Transiting Exoplanet Survey Satellite
Artist concept of TESS
|Mission type||Space observatory|
|Operator||NASA / MIT|
|Mission duration||Planned: 2 years|
|Launch mass||350 kg (772 lb)|
|Dimensions||3.7×1.2×1.5 m (12.1×3.9×4.9 ft)|
|Start of mission|
|Launch date||August 2017|
|Rocket||Falcon 9 v1.1|
|Launch site||Cape Canaveral SLC-40|
|Reference system||Highly elliptical|
|Semi-major axis||240,000 km (150,000 mi)|
|Perigee||108,000 km (67,000 mi)|
|Apogee||373,000 km (232,000 mi)|
The primary mission objective for TESS is to survey the brightest stars near the Earth for transiting 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 detected 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.
Led by the Massachusetts Institute of Technology with seed funding from Google, TESS was one of 11 proposals selected for NASA funding in September 2011, down from the original 42 submitted in February of that year. On April 5, 2013, it was announced that TESS, along with the Neutron Star Interior Composition Explorer (NICER), had been selected for launch in 2017.
The genesis of TESS began as early as 2006, when a design was developed from private funding by individuals, Google, and The Kavli Foundation. In 2008, MIT proposed that TESS become a full NASA mission and submitted it for the Small Explorer program at Goddard Space Flight Center, but it was not selected. It was resubmitted in 2010 as an Explorers program mission, and was approved in 2013 as a Medium Explorer mission.
The transit technique has been an successful way of studying and discovering exoplanets, and when launched TESS will join a growing fleet of telescopes studying in this area.
TESS is designed to carry out the first space-borne all-sky transiting exoplanet survey. It is equipped with four wide-angle telescopes and associated charge-coupled device (CCD) detectors. Science data will be transmitted to Earth every two weeks. Full-frame images with an effective exposure time of two hours will be transmitted as well, enabling scientists to search for unexpected, transient phenomena, such as the optical counterparts to gamma-ray bursts.
In order to obtain unobstructed imagery of both the northern and southern hemispheres of the sky, TESS will utilize a 2:1 lunar resonant orbit called P/2, a never-before-used orbit. The spacecraft's 373,000 km (232,000 mi) apogee is timed to keep the craft away from the Moon, which acts as a destabilizing agent. This highly elliptical orbit should remain stable for decades, and will keep TESS's cameras in a stable temperature range. The majority of the orbit is spent outside the Van Allen belts to avoid radiation damage to TESS. Every 13.7 days at its perigee of 108,000 km (67,000 mi), TESS will downlink the data it has collected during the orbit to Earth over a period of approximately three hours.
TESS's survey will focus on nearby G- and K-type stars with apparent magnitudes brighter than magnitude 12. Approximately 500,000 stars will be studied, including the 1,000 closest red dwarfs, across an area of sky 400 times larger than covered by the original Kepler mission. TESS is expected to discover more than 3,000 transiting exoplanet candidates, including those which are Earth sized or larger. Of those discoveries, an estimated twenty could be super-Earths located in the habitable zone around a star.
The survey is broken up into 26 observation sectors, each sector being 24° x 96°, with an overlap of sectors at the ecliptic poles to allow for additional sensitivity toward smaller and longer-period exoplanets in that region of the celestial sphere. The spacecraft will spend two 13.7 day orbits observing each sector, mapping the northern hemisphere of sky in its first year of operation and the southern hemisphere in its second year. Each of TESS's cameras will take one-minute exposures focused on specifically targeted stars as part of its transit search, and 30-minute full-frame exposures to search for other transient events.
Exoplanet candidates could later be investigated by the Automated Planet Finder telescope, the HARPS spectrometer and both the future ESPRESSO spectrometer and James Webb Space Telescope. The development team at MIT has suggested that the first manned interstellar space missions may be to planets discovered by TESS.
TESS uses an Orbital Sciences LEOStar-2 satellite bus, capable of three-axis stabilization using four hydrazine thrusters plus four reaction wheels providing better than three arc-second fine spacecraft pointing control. Power is provided by two single-axis solar arrays generating 400 watts. A Ka-band dish antenna will provide a 100 Mbit/s science downlink.
TESS will be launched in August 2017 on a SpaceX Falcon 9 v1.1 rocket from the Cape Canaveral Air Force Station. The total value of the contract is US$87 million. SpaceX was awarded the launch in December 2014.
The sole instrument on TESS is a package of four wide-field-of-view CCD cameras. Each camera features a low-noise, low-power 16.8 megapixel CCD detector created by the MIT Lincoln Laboratory. Each has a 24° × 24° field of view, a 100 mm (4 in) effective pupil diameter, a lens assembly with seven optical elements, and a bandpass range of 600 to 1000 nm.
Stable light source for tests
One of the issues facing the development of this type of instrument is a having an ultra-stable light source to test on. In 2015 a group at the University of Geneva made a breakthrough in the development of a stable light source. While this instrument was created to support ESA's CHEOPS exoplanet observatory, one was also ordered by the TESS program. Although both plan to look at bright nearby stars using the transit method, CHEOPS is focused on collecting more data on known exoplanets, including those found by TESS and other survey missions.
