The primary mission objective for TESS is to survey the brightest stars near the earth for transitioning exoplanets over a two-year period. The TESS project will use an array of wide-field cameras to perform an all-sky survey. It will scan nearby stars for exoplanets. With TESS, it will be possible to study the mass, size, density and orbit of a large cohort of small planets, including a sample of rocky worlds in the habitable zones of their host stars. TESS will provide prime targets for further characterization by the James Webb Space Telescope, as well as other large ground-based and space-based telescopes of the future.
Previous sky surveys with ground-based telescopes have mainly picked out giant exoplanets. In contrast, TESS will examine a large number of small planets around the very brightest stars in the sky. TESS will record the nearest and brightest main sequence stars hosting transiting exoplanets, which will forever be the most favorable targets for detailed investigations. 
Once launched, the telescope would conduct a two-year all-sky survey program for exploring transiting exoplanets around nearby and bright stars.TESS would be equipped with four wide-angle telescopes and charge-coupled device (CCD) detectors, with a total size of 67 megapixels. Science data, which are pixel subarrays around each of up to 10,000 target stars per field, are transmitted to Earth every two weeks for analysis. Full-frame images with an effective exposure time of two hours are transmitted to the ground as well, enabling astrophysicists to search the data for an unexpected, transient phenomenon, such as the optical counterpart to a gamma-ray burst.
TESS will carry out the first space-borne all-sky exoplanet transit survey, covering 400 times as much sky as any previous mission, including Kepler. It will identify thousands of new planets in the solar neighborhood, with a special focus on planets comparable in size to the Earth. TESS will be in a special orbit, one that is not too close, and not too far, from both the Earth and the Moon. As a result, every two weeks TESS will approach close enough to the Earth for high data-downlink rates, while remaining above the planet's harmful radiation belts. This special orbit will remain stable for decades, keeping TESS' sensitive cameras in a stable temperature range.
In order to obtain imagery from both locations in both northern and southern hemispheres of the sky, TESS will utilize a lunar resonant orbit called P/2, a never-before-used orbit. This highly elliptical orbit can be stable; the mission apogee can be timed to keep the craft away from the Moon, which acts as a destabilizing agent. The majority of the orbit is spent well outside the Van Allen belts, to avoid damage to TESS. Every 13.7 days at its orbit's perigee, TESS will downlink the data it has collected during the orbit to Earth over a period of approximately 3 hours.