The transiting exoplanet survey satellite

George R. Ricker, Joshua N. Winn, Roland Vanderspek, David W. Latham, Gáspár Bakos, Jacob L. Bean, Zachory K. Berta-Thompson, Timothy M. Brown, Lars Buchhave, Nathaniel Butler, R. Paul Butler, William J. Chaplin, David Charbonneau, Jørgen Christensen-Dalsgaard, Mark Clampin, Drake Deming, John Doty, Nathan De Lee, Courtney Dressing, E. W. Dunham & 38 others Michael Endl, Francois Fressin, Jian Ge, Thomas Henning, Matthew J. Holman, Andrew W. Howard, Shigeru Ida, Jon Jenkins, Garrett Jernigan, John A. Johnson, Lisa Kaltenegger, Nobuyuki Kawai, Hans Kjeldsen, Gregory Laughlin, Alan M. Levine, Douglas Lin, Jack J. Lissauer, Phillip Macqueen, Geoffrey Marcy, P. R. McCullough, Timothy D. Morton, Norio Narita, Martin Paegert, Enric Palle, Francesco Pepe, Joshua Pepper, Andreas Quirrenbach, S. A. Rinehart, Dimitar Sasselov, Bun'Ei Sato, Sara Seager, Alessandro Sozzetti, Keivan G. Stassun, Peter Sullivan, Andrew Szentgyorgyi, Guillermo Torres, Stephane Udry, Joel Villasenor

Research output: Chapter in Book/Report/Conference proceedingConference contribution

211 Citations (Scopus)

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<inf>C</inf> (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.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
PublisherSPIE
Volume9143
ISBN (Print)9780819496119
DOIs
StatePublished - 2014
EventSpace Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave - Montreal, Canada
Duration: Jun 22 2014Jun 27 2014

Other

OtherSpace Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave
CountryCanada
CityMontreal
Period6/22/146/27/14

Fingerprint

Exoplanets
extrasolar planets
Stars
Star
Satellites
Planets
stars
planets
Ecliptic
ecliptic
Brightness
brightness
Luminance
Kepler mission
intervals
Earth (planet)
dwarf stars
James Webb Space Telescope
Neptune (planet)
main sequence stars

Keywords

  • Exoplanet
  • Extrasolar planet
  • Photometry
  • Satellite
  • Transits

ASJC Scopus subject areas

  • Applied Mathematics
  • Computer Science Applications
  • Electrical and Electronic Engineering
  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics

Cite this

Ricker, G. R., Winn, J. N., Vanderspek, R., Latham, D. W., Bakos, G., Bean, J. L., ... Villasenor, J. (2014). The transiting exoplanet survey satellite. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 9143). [914320] SPIE. https://doi.org/10.1117/12.2063489

The transiting exoplanet survey satellite. / Ricker, George R.; Winn, Joshua N.; Vanderspek, Roland; Latham, David W.; Bakos, Gáspár; Bean, Jacob L.; Berta-Thompson, Zachory K.; Brown, Timothy M.; Buchhave, Lars; Butler, Nathaniel; Butler, R. Paul; Chaplin, William J.; Charbonneau, David; Christensen-Dalsgaard, Jørgen; Clampin, Mark; Deming, Drake; Doty, John; De Lee, Nathan; Dressing, Courtney; Dunham, E. W.; Endl, Michael; Fressin, Francois; Ge, Jian; Henning, Thomas; Holman, Matthew J.; Howard, Andrew W.; Ida, Shigeru; Jenkins, Jon; Jernigan, Garrett; Johnson, John A.; Kaltenegger, Lisa; Kawai, Nobuyuki; Kjeldsen, Hans; Laughlin, Gregory; Levine, Alan M.; Lin, Douglas; Lissauer, Jack J.; Macqueen, Phillip; Marcy, Geoffrey; McCullough, P. R.; Morton, Timothy D.; Narita, Norio; Paegert, Martin; Palle, Enric; Pepe, Francesco; Pepper, Joshua; Quirrenbach, Andreas; Rinehart, S. A.; Sasselov, Dimitar; Sato, Bun'Ei; Seager, Sara; Sozzetti, Alessandro; Stassun, Keivan G.; Sullivan, Peter; Szentgyorgyi, Andrew; Torres, Guillermo; Udry, Stephane; Villasenor, Joel.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 9143 SPIE, 2014. 914320.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Ricker, GR, Winn, JN, Vanderspek, R, Latham, DW, Bakos, G, Bean, JL, Berta-Thompson, ZK, Brown, TM, Buchhave, L, Butler, N, Butler, RP, Chaplin, WJ, Charbonneau, D, Christensen-Dalsgaard, J, Clampin, M, Deming, D, Doty, J, De Lee, N, Dressing, C, Dunham, EW, Endl, M, Fressin, F, Ge, J, Henning, T, Holman, MJ, Howard, AW, Ida, S, Jenkins, J, Jernigan, G, Johnson, JA, Kaltenegger, L, Kawai, N, Kjeldsen, H, Laughlin, G, Levine, AM, Lin, D, Lissauer, JJ, Macqueen, P, Marcy, G, McCullough, PR, Morton, TD, Narita, N, Paegert, M, Palle, E, Pepe, F, Pepper, J, Quirrenbach, A, Rinehart, SA, Sasselov, D, Sato, BE, Seager, S, Sozzetti, A, Stassun, KG, Sullivan, P, Szentgyorgyi, A, Torres, G, Udry, S & Villasenor, J 2014, The transiting exoplanet survey satellite. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 9143, 914320, SPIE, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, Montreal, Canada, 6/22/14. https://doi.org/10.1117/12.2063489
Ricker GR, Winn JN, Vanderspek R, Latham DW, Bakos G, Bean JL et al. The transiting exoplanet survey satellite. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 9143. SPIE. 2014. 914320 https://doi.org/10.1117/12.2063489
Ricker, George R. ; Winn, Joshua N. ; Vanderspek, Roland ; Latham, David W. ; Bakos, Gáspár ; Bean, Jacob L. ; Berta-Thompson, Zachory K. ; Brown, Timothy M. ; Buchhave, Lars ; Butler, Nathaniel ; Butler, R. Paul ; Chaplin, William J. ; Charbonneau, David ; Christensen-Dalsgaard, Jørgen ; Clampin, Mark ; Deming, Drake ; Doty, John ; De Lee, Nathan ; Dressing, Courtney ; Dunham, E. W. ; Endl, Michael ; Fressin, Francois ; Ge, Jian ; Henning, Thomas ; Holman, Matthew J. ; Howard, Andrew W. ; Ida, Shigeru ; Jenkins, Jon ; Jernigan, Garrett ; Johnson, John A. ; Kaltenegger, Lisa ; Kawai, Nobuyuki ; Kjeldsen, Hans ; Laughlin, Gregory ; Levine, Alan M. ; Lin, Douglas ; Lissauer, Jack J. ; Macqueen, Phillip ; Marcy, Geoffrey ; McCullough, P. R. ; Morton, Timothy D. ; Narita, Norio ; Paegert, Martin ; Palle, Enric ; Pepe, Francesco ; Pepper, Joshua ; Quirrenbach, Andreas ; Rinehart, S. A. ; Sasselov, Dimitar ; Sato, Bun'Ei ; Seager, Sara ; Sozzetti, Alessandro ; Stassun, Keivan G. ; Sullivan, Peter ; Szentgyorgyi, Andrew ; Torres, Guillermo ; Udry, Stephane ; Villasenor, Joel. / The transiting exoplanet survey satellite. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 9143 SPIE, 2014.
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