The Transiting Exoplanet Survey Satellite
arXiv:1406.0151 · doi:10.1117/1.JATIS.1.1.014003
Abstract
The Transiting Exoplanet Survey Satellite (TESS) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During its two-year mission, TESS will employ four wide-field optical CCD cameras to monitor at least 200,000 main-sequence dwarf stars with I = 4-13 for temporary drops in brightness caused by planetary transits. Each star will be observed for an interval ranging from one month to one year, depending mainly on the star's ecliptic latitude. The longest observing intervals will be for stars near the ecliptic poles, which are the optimal locations for follow-up observations with the James Webb Space Telescope. Brightness measurements of preselected target stars will be recorded every 2 min, and full frame images will be recorded every 30 min. TESS stars will be 10-100 times brighter than those surveyed by the pioneering Kepler mission. This will make TESS planets easier to characterize with follow-up observations. TESS is expected to find more than a thousand planets smaller than Neptune, including dozens that are comparable in size to the Earth. Public data releases will occur every four months, inviting immediate community-wide efforts to study the new planets. The TESS legacy will be a catalog of the nearest and brightest stars hosting transiting planets, which will endure as highly favorable targets for detailed investigations.
accepted for publication in the new, peer-reviewed SPIE Journal of Astronomical Telescopes, Instruments, and Systems (JATIS)
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- Small Planets in the Galactic Context: Host Star Kinematics, Iron, and Element Enhancement
- Flares and rotation of M dwarfs with habitable zones accessible to TESS planet detections
- Transiting Exoplanet Monitoring Project (TEMP). II. Refined System Parameters and Transit Timing Analysis of HAT-P-33b
- TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M dwarf host
- Spitzer transit follow-up of planet candidates from the K2 mission
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- The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk
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- The Pulsation Properties of Bootis Stars I. The Southern TESS Sample
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- Peering above the clouds of the warm Neptune GJ 436b with CRIRES+
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- NGTS clusters survey -- III: A low-mass eclipsing binary in the Blanco 1 open cluster spanning the fully convective boundary
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- The chemical evolution of the solar neighbourhood for planet-hosting stars
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- The roAp stars observed by the Kepler Space Telescope
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- Young stellar objects, accretion disks, and their variability with Rubin Observatory LSST
- Multi-campaign Asteroseismic Analysis of eight Solar-like pulsating stars observed by the K2 mission
- Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass
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- Departure from the Exact Location of Mean Motion Resonances Induced by the Gas Disk in the Systems Observed by Kepler
- The Exomoon Corridor for Multiple Moon Systems
- Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey: III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-Transit Jupiter Orbiting TOI-2010
- Long-Term Photometry of IC 348 with the YETI Network
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- The nature of the photometric variability of HgMn stars: A test of simulated light curves of ϕ Phe against the TESS data
- A High-Eccentricity Warm Jupiter Orbiting TOI-4127
- A long-period pre-ELM system discovered from LAMOST medium-resolution survey
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- The Sparse Atmospheric MOdel Sampling Analysis (SAMOSA) intercomparison: Motivations and protocol version 1.0. A CUISINES model intercomparison project
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- The Pulsating Eclipsing Binary TIC 309658221 in a 7.59 Day Orbit
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- V994 Her: A Unique Triply Eclipsing Sextuple Star System
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- Planet Hunters TESS III: two transiting planets around the bright G dwarf HD 152843
- NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey
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- Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941
- The TESS light curve of the eccentric eclipsing binary 1SWASP J011351.29+314909.7 -- no evidence for a very hot M-dwarf companion
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- TESS Giants Transiting Giants V -- Two hot Jupiters orbiting red-giant hosts
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- The TESS Triple-9 Catalog II: a new set of 999 uniformly-vetted exoplanet candidates
- Tilted discs in six poorly studied cataclysmic variables
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- Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
- TIC 219006972: A Compact, Coplanar Quadruple Star System Consisting of Two Eclipsing Binaries with an Outer Period of 168 days
- The nearby magnetic cool DZ white dwarf PM J08186-3110
- On asymmetric dark matter constraints from the asteroseismology of a subgiant star
- Validation of HD 183579b using archival radial velocities: a warm-neptune orbiting a bright solar analog
- TOI-1749: an M dwarf with a Trio of Planets including a Near-Resonant Pair
- An Eclipsing 47 minute Double White Dwarf Binary at 400 pc
- Extreme mass ratios and fast rotation in three massive binaries
- Simultaneous eROSITA and TESS observations of the ultra-active star AB~Doradus
- BRITE observations of Centauri and Lupi, the first non-eclipsing members of the new class of nascent binaries
- A review of planetary systems around HD 99492, HD 147379 and HD 190007 with HARPS-N
- A close-in puffy Neptune with hidden friends: The enigma of TOI 620
- A Geologically Robust Procedure For Observing Rocky Exoplanets to Ensure that Detection of Atmospheric Oxygen is an Earth-Like Biosignature
- The GAPS Programme at TNG -- XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone
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- The Puzzling Story of Flare Inactive Ultra Fast Rotating M dwarfs. I. Exploring their Magnetic Fields
- Rotation periods and shape asphericity in asteroid families based on TESS S1-S13 observations
- Simultaneous Detection of Optical Flares of the Magnetically Active M Dwarf Wolf 359
- Atomic diffusion in solar-like stars with MESA. Comparison with the Montreal/Montpellier and CESTAM stellar evolution codes
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- TIC-320687387 B: a long-period eclipsing M-dwarf close to the hydrogen burning limit
- Coralie radial-velocity search for companions around evolved stars (CASCADES) III. A new Jupiter host-star: in-depth analysis of HD 29399 using TESS data
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- An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542
- The CARMENES search for exoplanets around M dwarfs. Revisiting the GJ 581 multi-planetary system with new Doppler measurements from CARMENES, HARPS, and HIRES
- The Pre-He White Dwarfs in Eclipsing Binaries. IV. WASP 1814+48 with Multiperiodic Pulsations
- A search for transit timing variations in the HATS-18 planetary system
- Absolute dimensions and apsidal motion of the eclipsing binaries V889 Aql and V402 Lac
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- Two New White Dwarfs With Variable Magnetic Balmer Emission Lines
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- On the Utility of Transmission Color Analysis I: Differentiating Super-Earths and Sub-Neptunes
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- Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
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- Shallow Transits -- Deep Learning II: Identify Individual Exoplanetary Transits in Red Noise using Deep Learning
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