TESS is planned to use a 30 minute observation cadence for full-frame images, which has been noted for imposing a hard Nyquist limit that can be problematic for asteroseismology of stars. Many exoplanet hunters are also used for asterseismology.
- CHEOPS, future exoplanet mission
- COROT, 2006-2012 exoplanet observatory
- Kepler (spacecraft), 2009-present exoplanet observatory
- PLATO, 2024 exoplanet observatory
- Sagittarius Window Eclipsing Extrasolar Planet Search, 2006 exoplanet survey
- Beck, Joshua; Diller, George H. (December 16, 2014). "NASA Awards Launch Services Contract for Transiting Exoplanet Survey Satellite" (Press release). NASA. Retrieved December 17, 2014.
- "NASA FY 2015 President's Budget Request Summary" (PDF). NASA. March 10, 2014.
- Chandler, David (March 19, 2008). "MIT aims to search for Earth-like planets with Google's help". MIT News.
- Brown, Dwayne (September 29, 2011). "NASA Selects Science Investigations For Concept Studies" (Press release). NASA.
- Harrington, J. D. (April 5, 2013). "NASA Selects Explorer Investigations for Formulation" (Press release). NASA.
- "NASA selects MIT-led TESS project for 2017 mission". MIT News. April 5, 2013. Retrieved April 6, 2013.
- "Mission History". Transiting Exoplanet Survey Satellite. NASA. Retrieved October 23, 2015.
- Hand, Eric (June 22, 2009). "No SMEX-love for TESS". Nature. Retrieved October 23, 2015.
- "Medium-Class Explorers (MIDEX) Missions in Development". NASA. Retrieved October 23, 2015.
- Nowakowski, Tomasz (March 18, 2015). "ESA's CHEOPS Satellite: The Pharaoh of Exoplanet Hunting". Spaceflight Insider. Retrieved October 23, 2015.
- Ricker, George R. (June 26, 2014). Discovering New Earths and Super-Earths in the Solar Neighborhood. SPIE Astronomical Telescopes + Instrumentation. June 22–27, 2014. Montréal, Quebec, Canada. doi:10.1117/2.3201407.18.
- Keesey, Lori (July 31, 2013). "New Explorer Mission Chooses the 'Just-Right' Orbit". NASA.
- Seager, Sara (2011). "Exoplanet Space Missions". Massachusetts Institute of Technology. Retrieved April 7, 2013.
- Zastrow, Mark (May 30, 2013). "Exoplanets After Kepler: What’s next?". Sky & Telescope. Retrieved December 17, 2014.
- "TESS: Transiting Exoplanet Survey Satellite" (PDF). NASA. October 2014. FS-2014-1-120-GSFC. Retrieved December 17, 2014.
- Hadhazy, Adam (July 23, 2015). "Super-Earths Might Be Our Best Bet For Finding Alien Life". Discover. Retrieved October 23, 2015.
- Gilster, Paul (March 26, 2008). "TESS: All Sky Survey for Transiting Planets". Centauri Dreams. Tau Zero Foundation.
- "TESS: Discovering Exoplanets Orbiting Nearby Stars" (PDF). Orbital Sciences. 2014. FS011_13_2998. Retrieved December 17, 2014.
- Berger, Brian (December 17, 2014). "NASA Taps SpaceX To Launch TESS Satellite". SpaceNews. Retrieved October 31, 2015.
- Peach, Matthew (October 1, 2015). "Swiss group develops 'most stable light source' for satellite tests". Optics.org. Retrieved October 23, 2015.
- Nowakowski, Tomasz (March 17, 2015). "ESA's CHEOPS Satellite: The Pharaoh of Exoplanet Hunting". Astro Watch. Retrieved October 29, 2015.
- Murphy, Simon J. (November 2015). "The potential for super-Nyquist asteroseismology with TESS". Monthly Notices of the Royal Astronomical Society 453 (3): 2569–2575. arXiv:1508.02717. Bibcode:2015MNRAS.453.2569M. doi:10.1093/mnras/stv1842.
- "Asteroseismic data analysis with Kepler, K2, TESS and PLATO". FindaPhD.com. Retrieved October 31, 2015.
- Ricker, George R.; Winn, Joshua N.; Vanderspek, Roland; Latham, David W.; Bakos, Gáspár Á.; et al. (October 24, 2014). "Transiting Exoplanet Survey Satellite". Journal of Astronomical Telescopes, Instruments, and Systems 1 (1). arXiv:1406.0151. Bibcode:2014SPIE.9143E..20R. doi:10.1117/1.JATIS.1.1.014003.
- Stassun, Keivan (November 18, 2014). "TESS and Galactic Science" (PDF). California Institute of Technology.
|Wikimedia Commons has media related to Transiting Exoplanet Survey Satellite.|
- TESS website by NASA Goddard
- TESS website by Massachusetts Institute of Technology
- TESS website by the Kavli Foundation