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Transiting Exoplanet Survey Satellite

(observatory-satellite searching for transiting exoplanets)

Transiting Exoplanet Survey Satellite (TESS) is a spacecraft on a mission to survey 2,000,000 nearby stars for transiting planets, launched in April 2018 for a 2-year primary mission. It uses four wide-angle telescopes and stores three months' data, allowing it to prioritize transmission to ground stations of promising data. It aims for stars brighter than 12 magnitudes, G-type stars and K-type stars, as well as nearby M dwarves, small M-type stars. Any further approved mission extensions will offer the opportunity to catch additional infrequent transits, and to concentrate on the most favorable portions of the sky. The TESS project began as an offshoot of the High Energy Transient Explorer (HETE) gamma-ray burst series, originally called HETE-S (for Hot Exoplanet Transit Explorer-Survey), aiming to adapted HETE technology, making use of the ongoing improvements in optical CCDs to perform an all-sky survey for exoplanets.

TOI stands for TESS object of interest, a term for a possible planet, i.e., the location of observations that appear to reveal a transiting planet. TFOP (for TESS Follow-up Observation Program) is an effort to investigate TESS discoveries, e.g., to confirm whether a TOI is a planet. As of 12/2020, TESS has produced over 2400 candidates (TOIs), including at least 700 apparently between Earth and Neptune in radius, and 82 confirmed to be planets through follow-up observation.

The terms TESS Duo and TESS-bis have been used the a concept of launching a second TESS satellite. TESS spots many transients (e.g., supernovae) as well as SSSBs, and an additional TESS, taking advantage of the existing design, could offer immediate confirmation of apparent transients as well as parallax regarding solar system orbits.

Further reading:
TICTIC 410451752input catalog
TOITOI 700 dobject of interest

Referenced by pages:
AU Microscopii (AU Mic)
etendue (AΩ)
extra-solar planet
heartbeat star
LHS 3844 b
TOI 700 d
transit method