets it will use the transit method. The idea is that when a planet crosses in front of its star, the visual brightness of the star drops a small amount. According to these data, it is possible to determine the size of the planet. Theres another method that TESS doesn’t use but other exploring satellites do, wich is the radial velocity method. This method allows to determine the mass of exoplanets, so, with the information that both methods provide we can know the density of exoplanets and therefore infer information about their structure and composition.
Within its first 2 years of functioning, TESS is predicted to discover between a thousand and 10 thousand exoplanets that are Earth-size or larger, and it will definitively be a huge contribution in the exploration of our nearby solar systems.