EAS Publications Series
Volume 42, 2010Extrasolar Planets in Multi-Body Systems: Theory and Observations
|Page(s)||191 - 199|
|Published online||19 April 2010|
K. Goździewski, A. Niedzielski and J. Schneider (eds)
EAS Publications Series, 42 (2010) 191-199
Detectability of Earth-like Planets in Multi-Planet Systems: Preliminary Report
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
2 NASA Exoplanet Science Institute, Pasadena, CA, USA
3 Carnegie Institution of Washington, Washington, DC, USA
4 Space Telescope Science Institute, Baltimore, MD, USA
5 San Francisco State University, San Francisco, CA, USA
6 University of Florida, Gainesville, FL, USA
7 Ohio State University, Columbus, OH, USA
8 University of California at Berkeley, Berkeley, CA, USA
9 University of Tokyo, Tokyo, Japan
10 Princeton University, Princeton, NJ, USA
11 University of California at Santa Cruz, Santa Cruz, CA, USA
12 Southwest Research Institute, Boulder, CA, USA
13 Tennessee State University, Nashville, TN, USA
14 University of Colorado, Boulder, CO, USA
15 INAF – Osservatorio Astronomioco di Torino, Pino Torinese, Italy
We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind calculations designed to answer this question.
© EAS, EDP Sciences, 2010
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