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Transiting Exoplanet Survey Satellite (TESS)
| Content Provider | Semantic Scholar |
|---|---|
| Author | Ricker, George R. Winn, J. Vanderspek, Roland Latham, David Winstow Bakos, G. Bean, Jacob Berta-Thompson, Zachory K. Brown, Timothy M. Buchhave, Lars A. Butler, Nathaniel R. Butler, Rebecca P. Chaplin, William J. Charbonneau, David Christensen-Dalsgaard, Jørgen Clampin, Mark Drake L. Doty, John P. Lee, Nathan De Dressing, Courtney Dunham, Edward Wood Endl, Michael Fressin, François Ge, Jian Henning, Thomas Holman, Matthew J. Howard, Andrew W. Ida, Shigeru Jenkins, Jon Jernigan, Garrett Johnson, J. A. Kaltenegger, Lisa Kawai, Nobuyuki Kjeldsen, Hans Laughlin, Gregory Levine, Alan M. Lin, Douglas N. C. Lissauer, Jack J. Queen, Phillip J. Mac Marcy, Geoffrey W. McCullough, Peter Rankin Morton, Timothy D. Narita, Norio Paegert, Martin A. Pallé, Enric Pepe, F. Pepper, J. W. Quirrenbach, Andreas Rinehart, Stephen Andrew Sasselov, Dimitar D. Sato, Bun’ei Seager, Sara Sozzetti, Alessandro Stassun, Keivan G. Sullivan, Peter Szentgyorgyi, Andrew Harold Torres, Guillermo Udry, Stéphane Villasenor, Joel S. |
| Copyright Year | 2014 |
| 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 IC (approximately less than) 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. |
| File Format | PDF HTM / HTML |
| DOI | 10.1117/12.2063489 |
| Volume Number | 9143 |
| Alternate Webpage(s) | http://dspace.mit.edu/openaccess-disseminate/1721.1/97916 |
| Alternate Webpage(s) | https://doi.org/10.1117/12.2063489 |
| Journal | Astronomical Telescopes and Instrumentation |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |
