Published April 19, 2010
| Version public
Journal Article
Detectability of Earth-like Planets in Multi-Planet Systems: Preliminary Report
Creators
- Traub, W. A.1
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Beichman, C.2
- Boden, A. F.2
- Boss, A. P.3
- Casertano, S.4
- Catanzarite, J.1
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Fischer, D.5
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Ford, E. B.6
- Gould, A.7
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Halverson, S.8
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Howard, A.8
- Ida, S.9
- Kasdin, N. J.10
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Laughlin, G. P.11
- Levison, H. F.12
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Lin, D.11
- Makarov, V. V.2
- Marr, J.1
- Muterspaugh, M.13
- Raymond, S. N.14
- Savransky, D.10
- Shao, M.1
- Sozzetti, A.
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Zhai, C.1
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1.
Jet Propulsion Lab
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2.
NASA Exoplanet Science Institute
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3.
Carnegie Institution for Science
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4.
Space Telescope Science Institute
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5.
San Francisco State University
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6.
University of Florida
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7.
The Ohio State University
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8.
University of California, Berkeley
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9.
University of Tokyo
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10.
Princeton University
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11.
University of California, Santa Cruz
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12.
Southwest Research Institute
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13.
Tennessee State University
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14.
University of Colorado Boulder
Abstract
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.
Additional Information
© 2010 EAS, EDP Sciences. Published online 19 April 2010.Additional details
Identifiers
- Eprint ID
- 78767
- Resolver ID
- CaltechAUTHORS:20170705-124700317
Dates
- Created
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2017-07-05Created from EPrint's datestamp field
- Updated
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2021-11-15Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- Infrared Processing and Analysis Center (IPAC) , Physics Department